{"as_of":"2026-08-08T05:53:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:947e0c0a91d9fdb1fc1626e84f403cbc1fbeae1172643d4232784abba98e164e","coverage":[{"denominator":84,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":84,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T12:04:38.614827Z","state":"measured"},{"denominator":88,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":88,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T06:58:15.966490Z","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":"2026-05-20T04:08:02.814605Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"cited_work":{"arxiv_id":"2506.00847","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2506.00847","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"fd7b2da4-b198-4b8e-969a-6fde1cf81a70","year":2023},"citing_paper":{"arxiv_id":"2605.20162","last_updated":"2026-05-19T17:49:34Z","snapshot_observed_at":"2026-07-06T23:30:49.211483Z","submitted_at":"2026-05-19T17:49:34Z","title":"Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess and Predictions for JUNO","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-05-20T04:04:42.736350Z"},"links":{"cited_paper":"/paper/2506.00847","citing_paper":"/paper/2605.20162"},"observation_digest":"sha256:73209905ad3352994503c2f928edef36fae6965ab634f817b89a4eefe8400fad","observation_id":"7d975c15-1c78-4c36-9bb6-4dfd7697bae2","resolution":{"observed_at":"2026-05-20T04:08:02.817622Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.00847","snapshot_observed_at":"2026-07-14T03:40:31.236252Z","title":"R., Crocker, R","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.11716","last_updated":"2026-07-15T09:15:59Z","snapshot_observed_at":"2026-08-08T02:19:43.579927Z","submitted_at":"2026-07-13T15:42:11Z","title":"Stellar flares cannot explain the Galactic 511 keV emission","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-14T03:40:31.236252Z"},"links":{"cited_paper":"/paper/2506.00847","citing_paper":"/paper/2607.11716"},"observation_digest":"sha256:fb04f320bc61c8b48ed9064d3211da030433b037dfcc55fc2ceeec96962ee940","observation_id":"b2a10246-20cd-48dc-bbd4-92722a34f83a","resolution":{"observed_at":"2026-07-14T03:40:31.236252Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.00847","snapshot_observed_at":"2026-08-02T06:58:15.966490Z","title":"R., Crocker, R","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.11716","last_updated":"2026-07-15T09:15:59Z","snapshot_observed_at":"2026-08-08T02:19:43.579927Z","submitted_at":"2026-07-13T15:42:11Z","title":"Stellar flares cannot explain the Galactic 511 keV emission","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-02T06:58:15.966490Z"},"links":{"cited_paper":"/paper/2506.00847","citing_paper":"/paper/2607.11716"},"observation_digest":"sha256:0e0e7c70234a068f9a96f3c6f025285d3674976e38dcf970e4774a80995d34c8","observation_id":"9e341335-f81a-46f9-aa24-260441699ee1","resolution":{"observed_at":"2026-08-02T06:58:15.966490Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.00847","snapshot_observed_at":"2026-08-02T02:40:30.341528Z","title":"R., Crocker, R","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.14276","last_updated":"2026-07-15T18:35:32Z","snapshot_observed_at":"2026-08-02T23:20:28.894906Z","submitted_at":"2026-07-15T18:35:32Z","title":"Cosmological $\\gamma$-$\\gamma$ Pair-Production Background","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-02T02:40:30.341528Z"},"links":{"cited_paper":"/paper/2506.00847","citing_paper":"/paper/2607.14276"},"observation_digest":"sha256:ce0d45c5febadf1e3ecb067aad24902658e57da9c5cc5032aee69181663310f6","observation_id":"618541a8-9880-4021-8a86-a9c0b028d3dd","resolution":{"observed_at":"2026-08-02T02:40:30.341528Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2506.00847/citation-record","integrity":"/paper/2506.00847/integrity","json":"/paper/2506.00847/citation-record.json","paper":"/paper/2506.00847"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:37.216011Z","title":"Johnson, W","venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.216011Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:1bd439a054857e1d9da228e8db7784cc5ee7a6a1be2d9c9171e47d33317d4ae6","observation_id":"9954b1b3-b491-4cda-9172-4fae4fa124ac","resolution":{"observed_at":"2026-08-07T12:04:37.216011Z","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":"2026-08-07T12:04:37.378785Z","title":"Leventhal, C","venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.378785Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:2f6e2e8d4480141cb0078d9502f6584edf4492dca734241bce22b48d365e8405","observation_id":"eeeaf003-e473-4e4c-ad16-bcf808c0c3da","resolution":{"observed_at":"2026-08-07T12:04:37.378785Z","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":"2026-08-07T12:04:37.554934Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.554934Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:bf6e175925368afc9185b1ee0cc665f126f48575d2981661fda8a3682da2de7c","observation_id":"ed1273a9-bf28-4df7-b68d-3c25245c05ad","resolution":{"observed_at":"2026-08-07T12:04:37.554934Z","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":"2026-08-07T12:04:37.585227Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.585227Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:74d477d136ebb993baa0c7f9daa86529f90e75703013e1971dcab50836ad7c7d","observation_id":"7956db7c-ab94-4a78-8060-7bdcc3c3735d","resolution":{"observed_at":"2026-08-07T12:04:37.585227Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0502324","last_updated":"2005-02-17T13:37:49Z","snapshot_observed_at":"2026-08-07T13:47:19.182145Z","submitted_at":"2005-02-16T17:48:07Z","title":"Astrophysical constraints from gamma-ray spectroscopy","version":2},"cited_work":{"arxiv_id":"astro-ph/0502324","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0502324","snapshot_observed_at":"2026-08-07T12:04:42.114138Z","title":"Astrophysical constraints from gamma-ray spectroscopy","venue":"astro-ph","work_id":"ec77dbed-3543-4613-949b-1023ac1865bd","year":2005},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.593688Z"},"links":{"cited_paper":"/paper/astro-ph/0502324","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:be0738775f94d31abf25859d0c693ecee9bb7ddcc0b86a3d6d79e962d8fbdf8f","observation_id":"0e3c20f4-f67c-4fbf-b924-5fd1e276b8de","resolution":{"observed_at":"2026-08-07T12:04:42.143164Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1009.4620","last_updated":"2010-09-23T14:13:01Z","snapshot_observed_at":"2026-08-06T23:52:55.540446Z","submitted_at":"2010-09-23T14:13:01Z","title":"The 511 keV emission from positron annihilation in the Galaxy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1009.4620","snapshot_observed_at":"2026-08-07T12:04:37.615293Z","title":"Prantzos, C","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.615293Z"},"links":{"cited_paper":"/paper/1009.4620","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:814b239a5e72bfa92216cd8f6ece142995c0dee9567f3e2af9626684ed876b01","observation_id":"e78501d4-0704-4855-9d18-6a9bbdfa8892","resolution":{"observed_at":"2026-08-07T12:04:37.615293Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.05569","last_updated":"2019-03-13T16:10:17Z","snapshot_observed_at":"2026-07-06T07:39:02.306834Z","submitted_at":"2019-03-13T16:10:17Z","title":"Positron Annihilation in the Galaxy","version":1},"cited_work":{"arxiv_id":"1903.05569","doi":null,"metadata_source":"pith","pith_arxiv_id":"1903.05569","snapshot_observed_at":"2026-08-07T12:04:42.018778Z","title":"Positron Annihilation in the Galaxy","venue":"astro-ph.HE","work_id":"43b74dcb-51fa-4841-b8a3-79f6991820c6","year":2019},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.620108Z"},"links":{"cited_paper":"/paper/1903.05569","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:0f38df6d996f622e6db5176bbc4c330f5d485bdf9531e1d48ae6e36f00c778af","observation_id":"efbff27f-cf1a-40d0-82a2-855cba471d28","resolution":{"observed_at":"2026-08-07T12:04:42.053111Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.15582","last_updated":"2023-03-27T20:26:36Z","snapshot_observed_at":"2026-08-02T11:14:26.744383Z","submitted_at":"2023-03-27T20:26:36Z","title":"The Positron Puzzle","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.15582","snapshot_observed_at":"2026-08-07T12:04:37.624016Z","title":"Siegert, The