{"as_of":"2026-08-14T07:27:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:227933d2079941cdcb01aaf4b5bc041775791162a64b5a739373ba3c33ee0bb1","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-11T11:50:26.030339Z","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":"2026-06-27T04:20:32.722081Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1609.05911","last_updated":"2016-09-19T20:00:11Z","snapshot_observed_at":"2026-07-06T05:11:23.846651Z","submitted_at":"2016-09-19T20:00:11Z","title":"The link between turbulence, magnetic fields, filaments, and star formation in the Central Molecular Zone cloud G0.253+0.016","version":1},"cited_work":{"arxiv_id":"1609.05911","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.05911","snapshot_observed_at":"2026-06-27T04:20:32.722081Z","title":"The link between turbulence, magnetic fields, filaments, and star formation in the Central Molecular Zone cloud G0.253+0.016","venue":"astro-ph.GA","work_id":"a423fb3f-2003-4364-a610-b1780e05300e","year":2016},"citing_paper":{"arxiv_id":"2605.21672","last_updated":"2026-05-20T19:25:53Z","snapshot_observed_at":"2026-08-12T19:04:24.607505Z","submitted_at":"2026-05-20T19:25:53Z","title":"Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas","version":1},"reference_index":114,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1609.05911","citing_paper":"/paper/2605.21672"},"observation_digest":"sha256:3dec13946aa1a5f2ae15458811011acc808037dba18ad9ebc1ef6a98b8d8c9bd","observation_id":"abd417f3-10e7-4d23-bcd3-83341ee9ecac","resolution":{"observed_at":"2026-05-22T08:11:16.621463Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1609.05911","last_updated":"2016-09-19T20:00:11Z","snapshot_observed_at":"2026-07-06T05:11:23.846651Z","submitted_at":"2016-09-19T20:00:11Z","title":"The link between turbulence, magnetic fields, filaments, and star formation in the Central Molecular Zone cloud G0.253+0.016","version":1},"cited_work":{"arxiv_id":"1609.05911","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.05911","snapshot_observed_at":"2026-06-27T04:20:32.722081Z","title":"The link between turbulence, magnetic fields, filaments, and star formation in the Central Molecular Zone cloud G0.253+0.016","venue":"astro-ph.GA","work_id":"a423fb3f-2003-4364-a610-b1780e05300e","year":2016},"citing_paper":{"arxiv_id":"2606.25995","last_updated":"2026-06-24T16:07:47Z","snapshot_observed_at":"2026-08-03T00:26:16.310679Z","submitted_at":"2026-06-24T16:07:47Z","title":"The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1609.05911","citing_paper":"/paper/2606.25995"},"observation_digest":"sha256:16a7a71c2eba63eb04a2001c59dd76de4a309b55c4956883b5ba31b91b0cb70b","observation_id":"7b198f71-43eb-4bdd-bc21-012f4e8e85e0","resolution":{"observed_at":"2026-06-27T04:20:32.723604Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1609.05911/citation-record","integrity":"/paper/1609.05911/integrity","json":"/paper/1609.05911/citation-record.json","paper":"/paper/1609.05911"},"outbound":[],"paper":{"arxiv_id":"1609.05911","last_updated":"2016-09-19T20:00:11Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T05:11:23.846651Z","submitted_at":"2016-09-19T20:00:11Z","title":"The link between turbulence, magnetic fields, filaments, and star formation in the Central Molecular Zone cloud G0.253+0.016"},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1609.05911."}