Tom Abel
Professor of Particle Physics and Astrophysics and of Physics
Web page: http://web.stanford.edu/dept/physics/people/faculty/abel_tom.html
Bio
What were the first objects that formed in the Universe? Prof. Abel's group explores the first billion years of cosmic history using ab initio supercomputer calculations. He has shown from first principles that the very first luminous objects are very massive stars and has developed novel numerical algorithms using adaptive-mesh-refinement simulations that capture over 14 orders of magnitude in length and time scales. He currently continues his work on the first stars and first galaxies and their role in chemical enrichment and cosmological reionization. His group studies any of the first objects to form in the universe: first stars, first supernovae, first HII regions, first magnetic fields, first heavy elements, and so on. Most recently he is pioneering novel numerical algorithms to study collisionless fluids such as dark matter which makes up most of the mass in the Universe as well as astrophysical and terrestrial plasmas. He was the director of the Kavli Institute for Particle Astrophysics and Cosmology and Division Director at SLAC 2013-2018.
Administrative Appointments
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Terman Fellow, Stanford University (2007 - 2010)
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Director, Kavli Institute for Particle Astrophysics and Cosmology, Stanford/SLAC (2013 - 2018)
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Visiting Professor, Heidelberg Institute of Theoretical Studies (2010 - 2011)
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Visiting Professor, University of Heidelberg at Institute for Theoretical Astrophysics (2010 - 2011)
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Founding Head, KIPAC Computational Physics department at SLAC (2005 - 2005)
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Associate Professor Department of Physics, Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, and SLAC (2004 - Present)
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Associate Professor with tenure, Deptartment for Astronomy and Astrophysics, Pennsylvania State University (2004 - 2004)
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Assistant Professor, Department for Astronomy and Astrophysics, Pennsylvania State University (2002 - 2002)
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Wempe Lecturer, Astrophysical Institute, Potsdam (2001 - 2001)
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Postdoctoral Researcher, Institute of Astronomy, Cambridge (2001 - 2001)
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Postdoctoral Fellow, Harvard College Observatory (1999 - 2001)
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Visitor, Max Planck Institute for Astrophysics (1997 - 1999)
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Visiting Research Scholar, National Center for Supercomputing Applications (1996 - 1999)
Honors & Awards
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Elected Fellow of the AAAS, American Association for the Advancement of Science (2014)
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Lagrange Prize, Institute Lagrange de Paris (2011)
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NSF Career Award, National Science Foundation (2003-2008)
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Gordon Bell Prize Finalist, Association for Computing Machinery (2001)
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Wempe Prize, Leibniz-Institut für Astrophysik Potsdam (2000)
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Scholarship, Deutscher Akademischer Austausch Dienst (1993-1994)
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Oskar Karl Forster Scholarship, Universität Regensburg (1993)
Boards, Advisory Committees, Professional Organizations
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Associate Editor, Journal of Particle Astrophysics and Cosmology (JCAP) (2015 - Present)
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Organizer, Collisionless Fluids, a workshop at the Institute Lagrange de Paris & IAP (2014 - 2014)
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Organizer, KIPAC@10, Big Questions in Particle Astrophysics and Cosmology, KIPAC, Stanford (2013 - 2013)
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Advisory Board Member, Hayden Planetarium Space Show (2012 - 2013)
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Organizer, Kavli Futures Symposium, "Growing High Performance Computing in a Green Environment" (2010 - 2010)
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Organizer, Kavli Futures Symposium, "Solving Real Problems with imagined Computers", SLAC (2009 - 2009)
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Advisory Board Member, Hayden Planetarium Space Show (2008 - 2009)
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Organizer, Scientific Challenges for Understanding the Quantum Universe and the Role of Computation at the Extreme Scale, SLAC (2008 - 2008)
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Co-Organizer (with Alex Heger & Brian O'Shea), First Stars III (2007 - 2007)
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Co-Organizer (with C. McKee, P. Padoan, & A. Goodman), Star formation over cosmic time, KITP Santa Barbara (2007 - 2007)
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Co-Organizer (with Yong Qian, Alex Heger & Tim Beers), The First Stars and Evolution of the Early Universe, INT Seattle (2006 - 2006)
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Chair, GRB physics before SWIFT, State College (2004 - 2004)
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Co-Organizer (with Andrew Hamilton, Martin Hachnelt & Andrea Ghez), Formation of Supermassive Black Holes (2004 - 2004)
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Chair, First Stars II, Pennsylvania State University (2003 - 2003)
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Co-Organizer (with Rosie Wyse), The Baryonic Universe, Aspen Winter workshop (2003 - 2003)
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Consultant, National Geographic Magazine (2003 - 2003)
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Member, Astro 2010 (2002 - Present)
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Panel member, Department of Energy, Innovative & Novel Computational Impact on Theory and Experiment (INCITE) (2002 - Present)
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Postdoc review panel member, National Science Foundation (2002 - Present)
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Co-Organizer (with Achim Weiss & Vanessa Hill), First Stars (1999 - 1999)
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Referee, New Astronomy (1998 - Present)
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Referee, Nature (1998 - Present)
