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Herschel–SPIRE: an update on performance andplans

Published online by Cambridge University Press:  25 November 2011

M. Röllig ,
R. Simon ,
V. Ossenkopf ,
J. Stutzki ,
M.J. Griffin  and
T.L. Lim
M.J. Griffin
Affiliation:
School of Physics and Astronomy, Cardiff University, The Parade, Cardiff CF24 3AA, UK
T.L. Lim
Affiliation:
Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 0QX, UK
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Abstract

SPIRE, the Spectral and Photometric Imaging Receiver, is Herschel’ssubmillimetre camera and spectrometer. It comprises a three-band imaging photometeroperating at 250, 350 and 500 μm, and an imaging Fourier TransformSpectrometer (FTS) covering 194–671 μm. The instrument design and itsin-flight performance, calibration and data processing are outlined by Griffin etal. (2010) and Swinyard et al.(2010) in the Astronomy &Astrophysics special issue on first results from Herschel. Here weprovide a brief update on the status of SPIRE including some recent and futureenhancements to the data processing and calibration.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 52: Conditions and Impact of Star Formation , 2011 , pp. 9 - 14
Copyright
© EAS, EDP Sciences 2011

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References

Griffin, M.J., et al., 2010, A&A, 518, L3 PubMed
Moreno, R., 2010, Neptune and Uranus planetary brightness temperature tabulation, available fron ESA Herschel Science Centre
Pilbratt, G.L., et al., 2010, A&A, 518, L1
SPIRE Data Reduction Guide, 2010, Version 1.1, 29 October 2010, available from ESA Herschel Science Centre (http://herschel.esac.esa.int/hcss-doc-5.0/print/spire_dum/spire_dum.pdf)
SPIRE Observers’ Manual, 2010, Version 2.2, 29 November 2010, available from ESA Herschel Science Centre (http://herschel.esac.esa.int/Docs/SPIRE/pdf/spire_om.pdf)
SPIRE Pipeline Specification Manual, 2010, Version 1.6, 2 December 2010, available from ESA Herschel Science Centre (http://herschel.esac.esa.int/hcss-doc-5.0/print/spire_um/spire_um.pdf)
Swinyard, B.M., et al., 2010, A&A, 518, L4