Positron Puzzle, Ap&SS 368, 27 (2023), arXiv:2303.15582 [astro-ph.HE]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.624016Z"},"links":{"cited_paper":"/paper/2303.15582","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:b8622a0a4184b23b827bacb011b51df33f4d0164a27812e1317d79f670e3c303","observation_id":"10c5fe89-905b-4b66-91bd-9c0358ca7f9d","resolution":{"observed_at":"2026-08-07T12:04:37.624016Z","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":"2026-08-07T12:04:42.622070Z","title":null,"venue":null,"work_id":"9353fdc5-317a-4430-8559-712d24c6c680","year":1981},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.627933Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:07626c007ec5235326e82b9184b0d3be19c9a674b176f11e3a51425155531708","observation_id":"b8573457-dec7-4bc1-9501-edcc8fb5c5d3","resolution":{"observed_at":"2026-08-07T12:04:42.643168Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1512.00325","last_updated":"2015-12-01T16:38:46Z","snapshot_observed_at":"2026-08-05T09:12:31.882467Z","submitted_at":"2015-12-01T16:38:46Z","title":"Gamma-ray spectroscopy of Positron Annihilation in the Milky Way","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.00325","snapshot_observed_at":"2026-08-07T12:04:37.631616Z","title":"Siegert, R","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.631616Z"},"links":{"cited_paper":"/paper/1512.00325","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:2848e51adfe05db1ca29a8d60fdf7a2efd97d0247a22446580bec91e8e707393","observation_id":"29c40c14-e448-45f3-9d39-eb90c3b796ab","resolution":{"observed_at":"2026-08-07T12:04:37.631616Z","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":"2026-08-07T12:04:42.561827Z","title":"Chan and R","venue":null,"work_id":"db839b33-971a-48c3-9e20-970abfe33f3e","year":1993},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.635557Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:8bbbe883d972c39c2be6a2fd67b891758a01e0f2b841b9b49597c1e76a93bcfa","observation_id":"e5b69270-1547-4563-8731-0a2cb51a08e8","resolution":{"observed_at":"2026-08-07T12:04:42.583009Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0309442","last_updated":"2003-09-16T14:29:18Z","snapshot_observed_at":"2026-07-07T00:36:26.782280Z","submitted_at":"2003-09-16T14:29:18Z","title":"Early SPI/INTEGRAL contraints on the morphology of the 511 keV line emission in the 4th galactic quadrant","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0309442","snapshot_observed_at":"2026-08-07T12:04:37.639070Z","title":"Kn¨ odlseder, V","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.639070Z"},"links":{"cited_paper":"/paper/astro-ph/0309442","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:7c0d52807c6205cf7fe6862d36bc29b015b86f9e86c47f2e9be6bfa6e868c3f4","observation_id":"5c6cfe93-be2e-4083-9150-ed387c986c2a","resolution":{"observed_at":"2026-08-07T12:04:37.639070Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506026","last_updated":"2005-06-01T18:47:26Z","snapshot_observed_at":"2026-07-07T00:50:59.920722Z","submitted_at":"2005-06-01T18:47:26Z","title":"The all-sky distribution of 511 keV electron-positron annihilation emission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0506026","snapshot_observed_at":"2026-08-07T12:04:37.643002Z","title":"Kn¨ odlseder, P","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.643002Z"},"links":{"cited_paper":"/paper/astro-ph/0506026","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:0e1644ce18c6cf22e1edaabef5f50efdade76e9e69fbd0dcdb5f72708d9585a3","observation_id":"09b026dc-e74e-4014-a2d4-053bcc4a05ba","resolution":{"observed_at":"2026-08-07T12:04:37.643002Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0601673","last_updated":"2006-01-30T10:56:56Z","snapshot_observed_at":"2026-07-07T00:57:58.115447Z","submitted_at":"2006-01-30T10:56:56Z","title":"The sky distribution of positronium annihilation continuum emission measured with SPI/INTEGRAL","version":1},"cited_work":{"arxiv_id":"astro-ph/0601673","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0601673","snapshot_observed_at":"2026-08-07T12:04:41.907110Z","title":"The sky distribution of positronium annihilation continuum emission measured with SPI/INTEGRAL","venue":"astro-ph","work_id":"1a975d3f-d59d-48f9-a161-418f3d91b829","year":2006},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.647024Z"},"links":{"cited_paper":"/paper/astro-ph/0601673","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:5cec1440f9d91fd3ec15cf2dd00c89f3c2fed71d90752c7ff1e0cb505adb0860","observation_id":"c21ce4f4-cc83-43af-b44b-a72622f06118","resolution":{"observed_at":"2026-08-07T12:04:41.923090Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0511190","last_updated":"2005-12-13T13:50:50Z","snapshot_observed_at":"2026-07-07T00:55:41.327148Z","submitted_at":"2005-11-07T17:27:27Z","title":"On the intensity and spatial morphology of the 511 keV emission in the Milky Way","version":2},"cited_work":{"arxiv_id":"astro-ph/0511190","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0511190","snapshot_observed_at":"2026-08-07T12:04:41.834459Z","title":"On the intensity and spatial morphology of the 511 keV emission in the Milky Way","venue":"astro-ph","work_id":"3dbc903e-cd52-4acc-bcd4-4c6c6570bfbc","year":2005},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.651114Z"},"links":{"cited_paper":"/paper/astro-ph/0511190","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:6edd45fa85426cb39b11e4b98ecee156fbfe0df806f9e08152f54cbef61a17aa","observation_id":"677895a9-5ef1-48ab-b1d3-64108f5acd11","resolution":{"observed_at":"2026-08-07T12:04:41.860613Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1007.4753","last_updated":"2010-07-27T15:32:40Z","snapshot_observed_at":"2026-07-06T02:13:20.470291Z","submitted_at":"2010-07-27T15:32:40Z","title":"On the morphology of the electron-positron annihilation emission as seen by SPI/INTEGRAL","version":1},"cited_work":{"arxiv_id":"1007.4753","doi":null,"metadata_source":"pith","pith_arxiv_id":"1007.4753","snapshot_observed_at":"2026-08-07T12:04:41.759875Z","title":"On the morphology of the electron-positron annihilation emission as seen by SPI/INTEGRAL","venue":"astro-ph.HE","work_id":"7c93fa8d-ddf4-478c-9c2d-6b3b51ae8666","year":2010},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.654901Z"},"links":{"cited_paper":"/paper/1007.4753","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:9e2fd5d5f468af6297b886560b3f9051bc705771859db0524336adbc05472878","observation_id":"98440275-82dc-47ac-ace9-f4283c02fb82","resolution":{"observed_at":"2026-08-07T12:04:41.792058Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03495","last_updated":"2017-05-24T01:51:47Z","snapshot_observed_at":"2026-07-06T05:03:20.569229Z","submitted_at":"2016-07-12T20:00:22Z","title":"Diffuse Galactic antimatter from faint thermonuclear supernovae in old stellar populations","version":2},"cited_work":{"arxiv_id":"1607.03495","doi":null,"metadata_source":"pith","pith_arxiv_id":"1607.03495","snapshot_observed_at":"2026-08-07T12:04:41.694721Z","title":"Diffuse Galactic antimatter from faint thermonuclear supernovae in old stellar populations","venue":"astro-ph.HE","work_id":"68df4db4-f8c1-4ea3-8796-e49fa1cc87ea","year":2016},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.658914Z"},"links":{"cited_paper":"/paper/1607.03495","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:06add3c6f5877302ce3c54c61187376bfc67d52f28ea0eeb15074ccc1f39dd14","observation_id":"6fb192d4-eea6-4979-b313-f03175a394da","resolution":{"observed_at":"2026-08-07T12:04:41.719592Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2202.05417","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:41.638612Z","title":null,"venue":null,"work_id":"e5f3e503-f347-40fa-93ab-4c56ee372736","year":2022},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.662780Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:92fe34ba9c4e192e9a0eac26b86d0a262dc017de449b268d616b7316748c6000","observation_id":"d0a90931-c855-4c2b-be2a-7c8f3549564c","resolution":{"observed_at":"2026-08-07T12:04:41.661604Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0909.4022","last_updated":"2009-09-22T15:30:54Z","snapshot_observed_at":"2026-07-06T01:57:42.558030Z","submitted_at":"2009-09-22T15:30:54Z","title":"Positron