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Physics

D-Index
88
Citations
32413
World Ranking
2373
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1194

Overview

Michael Boylan-Kolchin is affiliated with The University of Texas at Austin in the United States and primarily works in the field of Physics and Astronomy. Their research spans several subfields including Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Statistical and Nonlinear Physics, and Electrical and Electronic Engineering.

Their scholarly output includes work on key topics such as:

  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Stellar, planetary, and galactic studies
  • Astrophysics and Star Formation Studies
  • Cosmology and Gravitation Theories
  • Dark Matter and Cosmic Phenomena
  • Gamma-ray bursts and supernovae

Michael Boylan-Kolchin has contributed extensively to scientific literature, publishing in frequent venues like:

  • arXiv (Cornell University)
  • Monthly Notices of the Royal Astronomical Society
  • The Astrophysical Journal
  • Nature Astronomy
  • The Astrophysical Journal Supplement Series

Among their recent significant papers are:

  • Stress testing ΛCDM with high-redshift galaxy candidates (2023, Nature Astronomy)
  • A dark matter profile to model diverse feedback-induced core sizes of ΛCDM haloes (2020, Monthly Notices of the Royal Astronomical Society)
  • Public Data Release of the FIRE-2 Cosmological Zoom-in Simulations of Galaxy Formation (2023, The Astrophysical Journal Supplement Series)
  • The impact of UV variability on the abundance of bright galaxies at z ≥ 9 (2023, Monthly Notices of the Royal Astronomical Society)
  • FIRE-3: updated stellar evolution models, yields, and microphysics and fitting functions for applications in galaxy simulations (2022, Monthly Notices of the Royal Astronomical Society)

Their work reflects frequent collaborations with other researchers, including:

  • Andrew Wetzel
  • James S. Bullock
  • Philip F. Hopkins
  • Claude-André Faucher-Giguère
  • Daniel R. Weisz

Best Publications

  • From dwarf spheroidals to cDs: Simulating the galaxy population in a LCDM cosmology

    Qi Guo;Simon White;Michael Boylan-Kolchin;Gabriella De Lucia

  • Too big to fail? The puzzling darkness of massive Milky Way subhaloes

    Michael Boylan-Kolchin;James S. Bullock;Manoj Kaplinghat

  • From dwarf spheroidals to cD galaxies: simulating the galaxy population in a ΛCDM cosmology

    Qi Guo;Simon White;Michael Boylan-Kolchin;Gabriella De Lucia

  • How do galaxies populate dark matter haloes

    Qi Guo;Simon White;Cheng Li;Michael Boylan-Kolchin

  • Resolving cosmic structure formation with the Millennium-II simulation

    Michael Boylan-Kolchin;Volker Springel;Simon D. M. White;Adrian Jenkins

  • Small-Scale Challenges to the $\Lambda$CDM Paradigm.

    James S. Bullock;Michael Boylan-Kolchin

  • FIRE-2 simulations: physics versus numerics in galaxy formation

    Philip F. Hopkins;Andrew Wetzel;Andrew Wetzel;Andrew Wetzel;Dušan Kereš;Claude André Faucher-Giguère

  • The Milky Way's bright satellites as an apparent failure of LCDM

    Michael Boylan-Kolchin;James S. Bullock;Manoj Kaplinghat

  • The Milky Way’s bright satellites as an apparent failure of ΛCDM

    Michael Boylan-Kolchin;James S. Bullock;Manoj Kaplinghat

  • Small-Scale Challenges to the ΛCDM Paradigm

    James S. Bullock;Michael Boylan-Kolchin

  • The merger rates and mass assembly histories of dark matter haloes in the two Millennium simulations

    Onsi Fakhouri;Chung-Pei Ma;Michael Boylan-Kolchin

  • Dynamical Friction and Galaxy Merging Timescales

    Michael Boylan-Kolchin;Chung-Pei Ma;Eliot Quataert

  • How do galaxies populate Dark Matter halos

    Qi Guo;Simon White;Cheng Li;Michael Boylan-Kolchin

  • Dynamical friction and galaxy merging time-scales

    Michael Boylan-Kolchin;Chung Pei Ma;Eliot Quataert

  • ELVIS: Exploring the Local Volume in Simulations

    Shea Garrison-Kimmel;Michael Boylan-Kolchin;Michael Boylan-Kolchin;James S. Bullock;Kyle Lee

  • Forged in FIRE: cusps, cores and baryons in low-mass dwarf galaxies

    Jose Oñorbe;Jose Oñorbe;Michael Boylan-Kolchin;Michael Boylan-Kolchin;James S. Bullock;Philip F. Hopkins

  • Galaxy formation in WMAP1 and WMAP7 cosmologies

    Qi Guo;Simon White;Raul E. Angulo;Bruno Henriques

  • Not so lumpy after all: modelling the depletion of dark matter subhaloes by Milky Way-like galaxies

    Shea Garrison-Kimmel;Andrew R. Wetzel;Andrew R. Wetzel;Andrew R. Wetzel;James S. Bullock;Philip F. Hopkins

  • The mass–concentration–redshift relation of cold dark matter haloes

    Aaron D. Ludlow;Julio F. Navarro;Raúl E. Angulo;Michael Boylan-Kolchin

  • Galaxy formation with BECDM - I. Turbulence and relaxation of idealized haloes.

    Philip Mocz;Mark Vogelsberger;Victor H. Robles;Jesús Zavala

Frequent Co-Authors

James S. Bullock
James S. Bullock University of California, Irvine
Philip F. Hopkins
Philip F. Hopkins California Institute of Technology
Claude André Faucher-Giguère
Claude André Faucher-Giguère Northwestern University
Dušan Kereš
Dušan Kereš University of California, San Diego
Daniel R. Weisz
Daniel R. Weisz University of California, Berkeley
Eliot Quataert
Eliot Quataert Princeton University
Volker Springel
Volker Springel Max Planck Institute for Astrophysics
Andrew A. Cole
Andrew A. Cole University of Tasmania
Antonio Aparicio
Antonio Aparicio University of La Laguna
Simon D. M. White
Simon D. M. White Max Planck Institute for Astrophysics

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