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of 4 812
pro vyhledávání: '"Myers, M"'
Autor:
Kasha, A., Myers, M., Hathon, L., Sakhaee-Pour, A., Sadooni, F., Nasser, M., Hussein, I., Al-Kuwari, H.A.
Publikováno v:
In Geoenergy Science and Engineering November 2023 230
Autor:
Muretta, JM *, Rajasekaran, D, Blat, Y, Little, S, Myers, M, Nair, C, Burdekin, B, Yuen, SL, Jimenez, N, Guhathakurta, P, Wilson, A, Thompson, AR, Surti, N, Connors, D, Chase, P, Harden, D, Barbieri, CM, Adam, L, Thomas, DD *
Publikováno v:
In SLAS Discovery July 2023 28(5):223-232
Akademický článek
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Autor:
Tanvir, N. R., Fynbo, J. P. U., Postigo, A. de Ugarte, Japelj, J., Wiersema, K., Malesani, D., Perley, D. A., Levan, A. J., Selsing, J., Cenko, S. B., Kann, D. A., Milvang-Jensen, B., Berger, E., Cano, Z., Chornock, R., Covino, S., Cucchiara, A., D'Elia, V., Goldoni, P., Gomboc, A., Heintz, K. E., Hjorth, J., Izzo, L., Jakobsson, P., Kaper, L., Kruehler, T., Laskar, T., Myers, M., Piranomonte, S., Pugliese, G., Sanchez-Ramirez, R., Schulze, S., Sparre, M., Stanway, E. R., Tagliaferri, G., Thoene, C. C., Vergani, S., Vreeswijk, P. M., Wijers, R. A. M. J., Watson, D., Xu, D.
The part played by stars in the ionization of the intergalactic medium remains an open question. A key issue is the proportion of the stellar ionizing radiation that escapes the galaxies in which it is produced. Spectroscopy of gamma-ray burst afterg
Externí odkaz:
http://arxiv.org/abs/1805.07318
Publikováno v:
In Journal of Environmental Management 1 September 2022 317
Autor:
Obenschain, S. P., Schmitt, A. J., Bates, J. W., Wolford, M. F., Myers, M. C., McGeoch, M. W., Karasik, M., Weaver, J. L.
Publikováno v:
Philosophical Transactions: Mathematical, Physical and Engineering Sciences, 2020 Nov . 378(2184), 1-12.
Externí odkaz:
https://www.jstor.org/stable/27101065
Autor:
Errard, J., Ade, P. A. R., Akiba, Y., Arnold, K., Atlas, M., Baccigalupi, C., Barron, D., Boettger, D., Borrill, J., Chapman, S., Chinone, Y., Cukierman, A., Delabrouille, J., Dobbs, M., Ducout, A., Elleflot, T., Fabbian, G., Feng, C., Feeney, S., Gilbert, A., Goeckner-Wald, N., Halverson, N. W., Hasegawa, M., Hattori, K., Hazumi, M., Hill, C., Holzapfel, W. L., Hori, Y., Inoue, Y., Jaehnig, G. C., Jaffe, A. H., Jeong, O., Katayama, N., Kaufman, J., Keating, B., Kermish, Z., Keskitalo, R., Kisner, T., Jeune, M. Le, Lee, A. T., Leitch, E. M., Leon, D., Linder, E., Matsuda, F., Matsumura, T., Miller, N. J., Myers, M. J., Navaroli, M., Nishino, H., Okamura, T., Paar, H., Peloton, J., Poletti, D., Puglisi, G., Rebeiz, G., Reichardt, C. L., Richards, P. L., Ross, C., Rotermund, K. M., Schenck, D. E., Sherwin, B. D., Siritanasak, P., Smecher, G., Stebor, N., Steinbach, B., Stompor, R., Suzuki, A., Tajima, O., Takakura, S., Tikhomirov, A., Tomaru, T., Whitehorn, N., Wilson, B., Yadav, A., Zahn, O.
