{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:RKNW7BYOCOYP2K7JTC4UKC3LEC","short_pith_number":"pith:RKNW7BYO","schema_version":"1.0","canonical_sha256":"8a9b6f870e13b0fd2be998b9450b6b208210fcf6410d6810626acfd8e25e07e3","source":{"kind":"arxiv","id":"1005.1846","version":1},"attestation_state":"computed","paper":{"title":"Herschel-SPIRE spectroscopy of G29.96-0.02: fitting the full SED","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Abergel, A. Zavagno, B. Swinyard, C. Gry, C. Joblin, D.A. Naylor, D. Pinheiro Gocalvez, D. Russeil, D. Ward-Thompson, E. Dartois, E. Habart, E. Polehampton, F. Boulanger, F. Motte, G. Davis, G. J. White, G. Lagache, G. Makiwa, H. Arab, H. Moseley, J. A. Rodon, J.M. Kirk, J.-P. Baluteau, J.-P. Bernard, K. Blagrave, K. Okumura, L. D. Anderson, L. Spencer, M.-A. Miville-Deschenes, M. Cohen, M. Compiegne, M. Huang, P. Ade, P. Andre, P. Cox, P. Martin, P. Saraceno, R. Emery, S. Bontemps, S. C. Jones, S. Madden, S. Molinari, S. Sidher, T. Fulton, T. Lim","submitted_at":"2010-05-11T14:38:34Z","abstract_excerpt":"We use the SPIRE Fourier-Transform Spectrometer (FTS) on-board the ESA Herschel Space Telescope to analyse the submillimetre spectrum of the Ultra-compact HII region G29.96-0.02. Spectral lines from species including 13CO, CO, [CI], and [NII] are detected. A sparse map of the [NII] emission shows at least one other HII region neighbouring the clump containing the UCHII. The FTS spectra are combined with ISO SWS and LWS spectra and fluxes from the literature to present a detailed spectrum of the source spanning three orders of magnitude in wavelength. The quality of the spectrum longwards of 10"},"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":"1005.1846","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-05-11T14:38:34Z","cross_cats_sorted":[],"title_canon_sha256":"887a95649f5f203df393b26cb092a274504b258b486d0f2ded87692dcc9ed7f3","abstract_canon_sha256":"7ca9a7ed16a68e0a6648d21aa0b2b3695b4ab195cbdaeb0db066e7f80321f5db"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:07:34.229419Z","signature_b64":"4pYrQKevdfeklRkYsfpjG8uAQUxw2GI/dCJoqwe12R/HTS9nXmZj29mTh+ShkOS67w92s/ncxjmIJuaPeWdiAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8a9b6f870e13b0fd2be998b9450b6b208210fcf6410d6810626acfd8e25e07e3","last_reissued_at":"2026-05-18T02:07:34.229000Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:07:34.229000Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Herschel-SPIRE spectroscopy of G29.96-0.02: fitting the full SED","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Abergel, A. Zavagno, B. Swinyard, C. Gry, C. Joblin, D.A. Naylor, D. Pinheiro Gocalvez, D. Russeil, D. Ward-Thompson, E. Dartois, E. Habart, E. Polehampton, F. Boulanger, F. Motte, G. Davis, G. J. White, G. Lagache, G. Makiwa, H. Arab, H. Moseley, J. A. Rodon, J.M. Kirk, J.-P. Baluteau, J.-P. Bernard, K. Blagrave, K. Okumura, L. D. Anderson, L. Spencer, M.-A. Miville-Deschenes, M. Cohen, M. Compiegne, M. Huang, P. Ade, P. Andre, P. Cox, P. Martin, P. Saraceno, R. Emery, S. Bontemps, S. C. Jones, S. Madden, S. Molinari, S. Sidher, T. Fulton, T. Lim","submitted_at":"2010-05-11T14:38:34Z","abstract_excerpt":"We use the SPIRE Fourier-Transform Spectrometer (FTS) on-board the ESA Herschel Space Telescope to analyse the submillimetre spectrum of the Ultra-compact HII region G29.96-0.02. Spectral lines from species including 13CO, CO, [CI], and [NII] are detected. A sparse map of the [NII] emission shows at least one other HII region neighbouring the clump containing the UCHII. The FTS spectra are combined with ISO SWS and LWS spectra and fluxes from the literature to present a detailed spectrum of the source spanning three orders of magnitude in wavelength. The quality of the spectrum longwards of 10"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.1846","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":"1005.1846","created_at":"2026-05-18T02:07:34.229051+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.1846v1","created_at":"2026-05-18T02:07:34.229051+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.1846","created_at":"2026-05-18T02:07:34.229051+00:00"},{"alias_kind":"pith_short_12","alias_value":"RKNW7BYOCOYP","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_16","alias_value":"RKNW7BYOCOYP2K7J","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_8","alias_value":"RKNW7BYO","created_at":"2026-05-18T12:26:13.927090+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/RKNW7BYOCOYP2K7JTC4UKC3LEC","json":"https://pith.science/pith/RKNW7BYOCOYP2K7JTC4UKC3LEC.json","graph_json":"https://pith.science/api/pith-number/RKNW7BYOCOYP2K7JTC4UKC3LEC/graph.json","events_json":"https://pith.science/api/pith-number/RKNW7BYOCOYP2K7JTC4UKC3LEC/events.json","paper":"https://pith.science/paper/RKNW7BYO"},"agent_actions":{"view_html":"https://pith.science/pith/RKNW7BYOCOYP2K7JTC4UKC3LEC","download_json":"https://pith.science/pith/RKNW7BYOCOYP2K7JTC4UKC3LEC.json","view_paper":"https://pith.science/paper/RKNW7BYO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.1846&json=true","fetch_graph":"https://pith.science/api/pith-number/RKNW7BYOCOYP2K7JTC4UKC3LEC/graph.json","fetch_events":"https://pith.science/api/pith-number/RKNW7BYOCOYP2K7JTC4UKC3LEC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RKNW7BYOCOYP2K7JTC4UKC3LEC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RKNW7BYOCOYP2K7JTC4UKC3LEC/action/storage_attestation","attest_author":"https://pith.science/pith/RKNW7BYOCOYP2K7JTC4UKC3LEC/action/author_attestation","sign_citation":"https://pith.science/pith/RKNW7BYOCOYP2K7JTC4UKC3LEC/action/citation_signature","submit_replication":"https://pith.science/pith/RKNW7BYOCOYP2K7JTC4UKC3LEC/action/replication_record"}},"created_at":"2026-05-18T02:07:34.229051+00:00","updated_at":"2026-05-18T02:07:34.229051+00:00"}