{"as_of":"2026-08-11T07:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f2eaf73684b9e31b440f1cd30a7ebf70de521e110963c36af8ef37065ee01748","coverage":[{"denominator":99,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":99,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T21:09:14.681309Z","state":"measured"},{"denominator":99,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":99,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2507.01085/citation-record","integrity":"/paper/2507.01085/integrity","json":"/paper/2507.01085/citation-record.json","paper":"/paper/2507.01085"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:04.151825Z","title":"S., Aguilar , G., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:04.151825Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:efeb003eb984d201065b8c991f2cf905bc3d444eeaf8d0a4140843cab6af812a","observation_id":"6ec58631-b292-4c75-9b06-5ece7018c815","resolution":{"observed_at":"2026-08-06T21:09:04.151825Z","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":"2026-08-06T21:09:04.222307Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:04.222307Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:48b326cc064d15aae9bbeeb946eb701d921b36536892aaf0b73e417c3385bb6e","observation_id":"6870edb8-7a5e-4ca7-a91e-244b47563a5f","resolution":{"observed_at":"2026-08-06T21:09:04.222307Z","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":"2026-08-06T21:09:04.354962Z","title":"& Stegun, I","venue":null,"work_id":null,"year":1948},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:04.354962Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:a6d160e8811d120873b0784c2eea13a4779fe2c60affd37dbc110400889a326b","observation_id":"d246d2b8-a42b-4970-909a-1a3226818e25","resolution":{"observed_at":"2026-08-06T21:09:04.354962Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.11230","last_updated":"2022-05-08T20:44:34Z","snapshot_observed_at":"2026-08-10T08:42:29.944740Z","submitted_at":"2019-09-24T23:42:19Z","title":"Carving out the low surface brightness universe with NoiseChisel","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.11230","snapshot_observed_at":"2026-08-06T21:09:04.453653Z","title":"2019, arXiv e-prints, arXiv:1909.11230","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:04.453653Z"},"links":{"cited_paper":"/paper/1909.11230","citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:6c81c716d3153083e9282084e5920d4e2c2914615f38546c0026b8e09c71db72","observation_id":"ed8d7785-be6b-4e1b-b8fe-fb7de9283ac7","resolution":{"observed_at":"2026-08-06T21:09:04.453653Z","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":"2026-08-06T21:09:04.583054Z","title":"& Ichikawa , T","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:04.583054Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:da7906a6c86ca8b3307dc5a635bda36c13b59d611bb391aea8eac585ace5b82d","observation_id":"9985eb5e-12c2-4e25-80a0-a7c4d8f7c8a3","resolution":{"observed_at":"2026-08-06T21:09:04.583054Z","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":"2026-08-06T21:09:04.655355Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:04.655355Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:1275806c669466adf47236b59dd965c2fd2df7180d4faaad994e55eb6a810763","observation_id":"3f1f77d7-9176-4a4d-ac4b-67a02aa9fc8c","resolution":{"observed_at":"2026-08-06T21:09:04.655355Z","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":"2026-08-06T21:09:04.693372Z","title":"P., Bendek, E., Monacelli, B., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:04.693372Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:dd00cfeef1dc9e3fad9d88c3cada160c66495f6f7f6c4e4a255de07d54529895","observation_id":"90cc627c-5da8-461b-926d-65ce4d7ab1b1","resolution":{"observed_at":"2026-08-06T21:09:04.693372Z","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":"2026-08-06T21:09:04.748744Z","title":"2008, , 683, L103","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:04.748744Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:2b17f10ea55b51e8eab140163793f89ce295923210cad930e644ef6f78f17aba","observation_id":"55dada98-2039-45d7-8942-8ce9b7587af1","resolution":{"observed_at":"2026-08-06T21:09:04.748744Z","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":"2026-08-06T21:09:04.808521Z","title":"2006, in Astronomical Society of the Pacific Conference Series, Vol","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:04.808521Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:58766135d88f2b97489bec61943cdf1f6aa89d5635461145e825315d53acb371","observation_id":"5d2659e0-bd01-4928-8e45-a9558c022d46","resolution":{"observed_at":"2026-08-06T21:09:04.808521Z","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":"2026-08-06T21:09:04.891549Z","title":"2010, SWarp: Resampling and Co-adding FITS Images Together , Astrophysics Source Code Library, record ascl:1010.068","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:04.891549Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:0d5ad7e6fd81ce7b114b96c5902d4f9c1f6c13fce9c3c0c4833490b74b8119f5","observation_id":"a31ef5d8-fc20-4713-a2f6-8addf398b83a","resolution":{"observed_at":"2026-08-06T21:09:04.891549Z","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":"2026-08-06T21:09:04.956832Z","title":"& Arnouts , S","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:04.956832Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:20986068eaad6384004878552153cdbd388f4a468a74ddd11f76c87f95148242","observation_id":"39212c1f-bcd1-435d-a5f1-3508438cd8fa","resolution":{"observed_at":"2026-08-06T21:09:04.956832Z","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":"2026-08-06T21:09:05.031106Z","title":"2019, astropy/photutils: