  The LaSilla/QUEST Variability Survey (LSQ) and the Carnegie Supernova Project
(CSP II) are collaborating to discover and obtain photometric light curves for
a large sample of low redshift (z < 0.1) Type Ia supernovae. The supernovae are
discovered in the LSQ survey using the 1 m ESO Schmidt telescope at the La
Silla Observatory with the 10 square degree QUEST camera. The follow-up
photometric observations are carried out using the 1 m Swope telescope and the
2.5 m du Pont telescopes at the Las Campanas Observatory. This paper describes
the survey, discusses the methods of analyzing the data and presents the light
curves for the first 31 Type Ia supernovae obtained in the survey. The SALT 2.4
supernova light curve fitter was used to analyze the photometric data, and the
Hubble diagram for this first sample is presented. The measurement errors for
these supernovae averaged 4%, and their intrinsic spread was 14%.
