{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:5ZKJKQGLMQC3H6ZOZOG7R2MWC6","short_pith_number":"pith:5ZKJKQGL","schema_version":"1.0","canonical_sha256":"ee549540cb6405b3fb2ecb8df8e99617a6ecf2aa1cdf7670cda778bab0f51938","source":{"kind":"arxiv","id":"astro-ph/0604058","version":1},"attestation_state":"computed","paper":{"title":"UV and FIR selected star-forming galaxies at z=0: differences and overlaps","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Alex S. Szalay, Barry F. Madore, Barry Y. Welsh, Bruno Milliard, C. Kevin Xu, David Schiminovich, D. Christopher Martin, Jorge Iglesias-P\\'aramo, Jose Donas, Karl Forster, Luciana Bianchi, Oswald H. W. Siegmund, Patrick Morrissey, Patrick N. Jelinsky, R. Michael Rich, Roger F. Malina, Sukyoung Yi, Susan G. Neff, Ted K. Wyder, Timothy M. Heckman, Todd Small, Tom A. Barlow, Tsutomu T. Takeuchi, Veronique Buat, Young-Wook Lee","submitted_at":"2006-04-04T12:41:53Z","abstract_excerpt":"We study two samples of local galaxies, one is UV (GALEX) selected and the other FIR (IRAS) selected, to address the question whether UV and FIR surveys see the two sides ('bright' and 'dark') of the star formation of the same population of galaxies or two different populations of star forming galaxies. No significant difference between the L$_{tot}$ ($=L_{60}+L_{FUV}$) luminosity functions of the UV and FIR samples is found. Also, after the correction for the `Malmquist bias' (bias for flux limited samples), the FIR-to-UV ratio v.s. L$_{tot}$ relations of the two samples are consistent with e"},"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/0604058","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-04-04T12:41:53Z","cross_cats_sorted":[],"title_canon_sha256":"0d2ad554c4727a0facbbc99a2f6b0b596abff0aee81bdfd87a8f10e68db57b8b","abstract_canon_sha256":"0c2cefbf848ca3422d89c9d6c1b6796dc71c62636dff06b34c7cfc8b19aa6eac"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:09:10.618713Z","signature_b64":"xhcXFzkUzVIoSDTEp1jcIemgOjir4Xs3uQg2PWJByHlSx4FKnrgIL2E8LNKtlFzvWbFTmamNUDaiHCYu9iyfDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ee549540cb6405b3fb2ecb8df8e99617a6ecf2aa1cdf7670cda778bab0f51938","last_reissued_at":"2026-05-18T01:09:10.618254Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:09:10.618254Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"UV and FIR selected star-forming galaxies at z=0: differences and overlaps","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Alex S. Szalay, Barry F. Madore, Barry Y. Welsh, Bruno Milliard, C. Kevin Xu, David Schiminovich, D. Christopher Martin, Jorge Iglesias-P\\'aramo, Jose Donas, Karl Forster, Luciana Bianchi, Oswald H. W. Siegmund, Patrick Morrissey, Patrick N. Jelinsky, R. Michael Rich, Roger F. Malina, Sukyoung Yi, Susan G. Neff, Ted K. Wyder, Timothy M. Heckman, Todd Small, Tom A. Barlow, Tsutomu T. Takeuchi, Veronique Buat, Young-Wook Lee","submitted_at":"2006-04-04T12:41:53Z","abstract_excerpt":"We study two samples of local galaxies, one is UV (GALEX) selected and the other FIR (IRAS) selected, to address the question whether UV and FIR surveys see the two sides ('bright' and 'dark') of the star formation of the same population of galaxies or two different populations of star forming galaxies. No significant difference between the L$_{tot}$ ($=L_{60}+L_{FUV}$) luminosity functions of the UV and FIR samples is found. Also, after the correction for the `Malmquist bias' (bias for flux limited samples), the FIR-to-UV ratio v.s. L$_{tot}$ relations of the two samples are consistent with e"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0604058","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":"astro-ph/0604058","created_at":"2026-05-18T01:09:10.618326+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0604058v1","created_at":"2026-05-18T01:09:10.618326+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0604058","created_at":"2026-05-18T01:09:10.618326+00:00"},{"alias_kind":"pith_short_12","alias_value":"5ZKJKQGLMQC3","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_16","alias_value":"5ZKJKQGLMQC3H6ZO","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_8","alias_value":"5ZKJKQGL","created_at":"2026-05-18T12:25:53.939244+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/5ZKJKQGLMQC3H6ZOZOG7R2MWC6","json":"https://pith.science/pith/5ZKJKQGLMQC3H6ZOZOG7R2MWC6.json","graph_json":"https://pith.science/api/pith-number/5ZKJKQGLMQC3H6ZOZOG7R2MWC6/graph.json","events_json":"https://pith.science/api/pith-number/5ZKJKQGLMQC3H6ZOZOG7R2MWC6/events.json","paper":"https://pith.science/paper/5ZKJKQGL"},"agent_actions":{"view_html":"https://pith.science/pith/5ZKJKQGLMQC3H6ZOZOG7R2MWC6","download_json":"https://pith.science/pith/5ZKJKQGLMQC3H6ZOZOG7R2MWC6.json","view_paper":"https://pith.science/paper/5ZKJKQGL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0604058&json=true","fetch_graph":"https://pith.science/api/pith-number/5ZKJKQGLMQC3H6ZOZOG7R2MWC6/graph.json","fetch_events":"https://pith.science/api/pith-number/5ZKJKQGLMQC3H6ZOZOG7R2MWC6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5ZKJKQGLMQC3H6ZOZOG7R2MWC6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5ZKJKQGLMQC3H6ZOZOG7R2MWC6/action/storage_attestation","attest_author":"https://pith.science/pith/5ZKJKQGLMQC3H6ZOZOG7R2MWC6/action/author_attestation","sign_citation":"https://pith.science/pith/5ZKJKQGLMQC3H6ZOZOG7R2MWC6/action/citation_signature","submit_replication":"https://pith.science/pith/5ZKJKQGLMQC3H6ZOZOG7R2MWC6/action/replication_record"}},"created_at":"2026-05-18T01:09:10.618326+00:00","updated_at":"2026-05-18T01:09:10.618326+00:00"}