The Planck High Frequency Instrument, a third generation CMB experiment, and a full sky submillimeter survey

被引：71

作者：

Lamarre, JM

Puget, JL

Bouchet, F

Ade, PAR

Benoit, A

Bernard, JP

Bock, J

De Bernardis, P

Charra, J

Couchot, F

Delabrouille, J

Efstathiou, G

Giard, M

Guyot, G

Lange, A

Maffei, B

Murphy, A

Pajot, F

Piat, M

Ristorcelli, I

Santos, D

Sudiwala, R

Sygnet, JF

Torre, JP

Yurchenko, V

Yvon, D

机构：

[1] Observ Paris, LERMA, F-75014 Paris, France

[2] Univ Paris 11, Inst Astrophys Spatiale, F-91405 Orsay, France

[3] Inst Astrophys, F-75014 Paris, France

[4] Cardiff Univ, Cardiff, S Glam, Wales

[5] CNRS, CRTBT, F-38026 Grenoble, France

[6] CESR, F-31018 Toulouse, France

[7] CALTECH, Jet Prop Lab, Pasadena, CA USA

[8] Univ Roma La Sapienza, Rome, Italy

[9] UPX, IN2P3, Lab Accelerateur Lineaire, F-91405 Orsay, France

[10] Coll France, PCC, F-75231 Paris, France

[11] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England

[12] CALTECH, Pasadena, CA 91125 USA

[13] State Univ Maynooth, Dept Phys, Maynooth, Kildare, Ireland

[14] ISN, IN2P3, F-38026 Grenoble, France

[15] CEA, SPP, DAPNIA, Gif Sur Yvette, France

来源：

NEW ASTRONOMY REVIEWS | 2003年 / 47卷 / 11-12期

关键词：

D O I：

10.1016/j.newar.2003.09.006

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The High Frequency Instrument (HFI) of Planck is the most sensitive CMB experiment ever planned. Statistical fluctuations (photon noise) of the CMB itself will be the major limitation to the sensitivity of the CMB channels. Higher frequency channels will measure galactic foregrounds. Together with the Low Frequency Instrument, this will make a unique tool to measure the full sky and to separate the various components of its spectrum. Measurement of the polarization of these various components will give a new picture of the CMB. In addition, HFI will provide the scientific community with new full sky maps of intensity and polarization at six frequencies, with unprecedented angular resolution and sensitivity. This paper describes the logics that prevailed to define the HFI and the performances expected from this instrument. It details several features of the HFI design that has not been published up to now. (C) 2003 Published by Elsevier B.V.

引用

页码：1017 / 1024

页数：8

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