{"as_of":"2026-08-22T21:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a5aa2896307f4531253650f7c1532e30a7aaa6084a303b50b8b69e28e94da080","coverage":[{"denominator":54,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":54,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T21:32:34.336814Z","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":"2026-08-22T06:32:14.747728+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T14:46:17.226546Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-13T03:07:09.267964Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.08050","snapshot_observed_at":"2026-08-06T14:46:17.226546Z","title":"Angel, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.17803","last_updated":"2026-06-09T14:29:51Z","snapshot_observed_at":"2026-08-17T15:54:05.597510Z","submitted_at":"2025-07-23T18:00:00Z","title":"The Dark Side of a Tera-Z Factory","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T14:46:17.226546Z"},"links":{"cited_paper":"/paper/2509.08050","citing_paper":"/paper/2507.17803"},"observation_digest":"sha256:1b33fea7b6a8e8a1d2fa173a82e00ea4587a7c38b8a11b918f70e49ee6203f50","observation_id":"c227f97b-0f15-445f-a2fa-471ddfe2f0a1","resolution":{"observed_at":"2026-08-06T14:46:17.226546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"cited_work":{"arxiv_id":"2509.08050","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2509.08050","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Angel, D","venue":null,"work_id":"bfbc17df-1924-44d7-8f9a-9056c83e5430","year":null},"citing_paper":{"arxiv_id":"2605.11082","last_updated":"2026-05-11T18:00:08Z","snapshot_observed_at":"2026-08-16T17:43:44.551361Z","submitted_at":"2026-05-11T18:00:08Z","title":"Dark Matter as a Source for Lepton Flavor Violation","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-13T03:02:31.859366Z"},"links":{"cited_paper":"/paper/2509.08050","citing_paper":"/paper/2605.11082"},"observation_digest":"sha256:5e6c45a62cdc9a6f3ef6c3e7a4c8ae8f83761d20fe87deec730ff1d912c23815","observation_id":"dc39ec89-cf45-4e66-9023-ba2061e6d24d","resolution":{"observed_at":"2026-05-13T03:07:09.269810Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2509.08050/citation-record","integrity":"/paper/2509.08050/integrity","json":"/paper/2509.08050/citation-record.json","paper":"/paper/2509.08050"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2212.07435","last_updated":"2022-12-14T19:00:00Z","snapshot_observed_at":"2026-08-18T20:04:38.161416Z","submitted_at":"2022-12-14T19:00:00Z","title":"A Search for Dark Matter Lines at the Galactic Center with 14 Years of Fermi Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.07435","snapshot_observed_at":"2026-08-04T21:32:28.664093Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:28.664093Z"},"links":{"cited_paper":"/paper/2212.07435","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:6aacfa658f0ab5d582eb614175d4b2a682f3a7bdb677c86d777e890bb54523f8","observation_id":"da52ae01-80bc-4a0b-b064-078775eeda4f","resolution":{"observed_at":"2026-08-04T21:32:28.664093Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.5481","last_updated":"2012-12-13T22:42:55Z","snapshot_observed_at":"2026-08-15T00:48:43.164956Z","submitted_at":"2012-08-27T20:00:00Z","title":"Gamma Ray Signals from Dark Matter: Concepts, Status and Prospects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.5481","snapshot_observed_at":"2026-08-04T21:32:28.776505Z","title":"Bringmann and C","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:28.776505Z"},"links":{"cited_paper":"/paper/1208.5481","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:76f1562bfc9fd19423c334abb53bdcdc41f61f07e6cd68545cca6084e62d374f","observation_id":"0005d661-1f43-440b-9488-ef5326d934ea","resolution":{"observed_at":"2026-08-04T21:32:28.776505Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.00014","last_updated":"2016-03-31T20:00:02Z","snapshot_observed_at":"2026-08-14T22:03:35.165042Z","submitted_at":"2016-03-31T20:00:02Z","title":"A review of indirect searches for particle dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.00014","snapshot_observed_at":"2026-08-04T21:32:28.877097Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:28.877097Z"},"links":{"cited_paper":"/paper/1604.00014","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:c6ce433d7aa18ca2faf7d06a96c61a8bab27d6037aa5ca2d150cfc2b59aaaa49","observation_id":"845d9363-5ab5-48f2-ae27-bc323daee9ef","resolution":{"observed_at":"2026-08-04T21:32:28.877097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.11561","last_updated":"2020-10-07T09:46:16Z","snapshot_observed_at":"2026-08-04T16:21:30.135541Z","submitted_at":"2020-08-26T13:42:19Z","title":"Status, Challenges and Directions in Indirect Dark Matter Searches","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.11561","snapshot_observed_at":"2026-08-04T21:32:28.953438Z","title":"Pérez de los Heros,Status, Challenges and Directions in Indirect Dark Matter Searches, Symmetry12(2020), no","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:28.953438Z"},"links":{"cited_paper":"/paper/2008.11561","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:cb28f78e00304c0ac1cdccf647abd4cf457a53da7799758aeda283472e278579","observation_id":"947f6745-f2b1-4716-baba-cc00c75cd2f2","resolution":{"observed_at":"2026-08-04T21:32:28.953438Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.5090","last_updated":"2012-02-08T18:21:30Z","snapshot_observed_at":"2026-08-17T13:51:35.031666Z","submitted_at":"2010-11-23T13:27:06Z","title":"Current and Future Constraints on Dark Matter from Prompt and Inverse-Compton Photon Emission in the Isotropic Diffuse Gamma-ray