Very low resolution disperser of CHEOPS NIR integral field spectrograph

Details Very low resolution disperser of CHEOPS NIR integral field spectrograph Very low resolution disperser of CHEOPS NIR integral field spectrograph

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004spie.5492.1431c&link_type=abstract

Ground-based Instrumentation for Astronomy. Edited by Alan F. M. Moorwood and Iye Masanori. Proceedings of the SPIE, Volume 5492

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The Integral Field Spectrograph (IFS) of CHEOPS, the 2nd generation VLT instrument for planet finding, will attain a very low resolution (R=15) in order to search for cold (and warm) planets in stellar neighbourhood. This will allow to exploit wide band integral field spectroscopy to perform differential photometry. The complete description of CHEOPS IFS is given as a separate contribution to this conference; in this paper the analysis and the project of the very low disperser are outlined.

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