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Professor Adrian Jenkins' Outputs (138)

Star Stream Velocity Distributions in Cold Dark Matter and Warm Dark Matter Galactic Halos (2024)
Journal Article
Carlberg, R. G., Jenkins, A., Frenk, C. S., & Cooper, A. P. (2024). Star Stream Velocity Distributions in Cold Dark Matter and Warm Dark Matter Galactic Halos. The Astrophysical Journal, 975(1), Article 135. https://doi.org/10.3847/1538-4357/ad7b35

The dark matter subhalos orbiting in a galactic halo perturb the orbits of stars in thin stellar streams. Over time, the random velocities in the streams develop non-Gaussian wings. The rate of velocity increase is approximately a random walk at a ra... Read More about Star Stream Velocity Distributions in Cold Dark Matter and Warm Dark Matter Galactic Halos.

The mass accretion history of dark matter haloes down to Earth mass (2023)
Journal Article
Liu, Y., Gao, L., Bose, S., Frenk, C. S., Jenkins, A., Springel, V., Wang, J., White, S. D. M., & Zheng, H. (2023). The mass accretion history of dark matter haloes down to Earth mass. Monthly Notices of the Royal Astronomical Society, 527(4), 11740-11750. https://doi.org/10.1093/mnras/stae003

We take advantage of the unprecedented dynamical range provided by the ‘Cosmic-Zoom’ project to study the mass accretion history (MAH) of present-day dark matter haloes o v er the entire mass range present in the Lambda cold dark matter paradigm when... Read More about The mass accretion history of dark matter haloes down to Earth mass.

FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning. (2023)
Journal Article
Kugel, R., Schaye, J., Schaller, M., Helly, J. C., Braspenning, J., Elbers, W., …Vernon, I. (2023). FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning. Monthly Notices of the Royal Astronomical Society, 526(4), 6103-6127. https://doi.org/10.1093/mnras/stad2540

To fully take advantage of the data provided by large-scale structure surveys, we need to quantify the potential impact of baryonic effects, such as feedback from active galactic nuclei (AGN) and star formation, on cosmological observables. In simula... Read More about FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning..

Where shadows lie: reconstruction of anisotropies in the neutrino sky (2023)
Journal Article
Elbers, W., Frenk, C. S., Jenkins, A., Li, B., Pascoli, S., Jasche, J., …Springel, V. (2023). Where shadows lie: reconstruction of anisotropies in the neutrino sky. Journal of Cosmology and Astroparticle Physics, 2023(10), Article 010. https://doi.org/10.1088/1475-7516/2023/10/010

The Cosmic Neutrino Background (CNB) encodes a wealth of information, but has not yet been observed directly. To determine the prospects of detection and to study its information content, we reconstruct the phase-space distribution of local relic neu... Read More about Where shadows lie: reconstruction of anisotropies in the neutrino sky.

The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys (2023)
Journal Article
Schaye, J., Kugel, R., Schaller, M., Helly, . J. C., Braspenning, J., Elbers, W., …Nobels, F. S. J. (2023). The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys. Monthly Notices of the Royal Astronomical Society, 526(4), 4978–5020. https://doi.org/10.1093/mnras/stad2419

We introduce the Virgo Consortium’s FLAMINGO suite of hydrodynamical simulations for cosmology and galaxy cluster physics. To ensure the simulations are sufficiently realistic for studies of large-scale structure, the subgrid prescriptions for stella... Read More about The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys.

The Milky Way’s plane of satellites is consistent with ΛCDM (2022)
Journal Article
Sawala, T., Cautun, M., Frenk, C., Helly, J., Jasche, J., Jenkins, A., …Schaller, M. (2023). The Milky Way’s plane of satellites is consistent with ΛCDM. Nature Astronomy, 7(4), 481-491. https://doi.org/10.1038/s41550-022-01856-z

The Milky Way is surrounded by 11 ‘classical’ satellite galaxies in a remarkable configuration: a thin plane that is possibly rotationally supported. Such a structure is thought to be highly unlikely to arise in the standard (ΛCDM) cosmological model... Read More about The Milky Way’s plane of satellites is consistent with ΛCDM.

Higher order initial conditions with massive neutrinos (2022)
Journal Article
Elbers, W., Frenk, C. S., Jenkins, A., Li, B., & Pascoli, S. (2022). Higher order initial conditions with massive neutrinos. Monthly Notices of the Royal Astronomical Society, 516(3), https://doi.org/10.1093/mnras/stac2365

The discovery that neutrinos have mass has important consequences for cosmology. The main effect of massive neutrinos is to suppress the growth of cosmic structure on small scales. Such growth can be accurately modelled using cosmological N-body simu... Read More about Higher order initial conditions with massive neutrinos.

SIBELIUS-DARK: a galaxy catalogue of the local volume from a constrained realization simulation (2022)
Journal Article
McAlpine, S., Helly, J. C., Schaller, M., Sawala, T., Lavaux, G., Jasche, J., …Johansson, P. H. (2022). SIBELIUS-DARK: a galaxy catalogue of the local volume from a constrained realization simulation. Monthly Notices of the Royal Astronomical Society, 512(4), 5823-5847. https://doi.org/10.1093/mnras/stac295

We present SIBELIUS-DARK, a constrained realization simulation of the local volume to a distance of 200 Mpc from the Milky Way. SIBELIUS-DARK is the first study of the ‘Simulations Beyond The Local Universe’ (SIBELIUS) project, which has the goal of... Read More about SIBELIUS-DARK: a galaxy catalogue of the local volume from a constrained realization simulation.

The SIBELIUS Project: E Pluribus Unum (2021)
Journal Article
Sawala, T., McAlpine, S., Jasche, J., Lavaux, G., Jenkins, A., Johansson, P. H., & Frenk, C. S. (2022). The SIBELIUS Project: E Pluribus Unum. Monthly Notices of the Royal Astronomical Society, 509(1), 1432-1446. https://doi.org/10.1093/mnras/stab2684

We introduce ‘Simulations Beyond The Local Universe’ (SIBELIUS) that connect the Local Group (LG) to its cosmic environment. We show that introducing hierarchical small-scale perturbations to a density field constrained on large scales by observation... Read More about The SIBELIUS Project: E Pluribus Unum.

Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation (2021)
Journal Article
Grand, R. J., Marinacci, F., Pakmor, R., Simpson, C. M., Kelly, A. J., Gómez, F. A., …White, S. D. (2021). Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation. Geometry & Topology, 507(4), 4953-4967. https://doi.org/10.1093/mnras/stab2492

We investigate the formation of the satellite galaxy population of a Milky Way-mass halo in a very highly resolved magnetohydrodynamic cosmological zoom-in simulation (baryonic mass resolution mb = 800 M⊙⁠). We show that the properties of the central... Read More about Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation.

Constraints on the properties of warm dark matter using the satellite galaxies of the Milky Way (2021)
Journal Article
Newton, O., Leo, M., Cautun, M., Jenkins, A., Frenk, C. S., Lovell, M. R., …Cole, S. (2021). Constraints on the properties of warm dark matter using the satellite galaxies of the Milky Way. Journal of Cosmology and Astroparticle Physics, 2021(08), Article 062. https://doi.org/10.1088/1475-7516/2021/08/062

The satellite galaxies of the Milky Way (MW) are effective probes of the underlying dark matter (DM) substructure, which is sensitive to the nature of the DM particle. In particular, a class of DM models have a power spectrum cut-off on the mass scal... Read More about Constraints on the properties of warm dark matter using the satellite galaxies of the Milky Way.

An optimal non-linear method for simulating relic neutrinos (2021)
Journal Article
Elbers, W., Frenk, C. S., Jenkins, A., Li, B., & Pascoli, S. (2021). An optimal non-linear method for simulating relic neutrinos. Monthly Notices of the Royal Astronomical Society, 507(2), 2614-2631. https://doi.org/10.1093/mnras/stab2260

Cosmology places the strongest current limits on the sum of neutrino masses. Future observations will further improve the sensitivity and this will require accurate cosmological simulations to quantify possible systematic uncertainties and to make pr... Read More about An optimal non-linear method for simulating relic neutrinos.

Indra: a public computationally accessible suite of cosmological N-body simulations (2021)
Journal Article
Falck, B., Wang, J., Jenkins, A., Lemson, G., Medvedev, D., Neyrinck, M. C., & Szalay, A. S. (2021). Indra: a public computationally accessible suite of cosmological N-body simulations. Monthly Notices of the Royal Astronomical Society, 506(2), 2659-2670. https://doi.org/10.1093/mnras/stab1823

Indra is a suite of large-volume cosmological N-body simulations with the goal of providing excellent statistics of the large-scale features of the distribution of dark matter. Each of the 384 simulations is computed with the same cosmological parame... Read More about Indra: a public computationally accessible suite of cosmological N-body simulations.

The origin of X-ray coronae around simulated disc galaxies (2021)
Journal Article
Kelly, A. J., Jenkins, A., & Frenk, C. S. (2021). The origin of X-ray coronae around simulated disc galaxies. Monthly Notices of the Royal Astronomical Society, 502(2), 2934-2951. https://doi.org/10.1093/mnras/stab255

The existence of hot, accreted gaseous coronae around massive galaxies is a long-standing central prediction of galaxy formation models in the ΛCDM cosmology. While observations now confirm that extraplanar hot gas is present around late-type galaxie... Read More about The origin of X-ray coronae around simulated disc galaxies.

Setting the stage: structures from Gaussian random fields (2021)
Journal Article
Sawala, T., Jenkins, A., McAlpine, S., Jasche, J., Lavaux, G., Johansson, P. H., & Frenk, C. S. (2021). Setting the stage: structures from Gaussian random fields. Monthly Notices of the Royal Astronomical Society, 501(4), 4759-4776. https://doi.org/10.1093/mnras/staa3568

We study structure formation in a set of cosmological simulations to uncover the scales in the initial density field that gave rise to the formation of present-day structures. Our simulations share a common primordial power spectrum (here Λ cold dark... Read More about Setting the stage: structures from Gaussian random fields.

A high-resolution cosmological simulation of a strong gravitational lens (2021)
Journal Article
Richings, J., Frenk, C., Jenkins, A., Robertson, A., & Schaller, M. (2021). A high-resolution cosmological simulation of a strong gravitational lens. Monthly Notices of the Royal Astronomical Society, 501(3), 4657-4668. https://doi.org/10.1093/mnras/staa4013

We present a cosmological hydrodynamical simulation of a 1013 M⊙ galaxy group and its environment (out to 10 times the virial radius) carried out using the EAGLE model of galaxy formation. Exploiting a novel technique to increase the resolution of th... Read More about A high-resolution cosmological simulation of a strong gravitational lens.

Universal structure of dark matter haloes over a mass range of 20 orders of magnitude (2020)
Journal Article
Wang, J., Bose, S., Frenk, C., Gao, L., Jenkins, A., Springel, V., & White, S. (2020). Universal structure of dark matter haloes over a mass range of 20 orders of magnitude. Nature, 585(7823), 39-42. https://doi.org/10.1038/s41586-020-2642-9

Cosmological models in which dark matter consists of cold elementary particles predict that the dark halo population should extend to masses many orders of magnitude below those at which galaxies can form1,2,3. Here we report a cosmological simulatio... Read More about Universal structure of dark matter haloes over a mass range of 20 orders of magnitude.

Subhalo destruction in the Apostle and Auriga simulations (2019)
Journal Article
Richings, J., Frenk, C., Jenkins, A., Robertson, A., Fattahi, A., Grand, R. J., …Oman, K. (2020). Subhalo destruction in the Apostle and Auriga simulations. Monthly Notices of the Royal Astronomical Society, 492(4), 5780-5793. https://doi.org/10.1093/mnras/stz3448

N-body simulations make unambiguous predictions for the abundance of substructures within dark matter halos. However, the inclusion of baryons in the simulations changes the picture because processes associated with the presence of a large galaxy in... Read More about Subhalo destruction in the Apostle and Auriga simulations.

No cores in dark matter-dominated dwarf galaxies with bursty star formation histories (2019)
Journal Article
Bose, S., Frenk, C. S., Jenkins, A., Fattahi, A., Gómez, F. A., Grand, R. J., …Springel, V. (2019). No cores in dark matter-dominated dwarf galaxies with bursty star formation histories. Monthly Notices of the Royal Astronomical Society, 486(4), 4790-4804. https://doi.org/10.1093/mnras/stz1168

Measurements of the rotation curves of dwarf galaxies are often interpreted as requiring a constant density core at the centre, at odds with the “cuspy” inner profiles predicted by N-body simulations of cold dark matter (CDM) haloes. It has been sugg... Read More about No cores in dark matter-dominated dwarf galaxies with bursty star formation histories.

