Alexandra Kozyreva, PhD
Affiliations: | 2010-2014 | Argelander Institute for Astronomy | Rheinische Friedrich-Wilhelms-Universität Bonn, Bonn, Nordrhein-Westfalen, Germany |
| 2015-2016 | Keele University, UK, Keele, England, United Kingdom | ||
| 2016- | Tel Aviv University, Tel Aviv-Yafo, Tel Aviv District, Israel |
Website:
http://www.astro.keele.ac.uk/~kozyreva/Google:
"Alexandra Kozyreva"Parents
Sign in to add mentor| Norbert Langer | grad student | 2014 | Universität Bonn |
| Sung-Chul Yoon | grad student | 2014 | Universität Bonn |
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Publications
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| Kozyreva A, Nakar E, Waldman R. (2019) The role of radioactive nickel in shaping the plateau phase of Type II supernovae Monthly Notices of the Royal Astronomical Society. 483: 1211-1223 |
| Kozyreva A, Kromer M, Noebauer UM, et al. (2018) OGLE14-073 – a promising pair-instability supernova candidate Monthly Notices of the Royal Astronomical Society. 479: 3106-3114 |
| Gilmer MS, Kozyreva A, Hirschi R, et al. (2017) Effects of Dimensionality on Pair-Instability Supernova Explosions Arxiv: Solar and Stellar Astrophysics. 20601 |
| Tolstov A, Zhiglo A, Nomoto K, et al. (2017) Ultraviolet Light Curves of Gaia16apd in Superluminous Supernova Models The Astrophysical Journal. 845 |
| Gilmer MS, Kozyreva A, Hirschi R, et al. (2017) Pair-instability Supernova Simulations: Progenitor Evolution, Explosion, and Light Curves The Astrophysical Journal. 846: 100 |
| Kozyreva A, Hirschi R, Blinnikov S, et al. (2016) How much radioactive nickel does ASASSN-15lh require? Monthly Notices of the Royal Astronomical Society. 459 |
| Kozyreva A, Gilmer M, Hirschi R, et al. (2016) Fast evolving pair-instability supernova models: evolution, explosion, light curves Monthly Notices of the Royal Astronomical Society. 464: 2854-2865 |
| Kozyreva A, Blinnikov S. (2015) Can pair-instability supernova models match the observations of superluminous supernovae? Monthly Notices of the Royal Astronomical Society. 454: 4357-4365 |
| Smidt J, Whalen DJ, Chatzopoulos E, et al. (2015) FINDING THE FIRST COSMIC EXPLOSIONS. IV. 90-140 M⊙ PAIR-INSTABILITY SUPERNOVAE Astrophysical Journal. 805 |
| Yoon SC, Kang J, Kozyreva A. (2015) Can very massive population iii stars produce a super-collapsar? Astrophysical Journal. 802 |