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タイトルThe Swift Mission and the REM Telescope
著者(英)Mason, K. O.; Barthelemy, S. D.; Hurley, K. C.; Gehrels, N.; Giommi, P.; White, N. E.; Nousek, J. A.; Chincarini, G.; Wells, A. A.; Burrow, D. N.
著者所属(英)NASA Goddard Space Flight Center
発行日2003-01-01
言語eng
内容記述Following a description of the science drive which originated the Swift Mission, this is US NASA MIDEX Mission with the collaboration of Italy and the UK, we will describe the status of the hardware and the observing strategy. The telemetry is carried out via the TDRSS satellite for those communications that need immediate response. The data transfer and the scheduled uploading of routine commands will be done through the ASI Malindi station in Kenia. Both in the US and in Europe a large effort will be done to follow the bursts with the maximum of efficiency and as soon as possible after the alert. We will describe how the ESO VLT telescopes are able to respond to the alert. To address the problematic of the dark bursts and to immediately follow up all of the bursts also in the Near Infrared we designed and built a 60 cm NIR Robotic telescope, REM, to be located on the ESO ground at Cerro La Silla. The instrumentation includes also a low dispersion spectrograph with the capability of multi wavelength optical photometry.
NASA分類Spacecraft Design, Testing and Performance
権利Copyright, Distribution within the U.S. granted by agreement


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