Open Access

Table B.2

Optical and NIR photometry taken in RUN IV.

VIS NIR
Source Obs Date g r i z Obs Date J K
[YYYY-MM-DD] [mag] [mag] [mag] [mag] [YYYY-MM-DD] [mag] [mag]
CY Tau - - - - - 2020-12-15 9.66 8.39
DE Tau 2020-10-23 13.50 12.31 11.34 10.79 2020-10-25 9.07 7.70
DI Tau 2020-12-14 13.48 12.19 11.31 10.95 2020-12-15 9.26 8.29
HD30171 2020-10-23 9.52 9.06 8.86 8.85 2020-10-25 7.83 7.32
IW Tau 2020-12-14 13.13 11.92 11.12 10.74 2020-12-15 9.13 8.21
LkCa 4 2020-12-14 13.19 11.96 11.20 10.85 - - -
LkCa 15 2020-12-13 13.11 12.01 11.42 11.20 2020-12-15 9.36 8.16
LkCa 21 2020-12-14 14.08 12.82 11.68 11.06 2020-12-15 9.36 8.36
SU Aur 2020-10-23 9.57 8.99 8.64 8.44 2020-10-25 7.17 5.82
V807 Tau 2020-10-23 11.96 10.91 10.14 9.85 2020-10-25 8.22 7.03
V819 Tau 2020-12-14 13.83 12.55 11.70 11.32 2020-12-15 9.33 8.31
V826 Tau 2020-10-23 12.32 11.44 10.71 10.39 2020-10-25 9.05 8.16
V827 Tau 2020-12-14 13.14 11.95 11.15 10.77 2020-12-15 9.07 8.16
V1070 Tau 2020-12-13 12.76 11.71 10.98 10.49 2020-12-15 9.02 8.16
V1098 Tau - - - - - 2020-10-25 8.30 -
V1115 Tau 2020-12-14 12.15 11.22 10.76 10.60 2020-12-15 9.27 8.48

Notes. Typical errors in photometric magnitudes are 0.1 mag. Photometric data for the past observing RUN are reported in Gangi et al. (2020).

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