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Far-Ultraviolet Performance of the Berkeley Spectrograph During the ORFEUS-SPAS II Mission

Mark Hurwitz·Stuart Bowyer·Robert Bristol·W. Van Dyke Dixon·Jean Dupuis·Jerry Edelstein·Patrick Jelinsky·Timothy P. Sasseen·Oswald Siegmund
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Abstract

The Berkeley spectrograph aboard the ORFEUS telescope made its second flight on the 14-day ORFEUS-SPAS II mission of the Space Shuttle Columbia in November/December 1996. Approximately half of the available observing time was dedicated to the Berkeley spectrograph, which was used by both Principal and Guest Investigators. The spectrograph's full bandpass is 390-1218 A; here we discuss its in-flight performance at far-ultraviolet (FUV) wavelengths, where most of the observations were performed. The instrument's effective area peaks at 8.9 +/- 0.5 cm^2 near 1020 A, and the mean spectral resolution is 95 km/s FWHM for point sources. Over most of the spectral range, the typical night-time background event rate in each spectral resolution element was about 0.003/s. Simultaneous background observations of an adjacent blank field were provided through a secondary, off-axis aperture. The Berkeley spectrograph's unique combination of sensitivity and resolution provided valuable observations of approximately 105 distinct astronomical targets, ranging in distance from the earth's own moon to some of the brightest AGN.

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Mark Hurwitz, Stuart Bowyer, Robert Bristol, W. Van Dyke Dixon, Jean Dupuis, Jerry Edelstein, Patrick Jelinsky, Timothy P. Sasseen, Oswald Siegmund. 1998-04-16. Far-Ultraviolet Performance of the Berkeley Spectrograph During the ORFEUS-SPAS II Mission. https://doi.org/10.1086/311388

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