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Table 2.

Observing log.

Galaxy Observing start S/N
Total exposure times on target (s)
Sec z Seeing Sky
ID UT date 450 650 2200 UV (Nexp × VIS (Nexp × NIR (Nexp × FWHM mode
(yyyy-mm-ddThh:mm) (nm) (nm) (nm) Integration) Integration) NDIT × DIT) (arcsec)
NGC 0584 2010-10-16T01:06 80 100 120 460 (2 × 230) 276 (2 × 138) 600 (2 × 1 × 300) 1.66–1.50 0.6 Offset
NGC 0636 2010-11-16T00:36 80 100 120 690 (3 × 230) 414 (3 × 138) 900 (3 × 1 × 300) 1.21–1.13 1.3 Offset
NGC 0897 2010-10-02T03:28 60 120 75 1060 (2 × 530) 876 (2 × 438) 1200 (2 × 2 × 300) 1.27–1.15 1.9 Offset
NGC 1357 2010-11-16T01:25 70 100 90 1280 (2 × 640) 1100 (2 × 550) 1440 (2 × 3 × 240) 1.44–1.22 1.7 Stare
NGC 1425 a 2010-10-06T06:27 100 120 85 2120 (4 × 530) 876 (2 × 438) 1200 (2 × 2 × 300) 1.03–1.01 1.8 Offset
NGC 1425 b 2010-11-17T02:07 80 110 100 1060 (2 × 530) 876 (2 × 438) 1200 (2 × 2 × 300) 1.21–1.11 0.9 Offset
NGC 1600 2010-11-25T07:37 40 80 50 1060 (2 × 530) 876 (2 × 438) 1200 (2 × 2 × 300) 1.11–1.19 1.7 Offset
NGC 1700 2010-11-21T03:49 70 100 160 690 (3 × 230) 414 (3 × 138) 900 (3 × 1 × 300) 1.19–1.12 2.5 Offset
NGC 2613 2010-11-25T07:16 40 90 108 1280 (2 × 640) 1100 (2 × 550) 1440 (2 × 3 × 240) 1.09–1.02 2.3 Offset
NGC 3115 2011-02-15T01:41 140 190 145 690 (3 × 230) 414 (3 × 138) 900 (3 × 1 × 300) 1.63–1.45 1.1 Stare
NGC 3377 2011-03-01T05:41 160 200 160 1060 (2 × 530) 876 (2 × 438) 1200 (2 × 2 × 300) 1.31–1.39 2.1 Offset
NGC 3379 2011-03-06T04:19 100 110 153 460 (2 × 230) 278 (2 × 138) 600 (2 × 1 × 300) 1.26–1.25 3.0 Offset
NGC 3423 2011-03-22T06:25 10 20 10 1280 (2 × 640) 1100 (2 × 550) 1440 (2 × 3 × 240) 1.59–2.08 0.8 Offset
NGC 4415 a 2011-02-18T05:00 10 20 10 1060 (2 × 530) 876 (2 × 438) 1200 (2 × 2 × 300) 1.45–1.31 1.0 Offset
NGC 4415 b 2011-02-18T05:43 10 20 12 1060 (2 × 530) 876 (2 × 438) 1200 (2 × 2 × 300) 1.31–1.23 1.1 Offset
NGC 7424 a 2010-11-15T00:57 30 45 6 640 (1 × 640) 550 (1 × 550) 1440 (2 × 3 × 240) 1.06–1.12 0.6 Stare
NGC 7424 b 2010-11-15T02:08 30 45 7 2560 (4 × 640) 1100 (4 × 550) 1440 (2 × 3 × 240) 1.16–1.30 0.9 Stare

Notes. All data were obtained under thin cloud conditions. Multiple entries for some galaxies indicate that they were observed more than once. Here Nexp is the number of exposures when the target was on the slit, regardless of the exact observing strategy, e.g. staring or generic offset.

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