{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:W6JBFRWTEDPUK2SUCP72WGZT6U","short_pith_number":"pith:W6JBFRWT","schema_version":"1.0","canonical_sha256":"b79212c6d320df456a5413ffab1b33f50ea2d1f545813ce9d32653c5f564e4ef","source":{"kind":"arxiv","id":"1803.11522","version":1},"attestation_state":"computed","paper":{"title":"The CARMA-NRO Orion Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"(10) Max-Planck-Institut f\\\"ur extraterrestrische Physik, (11) Department of Physics, (12) Department of Astrophysical, (13) Sorbonne Universit\\'e, 14), (14) California Institute of Technology, (15) Institut de Ci\\'encies del Cosmos, 16), (16) ICREA, (17) Universit\\\"at Heidelberg, 18), (18) Universit\\\"at Heidelberg, (19) East Asian Observatory, (20) Harvard-Smithsonian Center for Astrophysics, (21) Jet Propulsion Laboratory, (22) Department of Earth, (23) Astronomy Department, (24) Department of Astronomy, (25) National Radio Astronomy Observatory, (26) Institute for Theory, (27) Jodrell Bank Centre for Astrophysics, (28) Department of Physics, (29) Japan Womens University, (2) Joint ALMA Observatory, (30) College of Science, (3) National Astronomical Observatory of Japan, (4) Laboratoire AIM, (5) Department of Physics, 6), (6) I. Physikalisches Institut, (7) California Institute of Technology, (8) Haystack Observatory, (9) Max-Planck-Institut f\\\"ur Radioastronomie, Adam Ginsburg (25), \\'Alvaro S\\'anchez-Monge (6), Alyssa Goodman (20), Andrea Isella (5), Anika Schmiedeke (10, Anneila I. Sargent (7), Astronomy, Astrophysics 249-17, Astrophysics 301-17, Blakesley Burkhart (26), Cahill Center for Astronomy, California Institute of Technology, CEA/DSM-CNRS-Universit\\'e Paris Diderot, Chihomi Hara (24), Chile, CNRS, College of the Canyons, Computation, Dariusz C. Lis (13, Environment Sciences, France, Fumitaka Nakamura (3), Germany, Harvard-Smithsonian Center for Astrophysics, H\\'ector G. Arce (1), Ibaraki University, Interdisziplin\\\"ares Zentrum f\\\"ur Wissenschaftliches Rechnen, IRFU/Service d'Astrophysique, Jaime E. Pineda (10), Japan, Japan), Jens Kauffmann (8), Jesse R. Feddersen (1), Jin Koda (11), John Bally (12), John M. Carpenter (2), Jorge L. Pineda (21), Kazushige Sasaki (28), LERMA, Mar\\'ia Jos\\'e Maureira (1), Massachusetts Institute of Technology, Niigata University, Observatoire de Paris, Paolo Padoan (15, Paul Goldsmith (21), Peregrine McGehee (22), Peter J. Teuben (23), Peter Schilke (6), Pg. Llu\\'is Companys 23, Planetary Sciences, Ralf Klessen (17, Rice University, Rowan J. Smith (27), Ryohei Kawabe (3), School of Physics, Shun Ishii (2), Shuo Kong (1), Shuri Oyamada (29), Space, Spain, Steve Mairs (19), Stony Brook University, S\\\"umeyye T. Suri (6), The University of Tokyo, Thushara Pillai (9), UK, Universitat de Barcelona, Universit\\\"at zu K\\\"oln, Universit\\'e PSL, University of Colorado, University of Manchester, University of Maryland, USA, Volker Ossenkopf-Okada (6), Yale University, Yoshihiro Tanabe (30) ((1) Department of Astronomy, Yoshito Shimajiri (4), Yumiko Urasawa (28), Zentrum f\\\"ur Astronomie","submitted_at":"2018-03-30T15:54:54Z","abstract_excerpt":"We present the first results from a new, high resolution, $^{12}$CO(1-0), $^{13}$CO(1-0), and C$^{18}$O(1-0) molecular line survey of the Orion A cloud, hereafter referred to as the CARMA-NRO Orion Survey. CARMA