{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:KTPYXVWSY22FOXWY6Q2FRBOQGA","short_pith_number":"pith:KTPYXVWS","schema_version":"1.0","canonical_sha256":"54df8bd6d2c6b4575ed8f4345885d0302da5852f167fcdf8b0a9ff4c59cdcf1c","source":{"kind":"arxiv","id":"1005.4965","version":1},"attestation_state":"computed","paper":{"title":"Cold molecular gas in massive disk galaxies at z=1.5","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Chris L. Carilli, Daniel Stern, Dominik Riechers, Emanuele Daddi, Fabian Walter, Glenn E. Morrison, Helmut Dannerbauer, Jeff Wagg, Manuel Aravena, Melanie Krips","submitted_at":"2010-05-26T23:38:58Z","abstract_excerpt":"We report the detection of the CO J=1-0 emission line in three near-infrared selected star-forming galaxies at z~1.5 with the Very Large Array (VLA) and the Green Bank telescope (GBT). These observations directly trace the bulk of molecular gas in these galaxies. We find H_2 gas masses of 8.3 \\pm 1.9 x 10^{10} M_sun, 5.6 \\pm 1.4 x 10^{10} M_sun and 1.23 \\pm 0.34 x 10^{11} M_sun for BzK-4171, BzK-21000 and BzK-16000, respectively, assuming a conversion alpha_CO=3.6 M_sun (K km s^{-1} pc^{2})^{-1}. We combined our observations with previous CO 2-1 detections of these galaxies to study the proper"},"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":"1005.4965","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-05-26T23:38:58Z","cross_cats_sorted":[],"title_canon_sha256":"bdcc766b2bd2ca242099baab930988cdaf88c4d661fc340e650340319b8905d7","abstract_canon_sha256":"ea7726d4ad8f7ea66bff03552ed667a55768b392cde0a0cf003e4ad24d841df7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:07:07.560931Z","signature_b64":"S7sR4EEniQTkHQ5JK9SxHINAS00T0cJEuOxQiojFRz3LbKXv8uuGfS+ZaTZtRGuejIomz4t4XSr2Dv5EOOtgDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"54df8bd6d2c6b4575ed8f4345885d0302da5852f167fcdf8b0a9ff4c59cdcf1c","last_reissued_at":"2026-05-18T02:07:07.560274Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:07:07.560274Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cold molecular gas in massive disk galaxies at z=1.5","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Chris L. Carilli, Daniel Stern, Dominik Riechers, Emanuele Daddi, Fabian Walter, Glenn E. Morrison, Helmut Dannerbauer, Jeff Wagg, Manuel Aravena, Melanie Krips","submitted_at":"2010-05-26T23:38:58Z","abstract_excerpt":"We report the detection of the CO J=1-0 emission line in three near-infrared selected star-forming galaxies at z~1.5 with the Very Large Array (VLA) and the Green Bank telescope (GBT). These observations directly trace the bulk of molecular gas in these galaxies. We find H_2 gas masses of 8.3 \\pm 1.9 x 10^{10} M_sun, 5.6 \\pm 1.4 x 10^{10} M_sun and 1.23 \\pm 0.34 x 10^{11} M_sun for BzK-4171, BzK-21000 and BzK-16000, respectively, assuming a conversion alpha_CO=3.6 M_sun (K km s^{-1} pc^{2})^{-1}. We combined our observations with previous CO 2-1 detections of these galaxies to study the proper"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.4965","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":"1005.4965","created_at":"2026-05-18T02:07:07.560411+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.4965v1","created_at":"2026-05-18T02:07:07.560411+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.4965","created_at":"2026-05-18T02:07:07.560411+00:00"},{"alias_kind":"pith_short_12","alias_value":"KTPYXVWSY22F","created_at":"2026-05-18T12:26:09.077623+00:00"},{"alias_kind":"pith_short_16","alias_value":"KTPYXVWSY22FOXWY","created_at":"2026-05-18T12:26:09.077623+00:00"},{"alias_kind":"pith_short_8","alias_value":"KTPYXVWS","created_at":"2026-05-18T12:26:09.077623+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/KTPYXVWSY22FOXWY6Q2FRBOQGA","json":"https://pith.science/pith/KTPYXVWSY22FOXWY6Q2FRBOQGA.json","graph_json":"https://pith.science/api/pith-number/KTPYXVWSY22FOXWY6Q2FRBOQGA/graph.json","events_json":"https://pith.science/api/pith-number/KTPYXVWSY22FOXWY6Q2FRBOQGA/events.json","paper":"https://pith.science/paper/KTPYXVWS"},"agent_actions":{"view_html":"https://pith.science/pith/KTPYXVWSY22FOXWY6Q2FRBOQGA","download_json":"https://pith.science/pith/KTPYXVWSY22FOXWY6Q2FRBOQGA.json","view_paper":"https://pith.science/paper/KTPYXVWS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.4965&json=true","fetch_graph":"https://pith.science/api/pith-number/KTPYXVWSY22FOXWY6Q2FRBOQGA/graph.json","fetch_events":"https://pith.science/api/pith-number/KTPYXVWSY22FOXWY6Q2FRBOQGA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KTPYXVWSY22FOXWY6Q2FRBOQGA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KTPYXVWSY22FOXWY6Q2FRBOQGA/action/storage_attestation","attest_author":"https://pith.science/pith/KTPYXVWSY22FOXWY6Q2FRBOQGA/action/author_attestation","sign_citation":"https://pith.science/pith/KTPYXVWSY22FOXWY6Q2FRBOQGA/action/citation_signature","submit_replication":"https://pith.science/pith/KTPYXVWSY22FOXWY6Q2FRBOQGA/action/replication_record"}},"created_at":"2026-05-18T02:07:07.560411+00:00","updated_at":"2026-05-18T02:07:07.560411+00:00"}