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Arumugam","submitted_at":"2013-04-01T20:00:00Z","abstract_excerpt":"We quantify the fraction of the cosmic infrared background (CIB) that originates from galaxies identified in the UV/optical/near-infrared by stacking 81,250 (~35.7 arcmin^2) K-selected sources (K_AB < 24.0), split according to their rest-frame U - V vs. V - J colors into 72,216 star-forming and 9,034 quiescent galaxies, on maps from Spitzer/MIPS (24um), Herschel/SPIRE (250, 350, 500um), Herschel/PACS (100, 160um), and AzTEC (1100um). The fraction of the CIB resolved by our catalog is (69 $\\pm$ 15)% at 24um, (78 $\\pm$ 17)% at 70um, (58 $\\pm$ 13)% at 100um, (78 $\\pm$ 18)% at 160um, (80 $\\pm$ 17)"},"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":"1304.0446","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-04-01T20:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"8f0e9ca7561861676951bb63054cd16f4e311e43dec38809acc768d59ecf0ccb","abstract_canon_sha256":"b970e98a999ab1603ff45402fd1a2182d4cb46e2f63ce327dfdc16827b6b3906"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:50:50.397378Z","signature_b64":"4g+5BrOQfARn4BsDXh99YStt1yJEf7JuhbBfjzyrFyt4pcUPDgVL0rJ0EWsyYndJQQSkrc8mx7s+KNeccniiAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"079cae2b685072e898e46debac81005a16d1c113f783493491e4af81f0720dfd","last_reissued_at":"2026-05-18T01:50:50.396669Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:50:50.396669Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"HerMES: The Contribution to the Cosmic Infrared Background from Galaxies Selected by Mass and Redshift","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Conley, A. Cooray, B. Schulz, C. Bridge, D. Farrah, D. Scott, G. Marsden, G. W. Wilson, I. G. Roseboom, J. Bock, J. D. Vieira, J. Wardlow, K. Kohno, L. Moncelsi, L. Wang, M. Bethermin, M. P. Viero, M. S. Yun, M. Vaccari, M. Zemcov, P. Serra, R. F. Quadri, R. J. Assef, R. J. Ivison, R. J. Williams, S. Heinis, S. Ikarashi, S. J. Oliver, V. Arumugam","submitted_at":"2013-04-01T20:00:00Z","abstract_excerpt":"We quantify the fraction of the cosmic infrared background (CIB) that originates from galaxies identified in the UV/optical/near-infrared by stacking 81,250 (~35.7 arcmin^2) K-selected sources (K_AB < 24.0), split according to their rest-frame U - V vs. V - J colors into 72,216 star-forming and 9,034 quiescent galaxies, on maps from Spitzer/MIPS (24um), Herschel/SPIRE (250, 350, 500um), Herschel/PACS (100, 160um), and AzTEC (1100um). 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