{"as_of":"2026-08-07T20:59:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3bf48b884bfde171d8de09a0910622c02fceb62c5ac8dcebbc4a39fff6e2e972","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":15,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":15,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":15,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":15,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T04:22:34.723661Z","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":"2026-07-02T10:06:51.506807Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-08-07T04:22:34.723661Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.11191","last_updated":"2025-06-12T18:00:02Z","snapshot_observed_at":"2026-08-07T04:10:12.585529Z","submitted_at":"2025-06-12T18:00:02Z","title":"Spin-Dependent Scattering of Sub-GeV Dark Matter: Models and Constraints","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T04:22:34.723661Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2506.11191"},"observation_digest":"sha256:9defa4148a59aab0cdfa46f9f993e9303b7fd72892053c0189da9f8cee752623","observation_id":"fe65e741-3582-4043-a792-1ff8ea28b853","resolution":{"observed_at":"2026-08-07T04:22:34.723661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-08-06T15:29:11.480601Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.15956","last_updated":"2025-07-21T18:00:20Z","snapshot_observed_at":"2026-08-06T21:39:44.143714Z","submitted_at":"2025-07-21T18:00:20Z","title":"Sub-GeV Dark Matter Under Pressure from Direct Detection","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T15:29:11.480601Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2507.15956"},"observation_digest":"sha256:cd30a8ae133fa01d13b9d6d747c0735077a259fecc833d16fffd4c23610693d8","observation_id":"3a5e5e4f-b563-4dfc-bf47-0076c7093960","resolution":{"observed_at":"2026-08-06T15:29:11.480601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":"2112.03920","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-07-02T10:06:51.506807Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter,","venue":null,"work_id":"1c20be2b-17d6-4f6a-815b-b77ece774bd3","year":2023},"citing_paper":{"arxiv_id":"2509.07070","last_updated":"2026-05-19T17:47:54Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-09-08T18:00:01Z","title":"Reviving WIMP dark matter with temperature-dependent couplings","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-21T22:28:26.801795Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2509.07070"},"observation_digest":"sha256:3101e9eb5b9751e34818c58f4637f148ddcf5a26636344e5bea04b1f153bd043","observation_id":"d8946d5b-a23e-42a0-8296-809974467801","resolution":{"observed_at":"2026-05-21T22:30:43.008769Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-08-04T08:57:01.612070Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.18338","last_updated":"2026-06-29T09:20:06Z","snapshot_observed_at":"2026-08-07T10:08:47.110506Z","submitted_at":"2025-10-21T06:44:48Z","title":"Direct Detection of Leptophobic Dark Matter with Electronic Collective Excitations","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-04T08:57:01.612070Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2510.18338"},"observation_digest":"sha256:f3c80c00b56d881b97c9fb00240ba029ef7f64d5a7a29330cdc13669f4a10ae4","observation_id":"93cfe6c8-530c-4425-bdd0-9c0f3b289bdd","resolution":{"observed_at":"2026-08-04T08:57:01.612070Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-08-03T17:42:23.946956Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2512.09019","last_updated":"2026-07-17T20:34:47Z","snapshot_observed_at":"2026-08-07T08:16:46.056752Z","submitted_at":"2025-12-09T19:00:00Z","title":"Search for Dark Matter Annihilation and Decay with H$\\alpha$ Line