{"as_of":"2026-08-23T05:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b8f2436cd6045ef9976f9054ac93f907a9c619316f054428075a796bde0046ee","coverage":[{"denominator":49,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":49,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T19:08:51.853117Z","state":"measured"},{"denominator":49,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":49,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+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/2501.10622/citation-record","integrity":"/paper/2501.10622/integrity","json":"/paper/2501.10622/citation-record.json","paper":"/paper/2501.10622"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.649316Z","title":"A., Jones, B","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.649316Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:c245ad9b147618ea9ce8bd677db8e0aa6f07c8c2207fbd456ae7a575ecaa4818","observation_id":"500205b9-72a9-41ca-a635-6389e296959b","resolution":{"observed_at":"2026-08-10T19:08:51.649316Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1475-7516/2024/02/001","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:52.601754Z","title":"2024, JCAP, 2024, 001, doi: 10.1088/1475-7516/2024/02/001","venue":null,"work_id":"d9410c46-0d3e-4f4f-9cc2-8f037930b48f","year":2024},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.653642Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:fbd146146e85322180e12f6573738a4b9fe9082eee9b4779412ab64f9de1a0c5","observation_id":"97f6c458-f880-4b32-9729-75b3f328c34d","resolution":{"observed_at":"2026-08-10T19:08:52.606000Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.658004Z","title":"V ., & Rodionov, E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.658004Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:6c04181dc2d993855c2f8f34952d05e78af9df96e04bab29ccec522c36d0f2e6","observation_id":"ac273368-990b-4f14-9eed-4537e055003d","resolution":{"observed_at":"2026-08-10T19:08:51.658004Z","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":"2026-08-10T19:08:51.661883Z","title":"S., Wechsler, R","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.661883Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:7390890794e2a55c7a1587c8ac56400ffffa74c531cbe2395e21f171e53082bf","observation_id":"ba95c5fa-a128-46c7-9307-1dee03984f5f","resolution":{"observed_at":"2026-08-10T19:08:51.661883Z","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":"2026-08-10T19:08:53.064265Z","title":"1991, A&A, 251, 312","venue":null,"work_id":"bbe2be03-07d8-4fb5-ae84-b0b187a0122f","year":1991},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.666358Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:4496ae8eec449c8fac44a1bad0ef54345c98fc063ba65fedda4cda7633db48f0","observation_id":"fab81f9a-28de-4b81-8c34-7dc3bfb1484e","resolution":{"observed_at":"2026-08-10T19:08:53.069003Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.672138Z","title":null,"venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.672138Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:39f2cf9b8071aca9a88f19ac69c2361a59a456bbb902c026de033b4b7a98577c","observation_id":"b45decee-1844-4192-be7c-f23024247909","resolution":{"observed_at":"2026-08-10T19:08:51.672138Z","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":"2026-08-10T19:08:51.676351Z","title":"1992, in Distribution of Matter in the Universe, ed","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.676351Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:00a7e98e58f6820e44f54934bf20949d44a417bff1b7f5d3533ef23866e9349a","observation_id":"ab5e774c-7731-4a62-9b7e-87fb2af1ddd4","resolution":{"observed_at":"2026-08-10T19:08:51.676351Z","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":"2026-08-10T19:08:51.680981Z","title":"2007, in American Institute of Physics Conference Series, V ol","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.680981Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:5d930cb93d5357d29e171ebe24a22b340325179dc4cb3bb44d5a43bce807f312","observation_id":"223eff2c-b716-45c5-902d-04b59a54fc64","resolution":{"observed_at":"2026-08-10T19:08:51.680981Z","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":"2026-08-10T19:08:51.685841Z","title":"S., & White, S","venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.685841Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:f8830355887f30db9a4182b8edee123595eaaa0913ef98607dc98128af61d1d1","observation_id":"7a9e9b2e-b115-448e-beff-608913a0e81c","resolution":{"observed_at":"2026-08-10T19:08:51.685841Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/s11207-012-0109-3","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-19T11:03:45.297681Z","title":"2012, SoPh, 281, 863, doi: 10.1007/s11207-012-0109-3","venue":"Solar