{"as_of":"2026-08-11T20:09:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:209d5f929e48ba92c27132adaaad9899389571d98d3a55642b241affa71a15df","coverage":[{"denominator":64,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":64,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T22:40:43.517056Z","state":"measured"},{"denominator":65,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":65,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T15:44:04.799036Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-10T15:44:04.843288Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"cited_work":{"arxiv_id":"2501.01489","doi":null,"metadata_source":"pith","pith_arxiv_id":"2501.01489","snapshot_observed_at":"2026-08-10T15:44:04.843288Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","venue":"hep-ph","work_id":"2d711ea0-d9fe-4a9f-b94f-05174f34c910","year":2025},"citing_paper":{"arxiv_id":"2501.13849","last_updated":"2025-09-01T14:42:10Z","snapshot_observed_at":"2026-08-11T05:50:21.288751Z","submitted_at":"2025-01-23T17:16:15Z","title":"Dark Photon Polarimetry","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-10T15:44:04.799036Z"},"links":{"cited_paper":"/paper/2501.01489","citing_paper":"/paper/2501.13849"},"observation_digest":"sha256:668df83f0b8f908a0c7dffd05f6be6975347df07d963613aa0de44bdce6506b4","observation_id":"ac59fb9e-dd95-4274-8652-16c95b3b9038","resolution":{"observed_at":"2026-08-10T15:44:04.849430Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2501.01489/citation-record","integrity":"/paper/2501.01489/integrity","json":"/paper/2501.01489/citation-record.json","paper":"/paper/2501.01489"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:40:45.067589Z","title":null,"venue":null,"work_id":"38cc8c4b-a173-490b-a9dc-948ad87263ed","year":1979},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.133027Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:cb44c54d095d7a1ac66cf4e485c329e2f62d006830757558c39952954145d88f","observation_id":"7eb2bd74-a931-418d-ab07-7797d6b0f0c4","resolution":{"observed_at":"2026-08-10T22:40:45.074313Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-10T22:40:45.045658Z","title":null,"venue":null,"work_id":"1cd7a237-8979-4df5-993b-731507e9cdd1","year":1980},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.138837Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:da261fcdcb0bc9413d71c71d7e2b179a8f94dbdf69f23ad8d793c52b64579aaa","observation_id":"63f36ffe-e223-45dd-a011-a947ace8e189","resolution":{"observed_at":"2026-08-10T22:40:45.052104Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-10T22:40:43.144615Z","title":null,"venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.144615Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:eadba9504214340a394717a4cb684f15bb5fe0fab9f0ca94f81999fa7c205748","observation_id":"2a4e4c07-ca31-4cfd-b106-742823af5cb5","resolution":{"observed_at":"2026-08-10T22:40:43.144615Z","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":"2026-08-10T22:40:43.149952Z","title":null,"venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.149952Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:31e118030f2d68cae58ef8aa149571e1cedc11eb0e4cdf6eed0fa944b06119ff","observation_id":"a2fe3d9f-66e4-4fbb-9d1c-66e4bab473e9","resolution":{"observed_at":"2026-08-10T22:40:43.149952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.4037","last_updated":"2008-05-27T15:30:15Z","snapshot_observed_at":"2026-07-06T01:39:40.993263Z","submitted_at":"2008-05-27T15:30:15Z","title":"Continuous Global Symmetries and Hyperweak Interactions in String Compactifications","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.4037","snapshot_observed_at":"2026-08-10T22:40:43.154920Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.154920Z"},"links":{"cited_paper":"/paper/0805.4037","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:3bdd33ec9b0e2e07a89041b76cea5a6175abc13084707b78d4dec4995af1d1a0","observation_id":"4a1c0423-9034-4e8d-b151-0edf068966fe","resolution":{"observed_at":"2026-08-10T22:40:43.154920Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.0515","last_updated":"2009-09-15T08:36:23Z","snapshot_observed_at":"2026-07-06T02:00:43.795831Z","submitted_at":"2009-09-03T18:52:27Z","title":"Naturally Light Hidden Photons in LARGE Volume String Compactifications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.0515","snapshot_observed_at":"2026-08-10T22:40:43.160427Z","title":"Goodsell, J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.160427Z"},"links":{"cited_paper":"/paper/0909.0515","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:17954b06a83ed2e9e3f3d3f094636f0b2fb791e87b54eb340f1361ae2f762649","observation_id":"fd21eaf9-d814-45ba-89fd-c690e86428a8","resolution":{"observed_at":"2026-08-10T22:40:43.160427Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0807.3279","last_updated":"2008-11-04T17:19:59Z","snapshot_observed_at":"2026-07-06T01:42:47.076515Z","submitted_at":"2008-07-21T14:47:49Z","title":"Bosonic super-WIMPs as keV-scale dark matter","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0807.3279","snapshot_observed_at":"2026-08-10T22:40:43.166451Z","title":"Pospelov, A","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.166451Z"},"links":{"cited_paper":"/paper/0807.3279","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:691e6ff0c297a25b28e9446e681538a8e9a53212923600dc15a708409a185798","observation_id":"2738f317-0e85-41fc-b610-e5f936cccae1","resolution":{"observed_at":"2026-08-10T22:40:43.166451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0810.0713","last_updated":"2009-01-20T06:02:39Z","snapshot_observed_at":"2026-08-04T15:47:39.239482Z","submitted_at":"2008-10-06T19:59:30Z","title":"A Theory of Dark Matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0810.0713","snapshot_observed_at":"2026-08-10T22:40:43.172172Z","title":"Arkani-Hamed, D","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.172172Z"},"links":{"cited_paper":"/paper/0810.0713","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:ca460991a325f74af3ed470b973df3d3ebdd50ae3086de089a96be98f51012ed","observation_id":"46c184d6-2733-4553-b398-b14f2c944a61","resolution":{"observed_at":"2026-08-10T22:40:43.172172Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00039","last_updated":"2018-10-18T02:12:24Z","snapshot_observed_at":"2026-07-06T04:28:17.898643Z","submitted_at":"2015-08-31T20:23:22Z","title":"Heating up the Galaxy with Hidden Photons","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.00039","snapshot_observed_at":"2026-08-10T22:40:43.178772Z","title":"Dubovsky and G","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.178772Z"},"links":{"cited_paper":"/paper/1509.00039","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:36063bb8c7ef03e989008b9c197591bf973028f6921c4b14af11ebec25f3dfcb","observation_id":"768ff05f-963b-423d-a5b7-6f0a6994a38a","resolution":{"observed_at":"2026-08-10T22:40:43.178772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.2812","last_updated":"2011-10-04T01:13:41Z","snapshot_observed_at":"2026-07-06T02:27:43.046073Z","submitted_at":"2011-05-13T19:39:07Z","title":"Dark Light, Dark Matter and the Misalignment Mechanism","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.2812","snapshot_observed_at":"2026-08-10T22:40:43.186659Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.186659Z"},"links":{"cited_paper":"/paper/1105.2812","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:1b83a40753fcd568d55d2b6961403b4f8df37000fa98c6d3a04bd182d66399ef","observation_id":"7e1d610b-6b1d-4a39-8e0d-3cf13fe5cdf7","resolution":{"observed_at":"2026-08-10T22:40:43.186659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.5902","last_updated":"2012-06-14T13:52:57Z","snapshot_observed_at":"2026-07-06T02:41:53.175094Z","submitted_at":"2012-01-27T21:33:15Z","title":"WISPy Cold Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.5902","snapshot_observed_at":"2026-08-10T22:40:43.192894Z","title":"Arias, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.192894Z"},"links":{"cited_paper":"/paper/1201.5902","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:82991fb3a274b6f29e542e471695ab7ad30a11b12956888ee28f1b9c4eacd20f","observation_id":"a116e1b8-00b0-4e36-8a61-8d39268d3135","resolution":{"observed_at":"2026-08-10T22:40:43.192894Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.02102","last_updated":"2015-04-08T20:01:23Z","snapshot_observed_at":"2026-08-07T10:23:42.692512Z","submitted_at":"2015-04-08T20:01:23Z","title":"Vector Dark Matter from Inflationary Fluctuations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.02102","snapshot_observed_at":"2026-08-10T22:40:43.199138Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.199138Z"},"links":{"cited_paper":"/paper/1504.02102","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:f9886ff052161762361e26bf7dad9820a3bdaf1c7c8ce4a47e0ba2e001e2250d","observation_id":"4c3f526d-dc85-426f-a270-6b3431be02a8","resolution":{"observed_at":"2026-08-10T22:40:43.199138Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.07188","last_updated":"2018-10-16T18:00:00Z","snapshot_observed_at":"2026-08-05T14:55:33.384900Z","submitted_at":"2018-10-16T18:00:00Z","title":"Relic Abundance of Dark Photon Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.07188","snapshot_observed_at":"2026-08-10T22:40:43.205319Z","title":"Agrawal, N","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.205319Z"},"links":{"cited_paper":"/paper/1810.07188","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:476af24df378642d2f2cea564c2853de5606e6ff2f971fd3f80b62926466dd82","observation_id":"28f7b88e-f73c-4611-b106-64d5b673ac1d","resolution":{"observed_at":"2026-08-10T22:40:43.205319Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.07196","last_updated":"2019-05-02T17:21:11Z","snapshot_observed_at":"2026-08-10T07:38:32.267949Z","submitted_at":"2018-10-16T18:00:06Z","title":"Dark Photon Dark Matter Produced by Axion Oscillations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.07196","snapshot_observed_at":"2026-08-10T22:40:43.211473Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.211473Z"},"links":{"cited_paper":"/paper/1810.07196","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:bde31164c65231a1dd8afb88adf182785c2f251135209ebd8139b0d988721776","observation_id":"6905a92b-83af-4c20-92e6-16e2e5e81eb8","resolution":{"observed_at":"2026-08-10T22:40:43.211473Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.07195","last_updated":"2019-03-01T18:44:59Z","snapshot_observed_at":"2026-08-10T09:46:38.376122Z","submitted_at":"2018-10-16T18:00:05Z","title":"Parametric Resonance Production of Ultralight Vector Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.07195","snapshot_observed_at":"2026-08-10T22:40:43.217039Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.217039Z"},"links":{"cited_paper":"/paper/1810.07195","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:2260a691fc78bb7012d6f10a0eb0f4402083ac357d78b90b4c4d5a54042eba5a","observation_id":"397fb261-88f3-4f8a-a0db-8fa82c6d1d63","resolution":{"observed_at":"2026-08-10T22:40:43.217039Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.03312","last_updated":"2019-03-18T13:09:59Z","snapshot_observed_at":"2026-07-06T07:26:02.149340Z","submitted_at":"2019-01-10T18:31:28Z","title":"Dark Photon Dark Matter from a Network of Cosmic