Emission","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-03T17:42:23.946956Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2512.09019"},"observation_digest":"sha256:bce31a5336c2bc0d9d435bef5e60a5261e77336ca243bc78e127eb02c52211ca","observation_id":"35ad14d1-a645-4d98-ab6f-634f2c9b5187","resolution":{"observed_at":"2026-08-03T17:42:23.946956Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":"2112.03920","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-07-02T10:06:51.506807Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter,","venue":null,"work_id":"1c20be2b-17d6-4f6a-815b-b77ece774bd3","year":2023},"citing_paper":{"arxiv_id":"2602.04858","last_updated":"2026-06-23T09:20:24Z","snapshot_observed_at":"2026-08-03T04:31:42.595842Z","submitted_at":"2026-02-04T18:43:59Z","title":"Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-16T06:48:35.787193Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2602.04858"},"observation_digest":"sha256:ecab3c3e6ba27b7ab315fef95ffb170efe1c98d08bff139d75c74b8488340291","observation_id":"739795f9-ae98-4f32-8ef1-d9cab735b330","resolution":{"observed_at":"2026-05-16T06:50:42.882217Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-08-03T04:31:51.974346Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2602.04858","last_updated":"2026-06-23T09:20:24Z","snapshot_observed_at":"2026-08-03T04:31:42.595842Z","submitted_at":"2026-02-04T18:43:59Z","title":"Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-03T04:31:51.974346Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2602.04858"},"observation_digest":"sha256:5a758ddc5dcf2af854b8dc5d67e79164a521e33cf8307ca162b3e39d9e08c673","observation_id":"3fac013b-1a3f-47bd-8d45-4204e4efa395","resolution":{"observed_at":"2026-08-03T04:31:51.974346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":"2112.03920","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-07-02T10:06:51.506807Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter,","venue":null,"work_id":"1c20be2b-17d6-4f6a-815b-b77ece774bd3","year":2023},"citing_paper":{"arxiv_id":"2605.08080","last_updated":"2026-05-08T17:59:28Z","snapshot_observed_at":"2026-07-06T23:20:19.821342Z","submitted_at":"2026-05-08T17:59:28Z","title":"CMB Limits on the Absorption of Light Vector and Axial-Vector Dark Matter","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-11T01:54:09.895071Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2605.08080"},"observation_digest":"sha256:86393b55282375e288419c9160cebfd7994c15abfe05daf846e3a211703a2f75","observation_id":"d0ca9258-2850-4856-a503-b65ba03ef40b","resolution":{"observed_at":"2026-05-11T04:10:58.820764Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":"2112.03920","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-07-02T10:06:51.506807Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter,","venue":null,"work_id":"1c20be2b-17d6-4f6a-815b-b77ece774bd3","year":2023},"citing_paper":{"arxiv_id":"2605.15197","last_updated":"2026-07-29T13:49:49Z","snapshot_observed_at":"2026-08-02T14:03:29.096476Z","submitted_at":"2026-05-14T17:59:55Z","title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-15T02:53:41.149271Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2605.15197"},"observation_digest":"sha256:d3a98e203b842d14f583f34e7c1f5c133733fb402c8833c6861971e05a81b1f3","observation_id":"47b2b4a2-e5ac-43c0-ba31-0bfe4fbd547a","resolution":{"observed_at":"2026-05-15T02:59:41.903801Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-08-02T14:03:32.031261Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.15197","last_updated":"2026-07-29T13:49:49Z","snapshot_observed_at":"2026-08-02T14:03:29.096476Z","submitted_at":"2026-05-14T17:59:55Z","title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-02T14:03:32.031261Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2605.15197"},"observation_digest":"sha256:15f3be14b329319c954b99de7eeb670be6045ce8286f2bdd3b77592bc1c7e00a","observation_id":"d31fdc46-00e3-4280-a6fd-eacfaa99e0bb","resolution":{"observed_at":"2026-08-02T14:03:32.031261Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":"2112.03920","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-07-02T10:06:51.506807Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter,","venue":null,"work_id":"1c20be2b-17d6-4f6a-815b-b77ece774bd3","year":2023},"citing_paper":{"arxiv_id":"2606.03487","last_updated":"2026-06-02T11:05:08Z","snapshot_observed_at":"2026-07-06T23:43:46.458792Z","submitted_at":"2026-06-02T11:05:08Z","title":"Probing