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- W3100838581 abstract "We 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 $rm 2^{nd}$ 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 $7.1times10^{9},rm(frac{10}{mu}),rm{L_{odot}},$ likely arises from HII regions around massive stars, and the amount of Lyman continuum photons required to support the ionization indicate the presence of $(1.2-5.2)times10^{6},rm(frac{10}{mu})$ equivalent O5.5 or higher stars; where $mu$ would be the lensing magnification factor. The observed line luminosity also requires a minimum mass of $sim 2times 10^{8},rm(frac{10}{mu}),rm{M_{odot}},$ in ionized gas, that is $0.33%$ of the estimated total molecular gas mass of $6times10^{10},rm(frac{10}{mu}),rm{M_{odot}},$. 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 $rm(frac{10}{mu}),rm{M_{odot}},rm{yr^{-1}}$ and already has a stellar mass of $8times 10^{10},rm(frac{10}{mu}),rm{M_{odot}},$. 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." @default.
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- W3100838581 date "2018-04-05" @default.
- W3100838581 modified "2023-09-27" @default.
- W3100838581 title "Detection of [O iii] at<i>z</i>∼ 3: A Galaxy Above the Main Sequence, Rapidly Assembling Its Stellar Mass" @default.
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- W3100838581 doi "https://doi.org/10.3847/1538-4357/aab354" @default.
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