{"as_of":"2026-08-14T08:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:da8529a9152e1532117f6f556434906349123a57e862e52d01dd6d7c3b821d32","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":"2026-08-14T06:32:32.682623+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":"2026-08-02T02:31:12.826667Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.19932","last_updated":"2025-03-24T12:30:00Z","snapshot_observed_at":"2026-08-07T16:41:21.982635Z","submitted_at":"2025-03-24T12:30:00Z","title":"Exozodiacal dust as a limitation to exoplanet imaging and spectroscopy","version":1},"cited_work":{"arxiv_id":"2503.19932","doi":"10.48550/arxiv.2503.19932","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.19932","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"H., Debes, J., Hasegawa, Y., et al","venue":"ArXiv.org","work_id":"bbc8d226-7d35-40fc-93ab-c9356205da7a","year":2025},"citing_paper":{"arxiv_id":"2510.18231","last_updated":"2026-04-28T15:50:46Z","snapshot_observed_at":"2026-08-11T08:09:36.910238Z","submitted_at":"2025-10-21T02:30:48Z","title":"SKYSURF-11: A New Zodiacal Light Model Optimized for Optical Wavelengths","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-18T05:34:28.070345Z"},"links":{"cited_paper":"/paper/2503.19932","citing_paper":"/paper/2510.18231"},"observation_digest":"sha256:7e83ad136a59511b171c61dcaddfd28e6371edc37737e6fc7fd2664e57d49fd0","observation_id":"86c5adae-a9fe-4dd2-ba09-7fb507331788","resolution":{"observed_at":"2026-05-18T05:35:55.832113Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19932","last_updated":"2025-03-24T12:30:00Z","snapshot_observed_at":"2026-08-07T16:41:21.982635Z","submitted_at":"2025-03-24T12:30:00Z","title":"Exozodiacal dust as a limitation to exoplanet imaging and spectroscopy","version":1},"cited_work":{"arxiv_id":"2503.19932","doi":"10.48550/arxiv.2503.19932","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.19932","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"H., Debes, J., Hasegawa, Y., et al","venue":"ArXiv.org","work_id":"bbc8d226-7d35-40fc-93ab-c9356205da7a","year":2025},"citing_paper":{"arxiv_id":"2605.18953","last_updated":"2026-05-18T18:00:03Z","snapshot_observed_at":"2026-08-13T12:42:40.830236Z","submitted_at":"2026-05-18T18:00:03Z","title":"Astrometric exoplanet detection survives solar-like stellar contamination","version":1},"reference_index":157,"source":"arxiv_source","source_observed_at":"2026-05-20T08:13:03.123280Z"},"links":{"cited_paper":"/paper/2503.19932","citing_paper":"/paper/2605.18953"},"observation_digest":"sha256:3e6cb6c81a5cf501419b01475f9831758901e9d93e7b908e4ce5c61308a847b7","observation_id":"138af723-d542-4409-b16c-067b607be2e4","resolution":{"observed_at":"2026-05-20T08:13:07.798106Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19932","last_updated":"2025-03-24T12:30:00Z","snapshot_observed_at":"2026-08-07T16:41:21.982635Z","submitted_at":"2025-03-24T12:30:00Z","title":"Exozodiacal dust as a limitation to exoplanet imaging and spectroscopy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19932","snapshot_observed_at":"2026-08-02T02:31:12.826667Z","title":"H., Debes, J., Hasegawa, Y., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.14329","last_updated":"2026-07-15T19:47:30Z","snapshot_observed_at":"2026-08-13T06:41:55.332306Z","submitted_at":"2026-07-15T19:47:30Z","title":"The exozodi spectral effect: Residual habitable zone dust may bias exoEarth characterization","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-02T02:31:12.826667Z"},"links":{"cited_paper":"/paper/2503.19932","citing_paper":"/paper/2607.14329"},"observation_digest":"sha256:5095188d028e251eb4e3860fbb0d2ba3ca4d9cf8c0607cb245e6e148ecabbdff","observation_id":"73e186bf-3ec3-469a-80fe-bd8c51e9c3b7","resolution":{"observed_at":"2026-08-02T02:31:12.826667Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2503.19932/citation-record","integrity":"/paper/2503.19932/integrity","json":"/paper/2503.19932/citation-record.json","paper":"/paper/2503.19932"},"outbound":[],"paper":{"arxiv_id":"2503.19932","last_updated":"2025-03-24T12:30:00Z","latest_version":1,"primary_category":"astro-ph.IM","snapshot_observed_at":"2026-08-07T16:41:21.982635Z","submitted_at":"2025-03-24T12:30:00Z","title":"Exozodiacal dust as a limitation to exoplanet imaging and spectroscopy"},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2503.19932."}