Ultraviolet Astronomy: Astrophysical Perspectives of the Spektr-UF Project (WSO-UV)

Astrophysics ◽  
2021 ◽  
Author(s):  
B. M. Shustov
Keyword(s):  
Ultraviolet Astronomy

Ultraviolet Astronomy Beyond 2020

2009 ◽  
Author(s):  
Marc Postman ◽  
Matt Mountain ◽  
Michael E. Van Steenberg ◽  
George Sonneborn ◽  
H. Warren Moos ◽  
...  
Keyword(s):  
Ultraviolet Astronomy

The Space Telescope for Ultraviolet Astronomy WSO–UV

2010 ◽  
pp. 219-225 ◽  
Author(s):  
Ana I. Gómez de Castro ◽  
B. Shustov ◽  
M. Sachkov ◽  
N. Kappelmann ◽  
M. Huang ◽  
...  
Keyword(s):  
Ultraviolet Astronomy ◽  
Space Telescope

Ultraviolet Astronomy

2021 ◽  
pp. 117-143
Author(s):  
John Etienne Beckman
Keyword(s):  
Ultraviolet Astronomy

scholarly journals Extreme and Far Ultraviolet Astronomy from Voyagers 1 and 2

1990 ◽  
Vol 123 ◽  
pp. 49-57
Author(s):  
J.B. Holberg
Keyword(s):  
Photon Counting ◽  
Large Field ◽  
Data Sets ◽  
Diffuse Emission ◽  
Ultraviolet Astronomy ◽  
Wide Range ◽  
Valuable Complement ◽  
Scientific Results ◽  
Stellar Sources ◽  
Far Ultraviolet

AbstractThe instrumental characteristics, observational capabilities and scientific results of the Voyager 1 and 2 ultraviolet spectrometers are reviewed. These instruments provide current and ongoing access to low resolution spectra for a wide variety of astronomical sources in the 500 to 1700 Å band. Observations of the brightest OB stars and hot subluminous stars as faint as V = 15 mag. are possible. In the EUV, at wavelengths shortward of 900 Å, several new sources have been detected and a host of potential sources ruled out. In the Far UV, particularly at wavelengths between 900 and 1200 Å, Voyager is capable of observing a wide range of stellar and non-stellar sources. Such observations can often provide a valuable complement to IUE and other data sets at longer wavelengths. The Voyager spectrometers have proved remarkably stable photon counting instruments, capable of extremely long integration times. The long integration times, relatively large field of view, and location in the outer solar system also provide an ideal platform for observations of sources of faint diffuse emission, such as nebulae and the general sky background.

Digital micromirror array enabled integral field spectroscopy for far-ultraviolet astronomy

2018 ◽  
Author(s):  
Amanda R. Hendrix ◽  
Brian T. Fleming ◽  
Eric Schindhelm ◽  
Rachel M. Tyler ◽  
Emily M. Witt ◽  
...  
Keyword(s):  
Ultraviolet Astronomy ◽  
Integral Field Spectroscopy ◽  
Field Spectroscopy ◽  
Far Ultraviolet ◽  
Integral Field ◽  
Micromirror Array

Extreme Ultraviolet Astronomy

2000 ◽  
Vol 38 (1) ◽  
pp. 231-288 ◽  
Author(s):  
Stuart Bowyer ◽  
Jeremy J. Drake ◽  
Stéphane Vennes
Keyword(s):  
Extreme Ultraviolet ◽  
Ultraviolet Astronomy

Technologies and science archives for ultraviolet astronomy

2014 ◽  
Vol 354 (1) ◽  
pp. 125-141
Author(s):  
Noah Brosch ◽  
Martin Barstow ◽  
Jose Chirivella
Keyword(s):  
Ultraviolet Astronomy

Normal Incidence Multilayer Mirrors For Extreme Ultraviolet Astronomy

1984 ◽  
Author(s):  
Robert A. Stern ◽  
Bernhard M. Haisch ◽  
George Joki ◽  
Richard C. Catura
Keyword(s):  
Extreme Ultraviolet ◽  
Normal Incidence ◽  
Multilayer Mirrors ◽  
Ultraviolet Astronomy
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