The XMM-Newton optical/UV monitor telescope
K. O. MasonMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UKA. A. BreeveldMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UKR. MuchAstrophysics Division, Space Science Department of ESA, PO Box 299, 2200 AG Noordwijk, The NetherlandsM. CarterMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UKF. A. CórdovaDepartment of Physics, University of California, Santa Barbara, California 93106, USAM. CropperMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UKJ. L. A. FordhamDepartment of Physics and Astronomy, University College London, Gower Street, London, UKH. HuckleMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UKC. HoLos Alamos National Laboratory, PO Box 1663, Los Alamos, NM 87545, USAHajime KawakamiMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UKJ. A. KenneaDepartment of Physics, University of California, Santa Barbara, California 93106, USAT. KennedyMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UKJ. P. D. MittazMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UKD. PandelDepartment of Physics, University of California, Santa Barbara, California 93106, USAW. PriedhorskyLos Alamos National Laboratory, PO Box 1663, Los Alamos, NM 87545, USAT. P. SasseenDepartment of Physics, University of California, Santa Barbara, California 93106, USAR. ShireyDepartment of Physics, University of California, Santa Barbara, California 93106, USAPhil SmithMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UKJ. M. VreuxInstitut d'Astrophysique et de Géophysique, Université de Liège, 5 avenue de Cointe, 4000-Liège, Belgium
2001en
ABI
Аннотация
The XMM-OM instrument extends the spectral coverage of the XMM-Newton observatory into the ultraviolet and optical range. It provides imaging and time-resolved data on targets simultaneously with observations in the EPIC and RGS. It also has the ability to track stars in its field of view, thus providing an improved post-facto aspect solution for the spacecraft. An overview of the XMM-OM and its operation is given, together with current information on the performance of the instrument.
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