The impetus given to ground based Gamma ray Astronomy by the outstanding success of the CGRO mission has been very significant. Simultaneously, improvements in flux sensitivity of the Imaging Atmospheric Cerenkov Technique (IACT) and the practical realization of stereoscopic imaging using multiple telescopes has led to the establishment of a number of statistically compelling point sources of VHE (0.1 to 10 TeV) Gamma rays. Most of the discoveries have been independently confirmed by at least two groups. The current observational status of AGNs, pulsars, supernova remnants and the search for TeV counterparts of bursts will be summarised.
In the UHE energy range from 10 TeV to 1 PeV, searches for point sources are made using arrays of scintillation counters, wide angle Atmospheric Cerenkov detectors and large scale water Cerenkov counters. To date, no point sources have been identified and the limits set by the CASA air shower array will soon reach values predicted for the diffuse gamma ray background. Preliminary claims for evidence of photon emission from a number of close AGNs in the energy range from 30 to 100 TeV will be discussed.