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Referee, Science (1998 - Present)
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Referee, The Astrophysical Journal (1998 - Present)
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Referee, Monthly Notices of the Royal Astronomical Society (1998 - Present)
Professional Education
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Masters, University of Regensburg (1998)
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Ph.D, Ludwig Maximillians University Munich (1999)
2024-25 Courses
- Computational Physics
PHYSICS 113 (Spr) - Modern Astrophysics
PHYSICS 360 (Win) -
Independent Studies (2)
- Independent Research and Study
PHYSICS 190 (Aut, Spr, Sum) - Research
PHYSICS 490 (Aut, Win, Spr, Sum)
- Independent Research and Study
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Prior Year Courses
2022-23 Courses
- Computational Physics
PHYSICS 113 (Spr) - Special Topics in Astrophysics: Large Photometric Galaxy Surveys: From Pixels to Cosmology
PHYSICS 367 (Spr)
2021-22 Courses
- Computational Physics
PHYSICS 113 (Win)
- Computational Physics
Stanford Advisees
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Doctoral Dissertation Reader (AC)
Minjie Lei -
Doctoral Dissertation Advisor (AC)
Dylan Britt, Bryen Irving, Mati Mebratu -
Doctoral (Program)
Tara Dacunha, Jack Dinsmore, Viraj Manwadkar, Bernardita Ried Guachalla, Haley Stueber, Andrew Sullivan, Nan Wang -
Postdoctoral Research Mentor
Eric Moseley
All Publications
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ENZO: AN ADAPTIVE MESH REFINEMENT CODE FOR ASTROPHYSICS
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
2014; 211 (2)
View details for DOI 10.1088/0067-0049/211/2/19
View details for Web of Science ID 000334028600003
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The warm dark matter halo mass function below the cut-off scale
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2013; 434 (4): 3337-3347
View details for DOI 10.1093/mnras/stt1246
View details for Web of Science ID 000325262300052
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A new approach to simulating collisionless dark matter fluids
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2013; 434 (2): 1171-1191
View details for DOI 10.1093/mnras/stt1061
View details for Web of Science ID 000323638200018
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Tracing the dark matter sheet in phase space
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2012; 427 (1): 61-76
View details for DOI 10.1111/j.1365-2966.2012.21754.x
View details for Web of Science ID 000310675400006
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MAGNETIC FIELDS IN POPULATION III STAR FORMATION
ASTROPHYSICAL JOURNAL
2012; 745 (2)
View details for DOI 10.1088/0004-637X/745/2/154
View details for Web of Science ID 000300326800052
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OUTFLOW FEEDBACK REGULATED MASSIVE STAR FORMATION IN PARSEC-SCALE CLUSTER-FORMING CLUMPS
ASTROPHYSICAL JOURNAL
2010; 709 (1): 27-41
View details for DOI 10.1088/0004-637X/709/1/27
View details for Web of Science ID 000273282500003
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The Formation of Population III Binaries from Cosmological Initial Conditions
SCIENCE
2009; 325 (5940): 601-605
Abstract
Previous high-resolution cosmological simulations predicted that the first stars to appear in the early universe were very massive and formed in isolation. Here, we discuss a cosmological simulation in which the central 50 M(o) (where M(o) is the mass of the Sun) clump breaks up into two cores having a mass ratio of two to one, with one fragment collapsing to densities of 10(-8) grams per cubic centimeter. The second fragment, at a distance of approximately 800 astronomical units, is also optically thick to its own cooling radiation from molecular hydrogen lines but is still able to cool via collision-induced emission. The two dense peaks will continue to accrete from the surrounding cold gas reservoir over a period of approximately 10(5) years and will likely form a binary star system.
View details for DOI 10.1126/science.1173540
View details for Web of Science ID 000268493000047
View details for PubMedID 19589964
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MAGNETOHYDRODYNAMIC SIMULATIONS OF DISK GALAXY FORMATION: THE MAGNETIZATION OF THE COLD AND WARM MEDIUM
ASTROPHYSICAL JOURNAL
2009; 696 (1): 96-109
View details for DOI 10.1088/0004-637X/696/1/96
View details for Web of Science ID 000265350100010
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GALAXY MERGERS WITH ADAPTIVE MESH REFINEMENT: STAR FORMATION AND HOT GAS OUTFLOW
ASTROPHYSICAL JOURNAL LETTERS
2009; 694 (2): L123-L127
View details for DOI 10.1088/0004-637X/694/2/L123
View details for Web of Science ID 000264196600008
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How very massive metal-free stars start cosmological reionization
ASTROPHYSICAL JOURNAL
2008; 684 (1): 1-17
View details for Web of Science ID 000258730700001
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Resolving the formation of protogalaxies. II. Central gravitational collapse
ASTROPHYSICAL JOURNAL
2008; 682 (2): 745-757
View details for Web of Science ID 000258026100005
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The formation of the first star in the universe
SCIENCE
2002; 295 (5552): 93-98
Abstract
We describe results from a fully self-consistent three-dimensional hydrodynamical simulation of the formation of one of the first stars in the Universe. In current models of structure formation, dark matter initially dominates, and pregalactic objects form because of gravitational instability from small initial density perturbations. As they assemble via hierarchical merging, primordial gas cools through ro-vibrational lines of hydrogen molecules and sinks to the center of the dark matter potential well. The high-redshift analog of a molecular cloud is formed. As the dense, central parts of the cold gas cloud become self-gravitating, a dense core of approximately 100 M (where M is the mass of the Sun) undergoes rapid contraction. At particle number densities greater than 10(9) per cubic centimeter, a 1 M protostellar core becomes fully molecular as a result of three-body H2 formation. Contrary to analytical expectations, this process does not lead to renewed fragmentation and only one star is formed. The calculation is stopped when optical depth effects become important, leaving the final mass of the fully formed star somewhat uncertain. At this stage the protostar is accreting material very rapidly (approximately 10(-2) M year-1). Radiative feedback from the star will not only halt its growth but also inhibit the formation of other stars in the same pregalactic object (at least until the first star ends its life, presumably as a supernova). We conclude that at most one massive (M 1 M) metal-free star forms per pregalactic halo, consistent with recent abundance measurements of metal-poor galactic halo stars.
