Radially extended kinematics and stellar populations of the massive ellipticals NGC 1600, NGC 4125, and NGC 7619 - Constraints on the outer dark halo density profile

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Table 1:

List of the morphological classifications, B band luminosity, luminosity distance, receding velocity and effective radius of NGC 1600, NGC 4125 and NGC 7619.
Name	R_a	Dec	Type	$\log(L_B$ / $L_\odot$ )	Dis	Vel(km s^-1)	$R_{\rm e}$ ( arcsec)
NGC 1600	04 $^{\rm h}$ 31 $^{\rm m}$ 39 $^{\rm s}$	-05 ${\rm d}$ 11 $^{\rm m}$ 10 $^{\rm s}$	E3	11.03	64 Mpc	4681	45
NGC 4125	12 $^{\rm h}$ 08 $^{\rm m}$ 06 $^{\rm s}$	65 $^{\rm d}$ 10 $^{\rm m}$ 26 $^{\rm s}$	E6	10.80	20 Mpc	1356	58
NGC 7619	23 $^{\rm h}$ 20 $^{\rm m}$ 14 $^{\rm s}$	8 $^{\rm d}$ 12 $^{\rm m}$ 22 $^{\rm s}$	E2	10.58	46 Mpc	3760	32

Notes. Taken from O'Sullivan et al. (2001); Faber et al. (1989) and NED (NASA/IPAC Extragalactic Database).

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