The Planck High Frequency Instrument, a third generation CMB probe and the first submillimeter surveyor

J. M. Lamarre; J. L. Puget; M. Piat; P. A R Ade; A. Lange; A. Benoit; P. De Bernardis; F. R. Bouchet; J. Bock; F. X D Sert; R. Emery; M. Giard; B. Maffei; A. Murphy; J. P. Torre; R. Bhatia; R. Sudiwala; V. Yourchenko

doi:10.1117/12.461636

The Planck High Frequency Instrument, a third generation CMB probe and the first submillimeter surveyor

J. M. Lamarre, J. L. Puget, M. Piat, P. A R Ade, A. Lange, A. Benoit, P. De Bernardis, F. R. Bouchet, J. Bock, F. X D Sert, R. Emery, M. Giard, B. Maffei, A. Murphy, J. P. Torre, R. Bhatia, R. Sudiwala, V. Yourchenko

Research output: Chapter in Book/Conference proceeding › Conference contribution

Abstract

The High Frequency Instrument of the Planck satellite is dedicated to the measurement of the anisotropy of the Cosmic Microwave Background (CMB). Its main goal is to map the CMB with a sensitivity of ΔT/T=2.10-6 and an angular resolution of 5 arcmin in order to constrain cosmological parameters. Planck is a project of the European Space Agency based on a wide international collaboration, including United States and Canadian laboratories. The architecture of the satellite is driven by the thermal requirements resulting from the search for low photon noise. Especially, the passively cooled telescope should be at less than 50K, while a cascade of cryo-coolers will ensure the cooling of the HFI bolometers down to 0.1K. This last temperature will be produced by a gravity insensitive 3He/4He dilution cooler. This will be achieved at the L2 Lagrangian point of the Sun-Earth system. The whole sky will be observed two times in the 14 months mission with a scanning strategy based on a 1RPM rotation of the satellite. In addition to the cosmological parameters that can be derived from the CMB maps, Planck will deliver nine high sensitivity submillimeter maps of the whole sky that will constitute unique data available to the whole astronomical community.

Original language	English
Title of host publication	Proceedings of SPIE - The International Society for Optical Engineering\|Proc SPIE Int Soc Opt Eng
Editors	J.C. Mather
Pages	730-739
Number of pages	9
Volume	4850
DOIs	https://doi.org/10.1117/12.461636
Publication status	Published - 2002
Event	IR Space Telescopes and Instruments - waikoloa, HI Duration: 1 Jul 2002 → … http://<Go to ISI>://WOS:000182018700070

Publication series

Name	Proceedings of the Society of Photo-Optical Instrumentation Engineers (Spie)

Conference

Conference	IR Space Telescopes and Instruments
City	waikoloa, HI
Period	1/07/02 → …
Internet address	http://<Go to ISI>://WOS:000182018700070

Keywords

Cosmic Microwave Background
Cosmology
Submillimeter astronomy

Access to Document

10.1117/12.461636

Cite this

Lamarre, J. M., Puget, J. L., Piat, M., Ade, P. A. R., Lange, A., Benoit, A., De Bernardis, P., Bouchet, F. R., Bock, J., Sert, F. X. D., Emery, R., Giard, M., Maffei, B., Murphy, A., Torre, J. P., Bhatia, R., Sudiwala, R., & Yourchenko, V. (2002). The Planck High Frequency Instrument, a third generation CMB probe and the first submillimeter surveyor. In J. C. Mather (Ed.), Proceedings of SPIE - The International Society for Optical Engineering|Proc SPIE Int Soc Opt Eng (Vol. 4850, pp. 730-739). (Proceedings of the Society of Photo-Optical Instrumentation Engineers (Spie)). https://doi.org/10.1117/12.461636

Lamarre, J. M. ; Puget, J. L. ; Piat, M. et al. / The Planck High Frequency Instrument, a third generation CMB probe and the first submillimeter surveyor. Proceedings of SPIE - The International Society for Optical Engineering|Proc SPIE Int Soc Opt Eng. editor / J.C. Mather. Vol. 4850 2002. pp. 730-739 (Proceedings of the Society of Photo-Optical Instrumentation Engineers (Spie)).

