The History of Astrophysics in Antarctica
arXiv:astro-ph/0404277 · doi:10.1071/AS04037
Abstract
We examine the historical development of astrophysical science in Antarctica from the early 20th century until today. We find three temporally overlapping eras, each having a rather distinct beginning. These are the astrogeological era of meteorite discovery, the high energy era of particle detectors, and the photon astronomy era of microwave, sub--mm and infrared telescopes, sidelined by a few niche experiments at optical wavelengths. The favourable atmospheric and geophysical conditions are briefly examined, followed by an account of the major experiments and a summary of their results.
29 pages, 10 figures, 1 table Submitted to PASA in April 2004
References in corpus (4)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- High Resolution Observations of the CMB Power Spectrum with ACBAR
- The AST/RO Survey of the Galactic Center Region. I. The Inner 3 Degrees
- ACBAR: The Arcminute Cosmology Bolometer Array Receiver
Cited by in corpus (4)
- Astronomy in Antarctica
- Atmospheric scintillation at Dome C, Antarctica: implications for photometry and astrometry
- Science Programs for a 2 m-class Telescope at Dome C, Antarctica: PILOT, the Pathfinder for an International Large Optical Telescope
- Transit Search from Antarctica and Chile - Comparison and Combination