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Autor:
Holland, W. S., Bintley, D., Chapin, E. L., Chrysostomou, A., Davis, G. R., Dempsey, J. T., Duncan, W. D., Fich, M., Friberg, P., Halpern, M., Irwin, K. D., Jenness, T., Kelly, B. D., MacIntosh, M. J., Robson, E. I., Scott, D., Ade, P. A. R., Atad-Ettedgui, E., Berry, D. S., Craig, S. C., Gao, X., Gibb, A. G., Hilton, G. C., Hollister, M. I., Kycia, J. B., Lunney, D. W., McGregor, H., Montgomery, D., Parkes, W., Tilanus, R. P. J., Ullom, J. N., Walther, C. A., Walton, A. J., Woodcraft, A. L., Amiri, M., Atkinson, D., Burger, B., Chuter, T., Coulson, I. M., Doriese, W. B., Dunare, C., Economou, F., Niemack, M. D., Parsons, H. A. L., Reintsema, C. D., Sibthorpe, B., Smail, I., Sudiwala, R., Thomas, H. S.
SCUBA-2 is an innovative 10000 pixel bolometer camera operating at submillimetre wavelengths on the James Clerk Maxwell Telescope (JCMT). The camera has the capability to carry out wide-field surveys to unprecedented depths, addressing key questions
Externí odkaz:
http://arxiv.org/abs/1301.3650
Autor:
Burger, B., Herrmann, H.J.
Publikováno v:
In Physica A: Statistical Mechanics and its Applications 15 February 2019 516:125-132
Thesis (PhD (Geology))--University of Stellenbosch, 1997.
1123 leaves printed on single pages, preliminary pages and numbered pages 1-286. Includes bibliography, list of figures and tables and explanation of abbreviations used.
Digitized at
1123 leaves printed on single pages, preliminary pages and numbered pages 1-286. Includes bibliography, list of figures and tables and explanation of abbreviations used.
Digitized at
Externí odkaz:
http://hdl.handle.net/10019.1/4936
Autor:
O'Brient, R., Ade, P. A. R., Ahmed, Z., Aikin, R. W., Amiri, M., Benton, S., Bischoff, C., Bock, J. J., Bonetti, J. A., Brevik, J. A., Burger, B., Davis, G., Day, P., Dowell, C. D., Duband, L., Filippini, J. P., Fliescher, S., Golwala, S. R., Grayson, J., Halpern, M., Hasselfield, M., Hilton, G., Hristov, V. V., Hui, H., Irwin, K., Kernasovskiy, S., Kovac, J. M., Kuo, C. L., Leitch, E., Lueker, M., Megerian, K., Moncelsi, L., Netterfield, C. B., Nguyen, H. T., Ogburn IV, R. W., Pryke, C. L., Reintsema, C., Ruhl, J. E., Runyan, M. C., Schwarz, R., Sheehy, C. D., Staniszewski, Z., Sudiwala, R., Teply, G., Tolan, J. E., Turner, A. D., Tucker, R. S., Vieregg, A., Wiebe, D. V., Wilson, P., Wong, C. L., Wu, W. L. K., Yoon, K. W.
Between the BICEP2 and Keck Array experiments, we have deployed over 1500 dual polarized antenna coupled bolometers to map the Cosmic Microwave Background's polarization. We have been able to rapidly deploy these detectors because they are completely
Externí odkaz:
http://arxiv.org/abs/1208.1247
Autor:
Kernasovskiy, S., Ade, P. A. R., Aikin, R. W., Amiri, M., Benton, S., Bischoff, C., Bock, J. J., Bonetti, J. A., Brevik, J. A., Burger, B., Davis, G., Dowell, C. D., Duband, L., Filippini, J. P., Fliescher, S., Golwala, S. R., Halpern, M., Hasselfield, M., Hiltion, G., Hristov, V. V., Irwin, K., Kovac, J. M., Kuo, C. L., Leitch, E., Lueker, M., Netterfield, C. B., Nguyen, H. T., O'Brient, R., Ogburn IV, R. W., Pryke, C. L., Reintsema, C., Ruhl, J. E., Runyan, M. C., Schwarz, R., Sheehy, C. D., Staniszewski, Z., Sudiwala, R., Teply, G., Tolan, J. E., Turner, A. D., Vieregg, A., Wiebe, D. V., Wilson, P., Wongg, C. L.
