{"as_of":"2026-08-21T17:13:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:19002841d39c0b5a5a5958c558396d36ab70ec2698b675d433cd08bad18dbc12","coverage":[{"denominator":116,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T04:21:21.587471Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2608.10105/citation-record","integrity":"/paper/2608.10105/integrity","json":"/paper/2608.10105/citation-record.json","paper":"/paper/2608.10105"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.087000Z","title":"In our analysis, we assume a fixed sample age of ¯tage = 1 Gyr, corresponding to the time over which the sample has been recording damage tracks","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.087000Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:cbc98a3d74b7630f9c691e253eb8aac0922a310a0bd5916cd14f0ab863f941f2","observation_id":"4e41e89d-ca86-4fa8-b25c-f97f922b4b62","resolution":{"observed_at":"2026-08-14T04:21:21.087000Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.203340Z","title":null,"venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.203340Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:1c6c6a2139924ee75b925c6acf34cf11e4e95a25a395105ce138eaa315f9ed75","observation_id":"2613cca4-636b-42d7-807f-d50fe57789c4","resolution":{"observed_at":"2026-08-14T04:21:21.203340Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.207910Z","title":null,"venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.207910Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:c7b0d2b8e96968baebcf12697c3419a89cc863882dd540db62be7670a18824ad","observation_id":"3703e7ba-0e23-486a-853b-c902b2a7f89c","resolution":{"observed_at":"2026-08-14T04:21:21.207910Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.092703Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.092703Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:23bccb1a8e6977f509558ed5ca9a255aa5cfa0814a731ff3b717aa2ee69caa18","observation_id":"6ef53e23-432b-42a8-ac34-7d02ccfe1cc0","resolution":{"observed_at":"2026-08-14T04:21:21.092703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.097402Z","title":"5: Projected significance for rejecting the elastic standard SI (O s","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.097402Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:1d5ea50c7e686a494868b631f6acddf0293dc2b4e2e10b46fffed93bd2dc5afe","observation_id":"b9cc61d9-e4a4-4704-afd0-4d012053fe29","resolution":{"observed_at":"2026-08-14T04:21:21.097402Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.107925Z","title":"The left (right) panel corresponds to mχ = 5 GeV/c 2 (500 GeV/c 2)","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.107925Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:b2f13e47b4effed5cd469e5e9d62dfdf2bc46c52db74b326e58d62cd31149ae7","observation_id":"372efbc5-1aec-438c-bc6f-5b3c8471b7f7","resolution":{"observed_at":"2026-08-14T04:21:21.107925Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.128983Z","title":"This behavior is consistent with the qualitative features observed in Figs","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.128983Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:5b654ee46f2eb8af579721d29cdff86756bded7b04f2584a0e0d2bad894f2842","observation_id":"87048260-355c-4833-bb16-5895761abbd8","resolution":{"observed_at":"2026-08-14T04:21:21.128983Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.133855Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.133855Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:9aea5b1de72840b629b7beb1ada1b81478cb1d460467f5a4fb89a30f28a7dc11","observation_id":"bd758e91-46ea-4987-8ffa-c0998e5f408b","resolution":{"observed_at":"2026-08-14T04:21:21.133855Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.138238Z","title":"6: Projected significance for rejecting the inelastic standard SI (O s","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.138238Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:7f71f77bd3f2aaf179b60c453760db1ea731efe61f7966718af47e96480a84b5","observation_id":"70e16978-851d-41ff-85d9-9f29a437059f","resolution":{"observed_at":"2026-08-14T04:21:21.138238Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.142818Z","title":"Thep-value and corresponding significance (in units ofσ) are shown assuming a DM signal generated by non-standard NREFT operators (O s 3,O s 5,O s 8,O s 11,O s 12, andO s","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.142818Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:1e76147e6270b56203cccee1bebbe786e6b11c5f6a13bae86306f67a45684db2","observation_id":"04da3ac4-ecd0-4deb-809f-1422dc6fb0a1","resolution":{"observed_at":"2026-08-14T04:21:21.142818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.076121Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.076121Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:1c182b9eb84ee91e37fdc9a0cd0672d0aee1c53183decb6a4853468f85fa6a40","observation_id":"6778b80b-13f5-4dc2-a3c7-02c743651396","resolution":{"observed_at":"2026-08-14T04:21:21.076121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.146959Z","title":"The left (right) panel corresponds to δm = 50 keV/c2 (100 keV/c2)","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.146959Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:6e5f2c69700b12b91bb6a44852ba45e9c75f389e79b6e99bbd0efa5ad0143ee5","observation_id":"47137ec4-1f27-4200-a681-bde7ccbf0c64","resolution":{"observed_at":"2026-08-14T04:21:21.146959Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.151523Z","title":"7, where the contours shift progressively toward larger exposures for these operators","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.151523Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:18fa900a7155456c925de16c4f164805c94c05b73126ad78850445d18f2c2a0e","observation_id":"ce429c58-b099-4c03-a6f0-a941f67b70cd","resolution":{"observed_at":"2026-08-14T04:21:21.151523Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.082216Z","title":"14 To discriminate between two interactions, we compare two signal-plus-background hypotheses","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.082216Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:73e2c27fbd30131377ba6f4baccc90bf9c3ca333aed3fccbbae604268dbf89e1","observation_id":"eb1b77b3-95ba-47a7-a1c6-0479a4bc564f","resolution":{"observed_at":"2026-08-14T04:21:21.082216Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.155858Z","title":"Contours corresponding to 1σ–5σsignificance are shown as a function of DM mass and exposure for the low-resolution (LR,σ x = 15 nm) scenario","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.155858Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:999d543bc9bfd6606d42215426b987d631a7c508900deeb7bc6ec36bfd0d91bf","observation_id":"43ad03d8-27d0-48c6-b4c5-bbbd4fd06c38","resolution":{"observed_at":"2026-08-14T04:21:21.155858Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.160564Z","title":"observed for elastic scattering","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.160564Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:e7918c97ab9b7893895a6258445af7c82d80054e90eaf32db7481a6409202d2f","observation_id":"d090a037-92c2-46ad-a5eb-b35914b36ed4","resolution":{"observed_at":"2026-08-14T04:21:21.160564Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.165167Z","title":"Contours corresponding to 1σ–5σsignificance are shown as a function of DM mass and exposure for the low-resolution (LR,σ x = 15 nm) scenario","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.165167Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:52173873c263fd64bc1fd37b57f9afe00dbe8fb5afbbd49fb3bb6127dd84f3dc","observation_id":"c93d4fe0-e358-4a0d-bb0c-f3471c02ef9c","resolution":{"observed_at":"2026-08-14T04:21:21.165167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.173613Z","title":"The