[PDF] Top 20 The Atacama cosmology telescope: cosmology from galaxy clusters detected via the sunyaev zel'dovich effect
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The Atacama cosmology telescope: cosmology from galaxy clusters detected via the sunyaev zel'dovich effect
... object from their dust-corrected gri isophotal magnitude using the BPZ code (Ben´ıtez ...of the clusters in our sample have spectroscopic redshift in- formation available (see Table 1 for ... See full document
12
The Atacama cosmology telescope: high resolution sunyaev zel'dovich array observations of act sze selected clusters from the equatorial strip
... to the field (Cooray et ...of the SZE signal from radio sources could potentially bias flux and mass estimates from the ...SZE. The radio source fluxes extrapolated to 148 GHz ... See full document
12
Sunyaev zel'dovich effect observations of strong lensing galaxy clusters: probing the overconcentration problem
... for the clusters in this sample were computed from strong lensing models that were either derived for this work or taken from the literature (Table ...taken from the ... See full document
7
Atacama Cosmology Telescope: A measurement of the thermal Sunyaev Zel'dovich effect using the skewness of the CMB temperature distribution
... individual clusters in arcminute-scale CMB maps [8–12] or by measuring it statistically through its presence in the small-scale CMB power spectrum ...that the power spectrum is the best way to ... See full document
12
Detection of the Power Spectrum of Cosmic Microwave Background Lensing by the Atacama Cosmology Telescope
... minimize the effects of atmospheric noise and point ...along the Fourier axis corresponding to map declination are filtered out to reduce the effects of nonwhite atmospheric noise and scan- ... See full document
5
SPT CL J0205 5829: A z=1 32 EVOLVED MASSIVE GALAXY CLUSTER IN THE SOUTH POLE TELESCOPE SUNYAEV ZEL'DOVICH EFFECT SURVEY
... finds clusters via the Sunyaev–Zel’dovich (SZ; Sunyaev & Zel’dovich 1972) ...effect. The vast majority of baryonic mass of a galaxy cluster is in the ... See full document
10
Southern cosmology survey ii massive optically selected clusters from 70 square degrees of the sunyaev zel'dovich effect common survey area
... include the X-ray flux and temperature (Reiprich & B¨ohringer 2002; Kravtsov et ...optical galaxy richness of clusters (Becker et ...use the latest mass tracers for clusters of ... See full document
12
Evidence of galaxy cluster motions with the kinematic Sunyaev Zel'dovich effect
... sets. The first is a 148 GHz sky map from ACT, a dedicated microwave survey telescope in the Atacama Desert of ...Chile. The map covers a strip approximately 3 wide and 110 long ... See full document
6
Subaru weak lensing measurement of a z=0 81 cluster discovered by the Atacama Cosmology Telescope Survey
... The Sunyaev-Zel’dovich (SZ) effect, in which photons of the cosmic microwave background (CMB) scatter off electrons of the hot intracluster medium, is a powerful way of finding massive ... See full document
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THE ATACAMA COSMOLOGY TELESCOPE: LENSING OF CMB TEMPERATURE AND POLARIZATION DERIVED FROM COSMIC INFRARED BACKGROUND CROSS CORRELATION
... of the CMB temperature fi eld has rapidly progressed from fi rst detections ( Smith et ...measures from the CMB alone provide direct constraints on the evolution of gravitational ... See full document
9
High redshift cool core galaxy clusters detected via the Sunyaev Zel'dovich effect in the south pole telescope survey
... a galaxy contains an AGN, there is no definitive diagnostic that the AGN is emitting X-rays besides direct observation of ...with the high resolution data provided by Chandra, the best way of ... See full document
9
THE ATACAMA COSMOLOGY TELESCOPE: PHYSICAL PROPERTIES OF SUNYAEV ZEL'DOVICH EFFECT CLUSTERS ON THE CELESTIAL EQUATOR
... in the GMBCG (Hao et ...catalogs. The GMBCG catalog is an improved version of the MaxBCG method which used the SDSS ...designate the first reported alter- native name for each ...with ... See full document
18
The Atacama Cosmology Telescope: Sunyaev Zel'dovich selected galaxy clusters at 148 GHz from three seasons of data
... determining the Bayesian likelihood of cosmological and scaling relation parameters given the ACT cluster measurements, including redshift, SZ, and dynamical mass information, when ...for the ... See full document
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THE ATACAMA COSMOLOGY TELESCOPE: RELATION BETWEEN GALAXY CLUSTER OPTICAL RICHNESS AND SUNYAEV ZEL'DOVICH EFFECT
... in the catalog are ...is the positional accuracy of the cluster center. In the MaxBCG catalog, the cluster position is given by the location of the ...why the BCG ... See full document
10
The Atacama cosmology telescope: ACT CL J0102 4915 "el Gordo," A massive merging cluster at redshift 0 87
... maps from the ground and with the HST, which we are ...confirm the presence of an offset between the baryonic and dark matter distributions, as well as provide a robust mass estimate ... See full document
18
The Atacama cosmology telescope: a measurement of the cosmic microwave background power spectrum at 148 and 218 ghz from the 2008 southern survey
... across the array (such as a common mode) and c are the time streams associated with each pattern in ...solution. The maximum-likelihood solu- tion, m, is then given by solving the standard ... See full document
16
Hints toward cosmology: the need for cosmology in Peirce's philosophy
... following the hints collected in the present paper, we can reason- ably conclude that Peirce’s cosmological thought was never dismissed by him, even after the so-called “cosmological ...Moreover, ... See full document
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South pole telescope detections of the previously unconfirmed planck early sunyaev zel'dovich clusters in the southern hemisphere
... determine the flux and luminosity of each X-ray source, we used XSPEC 33 to model the instrument response within Posi- tion Sensitive Proportional Counter channels ...adjusted the normalization of ... See full document
7
Energy in higher derivative gravity via topological regularization
... to the usual mass parameter m in the absence of higher-curvature terms ( α ¼ β ¼ 0 ) or in the absence of a cosmological constant ( Λ ¼ 0 ...in the curvature, as the energy is linear in ... See full document
8
Separating the weak lensing and kinetic Sunyaev Zeldovich effects from cosmic microwave background temperature maps
... process, the successive troughs and crests of these modes tend to cancel when projected along the ˆ ...below, the OV effect arises from the modulation of the velocity ... See full document
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