Vth School of Astroparticle Physics
23 - 28 May 2016
OHP, Saint Michel l'Observatoire

Physics of the Universe in X-rays

Introduction and spectroscopy

Jean Ballet
 
IRFU CEA

Course
In the first part of the tutorial, I will present the procedure of X-ray data reduction. I will show the steps to follow from the download of the data set to the generation of the X-ray spectrum, for the case study of an XMM-Newton observation of an X-ray binary. I will point out the concepts and tools applied to X-ray astronomical data in general.  I will invite the participants to run some of the commands on their own in this workshop.
The second part of the tutorial will deal with the spectral analysis of an X-ray spectrum. I will invite the participants to perform a spectral analysis of the XMM-Newton spectrum generated during the data reduction session. I will guide them through the analysis using the standard X-ray fitting package XSPEC, with the objective to estimate the column density towards the target, the source flux and luminosity in the X-ray band, the type of physical process producing the X-ray continuum and the lines if present, and the properties of the plasma that may be inferred from the spectrum.

Outline
  1. X-ray data reduction: from the archives to the spectrum
  2. Spectral analysis of an X-ray spectrum

Jean Ballet is a staff astrophysicist at CEA in Saclay. He works on supernova remnants (thermal and non-thermal emission) and data analysis in general at high energies (X-rays and gamma-rays). He is responsible for the EPIC/MOS software on XMM-Newton, and for the catalog of sources of the Fermi/LAT instrument in gamma-rays.

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