{"as_of":"2026-08-16T07:16:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b4bf95e0801ebaec864a1b38db63f2d556039a4dd5ae1bca073261084c8d0dbb","coverage":[{"denominator":34,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":34,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T18:01:47.476683Z","state":"measured"},{"denominator":34,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":34,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+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/2608.10761/citation-record","integrity":"/paper/2608.10761/integrity","json":"/paper/2608.10761/citation-record.json","paper":"/paper/2608.10761"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2403.05608","last_updated":"2025-06-16T11:00:59Z","snapshot_observed_at":"2026-08-15T07:47:44.654516Z","submitted_at":"2024-03-08T10:21:36Z","title":"Search for anti-quark nuggets via their interaction with the LHC beam","version":3},"cited_work":{"arxiv_id":"2403.05608","doi":null,"metadata_source":"pith","pith_arxiv_id":"2403.05608","snapshot_observed_at":"2026-08-12T18:01:48.078976Z","title":"Search for anti-quark nuggets via their interaction with the LHC beam","venue":"hep-ex","work_id":"e7163c8b-a0a1-43fa-b396-2437d0a73390","year":2024},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.342023Z"},"links":{"cited_paper":"/paper/2403.05608","citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:8b8965b7c555ac224d9aee3fd5e37b519cdb46310050499db3395570581fcc7e","observation_id":"16bc676c-751a-4545-8b88-7a2be4cbe07a","resolution":{"observed_at":"2026-08-12T18:01:48.083822Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/0202161","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:48.059945Z","title":"‘Nonbaryonic’ dark matter as baryonic color superconductor.JCAP2003,10, 010, [hep- ph/0202161]","venue":null,"work_id":"236f5c8b-56b0-4b4d-b8ca-d63c55cae3a8","year":2003},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.347011Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:e3ae596b3cef4a0521b7ad48792c2d59fe1d2af66a25d2aae1742c016d8f1ef6","observation_id":"a852ef88-40cd-4595-8bff-be014c24094a","resolution":{"observed_at":"2026-08-12T18:01:48.066164Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T18:01:48.131156Z","title":"The DELight experiment","venue":null,"work_id":"98532b1d-6ea4-42b8-b710-980e3c9a5379","year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.351994Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:b172e4f817e83c63dbf26d727459ec62623ea9de4e06543331018251d68fb2aa","observation_id":"6e03b601-7b90-46c2-901e-b8e4b99109b7","resolution":{"observed_at":"2026-08-12T18:01:48.137076Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.110.115020","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:47.705022Z","title":"Statistics and sensitivity of axion wind detection with the homogeneous precession domain of superfluid helium-3","venue":null,"work_id":"c82f3f19-a5f3-4697-a8ca-d6217717f239","year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.356336Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:e56d4c193a79c2545c93132a19b13bbf5979c9b60483799bd5dc01af5c45b0d4","observation_id":"4bac0ec5-6f28-4cca-b41e-38304bf60664","resolution":{"observed_at":"2026-08-12T18:01:47.709384Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T18:01:47.360219Z","title":"Demonstration of the HeRALD superfluid helium detector concept","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.360219Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:acda08497b61b8a5772b14381ca781eac2a67f306d1e00e3e26676156781b4d3","observation_id":"1771de90-4cc9-4d6b-9dea-c6d8a0262426","resolution":{"observed_at":"2026-08-12T18:01:47.360219Z","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":"2026-08-12T18:01:47.368139Z","title":"DELight: A direct search experiment for light dark matter with superfluid helium","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.368139Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:12fe398bfd8ba289c80cd0a5e3f006e2e32975a8ec56ce29120e19a419867903","observation_id":"d2d9e243-939c-4222-b252-19d5ee240db5","resolution":{"observed_at":"2026-08-12T18:01:47.368139Z","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":"10.1142/9789812778000_","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:47.674414Z","title":"InLow Energy Solar Neutrino Detection; World Scientific, 2001; pp","venue":null,"work_id":"931ca245-a55e-4de8-9229-e21338ca601c","year":2001},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.372863Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:0924789de0cdea1f1eaccf54aa6a15c267a5c17c2582daff1abd92ab905f4da2","observation_id":"b9c7eaff-ec01-46db-8e38-56b8a6b87b38","resolution":{"observed_at":"2026-08-12T18:01:47.678396Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2105.08719","last_updated":"2021-05-18T17:59:59Z","snapshot_observed_at":"2026-08-13T19:20:24.885176Z","submitted_at":"2021-05-18T17:59:59Z","title":"Axion Quark Nuggets. Dark Matter and Matter-Antimatter asymmetry: theory, observations and future