{"as_of":"2026-08-19T14:23:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:82d37fdce8e1a74cf852fae2a266890bb58d93ca898dc86883b84c9065f0ff3e","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T14:49:10.231493Z","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":"2026-07-03T08:07:44.569482Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"0811.4278","last_updated":"2008-11-26T11:47:30Z","snapshot_observed_at":"2026-08-19T05:31:38.100482Z","submitted_at":"2008-11-26T11:47:30Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","version":1},"cited_work":{"arxiv_id":"0811.4278","doi":null,"metadata_source":"pith","pith_arxiv_id":"0811.4278","snapshot_observed_at":"2026-07-03T08:07:44.569482Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","venue":"astro-ph","work_id":"236dbd93-16d9-4590-8713-5b93e845ada3","year":2008},"citing_paper":{"arxiv_id":"2605.12602","last_updated":"2026-05-12T18:00:05Z","snapshot_observed_at":"2026-08-10T21:09:43.200797Z","submitted_at":"2026-05-12T18:00:05Z","title":"Tracking down the broadband polarimetric properties of PG 1553+113","version":1},"reference_index":121,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0811.4278","citing_paper":"/paper/2605.12602"},"observation_digest":"sha256:daaee602fde264f8e0108e26b5f9b059f3143622d2f6c0f0881a2b46f5774c26","observation_id":"d307b8a0-5153-474b-aa49-404b5fb71355","resolution":{"observed_at":"2026-05-14T20:32:55.633466Z","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":"0811.4278","last_updated":"2008-11-26T11:47:30Z","snapshot_observed_at":"2026-08-19T05:31:38.100482Z","submitted_at":"2008-11-26T11:47:30Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","version":1},"cited_work":{"arxiv_id":"0811.4278","doi":null,"metadata_source":"pith","pith_arxiv_id":"0811.4278","snapshot_observed_at":"2026-07-03T08:07:44.569482Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","venue":"astro-ph","work_id":"236dbd93-16d9-4590-8713-5b93e845ada3","year":2008},"citing_paper":{"arxiv_id":"2605.15867","last_updated":"2026-05-15T11:34:48Z","snapshot_observed_at":"2026-08-14T00:04:29.084755Z","submitted_at":"2026-05-15T11:34:48Z","title":"Spectral-Regime Overlap and Transition-like Behavior in the Blazar Population from Multi-Instrument X-ray and TeV Observations","version":1},"reference_index":177,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0811.4278","citing_paper":"/paper/2605.15867"},"observation_digest":"sha256:d80a28334a1a341dc0e98f45e2fb61bb4e165ec6700caaa4152a1c8e0d35000b","observation_id":"50d51737-0bb5-43fe-9a86-a6dcfbd7f735","resolution":{"observed_at":"2026-05-20T18:58:53.477539Z","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":"0811.4278","last_updated":"2008-11-26T11:47:30Z","snapshot_observed_at":"2026-08-19T05:31:38.100482Z","submitted_at":"2008-11-26T11:47:30Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","version":1},"cited_work":{"arxiv_id":"0811.4278","doi":null,"metadata_source":"pith","pith_arxiv_id":"0811.4278","snapshot_observed_at":"2026-07-03T08:07:44.569482Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","venue":"astro-ph","work_id":"236dbd93-16d9-4590-8713-5b93e845ada3","year":2008},"citing_paper":{"arxiv_id":"2606.27435","last_updated":"2026-06-25T18:00:12Z","snapshot_observed_at":"2026-08-15T06:59:29.797082Z","submitted_at":"2026-06-25T18:00:12Z","title":"Parsec-scale polarimetry and kinematics of a spine-sheath jet in the neutrino-blazar TXS 0506+056","version":1},"reference_index":293,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0811.4278","citing_paper":"/paper/2606.27435"},"observation_digest":"sha256:0b813e1bfaba7e9fce60420ff7c70d4f4a700b2c117ee08ac8de1b337bc395ce","observation_id":"69f4551b-6df8-42fa-a700-69684eac43fc","resolution":{"observed_at":"2026-06-29T02:03:00.025466Z","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":"0811.4278","last_updated":"2008-11-26T11:47:30Z","snapshot_observed_at":"2026-08-19T05:31:38.100482Z","submitted_at":"2008-11-26T11:47:30Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","version":1},"cited_work":{"arxiv_id":"0811.4278","doi":null,"metadata_source":"pith","pith_arxiv_id":"0811.4278","snapshot_observed_at":"2026-07-03T08:07:44.569482Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","venue":"astro-ph","work_id":"236dbd93-16d9-4590-8713-5b93e845ada3","year":2008},"citing_paper":{"arxiv_id":"2606.31510","last_updated":"2026-06-30T11:24:59Z","snapshot_observed_at":"2026-08-08T21:47:08.232047Z","submitted_at":"2026-06-30T11:24:59Z","title":"Magnetic field and plasma number density from radio and millimeter core measurements in AGN