Zobrazeno 1 - 10
of 157
pro vyhledávání: '"BHATIA, R. S."'
Autor:
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., Bartlett, J. G., Bernard, J. -Ph., Bhatia, R. S., Blanchard, A., Bock, J. J., Boscaleri, A., Bouchet, F. R., Bourrachot, A., Camus, P., Couchot, F., de Bernardis, P., Delabrouille, J., Desert, F. -X., Doré, O., Douspis, M., Dumoulin, L., Dupac, X., Filliatre, P., Fosalba, P., Ganga, K., Gannaway, F., Gautier, B., Giard, M., Giraud-Heraud, Y., Gispert, R., Guglielmi, L., Hamilton, J. -Ch., Hanany, S., Henrot-Versille, S., Kaplan, J., Lagache, G., Lamarre, J. -M., Lange, A. E., Macias-Perez, J. F., Madet, K., Maffei, B., Magneville, Ch., Marrone, D. P., Masi, S., Mayet, F., Murphy, A., Naraghi, F., Nati, F., Patanchon, G., Perrin, G., Piat, M., Ponthieu, N., Prunet, S., Puget, J. -L., Renault, C., Rosset, C., Santos, D., Starobinsky, A., Strukov, I., Sudiwala, R. V., Teyssier, R., Tristram, M., Tucker, C., Vanel, J. -C., Vibert, D., Wakui, E., Yvon, D.
Publikováno v:
Astron.Astrophys. 424 (2004) 571-582
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was launched by CNES from the Swedish Esrange base near
Externí odkaz:
http://arxiv.org/abs/astro-ph/0306222
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:
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., Bartlett, J. G., Bernard, J. -Ph., Bhatia, R. S., Blanchard, A., Bock, J. J., Boscaleri, A., Bouchet, F. R., Bourrachot, A., Camus, P., Couchot, F., de Bernardis, P., Delabrouille, J., Desert, F. -X., Doré, O., Douspis, M., Dumoulin, L., Dupac, X., Filliatre, P., Fosalba, P., Ganga, K., Gannaway, F., Gautier, B., Giard, M., Giraud-Heraud, Y., Gispert, R., Guglielmi, L., Hamilton, J. -Ch., Hanany, S., Henrot-Versille, S., Kaplan, J., Lagache, G., Lamarre, J. -M., Lange, A. E., Macias-Perez, J. F., Madet, K., Maffei, B., Magneville, Ch., Marrone, D. P., Masi, S., Mayet, F., Murphy, A., Naraghi, F., Nati, F., Patanchon, G., Perrin, G., Piat, M., Ponthieu, N., Prunet, S., Puget, J. -L., Renault, C., Rosset, C., Santos, D., Starobinsky, A., Strukov, I., Sudiwala, R. V., Teyssier, R., Tristram, M., Tucker, C., Vanel, J. -C., Vibert, D., Wakui, E., Yvon, D.
Publikováno v:
Astron.Astrophys. 399 (2003) L25-L30
We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l and large l coverage down to COBE scales, Archeops p
Externí odkaz:
http://arxiv.org/abs/astro-ph/0210306
Autor:
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., Bartlett, J. G., Bernard, J. -Ph., Bhatia, R. S., Blanchard, A., Bock, J. J., Boscaleri, A., Bouchet, F. R., Bourrachot, A., Camus, P., Couchot, F., de Bernardis, P., Delabrouille, J., Desert, F. -X., Doré, O., Douspis, M., Dumoulin, L., Dupac, X., Filliatre, P., Fosalba, P., Ganga, K., Gannaway, F., Gautier, B., Giard, M., Giraud-Heraud, Y., Gispert, R., Guglielmi, L., Hamilton, J. -Ch., Hanany, S., Henrot-Versille, S., Kaplan, J., Lagache, G., Lamarre, J. -M., Lange, A. E., Macias-Perez, J. F., Madet, K., Maffei, B., Magneville, Ch., Marrone, D. P., Masi, S., Mayet, F., Murphy, A., Naraghi, F., Nati, F., Patanchon, G., Perrin, G., Piat, M., Ponthieu, N., Prunet, S., Puget, J. -L., Renault, C., Rosset, C., Santos, D., Starobinsky, A., Strukov, I., Sudiwala, R. V., Teyssier, R., Tristram, M., Tucker, C., Vanel, J. -C., Vibert, D., Wakui, E., Yvon, D.
Publikováno v:
Astron.Astrophys.399:L19-L23,2003
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived as a precursor of the Planck HFI instrument by usin
Externí odkaz:
http://arxiv.org/abs/astro-ph/0210305
Publikováno v:
SPIE Proceedings, Waikaloa 2002
We have developed a bolometric detector that is intrinsically sensitive to linear polarization which is optimized for making measurements of the polarization of the cosmic microwave background radiation. The receiver consists of a pair of co-located
Externí odkaz:
http://arxiv.org/abs/astro-ph/0209132
Autor:
Crill, B. P., Ade, P. A. R., Artusa, D. R., Bhatia, R. S., Bock, J. J., Boscaleri, A., Cardoni, P., Church, S. E., Coble, K., deBernardis, P., deTroia, G., Farese, P., Ganga, K. M., Giacometti, M., Haynes, C. V., Hivon, E., Hristov, V. V., Iacoangeli, A., Jones, W. C., Lange, A. E., Martinis, L., Masi, S., Mason, P. V., Mauskopf, P. D., Miglio, L., Montroy, T., Netterfield, C. B., Paine, C. G., Pascale, E., Piacentini, F., Polenta, G., Pongetti, F., Romeo, G., Ruhl, J. E., Scaramuzzi, F., Sforna, D., Turner, A. D.
Publikováno v:
Astrophys.J.Suppl.148:527-541,2003
We describe BOOMERANG; a balloon-borne microwave telescope designed to map the Cosmic Microwave Background (CMB) at a resolution of 10' from the Long Duration Balloon (LDB) platform. The millimeter-wave receiver employs new technology in bolometers,
Externí odkaz:
http://arxiv.org/abs/astro-ph/0206254
The Polatron: A Millimeter-Wave Cosmic Microwave Background Polarimeter for the OVRO 5.5 m Telescope
Autor:
Philhour, B. J., Keating, B. G., Ade, P. A. R., Bhatia, R. S., Bock, J. J., Church, S. E., Glenn, J., Hinderks, J. R., Hristov, V. V., Jones, W. C., Kamionkowski, M., Kumar, D. E., Lange, A. E., Leong, J. R., Marrone, D. P., Mason, B. S., Mason, P. V., Shuman, M. M., Sirbi, G. I.
We describe the development of a bolometric receiver designed to measure the arcminute-scale polarization of the cosmic microwave background (CMB). The Polatron will be mounted at the Cassegrain focus of the 5.5 m telescope at the Owens Valley Radio
Externí odkaz:
http://arxiv.org/abs/astro-ph/0106543
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