Simulating Cosmic Reionization And The Radiation Backgrounds From The Epoch Of Reionization
Large-scale reionization simulations are described which combine the results of cosmological N-body simulations that model the evolving density and velocity fields and identify the galactic halo sources, with ray-tracing radiative transfer calculations which model the nonequilibrium ionization of th...
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Online Access: | http://hdl.handle.net/2152/29338 https://doi.org/10.1063/1.4754363 |
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ftunivtexas:oai:repositories.lib.utexas.edu:2152/29338 2023-05-15T18:22:25+02:00 Simulating Cosmic Reionization And The Radiation Backgrounds From The Epoch Of Reionization Shapiro, P. R. Iliev, I. T. Mellema, G. Ahn, K. Mao, Y. Friedrich, M. Datta, K. Park, H. Komatsu, E. Fernandez, E. Koda, J. Bovill, M. Pen, U. L. Shapiro, Paul R. Mao, Yi Park, Hyunbae Koda, Jun Bovill, Mia 2012 application/pdf http://hdl.handle.net/2152/29338 https://doi.org/10.1063/1.4754363 English eng First Stars Iv - from Hayashi to the Future Paul R. Shapiro, Ilian T. Iliev, G. Mellema, Kyungjin Ahn, Yi Mao, Martina Friedrich, Kanan Datta, Hyunbae Park, Eiichiro Komatsu, Elizabeth Fernandez, Jun Koda, Mia Bovill, and Ue-Li Pen. AIP Conference Proceedings 1480, 248 (2012); doi:10.1063/1.4754363 0094-243X http://hdl.handle.net/2152/29338 doi:10.1063/1.4754363 Administrative deposit of works to UT Digital Repository: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University. epoch of reionization first stars radiation backgrounds numerical simulation large-scale structure of the universe galaxies: high-redshift mesh refinement simulations south-pole telescope h-ii regions intergalactic medium cosmological reionization hydrogen reionization comparison project eddington tensor galaxy formation stellar sources astronomy & astrophysics Conference proceedings 2012 ftunivtexas https://doi.org/10.1063/1.4754363 2020-12-23T22:18:47Z Large-scale reionization simulations are described which combine the results of cosmological N-body simulations that model the evolving density and velocity fields and identify the galactic halo sources, with ray-tracing radiative transfer calculations which model the nonequilibrium ionization of the intergalactic medium. These simulations have been used to predict some of the signature effects of reionization on cosmic radiation backgrounds, including the CMB, near-IR, and redshifted 21cm backgrounds. We summarize some of our recent progress in this work, and address the question of whether observations of such signature effects can be used to distinguish the relative contributions of galaxies of different masses to reionization. Astronomy Conference Object South pole The University of Texas at Austin: Texas ScholarWorks South Pole AIP Conference Proceedings, 248 260 |
institution |
Open Polar |
collection |
The University of Texas at Austin: Texas ScholarWorks |
op_collection_id |
ftunivtexas |
language |
English |
topic |
epoch of reionization first stars radiation backgrounds numerical simulation large-scale structure of the universe galaxies: high-redshift mesh refinement simulations south-pole telescope h-ii regions intergalactic medium cosmological reionization hydrogen reionization comparison project eddington tensor galaxy formation stellar sources astronomy & astrophysics |
spellingShingle |
epoch of reionization first stars radiation backgrounds numerical simulation large-scale structure of the universe galaxies: high-redshift mesh refinement simulations south-pole telescope h-ii regions intergalactic medium cosmological reionization hydrogen reionization comparison project eddington tensor galaxy formation stellar sources astronomy & astrophysics Shapiro, P. R. Iliev, I. T. Mellema, G. Ahn, K. Mao, Y. Friedrich, M. Datta, K. Park, H. Komatsu, E. Fernandez, E. Koda, J. Bovill, M. Pen, U. L. Simulating Cosmic Reionization And The Radiation Backgrounds From The Epoch Of Reionization |
topic_facet |
epoch of reionization first stars radiation backgrounds numerical simulation large-scale structure of the universe galaxies: high-redshift mesh refinement simulations south-pole telescope h-ii regions intergalactic medium cosmological reionization hydrogen reionization comparison project eddington tensor galaxy formation stellar sources astronomy & astrophysics |
description |
Large-scale reionization simulations are described which combine the results of cosmological N-body simulations that model the evolving density and velocity fields and identify the galactic halo sources, with ray-tracing radiative transfer calculations which model the nonequilibrium ionization of the intergalactic medium. These simulations have been used to predict some of the signature effects of reionization on cosmic radiation backgrounds, including the CMB, near-IR, and redshifted 21cm backgrounds. We summarize some of our recent progress in this work, and address the question of whether observations of such signature effects can be used to distinguish the relative contributions of galaxies of different masses to reionization. Astronomy |
author2 |
Shapiro, Paul R. Mao, Yi Park, Hyunbae Koda, Jun Bovill, Mia |
format |
Conference Object |
author |
Shapiro, P. R. Iliev, I. T. Mellema, G. Ahn, K. Mao, Y. Friedrich, M. Datta, K. Park, H. Komatsu, E. Fernandez, E. Koda, J. Bovill, M. Pen, U. L. |
author_facet |
Shapiro, P. R. Iliev, I. T. Mellema, G. Ahn, K. Mao, Y. Friedrich, M. Datta, K. Park, H. Komatsu, E. Fernandez, E. Koda, J. Bovill, M. Pen, U. L. |
author_sort |
Shapiro, P. R. |
title |
Simulating Cosmic Reionization And The Radiation Backgrounds From The Epoch Of Reionization |
title_short |
Simulating Cosmic Reionization And The Radiation Backgrounds From The Epoch Of Reionization |
title_full |
Simulating Cosmic Reionization And The Radiation Backgrounds From The Epoch Of Reionization |
title_fullStr |
Simulating Cosmic Reionization And The Radiation Backgrounds From The Epoch Of Reionization |
title_full_unstemmed |
Simulating Cosmic Reionization And The Radiation Backgrounds From The Epoch Of Reionization |
title_sort |
simulating cosmic reionization and the radiation backgrounds from the epoch of reionization |
publishDate |
2012 |
url |
http://hdl.handle.net/2152/29338 https://doi.org/10.1063/1.4754363 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
First Stars Iv - from Hayashi to the Future Paul R. Shapiro, Ilian T. Iliev, G. Mellema, Kyungjin Ahn, Yi Mao, Martina Friedrich, Kanan Datta, Hyunbae Park, Eiichiro Komatsu, Elizabeth Fernandez, Jun Koda, Mia Bovill, and Ue-Li Pen. AIP Conference Proceedings 1480, 248 (2012); doi:10.1063/1.4754363 0094-243X http://hdl.handle.net/2152/29338 doi:10.1063/1.4754363 |
op_rights |
Administrative deposit of works to UT Digital Repository: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University. |
op_doi |
https://doi.org/10.1063/1.4754363 |
container_title |
AIP Conference Proceedings, |
container_start_page |
248 |
op_container_end_page |
260 |
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1766201837502857216 |