**Table 1:** Observed outbursts of WX Cet. Epoch of maximum (HJD-2 400 000), $V_{\rm max}$ , number of observations, decline gradient (mag d^-1), class, relevant time intervals, and references (R1 refers to visual and photographic estimates, R2 to phase-resolved photometry). The event of HJD 2431642 was probably observed at a late outburst state.
$T_{\rm max}$	$V_{\rm max}$	N	W [d]	grad	Cl	$\Delta t_{\rm N}$	$\Delta t_{\rm S}$	R1	R2
29 079	9.45	1	-	-	S			1
29 567	10.2	1	-	-	S		488	1
31 642	13.5	2	-	0.16:	S?			1
38 294	10.5	4	-	0.15	S			2
47 682	$\lesssim$ 10.8	53	20	0.14	S			3-7	9
47 864	12.55	10	$\leq$ 3	0.75	N	182		4, 9
48 086	13.0	3	$\leq$ 3	0.4:	N	222		3
48 191	13.3	1	-	-	N	105		4
48 447	12.2	12	15	0.09	S	256	765	4, 8	10
49 375	$\lesssim$ 11.7	10	15	0.09	S		928	4
49 618	13.6	1	-	-	N	243:		4
50 283	$\lesssim$ 11.5	37	16:	0.17	S		908	4	11
50 697	12.5	10	3	1.00	N			4
51 128	11.6	41	16	0.11	S		845	4	11-13
51 883	13.5	1	-	-	N			4
52 087	$\lesssim$ 11.8	9	16	0.13	S	204	959	4,14	15
53 346	12.0	13	15	0.10	S		1259	4	15

References: 1: Gaposhkin (1976); 2: Strohmeier (1964); 3: McIntosh (1991); 4: AAVSO data base; 5: McNaught et al. (1989); 6: Overbeek & Pearce (1989); 7: Pearce et al. (1989); 8: Bateson & Jones (1991); 9: O'Donoghue et al. (1991); 10: Kato (1995); 11: Patterson et al. (2003); 12: Kato et al. (2001); 13: Howell et al. (2002); 14: ASAS3 data base Pojmanski (2001) 15: this paper.

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