Physics","work_id":"63d08bd7-dc08-4780-9ae1-46103f197acf","year":2012},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.689785Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:961632ec898e3324e71af30eb4ce3c0116e59e77274c34071af79b881c1e97d6","observation_id":"efef79da-bf4b-4b6c-bbfd-48d5f2ab7841","resolution":{"observed_at":"2026-08-10T19:08:52.434313Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.693760Z","title":"J., & Hut, P","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.693760Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:88ed557131c8b93c4b17548002b713d1ffd241024aadd03fa3db7459781a5848","observation_id":"90e503ab-cd80-47f9-be1a-8589ccde9508","resolution":{"observed_at":"2026-08-10T19:08:51.693760Z","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":"2026-08-10T19:08:51.698474Z","title":"2006, A&A, 450, 9, doi: 10.1051/0004-6361:20041635","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.698474Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:bb3c96cd99014f4b5e40fbfc9de48e400151bd580e0623887e9ae6ddd6d79690","observation_id":"ee5c4340-d2eb-4033-9ea1-c533328efb73","resolution":{"observed_at":"2026-08-10T19:08:51.698474Z","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":"2026-08-10T19:08:51.703068Z","title":"E., Kashyap, V ., Rosner, R., & Lamb, D","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.703068Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:7823d54e81186d76e55a71ce7fc773a906a6e63f4aacfd39394e0ddac2c507b7","observation_id":"774791c4-a4ed-44ab-a1d2-667fa96be015","resolution":{"observed_at":"2026-08-10T19:08:51.703068Z","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":"2026-08-10T19:08:51.706342Z","title":"S., & White, S","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.706342Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:41a9a51b889e23d8dd017d1069c1deb15f57474119f638ee757f734c731e494c","observation_id":"d203da9f-7682-40bd-ade5-7d4df51d0616","resolution":{"observed_at":"2026-08-10T19:08:51.706342Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/174922","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:52.390878Z","title":"M., & Bertschinger, E","venue":null,"work_id":"76df1b75-aae5-4cdf-92e6-aa6cc2671c27","year":1994},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.710543Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:2626d2c187aa9751ef089a59eabb6d3529600ac0ef93b45e78a96957b1182bb7","observation_id":"fb641041-ad4e-449c-a749-a44101033aac","resolution":{"observed_at":"2026-08-10T19:08:52.394998Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9811393","last_updated":"1998-11-24T21:50:18Z","snapshot_observed_at":"2026-08-05T02:34:34.899927Z","submitted_at":"1998-11-24T21:50:18Z","title":"Group Identification in N-Body Simulations: SKID and DENMAX Versus Friends-of-Friends","version":1},"cited_work":{"arxiv_id":"astro-ph/9811393","doi":"10.48550/arxiv.astro-ph/9811393","metadata_source":"pith","pith_arxiv_id":"astro-ph/9811393","snapshot_observed_at":"2026-08-11T00:16:15.729268Z","title":"Group Identification in N-Body Simulations: SKID and DENMAX Versus Friends-of-Friends","venue":"astro-ph","work_id":"5bea17a1-5928-41b8-b1ae-26939b060f68","year":1998},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.714560Z"},"links":{"cited_paper":"/paper/astro-ph/9811393","citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:6ee207ccc233b56bf5334b0305cb05959f3123bc73240ad260d4d4ecccf0dacd","observation_id":"ad1bd97b-5dfa-4e96-b460-a52928cb6268","resolution":{"observed_at":"2026-08-10T19:08:52.383923Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/175725","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:52.362192Z","title":"A., Forman, W., Jones, C., & Murray, S","venue":null,"work_id":"227d31fb-5caf-419c-a8e3-dbb019bd25b2","year":1995},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.719735Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:68900c1575cc89847a025b19075938f0e6e6a62235bafccbc6d03f886a954dfa","observation_id":"4a3612f7-ac75-494b-b618-0cbd4286b5f2","resolution":{"observed_at":"2026-08-10T19:08:52.365836Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.723599Z","title":"2022, MNRAS, 509, 501, doi: 10.1093/mnras/stab2980","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.723599Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:67e57bf29c66b3467ba7a2e6c2fda85660c2e2f13c6023a5e25607e333cc4c5f","observation_id":"31bec4c4-1a7c-4107-aa6d-c37adf77e4c9","resolution":{"observed_at":"2026-08-10T19:08:51.723599Z","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":"2026-08-10T19:08:51.728040Z","title":"R., Millman, K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.728040Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:7bd9f26520067fe58ade60955b079ed98358b24df772d425384ea3ed9f587d79","observation_id":"27d52614-8e74-48a9-8b3b-34c88315aa49","resolution":{"observed_at":"2026-08-10T19:08:51.728040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.05455","last_updated":"2020-12-10T05:04:44Z","snapshot_observed_at":"2026-08-19T01:02:03.383324Z","submitted_at":"2020-12-10T05:04:44Z","title":"Anomalous