{"as_of":"2026-08-05T02:06:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f57a2a0d83242822c476b971616917384ca6bd09c982d81c2edadc56774f214c","coverage":[{"denominator":56,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":56,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-14T01:22:04.712990Z","state":"measured"},{"denominator":56,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":56,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-04T06:34:03.388597+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2603.28528/citation-record","integrity":"/paper/2603.28528/integrity","json":"/paper/2603.28528/citation-record.json","paper":"/paper/2603.28528"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"This study could not confirm previous claims of TeV halo emission from MSPs [21]","venue":null,"work_id":"b35ce3ab-19b3-486b-bc21-a590d597c7dd","year":2024},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:5a5cdb0d1ac824c887820d415867f12019d1f415b046daa14de42bea729936d4","observation_id":"7e636558-761d-4466-9327-69f38a02f811","resolution":{"observed_at":"2026-05-14T01:23:36.629468Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":"The complete sample of spider MSPs for which we search for TeV emission in HAWC data thus consists of 43 MSPs","venue":null,"work_id":"3aee8d5e-4ed3-4ae5-a8d3-8304e4bb2b9d","year":1903},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:49d521e2e78a99f57d47e6f31f6ab62e1736a597ec7f91b2e16409e2e6739c51","observation_id":"223c4657-b6ba-49f4-993c-1aa1abaf1649","resolution":{"observed_at":"2026-05-14T01:23:36.634256Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"5750e5cc-1085-47a0-80b5-488502711440","year":null},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:dc582f05c15bb533a1d3f28c9e12cec3aecb68c33d53c0be002a146a2fdad803","observation_id":"9f478268-2a43-4f09-94b1-bf17f10b6adf","resolution":{"observed_at":"2026-05-14T01:23:36.625099Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.11132","last_updated":"2023-07-20T16:23:37Z","snapshot_observed_at":"2026-07-06T15:56:38.019661Z","submitted_at":"2023-07-20T16:23:37Z","title":"The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars","version":1},"cited_work":{"arxiv_id":"2307.11132","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2307.11132","snapshot_observed_at":"2026-07-01T16:35:50.825468Z","title":"A., Abdollahi, S., Ajello, M., et al","venue":null,"work_id":"e427fcc9-bc82-41cb-93a3-9b3e5a0f82e8","year":2023},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2307.11132","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:00ed0c476cd8f4140f427156ea507b74139bc65b3f3f85bc0dfaf81b80003c27","observation_id":"589dd812-03b0-469c-be7a-d15d0cd40dbd","resolution":{"observed_at":"2026-05-14T01:23:34.857656Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1510.07048","last_updated":"2018-12-05T08:22:24Z","snapshot_observed_at":"2026-07-06T04:34:05.413579Z","submitted_at":"2015-10-23T20:05:32Z","title":"Teraelectronvolt pulsed emission from the Crab pulsar detected by MAGIC","version":2},"cited_work":{"arxiv_id":"1510.07048","doi":null,"metadata_source":"pith","pith_arxiv_id":"1510.07048","snapshot_observed_at":"2026-06-29T05:23:07.632108Z","title":"Ansoldi et al","venue":"astro-ph.HE","work_id":"2bce65a0-fede-43c8-afa4-c2cce125461a","year":2015},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/1510.07048","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:887ef82b9c1ec20aedca910d753b943e7f61235ece840ae53fa8ad32cc3efe23","observation_id":"35b7b02f-3c62-4bf1-8781-c42b7295245c","resolution":{"observed_at":"2026-05-14T01:23:34.868950Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2310.06181","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Aharonian et al","venue":null,"work_id":"2484cab2-3f13-42e0-915e-991e35ce6a67","year":2023},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:5040f83ea898e76ff02034033e94255669593512b4cfdc271a97bc649adcfe05","observation_id":"b4e96970-9169-4a95-9112-4423afe3b462","resolution":{"observed_at":"2026-05-14T01:23:34.785452Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2202.06899","last_updated":"2022-02-14T17:45:33Z","snapshot_observed_at":"2026-07-06T12:37:39.880827Z","submitted_at":"2022-02-14T17:45:33Z","title":"Gamma-ray halos around pulsars as the key to understanding cosmic ray transport in the Galaxy","version":1},"cited_work":{"arxiv_id":"2202.06899","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2202.06899","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"L´ opez-Coto, E","venue":null,"work_id":"e017774b-7de7-4f01-aeef-8829a7cbee0f","year":2022},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2202.06899","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:68f552fc76e9b9fc457c7a8fbee36cbac7953a67422eebcd7e4c7bae86c6fc23","observation_id":"59737545-0a1c-47ba-8fc5-bb93962eaf71","resolution":{"observed_at":"2026-05-14T01:23:34.799557Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.04011","last_updated":"2022-07-08T17:02:16Z","snapshot_observed_at":"2026-07-06T13:29:20.200379Z","submitted_at":"2022-07-08T17:02:16Z","title":"The Physics of Pulsar Halos: Research Progress and Prospect","version":1},"cited_work":{"arxiv_id":"2207.04011","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.04011","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Liu, Int","venue":null,"work_id":"ba124556-1c23-4830-b1a4-7487c30188f5","year":2022},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2207.04011","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:4124b2e6bb22ede29fa8c1430df0198dccc4999aed68273f73e9a671030cbf8f","observation_id":"85677393-dbfb-4de7-a1d8-56c318b26afe","resolution":{"observed_at":"2026-05-14T01:23:34.545957Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.13294","last_updated":"2022-09-27T10:33:29Z","snapshot_observed_at":"2026-07-06T13:56:46.961863Z","submitted_at":"2022-09-27T10:33:29Z","title":"Gamma-ray Pulsar Halos in the Galaxy","version":1},"cited_work":{"arxiv_id":"2209.13294","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2209.13294","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Fang, Front","venue":null,"work_id":"d5308f3b-299a-4174-ad2a-3ff37f9cce65","year":2022},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2209.13294","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:92c9d5aa0b077a5984ea0b17c3f3bdf87617819da31586a61833c10e3b4398e9","observation_id":"a5b7297d-581c-40ca-93e8-e580418b3a81","resolution":{"observed_at":"2026-05-14T01:23:34.792879Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.00659","last_updated":"2024-09-01T08:19:36Z","snapshot_observed_at":"2026-07-30T15:13:43.823033Z","submitted_at":"2024-09-01T08:19:36Z","title":"Gamma-ray halos around pulsars: impact on pulsar wind physics and galactic cosmic ray transport","version":1},"cited_work":{"arxiv_id":"2409.00659","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.00659","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Amato and S","venue":null,"work_id":"6baed8f9-209e-4986-b200-de7a4872717f","year":2024},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2409.00659","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:06bb558c9d9001a51b72fe2a7458fa886156e1a562b0cc312a9b20393844e82a","observation_id":"15ede37c-130f-46a0-9eab-21914141045d","resolution":{"observed_at":"2026-05-14T01:23:34.609559Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06223","last_updated":"2017-11-16T18:05:58Z","snapshot_observed_at":"2026-07-06T06:09:53.105661Z","submitted_at":"2017-11-16T18:05:58Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","version":1},"cited_work":{"arxiv_id":"1711.06223","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.06223","snapshot_observed_at":"2026-07-07T22:14:11.724134Z","title":"Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth","venue":"astro-ph.HE","work_id":"b520aeb4-1f31-495b-958d-05007de45598","year":2017},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/1711.06223","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:cf574080ddf043ed25d7bdf4534b5e585860bb1d2016cbfe84412fb5f7830bbe","observation_id":"6f709017-4141-46ca-a532-25ac3b7bdc72","resolution":{"observed_at":"2026-05-14T01:23:34.675858Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":"Albert et al","venue":null,"work_id":"9b4f9223-0c0b-48a1-bdd9-53a1182a4c50","year":2024},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:fc0d509e3a59f398dd48c1b91aabd98d6402e28cb2f6f54e8f1058fdd9ea67b4","observation_id":"86e90c81-38e1-4d8a-b7b9-532b7b4d955c","resolution":{"observed_at":"2026-05-14T01:23:36.615794Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.02631","last_updated":"2023-04-05T17:54:59Z","snapshot_observed_at":"2026-07-06T15:12:37.953383Z","submitted_at":"2023-04-05T17:54:59Z","title":"Detection of extended gamma-ray emission around the Geminga pulsar with H.E.S.S","version":1},"cited_work":{"arxiv_id":"2304.02631","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2304.02631","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Aharonian et al","venue":null,"work_id":"78fc3b5c-ce02-4cd4-979c-926a9bcde79c","year":2023},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2304.02631","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:f58e926a5b80bf639ac4b120592587395bc3aafe6591f21f0c0a00df33351b3f","observation_id":"a4b6c42a-4631-4c9e-9c33-9b6ecb049b0f","resolution":{"observed_at":"2026-05-14T01:23:34.509036Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.00175","last_updated":"2025-04-30T20:47:53Z","snapshot_observed_at":"2026-07-06T21:17:19.119854Z","submitted_at":"2025-04-30T20:47:53Z","title":"Extended TeV Halos May