{"as_of":"2026-07-23T01:33:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8eb928188d0e9e93994ed1894f98a4fe3529eeeba7a639cdcffa50a582106325","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":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-07-22T06:31:00.163083+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"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":"2026-06-28T14:02:16.652200Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1707.05269","last_updated":"2017-07-17T16:29:33Z","snapshot_observed_at":"2026-07-06T05:51:27.144284Z","submitted_at":"2017-07-17T16:29:33Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","version":1},"cited_work":{"arxiv_id":"1707.05269","doi":null,"metadata_source":"pith","pith_arxiv_id":"1707.05269","snapshot_observed_at":"2026-06-28T14:02:16.652200Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","venue":"astro-ph.GA","work_id":"b4dd144d-9de4-4d5f-8161-b5062e5be549","year":2017},"citing_paper":{"arxiv_id":"2604.12597","last_updated":"2026-04-14T11:25:05Z","snapshot_observed_at":"2026-07-06T23:00:46.620106Z","submitted_at":"2026-04-14T11:25:05Z","title":"Unveiling Dominant Toroidal Magnetic Fields in a Protostellar Outflow","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-05-10T14:55:52.318357Z"},"links":{"cited_paper":"/paper/1707.05269","citing_paper":"/paper/2604.12597"},"observation_digest":"sha256:c40804ed801785fb613d993234230aa30ad99ba90ef4a2164a16edde9c4442f7","observation_id":"2dd31510-2ef9-4808-83ba-ef5adf18bcf7","resolution":{"observed_at":"2026-05-11T11:26:02.517786Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-22T06:31:00.163083+00:00","source":"crossref"},{"observed_at":"2026-07-22T06:30:55.410749+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.05269","last_updated":"2017-07-17T16:29:33Z","snapshot_observed_at":"2026-07-06T05:51:27.144284Z","submitted_at":"2017-07-17T16:29:33Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","version":1},"cited_work":{"arxiv_id":"1707.05269","doi":null,"metadata_source":"pith","pith_arxiv_id":"1707.05269","snapshot_observed_at":"2026-06-28T14:02:16.652200Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","venue":"astro-ph.GA","work_id":"b4dd144d-9de4-4d5f-8161-b5062e5be549","year":2017},"citing_paper":{"arxiv_id":"2605.17708","last_updated":"2026-05-18T00:07:32Z","snapshot_observed_at":"2026-07-06T23:28:41.111402Z","submitted_at":"2026-05-18T00:07:32Z","title":"BISTRO Survey: Gravity-Dominated and Magnetically Regulated Star Formation in M17 SW","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1707.05269","citing_paper":"/paper/2605.17708"},"observation_digest":"sha256:28556f4063ae398db6992b20889cbeabb030a59689af20a1276739e5ab957193","observation_id":"99377a8a-9f0e-44a3-ab19-eeb71501004c","resolution":{"observed_at":"2026-05-19T23:07:50.373995Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-22T06:31:00.163083+00:00","source":"crossref"},{"observed_at":"2026-07-22T06:30:55.410749+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.05269","last_updated":"2017-07-17T16:29:33Z","snapshot_observed_at":"2026-07-06T05:51:27.144284Z","submitted_at":"2017-07-17T16:29:33Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","version":1},"cited_work":{"arxiv_id":"1707.05269","doi":null,"metadata_source":"pith","pith_arxiv_id":"1707.05269","snapshot_observed_at":"2026-06-28T14:02:16.652200Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","venue":"astro-ph.GA","work_id":"b4dd144d-9de4-4d5f-8161-b5062e5be549","year":2017},"citing_paper":{"arxiv_id":"2605.18438","last_updated":"2026-05-26T09:57:55Z","snapshot_observed_at":"2026-07-06T23:29:20.279470Z","submitted_at":"2026-05-18T14:09:56Z","title":"Velocity-resolved [O I] 63,145 um, [C II] 158 um, and OH mapping along the Orion BN/KL explosive outflow and irradiated shocks","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1707.05269","citing_paper":"/paper/2605.18438"},"observation_digest":"sha256:3c6e77aa3cc439cb65f7a6bd345314e34133aedd4c4e2b2f211ea10c98775aef","observation_id":"66f16614-1ce3-4f96-aa80-da40dfc90890","resolution":{"observed_at":"2026-05-20T09:23:09.843375Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-22T06:31:00.163083+00:00","source":"crossref"},{"observed_at":"2026-07-22T06:30:55.410749+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.05269","last_updated":"2017-07-17T16:29:33Z","snapshot_observed_at":"2026-07-06T05:51:27.144284Z","submitted_at":"2017-07-17T16:29:33Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","version":1},"cited_work":{"arxiv_id":"1707.05269","doi":null,"metadata_source":"pith","pith_arxiv_id":"1707.05269","snapshot_observed_at":"2026-06-28T14:02:16.652200Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","venue":"astro-ph.GA","work_id":"b4dd144d-9de4-4d5f-8161-b5062e5be549","year":2017},"citing_paper":{"arxiv_id":"2605.21101","last_updated":"2026-05-20T12:30:08Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-20T12:30:08Z","title":"B-Fields and Star Formation across Scales with TRAO (B-FROST): CO Abundances, Dynamics and Relative Orientations in the Translucent High Latitude Cloud