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Max-Planck-Institut für extraterrestrische Physik

- High-Energy Astrophysics -

Project:   OPTIMA

 

  MPEMPE   group High-Energy Astrophysics   group Projects   project OPTIMA

Project OPTIMA


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OPTIMA

OPTIMA
OPTIMA mounted at the Skinakas telescope
OPTIMA (Optical Pulsar TIMing Analyzer) is a high-speed photoncounter which is used to measure (gamma-ray) interesting objects, especially pulsars with high time resolution (10-6 s) and high sensitivity.

Meanwhile it is used to observe also other rapid variable objects from observatories world wide.

A detailed description is available in Kanbach und Straubmeier (2002) and more recently in Kanbach et al. (2008).

New developments include the possibility to measure with high time resolution also the polarisation of objects (OPTIMA photo-polarimeter (Kellner (2002), Kanbach et al. (2003)) and spectral colors in several bands simultaneously.

A special version - OPTIMA-burst - was used in 2006 and 2007 during 3-month campaigns at the Skinakas observatory (Crete, Greece) to observe Gamma Ray Bursts immediately after detection by the Swift satellite.
Again in 2008, 2009, and 2010 this instrument was installed at Skinakas observatory for campaigns of 2 months duration. Again, in June/July 2011 an Observing campaign will take place there (see "news").


Valid HTML 4.01! Last update: 2011-06-08 by   linkH. Steinle
Contact person:   linkG. Kanbach and linkArne Rau
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