The primary objective of the collaboration is to survey the equatorial regions of the sky using a 16 CCD chip camera in drift scan mode from a 1m Schmidt telescope at Observatorio Nacional de Llano del Hato, located about 2 hours north of Merida, Venezuela. Personally, I hope to contribute by finding quasars through their variability.
Quasars tend to vary in brightness in a stochastic, non-linear nature.
They should be able to be detected as variable objects with repeated scans over the same region of the sky over a range of time scales. Simbad Astronomical Database SkyView v2.3 USNO Astro. Satellite Page Time Service Dept.