{"as_of":"2026-08-08T16:07:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9b967c9cf57324fc75340b3ce11c681072c10b8a85bb00a7e05ac7bcfad5bd09","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T15:29:36.638624Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-19T18:32:43.167666Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2007.11374","last_updated":"2021-10-07T11:18:33Z","snapshot_observed_at":"2026-07-06T09:40:54.552055Z","submitted_at":"2020-07-22T12:37:34Z","title":"Omicron: a tool to characterize transient noise in gravitational-wave detectors","version":2},"cited_work":{"arxiv_id":"2007.11374","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2007.11374","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Robinet, N","venue":null,"work_id":"12827a97-9826-4fb0-a3aa-c85be9d37d39","year":2007},"citing_paper":{"arxiv_id":"2010.14527","last_updated":"2021-03-08T18:36:29Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-10-27T18:01:31Z","title":"GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","version":3},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-05-13T13:21:02.413921Z"},"links":{"cited_paper":"/paper/2007.11374","citing_paper":"/paper/2010.14527"},"observation_digest":"sha256:b9a04be1bd001e0910c264b112965f31067c5d9cdfbe207049f61008ed6d4137","observation_id":"8fadde5f-08ab-4888-a40c-c47bb5decf8e","resolution":{"observed_at":"2026-05-13T13:21:02.922036Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.11374","last_updated":"2021-10-07T11:18:33Z","snapshot_observed_at":"2026-07-06T09:40:54.552055Z","submitted_at":"2020-07-22T12:37:34Z","title":"Omicron: a tool to characterize transient noise in gravitational-wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.11374","snapshot_observed_at":"2026-08-07T15:29:36.638624Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.14949","last_updated":"2025-08-21T21:47:06Z","snapshot_observed_at":"2026-08-08T05:24:49.942316Z","submitted_at":"2025-05-20T22:21:38Z","title":"PINCH: Pipeline-Informed Noise Characterization in LIGO's Third Observing Run","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T15:29:36.638624Z"},"links":{"cited_paper":"/paper/2007.11374","citing_paper":"/paper/2505.14949"},"observation_digest":"sha256:c968a3b2dcc30ca0eca4e09a8c763ed3b5854ccac6ce756976a014cd9eb78aac","observation_id":"82510233-bebb-4bd0-9630-78fdb4f16998","resolution":{"observed_at":"2026-08-07T15:29:36.638624Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.11374","last_updated":"2021-10-07T11:18:33Z","snapshot_observed_at":"2026-07-06T09:40:54.552055Z","submitted_at":"2020-07-22T12:37:34Z","title":"Omicron: a tool to characterize transient noise in gravitational-wave detectors","version":2},"cited_work":{"arxiv_id":"2007.11374","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2007.11374","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Robinet, N","venue":null,"work_id":"12827a97-9826-4fb0-a3aa-c85be9d37d39","year":2007},"citing_paper":{"arxiv_id":"2508.13923","last_updated":"2026-04-22T13:01:30Z","snapshot_observed_at":"2026-07-06T22:15:03.520865Z","submitted_at":"2025-08-19T15:18:02Z","title":"Hunting for new glitches in LIGO data using community science","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-18T22:27:23.190259Z"},"links":{"cited_paper":"/paper/2007.11374","citing_paper":"/paper/2508.13923"},"observation_digest":"sha256:369f74f9b74bce1af8783ef9e1378d04e6ce1901a7d933d47946954dd1ad713f","observation_id":"d00db1d3-ad89-4b78-a27c-895bd6eb3f93","resolution":{"observed_at":"2026-05-18T22:31:52.987368Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.11374","last_updated":"2021-10-07T11:18:33Z","snapshot_observed_at":"2026-07-06T09:40:54.552055Z","submitted_at":"2020-07-22T12:37:34Z","title":"Omicron: a tool to characterize transient noise in gravitational-wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.11374","snapshot_observed_at":"2026-08-03T18:39:18.943544Z","title":"Robinet, N","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2512.04516","last_updated":"2026-07-07T13:12:33Z","snapshot_observed_at":"2026-08-06T20:33:38.679286Z","submitted_at":"2025-12-04T06:56:47Z","title":"Searching for binary black hole mergers with deep learning in Advanced LIGO's third observing run","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-03T18:39:18.943544Z"},"links":{"cited_paper":"/paper/2007.11374","citing_paper":"/paper/2512.04516"},"observation_digest":"sha256:3a7170bf51ef2b1bcb350bcd4d091bc6955be5061f9822de506f8e31b910228f","observation_id":"a3b927b2-1f8c-4a5b-8e38-196ff2cf4a00","resolution":{"observed_at":"2026-08-03T18:39:18.943544Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.11374","last_updated":"2021-10-07T11:18:33Z","snapshot_observed_at":"2026-07-06T09:40:54.552055Z","submitted_at":"2020-07-22T12:37:34Z","title":"Omicron: a tool to characterize transient noise in gravitational-wave detectors","version":2},"cited_work":{"arxiv_id":"2007.11374","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2007.11374","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Robinet, N","venue":null,"work_id":"12827a97-9826-4fb0-a3aa-c85be9d37d39","year":2007},"citing_paper":{"arxiv_id":"2603.06010","last_updated":"2026-04-10T18:03:54Z","snapshot_observed_at":"2026-07-06T22:48:04.438669Z","submitted_at":"2026-03-06T08:07:11Z","title":"Accelerated Time-domain Analysis for Gravitational Wave