transport in the interstellar medium","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.4022","snapshot_observed_at":"2026-08-07T12:04:37.666190Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.666190Z"},"links":{"cited_paper":"/paper/0909.4022","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:c86b72365c5fcb4ef515b5bc29b6c3f65876acc7f77463c81638cc322eec3eb0","observation_id":"4f85b763-ae6e-4a68-99a9-e170c67b2215","resolution":{"observed_at":"2026-08-07T12:04:37.666190Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.3008","last_updated":"2009-04-06T19:59:02Z","snapshot_observed_at":"2026-07-06T01:35:46.153755Z","submitted_at":"2007-11-19T23:56:15Z","title":"The Galactic Positron Annihilation Radiation & The Propagation of Positrons in the Interstellar Medium","version":3},"cited_work":{"arxiv_id":"0711.3008","doi":null,"metadata_source":"pith","pith_arxiv_id":"0711.3008","snapshot_observed_at":"2026-08-07T12:04:41.483685Z","title":"The Galactic Positron Annihilation Radiation & The Propagation of Positrons in the Interstellar Medium","venue":"astro-ph","work_id":"8acd7f0a-0ee2-4641-9b3a-037f92ba1340","year":2007},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.669832Z"},"links":{"cited_paper":"/paper/0711.3008","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:8519bd8684a9c7536951051b8e33dad623fdc83b483921453cfcf16d47a7942b","observation_id":"62589421-a46c-46eb-9abd-7c9c12985d6a","resolution":{"observed_at":"2026-08-07T12:04:41.524816Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0904.1025","last_updated":"2009-06-15T15:57:29Z","snapshot_observed_at":"2026-07-06T01:53:48.581253Z","submitted_at":"2009-04-06T22:24:54Z","title":"Is There a Dark Matter Signal in the Galactic Positron Annihilation Radiation?","version":3},"cited_work":{"arxiv_id":"0904.1025","doi":null,"metadata_source":"pith","pith_arxiv_id":"0904.1025","snapshot_observed_at":"2026-08-07T12:04:41.408243Z","title":"Is There a Dark Matter Signal in the Galactic Positron Annihilation Radiation?","venue":"astro-ph.HE","work_id":"48b7b612-fb95-434d-9e5c-f2c37290675a","year":2009},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.673532Z"},"links":{"cited_paper":"/paper/0904.1025","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:1f6115e293a80c093cd41fa13a595872c3f567b3ef0680073e71072c7b6b8e1d","observation_id":"eebc5c8e-cc2f-40d8-8a74-fe2b316de831","resolution":{"observed_at":"2026-08-07T12:04:41.422009Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1801.09365","last_updated":"2018-03-18T22:30:14Z","snapshot_observed_at":"2026-07-06T06:20:37.701340Z","submitted_at":"2018-01-29T05:20:47Z","title":"Positron Transport And Annihilation In The Galactic Bulge","version":2},"cited_work":{"arxiv_id":"1801.09365","doi":null,"metadata_source":"pith","pith_arxiv_id":"1801.09365","snapshot_observed_at":"2026-08-07T12:04:41.325356Z","title":"Positron Transport And Annihilation In The Galactic Bulge","venue":"astro-ph.HE","work_id":"452540f8-3335-47e5-a745-3c0cad455f5b","year":2018},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.677492Z"},"links":{"cited_paper":"/paper/1801.09365","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:3fd2f0684072f3c7337f020f2aa9aaaadc1cffb726f5eff0225eae9e1f8bfe1a","observation_id":"51638f38-2048-4ab9-933f-a6495672c569","resolution":{"observed_at":"2026-08-07T12:04:41.360507Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2109.03691","last_updated":"2021-09-08T14:54:12Z","snapshot_observed_at":"2026-07-06T11:45:39.359567Z","submitted_at":"2021-09-08T14:54:12Z","title":"Measuring the smearing of the Galactic 511 keV signal: positron propagation or supernova kicks?","version":1},"cited_work":{"arxiv_id":"2109.03691","doi":null,"metadata_source":"pith","pith_arxiv_id":"2109.03691","snapshot_observed_at":"2026-08-07T12:04:41.257675Z","title":"Measuring the smearing of the Galactic 511 keV signal: positron propagation or supernova kicks?","venue":"astro-ph.HE","work_id":"4a3545ab-b526-4413-b10f-036e759a923d","year":2021},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.681439Z"},"links":{"cited_paper":"/paper/2109.03691","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:2baa9af466411bbc215dfb67965874c926e3f0100437bae6a5e0a061ca26db59","observation_id":"cde6c4ea-4cbf-49df-acf0-621dc61a0255","resolution":{"observed_at":"2026-08-07T12:04:41.285205Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.04979","last_updated":"2024-04-24T13:28:52Z","snapshot_observed_at":"2026-07-06T16:44:55.494764Z","submitted_at":"2023-11-08T19:01:34Z","title":"Importance of cosmic ray propagation on sub-GeV dark matter constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.04979","snapshot_observed_at":"2026-08-07T12:04:37.685105Z","title":"De la Torre Luque, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.685105Z"},"links":{"cited_paper":"/paper/2311.04979","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:a0869b7e21e0c77a1890ab388611861e9184d48d2d9fc7fb1dcd7ea1590a15c9","observation_id":"e7e0100a-7a0d-4e46-88ce-d405becda115","resolution":{"observed_at":"2026-08-07T12:04:37.685105Z","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":"ph/0509760","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:41.172281Z","title":null,"venue":null,"work_id":"0a77aea8-94f8-4f78-8671-0dafc50a9712","year":2006},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.688680Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:17b53d0d9359ba50cdbba2d0049a3549c7832e53f32026c661f8ddac1040826f","observation_id":"088291a8-0b95-4152-882c-a38eaf3714a7","resolution":{"observed_at":"2026-08-07T12:04:41.200736Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0204183","last_updated":"2002-06-04T15:18:39Z","snapshot_observed_at":"2026-07-07T00:25:56.846184Z","submitted_at":"2002-04-11T19:05:44Z","title":"Cosmic Rays from Microquasars: a Narrow Component to the CR Spectrum?","version":2},"cited_work":{"arxiv_id":"astro-ph/0204183","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0204183","snapshot_observed_at":"2026-08-07T12:04:41.050636Z","title":"Cosmic Rays from Microquasars: a Narrow Component to the CR Spectrum?","venue":"astro-ph","work_id":"eb4e8f91-251d-4dfc-aa54-51458a351dc9","year":2002},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.692190Z"},"links":{"cited_paper":"/paper/astro-ph/0204183","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:fa3de174747517598c6eb5f5a4bc55ad6ad5125f763b60149a5ef7271a7c36c9","observation_id":"c96caf8f-5029-43f0-bc9a-951b235a821c","resolution":{"observed_at":"2026-08-07T12:04:41.079156Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0607296","last_updated":"2006-07-13T13:12:52Z","snapshot_observed_at":"2026-08-03T06:39:30.229939Z","submitted_at":"2006-07-13T13:12:52Z","title":"Microquasars as sources of positron annihilation radiation","version":1},"cited_work":{"arxiv_id":"astro-ph/0607296","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0607296","snapshot_observed_at":"2026-08-07T12:04:40.983746Z","title":"Microquasars as sources of positron annihilation radiation","venue":"astro-ph","work_id":"b70765db-9483-46c2-a2fc-673056d330ec","year":2006},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.696242Z"},"links":{"cited_paper":"/paper/astro-ph/0607296","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:17de05be28d5bea08cc37f6977772e70274936ce925cfcb830f4158abe57f8a2","observation_id":"cbc0be99-294c-4607-bb03-66d28a32058a","resolution":{"observed_at":"2026-08-07T12:04:41.007776Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.01169","last_updated":"2016-04-15T15:54:23Z","snapshot_observed_at":"2026-07-06T04:48:13.149101Z","submitted_at":"2016-03-03T16:51:14Z","title":"Positron annihilation signatures associated with the outburst of the microquasar V404 Cygni","version":2},"cited_work":{"arxiv_id":"1603.01169","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.01169","snapshot_observed_at":"2026-08-07T12:04:40.913201Z","title":"Positron annihilation signatures associated with the outburst of the microquasar V404 