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Table 1

Log of Nov. 2010 and May 2011 runs.

Date Mask FWHM(′′) Frame(airmass) t_exposure(t_ramp) N exposure

Nov. 1−2 ECDF-S 1 dark 1s(1s), 1s(1s), 3s(1s), 300s(5s) 10, 5, 5, 10
Nov. 1−2 ECDF-S 1 lamp 1s(1s) 10
Nov. 1−2 ECDF-S 1 flat 3s(1s) 10
Nov. 1−2 ECDF-S 1 0.8 NIR telluric standard 1s(1s) 20
Nov. 1−2 ECDF-S 1 0.8 science(1.13) 300s(5s) 58

Nov. 1−2 ECDF-S 2 dark 1s(1s), 300(5s) 10, 10
Nov. 1−2 ECDF-S 2 lamp 1s(1s) 10
Nov. 1−2 ECDF-S 2 flat 1s(1s) 10
Nov. 1−2 ECDF-S 2 0.8 NIR telluric standard 1s(1s) 25
Nov. 1−2 ECDF-S 2 0.8 science(1.15) 300s(5s) 56

May 19−20 SDSS dark 1s(1s), 3s(1s), 300s(5s) 10, 10, 10
May 19−20 SDSS lamp 1s(1s) 5
May 19−20 SDSS flat 3s(1s) 5
May 19−20 SDSS 1.0 NIR telluric standard 1s(1s) 10
May 19−20 SDSS 1.0 science(1.2) 300s(5s) 38

May 19−20 EHDF-S dark 1s(1s), 3s(1s), 300s(5s) 10, 10, 10
May 19−20 EHDF-S lamp 1s(1s) 5
May 19−20 EHDF-S flat 3s(1s) 5
May 19−20 EHDF-S 1.0 NIR telluric standard 1s(1s) 10
May 19−20 EHDF-S 1.0 science(1.3) 300s(5s) 32

Notes. The observations were carried out using the MMIRS HK grism and the H + K filter over 4 nights in three fields and four MOS masks. Column 1: observation date. Column 2: mask name. For a few sources of ECDF-S 1 and ECDF-S 2 masks we used a narrower slit of 0.5′′; a 0.7′′ wide slit was used for the majority of the sources. Column 3: FWHM estimated from the continua of standard stars. The seeing was 0.8′′(1′′) in Nov. (May) run. Column 4: type of calibration and science exposures performed for each mask (airmass is average). Column 5: individual frame exposures; the ramp time is also specified for each type of frame in parentheses (Appendix A). Column 6: number of each type of exposure. The total exposure time of the science frames was 4.8 (4.7) h for ECDF-S mask1 (mask2), 3.2 (2.7) h for SDSS (EHDF-S) mask.

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