Background","version":3},"cited_work":{"arxiv_id":"1011.5090","doi":null,"metadata_source":"pith","pith_arxiv_id":"1011.5090","snapshot_observed_at":"2026-08-04T21:32:36.872396Z","title":"Current and Future Constraints on Dark Matter from Prompt and Inverse-Compton Photon Emission in the Isotropic Diffuse Gamma-ray Background","venue":"hep-ph","work_id":"6c093d2d-09ce-4f4c-8690-6cb3a618c8fd","year":2010},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:29.017991Z"},"links":{"cited_paper":"/paper/1011.5090","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:4fb1baf319e3dcdf9e80ad5b312964690750abeb593186c6d9e0558aa9c6cbb9","observation_id":"ceaa33b9-fe05-4d0f-88c8-1d0bc3fe0658","resolution":{"observed_at":"2026-08-04T21:32:36.978219Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1002.3820","last_updated":"2010-10-28T15:37:42Z","snapshot_observed_at":"2026-08-17T13:51:32.954102Z","submitted_at":"2010-02-19T20:59:25Z","title":"Conservative Constraints on Dark Matter from the Fermi-LAT Isotropic Diffuse Gamma-Ray Background Spectrum","version":3},"cited_work":{"arxiv_id":"1002.3820","doi":null,"metadata_source":"pith","pith_arxiv_id":"1002.3820","snapshot_observed_at":"2026-08-04T21:32:36.725142Z","title":"Conservative Constraints on Dark Matter from the Fermi-LAT Isotropic Diffuse Gamma-Ray Background Spectrum","venue":"astro-ph.HE","work_id":"4263de9a-c6e1-4bd7-8aa2-7788363a6358","year":2010},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:29.088726Z"},"links":{"cited_paper":"/paper/1002.3820","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:63c367abe0608707e2c2f8175aba966a746c57f6c9283bf59ad8f584905e1a56","observation_id":"47eaa858-9be5-4560-8043-f69684c9c503","resolution":{"observed_at":"2026-08-04T21:32:36.793235Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1106.1874","last_updated":"2011-12-02T16:28:58Z","snapshot_observed_at":"2026-08-17T13:51:31.887788Z","submitted_at":"2011-06-09T18:38:22Z","title":"On the Relevance of Sharp Gamma-Ray Features for Indirect Dark Matter Searches","version":2},"cited_work":{"arxiv_id":"1106.1874","doi":null,"metadata_source":"pith","pith_arxiv_id":"1106.1874","snapshot_observed_at":"2026-08-04T21:32:36.564623Z","title":"On the Relevance of Sharp Gamma-Ray Features for Indirect Dark Matter Searches","venue":"hep-ph","work_id":"96d7884a-225e-4ef4-a797-b6620e457500","year":2011},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:29.228538Z"},"links":{"cited_paper":"/paper/1106.1874","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:64d4eb300abb0df28b7673cf4fc6e2b1977f1d22a6d63afdc43ac3c2d771622a","observation_id":"55be1b89-0eb4-4782-9e8d-50debf6f4644","resolution":{"observed_at":"2026-08-04T21:32:36.642018Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.2835","last_updated":"2012-12-19T22:30:17Z","snapshot_observed_at":"2026-08-17T13:51:53.925662Z","submitted_at":"2011-11-11T19:51:16Z","title":"Lower Limits on the Strengths of Gamma Ray Lines from WIMP Dark Matter Annihilation","version":2},"cited_work":{"arxiv_id":"1111.2835","doi":null,"metadata_source":"pith","pith_arxiv_id":"1111.2835","snapshot_observed_at":"2026-08-04T21:32:36.426156Z","title":"Lower Limits on the Strengths of Gamma Ray Lines from WIMP Dark Matter Annihilation","venue":"hep-ph","work_id":"2940ac86-cce9-4494-b564-686c705cf149","year":2011},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:29.336322Z"},"links":{"cited_paper":"/paper/1111.2835","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:658955205f7ab5b129b40bcd6ceebd314a4d38d7aad603352117921912fa1f4d","observation_id":"1000c858-5775-4fb8-9473-6cee527f0e8d","resolution":{"observed_at":"2026-08-04T21:32:36.474984Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1110.6151","last_updated":"2012-01-03T18:39:31Z","snapshot_observed_at":"2026-08-20T06:45:05.515858Z","submitted_at":"2011-10-27T18:20:51Z","title":"Constraints on WIMP and Sommerfeld-Enhanced Dark Matter Annihilation from HESS Observations of the Galactic Center","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.6151","snapshot_observed_at":"2026-08-04T21:32:29.445287Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:29.445287Z"},"links":{"cited_paper":"/paper/1110.6151","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:ade84c961d2a5a6101785a17cba788a3537bb4b2ecd9a045df347f03384d0096","observation_id":"a7c3ded3-db1c-4d80-8678-2d3e9a1ed4ae","resolution":{"observed_at":"2026-08-04T21:32:29.445287Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.00389","last_updated":"2016-04-26T22:53:12Z","snapshot_observed_at":"2026-08-14T22:29:53.687145Z","submitted_at":"2015-10-01T20:03:33Z","title":"New Limits on the Dark Matter Lifetime from Dwarf Spheroidal Galaxies using Fermi-LAT","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.00389","snapshot_observed_at":"2026-08-04T21:32:29.554203Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:29.554203Z"},"links":{"cited_paper":"/paper/1510.00389","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:00330d900fc693aa67e2cbae177cfdcf44de5a7e8827b6f1fb053f51f12f4938","observation_id":"d1bf4af3-1074-4319-bd9c-f9b9dee90dc0","resolution":{"observed_at":"2026-08-04T21:32:29.554203Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.4681","last_updated":"2013-09-24T12:49:30Z","snapshot_observed_at":"2026-08-15T00:13:27.946170Z","submitted_at":"2013-06-19T20:00:32Z","title":"Novel Gamma-ray Spectral Features in the Inert Doublet Model","version":2},"cited_work":{"arxiv_id":"1306.4681","doi":null,"metadata_source":"pith","pith_arxiv_id":"1306.4681","snapshot_observed_at":"2026-08-04T21:32:36.284916Z","title":"Novel Gamma-ray Spectral Features in the Inert Doublet