QUIJOTE 宇宙微波背景实验
天体物理学
2015-05-13 v1
摘要
我们介绍了 QUIJOTE (Q-U-I JOint TEnerife) 宇宙微波背景实验的当前状态，这是一个将于 2009 年初在泰德天文台开始运行的新仪器，旨在表征宇宙微波背景的极化以及银河系和河外辐射在 10-30 GHz 频率范围和较大角尺度上的其他过程。QUIJOTE 将成为 PLANCK 任务在低频段的重要补充，并且具有所需的灵敏度，如果张量标量比大于 r=0.05，则能够探测到原初引力波成分。
引用
@article{arxiv.0810.3141,
title = {The Quijote CMB Experiment},
author = {J. A. Rubino-Martin and R. Rebolo and M. Tucci and R. Genova-Santos and S. R. Hildebrandt and R. Hoyland and J. M. Herreros and F. Gomez-Renasco and C. Lopez Caraballo and E. Martinez-Gonzalez and P. Vielva and D. Herranz and F. J. Casas and E. Artal and B. Aja and L. de la Fuente and J. L. Cano and E. Villa and A. Mediavilla and J. P. Pascual and L. Piccirillo and B. Maffei and G. Pisano and R. A. Watson and R. Davis and R. Davies and R. Battye and R. Saunders and K. Grainge and P. Scott and M. Hobson and A. Lasenby and G. Murga and C. Gomez and A. Gomez and J. Arino and R. Sanquirce and J. Pan and A. Vizcarguenaga and B. Etxeita},
journal= {arXiv preprint arXiv:0810.3141},
year = {2015}
}
备注
9 pages, 5 figures. To appear in "Highlights of Spanish Astrophysics V", Proceedings of the VIII Scientific Meeting of the Spanish Astronomical Society (SEA) held in Santander, 7-11 July, 2008. Edited by J. Gorgas, L. J. Goicoechea, J. I. Gonzalez-Serrano, J. M. Diego