Calibration and data reduction for planet detection with SPHERE-IFS

Details Calibration and data reduction for planet detection with SPHERE-IFS Calibration and data reduction for planet detection with SPHERE-IFS

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008spie.7014e.119d&link_type=abstract

Ground-based and Airborne Instrumentation for Astronomy II. Edited by McLean, Ian S.; Casali, Mark M. Proceedings of the SPI

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The 2nd generation VLT instrument SPHERE will include an integral field spectrograph to enhance the capabilities of detection of planetary companions close to bright stars. SPHERE-IFS is foreseen to work in near IR (0.95-1.65 micron) at low spectral resolution. This paper describes the observing strategies, the adopted hardware solutions for calibrating the instrument, and the data reduction procedures that are mandatory for the achievement of the extreme contrast performances for which the instrument is designed.

Affiliated with

Also associated with

No associations

Rating

Calibration and data reduction for planet detection with SPHERE-IFS does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Calibration and data reduction for planet detection with SPHERE-IFS, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Calibration and data reduction for planet detection with SPHERE-IFS will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1059401