observations have been combined with single-dish data from the Nobeyama 45m telescope to provide extended images at about 0.01 pc resolution, with a dynamic range of approximately 1200 in spatial scale. Here we describe the practical details of the data combination in uv space, including flux scale matching, the conversion of single dish data to visibilities, and joint deconvolution of"},"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":"1803.11522","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-03-30T15:54:54Z","cross_cats_sorted":[],"title_canon_sha256":"b8869dce9a8461a382cbfa5431f86ea45d62226f17bee415d56cddebc67f53de","abstract_canon_sha256":"1ba55e4da15f5ad097732b3aee4f80e75a500069d632c4dd174e6778303964d5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:15:15.022515Z","signature_b64":"cGVg9vFoUW/7RXqz5KqhDn+WV8FBpNVkqWa1tHykbq+cIMLZ2vHIfyXDOewjJ/HK9AfeLsOx5Io8uLcMoSnTCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b79212c6d320df456a5413ffab1b33f50ea2d1f545813ce9d32653c5f564e4ef","last_reissued_at":"2026-05-18T00:15:15.021756Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:15:15.021756Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The CARMA-NRO Orion Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"(10) Max-Planck-Institut f\\\"ur extraterrestrische Physik, (11) Department of Physics, (12) Department of Astrophysical, (13) Sorbonne Universit\\'e, 14), (14) California Institute of Technology, (15) Institut de Ci\\'encies del Cosmos, 16), (16) ICREA, (17) Universit\\\"at Heidelberg, 18), (18) Universit\\\"at Heidelberg, (19) East Asian Observatory, (20) Harvard-Smithsonian Center for Astrophysics, (21) Jet Propulsion Laboratory, (22) Department of Earth, (23) Astronomy Department, (24) Department of Astronomy, (25) National Radio Astronomy Observatory, (26) Institute for Theory, (27) Jodrell Bank Centre for Astrophysics, (28) Department of Physics, (29) Japan Womens University, (2) Joint ALMA Observatory, (30) College of Science, (3) National Astronomical Observatory of Japan, (4) Laboratoire AIM, (5) Department of Physics, 6), (6) I. Physikalisches Institut, (7) California Institute of Technology, (8) Haystack Observatory, (9) Max-Planck-Institut f\\\"ur Radioastronomie, Adam Ginsburg (25), \\'Alvaro S\\'anchez-Monge (6), Alyssa Goodman (20), Andrea Isella (5), Anika Schmiedeke (10, Anneila I. Sargent (7), Astronomy, Astrophysics 249-17, Astrophysics 301-17, Blakesley Burkhart (26), Cahill Center for Astronomy, California Institute of Technology, CEA/DSM-CNRS-Universit\\'e Paris Diderot, Chihomi Hara (24), Chile, CNRS, College of the Canyons, Computation, Dariusz C. Lis (13, Environment Sciences, France, Fumitaka Nakamura (3), Germany, Harvard-Smithsonian Center for Astrophysics, H\\'ector G. Arce (1), Ibaraki University, Interdisziplin\\\"ares Zentrum f\\\"ur Wissenschaftliches Rechnen, IRFU/Service d'Astrophysique, Jaime E. Pineda (10), Japan, Japan), Jens Kauffmann (8), Jesse R. Feddersen (1), Jin Koda (11), John Bally (12), John M. Carpenter (2), Jorge L. Pineda (21), Kazushige Sasaki (28), LERMA, Mar\\'ia Jos\\'e Maureira (1), Massachusetts Institute of Technology, Niigata University, Observatoire de Paris, Paolo Padoan (15, Paul Goldsmith (21), Peregrine McGehee (22), Peter J. Teuben (23), Peter Schilke (6), Pg. Llu\\'is Companys 23, Planetary Sciences, Ralf Klessen (17, Rice