remaining spin-dependent operators accessible to halite paleo-detectors,O s 7,O s 9, andO s 14, yield mass-reconstruction projections similar to those shown in Fig","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.173613Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:b9ff1781bc591bce62c489a42967f1e8fe47b9f2f0bc0df20e9c3b5e5d610ee0","observation_id":"95a6c8b8-9ae5-4b16-8d06-eed57b3b4ff5","resolution":{"observed_at":"2026-08-14T04:21:21.173613Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.178434Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.178434Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:c372d81aab9c2496c9984a29993deb75a6424c1120b0a8e7b2d0fc68edc31068","observation_id":"bee06859-2726-4dab-843d-b7b5bd9f1ded","resolution":{"observed_at":"2026-08-14T04:21:21.178434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.192253Z","title":"As in the gypsum analysis, the discrimination power is significantly reduced for light DM particles in the LR scenario because of the limited sensitivity to short damage tracks","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.192253Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:0bbc5e03340d3197cb9fab0a606552984ff6cf47c86b8efc83c0d1b9db7b2ab8","observation_id":"d3622d46-8765-4972-860c-fa3bb8d8a6be","resolution":{"observed_at":"2026-08-14T04:21:21.192253Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.197924Z","title":"Drukier and L","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.197924Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:c5dbf6d1beb8757ec004a675d152aff16d736e6e7e011d80fe0f6aeba91f352b","observation_id":"693a5aff-ca05-4ea9-9a5a-d8bd6442b638","resolution":{"observed_at":"2026-08-14T04:21:21.197924Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.03764","last_updated":"2023-08-02T15:16:09Z","snapshot_observed_at":"2026-07-06T13:29:08.763456Z","submitted_at":"2022-07-08T09:10:04Z","title":"First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.03764","snapshot_observed_at":"2026-08-14T04:21:21.212483Z","title":"Aalberset al.(LZ), First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment, Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.212483Z"},"links":{"cited_paper":"/paper/2207.03764","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:b83751aecf05baf8438667234334392e43d6867116002e66a3aa9256d0eae292","observation_id":"37f22124-4c0e-4d19-ab2c-9a9403949ada","resolution":{"observed_at":"2026-08-14T04:21:21.212483Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.219819Z","title":"Agneset al.(DarkSide-50), Search for low-mass dark matter WIMPs with 12 ton-day exposure of DarkSide-50, Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.219819Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:c41421e150b444e029a8d9efe7f3c5488b692fabf1f7008d2474e9d3c19c9968","observation_id":"abaa5e0b-1533-4c65-b58d-06bdc8afc7c7","resolution":{"observed_at":"2026-08-14T04:21:21.219819Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.14729","last_updated":"2023-08-05T21:12:39Z","snapshot_observed_at":"2026-08-18T16:51:35.350753Z","submitted_at":"2023-03-26T14:13:02Z","title":"First Dark Matter Search with Nuclear Recoils from the XENONnT Experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.14729","snapshot_observed_at":"2026-08-14T04:21:21.225454Z","title":"Aprileet al.(XENON), First Dark Matter Search with Nuclear Recoils from the XENONnT Experiment, Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.225454Z"},"links":{"cited_paper":"/paper/2303.14729","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:44a4cc1557c7ec3c8956544ffa1d9f606ab30cfcc9656f98c0751fb6c08f738b","observation_id":"67d412f8-1fe0-41e4-beba-08a3efee086a","resolution":{"observed_at":"2026-08-14T04:21:21.225454Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.00664","last_updated":"2025-02-07T18:23:08Z","snapshot_observed_at":"2026-08-19T21:01:38.991439Z","submitted_at":"2024-08-01T15:59:50Z","title":"Dark Matter Search Results from 1.54 Tonne$\\cdot$Year Exposure of PandaX-4T","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.00664","snapshot_observed_at":"2026-08-14T04:21:21.230297Z","title":"Boet al.(PandaX), Dark Matter Search Results from 1.54 Tonne·Year Exposure of PandaX-4T, Phys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.230297Z"},"links":{"cited_paper":"/paper/2408.00664","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:6041291fd22dbad2de607de626280f5945b0d15e506c32c13313b2a33b30b65b","observation_id":"63faa001-cb39-4cc7-826b-ce88fc56c47b","resolution":{"observed_at":"2026-08-14T04:21:21.230297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.235808Z","title":"Agneseet al.(SuperCDMS), Projected Sensitivity of the SuperCDMS SNOLAB experiment, Phys","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.235808Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:bd253115bf9d33f327dc40e563e58f738b6634f99737159de6cc596815e649a1","observation_id":"d37e5576-8226-4257-b170-89e48c1d9acd","resolution":{"observed_at":"2026-08-14T04:21:21.235808Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.240231Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.240231Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:7e82638044fbed4037896bc3e91a6a888ab90b610a7e11049ac917ba5ef40efe","observation_id":"c79e5117-01d9-48e1-b1d4-e26afe526034","resolution":{"observed_at":"2026-08-14T04:21:21.240231Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.244390Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.244390Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:138bfea3d1d30f31fb9fe068212698a95850c8f3238f48cc17ec67badc659f34","observation_id":"e7701136-6ed7-4764-9f33-2ba5a0109484","resolution":{"observed_at":"2026-08-14T04:21:21.244390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.248931Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.248931Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:701471ef4c1700e3db069f46cb3331788b42de3241d2be96641c303251f4c8d4","observation_id":"6aa9be0c-8938-45c5-9d10-e9ec3b181f50","resolution":{"observed_at":"2026-08-14T04:21:21.248931Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.253554Z","title":"13: Projected significance for rejecting the elastic standard SD (O s","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.253554Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:71055f0b17559e40bff2fd4ce40236d7751d196d968691bc177b0e90827bfc9f","observation_id":"94fd9cb1-55aa-45df-be5f-1cee7814dcb2","resolution":{"observed_at":"2026-08-14T04:21:21.253554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.262781Z","title":"The left (right) panel corresponds tom χ = 5 GeV/c 2 (500 GeV/c 2)","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.262781Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:53315eab44da3c58bfeb4121140fc121af64513b0c2022c0fd4d99bb45f41eb0","observation_id":"b2adb7a9-4b65-4d49-87eb-af71cc08d340","resolution":{"observed_at":"2026-08-14T04:21:21.262781Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.268180Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.268180Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:f597822cc91b6f301c9a28863d511ab2caf6b859523cfd8918b33a067c98d110","observation_id":"bd98ff93-d23b-46f0-abd7-e67f713bbb50","resolution":{"observed_at":"2026-08-14T04:21:21.268180Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.272484Z","title":"14: Projected significance for rejecting the inelastic standard SD (O