View details for DOI 10.1126/science.1063991
View details for Web of Science ID 000173143100039
View details for PubMedID 11711636
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Photon-conserving radiative transfer around point sources in multidimensional numerical cosmology
ASTROPHYSICAL JOURNAL
1999; 523 (1): 66-71
View details for Web of Science ID 000082673300006
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The SAGA Survey. V. Modeling Satellite Systems around Milky Way-Mass Galaxies with Updated U<sc>niverse</sc>M<sc>achine</sc>
ASTROPHYSICAL JOURNAL
2024; 976 (1)
View details for DOI 10.3847/1538-4357/ad7f4c
View details for Web of Science ID 001357741600001
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Small-scale signatures of primordial non-Gaussianity in k-nearest neighbour cumulative distribution functions
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2024; 534 (3): 1621-1633
View details for DOI 10.1093/mnras/stae2108
View details for Web of Science ID 001328657300012
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The AGORA High-resolution Galaxy Simulations Comparison Project. IV. Halo and Galaxy Mass Assembly in a Cosmological Zoom-in Simulation at <i>z</i> ≤ 2
ASTROPHYSICAL JOURNAL
2024; 968 (2)
View details for DOI 10.3847/1538-4357/ad43de
View details for Web of Science ID 001251667700001
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GUPPY I: a code for reducing the storage requirements of cosmological simulations
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2024; 531 (1): 1870-1883
View details for DOI 10.1093/mnras/stae894
View details for Web of Science ID 001231710600008
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Classical field approximation of ultralight dark matter: Quantum break times, corrections, and decoherence
PHYSICAL REVIEW D
2024; 109 (8)
View details for DOI 10.1103/PhysRevD.109.083527
View details for Web of Science ID 001224283200003
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The AGORA High-resolution Galaxy Simulations Comparison Project. V. Satellite Galaxy Populations in a Cosmological Zoom-in Simulation of a Milky Way-Mass Halo
ASTROPHYSICAL JOURNAL
2024; 964 (2)
View details for DOI 10.3847/1538-4357/ad245b
View details for Web of Science ID 001189207100001
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The <i>AGORA</i> High-resolution Galaxy Simulations Comparison Project. VI. Similarities and Differences in the Circumgalactic Medium
ASTROPHYSICAL JOURNAL
2024; 962 (1)
View details for DOI 10.3847/1538-4357/ad12cb
View details for Web of Science ID 001156722400001
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Robust cosmological inference from non-linear scales with k-th nearest neighbour statistics
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2023; 527 (2): 1993-2009
View details for DOI 10.1093/mnras/stad3359
View details for Web of Science ID 001127751100045
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Simulating the UniverseThe Universe in a Box: Simulations and the Quest to Code the Cosmos Andrew Pontzen Riverhead Books, 2023. 272 pp.
Science (New York, N.Y.)
2023; 381 (6655): 276
Abstract
An accessible introduction to computational cosmology offers fodder for profound reflection.
View details for DOI 10.1126/science.adi4682
View details for PubMedID 37471543
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2D k-th nearest neighbour statistics: a highly informative probe of galaxy clustering
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2023; 522 (3): 3935-3947
View details for DOI 10.1093/mnras/stad1275
View details for Web of Science ID 000992509900016
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Computational fluid dynamics with the coupled discrete unified gas kinetic scheme (CDUGKS)
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2023; 521 (2): 3186-3200
View details for DOI 10.1093/mnras/stad770
View details for Web of Science ID 001189225900009
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Tracer-field cross-correlations with k-nearest neighbour distributions
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2023; 519 (4): 4856-4868
View details for DOI 10.1093/mnras/stac3813
View details for Web of Science ID 000927906300005
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Full forward model of galaxy clustering statistics with AbacusSummit light cones
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2023; 520 (4): 6283-6298
View details for DOI 10.1093/mnras/stad550
View details for Web of Science ID 000951346200013
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When quantum corrections alter the predictions of classical field theory for scalar field dark matter
PHYSICAL REVIEW D
2022; 106 (10)
View details for DOI 10.1103/PhysRevD.106.103002
View details for Web of Science ID 000886058300012
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Detection of spatial clustering in the 1000 richest SDSS DR8 redMaPPer clusters with nearest neighbor distributions
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2022; 514 (3): 3828-3843
View details for DOI 10.1093/mnras/stac1551
View details for Web of Science ID 000817616600010
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Single classical field description of interacting scalar fields
PHYSICAL REVIEW D
2022; 105 (3)
View details for DOI 10.1103/PhysRevD.105.036012
View details for Web of Science ID 000761170800003
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Modelling nearest neighbour distributions of biased tracers using hybrid effective field theory
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2022; 511 (2): 2765-2781
View details for DOI 10.1093/mnras/stac193
View details for Web of Science ID 000767860100017
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Self-similarity of k-nearest neighbour distributions in scale-free simulations
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2022; 509 (2): 2281-2288
View details for DOI 10.1093/mnras/stab3160
View details for Web of Science ID 000728381700051
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Field moment expansion method for interacting bosonic systems
PHYSICAL REVIEW D
2021; 104 (8)
View details for DOI 10.1103/PhysRevD.104.083007
View details for Web of Science ID 000704656000002
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The AGORA High-resolution Galaxy Simulations Comparison Project. III. Cosmological Zoom-in Simulation of a Milky Way-mass Halo
ASTROPHYSICAL JOURNAL
2021; 917 (2)
View details for DOI 10.3847/1538-4357/ac088a
View details for Web of Science ID 000685769800001
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Cosmological cross-correlations and nearest neighbour distributions
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2021; 504 (2): 2911-2923
View details for DOI 10.1093/mnras/stab961
View details for Web of Science ID 000659453800095
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First Star Formation in the Presence of Primordial Magnetic Fields
ASTROPHYSICAL JOURNAL LETTERS
2021; 909 (2)
View details for DOI 10.3847/2041-8213/abe8dd
View details for Web of Science ID 000627727800001
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Nearest neighbour distributions: New statistical measures for cosmological clustering
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2021; 500 (4): 5479–99
View details for DOI 10.1093/mnras/staa3604
View details for Web of Science ID 000606297700081
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Investigating the use of field solvers for simulating classical systems
PHYSICAL REVIEW D
2020; 101 (4)
View details for DOI 10.1103/PhysRevD.101.043011
View details for Web of Science ID 000513575900004
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High-redshift Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes: Stellar Feedback and Quasar Growth
ASTROPHYSICAL JOURNAL
2019; 887 (2)
View details for DOI 10.3847/1538-4357/ab510b
View details for Web of Science ID 000506012000014
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BAM: bias assignment method to generate mock catalogues
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2019; 483 (1): L58–L63
View details for DOI 10.1093/mnrasl/sly220
View details for Web of Science ID 000482178200012
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Reducing noise in cosmological N-body simulations with neutrinos
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
2018
View details for DOI 10.1088/1475-7516/2018/09/028
View details for Web of Science ID 000444908400005
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A new method for analyzing and visualizing plasma simulations using a phase-space tessellation
PHYSICS OF PLASMAS
2018; 25 (7)
View details for DOI 10.1063/1.5037348
View details for Web of Science ID 000440589100010
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Comparing fully general relativistic and Newtonian calculations of structure formation
PHYSICAL REVIEW D
2018; 97 (4)
View details for DOI 10.1103/PhysRevD.97.043509
View details for Web of Science ID 000424904800006
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Tracing the cosmic web
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2018; 473 (1): 1195–1217
View details for DOI 10.1093/mnras/stx1976
View details for Web of Science ID 000415653600090
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Ab Initio Simulations of a Supernova-driven Galactic Dynamo in an Isolated Disk Galaxy
ASTROPHYSICAL JOURNAL
2017; 843 (2)
View details for DOI 10.3847/1538-4357/aa799f
View details for Web of Science ID 000405278700013
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GRACKLE: a chemistry and cooling library for astrophysics
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2017; 466 (2): 2217-2234
View details for DOI 10.1093/mnras/stw3291
View details for Web of Science ID 000398284600069
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Particle acceleration in laser-driven magnetic reconnection
PHYSICS OF PLASMAS
2017; 24 (4)
View details for DOI 10.1063/1.4978627
View details for Web of Science ID 000400390700012
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Doppler effect on indirect detection of dark matter using dark matter only simulations
PHYSICAL REVIEW D
2017; 95 (6)
View details for DOI 10.1103/PhysRevD.95.063012
View details for Web of Science ID 000401982000001
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THE AGORA HIGH-RESOLUTION GALAXY SIMULATIONS COMPARISON PROJECT. II. ISOLATED DISK TEST
ASTROPHYSICAL JOURNAL
2016; 833 (2)
View details for DOI 10.3847/1538-4357/833/2/202
View details for Web of Science ID 000391169600077
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Voids in cosmological simulations over cosmic time
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2016; 458 (4): 4431-4442
View details for DOI 10.1093/mnras/stw615
View details for Web of Science ID 000375799500080
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Nonthermal Electron Energization from Magnetic Reconnection in Laser-Driven Plasmas.
