{"as_of":"2026-08-09T11:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ad59a0e5c1e0403e27d93994cda1b7c774ab18eec297200f9de12848d2b9b58d","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":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T11:42:10.492746Z","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":"2026-07-04T11:19:50.503561Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2104.06141","last_updated":"2021-06-07T08:20:21Z","snapshot_observed_at":"2026-08-09T09:50:54.877637Z","submitted_at":"2021-04-13T12:31:50Z","title":"Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817","version":3},"cited_work":{"arxiv_id":"2104.06141","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2104.06141","snapshot_observed_at":"2026-07-04T11:19:50.503561Z","title":"Sen and A","venue":null,"work_id":"dc882727-7eba-4dc6-9f84-b61d63312595","year":2021},"citing_paper":{"arxiv_id":"2105.06979","last_updated":"2021-05-14T17:33:32Z","snapshot_observed_at":"2026-08-08T20:42:33.884209Z","submitted_at":"2021-05-14T17:33:32Z","title":"The Radius of PSR J0740+6620 from NICER and XMM-Newton Data","version":1},"reference_index":108,"source":"arxiv_source","source_observed_at":"2026-05-17T07:01:41.436567Z"},"links":{"cited_paper":"/paper/2104.06141","citing_paper":"/paper/2105.06979"},"observation_digest":"sha256:c54474376fc9ef3cc5f7d7e9d46a8fdec7f86b36736a481df2c8dd918621c021","observation_id":"e3b4c43c-445e-4497-82ea-d25f7e72a03e","resolution":{"observed_at":"2026-05-17T07:01:41.540492Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06141","last_updated":"2021-06-07T08:20:21Z","snapshot_observed_at":"2026-08-09T09:50:54.877637Z","submitted_at":"2021-04-13T12:31:50Z","title":"Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817","version":3},"cited_work":{"arxiv_id":"2104.06141","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2104.06141","snapshot_observed_at":"2026-07-04T11:19:50.503561Z","title":"Sen and A","venue":null,"work_id":"dc882727-7eba-4dc6-9f84-b61d63312595","year":2021},"citing_paper":{"arxiv_id":"2503.19691","last_updated":"2026-03-04T15:53:07Z","snapshot_observed_at":"2026-07-06T20:58:27.929311Z","submitted_at":"2025-03-25T14:18:06Z","title":"Strongly Interacting Dark Matter admixed Neutron Stars","version":4},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-22T22:45:48.648963Z"},"links":{"cited_paper":"/paper/2104.06141","citing_paper":"/paper/2503.19691"},"observation_digest":"sha256:56eeba300818589b3ee18fc2400de00cdefec3d2813e80ec2a127adfe19715df","observation_id":"f38de277-48ab-4ca0-93b9-fc67345a1298","resolution":{"observed_at":"2026-05-22T22:47:13.415337Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06141","last_updated":"2021-06-07T08:20:21Z","snapshot_observed_at":"2026-08-09T09:50:54.877637Z","submitted_at":"2021-04-13T12:31:50Z","title":"Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.06141","snapshot_observed_at":"2026-08-05T11:42:10.492746Z","title":"Sen and A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.02325","last_updated":"2025-09-02T13:51:14Z","snapshot_observed_at":"2026-08-09T03:07:09.723512Z","submitted_at":"2025-09-02T13:51:14Z","title":"Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-05T11:42:10.492746Z"},"links":{"cited_paper":"/paper/2104.06141","citing_paper":"/paper/2509.02325"},"observation_digest":"sha256:1c47dbcf654dc87cda19e6b8f1df3d4590b27f03808b7da4bc53a84fdc3a25ae","observation_id":"f39ebc14-a233-4541-bbfc-4d3c2e9964f4","resolution":{"observed_at":"2026-08-05T11:42:10.492746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06141","last_updated":"2021-06-07T08:20:21Z","snapshot_observed_at":"2026-08-09T09:50:54.877637Z","submitted_at":"2021-04-13T12:31:50Z","title":"Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817","version":3},"cited_work":{"arxiv_id":"2104.06141","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2104.06141","snapshot_observed_at":"2026-07-04T11:19:50.503561Z","title":"Sen and A","venue":null,"work_id":"dc882727-7eba-4dc6-9f84-b61d63312595","year":2021},"citing_paper":{"arxiv_id":"2605.14447","last_updated":"2026-05-14T06:41:34Z","snapshot_observed_at":"2026-07-06T23:25:54.070869Z","submitted_at":"2026-05-14T06:41:34Z","title":"Bayesian analysis of density profile of light dark matter