Model","venue":"hep-ph","work_id":"de80b1df-0bec-411d-b303-874ece3fd895","year":2013},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:29.671665Z"},"links":{"cited_paper":"/paper/1306.4681","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:11cb4c0da2c280823b74c5b1792e3273434ac2fa8b15550daf9f9149f18c21c4","observation_id":"2983ca5a-dfa1-4cf9-bff5-0dd6bad40d77","resolution":{"observed_at":"2026-08-04T21:32:36.332138Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1602.05966","last_updated":"2016-07-05T11:51:00Z","snapshot_observed_at":"2026-08-14T22:09:42.970002Z","submitted_at":"2016-02-18T21:03:58Z","title":"Gamma-ray Limits on Neutrino Lines","version":2},"cited_work":{"arxiv_id":"1602.05966","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.05966","snapshot_observed_at":"2026-08-04T21:32:36.109913Z","title":"Gamma-ray Limits on Neutrino Lines","venue":"hep-ph","work_id":"7703cdf0-98cd-4a56-af12-869cd4bee241","year":2016},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:29.795776Z"},"links":{"cited_paper":"/paper/1602.05966","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:527f3baabf36e1e88f4b100cf352435f7ee9cda3a6e2a72d1bda6a338ead6e12","observation_id":"7ba0fe59-f093-4a66-a89e-6fc0fe1bbdc4","resolution":{"observed_at":"2026-08-04T21:32:36.185700Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1602.08501","last_updated":"2016-07-05T11:52:48Z","snapshot_observed_at":"2026-08-17T13:43:42.935311Z","submitted_at":"2016-02-26T21:00:24Z","title":"Extending Fermi-LAT and H.E.S.S. Limits on Gamma-ray Lines from Dark Matter Annihilation","version":2},"cited_work":{"arxiv_id":"1602.08501","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.08501","snapshot_observed_at":"2026-08-04T21:32:35.989163Z","title":"Extending Fermi-LAT and H.E.S.S. Limits on Gamma-ray Lines from Dark Matter Annihilation","venue":"astro-ph.HE","work_id":"fd23aa61-e2d2-4024-95ed-a313ff834409","year":2016},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:29.900951Z"},"links":{"cited_paper":"/paper/1602.08501","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:b07e1e95711673fc25347e428459d6608a7221a8df8efb5001d7fa5efdffcc79","observation_id":"fbcebdb0-2080-43e9-a038-894c2a457c65","resolution":{"observed_at":"2026-08-04T21:32:36.041527Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03133","last_updated":"2017-11-23T20:07:52Z","snapshot_observed_at":"2026-08-17T15:27:01.975452Z","submitted_at":"2017-11-08T19:35:32Z","title":"Searching for Secluded Dark Matter with H.E.S.S., Fermi-LAT, and Planck","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.03133","snapshot_observed_at":"2026-08-04T21:32:30.004917Z","title":"Profumo, F","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:30.004917Z"},"links":{"cited_paper":"/paper/1711.03133","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:3b5a7439dd1fcbc053ace16e2f6d7b09f6edcd946342729d33d0aa72ad41d19d","observation_id":"180898ce-3b04-415d-b1dd-9aadb2d0d0f0","resolution":{"observed_at":"2026-08-04T21:32:30.004917Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.10494","last_updated":"2019-04-23T13:44:00Z","snapshot_observed_at":"2026-08-17T15:08:45.620051Z","submitted_at":"2019-01-29T19:00:08Z","title":"Search for Semi-Annihilating Dark Matter with Fermi-LAT, H.E.S.S., Planck, and the Cherenkov Telescope Array","version":2},"cited_work":{"arxiv_id":"1901.10494","doi":null,"metadata_source":"pith","pith_arxiv_id":"1901.10494","snapshot_observed_at":"2026-08-04T21:32:35.843451Z","title":"Search for Semi-Annihilating Dark Matter with Fermi-LAT, H.E.S.S., Planck, and the Cherenkov Telescope Array","venue":"hep-ph","work_id":"95e7a00e-1b56-48b2-8e67-b1a6852080cd","year":2019},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:30.147816Z"},"links":{"cited_paper":"/paper/1901.10494","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:096f8bb6c151803f1406a29940ea23e867b6033af175fb7946a37c178cde2abb","observation_id":"35fa91ef-598c-4c1d-af5d-341f4a3a55b9","resolution":{"observed_at":"2026-08-04T21:32:35.914311Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2003.10416","last_updated":"2021-01-25T20:53:04Z","snapshot_observed_at":"2026-08-09T19:13:03.813473Z","submitted_at":"2020-03-23T17:44:40Z","title":"Strong constraints on thermal relic dark matter from Fermi-LAT observations of the Galactic Center","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.10416","snapshot_observed_at":"2026-08-04T21:32:30.279414Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:30.279414Z"},"links":{"cited_paper":"/paper/2003.10416","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:92e0450a898be7de5e31a5f368999dd38772f0ced379cdd4cb6b8aa978d41b6f","observation_id":"708ab878-7d75-4de1-9f13-a32bdf4d7b72","resolution":{"observed_at":"2026-08-04T21:32:30.279414Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.04053","last_updated":"2021-09-30T18:12:19Z","snapshot_observed_at":"2026-08-16T18:11:19.297825Z","submitted_at":"2021-07-08T18:05:59Z","title":"Indirect Searches for Secluded Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.04053","snapshot_observed_at":"2026-08-04T21:32:30.383453Z","title":"Siqueira, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:30.383453Z"},"links":{"cited_paper":"/paper/2107.04053","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:5b19cb0958482fc5d94cb79e28ab46cab73a3c0c06962a5fc72b8721da8c1e83","observation_id":"d845c8e2-36df-49f2-8d19-1536edf444ab","resolution":{"observed_at":"2026-08-04T21:32:30.383453Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.06789","last_updated":"2022-01-18T07:37:01Z","snapshot_observed_at":"2026-08-16T17:27:42.622152Z","submitted_at":"2022-01-18T07:37:01Z","title":"Galactic and Extragalactic Sources of Very High Energy Gamma-rays","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.06789","snapshot_observed_at":"2026-08-04T21:32:30.433554Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:30.433554Z"},"links":{"cited_paper":"/paper/2201.06789","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:5078c36711597d9dcaf2364d50367e39785c5620e1f92a387588c9e7aba1eb12","observation_id":"98baa7c3-c14a-4722-a719-965f67ad1b0f","resolution":{"observed_at":"2026-08-04T21:32:30.433554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.15860","last_updated":"2024-03-23T14:56:13Z","snapshot_observed_at":"2026-08-20T14:10:07.832472Z","submitted_at":"2024-03-23T14:56:13Z","title":"The Waning of the WIMP: Endgame?