{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:DS6XH4NRD5IX7IQWFHTA4QW42V","short_pith_number":"pith:DS6XH4NR","schema_version":"1.0","canonical_sha256":"1cbd73f1b11f517fa21629e60e42dcd551dac2a07cd1bcb8f7e3c68f0a6744be","source":{"kind":"arxiv","id":"1205.1351","version":1},"attestation_state":"computed","paper":{"title":"Cool and warm dust emission from M33 (HerM33es)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"B. Koribalski, B. Mookerjea, C. Buchbender, C. Henkel, C. Kramer, D. Calzetti, E. M. Xilouris, E. Rosolowsky, F. Bertoldi, F. Combes, F. Israel, F. S. Tabatabaei, F. van der Tak, G. Quintana-Lacaci, G. Stacey, J. Braine, M. Boquien, M. Gonzalez, M. Relano, P. Gratier, P. van der Werf, R. Beck, R. P. J. Tilanus, S. Akras, S. Anderl, S. Lord, S. Verley","submitted_at":"2012-05-07T11:43:42Z","abstract_excerpt":"We study the far-infrared emission from the nearby spiral galaxy M33 in order to investigate the dust physical properties such as the temperature and the luminosity density across the galaxy. Taking advantage of the unique wavelength coverage (100, 160, 250, 350 and 500 micron) of the Herschel Space Observatory and complementing our dataset with Spitzer-IRAC 5.8 and 8 micron and Spitzer-MIPS 24 and 70 micron data, we construct temperature and luminosity density maps by fitting two modified blackbodies of a fixed emissivity index of 1.5. We find that the 'cool' dust grains are heated at tempera"},"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":"1205.1351","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-05-07T11:43:42Z","cross_cats_sorted":[],"title_canon_sha256":"6a66a68862b8be33d8dd6d6efe77d9d7fa1b6330da3958688986c28b93ab9356","abstract_canon_sha256":"26b2468a88f12fb0d4d8363c089ca1ec322497860ea0e8cb9c8d3cecc613c6fe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:37.405993Z","signature_b64":"IQTKPb4d6303j7OYK41Xb5U+G24z6DAd77ysfkEu0N7IA4zJkokQX74sWHoTdd7xXYrhJ1I5aaEmJkKRrh85Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1cbd73f1b11f517fa21629e60e42dcd551dac2a07cd1bcb8f7e3c68f0a6744be","last_reissued_at":"2026-05-18T01:57:37.405392Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:37.405392Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cool and warm dust emission from M33 (HerM33es)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"B. Koribalski, B. Mookerjea, C. Buchbender, C. Henkel, C. Kramer, D. Calzetti, E. M. Xilouris, E. Rosolowsky, F. Bertoldi, F. Combes, F. Israel, F. S. Tabatabaei, F. van der Tak, G. Quintana-Lacaci, G. Stacey, J. Braine, M. Boquien, M. Gonzalez, M. Relano, P. Gratier, P. van der Werf, R. Beck, R. P. J. Tilanus, S. Akras, S. Anderl, S. Lord, S. Verley","submitted_at":"2012-05-07T11:43:42Z","abstract_excerpt":"We study the far-infrared emission from the nearby spiral galaxy M33 in order to investigate the dust physical properties such as the temperature and the luminosity density across the galaxy. Taking advantage of the unique wavelength coverage (100, 160, 250, 350 and 500 micron) of the Herschel Space Observatory and complementing our dataset with Spitzer-IRAC 5.8 and 8 micron and Spitzer-MIPS 24 and 70 micron data, we construct temperature and luminosity density maps by fitting two modified blackbodies of a fixed emissivity index of 1.5. We find that the 'cool' dust grains are heated at tempera"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1205.1351","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":"1205.1351","created_at":"2026-05-18T01:57:37.405473+00:00"},{"alias_kind":"arxiv_version","alias_value":"1205.1351v1","created_at":"2026-05-18T01:57:37.405473+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1205.1351","created_at":"2026-05-18T01:57:37.405473+00:00"},{"alias_kind":"pith_short_12","alias_value":"DS6XH4NRD5IX","created_at":"2026-05-18T12:27:04.183437+00:00"},{"alias_kind":"pith_short_16","alias_value":"DS6XH4NRD5IX7IQW","created_at":"2026-05-18T12:27:04.183437+00:00"},{"alias_kind":"pith_short_8","alias_value":"DS6XH4NR","created_at":"2026-05-18T12:27:04.183437+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/DS6XH4NRD5IX7IQWFHTA4QW42V","json":"https://pith.science/pith/DS6XH4NRD5IX7IQWFHTA4QW42V.json","graph_json":"https://pith.science/api/pith-number/DS6XH4NRD5IX7IQWFHTA4QW42V/graph.json","events_json":"https://pith.science/api/pith-number/DS6XH4NRD5IX7IQWFHTA4QW42V/events.json","paper":"https://pith.science/paper/DS6XH4NR"},"agent_actions":{"view_html":"https://pith.science/pith/DS6XH4NRD5IX7IQWFHTA4QW42V","download_json":"https://pith.science/pith/DS6XH4NRD5IX7IQWFHTA4QW42V.json","view_paper":"https://pith.science/paper/DS6XH4NR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1205.1351&json=true","fetch_graph":"https://pith.science/api/pith-number/DS6XH4NRD5IX7IQWFHTA4QW42V/graph.json","fetch_events":"https://pith.science/api/pith-number/DS6XH4NRD5IX7IQWFHTA4QW42V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DS6XH4NRD5IX7IQWFHTA4QW42V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DS6XH4NRD5IX7IQWFHTA4QW42V/action/storage_attestation","attest_author":"https://pith.science/pith/DS6XH4NRD5IX7IQWFHTA4QW42V/action/author_attestation","sign_citation":"https://pith.science/pith/DS6XH4NRD5IX7IQWFHTA4QW42V/action/citation_signature","submit_replication":"https://pith.science/pith/DS6XH4NRD5IX7IQWFHTA4QW42V/action/replication_record"}},"created_at":"2026-05-18T01:57:37.405473+00:00","updated_at":"2026-05-18T01:57:37.405473+00:00"}