Commonly Exist around Middle-Aged Pulsars","version":1},"cited_work":{"arxiv_id":"2505.00175","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.00175","snapshot_observed_at":"2026-07-10T04:46:46.680301Z","title":"Albert et al., Phys","venue":"astro-ph.HE","work_id":"01131b34-a6c9-43a7-bd02-356a088e437b","year":2025},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2505.00175","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:a3136b7b3d2b495398a0a799b919b3253c80ed701ea39d6a18eb6ec6c2cd3d05","observation_id":"8dfe9047-0979-480e-bf5a-fff34c3e2877","resolution":{"observed_at":"2026-05-14T01:23:34.577640Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.11955","last_updated":"2021-04-13T18:00:01Z","snapshot_observed_at":"2026-07-06T10:07:25.152925Z","submitted_at":"2020-10-22T18:00:01Z","title":"Galactic factories of cosmic-ray electrons and positrons","version":2},"cited_work":{"arxiv_id":"2010.11955","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.11955","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Evoli, E","venue":null,"work_id":"962ba5fd-206c-48a7-8e75-23f8505c0b56","year":2021},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2010.11955","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:8586d9f5aed4e9e8a0c3176747f74c02724a2abca6bf6b1563dc91e0079c9305","observation_id":"0ddfb212-c876-47d3-af89-a20f49205443","resolution":{"observed_at":"2026-05-14T01:23:34.711625Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2001.09985","last_updated":"2020-01-30T18:32:13Z","snapshot_observed_at":"2026-07-06T08:53:02.820171Z","submitted_at":"2020-01-27T18:59:59Z","title":"Contribution of pulsars to cosmic-ray positrons in light of recent observation of inverse-Compton halos","version":2},"cited_work":{"arxiv_id":"2001.09985","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2001.09985","snapshot_observed_at":"2026-07-04T14:09:52.800787Z","title":"Manconi, M","venue":null,"work_id":"a804b7e5-6d9f-4503-bea1-983928bda841","year":2020},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2001.09985","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:942c51da321d9ced1d2fd83428739fa840d39b44de6c41b0b515deca4ef7cfbe","observation_id":"cf106f1f-1ca1-40d7-a411-d0317eeb33e6","resolution":{"observed_at":"2026-05-14T01:23:34.490249Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10951","last_updated":"2025-02-13T19:00:01Z","snapshot_observed_at":"2026-07-06T19:33:21.541657Z","submitted_at":"2024-10-14T18:00:01Z","title":"Disclosing the catalog pulsars dominating the Galactic positron flux","version":2},"cited_work":{"arxiv_id":"2410.10951","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.10951","snapshot_observed_at":"2026-07-01T16:35:50.861720Z","title":"Orusa, S","venue":null,"work_id":"fa62f1a2-7637-4e69-98cc-bc7938d25397","year":2025},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2410.10951","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:a4778e08b18f1457675f2f8ca26576db5dd15d7cffa991e45e6a017b005c1624","observation_id":"48f425c2-a2c2-4362-9f7e-0029aadea975","resolution":{"observed_at":"2026-05-14T01:23:34.453761Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.05751","last_updated":"2021-01-14T17:50:20Z","snapshot_observed_at":"2026-07-06T10:32:36.184855Z","submitted_at":"2021-01-14T17:50:20Z","title":"The Emission Physics of Millisecond Pulsars","version":1},"cited_work":{"arxiv_id":"2101.05751","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2101.05751","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"70559706-e8db-4d65-ae8e-69ace9b7aa87","year":2022},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2101.05751","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:8f629236d6d0bd2cee9ed8e47bb9b9e19bcdf7c5d573f843c7fe78c83c73d154","observation_id":"b066f8c8-385d-470c-9ea1-76ab254c2990","resolution":{"observed_at":"2026-05-14T01:23:34.598023Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"cda70b6a-ab66-4191-9fa3-8dd013a4abac","year":2021},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:14c3a7023197a652e0adfec862f954de3a038cd4888b4a9315b0e8a0c4140d51","observation_id":"a127f281-7eef-4cae-842d-322c9e080cda","resolution":{"observed_at":"2026-05-14T01:23:36.572626Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2102.00061","last_updated":"2021-09-26T21:47:24Z","snapshot_observed_at":"2026-07-06T10:36:57.153159Z","submitted_at":"2021-01-29T20:50:23Z","title":"Evidence for a high-energy tail in the gamma-ray spectra of globular