Strings","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.03312","snapshot_observed_at":"2026-08-10T22:40:43.222731Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.222731Z"},"links":{"cited_paper":"/paper/1901.03312","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:6a95ff62d8985c550421cfcf1b6d42440df520a7edd4b2579c7ba90157381e12","observation_id":"e06f5481-8100-4515-ba90-6de5068789fb","resolution":{"observed_at":"2026-08-10T22:40:43.222731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.19390","last_updated":"2024-08-07T20:42:06Z","snapshot_observed_at":"2026-07-06T18:22:14.521977Z","submitted_at":"2024-05-29T18:00:00Z","title":"Gravitational Production of Completely Dark Photons with Nonminimal Couplings to Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.19390","snapshot_observed_at":"2026-08-10T22:40:43.228523Z","title":"Capanelli, L","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.228523Z"},"links":{"cited_paper":"/paper/2405.19390","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:667cfa601aedf63d7d88bc77bc2d9c7fe875f4af51d0360464d66a8bf030fb0c","observation_id":"0c2c6e49-e273-484c-9988-848033ddcc29","resolution":{"observed_at":"2026-08-10T22:40:43.228523Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.4806","last_updated":"2014-07-17T20:00:08Z","snapshot_observed_at":"2026-07-06T03:49:20.841197Z","submitted_at":"2014-07-17T20:00:08Z","title":"A Parametrically Enhanced Hidden Photon Search","version":1},"cited_work":{"arxiv_id":"1407.4806","doi":null,"metadata_source":"pith","pith_arxiv_id":"1407.4806","snapshot_observed_at":"2026-08-10T22:40:44.444366Z","title":"A Parametrically Enhanced Hidden Photon Search","venue":"hep-ph","work_id":"e2df5edd-372e-493a-92e3-ff6c342ebfbb","year":2014},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.234242Z"},"links":{"cited_paper":"/paper/1407.4806","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:9f194fbbe156474145b288feb63f63f6ad4ab3c1b7b86e1076d13807da003c0b","observation_id":"9609378b-e44d-42fc-88b6-b5cca0488e84","resolution":{"observed_at":"2026-08-10T22:40:44.453217Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.09334","last_updated":"2021-11-30T18:32:50Z","snapshot_observed_at":"2026-08-04T08:52:10.763446Z","submitted_at":"2021-04-19T14:22:15Z","title":"Searching for Dark Photons with Existing Haloscope Data","version":2},"cited_work":{"arxiv_id":"2104.09334","doi":null,"metadata_source":"pith","pith_arxiv_id":"2104.09334","snapshot_observed_at":"2026-08-10T22:40:44.409908Z","title":"Searching for Dark Photons with Existing Haloscope Data","venue":"hep-ph","work_id":"bbfad8f1-e529-427b-b05f-1f3785e676f9","year":2021},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.239487Z"},"links":{"cited_paper":"/paper/2104.09334","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:df5b0d36092804e46247c8fc83398cd3e2826892dc2f695b490957cb47067cd1","observation_id":"8ca46f80-e5bf-421b-ac36-46f612a17348","resolution":{"observed_at":"2026-08-10T22:40:44.416601Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2008.02209","last_updated":"2020-11-13T18:56:32Z","snapshot_observed_at":"2026-08-08T13:06:50.622080Z","submitted_at":"2020-08-05T16:25:06Z","title":"Constraining hidden photons via atomic force microscope measurements and the Plimpton-Lawton experiment","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.02209","snapshot_observed_at":"2026-08-10T22:40:43.244889Z","title":"Kroff and P","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.244889Z"},"links":{"cited_paper":"/paper/2008.02209","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:822a2c3051c2aaabc9bfa55a1190691ec9a2dc498b43545d7f891f678bc697ca","observation_id":"bced68fa-b02d-4097-b28d-7fbb78909f96","resolution":{"observed_at":"2026-08-10T22:40:43.244889Z","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":"2026-08-10T22:40:44.993659Z","title":null,"venue":null,"work_id":"1afbc121-54ce-4678-b726-d2e34dc9805a","year":1988},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.250306Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:e2de4e843cebe7ff5f7f985eaae68889ca46e6cbb7f792f105edd476f85ea3e4","observation_id":"8381601f-b9dd-4118-bce0-68ba56a821ab","resolution":{"observed_at":"2026-08-10T22:40:45.001138Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-10T22:40:44.972539Z","title":null,"venue":null,"work_id":"289f35b2-0a6f-4b2d-ba17-1beed9a35d5b","year":1971},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.256617Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:5e183497158dfe932da9a9924b746662a960607b0adee2340ce99abf2ed81128","observation_id":"0434ee2d-68e0-481d-a4fd-d3acace7e677","resolution":{"observed_at":"2026-08-10T22:40:44.978528Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-10T22:40:44.953678Z","title":null,"venue":null,"work_id":"a362c9e3-b5a6-41cd-a619-827db7d3285e","year":2005},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.263763Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:a56c1331df87de90cb484ebbcce600ad228ed9ed117af5580ba48495c71e5201","observation_id":"1f7e32f6-5143-49c2-ad9c-baa8e8b81755","resolution":{"observed_at":"2026-08-10T22:40:44.960762Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2105.06326","last_updated":"2022-03-16T03:53:59Z","snapshot_observed_at":"2026-08-08T14:48:41.085408Z","submitted_at":"2021-05-13T14:26:15Z","title":"Probing ultra-light dark photon from inverse Compton-like