• Created by Unknown User (jukka.h.nevalainen_2@touchstonenetwork.net), last modified on May 03, 2011 09:35

You are viewing an old version of this page. View the current version.

Compare with Current View Page History

« Previous Version 8 Next »

The tar files contain spectra, responses and background files necessary to reproduce the spectral analysis in Nevalainen et al., 2010, A&A, 523, 22.

SASv9.0 was used for processing the data. Calibration information is from December 2009.

The script files bestfit....xcm will set up the best fit. In more detail:

  • The scripts use a 1-temperature phabs x mekal model.
  • The column density is from Kalberla et al. (2005) and the absorption cross-sections are from  Balucinska-Church & McCammon (1992).
  • The scripts use the metal abundance table from Grevesse & Sauval (1998).
  • 2. and 3. term in the script file name are the inner and outer radii of the spectrum extraction annulus in arcmin.
  • *hard*, *soft* and *wide* refer to the fits done in 2.0-7.0 keV, 0.5-2.0 keV and 0.5-7.0 keV bands, respectively.

  • *fe* refers to the Fe XXV/XXVI fit in [6.45 - 7.25]/(1+z) band.



Cluster                                                                               Instrument

A1795            XMM-Newton/pn       XMM-Newton/MOS1      XMM-Newton/MOS2      Chandra/ACIS-S      Chandra/ACIS-I

A2029

A2052

A2199

A262

A3112

A3571

A85

Coma

HydraA

MKW3S

  • No labels