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.15860","snapshot_observed_at":"2026-08-04T21:32:30.532038Z","title":"Arcadi, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:30.532038Z"},"links":{"cited_paper":"/paper/2403.15860","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:b6c7061bcdd34e9b6ff04b73a4d62e1f813ea3da8786316ffdd86f17647bc4bd","observation_id":"acb32120-5812-4ae6-b764-cb864f2a98dd","resolution":{"observed_at":"2026-08-04T21:32:30.532038Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:32:37.067562Z","title":"Collaboration,CTAO Performance, 2025","venue":null,"work_id":"1e37412b-ac22-4b0e-869b-7ec06ecaa817","year":2025},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:30.645528Z"},"links":{"citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:0b426201346de4d1d8e081211a48f586419b9a076f08fd7636b501614bc051c2","observation_id":"a1aff24a-d64d-4560-ad31-d826ef474528","resolution":{"observed_at":"2026-08-04T21:32:37.115122Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.6632","last_updated":"2016-04-08T09:35:47Z","snapshot_observed_at":"2026-08-15T00:23:45.656427Z","submitted_at":"2013-03-26T20:00:01Z","title":"Gamma-ray boxes from axion-mediated dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.6632","snapshot_observed_at":"2026-08-04T21:32:30.766954Z","title":"Ibarra, H","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:30.766954Z"},"links":{"cited_paper":"/paper/1303.6632","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:b93829e8cd29d2313180efe2355b367bcaf6ab28ba0a070641b8c9164c0bd168","observation_id":"2fa49524-05c5-4ebf-b212-ca9ec8003a12","resolution":{"observed_at":"2026-08-04T21:32:30.766954Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.06797","last_updated":"2016-07-06T14:26:19Z","snapshot_observed_at":"2026-08-18T20:05:55.484790Z","submitted_at":"2015-03-23T20:00:28Z","title":"On the sensitivity of CTA to gamma-ray boxes from multi-TeV dark matter","version":2},"cited_work":{"arxiv_id":"1503.06797","doi":null,"metadata_source":"pith","pith_arxiv_id":"1503.06797","snapshot_observed_at":"2026-08-04T21:32:35.651220Z","title":"On the sensitivity of CTA to gamma-ray boxes from multi-TeV dark matter","venue":"astro-ph.HE","work_id":"41818b08-fc46-4c0e-bc2c-724efea84f96","year":2015},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:30.837136Z"},"links":{"cited_paper":"/paper/1503.06797","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:5686c6ebea5a3ae1e74d615135dff49e5c56787c3d03c356be86283b1140c7b6","observation_id":"aaa72c17-5409-4a72-8a71-7a5c70607086","resolution":{"observed_at":"2026-08-04T21:32:35.737749Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0710.3169","last_updated":"2008-09-13T09:29:55Z","snapshot_observed_at":"2026-08-15T10:29:43.918723Z","submitted_at":"2007-10-17T16:25:42Z","title":"New Gamma-Ray Contributions to Supersymmetric Dark Matter Annihilation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0710.3169","snapshot_observed_at":"2026-08-04T21:32:30.931830Z","title":"Bringmann, L","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:30.931830Z"},"links":{"cited_paper":"/paper/0710.3169","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:699143898951f9e1c1aa35c5a82380b0050c93b306df75a24893fa5476ef7471","observation_id":"b343b3f9-5f5e-49b1-ac80-b60e4818eb6e","resolution":{"observed_at":"2026-08-04T21:32:30.931830Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:32:31.062282Z","title":"Panci,Electroweak Multiplets as Dark Matter candidates: A brief review, 5, 2024.2405.05087","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:31.062282Z"},"links":{"citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:afadd084a722c8d5aa4cfd7be897e84112a7049cc41b99f10c37fdb134562ffc","observation_id":"53971b99-a4ec-42f7-939e-392801dd82c7","resolution":{"observed_at":"2026-08-04T21:32:31.062282Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.21199","last_updated":"2025-01-10T15:27:34Z","snapshot_observed_at":"2026-08-22T02:16:19.382205Z","submitted_at":"2024-10-28T16:43:58Z","title":"Cherenkov Telescope Array Observatory sensitivity to heavy Galactic Cosmic Rays and the shape of particle spectrum","version":2},"cited_work":{"arxiv_id":"2410.21199","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.21199","snapshot_observed_at":"2026-08-04T21:32:35.449415Z","title":"Cherenkov Telescope Array Observatory sensitivity to heavy Galactic Cosmic Rays and the shape of particle spectrum","venue":"astro-ph.HE","work_id":"9c8f1e12-35c3-4f48-af92-f9b798e36ceb","year":2024},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:31.180083Z"},"links":{"cited_paper":"/paper/2410.21199","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:9c508678c86ad357a6e5fb73ca415415224de5e20c7117df550ed6382c6cae41","observation_id":"36f1c738-affd-4cec-b39c-9a5dd9ca0bc9","resolution":{"observed_at":"2026-08-04T21:32:35.518989Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1705.01790","last_updated":"2017-05-04T10:49:16Z","snapshot_observed_at":"2026-08-19T14:43:01.506914Z","submitted_at":"2017-05-04T10:49:16Z","title":"Monte