scattering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.06326","snapshot_observed_at":"2026-08-10T22:40:43.269049Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.269049Z"},"links":{"cited_paper":"/paper/2105.06326","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:d9b1ee6943de62a9f027c5d712a79cea5e12cfdfb30bb917076b7d2b4442d453","observation_id":"4393390f-4988-4145-9068-cbe78eb10b10","resolution":{"observed_at":"2026-08-10T22:40:43.269049Z","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":"2026-08-10T22:40:44.934724Z","title":null,"venue":null,"work_id":"e862e629-2905-4fc8-8d86-353810f92af4","year":1973},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.274619Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:f228b404d38a684f326079c23df203ddba1441dae85d4438d377bb301768d36e","observation_id":"6df61bb8-16c2-46fa-a1d6-41b0bca914f4","resolution":{"observed_at":"2026-08-10T22:40:44.940330Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-10T22:40:44.911397Z","title":null,"venue":null,"work_id":"72eaa85a-d040-4e32-a148-7e1717d9cc41","year":1978},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.280829Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:1ad7f10d56db66d7ee2aa61951cdae870b8a04e0ce5fd22b9bed9a0213e1b9d7","observation_id":"f9d259e1-b4cc-470e-9ffe-bfb5416e240f","resolution":{"observed_at":"2026-08-10T22:40:44.918294Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-10T22:40:44.878242Z","title":null,"venue":null,"work_id":"cfeef030-1fbf-461a-9ccd-0a3f46121725","year":2022},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.287488Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:4d84b88c54c65d0e93666db7af4d0c8351b53352250c9414aa4f45e6e213c07a","observation_id":"0fad7c13-de77-48f8-b909-c4d68ab26e12","resolution":{"observed_at":"2026-08-10T22:40:44.889954Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2109.08168","last_updated":"2022-05-12T16:08:55Z","snapshot_observed_at":"2026-07-06T11:48:32.276462Z","submitted_at":"2021-09-16T18:00:09Z","title":"Impact of Dark Compton Scattering on Direct Dark Matter Absorption Searches","version":2},"cited_work":{"arxiv_id":"2109.08168","doi":null,"metadata_source":"pith","pith_arxiv_id":"2109.08168","snapshot_observed_at":"2026-08-10T22:40:44.314731Z","title":"Impact of Dark Compton Scattering on Direct Dark Matter Absorption Searches","venue":"hep-ex","work_id":"60ce6393-be91-48b2-b6b1-c392a285246e","year":2021},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.292337Z"},"links":{"cited_paper":"/paper/2109.08168","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:5ec2c9fea2af4412e831e700cf10d602693b9b41004193cc4a1b42c4614b22b2","observation_id":"3328d54e-0b57-403f-9d6d-72b6a847bf53","resolution":{"observed_at":"2026-08-10T22:40:44.321270Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.12797","last_updated":"2025-04-07T06:47:25Z","snapshot_observed_at":"2026-07-06T18:33:07.118735Z","submitted_at":"2024-06-18T17:02:58Z","title":"Dark Photon Dark Matter Radio Signal from the Milky Way Electron Density","version":3},"cited_work":{"arxiv_id":"2406.12797","doi":null,"metadata_source":"pith","pith_arxiv_id":"2406.12797","snapshot_observed_at":"2026-08-10T22:40:44.278734Z","title":"Dark Photon Dark Matter Radio Signal from the Milky Way Electron Density","venue":"hep-ph","work_id":"a69e4c22-3938-4ace-905c-0b4e31e9441a","year":2024},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.297695Z"},"links":{"cited_paper":"/paper/2406.12797","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:695a233e68076f93e81371511d71b66bc05ee977933272d59fe44e0dd4dce2ef","observation_id":"273be84b-85ea-4430-8c68-2c92fbff0000","resolution":{"observed_at":"2026-08-10T22:40:44.288882Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1008.5119","last_updated":"2011-01-10T16:13:14Z","snapshot_observed_at":"2026-07-06T02:14:47.686794Z","submitted_at":"2010-08-30T16:54:05Z","title":"Searches for Cosmic-Ray Electron Anisotropies with the Fermi Large Area Telescope","version":3},"cited_work":{"arxiv_id":"1008.5119","doi":null,"metadata_source":"pith","pith_arxiv_id":"1008.5119","snapshot_observed_at":"2026-08-10T22:40:44.251603Z","title":"Searches for Cosmic-Ray Electron Anisotropies with the Fermi Large Area Telescope","venue":"astro-ph.HE","work_id":"961903a7-10fc-4d6d-87de-da2606215d58","year":2010},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.303333Z"},"links":{"cited_paper":"/paper/1008.5119","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:c41cff687df6b89f27b84fddc2419153250bbc8ef48ffb117e799317e685e7f6","observation_id":"bc2dfea2-23c6-45ac-9098-7cf216914a74","resolution":{"observed_at":"2026-08-10T22:40:44.258626Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1509.06249","last_updated":"2015-10-08T16:02:40Z","snapshot_observed_at":"2026-07-06T04:30:32.328264Z","submitted_at":"2015-09-21T14:47:01Z","title":"Search for anisotropies in cosmic-ray positrons detected by the PAMELA experiment","version":2},"cited_work":{"arxiv_id":"1509.06249","doi":null,"metadata_source":"pith","pith_arxiv_id":"1509.06249","snapshot_observed_at":"2026-08-10T22:40:44.216384Z","title":"Search for anisotropies in cosmic-ray positrons detected by the PAMELA experiment","venue":"astro-ph.HE","work_id":"e7a23b57-4ec6-4004-96d5-3c2b77ae4a36","year":2015},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.308754Z"},"links":{"cited_paper":"/paper/1509.06249","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:4b60089d429953a219ce9cfc64aed04b3e52f96356495fc529e5de8eb6acb6a7","observation_id":"80b41afe-4db7-435e-b8e3-b55f278d4173","resolution":{"observed_at":"2026-08-10T22:40:44.223919Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-10T22:40:44.856215Z","title":"Peter Lepage, A new algorithm for adaptive multidimensional integration, Journal of Computational Physics 27, 192 (1978)","venue":null,"work_id":"2f195c1d-f9ca-4c71-91ea-5a068f8b3c0a","year":1978},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.315626Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:08eb3d5050db682a2b41d4f4fb9f29f882ec5954c4186d18007788793e4d489d","observation_id":"1269e031-da32-46c9-b385-7e851eae2030","resolution":{"observed_at":"2026-08-10T22:40:44.863860Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.03170","last_updated":"2021-06-24T04:53:48Z","snapshot_observed_at":"2026-07-06T10:57:17.838513Z","submitted_at":"2021-04-07T14:59:56Z","title":"An Ultra-long Wavelength