{"as_of":"2026-08-15T07:19:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:295b54786e1f6284d0b8109ebe7daf226b594be0c71865b259a586379ac8e36c","coverage":[{"denominator":39,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":39,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-10T05:30:29.237097Z","state":"measured"},{"denominator":39,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":39,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+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/2607.08552/citation-record","integrity":"/paper/2607.08552/integrity","json":"/paper/2607.08552/citation-record.json","paper":"/paper/2607.08552"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T05:36:48.910788Z","title":null,"venue":null,"work_id":"adb7bda5-2d04-4edf-ae64-6657d8aa0bc0","year":null},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:275414ea69f1c7468b9a23ff429a7dca07f461177c8f97052579aff947cc938b","observation_id":"0424f15f-4998-410e-b33e-65aac96dc6fd","resolution":{"observed_at":"2026-07-10T05:36:48.912164Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+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":"2026-07-10T05:36:48.908900Z","title":null,"venue":null,"work_id":"8a33cf4c-241d-4ae0-a951-47c9a0a6be1d","year":null},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:057758fd3877e8de9ec1aba24e2b48fbaac4079e03a6c0f354f2c2fa0e93c34e","observation_id":"5d2d5e15-774c-4cb2-893f-0264e12effee","resolution":{"observed_at":"2026-07-10T05:36:48.910246Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.5281/zenodo.21280724","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T05:36:48.441053Z","title":null,"venue":null,"work_id":"66f2970c-d72f-47c7-b05a-9f3957aaf415","year":null},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:bdf5147f2cf0d45ff8358bf4f897dca982500f7ccb7ff5c5fb1e8bc41445bb55","observation_id":"ad9ca35d-9a6a-45e1-b13f-2bd45d5882a9","resolution":{"observed_at":"2026-07-10T05:36:48.442227Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-07-18T00:50:57.404667+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-18T00:50:57.404667+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0404175","last_updated":"2004-08-13T15:46:27Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2004-04-21T13:12:59Z","title":"Particle Dark Matter: Evidence, Candidates and Constraints","version":2},"cited_work":{"arxiv_id":"hep-ph/0404175","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0404175","snapshot_observed_at":"2026-07-10T14:47:14.453944Z","title":"Particle Dark Matter: Evidence, Candidates and Constraints","venue":"hep-ph","work_id":"9f1f415a-e524-408a-8b8d-07c41bbab6c3","year":2004},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/hep-ph/0404175","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:c916a49b48aa5ec37ac35eb16dee0bbe29496d0e9eec9d93f97c41945f66c8d0","observation_id":"481ddeb8-cfc5-4e1e-8a50-538f00443c54","resolution":{"observed_at":"2026-07-10T05:36:48.632647Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1204.3622","last_updated":"2012-08-10T02:38:16Z","snapshot_observed_at":"2026-08-15T04:12:53.089037Z","submitted_at":"2012-04-16T20:00:00Z","title":"Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation","version":3},"cited_work":{"arxiv_id":"1204.3622","doi":"10.1103/physrevd.86.023506","metadata_source":"pith","pith_arxiv_id":"1204.3622","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation","venue":"hep-ph","work_id":"c78e99c0-7e5c-4920-a7f2-bcb57dc2b3b9","year":2012},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1204.3622","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:df50aa06a7b6730f094fc30940d00ef18c7c600082780635974dc70205836ff2","observation_id":"daf82591-60e6-4d9c-b301-81ea8f4c3c40","resolution":{"observed_at":"2026-07-10T05:36:48.608274Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1003.0904","last_updated":"2010-04-09T18:39:59Z","snapshot_observed_at":"2026-08-15T05:25:01.034020Z","submitted_at":"2010-03-04T00:36:02Z","title":"Dark Matter Candidates from Particle Physics and Methods of