Paper
1 June 1994 Breadboard phase of the XMM optical monitor
Scott D. Horner, David H. Lumb, France Anne Cordova, Cheng Ho, William C. Priedhorsky, Joe C. Chavez, J. Klarkowski, Mark S. Cropper, Howard E. Huckle, H. Kawakami, Keith O. Mason, John L. A. Fordham, Claude A. J. Jamar, Elio Antonello, David T. Leisawitz
Author Affiliations +
Abstract
A multi-national consortium of research groups are developing the XMM (x-ray multi-mirror mission) optical monitor to provide a capability for optical identification and photometry of x-ray sources observed by the XMM observatory. This will be the first multi-wavelength facility dedicated to monitoring the variability of diverse sources from the optical through to x-ray wavelengths. Here we describe the system design and discuss progress in the breadboard phase of the development program.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Scott D. Horner, David H. Lumb, France Anne Cordova, Cheng Ho, William C. Priedhorsky, Joe C. Chavez, J. Klarkowski, Mark S. Cropper, Howard E. Huckle, H. Kawakami, Keith O. Mason, John L. A. Fordham, Claude A. J. Jamar, Elio Antonello, and David T. Leisawitz "Breadboard phase of the XMM optical monitor", Proc. SPIE 2198, Instrumentation in Astronomy VIII, (1 June 1994); https://doi.org/10.1117/12.176811
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KEYWORDS
Sensors

X-rays

Stars

X-ray optics

Space telescopes

Telescopes

Charge-coupled devices

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