Physical review letters
2016; 116 (9): 095003-?
Abstract
The possibility of studying nonthermal electron energization in laser-driven plasma experiments of magnetic reconnection is studied using two- and three-dimensional particle-in-cell simulations. It is demonstrated that nonthermal electrons with energies more than an order of magnitude larger than the initial thermal energy can be produced in plasma conditions currently accessible in the laboratory. Electrons are accelerated by the reconnection electric field, being injected at varied distances from the X points, and in some cases trapped in plasmoids, before escaping the finite-sized system. Trapped electrons can be further energized by the electric field arising from the motion of the plasmoid. This acceleration gives rise to a nonthermal electron component that resembles a power-law spectrum, containing up to ∼8% of the initial energy of the interacting electrons and ∼24% of the initial magnetic energy. Estimates of the maximum electron energy and of the plasma conditions required to observe suprathermal electron acceleration are provided, paving the way for a new platform for the experimental study of particle acceleration induced by reconnection.
View details for DOI 10.1103/PhysRevLett.116.095003
View details for PubMedID 26991182
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Simplex-in-cell technique for collisionless plasma simulations
JOURNAL OF COMPUTATIONAL PHYSICS
2016; 304: 231-251
View details for DOI 10.1016/j.jcp.2015.10.017
View details for Web of Science ID 000365041900010
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The properties of cosmic velocity fields
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2015; 454 (4): 3920-3937
View details for DOI 10.1093/mnras/stv2179
View details for Web of Science ID 000368001600048
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An exact general remeshing scheme applied to physically conservative voxelization
JOURNAL OF COMPUTATIONAL PHYSICS
2015; 297: 340-356
View details for DOI 10.1016/j.jcp.2015.05.022
View details for Web of Science ID 000357541900020
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COLD ACCRETION IN EARLY GALAXY FORMATION AND ITS Ly alpha SIGNATURES
ASTROPHYSICAL JOURNAL
2015; 801 (1)
View details for DOI 10.1088/0004-637X/801/1/52
View details for Web of Science ID 000350488700052
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Towards noiseless gravitational lensing simulations
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2014; 444 (3): 2925-2937
View details for DOI 10.1093/mnras/stu1608
View details for Web of Science ID 000343399600070
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The birth of a galaxy - III. Propelling reionization with the faintest galaxies
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2014; 442 (3): 2560-2579
View details for DOI 10.1093/mnras/stu979
View details for Web of Science ID 000339924300051
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Escape of Ly alpha and continuum photons from star-forming galaxies
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2014; 440 (1): 776-786
View details for DOI 10.1093/mnras/stu299
View details for Web of Science ID 000334691900061
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REIONIZATION HISTORIES OF MILKY WAY MASS HALOS
ASTROPHYSICAL JOURNAL
2014; 785 (2)
View details for DOI 10.1088/0004-637X/785/2/134
View details for Web of Science ID 000335736800053
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THE AGORA HIGH-RESOLUTION GALAXY SIMULATIONS COMPARISON PROJECT
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
2014; 210 (1)
View details for DOI 10.1088/0067-0049/210/1/14
View details for Web of Science ID 000331237400005
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DWARF GALAXIES WITH IONIZING RADIATION FEEDBACK. II. SPATIALLY RESOLVED STAR FORMATION RELATION
ASTROPHYSICAL JOURNAL
2013; 779 (1)
View details for DOI 10.1088/0004-637X/779/1/8
View details for Web of Science ID 000328160100008
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DWARF GALAXIES WITH IONIZING RADIATION FEEDBACK. I. ESCAPE OF IONIZING PHOTONS
ASTROPHYSICAL JOURNAL
2013; 775 (2)
View details for DOI 10.1088/0004-637X/775/2/109
View details for Web of Science ID 000324734400029
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Small-scale primordial magnetic fields and anisotropies in the cosmic microwave background radiation
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
2013
View details for DOI 10.1088/1475-7516/2013/10/050
View details for Web of Science ID 000326979500050
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How closely do baryons follow dark matter on large scales?
