Herschel-SPIRE: an update on performance and plans

Details Herschel-SPIRE: an update on performance and plans Herschel-SPIRE: an update on performance and plans

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011eas....52....9g&link_type=abstract

EAS Publications Series, Volume 52, 2011, pp.9-14

Astronomy and Astrophysics

Astrophysics

Scientific paper

SPIRE, the Spectral and Photometric Imaging Receiver, is Herschel's submillimetre camera and spectrometer. It comprises a three-band imaging photometer operating at 250, 350 and 500 μm, and an imaging Fourier Transform Spectrometer (FTS) covering 194-671 μm. The instrument design and its in-flight performance, calibration and data processing are outlined by Griffin et al. (2010) and Swinyard et al. (2010) in the Astronomy & Astrophysics special issue on first results from Herschel. Here we provide a brief update on the status of SPIRE including some recent and future enhancements to the data processing and calibration.

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