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Table 3

Parameters of the WTTSs observed by CoRoT and/or FLAMES/VLT.

Mon IDa 2Mass IDb SpTc EW Hα d ErEW d W10%Hα d EW Hα e FUR06f α IRAC g
(kms-1)

CSIMon-000008 06414859+0954115 K5
CSIMon-000009 06420914+0948048 F5
CSIMon-000014 06420664+0941317 K7:M0
CSIMon-000015 06420911+0959027 K7:M0
CSIMon-000018 06411322+0955086 K3:K4 3.0 –2.73
CSIMon-000020 06420924+0944034 K7 w
CSIMon-000022 06410457+1000426 M4
CSIMon-000024 06415684+0947451 M1
CSIMon-000026 06410518+1000189 M4 6.5
CSIMon-000029 06410328+0957549 K7 1.5 –2.85
CSIMon-000033 06410726+0958311 K5 1.4 w –2.78

Notes. Only a portion of this table is shown here. A full version is available at the CDS. This table is ordered according to the Mon ID.

(a)

“CSIMon” is an internal identification of the CSI 2264 campaign.

(b)

2MASS identification.

(d)

Hα parameters obtained in this work using FLAMES spectra. We used the convention that positive Hα equivalent width indicates Hα in emission, and negative values indicate Hα in absorption. The uncertainties were calculated assuming a Poisson distribution.

(e)

Hα equivalent width obtained by Dahm & Simon (2005).

(f)

Classification as CTTS (c) and WTTS (w) by Fűrész et al. (2006).

(g)

αIRAC is the slope of the spectral energy distribution between 3.6 μm and 8 μm obtained by Teixeira et al. (2012).

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