Zobrazeno 1 - 10
of 97
pro vyhledávání: '"Torbet, E."'
Autor:
Masi, S, Ade, P, Bock, J, Bond, J, Borrill, J, Boscaleri, A, Cabella, P, Contaldi, C, Crill, B, de Bernardis, P, De Gasperis, G, de Oliveira-Costa, A, De Troia, G, Di Stefano, G, Ehlers, P, Hivon, E, Hristov, V, Iacoangeli, A, Jaffe, A, Jones, W, Kisner, T, Lange, A, MacTavish, C, Marini-Bettolo, C, Mason, P, Mauskopf, P, Montroy, T, Nati, F, Nati, L, Natoli, P, Netterfield, C, Pascale, E, Piacentini, F, Pogosyan, D, Polenta, G, Prunet, S, Ricciardi, S, Romeo, G, Ruhl, J, Santini, P, Tegmark, M, Torbet, E, Veneziani, M, Vittorio, N
We present the BOOMERanG-03 experiment and maps of the Stokes parameters I, Q, U of the microwave sky obtained during a 14 day balloon flight in 2003. Three regions of the southern sky were surveyed: a deep survey (~ 90 square degrees) and a shallow
Externí odkaz:
http://arxiv.org/abs/astro-ph/0507509
Autor:
Romer, A. K., Gomez, P. L., Cantalupo, C. M., Daub, M. D., Goldstein, J. H., Holzapfel, W. L., Kuo, C. L., Lange, A. E., Lueker, M., Newcomb, M., Peterson, J. B., Ruhl, J. E., Runyan, M. C., Torbet, E., Reichardt, C.
During 2001 and 2002, observations of several X-ray bright clusters of galaxies were conducted using the ACBAR Bolometer Array on the South Pole Viper telescope. A multi-frequency analysis of these clusters is currently underway. This multi-frequency
Externí odkaz:
http://arxiv.org/abs/astro-ph/0311261
Autor:
Montroy, T., Ade, P. A. R., Balbi, A., Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C. R., Crill, B. P., de Bernardis, P., De Gasperis, G., de Oliveira-Costa, A., De Troia, G., di Stefano, G., Ganga, K., Hivon, E., Hristov, V. V., Iacoangeli, A., Jaffe, A. H., Kisner, T. S., Jones, W. C., Lange, A. E., Masi, S., Mauskopf, P. D., MacTavish, C., Melchiorri, A., Nati, F., Natoli, P., Netterfield, C. B., Pascale, E., Piacentini, F., Pogosyan, D., Polenta, G., Prunet, S., Ricciardi, S., Romeo, G., Ruhl, J. E., Torbet, E., Tegmark, M., Vittorio, N.
Publikováno v:
New Astron.Rev.47:1057-1065,2003
BOOMERANG is a balloon-borne telescope designed for long duration (LDB) flights around Antarctica. The second LDB Flight of BOOMERANG took place in January 2003. The primary goal of this flight was to measure the polarization of the CMB. The receiver
Externí odkaz:
http://arxiv.org/abs/astro-ph/0305593
Autor:
Runyan, M. C., Ade, P. A. R., Bock, J. J., Bond, J. R., Cantalupo, C., Contaldi, C. R., Daub, M. D., Goldstein, J. H., Gomez, P. L., Holzapfel, W. L., Kuo, C. L., Lange, A. E., Lueker, M., Newcomb, M., Peterson, J. B., Pogosyan, D., Romer, A. K., Ruhl, J., Torbet, E., Woolsey, D.
We review the first science results from the Arcminute Cosmology Bolometer Array Receiver (ACBAR); a multifrequency millimeter-wave receiver optimized for observations of the Cosmic Microwave Background (CMB) and the Sunyaev-Zel'dovich (SZ) effect in
Externí odkaz:
http://arxiv.org/abs/astro-ph/0305553
Autor:
Runyan, M. C., Ade, P. A. R., Bhatia, R. S., Bock, J. J., Daub, M. D., Goldstein, J. H., Haynes, C. V., Holzapfel, W. L., Kuo, C. L., Lange, A. E., Leong, J., Lueker, M., Newcomb, M., Peterson, J. B., Ruhl, J., Sirbi, G., Torbet, E., Tucker, C., Turner, A. D., Woolsey, D.
