{"as_of":"2026-08-08T10:58:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:61d4bda6dbc5b10fbb61ff428e5b5734cabf55101dabb44296dc7eade5fb6535","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":"2026-08-08T06:32:00.761636+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":"2026-08-07T14:00:26.224983Z","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":"2026-05-20T04:08:03.020581Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2305.01913","last_updated":"2023-11-13T07:35:50Z","snapshot_observed_at":"2026-07-06T15:22:40.401971Z","submitted_at":"2023-05-03T06:08:29Z","title":"Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.01913","snapshot_observed_at":"2026-08-07T14:00:26.224983Z","title":"Akita and S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.20396","last_updated":"2025-05-26T18:00:01Z","snapshot_observed_at":"2026-08-07T14:39:03.787633Z","submitted_at":"2025-05-26T18:00:01Z","title":"Cosmological impact of $\\nu$DM interactions enhanced in narrow redshift ranges","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-07T14:00:26.224983Z"},"links":{"cited_paper":"/paper/2305.01913","citing_paper":"/paper/2505.20396"},"observation_digest":"sha256:00dc53fb96ceb09ca714720cfde217d55829fdf9673f062f623fc775491627c6","observation_id":"6240c39e-9115-415d-bde3-3a3a8cd49015","resolution":{"observed_at":"2026-08-07T14:00:26.224983Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.01913","last_updated":"2023-11-13T07:35:50Z","snapshot_observed_at":"2026-07-06T15:22:40.401971Z","submitted_at":"2023-05-03T06:08:29Z","title":"Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.01913","snapshot_observed_at":"2026-08-07T10:57:41.085221Z","title":"Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.04568","last_updated":"2025-08-05T00:29:22Z","snapshot_observed_at":"2026-08-07T12:22:40.520704Z","submitted_at":"2025-06-05T02:40:15Z","title":"Bounds and detection of MeV-scale dark matter annihilation to neutrinos","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-07T10:57:41.085221Z"},"links":{"cited_paper":"/paper/2305.01913","citing_paper":"/paper/2506.04568"},"observation_digest":"sha256:47db4fb81dc6e915a4bbffe990ec9039e579c89fdedd53e00f98a0d1de45ea13","observation_id":"0ed7bde2-6e81-4586-a70d-bc1cef7c5dab","resolution":{"observed_at":"2026-08-07T10:57:41.085221Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.01913","last_updated":"2023-11-13T07:35:50Z","snapshot_observed_at":"2026-07-06T15:22:40.401971Z","submitted_at":"2023-05-03T06:08:29Z","title":"Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.01913","snapshot_observed_at":"2026-08-07T05:04:00.135167Z","title":"Akita and S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.08993","last_updated":"2026-04-01T08:48:22Z","snapshot_observed_at":"2026-08-07T04:55:00.314675Z","submitted_at":"2025-06-10T17:11:22Z","title":"The Highest-Energy Neutrino Event Constrains Dark Matter-Neutrino Interactions","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T05:04:00.135167Z"},"links":{"cited_paper":"/paper/2305.01913","citing_paper":"/paper/2506.08993"},"observation_digest":"sha256:4c918cb624496e5d80a8b7682c47457eb611844958a2862ca565374e780a151e","observation_id":"bc61d0bc-0ea0-47a1-a0ba-b501e7a6d8f4","resolution":{"observed_at":"2026-08-07T05:04:00.135167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.01913","last_updated":"2023-11-13T07:35:50Z","snapshot_observed_at":"2026-07-06T15:22:40.401971Z","submitted_at":"2023-05-03T06:08:29Z","title":"Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.01913","snapshot_observed_at":"2026-08-06T21:08:41.213649Z","title":"Akita and S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.01000","last_updated":"2026-06-22T15:46:16Z","snapshot_observed_at":"2026-08-06T20:58:11.638947Z","submitted_at":"2025-07-01T17:51:21Z","title":"New Constraints on Neutrino-Dark Matter Interactions: A Comprehensive Analysis","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T21:08:41.213649Z"},"links":{"cited_paper":"/paper/2305.01913","citing_paper":"/paper/2507.01000"},"observation_digest":"sha256:2eada283a084b647c6d495405abd29cb7e362c0daba53bdff03caec84cdeaf50","observation_id":"5293c67d-2223-4c3e-84e3-0a8f6a369e74","resolution":{"observed_at":"2026-08-06T21:08:41.213649Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.01913","last_updated":"2023-11-13T07:35:50Z","snapshot_observed_at":"2026-07-06T15:22:40.401971Z","submitted_at":"2023-05-03T06:08:29Z","title":"Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations","version":2},"cited_work":{"arxiv_id":"2305.01913","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2305.01913","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Akita and S","venue":null,"work_id":"6f2f5c85-ac46-418e-bc2e-360257bbb760","year":2023},"citing_paper":{"arxiv_id":"2508.02869","last_updated":"2026-04-22T16:52:50Z","snapshot_observed_at":"2026-08-07T09:25:24.851950Z","submitted_at":"2025-08-04T19:55:16Z","title":"Attenuation of the ultra-high-energy