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The top documents tagged [variable sources]
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variable sources
Voeventnet.caltech.edu VOEventNet By Matthew J. Graham (Caltech)
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Astronomical Wide-field Imaging System for Europe MPE/USM Survey/GTO Projects Mark Neeser MPE / ESO Mark Neeser MPE / ESO Leiden Workshop Nov. 2005.
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EBFM Presentation
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A Novel 2stage
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ATNF Science Priorities: 2010 – 2015 Ball, Braun, Edwards, Feain, Hobbs, Johnston, McClure-Griffiths.
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1. 2 OUTLINE OVERVIEWOVERVIEW MAIN MISSION OBJECTIVESMAIN MISSION OBJECTIVES INSTRUMENTSINSTRUMENTS 1.LAT 2.GBM AGILE-EGRET-GLAST COMPARISIONAGILE-EGRET-GLAST.
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Wide field X (& UV ?) Identify transients, distribute alerts Candidate X (&UV)-transients SN breakouts XRF ’ s LL GRBs Unknown (eg BH-Stellar disruptions)?
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Became pressing issue when 1XMM catalogue showed a distinct excess of weak sources in MOS 2 emevents 7.10 marks flickering pixels and event clusters in.
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1 15.08.2015 22:56 EasyPreparation without Barcode Reader.
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Without barcode reader 20.08.2015 22:33. without barcode reader 20.08.2015 22:33 2. Select „Easy preparation“. Click OK. 1. Start PrepGilsonST program.
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Milliarcsecond Morphology of Scintillating & Non-scintillating Sources
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Observation of X-ray binaries with Skylark and Ariel 5 - some hits and some misses Ken Pounds University of Leicester.
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