jets","version":1},"reference_index":120,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0811.4278","citing_paper":"/paper/2606.31510"},"observation_digest":"sha256:075d6f8a6e9b44c851fed7a66229b896c20dcd69098a0aa4aa01cce11cbb3bd3","observation_id":"a442d89d-1ee8-46e2-ae54-fbf02fe8f286","resolution":{"observed_at":"2026-07-01T04:35:20.658989Z","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":"0811.4278","last_updated":"2008-11-26T11:47:30Z","snapshot_observed_at":"2026-08-19T05:31:38.100482Z","submitted_at":"2008-11-26T11:47:30Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","version":1},"cited_work":{"arxiv_id":"0811.4278","doi":null,"metadata_source":"pith","pith_arxiv_id":"0811.4278","snapshot_observed_at":"2026-07-03T08:07:44.569482Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","venue":"astro-ph","work_id":"236dbd93-16d9-4590-8713-5b93e845ada3","year":2008},"citing_paper":{"arxiv_id":"2607.01820","last_updated":"2026-07-02T07:33:43Z","snapshot_observed_at":"2026-08-13T01:39:46.815865Z","submitted_at":"2026-07-02T07:33:43Z","title":"Polarization Architecture of Steady GRMHD Jets from the Horizon to Infinity","version":1},"reference_index":108,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0811.4278","citing_paper":"/paper/2607.01820"},"observation_digest":"sha256:95b5f7a195f65495056fa050a42e9a7be6d88a8bdc24ed77aac7dc23ed0b6fcc","observation_id":"f4a80a6b-8c2e-4bc6-8aaa-f868849ac53b","resolution":{"observed_at":"2026-07-03T08:07:44.571064Z","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":"0811.4278","last_updated":"2008-11-26T11:47:30Z","snapshot_observed_at":"2026-08-19T05:31:38.100482Z","submitted_at":"2008-11-26T11:47:30Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.4278","snapshot_observed_at":"2026-08-06T00:40:22.836208Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.00996","last_updated":"2026-08-02T04:46:19Z","snapshot_observed_at":"2026-08-12T15:34:12.244862Z","submitted_at":"2026-08-02T04:46:19Z","title":"Radio-Gamma-Ray Properties and High-Energy Implications for Fermi Blazars","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-06T00:40:22.836208Z"},"links":{"cited_paper":"/paper/0811.4278","citing_paper":"/paper/2608.00996"},"observation_digest":"sha256:9d76fa9dbfe0cde02594eaac63b359a6b16a5f14faf8d64688386b9b6f7faac8","observation_id":"71106612-fa23-4a78-9225-cfc872dab8ff","resolution":{"observed_at":"2026-08-06T00:40:22.836208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.4278","last_updated":"2008-11-26T11:47:30Z","snapshot_observed_at":"2026-08-19T05:31:38.100482Z","submitted_at":"2008-11-26T11:47:30Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.4278","snapshot_observed_at":"2026-08-05T05:21:45.818525Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.03947","last_updated":"2026-08-04T17:12:22Z","snapshot_observed_at":"2026-08-08T22:44:34.977103Z","submitted_at":"2026-08-04T17:12:22Z","title":"Profile Analysis of the Multiwavelength 2.1-year Oscillations of PG 1553+113","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-05T05:21:45.818525Z"},"links":{"cited_paper":"/paper/0811.4278","citing_paper":"/paper/2608.03947"},"observation_digest":"sha256:7aa6f13aa4657321ff985a91af689c982eac883f3df7a76271d2836396749a62","observation_id":"1ffd0c57-2ed0-4bbe-9b81-d6e01872dac2","resolution":{"observed_at":"2026-08-05T05:21:45.818525Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.4278","last_updated":"2008-11-26T11:47:30Z","snapshot_observed_at":"2026-08-19T05:31:38.100482Z","submitted_at":"2008-11-26T11:47:30Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.4278","snapshot_observed_at":"2026-08-15T14:49:10.231493Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.04078","last_updated":"2026-08-04T18:00:00Z","snapshot_observed_at":"2026-08-18T07:27:47.930263Z","submitted_at":"2026-08-04T18:00:00Z","title":"The most extreme high-z radio quasars in the eRASS:1 X-ray survey","version":1},"reference_index":189,"source":"arxiv_source","source_observed_at":"2026-08-15T14:49:10.231493Z"},"links":{"cited_paper":"/paper/0811.4278","citing_paper":"/paper/2608.04078"},"observation_digest":"sha256:190a7d6c71973e5136e95f6ae767502a3766fef6ff166b6ef7ec2701cd8924c8","observation_id":"8c0bd358-4cdb-4345-bb57-3978ccd556dc","resolution":{"observed_at":"2026-08-15T14:49:10.231493Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/0811.4278/citation-record","integrity":"/paper/0811.4278/integrity","json":"/paper/0811.4278/citation-record.json","paper":"/paper/0811.4278"},"outbound":[],"paper":{"arxiv_id":"0811.4278","last_updated":"2008-11-26T11:47:30Z","latest_version":1,"primary_category":"astro-ph","snapshot_observed_at":"2026-08-19T05:31:38.100482Z","submitted_at":"2008-11-26T11:47:30Z","title":"Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies"},"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 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:0811.4278."}