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Confirmation of seven faint ATLAS variable star candidates
DOI: 10.5817/OEJV2021-0214 Bibcode: 2021OEJV..214....1T

Thomas, N.; Guan, C.

A pilot survey conducted at the Lookout Observatory has confirmed seven faint (V ~ 13 to 17) variables in the region of Kepler-76b that were recently discovered by the Asteroid Terrestrial-Impact Last Alert System (ATLAS). The ATLAS survey identified 315,000 probably variables within its wide-field survey in 2018. The faintness (down to r ~ 18) an…

2021 Open European Journal on Variable Stars
Gaia 1
L199, A new variable star in M13
DOI: 10.5817/OEJV2021-0213 Bibcode: 2021OEJV..213....1V

Violat-Bordonau, F.

During a routine study of the variable stars of Messier 13 (NGC 6205 = Cl 1639+365) we have discovered the variability of L199 (TYC 2588-1386-2), a red giant star member of the cluster: using the photometric data - in V band - obtained in the 2019 and 2020 campaigns we have verified its variability. Data from the Zwicky Transient Facility (ZTF) an…

2021 Open European Journal on Variable Stars
Gaia 1
Properties of the recently discovered Eclipsing Binary GSC 03421-01402
DOI: 10.5817/OEJV2021-0221 Bibcode: 2021OEJV..221....1L

Lloyd, Ch.; Screech, J.

GSC 03421-01402 is a low-amplitude eclipsing binary with a period of 7.6800475(44) d. The eclipsing binary is one component of a close pair identified in the Gaia EDR3 data with delta G = 0.45 mag. The light-curve suggests that the primary eclipse is total with an observed depth of 0.13 mag, but due to dilution the true depth could be approximatel…

2021 Open European Journal on Variable Stars
Gaia 0
GSC 03588-09315 is a low-amplitude delta Scuti variable
DOI: 10.5817/OEJV2021-0217 Bibcode: 2021OEJV..217....1L

Boyd, D.; Walker, G.; Lloyd, Ch. +3 more

Time-series observations of GSC 03588-09315 show it is a very low amplitude, multiperiodic delta Scuti variable at the limit of detectability. Five frequencies have been identified at 13.86819(24), 8.10026(79), 5.01966(79), 11.67281(55) and 8.17490(59) c/d with amplitudes of 10, 5, 5, 4, and 3 mmag respectively. The spectral energy distribution of…

2021 Open European Journal on Variable Stars
Gaia 0