All Tables

Table 1: Properties of the CCD cameras used during WeCAPP at Wendelstein (We) and Calar Alto (CA) Observatories. Both CCDs have a pixel size of $24~\mu{\rm m}$ .
Table 2: Extract from the WeCAPP catalogue of variable stars. We give the identification, the right ascension and declination, the assigned period and its significance s ( $0.1 \stackrel{\wedge}{=}$ un-significant, $70 \stackrel{\wedge}{=}$ highly significant) in R and I, the amplitude of variation in both bands, and finally a classification according to the scheme presented in Sects. 4 and 5. The variation amplitudes $\Delta F_R$ and $\Delta F_I$ are given in units of [10^-5 Jy].
Table 3: Coincidences between the WeCAPP catalogue of variable stars and the X-ray selected catalogue of point sources by Kaaret (2002). A search radius of 1 $\hbox {$^{\prime \prime }$ }$ was used. We give the identifier and WCS coordinates for the WeCAPP sources, and the identifier for the Kaaret (2002) sources. For sources coincident with the 2MASS catalogue Cutri et al. (2000), we give the 2MASS identifier also. We also show the difference $\Delta$ r of the matching of both catalogues for each of the correlated sources.
Table 4: Coincidences between the WeCAPP catalogue of variable stars and the X-ray selected catalogue of point sources by Kong et al. (2002). A search radius of 1 $\hbox {$^{\prime \prime }$ }$ was used. We give the identifier and WCS coordinates for the WeCAPP sources, and the identifier and IAU name for the Kong et al. (2002) sources. We also show the difference $\Delta$ r of the matching of both catalogues for each of the correlated sources. Symbols in the last row are taken from Kong et al. (2002), and they mark globular cluster counterparts (g, search radius 3 $\hbox {$^{\prime \prime }$ }$ ), X-ray variable sources (v), and X-ray transients (t).
Table 5: Coincidences between the WeCAPP catalogue of variable stars and the General Catalogue of Variable Stars (GCVS, Durlevich et al. 1996). A search radius of 1 $\hbox {$^{\prime \prime }$ }$ was used. We give the identifier, WCS coordinates and a classification for the WeCAPP sources, and the identifier and a classification according to the GCVS. We also the difference $\Delta$ r of the matching of both catalogues for each of the correlated sources.