A survey for Ly alpha galaxies at z~3.1
G. Ventimiglia, M. Arnaboldi, O. Gerhard

TL;DR
This paper surveys Ly alpha emission line galaxies at redshift around 3.1 using multislit imaging spectroscopy, detailing selection criteria and physical properties of the sample.
Contribution
It provides a comprehensive overview of Ly alpha galaxy detection at z~3.1 with new observational data and analysis methods.
Findings
Sample redshift distribution characterized
Flux and equivalent width distributions analyzed
Selection criteria for Ly alpha emitters established
Abstract
We describe the results of a deep survey for Ly alpha emission line galaxies at z~3.1, carried out with the multislit imaging spectroscopy (MSIS) technique, with the FORS2 spectrograph on VLT-UT1. We discuss the criteria used to select the emission line galaxies and present the main physical characteristics of the sample: redshift, observed flux and equivalent width distributions.
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Cosmology and Gravitation Theories
