MAGIC observations of the HMXB LS I <textbox>+61textbox> 303 in VHE gamma rays

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• 作者：T. Jogler ; V. Bosch-Ramon ; J. Cortina ; J.M. Paredes ; M.A. Perez-Torres ; M. Rib&#xf3 ; J. Rico ; N. Sidro ; D.F. Torres
• 关键词：LSI ; l13">tyle="text-decoration ; none ; color ; black" href="/science?_ob=MathURL&_method=retrieve&_udi=B6TJM-4RKMHV1-7&_mathId=mml13&_user=1067359&_cdi=5314&_rdoc=14&_acct=C000050221&_version=1&_userid=10&md5=a69cf697fd42bea86331ee179e3b1a
• 刊名：Nuclear Instruments and Methods in Physics Research Section A ; Accelerators ; Spectrometers ; Detectors and Associated Equipment
• 出版年：2008
• 期刊代码：41_01689002
• 类别：ph
• 出版时间：1 April 2008
• 卷：588
• 期：1-2
• 页码：33-36
• 文件大小：399 K

摘要

The MAGIC collaboration discovered with their 17 m diameter imaging atmospheric Cherenkov telescope, the High Mass X-ray Binary (HMXB) LS I l8">tyle="text-decoration:none; color:black" href="/science?_ob=MathURL&_method=retrieve&_udi=B6TJM-4RKMHV1-7&_mathId=mml8&_user=1067359&_cdi=5314&_rdoc=14&_acct=C000050221&_version=1&_userid=10&md5=49a7091aa3c0dc884fa931a140f73759" title="Click to view the MathML source" alt="Click to view the MathML source">+61 303 at VHE l9">lass="inlMMLBox">thURL&_method=retrieve&_udi=B6TJM-4RKMHV1-7&_mathId=mml9&_user=1067359&_cdi=5314&_rdoc=14&_acct=C000050221&_version=1&_userid=10&md5=9a3675dff3b73f33f6358f3d83618a38">ttp://www.sciencedirect.com/cache/MiamiImageURL/B6TJM-4RKMHV1-7-2R/0?wchp=dGLbVtz-zSkzS" alt="View the MathML source" title="View the MathML source" align="absbottom" border="0" height=16 width="138"/> l10">tyle="text-decoration:none; color:black" href="/science?_ob=MathURL&_method=retrieve&_udi=B6TJM-4RKMHV1-7&_mathId=mml10&_user=1067359&_cdi=5314&_rdoc=14&_acct=C000050221&_version=1&_userid=10&md5=ef3d947caf993df2bdb3ea97e394c320" title="Click to view the MathML source" alt="Click to view the MathML source">γ-rays. The emission from LS I l11">tyle="text-decoration:none; color:black" href="/science?_ob=MathURL&_method=retrieve&_udi=B6TJM-4RKMHV1-7&_mathId=mml11&_user=1067359&_cdi=5314&_rdoc=14&_acct=C000050221&_version=1&_userid=10&md5=b5a6c2dc261a770152a1d05477658a7a" title="Click to view the MathML source" alt="Click to view the MathML source">+61 303 was found to be variable, and the source was visible at energies above 200 GeV in different runs during some orbital phases only. These orbital phases do not coincide with the periastron passage. Here we report the results of the analysis of the LS I l12">tyle="text-decoration:none; color:black" href="/science?_ob=MathURL&_method=retrieve&_udi=B6TJM-4RKMHV1-7&_mathId=mml12&_user=1067359&_cdi=5314&_rdoc=14&_acct=C000050221&_version=1&_userid=10&md5=c38789537e6d8b741b3898554008c1ec" title="Click to view the MathML source" alt="Click to view the MathML source">+61 303 MAGIC observations.