R
Robyn E. Sanderson
Researcher at University of Pennsylvania
Publications - 106
Citations - 3177
Robyn E. Sanderson is an academic researcher from University of Pennsylvania. The author has contributed to research in topics: Galaxy & Milky Way. The author has an hindex of 23, co-authored 86 publications receiving 2330 citations. Previous affiliations of Robyn E. Sanderson include Kapteyn Astronomical Institute & Columbia University.
Papers
More filters
Journal ArticleDOI
FIRE-2 simulations: physics versus numerics in galaxy formation
Philip F. Hopkins,Andrew Wetzel,Andrew Wetzel,Andrew Wetzel,Dušan Kereš,Claude André Faucher-Giguère,Eliot Quataert,Michael Boylan-Kolchin,Norman Murray,Christopher C. Hayward,Shea Garrison-Kimmel,Cameron Hummels,Robert Feldmann,Robert Feldmann,Paul Torrey,Xiangcheng Ma,Daniel Anglés-Alcázar,Kung-Yi Su,Matthew E. Orr,Denise Schmitz,Ivanna Escala,Robyn E. Sanderson,Michael Y. Grudić,Zachary Hafen,Ji-hoon Kim,Alex Fitts,James S. Bullock,Coral Wheeler,T. K. Chan,Oliver D. Elbert,Desika Narayanan +30 more
TL;DR: The Feedback In Realistic Environments (FIRE) project explores feedback in cosmological galaxy formation simulations as mentioned in this paper, which has been used to explore new physics (e.g. magnetic fields).
Journal ArticleDOI
Not so lumpy after all: modelling the depletion of dark matter subhaloes by Milky Way-like galaxies
Shea Garrison-Kimmel,Andrew Wetzel,Andrew Wetzel,Andrew Wetzel,James S. Bullock,Philip F. Hopkins,Michael Boylan-Kolchin,Claude André Faucher-Giguère,Dušan Kereš,Eliot Quataert,Robyn E. Sanderson,Andrew S. Graus,Tyler Kelley +12 more
TL;DR: In this paper, the effects of baryons on subhalo populations in ΛCDM were explored using cosmological zoom-in baryonic simulations of MW-mass haloes from the Latte simulation suite, part of the Feedback In Realistic Environments (FIRE) project.
Journal ArticleDOI
The case for a directional dark matter detector and the status of current experimental efforts
S. P. Ahlen,Niayesh Afshordi,Niayesh Afshordi,James Battat,J. Billard,Nassim Bozorgnia,S. Burgos,T. Caldwell,T. Caldwell,J. M. Carmona,S. Cebrián,P. Colas,T. Dafni,E. J. Daw,D. Dujmic,A. Dushkin,William Fedus,Efrain J. Ferrer,D. Finkbeiner,Peter H. Fisher,J. Forbes,T. Fusayasu,J. Galán,T. Gamble,C. Ghag,Ioannis Giomataris,Michael Gold,Haley Louise Gomez,M. E. Gomez,Paolo Gondolo,Anne M. Green,C. Grignon,O. Guillaudin,C. Hagemann,Kaori Hattori,Shawn Wesley Henderson,N. Higashi,C. Ida,F.J. Iguaz,Andrew Inglis,I. G. Irastorza,Satoru Iwaki,A. C. Kaboth,Shigeto Kabuki,J. Kadyk,Nitya Kallivayalil,H. Kubo,Shunsuke Kurosawa,V. A. Kudryavtsev,T. Lamy,Richard C. Lanza,T. B. Lawson,A. Lee,E. R. Lee,T. Lin,D. Loomba,Jeremy Lopez,G. Luzón,T. Manobu,J. Martoff,F. Mayet,B. Mccluskey,E. H. Miller,Kentaro Miuchi,Jocelyn Monroe,B. Morgan,D. Muna,A. St. J. Murphy,Tatsuhiro Naka,K. Nakamura,M. Nakamura,T. Nakano,G.G. Nicklin,H. Nishimura,K. Niwa,Sean Paling,Joseph D. Parker,A. Petkov,M. Pipe,K. Pushkin,Matthew R. Robinson,Arturo Rodriguez Rodriguez,Jose Rodríguez-Quintero,T. Sahin,Robyn E. Sanderson,N. Sanghi,D. Santos,O. Sato,Tatsuya Sawano,G. Sciolla,Hiroyuki Sekiya,Tracy R. Slatyer,D. P. Snowden-Ifft,N. J. C. Spooner,A. Sugiyama,A. Takada,M. Takahashi,A. Takeda,Toru Tanimori,Kojiro Taniue,A. Tomás,H. Tomita,K. Tsuchiya,J. Turk,E. Tziaferi,K. Ueno,S. E. Vahsen,R. Vanderspek,J D Vergados,J.A. Villar,H. Wellenstein,I. Wolfe,R. K. Yamamoto,H. Yegoryan +113 more
TL;DR: The case for a dark matter detector with directional sensitivity was presented at the 2009 CYGNUS workshop on directional dark matter detection, and contributions from theorists and experimental groups in the field as mentioned in this paper.
Journal ArticleDOI
The Local Group on FIRE: dwarf galaxy populations across a suite of hydrodynamic simulations
Shea Garrison-Kimmel,Philip F. Hopkins,Andrew Wetzel,Andrew Wetzel,Andrew Wetzel,James S. Bullock,Michael Boylan-Kolchin,Dušan Kereš,Claude André Faucher-Giguère,Kareem El-Badry,Astrid Lamberts,Eliot Quataert,Robyn E. Sanderson +12 more
TL;DR: Garrison-Kimmel et al. as discussed by the authors presented a new set of high-resolution hydrodynamic cosmological zoom-in simulations that apply the Feedback In Realistic Environments physics to both Local Group (LG)-like and isolated Milky Way (MW)-like volumes (10 host systems in total with a baryonic particle mass ≃3500-7000M).
Journal ArticleDOI
Numerical experiments with rubble piles: equilibrium shapes and spins
TL;DR: In this paper, the shape and spin limits of self-gravitating "perfect" rubble piles are investigated, and it is shown that idealized rubble piles behave qualitatively in a manner similar to certain granular materials, at least in the limit where global shape readjustments and/or mass shedding begins.