A Window On The Earliest Star Formation: Extreme Photoionization Conditions of a High-Ionization, Low-Metallicity Lensed Galaxy at z~2
Danielle A. Berg, Dawn K. Erb, Matthew W. Auger, Max Pettini, and, Gabriel B. Brammer

TL;DR
This study presents detailed observations of a high-redshift, low-metallicity galaxy with extreme star-forming conditions, revealing strong UV emission lines and minimal outflows, serving as a local universe template for early galaxy formation.
Contribution
It provides new spectroscopic data on a highly magnified, low-metallicity galaxy at z~2, highlighting extreme ionization conditions and challenging existing stellar population models.
Findings
Strong nebular UV emission lines detected
Double-peaked LyA emission observed
Minimal outflows along the sightline
Abstract
We report new observations of SL2SJ021737-051329, a lens system consisting of a bright arc at z=1.84435, magnified ~17x by a massive galaxy at z=0.65. SL2SJ0217 is a low-mass (M <10^9 M*), low-metallicity (Z~1/20 Z*) galaxy, with extreme star-forming conditions that produce strong nebular UV emission lines in the absence of any apparent outflows. Here we present several notable features from rest-frame UV Keck/LRIS spectroscopy: (1) Very strong narrow emission lines are measured for CIV 1548,1550, HeII 1640, OIII] 1661,1666, SiIII] 1883,1892, and CIII] 1907,1909. (2) Double-peaked LyA emission is observed with a dominant blue peak and centered near the systemic velocity. (3) The low- and high-ionization absorption features indicate very little or no outflowing gas along the sightline to the lensed galaxy. The relative emission line strengths can be reproduced with a very…
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