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2M TELESCOPE

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ANTIPODAL TRANSIENT OBSERVATORY, HANLE

IIA and McDonell Center for the Space Sciences of Washington University, St. Louis, USA, will operate two 0.5-m f/10 Cassegrain telescopes for monitoring Active Galactic Nuclei. One of these telescopes will be located at IAO and the other in Arizona, USA. The two telescopes, 180 deg apart in longitude, would together constitute the Antipodal Transient Observatory.

The telescopes will be equipped with an optical CCD imager and be used in both robotic and remote observing modes. 70% of the telescope time will be used for continuous photometric monitoring of AGN, while the remaining time will be used for photometry of targest of opportunity and other programmes of interest.

Specifications:

TELESCOPE
Aperture 0.5 metres
Optics Ritchey-Chretien
Mount Equatorial
F-ratio f/3 primary; f/10 cassegrain
Image scale 41 arcsec/mm
FOV 7 arcmin; 60arcmin with corrector
Optical Imager
Detector 1K X 1K CCD of 24 micron pixel
Image scale 0.98 arcsec/pixel
FOV 17 X 17 arcmin
Filters Bessell UBVRI