The Rest-Frame Submillimeter Spectrum of High Redshift, Dusty, Star-Forming Galaxies from the SPT-SZ Survey ...
We present the average rest-frame spectrum of the final catalog of dusty star-forming galaxies (DSFGs) selected from the South Pole Telescope SZ survey (SPT-SZ) and measured with Band 3 of the Atacama Large Millimeter/submillimeter Array (ALMA). This work builds on the previous average rest-frame sp...
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ftdatacite:10.48550/arxiv.2210.11671 2023-06-11T04:16:47+02:00 The Rest-Frame Submillimeter Spectrum of High Redshift, Dusty, Star-Forming Galaxies from the SPT-SZ Survey ... Reuter, C. Spilker, J. S. Vieira, J. D. Marrone, D. P. Weiss, A. Aravena, M. Archipley, M. A. Chapman, S. C. Gonzalez, A. Greve, T. R. Hayward, C. C. Hill, R. Jarugula, S. Kim, S. Malkan, M. Phadke, K. A. Stark, A. A. Sulzenauer, N. Vizgan, D. 2022 https://dx.doi.org/10.48550/arxiv.2210.11671 https://arxiv.org/abs/2210.11671 unknown arXiv https://dx.doi.org/10.3847/1538-4357/acaf51 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Astrophysics of Galaxies astro-ph.GA FOS Physical sciences article-journal ScholarlyArticle Text Article 2022 ftdatacite https://doi.org/10.48550/arxiv.2210.1167110.3847/1538-4357/acaf51 2023-06-01T11:28:16Z We present the average rest-frame spectrum of the final catalog of dusty star-forming galaxies (DSFGs) selected from the South Pole Telescope SZ survey (SPT-SZ) and measured with Band 3 of the Atacama Large Millimeter/submillimeter Array (ALMA). This work builds on the previous average rest-frame spectrum, given in Spilker et al. (2014) for the first 22 sources, and is comprised of a total of 78 sources, normalized by their respective apparent dust masses. The spectrum spans $1.9$$<$z$<$$6.9$ and covers rest-frame frequencies of 240$-$800 GHz. Combining this data with low-J CO observations from the Australia Telescope Compact Array (ATCA), we detect multiple bright line features from $^{12}$CO, $[$CI$]$, and H$_2$O, as well as fainter molecular transitions from $^{13}$CO, HCN, HCO$^+$, HNC, CN, H$_2$O$^+$, and CH. We use these detections, along with limits from other molecules, to characterize the typical properties of the interstellar medium (ISM) for these high redshift DSFGs. We are able to divide ... : 26 pages, 10 figures, accepted for publication in ApJ ... Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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DataCite Metadata Store (German National Library of Science and Technology) |
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Astrophysics of Galaxies astro-ph.GA FOS Physical sciences |
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Astrophysics of Galaxies astro-ph.GA FOS Physical sciences Reuter, C. Spilker, J. S. Vieira, J. D. Marrone, D. P. Weiss, A. Aravena, M. Archipley, M. A. Chapman, S. C. Gonzalez, A. Greve, T. R. Hayward, C. C. Hill, R. Jarugula, S. Kim, S. Malkan, M. Phadke, K. A. Stark, A. A. Sulzenauer, N. Vizgan, D. The Rest-Frame Submillimeter Spectrum of High Redshift, Dusty, Star-Forming Galaxies from the SPT-SZ Survey ... |
topic_facet |
Astrophysics of Galaxies astro-ph.GA FOS Physical sciences |
description |
We present the average rest-frame spectrum of the final catalog of dusty star-forming galaxies (DSFGs) selected from the South Pole Telescope SZ survey (SPT-SZ) and measured with Band 3 of the Atacama Large Millimeter/submillimeter Array (ALMA). This work builds on the previous average rest-frame spectrum, given in Spilker et al. (2014) for the first 22 sources, and is comprised of a total of 78 sources, normalized by their respective apparent dust masses. The spectrum spans $1.9$$<$z$<$$6.9$ and covers rest-frame frequencies of 240$-$800 GHz. Combining this data with low-J CO observations from the Australia Telescope Compact Array (ATCA), we detect multiple bright line features from $^{12}$CO, $[$CI$]$, and H$_2$O, as well as fainter molecular transitions from $^{13}$CO, HCN, HCO$^+$, HNC, CN, H$_2$O$^+$, and CH. We use these detections, along with limits from other molecules, to characterize the typical properties of the interstellar medium (ISM) for these high redshift DSFGs. We are able to divide ... : 26 pages, 10 figures, accepted for publication in ApJ ... |
format |
Text |
author |
Reuter, C. Spilker, J. S. Vieira, J. D. Marrone, D. P. Weiss, A. Aravena, M. Archipley, M. A. Chapman, S. C. Gonzalez, A. Greve, T. R. Hayward, C. C. Hill, R. Jarugula, S. Kim, S. Malkan, M. Phadke, K. A. Stark, A. A. Sulzenauer, N. Vizgan, D. |
author_facet |
Reuter, C. Spilker, J. S. Vieira, J. D. Marrone, D. P. Weiss, A. Aravena, M. Archipley, M. A. Chapman, S. C. Gonzalez, A. Greve, T. R. Hayward, C. C. Hill, R. Jarugula, S. Kim, S. Malkan, M. Phadke, K. A. Stark, A. A. Sulzenauer, N. Vizgan, D. |
author_sort |
Reuter, C. |
title |
The Rest-Frame Submillimeter Spectrum of High Redshift, Dusty, Star-Forming Galaxies from the SPT-SZ Survey ... |
title_short |
The Rest-Frame Submillimeter Spectrum of High Redshift, Dusty, Star-Forming Galaxies from the SPT-SZ Survey ... |
title_full |
The Rest-Frame Submillimeter Spectrum of High Redshift, Dusty, Star-Forming Galaxies from the SPT-SZ Survey ... |
title_fullStr |
The Rest-Frame Submillimeter Spectrum of High Redshift, Dusty, Star-Forming Galaxies from the SPT-SZ Survey ... |
title_full_unstemmed |
The Rest-Frame Submillimeter Spectrum of High Redshift, Dusty, Star-Forming Galaxies from the SPT-SZ Survey ... |
title_sort |
rest-frame submillimeter spectrum of high redshift, dusty, star-forming galaxies from the spt-sz survey ... |
publisher |
arXiv |
publishDate |
2022 |
url |
https://dx.doi.org/10.48550/arxiv.2210.11671 https://arxiv.org/abs/2210.11671 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.3847/1538-4357/acaf51 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.2210.1167110.3847/1538-4357/acaf51 |
_version_ |
1768375396673257472 |