Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-28T01:01:58.418Z Has data issue: false hasContentIssue false

Ten years from the Antarctic Sub-millimeter Telescope and Remote Observatory

Published online by Cambridge University Press:  01 August 2006

Christopher L. Martin*
Affiliation:
Department of Physics and Astronomy, Oberlin College, Oberlin, OH 44074, USA email: Chris.Martin@oberlin.edu
Rights & Permissions [Opens in a new window]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Beginning with the winter season of 1995 and for the next ten years, the Antarctic Sub-mm Telescope and Remote Observatory (AST/RO, Stark et al. 1997; Stark et al. 2001; <http://www.cfa.harvard.edu/ASTRO/>), a 1.7m diameter, offset Gregorian telescope located at an altitude of 2847m at the Amundsen-Scott South Pole Station collected sub-mm and Terahertz data in the 1.3mm to 200μm wavelength bands. From its location just a few hundred meters away from the geophysical South Pole, AST/RO was the first sub-mm telescope to over-winter on the polar plateau, a location uniquely suited to high quality sub-mm observations due its very low humidity, high atmospheric stability and thin troposphere (Chamberlin et al. 1997).

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Bolatto, A. D. 2001, The Interstellar Medium in Low Metallicity Environments, PhD Thesis, Boston UniversityGoogle Scholar
Bolatto, A. D., Alberto, D., Jackson, J. M., Israel, F. P., et al. 2000a, ApJ, 545, 234CrossRefGoogle Scholar
Bolatto, A. D., Jackson, J. M., Kraemer, K. E., & Zhang, X. 2000b, ApJ (Letters), 541, L17CrossRefGoogle Scholar
Chamberlin, R. A., Lane, A. P., & Stark, A. A. 1997, ApJ, 476, 428CrossRefGoogle Scholar
Groppi, C. E. 2003, Submillimeter Heterodyne Spectroscopy of Star Forming Regions, PhD Thesis, University of ArizonaGoogle Scholar
Huang, M. 2001, Interstellar Carbon Under the Influence of H ii Regions, PhD Thesis, Boston UniversityGoogle Scholar
Ingalls, J. G. 1999, Carbon Gas in High Galactic Latitude Molecular Clouds, PhD Thesis, Boston UniversityGoogle Scholar
Kim, S. and Narayanan, D. 2006, PASJ, 58, 753CrossRefGoogle Scholar
Kulesa, C.A. 2002, Molecular Hydrogen and Its Ions in Dark Interstellar Clouds and Star-Forming Regions, PhD Thesis, University of ArizonaGoogle Scholar
Lane, A. P. 1998, in: Novack, G. & Landsberg, R. H. (eds.), Astrophysics From Antarctica, ASP-CS 141, 289Google Scholar
Martin, C. L., Walsh, W. M., Xiao, K.-C., et al. 2004, ApJS, 150, 239CrossRefGoogle Scholar
Staguhn, J. 1996, Observations Towards the Sgr C Region Near the Center of our Galaxy, PhD Thesis, University of CologneGoogle Scholar
Staguhn, J., Stutzki, J., Chamberlin, R. A., et al. 1997, ApJ, 491, 191CrossRefGoogle Scholar
Stark, A. A., Bally, J., Balm, S. P., et al. 2001 PASP, 113, 567CrossRefGoogle Scholar
Stark, A. A., et al. 1997, Rev. Sci. Instr., 68, 2200CrossRefGoogle Scholar
Zhang, X., Lee, Y., Bolatto, A., and Stark, A. A. 2001, ApJ, 553, 274CrossRefGoogle Scholar