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In 2008 January the 24th Chinese expedition team successfully deployed theChinese Small Telescope ARray (CSTAR) to DomeA, the highest point on theAntarctic plateau. CSTAR consists of four 14.5cm optical telescopes, each witha different filter (g, r, i and open) and has a 4.5degree x 4.5degree field ofview (FOV). It operates robotically as part of the Plateau Observatory, PLATO,with each telescope taking an image every 30 seconds throughout the yearwhenever it is dark. During 2008, CSTAR #1 performed almost flawlessly,acquiring more than 0.3 million i-band images for a total integration time of1728 hours during 158 days of observations. For each image taken under good skyconditions, more than 10,000 sources down to 16 mag could be detected. Weperformed aperture photometry on all the sources in the field to create thecatalog described herein. Since CSTAR has a fixed pointing centered on theSouth Celestial Pole (Dec =-90 degree), all the sources within the FOV of CSTARwere monitored continuously for several months. The photometric catalog can beused for studying any variability in these sources, and for the discovery oftransient sources such as supernovae, gamma-ray bursts and minor planets.

The First Release of the CSTAR Point Source Catalog from Dome A, Antarctica