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Stripe 82 (-50 to 59d, -1.25 to 1.25d) will be observed in four "squashed" tiles, 30d x 2.66d:  A: 300 to 330d, 330d (20-22h),  -1.33 to 1.33d B: 330 to 360/0d, 360/0d (22-24/0h),  -1.33 to 1.33d C: 0d to 30d, 30d (0-2h),  -1.33 to 1.33d D: 30 to 60d, 60d (2-4h),  -1.33 to 1.33d Because each tile is 30d long, a reasonable option is to divide each squashed tile into two or three "sub" tiles. In searching for calibrators, I found that some of the "sub-tiles" in the same tile should actually use the same calibrator. Therefore, some of the tiles can be observed as one 10x2.66d sub-tile, and one 20x2.66d sub-tile. Whether to start with the easternmost or westernmost sub-tile will depend on whether the full tile will be observed rising or setting. 
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- the NRAO calibrator list ("P" calibrator in both L and C band if possible, close to tile, bright in L and C band)  - Lorant's run to observe potential calibrators: www.aoc.nrao.edu/lsjouwer/Scal/run1/ http://www.aoc.nrao.edu/lsjouwer/Scal/run1/ (and run2)  - Lorant suggests J0016-0015, J2330+1100 (I think latter has structure)  LS: both have P in L and C for both A and B arrays