@inproceedings{6521e99443964622944e6e858bd5d9aa,

title = "The Planck High Frequency Instrument, a third generation CMB probe and the first submillimeter surveyor",

abstract = "The High Frequency Instrument of the Planck satellite is dedicated to the measurement of the anisotropy of the Cosmic Microwave Background (CMB). Its main goal is to map the CMB with a sensitivity of ΔT/T=2.10-6 and an angular resolution of 5 arcmin in order to constrain cosmological parameters. Planck is a project of the European Space Agency based on a wide international collaboration, including United States and Canadian laboratories. The architecture of the satellite is driven by the thermal requirements resulting from the search for low photon noise. Especially, the passively cooled telescope should be at less than 50K, while a cascade of cryo-coolers will ensure the cooling of the HFI bolometers down to 0.1K. This last temperature will be produced by a gravity insensitive 3He/4He dilution cooler. This will be achieved at the L2 Lagrangian point of the Sun-Earth system. The whole sky will be observed two times in the 14 months mission with a scanning strategy based on a 1RPM rotation of the satellite. In addition to the cosmological parameters that can be derived from the CMB maps, Planck will deliver nine high sensitivity submillimeter maps of the whole sky that will constitute unique data available to the whole astronomical community.",

keywords = "Cosmic Microwave Background, Cosmology, Submillimeter astronomy",

author = "Lamarre, {J. M.} and Puget, {J. L.} and M. Piat and Ade, {P. A R} and A. Lange and A. Benoit and {De Bernardis}, P. and Bouchet, {F. R.} and J. Bock and Sert, {F. X D} and R. Emery and M. Giard and B. Maffei and A. Murphy and Torre, {J. P.} and R. Bhatia and R. Sudiwala and V. Yourchenko",

note = "Times Cited: 17 Conference on IR Space Telescopes and Instruments AUG 24-28, 2002 WAIKOLOA, HI SPIE; IR Space Telescopes and Instruments ; Conference date: 01-07-2002",

year = "2002",

doi = "10.1117/12.461636",

language = "English",

volume = "4850",

series = "Proceedings of the Society of Photo-Optical Instrumentation Engineers (Spie)",

pages = "730--739",

editor = "J.C. Mather",

booktitle = "Proceedings of SPIE - The International Society for Optical Engineering|Proc SPIE Int Soc Opt Eng",

url = "http://<Go to ISI>://WOS:000182018700070",

}

Lamarre, JM, Puget, JL, Piat, M, Ade, PAR, Lange, A, Benoit, A, De Bernardis, P, Bouchet, FR, Bock, J, Sert, FXD, Emery, R, Giard, M, Maffei, B, Murphy, A, Torre, JP, Bhatia, R, Sudiwala, R & Yourchenko, V 2002, The Planck High Frequency Instrument, a third generation CMB probe and the first submillimeter surveyor. in JC Mather (ed.), Proceedings of SPIE - The International Society for Optical Engineering|Proc SPIE Int Soc Opt Eng. vol. 4850, Proceedings of the Society of Photo-Optical Instrumentation Engineers (Spie), pp. 730-739, IR Space Telescopes and Instruments, waikoloa, HI, 1/07/02. https://doi.org/10.1117/12.461636

The Planck High Frequency Instrument, a third generation CMB probe and the first submillimeter surveyor. / Lamarre, J. M.; Puget, J. L.; Piat, M. et al.
Proceedings of SPIE - The International Society for Optical Engineering|Proc SPIE Int Soc Opt Eng. ed. / J.C. Mather. Vol. 4850 2002. p. 730-739 (Proceedings of the Society of Photo-Optical Instrumentation Engineers (Spie)).

Research output: Chapter in Book/Conference proceeding › Conference contribution

TY - GEN

T1 - The Planck High Frequency Instrument, a third generation CMB probe and the first submillimeter surveyor

AU - Lamarre, J. M.

AU - Puget, J. L.