v0.7.1","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.031106Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:1b5fde7bbe5d29bf0e10c1fa8d055ff3f6adb7040d07d16bc669e7feac2a29f1","observation_id":"4fa174a8-f07c-4cb6-9658-3cd4139803ab","resolution":{"observed_at":"2026-08-06T21:09:05.031106Z","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":"2026-08-06T21:09:05.078564Z","title":"& Van Woerden, H","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.078564Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:ec62435b65c45a47027ab6a88621e0ade8332e0f3d86540eaf1a27c7cfe92e6d","observation_id":"cd9dbbe8-9b74-4999-9d85-36c8829764f9","resolution":{"observed_at":"2026-08-06T21:09:05.078564Z","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":"2026-08-06T21:09:05.135477Z","title":"& Trujillo , I","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.135477Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:39f067ca416c6969846743d117d8d5867908ea32df03f819278ccdf0d4e34ed3","observation_id":"de91022c-e821-4c04-8bf7-15f290d8c734","resolution":{"observed_at":"2026-08-06T21:09:05.135477Z","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":"2026-08-06T21:09:05.205518Z","title":"S., et al","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.205518Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:5571d801c69cae1adbd7c09b4e41523f4a455a07702eed6a5d51e3f23fdeda19","observation_id":"b7a2da2f-00f5-4829-a360-120761d612aa","resolution":{"observed_at":"2026-08-06T21:09:05.205518Z","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":"2026-08-06T21:09:05.235174Z","title":"E., McEwen, J","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.235174Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:5f3e8c359a5f4fb28175884e9e66605799f61f0873d127de31c94f2ea2984f1f","observation_id":"cb7ef70a-b44d-4baa-861b-ba937d096468","resolution":{"observed_at":"2026-08-06T21:09:05.235174Z","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":"2026-08-06T21:09:05.295432Z","title":"R., Trujillo, I., Golini, G., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.295432Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:69b4054abd109659deffedf852322f0f19ab16950eb4ae3ac699f26953530967","observation_id":"9d6afac3-8972-4752-a82b-0da6c3d66e34","resolution":{"observed_at":"2026-08-06T21:09:05.295432Z","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":"2026-08-06T21:09:05.361315Z","title":"2003, , 115, 763","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.361315Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:57586b72527197f53038a2068ca671f32d5a98e8cbbb8e144e57aa963be5ee8c","observation_id":"00a60462-c338-4182-9147-7af6f52620a3","resolution":{"observed_at":"2026-08-06T21:09:05.361315Z","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":"2026-08-06T21:09:05.424255Z","title":"J., & LSST Dark Energy Science Collaboration","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.424255Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:be29340f948dc7ffba66420e07a7423431c652b5d8679fa6b6fcedc9e4d6cf97","observation_id":"2005324a-f1c7-49a5-9afa-e15c0832c896","resolution":{"observed_at":"2026-08-06T21:09:05.424255Z","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":"2026-08-06T21:09:05.477027Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.477027Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:39c688b1dd7dc050ddd3bf0ca4a11f56296e7d8d9abb971208d6bff059bf9d5f","observation_id":"aaf1b4fe-ae4b-4e87-a574-246782aed750","resolution":{"observed_at":"2026-08-06T21:09:05.477027Z","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":"2026-08-06T21:09:22.399198Z","title":"G., Salo , H., et al","venue":null,"work_id":"f5c7b641-399c-4d12-ac73-7ee2720e8355","year":2012},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.555611Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:483652b3221e5af74fd95acc0316ec637dc55e52c6d9bbfae3de7bdbadc20b62","observation_id":"1007f7b4-ab0d-4112-8f7e-f08f8076f4e9","resolution":{"observed_at":"2026-08-06T21:09:22.404237Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.384975Z","title":"H., Arnaud , M., Pointecouteau , E., & Pratt , G","venue":null,"work_id":"e76ec34f-f918-4182-93a5-a6fd0a9b68d9","year":2006},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.616913Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:b3c214342e837a1ab59a7a09c8d838883cb097759f787673c4c6645424e4b8b1","observation_id":"0956b01b-566b-4b6d-891c-12dc68ac80c1","resolution":{"observed_at":"2026-08-06T21:09:22.389733Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:05.697466Z","title":"P., Ro s kar , R., & Loebman , S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.697466Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:b2ff6336a2fe4e3d755a5227bc860acc6193d1e0b8b096673628338d33a00bb4","observation_id":"7f3bc84a-dd53-4434-befd-e0ec8d67ab06","resolution":{"observed_at":"2026-08-06T21:09:05.697466Z","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":"2026-08-06T21:09:22.361949Z","title":"2022, , 667, A109","venue":null,"work_id":"79c385e1-9265-40e1-8692-81361038b871","year":2022},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.768118Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:5c7f64391b3089ad007bd5b216f508ff84eb2f41d262f3359ba98c6647e9a8de","observation_id":"8d1f5b8c-ba6a-43eb-81a1-8802edf8bd8d","resolution":{"observed_at":"2026-08-06T21:09:22.366471Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.346837Z","title":"2015, , 446, 