{"as_of":"2026-08-18T11:06:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bfaaa7bb8d16baefa7905861b85c2e84e6c2ffce30301532f054bd017cf1e5db","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":"2026-08-18T06:34:40.430872+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":"2026-08-10T18:07:29.063028Z","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":"2026-08-10T05:30:23.456663Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-10T05:30:23.456663Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2407.14896","last_updated":"2025-02-02T10:48:05Z","snapshot_observed_at":"2026-08-18T05:18:31.612773Z","submitted_at":"2024-07-20T15:11:04Z","title":"Probing 3D magnetic fields using starlight polarization and grain alignment theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.14896","snapshot_observed_at":"2026-08-10T18:07:29.063028Z","title":"2024, arXiv e-prints, arXiv:2407.14896, doi: 10.48550/arXiv.2407.14896","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.11634","last_updated":"2025-01-20T18:08:55Z","snapshot_observed_at":"2026-08-17T19:59:23.201622Z","submitted_at":"2025-01-20T18:08:55Z","title":"B-fields And dust in interstelLar fiLAments using Dust POLarization (BALLAD-POL): III. Grain alignment and disruption mechanisms in G34.43+0.24 using polarization observations from JCMT/POL-2","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-10T18:07:29.063028Z"},"links":{"cited_paper":"/paper/2407.14896","citing_paper":"/paper/2501.11634"},"observation_digest":"sha256:3c02c0ee09457afba6b4a9c9c2c2a6f200be9505d060b23dcc61c5712268e4ab","observation_id":"1870f26f-3359-490f-b249-82df7ec290b6","resolution":{"observed_at":"2026-08-10T18:07:29.063028Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.14896","last_updated":"2025-02-02T10:48:05Z","snapshot_observed_at":"2026-08-18T05:18:31.612773Z","submitted_at":"2024-07-20T15:11:04Z","title":"Probing 3D magnetic fields using starlight polarization and grain alignment theory","version":2},"cited_work":{"arxiv_id":"2407.14896","doi":"10.48550/arxiv.2407.14896","metadata_source":"pith","pith_arxiv_id":"2407.14896","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Probing 3D magnetic fields using starlight polarization and grain alignment theory","venue":"astro-ph.GA","work_id":"3b97d718-8e45-49f7-9018-c8c4e010c270","year":2024},"citing_paper":{"arxiv_id":"2507.07205","last_updated":"2025-07-09T18:27:00Z","snapshot_observed_at":"2026-08-18T04:20:00.097216Z","submitted_at":"2025-07-09T18:27:00Z","title":"B-fields And dust in interstelLar fiLAments using Dust POLarization (BALLAD-POL): IV. Grain alignment mechanisms in Cocoon Nebula (IC 5146) using polarization observations from JCMT/POL-2","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T18:52:22.730059Z"},"links":{"cited_paper":"/paper/2407.14896","citing_paper":"/paper/2507.07205"},"observation_digest":"sha256:4e7751a5efb4f0e9e76f05069a3a25164a0158759f41e0cdbbd2f0d9b80ab89e","observation_id":"8a0e88d9-610a-4f30-ae3a-00e275307071","resolution":{"observed_at":"2026-08-06T18:52:22.797048Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2407.14896/citation-record","integrity":"/paper/2407.14896/integrity","json":"/paper/2407.14896/citation-record.json","paper":"/paper/2407.14896"},"outbound":[],"paper":{"arxiv_id":"2407.14896","last_updated":"2025-02-02T10:48:05Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-18T05:18:31.612773Z","submitted_at":"2024-07-20T15:11:04Z","title":"Probing 3D magnetic fields using starlight polarization and grain alignment theory"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2407.14896."}