The total satellite population of the Milky Way (2018)
Journal Article
Newton, O., Cautun, M., Jenkins, A., Frenk, C. S., & Helly, J. C. (2018). The total satellite population of the Milky Way. Monthly Notices of the Royal Astronomical Society, 479(3), 2853-2870. https://doi.org/10.1093/mnras/sty1085

The total number and luminosity function of the population of dwarf galaxies of the Milky Way (MW) provide important constraints on the nature of the dark matter and on the astrophysics of galaxy formation at low masses. However, only a partial censu... Read More about The total satellite population of the Milky Way.

The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies (2017)
Journal Article
Barnes, D. J., Kay, S. T., Bahé, Y. M., Dalla Vecchia, C., McCarthy, I. G., Schaye, J., …White, S. D. (2017). The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies. Monthly Notices of the Royal Astronomical Society, 471(1), 1088-1106. https://doi.org/10.1093/mnras/stx1647

We introduce the Cluster-EAGLE (C-EAGLE) simulation project, a set of cosmological hydrodynamical zoom simulations of the formation of 30 galaxy clusters in the mass range of 1014 < M200/M⊙ < 1015.4 that incorporates the Hydrangea sample of Bahé et a... Read More about The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies.

The Hydrangea simulations: galaxy formation in and around massive clusters (2017)
Journal Article
Bahé, Y., Barnes, D., Dalla Vecchia, C., Kay, S., White, S., McCarthy, I., …Trayford, J. (2017). The Hydrangea simulations: galaxy formation in and around massive clusters. Monthly Notices of the Royal Astronomical Society, 470(4), 4186-4208. https://doi.org/10.1093/mnras/stx1403

We introduce the Hydrangea simulations, a suite of 24 cosmological hydrodynamic zoom-in simulations of massive galaxy clusters (M200c = 1014–1015.4 M⊙) with baryon particle masses of ∼106 M⊙. Designed to study the impact of the cluster environment on... Read More about The Hydrangea simulations: galaxy formation in and around massive clusters.

Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses (2017)
Journal Article
Campbell, D. J., Frenk, C. S., Jenkins, A., Eke, V. R., Navarro, J. F., Sawala, T., …Theuns, T. (2017). Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses. Monthly Notices of the Royal Astronomical Society, 469(2), 2335-2360. https://doi.org/10.1093/mnras/stx975

The observed stellar kinematics of dispersion-supported galaxies are often used to measure dynamical masses. Recently, several analytical relationships between the stellar line-of-sight velocity dispersion, the projected (2D) or deprojected (3D) half... Read More about Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses.

The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time (2017)
Journal Article
Grand, R., Gómez, F., Marinacci, F., Pakmor, R., Springel, V., Campbell, D., …White, S. (2017). The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time. Monthly Notices of the Royal Astronomical Society, 467(1), 179-207. https://doi.org/10.1093/mnras/stx071

We introduce a suite of 30 cosmological magneto-hydrodynamical zoom simulations of the formation of galaxies in isolated Milky Way mass dark haloes. These were carried out with the moving mesh code arepo, together with a comprehensive model for galax... Read More about The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time.

The redshift evolution of massive galaxy clusters in the MACSIS simulations (2016)
Journal Article
Barnes, D., Kay, S., Henson, M., McCarthy, I., Schaye, J., & Jenkins, A. (2017). The redshift evolution of massive galaxy clusters in the MACSIS simulations. Monthly Notices of the Royal Astronomical Society, 465(1), 213-233. https://doi.org/10.1093/mnras/stw2722

We present the MAssive ClusterS and Intercluster Structures (MACSIS) project, a suite of 390 clusters simulated with baryonic physics that yields realistic massive galaxy clusters capable of matching a wide range of observed properties. MACSIS extend... Read More about The redshift evolution of massive galaxy clusters in the MACSIS simulations.

Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations (2016)
Journal Article
Bose, S., Hellwing, W., Frenk, C., Jenkins, A., Lovell, M., Helly, J., …Gao, L. (2017). Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations. Monthly Notices of the Royal Astronomical Society, 464(4), 4520-4533. https://doi.org/10.1093/mnras/stw2686

We use the Copernicus Complexio (coco) high-resolution N-body simulations to investigate differences in the properties of small-scale structures in the standard cold dark matter (CDM) model and in a model with a cutoff in the initial power spectrum o... Read More about Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations.

The EAGLE simulations of galaxy formation: Public release of halo and galaxy catalogues (2016)
Journal Article
McAlpine, S., Helly, J., Schaller, M., Trayford, J., Qu, Y., Furlong, M., …Lemson, G. (2016). The EAGLE simulations of galaxy formation: Public release of halo and galaxy catalogues. Astronomy and computing, 15, 72-89. https://doi.org/10.1016/j.ascom.2016.02.004

We present the public data release of halo and galaxy catalogues extracted from the eagle suite of cosmological hydrodynamical simulations of galaxy formation. These simulations were performed with an enhanced version of the gadget code that includes... Read More about The EAGLE simulations of galaxy formation: Public release of halo and galaxy catalogues.

Vertical disc heating in Milky Way-sized galaxies in a cosmological context (2016)
Journal Article
Grand, R., Springel, V., Gómez, F., Marinacci, F., Pakmor, R., Campbell, D., & Jenkins, A. (2016). Vertical disc heating in Milky Way-sized galaxies in a cosmological context. Monthly Notices of the Royal Astronomical Society, 459(1), 199-219. https://doi.org/10.1093/mnras/stw601

Vertically extended, high velocity dispersion stellar distributions appear to be a ubiquitous feature of disc galaxies, and both internal and external mechanisms have been proposed to be the major driver of their formation. However, it is unclear to... Read More about Vertical disc heating in Milky Way-sized galaxies in a cosmological context.

The Copernicus Complexio: a high-resolution view of the small-scale Universe (2016)
Journal Article
Hellwing, W., Frenk, C., Cautun, M., Bose, S., Helly, J., Jenkins, A., …Cytowski, M. (2016). The Copernicus Complexio: a high-resolution view of the small-scale Universe. Monthly Notices of the Royal Astronomical Society, 457(4), 3492-3509. https://doi.org/10.1093/mnras/stw214

We introduce Copernicus Complexio (COCO), a high-resolution cosmological N-body simulation of structure formation in the ΛCDM model. COCO follows an approximately spherical region of radius ∼17.4 h−1 Mpc embedded in a much larger periodic cube that i... Read More about The Copernicus Complexio: a high-resolution view of the small-scale Universe.

