Table 6
Periods of the classical T Tauri stars observed with the FLAMES spectrograph obtained with photometric and spectroscopic diagnostics.
| Mon IDa | LC_2008 b | PCoRoT_2008 b | LC_2011 b | PCoRoT_2011 b | P Hα c | P HeI d | Regimee | Hα Typef | Ṁ Hα g |
| (days) | (days) | (days) | (days) | (M⊙/ yr) | |||||
|
|
|||||||||
| CSIMon-001099 | 1 | 3.31 | 1 | 3.38 | NP | – | S | IIB | 3.23e-09 |
| CSIMon-000103 | 1 | 1.67 | 1 | 3.35 | NP | – | I | 9.61e-09 | |
| CSIMon-000177 | 1 | 3.01 | 1 | 3.01 | NP | – | I | 9.29e-09 | |
| CSIMon-000335 | 1 | 4.51 | 1 | 4.58 | NP | – | I | 2.31e-09 | |
| CSIMon-000965 | 1 | 9.38 | 1 | 9.68 | NP | 9.4 | S | IIR | 1.76e-09 |
| CSIMon-000810 | 1 | 2.93 | 1 | 2.93 | NP | – | I | 1.24e-09 | |
| CSIMon-000964 | 1 | 3.34 | 1 | 3.32 | NP | – | I | 1.49e-09 | |
| CSIMon-000326 | 1 | 7.05 | 3 | NP | NP | I | 1.99e-09 | ||
| CSIMon-000220 | 1 | 0.76 | 3 | NP | – | I | 2.50e-10 | ||
| CSIMon-000804 | 1 | 3.23 | 3 | NP | – | I | 4.83e-10 | ||
| CSIMon-001033 | 1 | 14.15 | – | 6.30 | – | S | IIR | 4.69e-09 | |
| CSIMon-000250 | 2 | 4.16 | 2 | 8.93 | 7.5/8.9 | 8.6 | S | IIR | 1.44e-09 |
| CSIMon-000660 | 2 | 5.25 | 2 | 5.10 | 5.2 | – | S | IIIR | 1.45e-10 |
| CSIMon-000498 | 2 | 4.23 | 2 | 4.28 | NP | – | I | 1.00e-08 | |
| CSIMon-001199 | 2 | 3.75 | 2 | 3.61 | NP | – | IIB | 1.46e-09 | |
| CSIMon-000297 | 2 | 3.16 | 3 (E) | NP | – | IIR | 5.75e-09 | ||
| CSIMon-000928 | 2 | 4.96 | 3 | NP | 10.3 | I | 6.91e-10 | ||
| CSIMon-000654 | 2 | 4.66 | 3 (E) | NP | NP | I | 4.82e-09 | ||
| CSIMon-000441 | 2 | 4.06 | 3 (E) | NP | Noise | IIB | 3.24e-09 | ||
| CSIMon-000824 | 2 | 7.05 | – | NP | – | U | IVR | 3.28e-09 | |
| CSIMon-001144 | 3 (E) | 3 (E) | NP | Noise | II | 2.17e-09 | |||
| CSIMon-001275 | 3 | 3 | NP | – | IIIB | 2.51e-08 | |||
| CSIMon-000119 | 3 | 3 | NP | NP | IIIB | 3.34e-09 | |||
| CSIMon-000558 | 3 (A) | 3 | 11.70? | 10.5 | 10.7 | IIB | 6.06e-08 | ||
| CSIMon-000168 | 3 (E) | 3 (E) | NP | Noise | II | 3.77e-09 | |||
| CSIMon-000926 | 3 | 3 | NP | NP | I | 8.66e-09 | |||
| CSIMon-000681 | 3 (E) | 3 (E) | NP | NP | IIB | 4.49e-08 | |||
| CSIMon-000280 | 3 | 3 | NP | – | IIR | 5.90e-10 | |||
| CSIMon-000290 | 3 | 3 | NP | 8.3/11.4 | I | 2.25e-08 | |||
| CSIMon-000328 | 3 | 3 | NP | NP | I | 3.90e-09 | |||
| CSIMon-000448 | 3 | 3 | NP | Noise | I | 8.16e-09 | |||
| CSIMon-000314 | 3 (E) | 3 (E) | NP | Noise | I | 1.06e-08 | |||
