During its first observation cycle, between April 2005 and March 2006, the MAGIC telescope was able to observe nine different GRB events since their early beginning. Other observations have been performed during the following months in its second observation cycle. The observations, with an energy threshold spanning from 80 to 200 GeV, did not

From January until April 2008 the MAGIC Telescope has been monitoring the radio galaxy M87 during several nights. A significant and variable signal has been detected. Following an agreement between the HESS/MAGIC/VERITAS Cherenkov Telescopes, additional observations have been triggered. We will give a short overview of the results from the campaign

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High altitude scientific balloons have been used for many years to provide scientists with access to near space at a fraction of the cost of satellite based or sounding rocket experiments. In recent years, these balloons have been successfully used for long duration missions of up to 40 days. Longer missions, with durations of up to 100 days (Ultra

During Cycle 14 a total of 113 HST orbits were secured to observe five isolated dwarf galaxies, namely Tucana, LGS3, LeoA, IC1613, and Cetus. The aim of the project is a full characterization of the stellar content of these galaxies, in terms of their SFH, radial distributions, halo populations and variable stars. Deep (V≈29) F475W, F814W data

The color-magnitude diagram (CMD) is the most powerful tool to derive quantitative star formation histories (SFHs) of complex stellar systems which host populations with different ages and chemical compositions. We present some results from the LCID project, based on the analysis of deep HST/ACS CMDs reaching the oldest Main Sequence (MS) Turn Off