The Mosaic II CCD Imager
on the CTIO Blanco 4m


CTIO Support Scientists:
Andrea Kunder, Alistair Walker, Chris Smith, Tim Abbott
Primary contact: Andrea Kunder, akunder@ctio.noao.edu


The CTIO Mosaic II CCD imager is a near clone of 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 2011 when it will be replaced by The Dark Energy Camera (DECam).

DOCUMENTATION FOR USERS:


CALIBRATION DATA FOR MOSAIC REDUCTIONS:

16 Channel Mode:

8 Channel Mode:

  • Previous calibrations and information on Mosaic II.

    KNOWN PROBLEM AREAS:


    CTIO Mosaic Support Pages (internal use only)

  • Last updated: 05 April 2010

    Staff Contacts:
    Alistair Walker: awalker@noao.edu
    Chris Smith: csmith@noao.edu
    Knut Olsen: kolsen@noao.edu
    Tim Abbott: tabbott@noao.edu
    Andrea Kunder: akunder@ctio.noao.edu