s","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.272484Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:dcc2a4308f2dc83812170fd322bedabfde300f997ee1187210a5f647e16bb291","observation_id":"6b6f259a-06e5-4ba3-b317-19753d4bec2e","resolution":{"observed_at":"2026-08-14T04:21:21.272484Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.277019Z","title":"Thep-value and corresponding significance (in units ofσ) are shown assuming a DM signal generated by non-standard NREFT operators (O s 6,O s 7,O s 9,O s 10,O s 13, andO s","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.277019Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:af72e85de98ff2c41dbf3d36ec24019c1d75f5577f95216a8f48f22a88edffb3","observation_id":"eb777c05-8786-47dd-aac3-9d178368889c","resolution":{"observed_at":"2026-08-14T04:21:21.277019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.281009Z","title":"The left (right) panel corresponds toδ m = 50 keV (100 keV)","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.281009Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:209b9733c0606955a9830bd7777c2aef30b13f71d65b8a98007c90902c1dac60","observation_id":"2a06f5d0-f9ac-4439-83dc-ac1c91e9257d","resolution":{"observed_at":"2026-08-14T04:21:21.281009Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.286508Z","title":"Contours corresponding to 1σ–5σsignificance are shown as a function of DM mass and exposure for the low-resolution (LR,σ x = 15 nm) scenario","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.286508Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:02684ec469834680485f9474b3bd9f0e100c1f65b3b507e6a5a6c3e89726af0a","observation_id":"abbb0469-7cb9-47a7-992a-5d1f0f8df740","resolution":{"observed_at":"2026-08-14T04:21:21.286508Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.293090Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.293090Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:da6a25eeb53162e44015e904b7c5e3818626b0bc9ce03a4480d46309f87e8aee","observation_id":"89832fde-3175-4018-b952-708c529942fe","resolution":{"observed_at":"2026-08-14T04:21:21.293090Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.00006","last_updated":"2016-09-30T12:30:49Z","snapshot_observed_at":"2026-08-20T15:19:16.353403Z","submitted_at":"2016-09-30T12:30:49Z","title":"Projected Sensitivity of the SuperCDMS SNOLAB experiment","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.00006","snapshot_observed_at":"2026-08-14T04:21:21.297450Z","title":"Contours corresponding to 1σ–5σsignificance are shown as a function of DM mass and exposure for the low-resolution (LR,σ x = 15 nm) scenario","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.297450Z"},"links":{"cited_paper":"/paper/1610.00006","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:ef01f80454d5815cc53bcda0f2774e28a494775b619a9fa03fae2fac3eedb3bc","observation_id":"b524cdad-e346-4ecf-ba83-0c9854658fea","resolution":{"observed_at":"2026-08-14T04:21:21.297450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.08145","last_updated":"2017-07-25T18:31:41Z","snapshot_observed_at":"2026-08-15T13:52:27.411900Z","submitted_at":"2017-07-25T18:31:41Z","title":"DarkSide-20k: A 20 Tonne Two-Phase LAr TPC for Direct Dark Matter Detection at LNGS","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.08145","snapshot_observed_at":"2026-08-14T04:21:21.302208Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.302208Z"},"links":{"cited_paper":"/paper/1707.08145","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:11c460f55a62130cf0c1bf5a9ee9cccf6a94389b2437d4e75aef90ec21b804e1","observation_id":"2393b4c0-f8fb-4547-a7e0-abbf6b9ff257","resolution":{"observed_at":"2026-08-14T04:21:21.302208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.306820Z","title":"Aalberset al.(XLZD), The XLZD Design Book: Towards the Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics (2024), arXiv:2410.17137 [hep-ex]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.306820Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:d977ebcb9df6d261eb71d66e430c98323e7a2789efc5a1033799c6865eaff9a7","observation_id":"ae3feb9f-be2c-4045-addb-0d08725f38f7","resolution":{"observed_at":"2026-08-14T04:21:21.306820Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.07118","last_updated":"2023-05-16T17:53:43Z","snapshot_observed_at":"2026-08-16T16:01:52.020845Z","submitted_at":"2023-01-17T19:00:02Z","title":"Mineral Detection of Neutrinos and Dark Matter. A Whitepaper","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.07118","snapshot_observed_at":"2026-08-14T04:21:21.311083Z","title":"Baumet al., Mineral detection of neutrinos and dark matter","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.311083Z"},"links":{"cited_paper":"/paper/2301.07118","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:8cdec3a56dea45f2b4f6746db99cbf4ebacedf1355c67994b187979f2df6a272","observation_id":"cbe3327e-e1e6-4caf-b657-a07d42d8f335","resolution":{"observed_at":"2026-08-14T04:21:21.311083Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.01626","last_updated":"2024-05-02T18:00:00Z","snapshot_observed_at":"2026-08-21T15:27:18.439238Z","submitted_at":"2024-05-02T18:00:00Z","title":"Mineral Detection of Neutrinos and Dark Matter 2024. Proceedings","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.01626","snapshot_observed_at":"2026-08-14T04:21:21.315837Z","title":"Baumet al., Mineral Detection of Neutrinos and Dark Matter 2024","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.315837Z"},"links":{"cited_paper":"/paper/2405.01626","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:4b1cc0671163840f13365160ff8f7c22a23c2ee98e25df49d324a0902bb9f361","observation_id":"64e58a25-80d5-43b2-8280-e310a28164eb","resolution":{"observed_at":"2026-08-14T04:21:21.315837Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.20482","last_updated":"2025-08-28T06:59:44Z","snapshot_observed_at":"2026-08-18T00:56:43.503575Z","submitted_at":"2025-08-28T06:59:44Z","title":"Mineral Detection of Neutrinos and Dark Matter 2025 Proceedings","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.20482","snapshot_observed_at":"2026-08-14T04:21:21.320179Z","title":"Hiroseet al., Mineral Detection of Neutrinos and Dark Matter 2025 Proceedings (2025), arXiv:2508.20482 [physics.ins- det]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.320179Z"},"links":{"cited_paper":"/paper/2508.20482","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:2a928c5574ccd47e3abf2dc11681ef416465af7189025180252dbb7a821f7839","observation_id":"4c11695c-e85a-4939-9fc9-cb67210f0397","resolution":{"observed_at":"2026-08-14T04:21:21.320179Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.324589Z","title":null,"venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.324589Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:ae0d56e6ec0086232a88838c677a9da739d94ca52bc69b2ce347ab5bbf5fc4c9","observation_id":"d1e6a335-3573-46e0-bb2f-951ef737d479","resolution":{"observed_at":"2026-08-14T04:21:21.324589Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/9511055","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.001101Z","title":null,"venue":null,"work_id":"3d477cc7-9ec0-4b87-83f1-deb77892d519","year":1996},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.328766Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:21303bf26389ad52d660c03aa9b5269275dee1e554e0d8091c9546b7d6539560","observation_id":"39caa262-f2e7-4cef-b542-1b1e95472dc9","resolution":{"observed_at":"2026-08-14T04:21:23.010329Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.332916Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.332916Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:425da689bb77eb19a6de2925de957b918cc3bfc9163d88a340443f375a39ad8c","observation_id":"7d455b80-7766-4b63-a5eb-d548abeb01a0","resolution":{"observed_at":"2026-08-14T04:21:21.332916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.05991","last_updated":"2020-02-26T22:08:41Z","snapshot_observed_at":"2026-08-20T17:37:22.218740Z","submitted_at":"2018-06-15T14:08:46Z","title":"Searching