Plasma diagnostics of a giant stellar flare Carolin Liefke 1 Birgit Fuhrmeister 1 Ansgar Reiners 1,2 Jürgen H.M.M. Schmitt 1 1 Hamburger Sternwarte, 2.
Magnetic dissipation in Poynting dominated outflows Yuri Lyubarsky Ben-Gurion University.
The Physical Properties of Red Supergiants Emily Levesque IfA, University of Hawaii/SAO, Harvard Hot Massive Stars: A Lifetime of Influence Lowell Observatory.
Relations between concurrent hard X-ray sources in solar flares M. Battaglia and A. O. Benz Presented by Jeongwoo Lee NJIT/CSTR Journal Club 2007 October.
1 An Introduction to X-ray Spectral Fitting I: Getting started with XSPEC Other material XSPEC manual:
Bkg modeling for hot medium z Clusters Bkg modeling for hot medium z Clusters Alberto Leccardi Silvano Molendi.
CUC Oct 2014 CXC Jonathan McDowell. I will report on CIAO (user software) and the standard processing pipeline software, which come into being thanks.
Plasma diagnostics of a giant stellar flare
An XMM-Newton View of the Luminous X-ray Source Population of M101 Leigh Jenkins Tim Roberts, Robert Warwick, Roy Kilgard*, Martin Ward University of Leicester,
Bkg modeling for hot medium z Clusters
A Novel Technique for the Determination of IMF at Low Masses: A Few Results for Galaxies with Old Stellar Populations Nikolay Podorvanyuk 1 Igor Chilingarian.
Rutherford Appleton Laboratory Remote Sensing Group Tropospheric ozone retrieval from uv/vis spectrometery RAL Space - Remote Sensing Group Richard Siddans,
