ISM properties of a Massive Dusty Star-Forming Galaxy discovered at z \textasciitilde 7. Strandet, M. L., Weiß, A., De Breuck, C., 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., Fassnacht, C. D., Gonzalez, A. H., Greve, T. R., Gullberg, B., Hayward, C. C., Hezaveh, Y., Litke, K., Ma, J., Malkan, M., Menten, K. M., Miller, T., Murphy, E. J., Narayanan, D., Phadke, K. A., Rotermund, K. M., Spilker, J. S., & Sreevani, J. ArXiv e-prints, 1705:arXiv:1705.07912, May, 2017. ![ISM properties of a Massive Dusty Star-Forming Galaxy discovered at z \textasciitilde 7 [link]](https://bibbase.org/img/filetypes/link.svg "link")
Paper abstract bibtex We report the discovery and constrain the physical conditions of the interstellar medium of the highest-redshift millimeter-selected dusty star-forming galaxy (DSFG) to date, SPT-S J031132-5823.4 (hereafter SPT0311-58), at \$z=6.900 +/- 0.002\$. SPT0311-58 was discovered via its 1.4mm thermal dust continuum emission in the South Pole Telescope (SPT)-SZ survey. The spectroscopic redshift was determined through an ALMA 3mm frequency scan that detected CO(6-5), CO(7-6) and [CI](2-1), and subsequently confirmed by detections of CO(3-2) with ATCA and [CII] 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 [CI] 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_\{{\textbackslash}rm gas\} = 3.3 {\textbackslash}pm 1.9 {\textbackslash}times10{\textasciicircum}\{11\}{\textbackslash},M_\{{\textbackslash}odot\}\$. Its large mass and intense star formation is very rare for a source well into the Epoch of Reionization.
@article{strandet_ism_2017,
title = {{ISM} properties of a {Massive} {Dusty} {Star}-{Forming} {Galaxy} discovered at z {\textasciitilde} 7},
volume = {1705},
url = {http://adsabs.harvard.edu/abs/2017arXiv170507912S},
abstract = {We report the discovery and constrain the physical conditions of the interstellar medium of the highest-redshift millimeter-selected dusty star-forming galaxy (DSFG) to date, SPT-S J031132-5823.4 (hereafter SPT0311-58), at \$z=6.900 +/- 0.002\$. SPT0311-58 was discovered via its 1.4mm thermal dust continuum emission in the South Pole Telescope (SPT)-SZ survey. The spectroscopic redshift was determined through an ALMA 3mm frequency scan that detected CO(6-5), CO(7-6) and [CI](2-1), and subsequently confirmed by detections of CO(3-2) with ATCA and [CII] 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 [CI] 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\_\{{\textbackslash}rm gas\} = 3.3 {\textbackslash}pm 1.9 {\textbackslash}times10{\textasciicircum}\{11\}{\textbackslash},M\_\{{\textbackslash}odot\}\$. Its large mass and intense star formation is very rare for a source well into the Epoch of Reionization.},
urldate = {2017-05-30},
journal = {ArXiv e-prints},
author = {Strandet, M. L. and Weiß, A. and De Breuck, C. and Marrone, D. P. and Vieira, J. D. and Aravena, M. and Ashby, M. L. N. and Béthermin, M. 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 Gullberg, B. and Hayward, C. C. and Hezaveh, Y. and Litke, K. and Ma, J. and Malkan, M. and Menten, K. M. and Miller, T. and Murphy, E. J. and Narayanan, D. and Phadke, K. A. and Rotermund, K. M. and Spilker, J. S. and Sreevani, J.},
month = may,
year = {2017},
keywords = {Astrophysics - Astrophysics of Galaxies},
pages = {arXiv:1705.07912},
}
Downloads: 0