for Dark Matter with Paleo-Detectors","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.05991","snapshot_observed_at":"2026-08-14T04:21:21.337328Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.337328Z"},"links":{"cited_paper":"/paper/1806.05991","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:f94dc1123b6fbc96c3a06f3c6b54bcd76865a9987fedae8f44c3d6d9184e355d","observation_id":"77b3179c-299d-41d7-a18e-ace255067136","resolution":{"observed_at":"2026-08-14T04:21:21.337328Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.06844","last_updated":"2019-02-27T08:45:56Z","snapshot_observed_at":"2026-08-14T17:57:47.432700Z","submitted_at":"2018-11-16T15:12:20Z","title":"Paleo-detectors: Searching for Dark Matter with Ancient Minerals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.06844","snapshot_observed_at":"2026-08-14T04:21:21.341734Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.341734Z"},"links":{"cited_paper":"/paper/1811.06844","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:4362f4634e907ee89f0f5c6acfff8d65c9976af84bf4e6f10c3a433b20ff1003","observation_id":"8b403f64-f6c1-4215-b427-30ed9c302679","resolution":{"observed_at":"2026-08-14T04:21:21.341734Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.10549","last_updated":"2019-03-26T16:38:13Z","snapshot_observed_at":"2026-08-19T21:36:24.632942Z","submitted_at":"2018-11-26T17:52:46Z","title":"Digging for Dark Matter: Spectral Analysis and Discovery Potential of Paleo-Detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.10549","snapshot_observed_at":"2026-08-14T04:21:21.346471Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.346471Z"},"links":{"cited_paper":"/paper/1811.10549","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:8cc6d9bfbaec89fa4e430dc754b29f0ce7ac6f495efa1e77c4e987819b0fe37a","observation_id":"6033bb2a-5166-4a30-997b-88d65a259a4f","resolution":{"observed_at":"2026-08-14T04:21:21.346471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.10025","last_updated":"2019-10-07T17:37:33Z","snapshot_observed_at":"2026-08-21T15:27:35.421019Z","submitted_at":"2019-05-24T04:24:54Z","title":"A counter-top search for macroscopic dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.10025","snapshot_observed_at":"2026-08-14T04:21:21.351153Z","title":"Singh Sidhu, G","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.351153Z"},"links":{"cited_paper":"/paper/1905.10025","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:5beb54c995816bb61d2d9010c55651bbd19af4bc9d7b58de52f66a10fe88f74a","observation_id":"7c5b0a56-9e21-410a-9e6f-a7d3570df1f1","resolution":{"observed_at":"2026-08-14T04:21:21.351153Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.03998","last_updated":"2021-07-30T16:49:19Z","snapshot_observed_at":"2026-08-21T15:27:07.717566Z","submitted_at":"2021-05-09T19:12:39Z","title":"Ultra-Heavy Dark Matter Search with Electron Microscopy of Geological Quartz","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.03998","snapshot_observed_at":"2026-08-14T04:21:21.355549Z","title":"Ebadiet al., Ultraheavy dark matter search with electron microscopy of geological quartz, Phys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.355549Z"},"links":{"cited_paper":"/paper/2105.03998","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:fb3273cce5f21879d715a4548e2bca2b9c96930e5ed6e15d6d9138777d4ba9d2","observation_id":"e6e397eb-e459-4821-9abf-76a6809979b1","resolution":{"observed_at":"2026-08-14T04:21:21.355549Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.06473","last_updated":"2023-08-31T14:33:22Z","snapshot_observed_at":"2026-08-21T15:27:22.747527Z","submitted_at":"2021-05-13T18:00:00Z","title":"Old Rocks, New Limits: Excavated Ancient Mica Searches For Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.06473","snapshot_observed_at":"2026-08-14T04:21:21.360384Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.360384Z"},"links":{"cited_paper":"/paper/2105.06473","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:698882bc674a666088394f54e23f04339d97e856e2b959fb4a89e7b05fac55d0","observation_id":"2836a2f6-df27-4264-9216-63728f96dc6e","resolution":{"observed_at":"2026-08-14T04:21:21.360384Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.06559","last_updated":"2021-06-11T18:09:23Z","snapshot_observed_at":"2026-08-16T18:17:43.604520Z","submitted_at":"2021-06-11T18:09:23Z","title":"New Projections for Dark Matter Searches with Paleo-Detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.06559","snapshot_observed_at":"2026-08-14T04:21:21.365154Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.365154Z"},"links":{"cited_paper":"/paper/2106.06559","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:dca80be74470009183a9194e371bf77474b9fe17e33e1e381422400325b6a533","observation_id":"4782c502-9dad-492d-ad98-ee38694bf1d1","resolution":{"observed_at":"2026-08-14T04:21:21.365154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.08885","last_updated":"2025-04-11T18:00:01Z","snapshot_observed_at":"2026-08-16T12:41:56.295955Z","submitted_at":"2025-04-11T18:00:01Z","title":"Refining the sensitivity of new physics searches with ancient minerals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.08885","snapshot_observed_at":"2026-08-14T04:21:21.369519Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.369519Z"},"links":{"cited_paper":"/paper/2504.08885","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:8ce8b484ce6a0c602194e53d8899f1b51f5f67e4d0c6d48ae84eee0d32dd4b4a","observation_id":"b67ec6a4-0621-4aae-95e7-c998dc98215e","resolution":{"observed_at":"2026-08-14T04:21:21.369519Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.376051Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.376051Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:cc5bd53a675a29239a4604ed5d5122e9c85b403cb4d2e6a9ada160351512fb9e","observation_id":"73d522de-1813-41cc-aeab-f0c537bfa868","resolution":{"observed_at":"2026-08-14T04:21:21.376051Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.1591","last_updated":"2010-12-10T02:53:36Z","snapshot_observed_at":"2026-08-15T05:11:50.268835Z","submitted_at":"2010-08-09T20:20:05Z","title":"Non-relativistic effective theory of dark matter direct detection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.1591","snapshot_observed_at":"2026-08-14T04:21:21.380613Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.380613Z"},"links":{"cited_paper":"/paper/1008.1591","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:a6e6e201941d41881133106f46a26f86bddbd8c3817650369bdbf5f4f075f3be","observation_id":"e8558e76-fd10-4996-87b7-f904b41353fb","resolution":{"observed_at":"2026-08-14T04:21:21.380613Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.3542","last_updated":"2012-08-28T17:39:55Z","snapshot_observed_at":"2026-08-15T04:15:56.929365Z","submitted_at":"2012-03-15T20:00:03Z","title":"The Effective Field Theory of Dark Matter Direct Detection","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.3542","snapshot_observed_at":"2026-08-14T04:21:21.385850Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.385850Z"},"links":{"cited_paper":"/paper/1203.3542","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:9a76529e7f7e3fa3a5e6d6ebf763271c2a0e105403e34908e16f51c314c6c931","observation_id":"9dbd05eb-1a9d-44fa-8356-8ba5d14a7036","resolution":{"observed_at":"2026-08-14T04:21:21.385850Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.02614","last_updated":"2017-05-07T12:59:26Z","snapshot_observed_at":"2026-08-21T15:27:10.855653Z","submitted_at":"2017-05-07T12:59:26Z","title":"Effective