The CTIO Mosaic II CCD imager was developed together with the Mosaic I in use on the KPNO Mayall 4-m and 0.9-m telescopes and replaces the BTC camera previously used at prime focus on the V. M. Blanco 4-m telescope. Mosaic II will be retired in 2012 when it will be replaced by The Dark Energy Camera (DECam).


Detector: 8 2048x2048 SITe CCDs
FOV: 36x36 arcmin
Pixel scale: 0.27"/pixel
Filters: 5.75"x5.75". see Mosaic Filters
Wavelength range: 0.34-1.0 micron





CTIO Support Scientist
Staff Contacts:

Andrea Kunder : Primary contact
Sean Points :  
Alistair Walker :  
Chris Smith :  
Tim Abbott :  


Last updated: 9 August 2012