S
Shy Genel
Researcher at Columbia University
Publications - 216
Citations - 30664
Shy Genel is an academic researcher from Columbia University. The author has contributed to research in topics: Galaxy & Galaxy formation and evolution. The author has an hindex of 80, co-authored 195 publications receiving 24674 citations. Previous affiliations of Shy Genel include Tel Aviv University & York University.
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Journal ArticleDOI
Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe
Mark Vogelsberger,Shy Genel,Volker Springel,Volker Springel,Paul Torrey,Debora Sijacki,Dandan Xu,Gregory F. Snyder,Dylan Nelson,Lars Hernquist +9 more
TL;DR: The Illustris Project as mentioned in this paper is a series of large-scale hydrodynamical simulations of galaxy formation, which includes primordial and metal-line cooling with self-shielding corrections, stellar evolution, stellar feedback, gas recycling, chemical enrichment, supermassive black hole growth, and feedback from active galactic nuclei.
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THE SINS SURVEY: SINFONI INTEGRAL FIELD SPECTROSCOPY OF z ∼ 2 STAR-FORMING GALAXIES*
N. M. Förster Schreiber,Reinhard Genzel,Nicolas Bouché,Giovanni Cresci,Ric Davies,P. Buschkamp,Kristen L. Shapiro,Linda J. Tacconi,Erin K. S. Hicks,Shy Genel,Alice E. Shapley,Dawn K. Erb,Charles C. Steidel,Dieter Lutz,Frank Eisenhauer,Stefan Gillessen,Amiel Sternberg,Alvio Renzini,Andrea Cimatti,Emanuele Daddi,Jaron Kurk,Simon J. Lilly,Xu Kong,M. D. Lehnert,Nicole P. H. Nesvadba,Aprajita Verma,H. J. McCracken,Nobuo Arimoto,M. Mignoli,Masato Onodera +29 more
TL;DR: The Spectroscopic Imaging Survey in the near-infrared (near-IR) with SINFONI (SINS) of high-redshift galaxies is presented in this article.
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Properties of galaxies reproduced by a hydrodynamic simulation
Mark Vogelsberger,Shy Genel,Volker Springel,Volker Springel,Paul Torrey,Debora Sijacki,Dandan Xu,Gregory F. Snyder,Simeon Bird,Dylan Nelson,Lars Hernquist +10 more
TL;DR: A simulation that starts 12 million years after the Big Bang, and traces 13 billion years of cosmic evolution with 12 billion resolution elements in a cube of 106.5 megaparsecs a side yields a reasonable population of ellipticals and spirals, reproduces the observed distribution of galaxies in clusters and characteristics of hydrogen on large scales, and at the same time matches the ‘metal’ and hydrogen content of galaxies on small scales.
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Simulating galaxy formation with the IllustrisTNG model
Annalisa Pillepich,Annalisa Pillepich,Volker Springel,Volker Springel,Dylan Nelson,Shy Genel,Shy Genel,Jill Naiman,Rüdiger Pakmor,Lars Hernquist,Paul Torrey,Mark Vogelsberger,Rainer Weinberger,Federico Marinacci +13 more
TL;DR: In this article, an updated physical model to simulate the formation and evolution of galaxies in cosmological, large-scale gravity+magnetohydrodynamical simulations with the moving mesh code AREPO is introduced.
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First results from the IllustrisTNG simulations: matter and galaxy clustering
Volker Springel,Volker Springel,Rüdiger Pakmor,Annalisa Pillepich,Rainer Weinberger,Dylan Nelson,Lars Hernquist,Mark Vogelsberger,Shy Genel,Shy Genel,Paul Torrey,Federico Marinacci,Jill Naiman +12 more
TL;DR: In this article, the authors used the IllustrisTNG simulations to study the non-linear correlation functions and power spectra of baryons, dark matter, galaxies and haloes over an exceptionally large range of scales.