{"as_of":"2026-08-23T17:49:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e802fdf0cef22e0a15c84e7236edb9f9c88015c3817b4913b9464bdae07bb15e","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":"2026-08-23T06:30:58.430688+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":"2026-08-01T10:56:39.776162Z","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":2,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1410.8136","last_updated":"2015-05-20T19:37:17Z","snapshot_observed_at":"2026-08-14T23:13:45.045516Z","submitted_at":"2014-10-29T20:00:09Z","title":"Searching for Inflationary B-modes: Can dust emission properties be extrapolated from 350 GHz to 150 GHz?","version":2},"cited_work":{"arxiv_id":"1410.8136","doi":"10.1093/mnrasl/slv077","metadata_source":"pith","pith_arxiv_id":"1410.8136","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Searching for Inflationary B-modes: Can dust emission properties be extrapolated from 350 GHz to 150 GHz?","venue":"astro-ph.CO","work_id":"1d6861ca-2756-4383-aae1-efcfbcda9909","year":2014},"citing_paper":{"arxiv_id":"2607.03185","last_updated":"2026-07-03T10:43:50Z","snapshot_observed_at":"2026-08-14T07:23:44.883759Z","submitted_at":"2026-07-03T10:43:50Z","title":"DHARA: Data Handling and Automated Reduction pipeline for AIMPOL","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-07-12T04:17:05.392304Z"},"links":{"cited_paper":"/paper/1410.8136","citing_paper":"/paper/2607.03185"},"observation_digest":"sha256:7acafbea219286e51cbd38a71cda91241163fdc6585d9f498542358178b44b79","observation_id":"59ec363e-5ebd-48db-8078-f703e0127504","resolution":{"observed_at":"2026-07-12T04:18:28.358233Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-07-13T20:20:23.088749+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T20:20:23.088749+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1410.8136","last_updated":"2015-05-20T19:37:17Z","snapshot_observed_at":"2026-08-14T23:13:45.045516Z","submitted_at":"2014-10-29T20:00:09Z","title":"Searching for Inflationary B-modes: Can dust emission properties be extrapolated from 350 GHz to 150 GHz?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.8136","snapshot_observed_at":"2026-08-01T10:56:39.776162Z","title":"Tassis and V","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.20080","last_updated":"2026-07-22T12:33:59Z","snapshot_observed_at":"2026-08-18T17:08:15.565156Z","submitted_at":"2026-07-22T12:33:59Z","title":"Galactic Science with the LiteBIRD satellite: Spectral characterization of diffuse Galactic polarized emission at the angular power spectrum level","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-01T10:56:39.776162Z"},"links":{"cited_paper":"/paper/1410.8136","citing_paper":"/paper/2607.20080"},"observation_digest":"sha256:91b7cee2062ab4616c858d1e62bbce8141be6fbc95bfd21c3e283b1090dc2871","observation_id":"2b15fec2-befe-478f-96d4-2ce00f2aa8ac","resolution":{"observed_at":"2026-08-01T10:56:39.776162Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1410.8136/citation-record","integrity":"/paper/1410.8136/integrity","json":"/paper/1410.8136/citation-record.json","paper":"/paper/1410.8136"},"outbound":[],"paper":{"arxiv_id":"1410.8136","last_updated":"2015-05-20T19:37:17Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T23:13:45.045516Z","submitted_at":"2014-10-29T20:00:09Z","title":"Searching for Inflationary B-modes: Can dust emission properties be extrapolated from 350 GHz to 150 GHz?"},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1410.8136."}