Multiband photometric decomposition of nuclear stellar disks

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Table 2:

Photometric parameters of the nuclear stellar disks.
Galaxy	Filter	$\mu_0$	h		i	PA	L	Ref.
		[mag arcsec^-2]	['']	[pc]	[ $^\circ$ ]	[ $^\circ$ ]	[10⁶ $L_\odot$ ]
(1)	(2)	(3)	(4)		(5)	(6)	(7)	(8)
NGC 4458	F475W	$16.0^{\rm +0.3}_{-1.0}$	$0.24^{\rm +0.30}_{-0.07}$	$15^{\rm +18}_{-4 }$	$84^{\rm + 6}_{-13}$	7 $\pm 1$	$2.7^{\rm +3.3}_{-0.5}$	1
	F555W	$15.8^{\rm +0.2}_{-0.9}$	$0.24^{\rm +0.02}_{-0.04}$	$15^{\rm + 1}_{-2 }$	$82^{\rm + 8}_{-6}$	7 $\pm 1$	$3.3^{\rm +3.5}_{-0.5}$	1
	F814W	$14.3^{\rm +0.7}_{-0.7}$	$0.18^{\rm +0.99}_{-0.04}$	$11^{\rm + 6}_{-2 }$	$83^{\rm +7}_{-9 }$	7 $\pm 1$	$3.0^{\rm +3.0}_{-2.7}$	2
NGC 4478	F475W	$17.5^{\rm +1.4}_{-0.3}$	$0.55^{\rm +0.54}_{-0.34}$	$34^{\rm +32}_{-21}$	$78^{\rm +12}_{-12}$	153 $\pm 1$	$6.8^{\rm +0.9}_{-2.1}$	1
	F555W	$17.1^{\rm +1.3}_{-0.5}$	$0.63^{\rm +0.95}_{-0.25}$	$38^{\rm +58}_{-15}$	$78^{\rm +12}_{-11}$	$153\pm 1$	$10.5^{\rm +6.2}_{-3.6}$	1
	F814W	$15.8^{\rm +1.5}_{-0.8}$	$0.66^{\rm +0.54}_{-0.30}$	$40^{\rm +33}_{-19}$	$80^{\rm +10}_{-10}$	$153\pm 1$	$17.0^{\rm +5.6}_{-6.3}$	2
NGC 4570	F336W	$16.6^{\rm +0.7}_{-1.0}$	$0.31^{\rm +0.32}_{-0.04}$	$19^{\rm +20}_{-2 }$	$83^{\rm +7}_{-6}$	$158\pm 1$	$4.5^{\rm +7.9}_{-2.5}$	1
	F475W	$15.3^{\rm +0.3}_{-0.9}$	$0.27^{\rm +0.32}_{-0.07}$	$16^{\rm +20}_{-4 }$	$78^{\rm +12}_{-7}$	$158\pm 1$	$13.7^{\rm +6.9}_{-1.4}$	1
	F555W	$14.8^{\rm +0.7}_{-1.0}$	$0.32^{\rm +0.40}_{-0.05}$	$19^{\rm +25}_{-3 }$	$83^{\rm +7}_{-3}$	$158\pm 1$	$12.9^{\rm +16.0}_{-5.0}$	1
	F555W	14.8	...	23	...	...	19	3
	F814W	$13.2^{\rm +0.9}_{-0.9}$	$0.28^{\rm +0.35}_{-0.08}$	$17^{\rm +22}_{-5 }$	$81^{\rm + 9}_{- 6 }$	158 $\pm 1$	$22.4^{\rm +22.0}_{-10.0}$	1

Notes. Column (1): Galaxy name. Column (2): filter name. Column (3): disk central surface-brightness in the Vega magnitude system. Column (4): disk scale length. A distance of 12.6 Mpc was adopted for all the sample galaxies. Column (5): disk inclination. Column (6): disk position angle. Column (7): disk luminosity. Column (8): reference paper for the photometric decomposition.

References. 1 = This work, 2 = Morelli et al. (2004), 3 = Scorza & van den Bosch (1998).

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