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 5:

Linear transformation between indices measured by us and in LICK systems.
Index	Linear relation	rms	Lick/HET
	(Lick= $a\times~$ HET+b)
$H\beta$	1.091( $\pm$ 0.096)-0.327( $\pm$ 0.134)	0.085	0.780 $\pm$ 0.117
Mg_b	1.137( $\pm$ 0.025)-0.549( $\pm$ 0.129)	0.073	0.967 $\pm$ 0.0245
Fe5015	0.892( $\pm$ 0.105)+0.980( $\pm$ 0.663)	0.147	1.052 $\pm$ 0.0276
Fe5270	0.879( $\pm$ 0.135)+0.499( $\pm$ 0.471)	0.143	1.037 $\pm$ 0.0291
Fe5335	0.903( $\pm$ 0.085)+0.255( $\pm$ 0.321)	0.117	0.990 $\pm$ 0.0249
Fe5406	0.974( $\pm$ 0.127)+0.171( $\pm$ 0.265)	0.142	1.066 $\pm$ 0.0373

Notes. The second column displays the best linear relations, and the last column show the ratio of LICK systems to our measurements.

Source LaTeX | All tables | In the text

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