Open Access

Table D.1.

Membership analysis of all the members and candidate members of NGC 2244 used in this work. Only the first 10 lines are shown, the full table is available at the CDS.

ID RA DEC SpT AV Teff KMOS VIMOS M22a M17b Excessc Member
° ° [mag] [K] Obs Indd Obs Hαe
3 97.961 4.97661 M1.75 2.4 3590 N - Y N N Y N ?
5 97.96189 4.96056 M5.5 6.6 3100 Y Y N - - - Y Y
6 97.96191 4.95555 M6.0 3.0 2900 Y Y N - - - Y Y
18 97.96784 4.97609 M5.0 0.8 3100 Y Y Y N N Y N Y
25 97.97005 4.96949 M6.25 0.4 2775 N - Y Y N Y N Y
31 97.97226 4.95376 - 0.25 2600 N - N - Y - Y Y
32 97.97254 4.94106 M1.75 1.8 3500 N - Y N Y Y N Y
33 97.97304 4.94408 - 3.25 4600 N - N - Y Y Y Y
34 97.97431 4.97966 M3.5 0.8 3270 N - Y N N Y N ?
35 97.97451 4.95315 - 3.25 5000 N - N - Y - Y Y

aMembership in Mužić et al. (2022). bMembership in Meng et al. (2017). cInfrared excess key derived in Sect. 3.2. dKMOS gravity-sensitive spectral indices key defined in Sect. 3.1.4. eVIMOS Hα emission consistent with accretion.

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