{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:DK65R6DXBPG2VQOTD36O6KSDLL","short_pith_number":"pith:DK65R6DX","schema_version":"1.0","canonical_sha256":"1abdd8f8770bcdaac1d31efcef2a435aeddf9d7dafdf33a3fc5be8b738514623","source":{"kind":"arxiv","id":"1403.3615","version":1},"attestation_state":"computed","paper":{"title":"Herschel Far-IR counterparts of SDSS galaxies: Analysis of commonly used Star Formation Rate estimates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Bongiovanni, A. Ederoclite, A. M. P\\'erez Garc\\'ia, B. Magnelli, D. Lutz, F. Pozzi, G. Cresci, H. Dom\\'inguez S\\'anchez, I. Delvecchio, I. Oteo, J. Cepa, L. Riguccini, M. A. Lara-L\\'opez, M. S\\'anchez-Portal, P. Popesso, S. Berta","submitted_at":"2014-03-14T15:45:05Z","abstract_excerpt":"We study a hundred of galaxies from the spectroscopic Sloan Digital Sky Survey with individual detections in the Far-Infrared Herschel PACS bands (100 or 160 $\\mu$m) and in the GALEX Far-UltraViolet band up to z$\\sim$0.4 in the COSMOS and Lockman Hole fields. The galaxies are divided into 4 spectral and 4 morphological types. For the star forming and unclassifiable galaxies we calculate dust extinctions from the UV slope, the H$\\alpha$/H$\\beta$ ratio and the $L_{\\rm IR}/L_{\\rm UV}$ ratio. There is a tight correlation between the dust extinction and both $L_{\\rm IR}$ and metallicity. We calcula"},"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":"1403.3615","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-03-14T15:45:05Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"81db12ed18b86ab08827889ba1dd5b32f08d7ae672b046020208cdde5eb966ba","abstract_canon_sha256":"7b0c63459f818ff8ae271347300dbd6294dd51471d0ee10dd3f47470a5a07977"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:44:01.091411Z","signature_b64":"9e8aZdxMGkmeu8usnNSzcayykHnNcVdxQePTuBTX5N6+YQ4CELg7BWd86BpK19WEVDuqowaqeHBNKO/w1WNpAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1abdd8f8770bcdaac1d31efcef2a435aeddf9d7dafdf33a3fc5be8b738514623","last_reissued_at":"2026-05-18T01:44:01.090212Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:44:01.090212Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Herschel Far-IR counterparts of SDSS galaxies: Analysis of commonly used Star Formation Rate estimates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Bongiovanni, A. Ederoclite, A. M. P\\'erez Garc\\'ia, B. Magnelli, D. Lutz, F. Pozzi, G. Cresci, H. Dom\\'inguez S\\'anchez, I. Delvecchio, I. Oteo, J. Cepa, L. Riguccini, M. A. Lara-L\\'opez, M. S\\'anchez-Portal, P. Popesso, S. Berta","submitted_at":"2014-03-14T15:45:05Z","abstract_excerpt":"We study a hundred of galaxies from the spectroscopic Sloan Digital Sky Survey with individual detections in the Far-Infrared Herschel PACS bands (100 or 160 $\\mu$m) and in the GALEX Far-UltraViolet band up to z$\\sim$0.4 in the COSMOS and Lockman Hole fields. The galaxies are divided into 4 spectral and 4 morphological types. For the star forming and unclassifiable galaxies we calculate dust extinctions from the UV slope, the H$\\alpha$/H$\\beta$ ratio and the $L_{\\rm IR}/L_{\\rm UV}$ ratio. There is a tight correlation between the dust extinction and both $L_{\\rm IR}$ and metallicity. We calcula"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.3615","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":"1403.3615","created_at":"2026-05-18T01:44:01.090287+00:00"},{"alias_kind":"arxiv_version","alias_value":"1403.3615v1","created_at":"2026-05-18T01:44:01.090287+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.3615","created_at":"2026-05-18T01:44:01.090287+00:00"},{"alias_kind":"pith_short_12","alias_value":"DK65R6DXBPG2","created_at":"2026-05-18T12:28:25.294606+00:00"},{"alias_kind":"pith_short_16","alias_value":"DK65R6DXBPG2VQOT","created_at":"2026-05-18T12:28:25.294606+00:00"},{"alias_kind":"pith_short_8","alias_value":"DK65R6DX","created_at":"2026-05-18T12:28:25.294606+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/DK65R6DXBPG2VQOTD36O6KSDLL","json":"https://pith.science/pith/DK65R6DXBPG2VQOTD36O6KSDLL.json","graph_json":"https://pith.science/api/pith-number/DK65R6DXBPG2VQOTD36O6KSDLL/graph.json","events_json":"https://pith.science/api/pith-number/DK65R6DXBPG2VQOTD36O6KSDLL/events.json","paper":"https://pith.science/paper/DK65R6DX"},"agent_actions":{"view_html":"https://pith.science/pith/DK65R6DXBPG2VQOTD36O6KSDLL","download_json":"https://pith.science/pith/DK65R6DXBPG2VQOTD36O6KSDLL.json","view_paper":"https://pith.science/paper/DK65R6DX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1403.3615&json=true","fetch_graph":"https://pith.science/api/pith-number/DK65R6DXBPG2VQOTD36O6KSDLL/graph.json","fetch_events":"https://pith.science/api/pith-number/DK65R6DXBPG2VQOTD36O6KSDLL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DK65R6DXBPG2VQOTD36O6KSDLL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DK65R6DXBPG2VQOTD36O6KSDLL/action/storage_attestation","attest_author":"https://pith.science/pith/DK65R6DXBPG2VQOTD36O6KSDLL/action/author_attestation","sign_citation":"https://pith.science/pith/DK65R6DXBPG2VQOTD36O6KSDLL/action/citation_signature","submit_replication":"https://pith.science/pith/DK65R6DXBPG2VQOTD36O6KSDLL/action/replication_record"}},"created_at":"2026-05-18T01:44:01.090287+00:00","updated_at":"2026-05-18T01:44:01.090287+00:00"}