XMM SWIRE Dec06

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This is a page about the PRIMUS project.

The XMM SWIRE observations for December 2006 targets galaxies and QSOs detected the optical/IR imaging.

These masks follow the identical target selection as outlined in the XMM SWIRE October 2006 section. The Oct06 masks were discovered to have a 10x16 pixel nod rather than the intended 10x20 pixel nod. While these were not set, the original footprint of the Oct06 slits were correctly treated. The Dec06 masks (114-123) duplicate the Oct06 XMM SWIRE masks with the correct nod distance in place. None of the target selection changed.

Please see the XMM SWIRE Oct06 section for more details.

The designs for the December 2006 run are at

http://sdss.physics.nyu.edu/primus/design/xmm_swire/masks/dec06

Overall statistics for the primary sample (207) of the December 2006 run are at

http://sdss.physics.nyu.edu/primus/design/xmm_swire/masks/dec06/xmm_swire_dec06_stats.txt