{"as_of":"2026-08-10T03:40:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:80058c0ca733a00b79a774300ec53f5c25eb42b508b40891f504cd66f55cbd26","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":"2026-08-09T06:31:02.800959+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":"2026-08-07T22:32:29.053915Z","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":"2026-07-03T21:38:59.096469Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2204.11864","last_updated":"2022-04-25T18:00:01Z","snapshot_observed_at":"2026-08-09T15:16:06.185446Z","submitted_at":"2022-04-25T18:00:01Z","title":"Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.11864","snapshot_observed_at":"2026-08-07T06:05:52.813141Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.06171","last_updated":"2025-07-05T12:08:41Z","snapshot_observed_at":"2026-08-09T10:49:40.401534Z","submitted_at":"2025-06-06T15:34:00Z","title":"Primordial Black Holes and the First Stars","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T06:05:52.813141Z"},"links":{"cited_paper":"/paper/2204.11864","citing_paper":"/paper/2506.06171"},"observation_digest":"sha256:01f54eaa7ae6f9cc4b04379fb857e15d98a96159b3077c800e9d136efae51b89","observation_id":"58f1d0af-dded-4a31-9158-c789eac5865c","resolution":{"observed_at":"2026-08-07T06:05:52.813141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11864","last_updated":"2022-04-25T18:00:01Z","snapshot_observed_at":"2026-08-09T15:16:06.185446Z","submitted_at":"2022-04-25T18:00:01Z","title":"Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors","version":1},"cited_work":{"arxiv_id":"2204.11864","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.11864","snapshot_observed_at":"2026-07-03T21:38:59.096469Z","title":null,"venue":null,"work_id":"63da5bf1-8180-4f03-ac6d-34614a2081cc","year":2022},"citing_paper":{"arxiv_id":"2508.09965","last_updated":"2026-05-11T14:03:52Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-08-13T17:32:14Z","title":"GW231123: A Possible Primordial Black Hole Origin","version":2},"reference_index":128,"source":"pdf_text","source_observed_at":"2026-05-18T22:52:55.899162Z"},"links":{"cited_paper":"/paper/2204.11864","citing_paper":"/paper/2508.09965"},"observation_digest":"sha256:61fcfcede8a4cce9a1595062ec0032f21dea46a9d4624aee24a5091cdde431ed","observation_id":"4a51c28a-a4af-410e-a040-e2ff776a5383","resolution":{"observed_at":"2026-05-18T22:56:53.669637Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11864","last_updated":"2022-04-25T18:00:01Z","snapshot_observed_at":"2026-08-09T15:16:06.185446Z","submitted_at":"2022-04-25T18:00:01Z","title":"Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.11864","snapshot_observed_at":"2026-08-05T20:46:11.242837Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.09966","last_updated":"2025-08-13T17:32:40Z","snapshot_observed_at":"2026-08-08T10:08:20.845476Z","submitted_at":"2025-08-13T17:32:40Z","title":"January Food Benchmark (JFB): A Public Benchmark Dataset and Evaluation Suite for Multimodal Food Analysis","version":1},"reference_index":130,"source":"pdf_text","source_observed_at":"2026-08-05T20:46:11.242837Z"},"links":{"cited_paper":"/paper/2204.11864","citing_paper":"/paper/2508.09966"},"observation_digest":"sha256:e8fe8c2a48c0b42e50fa01f5de3667e18fd8a7fe96b0b27eca58ba91ecf7c437","observation_id":"a8b678a4-5687-49f2-a330-fd63f42f2461","resolution":{"observed_at":"2026-08-05T20:46:11.242837Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11864","last_updated":"2022-04-25T18:00:01Z","snapshot_observed_at":"2026-08-09T15:16:06.185446Z","submitted_at":"2022-04-25T18:00:01Z","title":"Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors","version":1},"cited_work":{"arxiv_id":"2204.11864","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.11864","snapshot_observed_at":"2026-07-03T21:38:59.096469Z","title":null,"venue":null,"work_id":"63da5bf1-8180-4f03-ac6d-34614a2081cc","year":2022},"citing_paper":{"arxiv_id":"2510.11861","last_updated":"2026-04-28T15:44:06Z","snapshot_observed_at":"2026-07-06T22:32:32.632779Z","submitted_at":"2025-10-13T19:15:03Z","title":"Impact of facility timing and coordination for next-generation gravitational-wave detectors","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-18T07:12:23.655235Z"},"links":{"cited_paper":"/paper/2204.11864","citing_paper":"/paper/2510.11861"},"observation_digest":"sha256:b4247c3820fa2c8ab672ba08d606045465bab5d6e3b3e6c8d773cfb6a4df2eee","observation_id":"acc2c190-cc66-4500-9229-5648a6a717a4","resolution":{"observed_at":"2026-05-18T07:12:26.823502Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11864","last_updated":"2022-04-25T18:00:01Z","snapshot_observed_at":"2026-08-09T15:16:06.185446Z","submitted_at":"2022-04-25T18:00:01Z","title":"Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors","version":1},"cited_work":{"arxiv_id":"2204.11864","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.11864","snapshot_observed_at":"2026-07-03T21:38:59.096469Z","title":null,"venue":null,"work_id":"63da5bf1-8180-4f03-ac6d-34614a2081cc","year":2022},"citing_paper":{"arxiv_id":"2604.11871","last_updated":"2026-04-13T18:00:00Z","snapshot_observed_at":"2026-08-08T06:16:06.638772Z","submitted_at":"2026-04-13T18:00:00Z","title":"Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