Inelastic Dark Matter via Cosmic-Ray Upscattering in NGC 1068","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-06-28T09:30:56.846406Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2606.03487"},"observation_digest":"sha256:597bee8dd3a998a0941e02044ff4ab49d2fbb1fbf7b3ec25a91463502220f4a8","observation_id":"28cc2b98-acad-44d2-a405-c280871c0084","resolution":{"observed_at":"2026-07-02T03:56:35.611621Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":"2112.03920","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-07-02T10:06:51.506807Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter,","venue":null,"work_id":"1c20be2b-17d6-4f6a-815b-b77ece774bd3","year":2023},"citing_paper":{"arxiv_id":"2607.00840","last_updated":"2026-07-07T15:47:31Z","snapshot_observed_at":"2026-08-02T07:05:48.906540Z","submitted_at":"2026-07-01T12:06:57Z","title":"Dark matter energy exchange in stars orbiting supermassive black holes","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-02T10:01:27.867493Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2607.00840"},"observation_digest":"sha256:50f80f2294d425b03b5a35286f7fe2292c3d6df2be8dbe6acfa70880b0418e51","observation_id":"c88e3653-8fd7-440d-8095-8894f1b57163","resolution":{"observed_at":"2026-07-02T10:06:51.508432Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-07-12T09:14:43.772818Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.00840","last_updated":"2026-07-07T15:47:31Z","snapshot_observed_at":"2026-08-02T07:05:48.906540Z","submitted_at":"2026-07-01T12:06:57Z","title":"Dark matter energy exchange in stars orbiting supermassive black holes","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-12T09:14:43.772818Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2607.00840"},"observation_digest":"sha256:dc04dfbb655fa3b2278695e234bf717d2a1df6582988ef7a4f2b21548d00670d","observation_id":"e6fc2a83-7201-457b-842c-10d62bdc9ba9","resolution":{"observed_at":"2026-07-12T09:14:43.772818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-07-13T06:21:08.244085Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.08838","last_updated":"2026-07-09T18:00:37Z","snapshot_observed_at":"2026-08-03T13:22:41.963703Z","submitted_at":"2026-07-09T18:00:37Z","title":"Dark Phoenix: dark matter relic from its own decay","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-13T06:21:08.244085Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2607.08838"},"observation_digest":"sha256:b37b7f38cbdbb983fe2918ebece34eea6bcb34c1850f230bf1dc3444f333d5aa","observation_id":"c112b2ff-a277-4975-8f33-cf40f65e7f62","resolution":{"observed_at":"2026-07-13T06:21:08.244085Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03920","snapshot_observed_at":"2026-08-02T00:17:55.106411Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.15098","last_updated":"2026-07-22T07:30:05Z","snapshot_observed_at":"2026-08-05T16:02:08.146598Z","submitted_at":"2026-07-16T15:10:08Z","title":"Inelastic Scattering Effects on Attenuation of Boosted Dark Matter","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-02T00:17:55.106411Z"},"links":{"cited_paper":"/paper/2112.03920","citing_paper":"/paper/2607.15098"},"observation_digest":"sha256:092e6e03d97fa9ec41c0b5284e2136f829c4751e9fad44d5c4537715561a035c","observation_id":"31904c6c-7eea-49b8-ba63-d13b54314e72","resolution":{"observed_at":"2026-08-02T00:17:55.106411Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2112.03920/citation-record","integrity":"/paper/2112.03920/integrity","json":"/paper/2112.03920/citation-record.json","paper":"/paper/2112.03920"},"outbound":[],"paper":{"arxiv_id":"2112.03920","last_updated":"2023-01-20T22:08:40Z","latest_version":2,"primary_category":"hep-ph","snapshot_observed_at":"2026-07-06T12:16:19.451255Z","submitted_at":"2021-12-07T19:00:00Z","title":"Maximizing Direct Detection with Highly Interactive Particle Relic 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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 15 inbound Pith citation observations for arXiv:2112.03920."}