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Table A.1.

Known and suspected variable stars from the VSX catalogue without well-determined parameters (period and amplitude) detected with MASCARA.

ASCC Identifier VSX ID VSX Var. Typea MASCARA V RA (J2000) Dec (J2000) Nr. Obs. Periodb (days) Amp.c (mmag) Epochd (HJD – 2 450 000)
7 027 HIP 9494 V0779 Cas EA: 6.69 02h02′09.3″ +75°30′08″ 8857 6.3530(7) 263 7203.5844
7 512 HIP 10309 NSV 15448 DSCTC: 6.45 02h12′49.9″ +79°41′30″ 9574 0.21: 7 7227.72
11 321 HD 21179 V0805 Cas SRB 6.39 03h30′19.4″ +71°51′50″ 7274 39.4(1) 110 7240.7
18 914 HIP 26940 NSV 16615 P 6.77 05h43′00.7″ +73°59′09″ 5912 0.088: 48 7201.718
22 011 HD 47505 EP Cam SRB 8.07 06h48′37.5″ +76°59′24″ 6223 39.6(1) 194 7234.7
22 755 HIP 34101 CM Cam FKCOM 6.99 07h04′15.1″ +75°24′41″ 5541 15.87(6) 65 7377.4
24 395 HIP 36978 NSV 17498 7.73 07h36′02.2″ +76°50′00″ 6165 23.1(4) 58 7306.7
26 716 TYC 4631-2314-1 NSV 3974 E 8.31 08h25′12.0″ +84°00′51″ 11785 1.1664(2) 139 7280.4131
27 874 HD 74225 FL Cam LB 7.01 08h50′46.6″ +78°09′55″ 5776 35.68(5) 207 7219.38
31 460 HIP 51111 NSV 18397 8.29 10h26′33.2″ +73°47′16″ 5616 22.2(4) 79 7192.4

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

(a)

Variability types in the ‘MASCARA’ column were visually estimated based on the shape, period and amplitude of the light curve. These are only included if they disagree with or complement the VSX catalogue. “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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