{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:K62XUSEUGC6CTVAX5T4CQ4CTMT","short_pith_number":"pith:K62XUSEU","schema_version":"1.0","canonical_sha256":"57b57a489430bc29d417ecf828705364c694190413a6167f9b93b50108e008af","source":{"kind":"arxiv","id":"astro-ph/0107092","version":1},"attestation_state":"computed","paper":{"title":"Infrared Observation of Hot Cores","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. Brandl (CRSR Ithaca), B. Stecklum (TLS Tautenburg), H. Linz (TLS Tautenburg), I. Pascucci (AIU Jena), M. Feldt (MPIA Heidelberg), Th. Henning (AIU Jena)","submitted_at":"2001-07-05T10:55:23Z","abstract_excerpt":"We report on mid-infrared imaging of hot cores performed with SpectroCam-10 and TIMMI2. The observations aimed at the detection of thermal emission presumably associated with the hot cores. Mid-infrared flux measurements are required to improve the luminosity and optical depth estimates for these sources. Results are presented for W3(H$_2$O), G9.62+0.19, G10.47+0.03, and the possible hot core candidate G232.620+0.996. They illustrate that the morphology of these sources cannot be described by simple geometries. Therefore, line-of-sight effects and considerable extinction even at mid-infrared w"},"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":"astro-ph/0107092","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-07-05T10:55:23Z","cross_cats_sorted":[],"title_canon_sha256":"fec96a97531bcbd3f5483fcfb6603a0a860755a0f836226d15d60362517f0e0d","abstract_canon_sha256":"e6ebd877202c87d117559a6c2c5275db0e718c92f87a15f934066a6d5e6e3bcd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:46:32.404965Z","signature_b64":"CNJvGCrpQdaGXEjrqbJNF6IWdMeuc2yWP3xgmKZ2KjqScP55zvLGS9iFGV669cXzxYxm4M/mhE/bo1XPl5znBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"57b57a489430bc29d417ecf828705364c694190413a6167f9b93b50108e008af","last_reissued_at":"2026-05-18T00:46:32.404304Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:46:32.404304Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Infrared Observation of Hot Cores","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. Brandl (CRSR Ithaca), B. Stecklum (TLS Tautenburg), H. Linz (TLS Tautenburg), I. Pascucci (AIU Jena), M. Feldt (MPIA Heidelberg), Th. Henning (AIU Jena)","submitted_at":"2001-07-05T10:55:23Z","abstract_excerpt":"We report on mid-infrared imaging of hot cores performed with SpectroCam-10 and TIMMI2. The observations aimed at the detection of thermal emission presumably associated with the hot cores. Mid-infrared flux measurements are required to improve the luminosity and optical depth estimates for these sources. Results are presented for W3(H$_2$O), G9.62+0.19, G10.47+0.03, and the possible hot core candidate G232.620+0.996. They illustrate that the morphology of these sources cannot be described by simple geometries. Therefore, line-of-sight effects and considerable extinction even at mid-infrared w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0107092","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":"astro-ph/0107092","created_at":"2026-05-18T00:46:32.404413+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0107092v1","created_at":"2026-05-18T00:46:32.404413+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0107092","created_at":"2026-05-18T00:46:32.404413+00:00"},{"alias_kind":"pith_short_12","alias_value":"K62XUSEUGC6C","created_at":"2026-05-18T12:25:50.254431+00:00"},{"alias_kind":"pith_short_16","alias_value":"K62XUSEUGC6CTVAX","created_at":"2026-05-18T12:25:50.254431+00:00"},{"alias_kind":"pith_short_8","alias_value":"K62XUSEU","created_at":"2026-05-18T12:25:50.254431+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/K62XUSEUGC6CTVAX5T4CQ4CTMT","json":"https://pith.science/pith/K62XUSEUGC6CTVAX5T4CQ4CTMT.json","graph_json":"https://pith.science/api/pith-number/K62XUSEUGC6CTVAX5T4CQ4CTMT/graph.json","events_json":"https://pith.science/api/pith-number/K62XUSEUGC6CTVAX5T4CQ4CTMT/events.json","paper":"https://pith.science/paper/K62XUSEU"},"agent_actions":{"view_html":"https://pith.science/pith/K62XUSEUGC6CTVAX5T4CQ4CTMT","download_json":"https://pith.science/pith/K62XUSEUGC6CTVAX5T4CQ4CTMT.json","view_paper":"https://pith.science/paper/K62XUSEU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0107092&json=true","fetch_graph":"https://pith.science/api/pith-number/K62XUSEUGC6CTVAX5T4CQ4CTMT/graph.json","fetch_events":"https://pith.science/api/pith-number/K62XUSEUGC6CTVAX5T4CQ4CTMT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/K62XUSEUGC6CTVAX5T4CQ4CTMT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/K62XUSEUGC6CTVAX5T4CQ4CTMT/action/storage_attestation","attest_author":"https://pith.science/pith/K62XUSEUGC6CTVAX5T4CQ4CTMT/action/author_attestation","sign_citation":"https://pith.science/pith/K62XUSEUGC6CTVAX5T4CQ4CTMT/action/citation_signature","submit_replication":"https://pith.science/pith/K62XUSEUGC6CTVAX5T4CQ4CTMT/action/replication_record"}},"created_at":"2026-05-18T00:46:32.404413+00:00","updated_at":"2026-05-18T00:46:32.404413+00:00"}