{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:SEWF3VAP2ZJI3GXXNNDPIUEYHR","short_pith_number":"pith:SEWF3VAP","schema_version":"1.0","canonical_sha256":"912c5dd40fd6528d9af76b46f450983c4c7be03349585499dc58db0f55dddac0","source":{"kind":"arxiv","id":"1302.4363","version":1},"attestation_state":"computed","paper":{"title":"Calibration of the total infrared luminosity of nearby galaxies from Spitzer and Herschel bands","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"B. Brandl, B. D. Johnson, B. Groves, B. T. Draine, C.-N. Hao, C. W. Engelbracht, D. A. Dale, D. Calzetti, E. Murphy, F. S. Tabatabaei, G. Aniano, G. Helou, H. Roussel, J. L. Hinz, K. D. Gordon, K. Sandstrom, K. V. Croxall, L. K. Hunt, M. Boquien, M. Galametz, R. A. Skibba, R. C. Kennicutt, Y. Li","submitted_at":"2013-02-18T17:33:41Z","abstract_excerpt":"We present new empirical calibrations to estimate resolved and integrated total infrared luminosities from Spitzer and Herschel bands used as monochromatic or combined tracers. We base our calibrations on resolved elements of nearby galaxies (3 to 30 Mpc) observed with Herschel. We perform a resolved SED modelling of these objects using the Draine and Li (2007) dust models and investigate the influence of the addition of SPIRE measurements in the estimation of LTIR. We find that using data up to 250 um leads to local LTIR values consistent with those obtained with a complete coverage (up to 50"},"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":"1302.4363","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-02-18T17:33:41Z","cross_cats_sorted":[],"title_canon_sha256":"4507090777f03177c82deadbad21c62c4ae6792d68d9d718d679fd3df0ac5bc1","abstract_canon_sha256":"754304b9b0dd5c0dc9bdacad0d656b79926bf7da8533f7c62550bccde0460d77"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:35.644292Z","signature_b64":"MV6RWlA2WrsSfx+idmsFQB/j36io1Hf9t9rdoDM/yds8liBxZHTVrtBifwNocpy5KRFwq4YRIVkqSKJTGJFzBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"912c5dd40fd6528d9af76b46f450983c4c7be03349585499dc58db0f55dddac0","last_reissued_at":"2026-05-18T01:51:35.643780Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:35.643780Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Calibration of the total infrared luminosity of nearby galaxies from Spitzer and Herschel bands","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"B. Brandl, B. D. Johnson, B. Groves, B. T. Draine, C.-N. Hao, C. W. Engelbracht, D. A. Dale, D. Calzetti, E. Murphy, F. S. Tabatabaei, G. Aniano, G. Helou, H. Roussel, J. L. Hinz, K. D. Gordon, K. Sandstrom, K. V. Croxall, L. K. Hunt, M. Boquien, M. Galametz, R. A. Skibba, R. C. Kennicutt, Y. Li","submitted_at":"2013-02-18T17:33:41Z","abstract_excerpt":"We present new empirical calibrations to estimate resolved and integrated total infrared luminosities from Spitzer and Herschel bands used as monochromatic or combined tracers. We base our calibrations on resolved elements of nearby galaxies (3 to 30 Mpc) observed with Herschel. We perform a resolved SED modelling of these objects using the Draine and Li (2007) dust models and investigate the influence of the addition of SPIRE measurements in the estimation of LTIR. We find that using data up to 250 um leads to local LTIR values consistent with those obtained with a complete coverage (up to 50"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1302.4363","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":"1302.4363","created_at":"2026-05-18T01:51:35.643866+00:00"},{"alias_kind":"arxiv_version","alias_value":"1302.4363v1","created_at":"2026-05-18T01:51:35.643866+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1302.4363","created_at":"2026-05-18T01:51:35.643866+00:00"},{"alias_kind":"pith_short_12","alias_value":"SEWF3VAP2ZJI","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"SEWF3VAP2ZJI3GXX","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"SEWF3VAP","created_at":"2026-05-18T12:27:59.945178+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/SEWF3VAP2ZJI3GXXNNDPIUEYHR","json":"https://pith.science/pith/SEWF3VAP2ZJI3GXXNNDPIUEYHR.json","graph_json":"https://pith.science/api/pith-number/SEWF3VAP2ZJI3GXXNNDPIUEYHR/graph.json","events_json":"https://pith.science/api/pith-number/SEWF3VAP2ZJI3GXXNNDPIUEYHR/events.json","paper":"https://pith.science/paper/SEWF3VAP"},"agent_actions":{"view_html":"https://pith.science/pith/SEWF3VAP2ZJI3GXXNNDPIUEYHR","download_json":"https://pith.science/pith/SEWF3VAP2ZJI3GXXNNDPIUEYHR.json","view_paper":"https://pith.science/paper/SEWF3VAP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1302.4363&json=true","fetch_graph":"https://pith.science/api/pith-number/SEWF3VAP2ZJI3GXXNNDPIUEYHR/graph.json","fetch_events":"https://pith.science/api/pith-number/SEWF3VAP2ZJI3GXXNNDPIUEYHR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SEWF3VAP2ZJI3GXXNNDPIUEYHR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SEWF3VAP2ZJI3GXXNNDPIUEYHR/action/storage_attestation","attest_author":"https://pith.science/pith/SEWF3VAP2ZJI3GXXNNDPIUEYHR/action/author_attestation","sign_citation":"https://pith.science/pith/SEWF3VAP2ZJI3GXXNNDPIUEYHR/action/citation_signature","submit_replication":"https://pith.science/pith/SEWF3VAP2ZJI3GXXNNDPIUEYHR/action/replication_record"}},"created_at":"2026-05-18T01:51:35.643866+00:00","updated_at":"2026-05-18T01:51:35.643866+00:00"}