{"as_of":"2026-08-12T22:49:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:59810e6144f81c51aecb8b8745f8ff39bad9742467ab8c78a0987a4a9ac0b4b7","coverage":[{"denominator":24,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":24,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T02:02:22.977432Z","state":"measured"},{"denominator":24,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":24,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2607.25587/citation-record","integrity":"/paper/2607.25587/integrity","json":"/paper/2607.25587/citation-record.json","paper":"/paper/2607.25587"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.824676Z","title":null,"venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.824676Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:beb92a427db55d7735630c930edcab900ea55139012d59ec120a321aeb336f24","observation_id":"334c14b9-2ae8-4a3f-a4fc-7b52d513f913","resolution":{"observed_at":"2026-08-01T02:02:22.824676Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.831321Z","title":"Studying the magnetic field of our galaxy, as well as other galaxies, is very important for understanding all the active processes occurring in galaxies","venue":null,"work_id":null,"year":1949},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.831321Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:ebf6f60461534f831a5928100bf8776180e53a8f3ff28c6e63336a46f58f3865","observation_id":"e94c9625-eae5-40a5-b2ec-56bc53eac366","resolution":{"observed_at":"2026-08-01T02:02:22.831321Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.839542Z","title":"The ATNF pulsar catalogue 2025 contains various data for approximately 4,000 pulsars","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.839542Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:f4b602c214027dbd33c5a5abb0fd4a411c20633294c76a4f88dc45c6cd0d5502","observation_id":"244253ed-d7a1-4d29-b011-a98d2aae6d11","resolution":{"observed_at":"2026-08-01T02:02:22.839542Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.845702Z","title":"This makes it possible to identify clearly distinguishable regions of large-scale","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.845702Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:a2bdb12d52a4df4e97ff3db02f450c6d9e835bfa99649302fe61ef10e65c9d3d","observation_id":"df5d352d-3fbd-4980-a56e-97c417b29998","resolution":{"observed_at":"2026-08-01T02:02:22.845702Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.851163Z","title":"The coordinates are d and h, as in the fig.2, but on this picture the mark RM200 indicates that 100 rad/m2 <│RM│<200rad/m2, and the mark RM100 indicates that 0 <│RM│<100rad/m2","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.851163Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:464bb45580edb66f629b7635f0f19bda30209e7210532798e80b0c166f17f339","observation_id":"2f9780f7-922a-4902-874d-10f6a17a2211","resolution":{"observed_at":"2026-08-01T02:02:22.851163Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.855969Z","title":"The resulting catalogue of RM values covers the sky area north of declination −400","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.855969Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:4a8342e274ad2bc518566367cff1e2cbabad04f17960b36fd7cfab9faa637bf1","observation_id":"6daabea4-389c-40f1-9d00-36c50a3eed3c","resolution":{"observed_at":"2026-08-01T02:02:22.855969Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.861182Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.861182Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:a203054ca2d44d35fcdc70fb509282a086b5c5bf893a795c78c247d6399699bc","observation_id":"fe58b4d7-b7ae-4e88-953c-22122a9f29c0","resolution":{"observed_at":"2026-08-01T02:02:22.861182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.868497Z","title":"Hiltner, Science 109, 166 (1949)","venue":null,"work_id":null,"year":1949},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.868497Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:f4fc6914ce9218ba56a8d6c583fa1507ea3134e635f6ccd81b57fc8278a0e340","observation_id":"a359521f-987b-4596-bfe2-1291296de089","resolution":{"observed_at":"2026-08-01T02:02:22.868497Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.873418Z","title":"Rev., 75, 1169","venue":null,"work_id":null,"year":1949},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.873418Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:95a0490cdecae586e10672209f4df4360b6543fd3078fe0e85be81986f2ee343","observation_id":"adc9423e-c2e9-4093-a57d-5558af678727","resolution":{"observed_at":"2026-08-01T02:02:22.873418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.878529Z","title":"O., 1950, Phis","venue":null,"work_id":null,"year":1950},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.878529Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:6ea83706a6f2befe9fff94d6b5283673e204b0a58db521312e46324b30710a4a","observation_id":"a7ff5d0b-04dc-413a-8188-830576fbe3ab","resolution":{"observed_at":"2026-08-01T02:02:22.878529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.883386Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.883386Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:6acf9b36541e3998174e9d3e86146b80755b077f6743cac394449818bcbe2d34","observation_id":"98a1eb56-353e-4a8f-8dbf-de68c56dc11e","resolution":{"observed_at":"2026-08-01T02:02:22.883386Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.5225","last_updated":"2013-06-04T19:07:22Z","snapshot_observed_at":"2026-07-06T03:02:33.289120Z","submitted_at":"2012-12-20T20:24:23Z","title