Ultraviolet Spectrography

Ultraviolet Spectrography is a spectroscopic method that measures the intensity of ultraviolet radiation as a function of wavelength to analyze the physical and chemical properties of astronomical sources, specifically distinguishing itself by its sensitivity to electronic transitions in hot stars, interstellar medium, and energetic astrophysical phenomena inaccessible at longer wavelengths.

97

Publications

4.6K

Citations

385

Authors

162

Institutions

Publications per year

2017–2026

8

Authors

385

  1. MS
    Mikhail Sachkov

    Institute of Astronomy, Russia

    4 publications · 145 citations

    4

    h-index

  2. MC
    M. C. Festou

    Observatoire Midi-Pyrénées, France

    4 publications · 438 citations

    4

    h-index

  3. WE
    W. E. McClintock

    Laboratory for Atmospheric and Space Physics, United States

    3 publications · 501 citations

    3

    h-index

  4. GM
    G. M. Lawrence

    Laboratory for Atmospheric and Space Physics, United States

    3 publications · 344 citations

    3

    h-index

  5. EW
    Erik Wilkinson

    University of Colorado Boulder, United States

    3 publications · 34 citations

    3

    h-index

1–5 of 385

Venues

  1. Applied Optics

    10 publications · 285 citations

    10

    h-index

  2. Review of Scientific Instruments

    7 publications · 175 citations

    7

    h-index

  3. The Astrophysical Journal

    ApJ · 6 publications · 405 citations

    6

    h-index

  4. 6

    h-index

  5. Journal of the Optical Society of America

    JOSA · 5 publications · 171 citations

    5

    h-index

1–5