Carlo Performance Studies for the Site Selection of the Cherenkov Telescope Array","version":1},"cited_work":{"arxiv_id":"1705.01790","doi":null,"metadata_source":"pith","pith_arxiv_id":"1705.01790","snapshot_observed_at":"2026-08-04T21:32:35.302224Z","title":"Monte Carlo Performance Studies for the Site Selection of the Cherenkov Telescope Array","venue":"astro-ph.IM","work_id":"e663344b-ab15-4644-800f-6855a14fc716","year":2017},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:31.286726Z"},"links":{"cited_paper":"/paper/1705.01790","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:343e0ff3f6f204687f5497ca862153bc82d21089ae1ff1c3a07c7fe4a4b219dd","observation_id":"e3f091bc-fc3f-40a6-a453-e942364588ec","resolution":{"observed_at":"2026-08-04T21:32:35.377780Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1507.08974","last_updated":"2016-04-06T12:43:55Z","snapshot_observed_at":"2026-08-14T22:38:07.627067Z","submitted_at":"2015-07-31T18:43:41Z","title":"Enhanced lines and box-shaped features in the gamma-ray spectrum from annihilating dark matter in the NMSSM","version":3},"cited_work":{"arxiv_id":"1507.08974","doi":null,"metadata_source":"pith","pith_arxiv_id":"1507.08974","snapshot_observed_at":"2026-08-04T21:32:35.179970Z","title":"Enhanced lines and box-shaped features in the gamma-ray spectrum from annihilating dark matter in the NMSSM","venue":"hep-ph","work_id":"703f765e-9ffb-40b0-8574-96eab09c4893","year":2015},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:31.384648Z"},"links":{"cited_paper":"/paper/1507.08974","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:fff324e978853ad024b097f4e44180edee13248d07d57bd8630e4261db78246e","observation_id":"5196eaa5-06c7-46e2-8df1-f631befc6658","resolution":{"observed_at":"2026-08-04T21:32:35.237675Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1506.05107","last_updated":"2015-10-14T12:19:08Z","snapshot_observed_at":"2026-08-14T22:44:10.155181Z","submitted_at":"2015-06-16T20:00:37Z","title":"Simplified Dirac Dark Matter Models and Gamma-Ray Lines","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.05107","snapshot_observed_at":"2026-08-04T21:32:31.459189Z","title":"Duerr, P","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:31.459189Z"},"links":{"cited_paper":"/paper/1506.05107","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:e97e6d894fb62c8d563b209621da53e273dc67a51cb906f8690c241ebde3113c","observation_id":"efb0a30f-d9bd-46ff-b6b8-619bc70500f8","resolution":{"observed_at":"2026-08-04T21:32:31.459189Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.07440","last_updated":"2017-04-09T19:41:09Z","snapshot_observed_at":"2026-08-14T21:51:24.530565Z","submitted_at":"2016-06-23T20:00:02Z","title":"Lines and Boxes: Unmasking Dynamical Dark Matter through Correlations in the MeV Gamma-Ray Spectrum","version":2},"cited_work":{"arxiv_id":"1606.07440","doi":null,"metadata_source":"pith","pith_arxiv_id":"1606.07440","snapshot_observed_at":"2026-08-04T21:32:35.054117Z","title":"Lines and Boxes: Unmasking Dynamical Dark Matter through Correlations in the MeV Gamma-Ray Spectrum","venue":"hep-ph","work_id":"de8b881f-5063-4697-b426-5d868f6ee37d","year":2016},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:31.522419Z"},"links":{"cited_paper":"/paper/1606.07440","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:f52af66a8ce4f8ce88be6eb7d414e8386a0848e84166292495fada960a2da0fb","observation_id":"e3d535f9-0932-41f0-ae22-219dc82f3528","resolution":{"observed_at":"2026-08-04T21:32:35.113389Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1810.07068","last_updated":"2018-10-16T15:14:28Z","snapshot_observed_at":"2026-08-14T18:13:48.684752Z","submitted_at":"2018-10-16T15:14:28Z","title":"Gamma-ray lines may reveal the CP nature of the dark matter particle","version":1},"cited_work":{"arxiv_id":"1810.07068","doi":null,"metadata_source":"pith","pith_arxiv_id":"1810.07068","snapshot_observed_at":"2026-08-04T21:32:34.945532Z","title":"Gamma-ray lines may reveal the CP nature of the dark matter particle","venue":"hep-ph","work_id":"8c44fede-9a0f-4309-ad5d-f1e0631faa06","year":2018},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:31.691068Z"},"links":{"cited_paper":"/paper/1810.07068","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:905c92ba4847d2e2f6f77e0de7b5f619d2ea30972b0c574b47a95da69c1ce814","observation_id":"0bdd89af-151c-48c0-bd1c-278b1d33e3a6","resolution":{"observed_at":"2026-08-04T21:32:34.984265Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2001.04946","last_updated":"2020-07-13T02:42:45Z","snapshot_observed_at":"2026-08-10T14:47:33.565760Z","submitted_at":"2020-01-14T18:05:42Z","title":"A Potentially Detectable Gamma-Ray Line in the Fermi Galactic Center Excess -- In Light of One-Step Cascade Annihilations of Secluded (Vector) Dark Matter via the Higgs Portal","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.04946","snapshot_observed_at":"2026-08-04T21:32:31.852382Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:31.852382Z"},"links":{"cited_paper":"/paper/2001.04946","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:4cd5c45093c28996ab94e4e68b3ff7d36922906f07f86e6d8d146d140f6a2e84","observation_id":"3520f8c8-8523-4c28-a480-8fed9b6fd3c6","resolution":{"observed_at":"2026-08-04T21:32:31.852382Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:32:31.994487Z","title":"Angel, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:31.994487Z"},"links":{"citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:09882640bfbd7c7b32bfde4dc172e085e29a53878216828030b582c4e767f35a","observation_id":"9a4364e0-4775-4abd-98b6-635dafc523c2","resolution":{"observed_at":"2026-08-04T21:32:31.994487Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.03281","last_updated":"2023-09-11T09:48:54Z","snapshot_observed_at":"2026-08-16T15:02:44.442019Z","submitted_at":"2023-09-06T18:00:30Z","title":"Gamma-Ray