Astronomy & Astrophysics

All Tables

Table 1: Power law, $Y=Y_0\;X^{\gamma}$ , parameterized X-ray scaling relations. The mean of the scatter is determined by a Gaussian model fit to the histogram of the scatter.
Table 2: Power law, $Y=Y_0\;X^{\gamma}$ , parameterized mass-observable scaling relations using weak lensing masses ( $M_{500}^{\rm wl}$ ) for the 19 LoCuSS clusters having weak lensing masses.
Table 3: See the caption in Table 2 except that the weak lensing masses, X-ray masses and $Y_{{\rm X}}$ parameters are determined within the radii ( $r_{500}^{Y_{\rm X},X}$ ) determined by the method described in Sect. 4.
Table 4: See the caption in Table 2 except that the weak lensing masses, X-ray masses and $Y_{{\rm X}}$ parameters are determined within the radii ( $r_{500}^{Y_{\rm X},{\rm wl}}$ ) determined by the method described in Sect. 6.2.3.
Table 5: See the caption in Table 2 except that the weak lensing masses, X-ray masses and $Y_{{\rm X}}$ parameters are determined within the radii ( $r_{500}^{Y_{\rm X},{\rm si}}$ ) determined by the method described in Sect. 6.2.4.
Table A.1:
Table A.2: Primary parameters. Column (1): cluster name; Col. (2): optical redshift (e.g. Böhringer et al. 2004; Smith et al. 2005; Bardeau et al. 2007); Col. (3): hydrogen column density (Dickey & Lockman 1990); Col. (4): truncation radius corresponding to a S/N of 3 of the observational surface brightness profile; Col. (5): volume averaged radial temperature profile of 0.2-0.5r₅₀₀; Cols. (6, 7): spectroscopic temperature and metallicity in the annulus of 0.2-0.5r₅₀₀; Cols. (8-10): bolometric luminosity including the < 0.2r₅₀₀ region, excluding the < 0.2r₅₀₀ region, and corrected for the < 0.2r₅₀₀ region, respectively.
Table B.1: Deduced properties of 37 LoCuSS galaxy clusters. Column (1): cluster name; Col. (2): electron number density of the inner most radial bin; Col. (3): entropy at 0.2 r₅₀₀; Col. (4): inner most radial bin of the surface brightness profile; Col. (5): cooling time measured at $r_{\rm cen}$ ; Col. (6): cooling radius; Col. (7): r₅₀₀; Cols. (8-10): gas mass, total mass and gas mass fraction at r₅₀₀, Col. (11): cluster morphology using the cluster classification in Jones & Forman (1992), 0 denotes ``single'', 1 denotes ``primary with small secondary'', 2 denotes ``elliptical'', 3 denotes ``off-center'' and 4 denotes ``complex''.
Table B.2: Power law, $Y=Y_0\;X^{\gamma}$ , parameterized entropy-temperature, entropy- $Y_{{\rm X}}$ and pressure- $Y_{{\rm X}}$ relations.
Table C.1: Deduced properties of 37 LoCuSS galaxy clusters at the radii ( $r^{Y_{\rm X},{\rm X}}_{500}$ ) determined by the method described in Sect. 4. Column (1): cluster name; Col. (2): $r^{Y_{\rm X},{\rm X}}_{500}$ ; Cols. (3): X-ray mass at $r^{Y_{\rm X},{\rm X}}_{500}$ ; Cols. (4, 5): weak lensing masses at $r^{Y_{\rm X},{\rm X}}_{500}$ for the D06 and B07 clusters.
Table C.2: Deduced properties of 37 LoCuSS galaxy clusters at the radii ( $r^{Y_{\rm X},{\rm wl}}_{500}$ ) determined by the method described in Sect. 6.2.3. Column (1): cluster name; Col. (2): $r^{Y_{\rm X},{\rm wl}}_{500}$ ; Col. (3): X-ray mass at $r^{Y_{\rm X},{\rm wl}}_{500}$ ; Cols. (4, 5): weak lensing masses at $r^{Y_{\rm X},{\rm wl}}_{500}$ for the D06 and B07 clusters.
Table C.3: Deduced properties of 37 LoCuSS galaxy clusters at the radii ( $r^{Y_{\rm X},{\rm si}}_{500}$ ) determined by the method described in Sect. 6.2.4. Column (1): cluster name; Col. (2): $r^{Y_{\rm X},{\rm si}}_{500}$ ; Col. (3): X-ray mass at $r^{Y_{\rm X},{\rm si}}_{500}$ ; Cols. (4, 5): weak lensing masses at $r^{Y_{\rm X},{\rm si}}_{500}$ for the D06 and B07 clusters.