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Table 2

Observation sequences used as science targets in this study.

Target name Observation night YYYY-MM-DD Condition Disc ?
2MASS J1604(a) 2015-06-09(b) Bad seeing Y (1)
BD-19 4288 2015-04-28 LWE N
HD 9054 2016-11-16 Bad seeing N
HD 13724 2018-08-18 Good seeing N
HD 16978 2016-09-15 Good seeing N
HD 37306 2015-10-28 Average N
HD 37484 2017-12-01 Bad seeing N
HD 59967 2018-03-27 Average N
HD 69830 2018-12-18 Average N
HD 100453 2016-01-19 Bad seeing Y (2)
HD 107301 2016-01-18 Bad seeing N
HD 111520 2016-05-14 WDH Y (3)
HD 113902 2016-06-05 WDH N
HD 121156 2017-02-05 Good seeing N
HD 123247 2015-04-05 LWE N
HD 126062 2016-04-08 Average N
2016-07-23 WDH N
HD 126135 2018-03-16 Good seeing N
HD 128987 2016-05-31 WDH N
HD 141569 2015-05-15 Average Y (4)
HD 147808 2016-04-14 LWE N
HD 165185 2019-09-06 WDH N
HD 181327 2015-05-09 Bad seeing Y (5)
HD 188228 2015-06-30 LWE N
HD 213398 2016-06-13 Bad seeing N
HR 4796 2015-02-02 Average Y (6)
TW HYA 2015-02-03 Average Y (7)

Notes. The observing condition and presence of a resolved disc are noted for each science cube. References are given for the first scattered light observations of the disc targets. Note that the observing conditions of the disc targets are listed here for completion, but are not taken into account in the analysis. (a)2MASS J16042165-2130284. (b)Observation taken with DB_K12 filter. References: (1) Mayama et al. (2012); (2) Wagner et al. (2015); (3) Padgett & Stapelfeldt (2016); (4) Augereau et al. (1999); Weinberger et al. (1999); (5) Schneider et al. (2006); (6) Schneider et al. (1999); (7) Krist et al. (2000).

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