ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7

M. L. Strandet; A. Weiss; C. De Breuck; D. P. Marrone; J. D. Vieira; M. Aravena; M. L.N. Ashby; M. Béthermin; M. S. Bothwell; C. M. Bradford; J. E. Carlstrom; S. C. Chapman; D. J.M. Cunningham; Chian Chou Chen; C. D. Fassnacht; A. H. Gonzalez; T. R. Greve; B. Gullberg; C. C. Hayward; Y. Hezaveh; K. Litke; J. Ma; M. Malkan; K. M. Menten; T. Miller; E. J. Murphy; D. Narayanan; K. A. Phadke; K. M. Rotermund; J. S. Spilker; J. Sreevani

doi:10.3847/2041-8213/aa74b0

ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7

M. L. Strandet
, A. Weiss
, C. De Breuck
, D. P. Marrone
, J. D. Vieira
, M. Aravena
, M. L.N. Ashby
, M. Béthermin
, M. S. Bothwell
, C. M. Bradford
, J. E. Carlstrom
, S. C. Chapman
, D. J.M. Cunningham
, Chian Chou Chen
, C. D. Fassnacht
, A. H. Gonzalez
, T. R. Greve
, B. Gullberg
, C. C. Hayward
, Y. Hezaveh

K. Litke, J. Ma, M. Malkan, K. M. Menten, T. Miller, E. J. Murphy, D. Narayanan, K. A. Phadke, K. M. Rotermund, J. S. Spilker, J. Sreevani

Astronomy

Research output: Contribution to journal › Article › peer-review

125 Scopus citations

Abstract

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 M_gas 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.

Original language	English (US)
Article number	L15
Journal	Astrophysical Journal Letters
Volume	842
Issue number	2
DOIs	https://doi.org/10.3847/2041-8213/aa74b0
State	Published - Jun 20 2017

Keywords

Early universe
Galaxies: high-redshift
Galaxies: star formation

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.3847/2041-8213/aa74b0

Cite this

Strandet, M. L., Weiss, A., Breuck, C. D., Marrone, D. P., Vieira, J. D., Aravena, M., Ashby, M. L. N., Béthermin, M., Bothwell, M. S., Bradford, C. M., Carlstrom, J. E., Chapman, S. C., Cunningham, D. J. M., Chen, C. C., Fassnacht, C. D., Gonzalez, A. H., Greve, T. R., Gullberg, B., Hayward, C. C., ... Sreevani, J. (2017). ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7. Astrophysical Journal Letters, 842(2), Article L15. https://doi.org/10.3847/2041-8213/aa74b0

Strandet, ML, Weiss, A, Breuck, CD, Marrone, DP, Vieira, JD, Aravena, M, Ashby, MLN, Béthermin, M, Bothwell, MS, Bradford, CM, Carlstrom, JE, Chapman, SC, Cunningham, DJM, Chen, CC, 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 2017, 'ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7', Astrophysical Journal Letters, vol. 842, no. 2, L15. https://doi.org/10.3847/2041-8213/aa74b0

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title = "ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7",

abstract = "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.",

keywords = "Early universe, Galaxies: high-redshift, Galaxies: star formation",

author = "Strandet, \{M. L.\} and A. Weiss and Breuck, \{C. De\} and Marrone, \{D. P.\} and Vieira, \{J. D.\} and M. Aravena and Ashby, \{M. L.N.\} and M. B{\'e}thermin and Bothwell, \{M. S.\} and Bradford, \{C. M.\} and Carlstrom, \{J. E.\} and Chapman, \{S. C.\} and Cunningham, \{D. J.M.\} and Chen, \{Chian Chou\} and Fassnacht, \{C. D.\} and Gonzalez, \{A. H.\} and Greve, \{T. R.\} and B. Gullberg and Hayward, \{C. C.\} and Y. Hezaveh and K. Litke and J. Ma and M. Malkan and Menten, \{K. M.\} and T. Miller and Murphy, \{E. J.\} and D. Narayanan and Phadke, \{K. A.\} and Rotermund, \{K. M.\} and Spilker, \{J. S.\} and J. Sreevani",

year = "2017",

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day = "20",

doi = "10.3847/2041-8213/aa74b0",

language = "English (US)",

volume = "842",

journal = "Astrophysical Journal Letters",

issn = "2041-8205",

publisher = "American Astronomical Society",

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TY - JOUR

T1 - ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7

AU - Strandet, M. L.

AU - Weiss, A.

AU - Breuck, C. De

AU - Marrone, D. P.

AU - Vieira, J. D.

AU - Aravena, M.

AU - Ashby, M. L.N.

AU - Béthermin, M.

AU - Bothwell, M. S.

AU - Bradford, C. M.

AU - Carlstrom, J. E.

AU - Chapman, S. C.

AU - Cunningham, D. J.M.

AU - Chen, Chian Chou

AU - Fassnacht, C. D.

AU - Gonzalez, A. H.

AU - Greve, T. R.

AU - Gullberg, B.

AU - Hayward, C. C.

AU - Hezaveh, Y.

AU - Litke, K.

AU - Ma, J.

AU - Malkan, M.

AU - Menten, K. M.

AU - Miller, T.

AU - Murphy, E. J.

AU - Narayanan, D.

AU - Phadke, K. A.

AU - Rotermund, K. M.

AU - Spilker, J. S.

AU - Sreevani, J.

PY - 2017/6/20

Y1 - 2017/6/20

N2 - 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.

AB - 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.

KW - Early universe

KW - Galaxies: high-redshift

KW - Galaxies: star formation

UR - https://www.scopus.com/pages/publications/85021238982

UR - https://www.scopus.com/pages/publications/85021238982#tab=citedBy

U2 - 10.3847/2041-8213/aa74b0

DO - 10.3847/2041-8213/aa74b0

M3 - Article

AN - SCOPUS:85021238982

SN - 2041-8205

VL - 842

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 2

M1 - L15

ER -

ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7

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