The APOSTLE simulations: solutions to the Local Group's cosmic puzzles (2016)
Journal Article
Sawala, T., Frenk, C. S., Fattahi, A., Navarro, J. F., Bower, R. G., Crain, R. A., …White, S. D. (2016). The APOSTLE simulations: solutions to the Local Group's cosmic puzzles. Monthly Notices of the Royal Astronomical Society, 457(2), 1931-1943. https://doi.org/10.1093/mnras/stw145

The Local Group galaxies offer some of the most discriminating tests of models of cosmic structure formation. For example, observations of the Milky Way (MW) and Andromeda satellite populations appear to be in disagreement with N-body simulations of... Read More about The APOSTLE simulations: solutions to the Local Group's cosmic puzzles.

The APOSTLE project: Local Group kinematic mass constraints and simulation candidate selection (2016)
Journal Article
Fattahi, A., Navarro, J. F., Sawala, T., Frenk, C. S., Oman, K. A., Crain, R. A., …Jenkins, A. (2016). The APOSTLE project: Local Group kinematic mass constraints and simulation candidate selection. Monthly Notices of the Royal Astronomical Society, 457(1), 844-856. https://doi.org/10.1093/mnras/stv2970

We use a large sample of isolated dark matter halo pairs drawn from cosmological N-body simulations to identify candidate systems whose kinematics match that of the Local Group (LG) of galaxies. We find, in agreement with the ‘timing argument’ and ea... Read More about The APOSTLE project: Local Group kinematic mass constraints and simulation candidate selection.

The chosen few: the low-mass haloes that host faint galaxies (2015)
Journal Article
Sawala, T., Frenk, C. S., Fattahi, A., Navarro, J. F., Theuns, T., Bower, R. G., …Schaye, J. (2016). The chosen few: the low-mass haloes that host faint galaxies. Monthly Notices of the Royal Astronomical Society, 456(1), 85-97. https://doi.org/10.1093/mnras/stv2597

Since reionization prevents star formation in most haloes less massive than 3 × 109 M⊙, dwarf galaxies only populate a fraction of existing dark matter haloes. We use hydrodynamic cosmological simulations of the Local Group to study the discriminatin... Read More about The chosen few: the low-mass haloes that host faint galaxies.

The Copernicus Complexio: Statistical Properties of Warm Dark Matter Haloes (2015)
Journal Article
Bose, S., Hellwing, W., Frenk, C., Jenkins, A., Lovell, M., Helly, J., & Li, B. (2016). The Copernicus Complexio: Statistical Properties of Warm Dark Matter Haloes. Monthly Notices of the Royal Astronomical Society, 455(1), 318-333. https://doi.org/10.1093/mnras/stv2294

The recent detection of a 3.5 keV X-ray line from the centres of galaxies and clusters by Bulbul et al. and Boyarsky et al. has been interpreted as emission from the decay of 7 keV sterile neutrinos which could make up the (warm) dark matter (WDM). A... Read More about The Copernicus Complexio: Statistical Properties of Warm Dark Matter Haloes.

Surface photometry of brightest cluster galaxies and intracluster stars in ΛCDM (2015)
Journal Article
Cooper, A., Gao, L., Guo, Q., Frenk, C., Jenkins, A., Springel, V., & White, S. (2015). Surface photometry of brightest cluster galaxies and intracluster stars in ΛCDM. Monthly Notices of the Royal Astronomical Society, 451(3), 2703-2722. https://doi.org/10.1093/mnras/stv1042

We simulate the phase-space distribution of stellar mass in nine massive Λ cold dark matter galaxy clusters by applying the semi-analytic particle tagging method of Cooper et al. to the Phoenix suite of high-resolution N-body simulations (M200 ≈ 7.5–... Read More about Surface photometry of brightest cluster galaxies and intracluster stars in ΛCDM.

Decaying dark matter: the case for a deep X-ray observation of Draco (2015)
Journal Article
Lovell, M., Bertone, G., Boyarsky, A., Jenkins, A., & Ruchayskiy, O. (2015). Decaying dark matter: the case for a deep X-ray observation of Draco. Monthly Notices of the Royal Astronomical Society, 451(2), 1573-1585. https://doi.org/10.1093/mnras/stv963

Recent studies of M31, the Galactic Centre (GC), and galaxy clusters have made tentative detections of an X-ray line at ∼3.5 keV that could be produced by decaying dark matter. We use high-resolution simulations of the Aquarius project to predict the... Read More about Decaying dark matter: the case for a deep X-ray observation of Draco.

Evolution of galaxy stellar masses and star formation rates in the EAGLE simulations (2015)
Journal Article
Furlong, M., Bower, R., Theuns, T., Schaye, J., Crain, R., Schaller, M., …Rosas-Guevara, Y. (2015). Evolution of galaxy stellar masses and star formation rates in the EAGLE simulations. Monthly Notices of the Royal Astronomical Society, 450(4), 4486-4504. https://doi.org/10.1093/mnras/stv852

We investigate the evolution of galaxy masses and star formation rates in the Evolution and Assembly of Galaxies and their Environment (eagle) simulations. These comprise a suite of hydrodynamical simulations in a Λ cold dark matter cosmogony with su... Read More about Evolution of galaxy stellar masses and star formation rates in the EAGLE simulations.

Baryon effects on the internal structure of ΛCDM haloes in the EAGLE simulations (2015)
Journal Article
Schaller, M., Frenk, C. S., Bower, R. G., Theuns, T., Jenkins, A., Schaye, J., …McCarthy, I. G. (2015). Baryon effects on the internal structure of ΛCDM haloes in the EAGLE simulations. Monthly Notices of the Royal Astronomical Society, 451(2), 1247-1267. https://doi.org/10.1093/mnras/stv1067

We investigate the internal structure and density profiles of haloes of mass 1010–1014 M⊙ in the Evolution and Assembly of Galaxies and their Environment (EAGLE) simulations. These follow the formation of galaxies in a Λ cold dark matter Universe and... Read More about Baryon effects on the internal structure of ΛCDM haloes in the EAGLE simulations.

The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations (2015)
Journal Article
Crain, R., Schaye, J., Bower, R., Furlong, M., Schaller, M., Theuns, T., …Trayford, J. (2015). The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations. Monthly Notices of the Royal Astronomical Society, 450(2), 1937-1961. https://doi.org/10.1093/mnras/stv725

We present results from 13 cosmological simulations that explore the parameter space of the ‘Evolution and Assembly of GaLaxies and their Environments’ (EAGLE) simulation project. Four of the simulations follow the evolution of a periodic cube L = 50... Read More about The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations.