clusters","version":3},"cited_work":{"arxiv_id":"2102.00061","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2102.00061","snapshot_observed_at":"2026-06-30T15:54:49.086853Z","title":null,"venue":null,"work_id":"c8c5057d-fe84-49a8-b2e8-e1c2765d1218","year":2021},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2102.00061","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:35118b628c7b52410ead126c3450544d97cdb0be454cd97858fb1b17015e8e32","observation_id":"ceabc14d-05a9-4a80-9c55-3efb7d4dc9fc","resolution":{"observed_at":"2026-05-14T01:23:34.820773Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.21641","last_updated":"2025-03-27T16:07:22Z","snapshot_observed_at":"2026-08-04T09:57:22.437507Z","submitted_at":"2025-03-27T16:07:22Z","title":"A possible GeV-TeV connection in the direction of the Globular Cluster UKS 1","version":1},"cited_work":{"arxiv_id":"2503.21641","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.21641","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"5707e06d-b214-4093-a599-a0183471659f","year":2025},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2503.21641","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:5a4953b82c70303be007fd211fb11fcde98b251f263fac8823dbd5166d95d043","observation_id":"694dbf16-81bc-42ca-8a8a-c6f579e45568","resolution":{"observed_at":"2026-05-14T01:23:34.848667Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"22e87783-73b2-40cc-9f07-93e9fcfdde38","year":2025},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:fdac79f2b930dc36c2144b8b2adf600858e57cda4cbf34b3351415e021ff91fb","observation_id":"0a2187bc-5c2b-4b20-965c-d4b19bd9de09","resolution":{"observed_at":"2026-05-14T01:23:36.544466Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.00014","last_updated":"2021-03-31T18:00:03Z","snapshot_observed_at":"2026-07-06T10:55:25.433719Z","submitted_at":"2021-03-31T18:00:03Z","title":"Evidence of TeV Halos Around Millisecond Pulsars","version":1},"cited_work":{"arxiv_id":"2104.00014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2104.00014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Hooper and T","venue":null,"work_id":"389dc3d5-0a15-4866-a55e-76b673edd36e","year":2022},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2104.00014","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:a29d9c7e49fadb8a2d92fedb1f98dcaab4d8edfff5215ca9d372a91bb1b3a915","observation_id":"bcbd194d-e62d-4a34-b9d6-e57b746de63e","resolution":{"observed_at":"2026-05-14T01:23:34.734051Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"3bab8899-185e-4344-8801-e794b019be00","year":2011},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:7b152d8453e0f9e85c60eca3e0f54bc8c40164d2a0799a6485bdc386bb707abb","observation_id":"84d652b1-e949-4e1c-b5e3-99b7e4f87f6a","resolution":{"observed_at":"2026-05-14T01:23:36.551760Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2505.11691","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"a637c4e3-92b8-44b8-946e-0f3996e90150","year":2025},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:39aa64bd3df2ece964ea2edc9a125b38ce7fc3a4483ee903b0568c694824ccbe","observation_id":"955d6447-5c2a-4643-9a9b-34fd50a4d32d","resolution":{"observed_at":"2026-05-14T01:23:34.695879Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01705","last_updated":"2021-08-03T18:59:46Z","snapshot_observed_at":"2026-07-06T11:35:14.629601Z","submitted_at":"2021-08-03T18:59:46Z","title":"\"Spider\" Millisecond Pulsar Binaries as Potential TeV Emitters","version":1},"cited_work":{"arxiv_id":"2108.01705","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.01705","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Wadiasingh, C","venue":null,"work_id":"8513093e-738c-4f89-b3c8-943330ff53ac","year":2021},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2108.01705","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:8e0470997524ebb1348b3149b3a8599d88a6a28cd24562d5bf2513e5e2b75341","observation_id":"9e4e63bb-3664-480c-9af8-9eb24ffc2021","resolution":{"observed_at":"2026-05-14T01:23:34.746830Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.00023","last_updated":"2022-02-28T19:00:05Z","snapshot_observed_at":"2026-07-06T12:42:34.337026Z","submitted_at":"2022-02-28T19:00:05Z","title":"Global Kinetic Modeling of the Intrabinary Shock in Spider Pulsars","version":1},"cited_work":{"arxiv_id":"2203.00023","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2203.00023","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cort´ es and L","venue":null,"work_id":"3a7717a4-b585-43eb-96c6-4303bc8030f2","year":2022},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2203.00023","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:01248477c0116b23e2940c3913f1d5ff396fb42ce59e33f0354419a5002c53eb","observation_id":"e6d57413-b3dc-4ed6-9f67-dcf8d1030c96","resolution":{"observed_at":"2026-05-14T01:23:34.557961Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.02674","last_updated":"2024-02-05T02:19:31Z","snapshot_observed_at":"2026-07-06T17:25:14.115360Z","submitted_at":"2024-02-05T02:19:31Z","title":"Modeling X-ray and gamma-ray emission from redback pulsar