{"as_of":"2026-08-06T02:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ec87f08dabc98e44bcf019d64d397dda6191eeaa838b4df15349b1140b876124","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":"2026-08-05T06:32:48.257954+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":"2026-07-11T11:50:26.030339Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":56,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1211.0041","last_updated":"2012-10-31T21:46:10Z","snapshot_observed_at":"2026-07-06T02:58:56.478549Z","submitted_at":"2012-10-31T21:46:10Z","title":"The Cosmology Large Angular Scale Surveyor (CLASS): 40 GHz optical design","version":1},"cited_work":{"arxiv_id":"1211.0041","doi":"10.1117/12.925464","metadata_source":"pith","pith_arxiv_id":"1211.0041","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The Cosmology Large Angular Scale Surveyor (CLASS): 40 GHz optical design","venue":"astro-ph.IM","work_id":"bbe17775-7207-4971-8a9d-ebf94a467621","year":2012},"citing_paper":{"arxiv_id":"2605.23489","last_updated":"2026-05-22T10:51:03Z","snapshot_observed_at":"2026-08-02T00:51:08.034872Z","submitted_at":"2026-05-22T10:51:03Z","title":"A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz","version":1},"reference_index":142,"source":"arxiv_source","source_observed_at":"2026-05-25T03:56:11.714959Z"},"links":{"cited_paper":"/paper/1211.0041","citing_paper":"/paper/2605.23489"},"observation_digest":"sha256:3cc3414747da9e9246f7977f76da48662bf2ef0617ca5f10825f159effe0f10b","observation_id":"e09d23eb-85df-4727-b269-42fea636d981","resolution":{"observed_at":"2026-05-25T03:56:36.410461Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1211.0041","last_updated":"2012-10-31T21:46:10Z","snapshot_observed_at":"2026-07-06T02:58:56.478549Z","submitted_at":"2012-10-31T21:46:10Z","title":"The Cosmology Large Angular Scale Surveyor (CLASS): 40 GHz optical design","version":1},"cited_work":{"arxiv_id":"1211.0041","doi":"10.1117/12.925464","metadata_source":"pith","pith_arxiv_id":"1211.0041","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The Cosmology Large Angular Scale Surveyor (CLASS): 40 GHz optical design","venue":"astro-ph.IM","work_id":"bbe17775-7207-4971-8a9d-ebf94a467621","year":2012},"citing_paper":{"arxiv_id":"2606.26576","last_updated":"2026-06-25T03:52:30Z","snapshot_observed_at":"2026-07-07T00:00:56.276365Z","submitted_at":"2026-06-25T03:52:30Z","title":"Detectors for CLASS-W2: The second 90 GHz telescope of the Cosmology Large Angular Scale Surveyor","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1211.0041","citing_paper":"/paper/2606.26576"},"observation_digest":"sha256:f48aa0797350586ded80df23e727fab451ce07ab7da7a0aae537d8aeb82acdcb","observation_id":"ca650e79-f08a-46bd-955b-75da41e6ded9","resolution":{"observed_at":"2026-06-26T04:28:59.243044Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1211.0041","last_updated":"2012-10-31T21:46:10Z","snapshot_observed_at":"2026-07-06T02:58:56.478549Z","submitted_at":"2012-10-31T21:46:10Z","title":"The Cosmology Large Angular Scale Surveyor (CLASS): 40 GHz optical design","version":1},"cited_work":{"arxiv_id":"1211.0041","doi":"10.1117/12.925464","metadata_source":"pith","pith_arxiv_id":"1211.0041","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The Cosmology Large Angular Scale Surveyor (CLASS): 40 GHz optical design","venue":"astro-ph.IM","work_id":"bbe17775-7207-4971-8a9d-ebf94a467621","year":2012},"citing_paper":{"arxiv_id":"2606.27110","last_updated":"2026-06-25T14:47:25Z","snapshot_observed_at":"2026-08-01T06:34:49.990206Z","submitted_at":"2026-06-25T14:47:25Z","title":"Probing Anomalous Microwave Emission with the Square Kilometre Array","version":1},"reference_index":263,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1211.0041","citing_paper":"/paper/2606.27110"},"observation_digest":"sha256:e3abbe0795765e58242a2761783dffa24dfa4e4325967ffb73aa45c8c93a7c10","observation_id":"e0251b5d-8432-4428-9b81-b1862cb6120a","resolution":{"observed_at":"2026-06-26T05:39:00.304569Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1211.0041/citation-record","integrity":"/paper/1211.0041/integrity","json":"/paper/1211.0041/citation-record.json","paper":"/paper/1211.0041"},"outbound":[],"paper":{"arxiv_id":"1211.0041","last_updated":"2012-10-31T21:46:10Z","latest_version":1,"primary_category":"astro-ph.IM","snapshot_observed_at":"2026-07-06T02:58:56.478549Z","submitted_at":"2012-10-31T21:46:10Z","title":"The Cosmology Large Angular Scale Surveyor (CLASS): 40 GHz optical design"},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1211.0041."}