{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:DNI3BZXSW6HAWXLNZLYNWAKIFW","short_pith_number":"pith:DNI3BZXS","schema_version":"1.0","canonical_sha256":"1b51b0e6f2b78e0b5d6dcaf0db01482dbba22b5f0b0d7ac1d6621fdfb1238e20","source":{"kind":"arxiv","id":"2306.01246","version":2},"attestation_state":"computed","paper":{"title":"Distance of PSR B0458+46 indicated by FAST HI absorption observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Chen Wang, D. J. Zhou, J. L. Han, J. Xu, L. G. Hou, Tao Hong, W. C. Jing, X. Y. Gao, Z. L. Yang","submitted_at":"2023-06-02T03:14:04Z","abstract_excerpt":"The pulsar B0458+46 was previously believed to have a distance of about 1.3$~$kpc and to be associated with a nearby supernova remnant, SNR HB9 (G160.9+2.6). We observe the neutral hydrogen (HI) absorption spectrum of PSR B0458+46 by using the Five-hundred-meter Aperture Spherical radio Telescope (FAST), and detect two absorption lines at radial velocities of $V_{\\rm LSR} = {-7.7}~{\\rm km~s}^{-1}$ and $-28.1~{\\rm km~s^{-1}}$. Based on the Galactic rotation curve with a modification factor correcting for the systematic stream in the anticenter region, we derive the kinematic distance of the far"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2306.01246","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-06-02T03:14:04Z","cross_cats_sorted":["astro-ph.GA","astro-ph.IM"],"title_canon_sha256":"c8b798d8a65c5ab066bf54908f0a53ec591ad8411e6af69fd5508b59cdf63ef5","abstract_canon_sha256":"d1e88c0b9ba6ec68b40dff06200319331a7c7d623aa47d6e109410f72c720bfc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:24:30.428134Z","signature_b64":"qWWRVYRx5Mx6oexjTf+7+CgaPPCkMPvs1lFeYEwGxwzxR0uTR2XMt6QjXndMBAL4W2Glnp7wslfRhgZK9KrqCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1b51b0e6f2b78e0b5d6dcaf0db01482dbba22b5f0b0d7ac1d6621fdfb1238e20","last_reissued_at":"2026-07-05T06:24:30.427705Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:24:30.427705Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Distance of PSR B0458+46 indicated by FAST HI absorption observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Chen Wang, D. J. Zhou, J. L. Han, J. Xu, L. G. Hou, Tao Hong, W. C. Jing, X. Y. Gao, Z. L. Yang","submitted_at":"2023-06-02T03:14:04Z","abstract_excerpt":"The pulsar B0458+46 was previously believed to have a distance of about 1.3$~$kpc and to be associated with a nearby supernova remnant, SNR HB9 (G160.9+2.6). We observe the neutral hydrogen (HI) absorption spectrum of PSR B0458+46 by using the Five-hundred-meter Aperture Spherical radio Telescope (FAST), and detect two absorption lines at radial velocities of $V_{\\rm LSR} = {-7.7}~{\\rm km~s}^{-1}$ and $-28.1~{\\rm km~s^{-1}}$. Based on the Galactic rotation curve with a modification factor correcting for the systematic stream in the anticenter region, we derive the kinematic distance of the far"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2306.01246","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2306.01246/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2306.01246","created_at":"2026-07-05T06:24:30.427762+00:00"},{"alias_kind":"arxiv_version","alias_value":"2306.01246v2","created_at":"2026-07-05T06:24:30.427762+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2306.01246","created_at":"2026-07-05T06:24:30.427762+00:00"},{"alias_kind":"pith_short_12","alias_value":"DNI3BZXSW6HA","created_at":"2026-07-05T06:24:30.427762+00:00"},{"alias_kind":"pith_short_16","alias_value":"DNI3BZXSW6HAWXLN","created_at":"2026-07-05T06:24:30.427762+00:00"},{"alias_kind":"pith_short_8","alias_value":"DNI3BZXS","created_at":"2026-07-05T06:24:30.427762+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06096","citing_title":"Exploring the Galactic plasma with pulsars in the SKA Era","ref_index":13,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DNI3BZXSW6HAWXLNZLYNWAKIFW","json":"https://pith.science/pith/DNI3BZXSW6HAWXLNZLYNWAKIFW.json","graph_json":"https://pith.science/api/pith-number/DNI3BZXSW6HAWXLNZLYNWAKIFW/graph.json","events_json":"https://pith.science/api/pith-number/DNI3BZXSW6HAWXLNZLYNWAKIFW/events.json","paper":"https://pith.science/paper/DNI3BZXS"},"agent_actions":{"view_html":"https://pith.science/pith/DNI3BZXSW6HAWXLNZLYNWAKIFW","download_json":"https://pith.science/pith/DNI3BZXSW6HAWXLNZLYNWAKIFW.json","view_paper":"https://pith.science/paper/DNI3BZXS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2306.01246&json=true","fetch_graph":"https://pith.science/api/pith-number/DNI3BZXSW6HAWXLNZLYNWAKIFW/graph.json","fetch_events":"https://pith.science/api/pith-number/DNI3BZXSW6HAWXLNZLYNWAKIFW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DNI3BZXSW6HAWXLNZLYNWAKIFW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DNI3BZXSW6HAWXLNZLYNWAKIFW/action/storage_attestation","attest_author":"https://pith.science/pith/DNI3BZXSW6HAWXLNZLYNWAKIFW/action/author_attestation","sign_citation":"https://pith.science/pith/DNI3BZXSW6HAWXLNZLYNWAKIFW/action/citation_signature","submit_replication":"https://pith.science/pith/DNI3BZXSW6HAWXLNZLYNWAKIFW/action/replication_record"}},"created_at":"2026-07-05T06:24:30.427762+00:00","updated_at":"2026-07-05T06:24:30.427762+00:00"}