MBM12","version":1},"reference_index":156,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1707.05269","citing_paper":"/paper/2605.21101"},"observation_digest":"sha256:b7719b4b3914304cc2c3ae579600d608de99e6452bd35cb7034852b0a5bf8118","observation_id":"11ca2b13-5514-457a-b8a4-3ddb610f75bc","resolution":{"observed_at":"2026-05-21T03:29:28.892710Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-22T06:31:00.163083+00:00","source":"crossref"},{"observed_at":"2026-07-22T06:30:55.410749+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.05269","last_updated":"2017-07-17T16:29:33Z","snapshot_observed_at":"2026-07-06T05:51:27.144284Z","submitted_at":"2017-07-17T16:29:33Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","version":1},"cited_work":{"arxiv_id":"1707.05269","doi":null,"metadata_source":"pith","pith_arxiv_id":"1707.05269","snapshot_observed_at":"2026-06-28T14:02:16.652200Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","venue":"astro-ph.GA","work_id":"b4dd144d-9de4-4d5f-8161-b5062e5be549","year":2017},"citing_paper":{"arxiv_id":"2606.02149","last_updated":"2026-06-01T12:16:31Z","snapshot_observed_at":"2026-07-06T23:42:35.063977Z","submitted_at":"2026-06-01T12:16:31Z","title":"The magnetic field of the Milky Way: an observational perspective","version":1},"reference_index":282,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1707.05269","citing_paper":"/paper/2606.02149"},"observation_digest":"sha256:145ff70f199a282e679d308f4d4e9de4fb4654a7854c81a96c3e4a192c338d5c","observation_id":"463d9b2c-a462-4e7f-bf88-b35299412bca","resolution":{"observed_at":"2026-06-28T14:02:16.653360Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-22T06:31:00.163083+00:00","source":"crossref"},{"observed_at":"2026-07-22T06:30:55.410749+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.05269","last_updated":"2017-07-17T16:29:33Z","snapshot_observed_at":"2026-07-06T05:51:27.144284Z","submitted_at":"2017-07-17T16:29:33Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","version":1},"cited_work":{"arxiv_id":"1707.05269","doi":null,"metadata_source":"pith","pith_arxiv_id":"1707.05269","snapshot_observed_at":"2026-06-28T14:02:16.652200Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","venue":"astro-ph.GA","work_id":"b4dd144d-9de4-4d5f-8161-b5062e5be549","year":2017},"citing_paper":{"arxiv_id":"2606.13123","last_updated":"2026-07-11T10:56:45Z","snapshot_observed_at":"2026-07-16T23:17:53.423400Z","submitted_at":"2026-06-11T09:50:18Z","title":"Grain Alignment and Dust Evolution Physics with Polarisation (GRADE-POL). II. On the physical basis of Serkowski and super-Serkowski polarisation spectra","version":1},"reference_index":265,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1707.05269","citing_paper":"/paper/2606.13123"},"observation_digest":"sha256:e64cac6ea5da14a12707f9551512903dbe5208dd241609b901658e97561e31a4","observation_id":"d61b9f43-6573-4bae-9a56-cb896b7c3b8e","resolution":{"observed_at":"2026-06-27T06:50:40.077830Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-22T06:31:00.163083+00:00","source":"crossref"},{"observed_at":"2026-07-22T06:30:55.410749+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.05269","last_updated":"2017-07-17T16:29:33Z","snapshot_observed_at":"2026-07-06T05:51:27.144284Z","submitted_at":"2017-07-17T16:29:33Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","version":1},"cited_work":{"arxiv_id":"1707.05269","doi":null,"metadata_source":"pith","pith_arxiv_id":"1707.05269","snapshot_observed_at":"2026-06-28T14:02:16.652200Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament","venue":"astro-ph.GA","work_id":"b4dd144d-9de4-4d5f-8161-b5062e5be549","year":2017},"citing_paper":{"arxiv_id":"2606.22090","last_updated":"2026-06-20T15:16:18Z","snapshot_observed_at":"2026-07-06T23:56:59.635251Z","submitted_at":"2026-06-20T15:16:18Z","title":"Measuring Magnetic Field Strengths in Galactic Star-forming Regions via the Zeeman Effect with the SKA","version":1},"reference_index":124,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1707.05269","citing_paper":"/paper/2606.22090"},"observation_digest":"sha256:783ac8485bedef225fb52c877cd2a143885fcf32418d063cfcd40bd472ab3ff4","observation_id":"6f5b8909-5698-4d98-8267-2e2b4fcbd30d","resolution":{"observed_at":"2026-06-26T11:59:26.809212Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-22T06:31:00.163083+00:00","source":"crossref"},{"observed_at":"2026-07-22T06:30:55.410749+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1707.05269/citation-record","integrity":"/paper/1707.05269/integrity","json":"/paper/1707.05269/citation-record.json","paper":"/paper/1707.05269"},"outbound":[],"paper":{"arxiv_id":"1707.05269","last_updated":"2017-07-17T16:29:33Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T05:51:27.144284Z","submitted_at":"2017-07-17T16:29:33Z","title":"The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament"},"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":"2026-07-22T06:31:00.163083+00:00","source":"crossref"},{"observed_at":"2026-07-22T06:30:55.410749+00:00","source":"retraction_watch"}],"thesis":"As of 23 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1707.05269."}