Sky Model with Absorption Effect","version":2},"cited_work":{"arxiv_id":"2104.03170","doi":null,"metadata_source":"pith","pith_arxiv_id":"2104.03170","snapshot_observed_at":"2026-08-10T22:40:44.185226Z","title":"An Ultra-long Wavelength Sky Model with Absorption Effect","venue":"astro-ph.GA","work_id":"17ff3c4d-d07d-44ff-9a59-b26392eeaa52","year":2021},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.320779Z"},"links":{"cited_paper":"/paper/2104.03170","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:5d6a032c9257746aea47a8a80bbaa0714d5be33424424709e029f0b06f774b85","observation_id":"50659784-b025-464f-a26d-1e04491ec382","resolution":{"observed_at":"2026-08-10T22:40:44.192023Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-08-10T22:40:43.328450Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.328450Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:e0ebba0180f1e4359e82502ce32f6039b0293b335154da5b150ab3b21bb7e06d","observation_id":"ce0d32cf-fca1-4c5e-be11-79e6c2c8e288","resolution":{"observed_at":"2026-08-10T22:40:43.328450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.4039","last_updated":"2012-02-21T15:08:57Z","snapshot_observed_at":"2026-07-06T02:43:06.181584Z","submitted_at":"2012-02-17T23:28:15Z","title":"Fermi-LAT Observations of the Diffuse Gamma-Ray Emission: Implications for Cosmic Rays and the Interstellar Medium","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.4039","snapshot_observed_at":"2026-08-10T22:40:43.336102Z","title":"Ackermann et al.(Fermi-LAT), Fermi-LAT Observations of the Diffuse Gamma-Ray Emission: Implications for Cosmic Rays and the Interstellar Medium, Astrophys","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.336102Z"},"links":{"cited_paper":"/paper/1202.4039","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:7216b127b28c300c5ca423b6cf6b2e34ed4171e8a05f302fdcf3dc4fb815148f","observation_id":"2d3ec29f-bd37-4e71-847c-905d73314923","resolution":{"observed_at":"2026-08-10T22:40:43.336102Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.3642","last_updated":"2011-08-08T17:22:45Z","snapshot_observed_at":"2026-07-06T02:14:22.545288Z","submitted_at":"2010-08-21T16:08:47Z","title":"GALPROP WebRun: an internet-based service for calculating galactic cosmic ray propagation and associated photon emissions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.3642","snapshot_observed_at":"2026-08-10T22:40:43.341310Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.341310Z"},"links":{"cited_paper":"/paper/1008.3642","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:866fc589314418368ba38c3de0934249e3f904021ca4ac7bb53dde122d63c6bd","observation_id":"31fa6f22-1957-4be3-aea6-2a292d280981","resolution":{"observed_at":"2026-08-10T22:40:43.341310Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.1171","last_updated":"2009-08-26T03:29:10Z","snapshot_observed_at":"2026-07-06T01:59:40.521117Z","submitted_at":"2009-08-08T14:29:42Z","title":"Fermi LAT Observation of Diffuse Gamma-Rays Produced Through Interactions between Local Interstellar Matter and High Energy Cosmic Rays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.1171","snapshot_observed_at":"2026-08-10T22:40:43.347087Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.347087Z"},"links":{"cited_paper":"/paper/0908.1171","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:285350e01bae6ae89dd35dd925bbfed945552c5a12c6d310034db4aeff630e65","observation_id":"a178c07e-b61e-40bd-b66b-6f9a161db449","resolution":{"observed_at":"2026-08-10T22:40:43.347087Z","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":"2026-08-10T22:40:44.836803Z","title":"Aguilar et al.(AMS), Towards Understanding the Origin of Cosmic-Ray Electrons, Phys","venue":null,"work_id":"3d3f28f7-3cca-42e3-870d-160add5c54bd","year":2019},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.354492Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:b9046b3df9590da04e2eaca7bc494f7b14cea8dcbc57da27a92468ed3bc86573","observation_id":"9f533dd1-314b-45e2-b601-030d87d3c957","resolution":{"observed_at":"2026-08-10T22:40:44.843294Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-10T22:40:44.814073Z","title":null,"venue":null,"work_id":"5ceaba85-d656-47a2-a258-9f9dbb774d5f","year":2016},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.359792Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:82b62bc8f12c68abf9d256bc727bc26fe610b7be4911be89376f4f43b508b518","observation_id":"af60c28f-476f-4392-bc22-551fe6e6a09e","resolution":{"observed_at":"2026-08-10T22:40:44.819552Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-10T22:40:44.792968Z","title":null,"venue":null,"work_id":"9a616d5e-c68b-48ed-bb5a-37985c6b2f47","year":2019},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.364936Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:2266f2521481be39af3119de516257bfe34ffdd80c4b7b8f96bf33e1b4aa949b","observation_id":"d34c0f2e-f8be-4686-9a55-76ec06222192","resolution":{"observed_at":"2026-08-10T22:40:44.800175Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9807162","last_updated":"1998-07-15T19:17:51Z","snapshot_observed_at":"2026-07-07T01:21:35.142355Z","submitted_at":"1998-07-15T19:17:51Z","title":"A New $\\Sigma-D$ Relation and Its Application to the Galactic Supernova Remnant Distribution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9807162","snapshot_observed_at":"2026-08-10T22:40:43.369946Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.369946Z"},"links":{"cited_paper":"/paper/astro-ph/9807162","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:c33ec11ceaca2fe2fcc97e1f9ab876fea9b2ef17b10551b1e8f407014df946b5","observation_id":"327c8c70-2c0a-4fef-9ee7-384b31b8d9c4","resolution":{"observed_at":"2026-08-10T22:40:43.369946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.4822","last_updated":"2011-08-24T12:21:26Z","snapshot_observed_at":"2026-07-06T02:32:52.761473Z","submitted_at":"2011-08-24T12:21:26Z","title":"The