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Table 2

Median photometry, variability amplitudes, light curve rms, J index, and color slopes for members discussed in this study.

CSIMon-#1 Var2 Class3 SpT4 medu medr ampu ampr rmsu rmsr J index σslope5
000007 * c K7 17.22 14.49 1.104 0.207 0.34 0.05 32.97 0.174 0.004
000009 w F5 18.21 14.99 0.019 0.010 0.005 0.003 0.11
000011 * c K7 16.76 15.09 1.008 0.429 0.34 0.14 58.26 0.642 0.008
000014 w K7:M0 18.88 14.25 0.023 0.007 0.006 0.003 0.20
000015 w K7:M0 19.39 14.55 0.028 0.008 0.008 0.003 0.60
000017 * c K5 18.41 14.94 0.216 0.130 0.06 0.04 8.50 1.52 0.15
000018 * w K3:K4.5 19.05 14.99 0.192 0.073 0.03 0.02 2.05 0.70 0.08
000020 * w K7 20.02 15.94 0.153 0.109 0.04 0.03 1.65 1.2 0.3
000022 w M4 21.80 17.72 0.238 0.044 0.06 0.016 0.20
000023 w M3 22.30 18.18 0.475 0.063 0.11 0.02 0.07

Notes. A full version of the table is available in electronic form at the CDS. A portion is shown here for guidance regarding its form and content.

(1)

Object identifiers adopted within the CSI 2264 project (see Cody et al. 2014).

(2)

Variability flag; objects that exhibit a distinct level of variability stronger than that for field stars, based on the J-index indicator, are marked with an asterisk.

(3)

“c” = CTTS; “w” = WTTS (classification from Venuti et al. 2014).

(4)

Spectral type estimates from Venuti et al. (2014).

(5)

rms uncertainty on Δr/ Δ(u − r) color slope.

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