The CARMENES search for exoplanets around M dwarfs - A deep transfer learning method to determine Teff and [M/H] of target stars

Open Access

Table 7

T_eff comparison for the stars not used in the training phase.

Karmn	T_eff,interf [K]	T_eff,DL [K]	T_eff,DTL [K]	T_eff,Schw19 [K]
J09144+526	3968 ± 42	4033 ± 60	3877 ± 16	4005 ± 51
J15194−077	3501 ± 58	3391 ± 47	3259 ± 24	3441 ± 51
J16581+257	3610 ± 61	3745 ± 43	3732 ± 11	3734 ± 51
J17578+046	3252 ± 23	3352 ± 55	3212 ± 48	3273 ± 51
J22532−142	3165 ± 25	3313 ± 55	3125 ± 37	3377 ± 51

Notes. Observed (‘interf’), DL-estimated (‘DL’), DTL-predicted (‘DTL’), and Schw19 values.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.