{"as_of":"2026-08-11T22:06:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fce5e35ae68b68635fb23a57742bba9cbe86a21f52c82038b8b7eaf1e547f424","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T14:21:59.678646Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1802.03440","last_updated":"2018-03-07T17:36:38Z","snapshot_observed_at":"2026-08-11T14:48:41.533467Z","submitted_at":"2018-02-09T20:19:47Z","title":"Constraining Stellar Coronal Mass Ejections Through Multi-Wavelength Analysis of the Active M Dwarf EQ Peg","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.03440","snapshot_observed_at":"2026-08-07T14:21:59.678646Z","title":"856(1):39","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.19228","last_updated":"2025-05-25T16:44:19Z","snapshot_observed_at":"2026-08-08T23:47:36.891151Z","submitted_at":"2025-05-25T16:44:19Z","title":"Coronal dimmings and what they tell us about solar and stellar coronal mass ejections","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-07T14:21:59.678646Z"},"links":{"cited_paper":"/paper/1802.03440","citing_paper":"/paper/2505.19228"},"observation_digest":"sha256:9d38a1646276f4d4a0f69f5d596f167ca5dc9b8ea7d9fd2dc63b9fcd7bdb17ef","observation_id":"262e9d4d-a348-4994-bb14-ffe025370fb6","resolution":{"observed_at":"2026-08-07T14:21:59.678646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.03440","last_updated":"2018-03-07T17:36:38Z","snapshot_observed_at":"2026-08-11T14:48:41.533467Z","submitted_at":"2018-02-09T20:19:47Z","title":"Constraining Stellar Coronal Mass Ejections Through Multi-Wavelength Analysis of the Active M Dwarf EQ Peg","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.03440","snapshot_observed_at":"2026-08-01T05:14:30.223335Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.22321","last_updated":"2026-07-24T13:59:34Z","snapshot_observed_at":"2026-08-07T03:33:43.264989Z","submitted_at":"2026-07-24T13:59:34Z","title":"Discovery of a radio-flaring M dwarf in a commensal transient search of the LADUMA field","version":1},"reference_index":168,"source":"arxiv_source","source_observed_at":"2026-08-01T05:14:30.223335Z"},"links":{"cited_paper":"/paper/1802.03440","citing_paper":"/paper/2607.22321"},"observation_digest":"sha256:b2b43fa5b5f22afe0846de5208fe565936fadc5baa72588f13416dd775bbd2a3","observation_id":"45c34d18-d8f0-4fc2-a020-82ed4329d018","resolution":{"observed_at":"2026-08-01T05:14:30.223335Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.03440","last_updated":"2018-03-07T17:36:38Z","snapshot_observed_at":"2026-08-11T14:48:41.533467Z","submitted_at":"2018-02-09T20:19:47Z","title":"Constraining Stellar Coronal Mass Ejections Through Multi-Wavelength Analysis of the Active M Dwarf EQ Peg","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.03440","snapshot_observed_at":"2026-08-01T06:15:38.729594Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.27531","last_updated":"2026-07-31T19:23:20Z","snapshot_observed_at":"2026-08-06T23:11:28.451108Z","submitted_at":"2026-07-29T23:49:51Z","title":"Stellar impact on exoplanetary atmospheric evolution and habitability","version":1},"reference_index":142,"source":"arxiv_source","source_observed_at":"2026-08-01T06:15:38.729594Z"},"links":{"cited_paper":"/paper/1802.03440","citing_paper":"/paper/2607.27531"},"observation_digest":"sha256:e3610ac15121a3e84696677d383482e8459ee36514d1ce78a22677f2f01e3974","observation_id":"29b7a052-3758-4c39-b568-f8074044711c","resolution":{"observed_at":"2026-08-01T06:15:38.729594Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.03440","last_updated":"2018-03-07T17:36:38Z","snapshot_observed_at":"2026-08-11T14:48:41.533467Z","submitted_at":"2018-02-09T20:19:47Z","title":"Constraining Stellar Coronal Mass Ejections Through Multi-Wavelength Analysis of the Active M Dwarf EQ Peg","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.03440","snapshot_observed_at":"2026-08-04T01:30:19.292503Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.27531","last_updated":"2026-07-31T19:23:20Z","snapshot_observed_at":"2026-08-06T23:11:28.451108Z","submitted_at":"2026-07-29T23:49:51Z","title":"Stellar impact on exoplanetary atmospheric evolution and habitability","version":2},"reference_index":142,"source":"arxiv_source","source_observed_at":"2026-08-04T01:30:19.292503Z"},"links":{"cited_paper":"/paper/1802.03440","citing_paper":"/paper/2607.27531"},"observation_digest":"sha256:a70276995a2f18641770e0b97ab58a88f9c483ab876e481e437854693adc9035","observation_id":"bc862a30-b9d4-4df0-a26f-15e96eca410e","resolution":{"observed_at":"2026-08-04T01:30:19.292503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.03440","last_updated":"2018-03-07T17:36:38Z","snapshot_observed_at":"2026-08-11T14:48:41.533467Z","submitted_at":"2018-02-09T20:19:47Z","title":"Constraining Stellar Coronal Mass Ejections Through Multi-Wavelength Analysis of the Active M Dwarf EQ Peg","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.03440","snapshot_observed_at":"2026-08-05T00:36:51.209630Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.00683","last_updated":"2026-08-01T14:08:52Z","snapshot_observed_at":"2026-08-09T11:55:51.902239Z","submitted_at":"2026-08-01T14:08:52Z","title":"ESCAPE: a small explorer mission to study the stellar drivers of exoplanet evolution","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-05T00:36:51.209630Z"},"links":{"cited_paper":"/paper/1802.03440","citing_paper":"/paper/2608.00683"},"observation_digest":"sha256:a01f4ea5e3e6297395143dbe2e08493d2fa1565f5dc0b05812a5214b0fe04e2a","observation_id":"24bf2137-354d-4a4d-8884-b0ea7f08f3fd","resolution":{"observed_at":"2026-08-05T00:36:51.209630Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1802.03440/citation-record","integrity":"/paper/1802.03440/integrity","json":"/paper/1802.03440/citation-record.json","paper":"/paper/1802.03440"},"outbound":[],"paper":{"arxiv_id":"1802.03440","last_updated":"2018-03-07T17:36:38Z","latest_version":2,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-11T14:48:41.533467Z","submitted_at":"2018-02-09T20:19:47Z","title":"Constraining Stellar Coronal Mass Ejections Through Multi-Wavelength Analysis of the Active M Dwarf EQ Peg"},"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 5 inbound Pith citation observations for arXiv:1802.03440."}