inverse proximity effect in unconventional-superconductor junctions","version":1},"cited_work":{"arxiv_id":"2012.05455","doi":null,"metadata_source":"pith","pith_arxiv_id":"2012.05455","snapshot_observed_at":"2026-08-10T19:08:52.961681Z","title":"Anomalous inverse proximity effect in unconventional-superconductor junctions","venue":"cond-mat.supr-con","work_id":"398ede22-c8df-40df-b124-8a494934338c","year":2020},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.731838Z"},"links":{"cited_paper":"/paper/2012.05455","citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:66b842c1ce8b9542c0d97173f1aba8fdd41c88cc0c93ee86fa0f47ab17af66fc","observation_id":"aba5e8f6-a0a8-471d-8eb4-263e1233f34e","resolution":{"observed_at":"2026-08-10T19:08:52.966244Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.737751Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.737751Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:8daa12febcf355cecce5a728058852a1cc2d605d4b54775aeec573747b912926","observation_id":"4c523975-b5ad-468d-8886-3862fbb6da76","resolution":{"observed_at":"2026-08-10T19:08:51.737751Z","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":"2026-08-10T19:08:51.742250Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.742250Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:93d5c1363e9a649b806c26b58d0c3bca85f39bd0ce8ceec5a8da813d5203be2f","observation_id":"fbf40d1e-4dff-4c72-b0c7-48b01ae3ac89","resolution":{"observed_at":"2026-08-10T19:08:51.742250Z","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":"2026-08-10T19:08:51.747980Z","title":"R., Muldrew, S","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.747980Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:bb934fabc790a0de379986bcb819f83b3c579106c04ea07aebafc391d202d40d","observation_id":"804a8aaf-41eb-47c9-b4b5-5c4a19a7ec0d","resolution":{"observed_at":"2026-08-10T19:08:51.747980Z","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":"2026-08-10T19:08:51.751088Z","title":"R., Lux, H., et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.751088Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:69f988c760995393131acdc81c4c40f1a2c2b7daafeb77ac96b40dde4a9a1090","observation_id":"5071ef6e-11a1-4e78-90d6-efc11582ba6e","resolution":{"observed_at":"2026-08-10T19:08:51.751088Z","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":"2026-08-10T19:08:51.756870Z","title":"R., & Knebe, A","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.756870Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:f4670175ae8a8772209726644aca88846ec331f2dd10829f2fea35af5df5d187","observation_id":"e0d5e4c9-c91b-417a-9bf8-aa3ca9d6b180","resolution":{"observed_at":"2026-08-10T19:08:51.756870Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/j.dark.2012.10.002","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:52.300658Z","title":"2012, Physics of the Dark Universe, 1, 50, doi: 10.1016/j.dark.2012.10.002","venue":null,"work_id":"f875b47b-dd27-476f-9931-96cebd3fa708","year":2012},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.761006Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:83c184477e1670c973eb83b6b2f760c199569ecdaa045bc99a58711fc853b88c","observation_id":"2e13ce23-0c65-4789-a6f7-2cd6527bcc8c","resolution":{"observed_at":"2026-08-10T19:08:52.305456Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.765297Z","title":"1994, MNRAS, 271, 676, doi: 10.1093/mnras/271.3.676","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.765297Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:7775a8324607650596a28ece1f4f4d56a234a052405d35f7ae638a111ff87028","observation_id":"8f7536b0-37b2-4050-b95d-b8023a7b0050","resolution":{"observed_at":"2026-08-10T19:08:51.765297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/307788","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:52.282208Z","title":"R., & Tagliaferri, G","venue":null,"work_id":"60c0ed39-05b8-44f7-9338-31dc0894b068","year":1999},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.770028Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:123650d07f3426f05f059df5f15a39b7b6dadb8ae0e9f63e16dbba4d04ff1dc3","observation_id":"348f193e-710f-4c1e-8277-fe1b445a796e","resolution":{"observed_at":"2026-08-10T19:08:52.286165Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.5281/zenodo.15015510","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:52.270660Z","title":"2025, CWTHF (Continuous Wavelet Transform Halo Finder), Zenodo, doi: 10.5281/zenodo.15015510","venue":null,"work_id":"23ae24f1-9744-4e4b-827c-04b9a20aadcd","year":2025},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.774554Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:b21e67de0583d0e3a8e6988cfedac3dfce1b4adb7c5f5d3f1191b04227bc8524","observation_id":"d408ba75-7ba7-4c43-9aff-15c83d55f559","resolution":{"observed_at":"2026-08-10T19:08:52.274736Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.778414Z","title":"2024, ApJ, 