Detection","version":2},"cited_work":{"arxiv_id":"1003.0904","doi":null,"metadata_source":"pith","pith_arxiv_id":"1003.0904","snapshot_observed_at":"2026-07-10T05:36:48.633826Z","title":"Dark Matter Candidates from Particle Physics and Methods of Detection","venue":"astro-ph.CO","work_id":"41aa3f7d-d51d-47ac-ae55-7153be74cec8","year":2010},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1003.0904","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:85ba23042eb29b5741d95f3d6c318a180d0052105cf90e9c78d8a65f703aab94","observation_id":"5b826883-b456-41d3-bfd7-11778aaf974d","resolution":{"observed_at":"2026-07-10T05:36:48.635156Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0910.2998","last_updated":"2009-11-11T19:55:59Z","snapshot_observed_at":"2026-08-15T05:36:33.173253Z","submitted_at":"2009-10-15T21:24:10Z","title":"Possible Evidence For Dark Matter Annihilation In The Inner Milky Way From The Fermi Gamma Ray Space Telescope","version":2},"cited_work":{"arxiv_id":"0910.2998","doi":null,"metadata_source":"pith","pith_arxiv_id":"0910.2998","snapshot_observed_at":"2026-07-10T05:36:48.622431Z","title":"Possible Evidence For Dark Matter Annihilation In The Inner Milky Way From The Fermi Gamma Ray Space Telescope","venue":"hep-ph","work_id":"6ea4082c-358a-4ddf-b65b-c52d17b2de89","year":2009},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/0910.2998","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:f759e0b1b58922fc26f88eec761f6d9a8d0379f42f103d13dba8f7585db99225","observation_id":"f68f5d0b-5ae7-47cf-9adc-65f1bf776ac2","resolution":{"observed_at":"2026-07-10T05:36:48.623944Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1409.0042","last_updated":"2014-08-29T21:36:33Z","snapshot_observed_at":"2026-08-14T23:21:24.067462Z","submitted_at":"2014-08-29T21:36:33Z","title":"Background model systematics for the Fermi GeV excess","version":1},"cited_work":{"arxiv_id":"1409.0042","doi":null,"metadata_source":"pith","pith_arxiv_id":"1409.0042","snapshot_observed_at":"2026-07-10T05:36:48.641925Z","title":"Background model systematics for the Fermi GeV excess","venue":"astro-ph.CO","work_id":"1568e9a0-c97c-4f3f-a251-1058270f8540","year":2014},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1409.0042","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:34d52aba5b5e029f720448fa4be867262f3503c2453a1ffa3d658e4ce804b94c","observation_id":"dee59ece-3cfa-4a29-9af7-86a6ee6b59b3","resolution":{"observed_at":"2026-07-10T05:36:48.643267Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1704.03910","last_updated":"2017-06-26T10:22:12Z","snapshot_observed_at":"2026-08-14T21:06:59.365897Z","submitted_at":"2017-04-12T19:37:39Z","title":"The Fermi Galactic Center GeV Excess and Implications for Dark Matter","version":2},"cited_work":{"arxiv_id":"1704.03910","doi":null,"metadata_source":"pith","pith_arxiv_id":"1704.03910","snapshot_observed_at":"2026-07-10T05:36:48.617625Z","title":"The Fermi Galactic Center GeV Excess and Implications for Dark Matter","venue":"astro-ph.HE","work_id":"5501006c-58a1-4c1d-ab5e-34e8e4a35935","year":2017},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1704.03910","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:83e0c2f1e43161b9c10cd79d51681a5d9d7f06c179adf8a2f924fb9c6f0fc103","observation_id":"f9708672-deb2-4b91-b71d-3d467f805b85","resolution":{"observed_at":"2026-07-10T05:36:48.618850Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1506.05104","last_updated":"2016-03-09T20:54:13Z","snapshot_observed_at":"2026-08-14T22:44:10.201285Z","submitted_at":"2015-06-16T20:00:31Z","title":"Strong support for the millisecond pulsar origin of the Galactic center GeV excess","version":3},"cited_work":{"arxiv_id":"1506.05104","doi":"10.1103/physrevlett.116.051102","metadata_source":"pith","pith_arxiv_id":"1506.05104","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Strong support for the millisecond pulsar origin of the Galactic center GeV