Astronomy","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-15T15:44:03.750959Z"},"links":{"cited_paper":"/paper/2007.11374","citing_paper":"/paper/2603.06010"},"observation_digest":"sha256:16f015a54492f1a9f02d1dd8c46adfbe0af89c4f29ef60054e8d79c11ff911b3","observation_id":"b3917d21-fd92-48ae-942d-359e65aef0fa","resolution":{"observed_at":"2026-05-15T15:46:12.442539Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.11374","last_updated":"2021-10-07T11:18:33Z","snapshot_observed_at":"2026-07-06T09:40:54.552055Z","submitted_at":"2020-07-22T12:37:34Z","title":"Omicron: a tool to characterize transient noise in gravitational-wave detectors","version":2},"cited_work":{"arxiv_id":"2007.11374","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2007.11374","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Robinet, N","venue":null,"work_id":"12827a97-9826-4fb0-a3aa-c85be9d37d39","year":2007},"citing_paper":{"arxiv_id":"2604.13687","last_updated":"2026-04-15T10:09:24Z","snapshot_observed_at":"2026-07-06T23:01:37.207817Z","submitted_at":"2026-04-15T10:09:24Z","title":"VIGILant: an automatic classification pipeline for glitches in the Virgo detector","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-10T12:41:50.796918Z"},"links":{"cited_paper":"/paper/2007.11374","citing_paper":"/paper/2604.13687"},"observation_digest":"sha256:c6ae6a11a6b3ba678ba97bb334638a5b670a2fdfcf183cde13bc6fd031d30266","observation_id":"ac698b1f-f683-42e0-9d48-953f36d8dbac","resolution":{"observed_at":"2026-05-11T11:41:06.277777Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.11374","last_updated":"2021-10-07T11:18:33Z","snapshot_observed_at":"2026-07-06T09:40:54.552055Z","submitted_at":"2020-07-22T12:37:34Z","title":"Omicron: a tool to characterize transient noise in gravitational-wave detectors","version":2},"cited_work":{"arxiv_id":"2007.11374","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2007.11374","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Robinet, N","venue":null,"work_id":"12827a97-9826-4fb0-a3aa-c85be9d37d39","year":2007},"citing_paper":{"arxiv_id":"2605.11703","last_updated":"2026-05-12T07:58:35Z","snapshot_observed_at":"2026-08-05T16:46:12.594370Z","submitted_at":"2026-05-12T07:58:35Z","title":"GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors","version":1},"reference_index":151,"source":"pdf_text","source_observed_at":"2026-05-13T05:27:45.004977Z"},"links":{"cited_paper":"/paper/2007.11374","citing_paper":"/paper/2605.11703"},"observation_digest":"sha256:811555bb37d5c5f671df448c210c4e4240c1caee0a3adf3c6f8aa153b473c08b","observation_id":"3a1e55aa-929d-4e45-9e43-8ea410085a2e","resolution":{"observed_at":"2026-05-13T05:32:19.952619Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.11374","last_updated":"2021-10-07T11:18:33Z","snapshot_observed_at":"2026-07-06T09:40:54.552055Z","submitted_at":"2020-07-22T12:37:34Z","title":"Omicron: a tool to characterize transient noise in gravitational-wave detectors","version":2},"cited_work":{"arxiv_id":"2007.11374","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2007.11374","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Robinet, N","venue":null,"work_id":"12827a97-9826-4fb0-a3aa-c85be9d37d39","year":2007},"citing_paper":{"arxiv_id":"2605.14143","last_updated":"2026-05-13T21:49:46Z","snapshot_observed_at":"2026-08-02T08:14:50.752438Z","submitted_at":"2026-05-13T21:49:46Z","title":"Scattered light noise at LIGO Livingston Observatory during O4","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-15T01:54:05.816784Z"},"links":{"cited_paper":"/paper/2007.11374","citing_paper":"/paper/2605.14143"},"observation_digest":"sha256:1dd730ac6ce2ca9f05324e95cc16f9f05e23da88c08bcaf3671d8c9f413545fd","observation_id":"1862854f-96cc-4a26-b49e-af80cda0ec6e","resolution":{"observed_at":"2026-05-15T01:58:29.316706Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.11374","last_updated":"2021-10-07T11:18:33Z","snapshot_observed_at":"2026-07-06T09:40:54.552055Z","submitted_at":"2020-07-22T12:37:34Z","title":"Omicron: a tool to characterize transient noise in gravitational-wave detectors","version":2},"cited_work":{"arxiv_id":"2007.11374","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2007.11374","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Robinet, N","venue":null,"work_id":"12827a97-9826-4fb0-a3aa-c85be9d37d39","year":2007},"citing_paper":{"arxiv_id":"2605.16183","last_updated":"2026-05-15T17:03:40Z","snapshot_observed_at":"2026-07-06T23:27:24.957966Z","submitted_at":"2026-05-15T17:03:40Z","title":"Rapid data quality investigations of gravitational-wave events with the Data Quality Report Builder toolkit","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-05-19T18:28:05.480261Z"},"links":{"cited_paper":"/paper/2007.11374","citing_paper":"/paper/2605.16183"},"observation_digest":"sha256:198bc3851bc45ee8526c73cccf6bbe9b52a2ab3848c68dc255902a1f393e248d","observation_id":"902fb9ff-4220-4c6d-9348-611920290e9c","resolution":{"observed_at":"2026-05-19T18:32:43.169375Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2007.11374/citation-record","integrity":"/paper/2007.11374/integrity","json":"/paper/2007.11374/citation-record.json","paper":"/paper/2007.11374"},"outbound":[],"paper":{"arxiv_id":"2007.11374","last_updated":"2021-10-07T11:18:33Z","latest_version":2,"primary_category":"astro-ph.IM","snapshot_observed_at":"2026-07-06T09:40:54.552055Z","submitted_at":"2020-07-22T12:37:34Z","title":"Omicron: a tool to characterize transient noise in gravitational-wave detectors"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2007.11374."}