Abstract
Our spectroscopic observations were spread across 5 nights in October
and November 2004 for Cl 0412, 7 nights in December 2005 and February
2005 for MS 1008, 5 nights between May and July 2005 for MS 2137.
For photometric data, we use both VLT/FORS2 and HST/ACS images. We
obtained imaging of the MS 1008, MS 2137 and Cl 0412 samples in the
ACS/F606W filter while we exploited existing imaging of MS 0451 in the
ACS/F814W filter from the ST-ECF HST archive. Ground based images were
taken in the B, V, R and I filters for the whole sample. The FORS2
filters B, V and I are close approximations to the Johnson-Cousins
photometric system while the R filter is a special filter for FORS2 that
is similar to the Cousins R .
(5 data files).
Original language | English |
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Journal | VizieR Online Data Catalog |
Volume | 352 |
Publication status | Published - Feb-2012 |
Keywords
- Clusters: galaxy
- Redshifts
- Photometry: UBVRI
- Morphology