excess","venue":"astro-ph.HE","work_id":"999843a5-b8c9-4589-8b52-a02aa8aeb7c8","year":2015},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1506.05104","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:31630577c46a4a40f71ac3885739ac60729fcc0a4f3479865384f80f9a45fbcc","observation_id":"e661eb3c-8e19-441f-95b9-99ac453a7a6f","resolution":{"observed_at":"2026-07-10T05:36:48.621360Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-07-13T22:20:00.300309+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T22:20:00.300309+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2507.07209","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T05:36:48.574154Z","title":"Totani, JCAP11, 080 (2025), arXiv:2507.07209 [astro-ph.HE]","venue":null,"work_id":"618cc28f-84c1-497e-899a-68903ffe2e91","year":2025},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:366b190584eba0c9918e958858bf092734581db66447fbbb29a485bf08ea6c7c","observation_id":"7d711dac-18d0-415a-9a13-eb8f22248c5d","resolution":{"observed_at":"2026-07-10T05:36:48.576152Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0902.1089","last_updated":"2009-02-06T17:44:53Z","snapshot_observed_at":"2026-08-15T05:55:34.030006Z","submitted_at":"2009-02-06T17:44:53Z","title":"The Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission","version":1},"cited_work":{"arxiv_id":"0902.1089","doi":null,"metadata_source":"pith","pith_arxiv_id":"0902.1089","snapshot_observed_at":"2026-07-10T23:57:44.372413Z","title":"The Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission","venue":"astro-ph.IM","work_id":"fabe2f87-380f-4f82-aafa-bad10d9fbcf0","year":2009},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/0902.1089","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:1c2c896e842632e11cf4b33533f3f296c99036626b708896fafe3e64935f94aa","observation_id":"98b5fbaa-a08a-457d-b532-7230567fd75a","resolution":{"observed_at":"2026-07-10T05:36:48.572669Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1005.5480","last_updated":"2010-10-18T02:18:46Z","snapshot_observed_at":"2026-08-15T05:17:48.169311Z","submitted_at":"2010-05-29T20:24:37Z","title":"Giant Gamma-ray Bubbles from Fermi-LAT: AGN Activity or Bipolar Galactic Wind?","version":3},"cited_work":{"arxiv_id":"1005.5480","doi":null,"metadata_source":"pith","pith_arxiv_id":"1005.5480","snapshot_observed_at":"2026-07-10T05:36:48.614952Z","title":"Giant Gamma-ray Bubbles from Fermi-LAT: AGN Activity or Bipolar Galactic Wind?","venue":"astro-ph.HE","work_id":"31f8b786-e510-4208-be51-a2a56e077d20","year":2010},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1005.5480","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:e4db80bd218149b4703ca8ee9b878b26e1499d3cf3b6f0a426d727bb7eb8d381","observation_id":"b7335b8c-3add-4ad1-889c-a86b90bc2cf4","resolution":{"observed_at":"2026-07-10T05:36:48.616498Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9508025","last_updated":"1995-08-07T09:36:00Z","snapshot_observed_at":"2026-07-07T01:11:37.947406Z","submitted_at":"1995-08-07T09:36:00Z","title":"The Structure of Cold Dark Matter Halos","version":1},"cited_work":{"arxiv_id":"astro-ph/9508025","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9508025","snapshot_observed_at":"2026-07-10T10:07:00.979456Z","title":"The Structure of Cold Dark Matter Halos","venue":"astro-ph","work_id":"89221cc3-65d9-4b41-ba70-b312d3068679","year":1995},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/astro-ph/9508025","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:357570611ce86eb960b57ef6ddc202f81651519167f7f7582f9b98aadb63aed2","observation_id":"215b880b-2afd-4260-9aea-f2cea05d763c","resolution":{"observed_at":"2026-07-10T05:36:48.613759Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1503.02641","last_updated":"2015-11-03T08:32:32Z","snapshot_observed_at":"2026-08-15T06:01:32.317256Z","submitted_at":"2015-03-09T19:41:42Z","title":"Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi-LAT Data","version":2},"cited_work":{"arxiv_id":"1503.02641","doi":null,"metadata_source":"pith","pith_arxiv_id":"1503.02641","snapshot_observed_at":"2026-07-10T05:36:48.650180Z","title":"Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi-LAT