Table 1: Summary of observations: each mask is named with the identification number of its primary target. The number of slitlets, of IR-peakers included, and of measured spectroscopic redshifts are reported.
Mask RA Dec PA AM t(exp) N N N
  J2006.4 J2006.4 [deg]   [s] (slits) (peak) (reds$^\ast$)
LH_247597 10:52:32.694 +57:46:27.896 110 1.55 3600 21 5 6
LH_575325 10:47:43.555 +59:09:22.974 131 1.35 4500 26 5 15
EN1_205467 16:09:42.168 +54:39:49.085 155 1.25 3600 24 3 18
EN1_282078 16:16:56.673 +55:32:02.568 179 1.26 5400 24 2 18
EN2_273717 16:33:33.569 +40:54:40.722 143 1.21 5400 23 3 15
LH_128777 10:59:03.752 +57:46:56.282 105 1.56 3600 29 3 11
LH_579894 10:48:09.714 +59:09:25.529 119 1.36 4500 24 6 9
EN1_341469 16:03:38.599 +54:23:52.565 180 1.23 5400 24 4 16
EN2_10334 16:42:09.003 +40:45:51.746 104 1.22 5400 25 2 20
EN2_172324 16:34:50.206 +41:00:10.745 145 1.08 4500 15 4 11

$^\ast$ Without accounting for serendipitous sources.


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