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Table 2:

Sample of the NIR catalogue of periodic variables in Paper I.

IDa
Ib [mag] $I_{\rm err}$ [mag] J [mag] $J_{\rm err}$ [mag] H [mag] $H_{\rm err}$ [mag] K [mag] $K_{\rm err}$ [mag] $\Delta (I-K)$c Flagd
1 15.535 0.002 13.540 0.030 12.820 0.040 12.510 0.030 -0.115 2MASS
3 13.205 0.001 11.284 0.001 10.970 0.001 10.116 0.000 0.109 UKIDSS
7 15.637 0.002 13.930 0.030 13.370 0.040 12.940 0.020 -0.013 2MASS
13 15.551 0.002 14.002 0.003 13.374 0.003 13.136 0.003 -0.125 UKIDSS
10384 17.954 0.054 14.960 -1.000 14.160 -1.000 13.520 -1.000 0.114 VLT
10387 17.674 0.011 14.770 0.020 13.660 0.030 13.070 0.020 0.334 2MASS
20323 14.495 0.001 12.260 0.020 11.210 0.030 10.810 0.020 0.145 2MASS
20325 15.397 0.005 13.140 0.040 12.410 0.040 12.100 0.040 -0.313 2MASS
20326 18.853 0.047 14.680 -1.000 13.270 -1.000 12.370 -1.000 1.683 VLT
20672 19.654 0.048 17.276 0.022 15.957 0.023 15.638 0.022 0.516 UKIDSS

Notes. The complete catalogue is available electronically at the CDS. (a) Identification numbers from Rodriguez-Ledesma et al. (2009); (b) I magnitudes from Rodriguez-Ledesma et al. (2009); (c)  $\Delta{(I-K)}>0.3$indicates the precense of a circumstellar disk; (d) This flag shows the origin of the NIR data. The possibilities are: 2MASS, UKIDSS, VLT. The VLT data set was not provided with individual photometric errors. A description of the estimated errors is available in Sect. 2.


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