Data","venue":"astro-ph.HE","work_id":"90bee6f9-64d9-4bca-931c-fc2f82cf9b01","year":2015},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1503.02641","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:05fbb2210fee033a8948f1dfb3414cbbacf9f55983551d934a22486995d9fccd","observation_id":"609dc7fe-0ede-485c-9fe2-9f5d128bbf94","resolution":{"observed_at":"2026-07-10T05:36:48.652057Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1812.06986","last_updated":"2020-02-12T14:28:44Z","snapshot_observed_at":"2026-08-15T01:46:25.331821Z","submitted_at":"2018-12-17T19:00:02Z","title":"A Global Analysis of Dark Matter Signals from 27 Dwarf Spheroidal Galaxies using 11 Years of Fermi-LAT Observations","version":2},"cited_work":{"arxiv_id":"1812.06986","doi":null,"metadata_source":"pith","pith_arxiv_id":"1812.06986","snapshot_observed_at":"2026-07-10T05:36:48.628116Z","title":"A Global Analysis of Dark Matter Signals from 27 Dwarf Spheroidal Galaxies using 11 Years of Fermi-LAT Observations","venue":"astro-ph.CO","work_id":"26a2f0ce-1a4f-4bc8-b983-01718900918d","year":2018},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1812.06986","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:f907883765ef7fdd0e68260b6f16d029b90a576e99eacc93147bd71f2eaff046","observation_id":"aae9a59e-4c62-4098-8387-66bc4de65db8","resolution":{"observed_at":"2026-07-10T05:36:48.629789Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.04982","last_updated":"2023-11-08T19:03:43Z","snapshot_observed_at":"2026-08-13T05:29:35.854950Z","submitted_at":"2023-11-08T19:03:43Z","title":"Legacy Analysis of Dark Matter Annihilation from the Milky Way Dwarf Spheroidal Galaxies with 14 Years of Fermi-LAT Data","version":1},"cited_work":{"arxiv_id":"2311.04982","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.04982","snapshot_observed_at":"2026-07-10T05:36:48.639289Z","title":"McDaniel, M","venue":"astro-ph.HE","work_id":"c79c0f0a-0b4c-4cd4-ba69-eca255f5a1b2","year":2023},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/2311.04982","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:52dd99ce707ee70c1a001cf59ded7a4331cbfe6f6c5f4cc439e4c24c9299b52b","observation_id":"e23648df-3829-4e15-8ef0-c6bd1464f3f9","resolution":{"observed_at":"2026-07-10T05:36:48.640736Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.3514","last_updated":"2013-03-14T17:01:50Z","snapshot_observed_at":"2026-08-15T00:25:10.041836Z","submitted_at":"2013-03-14T17:01:50Z","title":"Pass 8: Toward the Full Realization of the Fermi-LAT Scientific Potential","version":1},"cited_work":{"arxiv_id":"1303.3514","doi":"10.48550/arxiv.1303.3514","metadata_source":"pith","pith_arxiv_id":"1303.3514","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2013, arXiv e-prints","venue":"astro-ph.IM","work_id":"6842139e-8fad-4249-9d9d-0c9bd9da8971","year":2013},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1303.3514","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:b97c1e4d2e7159319285dc5ee2ef5e983f1eeb527312a16ea98bd357e30cae41","observation_id":"223b439f-94a0-45db-99b9-38513878d1d7","resolution":{"observed_at":"2026-07-10T05:36:48.655478Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-10T17:08:20.513766+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-10T17:08:20.513766+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1202.4039","last_updated":"2012-02-21T15:08:57Z","snapshot_observed_at":"2026-08-15T04:18:56.120471Z","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":"1202.4039","doi":null,"metadata_source":"pith","pith_arxiv_id":"1202.4039","snapshot_observed_at":"2026-07-10T05:36:48.587664Z","title":"Fermi-LAT Observations of the Diffuse Gamma-Ray Emission: Implications for Cosmic Rays and the Interstellar Medium","venue":"astro-ph.HE","work_id":"613d5716-fd29-4f0b-b9d6-ac2127a814b4","year":2012},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1202.4039","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:484cbdd67f8e3b2187e47ac091de400e9741f291960696dac2348716f169fad5","observation_id":"c5349c39-ea3e-4163-a0d0-563c4bf87647","resolution":{"observed_at":"2026-07-10T05:36:48.588972Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10045","last_updated":"2020-05-26T08:45:05Z","snapshot_observed_at":"2026-08-15T05:26:22.509315Z","submitted_at":"2019-02-26T16:43:19Z","title":"Fermi