interstellar cosmic-ray electron spectrum from synchrotron radiation and direct measurements","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.4822","snapshot_observed_at":"2026-08-10T22:40:43.375431Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.375431Z"},"links":{"cited_paper":"/paper/1108.4822","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:b8a3c09c8c5a72b7ab768c42f7e540aeab8402a6912d413f385610aa84ae81c0","observation_id":"b00f44bc-1abc-425f-b444-260b31e45c9c","resolution":{"observed_at":"2026-08-10T22:40:43.375431Z","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":"2026-08-10T22:40:43.381856Z","title":null,"venue":null,"work_id":null,"year":1965},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.381856Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:dc8b7be3c98e2f0658ecbddf6b4cb8198e6ec541411f020bc1ee82e749f99421","observation_id":"36df1e6e-4650-40a2-a8ac-560d9a95d168","resolution":{"observed_at":"2026-08-10T22:40:43.381856Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.0195","last_updated":"2010-10-22T14:02:36Z","snapshot_observed_at":"2026-07-06T01:59:38.523582Z","submitted_at":"2009-08-03T06:44:01Z","title":"Implications of High-Resolution Simulations on Indirect Dark Matter Searches","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.0195","snapshot_observed_at":"2026-08-10T22:40:43.387555Z","title":"Pieri, J","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.387555Z"},"links":{"cited_paper":"/paper/0908.0195","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:1d2d29a8e9682e915707a630fd704359fabd983b64e46a37f03cc30925724e76","observation_id":"aa5da81f-957b-46b1-92f5-08345d36d42f","resolution":{"observed_at":"2026-08-10T22:40:43.387555Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.12838","last_updated":"2023-05-26T18:08:45Z","snapshot_observed_at":"2026-08-06T11:27:50.996646Z","submitted_at":"2023-03-22T18:00:08Z","title":"The dark matter profile of the Milky Way inferred from its circular velocity curve","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.12838","snapshot_observed_at":"2026-08-10T22:40:43.393296Z","title":"Ou, A.-C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.393296Z"},"links":{"cited_paper":"/paper/2303.12838","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:958d1e63f204781ba08c191123178730b03865ebed4b6b383f76422708d401d3","observation_id":"7bbbd0e5-21a4-492a-8487-df16885a5330","resolution":{"observed_at":"2026-08-10T22:40:43.393296Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.09466","last_updated":"2018-12-04T14:36:46Z","snapshot_observed_at":"2026-07-06T07:09:51.109116Z","submitted_at":"2018-10-22T18:00:09Z","title":"The Circular Velocity Curve of the Milky Way from $5$ to $25$ kpc","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.09466","snapshot_observed_at":"2026-08-10T22:40:43.398882Z","title":"Eilers, D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.398882Z"},"links":{"cited_paper":"/paper/1810.09466","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:8732215bb96b0e17317395fb19fc76aaa249d0e534edf6efe98ac4424b8ff686","observation_id":"8918bd28-9e1d-4050-9694-d5c5f3919643","resolution":{"observed_at":"2026-08-10T22:40:43.398882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.04683","last_updated":"2017-07-21T10:11:19Z","snapshot_observed_at":"2026-08-07T07:48:35.100506Z","submitted_at":"2017-03-14T19:51:43Z","title":"First constraints on fuzzy dark matter from Lyman-$\\alpha$ forest data and hydrodynamical simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.04683","snapshot_observed_at":"2026-08-10T22:40:43.406061Z","title":"Irˇ siˇ c, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.406061Z"},"links":{"cited_paper":"/paper/1703.04683","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:1ff72c0ca35362b43dee2b2607a40de1f9986eabb84d4d7e1e863c0c482512b8","observation_id":"f4149861-ed34-4711-88bf-abce66d7718c","resolution":{"observed_at":"2026-08-10T22:40:43.406061Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.09619","last_updated":"2018-09-27T15:09:06Z","snapshot_observed_at":"2026-08-04T18:06:50.114689Z","submitted_at":"2018-09-24T18:00:03Z","title":"Lyman-$\\alpha$ forest and non-linear structure characterization in Fuzzy Dark Matter cosmologies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.09619","snapshot_observed_at":"2026-08-10T22:40:43.412106Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.412106Z"},"links":{"cited_paper":"/paper/1809.09619","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:9e5d76a7f339bba43dee0823073824eb3e740dcd3f53fff904c11c195a3d3270","observation_id":"932c65a6-0f3c-406d-b555-1ef2fcaebb30","resolution":{"observed_at":"2026-08-10T22:40:43.412106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.08297","last_updated":"2017-02-24T21:01:45Z","snapshot_observed_at":"2026-07-06T05:16:05.217762Z","submitted_at":"2016-10-26T12:25:05Z","title":"Ultralight scalars as cosmological dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.08297","snapshot_observed_at":"2026-08-10T22:40:43.418637Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.418637Z"},"links":{"cited_paper":"/paper/1610.08297","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:e856a7123e7a04ff0dd41ab2b9fffb8a7f147f6b82dc7b7fe716e5cabbac9df3","observation_id":"09d672b5-1e33-472f-84c6-a29fb884935a","resolution":{"observed_at":"2026-08-10T22:40:43.418637Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.05503","last_updated":"2020-07-16T01:48:23Z","snapshot_observed_at":"2026-08-09T14:59:24.847697Z","submitted_at":"2020-01-15T19:00:02Z","title":"The Subhalo Mass Function and Ultralight