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Table 2.

All observations.

OB Night Seeing Par. angle Flag
[”] [degrees]
NGC2110_1 2013-11-24 0.58 −148.4 1
NGC2110_2 2013-11-24 0.5 161.8 0
NGC2992_1 2014-02-26 0.73 −111.1 1
NGC2992_2 2014-02-25 0.76 −111.2 0
MCG523_1 2014-01-21 1.06 −77.4 1
MCG523_2 2014-01-21 0.95 −26.3 0
NGC3081_1 2014-02-19 0.58 −100.0 0
NGC3081_2 2014-02-19 0.8 99.4 1
ESO021_1 2016-08-01 0.41 50.0 1
NGC5728_1 2015-05-12 0.81 134.7 1
NGC5728_2 2015-07-15 0.78 139.4 0
ESO137_1 2015-05-18 1.03 −5.8 0
ESO137_2 2015-05-20 1.54 −3.9 0
ESO137_3 2015-06-23 0.8 −1.8 1
NGC7172_1 2015-08-11 1.13 −68.9 1
NGC7172_2 2015-08-11 1.44 11.8 0
NGC7582_1 2016-07-26 0.38 −67.8 0
NGC7582_2 2016-08-08 0.72 −39.7 1

NGC718_1 2015-12-04 0.6 144.7 1
NGC1079_1 2013-11-22 0.8 79.1 1
NGC1315_1 2013-12-10 0.89 −171.5 1
NGC1315_2 2013-12-10 0.93 104.8 0
NGC1947_1 2013-12-22 0.67 48.6 1
NGC1947_2 2014-02-07 1.21 42.5 0
ESO208_1 2013-12-11 0.61 −5.2 1
ESO208_2 2014-01-21 1.05 −12.9 0
NGC2775_1 2015-11-14 0.69 −132.2 1
NGC2775_2 2015-12-07 0.73 −149.5 0
NGC3175_1 2014-03-08 1.49 −92.5 1
NGC3175_2 2014-03-09 0.63 −89.5 0
NGC3351_1 2014-02-20 1.08 −150.2 1
NGC3351_2 2014-02-20 1.06 −176.5 0
ESO093_1 2014-01-21 1.44 −2.2 0
ESO093_2 2014-03-20 −1.0 −36.0 1
NGC3717_1 2014-03-21 1.37 −90.8 1
NGC3717_2 2014-03-21 1.22 −78.0 0
NGC3749_1 2014-03-21 1.58 −16.9 1
NGC3749_2 2014-03-31 −1.0 −90.3 0
NGC4224_1 2015-05-12 0.79 −169.6 1
NGC4254_1 2016-06-01 0.42 −178.1 1
NGC5037_1 2015-05-12 1.18 127.7 1
NGC5037_2 2016-02-03 0.76 −115.6 0
NGC5845_1 2015-05-22 −1.0 −173.0 0
NGC5845_2 2016-03-15 0.91 −142.5 1
NGC5921_1 2015-06-15 0.82 147.8 1
NGC5921_2 2015-06-23 0.86 −177.1 0
IC4653_1 2015-05-18 0.93 3.8 0
IC4653_3 2016-06-03 0.55 −49.7 1
NGC7727_1 2015-08-24 0.7 −139.9 1

Notes. Name of ESO observing block (OB), date of night began, seeing (−1 indicates that the measurement is not available), and parallactic angle at the start of the observation. The last column indicates whether this OB was used (flag = 1) for the further analysis or not (flag = 0). Top: AGNs. Bottom: Inactive galaxies. Please see Sect. 3.5 for more on the OB selection.

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