experiments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.08719","snapshot_observed_at":"2026-08-12T18:01:47.377106Z","title":"Axion quark nuggets","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.377106Z"},"links":{"cited_paper":"/paper/2105.08719","citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:07c639acebc591441f116e93b13bec3e081747c79cba1957a7e3de77e5981e09","observation_id":"964a7a93-6317-4aa5-a69d-57a0a2f26b2d","resolution":{"observed_at":"2026-08-12T18:01:47.377106Z","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":"2026-08-12T18:01:48.117665Z","title":"Superfluid helium cryogenics for the large hadron collider project at CERN.Cryogenics1994, 34, 1–8","venue":null,"work_id":"2ed67842-2323-416a-a0bb-984c8aabbe9f","year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.381165Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:ae72e499419bd810f948f83541a892cf1d0b785755179918349a07752036300e","observation_id":"5fe3329f-ae1e-4477-8867-0569e87d7fc3","resolution":{"observed_at":"2026-08-12T18:01:48.122442Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T18:01:47.385523Z","title":"https://doi.org/10.5170/CERN-2004-003-V-1","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.385523Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:7a6d974061cec05dac2dbef6d45c8da98063669a2a4f25cc622ffc7497bfe331","observation_id":"e1be16f2-0851-4c36-9dcc-7ad12eda7163","resolution":{"observed_at":"2026-08-12T18:01:47.385523Z","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":"2026-08-12T18:01:48.106143Z","title":"The technology of superfluid helium","venue":null,"work_id":"18a57ff3-727f-450e-af4a-17af17ef3b9f","year":2004},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.389432Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:fa5147273c6db50ee384c8ec5bb2cf90eef66238d700e8e6a9f8c74f933ef2bc","observation_id":"e05ca892-93b4-4af8-9f29-da3e58dc5ed4","resolution":{"observed_at":"2026-08-12T18:01:48.110484Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1475-7516/2008/01/023","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:47.657258Z","title":"Diffuse x-rays: directly observing dark matter?JCAP2008,2008, 023","venue":null,"work_id":"1dff13c8-d865-4a58-87c6-4fbc7531eef8","year":2008},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.393194Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:2d8afa7d579397fb793c064d7c2181821d4d5707eafc96d26c717551f2c259c2","observation_id":"f962c37a-f598-4994-bbdb-db6ae8fdb7a8","resolution":{"observed_at":"2026-08-12T18:01:47.661002Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T18:01:47.397270Z","title":"X-ray annual modulation observed by XMM-Newton and axion quark nugget dark matter.Phys","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.397270Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:84897e3895572eb050bbc5d9b69fd0360c3a752a4d7223d50a510e6b66daefdd","observation_id":"5f970a12-bb2d-42a5-95cf-7502ac179279","resolution":{"observed_at":"2026-08-12T18:01:47.397270Z","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":"10.3390/sym14030459","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:47.644811Z","title":"Infrasonic, acoustic and seismic waves produced by the axion quark nuggets.Symmetry2022,14, 459","venue":null,"work_id":"9fdc3126-5642-422d-8d74-e5fc002e8254","year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.400666Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:9ec7c0ebd42c5c8d19d1eef614c07368893af9ce430f73b1dee65e830010bc70","observation_id":"18188332-daa8-4046-9ba9-ba7e531f94f1","resolution":{"observed_at":"2026-08-12T18:01:47.650327Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T18:01:47.404523Z","title":"New capabilities of the FLUKA multi-purpose code.Front","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.404523Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:e835c008e07c3a60a53a8c49272e163a4512e3fa7f4eaceb9653f78e71a61916","observation_id":"81d68cf4-5289-4665-b24e-38dd6fe04947","resolution":{"observed_at":"2026-08-12T18:01:47.404523Z","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":"2026-08-12T18:01:47.408305Z","title":"Recent developments in Geant4.Nucl","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.408305Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:69d2ca8b6fede737878f24d992da14487a7e51fcd5235c6fbad3ee0acbe51e98","observation_id":"218bbc56-bf37-49db-99d3-8a48a757960b","resolution":{"observed_at":"2026-08-12T18:01:47.408305Z","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":"10.5170/cern-2004-008","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:47.623672Z","title":"The physics of superfluid helium","venue":null,"work_id":"a72898d8-b041-4702-b65c-480b50527260","year":2004},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.411668Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:2055639de1c441020575b46b666eacab8201b0aa8e4a86552f91eba8e7a45ad8","observation_id":"64e822a8-9fb2-4e54-a872-4abb49ca519e","resolution":{"observed_at":"2026-08-12T18:01:47.627977Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T18:01:48.092550Z","title":"COMSOL Multiphysics ® v","venue":null,"work_id":"70c7d88b-057d-4b6b-8b4d-5ad8dd5318f3","year":2024},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.415335Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:255a10f30394303952f275a90edcf95853525b85856025f8789a2b4527fb3a65","observation_id":"dab21112-480b-4f4f-81f7-df9b583430fd","resolution":{"observed_at":"2026-08-12T18:01:48.097459Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T18:01:47.418931Z","title":"The observed properties of liquid helium at the saturated vapor pressure.J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.418931Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:e701dc40e9e0603eb8ea10d7d9a91b4ed862ed178ca7eb98ce8317ed473594e2","observation_id":"8876ef2b-b2bf-4de4-8f1a-d2a665823149","resolution":{"observed_at":"2026-08-12T18:01:47.418931Z","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":"10.1016/s0079-6417(08)60134-1","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:47.605573Z","title":"Chapter III: The nature of the λ-transition in liquid helium","venue":null,"work_id":"2ac1c037-694d-4ed2-9a9d-875fa20a4a09","year":1961},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.422405Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:14b138709381475f3dbeb8115945205a38655b7fca922e9cdf357639ba7bb31a","observation_id":"e30cce19-b8ec-4b0f-83d2-b1e8e794cff7","resolution":{"observed_at":"2026-08-12T18:01:47.609657Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.101.043012","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:47.593937Z","title":"Axion quark nuggets and how a global network can discover them.Phys","venue":null,"work_id":"f319b8c1-a989-4949-9a66-64b24e7512b4","year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.426984Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:5549afee93b71c4aa9eddb669e1facedb562c3ba186d4d98b787e65fac78fe2f","observation_id":"a6564d92-2746-4566-8301-e115949b88aa","resolution":{"observed_at":"2026-08-12T18:01:47.597901Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T18:01:47.431116Z","title":"Streams and caustics: the fine-grained structure of Λ cold dark matter haloes.Mon","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.431116Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:83dae56425d31688c4b7917d1f4785a6dfbe53c8927880afa9dc09fb5770242b","observation_id":"d6c3ca46-95df-40ea-8e4c-15e409b398d6","resolution":{"observed_at":"2026-08-12T18:01:47.431116Z","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":"2026-08-12T18:01:47.434925Z","title":"On the possibility of Bose-star formation.Phys","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.434925Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:03de13e13ef7779a4404c8c3b39b6887fd09e91cf65a494584f16113b6484073","observation_id":"dd070a46-aa50-4242-bfef-62947624e449","resolution":{"observed_at":"2026-08-12T18:01:47.434925Z","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":"10.1103/physrevlett.71.3051","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:47.575650Z","title":"Axion miniclusters and Bose stars.Phys","venue":null,"work_id":"f0389533-2a62-4b95-bb40-49c9695f8070","year":1993},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.439515Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:c51816845cc101bb2f465556879714da715b84828eca2839e047ea3ea3d617eb","observation_id":"c60e1017-66e8-4ac0-9aa5-fe56990bfa0b","resolution":{"observed_at":"2026-08-12T18:01:47.579874Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T18:01:47.443353Z","title":"Gravitational focusing effects on streaming dark matter as a new detection concept.Phys","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.443353Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:fc34e62074569817cd7fb3b6f2dbbdb469fe08155b49e5d5e8cb063bdc8ca59d","observation_id":"4224ad59-5531-4956-9e77-b4bf65467ced","resolution":{"observed_at":"2026-08-12T18:01:47.443353Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/s0927-6505(03)00138-5","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:47.564533Z","title":"Gravitational lensing by the Sun of non-relativistic penetrating particles.Astropart","venue":null,"work_id":"bd3839d7-22de-4b39-9d81-334ae4720a17","year":2003},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.446920Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:2d91435dbfb3fc35e6d5be613188e5e739ccf10e47c44b4334d2ff66aa2fe156","observation_id":"bed81e39-a0e8-4f61-8931-e1eb776c63b2","resolution":{"observed_at":"2026-08-12T18:01:47.568659Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T18:01:47.451427Z","title":"Flux enhancement of slow-moving particles by Sun or Jupiter: Can they be detected on Earth?Astrophys","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.451427Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:5474a9fdfe446195c7fe0b82c5b23a377c0554722ec0684083fe029ee1cb9047","observation_id":"3f292d4e-f35e-4a1a-a012-e7954dc59d07","resolution":{"observed_at":"2026-08-12T18:01:47.451427Z","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":"10.3390/galaxies8020042","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:47.546013Z","title":"Gravitational