Full auto optical afterglow searching system: MIKOTS

Details Full auto optical afterglow searching system: MIKOTS Full auto optical afterglow searching system: MIKOTS

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ncimc..28..763t&link_type=abstract

Il Nuovo Cimento C, vol. 28, Issue 4, p.763

Physics

Scientific paper

Recently, to observe afterglow at various places has appeared necessary. To do so, we have set a fully automated afterglow searching system named MIKOTS. The aperture of our telescope, with a CCD camera, is 300 mm and the focal length is about 1000 mm. The CCD has 512×512 pixels size corresponding to a chip size of 10.2 mm ×10.2 mm. The field of view, resolution and lower limit magnitude are 37′.0×37′.0, and 18.1, respectively. This system can start observation less than 15 seconds after receiving the data from GCN.

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