This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy.

THE SOUTH POLE NEAR INFRARED SKY BRIGHTNESS

, , , , , , , and

© 1996. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A.
, , Citation H. T. Nguyen et al 1996 PASP 108 718 DOI 10.1086/133791

1538-3873/108/726/718

ABSTRACT

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 KDARK filter centered at 2.36 microns. In particular, the KDARK 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).

Export citation and abstract BibTeX RIS

10.1086/133791