Large Area Telescope Fourth Source Catalog","version":6},"cited_work":{"arxiv_id":"1902.10045","doi":null,"metadata_source":"pith","pith_arxiv_id":"1902.10045","snapshot_observed_at":"2026-07-10T05:36:48.568509Z","title":"2019, arXiv e-prints","venue":"astro-ph.HE","work_id":"6848a8b5-0197-4aab-b774-4d7cf0a21088","year":2019},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1902.10045","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:551aa9ad7725b1b45f43ae28ce7d8938e2914d4c2c2db36cdebf3a843fbad734","observation_id":"56cb5ed7-aa7b-4247-9be7-e9635628dd00","resolution":{"observed_at":"2026-07-10T05:36:48.569794Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.12546","last_updated":"2024-07-24T16:42:02Z","snapshot_observed_at":"2026-08-06T19:02:53.102574Z","submitted_at":"2023-07-24T06:24:23Z","title":"Fermi Large Area Telescope Fourth Source Catalog Data Release 4 (4FGL-DR4)","version":4},"cited_work":{"arxiv_id":"2307.12546","doi":"10.1088/0004-637x/721/2/1425","metadata_source":"pith","pith_arxiv_id":"2307.12546","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Fermi Large Area Telescope Fourth Source Catalog Data Release 4 (4FGL-DR4)","venue":"astro-ph.HE","work_id":"94d0b83b-a894-42a6-a62f-14989213ad60","year":2023},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/2307.12546","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:810e2d394517517c75d85a8081202beb72e415b0037a2a2631f5964a26cce7c7","observation_id":"7f5afd42-8df7-4d88-9cf8-b26eaa8faf56","resolution":{"observed_at":"2026-07-10T05:36:48.563705Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1202.3665","last_updated":"2013-11-25T15:56:48Z","snapshot_observed_at":"2026-07-06T02:43:00.981478Z","submitted_at":"2012-02-16T20:41:19Z","title":"emcee: The MCMC Hammer","version":4},"cited_work":{"arxiv_id":"1202.3665","doi":"10.1086/670067arxiv:1202.3665","metadata_source":"pith","pith_arxiv_id":"1202.3665","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"emcee: The MCMC Hammer","venue":"astro-ph.IM","work_id":"f9cc095b-e709-4c96-bccc-ffcef3254dbe","year":2012},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1202.3665","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:0964fd1abe7e43cd400cf37a0b84f17d2d5d67f3d60e675e521d279c0ca69da8","observation_id":"8d7109b1-d341-4ada-b929-4ebeb71bf636","resolution":{"observed_at":"2026-07-10T05:36:48.637980Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+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":"2026-07-10T05:36:48.907097Z","title":null,"venue":null,"work_id":"19c152f8-e72a-454c-ba9c-d850c1051941","year":1995},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:bf9942b2b3848bdcf446ed8867b77a557d7325b691089ea05e580601b14ef57d","observation_id":"31f3e001-0d1b-489b-bec6-eeec2e50309f","resolution":{"observed_at":"2026-07-10T05:36:48.908354Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+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":"2026-07-10T05:36:48.904942Z","title":null,"venue":null,"work_id":"7298dd7a-74a4-4c87-8fa3-f3d64e0a9816","year":1997},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:aae41fcabd7a1ac591c2477ad7175ebbd8243f7384a6410147cc08eaf4c8fc1a","observation_id":"d37eafab-c533-48c6-8d53-8c836439ffa6","resolution":{"observed_at":"2026-07-10T05:36:48.906379Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1305.4385","last_updated":"2013-09-24T13:11:03Z","snapshot_observed_at":"2026-08-15T00:17:21.254509Z","submitted_at":"2013-05-19T17:57:51Z","title":"The Second Fermi Large Area Telescope Catalog of Gamma-ray Pulsars","version":3},"cited_work":{"arxiv_id":"1305.4385","doi":null,"metadata_source":"pith","pith_arxiv_id":"1305.4385","snapshot_observed_at":"2026-07-10T05:36:48.603692Z","title":"The Second Fermi Large Area Telescope Catalog of Gamma-ray