Studying bright variable stars with the Multi-site All-Sky CAmeRA (MASCARA)

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Table B.1.

New candidate variable stars detected with MASCARA.

ASCC	Identifier	Var. type^a	V	RA (J2000)	Dec (J2000)	Nr. Obs.	Period^b (days)	Amp.^c (mmag)	Epoch^d (HJD–2 450 000)
3 132	HIP 4090	–	7.72	00^h52′29.0″	+79°50′26″	10048	8.00(3)	52	7306.77
3 347	TYC 4619-1223-1	P	8.14	00^h56′10.8″	+85°27′33″	11238	0.094:	18	7292.544
7 335	TYC 4503-2063-1	P	7.0	02^h08′56.1″	+79°20′45″	9294	0.5414(7)	16	7279.5832
7 988	HD 14382	P	7.82	02^h23′04.7″	+70°20′36″	7800	0.4457(8)	17	7279.6429
11 298	HD 20110	–	8.36	03^h29′50.9″	+84°02′20″	12276	33(1)	69	7212
20 609	TYC 4525-994-1	–	8.4	06^h17′55.6″	+76°40′29″	5497	82:	193	7269
23 934	HIP 36159	E	7.38	07^h26′57.6″	+75°36′44″	5942	3.68(2)	24	7349.78
28 165	HD 75544	P	7.32	08^h58′22.7″	+78°08′45″	5446	0.11:	13	7153.37
42 606	HIP 77211	P	8.16	15^h45′53.1″	+82°22′12″	10754	0.57:	19	7178.4
44 194	HD 149681	P	5.55	16^h25′43.5″	+78°57′49″	10229	0.05:	4	7192.457

Notes. The full version of this table is available in electronic form at the CDS.

^(a)

Variability types were visually estimated based on the shape, period and amplitude of the light curve. “E” indicates an eclipsing binary, “P” a pulsating variable.

^(b)

Errors correspond to a 3σ confidence interval. For entries marked with a colon (:), no such confidence interval could be determined – these are listed with two significant digits.

^(c)

Amplitude in the MASCARA band.

^(d)

Epoch of a minimum in brightness.

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