Cygni","venue":"astro-ph.HE","work_id":"f6d98f6c-211d-470f-bbc5-9742b1100555","year":2016},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.699958Z"},"links":{"cited_paper":"/paper/1603.01169","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:a088af3a1b7b21005e6c4b764216818fb1fad3600554ce1e591a782f61fa3e65","observation_id":"077e19cd-509e-4339-a082-43fa9848c549","resolution":{"observed_at":"2026-08-07T12:04:40.939173Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:42.484106Z","title":"Weidenspointner, G","venue":null,"work_id":"eb12a1db-f562-48cc-bc1e-195cf25efb9e","year":2008},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.703995Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:fbedb9136554efe97a5b917a5e0ceb2b55344f106361c525e260595bad9b2f89","observation_id":"6b3f33b2-d3d2-4d93-bd4c-c78deb9fd91f","resolution":{"observed_at":"2026-08-07T12:04:42.522827Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:42.425262Z","title":"Weidenspointner, G","venue":null,"work_id":"4d99dead-47c4-430d-ac5b-2189188c9e89","year":2008},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.707881Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:f174362ba04d376cfb73799b0a95abbf140014d214fbb150ad1de6a3474b5d0a","observation_id":"0fdd33e0-0ffd-4be8-9582-c82675a583d1","resolution":{"observed_at":"2026-08-07T12:04:42.452907Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1803.04370","last_updated":"2018-03-12T16:55:07Z","snapshot_observed_at":"2026-07-06T06:27:50.936953Z","submitted_at":"2018-03-12T16:55:07Z","title":"Galactic Binaries Can Explain the Fermi Galactic Center Excess and 511 keV Emission","version":1},"cited_work":{"arxiv_id":"1803.04370","doi":null,"metadata_source":"pith","pith_arxiv_id":"1803.04370","snapshot_observed_at":"2026-08-07T12:04:40.850660Z","title":"Galactic Binaries Can Explain the Fermi Galactic Center Excess and 511 keV Emission","venue":"astro-ph.HE","work_id":"ed3a5cc0-b8fc-4578-a4d1-ddb66381e1ce","year":2018},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.711957Z"},"links":{"cited_paper":"/paper/1803.04370","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:78e6107cb3075b828f21f53c356a71a80dfc1992bb710eb8a10f3fc67ff67868","observation_id":"4fe1937b-a682-40ba-8022-b6cd1f68687d","resolution":{"observed_at":"2026-08-07T12:04:40.867030Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.00133","last_updated":"2019-03-31T21:54:30Z","snapshot_observed_at":"2026-07-06T07:11:55.047580Z","submitted_at":"2018-10-31T21:46:44Z","title":"Positrons and 511 keV radiation as tracers of recent binary neutron star mergers","version":3},"cited_work":{"arxiv_id":"1811.00133","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.00133","snapshot_observed_at":"2026-08-07T12:04:40.789417Z","title":"Positrons and 511 keV radiation as tracers of recent binary neutron star mergers","venue":"astro-ph.HE","work_id":"1a20b9a5-fb9d-4721-baf0-b3200645292e","year":2018},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.716064Z"},"links":{"cited_paper":"/paper/1811.00133","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:f5b638e748d14609889c64ad0b02b0c6c756813f35898c66639109f84799fa7d","observation_id":"b57820aa-448c-4811-a6b7-564bb9346f67","resolution":{"observed_at":"2026-08-07T12:04:40.812768Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:37.720040Z","title":"Boehm, D","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.720040Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:b5192fea70dcf7de753c076c46ee80bcc5fd6d225e9725c4cc4385199adbf289","observation_id":"e53c2131-a17e-4d5e-b97f-6dee228e2bf7","resolution":{"observed_at":"2026-08-07T12:04:37.720040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0402220","last_updated":"2004-11-29T20:50:45Z","snapshot_observed_at":"2026-07-07T04:02:56.450035Z","submitted_at":"2004-02-20T21:43:33Z","title":"Possible Evidence For Axino Dark Matter In The Galactic Bulge","version":3},"cited_work":{"arxiv_id":"hep-ph/0402220","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0402220","snapshot_observed_at":"2026-08-07T12:04:40.648949Z","title":"Possible Evidence For Axino Dark Matter In The Galactic Bulge","venue":"hep-ph","work_id":"696e0856-f218-49e3-a613-591ee2cad230","year":2004},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.723728Z"},"links":{"cited_paper":"/paper/hep-ph/0402220","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:d6454a3bcaaa46fdec05360514a67335a5c8a745d6cb36577df5a2a34511572b","observation_id":"fbbad101-df5f-4241-b8fe-a3f42d3d9466","resolution":{"observed_at":"2026-08-07T12:04:40.678875Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0507142","last_updated":"2006-09-07T14:32:50Z","snapshot_observed_at":"2026-07-07T00:52:03.341999Z","submitted_at":"2005-07-06T18:12:58Z","title":"Constraints on dark matter and the shape of the Milky Way dark halo from the 511 keV line","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0507142","snapshot_observed_at":"2026-08-07T12:04:37.727960Z","title":"Ascasibar, P","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.727960Z"},"links":{"cited_paper":"/paper/astro-ph/0507142","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:9d53b9393c896898ef431cf087d8c871d025e1355d3530790cc8ef7783523154","observation_id":"8510ece4-8952-4ddc-95a0-a89db0c54bf6","resolution":{"observed_at":"2026-08-07T12:04:37.727960Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0703128","last_updated":"2007-03-12T17:58:37Z","snapshot_observed_at":"2026-08-01T19:02:24.242744Z","submitted_at":"2007-03-12T17:58:37Z","title":"The galactic 511 keV line from electroweak scale WIMPs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0703128","snapshot_observed_at":"2026-08-07T12:04:37.732458Z","title":"Pospelov and A","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.732458Z"},"links":{"cited_paper":"/paper/hep-ph/0703128","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:5c9e8ff3e94352e1dc0f2e72559dc9e290a24fe0c60a6765118de2db32604376","observation_id":"cab28a1d-8bcb-46ea-8bb6-bdcfb1ffa262","resolution":{"observed_at":"2026-08-07T12:04:37.732458Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0810.0713","last_updated":"2009-01-20T06:02:39Z","snapshot_observed_at":"2026-08-04T15:47:39.239482Z","submitted_at":"2008-10-06T19:59:30Z","title":"A Theory of Dark Matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0810.0713","snapshot_observed_at":"2026-08-07T12:04:37.736527Z","title":"Arkani-Hamed, D","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.736527Z"},"links":{"cited_paper":"/paper/0810.0713","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:5b5b3e574ffa12fc6d6643591f7a2b20276b9f88823d826a37c2fff18d748338","observation_id":"42dfda8f-7345-4a91-b019-dfbe5ba05e8b","resolution":{"observed_at":"2026-08-07T12:04:37.736527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.0997","last_updated":"2012-04-27T15:06:21Z","snapshot_observed_at":"2026-07-06T02:40:24.511144Z","submitted_at":"2012-01-04T21:00:01Z","title":"Interacting dark matter contribution to the Galactic 511 keV gamma ray emission: constraining the morphology with INTEGRAL/SPI observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.0997","snapshot_observed_at":"2026-08-07T12:04:37.740506Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.740506Z"},"links":{"cited_paper":"/paper/1201.0997","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:d81648310c87104f2bb49068a42a54992709f9c76c4228595b4a0aa8c179e0bc","observation_id":"8785e21a-7fa3-4da1-9ce5-91edcad190d3","resolution":{"observed_at":"2026-08-07T12:04:37.740506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.09105","last_updated":"2021-01-30T18:50:35Z","snapshot_observed_at":"2026-08-05T17:40:42.194184Z","submitted_at":"2020-07-17T16:32:50Z","title":"Dark matter models for the 511 keV galactic line predict keV electron recoils on Earth","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.09105","snapshot_observed_at":"2026-08-07T12:04:37.744996Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.744996Z"},"links":{"cited_paper":"/paper/2007.09105","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:12d2b7d9e77fe88f463000057d645e570fc28b9a8b0e7f5f922f76bccd6deaf5","observation_id":"2b855733-8c90-45c5-b9ee-e8a2e1c92ba1","resolution":{"observed_at":"2026-08-07T12:04:37.744996Z","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":"2026-08-07T12:04:37.749404Z","title":"De la Torre