Stellar populations of CL 0048-2942 (Serote+, 2005)

Physics

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Clusters: Galaxy, Redshifts, Equivalent Widths

Scientific paper

CL 0048-2942 was identified in optical images of the ESO Imaging Survey (Nonino et al., 1999A&AS..137...51N) by running a matched-filter detection algorithm (Lobo et al., 2000A&A...360..896L) on the I-band of that data set.
Images of the cluster field (each one covering square arcmin) were obtained through the B, V, R and I Bessel-Cousins filters at the La Silla ESO 3.6m telescope with the EFOSC2 camera. Standard data reduction was performed with IRAF.
Multi-object spectroscopy was performed during two runs at the VLT: a first campaign of two nights in September 1999 with the MOS unit of FORS1 (VLT UT1) provided partial coverage of selected objects in the cluster candidate field; further data were gathered during the second campaign, this time in service mode during the first semester of 2000, with the MOS unit of FORS2 (VLT UT2).
(4 data files).

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