{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:SOL75WALWS3K5PMY7PHBVUF7VO","short_pith_number":"pith:SOL75WAL","schema_version":"1.0","canonical_sha256":"9397fed80bb4b6aebd98fbce1ad0bfaba9c495e83332c811e9505cac747d052a","source":{"kind":"arxiv","id":"1008.4058","version":1},"attestation_state":"computed","paper":{"title":"The JCMT Nearby Galaxies Legacy Survey V: The CO(J=3-2) Distribution and Molecular Outflow in NGC~4631","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"B. E. Warren, C. D. Wilson, E. Brinks, F. P. Israel, G. J. Bendo, J. H. Knapen, Judith A. Irwin, P. van der Werf, Q. D. Wang, R. P. J. Tilanus, S. Muehle, S. Serjeant, T. Wiegert","submitted_at":"2010-08-24T14:44:37Z","abstract_excerpt":"We have made the first map of CO(J=3-2) emission covering the disk of the edge-on galaxy, NGC~4631, which is known for its spectacular gaseous halo. The strongest emission, which we model with a Gaussian ring,occurs within a radius of 5 kpc. Weaker disk emission is detected out to radii of 12 kpc, the most extensive molecular component yet seen in this galaxy. From comparisons with infrared data, we find that CO(J=3-2) emission more closely follows the hot dust component, rather than the cold dust,consistent with it being a good tracer of star formation. The first maps of $R_{3-2/1-0}$, H$_2$ "},"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":"1008.4058","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-08-24T14:44:37Z","cross_cats_sorted":[],"title_canon_sha256":"1f8b3a8dd9cba0c7577e8417148e5106ae2bd24b8bf8877f2e74bf50d83e755d","abstract_canon_sha256":"8a3b591ba2e8fc49f471ee04fcde9932fa338863750176908ded1c12e63274b5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T23:57:43.226781Z","signature_b64":"OtT6DvVxkgyabG+ttLk7lBXmHOryH3bH5qdqKQ3GG8xfcIdTZcvWwQXqh9wIL9Zy3QTstEq37HuHpdiFAH4NCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9397fed80bb4b6aebd98fbce1ad0bfaba9c495e83332c811e9505cac747d052a","last_reissued_at":"2026-07-04T23:57:43.226242Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T23:57:43.226242Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The JCMT Nearby Galaxies Legacy Survey V: The CO(J=3-2) Distribution and Molecular Outflow in NGC~4631","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"B. E. Warren, C. D. Wilson, E. Brinks, F. P. Israel, G. J. Bendo, J. H. Knapen, Judith A. Irwin, P. van der Werf, Q. D. Wang, R. P. J. Tilanus, S. Muehle, S. Serjeant, T. Wiegert","submitted_at":"2010-08-24T14:44:37Z","abstract_excerpt":"We have made the first map of CO(J=3-2) emission covering the disk of the edge-on galaxy, NGC~4631, which is known for its spectacular gaseous halo. The strongest emission, which we model with a Gaussian ring,occurs within a radius of 5 kpc. Weaker disk emission is detected out to radii of 12 kpc, the most extensive molecular component yet seen in this galaxy. From comparisons with infrared data, we find that CO(J=3-2) emission more closely follows the hot dust component, rather than the cold dust,consistent with it being a good tracer of star formation. The first maps of $R_{3-2/1-0}$, H$_2$ "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1008.4058","kind":"arxiv","version":1},"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/1008.4058/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":"1008.4058","created_at":"2026-07-04T23:57:43.226310+00:00"},{"alias_kind":"arxiv_version","alias_value":"1008.4058v1","created_at":"2026-07-04T23:57:43.226310+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1008.4058","created_at":"2026-07-04T23:57:43.226310+00:00"},{"alias_kind":"pith_short_12","alias_value":"SOL75WALWS3K","created_at":"2026-07-04T23:57:43.226310+00:00"},{"alias_kind":"pith_short_16","alias_value":"SOL75WALWS3K5PMY","created_at":"2026-07-04T23:57:43.226310+00:00"},{"alias_kind":"pith_short_8","alias_value":"SOL75WAL","created_at":"2026-07-04T23:57:43.226310+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/SOL75WALWS3K5PMY7PHBVUF7VO","json":"https://pith.science/pith/SOL75WALWS3K5PMY7PHBVUF7VO.json","graph_json":"https://pith.science/api/pith-number/SOL75WALWS3K5PMY7PHBVUF7VO/graph.json","events_json":"https://pith.science/api/pith-number/SOL75WALWS3K5PMY7PHBVUF7VO/events.json","paper":"https://pith.science/paper/SOL75WAL"},"agent_actions":{"view_html":"https://pith.science/pith/SOL75WALWS3K5PMY7PHBVUF7VO","download_json":"https://pith.science/pith/SOL75WALWS3K5PMY7PHBVUF7VO.json","view_paper":"https://pith.science/paper/SOL75WAL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1008.4058&json=true","fetch_graph":"https://pith.science/api/pith-number/SOL75WALWS3K5PMY7PHBVUF7VO/graph.json","fetch_events":"https://pith.science/api/pith-number/SOL75WALWS3K5PMY7PHBVUF7VO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SOL75WALWS3K5PMY7PHBVUF7VO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SOL75WALWS3K5PMY7PHBVUF7VO/action/storage_attestation","attest_author":"https://pith.science/pith/SOL75WALWS3K5PMY7PHBVUF7VO/action/author_attestation","sign_citation":"https://pith.science/pith/SOL75WALWS3K5PMY7PHBVUF7VO/action/citation_signature","submit_replication":"https://pith.science/pith/SOL75WALWS3K5PMY7PHBVUF7VO/action/replication_record"}},"created_at":"2026-07-04T23:57:43.226310+00:00","updated_at":"2026-07-04T23:57:43.226310+00:00"}