973, 39, doi: 10.3847/1538-4357/ad65d1","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.778414Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:35021ef041f4000ace6bf0ddbecec3e6cb5d988646d405ff3ec45035d8113761","observation_id":"845be9b8-ed31-498e-98e2-f4b1b858e532","resolution":{"observed_at":"2026-08-10T19:08:51.778414Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0253-6102/70/6/728","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:52.005168Z","title":"2018, Communications in Theoretical Physics, 70, 728, doi: 10.1088/0253-6102/70/6/728","venue":null,"work_id":"bb832621-4206-4b5b-9f6a-d3ff120edf9c","year":2018},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.783497Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:cfb13544a6a8b92bbf0c1cfbfe78dbe617164be3d9423610f3fcb948cb4b84bb","observation_id":"9b97ab07-e62d-4eff-a673-c666a5582906","resolution":{"observed_at":"2026-08-10T19:08:52.255409Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.788982Z","title":"2015, A&A, 574, A67, doi: 10.1051/0004-6361/201424566","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.788982Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:6f7b339259ea89ece2163b327f0e1e04aefc731e3091a7a67d6d6146480b3d48","observation_id":"1a11809f-654e-4576-bf56-08e1f7bc9038","resolution":{"observed_at":"2026-08-10T19:08:51.788982Z","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":"2026-08-10T19:08:51.793321Z","title":"2019, Computational Astrophysics and Cosmology, 6, 2, doi: 10.1186/s40668-019-0028-x","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.793321Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:6170606d58cedb632352b482f93778f8556a5a59d71964447c2a9a2ba0736a24","observation_id":"997594da-dfac-489b-8411-a7bc6eafbece","resolution":{"observed_at":"2026-08-10T19:08:51.793321Z","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":"2026-08-10T19:08:51.797427Z","title":"2006, A&A, 458, 441, doi: 10.1051/0004-6361:20065225","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.797427Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:c58767d4b995e1e9877186edb5085d6cf5a67c6e33da69fafe9cd58a23872a87","observation_id":"5f5b9f33-4aa7-4b9f-9619-0af3a41691b3","resolution":{"observed_at":"2026-08-10T19:08:51.797427Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/181462","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.966446Z","title":null,"venue":null,"work_id":"c446fcdf-1724-4eaf-9f05-9c3c321c929e","year":1974},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.800885Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:0fd7dd315c16fc07d9cfcfc9dcf2d172a696d34a5375a4006cf909ef5f3242dd","observation_id":"f5fe7a37-0e91-4dbe-b485-c2b161d5f09d","resolution":{"observed_at":"2026-08-10T19:08:51.971489Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.804320Z","title":"2010, A&A, 519, A94, doi: 10.1051/0004-6361/201014214","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.804320Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:e4e7e31586e00cd0077d6791483a41d726f5aba0d7fefdb629c3303ac3277ead","observation_id":"91327ddc-6952-403b-87e4-99a47cab1fce","resolution":{"observed_at":"2026-08-10T19:08:51.804320Z","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":"2026-08-10T19:08:51.807716Z","title":"H., & Schechter, P","venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.807716Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:8b8971b9af565b59ec1a0390c65fcfd3e981d38ce24a565d6b02f40f5d73a837","observation_id":"12d65416-5a75-4865-b96e-ef4ddbe3d7c7","resolution":{"observed_at":"2026-08-10T19:08:51.807716Z","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":"2026-08-10T19:08:51.811102Z","title":"B., Agertz, O., Moore, B., & Stadel, J","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.811102Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:076f1515cc751d5216e5aa2d3cd93bf2ed7b458793d45a89b657b85db44d3f77","observation_id":"f65fe2cf-4e59-4d33-86b6-fe6fe7f4487d","resolution":{"observed_at":"2026-08-10T19:08:51.811102Z","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":"2026-08-10T19:08:51.814121Z","title":"1993, ApJ, 409, 517, doi: 10.1086/172683","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.814121Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:9288cfad237106f4085cb381309fcf9399bafa58265635e1d717e4c6bd59f252","observation_id":"4908bc00-2c9d-4f9b-a059-fadc6219c1cc","resolution":{"observed_at":"2026-08-10T19:08:51.814121Z","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":"2026-08-10T19:08:51.817380Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.817380Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:48403e9347b9c77b71e0668d47f60d60c895dc7fa875ea653706aa091da0c56c","observation_id":"642a0ee0-a65a-4089-bc44-37500eb36214","resolution":{"observed_at":"2026-08-10T19:08:51.817380Z","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":"2026-08-10T19