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Table 1.

Summary of the MDLF observations.

Date Quality OB name

MDLF
22/23-Nov.-2017 A WFM_J0416_NOAO_1
10/11-Jan.-2018 A WFM_J0416_NOAO_2
21/22-Feb.-2018 C WFM_J0416_NOAO_3
12/13-Mar.-2018 X WFM_J0416_AO_1
4/5-Nov.-2018 A WFM_J0416_AO_10
5/6-Nov.-2018 B WFM_J0416_AO_1
5/6-Nov.-2018 A WFM_J0416_AO_2
6/7-Nov.-2018 A WFM_J0416_AO_4
2/3-Dec.-2018 A WFM_J0416_AO_11
4/5-Dec.-2018 A WFM_J0416_AO_13
12/13-Dec.-2018 A WFM_J0416_AO_14
11/12-Jan.-2019 B WFM_J0416_AO_5
16/17-Jan.-2019 C WFM_J0416_AO_6
25/26-Jan.-2019 A WFM_J0416_AO_6
27/28-Feb.-2019 A WFM_J0416_AO_17
28-Feb./1-Mar.-2019 A WFM_J0416_AO_7
3/4-Mar.-2019 A WFM_J0416_AO_8
2/3-Aug.-2019 A WFM_J0416_AO_9
30/31-Aug.-2019 A WFM_J0416_AO_18

GTO

17-Dec.-2014 A WFM_J0416_NOAO
17-Dec.-2014 A WFM_J0416_NOAO

Notes. The log of the observed OBs is reported. The typical exposure time (on sky) of each OB is 3340s. The bottom two rows refer to the previous 2 h observation from the GTO. The column “OB name” indicates the observing mode (“WFM” = wide field mode) and the use (or not) of the adaptive optics “AO/NOAO”, meaning “on/off”.

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