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2013; 434 (2): 1756-1764
View details for DOI 10.1093/mnras/stt1135
View details for Web of Science ID 000323638200065
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Single-Pass GPU-Raycasting for Structured Adaptive Mesh Refinement Data
SPIE Conference on Visualization and Data Analysis (VDA)
SPIE-INT SOC OPTICAL ENGINEERING. 2013
View details for DOI 10.1117/12.2008552
View details for Web of Science ID 000325425900008
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A Novel Approach to Visualizing Dark Matter Simulations
IEEE TRANSACTIONS ON VISUALIZATION AND COMPUTER GRAPHICS
2012; 18 (12): 2078-2087
Abstract
In the last decades cosmological N-body dark matter simulations have enabled ab initio studies of the formation of structure in the Universe. Gravity amplified small density fluctuations generated shortly after the Big Bang, leading to the formation of galaxies in the cosmic web. These calculations have led to a growing demand for methods to analyze time-dependent particle based simulations. Rendering methods for such N-body simulation data usually employ some kind of splatting approach via point based rendering primitives and approximate the spatial distributions of physical quantities using kernel interpolation techniques, common in SPH (Smoothed Particle Hydrodynamics)-codes. This paper proposes three GPU-assisted rendering approaches, based on a new, more accurate method to compute the physical densities of dark matter simulation data. It uses full phase-space information to generate a tetrahedral tessellation of the computational domain, with mesh vertices defined by the simulation's dark matter particle positions. Over time the mesh is deformed by gravitational forces, causing the tetrahedral cells to warp and overlap. The new methods are well suited to visualize the cosmic web. In particular they preserve caustics, regions of high density that emerge, when several streams of dark matter particles share the same location in space, indicating the formation of structures like sheets, filaments and halos. We demonstrate the superior image quality of the new approaches in a comparison with three standard rendering techniques for N-body simulation data.
View details for Web of Science ID 000310143100010
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A Novel Approach to Visualizing Dark Matter Simulations.
IEEE transactions on visualization and computer graphics
2012; 18 (12): 2078-2087
Abstract
In the last decades cosmological N-body dark matter simulations have enabled ab initio studies of the formation of structure in the Universe. Gravity amplified small density fluctuations generated shortly after the Big Bang, leading to the formation of galaxies in the cosmic web. These calculations have led to a growing demand for methods to analyze time-dependent particle based simulations. Rendering methods for such N-body simulation data usually employ some kind of splatting approach via point based rendering primitives and approximate the spatial distributions of physical quantities using kernel interpolation techniques, common in SPH (Smoothed Particle Hydrodynamics)-codes. This paper proposes three GPU-assisted rendering approaches, based on a new, more accurate method to compute the physical densities of dark matter simulation data. It uses full phase-space information to generate a tetrahedral tessellation of the computational domain, with mesh vertices defined by the simulation's dark matter particle positions. Over time the mesh is deformed by gravitational forces, causing the tetrahedral cells to warp and overlap. The new methods are well suited to visualize the cosmic web. In particular they preserve caustics, regions of high density that emerge, when several streams of dark matter particles share the same location in space, indicating the formation of structures like sheets, filaments and halos. We demonstrate the superior image quality of the new approaches in a comparison with three standard rendering techniques for N-body simulation data.
View details for DOI 10.1109/TVCG.2012.187
View details for PubMedID 26357114
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The birth of a galaxy - II. The role of radiation pressure
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2012; 427 (1): 311-326
View details for DOI 10.1111/j.1365-2966.2012.21809.x
View details for Web of Science ID 000310675400022
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WERE PROGENITORS OF LOCAL L* GALAXIES Ly alpha EMITTERS AT HIGH REDSHIFT?
ASTROPHYSICAL JOURNAL
2012; 754 (2)
View details for DOI 10.1088/0004-637X/754/2/118
View details for Web of Science ID 000306666700039
-
ART2: coupling Ly alpha line and multi-wavelength continuum radiative transfer
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2012; 424 (2): 884-901
View details for DOI 10.1111/j.1365-2966.2012.21228.x
View details for Web of Science ID 000306356800007
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THE EFFECT OF ABSORPTION SYSTEMS ON COSMIC REIONIZATION
ASTROPHYSICAL JOURNAL
2012; 747 (2)
View details for DOI 10.1088/0004-637X/747/2/126
View details for Web of Science ID 000302856400042
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THE BIRTH OF A GALAXY: PRIMORDIAL METAL ENRICHMENT AND STELLAR POPULATIONS
ASTROPHYSICAL JOURNAL
2012; 745 (1)
View details for DOI 10.1088/0004-637X/745/1/50
View details for Web of Science ID 000300316600050
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Interactive Stereoscopic Visualization of Large-Scale Astrophysical Simulations
Conference on Stereoscopic Displays and Applications XXIII (SD and A)/IS and T/SPIE Electronic Imaging - Science and Technology Symposium
SPIE-INT SOC OPTICAL ENGINEERING. 2012
View details for DOI 10.1117/12.909258
View details for Web of Science ID 000302558300091
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Turbulence and Small Scale Dynamo Action in Population III Star Formation
Conference on FIRST STARS IV - From Hayashi to the Future
AMER INST PHYSICS. 2012: 87–90
View details for DOI 10.1063/1.4754334
View details for Web of Science ID 000313272200013
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The Imprint of Pop III Stars on the First Galaxies
Conference on FIRST STARS IV - From Hayashi to the Future
AMER INST PHYSICS. 2012: 123–128
View details for DOI 10.1063/1.4754341
View details for Web of Science ID 000313272200020
- Cold accretion in early galaxy formation and its Lyman-alpha signatures The Astrophysical Journal 2012
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Investigation of Nitrogen and Carbon Co-implantation under Room Temperature and Cryo-condition
19th International Conference on Ion Implantation Technology (IIT)
AMER INST PHYSICS. 2012: 87–90
View details for DOI 10.1063/1.4766496
View details for Web of Science ID 000312160700019
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Magnetic Fields and Angular Momentum in Population III Star Formation
Conference on FIRST STARS IV - From Hayashi to the Future
AMER INST PHYSICS. 2012: 77–80
View details for DOI 10.1063/1.4754332
