Log of Nov. 2010 and May 2011 runs.
|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||1.0||NIR telluric standard||1s(1s)||10|
|May 19−20||EHDF-S||dark||1s(1s), 3s(1s), 300s(5s)||10, 10, 10|
|May 19−20||EHDF-S||1.0||NIR telluric standard||1s(1s)||10|
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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