binaries","version":1},"cited_work":{"arxiv_id":"2402.02674","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2402.02674","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"3c756620-377a-4d22-9251-0bb96796d65d","year":2024},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2402.02674","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:29df5cadbde2edf7157cb451ce09c1df1cdc9220fc1eff204e365c44b99afe45","observation_id":"2365b94f-beaa-4452-91de-506fd30c93b1","resolution":{"observed_at":"2026-05-14T01:23:34.682744Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.18663","last_updated":"2025-01-03T17:50:54Z","snapshot_observed_at":"2026-08-04T05:21:43.043816Z","submitted_at":"2024-06-26T18:03:42Z","title":"Enhanced particle acceleration in a pulsar wind interacting with a companion","version":2},"cited_work":{"arxiv_id":"2406.18663","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2406.18663","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Richard-Romei and B","venue":null,"work_id":"eeed7623-5fbe-4ca8-91bf-ffa920bc0962","year":2024},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2406.18663","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:7a5893f0f06d5a783ca0334b1e2506dcb0209364a3bf73ed9033b16a61a20cd5","observation_id":"0684982d-8cb9-414c-b3d3-023b418a6219","resolution":{"observed_at":"2026-05-14T01:23:34.835030Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.06988","last_updated":"2019-12-15T06:38:33Z","snapshot_observed_at":"2026-07-06T08:44:35.683645Z","submitted_at":"2019-12-15T06:38:33Z","title":"High Energy Radiation from Spider Pulsars","version":1},"cited_work":{"arxiv_id":"1912.06988","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.06988","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"4c475e20-c0e5-49a6-b3f7-5fb28bbfa058","year":2019},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/1912.06988","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:2c4eed5cbb9d04a2a248629f3198939f7e01891c7d1145046c24df5f8b79e5e9","observation_id":"8d7c2811-ab68-4ac8-8bfe-9cd4fd9388f9","resolution":{"observed_at":"2026-05-14T01:23:34.722812Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":"Abeysekara et al., Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrome- ters, Detectors and Associated Equipment1052, 168253 (2025)","venue":null,"work_id":"2194633b-2caa-428a-adf9-b104f5683e8c","year":2025},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:b9fbd8ebe6298120f77b3af973689de546f2f154d619bf2fdcf51798360b55d0","observation_id":"1888f78f-75ff-4838-90a6-606258668a6e","resolution":{"observed_at":"2026-05-14T01:23:36.540430Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1708.04032","last_updated":"2017-08-14T08:28:00Z","snapshot_observed_at":"2026-07-06T05:55:07.983254Z","submitted_at":"2017-08-14T08:28:00Z","title":"HAWC High Energy Upgrade with a Sparse Outrigger Array","version":1},"cited_work":{"arxiv_id":"1708.04032","doi":"10.22323/1.301.0806","metadata_source":"pith","pith_arxiv_id":"1708.04032","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"HAWC High Energy Upgrade with a Sparse Outrigger Array","venue":"astro-ph.IM","work_id":"6c7e7748-1248-43b5-911e-e2f0bf0cdea7","year":2017},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/1708.04032","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:95c1d15de22d26e827917714f52fe1f79bcdf240a09ef51bcc5e074e0f0b72d5","observation_id":"db902adc-108a-476c-b38a-dea4813da508","resolution":{"observed_at":"2026-05-14T01:23:34.841588Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":"Albert et al., The Astrophysical Journal972, 144 (2024), publisher: The American Astronomical Society","venue":null,"work_id":"057aed67-2fdd-4fd7-9ca4-ef0e7cd5eb10","year":2024},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:1dca6daf2cecf102030676427d4369865ccf939f90032ba5db18fabb6c6521cd","observation_id":"e802aab6-cc15-4c02-90ce-1ddf3d22cd99","resolution":{"observed_at":"2026-05-14T01:23:36.582425Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1507.08343","last_updated":"2015-07-29T23:29:00Z","snapshot_observed_at":"2026-07-06T04:25:18.071224Z","submitted_at":"2015-07-29T23:29:00Z","title":"The Multi-Mission Maximum Likelihood framework (3ML)","version":1},"cited_work":{"arxiv_id":"1507.08343","doi":"10.48550/arxiv.1507.08343","metadata_source":"pith","pith_arxiv_id":"1507.08343","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"The Multi-Mission Maximum Likelihood framework (3ML)","venue":"astro-ph.HE","work_id":"75e7f5ac-c7fb-480b-9dc8-779c4561ff18","year":2015},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/1507.08343","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:d707c8be2ccbcb970625dbc51e729b0a388150721e064edcf355f621f8211b3a","observation_id":"cd8ce8e7-e388-48aa-8d8e-413033ed035f","resolution":{"observed_at":"2026-05-14T01:23:34.813658Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":"Abeysekara