Minimizing Strong Telluric Absorption in Near‐Infrared Stellar Spectra-Reference-Cited by-同舟云学术

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Minimizing Strong Telluric Absorption in Near‐Infrared Stellar Spectra

Published:2004-01 Issue:815 Volume:116 Page:97-101
ISSN:0004-6280
Container-title:Publications of the Astronomical Society of the Pacific
language:en
Short-container-title:PUBL ASTRON SOC PAC

Author:

Kenworthy Matthew A.,Hanson Margaret M.

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference13 articles.

1. The He I 2.06 micron to BR gamma ratio in 12 planetary nebulae

2. CSHELL: a high spectral resolution 1-5-μm cryogenic echelle spectrograph for the IRTF

3. A Spectral Atlas of Hot, Luminous Stars at 2 Microns

4. Lord, S. D. 1992, A New Software Tool for Computing Earth’s Atmospheric Transmission of Near- and Far-Infrared Radiation (NASA Tech. Memo. 103957; Moffett Field: Ames Research Center)

5. Infrared helium-hydrogen line ratios as a measure of stellar effective temperature

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Synthesising, using, and correcting for telluric features in high-resolution astronomical spectra;Astronomy & Astrophysics;2010-11-19

2. A Medium Resolution Near‐Infrared Spectral Atlas of O and Early‐B Stars;The Astrophysical Journal Supplement Series;2005-11

3. QuantitativeHandKband spectroscopy of Galactic OB-stars at medium resolution;Astronomy & Astrophysics;2005-08-19

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