neutrino flux by dark matter scatterings","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-19T00:10:46.501265Z"},"links":{"cited_paper":"/paper/2305.01913","citing_paper":"/paper/2508.02869"},"observation_digest":"sha256:6ed809bef287418a909f309480de3672c334756b8c578d526fc04fbff2c43da1","observation_id":"db11e8b6-5e2c-4409-8e1e-02a73bbb8fc6","resolution":{"observed_at":"2026-05-19T00:11:55.923106Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.01913","last_updated":"2023-11-13T07:35:50Z","snapshot_observed_at":"2026-07-06T15:22:40.401971Z","submitted_at":"2023-05-03T06:08:29Z","title":"Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations","version":2},"cited_work":{"arxiv_id":"2305.01913","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2305.01913","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Akita and S","venue":null,"work_id":"6f2f5c85-ac46-418e-bc2e-360257bbb760","year":2023},"citing_paper":{"arxiv_id":"2511.13606","last_updated":"2026-05-03T15:38:21Z","snapshot_observed_at":"2026-07-06T22:36:08.495952Z","submitted_at":"2025-11-17T17:11:33Z","title":"Probing Dark Sector Particles Coupling to Neutrinos with Double Beta Decay","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-17T22:05:42.289408Z"},"links":{"cited_paper":"/paper/2305.01913","citing_paper":"/paper/2511.13606"},"observation_digest":"sha256:fbba5a6d73509ff9a0f4b145064872d0b97670d4062c640ccfc78cd4293524a7","observation_id":"645ce54b-70e2-4b49-8fd9-3dd2f0357236","resolution":{"observed_at":"2026-05-17T22:10:23.156166Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.01913","last_updated":"2023-11-13T07:35:50Z","snapshot_observed_at":"2026-07-06T15:22:40.401971Z","submitted_at":"2023-05-03T06:08:29Z","title":"Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.01913","snapshot_observed_at":"2026-08-03T21:29:34.832157Z","title":"Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.15430","last_updated":"2025-11-19T13:36:51Z","snapshot_observed_at":"2026-08-08T07:30:28.738526Z","submitted_at":"2025-11-19T13:36:51Z","title":"21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-03T21:29:34.832157Z"},"links":{"cited_paper":"/paper/2305.01913","citing_paper":"/paper/2511.15430"},"observation_digest":"sha256:4221979663983e6a72f1477926b84ba31ebec01e15503e6d130c710f102db97a","observation_id":"ff3d6154-46de-4a9a-b7b3-69596a6dd4e9","resolution":{"observed_at":"2026-08-03T21:29:34.832157Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.01913","last_updated":"2023-11-13T07:35:50Z","snapshot_observed_at":"2026-07-06T15:22:40.401971Z","submitted_at":"2023-05-03T06:08:29Z","title":"Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations","version":2},"cited_work":{"arxiv_id":"2305.01913","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2305.01913","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Akita and S","venue":null,"work_id":"6f2f5c85-ac46-418e-bc2e-360257bbb760","year":2023},"citing_paper":{"arxiv_id":"2605.20162","last_updated":"2026-05-19T17:49:34Z","snapshot_observed_at":"2026-07-06T23:30:49.211483Z","submitted_at":"2026-05-19T17:49:34Z","title":"Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess and Predictions for JUNO","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-05-20T04:04:42.736350Z"},"links":{"cited_paper":"/paper/2305.01913","citing_paper":"/paper/2605.20162"},"observation_digest":"sha256:09297684e60c7cb1a61db82fffe5575ee29eefbfe0d3543374d4f0fd02bf7fda","observation_id":"87579530-b00d-4c6d-ad9f-148471b201b9","resolution":{"observed_at":"2026-05-20T04:08:03.023292Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.01913","last_updated":"2023-11-13T07:35:50Z","snapshot_observed_at":"2026-07-06T15:22:40.401971Z","submitted_at":"2023-05-03T06:08:29Z","title":"Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.01913","snapshot_observed_at":"2026-08-02T00:29:43.266008Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.15020","last_updated":"2026-07-16T14:05:52Z","snapshot_observed_at":"2026-08-04T15:23:56.552301Z","submitted_at":"2026-07-16T14:05:52Z","title":"High resolution Lyman-{\\alpha} forest constraints on dark matter-neutrino scattering","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-02T00:29:43.266008Z"},"links":{"cited_paper":"/paper/2305.01913","citing_paper":"/paper/2607.15020"},"observation_digest":"sha256:990dd62290fb06a5e04444119c42a108abccfc7c83c9473a35abda74a212b962","observation_id":"dbd65d9d-e3d6-4ca9-a01b-6ad30ad6df21","resolution":{"observed_at":"2026-08-02T00:29:43.266008Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2305.01913/citation-record","integrity":"/paper/2305.01913/integrity","json":"/paper/2305.01913/citation-record.json","paper":"/paper/2305.01913"},"outbound":[],"paper":{"arxiv_id":"2305.01913","last_updated":"2023-11-13T07:35:50Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T15:22:40.401971Z","submitted_at":"2023-05-03T06:08:29Z","title":"Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2305.01913."}