{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:OKFLWH2U45OV5MCNOIP5JNKIBU","short_pith_number":"pith:OKFLWH2U","schema_version":"1.0","canonical_sha256":"728abb1f54e75d5eb04d721fd4b5480d1620e22660a2ee23775391c1b698e00e","source":{"kind":"arxiv","id":"2002.04040","version":1},"attestation_state":"computed","paper":{"title":"ALMA reveals the molecular gas properties of 5 star-forming galaxies across the main sequence at 3 < z < 3.5","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Alexander Karim, Andrea Enia, Brent Groves, Brian C. Lemaux, Bruno Ribeiro, Chiara Mancini, Daizhong Liu, Eduardo Ibar, Eva Schinnerer, Giulia Rodighiero, Laura Morselli, Lidia Tasca, Lucia Rodriguez-Munoz, Margherita Talia, Mark Sargent, Michael Romano, Olivier Le Fevre, Paolo Cassata, Stefano Fiore, Vernesa Smolcic","submitted_at":"2020-02-10T19:00:04Z","abstract_excerpt":"We present the detection of CO(5-4) with S/N> 7 - 13 and a lower CO transition with S/N > 3 (CO(4-3) for 4 galaxies, and CO(3-2) for one) with ALMA in band 3 and 4 in five main sequence star-forming galaxies with stellar masses 3-6x10^10 M/M_sun at 3 < z < 3.5. We find a good correlation between the total far-infrared luminosity LFIR and the luminosity of the CO(5-4) transition L'CO(5-4), where L'CO(5-4) increases with SFR, indicating that CO(5-4) is a good tracer of the obscured SFR in these galaxies. The two galaxies that lie closer to the star-forming main sequence have CO SLED slopes that "},"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":"2002.04040","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-02-10T19:00:04Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"7d73bf29a68c9b5b9b863808fd541e40fc861e46ac942eef92ccae25182fc0ab","abstract_canon_sha256":"9a31b032558cc249da264c31c5554147fb88f4e60b9742bf90902c06454c929d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:48:55.870989Z","signature_b64":"oQNV8ib02FhiiAoZKBsES8JByWvc22D4RUIvmL0N4683Fx8bj+SybjKQ9sFRKMgTZ/AKBykIUonOxE/TEYJ/Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"728abb1f54e75d5eb04d721fd4b5480d1620e22660a2ee23775391c1b698e00e","last_reissued_at":"2026-07-05T00:48:55.870398Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:48:55.870398Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ALMA reveals the molecular gas properties of 5 star-forming galaxies across the main sequence at 3 < z < 3.5","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Alexander Karim, Andrea Enia, Brent Groves, Brian C. Lemaux, Bruno Ribeiro, Chiara Mancini, Daizhong Liu, Eduardo Ibar, Eva Schinnerer, Giulia Rodighiero, Laura Morselli, Lidia Tasca, Lucia Rodriguez-Munoz, Margherita Talia, Mark Sargent, Michael Romano, Olivier Le Fevre, Paolo Cassata, Stefano Fiore, Vernesa Smolcic","submitted_at":"2020-02-10T19:00:04Z","abstract_excerpt":"We present the detection of CO(5-4) with S/N> 7 - 13 and a lower CO transition with S/N > 3 (CO(4-3) for 4 galaxies, and CO(3-2) for one) with ALMA in band 3 and 4 in five main sequence star-forming galaxies with stellar masses 3-6x10^10 M/M_sun at 3 < z < 3.5. We find a good correlation between the total far-infrared luminosity LFIR and the luminosity of the CO(5-4) transition L'CO(5-4), where L'CO(5-4) increases with SFR, indicating that CO(5-4) is a good tracer of the obscured SFR in these galaxies. The two galaxies that lie closer to the star-forming main sequence have CO SLED slopes that "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2002.04040","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/2002.04040/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":"2002.04040","created_at":"2026-07-05T00:48:55.870480+00:00"},{"alias_kind":"arxiv_version","alias_value":"2002.04040v1","created_at":"2026-07-05T00:48:55.870480+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2002.04040","created_at":"2026-07-05T00:48:55.870480+00:00"},{"alias_kind":"pith_short_12","alias_value":"OKFLWH2U45OV","created_at":"2026-07-05T00:48:55.870480+00:00"},{"alias_kind":"pith_short_16","alias_value":"OKFLWH2U45OV5MCN","created_at":"2026-07-05T00:48:55.870480+00:00"},{"alias_kind":"pith_short_8","alias_value":"OKFLWH2U","created_at":"2026-07-05T00:48:55.870480+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/OKFLWH2U45OV5MCNOIP5JNKIBU","json":"https://pith.science/pith/OKFLWH2U45OV5MCNOIP5JNKIBU.json","graph_json":"https://pith.science/api/pith-number/OKFLWH2U45OV5MCNOIP5JNKIBU/graph.json","events_json":"https://pith.science/api/pith-number/OKFLWH2U45OV5MCNOIP5JNKIBU/events.json","paper":"https://pith.science/paper/OKFLWH2U"},"agent_actions":{"view_html":"https://pith.science/pith/OKFLWH2U45OV5MCNOIP5JNKIBU","download_json":"https://pith.science/pith/OKFLWH2U45OV5MCNOIP5JNKIBU.json","view_paper":"https://pith.science/paper/OKFLWH2U","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2002.04040&json=true","fetch_graph":"https://pith.science/api/pith-number/OKFLWH2U45OV5MCNOIP5JNKIBU/graph.json","fetch_events":"https://pith.science/api/pith-number/OKFLWH2U45OV5MCNOIP5JNKIBU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OKFLWH2U45OV5MCNOIP5JNKIBU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OKFLWH2U45OV5MCNOIP5JNKIBU/action/storage_attestation","attest_author":"https://pith.science/pith/OKFLWH2U45OV5MCNOIP5JNKIBU/action/author_attestation","sign_citation":"https://pith.science/pith/OKFLWH2U45OV5MCNOIP5JNKIBU/action/citation_signature","submit_replication":"https://pith.science/pith/OKFLWH2U45OV5MCNOIP5JNKIBU/action/replication_record"}},"created_at":"2026-07-05T00:48:55.870480+00:00","updated_at":"2026-07-05T00:48:55.870480+00:00"}