The new generation CMB B-mode polarization experiment: POLARBEAR

The new generation CMB B-mode polarization experiment: POLARBEAR
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发表时间：
2010-11
期刊：
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影响因子：
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通讯作者：
The Polarbear Collaboration J. Errard;P. Ade;A. Anthony;K. Arnold;F. Aubin;D. Boettger;J. Borrill;C. Cantalupo;M. Dobbs;D. Flanigan;A. Ghribi;N. Halverson;M. Hazumi;W. Holzapfel;J. Howard;P. Hyland;A. Jaffe;B. Keating;T. Kisner;Z. Kermish;A. Lee;E. Linder;M. Lungu;T. Matsumura;N. Miller;X. Meng;M. Myers;H. Nishino;R. O’Brient;D. O'Dea;C. Reichardt;I. Schanning;A. Shimizu;C. Shimmin;M. Shimon;H. Spieler;B. Steinbach;R. Stompor;A. Suzuki;T. Tomaru;H. Tran;C. Tucker;E. Quealy;P. Richards;O. Z. L. AstroparticuleCosmologie;7. Universit'eParis;France.;D. Physics;U. California;Berkeley U.S.;S. O. Physics;Astronomy;U. Cardiff;U.K.;Department of Astrophysical;P. Sciences;U. Colorado;U.S.;Center for Computational Astrophysics;S. Sciences;San Diego;Computational Cosmology Center;L. B. N. Laboratory;Space Sciences Laboratory;Berkeley;P. Department;Mcgill University;Canada.;High Energy Accelerator Research Organization;Tsukuba;Ibaraki;Japan.;I. College;P. Division
The Polarbear Collaboration J. Errard;P. Ade;A. Anthony;K. Arnold;F. Aubin;D. Boettger;J. Borrill;C. Cantalupo;M. Dobbs;D. Flanigan;A. Ghribi;N. Halverson;M. Hazumi;W. Holzapfel;J. Howard;P. Hyland;A. Jaffe;B. Keating;T. Kisner;Z. Kermish;A. Lee;E. Linder;M. Lungu;T. Matsumura;N. Miller;X. Meng;M. Myers;H. Nishino;R. O’Brient;D. O'Dea;C. Reichardt;I. Schanning;A. Shimizu;C. Shimmin;M. Shimon;H. Spieler;B. Steinbach;R. Stompor;A. Suzuki;T. Tomaru;H. Tran;C. Tucker;E. Quealy;P. Richards;O. Z. L. AstroparticuleCosmologie;7. Universit'eParis;France.;D. Physics;U. California;Berkeley U.S.;S. O. Physics;Astronomy;U. Cardiff;U.K.;Department of Astrophysical;P. Sciences;U. Colorado;U.S.;Center for Computational Astrophysics;S. Sciences;San Diego;Computational Cosmology Center;L. B. N. Laboratory;Space Sciences Laboratory;Berkeley;P. Department;Mcgill University;Canada.;High Energy Accelerator Research Organization;Tsukuba;Ibaraki;Japan.;I. College;P. Division
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文献类型：
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作者：
The Polarbear Collaboration J. Errard;P. Ade;A. Anthony;K. Arnold;F. Aubin;D. Boettger;J. Borrill;C. Cantalupo;M. Dobbs;D. Flanigan;A. Ghribi;N. Halverson;M. Hazumi;W. Holzapfel;J. Howard;P. Hyland;A. Jaffe;B. Keating;T. Kisner;Z. Kermish;A. Lee;E. Linder;M. Lungu;T. Matsumura;N. Miller;X. Meng;M. Myers;H. Nishino;R. O’Brient;D. O'Dea;C. Reichardt;I. Schanning;A. Shimizu;C. Shimmin;M. Shimon;H. Spieler;B. Steinbach;R. Stompor;A. Suzuki;T. Tomaru;H. Tran;C. Tucker;E. Quealy;P. Richards;O. Z. L. AstroparticuleCosmologie;7. Universit'eParis;France.;D. Physics;U. California;Berkeley U.S.;S. O. Physics;Astronomy;U. Cardiff;U.K.;Department of Astrophysical;P. Sciences;U. Colorado;U.S.;Center for Computational Astrophysics;S. Sciences;San Diego;Computational Cosmology Center;L. B. N. Laboratory;Space Sciences Laboratory;Berkeley;P. Department;Mcgill University;Canada.;High Energy Accelerator Research Organization;Tsukuba;Ibaraki;Japan.;I. College;P. Division

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我们描述了被称为极熊的宇宙微波背景(CMB)偏振实验。这项实验将使用配备有强大的1200测辐射热计阵列接收器的专用环天望远镜，以前所未有的精度绘制CMB的偏振。我们总结了实验，它的目标和现状。
We describe the Cosmic Microwave Background (CMB) polarization experiment called Polarbear. This experiment will use the dedicated Huan Tran Telescope equipped with a powerful 1,200-bolometer array receiver to map the CMB polarization with unprecedented accuracy. We summarize the experiment, its goals, and current status.