[PDF] Top 20 The Atacama cosmology telescope: a measurement of the cosmic microwave background power spectrum at 148 and 218 ghz from the 2008 southern survey
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The Atacama cosmology telescope: a measurement of the cosmic microwave background power spectrum at 148 and 218 ghz from the 2008 southern survey
... generate the number of point sources in that bin as a Poisson realization from the model flux distribution dN/dS (the upper limit is chosen to be the approximate 5σ detection ... See full document
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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 ... See full document
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THE ATACAMA COSMOLOGY TELESCOPE: LENSING OF CMB TEMPERATURE AND POLARIZATION DERIVED FROM COSMIC INFRARED BACKGROUND CROSS CORRELATION
... obtained at 545 GHz using the Planck satellite that overlap the ACTPol D1, D5, and D6 survey ...regions. The Planck maps for the nominal mission were retrieved ... See full document
9
The Atacama Cosmology Telescope: Beam Measurements and the Microwave Brightness Temperatures of Uranus and Saturn
... describe the measurement of the beam profiles and window functions for the Atacama Cosmology Telescope (ACT), which operated from 2007 to 2010 with ... See full document
13
The Atacama cosmology telescope: Cross correlation of cosmic microwave background lensing and quasars
... measure the cross-correlation of Atacama cosmology telescope cosmic microwave background (CMB) lensing convergence maps with quasar maps made from the ... See full document
8
Subaru weak lensing measurement of a z=0 81 cluster discovered by the Atacama Cosmology Telescope Survey
... photons of the cosmic microwave background (CMB) scatter off electrons of the hot intracluster medium, is a powerful way of finding massive clusters, especially ... See full document
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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 ... See full document
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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 ... See full document
10
The Atacama cosmology telescope: extragalactic sources at 148 GHZ in the 2008 survey
... values. The ACT results are also consistent with counts reported by the SPT (Vieira et ...part of the WMAP 7 year analysis, Wright et ...counts at 30 GHz from WMAP, ... See full document
15
Detection of the Power Spectrum of Cosmic Microwave Background Lensing by the Atacama Cosmology Telescope
... minimize the effects of atmospheric noise and point ...‘‘stripe’’ of width ‘ ¼ 180 along the Fourier axis corresponding to map declination are filtered out to reduce the effects ... See full document
5
Evidence of Lensing of the Cosmic Microwave Background by Dark Matter Halos
... galaxy from the ACTPol temperature maps, we exclude all galaxies whose stamp does not fall entirely within the corresponding ACTPol ...find from simulations that this stamp size is roughly ... See full document
8
Microwave radiation and protein addition modulate hydration, pasting and gel rheological characteristics of rice and potato starches
... in the loss tangent, which meant a reinforcement of the elastic character of gels made from MW-treated starches or starch+protein blends compared to the untreated ...decreased ... See full document
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THE ATACAMA COSMOLOGY TELESCOPE: PHYSICAL PROPERTIES OF SUNYAEV ZEL'DOVICH EFFECT CLUSTERS ON THE CELESTIAL EQUATOR
... 2010a) and to establish qualitatively that the ACT clusters indeed comprise a massive sample, we present the RASS X-ray fluxes and luminosities for all of the confirmed ACT ... See full document
18
Cosmological parameters from pre planck cosmic microwave background measurements
... follow the method introduced in Ref. [8] to estimate the primary CMB bandpowers from both sets of spectra, marginalizing over the possible additional power from Galactic ... See full document
5
Separating the weak lensing and kinetic Sunyaev Zeldovich effects from cosmic microwave background temperature maps
... scales, the main features of the CMB are fluctuations generated at the last scattering surface (z ...through the interaction between the CMB and the ... See full document
6
The Atacama cosmology telescope: high resolution sunyaev zel'dovich array observations of act sze selected clusters from the equatorial strip
... on the S82 region as optical data are available from which we measure cluster redshifts and estimate cluster masses via richness and ...are the most massive systems, which provide ... See full document
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THE NuSTAR EXTRAGALACTIC SURVEY: A FIRST SENSITIVE LOOK AT THE HIGH ENERGY COSMIC X RAY BACKGROUND POPULATION
... photometry from different sources, which we list ...measured from 1.56 ks of dithered observations obtained with the Florida Infrared Imag- ing Multi-object Spectrograph on the Kitt ... See full document
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Luminosity functions of LMXBs in different stellar environments
... If the time span of observations is longer than the typical time scale of transient sources, averaging of their luminosity can also modify the shape of the ... See full document
15
Chronology, stratigraphy and hydrological modelling of extensive wetlands and paleolakes in the hyperarid core of the Atacama Desert during the late quaternary
... Paleobiogeography of the hyperarid core and cultural impacts The new emerging view of the hyperarid Atacama Desert during the late Pleistocene is one of ... See full document
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Impacto de las técnicas de calibración para el ARV en la caracterización de transistores de potencia de microondas mediante sistemas de sintonización de CargaThe impact of VNA calibration techniques on the load-pull characterization of microwave power transistors
... objective of the characterization of a device using a LP system is the evaluation of its performance under different loading conditions in order to determine the load under which ... See full document
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