Issue |
A&A
Volume 537, January 2012
|
|
---|---|---|
Article Number | A17 | |
Number of page(s) | 13 | |
Section | Astronomical instrumentation | |
DOI | https://doi.org/10.1051/0004-6361/201015120 | |
Published online | 20 December 2011 |
In-orbit performance of Herschel-HIFI⋆
1 SRON Netherlands Institute for Space Research, Landleven 12, 9747 AD Groningen, The Netherlands
e-mail: p.r.roelfsema@sron.nl
2 European Space Astronomy Centre, ESA, PO Box 78, 28691 Villanueva de la Cañada, Madrid, Spain
3 KOSMA, I. Physik. Institut, Universität zu Köln, Zülpicher Str. 77, 50937 Köln, Germany
4 NHSC, California Institute of Technology, Pasadena, California, USA
5 Chalmers University of Technology, 412 96 Göteborg, Sweden
6 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
7 Université de Toulouse, UPS-OMP, IRAP, Toulouse, France
8 CNRS, IRAP, 9 Av. colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France
9 Max-Planck Institute für Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany
10 Laboratoire d’Études du Rayonnement et de la Matière en Astrophysique, UMR 8112 CNRS/INSU, OP, ENS, UPMC, UCP, Paris, France
11 Osservatorio Astrofisico di Arcetri-INAF- Largo E. Fermi 5, 50100 Florence, Italy
12 Institute Fisica Spazio Interplanetario INAF, via Fosso del Cavaliere 100, 00133 Roma, Italy
13 Department of Astronomy, Stockholm University, 106 91 Stockholm, Sweden
14 Astronomical Institute, ETH, Zürich, 8093 Zürich, Switzerland
15 Centro de Astrobiología (INTA-CSIC), Ctra de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz, Madrid, Spain
16 Department of Physics & Astronomy, University of Waterloo, Waterloo, ON N2L 3G1, Canada
17 Joint Alma Observatory, Santiago, Chile
18 Leiden Observatory, Leiden University, PO Box 9513, 2300 RA, Leiden, The Netherlands
19 Physics Department, California Institute of Technology, Pasadena, California, USA
20 Space Research Centre of the Polish Academy of Sciences, Bartycka 18A, 00-716 Warsaw, Poland
21 Dept. of Experimental Physics, National University of Ireland, Maynooth, Co. Kildare, Ireland
22 Université de Bordeaux, Observatoire Aquitain des Sciences de l’Univers, 2 rue de l’Observatoire, BP 89, 33 271 Floirac Cedex, France
23 CNRS, UMR 5804, Laboratoire d’Astrophysique de Bordeaux, 2 rue de l’Observatoire, BP 89, 33 271 Floirac Cedex, France
24 National Observatory of Athens, Greece
25 Jet Propulsion Laboratories, Pasadena, California, USA
26 LERMA-LRA, UMR 8112 du CNRS, Observatoire de Paris, École Normale Supérieure, UPMC & UCP, rue Lhomond, 75231 Paris Cedex 05, France
27 Kapteyn Astronomical Institute, Landleven 12, 9747 AD Groningen, The Netherlands
28 Department of Physics and Astronomy, Institute for Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
29 Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI, 48109, USA
30 UJF-Grenoble, CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) UMR 5274, 38041 Grenoble, France
31 Astronomical Institute “Anton Pannekoek”, University of Amsterdam, Science Park XH, Amsterdam, The Netherlands
32 Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul Rabiańska 8, 87-100 Torún, Poland
Received: 31 May 2010
Accepted: 7 September 2011
Aims. In this paper the calibration and in-orbit performance of the Heterodyne Instrument for the Far-Infrared (HIFI) is described.
Methods. The calibration of HIFI is based on a combination of ground and in-flight tests. Dedicated ground tests to determine those instrument parameters that can only be measured accurately using controlled laboratory stimuli were carried out in the instrument level test (ILT) campaign. Special in-flight tests during the commissioning phase (CoP) and performance verification (PV) allowed the determination of the remaining instrument parameters. The various instrument observing modes, as specified in astronomical observation templates (AOTs), were validated in parallel during PV by observing selected celestial sources.
Results. The initial calibration and in-orbit performance of HIFI has been established. A first estimate of the calibration budget is given. The overall in-flight instrument performance agrees with the original specification. Issues remain at only a few frequencies.
Key words: methods: observational / space vehicles: instruments / instrumentation: spectrographs
© ESO, 2012
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.