Luque, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.749404Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:63d930da5f91b22bcbfce73c5fcb2065e8d971d80be0f670c5c289252e66627e","observation_id":"9cd47a03-ff22-4f19-8b17-4873ba20332f","resolution":{"observed_at":"2026-08-07T12:04:37.749404Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0702587","last_updated":"2007-05-10T16:16:34Z","snapshot_observed_at":"2026-07-07T01:07:24.441719Z","submitted_at":"2007-02-21T21:15:02Z","title":"Exciting Dark Matter and the INTEGRAL/SPI 511 keV signal","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0702587","snapshot_observed_at":"2026-08-07T12:04:37.753922Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.753922Z"},"links":{"cited_paper":"/paper/astro-ph/0702587","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:ca0639849fe6e915a9ff4ea8f9de23743fb45c51ef2df22df476e022884da06c","observation_id":"49560e82-22a9-4748-9fdd-399e9006a8b7","resolution":{"observed_at":"2026-08-07T12:04:37.753922Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0903.1037","last_updated":"2009-06-25T18:03:54Z","snapshot_observed_at":"2026-08-02T12:23:18.487574Z","submitted_at":"2009-03-05T18:00:42Z","title":"PAMELA, DAMA, INTEGRAL and Signatures of Metastable Excited WIMPs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0903.1037","snapshot_observed_at":"2026-08-07T12:04:37.758002Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.758002Z"},"links":{"cited_paper":"/paper/0903.1037","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:96489093d408480684a0262cafe929421d8107396a859c403f3f661d301a2de4","observation_id":"8812b81a-225e-42df-8538-5b3261263d65","resolution":{"observed_at":"2026-08-07T12:04:37.758002Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.4327","last_updated":"2009-10-24T22:52:11Z","snapshot_observed_at":"2026-07-06T01:53:50.355511Z","submitted_at":"2009-01-27T20:33:55Z","title":"A new twist on excited dark matter: implications for INTEGRAL, PAMELA/ATIC/PPB-BETS, DAMA","version":5},"cited_work":{"arxiv_id":"0901.4327","doi":null,"metadata_source":"pith","pith_arxiv_id":"0901.4327","snapshot_observed_at":"2026-08-07T12:04:40.410868Z","title":"A new twist on excited dark matter: implications for INTEGRAL, PAMELA/ATIC/PPB-BETS, DAMA","venue":"hep-ph","work_id":"e0ea342c-9a43-4fe8-9016-be58a52fa714","year":2009},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.762165Z"},"links":{"cited_paper":"/paper/0901.4327","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:0bce91afe4cbfb43b3bd5212b3840adbebea32806839de306749ae97354aaf98","observation_id":"cc1c175e-6037-433d-a2de-73faee31fb16","resolution":{"observed_at":"2026-08-07T12:04:40.435959Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0911.2222","last_updated":"2010-01-28T22:19:00Z","snapshot_observed_at":"2026-07-06T02:03:41.041380Z","submitted_at":"2009-11-12T18:39:50Z","title":"Exciting dark matter in the galactic center","version":3},"cited_work":{"arxiv_id":"0911.2222","doi":null,"metadata_source":"pith","pith_arxiv_id":"0911.2222","snapshot_observed_at":"2026-08-07T12:04:40.333379Z","title":"Exciting dark matter in the galactic center","venue":"hep-ph","work_id":"0bb4bcb8-989c-4f54-8928-e1780874bd8d","year":2009},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.766511Z"},"links":{"cited_paper":"/paper/0911.2222","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:4e2e72e296bf133e0975793275917680a923df1b973f58a4ef911a6518aaf2ee","observation_id":"b5184b57-5959-445e-9366-48f7ac863077","resolution":{"observed_at":"2026-08-07T12:04:40.363723Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1008.1784","last_updated":"2011-08-15T18:04:50Z","snapshot_observed_at":"2026-07-06T02:14:02.714262Z","submitted_at":"2010-08-10T20:00:02Z","title":"Metastable dark matter mechanisms for INTEGRAL 511 keV $\\gamma$ rays and DAMA/CoGeNT events","version":4},"cited_work":{"arxiv_id":"1008.1784","doi":null,"metadata_source":"pith","pith_arxiv_id":"1008.1784","snapshot_observed_at":"2026-08-07T12:04:40.269487Z","title":"Metastable dark matter mechanisms for INTEGRAL 511 keV $\\gamma$ rays and DAMA/CoGeNT events","venue":"hep-ph","work_id":"58acb1a7-9034-4ca0-94da-2cf9dfdae7a7","year":2010},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.772823Z"},"links":{"cited_paper":"/paper/1008.1784","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:b57e3a67713f69358958a633893581522a777e8a4f84ef2d4f08a0d275edbdd3","observation_id":"d2612fa0-5dff-41ec-b632-a22f4954530d","resolution":{"observed_at":"2026-08-07T12:04:40.293522Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1204.1965","last_updated":"2012-07-04T22:11:47Z","snapshot_observed_at":"2026-07-06T02:46:02.046654Z","submitted_at":"2012-04-09T19:59:58Z","title":"Abelian dark matter models for 511 keV gamma rays and direct detection","version":2},"cited_work":{"arxiv_id":"1204.1965","doi":null,"metadata_source":"pith","pith_arxiv_id":"1204.1965","snapshot_observed_at":"2026-08-07T12:04:40.209956Z","title":"Abelian dark matter models for 511 keV gamma rays and direct detection","venue":"hep-ph","work_id":"c3452fa0-3a71-401e-aefb-bab551d1b2b3","year":2012},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.778960Z"},"links":{"cited_paper":"/paper/1204.1965","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:b4fc92705049856360c71e40182395ae32c6f023281ec3b28abfd814b7a9036d","observation_id":"2b54c727-f7bf-46d5-b5ba-917ab980f09c","resolution":{"observed_at":"2026-08-07T12:04:40.232055Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.15114","last_updated":"2024-02-07T22:05:39Z","snapshot_observed_at":"2026-08-07T11:29:26.269467Z","submitted_at":"2023-07-27T18:00:02Z","title":"The Morphology of Exciting Dark Matter and the Galactic 511 keV Signal","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.15114","snapshot_observed_at":"2026-08-07T12:04:37.785130Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.785130Z"},"links":{"cited_paper":"/paper/2307.15114","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:fa6aad5362625ca56153036b7bbd8c9bfc4e6a4215e6b5c4a1106516860e304a","observation_id":"d5e2e6d1-74f3-4eb7-8cef-797e5f66180b","resolution":{"observed_at":"2026-08-07T12:04:37.785130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.09994","last_updated":"2019-12-16T22:03:15Z","snapshot_observed_at":"2026-07-06T08:02:24.956980Z","submitted_at":"2019-06-24T14:31:02Z","title":"Primordial black holes as a dark matter candidate are severely constrained by the Galactic Center 511 keV gamma-ray line","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.09994","snapshot_observed_at":"2026-08-07T12:04:37.794022Z","title":"Laha, Primordial Black Holes as a Dark Matter Can- didate Are Severely Constrained by the Galactic Cen- ter 511 keV γ -Ray Line, Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.794022Z"},"links":{"cited_paper":"/paper/1906.09994","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:806ebbb5fc9bb7762baa4608b520d1d0d6dd4102a1fb246a3db86e7dc31fa318","observation_id":"6ccf10c9-d7d5-46e4-b775-b9d2a7b96556","resolution":{"observed_at":"2026-08-07T12:04:37.794022Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07740","last_updated":"2019-12-16T19:33:31Z","snapshot_observed_at":"2026-07-06T08:01:13.299477Z","submitted_at":"2019-06-18T18:01:35Z","title":"Constraining primordial black hole abundance with the Galactic 511 keV line","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.07740","snapshot_observed_at":"2026-08-07T12:04:37.800185Z","title":"DeRocco and P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.800185Z"},"links":{"cited_paper":"/paper/1906.07740","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:b184dd6e3421a00bb1a6daa294822e15153c609d9bed4aa5bc0e2988748a0a08","observation_id":"f83c8000-e494-4373-bd3f-c8a1bbfec17c","resolution":{"observed_at":"2026-08-07T12:04:37.800185Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.01014","last_updated":"2020-09-01T17:29:46Z","snapshot_observed_at":"2026-08-08T02:19:02.755600Z","submitted_at":"2019-12-02T19:00:03Z","title":"Neutrino and Positron Constraints on Spinning Primordial Black