| CSIMon-000951 | 3 | 3 | NP | Noise | I | 3.21e-08 | |||
| CSIMon-000937 | 3 | 3 | NP | – | I | 7.24e-10 | |||
| CSIMon-000667 | 3 (E) | 3 (E) | 5.9 | – | S | IIB | 1.84e-09 | ||
| CSIMon-000945 | 3 (A) | 3 (A) | NP | 7.4 | I | 6.35e-09 | |||
| CSIMon-001022 | 3 (A) | 3 (A) | NP | 8.9/12.5 | IIIB | 6.31e-09 | |||
| CSIMon-000996 | 3 (A) | 3 (A) | 8.3 | 8.3 | I | 2.79e-08 | |||
| CSIMon-000510 | 3 (A) | 3 (A) | NP | NP | I | 2.87e-08 | |||
| CSIMon-000341 | 3 (A) | 3 (A) | NP | NP | I | 3.55e-08 | |||
| CSIMon-000370 | 3 | 3 | 11.82? | NP | NP | I | 2.55e-08 | ||
| CSIMon-000765 | 3 | 1 | 2.41 | NP | – | I | 6.48e-09 | ||
| CSIMon-000379 | 3 (E) | 2 | 3.68 | NP | – | S | IIR | 1.26e-09 | |
| CSIMon-001054 | 3 (E) | 2 | 4.08/8.17* | NP | 8.1 | I | 1.35e-08 | ||
| CSIMon-000296 | 3 (E) | 2 | 3.91 | NP | – | S | IIR | 1.73e-09 | |
| CSIMon-000811 | 3 (E) | 2 | 7.88 | 12.5 | 10.5 | S | IIR | 6.75e-09 | |
| CSIMon-000846 | 3 | – | NP | NP | I | – | |||
| CSIMon-000795 | 3 | – | NP | NP | IIB | 6.59e-08 | |||
| CSIMon-000457 | 3 | – | NP | – | IIIB | 6.01e-09 | |||
| CSIMon-000260 | 3 (E) | – | NP | 9.2 | IIB | 2.26e-08 | |||
| CSIMon-000893 | 3 | – | NP | NP | I | 1.02e-08 | |||
| CSIMon-000131 | – | 3 | NP | 9.1 | IIR | – | |||
| CSIMon-000423 | – | 3 | NP | Noise | I | 1.44e-08 | |||
| CSIMon-000632 | – | – | NP | Noise | IIB | 1.33e-08 | |||
| CSIMon-001287 | – | – | NP | Noise | IIR | 9.38e-08 | |||
| CSIMon-000603 | – | – | NP | Noise | IIIB | 6.07e-08 | |||
| CSIMon-000239 | – | – | 5.6 | – | ? | – | |||
| CSIMon-001128 | – | – | NP | Noise | I | 1.88e-08 | |||
Notes. This table is ordered by the classification of the CoRoT light-curve morphology from the 2008 campaign.
CoRoT light-curve morphology and photometric period obtained in this work: 1 = spot-like, 2 = AA Tau-like, 3 = non-periodic light curves. Accretion bursts stars and aperiodic extinction light curves are identified by (A) and (E), respectively.
Period obtained with HeI line 
from FLAMES spectra. Noise means that the HeI line is present on the spectrum but it is dominated by noise.
Accretion regime: S-stable and U-unstable, as discussed in Sect. 10.
Morphology of Hα line by Reipurth et al. (1996) discussed in Sect. 7.
The photometric period was obtained using Scargle periodogram and auto-correlation function, as explained in Sect. 9.1.
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