Pulsars","venue":"astro-ph.HE","work_id":"4f00bc92-0478-43f3-8480-bb961a1a4261","year":2013},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1305.4385","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:54d30fcebaf9592f9674706bf571b241c5caef0bbf2eff1196f057cb14e65610","observation_id":"45dcc827-1c3d-490e-afca-46545e3760b7","resolution":{"observed_at":"2026-07-10T05:36:48.604954Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1012.4515","last_updated":"2012-08-21T07:57:42Z","snapshot_observed_at":"2026-08-15T04:59:24.645522Z","submitted_at":"2010-12-21T00:19:58Z","title":"PPPC 4 DM ID: A Poor Particle Physicist Cookbook for Dark Matter Indirect Detection","version":4},"cited_work":{"arxiv_id":"1012.4515","doi":null,"metadata_source":"pith","pith_arxiv_id":"1012.4515","snapshot_observed_at":"2026-07-10T05:36:48.644515Z","title":"PPPC 4 DM ID: A Poor Particle Physicist Cookbook for Dark Matter Indirect Detection","venue":"hep-ph","work_id":"083ec8e5-16a7-48bf-9ddd-7ef1d811e5f6","year":2010},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1012.4515","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:61e3939110b2bffd461125919bb4b9145941f8e4ce18447e7a6b3df1e73d7d69","observation_id":"8471d502-038f-47e7-bcfd-1b6b274bd12f","resolution":{"observed_at":"2026-07-10T05:36:48.646047Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.13197","last_updated":"2020-07-31T18:32:23Z","snapshot_observed_at":"2026-08-09T02:16:33.503348Z","submitted_at":"2019-09-29T03:31:20Z","title":"Effective $J$-factors for Milky Way dwarf spheroidal galaxies with velocity-dependent annihilation","version":4},"cited_work":{"arxiv_id":"1909.13197","doi":null,"metadata_source":"pith","pith_arxiv_id":"1909.13197","snapshot_observed_at":"2026-07-10T05:36:48.577486Z","title":"Effective $J$-factors for Milky Way dwarf spheroidal galaxies with velocity-dependent annihilation","venue":"astro-ph.CO","work_id":"501007b9-9c70-4f89-9f61-0a6962dea416","year":2019},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1909.13197","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:abfcd6b2eea8b4d58baea772752bed3fc500084e258e37fa173476af75ffcd32","observation_id":"85275d73-0fc3-4c9a-8b98-59662948973e","resolution":{"observed_at":"2026-07-10T05:36:48.578800Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1702.00408","last_updated":"2017-06-17T01:42:20Z","snapshot_observed_at":"2026-08-14T21:18:25.623020Z","submitted_at":"2017-02-01T19:00:05Z","title":"Sommerfeld-Enhanced $J$-Factors For Dwarf Spheroidal Galaxies","version":2},"cited_work":{"arxiv_id":"1702.00408","doi":null,"metadata_source":"pith","pith_arxiv_id":"1702.00408","snapshot_observed_at":"2026-07-10T05:36:48.601279Z","title":"Sommerfeld-Enhanced $J$-Factors For Dwarf Spheroidal Galaxies","venue":"astro-ph.CO","work_id":"d491c534-6106-4c01-a5ad-b00b3cad9245","year":2017},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1702.00408","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:0ad57275e4ff2c29ccc8e22718bcac26883e4d39f815564e46a75ee9978b9f8e","observation_id":"4d1eb544-2d28-4c98-87e2-4859227eb311","resolution":{"observed_at":"2026-07-10T05:36:48.602507Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1005.4678","last_updated":"2010-09-28T22:03:43Z","snapshot_observed_at":"2026-08-15T05:18:09.302841Z","submitted_at":"2010-05-25T20:00:02Z","title":"Sommerfeld Enhancements for Thermal Relic Dark Matter","version":3},"cited_work":{"arxiv_id":"1005.4678","doi":null,"metadata_source":"pith","pith_arxiv_id":"1005.4678","snapshot_observed_at":"2026-07-10T05:36:48.580248Z","title":"Sommerfeld Enhancements for Thermal Relic Dark Matter","venue":"hep-ph","work_id":"5700bd67-a784-4b96-82ea-665bcdd119a7","year":2010},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1005.4678","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:4f1ddf7982c0f948a11f8f9d2fa62b0aa21b804c6c168c15dd5a057fe4785995","observation_id":"62e42542-2e41-46d1-83e2-0516a575fdd3","resolution":{"observed_at":"2026-07-10T05:36:48.581619Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0812.0072","last_updated":"2008-11-29T13:18:30Z","snapshot_observed_at":"2026-07-06T01:51:39.587171Z","submitted_at":"2008-11-29T13:18:30Z","title":"Breit-Wigner