120","venue":null,"work_id":"94a13037-86cf-4f8c-a18a-ddc0490bdfd4","year":2015},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.822436Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:b4e576b0eb842f2cbc43bc407115e92101806202729bdb26b5637c9b98e102a0","observation_id":"cd310354-0367-4155-aa15-31b7f001afb3","resolution":{"observed_at":"2026-08-06T21:09:22.352093Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.332595Z","title":"& Silk , J","venue":null,"work_id":"4565260e-a9e1-4790-a2e7-3c7d9454da9e","year":1983},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.888952Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:522dc43c884a35949358f52ea12cf7249e1536be0f61bc86bfb84b36e9782282","observation_id":"af9b1c4e-ed21-4755-8aa9-5c59fa36ecfb","resolution":{"observed_at":"2026-08-06T21:09:22.337417Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:05.995177Z","title":"2015, , 799, 226","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:05.995177Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:4b2808d330b724246a4423359226cb9da8ac71236564340ec597c6b4c4ec301e","observation_id":"19551152-332e-4581-bcc2-60b782b79e31","resolution":{"observed_at":"2026-08-06T21:09:05.995177Z","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":"2026-08-06T21:09:22.308448Z","title":null,"venue":null,"work_id":"c1ec83d1-df37-4fa0-8387-1b56e7a45e24","year":2008},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:06.096088Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:d2adcee78247414fb8e082dfbf7ca9bd13a4c71250c8a9a78f2aaaf9a8f2906e","observation_id":"aa877a39-e48d-4a71-b433-ab4749caef05","resolution":{"observed_at":"2026-08-06T21:09:22.313470Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.292567Z","title":"2024, , 683, A145","venue":null,"work_id":"6ee7d9d2-00c4-4022-a9d0-8fabaacc7d2e","year":2024},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:06.216454Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:769341ddd3d02c0e3fe044c980d25552d09e8e180d34ea8a2e5d767a25a39532","observation_id":"2ee3536e-e884-427a-933b-4a2d39cfcb1f","resolution":{"observed_at":"2026-08-06T21:09:22.298298Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.277753Z","title":"R., Rom \\'a n , J., & Trujillo , I","venue":null,"work_id":"fa5b9373-e147-4294-a614-8b12b7a835eb","year":2024},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:06.380929Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:7feb0721bcbc1fd489123b6bab22b3a5ff36228e76c0ae08288ec3cc5a4a32ba","observation_id":"e71eb820-67d3-43f0-91e9-42540040b0c7","resolution":{"observed_at":"2026-08-06T21:09:22.282014Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.261997Z","title":null,"venue":null,"work_id":"58a3f52e-e122-4e3b-9295-ee477102cd15","year":2011},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:06.489115Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:59dd757c141a32e5c01c655f378c5345d0c4a391d8f3d987d2a384e49adad09e","observation_id":"19f1b06c-4e9d-4c3b-92d4-c33442135012","resolution":{"observed_at":"2026-08-06T21:09:22.267269Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.247375Z","title":"2024, EAS2024, 1990","venue":null,"work_id":"08ad5369-e7d0-4547-9a90-2f5d949a92ca","year":2024},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:06.651798Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:6cfd227f7c8cd9d6557bdbfa59abefd5a687b3fcdb36197f366e2c9f053479ff","observation_id":"a5bcb85f-893c-4064-8f30-ae1df697a038","resolution":{"observed_at":"2026-08-06T21:09:22.252725Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.233460Z","title":null,"venue":null,"work_id":"c34b2235-caaf-47c5-8cc9-d76d84843926","year":2007},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:06.754319Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:3b9271d8bb5cf76f64d01152eea6913472a4d99bda382d80e4a27c2abac3bb84","observation_id":"3411cce2-ad7b-4a3f-8940-ba0ca3d7ca5b","resolution":{"observed_at":"2026-08-06T21:09:22.238000Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.218659Z","title":"& Akhlaghi , M","venue":null,"work_id":"b6dd7829-e920-4114-add1-873e625dc997","year":2024},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:06.864400Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:455da02f271f477ddeb66798d8d18f008bdb21128cdae081d43d9b9563c39c8d","observation_id":"e7e5abc4-b09d-418e-877d-c27ff5e0e4c6","resolution":{"observed_at":"2026-08-06T21:09:22.222959Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:06.965848Z","title":"2024, RNAAS, 8, 22","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:06.965848Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:78e8e0d2fbeeb45c57d2569d5cea002b57b10f1332afd80970632eef801c85f5","observation_id":"7e827827-f481-43f2-8b44-01df8e585098","resolution":{"observed_at":"2026-08-06T21:09:06.965848Z","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":"2026-08-06T21:09:22.194831Z","title":"2020, , 491, 5317","venue":null,"work_id":"5336f52c-9032-4ded-b631-133e4b9e543d","year":2020},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:07.083287Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:80cb9699a69300150094962edac4dee30926ff680953f2587a46b176aedd9634","observation_id":"48e08683-a29a-4ecc-9af3-406f190c2b6c","resolution":{"observed_at":"2026-08-06T21:09:22.199487Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:07.253625Z","title":"M., Tyson , J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:07.253625Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:f0cb24894da26564327d13edd225edd5ba5660dc4d7d6069404c7ea54440bfe8","observation_id":"9355e61f-ed36-4a29-9247-1affabbe178b","resolution":{"observed_at":"2026-08-06T21:09:07.253625Z","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":"2026-08-06T21:09:22.170613Z","title":null,"venue":null,"work_id":"3bb2313e-b4ca-41ca-aa65-639701b95643","year":2010},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:07.393683Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:ca3e92f845004f2ac7b67eb0e30d8f089efa0ead360047c281695e70b131f6ff","observation_id":"6ae09344-bac7-4462-9d97-b02831372e29","resolution":{"observed_at":"2026-08-06T21:09:22.175646Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.155852Z","title":null,"venue":null,"work_id":"592f9dbb-e371-4e98-89af-4b7c414b3715","year":1987},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:07.503465Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:94b0b49b4773ed19c1da1bef811ad66849da893b08dddf466aef780b133b5ea0","observation_id":"d176342e-e14f-4294-aaf7-9ba957b7ea7d","resolution":{"observed_at":"2026-08-06T21:09:22.160906Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.141762Z","title":"2022, Neurocomputing, 503, 259","venue":null,"work_id":"1b5b6bb8-37af-454e-8bdf-26c5640fe08b","year":2022},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:07.590786Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:690c54fe7095c1618a0492bee35d4354aa50a517d7c678680a075f73ddf9378f","observation_id":"6afb1808-78a3-4396-b8fb-3460527b9b70","resolution":{"observed_at":"2026-08-06T21:09:22.146812Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.127859Z","title":"A., Kuntschner , H., et al","venue":null,"work_id":"f6c2cea5-311e-4948-a909-d84169597ce8","year":2017},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:07.682840Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:cbbdd1fb20253386e25086e48ff18720020eedc34895ba225f228e555a72ae80","observation_id":"4f584eb8-e643-4e4c-b191-327a71e97cf0","resolution":{"observed_at":"2026-08-06T21:09:22.132703Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.114140Z","title":"1989, , 344, 685","venue":null,"work_id":"22fa1afb-66b7-4c32-accb-017f317fa5fe","year":1989},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:07.810732Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:2e19aff29ab0f24f997d327094934400a49ec44bed7ce7d27e45db533143ea94","observation_id":"379d8d30-bbd3-48ce-8746-11545462d01c","resolution":{"observed_at":"2026-08-06T21:09:22.118578Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.099848Z","title":"B., Eftekharzadeh, S., et al","venue":null,"work_id":"19675322-31fc-421f-926a-202aea5338a3","year":2020},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:07.961138Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:3deb62fb186cc9b30de4c9b37a557f0aff0c7df95a2e5cca64ee3afe55f86ef8","observation_id":"49207a69-fbcb-4ccd-ad2b-cd31d0b58a0d","resolution":{"observed_at":"2026-08-06T21:09:22.104468Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.085739Z","title":"W., Mierle, K., Blanton, M., & Roweis, S","venue":null,"work_id":"e1a7a1ed-58d4-4907-b633-aa2f7bf9444c","year":2010},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:08.123619Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:d37feb999052fd9131115bd78d1ae05b4a0e81a22c6059fe6923edd2a3b57070","observation_id":"f477a32b-ab8e-468a-872f-8e61508b90b6","resolution":{"observed_at":"2026-08-06T21:09:22.090273Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.069787Z","title":"K., Walter, F., Brinks, E., et al","venue":null,"work_id":"f4c3059e-0ca3-4e2d-831b-96d2497a58fe","year":2008},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:08.237279Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:94f00c4687bf60e1ac70d514fe37658b7d60a259032d46848b9578d13026e682","observation_id":"0a1fdfc0-880d-46af-8dc4-48f894e82f29","resolution":{"observed_at":"2026-08-06T21:09:22.075239Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.054829Z","title":null,"venue":null,"work_id":"a30248b9-862e-4084-bafb-15435476e3dd","year":1974},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:08.368725Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:e29f73d3666f8c03fe98051f533f63cc46e7dc60742c57d0733104aa25d733af","observation_id":"98d00df8-8500-4779-b79b-77b7aaef09b5","resolution":{"observed_at":"2026-08-06T21:09:22.059544Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:22.031465Z","title":null,"venue":null,"work_id":"4aa1370d-9254-4851-8564-470ead1ab2d8","year":2001},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:08.527780Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:42ca4851e8d207d97cbb9a7d4f19834933e10537d113b527fbac5c0361aa4b3f","observation_id":"c2a03d29-f538-4b3d-a7a1-a10720186434","resolution":{"observed_at":"2026-08-06T21:09:22.042048Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:21.739924Z","title":"A., Kaviraj , S., et al","venue":null,"work_id":"1ea6020c-2ca8-468c-ba8c-d4854c5a6e19","year":2021},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:08.656051Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:c4b57dc7320f18864ea1ca736dd9f0ffb7b8ed627036eac204d8074afb9f266a","observation_id":"dd87d4f7-391e-4c8f-8c80-4fd975d276f6","resolution":{"observed_at":"2026-08-06T21:09:21.887566Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:21.389428Z","title":"2012, , 427, 1102","venue":null,"work_id":"4b5821e6-4def-423e-8d9b-090be68fcf41","year":2012},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:08.761641Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:02ea3eb66272d4116a02e52515a642438a837ae949027c480ac56f04dc99a463","observation_id":"4ffabf2b-e2b6-432a-a632-d2b910bf272e","resolution":{"observed_at":"2026-08-06T21:09:21.527464Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:21.097321Z","title":"2023, , 