Abstract
FIREBall (the Faint Intergalactic Redshifted Emission Balloon) is a balloon-borne 1m telescope coupled to an ultraviolet fiber-fed spectrograph. FIREBall is designed to study the faint and diffuse emission of the warm hot intergalactic medium, until now detected primarily in absorption. FIREBall is a pathfinding mission to test new technology and make new constraints on the temperature and density of this gas. FIREBall has flown twice, the most recent flight (June 2009) a fully functioning science flight. Here we describe the spectrograph design, current setup, and calibration measurements from the campaign. © 2010 SPIE.
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CITATION STYLE
Tuttle, S. E., Schiminovich, D., Grange, R., Rahman, S., Matuszewski, M., Milliard, B., … Martin, D. C. (2010). FIREBALL: the first ultraviolet fiber fed spectrograph. In Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray (Vol. 7732, p. 773227). SPIE. https://doi.org/10.1117/12.857877
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