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Cluster NamezClusterParallel FieldHST
FOV		Regions
File
RADecRADec
Year 1:
Abell 27440.30800:14:21.2-30:23:50.100:13:53.6-30:22:54.3

regions
MACSJ0416.1-24030.39604:16:08.9-24:04:28.704:16:33.1-24:06:48.7
MACSJ0416-2403Image Removed

Image Added

regions
Year 2:
MACSJ0717.5+37450.54507:17:34.0+37:44:49.007:17:17.0+37:49:47.3

Image Modified

regions
MACSJ1149.5+22230.54311:49:36.3+22:23:58.111:49:40.5+22:18:02.3
Image Removed

Image Added

regions
Year 3:
Abell S1063 (RXCJ2248.7-4431)0.34822:48:44.4-44:31:48.522:49:17.7-44:32:43.8
RXCJ2248-4431Image Removed

Image Added

regions
Abell 3700.37502:39:52.9-01:34:36.502:40:13.4-01:37:32.8
Abell 370Image Removed

Image Added

regions

These were selected primarily on their predicted lensing strength*, their low/moderate zodiacal and Galactic backgrounds, their observability with ALMA and Mauna Kea, and their observability with HST and Spitzer. We've also looked at their suitability for deep radio observations, and their existing multi-wavelength data observations.

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