678, A62","venue":null,"work_id":"83da9f91-c415-41be-aae0-61d07edc529f","year":2023},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:08.942919Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:221d8c538a50c7b3c29e82bf995e49026d823c8508181889ed8ac18fe1ad2ff2","observation_id":"a80c27fa-ab41-4f4c-9e57-dd0d8f269fe9","resolution":{"observed_at":"2026-08-06T21:09:21.232061Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:20.774103Z","title":"& Knapen , J","venue":null,"work_id":"20fbdfb7-cfaa-4793-9c46-c7e8598ee027","year":2019},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:09.063151Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:db02ac2cc5397ea24af41e8c6a31c9db73d55f69b1441b227efa7a5a22ff1057","observation_id":"33f40d66-0c1d-4359-b85b-0d3ff00707d8","resolution":{"observed_at":"2026-08-06T21:09:20.856562Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:20.717859Z","title":null,"venue":null,"work_id":"9ad86211-b079-4c2d-9c9e-e1ba6fe648c4","year":2018},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:09.163929Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:cbf6573d7da279e289d2b51ff761a344e49e0b2675a04fbcf6b0a93f9881dec1","observation_id":"390ad36e-1bd8-4108-8a6c-16c73dab6017","resolution":{"observed_at":"2026-08-06T21:09:20.764208Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:20.575543Z","title":"C., Durrell , P","venue":null,"work_id":"25de7f15-e812-4a64-b86e-8fe330f325af","year":2015},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:09.254786Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:f6dde01009aee66fdee3665276e26bab19583837bc338c8738c2904c9faee2ab","observation_id":"137cd9a3-a354-4f3f-834d-5680d4e3a59e","resolution":{"observed_at":"2026-08-06T21:09:20.648399Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:20.445797Z","title":null,"venue":null,"work_id":"1fe9dfb8-ac58-447a-b21a-758b570ea00f","year":2011},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:09.369447Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:30fa74759709158990cb841975d1104af00e0e2461e6589c2ebbb1eaf9674a7a","observation_id":"ea657f56-0d77-44b3-a87a-acf42ae2552e","resolution":{"observed_at":"2026-08-06T21:09:20.508657Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:20.351049Z","title":"S., & Santucci, G","venue":null,"work_id":"9849c07c-bc76-42cc-95bf-2811df4b7912","year":2021},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:09.462294Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:9f53a9c04dfff87d4aa63eeb05aeb0f4828ea870351d286d51521300fc3bf126","observation_id":"5375ff0f-2c3a-411b-985d-693ec8b3cd4d","resolution":{"observed_at":"2026-08-06T21:09:20.400091Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:20.235436Z","title":"2024, , 681, A15","venue":null,"work_id":"6a43b8f4-06be-4cfd-8a3f-d7ecaf5fcd64","year":2024},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:09.554259Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:0f5d49db5bbe50538d6a624c89ad6c83a22ed54720304619d9de0c1529201bc5","observation_id":"2c4e4944-496d-446b-85ff-4d20533018ad","resolution":{"observed_at":"2026-08-06T21:09:20.290073Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:20.114518Z","title":"1999, in Proceedings 10th International Conference on Image Analysis and Processing, IEEE, 394--399","venue":null,"work_id":"f02d72c9-8fb4-4625-9e6e-c6810c91f58f","year":1999},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:09.656800Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:88ccab5415ec6ff68118f4671ae1fe8de013a92ac79552e98caf3b1e879c442d","observation_id":"8e458128-48ea-4b27-8d27-fc9287128760","resolution":{"observed_at":"2026-08-06T21:09:20.161579Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:09.764965Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:09.764965Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:e35034e9af8c8a16495378c8143d35d85f521e986794073bffc8380a1a4e3a1d","observation_id":"88fa52d0-0a3b-49fe-9e71-06ba1ce9e09a","resolution":{"observed_at":"2026-08-06T21:09:09.764965Z","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":"2026-08-06T21:09:19.981855Z","title":null,"venue":null,"work_id":"2caf65bc-8bf2-415a-8887-18b2613b2769","year":2007},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:09.894667Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:b398c7a26eb3bfe28d05309351e488650b3eeb58337f389f8d5939749255cf3e","observation_id":"8e45e21c-11e0-4840-bcbd-e1ebd62b5b78","resolution":{"observed_at":"2026-08-06T21:09:20.031639Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:19.868609Z","title":null,"venue":null,"work_id":"e808ec6f-294f-4dcf-9e0a-f2d03a8bf854","year":2010},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:10.001069Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:6dc8318d79290edf6f424d4b9eb44ef4e6d22b5bd0135c5ad16983dd31403fa1","observation_id":"d57853b6-f9c7-48d6-b374-7ee9268846ce","resolution":{"observed_at":"2026-08-06T21:09:19.926620Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:19.732720Z","title":null,"venue":null,"work_id":"5a94314a-4d2d-4505-acc1-a0cc82b2a1ee","year":2017},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:10.096062Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:049758837a71bd2c7e8b2383c01ccd672511d49ce647900a594badc41e8a9105","observation_id":"3e390a53-ab17-49af-af33-6175ea04d04f","resolution":{"observed_at":"2026-08-06T21:09:19.786183Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:19.638929Z","title":null,"venue":null,"work_id":"5e711ff2-138b-4632-a5a5-ca1d06afe761","year":2017},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:10.185696Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:5ade52117d1dc0ffbae43f35f104a55312f1a62fcd5180d682a4ba29a5f8f2dd","observation_id":"4e43288d-01d7-47ae-bdbd-9d95e0092775","resolution":{"observed_at":"2026-08-06T21:09:19.677368Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:10.258006Z","title":"& Trujillo , I","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:10.258006Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:c0cd429112ba3702f6406281f43ce2482870af1c3dcd9f498fd3c56c7a72ae2c","observation_id":"82cad976-5b56-4a08-9a01-06b22b47456c","resolution":{"observed_at":"2026-08-06T21:09:10.258006Z","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":"2026-08-06T21:09:10.391324Z","title":"M., Sip o cz , B","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:10.391324Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:15ab8db5eadd337d10934ed4499308c26e27d498c1914041c125f026a3da5bab","observation_id":"93b550b7-08b2-4e51-be03-301439087d5e","resolution":{"observed_at":"2026-08-06T21:09:10.391324Z","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":"2026-08-06T21:09:19.479898Z","title":null,"venue":null,"work_id":"1e72361b-5296-4565-8854-89aef76437eb","year":1972},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:10.498523Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:743b8a6df75b0bc24c468092b61d7d01710503f20ade41f1a35a0e1806122f2c","observation_id":"be827136-31ae-42fc-8222-6595f0b28624","resolution":{"observed_at":"2026-08-06T21:09:19.558701Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:19.334047Z","title":"L., Domingo, J., & Barfeh, D","venue":null,"work_id":"2e9ddfb3-118a-46e1-8079-94a24ad64a67","year":2020},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:10.621865Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:e657e42c1ef76e1bd8c523ca75c7b7c309f82b83aac8e56f565b18c6c768dcb2","observation_id":"1bdb3ae7-0436-4646-8122-0440e6ca4082","resolution":{"observed_at":"2026-08-06T21:09:19.403947Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:19.167395Z","title":"M., Mosenkov , A., Lee-Saunders , H., et al","venue":null,"work_id":"e2c1361a-2ee8-44f1-810c-22c89118f325","year":2019},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:10.733027Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:29dcc14d84d92022a57044b1f78e8f89087f4056eee40a5eb30a036590064ef6","observation_id":"9d5af72b-8722-4f82-9a59-769214c943d7","resolution":{"observed_at":"2026-08-06T21:09:19.246906Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:19.011537Z","title":"E., van Zee , L., Barnes , K","venue":null,"work_id":"785f45d4-b7ac-47b7-ad66-6365f642553f","year":2016},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:10.868192Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:cdec374eb98c21ad98549297fc928ae65bfc535d8974cf222c2f1f5d959e36f1","observation_id":"cea0fad9-fe71-4952-98d4-a6a3f81edd4b","resolution":{"observed_at":"2026-08-06T21:09:19.090237Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:18.857991Z","title":null,"venue":null,"work_id":"b969847a-5fde-4f8f-a1ed-0253db097b83","year":1972},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:10.967010Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:f25253cf6921aef944f95f04e4ebd302d480e626ad33cc24e0a9fab689667c0c","observation_id":"f93f709a-6593-43f9-bbfe-e0197bf85ca2","resolution":{"observed_at":"2026-08-06T21:09:18.911666Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:11.114296Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:11.114296Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:b9cbca5c541c8535c59ada5528ddb21f39fa7acd007b45c1d981253025e45952","observation_id":"f2a83ca2-4f5e-4ad5-be27-efa8a2f0ddd2","resolution":{"observed_at":"2026-08-06T21:09:11.114296Z","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":"2026-08-06T21:09:18.669810Z","title":"M., Ahvazi , N., et al","venue":null,"work_id":"cbac52a5-a5e5-4623-b7a4-eeed25c3ef36","year":2023},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:11.204387Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:7337da8676be8a762b722551901a14dc9b1a4fe7bf7782120576cc7aa58110ea","observation_id":"f5cb65ee-031b-44bc-969c-43a5d3e01715","resolution":{"observed_at":"2026-08-06T21:09:18.759478Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:18.523276Z","title":"& Trujillo , I","venue":null,"work_id":"257be545-c88b-44a7-b317-91b8abbe7d68","year":2018},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:11.342795Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:96ff4535eb5d7807719fb6d2f1f90fd38e0b8c5e3a132652125d147c0ed0ff67","observation_id":"8c3e6bc5-1f81-4093-b5fd-756fe0607ac9","resolution":{"observed_at":"2026-08-06T21:09:18.579003Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:18.379459Z","title":"2020, , 644, A42","venue":null,"work_id":"2ce90a28-14cb-45bb-94f3-de58585a962a","year":2020},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:11.473472Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:b84c2af41b17693e095e99269721b27023894e4f96ea09be48992f309db9b004","observation_id":"b8855f1f-3b24-4786-a74d-0f10597c4332","resolution":{"observed_at":"2026-08-06T21:09:18.444467Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:18.213777Z","title":"P., Stinson , G","venue":null,"work_id":"059f2013-2dff-4dc1-98e6-399d5557b968","year":2008},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:11.575110Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:1a6e5e3394bc012b0b0b4b30c4a6cf9886f63d813f58e6a29543aeb25d731696","observation_id":"bbee70d7-6427-4fc8-bb05-e5f2330c991a","resolution":{"observed_at":"2026-08-06T21:09:18.282996Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:11.725688Z","title":"2014, , 567, A97","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:11.725688Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:d10f1d68059c343b7f910886e672460b144899582743b1563f57e58e4cfa2889","observation_id":"cce736d9-e134-4d15-a9e5-64eab47dfb07","resolution":{"observed_at":"2026-08-06T21:09:11.725688Z","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":"2026-08-06T21:09:11.853165Z","title":"2015, , 