View details for Web of Science ID 000313272200011
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GALAXY FORMATION WITH SELF-CONSISTENTLY MODELED STARS AND MASSIVE BLACK HOLES. I. FEEDBACK-REGULATED STAR FORMATION AND BLACK HOLE GROWTH
ASTROPHYSICAL JOURNAL
2011; 738 (1)
View details for DOI 10.1088/0004-637X/738/1/54
View details for Web of Science ID 000294015500054
-
COMPARING NUMERICAL METHODS FOR ISOTHERMAL MAGNETIZED SUPERSONIC TURBULENCE
ASTROPHYSICAL JOURNAL
2011; 737 (1)
View details for DOI 10.1088/0004-637X/737/1/13
View details for Web of Science ID 000293332200013
-
Multi-scale initial conditions for cosmological simulations
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2011; 415 (3): 2101-2121
View details for DOI 10.1111/j.1365-2966.2011.18820.x
View details for Web of Science ID 000294173900010
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ENZO+MORAY: radiation hydrodynamics adaptive mesh refinement simulations with adaptive ray tracing
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2011; 414 (4): 3458-3491
View details for DOI 10.1111/j.1365-2966.2011.18646.x
View details for Web of Science ID 000293178600053
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rpSPH: a novel smoothed particle hydrodynamics algorithm
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2011; 413 (1): 271-285
View details for DOI 10.1111/j.1365-2966.2010.18133.x
View details for Web of Science ID 000289525000021
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The first stars, as seen by supercomputers
PHYSICS TODAY
2011; 64 (4): 51-56
View details for Web of Science ID 000289397900017
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Extremely metal-poor stars in classical dwarf spheroidal galaxies: Fornax, Sculptor, and Sextans (vol 524, pg A58, 2010)
ASTRONOMY & ASTROPHYSICS
2011; 527
View details for DOI 10.1051/0004-6361/201014733e
View details for Web of Science ID 000287484100001
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EFFECTS OF VARYING THE THREE-BODY MOLECULAR HYDROGEN FORMATION RATE IN PRIMORDIAL STAR FORMATION
ASTROPHYSICAL JOURNAL
2011; 726 (1)
View details for DOI 10.1088/0004-637X/726/1/55
View details for Web of Science ID 000285411300055
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yt: A MULTI-CODE ANALYSIS TOOLKIT FOR ASTROPHYSICAL SIMULATION DATA
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
2011; 192 (1)
View details for DOI 10.1088/0067-0049/192/1/9
View details for Web of Science ID 000285710500009
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HIGH-ENTROPY POLAR REGIONS AROUND THE FIRST PROTOSTARS
ASTROPHYSICAL JOURNAL LETTERS
2010; 725 (2): L140-L144
View details for DOI 10.1088/2041-8205/725/2/L140
View details for Web of Science ID 000285051400007
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Extremely metal-poor stars in classical dwarf spheroidal galaxies: Fornax, Sculptor, and Sextans
ASTRONOMY & ASTROPHYSICS
2010; 524
View details for DOI 10.1051/0004-6361/201014733
View details for Web of Science ID 000284625300033
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Adaptive mesh fluid simulations on GPU
NEW ASTRONOMY
2010; 15 (7): 581-589
View details for DOI 10.1016/j.newast.2009.10.002
View details for Web of Science ID 000278639200001
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LOWERING THE CHARACTERISTIC MASS OF CLUSTER STARS BY MAGNETIC FIELDS AND OUTFLOW FEEDBACK
ASTROPHYSICAL JOURNAL LETTERS
2010; 720 (1): L26-L30
View details for DOI 10.1088/2041-8205/720/1/L26
View details for Web of Science ID 000281610100006
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THE IMPACT OF INHOMOGENEOUS REIONIZATION ON THE SATELLITE GALAXY POPULATION OF THE MILKY WAY
ASTROPHYSICAL JOURNAL
2010; 710 (1): 408-420
View details for DOI 10.1088/0004-637X/710/1/408
View details for Web of Science ID 000273850800035
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Computational Eulerian hydrodynamics and Galilean invariance
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2010; 401 (4): 2463-2476
View details for DOI 10.1111/j.1365-2966.2009.15823.x
View details for Web of Science ID 000273687800025
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Visualizing the Reionization of the Universe on Programmable Graphics Hardware
4th International Conference on Numerical Modeling of Space Plasma Flows Astronum 2009
ASTRONOMICAL SOC PACIFIC. 2010: 311–316
View details for Web of Science ID 000287839100046
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Population III Binary Formation
1st International Conference on Stars and Galaxies: Challenges for the Next Decade
AMER INST PHYSICS. 2010: 41–44
View details for Web of Science ID 000288517300006
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CONNECTING REIONIZATION TO THE LOCAL UNIVERSE
ASTROPHYSICAL JOURNAL LETTERS
2009; 703 (2): L167-L171
View details for DOI 10.1088/0004-637X/703/2/L167
View details for Web of Science ID 000270014600016
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ACCRETION ONTO THE FIRST STELLAR-MASS BLACK HOLES
ASTROPHYSICAL JOURNAL LETTERS
2009; 701 (2): L133-L137
View details for DOI 10.1088/0004-637X/701/2/L133
View details for Web of Science ID 000268867900016
-
Resolving the formation of protogalaxies. III. Feedback from the first stars
ASTROPHYSICAL JOURNAL
2008; 685 (1): 40-56
View details for Web of Science ID 000259314200004
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Uncertainties in H-2 and HD chemistry and cooling and their role in early structure formation
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2008; 388 (4): 1627-1651
View details for DOI 10.1111/j.1365-2966.2008.13224.x
View details for Web of Science ID 000258222800013
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Relativistic hydrodynamic flows using spatial and temporal adaptive structured mesh refinement
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
2008; 176 (2): 467-483
View details for Web of Science ID 000257672200009
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Metal cooling in simulations of cosmic structure formation
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2008; 385 (3): 1443-1454
View details for DOI 10.1111/j.1365-2966.2008.12922.x
View details for Web of Science ID 000254604600024
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Dynamical treatment of virialization heating in galaxy formation
ASTROPHYSICAL JOURNAL
2008; 672 (2): 752-756
View details for Web of Science ID 000253454100002
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Towards forming a primordial protostar in a cosmological AMR simulation
International Conference on First Stars III
AMER INST PHYSICS. 2008: 16–20
View details for Web of Science ID 000254472200002
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The Star Formation History and Stellar Population Structures in the Sextans Dwarf Spheroidal Galaxy
International Conference on Panoramic Views of Galaxy Formation and Evolution
ASTRONOMICAL SOC PACIFIC. 2008: 469–470
View details for Web of Science ID 000262978800123
- Conference Summary Proceedings of the First Stars III edited by O'Shea, B. W., Heger, A., Abel, T. 2008
