Pre-HEAT: submillimeter site testing and astronomical spectra from Dome A, Antarctica

@inproceedings{Kulesa2008PreHEATSS,
  title={Pre-HEAT: submillimeter site testing and astronomical spectra from Dome A, Antarctica},
  author={C. Kulesa and C. Walker and M. Schein and D. Golish and N. Tothill and P. Siegel and S. Weinreb and G. Jones and J. Bardin and K. Jacobs and C. L. Martin and J. Storey and M. Ashley and J. Lawrence and D. Luong-Van and J. Everett and L. Wang and L. Feng and Z. Zhu and J. Yan and J. Yang and Xiu-lu Zhang and X. Cui and X. Yuan and J. Hu and Z. Xu and Z. Jiang and H. Yang and Y. Li and B. Sun and W. Qin and Z. Shang},
  booktitle={Astronomical Telescopes + Instrumentation},
  year={2008}
}
Pre-HEAT is a 20 cm aperture submillimeter-wave telescope with a 660 GHz (450 micron) Schottky diode heterodyne receiver and digital FFT spectrometer for the Plateau Observatory (PLATO) developed by the University of New South Wales. In January 2008 it was deployed to Dome A, the summit of the Antarctic plateau, as part of a scientific traverse led by the Polar Research Institute of China and the Chinese Academy of Sciences. Dome A may be one of the best sites in the world for ground based… Expand
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