[PDF] Top 20 The Atacama cosmology telescope: extragalactic sources at 148 GHZ in the 2008 survey
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The Atacama cosmology telescope: extragalactic sources at 148 GHZ in the 2008 survey
... for the matched ...component. The CMB spectrum is taken from WMAP5 (Nolta et al. 2009). The undetected sources and the SZ effect from galaxy clusters are one-dimensional templates fit ... See full document
15
THE ATACAMA COSMOLOGY TELESCOPE: A MEASUREMENT OF THE PRIMORDIAL POWER SPECTRUM
... on the primordial power spectrum of adiabatic fluctuations using data from the 2008 Southern Survey of the Atacama Cosmology Telescope (ACT) in combination ... See full document
10
The Atacama Cosmology Telescope: likelihood for small scale CMB data
... Abstract. The Atacama Cosmology Telescope has measured the angular power spectra of microwave fluctuations to arcminute scales at frequencies of 148 and 218 GHz, ... See full document
33
Subaru weak lensing measurement of a z=0 81 cluster discovered by the Atacama Cosmology Telescope Survey
... of the most luminous SZ clus- ters discovered in the 148-GHz ACT map of 268 square degrees, which is a part of 500 square degrees in its equatorial survey field taken ... See full document
17
The Atacama cosmology telescope: calibration with the Wilkinson microwave anisotropy probe using cross correlations
... directions at constant elevation each ...field at the same elevation twice a night: once as the field rises, once as it ...changes the scan angle, resulting in cross- linking, ... See full document
9
The Atacama cosmology telescope: ACT CL J0102 4915 "el Gordo," A massive merging cluster at redshift 0 87
... that in the presence of an intracluster magnetic field can produce synchrotron ...Sky Survey (SUMSS) archival data at 843 MHz. The radio mosaic at the cluster location has ... See full document
18
Detection of the Power Spectrum of Cosmic Microwave Background Lensing by the Atacama Cosmology Telescope
... as in [6]) are further processed to minimize the effects of atmospheric noise and point ...along the Fourier axis corresponding to map declination are filtered out to reduce the effects of ... See full document
5
THE ATACAMA COSMOLOGY TELESCOPE: PHYSICAL PROPERTIES OF SUNYAEV ZEL'DOVICH EFFECT CLUSTERS ON THE CELESTIAL EQUATOR
... that the ACT clusters indeed comprise a massive sample, we present the RASS X-ray fluxes and luminosities for all of the confirmed ACT clusters, regardless of the significance of the ... See full document
18
The Atacama cosmology telescope: cosmological parameters from the 2008 power spectrum
... on the Chajnantor Science preserve, which was made possible by the Chilean Comisi´on Nacional de Investigaci´on Cient´ıfica y ...for the assistance we received at various times from the ... See full document
20
The Atacama Cosmology Telescope: Beam Measurements and the Microwave Brightness Temperatures of Uranus and Saturn
... observer. The model is symmetric about B = 0 by construction. As the absolute value of B increases, the increased radiation from the rings and decreased flux from the obscured disk ... See full document
13
The Atacama cosmology telescope: high resolution sunyaev zel'dovich array observations of act sze selected clusters from the equatorial strip
... radio sources is higher in cluster regions compared to the field (Cooray et ...of the SZE signal from radio sources could potentially bias flux and mass estimates from the ... See full document
12
THE NuSTAR EXTRAGALACTIC SURVEY: A FIRST SENSITIVE LOOK AT THE HIGH ENERGY COSMIC X RAY BACKGROUND POPULATION
... different sources, which we list ...with the Florida Infrared Imag- ing Multi-object Spectrograph on the Kitt Peak ...m telescope. The data were obtained on UT 2012 October 17 in ... See full document
20
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 ...al. 2008; Das et ...from the CMB alone provide direct constraints on the evolution of gravitational ... See full document
9
The Atacama cosmology telescope: a measurement of the cosmic microwave background power spectrum at 148 and 218 ghz from the 2008 southern survey
... of the CMB power spectrum over the range of multipoles 500 < < 10,000 from the Atacama Cosmology Telescope (ACT) using the 148 GHz and 218 GHz ... See full document
16
Atacama Cosmology Telescope: A measurement of the thermal Sunyaev Zel'dovich effect using the skewness of the CMB temperature distribution
... point sources, a small residual point source contamination of the signal could remain, leading to an underestimate of the amplitude of the tSZ ...vary the level at which point ... See full document
12
The Atacama Cosmology Telescope: Sunyaev Zel'dovich selected galaxy clusters at 148 GHz from three seasons of data
... beyond the UPP prescription. Assuming a concordance cosmology, the UPP scalings are found to be nearly identical to an adiabatic model, while a model incorporating non-thermal pressure better matches ... See full document
63
GRAWITA: VLT Survey Telescope observations of the gravitational wave sources GW150914 and GW151226
... of sources provided by the ph-pipe is ...by the diff-pipe. The smaller number of sources detected by the ph-pipeis due to (i) the removal of all the ‘bright’ and/or ... See full document
16
Evidence for Dark Energy from the Cosmic Microwave Background Alone Using the Atacama Cosmology Telescope Lensing Measurements
... observing the CMB at higher resolution, however, one can break the geometric degeneracy using the effect of gravity on the CMB [14]: the deflection of CMB photons on arc minute ... See full document
5
NUSTAR Unveils a Heavily Obscured Low luminosity Active Galactic Nucleus in the Luminous Infrared Galaxy NGC 6286
... which at the distance of the source corresponds to ∼ ...plasma in a star-forming region, to scattered radiation from the AGN to X-ray binaries, or to shocks created by the ... See full document
13
Searching for extragalactic sources in the VISTA variables in the Via láctea survey
... m. The VVV is one of the six largest ESO public surveys conducted using this telescope without any overlapping ...regions. The VVV images ( Tiles ) are produced by six single pointing ... See full document
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