Hole Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.01014","snapshot_observed_at":"2026-08-07T12:04:37.806423Z","title":"Dasgupta, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.806423Z"},"links":{"cited_paper":"/paper/1912.01014","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:8d07348c16c6aae9bd3c55a253b4b62368561218f13bac6f479619f7d560264f","observation_id":"0626725e-d166-4fff-a030-a301a027d8a1","resolution":{"observed_at":"2026-08-07T12:04:37.806423Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.08611","last_updated":"2022-04-08T00:36:53Z","snapshot_observed_at":"2026-07-06T10:50:08.486666Z","submitted_at":"2021-03-15T18:00:04Z","title":"The 511 keV Excess and Primordial Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.08611","snapshot_observed_at":"2026-08-07T12:04:37.814978Z","title":"Keith and D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.814978Z"},"links":{"cited_paper":"/paper/2103.08611","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:4f8e231565e15b47d83949c70fe3563447e4d67ff87ef04f78bc9e69c3197151","observation_id":"1ed98d0b-493b-4a1e-a4d3-66dec22a9915","resolution":{"observed_at":"2026-08-07T12:04:37.814978Z","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":"2026-08-07T12:04:37.823851Z","title":"De la Torre Luque, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.823851Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:933e22ec9aedf6a1ee0e6f22c43f20b88628da2c27830b225f83ba3b737e1023","observation_id":"1c1bbb04-3d88-4dcd-b624-077c71fa7d4b","resolution":{"observed_at":"2026-08-07T12:04:37.823851Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.11804","last_updated":"2021-02-04T10:05:56Z","snapshot_observed_at":"2026-07-06T09:41:06.298363Z","submitted_at":"2020-07-23T05:41:42Z","title":"Constraints on a mixed model of dark matter particles and primordial black holes from the Galactic 511 keV line","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.11804","snapshot_observed_at":"2026-08-07T12:04:37.832102Z","title":"Cai, Y.-C","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.832102Z"},"links":{"cited_paper":"/paper/2007.11804","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:b2411101e680fa210daf7195dbe8ff2e61ec158050832bf3c62d18ed040f1025","observation_id":"6aab2c42-72ae-4413-8040-09d63fc2e7c9","resolution":{"observed_at":"2026-08-07T12:04:37.832102Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.16379","last_updated":"2025-09-05T09:00:53Z","snapshot_observed_at":"2026-07-06T19:37:20.613838Z","submitted_at":"2024-10-21T18:00:09Z","title":"511 keV Galactic Photons from a Dark Matter Spike","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.16379","snapshot_observed_at":"2026-08-07T12:04:37.840886Z","title":"De la Torre Luque, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.840886Z"},"links":{"cited_paper":"/paper/2410.16379","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:bb5a39dd475692a75800e40939d6703ae49ce6589503beeb5092acf31d9386a8","observation_id":"264cd34c-8911-4f9b-84bd-8bc0736825a6","resolution":{"observed_at":"2026-08-07T12:04:37.840886Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0512411","last_updated":"2006-08-15T19:34:33Z","snapshot_observed_at":"2026-07-07T00:56:58.454677Z","submitted_at":"2005-12-15T20:55:35Z","title":"Stringent Constraint on Galactic Positron Production","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0512411","snapshot_observed_at":"2026-08-07T12:04:37.849701Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.849701Z"},"links":{"cited_paper":"/paper/astro-ph/0512411","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:bdfdb73bc4e7b7ca15256f7aaa8f708e7096d150cadeee0b78bef57b5d338513","observation_id":"5b7111f5-4e90-4f66-9c7b-b02641c1608a","resolution":{"observed_at":"2026-08-07T12:04:37.849701Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0607374","last_updated":"2006-08-25T10:41:35Z","snapshot_observed_at":"2026-07-07T01:01:47.805745Z","submitted_at":"2006-07-17T13:17:28Z","title":"Continuum gamma-ray emission from light dark matter positrons and electrons","version":2},"cited_work":{"arxiv_id":"astro-ph/0607374","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0607374","snapshot_observed_at":"2026-08-07T12:04:39.966654Z","title":"Continuum gamma-ray emission from light dark matter positrons and electrons","venue":"astro-ph","work_id":"7a604cdb-76aa-44ad-ac54-52180a72cc0f","year":2006},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.859129Z"},"links":{"cited_paper":"/paper/astro-ph/0607374","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:42f12d47ec897d0990c47334263458ce6c6d936c778b2a740e53bf721b059970","observation_id":"d38aaf30-53d8-4348-89fd-8819feb164bf","resolution":{"observed_at":"2026-08-07T12:04:39.994293Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0702061","last_updated":"2007-02-02T11:13:24Z","snapshot_observed_at":"2026-07-07T01:06:50.744388Z","submitted_at":"2007-02-02T11:13:24Z","title":"Constraints on the injection energy of positrons in the Galactic centre region","version":1},"cited_work":{"arxiv_id":"astro-ph/0702061","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0702061","snapshot_observed_at":"2026-08-07T12:04:39.894008Z","title":"Constraints on the injection energy of positrons in the Galactic centre region","venue":"astro-ph","work_id":"0daaf927-30c3-4dab-9024-dbf7fc916262","year":2007},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.869549Z"},"links":{"cited_paper":"/paper/astro-ph/0702061","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:a65514e2301a373f7ab0e66aeb76e6886c0e134cc58410150935223454c96501","observation_id":"9500fc83-2951-4dec-aeb2-fb63ca1a05e1","resolution":{"observed_at":"2026-08-07T12:04:39.929599Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0711.4866","last_updated":"2007-11-30T04:11:22Z","snapshot_observed_at":"2026-07-06T01:32:55.493041Z","submitted_at":"2007-11-30T04:11:22Z","title":"Secluded WIMP Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.4866","snapshot_observed_at":"2026-08-07T12:04:37.879081Z","title":"Pospelov, A","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.879081Z"},"links":{"cited_paper":"/paper/0711.4866","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:6150fd8eeb07b6cbab3a7ef0f30e738894209196710c6c10cac727437edab27f","observation_id":"54711776-0a0f-492b-a9e8-484152a175d1","resolution":{"observed_at":"2026-08-07T12:04:37.879081Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.03811","last_updated":"2015-08-04T02:00:37Z","snapshot_observed_at":"2026-07-06T04:20:39.291510Z","submitted_at":"2015-06-11T20:00:20Z","title":"Indirect Dark Matter Signatures in the Cosmic Dark Ages I. Generalizing the Bound on s-wave Dark Matter Annihilation from Planck","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.03811","snapshot_observed_at":"2026-08-07T12:04:37.893911Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.893911Z"},"links":{"cited_paper":"/paper/1506.03811","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:b04147595ba5e20f46fbc991be9da066a64612eaf88e5b1b576f349e6c905c7e","observation_id":"3f211d6d-9911-48dc-9165-63fc8df41851","resolution":{"observed_at":"2026-08-07T12:04:37.893911Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.13838","last_updated":"2022-09-19T14:03:24Z","snapshot_observed_at":"2026-07-06T13:36:10.430479Z","submitted_at":"2022-07-28T00:27:20Z","title":"Cosmic Ray Interstellar Propagation Tool using It\\^o Calculus (criptic): software for simultaneous calculation of cosmic ray transport and observational signatures","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.13838","snapshot_observed_at":"2026-08-07T12:04:37.902980Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.902980Z"},"links":{"cited_paper":"/paper/2207.13838","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:2c2e0c1099e4185aac56f71a0d1a4f4080d03fcda6bf2c513d49d9c1f084b0ff","observation_id":"eba4ba38-c047-4a4a-8cab-219fd2fcb091","resolution":{"observed_at":"2026-08-07T12:04:37.902980Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.10139","last_updated":"2017-10-27T14:00:16Z","snapshot_observed_at":"2026-07-06T06:06:24.254908Z","submitted_at":"2017-10-27T14:00:16Z","title":"INTEGRAL/SPI $\\gamma$-ray line spectroscopy","version":1},"cited_work":{"arxiv_id":"1710.10139","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.10139","snapshot_observed_at":"2026-08-07T12:04:39.778805Z","title":"INTEGRAL/SPI $\\gamma$-ray line