et al., PoSICRC2021, 828 (2021)","venue":null,"work_id":"70905b17-0d59-48f4-ad44-ebefe5d1aa8b","year":2021},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:fd0d9fb3bec00dbfe4eb3680227520c4766d74d83f3e8f75a59d5ae592cf520c","observation_id":"e2244ecf-3a0b-4920-b483-c9c0fcfcf257","resolution":{"observed_at":"2026-05-14T01:23:36.567448Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":"Brun and F","venue":null,"work_id":"7772de4b-d0c3-4060-85ad-15adddb252e9","year":1997},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:514d1ab56ce4dfd5dcce20b3238a5f458dbcc959eb35ee91e9fb3b24ca0f8dee","observation_id":"88606ebd-0bfd-482b-a377-2d41eebb9a6b","resolution":{"observed_at":"2026-05-14T01:23:36.558701Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0412641","last_updated":"2004-12-28T06:23:19Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2004-12-28T06:23:19Z","title":"The ATNF Pulsar Catalogue","version":1},"cited_work":{"arxiv_id":"astro-ph/0412641","doi":"10.1086/428488","metadata_source":"pith","pith_arxiv_id":"astro-ph/0412641","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"N., Hobbs G","venue":"astro-ph","work_id":"07a5f92c-6d52-4a6a-a928-14b1ed893f48","year":2004},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/astro-ph/0412641","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:50b6b76678987a428f5160fcd54d4d8b734e196104249030998536bd22697817","observation_id":"061f9556-0063-4ca2-9beb-75198a3cfe8a","resolution":{"observed_at":"2026-05-14T01:23:34.378837Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-11T18:20:25.108793+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T18:20:25.108793+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":"Morello et al., Monthly Notices of the Royal Astro- nomical Society483, 3673 (2019)","venue":null,"work_id":"de84a3f1-5ff3-4980-bd96-1273cf479a6d","year":2019},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:bfabffceaec6ae34b8cdf248689dbcfb5a7fbf52c4dcf1e7e3171962a461d8b5","observation_id":"69a3a376-07ce-4560-9089-454be3ad34f0","resolution":{"observed_at":"2026-05-14T01:23:36.605090Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"ce48bdea-236c-406f-ab0f-e58019955598","year":1938},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:5d033af0b0df6f10c1911849f8314ff89ea9bbd70a29d8beae61fc50128632fd","observation_id":"d86bd529-e876-454f-a8a6-a3167db615af","resolution":{"observed_at":"2026-05-14T01:23:36.599131Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"e2dfada0-e1c1-459b-bcf2-7045198550aa","year":2017},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:96735856273876b21adf61713cb673c38aa76cf9fbaa34aad2f4122e92d656bf","observation_id":"d30db13d-719c-49b3-a70c-6f643a03c2be","resolution":{"observed_at":"2026-05-14T01:23:36.610299Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1701.01778","last_updated":"2017-01-06T23:43:53Z","snapshot_observed_at":"2026-07-06T05:25:21.010274Z","submitted_at":"2017-01-06T23:43:53Z","title":"Observation of the Crab Nebula with the HAWC Gamma-Ray Observatory","version":1},"cited_work":{"arxiv_id":"1701.01778","doi":null,"metadata_source":"pith","pith_arxiv_id":"1701.01778","snapshot_observed_at":"2026-07-01T02:05:14.253523Z","title":"Observation of the Crab Nebula with the HAWC Gamma-Ray Observatory","venue":"astro-ph.HE","work_id":"ad72a58e-b1ff-4de9-90a8-7aa2d64084a1","year":2017},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/1701.01778","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:856152cc4aa20c49647203fd295412bca1b6e7abb3c685deafacf7b032f8f600","observation_id":"3b704c7c-90b1-4c0b-bf0b-c9895d178096","resolution":{"observed_at":"2026-05-14T01:23:34.466428Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":"Groetsch and The HAWC Collaboration Team (2023) p","venue":null,"work_id":"b439ff63-916f-4606-a9ca-7f4549d92e86","year":2023},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:5d9c2c8438826c8add7ffed2b0808e3814d9d03b5caa91158f8d8994d830b4c1","observation_id":"7b2353bd-7fff-4792-8a7d-f24829257d46","resolution":{"observed_at":"2026-05-14T01:23:36.577044Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"e8810103-2095-43d7-a9fc-d5ec48b32763","year":1988},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:3e88afeadca1468ff82823e5ac4cb55aeceb603c28004f0e6bdf5169149a20c8","observation_id":"d7b994a1-cd8b-4019-ab18-3457b9a08c42","resolution":{"observed_at":"2026-05-14T01:23:36.587074Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"1706.01378","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"06eca93c-23ab-4b1e-b43f-36b6607ab8d6","year":2017},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:2ab0383fd3a0e976a6da59e8993609204c19611dec8d7f75f945857d5124385d","observation_id":"e45f7148-8610-4e95-834e-654c0402ea74","resolution":{"observed_at":"2026-05-14T01:23:34.805915Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.01125","last_updated":"2020-10-02T17:49:51Z","snapshot_observed_at":"2026-07-06T10:01:03.641960Z","submitted_at":"2020-10-02T17:49:51Z","title":"X-ray