{"as_of":"2026-08-11T18:58:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:13e2b873fc995d16e68c93dc8ac87254d7ac596ce1a5a402efb469d6b3c41f93","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":"2026-08-11T06:34:44.6726+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":"2026-08-10T22:18:28.282576Z","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":77,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1409.6724","last_updated":"2015-04-18T16:43:31Z","snapshot_observed_at":"2026-07-06T03:55:22.933759Z","submitted_at":"2014-09-23T20:00:07Z","title":"CO/H2, C/CO, OH/CO, and OH/O2 in Dense Interstellar Gas: From High Ionization to Low Metallicity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.6724","snapshot_observed_at":"2026-08-10T22:18:28.282576Z","title":"& Sternberg, A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.02051","last_updated":"2025-01-09T16:16:29Z","snapshot_observed_at":"2026-08-10T22:12:17.776232Z","submitted_at":"2025-01-03T19:00:01Z","title":"Abundant Water from Early Supernovae at Cosmic Dawn","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-10T22:18:28.282576Z"},"links":{"cited_paper":"/paper/1409.6724","citing_paper":"/paper/2501.02051"},"observation_digest":"sha256:577941ed27ac3dde838fc2140e55e8d6a9be41f3dc42aea6ef53a6207d6f64fb","observation_id":"c37ecebd-189f-4657-a258-062fa5b92f44","resolution":{"observed_at":"2026-08-10T22:18:28.282576Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.6724","last_updated":"2015-04-18T16:43:31Z","snapshot_observed_at":"2026-07-06T03:55:22.933759Z","submitted_at":"2014-09-23T20:00:07Z","title":"CO/H2, C/CO, OH/CO, and OH/O2 in Dense Interstellar Gas: From High Ionization to Low Metallicity","version":2},"cited_work":{"arxiv_id":"1409.6724","doi":"10.1093/mnras/stv851","metadata_source":"pith","pith_arxiv_id":"1409.6724","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"CO/H2, C/CO, OH/CO, and OH/O2 in Dense Interstellar Gas: From High Ionization to Low Metallicity","venue":"astro-ph.GA","work_id":"f9b5bf7f-9ba7-487c-be2f-183d0be00306","year":2014},"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":99,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1409.6724","citing_paper":"/paper/2606.25995"},"observation_digest":"sha256:118306159db7dbab61a6b31b7050c23a2702a739bcca090d9204a869d4de3092","observation_id":"e743ef67-e68a-4b0f-8c5e-696c6a4e7493","resolution":{"observed_at":"2026-06-27T04:20:32.341773Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1409.6724","last_updated":"2015-04-18T16:43:31Z","snapshot_observed_at":"2026-07-06T03:55:22.933759Z","submitted_at":"2014-09-23T20:00:07Z","title":"CO/H2, C/CO, OH/CO, and OH/O2 in Dense Interstellar Gas: From High Ionization to Low Metallicity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.6724","snapshot_observed_at":"2026-08-03T00:39:21.815543Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28727","last_updated":"2026-07-30T18:00:02Z","snapshot_observed_at":"2026-08-09T21:45:50.012639Z","submitted_at":"2026-07-30T18:00:02Z","title":"End-to-end differentiable retrieval of molecular spectra using hydrodynamics, chemistry, and radiative transfer","version":1},"reference_index":206,"source":"arxiv_source","source_observed_at":"2026-08-03T00:39:21.815543Z"},"links":{"cited_paper":"/paper/1409.6724","citing_paper":"/paper/2607.28727"},"observation_digest":"sha256:353790916c748791fbf2df917bc8c6353f5389c0d81b0cf8e2c0a8ea8cbf8ee0","observation_id":"3b1b39dc-7090-43a4-957e-5ae79aba1ae7","resolution":{"observed_at":"2026-08-03T00:39:21.815543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1409.6724/citation-record","integrity":"/paper/1409.6724/integrity","json":"/paper/1409.6724/citation-record.json","paper":"/paper/1409.6724"},"outbound":[],"paper":{"arxiv_id":"1409.6724","last_updated":"2015-04-18T16:43:31Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T03:55:22.933759Z","submitted_at":"2014-09-23T20:00:07Z","title":"CO/H2, C/CO, OH/CO, and OH/O2 in Dense Interstellar Gas: From High Ionization to Low Metallicity"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1409.6724."}