{"as_of":"2026-08-13T07:08:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c86c4f116bc160cfdacd4b50f985ad136cde41917d615e9e460a33092ad04ce8","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T19:28:33.571312Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-04T20:20:06.837609Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2006.13929","last_updated":"2020-12-07T14:36:09Z","snapshot_observed_at":"2026-08-04T02:05:00.665984Z","submitted_at":"2020-06-24T17:58:07Z","title":"New limits on dark photons from solar emission and keV scale dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.13929","snapshot_observed_at":"2026-08-11T19:28:33.571312Z","title":"New limits on dark photons from solar emission and keV scale dark matter,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06883","last_updated":"2024-12-09T19:00:00Z","snapshot_observed_at":"2026-08-12T15:35:25.027665Z","submitted_at":"2024-12-09T19:00:00Z","title":"Dark Astronomy with Dark Matter Detectors","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-11T19:28:33.571312Z"},"links":{"cited_paper":"/paper/2006.13929","citing_paper":"/paper/2412.06883"},"observation_digest":"sha256:6d08a3dc3df51b8b90bb7a9a2a23620dee0afeeef13584721ce53dcdd8009a42","observation_id":"5793afb4-2b62-4be5-b183-e5a6a0398407","resolution":{"observed_at":"2026-08-11T19:28:33.571312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.13929","last_updated":"2020-12-07T14:36:09Z","snapshot_observed_at":"2026-08-04T02:05:00.665984Z","submitted_at":"2020-06-24T17:58:07Z","title":"New limits on dark photons from solar emission and keV scale dark matter","version":2},"cited_work":{"arxiv_id":"2006.13929","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2006.13929","snapshot_observed_at":"2026-07-04T20:20:06.837609Z","title":"New limits on dark photons from solar emission and keV scale dark matter","venue":null,"work_id":"aaabc7b8-cb0f-4a4e-b651-50cc83dbc540","year":2020},"citing_paper":{"arxiv_id":"2507.12860","last_updated":"2026-05-14T07:13:43Z","snapshot_observed_at":"2026-08-13T07:04:45.852032Z","submitted_at":"2025-07-17T07:32:56Z","title":"Detecting dark matter using optically trapped Rydberg atom tweezer arrays","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-19T05:02:13.495465Z"},"links":{"cited_paper":"/paper/2006.13929","citing_paper":"/paper/2507.12860"},"observation_digest":"sha256:813cff0c0418d00926c5002974c1cf8e5a4c1d73eb4bf7be8a82b00851e5ce31","observation_id":"e07f9888-81fd-42c9-b939-166ce96918a8","resolution":{"observed_at":"2026-05-19T05:02:58.896407Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.13929","last_updated":"2020-12-07T14:36:09Z","snapshot_observed_at":"2026-08-04T02:05:00.665984Z","submitted_at":"2020-06-24T17:58:07Z","title":"New limits on dark photons from solar emission and keV scale dark matter","version":2},"cited_work":{"arxiv_id":"2006.13929","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2006.13929","snapshot_observed_at":"2026-07-04T20:20:06.837609Z","title":"New limits on dark photons from solar emission and keV scale dark matter","venue":null,"work_id":"aaabc7b8-cb0f-4a4e-b651-50cc83dbc540","year":2020},"citing_paper":{"arxiv_id":"2507.13432","last_updated":"2026-05-06T13:38:02Z","snapshot_observed_at":"2026-07-06T21:58:56.405149Z","submitted_at":"2025-07-17T18:00:00Z","title":"INTEGRAL, eROSITA and Voyager Constraints on Light Bosonic Dark Matter: ALPs, Dark Photons, Scalars, $B-L$ and $L_{i}-L_{j}$ Vectors","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-05-19T04:12:50.022588Z"},"links":{"cited_paper":"/paper/2006.13929","citing_paper":"/paper/2507.13432"},"observation_digest":"sha256:4636643bba2f60daeb039b1645bb33702ec9e069079e0850d4f51cde9f291aac","observation_id":"78a0c59b-8867-4408-8243-d68b439e6cd4","resolution":{"observed_at":"2026-05-19T04:12:59.481165Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.13929","last_updated":"2020-12-07T14:36:09Z","snapshot_observed_at":"2026-08-04T02:05:00.665984Z","submitted_at":"2020-06-24T17:58:07Z","title":"New limits on dark photons from solar emission and keV scale dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.13929","snapshot_observed_at":"2026-08-06T15:00:44.611899Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.17782","last_updated":"2025-08-15T22:20:57Z","snapshot_observed_at":"2026-08-13T05:10:01.402176Z","submitted_at":"2025-07-23T04:36:21Z","title":"SPLENDOR: a novel detector platform to search for light dark matter with narrow-gap semiconductors","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-06T15:00:44.611899Z"},"links":{"cited_paper":"/paper/2006.13929","citing_paper":"/paper/2507.17782"},"observation_digest":"sha256:9d46b3ce7651f41ebd211b057b4fd36937dbee97be864095c22a551a0cbacd20","observation_id":"20161003-ea9b-414e-9339-34850a60dde5","resolution":{"observed_at":"2026-08-06T15:00:44.611899Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.13929","last_updated":"2020-12-07T14:36:09Z","snapshot_observed_at":"2026-08-04T02:05:00.665984Z","submitted_at":"2020-06-24T17:58:07Z","title":"New limits on dark photons from solar emission and keV scale dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.13929","snapshot_observed_at":"2026-08-04T00:27:33.103265Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.01655","last_updated":"2026-05-25T08:29:50Z","snapshot_observed_at":"2026-08-06T16:46:47.451372Z","submitted_at":"2025-11-03T15:17:25Z","title":"Direct detection of solar chameleons with electron recoil data from XENONnT","version":2},"reference_index":253,"source":"pdf_text","source_observed_at":"2026-08-04T00:27:33.103265Z"},"links":{"cited_paper":"/paper/2006.13929","citing_paper":"/paper/2511.01655"},"observation_digest":"sha256:faa668e3f37733ad44799ac3d62f9da0a15db7e467deeef367a16013266cdfac","observation_id":"adcc795a-a12a-4d81-827c-b3691a2e3264","resolution":{"observed_at":"2026-08-04T00:27:33.103265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.13929","last_updated":"2020-12-07T14:36:09Z","snapshot_observed_at":"2026-08-04T02:05:00.665984Z","submitted_at":"2020-06-24T17:58:07Z","title":"New limits on dark photons from solar emission and keV scale dark matter","version":2},"cited_work":{"arxiv_id":"2006.13929","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2006.13929","snapshot_observed_at":"2026-07-04T20:20:06.837609Z","title":"New limits on dark photons from solar emission and keV scale dark matter","venue":null,"work_id":"aaabc7b8-cb0f-4a4e-b651-50cc83dbc540","year":2020},"citing_paper":{"arxiv_id":"2605.15820","last_updated":"2026-05-15T10:19:29Z","snapshot_observed_at":"2026-08-06T01:47:27.078451Z","submitted_at":"2026-05-15T10:19:29Z","title":"A Near-Cutoff Waveguide Haloscope for sub-meV Dark Matter","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-05-20T17:33:32.537587Z"},"links":{"cited_paper":"/paper/2006.13929","citing_paper":"/paper/2605.15820"},"observation_digest":"sha256:ea2b33ed89e6b2cd88c26c6c7a70a771d2c89615caaa468b9496b2a7ca10e424","observation_id":"57ac40c9-5761-40a4-86c2-80a6f8e4fdbf","resolution":{"observed_at":"2026-05-20T17:33:36.559550Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.13929","last_updated":"2020-12-07T14:36:09Z","snapshot_observed_at":"2026-08-04T02:05:00.665984Z","submitted_at":"2020-06-24T17:58:07Z","title":"New limits on dark photons from solar emission and keV scale dark