From: 	  fmasci@ipac.caltech.edu
	Subject: 	our first flight mosaic
	Date: 	December 23, 2009 1:12:34 PM PST
	To: 	  wise.detectors@kromos.jpl.nasa.gov
	Cc: 	  wise-staff@ipac.caltech.edu,
                  docushare_detectors_earchive@alpha-lib.jpl.nasa.gov


Don't get too excited, this one's made from w1 dark frames only, mainly to test our multi-frame outlier rejection algorithms and assess the impact of output channel noise. As a worst case scenario, I include frames from several SAA passes. Dimensions are the same as a nominal Atlas Image: ~1.56 deg. on a side. Input frames were first dark subtracted using a super dark.

Products are on the WSDC's password protected web server. For those who cannot find their password, please contact Roc or Stefanie: [626 395]-1828 or -1926.

depth of coverage map [color bar gives depths]:
http://wise2.ipac.caltech.edu/staff/fmasci/drk_coverage.jpg

dark intensity co-add [grid is ecliptic]:
http://wise2.ipac.caltech.edu/staff/fmasci/drk_intensity.jpg

movie of the individual frames marching across the co-add footprint. Note the SAA passes:
http://wise2.ipac.caltech.edu/staff/fmasci/drkmovie.gif

Regards, Frank