spectroscopy","venue":"astro-ph.IM","work_id":"06ebfbea-955c-47bc-8c60-9fd4086ba2b3","year":2017},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.911151Z"},"links":{"cited_paper":"/paper/1710.10139","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:4c654556746e97bb97b43f59bb7e44fe9e1d276961d6ba4418ca195b375b09b6","observation_id":"fa42e3f5-574c-42a1-b6ac-db9b1d18cd9e","resolution":{"observed_at":"2026-08-07T12:04:39.808063Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2202.04574","last_updated":"2022-02-09T17:14:28Z","snapshot_observed_at":"2026-07-06T12:36:08.031641Z","submitted_at":"2022-02-09T17:14:28Z","title":"Diffuse Galactic emission spectrum between 0.5 and 8.0 MeV","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.04574","snapshot_observed_at":"2026-08-07T12:04:37.945574Z","title":"Siegert, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.945574Z"},"links":{"cited_paper":"/paper/2202.04574","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:55d72264309ddbd49169e9630d78ea3bc47ee58da80b1e08fc7f8f3f7aed1a46","observation_id":"dc712e62-89b8-4d1e-baa8-31c9d18d0250","resolution":{"observed_at":"2026-08-07T12:04:37.945574Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.0864","last_updated":"2010-10-05T12:30:24Z","snapshot_observed_at":"2026-07-06T02:16:16.503242Z","submitted_at":"2010-10-05T12:30:24Z","title":"Positron annihilation spectrum from the Galactic Centre region observed by SPI/INTEGRAL, revisited: annihilation in a cooling ISM?","version":1},"cited_work":{"arxiv_id":"1010.0864","doi":null,"metadata_source":"pith","pith_arxiv_id":"1010.0864","snapshot_observed_at":"2026-08-07T12:04:39.724493Z","title":"Positron annihilation spectrum from the Galactic Centre region observed by SPI/INTEGRAL, revisited: annihilation in a cooling ISM?","venue":"astro-ph.HE","work_id":"48da0f59-280d-4f57-89c2-81c8ca484590","year":2010},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:37.983112Z"},"links":{"cited_paper":"/paper/1010.0864","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:04445f884b11afe392ac8da3d0198142fa9b375664ab8fc171fc0557439317c5","observation_id":"efbf59ba-9193-439f-90d1-3163c93e595f","resolution":{"observed_at":"2026-08-07T12:04:39.742691Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:38.014411Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.014411Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:cbe009affb19a5997ca5b4c5b79b45eaa87351140e71808ed843febbd550f3f5","observation_id":"01f30d29-ab8d-4490-a51a-8bc4fafa5753","resolution":{"observed_at":"2026-08-07T12:04:38.014411Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0409403","last_updated":"2004-09-16T14:47:00Z","snapshot_observed_at":"2026-07-07T00:44:43.184246Z","submitted_at":"2004-09-16T14:47:00Z","title":"Gamma-Ray Constraint on Galactic Positron Production by MeV Dark Matter","version":1},"cited_work":{"arxiv_id":"astro-ph/0409403","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0409403","snapshot_observed_at":"2026-08-07T12:04:39.606582Z","title":"Gamma-Ray Constraint on Galactic Positron Production by MeV Dark Matter","venue":"astro-ph","work_id":"3840480f-03ab-4e03-9b2a-7f1ff359a637","year":2004},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.051120Z"},"links":{"cited_paper":"/paper/astro-ph/0409403","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:2a3c8daac91287424dafb3a14aecc391e7bd709e4838828965fd6196c46956cd","observation_id":"b4c27f39-040e-404c-a61c-8093b2d3d419","resolution":{"observed_at":"2026-08-07T12:04:39.624034Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0606058","last_updated":"2006-06-06T08:06:01Z","snapshot_observed_at":"2026-07-07T04:11:13.230929Z","submitted_at":"2006-06-06T08:06:01Z","title":"Revisiting Bremsstrahlung emission associated with Light Dark Matter annihilations","version":1},"cited_work":{"arxiv_id":"hep-ph/0606058","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0606058","snapshot_observed_at":"2026-08-07T12:04:39.535504Z","title":"Revisiting Bremsstrahlung emission associated with Light Dark Matter annihilations","venue":"hep-ph","work_id":"866b6b6c-9e32-4c61-a4ad-579be9e7cb1d","year":2006},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.084923Z"},"links":{"cited_paper":"/paper/hep-ph/0606058","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:03ed596bef870dfc883a5960b3ef102cd70ab74de7915484c41179e082856258","observation_id":"f4e235ec-7537-46e1-b588-990cefd3e753","resolution":{"observed_at":"2026-08-07T12:04:39.561991Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1205.1194","last_updated":"2012-05-06T09:00:36Z","snapshot_observed_at":"2026-07-06T02:47:36.601601Z","submitted_at":"2012-05-06T09:00:36Z","title":"Galactic annihilation emission from nucleosynthesis positrons","version":1},"cited_work":{"arxiv_id":"1205.1194","doi":null,"metadata_source":"pith","pith_arxiv_id":"1205.1194","snapshot_observed_at":"2026-08-07T12:04:39.465607Z","title":"Galactic annihilation emission from nucleosynthesis positrons","venue":"astro-ph.HE","work_id":"8d195dbc-4457-4d10-9d96-7ea0887bff7d","year":2012},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.113197Z"},"links":{"cited_paper":"/paper/1205.1194","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:f006c5819e1ad909c26e986a36c3589a35d19837d29409f95346a01b9fcc9a49","observation_id":"5b4bef20-c6b0-4787-9081-94cd59db731d","resolution":{"observed_at":"2026-08-07T12:04:39.490886Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504186","last_updated":"2005-04-07T18:37:05Z","snapshot_observed_at":"2026-07-07T00:49:40.834673Z","submitted_at":"2005-04-07T18:37:05Z","title":"The lives and deaths of positrons in the interstellar medium","version":1},"cited_work":{"arxiv_id":"astro-ph/0504186","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0504186","snapshot_observed_at":"2026-08-07T12:04:39.398145Z","title":"The lives and deaths of positrons in the interstellar medium","venue":"astro-ph","work_id":"9fab8cd8-d3f1-4840-9e0c-73a0fde304b8","year":2005},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.143078Z"},"links":{"cited_paper":"/paper/astro-ph/0504186","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:ea0965d9c4377f244851c350e5478827001360683d8aa51c2e1a5ab19517e11d","observation_id":"3eea9372-721e-4f93-b715-1250aa636a99","resolution":{"observed_at":"2026-08-07T12:04:39.422546Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:42.376865Z","title":"Ore and J","venue":null,"work_id":"462e802c-bfe5-4846-b51f-bf6246954a2c","year":1949},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.180769Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:9a9784cb3835b50d3958c1260d92d09111a9756532b47f70c14dff4c15674b1d","observation_id":"239827ef-1515-4b8a-9261-bf7e2dfcbb30","resolution":{"observed_at":"2026-08-07T12:04:42.391297Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/0605420","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:39.336681Z","title":"Krivonos, M","venue":null,"work_id":"cae9f624-3e9d-4263-be25-74a936be7063","year":2007},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.216824Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:bb4cb7dccad9caac9b9a5502b171598fbac86c61bb2a046512aaaaaf4effd2d6","observation_id":"e656ea60-24f4-4090-87bb-17eaef761398","resolution":{"observed_at":"2026-08-07T12:04:39.363548Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2008.10665","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:39.185060Z","title":"Lutovinov, V","venue":null,"work_id":"5cf0ee4a-7b96-4f78-b78f-4f2e94323e83","year":2020},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.252513Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:1d3f7c9010cc393c65a28e441d8440ad5048ffbc5b9675a275bf54c786489532","observation_id":"611252cc-7215-48b1-8807-2390db18e33e","resolution":{"observed_at":"2026-08-07T12:04:39.220751Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2202.07483","last_updated":"2023-01-11T09:49:22Z","snapshot_observed_at":"2026-07-06T12:38:02.234243Z","submitted_at":"2022-02-15T14:49:22Z","title":"Strong constraints on primordial black hole dark matter from 16 years of INTEGRAL/SPI observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.07483","snapshot_observed_at":"2026-08-07T12:04:38.278938Z","title":"Berteaud, F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.278938Z"},"links":{"cited_paper":"/paper/2202.07483","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:0dacbbae878618e0f93a6a8921a977f1abf6bf28a6497568a340547856c4eba7","observation_id":"5d10c47f-3a2b-4639-b092-ad1087a07e6e","resolution":{"observed_at":"2026-08-07T12:04:38.278938Z","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":"2026-08-07T12:04:38.313895Z","title":"Calore, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.313895Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:d245ab92cd2fe4499bb62fd5b25f4b1d73cb8456e94b072a468d4f31f8453682","observation_id":"df40956f-884c-4963-b92b-cae3fdefd0f0","resolution":{"observed_at":"2026-08-07T12:04:38.313895Z","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":"10.5281/zenodo.6505275","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:38.677374Z","title":"Siegert, Galactic Diffuse Emission Spectrum between 0.5 and 8.0 MeV and between 30 keV and 8 MeV for the search of PBH Dark Matter, 10.5281/zenodo.6505275 (2021)","venue":null,"work_id":"cdbec27e-e43a-439c-9cd9-3aa157345dab","year":2021},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.326216Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:cbe2095a9f7d7d510aa7c0838cb646c87560f3dcfc38cc147ffe8bda2599b89f","observation_id":"b97b9505-cbdb-4380-b9f4-770c4c4e07a1","resolution":{"observed_at":"2026-08-07T12:04:38.706711Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.08419","last_updated":"2019-06-20T02:35:06Z","snapshot_observed_at":"2026-08-07T16:22:42.783654Z","submitted_at":"2019-06-20T02:35:06Z","title":"The Dark Matter Profiles in the Milky Way","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.08419","snapshot_observed_at":"2026-08-07T12:04:38.343155Z","title":"Lin and X","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.343155Z"},"links":{"cited_paper":"/paper/1906.08419","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:0c9f8410c22d814aa182b4da9aa18993f31c902bbcefa3b212fed7f0ff0adadc","observation_id":"f1a398c5-c88e-4a8c-b1c8-f4c4fb37465d","resolution":{"observed_at":"2026-08-07T12:04:38.343155Z","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":"2026-08-07T12:04:38.361075Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.361075Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:ee855b46fe39bc23f1265912d52f50335ec791777825c5d7b9d53ea6e44d5c93","observation_id":"e2f08a11-b93f-4612-a01d-b968b3ce49ff","resolution":{"observed_at":"2026-08-07T12:04:38.361075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.03319","last_updated":"2015-09-10T20:05:48Z","snapshot_observed_at":"2026-07-06T04:29:32.165102Z","submitted_at":"2015-09-10T20:05:48Z","title":"naima: a Python package for inference of relativistic particle energy distributions from observed nonthermal spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.03319","snapshot_observed_at":"2026-08-07T12:04:38.376147Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.376147Z"},"links":{"cited_paper":"/paper/1509.03319","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:c9f71c8e0faf70a646304240f19ceedef347f92d529cfc6d87afb76c1fecef7b","observation_id":"d433ddd0-2f27-4eea-9c91-1f26b0203117","resolution":{"observed_at":"2026-08-07T12:04:38.376147Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.7971","last_updated":"2014-01-24T15:04:38Z","snapshot_observed_at":"2026-07-06T03:26:52.362074Z","submitted_at":"2013-10-29T21:32:09Z","title":"Simple analytical approximations for treatment of inverse Compton scattering of relativistic electrons in the black-body radiation field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.7971","snapshot_observed_at":"2026-08-07T12:04:38.408478Z","title":"Khangulyan, F","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.408478Z"},"links":{"cited_paper":"/paper/1310.7971","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:183b0ace257e73210e31ac453b54f09c3e752d2625f76022d406ba3eb005362a","observation_id":"fbb80366-8cf8-48b2-a1c3-794200b70b8c","resolution":{"observed_at":"2026-08-07T12:04:38.408478Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.03488","last_updated":"2023-02-08T00:55:48Z","snapshot_observed_at":"2026-07-06T14:15:13.228518Z","submitted_at":"2022-11-07T12:19:21Z","title":"The cosmic ray ionisation and $\\gamma$-ray budgets of star-forming galaxies","version":2},"cited_work":{"arxiv_id":"2211.03488","doi":null,"metadata_source":"pith","pith_arxiv_id":"2211.03488","snapshot_observed_at":"2026-08-07T12:04:38.779976Z","title":"The cosmic ray ionisation and $\\gamma$-ray budgets of star-forming galaxies","venue":"astro-ph.GA","work_id":"d3e43be4-6639-4ff7-903b-4f6311515daf","year":2022},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.445311Z"},"links":{"cited_paper":"/paper/2211.03488","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:f7f13671a7824ecbc470803853531d0c1601cee5db8590e970eeadc711033b1b","observation_id":"b6418b46-524e-4c84-915b-627f64fbedaf","resolution":{"observed_at":"2026-08-07T12:04:38.809374Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:42.307264Z","title":null,"venue":null,"work_id":"2655cd82-1211-489c-83ea-6c60b66035ea","year":2000},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.481333Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:ff7dcb65ad10917a184612f6df8ebf1a32e9f35575621e66cbbfb0aa8273c28c","observation_id":"e6b5dff3-77aa-4332-b897-a6ecf9482a9e","resolution":{"observed_at":"2026-08-07T12:04:42.336495Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:42.257120Z","title":null,"venue":null,"work_id":"dfd55d79-4a03-4b54-babf-df1011174be0","year":1972},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.514788Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:27f852a7c7aa96d25a3f3377f5f4adb47ce61c8246fd2000d9c573ce8c403a67","observation_id":"f6e9bb0e-f45f-4e49-87f2-f11571205c79","resolution":{"observed_at":"2026-08-07T12:04:42.277517Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:04:42.185003Z","title":null,"venue":null,"work_id":"7c8425fc-e430-495a-b14b-92a62a131a57","year":1970},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.542368Z"},"links":{"citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:d513516de1977a95651367f40bb4689297d6fff630f9a502812a6873bb09b4e7","observation_id":"3cc21193-1f53-42df-b5ff-79c80683246d","resolution":{"observed_at":"2026-08-07T12:04:42.216026Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"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":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.3665","snapshot_observed_at":"2026-08-07T12:04:38.578493Z","title":"Foreman-Mackey, D","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.578493Z"},"links":{"cited_paper":"/paper/1202.3665","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:8324f92cbb54a9bf17591b640b67f6c16b05fadc5cb80ba6a2b6c5c2294322cb","observation_id":"e07b33c1-cf81-4883-9157-1a69d9877f87","resolution":{"observed_at":"2026-08-07T12:04:38.578493Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.3144","last_updated":"2010-01-20T20:50:35Z","snapshot_observed_at":"2026-07-06T02:02:41.083250Z","submitted_at":"2010-01-18T21:10:02Z","title":"Galactic Substructure and Dark Matter Annihilation in the Milky Way Halo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.3144","snapshot_observed_at":"2026-08-07T12:04:38.614827Z","title":"Kamionkowski, S","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-07T12:04:38.614827Z"},"links":{"cited_paper":"/paper/1001.3144","citing_paper":"/paper/2506.00847"},"observation_digest":"sha256:93ce02c8bcfcb407ac90583dd3ccba15911c167cefe022da24fe4480ea351f59","observation_id":"923357fd-da61-406c-af15-8ad55e666a9e","resolution":{"observed_at":"2026-08-07T12:04:38.614827Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2506.00847","last_updated":"2025-06-01T05:58:16Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-08T02:19:21.812864Z","submitted_at":"2025-06-01T05:58:16Z","title":"Relaxation of Energy Constraints for Positrons Generating the Galactic Annihilation Signal"},"reference_resolution":{"displayed":84,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":45,"verified_exact":34,"verified_fuzzy":4},"total_outbound_references":84},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 84 of 84 outbound references and 4 inbound Pith citation observations for arXiv:2506.00847."}