Enhancement of Dark Matter Annihilation","version":1},"cited_work":{"arxiv_id":"0812.0072","doi":null,"metadata_source":"pith","pith_arxiv_id":"0812.0072","snapshot_observed_at":"2026-07-10T05:36:48.598960Z","title":"Breit-Wigner Enhancement of Dark Matter Annihilation","venue":"hep-ph","work_id":"27ce3eaf-d8cf-486e-9470-7facc94a3cef","year":2008},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/0812.0072","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:e355fc3d3a43c1aee1c7ae4b4099430ea51120ca7df3ec3900d45338df027519","observation_id":"b7c7d870-eaeb-4e93-abfb-0a9b8f7e86fd","resolution":{"observed_at":"2026-07-10T05:36:48.600133Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0901.1450","last_updated":"2009-03-04T14:54:12Z","snapshot_observed_at":"2026-08-15T05:57:42.558653Z","submitted_at":"2009-01-11T15:25:33Z","title":"Enhancement of Dark Matter Annihilation via Breit-Wigner Resonance","version":2},"cited_work":{"arxiv_id":"0901.1450","doi":null,"metadata_source":"pith","pith_arxiv_id":"0901.1450","snapshot_observed_at":"2026-07-10T05:36:48.595874Z","title":"Enhancement of Dark Matter Annihilation via Breit-Wigner Resonance","venue":"hep-ph","work_id":"2705c0bc-7d51-443a-a448-c366074cfbdd","year":2009},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/0901.1450","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:dce04fa6d79b4d310d02580f674e769a47110fed843bcbd7a1fa2a9a761b639c","observation_id":"5a71b815-094e-4d37-9cee-9a57cd82d9e4","resolution":{"observed_at":"2026-07-10T05:36:48.597731Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2512.01404","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T05:36:48.565623Z","title":"Resonant Annihilation of WIMP Dark Matter for Halo Gamma Ray Signal","venue":null,"work_id":"a2b6809a-9a3b-4a61-97b6-1f95f17e1dc4","year":2025},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:5a5e231914b517148f60e91f24604b6043d2635dbece92eaf7aa53cce890bfde","observation_id":"87c5aefd-4d0d-4d5f-ac43-f12f5b8dd914","resolution":{"observed_at":"2026-07-10T05:36:48.567306Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2512.24662","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T05:36:48.592693Z","title":null,"venue":null,"work_id":"cd437c01-1f13-4e92-8620-c96e9d781028","year":2025},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:525936d48e9f14a07c8813ad5cfccc4388b7e61f2cd1b3a0298b3454a8619a27","observation_id":"195f40b5-f19f-4d3a-8a27-4bfba0d0cc5b","resolution":{"observed_at":"2026-07-10T05:36:48.594228Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2604.05016","last_updated":"2026-04-06T18:00:00Z","snapshot_observed_at":"2026-08-14T11:38:53.482888Z","submitted_at":"2026-04-06T18:00:00Z","title":"Electroweak Doublet Dark Matter for a Galactic Halo Gamma-Ray Excess","version":1},"cited_work":{"arxiv_id":"2604.05016","doi":null,"metadata_source":"pith","pith_arxiv_id":"2604.05016","snapshot_observed_at":"2026-07-10T05:36:48.590136Z","title":"Electroweak Doublet Dark Matter for a Galactic Halo Gamma-Ray Excess","venue":"hep-ph","work_id":"d4a05603-6d63-4ba3-8896-37ad34ff8d06","year":2026},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/2604.05016","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:a79c8b8ee76cdc2792887bbc1c3b4a9b3eee5e91f0b3856a31d8ec84aeaad804","observation_id":"d3f27f5e-db41-4948-a8c8-834aa39c2b29","resolution":{"observed_at":"2026-07-10T05:36:48.591507Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0810.0713","last_updated":"2009-01-20T06:02:39Z","snapshot_observed_at":"2026-08-13T11:12:34.834744Z","submitted_at":"2008-10-06T19:59:30Z","title":"A Theory of Dark Matter","version":3},"cited_work":{"arxiv_id":"0810.0713","doi":null,"metadata_source":"pith","pith_arxiv_id":"0810.0713","snapshot_observed_at":"2026-07-10T05:36:48.609794Z","title":"A Theory of Dark