Open Access

Table B.3

Results from the 2-Teff modeling for sources showing a strong presence of spots.

Source Obs Date [YYYY-MM-DD] Trotfit (±err) [K] Thot [K] Whot [%] Tcool [K] Wcool [%] Teff [K]
Accreting sources

BP Tau 2020-01-26 4176 (84) 4200 45 3100 55 3717
DK Tau 2018-12-08 4283 (155) 4300 53 3300 47 3923
DN Tau 2019-11-01 4060 (121) 4000 72 3200 28 3823
DQ Tau 2019-11-02 4044 (103) 4000 68 3200 32 3795
DS Tau 2019-11-01 4183 (87) 4200 61 3100 39 3876
GG Tau A 2018-12-09 4186 (121) 4200 76 3300 24 4034
GI Tau 2020-01-26 3957 (140) 4000 73 3100 27 3815
IP Tau 2018-12-09 4038 (119) 4000 67 3100 33 3770
UY Aur 2018-12-08 4086 (138) 4100 58 3100 42 3773
V836 Tau 2019-11-02 4444 (86) 4400 11 3100 89 3333
2020-01-26 4398 (105) 4400 10 3100 90 3313

Non-accreting sources

DI Tau 2020-12-13 3965 (75) 4000 54 3200 46 3695
IW Tau 2020-12-13 4125 (92) 4100 44 3200 56 3678
LkCa 4 2020-12-13 4085 (152) 4100 20 3100 80 3379
V819 Tau 2020-12-14 4486 (62) 4500 73 3500 27 4293
V827 Tau 2020-12-13 4180 (106) 4200 35 3200 65 3648
V1070 Tau 2020-12-13 4208 (77) 4200 61 3200 39 3897

Notes. TROTFIT is the temperature as derived by ROTFIT on the basis of the high-resolution optical HARPS-N spectra. In the modeling, Thot is fixed to the closest value found by ROTFIT while Tcool and the weighting factors are leaved as free parameters; their best-fit values are reported in the table. Final effective temperatures, as computed as from Eq. 1, are reported in the last column.

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