Paper
16 August 1988 IMAPS: A High-Resolution, Echelle Spectrograph To Record Far-Ultraviolet Spectra Of Stars From Sounding Rockets
E. B. Jenkins, C. L. Joseph, D. Long, P. M. Zucchino, G. R. Carruthers, M. Bottema, W. A. Delamere
Author Affiliations +
Abstract
We have incorporated contemporary grating and detector technologies into the design of a new sounding rocket payload which consists of a slitless, objective grating spectrograph with no transmission elements in the opti-cal train (or detector). Built several years ago, this instrument has an effective collecting area of about 4 cm2 and can record spectra of point-like sources at a wavelength resolution of 0.004Å (profile FWITM) and with a sample interval (pixel width) of 0.002Å. It is designed to give continuous coverage over the wavelength range 950 < X < 1150A, a region of immense importance to our research on the interstellar medium. The instrument, called the Interstellar Medium Absorption Profile Spectrograph (IMAPS), has flown on a Black Brant rocket and obtained a spectrum of superb quality on an early-type star, π Scorpii. Data obtained on this flight also demonstrated the excellent response of our imaging detector, which uses an electron-bombarded CCD to register individual photoevents.
© (1988) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
E. B. Jenkins, C. L. Joseph, D. Long, P. M. Zucchino, G. R. Carruthers, M. Bottema, and W. A. Delamere "IMAPS: A High-Resolution, Echelle Spectrograph To Record Far-Ultraviolet Spectra Of Stars From Sounding Rockets", Proc. SPIE 0932, Ultraviolet Technology II, (16 August 1988); https://doi.org/10.1117/12.946893
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Cited by 23 scholarly publications.
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KEYWORDS
Charge-coupled devices

Sensors

Rockets

Ions

Absorption

Ultraviolet radiation

Stars

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