":"Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.5225","snapshot_observed_at":"2026-08-01T02:02:22.888841Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.888841Z"},"links":{"cited_paper":"/paper/1212.5225","citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:149394c5f2f0f20f7e85defe9ed85141820bb3eeb8a0170fade9da8d0557ba43","observation_id":"0e91f3a7-9e4e-4e33-a85f-0ded80b4b5f6","resolution":{"observed_at":"2026-08-01T02:02:22.888841Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.895096Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.895096Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:d32d5e8fcdfd41acb6ce01d8cf2b675f81a644e372adf16434d9afcc114f0ea3","observation_id":"5c14517c-a12a-4742-bb9e-b4bf0ab1790b","resolution":{"observed_at":"2026-08-01T02:02:22.895096Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.901714Z","title":"Simard-Normandin and P","venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.901714Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:33ac860adfde91e48290e1efa235c0fdd754c3afc2e3ab99fd0b4651cda914bb","observation_id":"1e16f55c-8d7a-4c46-8e61-da39d7a3d9b9","resolution":{"observed_at":"2026-08-01T02:02:22.901714Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.906942Z","title":"R.; Makarov, A","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.906942Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:2345ac5b22129b9f7e651079a59d4c39166b95e923ad8ecac4d3070ef8eee8f7","observation_id":"31e7fee9-f1dc-47b4-a8e5-90699f0b44b7","resolution":{"observed_at":"2026-08-01T02:02:22.906942Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.914436Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.914436Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:56f09ffa1c99f82c0659597eb1e18d2b94695430924774e58e86cede1f291804","observation_id":"6111f991-cb1f-43a3-a5ca-b5a6de42e6ab","resolution":{"observed_at":"2026-08-01T02:02:22.914436Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.925015Z","title":"N., 1974","venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.925015Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:6829c2d66747a7f3fd7eb3eae774a7fedb65493e128f6552ce34529cf52e8e9d","observation_id":"630a461c-cc39-472e-8867-8ca52c5854d5","resolution":{"observed_at":"2026-08-01T02:02:22.925015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.937625Z","title":"R.; Makarov, A","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.937625Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:45d893659b298e87caa40cfe742d1f06cfd6d570cb317641b0ef0d778db94b14","observation_id":"23dcee01-02a2-42b7-9f92-fef6224416da","resolution":{"observed_at":"2026-08-01T02:02:22.937625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.946196Z","title":"L., 2024, ApJ, 966, 240","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.946196Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:1e4760710147efaf19ecd51d623df3e0061908f709482fd2c4f5e499166e94c6","observation_id":"88cb58f3-5a72-47f0-97c0-f28f39e8223c","resolution":{"observed_at":"2026-08-01T02:02:22.946196Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.953373Z","title":"R.; Stil, J","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.953373Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:51126fdb3d5e83b8f5486a722ee9e291776d260e83b8250b039a646aceb22b1a","observation_id":"540bde02-5781-4c54-abd6-c258da70de09","resolution":{"observed_at":"2026-08-01T02:02:22.953373Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.959667Z","title":null,"venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.959667Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:91e355c13c9391ff5a7282d16b3bfe6a7aa33832f388d95ca241b9fd5cab0d7d","observation_id":"fdc8a48a-9dc4-43a0-9d71-1cb42f8c41d6","resolution":{"observed_at":"2026-08-01T02:02:22.959667Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.964365Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.964365Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:6a7b3841e4cce52707b1c79ddc3d1905645a70458289f353ef0653120176c1ba","observation_id":"f8322523-9a6f-4c69-bcc0-c4dccb02f864","resolution":{"observed_at":"2026-08-01T02:02:22.964365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.971175Z","title":"R.; Mikhailov, E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.971175Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:1a162809311ba89145836641cbe9bdc9e1e9c58bf8e66f82aa1cdab439bc755b","observation_id":"81f2f094-57db-4085-920f-e1a41f2bd4d9","resolution":{"observed_at":"2026-08-01T02:02:22.971175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T02:02:22.977432Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-01T02:02:22.977432Z"},"links":{"citing_paper":"/paper/2607.25587"},"observation_digest":"sha256:6cd5614363951838698171400fab553c014542f7f26193e86144358d9bc1aec7","observation_id":"ef537f39-7c0d-41e0-b088-fa493d5b4423","resolution":{"observed_at":"2026-08-01T02:02:22.977432Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.25587","last_updated":"2026-07-28T11:17:42Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-12T14:31:09.323880Z","submitted_at":"2026-07-28T11:17:42Z","title":"Distribution of the magnetic field relative to the plane of the Galaxy in the region of the Sagittarius spiral arm"},"reference_resolution":{"displayed":24,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":23,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":24},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 24 of 24 outbound references and 0 inbound Pith citation observations for arXiv:2607.25587."}