ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7
We report the discovery and constrain the physical conditions of the interstellar medium of the highest-redshift millimeter-selected dusty star-forming galaxy to date, SPT-S J031132-5823.4 (hereafter SPT0311-58), at z = 6.900 ± 0.002. SPT0311-58 was discovered via its 1.4 mm thermal dust continuum e...
Published in: | The Astrophysical Journal Letters |
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eScholarship, University of California
2017
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Online Access: | https://escholarship.org/uc/item/1qf5k0r7 https://escholarship.org/content/qt1qf5k0r7/qt1qf5k0r7.pdf https://doi.org/10.3847/2041-8213/aa74b0 |
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ftcdlib:oai:escholarship.org:ark:/13030/qt1qf5k0r7 2024-09-15T18:36:47+00:00 ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7 Strandet, ML Weiss, A De Breuck, C Marrone, DP Vieira, JD Aravena, M Ashby, MLN Béthermin, M Bothwell, MS Bradford, CM Carlstrom, JE Chapman, SC Cunningham, DJM Chen, Chian-Chou Fassnacht, CD Gonzalez, AH Greve, TR Gullberg, B Hayward, CC Hezaveh, Y Litke, K Ma, J Malkan, M Menten, KM Miller, T Murphy, EJ Narayanan, D Phadke, KA Rotermund, KM Spilker, JS Sreevani, J l15 2017-06-20 application/pdf https://escholarship.org/uc/item/1qf5k0r7 https://escholarship.org/content/qt1qf5k0r7/qt1qf5k0r7.pdf https://doi.org/10.3847/2041-8213/aa74b0 unknown eScholarship, University of California qt1qf5k0r7 https://escholarship.org/uc/item/1qf5k0r7 https://escholarship.org/content/qt1qf5k0r7/qt1qf5k0r7.pdf doi:10.3847/2041-8213/aa74b0 public The Astrophysical Journal Letters, vol 842, iss 2 early universe galaxies: high-redshift galaxies: star formation astro-ph.GA Astronomical and Space Sciences Astronomy & Astrophysics article 2017 ftcdlib https://doi.org/10.3847/2041-8213/aa74b0 2024-06-28T06:28:20Z We report the discovery and constrain the physical conditions of the interstellar medium of the highest-redshift millimeter-selected dusty star-forming galaxy to date, SPT-S J031132-5823.4 (hereafter SPT0311-58), at z = 6.900 ± 0.002. SPT0311-58 was discovered via its 1.4 mm thermal dust continuum emission in the South Pole Telescope (SPT)-SZ survey. The spectroscopic redshift was determined through an Atacama Large Millimeter/submillimeter Array 3 mm frequency scan that detected CO(6-5), CO(7-6), and [C I](2-1), and subsequently was confirmed by detections of CO(3-2) with the Australia Telescope Compact Array and [C II] with APEX. We constrain the properties of the ISM in SPT0311-58 with a radiative transfer analysis of the dust continuum photometry and the CO and [C I] line emission. This allows us to determine the gas content without ad hoc assumptions about gas mass scaling factors. SPT0311-58 is extremely massive, with an intrinsic gas mass of Mgas 3.3±1.9×1011 M. Its large mass and intense star formation is very rare for a source well into the epoch of reionization. Article in Journal/Newspaper South pole University of California: eScholarship The Astrophysical Journal Letters 842 2 L15 |
institution |
Open Polar |
collection |
University of California: eScholarship |
op_collection_id |
ftcdlib |
language |
unknown |
topic |
early universe galaxies: high-redshift galaxies: star formation astro-ph.GA Astronomical and Space Sciences Astronomy & Astrophysics |
spellingShingle |
