HerMES: THE CONTRIBUTION TO THE COSMIC INFRARED BACKGROUND FROM GALAXIES SELECTED BY MASS AND REDSHIFT
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 super(-2)) K-selected sources (K sub(AB) < 24.0) split according to their rest-frame U - V versus V - J colors into 72,216 sta...
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| Veröffentlicht in: | The Astrophysical journal 2013-12, Vol.779 (1), p.1-23 |
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| creator | Viero, M P MONCELSI, L Quadri, R F Arumugam, V Assef, R J BETHERMIN, M Bock, J Bridge, C Casey, C M Conley, A |
| description | 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 super(-2)) K-selected sources (K sub(AB) < 24.0) split according to their rest-frame U - V versus V - J colors into 72,216 star-forming and 9034 quiescent galaxies, on maps from Spitzer/MIPS (24 mu m), Herschel/PACS (100, 160 mu m), Herschel/SPIRE (250, 350, 500 mu m), and AzTEC (1100 mu m). Of that total, about 95% originates from star-forming galaxies, while the remaining 5% is from apparently quiescent galaxies. The CIB at [lambda] [lap] 200 mu m appears to be sourced predominantly from galaxies at z [lap] 1, while at [lambda] [gap] 200 mu the bulk originates from 1 [lap] z [lap] 2. Stacking analyses were performed using simstack, a novel algorithm designed to account for possible biases in the stacked flux density due to clustering. It is made available to the public at www.astro.caltech.edu/~viero/viero_homepage/toolbox.html. |
| doi_str_mv | 10.1088/0004-637X/779/1/32 |
| format | Article |
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Of that total, about 95% originates from star-forming galaxies, while the remaining 5% is from apparently quiescent galaxies. The CIB at [lambda] [lap] 200 mu m appears to be sourced predominantly from galaxies at z [lap] 1, while at [lambda] [gap] 200 mu the bulk originates from 1 [lap] z [lap] 2. Stacking analyses were performed using simstack, a novel algorithm designed to account for possible biases in the stacked flux density due to clustering. 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Of that total, about 95% originates from star-forming galaxies, while the remaining 5% is from apparently quiescent galaxies. The CIB at [lambda] [lap] 200 mu m appears to be sourced predominantly from galaxies at z [lap] 1, while at [lambda] [gap] 200 mu the bulk originates from 1 [lap] z [lap] 2. Stacking analyses were performed using simstack, a novel algorithm designed to account for possible biases in the stacked flux density due to clustering. It is made available to the public at www.astro.caltech.edu/~viero/viero_homepage/toolbox.html.</description><subject>ALGORITHMS</subject><subject>Astrophysics</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>COLOR</subject><subject>COSMOLOGY</subject><subject>DENSITY</subject><subject>EVOLUTION</subject><subject>Flux</subject><subject>FLUX DENSITY</subject><subject>GALAXIES</subject><subject>Infrared</subject><subject>LUMINOSITY</subject><subject>MASS</subject><subject>PERTURBED ANGULAR CORRELATION</subject><subject>RED SHIFT</subject><subject>Sciences of the Universe</subject><subject>Spires</subject><subject>Stacking</subject><subject>Star formation</subject><subject>STARS</subject><subject>UNIVERSE</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNqN0U1rpEAQBuBmSWAnH38gp4a9JAczXf2hbW7GOKOsM4I6kD012rbEMBkntlnYfx9lQs57Kqp4qih4EboBcg9EyiUhhDsu856XnucvYcnoD7QAwaTDmfDO0OIb_EQX1r7OLfX9BWpjM2yi4gGXcYTDbFvmyeOuTLItLrOvWbFJQpxsV3mQR0_4MQh_r_Nst33Cqzzb4HWQBs9JVOAiSqOwnMUfvAmKAgcTmTaKOFmVV-i8rfbWXH_VS7RbRWUYO2m2TsIgdTTnMDq1r4Xrti4TRNeceNSQBoSkFdNAKqhrQhuAujKSi5r5DTGeaMCQtmlYA5ywS_TrdLe3Y6es7kajX3R_OBg9KkoZl4KLSd2d1Eu1V8ehe6uGf6qvOhUHqZpnBDjzuev-hcnenuxx6N8_jB3VW2e12e-rg-k_rAIPpM-kJ8l_0Omuz6nkE6Unqofe2sG0328AUXOiak5IzYGpKVEFilH2Cat5iFs</recordid><startdate>20131210</startdate><enddate>20131210</enddate><creator>Viero, M P</creator><creator>MONCELSI, L</creator><creator>Quadri, R F</creator><creator>Arumugam, V</creator><creator>Assef, R J</creator><creator>BETHERMIN, M</creator><creator>Bock, J</creator><creator>Bridge, C</creator><creator>Casey, C M</creator><creator>Conley, A</creator><general>American Astronomical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>1XC</scope><scope>OTOTI</scope></search><sort><creationdate>20131210</creationdate><title>HerMES: THE CONTRIBUTION TO THE COSMIC INFRARED BACKGROUND FROM GALAXIES SELECTED BY MASS AND REDSHIFT</title><author>Viero, M P ; 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| subjects | ALGORITHMS Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY COLOR COSMOLOGY DENSITY EVOLUTION Flux FLUX DENSITY GALAXIES Infrared LUMINOSITY MASS PERTURBED ANGULAR CORRELATION RED SHIFT Sciences of the Universe Spires Stacking Star formation STARS UNIVERSE |
| title | HerMES: THE CONTRIBUTION TO THE COSMIC INFRARED BACKGROUND FROM GALAXIES SELECTED BY MASS AND REDSHIFT |
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