Lines in 15 Years of Fermi-LAT Data: New Constraints on Higgs Portal Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.03281","snapshot_observed_at":"2026-08-04T21:32:32.083509Z","title":"De La Torre Luque, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:32.083509Z"},"links":{"cited_paper":"/paper/2309.03281","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:3519a3286be801fd860f659315e5ec861b56b85ac8c8597466e0fc3997b98e25","observation_id":"4466064b-7820-4214-a101-9ba725541f63","resolution":{"observed_at":"2026-08-04T21:32:32.083509Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.16762","last_updated":"2023-08-31T14:30:19Z","snapshot_observed_at":"2026-08-19T09:02:10.875623Z","submitted_at":"2023-08-31T14:30:19Z","title":"Search for the gamma-ray spectral lines with the DAMPE and the Fermi-LAT observations","version":1},"cited_work":{"arxiv_id":"2308.16762","doi":null,"metadata_source":"pith","pith_arxiv_id":"2308.16762","snapshot_observed_at":"2026-08-04T21:32:34.776422Z","title":"Search for the gamma-ray spectral lines with the DAMPE and the Fermi-LAT observations","venue":"astro-ph.HE","work_id":"3e2339e5-57ac-484c-a19d-fa7b35009fb2","year":2023},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:32.212086Z"},"links":{"cited_paper":"/paper/2308.16762","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:6b142af1aa193d6b4444688d7c2bdbb25cffc43b52add9aa9b0909d99638280d","observation_id":"83804213-d8b9-4618-a6f7-d4cc7ee2720d","resolution":{"observed_at":"2026-08-04T21:32:34.836785Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.01705","last_updated":"2025-12-03T08:11:10Z","snapshot_observed_at":"2026-08-13T12:44:27.712598Z","submitted_at":"2024-06-03T18:03:11Z","title":"Dark Matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.01705","snapshot_observed_at":"2026-08-04T21:32:32.315100Z","title":"Cirelli, A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:32.315100Z"},"links":{"cited_paper":"/paper/2406.01705","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:dac7f03535ebe4b7eaa671d185b614a722e96efbf8429316ad2a082c44c7a906","observation_id":"2c102bbe-1ee2-464f-bafb-392d2f4143f5","resolution":{"observed_at":"2026-08-04T21:32:32.315100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0808.3384","last_updated":"2009-11-03T20:50:41Z","snapshot_observed_at":"2026-08-17T07:10:59.004952Z","submitted_at":"2008-08-25T16:51:32Z","title":"Deducing the nature of dark matter from direct and indirect detection experiments in the absence of collider signatures of new physics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0808.3384","snapshot_observed_at":"2026-08-04T21:32:32.388690Z","title":"Beltran, D","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:32.388690Z"},"links":{"cited_paper":"/paper/0808.3384","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:9cc5cba3c4b32d29938f14a1d7417a22a2ae4e20b3576d4868eee13492a84070","observation_id":"ebe963eb-8ead-4e95-8c86-334799d76361","resolution":{"observed_at":"2026-08-04T21:32:32.388690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.1591","last_updated":"2010-12-10T02:53:36Z","snapshot_observed_at":"2026-08-15T05:11:50.268835Z","submitted_at":"2010-08-09T20:20:05Z","title":"Non-relativistic effective theory of dark matter direct detection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.1591","snapshot_observed_at":"2026-08-04T21:32:32.483050Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:32.483050Z"},"links":{"cited_paper":"/paper/1008.1591","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:ba3f1f1b57e160d70e660e1810e30e453207191ddcf4925865e03e1d81521a0d","observation_id":"fe7bd03d-4d02-4fdb-a936-6c9c3799ad1b","resolution":{"observed_at":"2026-08-04T21:32:32.483050Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.1783","last_updated":"2011-04-01T21:32:30Z","snapshot_observed_at":"2026-08-15T05:11:44.979752Z","submitted_at":"2010-08-10T20:00:01Z","title":"Constraints on Dark Matter from Colliders","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.1783","snapshot_observed_at":"2026-08-04T21:32:32.586606Z","title":"Goodman, M","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:32.586606Z"},"links":{"cited_paper":"/paper/1008.1783","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:8f79d55ab67d8f0d83632fea4898c85d2a7aeff9d9b088d31b8db7f7c3ae4825","observation_id":"15ca7483-6189-4b32-8952-ce88b3ea1697","resolution":{"observed_at":"2026-08-04T21:32:32.586606Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1002.4137","last_updated":"2010-08-23T21:40:15Z","snapshot_observed_at":"2026-08-15T05:25:49.735190Z","submitted_at":"2010-02-22T16:52:38Z","title":"Maverick dark matter at colliders","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1002.4137","snapshot_observed_at":"2026-08-04T21:32:32.676579Z","title":"Beltran, D","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:32.676579Z"},"links":{"cited_paper":"/paper/1002.4137","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:65252ad9a7d7d5c65388f404b34f9ddd0e2de1680885efa8ce87fe572337d52d","observation_id":"9bc9b0c6-d2ef-4c6e-b09b-9ef2e0470e7a","resolution":{"observed_at":"2026-08-04T21:32:32.676579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.3542","last_updated":"2012-08-28T17:39:55Z","snapshot_observed_at":"2026-08-15T04:15:56.929365Z","submitted_at":"2012-03-15T20:00:03Z","title":"The Effective Field Theory of Dark Matter Direct