University, Rowan J. Smith (27), Ryohei Kawabe (3), School of Physics, Shun Ishii (2), Shuo Kong (1), Shuri Oyamada (29), Space, Spain, Steve Mairs (19), Stony Brook University, S\\\"umeyye T. Suri (6), The University of Tokyo, Thushara Pillai (9), UK, Universitat de Barcelona, Universit\\\"at zu K\\\"oln, Universit\\'e PSL, University of Colorado, University of Manchester, University of Maryland, USA, Volker Ossenkopf-Okada (6), Yale University, Yoshihiro Tanabe (30) ((1) Department of Astronomy, Yoshito Shimajiri (4), Yumiko Urasawa (28), Zentrum f\\\"ur Astronomie","submitted_at":"2018-03-30T15:54:54Z","abstract_excerpt":"We present the first results from a new, high resolution, $^{12}$CO(1-0), $^{13}$CO(1-0), and C$^{18}$O(1-0) molecular line survey of the Orion A cloud, hereafter referred to as the CARMA-NRO Orion Survey. CARMA observations have been combined with single-dish data from the Nobeyama 45m telescope to provide extended images at about 0.01 pc resolution, with a dynamic range of approximately 1200 in spatial scale. Here we describe the practical details of the data combination in uv space, including flux scale matching, the conversion of single dish data to visibilities, and joint deconvolution of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1803.11522","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":"1803.11522","created_at":"2026-05-18T00:15:15.021888+00:00"},{"alias_kind":"arxiv_version","alias_value":"1803.11522v1","created_at":"2026-05-18T00:15:15.021888+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1803.11522","created_at":"2026-05-18T00:15:15.021888+00:00"},{"alias_kind":"pith_short_12","alias_value":"W6JBFRWTEDPU","created_at":"2026-05-18T12:32:59.047623+00:00"},{"alias_kind":"pith_short_16","alias_value":"W6JBFRWTEDPUK2SU","created_at":"2026-05-18T12:32:59.047623+00:00"},{"alias_kind":"pith_short_8","alias_value":"W6JBFRWT","created_at":"2026-05-18T12:32:59.047623+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/W6JBFRWTEDPUK2SUCP72WGZT6U","json":"https://pith.science/pith/W6JBFRWTEDPUK2SUCP72WGZT6U.json","graph_json":"https://pith.science/api/pith-number/W6JBFRWTEDPUK2SUCP72WGZT6U/graph.json","events_json":"https://pith.science/api/pith-number/W6JBFRWTEDPUK2SUCP72WGZT6U/events.json","paper":"https://pith.science/paper/W6JBFRWT"},"agent_actions":{"view_html":"https://pith.science/pith/W6JBFRWTEDPUK2SUCP72WGZT6U","download_json":"https://pith.science/pith/W6JBFRWTEDPUK2SUCP72WGZT6U.json","view_paper":"https://pith.science/paper/W6JBFRWT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1803.11522&json=true","fetch_graph":"https://pith.science/api/pith-number/W6JBFRWTEDPUK2SUCP72WGZT6U/graph.json","fetch_events":"https://pith.science/api/pith-number/W6JBFRWTEDPUK2SUCP72WGZT6U/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/W6JBFRWTEDPUK2SUCP72WGZT6U/action/timestamp_anchor","attest_storage":"https://pith.science/pith/W6JBFRWTEDPUK2SUCP72WGZT6U/action/storage_attestation","attest_author":"https://pith.science/pith/W6JBFRWTEDPUK2SUCP72WGZT6U/action/author_attestation","sign_citation":"https://pith.science/pith/W6JBFRWTEDPUK2SUCP72WGZT6U/action/citation_signature","submit_replication":"https://pith.science/pith/W6JBFRWTEDPUK2SUCP72WGZT6U/action/replication_record"}},"created_at":"2026-05-18T00:15:15.021888+00:00","updated_at":"2026-05-18T00:15:15.021888+00:00"}