{"_id":"RGmSCmGqjoppd47Kc","bibbaseid":"strandet-wei-debreuck-marrone-vieira-aravena-ashby-bthermin-etal-ismpropertiesofamassivedustystarforminggalaxydiscoveredatztextasciitilde7-2017","author_short":["Strandet, M. L.","Weiß, A.","De Breuck, C.","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.","Fassnacht, C. D.","Gonzalez, A. H.","Greve, T. R.","Gullberg, B.","Hayward, C. C.","Hezaveh, Y.","Litke, K.","Ma, J.","Malkan, M.","Menten, K. M.","Miller, T.","Murphy, E. J.","Narayanan, D.","Phadke, K. A.","Rotermund, K. M.","Spilker, J. S.","Sreevani, J."],"bibdata":{"bibtype":"article","type":"article","title":"ISM properties of a Massive Dusty Star-Forming Galaxy discovered at z \\textasciitilde 7","volume":"1705","url":"http://adsabs.harvard.edu/abs/2017arXiv170507912S","abstract":"We report the discovery and constrain the physical conditions of the interstellar medium of the highest-redshift millimeter-selected dusty star-forming galaxy (DSFG) to date, SPT-S J031132-5823.4 (hereafter SPT0311-58), at \\$z=6.900 +/- 0.002\\$. SPT0311-58 was discovered via its 1.4mm thermal dust continuum emission in the South Pole Telescope (SPT)-SZ survey. The spectroscopic redshift was determined through an ALMA 3mm frequency scan that detected CO(6-5), CO(7-6) and [CI](2-1), and subsequently confirmed by detections of CO(3-2) with ATCA and [CII] 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 [CI] 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_\\{{\\textbackslash}rm gas\\} = 3.3 {\\textbackslash}pm 1.9 {\\textbackslash}times10{\\textasciicircum}\\{11\\}{\\textbackslash},M_\\{{\\textbackslash}odot\\}\\$. Its large mass and intense star formation is very rare for a source well into the Epoch of Reionization.","urldate":"2017-05-30","journal":"ArXiv e-prints","author":[{"propositions":[],"lastnames":["Strandet"],"firstnames":["M.","L."],"suffixes":[]},{"propositions":[],"lastnames":["Weiß"],"firstnames":["A."],"suffixes":[]},{"propositions":[],"lastnames":["De","Breuck"],"firstnames":["C."],"suffixes":[]},{"propositions":[],"lastnames":["Marrone"],"firstnames":["D.","P."],"suffixes":[]},{"propositions":[],"lastnames":["Vieira"],"firstnames":["J.","D."],"suffixes":[]},{"propositions":[],"lastnames":["Aravena"],"firstnames":["M."],"suffixes":[]},{"propositions":[],"lastnames":["Ashby"],"firstnames":["M.","L.","N."],"suffixes":[]},{"propositions":[],"lastnames":["Béthermin"],"firstnames":["M."],"suffixes":[]},{"propositions":[],"lastnames":["Bothwell"],"firstnames":["M.","S."],"suffixes":[]},{"propositions":[],"lastnames":["Bradford"],"firstnames":["C.","M."],"suffixes":[]},{"propositions":[],"lastnames":["Carlstrom"],"firstnames":["J.","E."],"suffixes":[]},{"propositions":[],"lastnames":["Chapman"],"firstnames":["S.","C."],"suffixes":[]},{"propositions":[],"lastnames":["Cunningham"],"firstnames":["D.","J.","M."],"suffixes":[]},{"propositions":[],"lastnames":["Chen"],"firstnames":["Chian-Chou"],"suffixes":[]},{"propositions":[],"lastnames":["Fassnacht"],"firstnames":["C.","D."],"suffixes":[]},{"propositions":[],"lastnames":["Gonzalez"],"firstnames":["A.","H."],"suffixes":[]},{"propositions":[],"lastnames":["Greve"],"firstnames":["T.","R."],"suffixes":[]},{"propositions":[],"lastnames":["Gullberg"],"firstnames":["B."],"suffixes":[]},{"propositions":[],"lastnames":["Hayward"],"firstnames":["C.","C."],"suffixes":[]},{"propositions":[],"lastnames":["Hezaveh"],"firstnames":["Y."],"suffixes":[]},{"propositions":[],"lastnames":["Litke"],"firstnames":["K."],"suffixes":[]},{"propositions":[],"lastnames":["Ma"],"firstnames":["J."],"suffixes":[]},{"propositions":[],"lastnames":["Malkan"],"firstnames":["M."],"suffixes":[]},{"propositions":[],"lastnames":["Menten"],"firstnames":["K.","M."],"suffixes":[]},{"propositions":[],"lastnames":["Miller"],"firstnames":["T."],"suffixes":[]},{"propositions":[],"lastnames":["Murphy"],"firstnames":["E.","J."],"suffixes":[]},{"propositions":[],"lastnames":["Narayanan"],"firstnames":["D."],"suffixes":[]},{"propositions":[],"lastnames":["Phadke"],"firstnames":["K.","A."],"suffixes":[]},{"propositions":[],"lastnames":["Rotermund"],"firstnames":["K.","M."],"suffixes":[]},{"propositions":[],"lastnames":["Spilker"],"firstnames":["J.","S."],"suffixes":[]},{"propositions":[],"lastnames":["Sreevani"],"firstnames":["J."],"suffixes":[]}],"month":"May","year":"2017","keywords":"Astrophysics - Astrophysics of Galaxies","pages":"arXiv:1705.07912","bibtex":"@article{strandet_ism_2017,\n\ttitle = {{ISM} properties of a {Massive} {Dusty} {Star}-{Forming} {Galaxy} discovered at z {\\textasciitilde} 7},\n\tvolume = {1705},\n\turl = {http://adsabs.harvard.edu/abs/2017arXiv170507912S},\n\tabstract = {We report the discovery and constrain the physical conditions of the interstellar medium of the highest-redshift millimeter-selected dusty star-forming galaxy (DSFG) to date, SPT-S J031132-5823.4 (hereafter SPT0311-58), at \\$z=6.900 +/- 0.002\\$. SPT0311-58 was discovered via its 1.4mm thermal dust continuum emission in the South Pole Telescope (SPT)-SZ survey. The spectroscopic redshift was determined through an ALMA 3mm frequency scan that detected CO(6-5), CO(7-6) and [CI](2-1), and subsequently confirmed by detections of CO(3-2) with ATCA and [CII] 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 [CI] 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\\_\\{{\\textbackslash}rm gas\\} = 3.3 {\\textbackslash}pm 1.9 {\\textbackslash}times10{\\textasciicircum}\\{11\\}{\\textbackslash},M\\_\\{{\\textbackslash}odot\\}\\$. Its large mass and intense star formation is very rare for a source well into the Epoch of Reionization.},\n\turldate = {2017-05-30},\n\tjournal = {ArXiv e-prints},\n\tauthor = {Strandet, M. L. and Weiß, A. and De Breuck, C. and Marrone, D. P. and Vieira, J. D. and Aravena, M. and Ashby, M. L. N. and Béthermin, M. 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 Gullberg, B. and Hayward, C. C. and Hezaveh, Y. and Litke, K. and Ma, J. and Malkan, M. and Menten, K. M. and Miller, T. and Murphy, E. J. and Narayanan, D. and Phadke, K. A. and Rotermund, K. M. and Spilker, J. S. and Sreevani, J.},\n\tmonth = may,\n\tyear = {2017},\n\tkeywords = {Astrophysics - Astrophysics of Galaxies},\n\tpages = {arXiv:1705.07912},\n}\n\n","author_short":["Strandet, M. L.","Weiß, A.","De Breuck, C.","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.","Fassnacht, C. D.","Gonzalez, A. H.","Greve, T. R.","Gullberg, B.","Hayward, C. C.","Hezaveh, Y.","Litke, K.","Ma, J.","Malkan, M.","Menten, K. M.","Miller, T.","Murphy, E. J.","Narayanan, D.","Phadke, K. A.","Rotermund, K. M.","Spilker, J. S.","Sreevani, J."],"key":"strandet_ism_2017","id":"strandet_ism_2017","bibbaseid":"strandet-wei-debreuck-marrone-vieira-aravena-ashby-bthermin-etal-ismpropertiesofamassivedustystarforminggalaxydiscoveredatztextasciitilde7-2017","role":"author","urls":{"Paper":"http://adsabs.harvard.edu/abs/2017arXiv170507912S"},"keyword":["Astrophysics - Astrophysics of Galaxies"],"metadata":{"authorlinks":{}}},"bibtype":"article","biburl":"https://bibbase.org/zotero/polyphant","dataSources":["7gvjSdWrEu7z5vjjj"],"keywords":["astrophysics - astrophysics of galaxies"],"search_terms":["ism","properties","massive","dusty","star","forming","galaxy","discovered","textasciitilde","strandet","weiß","de breuck","marrone","vieira","aravena","ashby","béthermin","bothwell","bradford","carlstrom","chapman","cunningham","chen","fassnacht","gonzalez","greve","gullberg","hayward","hezaveh","litke","ma","malkan","menten","miller","murphy","narayanan","phadke","rotermund","spilker","sreevani"],"title":"ISM properties of a Massive Dusty Star-Forming Galaxy discovered at z \\textasciitilde 7","year":2017}