focusing of low-velocity dark matter on the Earth’s surface.Galaxies2020,8","venue":null,"work_id":"26661c9a-74bf-42ae-a9c5-b1fe159cf07b","year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.455073Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:ee2bdc2fd35b18bb06db86ace8a1d0e38ccf934d0b25bd7b3e389fecb3b0fa89","observation_id":"ea81080f-2c5f-4b3e-8241-c3f3e64148f5","resolution":{"observed_at":"2026-08-12T18:01:47.550059Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/814/2/122","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:47.534331Z","title":"Dense dark matter hairs spreading out from Earth, Jupiter, and other compact bodies.Astrophys","venue":null,"work_id":"4af1c21e-bd3d-4ec1-863c-a01990e7bfcf","year":2015},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.459237Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:f18ee27001fdde1fc50831bae41f253fd0968ed7ac014013f359c9c1b7369ea1","observation_id":"d4db6b01-5143-41c3-af80-c311ae78c576","resolution":{"observed_at":"2026-08-12T18:01:47.538562Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.108.083001","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T18:01:47.519545Z","title":"Searching for axion streams with the echo method.Phys","venue":null,"work_id":"9d0bd86c-6f06-4021-b082-f445c64c7e8c","year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.462784Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:e306df59216cbfd1345f3c2084fc64db488ab784a1712aa8a51feb73dcb9dfa6","observation_id":"922c71a8-5296-41ad-a2b6-384a8550e3f6","resolution":{"observed_at":"2026-08-12T18:01:47.525986Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03666","last_updated":"2017-05-06T16:43:53Z","snapshot_observed_at":"2026-08-15T00:22:29.465523Z","submitted_at":"2016-02-11T10:32:20Z","title":"The Sun and its Planets as detectors for invisible matter","version":5},"cited_work":{"arxiv_id":"1602.03666","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.03666","snapshot_observed_at":"2026-08-12T18:01:47.739805Z","title":"The Sun and its Planets as detectors for invisible matter","venue":"astro-ph.SR","work_id":"fe9f6653-a2c2-4de7-8d85-b2dc19af84ef","year":2016},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.466471Z"},"links":{"cited_paper":"/paper/1602.03666","citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:f0d2f1eb4ffb92c5233031a99c66810668f399abe9fc47b7e276ce5fa95a6b5f","observation_id":"d0b97df6-9cf8-4814-a9dd-5bf4684bd9e6","resolution":{"observed_at":"2026-08-12T18:01:47.748298Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T18:01:47.470207Z","title":"Mysterious anomalies in Earth’s atmosphere and strongly interacting dark matter.Symmetry2025,17","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.470207Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:4c67a3e26381d8dd2ce44506b4937b6e1833c12765e564495103ba6bc27cfffe","observation_id":"fe3706e3-b736-41dc-95c2-848a0ac917ad","resolution":{"observed_at":"2026-08-12T18:01:47.470207Z","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":"2026-08-12T18:01:47.473439Z","title":"The 27-day variations of plasma densities and temperatures in the topside ionosphere.J","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.473439Z"},"links":{"citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:0aab9bc43eaac99257ea56d214e30c381064e8d060fa380ae4fe3d198b81ce9b","observation_id":"e861799e-bde0-4172-86ac-37185ed8e3a3","resolution":{"observed_at":"2026-08-12T18:01:47.473439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2602.10562","last_updated":"2026-06-18T22:41:43Z","snapshot_observed_at":"2026-08-15T07:46:14.676170Z","submitted_at":"2026-02-11T06:18:42Z","title":"Unidentified falling objects in the LHC as dark matter signals","version":2},"cited_work":{"arxiv_id":"2602.10562","doi":null,"metadata_source":"pith","pith_arxiv_id":"2602.10562","snapshot_observed_at":"2026-08-12T18:01:47.721112Z","title":"Unidentified falling objects in the LHC as dark matter signals","venue":"hep-ph","work_id":"d96ee295-e5c5-4707-a48d-5c6df304b7b7","year":2026},"citing_paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T18:01:47.476683Z"},"links":{"cited_paper":"/paper/2602.10562","citing_paper":"/paper/2608.10761"},"observation_digest":"sha256:fd28f2647a77beeffc65ac7944054f6ff542c0a2ee8932db2856842a3b7c419e","observation_id":"50295705-2af4-4343-8125-aaee2b8bb07b","resolution":{"observed_at":"2026-08-12T18:01:47.726167Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2608.10761","last_updated":"2026-08-11T10:20:33Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-15T07:47:04.760891Z","submitted_at":"2026-08-11T10:20:33Z","title":"Superfluid He-4 as Dark Matter Detectors"},"reference_resolution":{"displayed":34,"state_counts":{"malformed_identifier":2,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":13,"verified_exact":16,"verified_fuzzy":3},"total_outbound_references":34},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 34 of 34 outbound references and 0 inbound Pith citation observations for arXiv:2608.10761."}