{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:WMN2N6443GIEJDY7MLSGATHXLY","short_pith_number":"pith:WMN2N644","schema_version":"1.0","canonical_sha256":"b31ba6fb9cd990448f1f62e4604cf75e270004532b10dc8fd30605e47a3cfc02","source":{"kind":"arxiv","id":"astro-ph/0206337","version":1},"attestation_state":"computed","paper":{"title":"Submillimeter dust emission of the M17 complex measured with PRONAOS","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. Stepnik, C. Meny, E. Pointecouteau, F. Pajot, G. Serra, I. Ristorcelli, J.-M. Lamarre, J.-P. Bernard, J.-P. Torre, M. Giard, N. Boudet, Toulouse), Xavier Dupac (CESR","submitted_at":"2002-06-19T16:56:32Z","abstract_excerpt":"We map a 50' x 30' area in and around the M17 molecular complex with the French submillimeter balloon-borne telescope PRONAOS, in order to better understand the thermal emission of cosmic dust and the structure of the interstellar medium. The PRONAOS-SPM instrument has an angular resolution of about 3', corresponding to a size of 2 pc at the distance of this complex, and a high sensitivity up to 0.8 MJy/sr. The observations are made in four wide submillimeter bands corresponding to effective wavelengths of 200, 260, 360 and 580 um. Using an improved map-making method for PRONAOS data, we map t"},"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/0206337","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2002-06-19T16:56:32Z","cross_cats_sorted":[],"title_canon_sha256":"b7f8fdfddcebd42449b44a6c9c132df9d729dbe3871482b7a221e70435f3ad84","abstract_canon_sha256":"980d6804a196d6cfcee9f9aec45c16eeaf2bb40d534afe7b3ae623debad6d0ba"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:30:14.792518Z","signature_b64":"1dKsgLb0nsWq6GEqHqkrnwIQXbgktsM8XNqVUd4rvL4ufoLrDCI7iGiDjd4BfO8zpJ+/bC/yNto64/3B1JwMCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b31ba6fb9cd990448f1f62e4604cf75e270004532b10dc8fd30605e47a3cfc02","last_reissued_at":"2026-07-04T16:30:14.792090Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:30:14.792090Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Submillimeter dust emission of the M17 complex measured with PRONAOS","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. Stepnik, C. Meny, E. Pointecouteau, F. Pajot, G. Serra, I. Ristorcelli, J.-M. Lamarre, J.-P. Bernard, J.-P. Torre, M. Giard, N. Boudet, Toulouse), Xavier Dupac (CESR","submitted_at":"2002-06-19T16:56:32Z","abstract_excerpt":"We map a 50' x 30' area in and around the M17 molecular complex with the French submillimeter balloon-borne telescope PRONAOS, in order to better understand the thermal emission of cosmic dust and the structure of the interstellar medium. The PRONAOS-SPM instrument has an angular resolution of about 3', corresponding to a size of 2 pc at the distance of this complex, and a high sensitivity up to 0.8 MJy/sr. The observations are made in four wide submillimeter bands corresponding to effective wavelengths of 200, 260, 360 and 580 um. Using an improved map-making method for PRONAOS data, we map t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0206337","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0206337/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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/0206337","created_at":"2026-07-04T16:30:14.792142+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0206337v1","created_at":"2026-07-04T16:30:14.792142+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0206337","created_at":"2026-07-04T16:30:14.792142+00:00"},{"alias_kind":"pith_short_12","alias_value":"WMN2N6443GIE","created_at":"2026-07-04T16:30:14.792142+00:00"},{"alias_kind":"pith_short_16","alias_value":"WMN2N6443GIEJDY7","created_at":"2026-07-04T16:30:14.792142+00:00"},{"alias_kind":"pith_short_8","alias_value":"WMN2N644","created_at":"2026-07-04T16:30:14.792142+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/WMN2N6443GIEJDY7MLSGATHXLY","json":"https://pith.science/pith/WMN2N6443GIEJDY7MLSGATHXLY.json","graph_json":"https://pith.science/api/pith-number/WMN2N6443GIEJDY7MLSGATHXLY/graph.json","events_json":"https://pith.science/api/pith-number/WMN2N6443GIEJDY7MLSGATHXLY/events.json","paper":"https://pith.science/paper/WMN2N644"},"agent_actions":{"view_html":"https://pith.science/pith/WMN2N6443GIEJDY7MLSGATHXLY","download_json":"https://pith.science/pith/WMN2N6443GIEJDY7MLSGATHXLY.json","view_paper":"https://pith.science/paper/WMN2N644","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0206337&json=true","fetch_graph":"https://pith.science/api/pith-number/WMN2N6443GIEJDY7MLSGATHXLY/graph.json","fetch_events":"https://pith.science/api/pith-number/WMN2N6443GIEJDY7MLSGATHXLY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WMN2N6443GIEJDY7MLSGATHXLY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WMN2N6443GIEJDY7MLSGATHXLY/action/storage_attestation","attest_author":"https://pith.science/pith/WMN2N6443GIEJDY7MLSGATHXLY/action/author_attestation","sign_citation":"https://pith.science/pith/WMN2N6443GIEJDY7MLSGATHXLY/action/citation_signature","submit_replication":"https://pith.science/pith/WMN2N6443GIEJDY7MLSGATHXLY/action/replication_record"}},"created_at":"2026-07-04T16:30:14.792142+00:00","updated_at":"2026-07-04T16:30:14.792142+00:00"}