Detection","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.3542","snapshot_observed_at":"2026-08-04T21:32:32.790827Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:32.790827Z"},"links":{"cited_paper":"/paper/1203.3542","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:8660be42eb82bd65c136261804b71935124c3efa80d3d28262f66337c3982912","observation_id":"4676203f-0b9e-4b24-b05a-cf6f57bdfc31","resolution":{"observed_at":"2026-08-04T21:32:32.790827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.01788","last_updated":"2021-08-19T11:27:40Z","snapshot_observed_at":"2026-08-16T18:33:54.249013Z","submitted_at":"2021-04-05T06:23:55Z","title":"Effective Theories with Dark Matter Applications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.01788","snapshot_observed_at":"2026-08-04T21:32:32.908945Z","title":"Bhattacharya and J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:32.908945Z"},"links":{"cited_paper":"/paper/2104.01788","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:2ca0b6e4a0441ab85ea56cc92cd97b89fd258da2e8957f346c61d9e617b67d11","observation_id":"86727f54-d611-456e-b82d-911e492b8741","resolution":{"observed_at":"2026-08-04T21:32:32.908945Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:32:33.027803Z","title":"Gondolo and G","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:33.027803Z"},"links":{"citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:1018c9976bf1aa2dab2d334f2056e160ef9fbbaa9f4f77deb7f3bb65588c77b3","observation_id":"41aded0f-f247-41b3-8ca7-1bcf1d4da28c","resolution":{"observed_at":"2026-08-04T21:32:33.027803Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.02696","last_updated":"2022-01-04T03:35:38Z","snapshot_observed_at":"2026-08-16T17:58:29.771628Z","submitted_at":"2021-09-06T19:03:37Z","title":"Les Houches Lectures on Indirect Detection of Dark Matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.02696","snapshot_observed_at":"2026-08-04T21:32:33.115132Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:33.115132Z"},"links":{"cited_paper":"/paper/2109.02696","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:5fc532fed0cccd24929713c56dce4a575b9d43589e6b9627ba2e6fee48405a09","observation_id":"cf34c971-d644-4429-8e30-bb71d0169a94","resolution":{"observed_at":"2026-08-04T21:32:33.115132Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.0021","last_updated":"2013-04-30T20:31:11Z","snapshot_observed_at":"2026-08-15T00:19:23.067896Z","submitted_at":"2013-04-30T20:31:11Z","title":"Dark matter coupling to electroweak gauge and Higgs bosons: an effective field theory approach","version":1},"cited_work":{"arxiv_id":"1305.0021","doi":null,"metadata_source":"pith","pith_arxiv_id":"1305.0021","snapshot_observed_at":"2026-08-04T21:32:34.601015Z","title":"Dark matter coupling to electroweak gauge and Higgs bosons: an effective field theory approach","venue":"hep-ph","work_id":"31dece5a-f3e9-4005-b706-4e7a52466e5f","year":2013},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:33.195523Z"},"links":{"cited_paper":"/paper/1305.0021","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:1a06ea0c3d874df7f9a14a8dd9af89531a75f6c310956ea5be2681de800ee5c4","observation_id":"14a92b0c-6ba8-4e42-ba86-3a93b05e98c1","resolution":{"observed_at":"2026-08-04T21:32:34.647775Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1007.5515","last_updated":"2010-07-30T18:43:27Z","snapshot_observed_at":"2026-08-15T05:12:31.530975Z","submitted_at":"2010-07-30T18:43:27Z","title":"Direct Detection of Dark Matter Electromagnetic Dipole Moments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1007.5515","snapshot_observed_at":"2026-08-04T21:32:33.265071Z","title":"Banks, J.-F","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:33.265071Z"},"links":{"cited_paper":"/paper/1007.5515","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:fa620c4e72e3213011d9517d8be2aaae72e49f5c49483fc8901f5c0d8ad9feb1","observation_id":"aec9804a-31bd-4939-aad7-c1e41e7ac172","resolution":{"observed_at":"2026-08-04T21:32:33.265071Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.12785","last_updated":"2021-04-26T18:00:03Z","snapshot_observed_at":"2026-08-18T22:15:18.968764Z","submitted_at":"2021-04-26T18:00:03Z","title":"Appendiciario -- A hands-on manual on the theory of direct Dark Matter detection","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.12785","snapshot_observed_at":"2026-08-04T21:32:33.377065Z","title":"Del Nobile,The Theory of Direct Dark Matter Detection: A Guide to Computations, 2104.12785","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:33.377065Z"},"links":{"cited_paper":"/paper/2104.12785","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:f620f5750ff33b8c7be81a10f81d23238c62aa4996cb394dd4578e1abca228d7","observation_id":"7e9e436f-2f3b-4012-afa8-9d9d24692ee6","resolution":{"observed_at":"2026-08-04T21:32:33.377065Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.00033","last_updated":"2019-05-20T08:30:35Z","snapshot_observed_at":"2026-08-18T20:22:59.404136Z","submitted_at":"2018-09-28T18:31:28Z","title":"Faint Light from Dark Matter: Classifying and Constraining Dark Matter-Photon Effective Operators","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.00033","snapshot_observed_at":"2026-08-04T21:32:33.444572Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:33.444572Z"},"links":{"cited_paper":"/paper/1810.00033","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:4f4abef50f8b3f955e16a97a293d696a61ad6273eaf2b2ea033ea5f83d37ced0","observation_id":"e1104245-1b5b-49d1-ae5b-613dbe426339","resolution":{"observed_at":"2026-08-04T21:32:33.444572Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1002.1912","last_updated":"2010-02-09T16:47:27Z","snapshot_observed_at":"2026-08-15T05:26:59.273724Z","submitted_at":"2010-02-09T16:47:27Z","title":"Direct