{"as_of":"2026-08-21T02:33:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7c67b12077c201e4c6ca6d743532a87e3b1103ff0c6897903c22ccd0bdd6d636","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":11,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":11,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":11,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":11,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T04:13:35.201423Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-07T17:24:00.778672Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2203.08539","last_updated":"2022-03-16T11:04:56Z","snapshot_observed_at":"2026-08-19T21:51:25.111817Z","submitted_at":"2022-03-16T11:04:56Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.08539","snapshot_observed_at":"2026-08-16T04:13:35.201423Z","title":"Driver, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.01776","last_updated":"2025-08-31T04:35:38Z","snapshot_observed_at":"2026-08-17T09:35:45.096650Z","submitted_at":"2025-05-03T10:27:06Z","title":"Mapping Nearby Galaxies with Apache Point Observatory: Group and field galaxies' morphologies in the colour-magnitude plane","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-16T04:13:35.201423Z"},"links":{"cited_paper":"/paper/2203.08539","citing_paper":"/paper/2505.01776"},"observation_digest":"sha256:35428dd6c921645b7e67e274bf2c558f5b7432e95bce3954446e3c63fb95919d","observation_id":"ce63cf19-0b02-4652-89bf-3efdc13c374a","resolution":{"observed_at":"2026-08-16T04:13:35.201423Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.08539","last_updated":"2022-03-16T11:04:56Z","snapshot_observed_at":"2026-08-19T21:51:25.111817Z","submitted_at":"2022-03-16T11:04:56Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","version":1},"cited_work":{"arxiv_id":"2203.08539","doi":null,"metadata_source":"pith","pith_arxiv_id":"2203.08539","snapshot_observed_at":"2026-07-07T17:24:00.778672Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","venue":"astro-ph.GA","work_id":"4aece8b8-0bcb-4df3-9a35-1f0a2039db53","year":2022},"citing_paper":{"arxiv_id":"2605.01963","last_updated":"2026-05-03T16:50:00Z","snapshot_observed_at":"2026-07-31T21:42:31.294100Z","submitted_at":"2026-05-03T16:50:00Z","title":"Constraints on Halo Gas Profiles from Joint kSZ and Galaxy Clustering Analysis of ACT DR6 and CMASS","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-08T19:30:05.210473Z"},"links":{"cited_paper":"/paper/2203.08539","citing_paper":"/paper/2605.01963"},"observation_digest":"sha256:88093ca30b5a16f890c1de28b73bcf0ae9bc714546fa4e6cd3c606c2639c78c1","observation_id":"1db5f218-b783-4104-ba58-c0e8bf7af595","resolution":{"observed_at":"2026-05-09T05:50:26.656423Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.08539","last_updated":"2022-03-16T11:04:56Z","snapshot_observed_at":"2026-08-19T21:51:25.111817Z","submitted_at":"2022-03-16T11:04:56Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","version":1},"cited_work":{"arxiv_id":"2203.08539","doi":null,"metadata_source":"pith","pith_arxiv_id":"2203.08539","snapshot_observed_at":"2026-07-07T17:24:00.778672Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","venue":"astro-ph.GA","work_id":"4aece8b8-0bcb-4df3-9a35-1f0a2039db53","year":2022},"citing_paper":{"arxiv_id":"2605.06790","last_updated":"2026-05-07T18:00:11Z","snapshot_observed_at":"2026-08-17T13:03:30.037348Z","submitted_at":"2026-05-07T18:00:11Z","title":"Machine Learning Techniques for Astrophysics and Cosmology: Photometric Redshifts","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-11T00:51:26.783868Z"},"links":{"cited_paper":"/paper/2203.08539","citing_paper":"/paper/2605.06790"},"observation_digest":"sha256:40224c44eda1ba1f68cfceaf8f05fc9b9897eaa32e1bd06502a130d1d1409192","observation_id":"6af7375f-4f12-467e-9903-28fa40d8d2ab","resolution":{"observed_at":"2026-05-11T05:10:53.833358Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.08539","last_updated":"2022-03-16T11:04:56Z","snapshot_observed_at":"2026-08-19T21:51:25.111817Z","submitted_at":"2022-03-16T11:04:56Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.08539","snapshot_observed_at":"2026-07-11T19:34:01.972164Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.04384","last_updated":"2026-07-05T16:23:07Z","snapshot_observed_at":"2026-08-17T12:56:36.783082Z","submitted_at":"2026-07-05T16:23:07Z","title":"KiDS-Legacy: