Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15..536k&link_type=abstract
Highlights of Astronomy, Volume 15, p. 536-536
Astronomy and Astrophysics
Astronomy
Scientific paper
The advantages of a high altitude, dry site for ground-based astronomy at infrared (IR) wavelengths are well-known: the lower temperature and pressure associated with increased altitude reduce the emissivities of both atmosphere and telescope, and a lower atmospheric absorption improves the transmission of IR radiation. The next generation of IR instruments under development (for ELTs) will open up a new discovery space, particularly in high-resolution (HR) spectroscopy, which will not have a space-based counterpart and has proven to be a powerful tool for studying all stages of stellar evolution (e.g. (e.g. Jaffle et al., 2003). I present here a summary of quantitative work into transmission-dependent aspects of HR IR spectroscopy at high and low altitudes.
No associations
LandOfFree
SpS1-High-resolution infrared spectroscopy at high and low altitudes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with SpS1-High-resolution infrared spectroscopy at high and low altitudes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SpS1-High-resolution infrared spectroscopy at high and low altitudes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1485557