Bent by baryons: the low-mass galaxy-halo relation (2015)
Journal Article
Sawala, T., Frenk, C., Fattahi, A., Navarro, J., Bower, R., Crain, R., …Theuns, T. (2015). Bent by baryons: the low-mass galaxy-halo relation. Monthly Notices of the Royal Astronomical Society, 448(3), 2941-2947. https://doi.org/10.1093/mnras/stu2753

The relation between galaxies and dark matter haloes is of vital importance for evaluating theoretical predictions of structure formation and galaxy formation physics. We use hydrodynamic cosmological simulations of the Local Group to show that the w... Read More about Bent by baryons: the low-mass galaxy-halo relation.

Cosmological simulations of galaxy clusters with feedback from active galactic nuclei: profiles and scaling relations (2014)
Journal Article
Pike, S. R., Kay, S. T., Newton, R. D., Thomas, P. A., & Jenkins, A. (2014). Cosmological simulations of galaxy clusters with feedback from active galactic nuclei: profiles and scaling relations. Monthly Notices of the Royal Astronomical Society, 445(2), 1774-1796. https://doi.org/10.1093/mnras/stu1788

We present results from a new set of 30 cosmological simulations of galaxy clusters, including the effects of radiative cooling, star formation, supernova feedback, black hole growth and AGN feedback. We first demonstrate that our AGN model is capabl... Read More about Cosmological simulations of galaxy clusters with feedback from active galactic nuclei: profiles and scaling relations.

The EAGLE project: simulating the evolution and assembly of galaxies and their environments (2014)
Journal Article
Schaye, J., Crain, R. A., Bower, R. G., Furlong, M., Schaller, M., Theuns, T., …Trayford, J. (2015). The EAGLE project: simulating the evolution and assembly of galaxies and their environments. Monthly Notices of the Royal Astronomical Society, 446(1), 521-554. https://doi.org/10.1093/mnras/stu2058

We introduce the Virgo Consortium's Evolution and Assembly of GaLaxies and their Environments (EAGLE) project, a suite of hydrodynamical simulations that follow the formation of galaxies and supermassive black holes in cosmologically representative v... Read More about The EAGLE project: simulating the evolution and assembly of galaxies and their environments.

Dwarf galaxies in CDM and SIDM with baryons: observational probes of the nature of dark matter (2014)
Journal Article
Vogelsberger, M., Zavala, J., Simpson, C., & Jenkins, A. (2014). Dwarf galaxies in CDM and SIDM with baryons: observational probes of the nature of dark matter. Monthly Notices of the Royal Astronomical Society, 444(4), 3684-3698. https://doi.org/10.1093/mnras/stu1713

We present the first cosmological simulations of dwarf galaxies, which include dark matter self-interactions and baryons. We study two dwarf galaxies within cold dark matter, and four different elastic self-interacting scenarios with constant and vel... Read More about Dwarf galaxies in CDM and SIDM with baryons: observational probes of the nature of dark matter.

The properties of warm dark matter haloes (2014)
Journal Article
Lovell, M. R., Frenk, C. S., Eke, V. R., Jenkins, A., Gao, L., & Theuns, T. (2014). The properties of warm dark matter haloes. Monthly Notices of the Royal Astronomical Society, 439(1), 300-317. https://doi.org/10.1093/mnras/stt2431

Well-motivated elementary particle candidates for the dark matter, such as the sterile neutrino, behave as warm dark matter (WDM). For particle masses of the order of a keV, free streaming produces a cutoff in the linear fluctuation power spectrum at... Read More about The properties of warm dark matter haloes.

A new way of setting the phases for cosmological multiscale Gaussian initial conditions (2013)
Journal Article
Jenkins, A. (2013). A new way of setting the phases for cosmological multiscale Gaussian initial conditions. Monthly Notices of the Royal Astronomical Society, 434(3), 2094-2120. https://doi.org/10.1093/mnras/stt1154

We describe how to define an extremely large discrete realization of a Gaussian white noise field that has a hierarchical structure and the property that the value of any part of the field can be computed quickly. Tiny subregions of such a field can... Read More about A new way of setting the phases for cosmological multiscale Gaussian initial conditions.

The abundance of (not just) dark matter haloes (2013)
Journal Article
Sawala, T., Frenk, C., Crain, R., Jenkins, A., Schaye, J., Theuns, T., & Zavala, J. (2013). The abundance of (not just) dark matter haloes. Monthly Notices of the Royal Astronomical Society, 431(2), 1366-1382. https://doi.org/10.1093/mnras/stt259

We study the effect of baryons on the abundance of structures and substructures in a Λ cold dark matter (CDM) cosmology, using a pair of high-resolution cosmological simulations from the Galaxies-Intergalactic Medium Interaction Calculation project.... Read More about The abundance of (not just) dark matter haloes.

Dark matter halo merger histories beyond cold dark matter - I. Methods and application to warm dark matter (2013)
Journal Article
Benson, A., Farahi, A., Cole, S., Moustakas, L., Jenkins, A., Lovell, M., …Frenk, C. (2013). Dark matter halo merger histories beyond cold dark matter - I. Methods and application to warm dark matter. Monthly Notices of the Royal Astronomical Society, 428(2), 1774-1789. https://doi.org/10.1093/mnras/sts159

We describe a methodology to accurately compute halo mass functions, progenitor mass functions, merger rates and merger trees in non-cold dark matter universes using a self-consistent treatment of the generalized extended Press–Schechter formalism. O... Read More about Dark matter halo merger histories beyond cold dark matter - I. Methods and application to warm dark matter.

Scaling relations for galaxy clusters in the Millennium-XXL simulation (2012)
Journal Article
Angulo, R., Springel, V., White, S., Jenkins, A., Baugh, C., & Frenk, C. (2012). Scaling relations for galaxy clusters in the Millennium-XXL simulation. Monthly Notices of the Royal Astronomical Society, 426(3), 2046-2062. https://doi.org/10.1111/j.1365-2966.2012.21830.x

We present a very large high-resolution cosmological N-body simulation, the Millennium-XXL or MXXL, which uses 303 billion particles to represent the formation of dark matter structures throughout a 4.1 Gpc box in a Λ cold dark matter cosmology. We c... Read More about Scaling relations for galaxy clusters in the Millennium-XXL simulation.