Bosonic Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.05503","snapshot_observed_at":"2026-08-10T22:40:43.425192Z","title":"Schutz, Subhalo mass function and ultralight bosonic dark matter, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.425192Z"},"links":{"cited_paper":"/paper/2001.05503","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:f58ab6af8c74552dc7c5e61f6cd3bb6543cf12493f4d38aba12fbb1c4aa59688","observation_id":"8d44e327-e922-41ec-982e-8c6dbe4813f5","resolution":{"observed_at":"2026-08-10T22:40:43.425192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.00022","last_updated":"2021-03-01T18:00:36Z","snapshot_observed_at":"2026-07-06T09:43:35.929296Z","submitted_at":"2020-07-31T18:13:09Z","title":"Milky Way Satellite Census. III. Constraints on Dark Matter Properties from Observations of Milky Way Satellite Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.00022","snapshot_observed_at":"2026-08-10T22:40:43.430530Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.430530Z"},"links":{"cited_paper":"/paper/2008.00022","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:4e44a5120e3f8ab07c2f2e94fa4cf0fa23fe20623923e36e704f2f23c0942c86","observation_id":"24dbb617-385b-49f8-963b-496f6f0bdb52","resolution":{"observed_at":"2026-08-10T22:40:43.430530Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.05750","last_updated":"2022-03-18T18:12:55Z","snapshot_observed_at":"2026-08-06T02:23:04.745088Z","submitted_at":"2022-03-11T04:42:06Z","title":"Not so fuzzy: excluding FDM with sizes and stellar kinematics of ultra-faint dwarf galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.05750","snapshot_observed_at":"2026-08-10T22:40:43.436672Z","title":"Dalal and A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.436672Z"},"links":{"cited_paper":"/paper/2203.05750","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:4bc114ec0333cadbda9cfff79b9efedfcfc909d0d2a31cf35385f7a98f54f768","observation_id":"7c57851b-5374-4e4a-b79d-949c608e0674","resolution":{"observed_at":"2026-08-10T22:40:43.436672Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.10919","last_updated":"2019-06-12T14:07:05Z","snapshot_observed_at":"2026-07-06T07:23:46.396438Z","submitted_at":"2018-12-28T07:59:11Z","title":"Galactic Center Gas Clouds and Novel Bounds on Ultra-Light Dark Photon, Vector Portal, Strongly Interacting, Composite, and Super-Heavy Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.10919","snapshot_observed_at":"2026-08-10T22:40:43.441973Z","title":"Bhoonah, J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.441973Z"},"links":{"cited_paper":"/paper/1812.10919","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:cf6fc165b9d244b58f44eae8954b2b3fdb1832e0f47ad3f860492139575906a9","observation_id":"61fac84f-342c-4ab7-9a19-f2194a8f7b64","resolution":{"observed_at":"2026-08-10T22:40:43.441973Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.12190","last_updated":"2021-06-30T18:00:02Z","snapshot_observed_at":"2026-08-10T18:50:17.084766Z","submitted_at":"2019-03-28T18:00:19Z","title":"Gas-rich dwarf galaxies as a new probe of dark matter interactions with ordinary matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.12190","snapshot_observed_at":"2026-08-10T22:40:43.447438Z","title":"Wadekar and G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.447438Z"},"links":{"cited_paper":"/paper/1903.12190","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:bc59266c6183873646de64b93cd37ce1a5efe3e8ca9714320553ca1e3855f0d7","observation_id":"208c855f-37a2-4ac5-b75c-b4d2900bf8ce","resolution":{"observed_at":"2026-08-10T22:40:43.447438Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.08852","last_updated":"2021-11-30T06:19:41Z","snapshot_observed_at":"2026-08-06T04:48:34.824598Z","submitted_at":"2021-08-19T18:00:01Z","title":"Search for dark-photon dark matter in the SuperMAG geomagnetic field dataset","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.08852","snapshot_observed_at":"2026-08-10T22:40:43.452933Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.452933Z"},"links":{"cited_paper":"/paper/2108.08852","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:fb73dc54c42cc6645e538b769170e8c42f2b6f22cca5bdf2b301027ee647aff2","observation_id":"95aa9eef-bf1d-4507-b0aa-6e3581db2d1f","resolution":{"observed_at":"2026-08-10T22:40:43.452933Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.16045","last_updated":"2024-12-26T16:03:14Z","snapshot_observed_at":"2026-07-06T19:07:20.444206Z","submitted_at":"2024-08-28T18:00:00Z","title":"Search for ultralight dark matter in the SuperMAG high-fidelity dataset","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.16045","snapshot_observed_at":"2026-08-10T22:40:43.459212Z","title":"Friel, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.459212Z"},"links":{"cited_paper":"/paper/2408.16045","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:8be865a738012e4bdcd954d430bdeed4ab9b01920b06e8427503abd95202b6cb","observation_id":"ec92563a-cb60-4a8a-9425-1f732dd5cb14","resolution":{"observed_at":"2026-08-10T22:40:43.459212Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.05086","last_updated":"2020-03-25T15:04:15Z","snapshot_observed_at":"2026-08-09T23:03:58.203586Z","submitted_at":"2019-11-12T19:00:02Z","title":"The Cosmological Evolution of Light Dark Photon Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.05086","snapshot_observed_at":"2026-08-10T22:40:43.467836Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.467836Z"},"links":{"cited_paper":"/paper/1911.05086","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:faff7694fa3f72edba6d03178299a3f8e86e3419a68fd9714b859556d4c04c87","observation_id":"1cf2a568-2d60-4586-acec-b8690d72778e","resolution":{"observed_at":"2026-08-10T22:40:43.467836Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.13698","last_updated":"2020-06-22T07:58:58Z","snapshot_observed_at":"2026-07-06T09:08:28.873280Z","submitted_at":"2020-03-30T18:00:01Z","title":"Dark