The consistency test of the large-scale structure with Bernardeau-Nishimichi-Taruya transform","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-07-11T19:34:01.972164Z"},"links":{"cited_paper":"/paper/2203.08539","citing_paper":"/paper/2607.04384"},"observation_digest":"sha256:a559af684ae88f4d6c86cd05941c4d795d4f8d7dd1a159c9235bf9a7f6b0722c","observation_id":"b976416d-a12e-440d-a5b4-dd3f72c7294c","resolution":{"observed_at":"2026-07-11T19:34:01.972164Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.08539","last_updated":"2022-03-16T11:04:56Z","snapshot_observed_at":"2026-08-19T21:51:25.111817Z","submitted_at":"2022-03-16T11:04:56Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","version":1},"cited_work":{"arxiv_id":"2203.08539","doi":null,"metadata_source":"pith","pith_arxiv_id":"2203.08539","snapshot_observed_at":"2026-07-07T17:24:00.778672Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","venue":"astro-ph.GA","work_id":"4aece8b8-0bcb-4df3-9a35-1f0a2039db53","year":2022},"citing_paper":{"arxiv_id":"2607.05326","last_updated":"2026-07-06T17:02:03Z","snapshot_observed_at":"2026-08-14T20:46:31.399566Z","submitted_at":"2026-07-06T17:02:03Z","title":"Weak Evolution of Cosmic Atomic Hydrogen over the Past 4.5 Billion Years","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-07-07T17:16:56.936970Z"},"links":{"cited_paper":"/paper/2203.08539","citing_paper":"/paper/2607.05326"},"observation_digest":"sha256:274b638b91c7b1d71e32e9d5903c5782b3afbfee817ab05e27eb57f5aceda576","observation_id":"cf148eee-4e40-4f89-840d-005f841a3c82","resolution":{"observed_at":"2026-07-07T17:24:00.780185Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.08539","last_updated":"2022-03-16T11:04:56Z","snapshot_observed_at":"2026-08-19T21:51:25.111817Z","submitted_at":"2022-03-16T11:04:56Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.08539","snapshot_observed_at":"2026-07-14T05:32:07.775931Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.11448","last_updated":"2026-07-13T11:59:50Z","snapshot_observed_at":"2026-08-15T00:30:40.610419Z","submitted_at":"2026-07-13T11:59:50Z","title":"Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-07-14T05:32:07.775931Z"},"links":{"cited_paper":"/paper/2203.08539","citing_paper":"/paper/2607.11448"},"observation_digest":"sha256:c223c9d64ffbceb219afcd7668bdfdeab26801b5c4c6e4b49ac5817a1dbfcf47","observation_id":"9cf0d0fc-c427-4d62-9c32-18de0e221387","resolution":{"observed_at":"2026-07-14T05:32:07.775931Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.08539","last_updated":"2022-03-16T11:04:56Z","snapshot_observed_at":"2026-08-19T21:51:25.111817Z","submitted_at":"2022-03-16T11:04:56Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.08539","snapshot_observed_at":"2026-08-02T00:50:15.556893Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14901","last_updated":"2026-07-16T12:17:52Z","snapshot_observed_at":"2026-08-15T18:41:04.932439Z","submitted_at":"2026-07-16T12:17:52Z","title":"The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations","version":1},"reference_index":187,"source":"arxiv_source","source_observed_at":"2026-08-02T00:50:15.556893Z"},"links":{"cited_paper":"/paper/2203.08539","citing_paper":"/paper/2607.14901"},"observation_digest":"sha256:b2f8ad498b62ea51e21f74eb15a4080153875afc8956d175958a37897e9af7c5","observation_id":"079e15f7-edd1-4419-aa11-6da5d9a09b11","resolution":{"observed_at":"2026-08-02T00:50:15.556893Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.08539","last_updated":"2022-03-16T11:04:56Z","snapshot_observed_at":"2026-08-19T21:51:25.111817Z","submitted_at":"2022-03-16T11:04:56Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.08539","snapshot_observed_at":"2026-08-01T08:26:06.696036Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.21140","last_updated":"2026-07-23T10:17:57Z","snapshot_observed_at":"2026-08-16T04:49:39.914531Z","submitted_at":"2026-07-23T10:17:57Z","title":"What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-01T08:26:06.696036Z"},"links":{"cited_paper":"/paper/2203.08539","citing_paper":"/paper/2607.21140"},"observation_digest":"sha256:9c1683eb58aee786fffd85fb4f87d72bcfe4e40c1e7db8e1541051a5bb59a395","observation_id":"d9c5b079-3ab5-4ea1-941d-9f46ba946304","resolution":{"observed_at":"2026-08-01T08:26:06.696036Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.08539","last_updated":"2022-03-16T11:04:56Z","snapshot_observed_at":"2026-08-19T21:51:25.111817Z","submitted_at":"2022-03-16T11:04:56Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.08539","snapshot_observed_at":"2026-08-01T08:11:14.650290Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.21225","last_updated":"2026-07-23T11:39:52Z","snapshot_observed_at":"2026-08-20T11:16:35.889890Z","submitted_at":"2026-07-23T11:39:52Z","title":"The Stellar Mass Function of Gas-Rich Galaxies and the Underlying $M_{\\rm HI}-M_{\\rm star}$ Scaling Relation in the Local Universe","version":1},"reference_index":145,"source":"arxiv_source","source_observed_at":"2026-08-01T08:11:14.650290Z"},"links":{"cited_paper":"/paper/2203.08539","citing_paper":"/paper/2607.21225"},"observation_digest":"sha256:4af146526edf274f97f72ec5d780d3bb47f71d67befd5e75bc91d4eb35cb2bc1","observation_id":"0cecf282-ed4b-49d0-acea-a62ca34055ef","resolution":{"observed_at":"2026-08-01T08:11:14.650290Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.08539","last_updated":"2022-03-16T11:04:56Z","snapshot_observed_at":"2026-08-19T21:51:25.111817Z","submitted_at":"2022-03-16T11:04:56Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.08539","snapshot_observed_at":"2026-08-08T18:53:59.747825Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.04371","last_updated":"2026-08-05T02:21:38Z","snapshot_observed_at":"2026-08-14T08:31:59.450484Z","submitted_at":"2026-08-05T02:21:38Z","title":"FAST Ultra-Deep Survey: the baryonic Tully-Fisher relation in FUDS0 field","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-08T18:53:59.747825Z"},"links":{"cited_paper":"/paper/2203.08539","citing_paper":"/paper/2608.04371"},"observation_digest":"sha256:df8443e214692212ed0f0be0c9901f272f69dc144516e54d11329a7b19776f33","observation_id":"4b051ee8-c17a-4663-a4f0-e0a6ebf40dfd","resolution":{"observed_at":"2026-08-08T18:53:59.747825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.08539","last_updated":"2022-03-16T11:04:56Z","snapshot_observed_at":"2026-08-19T21:51:25.111817Z","submitted_at":"2022-03-16T11:04:56Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.08539","snapshot_observed_at":"2026-08-07T22:22:29.927495Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05854","last_updated":"2026-08-17T08:08:30Z","snapshot_observed_at":"2026-08-20T23:17:01.807126Z","submitted_at":"2026-08-06T10:31:38Z","title":"Investigating radio source population $\\&$ spatial characteristics of diffuse Galactic synchrotron emission in the GAMA-23 field with uGMRT Band-3","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-07T22:22:29.927495Z"},"links":{"cited_paper":"/paper/2203.08539","citing_paper":"/paper/2608.05854"},"observation_digest":"sha256:18214edb1d25f0bb630f6a4783757a9cbbb4fb185df7bef887a9944b2caeaf8a","observation_id":"334a0f75-60d0-472f-a28f-50df81a82224","resolution":{"observed_at":"2026-08-07T22:22:29.927495Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2203.08539/citation-record","integrity":"/paper/2203.08539/integrity","json":"/paper/2203.08539/citation-record.json","paper":"/paper/2203.08539"},"outbound":[],"paper":{"arxiv_id":"2203.08539","last_updated":"2022-03-16T11:04:56Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-19T21:51:25.111817Z","submitted_at":"2022-03-16T11:04:56Z","title":"Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2203.08539."}