Table 1: Observations of NGC 5253. Exp. time is the total exposure time (for composite images). FWHM is the Full Width Half Maximum of a point source.
Filter Instrument Mean wav. (Å) Bandpass (Å) Exp. time (s) FWHM

F547M WFPC2 @ HST 5484.0 483.1 1600 $0\hbox{$.\!\!^{\prime\prime}$ }17$

F656N WFPC2 @ HST 6564.0 21.4 3600 $0\hbox{$.\!\!^{\prime\prime}$ }17$

F673N WFPC2 @ HST 6732.2 21.4 2400 $0\hbox{$.\!\!^{\prime\prime}$ }17$

F814W WFPC2 @ HST 7921.0 1488.8 1160 $0\hbox{$.\!\!^{\prime\prime}$ }15$

Ks ISAAC @ VLT 21 600 2700 300 $0\hbox{$.\!\!^{\prime\prime}$ }40$

**Table 1:** Observations of NGC 5253. *Exp. time* is the total exposure time (for composite images). *FWHM* is the Full Width Half Maximum of a point source.
Filter	Instrument	Mean wav. (Å)	Bandpass (Å)	Exp. time (s)	FWHM
F547M	WFPC2 @ HST	5484.0	483.1	1600	$0\hbox{$.\!\!^{\prime\prime}$ }17$
F656N	WFPC2 @ HST	6564.0	21.4	3600	$0\hbox{$.\!\!^{\prime\prime}$ }17$
F673N	WFPC2 @ HST	6732.2	21.4	2400	$0\hbox{$.\!\!^{\prime\prime}$ }17$
F814W	WFPC2 @ HST	7921.0	1488.8	1160	$0\hbox{$.\!\!^{\prime\prime}$ }15$
Ks	ISAAC @ VLT	21 600	2700	300	$0\hbox{$.\!\!^{\prime\prime}$ }40$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 Photometry of the clusters and the color-color diagram
	4 Analysis and discussion
	5 Summary and conclusions
	References