Photon Dark Matter in the Presence of Inhomogeneous Structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.13698","snapshot_observed_at":"2026-08-10T22:40:43.474507Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.474507Z"},"links":{"cited_paper":"/paper/2003.13698","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:08a66f585cda7966f6cae66251ad563fbecd422c3d3e4782e629e1e747516b21","observation_id":"d454582b-8e94-4252-8c3c-ea7dfc434445","resolution":{"observed_at":"2026-08-10T22:40:43.474507Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.06733","last_updated":"2020-04-26T08:54:47Z","snapshot_observed_at":"2026-08-08T05:14:38.571947Z","submitted_at":"2020-04-14T18:00:04Z","title":"Modeling Dark Photon Oscillations in Our Inhomogeneous Universe","version":2},"cited_work":{"arxiv_id":"2004.06733","doi":null,"metadata_source":"pith","pith_arxiv_id":"2004.06733","snapshot_observed_at":"2026-08-10T22:40:43.691860Z","title":"Modeling Dark Photon Oscillations in Our Inhomogeneous Universe","venue":"astro-ph.CO","work_id":"0b4e7461-d116-463c-af85-27428c523a38","year":2020},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.482418Z"},"links":{"cited_paper":"/paper/2004.06733","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:d1633bab9cb66453d22bc4d12869d4142c32793f37f1dd0c377330691bfd0d52","observation_id":"251f98a9-3c6d-4f7d-ac7b-0322602148c8","resolution":{"observed_at":"2026-08-10T22:40:43.698754Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.05165","last_updated":"2020-12-09T20:41:38Z","snapshot_observed_at":"2026-08-05T17:17:58.990846Z","submitted_at":"2020-02-12T19:00:00Z","title":"Dark Photon Oscillations in Our Inhomogeneous Universe","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.05165","snapshot_observed_at":"2026-08-10T22:40:43.489319Z","title":"Caputo, H","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.489319Z"},"links":{"cited_paper":"/paper/2002.05165","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:9ac72b85c35f5fc7e086af77f5ee8e836e92ee5bd4567840f18918d7dc94744f","observation_id":"98b0526e-5a22-4889-9ab8-36301c108a07","resolution":{"observed_at":"2026-08-10T22:40:43.489319Z","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":"2026-08-10T22:40:44.758867Z","title":"Kasper, T","venue":null,"work_id":"fe6144cc-190f-4392-aa82-ae585a721654","year":2022},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.498706Z"},"links":{"citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:fba8e260e617e06de6c92dc72bba3e1ad83b5df90ff109a68a28f90896c8da79","observation_id":"cfccba01-1fb8-4730-8e33-44f0f9d0f5b5","resolution":{"observed_at":"2026-08-10T22:40:44.766802Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.10245","last_updated":"2017-10-27T17:11:38Z","snapshot_observed_at":"2026-07-06T06:06:28.684685Z","submitted_at":"2017-10-27T17:11:38Z","title":"NOIRE Study Report: Towards a Low Frequency Radio Interferometer in Space","version":1},"cited_work":{"arxiv_id":"1710.10245","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.10245","snapshot_observed_at":"2026-08-10T22:40:43.627667Z","title":"NOIRE Study Report: Towards a Low Frequency Radio Interferometer in Space","venue":"astro-ph.IM","work_id":"70dbfaf4-3b72-413c-be31-84eefb08f729","year":2017},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.504312Z"},"links":{"cited_paper":"/paper/1710.10245","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:c3e925cf55ce0bddc2e6999e6015f94dc2c6cba3735fc070ca6f0f734c95bfbc","observation_id":"c5ba26b4-c470-4e54-96e7-df03cba1841a","resolution":{"observed_at":"2026-08-10T22:40:43.633934Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.16409","last_updated":"2024-03-25T03:56:19Z","snapshot_observed_at":"2026-07-06T17:49:52.751335Z","submitted_at":"2024-03-25T03:56:19Z","title":"Large-scale Array for Radio Astronomy on the Farside","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.16409","snapshot_observed_at":"2026-08-10T22:40:43.510341Z","title":"Chen et al., Large-scale Array for Radio Astronomy on the Farside, Phil","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.510341Z"},"links":{"cited_paper":"/paper/2403.16409","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:89c771ce1e1fbfed98016ac35434f0ddf8a37f529af8c2459316e02be6a20c81","observation_id":"2f938d66-a863-40a8-b1e0-125a5562a680","resolution":{"observed_at":"2026-08-10T22:40:43.510341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.07173","last_updated":"2024-07-09T18:37:26Z","snapshot_observed_at":"2026-08-06T09:24:51.733544Z","submitted_at":"2024-07-09T18:37:26Z","title":"LuSEE-Night power requirements and power generation strategy","version":1},"cited_work":{"arxiv_id":"2407.07173","doi":null,"metadata_source":"pith","pith_arxiv_id":"2407.07173","snapshot_observed_at":"2026-08-10T22:40:43.572511Z","title":"LuSEE-Night power requirements and power generation strategy","venue":"astro-ph.IM","work_id":"3a74c936-02ac-42de-b905-f14f15e7076d","year":2024},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.517056Z"},"links":{"cited_paper":"/paper/2407.07173","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:d67a35a16590cc8b2125baa08024ff81fb2828a8ceb1a19d565fc103ebcea5aa","observation_id":"866d7823-a710-4146-b13e-e09ec6556379","resolution":{"observed_at":"2026-08-10T22:40:43.580857Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter"},"reference_resolution":{"displayed":64,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":51,"verified_exact":10,"verified_fuzzy":3},"total_outbound_references":64},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 64 of 64 outbound references and 1 inbound Pith citation observation for arXiv:2501.01489."}