A MEASUREMENT OF THE SECONDARY-CMB AND MILLIMETER-WAVE-FOREGROUND BISPECTRUM USING 800 deg2 OF SOUTH POLE TELESCOPE DATA

被引:51
作者
Crawford, T. M. [1 ,2 ]
Schaffer, K. K. [1 ,3 ,4 ]
Bhattacharya, S. [1 ,5 ]
Aird, K. A. [6 ]
Benson, B. A. [1 ,3 ]
Bleem, L. E. [1 ,7 ]
Carlstrom, J. E. [1 ,2 ,3 ,7 ,8 ]
Chang, C. L. [1 ,3 ,8 ]
Cho, H-M. [9 ]
Crites, A. T. [1 ,2 ]
de Haan, T. [10 ]
Dobbs, M. A. [10 ]
Dudley, J. [10 ]
George, E. M. [11 ]
Halverson, N. W. [12 ,13 ]
Holder, G. P. [10 ]
Holzapfel, W. L. [11 ]
Hoover, S. [1 ,7 ]
Hou, Z. [14 ]
Hrubes, J. D. [6 ]
Keisler, R. [1 ,7 ]
Knox, L. [14 ]
Lee, A. T. [11 ,15 ]
Leitch, E. M. [1 ,2 ]
Lueker, M. [16 ]
Luong-Van, D. [6 ]
McMahon, J. J. [17 ]
Mehl, J. [1 ,8 ]
Meyer, S. S. [1 ,2 ,3 ,7 ]
Millea, M. [14 ]
Mocanu, L. M. [1 ,2 ]
Mohr, J. J. [18 ,19 ,20 ]
Montroy, T. E. [21 ]
Padin, S. [1 ,2 ,16 ]
Plagge, T. [1 ,2 ]
Pryke, C. [22 ]
Reichardt, C. L. [11 ]
Ruhl, J. E. [21 ]
Sayre, J. T. [21 ]
Shaw, L. [10 ]
Shirokoff, E. [11 ]
Spieler, H. G. [15 ]
Staniszewski, Z. [21 ]
Stark, A. A. [23 ]
Story, K. T. [1 ,7 ]
van Engelen, A. [10 ]
Vanderlinde, K. [10 ]
Vieira, J. D. [16 ]
Williamson, R. [1 ,2 ]
Zahn, O. [24 ,25 ]
机构
[1] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[2] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[3] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
[4] Sch Art Inst Chicago, Liberal Arts Dept, Chicago, IL 60603 USA
[5] Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA
[6] Univ Chicago, Chicago, IL 60637 USA
[7] Univ Chicago, Dept Phys, Chicago, IL 60637 USA
[8] Argonne Natl Lab, Argonne, IL 60439 USA
[9] NIST Quantum Devices Grp, Boulder, CO 80305 USA
[10] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada
[11] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[12] Univ Colorado, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USA
[13] Univ Colorado, Dept Phys, Boulder, CO 80309 USA
[14] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA
[15] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA
[16] CALTECH, Pasadena, CA 91125 USA
[17] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA
[18] Univ Munich, Dept Phys, D-81679 Munich, Germany
[19] Excellence Cluster Universe, D-85748 Garching, Germany
[20] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[21] Case Western Reserve Univ, Ctr Educ & Res Cosmol & Astrophys, Dept Phys, Cleveland, OH 44106 USA
[22] Univ Minnesota, Dept Phys, Minneapolis, MN 55455 USA
[23] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[24] Univ Calif Berkeley, Dept Phys, Berkeley Ctr Cosmol Phys, Berkeley, CA 94720 USA
[25] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA
基金
美国国家科学基金会;
关键词
cosmic background radiation; cosmology: observations; methods: data analysis; MICROWAVE BACKGROUND ANISOTROPIES; PROBE WMAP OBSERVATIONS; ATACAMA COSMOLOGY TELESCOPE; X-RAY OBSERVATIONS; POWER SPECTRUM; GALAXY CLUSTERS; NUMBER COUNTS; IMPROVED CONSTRAINTS; PRESSURE PROFILES; NON-GAUSSIANITY;
D O I
10.1088/0004-637X/784/2/143