elucidating the properties of dark matter admixed neutron stars in the presence of hyperons","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-15T01:47:28.438537Z"},"links":{"cited_paper":"/paper/2104.06141","citing_paper":"/paper/2605.14447"},"observation_digest":"sha256:8162546d78fd34fcdfbcb1c93169bcfb1cdca4226b62fee7947c24b49cc997b0","observation_id":"432e63e5-6b9f-4dbb-824b-48b029889416","resolution":{"observed_at":"2026-05-15T01:48:28.304662Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06141","last_updated":"2021-06-07T08:20:21Z","snapshot_observed_at":"2026-08-09T09:50:54.877637Z","submitted_at":"2021-04-13T12:31:50Z","title":"Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817","version":3},"cited_work":{"arxiv_id":"2104.06141","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2104.06141","snapshot_observed_at":"2026-07-04T11:19:50.503561Z","title":"Sen and A","venue":null,"work_id":"dc882727-7eba-4dc6-9f84-b61d63312595","year":2021},"citing_paper":{"arxiv_id":"2606.23620","last_updated":"2026-06-22T17:17:59Z","snapshot_observed_at":"2026-08-08T04:12:58.276410Z","submitted_at":"2026-06-22T17:17:59Z","title":"Observables and conformal properties of dark matter admixed isentropic neutron stars","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-06-26T08:02:28.544158Z"},"links":{"cited_paper":"/paper/2104.06141","citing_paper":"/paper/2606.23620"},"observation_digest":"sha256:5039d6bc60d695094a2a74ed94c3b00acaae22dd8fb92dbfa5e35cbd0c356207","observation_id":"9f7327cd-4d0d-4263-81f4-b9721cba1d85","resolution":{"observed_at":"2026-07-04T11:19:50.505467Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06141","last_updated":"2021-06-07T08:20:21Z","snapshot_observed_at":"2026-08-09T09:50:54.877637Z","submitted_at":"2021-04-13T12:31:50Z","title":"Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817","version":3},"cited_work":{"arxiv_id":"2104.06141","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2104.06141","snapshot_observed_at":"2026-07-04T11:19:50.503561Z","title":"Sen and A","venue":null,"work_id":"dc882727-7eba-4dc6-9f84-b61d63312595","year":2021},"citing_paper":{"arxiv_id":"2607.00888","last_updated":"2026-07-01T12:54:11Z","snapshot_observed_at":"2026-08-02T11:37:51.086281Z","submitted_at":"2026-07-01T12:54:11Z","title":"A self-consistent single-fluid framework for neutron stars admixed with mirror dark matter","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-07-02T08:36:45.802728Z"},"links":{"cited_paper":"/paper/2104.06141","citing_paper":"/paper/2607.00888"},"observation_digest":"sha256:11dfeafaf5c0447316d43586f17ab87543e7bdf38b0bd1d5f0ccef3c5741553c","observation_id":"f257d0be-b457-4af4-a92b-88e6d9d673d3","resolution":{"observed_at":"2026-07-02T08:46:48.754805Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06141","last_updated":"2021-06-07T08:20:21Z","snapshot_observed_at":"2026-08-09T09:50:54.877637Z","submitted_at":"2021-04-13T12:31:50Z","title":"Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.06141","snapshot_observed_at":"2026-08-02T00:38:33.503007Z","title":"Sen and A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.14979","last_updated":"2026-07-16T13:31:14Z","snapshot_observed_at":"2026-08-08T23:04:28.288060Z","submitted_at":"2026-07-16T13:31:14Z","title":"A self-consistent Higgs-portal framework for dark matter--admixed neutron stars: Collider-motivated benchmarks meet multimessenger constraints","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-02T00:38:33.503007Z"},"links":{"cited_paper":"/paper/2104.06141","citing_paper":"/paper/2607.14979"},"observation_digest":"sha256:7351070d205eee594843cb144205cfcd0f64aca53f46cac6e35824d973ad7eca","observation_id":"e4dab0e5-2148-461e-bc60-bd1e09ef87a2","resolution":{"observed_at":"2026-08-02T00:38:33.503007Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2104.06141/citation-record","integrity":"/paper/2104.06141/integrity","json":"/paper/2104.06141/citation-record.json","paper":"/paper/2104.06141"},"outbound":[],"paper":{"arxiv_id":"2104.06141","last_updated":"2021-06-07T08:20:21Z","latest_version":3,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-09T09:50:54.877637Z","submitted_at":"2021-04-13T12:31:50Z","title":"Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2104.06141."}