ucb-phys229-2019spring-final-project

Spring 2019 PHYS229 final project in UCB

https://github.com/ickc/ucb-phys229-2019spring-final-project

Science Score: 31.0%

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Last synced: 9 months ago · JSON representation ·

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Spring 2019 PHYS229 final project in UCB

Basic Info
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  • Stars: 0
  • Watchers: 2
  • Forks: 0
  • Open Issues: 0
  • Releases: 1
Created about 7 years ago · Last pushed about 7 years ago
Metadata Files
Readme License Citation

README.md

Description

Final project of PHYS 229 at UCB in Spring 2019:

For your P229 final project I would like you to run the 21cmfast code (https://github.com/andreimesinger/21cmFAST) varying several of its parameters to produce ionization histories. Then use CAMB or CLASS (preferred) to compute how the temperature and polarization angular power spectra of the CMB would change if the Universe reionized in this manner. You can either submit an iPython notebook or a PDF file describing your results.

See report here.

Organization

21cmFAST.taskpaper

: Notes and todos

notebook

: Jupyter notebooks used

install

: convenient scripts to install the necessary environments

bin

: scripts written to generate the outputs

Owner

  • Name: Kolen Cheung
  • Login: ickc
  • Kind: user
  • Location: Exeter, UK
  • Company: University of Exeter

Citation (citation.bib)

@article{2018arXiv180706209P,
author = {Collaboration, Planck and Aghanim, N and Akrami, Y and Ashdown, M and Aumont, J and Baccigalupi, C and Ballardini, M and Banday, A J and Barreiro, R B and Bartolo, N and Basak, S and Battye, R and Benabed, K and Bernard, J P and Bersanelli, M and Bielewicz, P and Bock, J J and Bond, J R and Borrill, J and Bouchet, F R and Boulanger, F and Bucher, M and Burigana, C and Butler, R C and Calabrese, E and Cardoso, J F and Carron, J and Challinor, A and Chiang, H C and Chluba, J and Colombo, L P L and Combet, C and Contreras, D and Crill, B P and Cuttaia, F and de Bernardis, P and de Zotti, G and Delabrouille, J and Delouis, J M and Di Valentino, E and Diego, J M and Dore, O and Douspis, M and Ducout, A and Dupac, X and Dusini, S and Efstathiou, G and Elsner, F and Ensslin, T A and Eriksen, H K and Fantaye, Y and Farhang, M and Fergusson, J and Fernandez-Cobos, R and Finelli, F and Forastieri, F and Frailis, M and Franceschi, E and Frolov, A and Galeotta, S and Galli, S and Ganga, K and G{\'e}nova-Santos, R T and Gerbino, M and Ghosh, T and Gonzalez-Nuevo, J and Gorski, K M and Gratton, S and Gruppuso, A and Gudmundsson, J E and Hamann, J and Handley, W and Herranz, D and Hivon, E and Huang, Z and Jaffe, A H and Jones, W C and Karakci, A and Keihanen, E and Keskitalo, R and Kiiveri, K and Kim, J and Kisner, T S and Knox, L and Krachmalnicoff, N and Kunz, M and Kurki-Suonio, H and Lagache, G and Lamarre, J M and Lasenby, A and Lattanzi, M and Lawrence, C R and Le Jeune, M and Lemos, P and Lesgourgues, J and Levrier, F and Lewis, A and Liguori, M and Lilje, P B and Lilley, M and Lindholm, V and Lopez-Caniego, M and Lubin, P M and Ma, Y Z and Macias-Perez, J F and Maggio, G and Maino, D and Mandolesi, N and Mangilli, A and Marcos-Caballero, A and Maris, M and Martin, P G and Martinelli, M and Martinez-Gonzalez, E and Matarrese, S and Mauri, N and McEwen, J D and Meinhold, P R and Melchiorri, A and Mennella, A and Migliaccio, M and Millea, M and Mitra, S and Miville-Deschenes, M A and Molinari, D and Montier, L and Morgante, G and Moss, A and Natoli, P and Norgaard-Nielsen, H U and Pagano, L and Paoletti, D and Partridge, B and Patanchon, G and Peiris, H V and Perrotta, F and Pettorino, V and Piacentini, F and Polastri, L and Polenta, G and Puget, J L and Rachen, J P and Reinecke, M and Remazeilles, M and Renzi, A and Rocha, G and Rosset, C and Roudier, G and Rubino-Martin, J A and Ruiz-Granados, B and Salvati, L and Sandri, M and Savelainen, M and Scott, D and Shellard, E P S and Sirignano, C and Sirri, G and Spencer, L D and Sunyaev, R and Suur-Uski, A S and Tauber, J A and Tavagnacco, D and Tenti, M and Toffolatti, L and Tomasi, M and Trombetti, T and Valenziano, L and Valiviita, J and Van Tent, B and Vibert, L and Vielva, P and Villa, F and Vittorio, N and Wandelt, B D and Wehus, I K and White, M and White, S D M and Zacchei, A and Zonca, A},
title = {{Planck 2018 results. VI. Cosmological parameters}},
journal = {arXiv.org},
year = {2018},
eprint = {1807.06209},
eprinttype = {arxiv},
eprintclass = {astro-ph.CO},
pages = {arXiv:1807.06209},
month = jul,
annote = {71 pages. Parameter tables and chains available at https://wiki.cosmos.esa.int/planck-legacy-archive/index.php/Cosmological_Parameters}
}

@article{Blas:2011jb,
author = {Blas, Diego and Lesgourgues, Julien and Tram, Thomas},
title = {{The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes}},
journal = {arXiv.org},
year = {2011},
eprint = {1104.2933},
eprinttype = {arxiv},
eprintclass = {astro-ph.CO},
number = {07},
pages = {034--034},
month = apr,
annote = {35 pages, 10 figures, 5 tables. Ultra-relativistic fluid approximation better justified in a new Appendix B. Version accepted in JCAP. Code available at http://class-code.net}
}

@article{Park:2018go,
author = {Park, Jaehong and Mesinger, Andrei and Greig, Bradley and Gillet, Nicolas},
title = {{Inferring the astrophysics of reionization and cosmic dawn from galaxy luminosity functions and the 21-cm signal}},
journal = {arXiv.org},
year = {2018},
eprint = {1809.08995},
eprinttype = {arxiv},
eprintclass = {astro-ph.GA},
number = {1},
pages = {933--949},
month = sep,
annote = {16 pages, 8 figures and 2 tables. Associated movies are available at http://homepage.sns.it/mesinger/21CMMC.html. Updated to match the published version. All results and conclusions remain unchanged}
}

GitHub Events

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Kolen Cheung c****n@g****m 24

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