Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations ...
We use public data from the South Pole Telescope (SPT) and Atacama Cosmology Telescope (ACT) to measure radial profiles of the thermal Sunyaev-Zel'dovich (tSZ) effect and dust emission around massive quiescent galaxies at $z\approx1.$ Using survey data from the Dark Energy Survey (DES) and Wide...
Main Authors: | , , , , , |
---|---|
Format: | Article in Journal/Newspaper |
Language: | unknown |
Published: |
arXiv
2023
|
Subjects: | |
Online Access: | https://dx.doi.org/10.48550/arxiv.2306.04760 https://arxiv.org/abs/2306.04760 |
id |
ftdatacite:10.48550/arxiv.2306.04760 |
---|---|
record_format |
openpolar |
spelling |
ftdatacite:10.48550/arxiv.2306.04760 2023-11-05T03:45:06+01:00 Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations ... Meinke, Jeremy Cohen, Seth Moore, Jenna Böckmann, Kathrin Mauskopf, Philip Scannapieco, Evan 2023 https://dx.doi.org/10.48550/arxiv.2306.04760 https://arxiv.org/abs/2306.04760 unknown arXiv https://dx.doi.org/10.3847/1538-4357/acdcf4 Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 Astrophysics of Galaxies astro-ph.GA Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Article Text article-journal ScholarlyArticle 2023 ftdatacite https://doi.org/10.48550/arxiv.2306.0476010.3847/1538-4357/acdcf4 2023-10-09T10:16:22Z We use public data from the South Pole Telescope (SPT) and Atacama Cosmology Telescope (ACT) to measure radial profiles of the thermal Sunyaev-Zel'dovich (tSZ) effect and dust emission around massive quiescent galaxies at $z\approx1.$ Using survey data from the Dark Energy Survey (DES) and Wide-Field infrared Survey Explorer (WISE), we selected $387,627$ quiescent galaxies within the ACT field, with a mean stellar $\log_{10}(M_{\star}/\rm{M_{\odot}})$ of $11.40$. A subset of $94,452$ galaxies, with a mean stellar $\log_{10}(M_{\star}/\rm{M_{\odot}})$ of $11.36,$ are also covered by SPT. In $0.5$ arcminute radial bins around these galaxies, we detect the tSZ profile at levels up to $11σ$, and dust profile up to $20σ.$ Both profiles are extended, and the dust profile slope at large radii is consistent with galaxy clustering. We analyze the thermal energy and dust mass versus stellar mass via integration within $R=2.0$ arcminute circular apertures and fit them with a forward-modeled power-law to correct for our ... : 23 pages, 12 figures, accepted for publication in ApJ ... Article in Journal/Newspaper South pole DataCite Metadata Store (German National Library of Science and Technology) |
institution |
Open Polar |
collection |
DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
unknown |
topic |
Astrophysics of Galaxies astro-ph.GA Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
spellingShingle |
Astrophysics of Galaxies astro-ph.GA Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Meinke, Jeremy Cohen, Seth Moore, Jenna Böckmann, Kathrin Mauskopf, Philip Scannapieco, Evan Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations ... |
topic_facet |
Astrophysics of Galaxies astro-ph.GA Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
description |
We use public data from the South Pole Telescope (SPT) and Atacama Cosmology Telescope (ACT) to measure radial profiles of the thermal Sunyaev-Zel'dovich (tSZ) effect and dust emission around massive quiescent galaxies at $z\approx1.$ Using survey data from the Dark Energy Survey (DES) and Wide-Field infrared Survey Explorer (WISE), we selected $387,627$ quiescent galaxies within the ACT field, with a mean stellar $\log_{10}(M_{\star}/\rm{M_{\odot}})$ of $11.40$. A subset of $94,452$ galaxies, with a mean stellar $\log_{10}(M_{\star}/\rm{M_{\odot}})$ of $11.36,$ are also covered by SPT. In $0.5$ arcminute radial bins around these galaxies, we detect the tSZ profile at levels up to $11σ$, and dust profile up to $20σ.$ Both profiles are extended, and the dust profile slope at large radii is consistent with galaxy clustering. We analyze the thermal energy and dust mass versus stellar mass via integration within $R=2.0$ arcminute circular apertures and fit them with a forward-modeled power-law to correct for our ... : 23 pages, 12 figures, accepted for publication in ApJ ... |
format |
Article in Journal/Newspaper |
author |
Meinke, Jeremy Cohen, Seth Moore, Jenna Böckmann, Kathrin Mauskopf, Philip Scannapieco, Evan |
author_facet |
Meinke, Jeremy Cohen, Seth Moore, Jenna Böckmann, Kathrin Mauskopf, Philip Scannapieco, Evan |
author_sort |
Meinke, Jeremy |
title |
Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations ... |
title_short |
Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations ... |
title_full |
Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations ... |
title_fullStr |
Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations ... |
title_full_unstemmed |
Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations ... |
title_sort |
evidence of extended dust and feedback around z$\approx$1 quiescent galaxies via millimeter observations ... |
publisher |
arXiv |
publishDate |
2023 |
url |
https://dx.doi.org/10.48550/arxiv.2306.04760 https://arxiv.org/abs/2306.04760 |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.3847/1538-4357/acdcf4 |
op_rights |
Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 |
op_doi |
https://doi.org/10.48550/arxiv.2306.0476010.3847/1538-4357/acdcf4 |
_version_ |
1781706482471927808 |