Paper
1 July 1990 Optical monitor for x-ray satellites
Elio Antonello, Oberto Citterio, Francesco Mazzoleni, Andrea Mariani, Paolo Pili, Pasquale Lombardi
Author Affiliations +
Abstract
The Optical Monitor is a part of the JET-X experiment which will fly on board the Soviet satellite Spectrum-X-Gamma. The reflector is a Ritchey-Chretien with an aperture of 260 mm, and there are two frame transfer CCD detectors. The scientific objectives of the Optical Monitor are observations in the optical and UV bands simultaneously with X-ray, the real time identification of X-ray sources with mv less than or equal to 22 and detection of their variability, the improvement of the post-facto spacecraft attitude reconstruction for the X-ray observations, and the serendipitous mode search for microvariability of the bright stars to develop the research field of asteroseismology. Since long integration times are required for the faint object detection, a dedicated servo loop operating on the secondary mirror is developed for the stabilization of the images against the drift of the satellite.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Elio Antonello, Oberto Citterio, Francesco Mazzoleni, Andrea Mariani, Paolo Pili, and Pasquale Lombardi "Optical monitor for x-ray satellites", Proc. SPIE 1235, Instrumentation in Astronomy VII, (1 July 1990); https://doi.org/10.1117/12.19151
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Stars

Mirrors

Sensors

Geometrical optics

Cameras

Astronomy

Satellites

RELATED CONTENT


Back to Top