Through Very-High-Energy Intrabinary Shock Emission from Black Widows and Redbacks","version":1},"cited_work":{"arxiv_id":"2010.01125","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.01125","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"3571b325-9071-4d6a-a321-793661cd4dc0","year":2020},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2010.01125","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:96a528939e258eef27db057a86e26f1f02d421c60c6a60e70f3dd41b180c418b","observation_id":"1519ef1e-874b-4295-bd35-5b15f6024d80","resolution":{"observed_at":"2026-05-14T01:23:34.656980Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"5a0f3851-a4c3-4f01-89b0-2d22e58c5fc5","year":2014},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:47a4848315290906613ada646dabdaf9860f0ffd8aa7ee2f631770a0db813da5","observation_id":"43dbf91f-1551-49fb-afdf-2ebe0ec7a2ae","resolution":{"observed_at":"2026-05-14T01:23:36.620261Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.09060","last_updated":"2020-10-21T15:50:42Z","snapshot_observed_at":"2026-07-06T10:05:32.402496Z","submitted_at":"2020-10-18T18:39:30Z","title":"Transitional millisecond pulsars","version":2},"cited_work":{"arxiv_id":"2010.09060","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.09060","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Papitto and D","venue":null,"work_id":"92c9d6b7-724b-4d2b-88cc-0a083150eff1","year":2021},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2010.09060","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:6f1dd5994c6aa11997f6be950c4dfa81bfbf9155d5076a20d343e2b22b3a0bc0","observation_id":"4bb62ffd-54d7-4ea2-ba45-b97be86b99cd","resolution":{"observed_at":"2026-05-14T01:23:34.767032Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2508.20952","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Vecchiotti and M","venue":null,"work_id":"61b9eb48-ef82-4449-9b25-37692ad21f4d","year":2025},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:239894b1cc44259464cae4b34016430a350528ce1e7775c02940682e7a3c7836","observation_id":"e0554036-b6ce-488b-a7e4-5684ddf56059","resolution":{"observed_at":"2026-05-14T01:23:34.531546Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+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":"2026-06-05T21:23:00.469572Z","title":"L´ opez-Oramas (CTAO), EPJ Web Conf.319, 01002 (2025)","venue":null,"work_id":"a599e9b1-0778-4d05-8518-d789f2cb10e7","year":2025},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:c777e83fe0a8280ad7b5148e4ca2c9f0e5caa2493b2a80cd8f87871fc2b2c9e5","observation_id":"9ee607b2-0c1a-4170-a21c-29d3c05d8be8","resolution":{"observed_at":"2026-05-14T01:23:36.563883Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.04733","last_updated":"2024-05-24T10:47:26Z","snapshot_observed_at":"2026-07-06T17:26:43.251349Z","submitted_at":"2024-02-07T10:35:31Z","title":"The Galactic center excess at the highest energies: morphology and photon-count statistics","version":2},"cited_work":{"arxiv_id":"2402.04733","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2402.04733","snapshot_observed_at":"2026-07-01T16:35:50.780017Z","title":"Manconi, F","venue":null,"work_id":"a0b7df2f-342d-4b6c-8e90-25cf15c4408e","year":2024},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2402.04733","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:65946a01cd83b891822193c020c0b7444a7e173b2681352bc1565a6b3d320341","observation_id":"b3bf4595-065b-4465-a15e-66653da5ca57","resolution":{"observed_at":"2026-05-14T01:23:34.521539Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2106.00222","last_updated":"2022-05-02T10:20:11Z","snapshot_observed_at":"2026-07-06T11:14:37.660839Z","submitted_at":"2021-06-01T04:26:34Z","title":"Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal","version":2},"cited_work":{"arxiv_id":"2106.00222","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2106.00222","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Gautam, R","venue":null,"work_id":"68d81d39-e316-43ed-befc-01f55afb722e","year":2022},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2106.00222","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:afc853bcf6fe9bb7e1863c4a1948a9c9a2ff98bfa1c3efd2ac6a306d0e513f83","observation_id":"e6349608-f601-473f-ae54-f40598175b2b","resolution":{"observed_at":"2026-05-14T01:23:34.482306Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2102.05648","last_updated":"2021-06-26T13:05:17Z","snapshot_observed_at":"2026-07-06T10:40:18.796086Z","submitted_at":"2021-02-10T18:59:42Z","title":"Cherenkov Telescope Array sensitivity