Characterizing the ISM using Fine-Structure Lines in a z=5.7 Hyper-Starburst Galaxy Merger
SPT0346-52 is a gravitationally lensed dusty star-forming galaxy at z~5.7 from the South Pole Telescope sample1. It is an extremely luminous hyper-starburst system with intrinsic far-infrared luminosity > 10 13 Lsun and star formation rate density ~4200 Msunyr -1 kpc 2 . Based on ALMA observation...
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ftzenodo:oai:zenodo.org:3629494 2024-09-15T18:36:44+00:00 Characterizing the ISM using Fine-Structure Lines in a z=5.7 Hyper-Starburst Galaxy Merger Katrina Litke 2020-01-27 https://doi.org/10.5281/zenodo.3629494 unknown Zenodo https://zenodo.org/communities/almabo19 https://doi.org/10.5281/zenodo.3629493 https://doi.org/10.5281/zenodo.3629494 oai:zenodo.org:3629494 info:eu-repo/semantics/openAccess Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode ALMABO19, Views on the Interstellar Medium in the ALMA era info:eu-repo/semantics/conferencePoster 2020 ftzenodo https://doi.org/10.5281/zenodo.362949410.5281/zenodo.3629493 2024-07-26T06:24:19Z SPT0346-52 is a gravitationally lensed dusty star-forming galaxy at z~5.7 from the South Pole Telescope sample1. It is an extremely luminous hyper-starburst system with intrinsic far-infrared luminosity > 10 13 Lsun and star formation rate density ~4200 Msunyr -1 kpc 2 . Based on ALMA observations of [CII]158 emission, we have determined the prodigious star formation rate density is likely driven by a major merger of two components. Continuing this work, we have ALMA Bands 6 and 7 observations of four fine structure lines in this dusty starforming galaxy: [CII]158, [OI]145, [NII]205, [NII]122. We use a pixelated, interferometric lensing reconstruction code to model the visibilities observed by ALMA and "de-lens" emission to obtain the spatially resolved interstellar medium (ISM) in the source-plane. Conference Object South pole Zenodo |
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SPT0346-52 is a gravitationally lensed dusty star-forming galaxy at z~5.7 from the South Pole Telescope sample1. It is an extremely luminous hyper-starburst system with intrinsic far-infrared luminosity > 10 13 Lsun and star formation rate density ~4200 Msunyr -1 kpc 2 . Based on ALMA observations of [CII]158 emission, we have determined the prodigious star formation rate density is likely driven by a major merger of two components. Continuing this work, we have ALMA Bands 6 and 7 observations of four fine structure lines in this dusty starforming galaxy: [CII]158, [OI]145, [NII]205, [NII]122. We use a pixelated, interferometric lensing reconstruction code to model the visibilities observed by ALMA and "de-lens" emission to obtain the spatially resolved interstellar medium (ISM) in the source-plane. |
format |
Conference Object |
author |
Katrina Litke |
spellingShingle |
Katrina Litke Characterizing the ISM using Fine-Structure Lines in a z=5.7 Hyper-Starburst Galaxy Merger |
author_facet |
Katrina Litke |
author_sort |
Katrina Litke |
title |
Characterizing the ISM using Fine-Structure Lines in a z=5.7 Hyper-Starburst Galaxy Merger |
title_short |
Characterizing the ISM using Fine-Structure Lines in a z=5.7 Hyper-Starburst Galaxy Merger |
title_full |
Characterizing the ISM using Fine-Structure Lines in a z=5.7 Hyper-Starburst Galaxy Merger |
title_fullStr |
Characterizing the ISM using Fine-Structure Lines in a z=5.7 Hyper-Starburst Galaxy Merger |
title_full_unstemmed |
Characterizing the ISM using Fine-Structure Lines in a z=5.7 Hyper-Starburst Galaxy Merger |
title_sort |
characterizing the ism using fine-structure lines in a z=5.7 hyper-starburst galaxy merger |
publisher |
Zenodo |
publishDate |
2020 |
url |
https://doi.org/10.5281/zenodo.3629494 |
genre |
South pole |
genre_facet |
South pole |
op_source |
ALMABO19, Views on the Interstellar Medium in the ALMA era |
op_relation |
https://zenodo.org/communities/almabo19 https://doi.org/10.5281/zenodo.3629493 https://doi.org/10.5281/zenodo.3629494 oai:zenodo.org:3629494 |
op_rights |
info:eu-repo/semantics/openAccess Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode |
op_doi |
https://doi.org/10.5281/zenodo.362949410.5281/zenodo.3629493 |
_version_ |
1810480444214345728 |