We summarize an ongoing observational program, which combines HST imaging, VLT spectroscopy and exploits gravitational lensing of massive clusters, to identify faint lyman-α emitters (3.2 < z < 6.3).
Spectroscopic identification of high redshift lensed galaxies
MERCURIO, AMATA;
2017-01-01
Abstract
We summarize an ongoing observational program, which combines HST imaging, VLT spectroscopy and exploits gravitational lensing of massive clusters, to identify faint lyman-α emitters (3.2 < z < 6.3).File in questo prodotto:
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