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个人简介
F.-S. Kitaura started Physics at the UCM after passing the University selection exams with the highest possible qualification in Physics and Mathematics. He obtained degrees in Physics with specialisations in Theoretical Physics and Astrophysics, UCM (2002) and TUM (2003), respectively. He started working on "hydrodynamical simulations with Boltzmann neutrino transport of the low mass end progenitor stars producing core-collapse (neutron stars) Supernovae explosions" during his master thesis (2003). His first author paper on this subject gathers more than 400 citations and led to a press release of the MPA in 2006 and of the whole Max Planck Society in 2007. In mid 2004 he received an IMPRS fellowship which permitted him to work on any subject at the MPA. After being inspired by an intensive school on astro-statistics at Penn University in 2005, he focused his research to study the cosmological large-scale structure (LSS) from galaxy surveys with statistical Data Analysis/Data Mining/Big Data tools. His PhD thesis “Cosmic Cartography: Bayesian Reconstruction of the Cosmological Large-Scale Structure” with advisors S. White and G. Boerner (December 20 2007) including some Supernova work received a perfect score in the written part and was altogether rated Magna Cum Laude by the LMU commission.
In 2008 he was granted a Marie-Curie fellowship from the EU to further develop his techniques to study the LSS from the Lyman-alpha forest with A. Ferrara at SISSA (Trieste) and at SNS (Pisa). The work he developed during this period joined for the first time peculiar velocity, power- spectrum and density reconstructions. He then got several grants in the period end of 2010 till mid 2011 from The Cluster of Excellence and the Max-Planck Society in Munich. In mid 2011 he was awarded with the Karl-Schwarzschild fellowship to work at the AIP in Potsdam. There he combined his statistical data analysis tools with higher order perturbation theory to make the first self-consistent phase-space analysis of the initial conditions and cosmic web of the Local Universe. This led to a press release at the Royal Astronomical Society in 2012 and applications of this work have appeared in National Geographic January 2015. He led the massive production of light-cone galaxy mocks project for the BOSS DR11/DR12 survey 2016, which set the error bars on the cosmological parameters 2017.
He co-authored a paper finding evidence for dynamical dark energy in Nature Astronomy 2017.
He has large number of publications (about 100) presenting original break through methods, becoming a renown expert in the field of LSS modelling and analysis, being invited in numerous international conferences (more than 30 times since 2007), and being awarded with the Leibniz Society young promising researchers prize (2013). Since 2008 he has worked as a referee for A\&A, ApJ, JCAP and MNRAS. He has given courses on Cosmology and Data Analysis at SNS (2009) (Pisa), at the Kapteyn Institute (2011) (Groningen), at the LMU (2011), at the Potsdam University (2013-2014), and at the Summer School in Corfu on Dark Energy (2014). Since 2017 he is Professor at ULL.
He was co-lead of the BAO reconstruction working group in EUCLID, co-PI of the cosmology science case in 4MOST for 2 years, co-lead of the data analysis tools in J-PAS. In June 2016 he won a Severo Ochoa grant to lead a group in cosmology large scale structure at the IAC and in July 2016 he obtained the Ramon y Cajal tenure track position from the Spanish government to work as a Professor at the ULL.
In 2017 he won as a co-PI a PRACE grant, and a Spanish national funding as the PI.
研究兴趣
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arxiv(2024)
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Daniel Forero-Sánchez,Francisco-Shu Kitaura,Francesco Sinigaglia, Jose María Coloma-Nadal,Jean-Paul Kneib
arxiv(2024)
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ASTRONOMY & ASTROPHYSICS (2024)
ASTRONOMY & ASTROPHYSICS (2024)
arXiv (Cornell University)no. 3 (2023): 3737-3745
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