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a measurement of the angular bispectrum of the millimeter-wave sky in observing bands centered at roughly 95, 150, and 220 GHz, on angular scales of 1' less than or similar to theta less than or similar to 10' (multipole number 1000 less than or similar to l less than or similar to 10,000). At these frequencies and angular scales, the main contributions to the bispectrum are expected to be the thermal Sunyaev-Zel'dovich (tSZ) effect and emission from extragalactic sources, predominantly dusty, star-forming galaxies (DSFGs) and active galactic nuclei. We measure the bispectrum in 800 deg(2) of three-band South Pole Telescope data, and we use a multi-frequency fitting procedure to separate the bispectrum of the tSZ effect from the extragalactic source contribution. We simultaneously detect the bispectrum of the tSZ effect at > 10 sigma, the unclustered component of the extragalactic source bispectrum at > 5 sigma in each frequency band, and the bispectrum due to the clustering of DSFGs-i.e., the clustered cosmic infrared background (CIB) bispectrum-at > 5 sigma. This is the first reported detection of the clustered CIB bispectrum. We use the measured tSZ bispectrum amplitude, compared to model predictions, to constrain the normalization of the matter power spectrum to be s sigma = 0.787 +/- 0.031 and to predict the amplitude of the tSZ power spectrum at l = 3000. This prediction improves our ability to separate the thermal and kinematic contributions to the total SZ power spectrum. The addition of bispectrum data improves our constraint on the tSZ power spectrum amplitude by a factor of two compared to power spectrum measurements alone and demonstrates a preference for a nonzero kinematic SZ ( kSZ) power spectrum, with a derived constraint on the kSZ amplitude at l = 3000 of A(kSZ) = 2.9 +/- 1.6 mu K-2, or A(kSZ) = 2.6 +/- 1.8 mu K-2 if the default AkSZ > 0 prior is removed.
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页数:21
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共 88 条
[1]   Gauge-invariant second-order perturbations and non-Gaussianity from inflation [J].
Acquaviva, V ;
Bartolo, N ;
Matarrese, S ;
Riotto, A .
NUCLEAR PHYSICS B, 2003, 667 (1-2) :119-148
[2]   Constraining thermal dust emission in distant galaxies with number counts and angular power spectra [J].
Addison, G. E. ;
Dunkley, J. ;
Bond, J. R. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, 436 (02) :1896-1917
[3]   POWER-LAW TEMPLATE FOR INFRARED POINT-SOURCE CLUSTERING [J].
Addison, Graeme E. ;
Dunkley, Joanna ;
Hajian, Amir ;
Viero, Marco ;
Bond, J. Richard ;
Das, Sudeep ;
Devlin, Mark J. ;
Halpern, Mark ;
Hincks, Adam D. ;
Hlozek, Renee ;
Marriage, Tobias A. ;
Moodley, Kavilan ;
Page, Lyman A. ;
Reese, Erik D. ;
Scott, Douglas ;
Spergel, David N. ;
Staggs, Suzanne T. ;
Wollack, Edward .
ASTROPHYSICAL JOURNAL, 2012, 752 (02)
[4]   Planck intermediate results V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect [J].
Ade, P. A. R. ;
Aghanim, N. ;
Arnaud, M. ;
Ashdown, M. ;
Atrio-Barandela, F. ;
Aumont, J. ;
Baccigalupi, C. ;
Balbi, A. ;
Banday, A. J. ;
Barreiro, R. B. ;
Bartlett, J. G. ;
Battaner, E. ;
Benabed, K. ;
Benoit, A. ;
Bernard, J. -P. ;
Bersanelli, M. ;
Bhatia, R. ;
Bikmaev, I. ;
Bobin, J. ;
Boehringer, H. ;
Bonaldi, A. ;
Bond, J. R. ;
Borgani, S. ;
Borrill, J. ;
Bouchet, F. R. ;
Bourdin, H. ;
Brown, M. L. ;
Burenin, R. ;
Burigana, C. ;
Cabella, P. ;
Cardoso, J. -F. ;
Carvalho, P. ;
Castex, G. ;
Catalano, A. ;
Cayon, L. ;
Chamballu, A. ;
Chiang, L. -Y ;
Chon, G. ;
Christensen, P. R. ;
Churazov, E. ;
Clements, D. L. ;
Colafrancesco, S. ;
Colombi, S. ;
Colombo, L. P. L. ;
Comis, B. ;
Coulais, A. ;
Crill, B. P. ;
Cuttaia, F. ;
Da Silva, A. ;
Dahle, H. .
ASTRONOMY & ASTROPHYSICS, 2013, 550
[5]   Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample [J].