detection of WIMPs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1002.1912","snapshot_observed_at":"2026-08-04T21:32:33.520141Z","title":null,"venue":null,"work_id":null,"year":1912},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:33.520141Z"},"links":{"cited_paper":"/paper/1002.1912","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:faf676ce3a303a153b181ed5ba8a3bb210cea906c474c8b8f06a376d5d654b2f","observation_id":"3d7c7ff9-3b18-4ce2-aaf5-2544584fabe2","resolution":{"observed_at":"2026-08-04T21:32:33.520141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.5955","last_updated":"2015-11-15T19:59:04Z","snapshot_observed_at":"2026-08-15T00:09:27.348799Z","submitted_at":"2013-07-23T06:15:31Z","title":"Tools for model-independent bounds in direct dark matter searches","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.5955","snapshot_observed_at":"2026-08-04T21:32:33.689556Z","title":"Cirelli, E","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:33.689556Z"},"links":{"cited_paper":"/paper/1307.5955","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:e6a98908437dc58b594ca60e18f92de8a80990429c99c5ba693229c365407f76","observation_id":"b79240e5-db4d-4618-a7b9-7ca2f3ff5a94","resolution":{"observed_at":"2026-08-04T21:32:33.689556Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.00368","last_updated":"2017-08-29T16:08:31Z","snapshot_observed_at":"2026-08-14T21:32:25.776032Z","submitted_at":"2016-11-01T20:00:03Z","title":"Chiral Effective Theory of Dark Matter Direct Detection","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.00368","snapshot_observed_at":"2026-08-04T21:32:33.787093Z","title":"Bishara, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:33.787093Z"},"links":{"cited_paper":"/paper/1611.00368","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:a9bfb91e0c228c3fedd7f22a55a4fbb0a3c37f902f49ea1c58baf9bad5418280","observation_id":"eecf1118-0aac-49ce-825e-6599786524e4","resolution":{"observed_at":"2026-08-04T21:32:33.787093Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.02678","last_updated":"2017-08-08T23:43:28Z","snapshot_observed_at":"2026-08-14T20:42:27.346153Z","submitted_at":"2017-08-08T23:43:28Z","title":"DirectDM: a tool for dark matter direct detection","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.02678","snapshot_observed_at":"2026-08-04T21:32:33.909008Z","title":"Bishara, J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:33.909008Z"},"links":{"cited_paper":"/paper/1708.02678","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:3aeb27e24c7fc4d9469019db1cee69d6fa6abb508977621618a6ff019377d8e6","observation_id":"61e6e691-a07a-4518-bd1e-aa627a620b9c","resolution":{"observed_at":"2026-08-04T21:32:33.909008Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.06998","last_updated":"2017-11-14T17:28:34Z","snapshot_observed_at":"2026-08-17T16:49:39.328103Z","submitted_at":"2017-07-21T18:00:00Z","title":"From quarks to nucleons in dark matter direct detection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.06998","snapshot_observed_at":"2026-08-04T21:32:34.087842Z","title":"Bishara, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:34.087842Z"},"links":{"cited_paper":"/paper/1707.06998","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:6f3165009fe88cda5db21bd2c28f048ca4e77780798d64caa5103ac8ec682d3c","observation_id":"e64d02f5-2839-4539-9042-dfbe05df888f","resolution":{"observed_at":"2026-08-04T21:32:34.087842Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.10218","last_updated":"2023-05-23T17:16:05Z","snapshot_observed_at":"2026-08-17T04:15:36.758157Z","submitted_at":"2017-10-27T16:07:30Z","title":"Effective Field Theory for Dark Matter Direct Detection up to Dimension Seven","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.10218","snapshot_observed_at":"2026-08-04T21:32:34.208258Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:34.208258Z"},"links":{"cited_paper":"/paper/1710.10218","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:a7f398ab49cb2409fb33f8250d626fadc9bfdc26403c51e39267b82e78a4e6de","observation_id":"c86c55c3-afc7-4e9c-93c0-b2ee06240953","resolution":{"observed_at":"2026-08-04T21:32:34.208258Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1308.6288","last_updated":"2013-08-28T20:00:08Z","snapshot_observed_at":"2026-08-15T00:05:08.250977Z","submitted_at":"2013-08-28T20:00:08Z","title":"Model-independent WIMP Scattering Responses and Event Rates: A Mathematica Package for Experimental Analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1308.6288","snapshot_observed_at":"2026-08-04T21:32:34.336814Z","title":"Anand, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-04T21:32:34.336814Z"},"links":{"cited_paper":"/paper/1308.6288","citing_paper":"/paper/2509.08050"},"observation_digest":"sha256:a0996fd5d2b8e122f6b7ff991eb5009b97630337be3db96bd4b04f525e49beca","observation_id":"26b6e996-aa3c-418b-9df9-d5ee1fa8b231","resolution":{"observed_at":"2026-08-04T21:32:34.336814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2509.08050","last_updated":"2025-09-09T18:00:02Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-17T13:51:37.667139Z","submitted_at":"2025-09-09T18:00:02Z","title":"Constraining Effective Field Theories for dark matter candidates annihilating into gamma-ray lines with CTAO"},"reference_resolution":{"displayed":54,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":37,"verified_exact":16,"verified_fuzzy":1},"total_outbound_references":54},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 54 of 54 outbound references and 2 inbound Pith citation observations for arXiv:2509.08050."}