The journey of QSO haloes from z ∼ 6 to the present (2012)
Journal Article
Angulo, R., Springel, V., White, S., Cole, S., Jenkins, A., Baugh, C., & Frenk, C. (2012). The journey of QSO haloes from z ∼ 6 to the present. Monthly Notices of the Royal Astronomical Society, 425(4), 2722-2730. https://doi.org/10.1111/j.1365-2966.2012.21783.x

We apply a recently developed scaling technique to the Millennium-XXL, one of the largest cosmological N-body simulations carried out to date (3 × 1011 particles within a cube of volume ∼70 Gpc3). This allows us to investigate the cosmological parame... Read More about The journey of QSO haloes from z ∼ 6 to the present.

The Phoenix Project: the dark side of rich Galaxy clusters (2012)
Journal Article
Gao, L., Navarro, J., Frenk, C., Jenkins, A., Springel, V., & White, S. (2012). The Phoenix Project: the dark side of rich Galaxy clusters. Monthly Notices of the Royal Astronomical Society, 425(3), 2169-2186. https://doi.org/10.1111/j.1365-2966.2012.21564.x

We introduce the Phoenix Project, a set of Λ cold dark matter (CDM) simulations of the dark matter component of nine rich galaxy clusters. Each cluster is simulated at least at two different numerical resolutions. For eight of them, the highest resol... Read More about The Phoenix Project: the dark side of rich Galaxy clusters.

The Aquila comparison project : the effects of feedback and numerical methods on simulations of galaxy formation (2012)
Journal Article
Scannapieco, C., Wadepuhl, M., Parry, O., Navarro, J., Jenkins, A., Springel, V., …Woods, R. (2012). The Aquila comparison project : the effects of feedback and numerical methods on simulations of galaxy formation. Monthly Notices of the Royal Astronomical Society, 423(2), 1726-1749. https://doi.org/10.1111/j.1365-2966.2012.20993.x

We compare the results of various cosmological gas-dynamical codes used to simulate the formation of a galaxy in the Λ cold dark matter structure formation paradigm. The various runs (13 in total) differ in their numerical hydrodynamical treatment [s... Read More about The Aquila comparison project : the effects of feedback and numerical methods on simulations of galaxy formation.

The haloes of bright satellite galaxies in a warm dark matter universe (2012)
Journal Article
Lovell, M., Eke, V., Frenk, C., Gao, L., Jenkins, A., Theuns, T., …Ruchayskiy, O. (2012). The haloes of bright satellite galaxies in a warm dark matter universe. Monthly Notices of the Royal Astronomical Society, 420(3), 2318-2324. https://doi.org/10.1111/j.1365-2966.2011.20200.x

High-resolution N-body simulations of galactic cold dark matter haloes indicate that we should expect to find a few satellite galaxies around the Milky Way whose haloes have a maximum circular velocity in excess of 40 km s−1. Yet, with the exception... Read More about The haloes of bright satellite galaxies in a warm dark matter universe.

Where will supersymmetric dark matter first be seen? (2012)
Journal Article
Gao, L., Frenk, C., Jenkins, A., Springel, V., & White, S. (2012). Where will supersymmetric dark matter first be seen?. Monthly Notices of the Royal Astronomical Society, 419(2), 1721-1726. https://doi.org/10.1111/j.1365-2966.2011.19836.x

If the dark matter consists of supersymmetric particles, γ-ray observatories such as the Large Area Telescope aboard the Fermi satellite may detect annihilation radiation from the haloes of galaxies and galaxy clusters. Much recent effort has been de... Read More about Where will supersymmetric dark matter first be seen?.

A halo expansion technique for approximating simulated dark matter haloes (2011)
Journal Article
Lowing, B., Jenkins, A., Eke, V., & Frenk, C. (2011). A halo expansion technique for approximating simulated dark matter haloes. Monthly Notices of the Royal Astronomical Society, 416(4), 2697-2711. https://doi.org/10.1111/j.1365-2966.2011.19222.x

We apply a basis function expansion method to create a time-evolving density/potential approximation of the late growth of simulated N-body dark matter haloes. We demonstrate how the potential of a halo from the Aquarius Project can be accurately rep... Read More about A halo expansion technique for approximating simulated dark matter haloes.

The link between galactic satellite orbits and subhalo accretion. (2011)
Journal Article
Lovell, M., Eke, V., Frenk, C., & Jenkins, A. (2011). The link between galactic satellite orbits and subhalo accretion. Monthly Notices of the Royal Astronomical Society, 413(4), 3013-3021. https://doi.org/10.1111/j.1365-2966.2011.18377.x

We calculate the orbital angular momentum of dark matter subhaloes in the Aquarius simulations of cold dark matter (CDM) galactic haloes. We calculate the orientation of their angular momentum relative to that of the spin vector of their host halo an... Read More about The link between galactic satellite orbits and subhalo accretion..

Galactic stellar haloes in the CDM model (2010)
Journal Article
Cooper, A., Cole, S., Frenk, C., White, S., Helly, J., Benson, A., …Wang, J. (2010). Galactic stellar haloes in the CDM model. Monthly Notices of the Royal Astronomical Society, 406(2), 744-766. https://doi.org/10.1111/j.1365-2966.2010.16740.x

We present six simulations of galactic stellar haloes formed by the tidal disruption of accreted dwarf galaxies in a fully cosmological setting. Our model is based on the Aquarius project, a suite of high-resolution N-body simulations of individual d... Read More about Galactic stellar haloes in the CDM model.

How common is the Milky Way-satellite system alignment? (2009)
Journal Article
Libeskind, N., Frenk, C., Cole, S., Jenkins, A., & Helly, J. (2009). How common is the Milky Way-satellite system alignment?. Monthly Notices of the Royal Astronomical Society, 399(2), 550-558. https://doi.org/10.1111/j.1365-2966.2009.15315.x

The highly flattened distribution of satellite galaxies in the Milky Way (MW) presents a number of puzzles. First, its polar alignment stands out from the planar alignments commonly found in other galaxies. Secondly, recent proper-motion measurements... Read More about How common is the Milky Way-satellite system alignment?.

The redshift dependence of the structure of massive Λ cold dark matter haloes (2008)
Journal Article
Gao, L., Navarro, J., Cole, S., Frenk, C., White, S., Springel, V., …Neto, A. (2008). The redshift dependence of the structure of massive Λ cold dark matter haloes. Monthly Notices of the Royal Astronomical Society, 387(2), 536-544. https://doi.org/10.1111/j.1365-2966.2008.13277.x

We use two very large cosmological simulations to study how the density profiles of relaxed Λ cold dark matter dark haloes depend on redshift and on halo mass. We confirm that these profiles deviate slightly but systematically from the NFW form and a... Read More about The redshift dependence of the structure of massive Λ cold dark matter haloes.

Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology (2008)
Journal Article
Evrard, A., Bialek, J., Busha, M., White, M., Habib, S., Heitmann, K., …Diemand, J. (2008). Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology. Astrophysical Journal, 672(1), 122-137. https://doi.org/10.1086/521616

We present a precise estimate of the bulk virial scaling relation of halos formed via hierarchical clustering in an ensemble of simulated cold dark matter cosmologies. The result is insensitive to cosmological parameters; the presence of a trace, dis... Read More about Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology.

A marked correlation function analysis of halo formation times in the Millennium Simulation (2006)
Journal Article
Harker, G., Cole, S., Helly, J., Frenk, C., & Jenkins, A. (2006). A marked correlation function analysis of halo formation times in the Millennium Simulation. Monthly Notices of the Royal Astronomical Society, 367(3), 1039-1049. https://doi.org/10.1111/j.1365-2966.2006.10022.x

We study the environmental dependence of the formation epoch of dark matter haloes in the Millennium Simulation: a ten billion particle N-body simulation of standard Lambda cold dark matter cosmology. A sensitive test of this dependence – the marked... Read More about A marked correlation function analysis of halo formation times in the Millennium Simulation.

The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies. (2006)
Journal Article
Croton, D., Springel, V., White, D., De Lucia, G., Frenk, C., & Jenkins, A. (2006). The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies. Monthly Notices of the Royal Astronomical Society, 365(1), 11-28. https://doi.org/10.1111/j.1365-2966.2005.09675.x

We simulate the growth of galaxies and their central supermassive black holes by implementing a suite of semi-analytic models on the output of the Millennium Run, a very large simulation of the concordance Λ cold dark matter cosmogony. Our procedures... Read More about The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies..

Effects of feedback on the morphology of galaxy discs (2005)
Journal Article
Okamoto, T., Eke, V., Frenk, C., & Jenkins, A. (2005). Effects of feedback on the morphology of galaxy discs. Monthly Notices of the Royal Astronomical Society, 363(4), 1299-1314. https://doi.org/10.1111/j.1365-2966.2005.09525.x

We have performed hydrodynamic simulations of galaxy formation in a cold dark matter (ΛCDM) universe. We have followed galaxy formation in a dark matter halo, chosen to have a relatively quiet recent merger history, using different models for star fo... Read More about Effects of feedback on the morphology of galaxy discs.

The first generation of star-forming haloes. (2005)
Journal Article
Reed, D., Bower, R., Frenk, C., Gao, L., Jenkins, A., Theuns, T., & White, S. (2005). The first generation of star-forming haloes. Monthly Notices of the Royal Astronomical Society, 363(2), 393-404. https://doi.org/10.1111/j.1365-2966.2005.09416.x

We model gas cooling in high-resolution N-body simulations in order to investigate the formation of the first generation of stars. We follow a region of a Lambda cold dark matter (ΛCDM) universe especially selected to contain a rich cluster by the pr... Read More about The first generation of star-forming haloes..

The distribution of satellite galaxies: the great pancake. (2005)
Journal Article
Libeskind, N. I., Frenk, C. S., Cole, S., Helly, J. C., Jenkins, A., Navarro, J. F., & Power, C. (2005). The distribution of satellite galaxies: the great pancake. Monthly Notices of the Royal Astronomical Society, 363(1), 146-152. https://doi.org/10.1111/j.1365-2966.2005.09425.x

The 11 known satellite galaxies within 250 kpc of the Milky Way lie close to a great circle on the sky. We use high-resolution N-body simulations of galactic dark matter haloes to test if this remarkable property can be understood within the context... Read More about The distribution of satellite galaxies: the great pancake..

Early structure in Lambda CDM (2005)
Journal Article
Gao, L., White, S., Jenkins, A., Frenk, C., & Springel, V. (2005). Early structure in Lambda CDM. Monthly Notices of the Royal Astronomical Society, 363(2), 379-392. https://doi.org/10.1111/j.1365-2966.2005.09509.x

We use a novel technique to simulate the growth of one of the most massive progenitors of a supercluster region from redshift z 80, when its mass was about 10 M, until the present day. Our nested sequence of N-body resimulations allows us to study in... Read More about Early structure in Lambda CDM.

The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications (2005)
Journal Article
Cole, S., Percival, W., Peacock, J., Norberg, P., Baugh, C., Frenk, C., …Taylor, K. (2005). The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications. Monthly Notices of the Royal Astronomical Society, 362(2), 505-534. https://doi.org/10.1111/j.1365-2966.2005.09318.x

We present a power-spectrum analysis of the final 2dF Galaxy Redshift Survey (2dFGRS), employing a direct Fourier method. The sample used comprises 221 414 galaxies with measured redshifts. We investigate in detail the modelling of the sample selecti... Read More about The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications.

Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters (2005)
Journal Article
Angulo, R., Baugh, C., Frenk, C., Bower, R., Jenkins, A., & Morris, S. (2005). Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters. Monthly Notices of the Royal Astronomical Society, 362(1), L25-L29. https://doi.org/10.1111/j.1745-3933.2005.00067.x

Acoustic oscillations in the baryon–photon fluid leave a signature in the matter power spectrum. The overall shape of the spectrum and the wavelength of the oscillations depend upon the sound horizon scale at recombination. Using the Λ cold dark matt... Read More about Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters.

Simulations of the formation, evolution and clustering of galaxies and quasars (2005)
Journal Article
Springel, V., White, S., Jenkins, A., Frenk, C., Yoshida, N., Gao, L., …Pearce, F. (2005). Simulations of the formation, evolution and clustering of galaxies and quasars. Nature, 435(7042), 629-636. https://doi.org/10.1038/nature03597

The cold dark matter model has become the leading theoretical picture for the formation of structure in the Universe. This model, together with the theory of cosmic inflation, makes a clear prediction for the initial conditions for structure formatio... Read More about Simulations of the formation, evolution and clustering of galaxies and quasars.

The inner structure of ACDM haloes - III. Universality and asymptotic slopes (2004)
Journal Article
Navarro, J., Hayashi, E., Power, C., Jenkins, A., Frenk, C., White, S., …Quinn, T. (2004). The inner structure of ACDM haloes - III. Universality and asymptotic slopes. Monthly Notices of the Royal Astronomical Society, 349(3), 1039-1051. https://doi.org/10.1111/j.1365-2966.2004.07586.x

We investigate the mass profile of cold dark matter (ΛCDM) haloes using a suite of numerical simulations spanning five decades in halo mass, from dwarf galaxies to rich galaxy clusters. These haloes typically have a few million particles within the v... Read More about The inner structure of ACDM haloes - III. Universality and asymptotic slopes.

