A technique for ultra-high resolution, high signal-to-noise spectroscopy in the far ultraviolet

Details A technique for ultra-high resolution, high signal-to-noise spectroscopy in the far ultraviolet A technique for ultra-high resolution, high signal-to-noise spectroscopy in the far ultraviolet

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...196.4001g&link_type=abstract

American Astronomical Society, 196th AAS Meeting, #40.01; Bulletin of the American Astronomical Society, Vol. 32, p.737

Physics

Optics

Scientific paper

Ultra-high resolution (R > 500,000) spectroscopy with high signal-to-noise (S/N > 50/1) can be achieved in the far ultraviolet with existing optics and detectors when combined in the appropraite manner. I present a design to achieve spectroscopy at this level for use in detailed studies of the morphology and physical conditions of the interstellar medium.

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