-
Black hole remnants of the first stars
International Conference on First Stars III
AMER INST PHYSICS. 2008: 432–434
View details for Web of Science ID 000254472200096
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The Biermann battery and early structure formation
International Conference on First Stars III
AMER INST PHYSICS. 2008: 39–41
View details for Web of Science ID 000254472200008
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How the first stars shaped the first galaxies
International Conference on First Stars III
AMER INST PHYSICS. 2008: 400–404
View details for Web of Science ID 000254472200090
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Galaxy evolution with adaptive mesh refinement
International Conference on First Stars III
AMER INST PHYSICS. 2008: 429–431
View details for Web of Science ID 000254472200095
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Simulating stellar birth and death
International Conference on First Stars III
AMER INST PHYSICS. 2008: 507–509
View details for Web of Science ID 000254472200111
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Suppression of H-2 cooling in the ultraviolet background
ASTROPHYSICAL JOURNAL
2007; 671 (2): 1559-1567
View details for Web of Science ID 000253331600039
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Dynamical expansion of HII regions from ultracompact to compact sizes in turbulent, self-gravitating molecular clouds
ASTROPHYSICAL JOURNAL
2007; 668 (2): 980-992
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Supermassive black hole growth and merger rates from cosmological N-body simulations
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2007; 380 (4): 1533-1540
View details for DOI 10.1111/j.1365-2966.2007.12162.x
View details for Web of Science ID 000250010200019
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Quasar HII regions during cosmic reionization
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2007; 380 (1): L30-L34
View details for DOI 10.1111/j.1745-3933.2007.00342.x
View details for Web of Science ID 000249422900007
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Resolving the formation of protogalaxies. I. virialization
ASTROPHYSICAL JOURNAL
2007; 665 (2): 899-910
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The first generation of stars in the Lambda cold dark matter cosmology
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2007; 378 (2): 449-468
View details for DOI 10.1111/j.1365-2966.2007.11814.x
View details for Web of Science ID 000247262600005
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The HII region of a primordial star
ASTROPHYSICAL JOURNAL
2007; 659 (2): L87-L90
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Numerical simulations of the metallicity distribution in dwarf spheroidal galaxies
CRAL International Conference on Chemodynamics - From First Stars to Local Galaxies
E D P SCIENCES. 2007: 15–20
View details for DOI 10.1051/eas:2007051
View details for Web of Science ID 000247414600002
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Formation of primordial stars in a Lambda CDM universe
ASTROPHYSICAL JOURNAL
2006; 652 (1): 6-25
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The role of primordial kicks on black hole merger rates
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2006; 372 (4): 1540-1548
View details for DOI 10.1111/j.1365-2966.2006.11013.x
View details for Web of Science ID 000241626100008
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A new view of the Dwarf spheroidal satellites of the Milky Way from VLT FLAMES: Where are the very metal-poor stars?
ASTROPHYSICAL JOURNAL
2006; 651 (2): L121-L124
View details for Web of Science ID 000241825100011
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The DART imaging and CaT survey of the Fornax dwarf spheroidal galaxy
ASTRONOMY & ASTROPHYSICS
2006; 459 (2): 423-U148
View details for DOI 10.1051/0004-6361:20065720
View details for Web of Science ID 000241822800012
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An excursion set model of the cosmic web: The abundance of sheets, filaments, and halos
ASTROPHYSICAL JOURNAL
2006; 645 (2): 783-791
View details for Web of Science ID 000239053900001
- GPU-Assisted Raycasting for Cosmological Adaptive Mesh Refinement Simulations Volume Graphics 2006; 103
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The formation of primordial luminous objects
SIGRAV School on the Joint Evolution of Black Holes and Galaxies
CRC PRESS-TAYLOR & FRANCIS GROUP. 2006: 239–289
View details for Web of Science ID 000235628100005
- Numerical simulations of the metallicity distribution in dwarf spheroidal galaxies edited by Emsellem , Wozniak , Massacrier , Gonzalez , Devriendt , Champavert 2006
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The number of supernovae from primordial stars in the universe
ASTROPHYSICAL JOURNAL
2005; 629 (2): 615-624
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Forming a primordial star in a relic HII region
ASTROPHYSICAL JOURNAL
2005; 628 (1): L5-L8
View details for Web of Science ID 000230720800002
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Introducing Enzo, an AMR cosmology application
Workshop on Adaptive Mesh Refinement Methods
SPRINGER-VERLAG BERLIN. 2005: 341–350
View details for Web of Science ID 000226971600024
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Two distinct ancient components in the Sculptor dwarf spheroidal galaxy: First results from the dwarf abundances and radial velocities team
ASTROPHYSICAL JOURNAL
2004; 617 (2): L119-L122
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Radiation hydrodynamic evolution of primordial HII regions
ASTROPHYSICAL JOURNAL
2004; 610 (1): 14-22
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Initial ionization of compressible turbulence
ASTROPHYSICAL JOURNAL
2004; 610 (1): 339-350
View details for Web of Science ID 000222699700032
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Cosmic reionization by stellar sources: population III stars
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2004; 350 (1): 47-65
View details for DOI 10.1111/j.1365-2966.2004.07636.x
View details for Web of Science ID 000220979300010
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Detectability of long gamma-ray burst afterglows from very high redshifts
ASTROPHYSICAL JOURNAL
2004; 604 (2): 508-520
View details for Web of Science ID 000220522300004
-
Fragmentation and the formation of primordial protostars: the possible role of collision-induced emission
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2004; 348 (3): 1019-1034
View details for DOI 10.1111/j.1365-2966.2004.07422.x
View details for Web of Science ID 000220160700030
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Detectability of long GRB afterglows from very high redshifts
Gamma-Ray Burst Symposium
AMER INST PHYSICS. 2004: 518–521
View details for Web of Science ID 000224719700109
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The influence of supershells and galactic outflows on the escape of ionizing radiation from dwarf starburst galaxies
