MOA-cam3: a wide-field mosaic CCD camera for a gravitational microlensing survey in New Zealand
arXiv:0804.0653 · doi:10.1007/s10686-007-9082-5
Abstract
We have developed a wide-field mosaic CCD camera, MOA-cam3, mounted at the prime focus of the Microlensing Observations in Astrophysics (MOA) 1.8-m telescope. The camera consists of ten E2V CCD4482 chips, each having 2kx4k pixels, and covers a 2.2 deg^2 field of view with a single exposure. The optical system is well optimized to realize uniform image quality over this wide field. The chips are constantly cooled by a cryocooler at -80C, at which temperature dark current noise is negligible for a typical 1-3 minute exposure. The CCD output charge is converted to a 16-bit digital signal by the GenIII system (Astronomical Research Cameras Inc.) and readout is within 25 seconds. Readout noise of 2--3 ADU (rms) is also negligible. We prepared a wide-band red filter for an effective microlensing survey and also Bessell V, I filters for standard astronomical studies. Microlensing studies have entered into a new era, which requires more statistics, and more rapid alerts to catch exotic light curves. Our new system is a powerful tool to realize both these requirements.
Experimental Astronomy in press
References in corpus (9)
- A method for optimal image subtraction
- The MACHO Project: Microlensing Results from 5.7 Years of LMC Observations
- Possible Gravitational Microlensing of a Star in the Large Magellanic Cloud
- Subaru Prime Focus Camera -- Suprime-Cam --
- Discovery of a Cool Planet of 5.5 Earth Masses Through Gravitational Microlensing
- Real-Time Difference Imaging Analysis of MOA Galactic Bulge Observations During 2000
- Detecting Earth-Mass Planets with Gravitational Microlensing
- A Jovian-mass Planet in Microlensing Event OGLE-2005-BLG-071
- Microlensing optical depth towards the Galactic bulge from MOA observations during 2000 with Difference Image Analysis
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