Ade, P. A. R. ;
Aghanim, N. ;
Arnaud, M. ;
Ashdown, M. ;
Aumont, J. ;
Baccigalupi, C. ;
Balbi, A. ;
Banday, A. J. ;
Barreiro, R. B. ;
Bartelmann, M. ;
Bartlett, J. G. ;
Battaner, E. ;
Battye, R. ;
Benabed, K. ;
Benoit, A. ;
Bernard, J-P ;
Bersanelli, M. ;
Bhatia, R. ;
Bock, J. J. ;
Bonaldi, A. ;
Bond, J. R. ;
Borrill, J. ;
Bouchet, F. R. ;
Brown, M. L. ;
Bucher, M. ;
Burigana, C. ;
Cabella, P. ;
Cantalupo, C. M. ;
Cardoso, J-F ;
Carvalho, P. ;
Catalano, A. ;
Cayon, L. ;
Challinor, A. ;
Chamballu, A. ;
Chary, R-R ;
Chiang, L-Y ;
Chiang, C. ;
Chon, G. ;
Christensen, P. R. ;
Churazov, E. ;
Clements, D. L. ;
Colafrancesco, S. ;
Colombi, S. ;
Couchot, F. ;
Coulais, A. ;
Crill, B. P. ;
Cuttaia, F. ;
Da Silva, A. ;
Dahle, H. ;
Danese, L. .
ASTRONOMY & ASTROPHYSICS, 2011, 536
[6]   Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters [J].
Allen, S. W. ;
Rapetti, D. A. ;
Schmidt, R. W. ;
Ebeling, H. ;
Morris, R. G. ;
Fabian, A. C. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2008, 383 (03) :879-896
[7]   The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the YSZ-M500 relation [J].
Arnaud, M. ;
Pratt, G. W. ;
Piffaretti, R. ;
Boehringer, H. ;
Croston, J. H. ;
Pointecouteau, E. .
ASTRONOMY & ASTROPHYSICS, 2010, 517
[8]   COSMOLOGICAL CONSTRAINTS FROM SUNYAEV-ZEL'DOVICH-SELECTED CLUSTERS WITH X-RAY OBSERVATIONS IN THE FIRST 178 deg2 OF THE SOUTH POLE TELESCOPE SURVEY [J].
Benson, B. A. ;
de Haan, T. ;
Dudley, J. P. ;
Reichardt, C. L. ;
Aird, K. A. ;
Andersson, K. ;
Armstrong, R. ;
Ashby, M. L. N. ;
Bautz, M. ;
Bayliss, M. ;
Bazin, G. ;
Bleem, L. E. ;
Brodwin, M. ;
Carlstrom, J. E. ;
Chang, C. L. ;
Cho, H. M. ;
Clocchiatti, A. ;
Crawford, T. M. ;
Crites, A. T. ;
Desai, S. ;
Dobbs, M. A. ;
Foley, R. J. ;
Forman, W. R. ;
George, E. M. ;
Gladders, M. D. ;
Gonzalez, A. H. ;
Halverson, N. W. ;
Harrington, N. ;
High, F. W. ;
Holder, G. P. ;
Holzapfel, W. L. ;
Hoover, S. ;
Hrubes, J. D. ;
Jones, C. ;
Joy, M. ;
Keisler, R. ;
Knox, L. ;
Lee, A. T. ;
Leitch, E. M. ;
Liu, J. ;
Lueker, M. ;
Luong-Van, D. ;
Mantz, A. ;
Marrone, D. P. ;
McDonald, M. ;
McMahon, J. J. ;
Mehl, J. ;
Meyer, S. S. ;
Mocanu, L. ;
Mohr, J. J. .
ASTROPHYSICAL JOURNAL, 2013, 763 (02)
[9]   Modeling the evolution of infrared galaxies: a parametric backward evolution model [J].
Bethermin, M. ;
Dole, H. ;
Lagache, G. ;
Le Borgne, D. ;
Penin, A. .
ASTRONOMY & ASTROPHYSICS, 2011, 529
[10]   A UNIFIED EMPIRICAL MODEL FOR INFRARED GALAXY COUNTS BASED ON THE OBSERVED PHYSICAL EVOLUTION OF DISTANT GALAXIES [J].
Bethermin, Matthieu ;
Daddi, Emanuele ;
Magdis, Georgios ;
Sargent, Mark T. ;
Hezaveh, Yashar ;
Elbaz, David ;
Le Borgne, Damien ;
Mullaney, James ;
Pannella, Maurilio ;
Buat, Veronique ;
Charmandaris, Vassilis ;
Lagache, Guilaine ;
Scott, Douglas .
ASTROPHYSICAL JOURNAL LETTERS, 2012, 757 (02)