Table 1: Observing log of the WX Eri observations. The fourth column gives the photometric shift (in magnitudes, V) needed to bring the data to the same scale (see text).

Telescope	Instrument	Filter	Phot.shift	Observer(s)	Hrs of meas.
SAAO 1.0-m	SAAO CCD	B,V	0.000	TA	15.5
Beersel Hills 0.4-m	SBIG-ST7E CCD	V	-0.043	PVC, PL	7.0
Las Campanas 1.3-m	8kMOSAIC	V	-0.029	HWD	4.6
Hoher List 1.0-m	HOLICAM	V	0.029	PL, PVC	2.4
ESO 1.54-m	DFOSC	V	0.050	CS	1.9
Esteve Duran 0.6-m	CCD	V	0.025	EG-M	1.0
Total					32.4