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

Jean Michael Lamarre; J. L. Puget; F. Bouchet; P. A R Ade; A. Benoit; J. P. Bernard; J. Bock; P. De Bernardis; J. Charra; F. Couchot; J. Delabrouille; G. Efstathiou; M. Giard; G. Guyot; A. Lange; B. Maffei; A. Murphy; F. Pajot; M. Piat; I. Ristorcelli; D. Santos; R. Sudiwala; J. F. Sygnet; J. P. Torre; V. Yurchenko; D. Yvon

doi:10.1016/j.newar.2003.09.006

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

Jean Michael Lamarre
, J. L. Puget
, F. Bouchet
, P. A R Ade
, A. Benoit
, J. P. Bernard
, J. Bock
, P. De Bernardis
, J. Charra
, F. Couchot
, J. Delabrouille
, G. Efstathiou
, M. Giard
, G. Guyot
, A. Lange
, B. Maffei
, A. Murphy
, F. Pajot
, M. Piat
, I. Ristorcelli

D. Santos, R. Sudiwala, J. F. Sygnet, J. P. Torre, V. Yurchenko, D. Yvon

Research output: Contribution to journal › Article › peer-review

Abstract

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. © 2003 Published by Elsevier B.V.

Original language	English
Pages (from-to)	1017-1024
Number of pages	7
Journal	New Astronomy Reviews
Volume	47
Issue number	11-12
DOIs	https://doi.org/10.1016/j.newar.2003.09.006
Publication status	Published - Dec 2003

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Lamarre, J. M., Puget, J. L., Bouchet, F., Ade, P. A. R., Benoit, A., Bernard, J. P., 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., ... Yvon, D. (2003). The Planck High Frequency Instrument, a third generation CMB experiment, and a full sky submillimeter survey. New Astronomy Reviews, 47(11-12), 1017-1024. https://doi.org/10.1016/j.newar.2003.09.006

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

abstract = "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. {\textcopyright} 2003 Published by Elsevier B.V.",

author = "Lamarre, \{Jean Michael\} and Puget, \{J. L.\} and F. Bouchet and Ade, \{P. A R\} and A. Benoit and Bernard, \{J. P.\} and J. Bock and \{De Bernardis\}, P. and J. Charra and F. Couchot and J. Delabrouille and G. Efstathiou and M. Giard and G. Guyot and A. Lange and B. Maffei and A. Murphy and F. Pajot and M. Piat and I. Ristorcelli and D. Santos and R. Sudiwala and Sygnet, \{J. F.\} and Torre, \{J. P.\} and V. Yurchenko and D. Yvon",

year = "2003",

month = dec,

doi = "10.1016/j.newar.2003.09.006",

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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 2003, 'The Planck High Frequency Instrument, a third generation CMB experiment, and a full sky submillimeter survey', New Astronomy Reviews, vol. 47, no. 11-12, pp. 1017-1024. https://doi.org/10.1016/j.newar.2003.09.006

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T1 - The Planck High Frequency Instrument, a third generation CMB experiment, and a full sky submillimeter survey

AU - Lamarre, Jean Michael

AU - Puget, J. L.

AU - Bouchet, F.

AU - Ade, P. A R

AU - Benoit, A.

AU - Bernard, J. P.

AU - Bock, J.

AU - De Bernardis, P.

AU - Charra, J.

AU - Couchot, F.

AU - Delabrouille, J.

AU - Efstathiou, G.

AU - Giard, M.

AU - Guyot, G.

AU - Lange, A.

AU - Maffei, B.

AU - Murphy, A.

AU - Pajot, F.

AU - Piat, M.

AU - Ristorcelli, I.

AU - Santos, D.

AU - Sudiwala, R.

AU - Sygnet, J. F.

AU - Torre, J. P.

AU - Yurchenko, V.

AU - Yvon, D.

PY - 2003/12

Y1 - 2003/12

N2 - 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. © 2003 Published by Elsevier B.V.

AB - 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. © 2003 Published by Elsevier B.V.

U2 - 10.1016/j.newar.2003.09.006

DO - 10.1016/j.newar.2003.09.006

M3 - Article

VL - 47

SP - 1017

EP - 1024

JO - New Astronomy Reviews

JF - New Astronomy Reviews

IS - 11-12

ER -

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

Abstract

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