{"as_of":"2026-08-18T05:08:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:374a54831ffe6f2020cd5acb6d78427cafa3b85e47ec1d8d7581f69e09564b01","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:21:48.518077Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":14,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2208.14974","last_updated":"2023-09-07T10:45:54Z","snapshot_observed_at":"2026-08-16T19:36:38.008886Z","submitted_at":"2022-08-31T17:16:34Z","title":"Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.14974","snapshot_observed_at":"2026-08-11T21:32:31.374774Z","title":"2022, arXiv e-prints, arXiv:2208.14974","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.04542","last_updated":"2024-12-05T19:00:00Z","snapshot_observed_at":"2026-08-15T15:06:40.388907Z","submitted_at":"2024-12-05T19:00:00Z","title":"Efficient Ionizers with Low H$\\boldsymbol{\\beta}$+[OIII] Equivalent Widths: JADES Spectroscopy of a Peculiar High-z Population","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-11T21:32:31.374774Z"},"links":{"cited_paper":"/paper/2208.14974","citing_paper":"/paper/2412.04542"},"observation_digest":"sha256:411d6fffbc18c742233fa6cf6b15aa6bbe1e053c653baada75b57e1780171731","observation_id":"13d64587-8190-459f-ad88-08d30d8924ff","resolution":{"observed_at":"2026-08-11T21:32:31.374774Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14974","last_updated":"2023-09-07T10:45:54Z","snapshot_observed_at":"2026-08-16T19:36:38.008886Z","submitted_at":"2022-08-31T17:16:34Z","title":"Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.14974","snapshot_observed_at":"2026-08-15T21:21:48.518077Z","title":"2017,MNRAS, 466, 798, doi: 10.1093/mnras/stw3020 —","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.10078","last_updated":"2025-05-15T08:32:30Z","snapshot_observed_at":"2026-08-18T02:06:27.792677Z","submitted_at":"2025-05-15T08:32:30Z","title":"Clumpy Starburst in a Local Dwarf Galaxy, NGC 1522","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T21:21:48.518077Z"},"links":{"cited_paper":"/paper/2208.14974","citing_paper":"/paper/2505.10078"},"observation_digest":"sha256:b3067895a4446fb5c6eb654e1120fd0305a6d6ac9541f7edea77e0c4fa484092","observation_id":"b2cc048c-e48d-46de-8d85-77db7357b378","resolution":{"observed_at":"2026-08-15T21:21:48.518077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14974","last_updated":"2023-09-07T10:45:54Z","snapshot_observed_at":"2026-08-16T19:36:38.008886Z","submitted_at":"2022-08-31T17:16:34Z","title":"Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.14974","snapshot_observed_at":"2026-08-07T10:50:57.556627Z","title":"2017, MNRAS, 466, 798, doi: 10.1093/mnras/stw3020 —","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.04522","last_updated":"2025-06-05T00:05:45Z","snapshot_observed_at":"2026-08-14T13:35:06.483076Z","submitted_at":"2025-06-05T00:05:45Z","title":"Fast Luminous Extragalactic Transients in the VLA Sky Survey: Implications for the rates of Accretion-Induced Collapse Events, Fast Blue Optical Transients and Gamma Ray Burst Afterglows","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T10:50:57.556627Z"},"links":{"cited_paper":"/paper/2208.14974","citing_paper":"/paper/2506.04522"},"observation_digest":"sha256:5c11cbf1caabb06dfcbb3cb27c7522c592bdff321782e729393731c9d5276720","observation_id":"f12ed4f5-2d55-41c7-9a30-7b71c0a07ddd","resolution":{"observed_at":"2026-08-07T10:50:57.556627Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14974","last_updated":"2023-09-07T10:45:54Z","snapshot_observed_at":"2026-08-16T19:36:38.008886Z","submitted_at":"2022-08-31T17:16:34Z","title":"Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8","version":2},"cited_work":{"arxiv_id":"2208.14974","doi":"10.48550/arxiv.2208.14974","metadata_source":"pith","pith_arxiv_id":"2208.14974","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8","venue":"astro-ph.GA","work_id":"7c6f1b4d-9dd1-4521-91e8-721c68f54b5b","year":2022},"citing_paper":{"arxiv_id":"2606.11367","last_updated":"2026-06-09T18:48:11Z","snapshot_observed_at":"2026-08-14T05:51:33.459927Z","submitted_at":"2026-06-09T18:48:11Z","title":"Studying hot evolved stars with ultraviolet spectroscopy","version":1},"reference_index":192,"source":"arxiv_source","source_observed_at":"2026-06-27T11:23:20.339014Z"},"links":{"cited_paper":"/paper/2208.14974","citing_paper":"/paper/2606.11367"},"observation_digest":"sha256:a065011aa78250f6b5ffb82b68df1b162a7d964dcd6bfbddf0785a227bb75f3b","observation_id":"ccc08e5e-bc61-455e-91eb-9134cd69cd22","resolution":{"observed_at":"2026-06-28T03:11:31.054701Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14974","last_updated":"2023-09-07T10:45:54Z","snapshot_observed_at":"2026-08-16T19:36:38.008886Z","submitted_at":"2022-08-31T17:16:34Z","title":"Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.14974","snapshot_observed_at":"2026-07-12T09:44:28.146054Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.00105","last_updated":"2026-07-06T13:25:42Z","snapshot_observed_at":"2026-08-13T09:45:14.522491Z","submitted_at":"2026-06-30T19:45:20Z","title":"AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN","version":2},"reference_index":106,"source":"arxiv_source","source_observed_at":"2026-07-12T09:44:28.146054Z"},"links":{"cited_paper":"/paper/2208.14974","citing_paper":"/paper/2607.00105"},"observation_digest":"sha256:1673c24ad700f41828f9adde96f3af704c0f13b8742ebf45815bc9029af052df","observation_id":"7c3980a5-4633-491f-8c1f-afd96eb44dc3","resolution":{"observed_at":"2026-07-12T09:44:28.146054Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14974","last_updated":"2023-09-07T10:45:54Z","snapshot_observed_at":"2026-08-16T19:36:38.008886Z","submitted_at":"2022-08-31T17:16:34Z","title":"Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.14974","snapshot_observed_at":"2026-07-12T07:37:06.339592Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.02704","last_updated":"2026-07-02T18:47:11Z","snapshot_observed_at":"2026-08-17T17:40:24.660237Z","submitted_at":"2026-07-02T18:47:11Z","title":"S-PLUS Clusters And Large-scale Environments (SCALE): I. A catalog of known clusters and groups in DR5 and a pilot study of Abell 4038","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-07-12T07:37:06.339592Z"},"links":{"cited_paper":"/paper/2208.14974","citing_paper":"/paper/2607.02704"},"observation_digest":"sha256:9c6ef084736a3067c74ce708cb7bb9e9bc9f6433b4347cfdfdfbc82a76539e4e","observation_id":"d6bf2c89-d989-4fa6-97bb-c27225eeb9e5","resolution":{"observed_at":"2026-07-12T07:37:06.339592Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14974","last_updated":"2023-09-07T10:45:54Z","snapshot_observed_at":"2026-08-16T19:36:38.008886Z","submitted_at":"2022-08-31T17:16:34Z","title":"Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8","version":2},"cited_work":{"arxiv_id":"2208.14974","doi":"10.48550/arxiv.2208.14974","metadata_source":"pith","pith_arxiv_id":"2208.14974","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8","venue":"astro-ph.GA","work_id":"7c6f1b4d-9dd1-4521-91e8-721c68f54b5b","year":2022},"citing_paper":{"arxiv_id":"2607.07818","last_updated":"2026-07-08T18:03:05Z","snapshot_observed_at":"2026-08-13T13:38:24.044750Z","submitted_at":"2026-07-08T18:03:05Z","title":"The DESI View of the Faint Radio Source Population in LoTSS DR2","version":1},"reference_index":119,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2208.14974","citing_paper":"/paper/2607.07818"},"observation_digest":"sha256:ca4dcd6a5dc26a60422e1775cba68861c82bbf3d67f5de762d7cfb9091e889ac","observation_id":"569a4c10-8f2b-4a09-82b0-190ebeff943c","resolution":{"observed_at":"2026-07-10T17:27:26.560730Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14974","last_updated":"2023-09-07T10:45:54Z","snapshot_observed_at":"2026-08-16T19:36:38.008886Z","submitted_at":"2022-08-31T17:16:34Z","title":"Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.14974","snapshot_observed_at":"2026-08-07T00:14:53.619407Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.02725","last_updated":"2026-08-03T18:00:02Z","snapshot_observed_at":"2026-08-13T09:09:45.039750Z","submitted_at":"2026-08-03T18:00:02Z","title":"AT 2022csn: A Photometrically Peculiar Optical/UV Tidal Disruption Event in a Type II AGN","version":1},"reference_index":104,"source":"arxiv_source","source_observed_at":"2026-08-07T00:14:53.619407Z"},"links":{"cited_paper":"/paper/2208.14974","citing_paper":"/paper/2608.02725"},"observation_digest":"sha256:30961bfc4e7edc3e6897e385dcf3b0371623450643f490c6fad219b150ea35da","observation_id":"6218d574-229e-4d57-a3cb-a4bd71092798","resolution":{"observed_at":"2026-08-07T00:14:53.619407Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14974","last_updated":"2023-09-07T10:45:54Z","snapshot_observed_at":"2026-08-16T19:36:38.008886Z","submitted_at":"2022-08-31T17:16:34Z","title":"Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.14974","snapshot_observed_at":"2026-08-14T04:18:57.241514Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10163","last_updated":"2026-08-12T12:23:45Z","snapshot_observed_at":"2026-08-16T12:53:46.849199Z","submitted_at":"2026-08-10T19:31:42Z","title":"CORN -- Chronometers of Relic Nature I: The first estimate of the expansion rate of the Universe using compact relic galaxies","version":2},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-14T04:18:57.241514Z"},"links":{"cited_paper":"/paper/2208.14974","citing_paper":"/paper/2608.10163"},"observation_digest":"sha256:3b036778f6d753bfc68135ad0d996ebfef480be65fd1f2b14e2ab3f7315cc42f","observation_id":"fe9c4481-ce30-42e6-bbc3-5f9bf618899d","resolution":{"observed_at":"2026-08-14T04:18:57.241514Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2208.14974/citation-record","integrity":"/paper/2208.14974/integrity","json":"/paper/2208.14974/citation-record.json","paper":"/paper/2208.14974"},"outbound":[],"paper":{"arxiv_id":"2208.14974","last_updated":"2023-09-07T10:45:54Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-16T19:36:38.008886Z","submitted_at":"2022-08-31T17:16:34Z","title":"Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8"},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2208.14974."}