Publikováno v:
Astrophys.J.Suppl. 149 (2003) 265
We describe the Arcminute Cosmology Bolometer Array Receiver (ACBAR); a multifrequency millimeter-wave receiver designed for observations of the Cosmic Microwave Background (CMB) and the Sunyaev-Zel'dovich effect in clusters of galaxies. The ACBAR fo
Externí odkaz:
http://arxiv.org/abs/astro-ph/0303515
Autor:
Gomez, P. L., Romer, A. K., Peterson, J. B., Cantalupo, C. M., Holzapfel, S. W. L., Kuo, C. L., Newcomb, M., Ruhl, J., Goldstein, J., Torbet, E., Runyan, M. C.
As part of a combined Sunyaev-Zeldovich Effect (SZE), X-ray and weak lensing survey of low redshift (z<0.1) X-ray clusters, we present SZE images of the z=0.059 X-ray cluster Abell 3266 at three observing frequencies (150, 220, 275 GHz) and after the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0301024
Autor:
Goldstein, J. H., Ade, P. A. R., Bock, J. J., Bond, J. R., Cantalupo, C., Contaldi, C. R., Daub, M. D., Holzapfel, W. L., Kuo, C., Lange, A. E., Lueker, M., Newcomb, M., Peterson, J. B., Pogosyan, D., Ruhl, J. E., Runyan, M. C., Torbet, E.
Publikováno v:
Astrophys.J. 599 (2003) 773-785
We report an investigation of cosmological parameters based on the measurements of anisotropy in the cosmic microwave background radiation (CMB) made by ACBAR. We use the ACBAR data in concert with other recent CMB measurements to derive Bayesian est
Externí odkaz:
http://arxiv.org/abs/astro-ph/0212517
Autor:
Kuo, C. L., Ade, P. A. R., Bock, J. J., Cantalupo, C., Daub, M. D., Goldstein, J., Holzapfel, W. L., Lange, A. E., Lueker, M., Newcomb, M., Peterson, J. B., Ruhl, J., Runyan, M. C., Torbet, E.
Publikováno v:
Astrophys.J.600:32-51,2004
We report the first measurements of anisotropy in the cosmic microwave background (CMB) radiation with the Arcminute Cosmology Bolometer Array Receiver (ACBAR). The instrument was installed on the 2.1m Viper telescope at the South Pole in January 200
Externí odkaz:
http://arxiv.org/abs/astro-ph/0212289
Autor:
Miller, A., Beach, J., Bradley, S., Devlin, M. J., Caldwell, R., Chapman, H., Dorwart, W. B., Herbig, T., Jones, D., Monnelly, G., Netterfield, C. B., Nolta, M., Page, L. A., Puchalla, J., Robertson, T., Torbet, E., Tran, H. T., Vinje, W. E.
Publikováno v:
Astrophys.J.Suppl. 140 (2002) 115-142
We describe two related experiments that measured the anisotropy in the cosmic microwave background (CMB). QMAP was a balloon-borne telescope that flew twice in 1996, collecting data on degree angular scales with an array of six high electron mobilit
Externí odkaz:
http://arxiv.org/abs/astro-ph/0108030
Autor:
Puchalla, J. L., Caldwell, R., Cruz, K. L., Devlin, M. J., Dorwart, W. B., Herbig, T., Miller, A. D., Nolta, M. R., Page, L. A., Torbet, E., Tran, H. T.
We present multi-frequency maps of a portion of the Galactic Plane centered on a declination of -60 degrees with resolutions ranging from 0.2 to 0.9 degrees. The maps are optimized to detect unresolved source emission and are cross-calibrated against
Externí odkaz:
http://arxiv.org/abs/astro-ph/0005420