{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:4IGORFKWA36JOQO4VTUYZ5VUVZ","short_pith_number":"pith:4IGORFKW","schema_version":"1.0","canonical_sha256":"e20ce8955606fc9741dcace98cf6b4ae7280458a0e1adf6c9fc2f1a448475d2e","source":{"kind":"arxiv","id":"1210.3082","version":3},"attestation_state":"computed","paper":{"title":"A possible influence of magnetic fields on the rotation of gas in NGC 253","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Jan P\\c{e}kala, Joanna Ja{\\l}ocha, {\\L}ukasz Bratek, Marek Kutschera","submitted_at":"2012-10-10T23:02:58Z","abstract_excerpt":"The magnetic fields that are present in the galaxy NGC 253 are exceptionally strong. This means that they can influence the rotation of matter and hence the mass-to-light ratio. In this context, we address the issue of the presence of a non-baryonic dark matter halo in this galaxy."},"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":"1210.3082","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-10-10T23:02:58Z","cross_cats_sorted":[],"title_canon_sha256":"628da128540b7efd8775455d2a284ee79b273cd9b7db2ae70c79a551a8535a28","abstract_canon_sha256":"cf802583b8e2d602f2314567cc389747e8fd3b2117699c57ca96ca239fcf201d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:53:27.286091Z","signature_b64":"tOIqSDpWRwfO7Y7sm47b9utau85y9nNdm1AYxlovlxz1iaOqbZFsleNZaqItCgPOa2WSWPio6A+qJXsyFMjvDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e20ce8955606fc9741dcace98cf6b4ae7280458a0e1adf6c9fc2f1a448475d2e","last_reissued_at":"2026-05-18T02:53:27.285453Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:53:27.285453Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A possible influence of magnetic fields on the rotation of gas in NGC 253","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Jan P\\c{e}kala, Joanna Ja{\\l}ocha, {\\L}ukasz Bratek, Marek Kutschera","submitted_at":"2012-10-10T23:02:58Z","abstract_excerpt":"The magnetic fields that are present in the galaxy NGC 253 are exceptionally strong. This means that they can influence the rotation of matter and hence the mass-to-light ratio. In this context, we address the issue of the presence of a non-baryonic dark matter halo in this galaxy."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.3082","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1210.3082","created_at":"2026-05-18T02:53:27.285560+00:00"},{"alias_kind":"arxiv_version","alias_value":"1210.3082v3","created_at":"2026-05-18T02:53:27.285560+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.3082","created_at":"2026-05-18T02:53:27.285560+00:00"},{"alias_kind":"pith_short_12","alias_value":"4IGORFKWA36J","created_at":"2026-05-18T12:26:53.410803+00:00"},{"alias_kind":"pith_short_16","alias_value":"4IGORFKWA36JOQO4","created_at":"2026-05-18T12:26:53.410803+00:00"},{"alias_kind":"pith_short_8","alias_value":"4IGORFKW","created_at":"2026-05-18T12:26:53.410803+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4IGORFKWA36JOQO4VTUYZ5VUVZ","json":"https://pith.science/pith/4IGORFKWA36JOQO4VTUYZ5VUVZ.json","graph_json":"https://pith.science/api/pith-number/4IGORFKWA36JOQO4VTUYZ5VUVZ/graph.json","events_json":"https://pith.science/api/pith-number/4IGORFKWA36JOQO4VTUYZ5VUVZ/events.json","paper":"https://pith.science/paper/4IGORFKW"},"agent_actions":{"view_html":"https://pith.science/pith/4IGORFKWA36JOQO4VTUYZ5VUVZ","download_json":"https://pith.science/pith/4IGORFKWA36JOQO4VTUYZ5VUVZ.json","view_paper":"https://pith.science/paper/4IGORFKW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1210.3082&json=true","fetch_graph":"https://pith.science/api/pith-number/4IGORFKWA36JOQO4VTUYZ5VUVZ/graph.json","fetch_events":"https://pith.science/api/pith-number/4IGORFKWA36JOQO4VTUYZ5VUVZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4IGORFKWA36JOQO4VTUYZ5VUVZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4IGORFKWA36JOQO4VTUYZ5VUVZ/action/storage_attestation","attest_author":"https://pith.science/pith/4IGORFKWA36JOQO4VTUYZ5VUVZ/action/author_attestation","sign_citation":"https://pith.science/pith/4IGORFKWA36JOQO4VTUYZ5VUVZ/action/citation_signature","submit_replication":"https://pith.science/pith/4IGORFKWA36JOQO4VTUYZ5VUVZ/action/replication_record"}},"created_at":"2026-05-18T02:53:27.285560+00:00","updated_at":"2026-05-18T02:53:27.285560+00:00"}