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Multi-wavelength lens reconstruction of a Planck and Herschel-detected star-bursting galaxy
File | Description | Size | Format | |
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Timmons_2016_ApJ_829_21.pdf | Published version | 10 MB | Adobe PDF | View/Open |
Title: | Multi-wavelength lens reconstruction of a Planck and Herschel-detected star-bursting galaxy |
Authors: | Timmons, N Cooray, A Riechers, DA Nayyeri, H Fu, H Jullo, E Gladders, MD Baes, M Bussmann, RS Calanog, J Clements, DL Da Cunha, E Dye, S Eales, SA Furlanetto, C Gonzalez-Nuevo, J Greenslade, J Gurwell, M Messias, H Michalowski, MJ Oteo, I Perez-Fournon, I Scott, D Valiante, E |
Item Type: | Journal Article |
Abstract: | We present a source-plane reconstruction of a Herschel and Planck-detected gravitationally lensed dusty star-forming galaxy (DSFG) at z = 1.68 using Hubble, Submillimeter Array (SMA), and Keck observations. The background submillimeter galaxy (SMG) is strongly lensed by a foreground galaxy cluster at z = 0.997 and appears as an arc with a length of ~15'' in the optical images. The continuum dust emission, as seen by SMA, is limited to a single knot within this arc. We present a lens model with source-plane reconstructions at several wavelengths to show the difference in magnification between the stars and dust, and highlight the importance of multi-wavelength lens models for studies involving lensed DSFGs. We estimate the physical properties of the galaxy by fitting the flux densities to model spectral energy distributions leading to a magnification-corrected star-formation rate (SFR) of 390 ± 60 M ${}_{\odot }$ yr−1 and a stellar mass of $1.1\pm 0.4\times {10}^{11}$ ${M}_{\odot }$. These values are consistent with high-redshift massive galaxies that have formed most of their stars already. The estimated gas-to-baryon fraction, molecular gas surface density, and SFR surface density have values of 0.43 ± 0.13, 350 ± 200 ${M}_{\odot }$ pc−2, and $\sim 12\pm 7\,$ M ${}_{\odot }$ yr−1 kpc−2, respectively. The ratio of SFR surface density to molecular gas surface density puts this among the most star-forming systems, similar to other measured SMGs and local ULIRGs. |
Issue Date: | 16-Sep-2016 |
Date of Acceptance: | 15-Jul-2016 |
URI: | http://hdl.handle.net/10044/1/42854 |
DOI: | http://dx.doi.org/10.3847/0004-637X/829/1/21 |
ISSN: | 1538-4357 |
Publisher: | American Astronomical Society |
Journal / Book Title: | Astrophysical Journal |
Volume: | 829 |
Issue: | 1 |
Copyright Statement: | © 2016 The American Astronomical Society. All rights reserved. |
Sponsor/Funder: | Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) |
Funder's Grant Number: | SPIRE/SOW/07020F ST/F01239X/1 ST/F012373/1 ST/H001239/1 ST/G001901/1 ST/G003874/1 ST/J004812/1 ST/J001368/1 ST/K006401/1 ST/K004131/1 ST/M003558/1 ST/P000568/1 |
Keywords: | Science & Technology Physical Sciences Astronomy & Astrophysics cosmology: observations galaxies: evolution infrared: galaxies submillimeter: galaxies DEEP-FIELD-SOUTH LUMINOUS SUBMILLIMETER GALAXIES SEQUENCE CLUSTER SURVEY MOLECULAR GAS FORMING GALAXIES HIGH-REDSHIFT INFRARED-EMISSION MASSIVE GALAXIES FORMATION RATES STELLAR MASSES 0201 Astronomical And Space Sciences 0305 Organic Chemistry 0306 Physical Chemistry (Incl. Structural) |
Publication Status: | Published |
Open Access location: | https://arxiv.org/pdf/1512.03059 |
Article Number: | ARTN 21 |
Appears in Collections: | Physics Astrophysics |