:08:53.052560Z","title":null,"venue":null,"work_id":"0c118d99-cf9e-486d-b908-28c4805f73d5","year":2001},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.821411Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:ffda0ef5b723dbf752ff0599b124f16515d0ff014c5e8a57e82315992d776432","observation_id":"17b84e4f-da5f-4bdb-b617-0ebf015e6602","resolution":{"observed_at":"2026-08-10T19:08:53.057296Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.825186Z","title":"J., Smith, B","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.825186Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:d10450aacd7a7448ab248a6e808cbd02846239424d13633ebd34b97e24d75462","observation_id":"be68ef43-2853-4906-8f94-c52e2e9ec586","resolution":{"observed_at":"2026-08-10T19:08:51.825186Z","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":"4215.2018","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:52.799552Z","title":"B., & Babyk, I","venue":null,"work_id":"34a0743b-5203-4fde-be2e-52c4870d3f7e","year":2018},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.828633Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:edcf78a6eaa1e4f6707e946ab92bb223c73e25aa9c663cc027efaec4149f0d23","observation_id":"002eafab-f92d-48c2-9b99-c62d86afb9ad","resolution":{"observed_at":"2026-08-10T19:08:52.806896Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T19:08:51.833517Z","title":"2020, ApJS, 250, 2, doi: 10.3847/1538-4365/ab9d82","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.833517Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:fd496a86235ed3292f68f5c4cc239fc1afe84a397c440d421867d8c44edada40","observation_id":"03801a9c-d06a-4b4b-85f0-830e4255b0c9","resolution":{"observed_at":"2026-08-10T19:08:51.833517Z","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":"2026-08-10T19:08:51.838452Z","title":"E., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.838452Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:b50e2b9e73ae415c3af2b63e1033b016be25d64b3a0127c1cfedbe4fec58f198","observation_id":"cbca9220-805e-49dd-a3e8-c61973900b00","resolution":{"observed_at":"2026-08-10T19:08:51.838452Z","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":"2026-08-10T19:08:51.841926Z","title":"2008, MNRAS, 387, 601, doi: 10.1111/j.1365-2966.2008.13292.x","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.841926Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:7acdf09b8302fe487ea6cac55dad602b96fdbd75fb9861595c3448aef73ed368","observation_id":"ec8bab95-b1ee-496e-b996-a469758fd971","resolution":{"observed_at":"2026-08-10T19:08:51.841926Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.13876","last_updated":"2024-12-21T22:53:21Z","snapshot_observed_at":"2026-08-16T13:23:59.777878Z","submitted_at":"2024-08-25T15:53:57Z","title":"Capturing primordial non-Gaussian signatures in the late Universe by multi-scale extrema of the cosmic log-density field","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.13876","snapshot_observed_at":"2026-08-10T19:08:51.845629Z","title":"2021, Communications in Theoretical Physics, 73, 095402, doi: 10.1088/1572-9494/ac10be —","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.845629Z"},"links":{"cited_paper":"/paper/2408.13876","citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:1caa1802a9932eaafdfee079a23439ffd6578ec2bdf87f1ba12b38cacef822fd","observation_id":"121f5154-4b41-4133-8921-f5690d9a68fb","resolution":{"observed_at":"2026-08-10T19:08:51.845629Z","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":"2026-08-10T19:08:51.849418Z","title":"2022, ApJ, 934, 77, doi: 10.3847/1538-4357/ac752c","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.849418Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:7830c8520e89c2e20bb81e240e4ee912e3a47378ebbf34a643dafff5800ebb03","observation_id":"a237978d-98f4-4528-9921-3a267185140d","resolution":{"observed_at":"2026-08-10T19:08:51.849418Z","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":"2026-08-10T19:08:51.853117Z","title":"H., Hernquist, L., & Katz, N","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-10T19:08:51.853117Z"},"links":{"citing_paper":"/paper/2501.10622"},"observation_digest":"sha256:7e21fe6dfd1cb33b11c997bd2a546373dc0af75fc7b19b8fa18c3e8b38235011","observation_id":"762e7257-ff22-4da5-9263-20358d36b0e9","resolution":{"observed_at":"2026-08-10T19:08:51.853117Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2501.10622","last_updated":"2025-03-20T08:03:21Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-18T00:30:15.717115Z","submitted_at":"2025-01-18T01:36:07Z","title":"CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform"},"reference_resolution":{"displayed":49,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":36,"verified_exact":10,"verified_fuzzy":1},"total_outbound_references":49},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 49 of 49 outbound references and 0 inbound Pith citation observations for arXiv:2501.10622."}