Gamma-Ray Burst Optical/Near-Infrared Detector

"A photograph of the GROND instrument"
The GROND instrument mounted on the 2.2m telescope at the La Silla Observatory (lower left corner, blue cylinder).

The Gamma-Ray Burst Optical/Near-Infrared Detector (GROND) is an imaging instrument used to investigate Gamma-Ray Burst afterglows and do follow-up observations on transiting exoplanets. It is operated at the MPG 2.2m telescope at the La Silla Observatory.[1][2][3]

Discoveries

See also

Notes

    References

    1. http://www.mpe.mpg.de/~saglia/journals_pdf/snellen2009.pdf
    2. http://www.aanda.org/articles/aa/full_html/2012/03/aa18336-11/aa18336-11.html
    3. "GROND Takes Off" (Press release). European Organisation for Astronomical Research in the Southern Hemisphere (ESO). 2007-07-06. Retrieved 2009-02-23.
    4. "NASA's Swift Catches Farthest Ever Gamma-Ray Burst" (Press release). NASA. 2008-09-19. Retrieved 2009-02-23.
    5. Greiner, Jochen et al. (2008-10-13). "GRB 080913 at redshift 6.7". arXiv:0810.2314.
    6. "NASA's Fermi Telescope Sees Most Extreme Gamma-ray Blast Yet" (Press release). NASA. 2009-02-19. Retrieved 2009-02-23.
    7. Greiner, Jochen et al. (2009-02-04). "The redshift and afterglow of the extremely energetic gamma-ray burst GRB 080916C". arXiv:0902.0761.

    External links