{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:BMW5OOEB4TM2XILTTTMIGWOTEP","short_pith_number":"pith:BMW5OOEB","schema_version":"1.0","canonical_sha256":"0b2dd73881e4d9aba1739cd88359d323cf9b0190f608feade126b2f7a7a5d7d4","source":{"kind":"arxiv","id":"1811.02967","version":1},"attestation_state":"computed","paper":{"title":"ALMA observations of massive molecular gas reservoirs in dusty early-type galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. E. Sansom, C. Popescu, D. H. W. Glass, G. J. Bendo, K. Rowlands, L. Dunne, M. Smith, N. Bourne, S. Eales, S. Kaviraj, S. Viaene, T. A. Davis","submitted_at":"2018-11-07T16:32:30Z","abstract_excerpt":"Unresolved gas and dust observations show a surprising diversity in the amount of interstellar matter in early-type galaxies. Using ALMA observations we resolve the ISM in z$\\sim$0.05 early-type galaxies. From a large sample of early-type galaxies detected in the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) we selected five of the dustiest cases, with dust masses M$_d\\sim$several$\\times10^7$M$_\\odot$, with the aim of mapping their submillimetre continuum and $^{12}$CO(2-1) line emission distributions. These observations reveal molecular gas disks. There is a lack of associated,"},"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":"1811.02967","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-11-07T16:32:30Z","cross_cats_sorted":[],"title_canon_sha256":"5544d991351bb6077691eaa850c966dff8d65f22db65f3a503020cc65483594c","abstract_canon_sha256":"e21a0f8bd6e657509e6e245e4373369a845cf87b706726db1aa405a835966290"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:01:20.259082Z","signature_b64":"2xXw119BLxdvAHpkaEVfIXqbgvXoUy23EaDV0JMjiCSyW8wlmP6Z7cvtl/fOz/XTUhhuwu8r1uRp7pxtX+SyDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0b2dd73881e4d9aba1739cd88359d323cf9b0190f608feade126b2f7a7a5d7d4","last_reissued_at":"2026-05-18T00:01:20.258464Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:01:20.258464Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ALMA observations of massive molecular gas reservoirs in dusty early-type galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. E. Sansom, C. Popescu, D. H. W. Glass, G. J. Bendo, K. Rowlands, L. Dunne, M. Smith, N. Bourne, S. Eales, S. Kaviraj, S. Viaene, T. A. Davis","submitted_at":"2018-11-07T16:32:30Z","abstract_excerpt":"Unresolved gas and dust observations show a surprising diversity in the amount of interstellar matter in early-type galaxies. Using ALMA observations we resolve the ISM in z$\\sim$0.05 early-type galaxies. From a large sample of early-type galaxies detected in the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) we selected five of the dustiest cases, with dust masses M$_d\\sim$several$\\times10^7$M$_\\odot$, with the aim of mapping their submillimetre continuum and $^{12}$CO(2-1) line emission distributions. These observations reveal molecular gas disks. There is a lack of associated,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.02967","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":"1811.02967","created_at":"2026-05-18T00:01:20.258540+00:00"},{"alias_kind":"arxiv_version","alias_value":"1811.02967v1","created_at":"2026-05-18T00:01:20.258540+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1811.02967","created_at":"2026-05-18T00:01:20.258540+00:00"},{"alias_kind":"pith_short_12","alias_value":"BMW5OOEB4TM2","created_at":"2026-05-18T12:32:16.446611+00:00"},{"alias_kind":"pith_short_16","alias_value":"BMW5OOEB4TM2XILT","created_at":"2026-05-18T12:32:16.446611+00:00"},{"alias_kind":"pith_short_8","alias_value":"BMW5OOEB","created_at":"2026-05-18T12:32:16.446611+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/BMW5OOEB4TM2XILTTTMIGWOTEP","json":"https://pith.science/pith/BMW5OOEB4TM2XILTTTMIGWOTEP.json","graph_json":"https://pith.science/api/pith-number/BMW5OOEB4TM2XILTTTMIGWOTEP/graph.json","events_json":"https://pith.science/api/pith-number/BMW5OOEB4TM2XILTTTMIGWOTEP/events.json","paper":"https://pith.science/paper/BMW5OOEB"},"agent_actions":{"view_html":"https://pith.science/pith/BMW5OOEB4TM2XILTTTMIGWOTEP","download_json":"https://pith.science/pith/BMW5OOEB4TM2XILTTTMIGWOTEP.json","view_paper":"https://pith.science/paper/BMW5OOEB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1811.02967&json=true","fetch_graph":"https://pith.science/api/pith-number/BMW5OOEB4TM2XILTTTMIGWOTEP/graph.json","fetch_events":"https://pith.science/api/pith-number/BMW5OOEB4TM2XILTTTMIGWOTEP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BMW5OOEB4TM2XILTTTMIGWOTEP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BMW5OOEB4TM2XILTTTMIGWOTEP/action/storage_attestation","attest_author":"https://pith.science/pith/BMW5OOEB4TM2XILTTTMIGWOTEP/action/author_attestation","sign_citation":"https://pith.science/pith/BMW5OOEB4TM2XILTTTMIGWOTEP/action/citation_signature","submit_replication":"https://pith.science/pith/BMW5OOEB4TM2XILTTTMIGWOTEP/action/replication_record"}},"created_at":"2026-05-18T00:01:20.258540+00:00","updated_at":"2026-05-18T00:01:20.258540+00:00"}