-10T15:27:10.838625Z"},"links":{"cited_paper":"/paper/2204.11864","citing_paper":"/paper/2604.11871"},"observation_digest":"sha256:1716b72964e5790908e0f12c14a7a779773ce6537c517ff469515ff53a6c8929","observation_id":"a9c87b52-7c77-4fdd-a39e-67686d89aa1d","resolution":{"observed_at":"2026-05-11T10:31:03.163680Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11864","last_updated":"2022-04-25T18:00:01Z","snapshot_observed_at":"2026-08-09T15:16:06.185446Z","submitted_at":"2022-04-25T18:00:01Z","title":"Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors","version":1},"cited_work":{"arxiv_id":"2204.11864","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.11864","snapshot_observed_at":"2026-07-03T21:38:59.096469Z","title":null,"venue":null,"work_id":"63da5bf1-8180-4f03-ac6d-34614a2081cc","year":2022},"citing_paper":{"arxiv_id":"2604.22462","last_updated":"2026-04-24T11:29:09Z","snapshot_observed_at":"2026-08-03T04:43:07.092134Z","submitted_at":"2026-04-24T11:29:09Z","title":"Machine Learning for Multi-messenger Probes of New Physics and Cosmology: A Review and Perspective","version":1},"reference_index":148,"source":"pdf_text","source_observed_at":"2026-05-08T11:02:17.987425Z"},"links":{"cited_paper":"/paper/2204.11864","citing_paper":"/paper/2604.22462"},"observation_digest":"sha256:9c475b671fcaa61ce9c8520b3e88dce1636e55446626eb3f461859f10e1bbf72","observation_id":"94c0ad1b-69d2-43a4-b104-b7de85ee19d3","resolution":{"observed_at":"2026-05-11T19:46:14.060121Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11864","last_updated":"2022-04-25T18:00:01Z","snapshot_observed_at":"2026-08-09T15:16:06.185446Z","submitted_at":"2022-04-25T18:00:01Z","title":"Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors","version":1},"cited_work":{"arxiv_id":"2204.11864","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.11864","snapshot_observed_at":"2026-07-03T21:38:59.096469Z","title":null,"venue":null,"work_id":"63da5bf1-8180-4f03-ac6d-34614a2081cc","year":2022},"citing_paper":{"arxiv_id":"2606.17617","last_updated":"2026-06-16T07:23:25Z","snapshot_observed_at":"2026-07-06T23:53:11.869569Z","submitted_at":"2026-06-16T07:23:25Z","title":"Synergy between CSST and future gravitational-wave detectors: Probing primordial black holes by cross-correlating dark sirens with galaxies","version":1},"reference_index":115,"source":"pdf_text","source_observed_at":"2026-06-27T00:15:57.187962Z"},"links":{"cited_paper":"/paper/2204.11864","citing_paper":"/paper/2606.17617"},"observation_digest":"sha256:0bb675ccdaf2b21627063c4a24365d4e322e87484d7f0ad1a548ce24c5153544","observation_id":"e5fb3b3a-261f-4b40-9716-b46b0db36270","resolution":{"observed_at":"2026-07-03T21:38:59.097933Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11864","last_updated":"2022-04-25T18:00:01Z","snapshot_observed_at":"2026-08-09T15:16:06.185446Z","submitted_at":"2022-04-25T18:00:01Z","title":"Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.11864","snapshot_observed_at":"2026-07-14T06:46:02.916338Z","title":"Constraining High-redshift Stellar-mass Primordial Black Holes with Next-generation Ground-based Gravitational-wave Detectors,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.11145","last_updated":"2026-07-13T06:33:06Z","snapshot_observed_at":"2026-08-07T14:24:43.258286Z","submitted_at":"2026-07-13T06:33:06Z","title":"Reconstruction of Primordial Power Spectrum from Gravitational Waves of High-Redshift Black Hole Binaries","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-07-14T06:46:02.916338Z"},"links":{"cited_paper":"/paper/2204.11864","citing_paper":"/paper/2607.11145"},"observation_digest":"sha256:d94afe9e12217c9fdfc4c82d82008353719087f700a812f711c3183c96e40d49","observation_id":"f974b866-82cd-4d5b-b6db-294743be77c9","resolution":{"observed_at":"2026-07-14T06:46:02.916338Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11864","last_updated":"2022-04-25T18:00:01Z","snapshot_observed_at":"2026-08-09T15:16:06.185446Z","submitted_at":"2022-04-25T18:00:01Z","title":"Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.11864","snapshot_observed_at":"2026-08-07T22:32:29.053915Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.05846","last_updated":"2026-08-06T10:19:40Z","snapshot_observed_at":"2026-08-09T23:11:42.159527Z","submitted_at":"2026-08-06T10:19:40Z","title":"Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-07T22:32:29.053915Z"},"links":{"cited_paper":"/paper/2204.11864","citing_paper":"/paper/2608.05846"},"observation_digest":"sha256:0d06f437ff5dd4d69e0a2dcc96f4ac36d1c0c14ba0f7c1feb8d51339aca86bfd","observation_id":"d52799a1-7bf0-4cbb-8a04-fe14ac3edea9","resolution":{"observed_at":"2026-08-07T22:32:29.053915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2204.11864/citation-record","integrity":"/paper/2204.11864/integrity","json":"/paper/2204.11864/citation-record.json","paper":"/paper/2204.11864"},"outbound":[],"paper":{"arxiv_id":"2204.11864","last_updated":"2022-04-25T18:00:01Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-09T15:16:06.185446Z","submitted_at":"2022-04-25T18:00:01Z","title":"Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based 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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2204.11864."}