R. Toma

TL;DR: OmegaWhite as mentioned in this paper is a wide-field high-cadence $g$-band synoptic survey which aims to unveil the Galactic population of short-period variable stars (with periods $<$ 80 min), including ultracompact binary star systems and stellar pulsators.

TL;DR: OmegaWhite is a wide field, high cadence, synoptic survey targeting fields in the southern Galactic plane, with the aim of discovering short period variable stars.

TL;DR: In this paper, the authors presented photometric and spectroscopic follow-up observations of short-period variables discovered in the OmegaWhite survey: a wide-field high-cadence g-band synoptic survey targeting the Galactic Plane.

TL;DR: In this paper, the discovery and follow-up observations of the second known variable warm DQ white dwarf OWJ175358.9 (OW J1753−3107) are presented.

TL;DR: In this article , the authors presented the results of a search for short-period variable stars in the field of 20 open clusters using light curves with ∼3 min cadence and a duration of 2 hrs made using the OmegaWhite survey.