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The original ROTSE-I had 4 telephoto lenses of 11 cm aperture, covering a 16x16 degree field of view. This detected the first afterglow of a GRB while the burst was still ongoing, but this was the only burst detected by ROTSE or the very similar
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and SWIFT could provide smaller error boxes, making a huge field of view unnecessary. This led to the design of ROTSE-III, a more or less conventional telescope designed for fast slewing and operation at multiple locations around the world.
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Akerlof, C.W. and Ashley, MCB and
Casperson, DE and Epps, HW and Kehoe, RL and Marshall, SL and McGowan, KE and McKay, TA and Phillips, MA and Rykoff, E.S.; et al. (2002). "The ROTSE-III robotic telescope system".
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This article about a specific observatory, telescope or astronomical instrument is a
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The ROTSE project is a collaboration of astrophysicists from the
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144:. Retrieved
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