Optical Follow-Up Observations of GRBs at the Klet' Observatory

Details Optical Follow-Up Observations of GRBs at the Klet' Observatory Optical Follow-Up Observations of GRBs at the Klet' Observatory

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..662..363p&link_type=abstract

GAMMA-RAY BURST AND AFTERGLOW ASTRONOMY 2001: A Workshop Celebrating the First Year of the HETE Mission. AIP Conference Proceed

Astronomy and Astrophysics

Astronomy

Gamma-Ray Sources, Gamma-Ray Bursts, X- And Gamma-Ray Telescopes And Instrumentation, Charge-Coupled Devices, Image Detectors, And Ir Detector Arrays

Scientific paper

The 57 cm telescope of the Klet' Observatory has been used for follow-up observations of selected GRBs. Limiting magnitudes as deep as mag 22 have been obtained. The results obtained are presented and discussed. We also address the capabilities of the current system for GRB analyses as well as further improvements including the newly developed 1.06 m aperture CCD telescope.

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