ASTROPHYSICAL JOURNAL
2003; 599 (1): 50-69
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-
The angular momentum of gas in protogalaxies - II. The impact of pre-heating
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2003; 346 (1): 177-185
View details for Web of Science ID 000186533100019
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Cosmic reionization by stellar sources: Population II stars
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2003; 344 (2): 607-624
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Simulations of early structure formation: Primordial gas clouds
ASTROPHYSICAL JOURNAL
2003; 592 (2): 645-663
View details for Web of Science ID 000184408100001
-
Numerical simulations of high-redshift star formation in dwarf galaxies
ASTROPHYSICAL JOURNAL
2003; 587 (1): 13-24
View details for Web of Science ID 000182105600002
-
The nature of the ionizing background at z approximate to 2.5-5
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2003; 340 (2): 473-484
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Effects of a soft X-ray background on structure formation at high redshift
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2003; 338 (2): 273-286
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-
The number of supernovae from primordial stars in the universe
13th Annual Astrophysics Conference
AMER INST PHYSICS. 2003: 97–100
View details for Web of Science ID 000183411200011
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The angular momentum of gas in protogalaxies. I. Implications for the formation of disk galaxies
ASTROPHYSICAL JOURNAL
2002; 576 (1): 21-35
View details for Web of Science ID 000177589100002
-
Cosmological hydrogen reionization with three-dimensional radiative transfer
ASTROPHYSICAL JOURNAL
2002; 572 (2): 695-704
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-
The epoch of helium reionization
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2002; 332 (3): 601-616
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Adaptive ray tracing for radiative transfer around point sources
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2002; 330 (3): L53-L56
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Radio foregrounds for the 21 centimeter tomography of the neutral intergalactic medium at high redshifts
ASTROPHYSICAL JOURNAL
2002; 564 (2): 576-580
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- Effects of a Soft X-ray Background on Structure Formation at High Redshift The Astrophysical Journal 2002; 540
-
The initial mode of star formation
Workshop on Modes of Star Formation and the Origin of Field Populations
ASTRONOMICAL SOC PACIFIC. 2002: 213–222
View details for Web of Science ID 000180752500031
- The Basic Building Blocks of Galaxies edited by Sauvage, M., Stasinska, G., Vigroux, L., Schaerer, D., Madden, S. 2002
-
Evolution and explosion of very massive primordial stars
MPA/ESO/MPE/USM Joint Astronomy Conference on Lighthouses of the Universe
SPRINGER-VERLAG BERLIN. 2002: 369–375
View details for Web of Science ID 000179560500057
-
Simulating reionization in numerical cosmology
NEW ASTRONOMY
2001; 6 (6): 359-379
View details for Web of Science ID 000170294900002
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Multi-dimensional cosmological radiative transfer with a Variable Eddington Tensor formalism
NEW ASTRONOMY
2001; 6 (7): 437-455
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-
Photon consumption in minihalos during cosmological reionization
ASTROPHYSICAL JOURNAL
2001; 551 (2): 599-607
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-
Simulations of pregalactic structure formation with radiative feedback
ASTROPHYSICAL JOURNAL
2001; 548 (2): 509-521
View details for Web of Science ID 000167204900001
-
Forming the first star in the Universe
International Meeting on Physics of Galaxy Formation
ASTRONOMICAL SOC PACIFIC. 2001: 129–136
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-
The formation and fragmentation of primordial molecular clouds
ASTROPHYSICAL JOURNAL
2000; 540 (1): 39-44
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-
The radiative feedback of the first cosmological objects
ASTROPHYSICAL JOURNAL
2000; 534 (1): 11-24
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-
Intergalactic H-2 photodissociation and the soft ultraviolet background produced by population III objects
ASTROPHYSICAL JOURNAL
2000; 533 (2): 594-600
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- Three Dimensional Radiative Transfer in Numerical Cosmology edited by Franco, J. 2000
-
First structure formation and the first stars
MPA/ESO Workshop on the First Stars
SPRINGER-VERLAG BERLIN. 2000: 250–260
View details for Web of Science ID 000088721200046
-
The role of H-2 molecules in cosmological structure formation
International Conference on H(2) in Space
CAMBRIDGE UNIV PRESS. 2000: 237–246
View details for Web of Science ID 000173071700035
- The First Stars edited by Weiss, A., Abel, T., Hill, V. 2000
-
Radiative transfer effects during photoheating of the intergalactic medium
ASTROPHYSICAL JOURNAL
1999; 520 (1): L13-L16
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-
Absorption-line signatures of gas in dark matter minihalos
ASTRONOMICAL JOURNAL
1999; 117 (5): 2063-2076
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- From Cosmological Initial Conditions to Primordial Protostellar Cloud Cores edited by Börner, G., Mo, H. 1999
-
From cosmological initial conditions to primordial protostellar cloud cores
9th Astrophysics Conference
AMER INST PHYSICS. 1999: 58–62
View details for Web of Science ID 000080797800006
- First Structure Formation Evolution of Large Scale Structure: From Recombination to Garching edited by Banday, T., Sheth, R. K., Costa, L. N. 1999
-
First structure formation. I. Primordial star-forming regions in hierarchical models
ASTROPHYSICAL JOURNAL
1998; 508 (2): 518-529
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-
First structure formation. II. Cosmic string plus hot dark matter models
ASTROPHYSICAL JOURNAL
1998; 508 (2): 530-534
View details for Web of Science ID 000077780500007
-
A "minihalo" model for the Lyman limit absorption systems at high redshift
ASTROPHYSICAL JOURNAL
1998; 494 (2): L151-L154
View details for Web of Science ID 000072292600006
- Simulating First Structure Formation H2 in the early Universe edited by Palla, F., Galli, D., Corbelli, E. Memorie Della Societa Astronomica Italiana. 1998
-
How small were the first cosmological objects?
ASTROPHYSICAL JOURNAL
1997; 474 (1): 1-12
View details for Web of Science ID A1997WA68200001
-
Modeling primordial gas in numerical cosmology
NEW ASTRONOMY
1997; 2 (3): 181-207
View details for Web of Science ID A1997XJ23200001
-
Cosmological hydrodynamics with multi-species chemistry and nonequilibrium ionization and cooling
NEW ASTRONOMY
1997; 2 (3): 209-224
View details for Web of Science ID A1997XJ23200002
-
Primordial star forming regions in a CDM universe
7th Annual October Astrophysics Conference on Star Formation, Near and Far
AMER INST PHYSICS. 1997: 329–33
View details for Web of Science ID A1997BJ23B00054