{"as_of":"2026-08-20T01:21:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ec979b73b76f8e100d5c537903928ddfa24291611029fe955df39621aca02c55","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T15:20:03.151930Z","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":"2026-07-13T14:39:39.616184Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2104.06802","last_updated":"2021-04-14T12:06:03Z","snapshot_observed_at":"2026-08-16T18:31:40.583969Z","submitted_at":"2021-04-14T12:06:03Z","title":"X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.06802","snapshot_observed_at":"2026-08-11T05:41:09.093958Z","title":"X-ray emission from magnetized neutron star atmospheres at low mass-accretion rates","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.17275","last_updated":"2024-12-23T04:56:56Z","snapshot_observed_at":"2026-08-18T01:45:24.635939Z","submitted_at":"2024-12-23T04:56:56Z","title":"X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries","version":1},"reference_index":107,"source":"pdf_text","source_observed_at":"2026-08-11T05:41:09.093958Z"},"links":{"cited_paper":"/paper/2104.06802","citing_paper":"/paper/2412.17275"},"observation_digest":"sha256:277c332d07ef4ab6c74546764d76a20b87e4ea36f700dd02d234fb8ae8336cbe","observation_id":"d9062d61-22f6-4558-8825-3f611b81737e","resolution":{"observed_at":"2026-08-11T05:41:09.093958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06802","last_updated":"2021-04-14T12:06:03Z","snapshot_observed_at":"2026-08-16T18:31:40.583969Z","submitted_at":"2021-04-14T12:06:03Z","title":"X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.06802","snapshot_observed_at":"2026-08-07T05:18:38.533074Z","title":"u rst , author J. A. \\ Garc \\' a , author N. Shakura , author P. A. \\ Becker , author M. T. \\ Wolff , author K. Pottschmidt , author L. H \\","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.08369","last_updated":"2025-09-08T08:13:57Z","snapshot_observed_at":"2026-08-16T12:54:34.097163Z","submitted_at":"2025-06-10T02:28:03Z","title":"Physics of Strong Magnetism with eXTP","version":2},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-07T05:18:38.533074Z"},"links":{"cited_paper":"/paper/2104.06802","citing_paper":"/paper/2506.08369"},"observation_digest":"sha256:c4fd904a9366493d3d1b272643d0be87f2b61b40aa9f992c328d7a7fea964f36","observation_id":"f257ee41-0103-4292-bb1e-37c1460f3845","resolution":{"observed_at":"2026-08-07T05:18:38.533074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06802","last_updated":"2021-04-14T12:06:03Z","snapshot_observed_at":"2026-08-16T18:31:40.583969Z","submitted_at":"2021-04-14T12:06:03Z","title":"X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum","version":1},"cited_work":{"arxiv_id":"2104.06802","doi":null,"metadata_source":"pith","pith_arxiv_id":"2104.06802","snapshot_observed_at":"2026-07-13T14:39:39.616184Z","title":"X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum","venue":"astro-ph.HE","work_id":"a7b9c14f-c15d-4c97-baf4-bbbc3642eb1e","year":2021},"citing_paper":{"arxiv_id":"2604.01219","last_updated":"2026-04-01T17:57:47Z","snapshot_observed_at":"2026-08-16T22:16:24.867850Z","submitted_at":"2026-04-01T17:57:47Z","title":"Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-13T14:30:13.573690Z"},"links":{"cited_paper":"/paper/2104.06802","citing_paper":"/paper/2604.01219"},"observation_digest":"sha256:19689570a280f15db03421a638d84755eda66bd0ba48794315f2279fed473afc","observation_id":"e40f2caf-7aee-4156-85b4-8792d85776fc","resolution":{"observed_at":"2026-07-13T14:39:39.617987Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06802","last_updated":"2021-04-14T12:06:03Z","snapshot_observed_at":"2026-08-16T18:31:40.583969Z","submitted_at":"2021-04-14T12:06:03Z","title":"X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.06802","snapshot_observed_at":"2026-07-14T12:29:39.967082Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10342","last_updated":"2026-07-11T15:04:08Z","snapshot_observed_at":"2026-08-19T10:12:03.614947Z","submitted_at":"2026-07-11T15:04:08Z","title":"Magnetospheric flows in X-ray pulsars II: Heating, cooling and ionization degree at sub-critical accretion","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-07-14T12:29:39.967082Z"},"links":{"cited_paper":"/paper/2104.06802","citing_paper":"/paper/2607.10342"},"observation_digest":"sha256:8a4c76ced3b9b727826ae0e87430dd85861edae7e4803f0361ece833fb1d0959","observation_id":"ceb70be5-c232-427b-a263-1b548c34378f","resolution":{"observed_at":"2026-07-14T12:29:39.967082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06802","last_updated":"2021-04-14T12:06:03Z","snapshot_observed_at":"2026-08-16T18:31:40.583969Z","submitted_at":"2021-04-14T12:06:03Z","title":"X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.06802","snapshot_observed_at":"2026-08-12T18:32:11.220584Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10733","last_updated":"2026-08-11T09:53:11Z","snapshot_observed_at":"2026-08-17T16:52:17.428952Z","submitted_at":"2026-08-11T09:53:11Z","title":"Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required?","version":1},"reference_index":128,"source":"arxiv_source","source_observed_at":"2026-08-12T18:32:11.220584Z"},"links":{"cited_paper":"/paper/2104.06802","citing_paper":"/paper/2608.10733"},"observation_digest":"sha256:f368adbe39b73281e67d7147d4d429950e4289dfd4e8fb194d40ba0a13bbee80","observation_id":"fd6b26c4-0733-4660-9c88-456453106a38","resolution":{"observed_at":"2026-08-12T18:32:11.220584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06802","last_updated":"2021-04-14T12:06:03Z","snapshot_observed_at":"2026-08-16T18:31:40.583969Z","submitted_at":"2021-04-14T12:06:03Z","title":"X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.06802","snapshot_observed_at":"2026-08-14T15:20:03.151930Z","title":"doi:10.1051/0004-6361/202040228 , archiveprefix =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13259","last_updated":"2026-08-13T13:58:49Z","snapshot_observed_at":"2026-08-19T15:50:52.342289Z","submitted_at":"2026-08-13T13:58:49Z","title":"The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs","version":1},"reference_index":249,"source":"arxiv_source","source_observed_at":"2026-08-14T15:20:03.151930Z"},"links":{"cited_paper":"/paper/2104.06802","citing_paper":"/paper/2608.13259"},"observation_digest":"sha256:bd51e96d8826d17e81f467576226571c006487168039b922610564b59b9d0b7d","observation_id":"85b3ca2f-e27f-4cfb-8a3e-401c662048fe","resolution":{"observed_at":"2026-08-14T15:20:03.151930Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2104.06802/citation-record","integrity":"/paper/2104.06802/integrity","json":"/paper/2104.06802/citation-record.json","paper":"/paper/2104.06802"},"outbound":[],"paper":{"arxiv_id":"2104.06802","last_updated":"2021-04-14T12:06:03Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-16T18:31:40.583969Z","submitted_at":"2021-04-14T12:06:03Z","title":"X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum"},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2104.06802."}