Zobrazeno 1 - 7
of 7
pro vyhledávání: '"WILBANKS, T. M."'
Autor:
Holzapfel, W. L., Wilbanks, T. M., Ade, P. A. R., Church, S. E., Fischer, M. L., Mauskopf, P. D., Osgood, D. E., Lange, A. E.
Measurements of the Sunyaev-Zel'dovich (S-Z) effect towards distant clusters of galaxies can be used to determine the Hubble constant and the radial component of cluster peculiar velocities. Determination of the cluster peculiar velocity requires the
Externí odkaz:
http://arxiv.org/abs/astro-ph/9702222
Autor:
Holzapfel, W. L., Arnaud, M., Ade, P. A. R., Church, S. E., Fischer, M. L., Mauskopf, P. D., Rephaeli, Y., Wilbanks, T. M., Lange, A. E.
We report 2.1 mm observations of the Sunyaev-Zel'dovich (S-Z) effect; these observations confirm our previous detection of a decrement in the Cosmic Microwave Background intensity towards the cluster Abell 2163. The S-Z data are analyzed using the re
Externí odkaz:
http://arxiv.org/abs/astro-ph/9702224
Autor:
Holzapfel, W. L., Ade, P. A. R., Church, S. E., Mauskopf, P. D., Rephaeli, Y., Wilbanks, T. M., Lange, A. E.
We report millimeter-wavelength observations of the Sunyaev-Zel'dovich (S-Z) effect in two distant galaxy clusters. A relativistically correct analysis of the S-Z data is combined with the results of X-ray observations to determine the radial peculia
Externí odkaz:
http://arxiv.org/abs/astro-ph/9702223
An Upper Limit to Arcminute Scale Anisotropy in the Cosmic Microwave Background Radiation at 142 GHz
Autor:
Church, S. E., Ganga, K. M., Ade, P. A. R., Holzapfel, W. L., Mauskopf, P. D., Wilbanks, T. M., Lange, A. E.
We present limits to anisotropies in the cosmic microwave background radiation (CMB) at angular scales of a few arcminutes. The observations were made at a frequency of 142 GHz using a 6-element bolometer array (the Sunyaev-Zel'dovich Infrared Experi
Externí odkaz:
http://arxiv.org/abs/astro-ph/9702196
Autor:
Church, S. E., Mauskopf, P. D., Ade, P. A. R., Devlin, M. J., Holzapfel, W. L., Wilbanks, T. M., Lange, A. E.
We have searched for mm-wave emission from compact objects in two fields, each approximately 1 square degree in size, taken from regions of the sky in which degree-scale structure in the Cosmic Background Radiation (CBR) has recently been reported. T
Externí odkaz:
http://arxiv.org/abs/astro-ph/9409020
Publikováno v:
Annals of the New York Academy of Sciences; 1993, Vol. 688 Issue 1, p798-800, 3p
Publikováno v:
Applied optics [Appl Opt] 1992 Dec 01; Vol. 31 (34), pp. 7214-8.