{"as_of":"2026-08-11T01:02:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3f9151bd29856af351b494284236e9c07f6b01bdde4cae99a856b04b6d495b49","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-11T11:50:26.030339Z","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":"2026-06-27T10:00:49.905186Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1702.04371","last_updated":"2017-02-14T20:03:51Z","snapshot_observed_at":"2026-07-06T05:30:03.873605Z","submitted_at":"2017-02-14T20:03:51Z","title":"Reconstruction of Galaxy Star Formation Histories through SED Fitting: The Dense Basis Approach","version":1},"cited_work":{"arxiv_id":"1702.04371","doi":null,"metadata_source":"pith","pith_arxiv_id":"1702.04371","snapshot_observed_at":"2026-06-27T10:00:49.905186Z","title":"Reconstruction of Galaxy Star Formation Histories through SED Fitting: The Dense Basis Approach","venue":"astro-ph.GA","work_id":"18ffb00f-7996-4ea8-8ca7-0693a1c1a4fe","year":2017},"citing_paper":{"arxiv_id":"2606.12355","last_updated":"2026-06-10T17:27:12Z","snapshot_observed_at":"2026-07-06T23:51:17.719874Z","submitted_at":"2026-06-10T17:27:12Z","title":"Between Degeneracy and Evolution: UV-to-optical Insights into the BH$^*$ Model in Little Red Dots","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1702.04371","citing_paper":"/paper/2606.12355"},"observation_digest":"sha256:1a0cf7c4a941e8340415da4f756e675b414e39b780a7c0ff0a5294999f7f7d4a","observation_id":"ad3ce918-c380-46b0-9c26-fdf27f949014","resolution":{"observed_at":"2026-06-27T10:00:49.906664Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1702.04371","last_updated":"2017-02-14T20:03:51Z","snapshot_observed_at":"2026-07-06T05:30:03.873605Z","submitted_at":"2017-02-14T20:03:51Z","title":"Reconstruction of Galaxy Star Formation Histories through SED Fitting: The Dense Basis Approach","version":1},"cited_work":{"arxiv_id":"1702.04371","doi":null,"metadata_source":"pith","pith_arxiv_id":"1702.04371","snapshot_observed_at":"2026-06-27T10:00:49.905186Z","title":"Reconstruction of Galaxy Star Formation Histories through SED Fitting: The Dense Basis Approach","venue":"astro-ph.GA","work_id":"18ffb00f-7996-4ea8-8ca7-0693a1c1a4fe","year":2017},"citing_paper":{"arxiv_id":"2606.21651","last_updated":"2026-06-19T18:00:00Z","snapshot_observed_at":"2026-08-02T14:15:26.609490Z","submitted_at":"2026-06-19T18:00:00Z","title":"Resolved Ages and Stellar Metallicities in Progenitors of Milky Way Analogs: A Closer Look at their Star Formation Histories since $z=5$","version":1},"reference_index":142,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1702.04371","citing_paper":"/paper/2606.21651"},"observation_digest":"sha256:0ca367746178d412b3b91e7a49ebfa23cc296fa10686dc3d08271ab803f9d3a9","observation_id":"32409f75-e255-4ede-8d87-eed9a2deb15d","resolution":{"observed_at":"2026-06-26T13:39:31.094401Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1702.04371/citation-record","integrity":"/paper/1702.04371/integrity","json":"/paper/1702.04371/citation-record.json","paper":"/paper/1702.04371"},"outbound":[],"paper":{"arxiv_id":"1702.04371","last_updated":"2017-02-14T20:03:51Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T05:30:03.873605Z","submitted_at":"2017-02-14T20:03:51Z","title":"Reconstruction of Galaxy Star Formation Histories through SED Fitting: The Dense Basis Approach"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1702.04371."}