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Table 1

Spectral types, photometry, and luminosities for the stars studied.

Star Instrument Observation date SN Spectral type J K Mbol
AM Cen GEMINI-S/Phoenix 2016-May-18 110 SC 3.22 1.75 −5.29
BB Tau TNG/Giano-b 2017-Nov-21 157 SC7 4.97 3.07 −5.03
IY Hya GEMINI-S/Phoenix 2017-Oct-24 157 C 5.91 1.96 −6.90
TNG/Giano-b 2018-Jul-9 112
CAHA/Carmenes(a) 2018-Mar-30 108
R Cmi TNG/Giano-b 2017-Nov-21 173 SC4 3.69 2.42 −5.54
R Gem TNG/Giano-b 2017-Nov-21 310 SC/S3 2.53 1.46 −4.65
RX Sct GEMINI-S/Phoenix 2017-Nov-3 185 C5 3.44 1.65 −4.89
S Cam TNG/Giano-b 2017-Nov-9 96 C 4.18 2.53 −5.12
Sgr 9 GEMINI-S/Phoenix 2017-Oct-31 56 C 12.09 9.42 −4.81
SZ Sgr GEMINI-S/Phoenix 2017-Nov-3 200 C5 3.73 2.15 −5.72
V372 Mon TNG/Giano-b 2018-Mar-26 105 SC7 4.78 3.00 −4.50
ZZ Gem TNG/Giano-b 2018-Apr-16 156 C 4.80 2.98 −4.49
HD 121477 TNG/Giano-b 2018-Apr-16 245 CH/Ba4 5.12 4.15 −2.36
HD 123396 GEMINI-S/Phoenix 2009-Jun-24 200 CH/Ba 6.88 6.14 −0.70

Notes. Spectral types and IR photometry are taken from the SIMBAD database. (a) The spectrum of IY Hya obtained with Carmenes was only to derive its s-element abundances. However, because of the difficulty in the analysis of its IR spectrum at ~2.3 μm, we discarded this star in the final chemical analysis (see text).

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