field theory search for high-energy nuclear recoils using the XENON100 dark matter detector","version":1},"cited_work":{"arxiv_id":"1705.02614","doi":null,"metadata_source":"pith","pith_arxiv_id":"1705.02614","snapshot_observed_at":"2026-08-14T04:21:22.581402Z","title":"Effective field theory search for high-energy nuclear recoils using the XENON100 dark matter detector","venue":"astro-ph.CO","work_id":"bac858bb-bc82-4ff6-9adc-0c303bdc1cd4","year":2017},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.390581Z"},"links":{"cited_paper":"/paper/1705.02614","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:4c4ebad958d66a4dffbffef1bd66924509da1d73afa46b5f3523e73ea5ba2630","observation_id":"03baaaa2-d5c6-4052-aaa0-3a05aa01d81c","resolution":{"observed_at":"2026-08-14T04:21:22.587131Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1807.01936","last_updated":"2019-04-01T02:51:02Z","snapshot_observed_at":"2026-08-21T15:27:20.339164Z","submitted_at":"2018-07-05T10:35:14Z","title":"PandaX-II Constraints on Spin-Dependent WIMP-Nucleon Effective Interactions","version":2},"cited_work":{"arxiv_id":"1807.01936","doi":null,"metadata_source":"pith","pith_arxiv_id":"1807.01936","snapshot_observed_at":"2026-08-14T04:21:22.552693Z","title":"PandaX-II Constraints on Spin-Dependent WIMP-Nucleon Effective Interactions","venue":"hep-ex","work_id":"8b3216e2-9300-4a86-9a03-b970a150784e","year":2018},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.395244Z"},"links":{"cited_paper":"/paper/1807.01936","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:218c1f71b41a2aafd4ecbca6caae036ad591d7d08b4f2163d95a71168e43c197","observation_id":"ecdb22fe-5172-415b-a661-8c518ee3182c","resolution":{"observed_at":"2026-08-14T04:21:22.559042Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.11683","last_updated":"2022-05-24T00:41:39Z","snapshot_observed_at":"2026-08-21T15:27:21.852802Z","submitted_at":"2022-05-24T00:41:39Z","title":"Effective Field Theory Analysis of CDMSlite Run 2 Data","version":1},"cited_work":{"arxiv_id":"2205.11683","doi":null,"metadata_source":"pith","pith_arxiv_id":"2205.11683","snapshot_observed_at":"2026-08-14T04:21:22.532987Z","title":"Effective Field Theory Analysis of CDMSlite Run 2 Data","venue":"astro-ph.CO","work_id":"5b96002d-6759-4776-b229-84503c14d903","year":2022},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.399996Z"},"links":{"cited_paper":"/paper/2205.11683","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:b688851ff9387a8c1dfeef54a98b265d37e4c72f4ffdec4c4ba982813d3c931c","observation_id":"00e384eb-cbb3-493e-9d9a-83c6f04fa559","resolution":{"observed_at":"2026-08-14T04:21:22.537575Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.02030","last_updated":"2024-02-26T19:05:02Z","snapshot_observed_at":"2026-08-16T14:37:48.346526Z","submitted_at":"2023-12-04T16:51:25Z","title":"First Constraints on WIMP-Nucleon Effective Field Theory Couplings in an Extended Energy Region From LUX-ZEPLIN","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.02030","snapshot_observed_at":"2026-08-14T04:21:21.404556Z","title":"Aalberset al.(LZ), First constraints on WIMP-nucleon effective field theory couplings in an extended energy region from LUX-ZEPLIN, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.404556Z"},"links":{"cited_paper":"/paper/2312.02030","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:5ed1921ef6130caefb16f2d32cf989eae66f244b1cb5e38347597017482f5d92","observation_id":"4e1ebb63-40c5-4071-98ed-2516cc554a6f","resolution":{"observed_at":"2026-08-14T04:21:21.404556Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0703217","last_updated":"2007-08-07T21:15:16Z","snapshot_observed_at":"2026-08-15T10:44:21.793466Z","submitted_at":"2007-03-20T13:52:03Z","title":"Determining the WIMP mass using direct detection experiments","version":2},"cited_work":{"arxiv_id":"hep-ph/0703217","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0703217","snapshot_observed_at":"2026-08-14T04:21:22.475794Z","title":"Determining the WIMP mass using direct detection experiments","venue":"hep-ph","work_id":"7b65f07c-c394-4afc-8bd3-f34ec3a8bd38","year":2007},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.409139Z"},"links":{"cited_paper":"/paper/hep-ph/0703217","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:a1c5ee89f112da7634ac47c1d4f26e0154e2eb6afbb29aae799e9e6f104dab67","observation_id":"348d375d-0367-47f0-bc1a-7013b77c2731","resolution":{"observed_at":"2026-08-14T04:21:22.481616Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0805.1704","last_updated":"2008-06-04T17:55:32Z","snapshot_observed_at":"2026-08-20T01:19:06.877619Z","submitted_at":"2008-05-12T18:11:13Z","title":"Determining the WIMP mass from a single direct detection experiment, a more detailed study","version":2},"cited_work":{"arxiv_id":"0805.1704","doi":null,"metadata_source":"pith","pith_arxiv_id":"0805.1704","snapshot_observed_at":"2026-08-14T04:21:22.449469Z","title":"Determining the WIMP mass from a single direct detection experiment, a more detailed study","venue":"hep-ph","work_id":"a03e8f55-5921-468a-8b3d-1640df830666","year":2008},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.413864Z"},"links":{"cited_paper":"/paper/0805.1704","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:cad154087d16f2f2c1d8dd01159e289e1d09bd89387af33abc3bb679e0ab5f64","observation_id":"53e6a169-6747-48d7-a90f-e45fc1bcc0fa","resolution":{"observed_at":"2026-08-14T04:21:22.454657Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.04117","last_updated":"2018-11-13T15:57:24Z","snapshot_observed_at":"2026-08-16T01:48:48.552128Z","submitted_at":"2018-05-10T18:00:12Z","title":"Dark Matter Model or Mass, but Not Both: Assessing Near-Future Direct Searches with Benchmark-free Forecasting","version":2},"cited_work":{"arxiv_id":"1805.04117","doi":null,"metadata_source":"pith","pith_arxiv_id":"1805.04117","snapshot_observed_at":"2026-08-14T04:21:22.428827Z","title":"Dark Matter Model or Mass, but Not Both: Assessing Near-Future Direct Searches with Benchmark-free Forecasting","venue":"hep-ph","work_id":"6f0b6761-09d7-4bec-bdd3-e770d2e00d66","year":2018},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.418407Z"},"links":{"cited_paper":"/paper/1805.04117","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:30f55a42be28de738db96e23951f38c4c6ec3300b473eb161d9514f53f4d8a78","observation_id":"d6176212-6253-43bb-92f7-403bf685727b","resolution":{"observed_at":"2026-08-14T04:21:22.433964Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1810.05576","last_updated":"2018-10-18T16:05:18Z","snapshot_observed_at":"2026-08-14T18:15:34.985040Z","submitted_at":"2018-10-12T15:25:07Z","title":"Opening the energy window on direct dark matter detection","version":2},"cited_work":{"arxiv_id":"1810.05576","doi":null,"metadata_source":"pith","pith_arxiv_id":"1810.05576","snapshot_observed_at":"2026-08-14T04:21:22.408760Z","title":"Opening the energy window on direct dark matter detection","venue":"hep-ph","work_id":"d150c59e-1149-4259-81de-e3b8ba1f0a6b","year":2018},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.423260Z"},"links":{"cited_paper":"/paper/1810.05576","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:0d96a1bca12161b75cc00b3d3717ffd43b308bd62f9bffe8f5d471bb093c656a","observation_id":"2440a13e-6031-497a-9157-95174ea07d88","resolution":{"observed_at":"2026-08-14T04:21:22.413796Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1505.07406","last_updated":"2015-05-27T17:22:48Z","snapshot_observed_at":"2026-08-21T15:27:18.644121Z","submitted_at":"2015-05-27T17:22:48Z","title":"New