AU - Piat, M.

AU - Ade, P. A R

AU - Lange, A.

AU - Benoit, A.

AU - De Bernardis, P.

AU - Bouchet, F. R.

AU - Bock, J.

AU - Sert, F. X D

AU - Emery, R.

AU - Giard, M.

AU - Maffei, B.

AU - Murphy, A.

AU - Torre, J. P.

AU - Bhatia, R.

AU - Sudiwala, R.

AU - Yourchenko, V.

N1 - Times Cited: 17 Conference on IR Space Telescopes and Instruments AUG 24-28, 2002 WAIKOLOA, HI SPIE

PY - 2002

Y1 - 2002

N2 - The High Frequency Instrument of the Planck satellite is dedicated to the measurement of the anisotropy of the Cosmic Microwave Background (CMB). Its main goal is to map the CMB with a sensitivity of ΔT/T=2.10-6 and an angular resolution of 5 arcmin in order to constrain cosmological parameters. Planck is a project of the European Space Agency based on a wide international collaboration, including United States and Canadian laboratories. The architecture of the satellite is driven by the thermal requirements resulting from the search for low photon noise. Especially, the passively cooled telescope should be at less than 50K, while a cascade of cryo-coolers will ensure the cooling of the HFI bolometers down to 0.1K. This last temperature will be produced by a gravity insensitive 3He/4He dilution cooler. This will be achieved at the L2 Lagrangian point of the Sun-Earth system. The whole sky will be observed two times in the 14 months mission with a scanning strategy based on a 1RPM rotation of the satellite. In addition to the cosmological parameters that can be derived from the CMB maps, Planck will deliver nine high sensitivity submillimeter maps of the whole sky that will constitute unique data available to the whole astronomical community.

AB - The High Frequency Instrument of the Planck satellite is dedicated to the measurement of the anisotropy of the Cosmic Microwave Background (CMB). Its main goal is to map the CMB with a sensitivity of ΔT/T=2.10-6 and an angular resolution of 5 arcmin in order to constrain cosmological parameters. Planck is a project of the European Space Agency based on a wide international collaboration, including United States and Canadian laboratories. The architecture of the satellite is driven by the thermal requirements resulting from the search for low photon noise. Especially, the passively cooled telescope should be at less than 50K, while a cascade of cryo-coolers will ensure the cooling of the HFI bolometers down to 0.1K. This last temperature will be produced by a gravity insensitive 3He/4He dilution cooler. This will be achieved at the L2 Lagrangian point of the Sun-Earth system. The whole sky will be observed two times in the 14 months mission with a scanning strategy based on a 1RPM rotation of the satellite. In addition to the cosmological parameters that can be derived from the CMB maps, Planck will deliver nine high sensitivity submillimeter maps of the whole sky that will constitute unique data available to the whole astronomical community.

KW - Cosmic Microwave Background

KW - Cosmology

KW - Submillimeter astronomy

U2 - 10.1117/12.461636

DO - 10.1117/12.461636

M3 - Conference contribution

VL - 4850

T3 - Proceedings of the Society of Photo-Optical Instrumentation Engineers (Spie)

SP - 730

EP - 739

BT - Proceedings of SPIE - The International Society for Optical Engineering|Proc SPIE Int Soc Opt Eng

A2 - Mather, J.C.

T2 - IR Space Telescopes and Instruments

Y2 - 1 July 2002

ER -

Lamarre JM, Puget JL, Piat M, Ade PAR, Lange A, Benoit A et al. The Planck High Frequency Instrument, a third generation CMB probe and the first submillimeter surveyor. In Mather JC, editor, Proceedings of SPIE - The International Society for Optical Engineering|Proc SPIE Int Soc Opt Eng. Vol. 4850. 2002. p. 730-739. (Proceedings of the Society of Photo-Optical Instrumentation Engineers (Spie)). doi: 10.1117/12.461636

The Planck High Frequency Instrument, a third generation CMB probe and the first submillimeter surveyor

Abstract

Publication series

Conference

Keywords

Access to Document

Fingerprint

Cite this