Galaxy evolution in Local Group analogs - I. A GALEX study of nearby groups dominated by late-type galaxies

A. Marino; L. Bianchi; R. Rampazzo; L. M. Buson; D. Bettoni

doi:10.1051/0004-6361/200913216

Home

All issues

Volume 511 (February 2010)

A&A, 511 (2010) A29

Full HTML

Free Access

Table 4:

SDSS photometry of LGG 225 members.
Galaxy	u	g	r	i	z
	[AB mag]	[AB mag]	[AB mag]	[AB mag]	[AB mag]
NGC 3370	13.31 $\pm$ 0.06	12.31 $\pm$ 0.02	11.85 $\pm$ 0.03	11.59 $\pm$ 0.03	11.38 $\pm$ 0.06
NGC 3443^b	15.91 $\pm$ 0.14	14.79 $\pm$ 0.05	14.33 $\pm$ 0.05	14.11 $\pm$ 0.06	13.90 $\pm$ 0.18
NGC 3447^b	14.47 $\pm$ 0.12	13.22 $\pm$ 0.04	12.90 $\pm$ 0.05	12.78 $\pm$ 0.06	12.06 $\pm$ 0.10
NGC 3447A	15.34 $\pm$ 0.16	14.89 $\pm$ 0.09	14.71 $\pm$ 0.13	14.65 $\pm$ 0.19	14.32 $\pm$ 0.44
NGC 3454	15.08 $\pm$ 0.12	13.84 $\pm$ 0.03	13.23 $\pm$ 0.03	12.91 $\pm$ 0.04	12.66 $\pm$ 0.09
NGC 3455	13.98 $\pm$ 0.09	13.02 $\pm$ 0.03	12.66 $\pm$ 0.04	12.50 $\pm$ 0.05	12.31 $\pm$ 0.12
NGC 3457	14.69 $\pm$ 0.06	13.05 $\pm$ 0.02	12.37 $\pm$ 0.02	12.01 $\pm$ 0.02	11.77 $\pm$ 0.04
NGC 3501	14.41 $\pm$ 0.07	13.06 $\pm$ 0.02	12.40 $\pm$ 0.02	11.99 $\pm$ 0.03	11.68 $\pm$ 0.05
NGC 3507^a,b	12.16 $\pm$ 0.02	10.75 $\pm$ 0.02	10.18 $\pm$ 0.02	9.78 $\pm$ 0.02	9.62 $\pm$ 0.03
NGC 3522	15.16 $\pm$ 0.11	13.59 $\pm$ 0.03	12.88 $\pm$ 0.02	12.52 $\pm$ 0.03	12.37 $\pm$ 0.06
UGC 6022	16.94 $\pm$ 0.35	15.84 $\pm$ 0.11	15.52 $\pm$ 0.14	15.38 $\pm$ 0.19	15.07 $\pm$ 0.51
UGC 6035^a	13.77 $\pm$ 0.11	12.90 $\pm$ 0.04	12.21 $\pm$ 0.06	11.75 $\pm$ 0.05	10.92 $\pm$ 0.13
UGC 6083	16.31 $\pm$ 0.17	15.17 $\pm$ 0.05	14.71 $\pm$ 0.06	14.43 $\pm$ 0.07	14.35 $\pm$ 0.23
UGC 6112^b	15.22 $\pm$ 0.14	14.29 $\pm$ 0.05	13.94 $\pm$ 0.06	13.76 $\pm$ 0.08	13.75 $\pm$ 0.31
UGC 6171^a	15.50 $\pm$ 0.15	13.41 $\pm$ 0.05	13.03 $\pm$ 0.06	12.79 $\pm$ 0.06	12.69 $\pm$ 0.14

Notes. ^(a) Magnitude of the foreground stars have been subtracted; ^(b) Galaxy is near SDSS edge, magnitudes have been computed in a reduced area (elliptical aperture with $a=0.5\hbox{$^\prime$ }$ , $b=0.3\hbox{$^\prime$ }$ for NGC 3443, with $a=1.6\hbox{$^\prime$ }$ , $b=0.8\hbox{$^\prime$ }$ for NGC 3447, with $a=1\hbox{$^\prime$ }$ , $b=0.4\hbox{$^\prime$ }$ for UGC 6112 and aperture of radius 0.9 $^\prime$ for NGC 3507 respectively, and scaled to the total area using the UV ratio to derive their mass.

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.