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GLIMPSE Galactic Legacy Infrared Mid-Plane Survey Extraordinaire A SIRTF Legacy Science Program |
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Time will be scheduled during early SIRTF operations to validate our observing strategy (OSV). The GLIMPSE OSV region is chosen to sample a range of stellar densities and diffuse background levels characteristic of the inner Galactic plane. The observations will probably take place in late December 2003.
With the SIRTF launch date of August 25, 2003, the GLIMPSE OSV target is RCW49:
RCW49 3-color image (2MASS J,H,K)(0.5 x 0.5 deg)
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RCW49 3-color image (2MASS J,K,MSX A)(0.5 x 0.5 deg)
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RCW49 3-color image (2MASS J,H,K)(0.8 x 0.8 deg)
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RCW49 3-color image (2MASS J,K,MSX A)(0.8 x 0.8 deg)
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3 color images:
2mass j,h,k (small jpg file)(big jpg file)
(small ps file)(big ps file)
(small tif file)(big tif file)
2mass j,k + MSX A (small jpg file)(big jpg file)
(small ps file)(big ps file)
(small tif file)(big tif file)
The OSV will consist of four 1 deg x 0.17 deg AORs nearly identical to normal GLIMPSE AORs. These will be repeated with varying frame offsets (along the strip direction) and overlaps (between strips). The GLIMPSE OSV will also perform a single 2 deg x 0.17 deg AOR to allow the evaluation of the pointing reconstruction accuracy for the full half hour it takes to do a single diagonal band across the Galactic plane.
to UW-Madison Astronomy Department home page
to
University of Wisconsin-Madison home page
this page is: http://www.astro.wisc.edu/glimpse/Team/osv/osv.html
12-11-03
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