Planck-HFI optical design and pre-flight performances

B. Maffei; F. Noviello; G. Savini; J. A. Murphy; J. M. Lamarre; P. A.R. Ade; F. R. Bouchet; J. Brossard; A. Catalano; R. Colgan; R. Gispert; E. Gleeson; C. V. Haynes; W. C. Jones; A. E. Lange; Y. Longval; I. McAuley; H. U. Nørgaard-Nielsen; F. Pajot; T. Peacocke; G. Pisano; J. L. Puget; I. Ristorcelli; R. Sudiwala; J. Tauber; R. J. Wylde; V. Yurchenko

Planck-HFI optical design and pre-flight performances

B. Maffei, F. Noviello, G. Savini, J. A. Murphy, J. M. Lamarre, P. A.R. Ade, F. R. Bouchet, J. Brossard, A. Catalano, R. Colgan, R. Gispert, E. Gleeson, C. V. Haynes, W. C. Jones, A. E. Lange, Y. Longval, I. McAuley, H. U. Nørgaard-Nielsen, F. Pajot, T. PeacockeG. Pisano, J. L. Puget, I. Ristorcelli, R. Sudiwala, J. Tauber, R. J. Wylde, V. Yurchenko

Physics

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

2 Scopus citations

Abstract

Planck is a European Space Agency (ESA) satellite, launched in May 2009, which is mapping the Cosmic Microwave Background anisotropies in intensity and polarisation with un-precedented detail and sensitivity. It will also provide full-sky maps of astrophysical foregrounds. An accurate knowledge of the telescope beam patterns is an essential element for a correct analysis of the acquired astrophysical data. We present the optical design of the High Frequency Instrument (HFI) together with the optical performances measured during the ground calibration campaigns. We report on the evolution of the knowledge of the pre-launch HFI beam patterns when coupled to the telescope, and on their significance for the HFI data analysis procedure.

Original language	English (US)
Title of host publication	EuCAP 2010 - The 4th European Conference on Antennas and Propagation
Publisher	IEEE Computer Society
ISBN (Print)	9788476534724
State	Published - 2010
Event	4th European Conference on Antennas and Propagation, EuCAP 2010 - Barcelona, Spain Duration: Apr 12 2010 → Apr 16 2010

Publication series

Name	EuCAP 2010 - The 4th European Conference on Antennas and Propagation

Other

Other	4th European Conference on Antennas and Propagation, EuCAP 2010
Country/Territory	Spain
City	Barcelona
Period	4/12/10 → 4/16/10

All Science Journal Classification (ASJC) codes

Computer Networks and Communications
Electrical and Electronic Engineering

Cite this

Maffei, B., Noviello, F., Savini, G., Murphy, J. A., Lamarre, J. M., Ade, P. A. R., Bouchet, F. R., Brossard, J., Catalano, A., Colgan, R., Gispert, R., Gleeson, E., Haynes, C. V., Jones, W. C., Lange, A. E., Longval, Y., McAuley, I., Nørgaard-Nielsen, H. U., Pajot, F., ... Yurchenko, V. (2010). Planck-HFI optical design and pre-flight performances. In EuCAP 2010 - The 4th European Conference on Antennas and Propagation Article 5505697 (EuCAP 2010 - The 4th European Conference on Antennas and Propagation). IEEE Computer Society.

@inproceedings{4ae556ccdcb84a1f8668de39fc2ccbe1,

title = "Planck-HFI optical design and pre-flight performances",

abstract = "Planck is a European Space Agency (ESA) satellite, launched in May 2009, which is mapping the Cosmic Microwave Background anisotropies in intensity and polarisation with un-precedented detail and sensitivity. It will also provide full-sky maps of astrophysical foregrounds. An accurate knowledge of the telescope beam patterns is an essential element for a correct analysis of the acquired astrophysical data. We present the optical design of the High Frequency Instrument (HFI) together with the optical performances measured during the ground calibration campaigns. We report on the evolution of the knowledge of the pre-launch HFI beam patterns when coupled to the telescope, and on their significance for the HFI data analysis procedure.",

author = "B. Maffei and F. Noviello and G. Savini and Murphy, {J. A.} and Lamarre, {J. M.} and Ade, {P. A.R.} and Bouchet, {F. R.} and J. Brossard and A. Catalano and R. Colgan and R. Gispert and E. Gleeson and Haynes, {C. V.} and Jones, {W. C.} and Lange, {A. E.} and Y. Longval and I. McAuley and N{\o}rgaard-Nielsen, {H. U.} and F. Pajot and T. Peacocke and G. Pisano and Puget, {J. L.} and I. Ristorcelli and R. Sudiwala and J. Tauber and Wylde, {R. J.} and V. Yurchenko",

