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Table 2.

Observational parameters of our sample of full disk systems.

Mon ID (a) TwoMass ID (b) SpT (c) EWHα(d) W10%Hα(d) EWHα(e) Class (f) αIRAC(g) R(h) T(h) UVExc.(h) UVExc.(h) Hα(d) Dist (i)
(Å) (km s−1) (Å) (R) (K) (mag) (M yr−1) (M yr−1) (pc)
Mon-000007 06415304+0958028 K7 c −1.47 4000. −0.650 6.0E−08
Mon-000017 06413199+1000244 K5 13.1 c −2.69 1.45 4395. −0.270 5.8E−09 694.0
Mon-000028 06410511+0958461 M3.5 294.5 c −1.64 0.57 3300. −1.400 7.4E−10 705.8
Mon-000056 06415315+0950474 K5 1.8 c −1.36 1.52 4395. 0.010 5.8E−09 756.8
Mon-000059 06410334+1000478 M4 c −1.44 0.76 3230. −1.110 1.2E−09 788.8
Mon-000063 06411193+0959412 M2.5 19.4 c −1.37 1.19 3430. −1.030 6.2E−09 748.9
Mon-000064 06411070+0957424 M1.5 3.5 w −1.15 1.62 3590. −0.320 4.7E−09 736.4
Mon-000080 06411795+1004021 M3 w −1.12 1.17 3360. −0.460 1.9E−09 723.2
Mon-000081 06405978+1002126 M2 155.0 c −1.01 1.00 3500. −1.340 5.4E−09 667.7
Mon-000090 06410896+0933460 M3 51.0 c −0.88 2.26 3360. −0.550 1.1E−08 786.6
Mon-000099 06411610+0926435 M4.5 w −1.44 1.16 3175. 0.360 1.1E−10 743.3
Mon-000103 06405954+0935109 K6 15.6 401 6.4 c −1.14 3.84 4200. 0.591 9.6E−09 658.2
Mon-000106 06405272+0928437 M0.5 c −1.40 0.74 3800. −1.260 1.3E−09 764.8
Mon-000113 06410028+0928341 K6 314.6 c −1.25 0.71 4200. −2.380 6.3E−09 672.4
Mon-000117 06405413+0948434 M2.5 353.0 c −2.34 1.21 3430. −2.090 3.4E−08 752.9
Mon-000119 06412100+0933361 K6 10.5 466 10.6 c −1.44 2.04 4200. −0.147 3.3E−09
Mon-000126 06405783+0941201 M0 26.4 c −1.09 2.02 3920. −0.540 2.1E−08 573.7
Mon-000136 06411599+0926094 M0 174.1 c −0.53 1.99 3920. −1.150 1.6E−08 792.4
Mon-000137 06404712+0942077 M2 11.4 c −1.54 1.36 3500. −0.360 2.9E−09 557.9
Mon-000145 06412346+0945586 K7 4.0 w −2.46 1.39 4000. 0.050 820.3
Mon-000153 06405990+0947044 M3 39.9 c −1.71 1.35 3360. −1.220 9.1E−09 791.7
Mon-000165 06410481+0944333 K4.5 92.9 c −0.62 0.76 4490. −1.580 1.5E−09 743.8
Mon-000168 06414287+0925084 K5:M0 44.9 390 86.0 c −1.38 1.20 4157. −1.450 1.1E−08 3.8E−09 776.0

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. Here, CSI was omitted for brevity.

(b)

2Mass identification.

(c)

Spectral type obtained by Venuti et al. (2014).

(d)

Hα parameters obtained using FLAMES spectra by Sousa et al. (2016). They used the convention that positive Hα equivalent width indicates Hα in emission, and negative values correspond to Hα in absorption.

(e)

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

(f)

Classification as CTTS (c) and WTTS (w) by Sousa et al. (2016) and Venuti et al. (2014).

(g)

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

(h)

Parameters obtained using CFHT data by Venuti et al. (2014).

(i)

Distance from the Sun which was obtained from the Gaia parallax data, following (Luri et al. 2018).

The systems Mon-000168, Mon-000358, Mon-000361, Mon-000687, Mon-000753 could be classified as transition disk using transition disk select criteria from Grant et al. (2018), see text.

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