{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:CUKOWJC2V7Z37UPAGW5PXZ3YXJ","short_pith_number":"pith:CUKOWJC2","schema_version":"1.0","canonical_sha256":"1514eb245aaff3bfd1e035bafbe778ba6db9c80104e561742c0887b47da42831","source":{"kind":"arxiv","id":"1302.5699","version":1},"attestation_state":"computed","paper":{"title":"Vindicating single-T modified blackbody fits to Herschel SEDs (Research Note)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Simone Bianchi","submitted_at":"2013-02-22T21:00:00Z","abstract_excerpt":"I show here that the bulk of the dust mass in a galaxy can be equivalently estimated from: i) the full spectral energy distribution of dust emission, using the approach of Draine & Lee (2007) that includes a distribution of dust grains and a range of interstellar radiation field intensities; ii) the emission in the wavelength range 100um <= lambda <= 500um (covered by the Herschel Space Observatory), by fitting to the data a simpler single temperature modified blackbody. Recent claims on the contrary (Dale et al. 2012) should be interpreted as a caveat to use in the simpler fits an absorption "},"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":"1302.5699","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-22T21:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"e02ce10352aee2867849d8cb39747463397e39aa04beb52033e056926ca2f3e2","abstract_canon_sha256":"f691564fcd11238299ef4f640ba50089eaf2229bfaf4603b8d4576053317ace9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:33.973588Z","signature_b64":"6j3oE+jfS8RvzK+5dwAOLsApM5cDUgEVyotBGD4awRiFKyO+wrwctI7QnNidKUq1Ero3YtqAvkXwsPwKaVjfCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1514eb245aaff3bfd1e035bafbe778ba6db9c80104e561742c0887b47da42831","last_reissued_at":"2026-05-18T01:51:33.973119Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:33.973119Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Vindicating single-T modified blackbody fits to Herschel SEDs (Research Note)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Simone Bianchi","submitted_at":"2013-02-22T21:00:00Z","abstract_excerpt":"I show here that the bulk of the dust mass in a galaxy can be equivalently estimated from: i) the full spectral energy distribution of dust emission, using the approach of Draine & Lee (2007) that includes a distribution of dust grains and a range of interstellar radiation field intensities; ii) the emission in the wavelength range 100um <= lambda <= 500um (covered by the Herschel Space Observatory), by fitting to the data a simpler single temperature modified blackbody. Recent claims on the contrary (Dale et al. 2012) should be interpreted as a caveat to use in the simpler fits an absorption "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1302.5699","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":"1302.5699","created_at":"2026-05-18T01:51:33.973204+00:00"},{"alias_kind":"arxiv_version","alias_value":"1302.5699v1","created_at":"2026-05-18T01:51:33.973204+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1302.5699","created_at":"2026-05-18T01:51:33.973204+00:00"},{"alias_kind":"pith_short_12","alias_value":"CUKOWJC2V7Z3","created_at":"2026-05-18T12:27:40.988391+00:00"},{"alias_kind":"pith_short_16","alias_value":"CUKOWJC2V7Z37UPA","created_at":"2026-05-18T12:27:40.988391+00:00"},{"alias_kind":"pith_short_8","alias_value":"CUKOWJC2","created_at":"2026-05-18T12:27:40.988391+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2506.13851","citing_title":"Interstellar dust production, destruction and effects of dust depletion in galaxies","ref_index":194,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CUKOWJC2V7Z37UPAGW5PXZ3YXJ","json":"https://pith.science/pith/CUKOWJC2V7Z37UPAGW5PXZ3YXJ.json","graph_json":"https://pith.science/api/pith-number/CUKOWJC2V7Z37UPAGW5PXZ3YXJ/graph.json","events_json":"https://pith.science/api/pith-number/CUKOWJC2V7Z37UPAGW5PXZ3YXJ/events.json","paper":"https://pith.science/paper/CUKOWJC2"},"agent_actions":{"view_html":"https://pith.science/pith/CUKOWJC2V7Z37UPAGW5PXZ3YXJ","download_json":"https://pith.science/pith/CUKOWJC2V7Z37UPAGW5PXZ3YXJ.json","view_paper":"https://pith.science/paper/CUKOWJC2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1302.5699&json=true","fetch_graph":"https://pith.science/api/pith-number/CUKOWJC2V7Z37UPAGW5PXZ3YXJ/graph.json","fetch_events":"https://pith.science/api/pith-number/CUKOWJC2V7Z37UPAGW5PXZ3YXJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CUKOWJC2V7Z37UPAGW5PXZ3YXJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CUKOWJC2V7Z37UPAGW5PXZ3YXJ/action/storage_attestation","attest_author":"https://pith.science/pith/CUKOWJC2V7Z37UPAGW5PXZ3YXJ/action/author_attestation","sign_citation":"https://pith.science/pith/CUKOWJC2V7Z37UPAGW5PXZ3YXJ/action/citation_signature","submit_replication":"https://pith.science/pith/CUKOWJC2V7Z37UPAGW5PXZ3YXJ/action/replication_record"}},"created_at":"2026-05-18T01:51:33.973204+00:00","updated_at":"2026-05-18T01:51:33.973204+00:00"}