year = "2010",

language = "English (US)",

isbn = "9788476534724",

series = "EuCAP 2010 - The 4th European Conference on Antennas and Propagation",

publisher = "IEEE Computer Society",

booktitle = "EuCAP 2010 - The 4th European Conference on Antennas and Propagation",

address = "United States",

note = "4th European Conference on Antennas and Propagation, EuCAP 2010 ; Conference date: 12-04-2010 Through 16-04-2010",

}

Maffei, B, Noviello, F, Savini, G, Murphy, JA, Lamarre, JM, Ade, PAR, Bouchet, FR, Brossard, J, Catalano, A, Colgan, R, Gispert, R, Gleeson, E, Haynes, CV, Jones, WC, Lange, AE, Longval, Y, McAuley, I, Nørgaard-Nielsen, HU, Pajot, F, Peacocke, T, Pisano, G, Puget, JL, Ristorcelli, I, Sudiwala, R, Tauber, J, Wylde, RJ & Yurchenko, V 2010, Planck-HFI optical design and pre-flight performances. in EuCAP 2010 - The 4th European Conference on Antennas and Propagation., 5505697, EuCAP 2010 - The 4th European Conference on Antennas and Propagation, IEEE Computer Society, 4th European Conference on Antennas and Propagation, EuCAP 2010, Barcelona, Spain, 4/12/10.

TY - GEN

T1 - Planck-HFI optical design and pre-flight performances

AU - Maffei, B.

AU - Noviello, F.

AU - Savini, G.

AU - Murphy, J. A.

AU - Lamarre, J. M.

AU - Ade, P. A.R.

AU - Bouchet, F. R.

AU - Brossard, J.

AU - Catalano, A.

AU - Colgan, R.

AU - Gispert, R.

AU - Gleeson, E.

AU - Haynes, C. V.

AU - Jones, W. C.

AU - Lange, A. E.

AU - Longval, Y.

AU - McAuley, I.

AU - Nørgaard-Nielsen, H. U.

AU - Pajot, F.

AU - Peacocke, T.

AU - Pisano, G.

AU - Puget, J. L.

AU - Ristorcelli, I.

AU - Sudiwala, R.

AU - Tauber, J.

AU - Wylde, R. J.

AU - Yurchenko, V.

PY - 2010

Y1 - 2010

N2 - Planck is a European Space Agency (ESA) satellite, launched in May 2009, which is mapping the Cosmic Microwave Background anisotropies in intensity and polarisation with un-precedented detail and sensitivity. It will also provide full-sky maps of astrophysical foregrounds. An accurate knowledge of the telescope beam patterns is an essential element for a correct analysis of the acquired astrophysical data. We present the optical design of the High Frequency Instrument (HFI) together with the optical performances measured during the ground calibration campaigns. We report on the evolution of the knowledge of the pre-launch HFI beam patterns when coupled to the telescope, and on their significance for the HFI data analysis procedure.

AB - Planck is a European Space Agency (ESA) satellite, launched in May 2009, which is mapping the Cosmic Microwave Background anisotropies in intensity and polarisation with un-precedented detail and sensitivity. It will also provide full-sky maps of astrophysical foregrounds. An accurate knowledge of the telescope beam patterns is an essential element for a correct analysis of the acquired astrophysical data. We present the optical design of the High Frequency Instrument (HFI) together with the optical performances measured during the ground calibration campaigns. We report on the evolution of the knowledge of the pre-launch HFI beam patterns when coupled to the telescope, and on their significance for the HFI data analysis procedure.

UR - http://www.scopus.com/inward/record.url?scp=77955313604&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=77955313604&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:77955313604

SN - 9788476534724

T3 - EuCAP 2010 - The 4th European Conference on Antennas and Propagation

BT - EuCAP 2010 - The 4th European Conference on Antennas and Propagation

PB - IEEE Computer Society

T2 - 4th European Conference on Antennas and Propagation, EuCAP 2010

Y2 - 12 April 2010 through 16 April 2010

ER -

Planck-HFI optical design and pre-flight performances

Abstract

Publication series

Other

All Science Journal Classification (ASJC) codes

Other files and links

Fingerprint

Cite this