{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:EMXRHWX6CDTX4HYO3SXHN2JJQP","short_pith_number":"pith:EMXRHWX6","schema_version":"1.0","canonical_sha256":"232f13dafe10e77e1f0edcae76e92983fbad95b09fa1e0c7df407142389cf17a","source":{"kind":"arxiv","id":"1305.1119","version":1},"attestation_state":"computed","paper":{"title":"Far-Infrared Spectroscopy of the Galactic Center. Hot Molecular Gas: Shocks versus Radiation near SgrA*","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Contursi, D. A. Neufeld, D. C. Lis, E. T. Polehampton, Javier R. Goicoechea, J. Cernicharo, M. De Luca, M. Etxaluze, M. Gerin, N. Indriolo, P. Encrenaz, P. Sonnentrucker, T. A. Bell","submitted_at":"2013-05-06T08:56:32Z","abstract_excerpt":"We present a 52-671um spectral scan toward SgrA* taken with the PACS and SPIRE spectrometers onboard Herschel. The achieved angular resolution allows us to separate, for the first time at far-IR wavelengths, the emission toward the central cavity (gas in the inner central parsec of the galaxy) from that of the surrounding circum-nuclear disk. The spectrum toward SgrA* is dominated by strong [OIII], [OI], [CII], [NIII], [NII], and [CI] fine structure lines (in decreasing order of luminosity) arising in gas irradiated by UV-photons from the central stellar cluster. In addition, rotationally exci"},"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":"1305.1119","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-05-06T08:56:32Z","cross_cats_sorted":[],"title_canon_sha256":"2c55bc4ae3b4106a477f046054b30b1c5cf5cc7e80c977ac81c6ed8a72581e09","abstract_canon_sha256":"e588c308de5fe08a8dccb6db48e5fda5d311edeca43ccae942ab509ccf513d69"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:50:11.936200Z","signature_b64":"KcbzuU617L+LnVpvHqsiOkLaxjvvIpGPlgs8TAwD8ue6DvxKW4k3M7b5Hn2CkCQE5K+3fOIS5443GjsrPg/KDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"232f13dafe10e77e1f0edcae76e92983fbad95b09fa1e0c7df407142389cf17a","last_reissued_at":"2026-05-18T01:50:11.935212Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:50:11.935212Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Far-Infrared Spectroscopy of the Galactic Center. Hot Molecular Gas: Shocks versus Radiation near SgrA*","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Contursi, D. A. Neufeld, D. C. Lis, E. T. Polehampton, Javier R. Goicoechea, J. Cernicharo, M. De Luca, M. Etxaluze, M. Gerin, N. Indriolo, P. Encrenaz, P. Sonnentrucker, T. A. Bell","submitted_at":"2013-05-06T08:56:32Z","abstract_excerpt":"We present a 52-671um spectral scan toward SgrA* taken with the PACS and SPIRE spectrometers onboard Herschel. The achieved angular resolution allows us to separate, for the first time at far-IR wavelengths, the emission toward the central cavity (gas in the inner central parsec of the galaxy) from that of the surrounding circum-nuclear disk. The spectrum toward SgrA* is dominated by strong [OIII], [OI], [CII], [NIII], [NII], and [CI] fine structure lines (in decreasing order of luminosity) arising in gas irradiated by UV-photons from the central stellar cluster. In addition, rotationally exci"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1305.1119","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":"1305.1119","created_at":"2026-05-18T01:50:11.935351+00:00"},{"alias_kind":"arxiv_version","alias_value":"1305.1119v1","created_at":"2026-05-18T01:50:11.935351+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1305.1119","created_at":"2026-05-18T01:50:11.935351+00:00"},{"alias_kind":"pith_short_12","alias_value":"EMXRHWX6CDTX","created_at":"2026-05-18T12:27:43.054852+00:00"},{"alias_kind":"pith_short_16","alias_value":"EMXRHWX6CDTX4HYO","created_at":"2026-05-18T12:27:43.054852+00:00"},{"alias_kind":"pith_short_8","alias_value":"EMXRHWX6","created_at":"2026-05-18T12:27:43.054852+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/EMXRHWX6CDTX4HYO3SXHN2JJQP","json":"https://pith.science/pith/EMXRHWX6CDTX4HYO3SXHN2JJQP.json","graph_json":"https://pith.science/api/pith-number/EMXRHWX6CDTX4HYO3SXHN2JJQP/graph.json","events_json":"https://pith.science/api/pith-number/EMXRHWX6CDTX4HYO3SXHN2JJQP/events.json","paper":"https://pith.science/paper/EMXRHWX6"},"agent_actions":{"view_html":"https://pith.science/pith/EMXRHWX6CDTX4HYO3SXHN2JJQP","download_json":"https://pith.science/pith/EMXRHWX6CDTX4HYO3SXHN2JJQP.json","view_paper":"https://pith.science/paper/EMXRHWX6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1305.1119&json=true","fetch_graph":"https://pith.science/api/pith-number/EMXRHWX6CDTX4HYO3SXHN2JJQP/graph.json","fetch_events":"https://pith.science/api/pith-number/EMXRHWX6CDTX4HYO3SXHN2JJQP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EMXRHWX6CDTX4HYO3SXHN2JJQP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EMXRHWX6CDTX4HYO3SXHN2JJQP/action/storage_attestation","attest_author":"https://pith.science/pith/EMXRHWX6CDTX4HYO3SXHN2JJQP/action/author_attestation","sign_citation":"https://pith.science/pith/EMXRHWX6CDTX4HYO3SXHN2JJQP/action/citation_signature","submit_replication":"https://pith.science/pith/EMXRHWX6CDTX4HYO3SXHN2JJQP/action/replication_record"}},"created_at":"2026-05-18T01:50:11.935351+00:00","updated_at":"2026-05-18T01:50:11.935351+00:00"}