The Keck Array (SPUD) began observing the cosmic microwave background's polarization in the winter of 2011 at the South Pole. The Keck Array follows the success of the predecessor experiments Bicep and Bicep2, using five on-axis refracting telescopes
Externí odkaz:
http://arxiv.org/abs/1208.0857
Autor:
Ogburn IV, R. W., Ade, P. A. R., Aikin, R. W., Amiri, M., Benton, S. J., Bischoff, C. A., Bock, J. J., Bonetti, J. A., Brevik, J. A., Bullock, E., Burger, B., Davis, G., Dowell, C. D., Duband, L., Filippini, J. P., Fliescher, S., Golwala, S. R., Gordon, M., Halpern, M., Hasselfield, M., Hilton, G., Hristov, V. V., Hui, H., Irwin, K., Kaufman, J. P., Keating, B. G., Kernasovskiy, S. A., Kovac, J. M., Kuo, C. L., Leitch, E. M., Lueker, M., Montroy, T., Netterfield, C. B., Nguyen, H. T., O'Brient, R., Orlando, A., Pryke, C. L., Reintsema, C., Richter, S., Ruhl, J. E., Runyan, M. C., Schwarz, R., Sheehy, C. D., Staniszewski, Z. K., Sudiwala, R. V., Teply, G. P., Thompson, K., Tolan, J. E., Turner, A. D., Vieregg, A. G., Wiebe, D. V., Wilson, P., Wong, C. L.
The BICEP2 and Keck Array experiments are designed to measure the polarization of the cosmic microwave background (CMB) on angular scales of 2-4 degrees (l=50-100). This is the region in which the B-mode signal, a signature prediction of cosmic infla
Externí odkaz:
http://arxiv.org/abs/1208.0638
Autor:
Fraisse, A. A., Ade, P. A. R., Amiri, M., Benton, S. J., Bock, J. J., Bond, J. R., Bonetti, J. A., Bryan, S., Burger, B., Chiang, H. C., Clark, C. N., Contaldi, C. R., Crill, B. P., Davis, G., Doré, O., Farhang, M., Filippini, J. P., Fissel, L. M., Gandilo, N. N., Golwala, S., Gudmundsson, J. E., Hasselfield, M., Hilton, G., Holmes, W., Hristov, V. V., Irwin, K., Jones, W. C., Kuo, C. L., MacTavish, C. J., Mason, P. V., Montroy, T. E., Morford, T. A., Netterfield, C. B., O'Dea, D. T., Rahlin, A. S., Reintsema, C., Ruhl, J. E., Runyan, M. C., Schenker, M. A., Shariff, J. A., Soler, J. D., Trangsrud, A., Tucker, C., Tucker, R. S., Turner, A. D., Wiebe, D.
Publikováno v:
JCAP04(2013)047
We evaluate the ability of SPIDER, a balloon-borne polarimeter, to detect a divergence-free polarization pattern ("B-modes") in the Cosmic Microwave Background (CMB). In the inflationary scenario, the amplitude of this signal is proportional to that
Externí odkaz:
http://arxiv.org/abs/1106.3087
Autor:
Filippini, J. P., Ade, P. A. R., Amiri, M., Benton, S. J., Bihary, R., Bock, J. J., Bond, J. R., Bonetti, J. A., Bryan, S. A., Burger, B., Chiang, H. C., Contaldi, C. R., Crill, B. P., Doré, O., Farhang, M., Fissel, L. M., Gandilo, N. N., Golwala, S. R., Gudmundsson, J. E., Halpern, M., Hasselfield, M., Hilton, G., Holmes, W., Hristov, V. V., Irwin, K. D., Jones, W. C., Kuo, C. L., MacTavish, C. J., Mason, P. V., Montroy, T. E., Morford, T. A., Netterfield, C. B., O'Dea, D. T., Rahlin, A. S., Reintsema, C. D., Ruhl, J. E., Runyan, M. C., Schenker, M. A., Shariff, J. A., Soler, J. D., Trangsrud, A., Tucker, C., Tucker, R. S., Turner, A. D.
We describe SPIDER, a balloon-borne instrument to map the polarization of the millimeter-wave sky with degree angular resolution. Spider consists of six monochromatic refracting telescopes, each illuminating a focal plane of large-format antenna-coup
Externí odkaz:
http://arxiv.org/abs/1106.2158
Autor:
Sheehy, C. D., Ade, P. A. R., Aikin, R. W., Amiri, M., Benton, S., Bischoff, C., Bock, J. J., Bonetti, J. A., Brevik, J. A., Burger, B., Dowell, C. D., Duband, L., Filippini, J. P., Golwala, S. R., Halpern, M., Hasselfield, M., Hilton, G., Hristov, V. V., Irwin, K., Kaufman, J. P., Keating, B. G., Kovac, J. M., Kuo, C. L., Lange, A. E., Leitch, E. M., Lueker, M., Netterfield, C. B., Nguyen, H. T., Ogburn IV, R. W., Orlando, A., Pryke, C. L., Reintsema, C., Richter, S., Ruhl, J. E., Runyan, M. C., Staniszewski, Z., Stokes, S., Sudiwala, R., Teply, G., Thompson, K. L., Tolan, J. E., Turner, A. D., Wilson, P., Wong, C. L.
The Keck Array is a cosmic microwave background (CMB) polarimeter that will begin observing from the South Pole in late 2010. The initial deployment will consist of three telescopes similar to BICEP2 housed in ultra-compact, pulse tube cooled cryosta
Externí odkaz:
http://arxiv.org/abs/1104.5516