Cosmic structure growth and dark energy (2003)
Journal Article
Linder, E., & Jenkins, A. (2003). Cosmic structure growth and dark energy. Monthly Notices of the Royal Astronomical Society, 346(2), 573-583. https://doi.org/10.1046/j.1365-2966.2003.07112.x

Dark energy has a dramatic effect on the dynamics of the Universe, causing the recently discovered acceleration of the expansion. The dynamics are also central to the behaviour of the growth of large-scale structure, offering the possibility that obs... Read More about Cosmic structure growth and dark energy.

The halo occupation distribution and the physics of galaxy formation (2003)
Journal Article
Berlind, A., Weinberg, D., Benson, A., Baugh, C., Cole, S., Davé, R., …Lacey, C. (2003). The halo occupation distribution and the physics of galaxy formation. Astrophysical Journal, 593(1), 1-25. https://doi.org/10.1086/376517

The halo occupation distribution (HOD) describes the bias between galaxies and dark matter by specifying (1) the probability P(N|M) that a halo of virial mass M contains N galaxies of a particular class and (2) the relative spatial and velocity distr... Read More about The halo occupation distribution and the physics of galaxy formation.

Stable clustering, the halo model and non-linear cosmological power spectra (2003)
Journal Article
Smith, R., Peacock, J., Jenkins, A., White, S., Frenk, C., Pearce, F., …Couchman, H. (2003). Stable clustering, the halo model and non-linear cosmological power spectra. Monthly Notices of the Royal Astronomical Society, 341(4), 1311-1332. https://doi.org/10.1046/j.1365-8711.2003.06503.x

We present the results of a large library of cosmological N-body simulations, using power-law initial spectra. The non-linear evolution of the matter power spectra is compared with the predictions of existing analytic scaling formulae based on the wo... Read More about Stable clustering, the halo model and non-linear cosmological power spectra.

The inner structure of ΛCDM haloes - I. A numerical convergence study (2003)
Journal Article
Power, C., Navarro, J., Jenkins, A., Frenk, C., White, S., Springel, V., …Quinn, T. (2003). The inner structure of ΛCDM haloes - I. A numerical convergence study. Monthly Notices of the Royal Astronomical Society, 338(1), 14-34. https://doi.org/10.1046/j.1365-8711.2003.05925.x

We present a comprehensive set of convergence tests which explore the role of various numerical parameters on the equilibrium structure of a simulated dark matter halo. We report on results obtained with two independent, state-of-the-art, multi-stepp... Read More about The inner structure of ΛCDM haloes - I. A numerical convergence study.

Simulations of galaxy formation in a cosmological volume (2001)
Journal Article
Pearce, F., Jenkins, A., Frenk, C., White, S., Thomas, P., Couchman, H., …Efstathiou, G. (2001). Simulations of galaxy formation in a cosmological volume. Monthly Notices of the Royal Astronomical Society, 326(2), 649-666. https://doi.org/10.1046/j.1365-8711.2001.04616.x

We present results of large N-body–hydrodynamic simulations of galaxy formation. Our simulations follow the formation of galaxies in cubic volumes of side 100 Mpc, in two versions of the cold dark matter (CDM) cosmogony: the standard, Ω=1 SCDM model... Read More about Simulations of galaxy formation in a cosmological volume.

The mass function of dark matter haloes (2001)
Journal Article
Jenkins, A., Frenk, C., White, S., Colberg, J., Cole, S., Evrard, A., …Yoshida, N. (2001). The mass function of dark matter haloes. Monthly Notices of the Royal Astronomical Society, 321(2), 372-384. https://doi.org/10.1046/j.1365-8711.2001.04029.x

We combine data from a number of N-body simulations to predict the abundance of dark haloes in cold dark matter (CDM) universes over more than four orders of magnitude in mass. A comparison of different simulations suggests that the dominant uncertai... Read More about The mass function of dark matter haloes.

Experimental cosmic statistics - II. Distribution (2000)
Journal Article
Szapudi, I., Colombi, S., Jenkins, A., & Colberg, J. (2000). Experimental cosmic statistics - II. Distribution. Monthly Notices of the Royal Astronomical Society, 313, 725-733

Experimental cosmic statistics - I. Variance (2000)
Journal Article
Colombi, S., Szapudi, I., Jenkins, A., & Colberg, J. (2000). Experimental cosmic statistics - I. Variance. Monthly Notices of the Royal Astronomical Society, 313, 711-724

Collisional versus Collisionless Dark Matter (2000)
Journal Article
Moore, B., Gelato, S., Jenkins, A., Pearce, F., & Quilis, V. (2000). Collisional versus Collisionless Dark Matter. Astrophysical Journal, 535, L21-L24

Clustering of galaxy clusters in cold dark matter universes (2000)
Journal Article
Colberg, J., White, S., Yoshida, N., MacFarland, T., Jenkins, A., Frenk, C., …Thomas, P. (2000). Clustering of galaxy clusters in cold dark matter universes. Monthly Notices of the Royal Astronomical Society, 319(1), 209-214

Peculiar velocities of galaxy clusters (2000)
Journal Article
Colberg, J., White, S., MacFarland, T., Jenkins, A., Pearce, F., Frenk, C., …Couchman, H. (2000). Peculiar velocities of galaxy clusters. Monthly Notices of the Royal Astronomical Society, 313(2), 229-236

Evolution of structure in cold dark matter universes (1998)
Journal Article
Jenkins, A., Frenk, C., Pearce, F., Thomas, P., Colberg, J., White, S., …Nelson, A. (1998). Evolution of structure in cold dark matter universes. Astrophysical Journal, 499(1), 20-+

SPH/Gravity on a MIMD Parallel Computer (1994)
Journal Article
Antonioletti, M., Jenkins, A., & Nelson, A. (1994). SPH/Gravity on a MIMD Parallel Computer. Memorie Della Società Astronomica Italiana, 65, 1213-

Dynamics of Gas Near the Galactic Centre (1994)
Journal Article
Jenkins, A., & Binney, J. (1994). Dynamics of Gas Near the Galactic Centre. Monthly Notices of the Royal Astronomical Society, 270, 703-

Spiral heating of galactic discs (1990)
Journal Article
Jenkins, A., & Binney, J. (1990). Spiral heating of galactic discs. Monthly Notices of the Royal Astronomical Society, 245, 305-317