Resolved Spectroscopy of a z = 5 Gravitationally Lensed Galaxy with the VIMOS IFU

Details Resolved Spectroscopy of a z = 5 Gravitationally Lensed Galaxy with the VIMOS IFU Resolved Spectroscopy of a z = 5 Gravitationally Lensed Galaxy with the VIMOS IFU

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005msngr.121...33s&link_type=abstract

The Messenger (ISSN0722-6691), No.121, p. 33-37 (September 2005)

Physics

Scientific paper

We have used the VIMOS IFU to spatially resolve and study the star-forming, galactic superwinds and metal-enrichment properties in a highly magnified gravitationally lensed galaxy at z = 5 (i.e., seen when the Universe was only ~ 10 % of its current age). These results are allowing us to study galaxy formation and evolution in a level of detail never before possible and provide exciting possibilities for future studies of galaxies at these early times.

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