{"as_of":"2026-08-11T15:31:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:960d0f04cafb5930064ac0e83d123a30397abf6bb37a84b48d7f4a9e08f013e9","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T04:43:52.984603Z","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":"2026-08-10T05:30:23.456663Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-10T05:30:23.456663Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2402.05184","last_updated":"2024-02-07T19:00:35Z","snapshot_observed_at":"2026-07-06T17:27:03.686119Z","submitted_at":"2024-02-07T19:00:35Z","title":"A self-consistent data-driven model for determining stellar parameters from optical and near-IR spectra","version":1},"cited_work":{"arxiv_id":"2402.05184","doi":"10.48550/arxiv.2402.05184","metadata_source":"pith","pith_arxiv_id":"2402.05184","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"A self-consistent data-driven model for determining stellar parameters from optical and near-IR spectra","venue":"astro-ph.SR","work_id":"6b4d963c-51b0-4173-ac6d-0dac2978d568","year":2024},"citing_paper":{"arxiv_id":"2506.09826","last_updated":"2025-06-11T15:06:26Z","snapshot_observed_at":"2026-08-07T04:37:02.603600Z","submitted_at":"2025-06-11T15:06:26Z","title":"ABYSS III: Observing accretion activity in young stars through empirical veiling measurements","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T04:43:52.984603Z"},"links":{"cited_paper":"/paper/2402.05184","citing_paper":"/paper/2506.09826"},"observation_digest":"sha256:663ef732f655ec6971af07845147095cd3e565a078c5dbb31c11e0feb434f073","observation_id":"9949268b-5141-4744-806b-3c6f9a02d623","resolution":{"observed_at":"2026-08-07T04:43:54.511359Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.05184","last_updated":"2024-02-07T19:00:35Z","snapshot_observed_at":"2026-07-06T17:27:03.686119Z","submitted_at":"2024-02-07T19:00:35Z","title":"A self-consistent data-driven model for determining stellar parameters from optical and near-IR spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.05184","snapshot_observed_at":"2026-08-01T20:35:53.226342Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.16585","last_updated":"2026-07-18T01:57:26Z","snapshot_observed_at":"2026-08-06T17:07:05.033305Z","submitted_at":"2026-07-18T01:57:26Z","title":"Effective temperatures estimation of low-mass stars and identification of T Tauri stars in LAMOST DR10 using machine learning","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-01T20:35:53.226342Z"},"links":{"cited_paper":"/paper/2402.05184","citing_paper":"/paper/2607.16585"},"observation_digest":"sha256:83cde778e44fd03b8e997810392b1e8504ce788a1ad2fcea633bed0120a3434b","observation_id":"cb59df30-e8f4-4eb1-9a1f-909095fdf7e3","resolution":{"observed_at":"2026-08-01T20:35:53.226342Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.05184","last_updated":"2024-02-07T19:00:35Z","snapshot_observed_at":"2026-07-06T17:27:03.686119Z","submitted_at":"2024-02-07T19:00:35Z","title":"A self-consistent data-driven model for determining stellar parameters from optical and near-IR spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.05184","snapshot_observed_at":"2026-08-01T04:28:40.677071Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.22822","last_updated":"2026-07-28T14:26:38Z","snapshot_observed_at":"2026-08-08T13:40:23.196087Z","submitted_at":"2026-07-24T18:01:06Z","title":"BOSS-CLAM: Utilizing a Constrained Linear Absorption Model to Infer Stellar Parameters from BOSS Spectra","version":2},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-01T04:28:40.677071Z"},"links":{"cited_paper":"/paper/2402.05184","citing_paper":"/paper/2607.22822"},"observation_digest":"sha256:3157a536133a0ebf0d58b1a60c878077d857abde9c83b0c32548cc6c63f94b04","observation_id":"747843af-5495-4c7f-8a1e-bdf98ece0cd4","resolution":{"observed_at":"2026-08-01T04:28:40.677071Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.05184","last_updated":"2024-02-07T19:00:35Z","snapshot_observed_at":"2026-07-06T17:27:03.686119Z","submitted_at":"2024-02-07T19:00:35Z","title":"A self-consistent data-driven model for determining stellar parameters from optical and near-IR spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.05184","snapshot_observed_at":"2026-08-01T00:41:50.036561Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.26149","last_updated":"2026-07-28T18:00:39Z","snapshot_observed_at":"2026-08-06T23:47:51.776966Z","submitted_at":"2026-07-28T18:00:39Z","title":"The Twentieth Data Release of the Sloan Digital Sky Survey: First All-Sky BOSS Spectra, eROSITA-SDSS-V Mapper Coordinated Observations, and a Preview of the Local Volume Mapper","version":1},"reference_index":248,"source":"arxiv_source","source_observed_at":"2026-08-01T00:41:50.036561Z"},"links":{"cited_paper":"/paper/2402.05184","citing_paper":"/paper/2607.26149"},"observation_digest":"sha256:50f3ade2c3a774f9217e2d5f271c0a12bdec98ddda2b84e56a1765e4deb30f92","observation_id":"bc73a379-2d3f-4a8f-b0b7-e3a8a22dd49d","resolution":{"observed_at":"2026-08-01T00:41:50.036561Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2402.05184/citation-record","integrity":"/paper/2402.05184/integrity","json":"/paper/2402.05184/citation-record.json","paper":"/paper/2402.05184"},"outbound":[],"paper":{"arxiv_id":"2402.05184","last_updated":"2024-02-07T19:00:35Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T17:27:03.686119Z","submitted_at":"2024-02-07T19:00:35Z","title":"A self-consistent data-driven model for determining stellar parameters from optical and near-IR spectra"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2402.05184."}