Nguyen, H. T. et al., 1996, Publications of the Astronomical Society of the Pacific, 108, 718 | View on ADS (1996PASP..108..718N) | Access via DOI
We report our finding that the South Pole is the darkest known Earth-based site for near infrared astronomical observations. For this reason it has great potentail for the most sensitive surveys of distant or faint objects. We find that the south polar sky background is substantially darker in the standard near infrared J, H, and K filters, and in an optimized K_DARK filter centered at 2.36 microns. In particular, the K_DARK background at the South Pole is only 162 +/- 67 mu-Jy arcsec^-2 at the zenith. This is consistent with the results described in an accompanying paper by Ashley et al. 1996, and is comparable to the sky brightness measured by high altitude balloon in the 2.4 micron (Matsumoto et al. 1994). (SECTION: Atmospheric Phenomena and Seeing)
This publication has been tagged as:
Characteristics/Sky brightness & stability
Hemisphere/Antarctic
Site/South Pole
Type/In-situ or ground-based observations
Wavelength/Infrared
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