to the putative millisecond pulsar population responsible for the Galactic center excess","version":3},"cited_work":{"arxiv_id":"2102.05648","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2102.05648","snapshot_observed_at":"2026-07-01T16:35:50.864062Z","title":"Macias, H","venue":null,"work_id":"666dae63-2a02-4d20-a2ee-3166b48281c8","year":2021},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2102.05648","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:5c990cbec995b5b02ff23c72a610ebb2bc484ae9f7ab9fa34f11892191d05ff5","observation_id":"7944451c-302a-467a-9414-ba7a0bbc003f","resolution":{"observed_at":"2026-05-14T01:23:34.590009Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.12574","last_updated":"2023-04-25T05:01:41Z","snapshot_observed_at":"2026-07-06T15:19:39.223171Z","submitted_at":"2023-04-25T05:01:41Z","title":"Constraints on the $e^{\\pm }$ Pair Injection of Pulsar Halos: Implications from the Galactic Diffuse Multi-TeV Gamma-ray Emission","version":1},"cited_work":{"arxiv_id":"2304.12574","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2304.12574","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Yan and R.-Y","venue":null,"work_id":"129b5278-82ee-49c2-b93d-4525fba4e525","year":2023},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2304.12574","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:04ea5c24adf390a1eff76b0883064bd96ee1eea6591c0df8f8e03d24ef93a8b5","observation_id":"baafa4a1-41fe-47ab-bbff-c9c85b36837e","resolution":{"observed_at":"2026-05-14T01:23:34.758344Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.00051","last_updated":"2024-10-16T18:12:22Z","snapshot_observed_at":"2026-07-06T15:36:07.713593Z","submitted_at":"2023-05-31T18:00:00Z","title":"Diffuse Ultra-High-Energy Gamma-Ray Emission From TeV Halos","version":2},"cited_work":{"arxiv_id":"2306.00051","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2306.00051","snapshot_observed_at":"2026-07-03T02:57:35.326678Z","title":"Dekker, I","venue":null,"work_id":"b367414f-87c8-4f0c-b0bb-0832765a6f12","year":2024},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2306.00051","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:6ef9cb3083f04a06ec0b520a67545f6b7ce6affa7d243816ba6531ac754ff71e","observation_id":"9af742ac-0f64-405f-a251-3d73fb21138b","resolution":{"observed_at":"2026-05-14T01:23:34.498868Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.02828","last_updated":"2024-07-16T10:14:33Z","snapshot_observed_at":"2026-07-06T16:27:39.431612Z","submitted_at":"2023-10-04T13:52:46Z","title":"Prospects for a survey of the Galactic plane with the Cherenkov Telescope Array","version":2},"cited_work":{"arxiv_id":"2310.02828","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2310.02828","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Abe et al","venue":null,"work_id":"54175483-96c7-4835-b0f6-6ab8b0bb68bd","year":null},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2310.02828","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:3408395ad7740b2d78e607ebb2e685ed3023c4a64c1b09ab8c7524b719c443b6","observation_id":"a70af944-20fc-4d74-9b21-a2cb0dda5f4b","resolution":{"observed_at":"2026-05-14T01:23:34.567961Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03731","last_updated":"2024-07-27T10:11:58Z","snapshot_observed_at":"2026-07-06T17:40:29.558340Z","submitted_at":"2024-03-06T14:20:39Z","title":"Detection prospects of very and ultra high-energy gamma rays from extended sources with ASTRI, CTA, and LHAASO","version":2},"cited_work":{"arxiv_id":"2403.03731","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2403.03731","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Celli and G","venue":null,"work_id":"1108c119-61fe-4b8d-80fa-074a3aff315c","year":2024},"citing_paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-14T01:22:04.712990Z"},"links":{"cited_paper":"/paper/2403.03731","citing_paper":"/paper/2603.28528"},"observation_digest":"sha256:073da04bd8b06621d16655e353343f5f1c4f0276dfb6c8a70769a509d88743a9","observation_id":"cac7292c-fd44-48e7-bb16-b0cba752b0ad","resolution":{"observed_at":"2026-05-14T01:23:34.646250Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2603.28528","last_updated":"2026-03-30T14:53:58Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T22:51:05.074191Z","submitted_at":"2026-03-30T14:53:58Z","title":"Search for TeV emission from spider millisecond pulsars with HAWC"},"reference_resolution":{"displayed":56,"state_counts":{"malformed_identifier":2,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":8,"verified_exact":37,"verified_fuzzy":8},"total_outbound_references":56},"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":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 56 of 56 outbound references and 0 inbound Pith citation observations for arXiv:2603.28528."}