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Table 2.

Best-fit results.

NFW SIS Sérsic n = 4 Burkert
log10(Mr200) C log10(Mr200) log10e) θe (arcsec) ρ0(10−2M pc−3) rc (kpc)
Galaxies npix = 2000 σ = 0.3 12.6 8.0 12.0 12.0 1.0 11.5 10
npix = 400 σ = 2.4 12.5 8.5 11.4 11.6 1.6 2.1 40

QSOs npix = 2000 σ = 0.3 12.4 8.9 12.0 12.0 2.1 5.5 20
npix = 400 σ = 2.4 12.1 10.0 11.7 11.9 5.2 0.8 100

Clusters Wen catalogue npix = 2000 σ = 0.3 12.5 8.0 12.0 12.8 1.0 6.7 15
npix = 400 σ = 2.4 12.4 8.5 11.7 12.0 3.3 1.0 60

Clusters Zou catalogue npix = 2000 σ = 0.3 13.0 5.4 12.0 11.9 3.3 5.0 20
npix = 400 σ = 2.4 12.9 5.4 12.0 11.9 3.3 0.8 80

Notes. From left to right: sample name, pixel number and smoothing, σ (in arcsec), parameter values for the NFW, SIS (both masses in M), and Sérsic (Σe in M Mpc−2) and Burkert best fits. The uncertainty associated with each value is represented by the decimal place.

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