early universe galaxies: high-redshift galaxies: star formation astro-ph.GA Astronomical and Space Sciences Astronomy & Astrophysics Strandet, ML Weiss, A De Breuck, C Marrone, DP Vieira, JD Aravena, M Ashby, MLN Béthermin, M Bothwell, MS Bradford, CM Carlstrom, JE Chapman, SC Cunningham, DJM Chen, Chian-Chou Fassnacht, CD Gonzalez, AH Greve, TR Gullberg, B Hayward, CC Hezaveh, Y Litke, K Ma, J Malkan, M Menten, KM Miller, T Murphy, EJ Narayanan, D Phadke, KA Rotermund, KM Spilker, JS Sreevani, J ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7 |
topic_facet |
early universe galaxies: high-redshift galaxies: star formation astro-ph.GA Astronomical and Space Sciences Astronomy & Astrophysics |
description |
We report the discovery and constrain the physical conditions of the interstellar medium of the highest-redshift millimeter-selected dusty star-forming galaxy to date, SPT-S J031132-5823.4 (hereafter SPT0311-58), at z = 6.900 ± 0.002. SPT0311-58 was discovered via its 1.4 mm thermal dust continuum emission in the South Pole Telescope (SPT)-SZ survey. The spectroscopic redshift was determined through an Atacama Large Millimeter/submillimeter Array 3 mm frequency scan that detected CO(6-5), CO(7-6), and [C I](2-1), and subsequently was confirmed by detections of CO(3-2) with the Australia Telescope Compact Array and [C II] with APEX. We constrain the properties of the ISM in SPT0311-58 with a radiative transfer analysis of the dust continuum photometry and the CO and [C I] line emission. This allows us to determine the gas content without ad hoc assumptions about gas mass scaling factors. SPT0311-58 is extremely massive, with an intrinsic gas mass of Mgas 3.3±1.9×1011 M. Its large mass and intense star formation is very rare for a source well into the epoch of reionization. |
format |
Article in Journal/Newspaper |
author |
Strandet, ML Weiss, A De Breuck, C Marrone, DP Vieira, JD Aravena, M Ashby, MLN Béthermin, M Bothwell, MS Bradford, CM Carlstrom, JE Chapman, SC Cunningham, DJM Chen, Chian-Chou Fassnacht, CD Gonzalez, AH Greve, TR Gullberg, B Hayward, CC Hezaveh, Y Litke, K Ma, J Malkan, M Menten, KM Miller, T Murphy, EJ Narayanan, D Phadke, KA Rotermund, KM Spilker, JS Sreevani, J |
author_facet |
Strandet, ML Weiss, A De Breuck, C Marrone, DP Vieira, JD Aravena, M Ashby, MLN Béthermin, M Bothwell, MS Bradford, CM Carlstrom, JE Chapman, SC Cunningham, DJM Chen, Chian-Chou Fassnacht, CD Gonzalez, AH Greve, TR Gullberg, B Hayward, CC Hezaveh, Y Litke, K Ma, J Malkan, M Menten, KM Miller, T Murphy, EJ Narayanan, D Phadke, KA Rotermund, KM Spilker, JS Sreevani, J |
author_sort |
Strandet, ML |
title |
ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7 |
title_short |
ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7 |
title_full |
ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7 |
title_fullStr |
ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7 |
title_full_unstemmed |
ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7 |
title_sort |
ism properties of a massive dusty star-forming galaxy discovered at z ∼ 7 |
publisher |
eScholarship, University of California |
publishDate |
2017 |
url |
https://escholarship.org/uc/item/1qf5k0r7 https://escholarship.org/content/qt1qf5k0r7/qt1qf5k0r7.pdf https://doi.org/10.3847/2041-8213/aa74b0 |
op_coverage |
l15 |
genre |
South pole |
genre_facet |
South pole |
op_source |
The Astrophysical Journal Letters, vol 842, iss 2 |
op_relation |
qt1qf5k0r7 https://escholarship.org/uc/item/1qf5k0r7 https://escholarship.org/content/qt1qf5k0r7/qt1qf5k0r7.pdf doi:10.3847/2041-8213/aa74b0 |
op_rights |
public |
op_doi |
https://doi.org/10.3847/2041-8213/aa74b0 |
container_title |
The Astrophysical Journal Letters |
container_volume |
842 |
container_issue |
2 |
container_start_page |
L15 |
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1810480497656070144 |