matter","version":2},"cited_work":{"arxiv_id":"2006.13929","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2006.13929","snapshot_observed_at":"2026-07-04T20:20:06.837609Z","title":"New limits on dark photons from solar emission and keV scale dark matter","venue":null,"work_id":"aaabc7b8-cb0f-4a4e-b651-50cc83dbc540","year":2020},"citing_paper":{"arxiv_id":"2605.30416","last_updated":"2026-05-28T18:00:02Z","snapshot_observed_at":"2026-08-12T14:36:05.365379Z","submitted_at":"2026-05-28T18:00:02Z","title":"A Bandpass Axion Or: How I Learned To Stop Worrying About Stars And Love The Lab","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-06-29T06:21:11.178914Z"},"links":{"cited_paper":"/paper/2006.13929","citing_paper":"/paper/2605.30416"},"observation_digest":"sha256:0667d696cc11a91cc90349ea96a47cda79fe834ac2f64bc2d1d5f4c59d03a5eb","observation_id":"191db111-273b-4d5c-814d-5556594ced12","resolution":{"observed_at":"2026-06-29T06:23:08.848595Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.13929","last_updated":"2020-12-07T14:36:09Z","snapshot_observed_at":"2026-08-04T02:05:00.665984Z","submitted_at":"2020-06-24T17:58:07Z","title":"New limits on dark photons from solar emission and keV scale dark matter","version":2},"cited_work":{"arxiv_id":"2006.13929","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2006.13929","snapshot_observed_at":"2026-07-04T20:20:06.837609Z","title":"New limits on dark photons from solar emission and keV scale dark matter","venue":null,"work_id":"aaabc7b8-cb0f-4a4e-b651-50cc83dbc540","year":2020},"citing_paper":{"arxiv_id":"2606.25779","last_updated":"2026-06-24T12:56:46Z","snapshot_observed_at":"2026-07-07T00:00:12.737052Z","submitted_at":"2026-06-24T12:56:46Z","title":"Dark Photons from Red Dwarfs","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-06-25T20:27:04.894292Z"},"links":{"cited_paper":"/paper/2006.13929","citing_paper":"/paper/2606.25779"},"observation_digest":"sha256:7c6b5c9a6e9a9615b933675ec19bf8bd644a5c32413acbffd77bad13b3090bf0","observation_id":"660947fc-e3b6-48d2-9c9c-6f5e3ea4c46a","resolution":{"observed_at":"2026-07-04T20:20:06.839296Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.13929","last_updated":"2020-12-07T14:36:09Z","snapshot_observed_at":"2026-08-04T02:05:00.665984Z","submitted_at":"2020-06-24T17:58:07Z","title":"New limits on dark photons from solar emission and keV scale dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.13929","snapshot_observed_at":"2026-08-01T08:28:09.315448Z","title":"New limits on dark photons from solar emission and keV scale dark matter,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.21168","last_updated":"2026-07-23T10:55:45Z","snapshot_observed_at":"2026-08-11T18:19:59.621944Z","submitted_at":"2026-07-23T10:55:45Z","title":"MeV Electrophilic Axion-like Particles from Sun","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-01T08:28:09.315448Z"},"links":{"cited_paper":"/paper/2006.13929","citing_paper":"/paper/2607.21168"},"observation_digest":"sha256:d91323fd6322082ca9a4ca115d6df811737f6d813ab56375a45022c5c33abfea","observation_id":"934dd07e-46d9-47d6-9190-84153a33d8fd","resolution":{"observed_at":"2026-08-01T08:28:09.315448Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2006.13929/citation-record","integrity":"/paper/2006.13929/integrity","json":"/paper/2006.13929/citation-record.json","paper":"/paper/2006.13929"},"outbound":[],"paper":{"arxiv_id":"2006.13929","last_updated":"2020-12-07T14:36:09Z","latest_version":2,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-04T02:05:00.665984Z","submitted_at":"2020-06-24T17:58:07Z","title":"New limits on dark photons from solar emission and keV scale dark matter"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2006.13929."}