Matter","venue":"hep-ph","work_id":"3619ef0b-8b19-435c-b717-27543700fe24","year":2008},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/0810.0713","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:bc10a9ca7babe1077ad2064713986dfa4ea4ea093823631b8d907a7e4a534c81","observation_id":"474c9c48-cd6f-42b3-81cf-4641717117d7","resolution":{"observed_at":"2026-07-10T05:36:48.611158Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1502.02007","last_updated":"2015-05-18T08:20:59Z","snapshot_observed_at":"2026-08-14T23:01:03.047093Z","submitted_at":"2015-02-06T19:59:30Z","title":"Constraints on decaying dark matter from the extragalactic gamma-ray background","version":2},"cited_work":{"arxiv_id":"1502.02007","doi":null,"metadata_source":"pith","pith_arxiv_id":"1502.02007","snapshot_observed_at":"2026-07-10T05:36:48.647143Z","title":"Constraints on decaying dark matter from the extragalactic gamma-ray background","venue":"astro-ph.CO","work_id":"bada8eff-e561-4f44-b667-6c692e29bc80","year":2015},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1502.02007","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:169df3c61a3e14ad96f086103c1b6543cf42f4240e22b34d803f51f8a02a438f","observation_id":"d0dad2f0-961c-4bec-aecf-eab9547c6251","resolution":{"observed_at":"2026-07-10T05:36:48.648605Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1612.05638","last_updated":"2019-06-21T16:47:20Z","snapshot_observed_at":"2026-08-14T21:25:02.654697Z","submitted_at":"2016-12-16T21:00:00Z","title":"Gamma-ray Constraints on Decaying Dark Matter and Implications for IceCube","version":3},"cited_work":{"arxiv_id":"1612.05638","doi":null,"metadata_source":"pith","pith_arxiv_id":"1612.05638","snapshot_observed_at":"2026-07-10T05:36:48.585235Z","title":"Gamma-ray Constraints on Decaying Dark Matter and Implications for IceCube","venue":"hep-ph","work_id":"440f8fd4-4f7a-4a7b-a81e-1b5007224408","year":2016},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1612.05638","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:489f6bd10b5848ff18163ef73ea72e38a10d8cec3244089b28dbcba33d2273c3","observation_id":"c7075b75-7f98-47c9-8b33-e30258771cbe","resolution":{"observed_at":"2026-07-10T05:36:48.586496Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.05988","last_updated":"2018-11-14T19:00:12Z","snapshot_observed_at":"2026-08-14T17:59:12.334963Z","submitted_at":"2018-11-14T19:00:12Z","title":"Constraints on Decaying Dark Matter from the Isotropic Gamma-Ray Background","version":1},"cited_work":{"arxiv_id":"1811.05988","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.05988","snapshot_observed_at":"2026-07-10T05:36:48.625119Z","title":"Constraints on Decaying Dark Matter from the Isotropic Gamma-Ray Background","venue":"astro-ph.HE","work_id":"1244dae5-2708-4891-b66c-f4506068c33d","year":2018},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"cited_paper":"/paper/1811.05988","citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:ccd51bf290855ea59993a725bba90c72269894e88ef1f4f9d28cb86f72dcd875","observation_id":"1eac6252-83c8-419d-b43c-8760bdb8d8bf","resolution":{"observed_at":"2026-07-10T05:36:48.626744Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2512.12176","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T05:36:48.582787Z","title":"Wang and K.-K","venue":null,"work_id":"21d98497-c84f-4cec-9a3c-181baa072dd2","year":2026},"citing_paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-10T05:30:29.237097Z"},"links":{"citing_paper":"/paper/2607.08552"},"observation_digest":"sha256:fb6eaf7277c8a348e6d5ebb730ffc1c398b9cdf87e31b21e027e87f9a53e09ad","observation_id":"20290727-df10-4b92-a145-2979d2f5e965","resolution":{"observed_at":"2026-07-10T05:36:48.584100Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2607.08552","last_updated":"2026-07-09T14:43:44Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-09T10:06:38.852745Z","submitted_at":"2026-07-09T14:43:44Z","title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation"},"reference_resolution":{"displayed":39,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":4,"verified_exact":33,"verified_fuzzy":0},"total_outbound_references":39},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 39 of 39 outbound references and 0 inbound Pith citation observations for arXiv:2607.08552."}