{"as_of":"2026-08-05T09:29:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a4a1f5ff2dec982f2b35ec7cc80d3bc0afd7c0562010e7a912dbd828d614883c","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":"2026-08-05T06:32:48.257954+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":"2026-07-12T09:44:28.146054Z","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":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":54,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1707.06651","last_updated":"2017-08-16T21:24:37Z","snapshot_observed_at":"2026-07-06T05:52:02.469903Z","submitted_at":"2017-07-20T18:00:01Z","title":"The NuSTAR Serendipitous Survey: Hunting for The Most Extreme Obscured AGN at >10 keV","version":2},"cited_work":{"arxiv_id":"1707.06651","doi":"10.3847/1538-4357/aa8176","metadata_source":"pith","pith_arxiv_id":"1707.06651","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The NuSTAR Serendipitous Survey: Hunting for The Most Extreme Obscured AGN at >10 keV","venue":"astro-ph.HE","work_id":"0e6ce2b3-a8c9-4c3a-b172-acb44dc94e07","year":2017},"citing_paper":{"arxiv_id":"2605.17547","last_updated":"2026-05-17T17:01:24Z","snapshot_observed_at":"2026-07-06T23:28:30.942078Z","submitted_at":"2026-05-17T17:01:24Z","title":"Population synthesis of active galactic nuclei based on the radiation-regulated unification model","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1707.06651","citing_paper":"/paper/2605.17547"},"observation_digest":"sha256:0e365a6fad40aa0c99c12c2966c2067495f93e567339aa025e94391f673fc6c3","observation_id":"4a12128e-bb7d-47b4-acd1-525ed68ec0b4","resolution":{"observed_at":"2026-05-19T22:42:49.870515Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-05-23T09:53:24.288866+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-23T09:53:24.288866+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.06651","last_updated":"2017-08-16T21:24:37Z","snapshot_observed_at":"2026-07-06T05:52:02.469903Z","submitted_at":"2017-07-20T18:00:01Z","title":"The NuSTAR Serendipitous Survey: Hunting for The Most Extreme Obscured AGN at >10 keV","version":2},"cited_work":{"arxiv_id":"1707.06651","doi":"10.3847/1538-4357/aa8176","metadata_source":"pith","pith_arxiv_id":"1707.06651","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The NuSTAR Serendipitous Survey: Hunting for The Most Extreme Obscured AGN at >10 keV","venue":"astro-ph.HE","work_id":"0e6ce2b3-a8c9-4c3a-b172-acb44dc94e07","year":2017},"citing_paper":{"arxiv_id":"2607.00105","last_updated":"2026-07-06T13:25:42Z","snapshot_observed_at":"2026-08-03T02:31:07.455316Z","submitted_at":"2026-06-30T19:45:20Z","title":"AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN","version":1},"reference_index":170,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1707.06651","citing_paper":"/paper/2607.00105"},"observation_digest":"sha256:e7e6d2588636dab86b9c92d87981d01bc0083fafeaaab0f62c593bf43a1b4c1d","observation_id":"3aeeefb4-70de-4551-b72f-4c61be163a51","resolution":{"observed_at":"2026-07-02T18:17:16.785512Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-05-23T09:53:24.288866+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-23T09:53:24.288866+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.06651","last_updated":"2017-08-16T21:24:37Z","snapshot_observed_at":"2026-07-06T05:52:02.469903Z","submitted_at":"2017-07-20T18:00:01Z","title":"The NuSTAR Serendipitous Survey: Hunting for The Most Extreme Obscured AGN at >10 keV","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.06651","snapshot_observed_at":"2026-07-12T09:44:28.146054Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.00105","last_updated":"2026-07-06T13:25:42Z","snapshot_observed_at":"2026-08-03T02:31:07.455316Z","submitted_at":"2026-06-30T19:45:20Z","title":"AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN","version":2},"reference_index":172,"source":"arxiv_source","source_observed_at":"2026-07-12T09:44:28.146054Z"},"links":{"cited_paper":"/paper/1707.06651","citing_paper":"/paper/2607.00105"},"observation_digest":"sha256:74f86b41974b29295208954fa69dcac359b5b4f58e79fd5392797a9e0907aff7","observation_id":"abce832f-c7ab-4392-ab1c-2b72b03557f4","resolution":{"observed_at":"2026-07-12T09:44:28.146054Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1707.06651/citation-record","integrity":"/paper/1707.06651/integrity","json":"/paper/1707.06651/citation-record.json","paper":"/paper/1707.06651"},"outbound":[],"paper":{"arxiv_id":"1707.06651","last_updated":"2017-08-16T21:24:37Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T05:52:02.469903Z","submitted_at":"2017-07-20T18:00:01Z","title":"The NuSTAR Serendipitous Survey: Hunting for The Most Extreme Obscured AGN at >10 keV"},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1707.06651."}