{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:OKPC4KA3AYDP37JNHFRH4XJ5D2","short_pith_number":"pith:OKPC4KA3","schema_version":"1.0","canonical_sha256":"729e2e281b0606fdfd2d39627e5d3d1ea7419ae40683a5ea958fb06b5d976678","source":{"kind":"arxiv","id":"1403.4249","version":1},"attestation_state":"computed","paper":{"title":"A $10^{10}$ Solar Mass Flow of Molecular Gas in the Abell 1835 Brightest Cluster Galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. C. Edge, A. C. Fabian, A. N. Vantyghem, B. R. McNamara, C.C. Kirkpatrick, C. P. O'Dea, E. Egami, F. Combes, G.M. Voit, G. Tremblay, H.R. Russell, J.B.R. Oonk, J. N. Bregman, M. Donahue, N. W. Murray, P. E. J. Nulsen, P. Salome, R. A. Main, S. A. Baum, S. Hamer","submitted_at":"2014-03-17T20:00:26Z","abstract_excerpt":"We report ALMA Early Science observations of the Abell 1835 brightest cluster galaxy (BCG) in the CO (3-2) and CO (1-0) emission lines. We detect $5\\times 10^{10}~\\rm M_\\odot$ of molecular gas within 10 kpc of the BCG. Its ensemble velocity profile width of $\\sim 130 ~\\rm km~s^{-1}$ FWHM is too narrow for the molecular cloud sto be supported in the galaxy by dynamic pressure. The gas may instead be supported in a rotating, turbulent disk oriented nearly face-on. Roughly $10^{10}~\\rm M_\\odot$ of molecular gas is projected $3-10 ~\\rm kpc$ to the north-west and to the east of the nucleus with lin"},"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":"1403.4249","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-03-17T20:00:26Z","cross_cats_sorted":[],"title_canon_sha256":"908c5af3879d80b4768456db2249230adc527bcbde6ac3414086b657c0a0f167","abstract_canon_sha256":"ba89b1b24edac0923f7068529f0f8753a0dccca77922ea14940622136f589fac"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:56:06.124950Z","signature_b64":"+/Zk8so9AFeOWCcn5Pa3o/j2QRhKT+7WKfytahLDSyDv3JZm+aLrBVaSVYOwp/Q+CcFMEECAtnMZuQP5lf9JAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"729e2e281b0606fdfd2d39627e5d3d1ea7419ae40683a5ea958fb06b5d976678","last_reissued_at":"2026-05-18T02:56:06.124488Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:56:06.124488Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A $10^{10}$ Solar Mass Flow of Molecular Gas in the Abell 1835 Brightest Cluster Galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. C. Edge, A. C. Fabian, A. N. Vantyghem, B. R. McNamara, C.C. Kirkpatrick, C. P. O'Dea, E. Egami, F. Combes, G.M. Voit, G. Tremblay, H.R. Russell, J.B.R. Oonk, J. N. Bregman, M. Donahue, N. W. Murray, P. E. J. Nulsen, P. Salome, R. A. Main, S. A. Baum, S. Hamer","submitted_at":"2014-03-17T20:00:26Z","abstract_excerpt":"We report ALMA Early Science observations of the Abell 1835 brightest cluster galaxy (BCG) in the CO (3-2) and CO (1-0) emission lines. We detect $5\\times 10^{10}~\\rm M_\\odot$ of molecular gas within 10 kpc of the BCG. Its ensemble velocity profile width of $\\sim 130 ~\\rm km~s^{-1}$ FWHM is too narrow for the molecular cloud sto be supported in the galaxy by dynamic pressure. The gas may instead be supported in a rotating, turbulent disk oriented nearly face-on. Roughly $10^{10}~\\rm M_\\odot$ of molecular gas is projected $3-10 ~\\rm kpc$ to the north-west and to the east of the nucleus with lin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.4249","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":""},"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":"1403.4249","created_at":"2026-05-18T02:56:06.124554+00:00"},{"alias_kind":"arxiv_version","alias_value":"1403.4249v1","created_at":"2026-05-18T02:56:06.124554+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.4249","created_at":"2026-05-18T02:56:06.124554+00:00"},{"alias_kind":"pith_short_12","alias_value":"OKPC4KA3AYDP","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_16","alias_value":"OKPC4KA3AYDP37JN","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_8","alias_value":"OKPC4KA3","created_at":"2026-05-18T12:28:41.024544+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/OKPC4KA3AYDP37JNHFRH4XJ5D2","json":"https://pith.science/pith/OKPC4KA3AYDP37JNHFRH4XJ5D2.json","graph_json":"https://pith.science/api/pith-number/OKPC4KA3AYDP37JNHFRH4XJ5D2/graph.json","events_json":"https://pith.science/api/pith-number/OKPC4KA3AYDP37JNHFRH4XJ5D2/events.json","paper":"https://pith.science/paper/OKPC4KA3"},"agent_actions":{"view_html":"https://pith.science/pith/OKPC4KA3AYDP37JNHFRH4XJ5D2","download_json":"https://pith.science/pith/OKPC4KA3AYDP37JNHFRH4XJ5D2.json","view_paper":"https://pith.science/paper/OKPC4KA3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1403.4249&json=true","fetch_graph":"https://pith.science/api/pith-number/OKPC4KA3AYDP37JNHFRH4XJ5D2/graph.json","fetch_events":"https://pith.science/api/pith-number/OKPC4KA3AYDP37JNHFRH4XJ5D2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OKPC4KA3AYDP37JNHFRH4XJ5D2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OKPC4KA3AYDP37JNHFRH4XJ5D2/action/storage_attestation","attest_author":"https://pith.science/pith/OKPC4KA3AYDP37JNHFRH4XJ5D2/action/author_attestation","sign_citation":"https://pith.science/pith/OKPC4KA3AYDP37JNHFRH4XJ5D2/action/citation_signature","submit_replication":"https://pith.science/pith/OKPC4KA3AYDP37JNHFRH4XJ5D2/action/replication_record"}},"created_at":"2026-05-18T02:56:06.124554+00:00","updated_at":"2026-05-18T02:56:06.124554+00:00"}