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• W2123690899 startingPage "140" @default.
• W2123690899 abstract "We present Hubble Space Telescope (HST) WFC3 imaging and grism spectroscopy observations of the {it Herschel}-selected gravitationally-lensed starburst galaxy HATLASJ1429-0028. The lensing system consists of an edge-on foreground disk galaxy at $z=0.218$ with a nearly complete Einstein ring of the infrared luminous galaxy at $z=1.027$. The WFC3 spectroscopy with G102 and G141 grisms, covering the wavelength range of 0.8 to 1.7 $mu$m, resulted in detections of H$alpha$+[NII], H$beta$, [SII], and [OIII] for the background galaxy from which we measure line fluxes and ratios. The Balmer line ratio H$alpha$/H$beta$ of $7.5 pm 4.4$, when corrected for [NII], results in an extinction for the starburst galaxy of $E(B-V)=0.8 pm 0.5$. The $Halpha$ based star-formation rate, when corrected for extinction, is $60 pm 50$ M$_{odot}$ yr$^{-1}$, lower than the instantaneous star-formation rate of 390 $pm$ 90 M$_{odot}$ yr$^{-1}$ from the total IR luminosity. We also compare the nebular line ratios of HATLASJ1429-0028 with other star-forming and sub-mm bright galaxies. The nebular line ratios are consistent with an intrinsic ultra-luminous infrared galaxy with no evidence for excitation by an active galactic nucleus (AGN). We estimate the metallicity, $12 + log(O/H)$, of HATLASJ1429-0028 to be 8.49 $pm$ 0.16. Such a low value is below the average relations for stellar mass vs. metallicity of galaxies at $z sim 1$ for a galaxy with stellar mass of $sim 2 times 10^{11}$ M$_{odot}$. The combination of high stellar mass, lack of AGN indicators, low metallicity, and the high star-formation rate of HATLASJ1429-0028 suggest that this galaxy is currently undergoing a rapid formation." @default.
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• W2123690899 date "2015-05-28" @default.
• W2123690899 modified "2023-09-26" @default.
• W2123690899 title "EXTINCTION AND NEBULAR LINE PROPERTIES OF AHERSCHEL-SELECTED LENSED DUSTY STARBURST ATz= 1.027" @default.
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• W2123690899 doi "https://doi.org/10.1088/0004-637x/805/2/140" @default.
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