Publikováno v:
The Astrophysical Journal, Volume 809, Issue 1, article id. 63, 19 pp. (2015)
Atmosphere is one of the most important noise sources for ground-based cosmic microwave background (CMB) experiments. By increasing optical loading on the detectors, it amplifies their effective noise, while its fluctuations introduce spatial and tem
Externí odkaz:
http://arxiv.org/abs/1501.07911
Autor:
Barron, D., Ade, P. A. R., Akiba, Y., Aleman, C., Arnold, K., Atlas, M., Bender, A., Boettger, D., Borrill, J., Chapman, S., Chinone, Y., Cukierman, A., Dobbs, M., Elleflot, T., Errard, J., Fabbian, G., Feng, C., Gilbert, A., Goeckner-Wald, N., Halverson, N. W., Hasegawa, M., Hattori, K., Hazumi, M., Holzapfel, W. L., Hori, Y., Inoue, Y., Jaehnig, G. C., Jaffe, A. H., Katayama, N., Keating, B., Kermish, Z., Keskitalo, R., Kisner, T., Jeune, M. Le, Lee, A. T., Leitch, E. M., Linder, E., Matsuda, F., Matsumura, T., Meng, X., Morii, H., Myers, M. J., Navaroli, M., Nishino, H., Okamura, T., Paar, H., Peloton, J., Poletti, D., Raum, C., Rebeiz, G., Reichardt, C. L., Richards, P. L., Ross, C., Rotermund, K., Schenck, D. E., Sherwin, B. D., Shirley, I., Sholl, M., Siritanasak, P., Smecher, G., Stebor, N., Steinbach, B., Stompor, R., Suzuki, A., Suzuki, J., Takada, S., Takakura, S., Tomaru, T., Wilson, B., Yadav, A., Yamaguchi, H., Zahn, O.
Publikováno v:
Proc. SPIE 9153 (915335), 2014
POLARBEAR-2 is a next-generation receiver for precision measurements of the polarization of the cosmic microwave background (Cosmic Microwave Background (CMB)). Scheduled to deploy in early 2015, it will observe alongside the existing POLARBEAR-1 rec
Externí odkaz:
http://arxiv.org/abs/1410.7488
Autor:
Benson, B. A., Ade, P. A. R., Ahmed, Z., Allen, S. W., Arnold, K., Austermann, J. E., Bender, A. N., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H. M., Ciocys, S. T., Cliche, J. F., Crawford, T. M., Cukierman, A., de Haan, T., Dobbs, M. A., Dutcher, D., Everett, W., Gilbert, A., Halverson, N. W., Hanson, D., Harrington, N. L., Hattori, K., Henning, J. W., Hilton, G. C., Holder, G. P., Holzapfel, W. L., Irwin, K. D., Keisler, R., Knox, L., Kubik, D., Kuo, C. L., Lee, A. T., Leitch, E. M., Li, D., McDonald, M., Meyer, S. S., Montgomery, J., Myers, M., Natoli, T., Nguyen, H., Novosad, V., Padin, S., Pan, Z., Pearson, J., Reichardt, C. L., Ruhl, J. E., Saliwanchik, B. R., Simard, G., Smecher, G., Sayre, J. T., Shirokoff, E., Stark, A. A., Story, K., Suzuki, A., Thompson, K. L., Tucker, C., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Wang, G., Yefremenko, V., Yoon, K. W.
We describe the design of a new polarization sensitive receiver, SPT-3G, for the 10-meter South Pole Telescope (SPT). The SPT-3G receiver will deliver a factor of ~20 improvement in mapping speed over the current receiver, SPTpol. The sensitivity of
Externí odkaz:
http://arxiv.org/abs/1407.2973
Autor:
The POLARBEAR Collaboration, Ade, P. A. R., Akiba, Y., Anthony, A. E., Arnold, K., Atlas, M., Barron, D., Boettger, D., Borrill, J., Chapman, S., Chinone, Y., Dobbs, M., Elleflot, T., Errard, J., Fabbian, G., Feng, C., Flanigan, D., Gilbert, A., Grainger, W., Halverson, N. W., Hasegawa, M., Hattori, K., Hazumi, M., Holzapfel, W. L., Hori, Y., Howard, J., Hyland, P., Inoue, Y., Jaehnig, G. C., Jaffe, A. H., Keating, B., Kermish, Z., Keskitalo, R., Kisner, T., Jeune, M. Le, Lee, A. T., Leitch, E. M., Linder, E., Lungu, M., Matsuda, F., Matsumura, T., Meng, X., Miller, N. J., Morii, H., Moyerman, S., Myers, M. J., Navaroli, M., Nishino, H., Paar, H., Peloton, J., Poletti, D., Quealy, E., Rebeiz, G., Reichardt, C. L., Richards, P. L., Ross, C., Schanning, I., Schenck, D. E., Sherwin, B. D., Shimizu, A., Shimmin, C., Shimon, M., Siritanasak, P., Smecher, G., Spieler, H., Stebor, N., Steinbach, B., Stompor, R., Suzuki, A., Takakura, S., Tomaru, T., Wilson, B., Yadav, A., Zahn, O.
Publikováno v:
Astrophysical Journal, 794:171, 2014
We report a measurement of the B-mode polarization power spectrum in the cosmic microwave background (CMB) using the POLARBEAR experiment in Chile. The faint B-mode polarization signature carries information about the Universe's entire history of gra
Externí odkaz:
http://arxiv.org/abs/1403.2369