CFHT WIRCam software architecture and implementation

Details CFHT WIRCam software architecture and implementation CFHT WIRCam software architecture and implementation

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spie.6274e..16v&link_type=abstract

Advanced Software and Control for Astronomy. Edited by Lewis, Hilton; Bridger, Alan. Proceedings of the SPIE, Volume 6274, pp.

Astronomy and Astrophysics

Astronomy

Scientific paper

The Canada-France-Hawaii Telescope (CFHT) is now operating a Wide Field Infrared Camera (WIRCam) with a 20.5' x 20.5' field of view. The camera uses a mosaic of four Rockwell HAWAII-2RG detectors enabling subsample readouts at a rate of 50Hz for guiding and fast parallel readout of 32 amplifiers per detector for science. This paper will discuss the software architecture and implementation used to optimize the scientific productivity of the instrument as well as our experience during the first semester of use.

Affiliated with

Also associated with

No associations

Rating

CFHT WIRCam software architecture and implementation 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 CFHT WIRCam software architecture and implementation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CFHT WIRCam software architecture and implementation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1893480