directional signatures from the non-relativistic effective field theory of dark matter","version":1},"cited_work":{"arxiv_id":"1505.07406","doi":null,"metadata_source":"pith","pith_arxiv_id":"1505.07406","snapshot_observed_at":"2026-08-14T04:21:22.387438Z","title":"New directional signatures from the non-relativistic effective field theory of dark matter","venue":"hep-ph","work_id":"c1d137e0-7ebd-49cc-987b-324589dc569e","year":2015},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.428468Z"},"links":{"cited_paper":"/paper/1505.07406","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:8f94a6554d8eaedb684b681cd79447c9dfc7c9e6f8e43deae2784a094631cf6c","observation_id":"9be1cf62-8046-4289-83ed-514e4bc72a54","resolution":{"observed_at":"2026-08-14T04:21:22.392393Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1802.04294","last_updated":"2018-05-31T17:27:14Z","snapshot_observed_at":"2026-08-21T15:27:18.791892Z","submitted_at":"2018-02-12T19:00:28Z","title":"Discriminating WIMP-nucleus response functions in present and future XENON-like direct detection experiments","version":2},"cited_work":{"arxiv_id":"1802.04294","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.04294","snapshot_observed_at":"2026-08-14T04:21:22.364178Z","title":"Discriminating WIMP-nucleus response functions in present and future XENON-like direct detection experiments","venue":"hep-ph","work_id":"fb691bee-b5da-431e-a117-1f094e9be54f","year":2018},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.433579Z"},"links":{"cited_paper":"/paper/1802.04294","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:ac2501ddaa328bf408c8bcf287914d3f19f9824c993daea1baa556215e70cdf5","observation_id":"310104fb-80fb-404b-9de4-746be6b2f92a","resolution":{"observed_at":"2026-08-14T04:21:22.369853Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1308.6288","last_updated":"2013-08-28T20:00:08Z","snapshot_observed_at":"2026-08-15T00:05:08.250977Z","submitted_at":"2013-08-28T20:00:08Z","title":"Model-independent WIMP Scattering Responses and Event Rates: A Mathematica Package for Experimental Analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1308.6288","snapshot_observed_at":"2026-08-14T04:21:21.438148Z","title":"Anand, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.438148Z"},"links":{"cited_paper":"/paper/1308.6288","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:37a2010fab97c0794304b4d8eb0f8cc990ff05c23c4171da33a1506d44497334","observation_id":"f492476b-b363-4074-95da-18bb00fd98b6","resolution":{"observed_at":"2026-08-14T04:21:21.438148Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.04210","last_updated":"2022-03-08T17:19:41Z","snapshot_observed_at":"2026-08-16T17:16:06.251374Z","submitted_at":"2022-03-08T17:19:41Z","title":"Complementarity of experiments in probing the non-relativistic effective theory of dark matter-nucleon interactions","version":1},"cited_work":{"arxiv_id":"2203.04210","doi":null,"metadata_source":"pith","pith_arxiv_id":"2203.04210","snapshot_observed_at":"2026-08-14T04:21:22.329553Z","title":"Complementarity of experiments in probing the non-relativistic effective theory of dark matter-nucleon interactions","venue":"hep-ph","work_id":"cd2381ae-e102-4b5d-8798-d255b80fe418","year":2022},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.442544Z"},"links":{"cited_paper":"/paper/2203.04210","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:7151b5e9983fa14cb6113750b1127a15f692ffcae26e7f9626d5337ea67e606d","observation_id":"36eb6d21-b088-4fb1-a603-8ae43e23a88f","resolution":{"observed_at":"2026-08-14T04:21:22.334651Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0101138","last_updated":"2001-01-15T22:40:04Z","snapshot_observed_at":"2026-08-18T00:20:14.998209Z","submitted_at":"2001-01-15T22:40:04Z","title":"Inelastic Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0101138","snapshot_observed_at":"2026-08-14T04:21:21.447195Z","title":"Tucker-Smith and N","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.447195Z"},"links":{"cited_paper":"/paper/hep-ph/0101138","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:074ba2d4ec39e5d638d6e1b923da228ac084719bbb184bb71556159c87b77d5a","observation_id":"172ba20b-7b5b-4560-bce9-4d541c9a6aa3","resolution":{"observed_at":"2026-08-14T04:21:21.447195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.0536","last_updated":"2014-09-01T20:00:20Z","snapshot_observed_at":"2026-08-14T23:21:10.630838Z","submitted_at":"2014-09-01T20:00:20Z","title":"A Model Independent Approach to Inelastic Dark Matter Scattering","version":1},"cited_work":{"arxiv_id":"1409.0536","doi":null,"metadata_source":"pith","pith_arxiv_id":"1409.0536","snapshot_observed_at":"2026-08-14T04:21:22.289587Z","title":"A Model Independent Approach to Inelastic Dark Matter Scattering","venue":"hep-ph","work_id":"42aabf61-46aa-4ebd-a357-a57d63e69316","year":2014},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.452105Z"},"links":{"cited_paper":"/paper/1409.0536","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:d6e0990457ebee763ff17ea70803e02894cb498a9c0cfd572f97babbb9875ac9","observation_id":"3dc77252-9e5c-4a7b-9664-b7ea3fd8a49c","resolution":{"observed_at":"2026-08-14T04:21:22.295447Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2605.13659","last_updated":"2026-05-13T15:17:54Z","snapshot_observed_at":"2026-08-02T08:51:23.593118Z","submitted_at":"2026-05-13T15:17:54Z","title":"Calorimetric approach to paleo-detection of dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2605.13659","snapshot_observed_at":"2026-08-14T04:21:21.456856Z","title":"Hedges and P","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.456856Z"},"links":{"cited_paper":"/paper/2605.13659","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:f338cffb99df9d1d136301cb09a3b5c7512d6377797f03f202081faa4eedf7d5","observation_id":"87955965-5b3f-49c4-a58a-7d6351579404","resolution":{"observed_at":"2026-08-14T04:21:21.456856Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.00599","last_updated":"2025-06-18T21:09:46Z","snapshot_observed_at":"2026-08-16T18:27:31.825368Z","submitted_at":"2021-05-03T02:06:25Z","title":"Recommended conventions for reporting results from direct dark matter searches","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.00599","snapshot_observed_at":"2026-08-14T04:21:21.461678Z","title":"Baxteret al., Recommended conventions for reporting results from direct dark matter searches, Eur","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.461678Z"},"links":{"cited_paper":"/paper/2105.00599","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:1a3eeaa6dacd86a3c05fda3b692b968655b75152a76ea0c8c1e5aeb0d196d578","observation_id":"bbc8bb9d-03d6-4e51-901e-6e2b4ad7684c","resolution":{"observed_at":"2026-08-14T04:21:21.461678Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.1938","last_updated":"2014-06-13T10:16:53Z","snapshot_observed_at":"2026-08-14T23:38:20.914826Z","submitted_at":"2014-04-07T20:13:34Z","title":"The Local Dark Matter Density","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.1938","snapshot_observed_at":"2026-08-14T04:21:21.467118Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.467118Z"},"links":{"cited_paper":"/paper/1404.1938","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:4dd860eddd763c33598f1b53470210aedd857793f55fbd348f1a007c475ed145","observation_id":"205898ec-24e9-4f4c-83ae-ad489a23e8e5","resolution":{"observed_at":"2026-08-14T04:21:21.467118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.471958Z","title":"Sch¨ onrich, J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.471958Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:a58e6868a1cdfb1faece52918dc8df0b23b960e581d29ff3073e9948ac605644","observation_id":"c901845e-ac54-435d-8ec7-54772cb82358","resolution":{"observed_at":"2026-08-14T04:21:21.471958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.812230Z","title":"Sch¨ onrich, Galactic rotation and solar motion from stellar kinematics, Monthly Notices of the Royal Astronomical Society427, 274–287 (2012)","venue":null,"work_id":"e6ef033d-062b-4b17-8b0a-50122401dc66","year":2012},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.477343Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:76d92e6251a53de6da507e3b8fb9c682119c72b75972274054b0bc42f6d939c2","observation_id":"b2145e56-b3b5-4dce-8655-a08b572b0144","resolution":{"observed_at":"2026-08-14T04:21:23.816896Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.799222Z","title":"Bland-Hawthorn and O","venue":null,"work_id":"2cf7dfec-6267-4d87-8a66-08217df5383a","year":2016},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.482035Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:a514c1f52c6c976b8205a9c10535b70e4045dbe26e50095903b8deb086fb4f39","observation_id":"005af674-b931-4df5-a73c-e4c04ac49c85","resolution":{"observed_at":"2026-08-14T04:21:23.803300Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.779813Z","title":"Abuteret al., Improved gravity astrometric accuracy from modeling optical aberrations, Astron.; Astrophys.647, A59 (2021)","venue":null,"work_id":"8d6e6f25-be17-4f26-85b2-9972e9fbbcf4","year":2021},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.486391Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:c570cafb4d0d7b86586b31470b143423ac28dffe54e6a4bd8b94326d6c4dfbbd","observation_id":"527e10fd-8bb4-4e86-bbd4-7782dfd1040f","resolution":{"observed_at":"2026-08-14T04:21:23.786589Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.764941Z","title":null,"venue":null,"work_id":"44c03a64-ba24-4d36-9e7e-1c850bf79c38","year":2007},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.491412Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:ebfbb25430846284dfb86143354178285b03a932eeb52962a355688f776279c7","observation_id":"5868720e-b387-4564-84c3-b0418cbe6ea7","resolution":{"observed_at":"2026-08-14T04:21:23.770257Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2106.06207","last_updated":"2021-06-11T07:27:58Z","snapshot_observed_at":"2026-08-21T15:27:58.983571Z","submitted_at":"2021-06-11T07:27:58Z","title":"WimPyDD: an object-oriented Python code for the calculation of WIMP direct detection signals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.06207","snapshot_observed_at":"2026-08-14T04:21:21.495571Z","title":"Jeong, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.495571Z"},"links":{"cited_paper":"/paper/2106.06207","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:d242cd36627d1d84388339da5a5251966f256349bba91f0cd62e86e281bd9b03","observation_id":"51dc40e7-6c4e-4d36-9dae-3aadea21597f","resolution":{"observed_at":"2026-08-14T04:21:21.495571Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.09187","last_updated":"2022-09-21T16:54:09Z","snapshot_observed_at":"2026-08-21T15:27:21.482962Z","submitted_at":"2022-09-19T17:12:09Z","title":"dmscatter: A Fast Program for WIMP-Nucleus Scattering","version":2},"cited_work":{"arxiv_id":"2209.09187","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.09187","snapshot_observed_at":"2026-08-14T04:21:22.197754Z","title":"dmscatter: A Fast Program for WIMP-Nucleus Scattering","venue":"nucl-th","work_id":"aa0fb9a8-6a0c-48b9-9958-60af40d27413","year":2022},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.499956Z"},"links":{"cited_paper":"/paper/2209.09187","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:21242c9be30ff9b9e408db71773a206bae5ecdd807df711b347574aad8454ca7","observation_id":"2a1a335b-ec43-4ba5-bd8d-05b264b1fca3","resolution":{"observed_at":"2026-08-14T04:21:22.205244Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.750692Z","title":null,"venue":null,"work_id":"37bf3c54-c6a7-4a76-9251-9c72571803ae","year":2010},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.504742Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:b4999366f73c0b9fc0f956a9c8d35ce93939d7de94bcb6bdea9e8715ce8e4354","observation_id":"c362b497-f69d-4743-bfeb-fb43689f3f3f","resolution":{"observed_at":"2026-08-14T04:21:23.754920Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:21.509245Z","title":"Galelli, L","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.509245Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:120842c38c9e090f8327bfa77ac9474a1c0a4a364e96f66a380404c04266c7da","observation_id":"dc8ba9c8-6029-4356-991f-866e53ade021","resolution":{"observed_at":"2026-08-14T04:21:21.509245Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2604.09732","last_updated":"2026-04-09T16:05:30Z","snapshot_observed_at":"2026-08-14T07:08:30.891515Z","submitted_at":"2026-04-09T16:05:30Z","title":"Toward Neutrino and Dark Matter Detection with Ancient Minerals: TEM Study of Heavy-Ion Tracks in Olivine","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2604.09732","snapshot_observed_at":"2026-08-14T04:21:21.513523Z","title":"Calabrese-Day, E","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.513523Z"},"links":{"cited_paper":"/paper/2604.09732","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:8d9770da32a5b6d447420cac6803911199f0532816b2b67794db20521d4f73ad","observation_id":"3215e42c-a43b-4269-838a-1412e51bf454","resolution":{"observed_at":"2026-08-14T04:21:21.513523Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.736687Z","title":null,"venue":null,"work_id":"2b33458a-8936-481e-aaa0-eb755de7f0e5","year":2012},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.517972Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:ab71547a22389ac6505d55adb99e355ee97ae15cdd81ef2ea4fb673c7f1fd680","observation_id":"7b64fa66-1d00-419f-a706-00962dc99502","resolution":{"observed_at":"2026-08-14T04:21:23.741559Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.723810Z","title":"van Gastel, G","venue":null,"work_id":"8bcc8954-30a1-45b2-a65e-637b0d97485d","year":2012},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.522138Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:c23de31b3c0be46b419d2f9da70f1db4b29aeed2af73c99792314a271fb384bc","observation_id":"b4aef394-2d5e-404a-82b1-cf24d272ee59","resolution":{"observed_at":"2026-08-14T04:21:23.728162Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.697433Z","title":null,"venue":null,"work_id":"5b7dc2db-f8f1-4759-a434-a155d1a02250","year":2013},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.526508Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:a62227edce1a0c9ba6ad99c4e60f9c620de6b35f0217879e4fd357055b417a7f","observation_id":"88ef2c01-6a2a-4f6c-8038-866ab180332f","resolution":{"observed_at":"2026-08-14T04:21:23.706162Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.678377Z","title":null,"venue":null,"work_id":"205dbc39-3a48-4466-836f-cd690d7c72a3","year":2015},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.531242Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:d9554f40b4f02211c0d92073f7026f03f1afc2e3cd890e1595a66bbee2005ae4","observation_id":"7b387e71-5d9c-47dc-9f2d-92bbca036495","resolution":{"observed_at":"2026-08-14T04:21:23.683054Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.661550Z","title":null,"venue":null,"work_id":"b95b178c-6c2d-4cad-b20a-18dc5045