Glossary of abbreviations used in data files. For further information, please contact me.
Ponman, Sanderson & Finoguenov, 2003, MNRAS, 343, 331
- Links to paper: [ADS] [astro-ph]
- The self-similar relations for figs 5 & 6 are:
S(0.1*R200) = 46.2 * kT
S_500 = 220 * kT - The best-fit line for the fig 4 (0.1*R200 vs. kT) data is:
S(0.1*R200) = 119.4 * kT^0.65
- Click here for a table of unbinned cluster data (excluding the 2 galaxies)
- Click here for fig.5 binned data
- Click here for fig.6 binned data
- Click here for fig.7 binned data
- Click here for fig.8 binned data
Sanderson et al., 2003, MNRAS, 340, 989
- Links to paper: [ADS] [astro-ph]
- Click here for a table of data (includes total mass, gas fraction & emission-weighted mean temperature within r500)
- Click here for a table of the cluster model parameters
Sanderson, Ponman & O’Sullivan, 2006, MNRAS, 372, 1496
- Links to paper: [ADS] [astro-ph]
- Data for Table 1 and Table 2
- Mean deprojected temperature profile and error envelope from Fig.7 for cool core and non-cool core clusters
Sanderson, O'Sullivan & Ponman, 2009, MNRAS, 395, 764
- Links to paper: [ADS] [arXiv]
- Data for Table 2
- Binned metallicity profile data from Figure 10, for cool core and non-cool core clusters
- *NEW Jan 2011* smoothed entropy profile data, used in figures 3 & 7
- Colour and/or larger font postscript/pdf versions of selected figures, suitable for presentations, here: Figures 2, 3, 4, 5, 6, 10, 11, 12, 13