Localising the H.E.S.S. Galactic Centre point source
Abstract
Observations by the H.E.S.S. system of imaging atmospheric Cherenkov telescopes provide the most sensitive measurements of the Galactic Centre region in the energy range 150 GeV - 30 TeV. The vicinity of the kinetic centre of our galaxy harbours numerous objects which could potentially accelerate particles to very high energies (VHE, > 100 GeV) and thus produce the Gamma-ray flux observed. Within statistical and systematic errors, the centroid of the point-like emission measured by H.E.S.S. was found to be in good agreement with the position of the supermassive black hole Sgr A* and the recently discovered PWN candidate G359.95-0.04. Given a systematic pointing error of about 30'', a possible association with the SNR Sgr A East could not be ruled out with the 2004 H.E.S.S. data. In this contribution an update is given on the position of the H.E.S.S. Galactic Centre source using 2005/2006 data. The systematic pointing error is reduced to 6'' per axis using guiding telescopes for pointing corrections, making it possible to exclude with high significance Sgr A East as the source of the VHE Gamma-Rays.
Cite
@article{arxiv.0709.3729,
title = {Localising the H.E.S.S. Galactic Centre point source},
author = {C. van Eldik and O. Bolz and I. Braun and G. Hermann and J. Hinton and W. Hofmann},
journal= {arXiv preprint arXiv:0709.3729},
year = {2008}
}
Comments
4 pages, 2 figures, contribution to the 30th International Cosmic Ray Conference in Merida, Mexico, July 2007