Zobrazeno 1 - 10
of 145
pro vyhledávání: '"Wünsche, C."'
Autor:
Wuensche, C. A., Reitano, L., Peel, M. W., Browne, I. W. A., Maffei, B., Abdalla, E., Radcliffe, C., Abdalla, F., Barosi, L., Liccardo, V., Mericia, E., Pisano, G., Strauss, C., Vieira, F., Villela, T., Wang, B.
The Baryon acoustic oscillations from Integrated Neutral Gas Observations (BINGO) telescope is a 40-m~class radio telescope under construction that has been designed to measure the large-angular-scale intensity of HI emission at 980--1260 MHz and hen
Externí odkaz:
http://arxiv.org/abs/1911.13188
Autor:
Peel, M. W., Wuensche, C. A., Abdalla, E., Anton, S., Barosi, L., Browne, I. W. A., Caldas, M., Dickinson, C., Fornazier, K. S. F., Monstein, C., Strauss, C., Tancredi, G., Villela, T.
The Baryon acoustic oscillations from Integrated Neutral Gas Observations (BINGO) telescope is a new 40-m class radio telescope to measure the large-angular-scale intensity of Hi emission at 980-1260 MHz to constrain dark energy parameters. As it nee
Externí odkaz:
http://arxiv.org/abs/1811.09464
BINGO is a unique radio telescope designed to make the first detection of Baryon Acoustic Oscillations (BAO) at radio frequencies. This will be achieved by measuring the distribution of neutral hydrogen gas at cosmological distances using a technique
Externí odkaz:
http://arxiv.org/abs/1803.01644
Publikováno v:
ApJ 826 121 (2016)
Evidences for late-time acceleration of the Universe are provided by multiple probes, such as Type Ia supernovae, the cosmic microwave background (CMB) and large-scale structure (LSS). In this work, we focus on the integrated Sachs--Wolfe (ISW) effec
Externí odkaz:
http://arxiv.org/abs/1512.00641
We present an upgraded combined estimator, based on Minkowski Functionals and Neural Networks, with excellent performance in detecting primordial non-Gaussianity in simulated maps that also contain a weighted mixture of Galactic contaminations, besid
Externí odkaz:
http://arxiv.org/abs/1409.3876
Publikováno v:
JCAP05(2014)039
Sunyaev-Zel'dovich (SZ) surveys are promising probes of cosmology - in particular for Dark Energy (DE) -, given their ability to find distant clusters and provide estimates for their mass. However, current SZ catalogs contain tens to hundreds of obje
Externí odkaz:
http://arxiv.org/abs/1312.4430
The extensive search for deviations from Gaussianity in cosmic microwave background radiation (CMB) data is very important due to the information about the very early moments of the universe encoded there. Recent analyses from Planck CMB data do not
Externí odkaz:
http://arxiv.org/abs/1312.3293
Autor:
Wuensche, C. A., Villela, T.
This article is a report of 25 years of Cosmic Microwave Background activities at INPE. Starting from balloon flights to measure the dipole anisotropy caused by the Earth's motion inside the CMB radiation field, whose radiometer was a prototype of th
Externí odkaz:
http://arxiv.org/abs/1002.4902
Autor:
Kogut, A., Fixsen, D. J., Levin, S. M., Limon, M., Lubin, P. M., Mirel, P., Seiffert, M., Singal, J., Villela, T., Wollack, E., Wuensche, C. A.
Publikováno v:
Astrophys.J.734:4,2011
We use absolutely calibrated data from the ARCADE 2 flight in July 2006 to model Galactic emission at frequencies 3, 8, and 10 GHz. The spatial structure in the data is consistent with a superposition of free-free and synchrotron emission. Emission w
Externí odkaz:
http://arxiv.org/abs/0901.0562
Autor:
Singal, J., Fixsen, D. J., Kogut, A., Levin, S., Limon, M., Lubin, P., Mirel, P., Seiffert, M., Villela, T., Wollack, E., Wuensche, C. A.
Publikováno v:
Astrophys.J.730:138,2011
The second generation Absolute Radiometer for Cosmology, Astrophysics, and Diffuse Emission (ARCADE 2) instrument is a balloon-borne experiment to measure the radiometric temperature of the cosmic microwave background and Galactic and extra-Galactic
Externí odkaz:
http://arxiv.org/abs/0901.0546