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20 April 2024
 
  » arxiv » 1803.1839

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Detection of [O III] at z~3: A Galaxy above the Main Sequence, Rapidly Assembling its Stellar Mass
Amit Vishwas ; Carl Ferkinhoff ; Thomas Nikola ; Stephen C. Parshley ; Justin P. Schoenwald ; Gordon J. Stacey ; Sarah J.U. Higdon ; James L. Higdon ; Axel Weiß ; Rolf Güsten ; Karl M. Menten ;
Date 5 Mar 2018
AbstractWe detect bright emission in the far infrared fine structure [O III] 88$mu$m line from a strong lensing candidate galaxy, H-ATLAS J113526.3-014605, hereafter G12v2.43, at z=3.127, using the $ m 2^{nd}$ generation Redshift (z) and Early Universe Spectrometer (ZEUS-2) at the Atacama Pathfinder Experiment Telescope (APEX). This is only the fifth detection of this far-IR line from a sub-millimeter galaxy at the epoch of galaxy assembly. The observed [O III] luminosity of $7.1 imes10^{9}, m(frac{10}{mu}), m{L_{odot}},$ likely arises from HII regions around massive stars, and the amount of Lyman continuum photons required to support the ionization indicate the presence of $(1.2-5.2) imes10^{6}, m(frac{10}{mu})$ equivalent O5.5 or higher stars; where $mu$ would be the lensing magnification factor. The observed line luminosity also requires a minimum mass of $sim 2 imes 10^{8}, m(frac{10}{mu}), m{M_{odot}},$ in ionized gas, that is $0.33\%$ of the estimated total molecular gas mass of $6 imes10^{10}, m(frac{10}{mu}), m{M_{odot}},$. We compile multi-band photometry tracing rest-frame UV to millimeter continuum emission to further constrain the properties of this dusty high redshift star-forming galaxy. Via SED modeling we find G12v2.43 is forming stars at a rate of 916 $ m(frac{10}{mu}), m{M_{odot}}, m{yr^{-1}}$ and already has a stellar mass of $8 imes 10^{10}, m(frac{10}{mu}), m{M_{odot}},$. We also constrain the age of the current starburst to be $leqslant$ 5 million years, making G12v2.43 a gas rich galaxy lying above the star-forming main sequence at z$sim$3, undergoing a growth spurt and, could be on the main sequence within the derived gas depletion timescale of $sim$66 million years.
Source arXiv, 1803.1839
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