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Ch'ing-Sung Yu
On the continuous hydrogen absorption in spectra of class A starsLick Observatory Bulletins, 375
H. Dekker, S. D’odorico, A. Kaufer, B. Delabre, H. Kotzlowski (2000)
Design, construction, and performance of UVES, the echelle spectrograph for the UT2 Kueyen Telescope at the ESO Paranal Observatory, 4008
L. Epstein (1967)
ALL-REFLECTING SCHMIDT CAMERAPublications of the Astronomical Society of the Pacific, 79
G. Lemaitre, L. Vigroux (1988)
All-Reflective Aspherized Grating Spectrographs at the Prime Focus of the CFHT
I. Naĭdenov, V. Panchuk, M. Yushkin (2007)
Stokes polarimeter with an image slicerAstrophysical Bulletin, 62
D. Walker, F. Diego (1985)
Design philosophy of the forthcoming échelle spectrographs for the AAT and LPOMonthly Notices of the Royal Astronomical Society, 217
H. Jensen (1933)
Über die Temperaturskalen der FixsterneAstronomische Nachrichten, 248
L. Robinson (1988)
Instrumentation for Ground-Based Optical Astronomy
James Owens (1967)
Optical refractive index of air: dependence on pressure, temperature and composition.Applied optics, 6 1
K. Noguchi, W. Aoki, S. Kawanomoto, H. Ando, S. Honda, H. Izumiura, E. Kambe, K. Okita, K. Sadakane, B. Sato, A. Tajitsu, M. Takada-Hidai, W. Tanaka, E. Watanabe, Michitoshi Yoshida (2002)
High Dispersion Spectrograph (HDS) for the Subaru TelescopePublications of the Astronomical Society of Japan, 54
S. Vogt (1987)
THE LICK OBSERVATORY HAMILTON ECHELLE SPECTROMETER.Publications of the Astronomical Society of the Pacific, 99
J. London, D. Bojkov, S. Oltmans, I. Kelley (1976)
Atlas of the global distribution of total ozone, July 1957 - June 1967
R. Hudson (1974)
Absorption cross sections of stratospheric moleculesCanadian Journal of Chemistry, 52
B. Karpov (1934)
A study of hydrogen emission in stars of class B0-B5Lick Observatory Bulletins, 16
B. Lasker (1966)
A LIQUID-FILTER CELL FOR TELESCOPE USEPublications of the Astronomical Society of the Pacific, 78
A. Filippenko (1982)
THE IMPORTANCE OF ATMOSPHERIC DIFFERENTIAL REFRACTION IN SPECTROPHOTOMETRY.Publications of the Astronomical Society of the Pacific, 94
L. Robinson, D. Latham (1988)
Instrumentation for ground-based optical astronomy. Present and future. The Ninth Santa Cruz Summer Workshop in Astronomy and Astrophysics,held at the Lick Observatory, Santa Cruz, CA, USA, 13 - 24 July 1987.
We present a historical note on the main spectroscopy instruments close to the short-wave boundary of the optical atmospheric window. Ground-based ultraviolet observations imposemore stringent requirements to the optics of telescopes and spectrographs, as well as to the calibration means. We have to bear in mind the seasonal variations of the optical properties of the Earth’s atmosphere. We consider the capabilities of ultraviolet observations with high spectral resolution on the 6-m BTA telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences.
Astrophysical Bulletin – Springer Journals
Published: Dec 18, 2009
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