Dark Matter Substructure Detection Using Spatially Resolved Spectroscopy of Lensed Dusty Galaxies
We investigate how strong lensing of dusty, star-forming galaxies (DSFGs) by foreground galaxies can be used as a probe of dark matter halo substructure. We find that spatially resolved spectroscopy of lensed sources allows dramatic improvements to measurements of lens parameters. In particular, we...
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American Astronomical Society
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ftcaltechauth:oai:authors.library.caltech.edu:38260 2023-05-15T18:22:52+02:00 Dark Matter Substructure Detection Using Spatially Resolved Spectroscopy of Lensed Dusty Galaxies Hezaveh, Yashar Dalal, Neal Holder, Gilbert Kuhlen, Michael Marrone, Daniel Murray, Norman Vieira, Joaquin 2013-04-10 application/pdf https://authors.library.caltech.edu/38260/ https://authors.library.caltech.edu/38260/1/0004-637X_767_1_9.pdf https://resolver.caltech.edu/CaltechAUTHORS:20130503-102939560 en eng American Astronomical Society https://authors.library.caltech.edu/38260/1/0004-637X_767_1_9.pdf Hezaveh, Yashar and Dalal, Neal and Holder, Gilbert and Kuhlen, Michael and Marrone, Daniel and Murray, Norman and Vieira, Joaquin (2013) Dark Matter Substructure Detection Using Spatially Resolved Spectroscopy of Lensed Dusty Galaxies. Astrophysical Journal, 767 (1). Art. No. 9. ISSN 0004-637X. doi:10.1088/0004-637X/767/1/9. https://resolver.caltech.edu/CaltechAUTHORS:20130503-102939560 <https://resolver.caltech.edu/CaltechAUTHORS:20130503-102939560> other Article PeerReviewed 2013 ftcaltechauth https://doi.org/10.1088/0004-637X/767/1/9 2021-11-11T18:53:39Z We investigate how strong lensing of dusty, star-forming galaxies (DSFGs) by foreground galaxies can be used as a probe of dark matter halo substructure. We find that spatially resolved spectroscopy of lensed sources allows dramatic improvements to measurements of lens parameters. In particular, we find that modeling of the full, three-dimensional (angular position and radial velocity) data can significantly facilitate substructure detection, increasing the sensitivity of observables to lower mass subhalos. We carry out simulations of lensed dusty sources observed by early ALMA (Cycle 1) and use a Fisher matrix analysis to study the parameter degeneracies and mass detection limits of this method. We find that even with conservative assumptions, it is possible to detect galactic dark matter subhalos of ~10^8 M_☉ with high significance in most lensed DSFGs. Specifically, we find that in typical DSFG lenses, there is a ~55% probability of detecting a substructure with M > 10^8 M_☉ with more than 5σ detection significance in each lens, if the abundance of substructure is consistent with previous lensing results. The full ALMA array, with its significantly enhanced sensitivity and resolution, should improve these estimates considerably. Given the sample of ~100 lenses provided by surveys such as the South Pole Telescope, our understanding of dark matter substructure in typical galaxy halos is poised to improve dramatically over the next few years. Article in Journal/Newspaper South pole Caltech Authors (California Institute of Technology) South Pole The Astrophysical Journal 767 1 9 |
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Caltech Authors (California Institute of Technology) |
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English |
description |
We investigate how strong lensing of dusty, star-forming galaxies (DSFGs) by foreground galaxies can be used as a probe of dark matter halo substructure. We find that spatially resolved spectroscopy of lensed sources allows dramatic improvements to measurements of lens parameters. In particular, we find that modeling of the full, three-dimensional (angular position and radial velocity) data can significantly facilitate substructure detection, increasing the sensitivity of observables to lower mass subhalos. We carry out simulations of lensed dusty sources observed by early ALMA (Cycle 1) and use a Fisher matrix analysis to study the parameter degeneracies and mass detection limits of this method. We find that even with conservative assumptions, it is possible to detect galactic dark matter subhalos of ~10^8 M_☉ with high significance in most lensed DSFGs. Specifically, we find that in typical DSFG lenses, there is a ~55% probability of detecting a substructure with M > 10^8 M_☉ with more than 5σ detection significance in each lens, if the abundance of substructure is consistent with previous lensing results. The full ALMA array, with its significantly enhanced sensitivity and resolution, should improve these estimates considerably. Given the sample of ~100 lenses provided by surveys such as the South Pole Telescope, our understanding of dark matter substructure in typical galaxy halos is poised to improve dramatically over the next few years. |
format |
Article in Journal/Newspaper |
author |
Hezaveh, Yashar Dalal, Neal Holder, Gilbert Kuhlen, Michael Marrone, Daniel Murray, Norman Vieira, Joaquin |
spellingShingle |
Hezaveh, Yashar Dalal, Neal Holder, Gilbert Kuhlen, Michael Marrone, Daniel Murray, Norman Vieira, Joaquin Dark Matter Substructure Detection Using Spatially Resolved Spectroscopy of Lensed Dusty Galaxies |
author_facet |
Hezaveh, Yashar Dalal, Neal Holder, Gilbert Kuhlen, Michael Marrone, Daniel Murray, Norman Vieira, Joaquin |
author_sort |
Hezaveh, Yashar |
title |
Dark Matter Substructure Detection Using Spatially Resolved Spectroscopy of Lensed Dusty Galaxies |
title_short |
Dark Matter Substructure Detection Using Spatially Resolved Spectroscopy of Lensed Dusty Galaxies |
title_full |
Dark Matter Substructure Detection Using Spatially Resolved Spectroscopy of Lensed Dusty Galaxies |
title_fullStr |
Dark Matter Substructure Detection Using Spatially Resolved Spectroscopy of Lensed Dusty Galaxies |
title_full_unstemmed |
Dark Matter Substructure Detection Using Spatially Resolved Spectroscopy of Lensed Dusty Galaxies |
title_sort |
dark matter substructure detection using spatially resolved spectroscopy of lensed dusty galaxies |
publisher |
American Astronomical Society |
publishDate |
2013 |
url |
https://authors.library.caltech.edu/38260/ https://authors.library.caltech.edu/38260/1/0004-637X_767_1_9.pdf https://resolver.caltech.edu/CaltechAUTHORS:20130503-102939560 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://authors.library.caltech.edu/38260/1/0004-637X_767_1_9.pdf Hezaveh, Yashar and Dalal, Neal and Holder, Gilbert and Kuhlen, Michael and Marrone, Daniel and Murray, Norman and Vieira, Joaquin (2013) Dark Matter Substructure Detection Using Spatially Resolved Spectroscopy of Lensed Dusty Galaxies. Astrophysical Journal, 767 (1). Art. No. 9. ISSN 0004-637X. doi:10.1088/0004-637X/767/1/9. https://resolver.caltech.edu/CaltechAUTHORS:20130503-102939560 <https://resolver.caltech.edu/CaltechAUTHORS:20130503-102939560> |
op_rights |
other |
op_doi |
https://doi.org/10.1088/0004-637X/767/1/9 |
container_title |
The Astrophysical Journal |
container_volume |
767 |
container_issue |
1 |
container_start_page |
9 |
_version_ |
1766202281020096512 |