bd13","year":2017},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.536414Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:9bb392a9951db6b44fd4a9c70355f538c74893431e11ab7839db369e01be9493","observation_id":"8ae93f54-ddee-48db-b5f9-76587d0835f4","resolution":{"observed_at":"2026-08-14T04:21:23.667961Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.646538Z","title":null,"venue":null,"work_id":"394e1cb3-2895-4d44-af6d-6c4051167cf8","year":2018},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.540831Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:b866e277397bd1a50db1e87bcec188615de2dc87a545f7c28ec722c1e8fd4a27","observation_id":"9b5cab20-2c62-4253-9eac-2711ddc64e85","resolution":{"observed_at":"2026-08-14T04:21:23.651554Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.631202Z","title":"Rodriguez, W","venue":null,"work_id":"52b08a44-0e0d-4f39-8112-a82f314e0690","year":2014},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.545947Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:f2e36043497f49eb655f2ad1d77eb3f496131a71de4c95b63bdaa592b7118dc3","observation_id":"d6872897-898e-4bd5-9b59-4b755de361f5","resolution":{"observed_at":"2026-08-14T04:21:23.635905Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.609921Z","title":"Schaff, M","venue":null,"work_id":"805f2d60-2cfe-472d-a2e5-42ce61677e6e","year":2015},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.550683Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:f4b380401a12ea53a9dc37e795c5c586e0c28f7a7c65abba6b6bf1f10969f7a5","observation_id":"c0c6f43f-8e61-4270-b096-5c3da435c361","resolution":{"observed_at":"2026-08-14T04:21:23.618171Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:23.566439Z","title":"Holler, A","venue":null,"work_id":"19b2f29d-67a5-48da-abc1-c1984fbd40f0","year":2014},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.555448Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:ebe0794966bf262d642598b1f8447b10e3953453e1c118c0b3865b597d0a3840","observation_id":"d761b960-a8a6-49ec-969d-42f72d78a0b3","resolution":{"observed_at":"2026-08-14T04:21:23.575778Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.05800","last_updated":"2020-05-13T17:46:32Z","snapshot_observed_at":"2026-08-14T16:16:01.710301Z","submitted_at":"2019-06-13T16:34:42Z","title":"Paleo-Detectors for Galactic Supernova Neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.05800","snapshot_observed_at":"2026-08-14T04:21:21.559896Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.559896Z"},"links":{"cited_paper":"/paper/1906.05800","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:5213465ec9ef0698568130cfc1d28fd56224c18b464b37283a7ec4b5706525ed","observation_id":"ed7cd28c-2340-40af-bdce-fcde432a703f","resolution":{"observed_at":"2026-08-14T04:21:21.559896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0512125","last_updated":"2005-12-06T19:09:53Z","snapshot_observed_at":"2026-07-07T00:56:37.931894Z","submitted_at":"2005-12-05T20:17:28Z","title":"Muon-Induced Background Study for Underground Laboratories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0512125","snapshot_observed_at":"2026-08-14T04:21:21.564819Z","title":"Mei and A","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.564819Z"},"links":{"cited_paper":"/paper/astro-ph/0512125","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:25660dd0d249bb7fb2c07da6af1711bd6be38485b50d81eab4d6a0e5d6751bc6","observation_id":"fe7edd66-e2da-4ab0-9505-519501c4508c","resolution":{"observed_at":"2026-08-14T04:21:21.564819Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.08394","last_updated":"2020-11-30T17:10:20Z","snapshot_observed_at":"2026-08-21T15:26:55.159618Z","submitted_at":"2020-04-17T18:00:01Z","title":"Measuring Changes in the Atmospheric Neutrino Rate Over Gigayear Timescales","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.08394","snapshot_observed_at":"2026-08-14T04:21:21.569813Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.569813Z"},"links":{"cited_paper":"/paper/2004.08394","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:44d7106d0faf67c5280aae771b2bd02f24dfb42f66d860b7ce19aaf197eb89e9","observation_id":"afb7dc67-cfa5-4a5c-8f64-826d3a6157b1","resolution":{"observed_at":"2026-08-14T04:21:21.569813Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.01755","last_updated":"2021-03-04T15:44:53Z","snapshot_observed_at":"2026-08-21T15:27:59.510582Z","submitted_at":"2021-02-02T21:09:31Z","title":"Measuring solar neutrinos over Gigayear timescales with Paleo Detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.01755","snapshot_observed_at":"2026-08-14T04:21:21.574394Z","title":"Tapia-Arellano and S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.574394Z"},"links":{"cited_paper":"/paper/2102.01755","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:80beb87fca214cbaca311a92355979288322f8a31f72d71465b185b15777aaf6","observation_id":"ac4686b1-221a-4010-8f84-e73fac290727","resolution":{"observed_at":"2026-08-14T04:21:21.574394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.07499","last_updated":"2020-09-25T14:16:13Z","snapshot_observed_at":"2026-08-19T21:05:54.436202Z","submitted_at":"2020-02-18T11:37:40Z","title":"Can we overcome the neutrino floor at high masses?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.07499","snapshot_observed_at":"2026-08-14T04:21:21.578814Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.578814Z"},"links":{"cited_paper":"/paper/2002.07499","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:f813914d71bafcaef92f7bbbfca336386cf3b32af708eb0139562a8ad243e42a","observation_id":"902652b8-dc12-4286-89f7-521f4efadf97","resolution":{"observed_at":"2026-08-14T04:21:21.578814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/0310859","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:21:22.020636Z","title":"Cappellaro, R","venue":null,"work_id":"7738b50f-57a4-4b83-829c-43d36cc46c1b","year":2005},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.583377Z"},"links":{"citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:70f98300bdf1ba7f067da315610600bc870c4f41b91cad18d7fc5910efb83fd8","observation_id":"acb7a604-400f-4b89-9b85-1d459b958b37","resolution":{"observed_at":"2026-08-14T04:21:22.029288Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0601015","last_updated":"2006-01-04T09:53:31Z","snapshot_observed_at":"2026-08-21T15:33:57.465582Z","submitted_at":"2006-01-01T17:11:40Z","title":"Radioactive 26Al and massive stars in the Galaxy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0601015","snapshot_observed_at":"2026-08-14T04:21:21.587471Z","title":"Diehlet al., Radioactive Al-26 and massive stars in the galaxy, Nature439, 45 (2006), arXiv:astro-ph/0601015","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors","version":1},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-08-14T04:21:21.587471Z"},"links":{"cited_paper":"/paper/astro-ph/0601015","citing_paper":"/paper/2608.10105"},"observation_digest":"sha256:141827d44f128603205e5b9621eef25896eb2e7bfb5f94336e92d92141dfe90c","observation_id":"501f7adc-3823-4d57-9b95-f5f83e352b3b","resolution":{"observed_at":"2026-08-14T04:21:21.587471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.10105","last_updated":"2026-08-10T18:13:57Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-18T06:36:20.533445Z","submitted_at":"2026-08-10T18:13:57Z","title":"Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":79,"verified_exact":14,"verified_fuzzy":7},"total_outbound_references":116},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 100 of 116 outbound references and 0 inbound Pith citation observations for arXiv:2608.10105."}