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Table C.1.

Spectroscopic indicators and spectral types (extract).

source_id pEW(Li) epEW(Li) refLi EW(Hα) eEW(Hα) refHa veiled pEW(Na) epEW(Na) refNa SpT refSpT

Gaia DR3 Å Å Å Å Å Å
3216486478101979520 0.57 0.02 2,3 21.0 2.0 3,7 Y 1.6 0.1 7 M1.0 2
3216500531234897920 0.41 0.03 3 23.4 2.4 3,7 Y K4 3
3216447239280699008 3.1 0.3 7 N K7.0 7
3216524651771210240 0.52 0.09 3 10.5 0.7 3 Y M0 3
3216521765553185152 0.19 0.09 3 17.0 1.0 3 Y M1.5 3
3216446689524900480 2.6 0.3 7 N K7.0 7
3216500634314117504 3.7 0.4 7 N M1.0 7
3216446002330124416 0.45 0.07 3 8.1 0.6 3 N M7 3
3216496030109176448 0.73 0.10 6 4.0 0.8 6 N M3 6
3216445899250910976 0.25 0.25 3,7 47.5 30.1 3,7 Y K7 3
3216497267059750912 0.35 0.10 6 60.0 7.0 6 Y M5.5 6
3216501527667171712 3.3 0.3 7 N 1.6 0.1 7 M1.5 7
3216497713736341248 0.65 0.15 6 38.9 7.6 6,7 Y 1.7 0.0 5 M4 6
3216524720490689024 2.3 0.0 5
3216501871264551040 14.4 1.4 7 Y 2.5 0.2 7 M3.5 7
3216498022973982336 0.56 0.08 4 2.0 0.4 4,5
3216494793158603392 9.9 1.0 7 N 2.2 0.2 7 M5.0 7
3216496476785764736 0.37 0.07 4 2.0 0.3 4,5
3216110234671579648 0.51 0.08 4 N 2.1 0.2 4,5 M4.5 7
3216109861009561728 0.61 0.02 3,6 5.8 1.6 3,6,7 Y K8 6
3216494793158602368 0.44 0.05 3 1.5 0.2 3 N K0 3
3216486203224073088 K9.5 2
3216488333527834880 0.58 0.06 4 1.8 0.1 4
3216108933296640640 0.57 0.00 2 1.8 0.0 5 M4.5 2
3216486271943551616 0.59 0.00 2 3.8 0.4 7 N K9.5 2
3216439057367561472 0.63 0.14 4 2.4 0.0 4,5
3216446380287243392 0.72 0.15 6 20.5 6.0 6 Y 2.4 0.0 5 M5.5 6
3216486924778686976 0.15 0.15 2,7 77.8 7.8 7 Y 1.1 0.2 7 M3.5 2
3216497988614248832 8.2 0.8 7 N 2.4 0.2 7 M2.0 7
3216486233291778944 0.51 0.06 2 5.2 0.5 7 N 0.8 0.2 7 M4.5 2
3216109723570616320 0.55 0.06 4 2.5 0.0 4,5
3216442355903486080 0.31 0.07 3,4 125.0 15.0 3 Y 2.7 0.2 4,5 M6.5 3
3216111952658344064 0.61 0.04 4 14.3 1.4 7 N 2.1 0.4 4,5,7 M5.5 7
3216112919026100352 0.54 0.06 4 15.5 1.6 7 N 2.3 0.1 4,5,7 M5.0 7

Notes. If measurements are available in multiple catalogues, we computed the mean value and standard deviation. Corresponding references are provided for each catalogue. Chromospheric criterion from Barrado y Navascués & Martín (2003) is used to distinguish between veiled (Y) and non-veiled (N) stars. The entire table for all stars with available spectroscopy is available only in electronic form at the CDS.

References. (2) Sacco et al. (2008), (3) Caballero et al. (2019), (4) Kenyon et al. (2005), (5) Maxted et al. (2008), (6) Zapatero Osorio et al. (2002), (7) Hernández et al. (2014).

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