577, A106","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:11.853165Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:8189733cc666d60d44de2ea5d093b299f7371c51069847ce0826724295fc7107","observation_id":"e77eb0cd-0cca-45ea-a46f-09a2937dc856","resolution":{"observed_at":"2026-08-06T21:09:11.853165Z","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":"2026-08-06T21:09:17.958910Z","title":"2011, Numerical Analysis, 2nd edn","venue":null,"work_id":"c1f1872b-55df-4ca0-aea9-f2f93469e5ca","year":2011},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:11.962574Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:2804a418551772c229fecbc0380ea249df0f3767cbea1b3d57a6244ef918311a","observation_id":"ad563c85-e8c7-494e-b4a7-05ea3bb44515","resolution":{"observed_at":"2026-08-06T21:09:18.089783Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:17.769605Z","title":"2022, , 662, A112","venue":null,"work_id":"8dbd4e91-c9cf-48bd-9e9f-82371205057e","year":2022},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:12.094328Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:6813a0f5109e3e440366c162cc9a1a04261ff8b36b2929b77c0ee9c4fc681ea7","observation_id":"1416f0d0-204c-46d8-ba38-ac0d57d022f8","resolution":{"observed_at":"2026-08-06T21:09:17.865030Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:17.589621Z","title":"2004, , 609, 667","venue":null,"work_id":"4f402160-6a98-4a8c-bca1-deba41be312e","year":2004},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:12.202016Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:3cd21dfa12baeeba6074e61f9937068d3fef5821252349455ac7d9e2ad240ce3","observation_id":"9df61ce4-201f-41d3-a2fc-d6b95f4164e2","resolution":{"observed_at":"2026-08-06T21:09:17.694292Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:12.349461Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:12.349461Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:96ccd0af7cb8a136a894778ba4c296be22efd89dfb3f4c7bc6bd8ec352b3c61a","observation_id":"5d2b1762-f159-4f18-87da-420a5cc3ac57","resolution":{"observed_at":"2026-08-06T21:09:12.349461Z","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":"2026-08-06T21:09:17.370791Z","title":"2025, OJA, 8, 73","venue":null,"work_id":"be84ad89-fac2-49eb-bdd2-082a633cc2bb","year":2025},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:12.478452Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:a1ef22c3b5b884d90f4d044fc4723523e37117055679e47c9765854fc6897721","observation_id":"ce801b8a-5b65-43ec-8494-4a7c848431b6","resolution":{"observed_at":"2026-08-06T21:09:17.465026Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:17.201006Z","title":null,"venue":null,"work_id":"9020992c-74d0-4408-aa77-78e8c79272de","year":2014},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:12.649036Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:4dfcf968eb1c05837ac23586d2fee74acd47d2fb69f1997dcad8f6e495fb8dc3","observation_id":"02945d69-c9a4-44e8-a3a4-69e71311205c","resolution":{"observed_at":"2026-08-06T21:09:17.292897Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:17.016229Z","title":"V., van Zee , L., Salim , S., et al","venue":null,"work_id":"0c47e6dd-16f8-4d94-9b8c-e281bb77b7b1","year":2021},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:12.798750Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:b7b6f84adac4e96a06f49f868466ba57c74f763f4a895e2039ccc89880500d85","observation_id":"c3e55fd7-ebdb-44aa-b4e8-0bb830abb4b7","resolution":{"observed_at":"2026-08-06T21:09:17.114871Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:16.793171Z","title":"& Murtagh, F","venue":null,"work_id":"4cccedc5-9ab0-470e-b9ce-0ba3c7b33ca8","year":1994},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:12.916176Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:0981e6fdfe312ef48d44709914c34a16ccd80c71955cd9502c6ac9aec88a64c5","observation_id":"bb2ab289-3ae2-4cd2-9e3d-6d0e11f56b00","resolution":{"observed_at":"2026-08-06T21:09:16.913031Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:16.484798Z","title":"& Murtagh, F","venue":null,"work_id":"d43667a5-9b13-4ece-b392-7f45667e8a70","year":2007},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:13.039237Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:42e5046ff671e9ce94620c2dc297b4dd080ec257035051e60f09bdc69c33fe12","observation_id":"21f2d95a-8106-4eb9-bded-2ba2faf64fd1","resolution":{"observed_at":"2026-08-06T21:09:16.603806Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:16.248390Z","title":null,"venue":null,"work_id":"2bb73335-adfa-40cd-9972-c65644bb8b96","year":2010},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:13.184313Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:3ed51ce3d8528f74ececc3013338cfb9112f07235896803d7eb2087c5f8619ee","observation_id":"afa67470-1218-4ca3-9115-879c75464dbb","resolution":{"observed_at":"2026-08-06T21:09:16.348935Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:16.048840Z","title":"L., Pires , S., & R \\'e fr \\'e gier , A","venue":null,"work_id":"0273257f-a897-4bba-83c4-d4c7000235b9","year":2006},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:13.283520Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:7d7737e62d642fbcd21c272f5dab1b069f44e9b77898fe39a6fc078fd7199586","observation_id":"85abbe41-8633-414e-915c-98cd4b9f25e0","resolution":{"observed_at":"2026-08-06T21:09:16.117225Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:15.828583Z","title":"& Toomre , J","venue":null,"work_id":"55a79973-e399-4043-9723-031cf089a9d9","year":1972},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:13.407455Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:5ccab86d83af9852ab167900c6e6cd362ea552869ab585056940b4ae311cd487","observation_id":"6435fde4-eced-4fd0-9da0-4e00c9c406b5","resolution":{"observed_at":"2026-08-06T21:09:15.944493Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:15.629166Z","title":null,"venue":null,"work_id":"c475fa30-5f00-4ce4-81cd-9e0be05a2e53","year":2001},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:13.563159Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:1347ce42cbe1d4c1da885b0401bdb27c6ed6a98a8a274de744243f2ab7482194","observation_id":"797c6644-54a4-4ee8-a155-9d6d3bed99c5","resolution":{"observed_at":"2026-08-06T21:09:15.685555Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:13.680813Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:13.680813Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:5579188b2814f83bb20014d4656af6434da3209fcf56c85db5df6ba623e9d732","observation_id":"89f01bb4-e948-49fa-9e21-75ee4f2216d3","resolution":{"observed_at":"2026-08-06T21:09:13.680813Z","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":"2026-08-06T21:09:13.836682Z","title":"2021, , 654, A40","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:13.836682Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:297c9ab57869499fc5508676806d47fc3874794f6b0ab81e170b81a7c156fd66","observation_id":"74ffa3a1-bc6e-4749-ac43-6b698fd88535","resolution":{"observed_at":"2026-08-06T21:09:13.836682Z","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":"2026-08-06T21:09:13.966017Z","title":"& Fliri , J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:13.966017Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:fa571992531504e2a0ec2c421ad1ba13d4abbc124cf6f2d5d22be277098b4ee3","observation_id":"0375ecf7-9735-4e71-acb6-9f2dc8be414c","resolution":{"observed_at":"2026-08-06T21:09:13.966017Z","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":"2026-08-06T21:09:15.387994Z","title":"C., & Varoquaux , G","venue":null,"work_id":"b554362b-743f-4600-b2de-dab8a635e84a","year":2011},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:14.072031Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:ac16587a9f34a1ff24b7482535d0ca1662604c9b4b7c42eac37aa4570c9279c2","observation_id":"d2332aab-f1cd-4a50-8f12-2ea1a239de63","resolution":{"observed_at":"2026-08-06T21:09:15.484459Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:15.209557Z","title":"2025, , 693, A232","venue":null,"work_id":"7ea6b600-9425-43e9-a05c-737cb0697f99","year":2025},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:14.177886Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:5c8c5cf059cabad6224423286cbd1788ee5a8267a712df089cc44978a0707635","observation_id":"12c2e636-1099-48cf-a539-b4bad3e31552","resolution":{"observed_at":"2026-08-06T21:09:15.303569Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:14.268423Z","title":null,"venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:14.268423Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:c59238c28064b6c99083957855e7ee56780059720be3e787940a6d7b7a12fe9b","observation_id":"20445664-ef9e-47a0-b5a0-94908c1161de","resolution":{"observed_at":"2026-08-06T21:09:14.268423Z","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":"2026-08-06T21:09:14.969288Z","title":"& Ahn, C","venue":null,"work_id":"72e1485a-6ff1-4c6e-91fb-4eaefe20b04b","year":2014},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:14.350944Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:31cb679974941697eb0ec6fb8470a5721e3cc3e163dfabe71805133a03460bd8","observation_id":"9970da0b-9937-4bee-ad94-93e277d06bdc","resolution":{"observed_at":"2026-08-06T21:09:15.072626Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:14.830858Z","title":"2024, , 168, 69","venue":null,"work_id":"059a71c1-11f4-4c0c-9bf8-12f4d4970043","year":2024},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:14.461890Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:4e8c8d29b05c3d83c374d76d703446a2628c9e83d036c6aed0d1b0274c584905","observation_id":"187e268c-e189-4be0-8926-36ff1cc385c1","resolution":{"observed_at":"2026-08-06T21:09:14.894850Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:09:14.604739Z","title":", \" * write output.state after.block = add.period write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:14.604739Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:e07379fef13f467450c7d1b75d7d595e1ed602912be7a02845f3cf89dd73fc69","observation_id":"1d6def4e-fc52-4bd5-abfa-bad013536e88","resolution":{"observed_at":"2026-08-06T21:09:14.604739Z","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":"2026-08-06T21:09:14.681309Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges","version":2},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-06T21:09:14.681309Z"},"links":{"citing_paper":"/paper/2507.01085"},"observation_digest":"sha256:f46454cb99758792d23e09cb0613c3642478333d2930113c476a065ea2329fe4","observation_id":"f349f3b0-dc39-4b9e-9bf4-3f6ce2765681","resolution":{"observed_at":"2026-08-06T21:09:14.681309Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.01085","last_updated":"2025-08-08T22:57:30Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-10T08:42:42.973979Z","submitted_at":"2025-07-01T18:00:00Z","title":"LIGHTS. A robust technique to identify galaxy edges"},"reference_resolution":{"displayed":99,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":55,"verified_exact":0,"verified_fuzzy":44},"total_outbound_references":99},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 99 of 99 outbound references and 0 inbound Pith citation observations for arXiv:2507.01085."}