The H.E.S.S. survey of the inner Galactic plane Export

@article{CR_Gamma_HESS survey, abstract = {The High Energy Stereoscopic System (H.E.S.S.), located in the Khomas Highlands of Namibia, is an array of four imaging atmospheric-Cherenkov telescopes designed to detect gamma-rays in the very high energy (VHE; \> 100 GeV) domain. Its high sensitivity and large field-of-view (5 deg) make it an ideal instrument to perform a survey within the Galactic plane for new VHE sources. Previous observations in 2004/2005 resulted in numerous detections of VHE gamma-ray emitters in the region l = 330 deg - 30 deg Galactic longitude. Recently the survey was extended, covering the regions l = 280 deg - 330 deg and l = 30 deg - 60 deg, leading to the discovery of several previously unknown sources with high statistical significance. The current status of the survey will be presented.}, archivePrefix = {arXiv}, author = {Hoppe, S. and Collaboration, H. E. S. S.}, citeulike-article-id = {3090840}, citeulike-linkout-0 = {http://arxiv.org/abs/0710.3528}, citeulike-linkout-1 = {http://arxiv.org/pdf/0710.3528}, day = {18}, eprint = {0710.3528}, keywords = {galactic, gamma-ray, hess, survey}, month = {Oct}, posted-at = {2008-08-06 15:16:41}, priority = {2}, title = {The H.E.S.S. survey of the inner Galactic plane}, url = {http://arxiv.org/abs/0710.3528}, year = {2007} }

TY - JOUR ID - CR_Gamma_HESS survey L3 - citeulike-article-id:3090840 N2 - The High Energy Stereoscopic System (H.E.S.S.), located in the Khomas Highlands of Namibia, is an array of four imaging atmospheric-Cherenkov telescopes designed to detect gamma-rays in the very high energy (VHE; > 100 GeV) domain. Its high sensitivity and large field-of-view (5 deg) make it an ideal instrument to perform a survey within the Galactic plane for new VHE sources. Previous observations in 2004/2005 resulted in numerous detections of VHE gamma-ray emitters in the region l = 330 deg - 30 deg Galactic longitude. Recently the survey was extended, covering the regions l = 280 deg - 330 deg and l = 30 deg - 60 deg, leading to the discovery of several previously unknown sources with high statistical significance. The current status of the survey will be presented. TI - The H.E.S.S. survey of the inner Galactic plane KW - galactic KW - gamma-ray KW - hess KW - survey AU - Hoppe, S AU - Collaboration, HESS PY - 2007/Oct/18/ UR - http://arxiv.org/abs/0710.3528 ER -