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Table 1

Stars with AA Tau-like and variable extinction dominated light curves.

CSIMon ID CoRoT ID 2MASS RA Dec Sp type LC type LC type P (days) P (days) vsini α IRAC [F(disk)/F(star)]4.5μm
(2008) (2011) (2008) (2011) (km s-1)

CSIMon–000056a 223994760 06415315+0950474 6:41:53.16 +9:50:47.4 K5 AAT AAT 5.71 5.86 11.1 ± 2.2 –1.21 1.0
CSIMon–000126 616895876 06405783+0941201 6:40:57.84 +9:41:20.1 M0 Ap 0.35b 14.0 ± 2.0 –1.04 4.8
CSIMon–000250* 223980688 06410050+0945031 6:41:00.50 +9:45:03.1 K3 AATc AAT 8.32 8.93 9.8 ± 2.2 –2.10 2.1
CSIMon–000296* 500007209 06405059+0954573 6:40:50.59 +9:54:57.3 K2 Ap AAT 2.51b 3.91 17.3 ± 2.6 –2.14 1.6
CSIMon–000297* 223976747 06404516+0928444 6:40:45.16 +9:28:44.4 K2 AAT Ap 3.16 30.8 ± 1.8 –2.24 1.6
CSIMon–000314 500007930 06404459+0932261 6:40:44.59 +9:32:26.2 M3 Ap Ap 3.38b 24.0 ± 2.0 –2.61 0.7
CSIMon–000325a 605538641 06405934+0955201 6:40:59.34 +9:55:20.2 G5Vc Ap –1.38
CSIMon–000358 400007959 06410673+0947275 6:41:06.73 +9:47:27.6 M3 Ap AAT 5.86 –1.55 1.3
CSIMon–000379* 223981811 06410497+0950460 6:41:04.97 +9:50:46.1 K2 Ap AATc 3.73b 3.68 25.0 ± 1.2 –1.91 2.2
CSIMon–000433 616919770 06410111+0934522 6:41:01.11 +9:34:52.2 M1 Ap –2.05
CSIMon–000441* 223980048 06405809+0936533 6:40:58.10 +9:36:53.3 M2 AAT Ap 4.06 –1.41 1.0
CSIMon–000456 616872585 06405154+0943242 6:40:51.54 +9:43:24.2 K4 AAT 5.03 19.3 ± 1.5 –1.62 2.5
CSIMon–000498* 500007120 06404750+0949289 6:40:47.50 +9:49:28.9 K3 AATc AAT 4.23 4.28 24.1 ± 2.4 –1.41 2.9
CSIMon–000619 603402479 06411475+0934134 6:41:14.75 +9:34:13.4 K8.5 Ap Ap –1.11 11.5
CSIMon–000654* 500007610 06405949+0929517 6:40:59.50 +9:29:51.7 M3 AATc Ap 4.66 18.0 ± 3.0 –0.92
CSIMon–000660* 223980693 06410051+0929159 6:41:00.51 +9:29:15.9 K4 AAT AAT 5.25 5.25 21.4 ± 2.5 –1.72 3.4
CSIMon–000667* 223987997 06412878+0938388 6:41:28.78 +9:38:38.8 K3 Ap Ap 24.0 ± 2.0 –0.54 1.5
CSIMon–000717 616943877 06411511+0926443 6:41:15.11 +9:26:44.3 M0.5 Ap –1.43 1.4
CSIMon–000774 223980264 06405884+0930573 6:40:58.84 +9:30:57.3 K2.5 AAT Ap 3.46 30.7 ± 1.3 –1.25 2.1
CSIMon–000811* 500007460 06404321+0947072 6:40:43.21 +9:47:07.2 K6 Ap AAT 7.88 13.5 ± 1.7 –1.08 3.0
CSIMon–000824* 223981023 06410183+0938411 6:41:01.84 +9:38:41.1 K4 AAT 7.05 14.8 ± 1.4 –2.02
CSIMon–000928* 223987178 06412562+0934429 6:41:25.62 +9:34:43.0 M0 AAT Ap 9.92 20.1 ± 2.8 –1.11 1.4
CSIMon–001037 223973200 06403086+0934405 6:40:30.86 +9:34:40.5 K1 Ap Ap 8.93b 32.0 ± 3.0 –1.29 11.3
CSIMon–001038 602095739 06402262+0949462 6:40:22.62 +9:49:46.3 M0 Ap –1.73 3.0
CSIMon–001054* 400007538 06403652+0950456 6:40:36.52 +9:50:45.6 M2 Ap AATc 4.08 20.4 ± 2.0 –1.10 2.0
CSIMon–001131 223957455 06393441+0954512 6:39:34.41 +9:54:51.2 M2 Ap AAT 5.15b 5.18 8.8 ± 1.7 –1.38 1.4
CSIMon–001140 223959618 06394147+0946196 6:39:41.47 +9:46:19.7 K4 AAT AAT 3.87 3.90 19.8 ± 2.3 –2.37 0.8
CSIMon–001144* 223971231 06402309+0927423 6:40:23.09 +9:27:42.3 K5 Ap Ap 24.0 ± 3.0 –1.73 3.75
CSIMon–001167* 400007528 06403787+0934540 6:40:37.87 +9:34:54.0 M3 Ap AATc 8.30b 8.78 11.3 ± 2.1 –1.87 1.2
CSIMon–001296 223948127 06390374+0940234 6:39:03.75 +9:40:23.4 K7 Ap AAT 9.75 11.0 ± 1.6 –1.47
CSIMon–001308 223964667 06395924+0927245 6:39:59.24 +9:27:24.5 M0 AAT AAT 6.45 6.68 9.9 ± 2.0 –1.87 0.7
CSIMon–006986 223950070 06390996+1005127 6:39:09.96 +10:05:12.7 K7:M1 AATc 6.16 –1.22
CSIMon–014132a 602070634 06390355+0916159 6:39:03.55 +9:16:16.0 M3.5 AAT 4.48 –1.50

Notes. The first three columns show the identification of each star using our internal CSI 2264 naming scheme, the identification assigned to each star by the CoRoT satellite, and the respective 2MASS identification. In the cases where a star was observed twice by CoRoT and assigned a different identification in each epoch, we use the one given in the first epoch. An asterisk following the CSIMon ID indicates that we have FLAMES/GIRAFFE spectra, and a dagger indicates that we have FLAMES/UVES spectra, both simultaneous with the second CoRoT epoch. The fourth and fifth columns show each star’s coordinates, and the sixth column shows their spectral types, taken from Venuti et al. (2014), except where specified. The seventh and eighth columns show the classification given to the light curve (LC) in each epoch (2008 March observations and 2011 December observations). The ninth and tenth columns show the periods that were measured for each CoRoT light curve in the first (2008) and second (2011) epochs. The eleventh column shows the values of projected rotational velocity vsini measured using FLAMES spectra when available, or Hectochelle spectra otherwise. The twelfth column shows the αIRAC index calculated for each star, which corresponds to the slope of the spectral energy distribution between 3.6 μm and 8 μm. The thirteenth column shows the ratio of disk flux to stellar flux at 4.5 μm, estimated from each star’s SED.

(a)

There is not enough spectral information to classify these stars as CTTS, though they have IR excess and show variability characteristic of CTTS.

(b)

Low probability periods found during a periodogram analysis of the light curves.

(c)

Spectral type from Young (1978).

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