{"as_of":"2026-08-17T21:03:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:cfbbff0215b0ccd66637fe09055294099b556262accc7b998800e9f7751db900","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T04:33:52.650181Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-11T07:20:58.469970Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2309.03082","last_updated":"2023-09-06T15:28:50Z","snapshot_observed_at":"2026-08-16T15:02:47.839783Z","submitted_at":"2023-09-06T15:28:50Z","title":"The Hawaii Infrared Parallax Program. VI. The Fundamental Properties of 1000+ Ultracool Dwarfs and Planetary-mass Objects Using Optical to Mid-IR SEDs and Comparison to BT-Settl and ATMO 2020 Model Atmospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.03082","snapshot_observed_at":"2026-08-16T04:33:52.650181Z","title":"C., Best, W","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.00978","last_updated":"2025-05-02T03:40:25Z","snapshot_observed_at":"2026-08-16T04:27:57.506962Z","submitted_at":"2025-05-02T03:40:25Z","title":"A Survey Of Model Fits to Brown Dwarf Spectra Through the L-T Sequence","version":1},"reference_index":110,"source":"pdf_text","source_observed_at":"2026-08-16T04:33:52.650181Z"},"links":{"cited_paper":"/paper/2309.03082","citing_paper":"/paper/2505.00978"},"observation_digest":"sha256:2249c173903f97c6adaf5ba52cf1bdb22853c2a8cfc88a566e8756c651786be5","observation_id":"48260190-aad2-49b6-a6f1-7e5465eb5ded","resolution":{"observed_at":"2026-08-16T04:33:52.650181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.03082","last_updated":"2023-09-06T15:28:50Z","snapshot_observed_at":"2026-08-16T15:02:47.839783Z","submitted_at":"2023-09-06T15:28:50Z","title":"The Hawaii Infrared Parallax Program. VI. The Fundamental Properties of 1000+ Ultracool Dwarfs and Planetary-mass Objects Using Optical to Mid-IR SEDs and Comparison to BT-Settl and ATMO 2020 Model Atmospheres","version":1},"cited_work":{"arxiv_id":"2309.03082","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.03082","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"C., Best, W","venue":null,"work_id":"64155350-38e4-4e3f-bb7d-9f16d3e63c9d","year":2023},"citing_paper":{"arxiv_id":"2604.09845","last_updated":"2026-04-10T19:18:26Z","snapshot_observed_at":"2026-08-16T20:35:44.829850Z","submitted_at":"2026-04-10T19:18:26Z","title":"Spectroscopic Characterization of WD J000801.25-350450 and its Two Co-Moving Companions","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-10T17:13:15.887505Z"},"links":{"cited_paper":"/paper/2309.03082","citing_paper":"/paper/2604.09845"},"observation_digest":"sha256:7991dd610563535bd00a079ee5e63f690b994a5d1a0abe303cdfb908b1bd975a","observation_id":"b4171415-6f03-4983-9d24-aef6e9ea9eb2","resolution":{"observed_at":"2026-05-11T07:20:58.474021Z","resolver_source":"arxiv_id","status":"verified_exact"},"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":"2309.03082","last_updated":"2023-09-06T15:28:50Z","snapshot_observed_at":"2026-08-16T15:02:47.839783Z","submitted_at":"2023-09-06T15:28:50Z","title":"The Hawaii Infrared Parallax Program. VI. The Fundamental Properties of 1000+ Ultracool Dwarfs and Planetary-mass Objects Using Optical to Mid-IR SEDs and Comparison to BT-Settl and ATMO 2020 Model Atmospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.03082","snapshot_observed_at":"2026-08-15T14:36:52.552146Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.06454","last_updated":"2026-08-06T18:00:01Z","snapshot_observed_at":"2026-08-16T16:49:35.239006Z","submitted_at":"2026-08-06T18:00:01Z","title":"The Sonora Substellar Atmosphere Models. VII. Flame Skimmer: Cloud-free Atmospheric and Evolutionary Models for the Coldest Substellar Objects","version":1},"reference_index":296,"source":"arxiv_source","source_observed_at":"2026-08-15T14:36:52.552146Z"},"links":{"cited_paper":"/paper/2309.03082","citing_paper":"/paper/2608.06454"},"observation_digest":"sha256:84098b7dbada3422f414264388e8dd1138a91a0a2e12f48ea01875f4d8f6deaf","observation_id":"1a1b7317-36a9-464b-a726-ca2417c510eb","resolution":{"observed_at":"2026-08-15T14:36:52.552146Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2309.03082/citation-record","integrity":"/paper/2309.03082/integrity","json":"/paper/2309.03082/citation-record.json","paper":"/paper/2309.03082"},"outbound":[],"paper":{"arxiv_id":"2309.03082","last_updated":"2023-09-06T15:28:50Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-16T15:02:47.839783Z","submitted_at":"2023-09-06T15:28:50Z","title":"The Hawaii Infrared Parallax Program. VI. The Fundamental Properties of 1000+ Ultracool Dwarfs and Planetary-mass Objects Using Optical to Mid-IR SEDs and Comparison to BT-Settl and ATMO 2020 Model Atmospheres"},"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 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2309.03082."}