The DOI matches its Crossref record; 115 of the 115 references it cites were found in a registry or an index.
Baryon effects on the internal structure of ΛCDM haloes in the EAGLE simulations
Open accessAbstract
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 include a treatment of the baryon physics thought to be relevant. The EAGLE simulations reproduce the observed present-day galaxy stellar mass function, as well as many other properties of the galaxy population as a function of time. We find significant differences between the masses of haloes in the EAGLE simulations and in simulations that follow only the dark matter component. Nevertheless, haloes are well described by the Navarro–Frenk–White density profile at radii larger than ∼5 per cent of the virial radius but, closer to the centre, the presence of stars can produce cuspier profiles. Central enhancements in the total mass profile are most important in haloes of mass 1012–1013 M⊙, where the stellar fraction peaks. Over the radial range where they are well resolved, the resulting galaxy rotation curves are in very good agreement with observational data for galaxies with stellar mass M* < 5 × 1010 M⊙. We present an empirical fitting function that describes the total mass profiles and show that its parameters are strongly correlated with halo mass.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
The source backs part of the claim, not all of it — or backs it for a different population, condition or comparison.
In the citing paper
“As argued in previous studies (e.g. Neto et al. 2007; Schaller et al. 2015), we limit the fits to the radial range [0 . 05 , 1] R 200 .”
From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as Schaller et al. 2015
Experimental — accuracy not yet measuredThe cited source says what the claim attributes to it.
In the citing paper
“The EAGLE model reproduces galaxy rotation curves (Schaller et al. 2015), the bimodal distribution of star formation rates and the cosmic star formation history (Furlong et al. 2015), the Hubble sequence of galaxy morphologies (Trayford et al. 2015) and the Tully-Fisher relation over a wide range of galaxy masses (Ferrero et al. 2017).”
From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as Schaller et al. 2015
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
A Universal Density Profile from Hierarchical Clustering
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997) · The Astrophysical Journal · doi:10.1086/304888 · Cited by 9,917
Self-citationGalactic Stellar and Substellar Initial Mass Function
Chabrier, G. (2003) · Publications of the Astronomical Society of the Pacific · doi:10.1086/376392 · Cited by 9,071
The Structure of Cold Dark Matter Halos
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · The Astrophysical Journal · doi:10.1086/177173 · Cited by 8,544 · cited 4×
“…et al. (2010) is many orders of magnitude below the gas density in the star-forming cores of molecular clouds, it probably allows a substantial amount of gas to dominate the potential in the central regions prior to a starburst, as required for the Navarro et al. (1996a) mechanism to operate.”
InfluentialSelf-citationPlanck 2013 results. XVI. Cosmological parameters
Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321591 · Cited by 8,459
The cosmological simulation code gadget-2
Springel, V. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09655.x · Cited by 6,368
A Universal Density Profile from Hierarchical ClusteringPreprint
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · Cited by 6,275
Self-citationSmoothed Particle Hydrodynamics
Monaghan, J. J. (1992) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.30.1.543 · Cited by 5,183
The Global Schmidt law in star forming galaxies
Kennicutt, R., & Jr. (1997) · The Astrophysical Journal · doi:10.1086/305588 · Cited by 4,027
Galactic Stellar and Substellar Initial Mass FunctionPreprint
Chabrier, G. (2003) · Cited by 4,012
Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering
White, S. D. M., & Rees, M. J. (1978) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/183.3.341 · Cited by 3,919
Research works printed but not linked: 8
- Correa, 2015, MNRAS, 1521
- Crain, 2015, MNRAS, 1937
- Duffy, 2010, MNRAS, 105, 2161
- Dutton, 2011, MNRAS, 410, 1660
- Einasto, 1965, Tr. Astrofiz. Inst. Alma-Ata, 5, 87
- Monaghan, 1992, ARA&A, 30, 74, 10.1146/annurev.aa.30.090192.002551 · DOI
- Portinari, 1998, A&A, 334, 505
- Price, 2010, J. Comput. Phys., 231
Cited by
Sorted by citations
Simulating galaxy formation with the IllustrisTNG model
Pillepich, A., Springel, V., Nelson, D., Genel, S., Naiman, J., Pakmor, R., Hernquist, L., Torrey, P., Vogelsberger, M., Weinberger, R., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx2656 · Cited by 2,007
The APOSTLE simulations: solutions to the Local Group's cosmic puzzles
Sawala, T., Frenk, C. S., Fattahi, A., Navarro, J. F., Bower, R. G., Crain, R. A., Vecchia, C. D., Furlong, M., Helly, J. C., Jenkins, A. R., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw145 · Cited by 593
Self-citationThe Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time
Grand, R. J. J., Gómez, F. A., Marinacci, F., Pakmor, R., Springel, V., Campbell, D. J. R., Frenk, C. S., Jenkins, A., & White, S. D. M. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx071 · Cited by 557
Self-citationThe illustris simulation: Public data release
Nelson, D., Pillepich, A., Genel, S., Vogelsberger, M., Springel, V., Torrey, P., Rodriguez-Gomez, V., Sijacki, D., Snyder, G. F., Griffen, B. F., et al. (2015) · Astronomy and Computing · doi:10.1016/j.ascom.2015.09.003 · Cited by 525
The eagle simulations of galaxy formation: Public release of halo and galaxy catalogues
McAlpine, S., Helly, J. C., Schaller, M., Trayford, J. W., Qu, Y., Furlong, M., Bower, R. G., Crain, R. A., Schaye, J., Theuns, T., et al. (2016) · Astronomy and Computing · doi:10.1016/j.ascom.2016.02.004 · Cited by 491
Self-citationThe unexpected diversity of dwarf galaxy rotation curves
Oman, K. A., Navarro, J. F., Fattahi, A., Frenk, C. S., Sawala, T., White, S. D. M., Bower, R. G., Crain, R. A., Furlong, M., Schaller, M., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1504 · Cited by 545
Self-citationThe EAGLE simulation of galaxy formation: public release of halo and galaxy catalogues
McAlpine, S., Helly, J. C., Schaller, M., Trayford, J. W., Qu, Y., Furlong, M., Bower, R. G., Crain, R. A., Schaye, J., Theuns, T., et al. (2016) · Liverpool John Moores University · Cited by 428
Self-citationThe illustris simulation: Public data releasePreprint
Nelson, D., Pillepich, A., Genel, S., Vogelsberger, M., Springel, V., Torrey, P., Rodríguez-Gómez, V., Sijacki, D., Snyder, G. F., Griffen, B. F., et al. (2015) · DSpace@MIT (Massachusetts Institute of Technology) · doi:10.17863/cam.30872 · Cited by 421
Portail, M., Gerhard, O., Wegg, C., & Ness, M. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2819 · Cited by 378
The milky way total mass profile as inferred from Gaia DR2
Cautun, M., Benítez-Llambay, A., Deason, A. J., Frenk, C. S., Fattahi, A., Gómez, F. A., Grand, R. J. J., Oman, K. A., Navarro, J. F., & Simpson, C. M. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa1017 · Cited by 332
“More general profiles, such as the Schaller et al. (2015) or the Dekel et al. (2017) ones, have more free parameters and potentially can provide a better match to the contracted halo profile.”
BackgroundMethodResultInfluentialSelf-citationThe Milky Way total mass profile as inferred from Gaia DR2
Cautun, M., Benitez-Llambay, A., Deason, A. J., Frenk, C. S., Fattahi, A., Gómez, F. A., Grand, R. J. J., Oman, K. A., Navarro, J. F., & Simpson, C. M. (2019) · arXiv · doi:10.48550/arxiv.1911.04557 · Cited by 335
Self-citationNIHAO – IV: core creation and destruction in dark matter density profiles across cosmic time
Tollet, É., Macciò, A. V., Dutton, A. A., Stinson, G. S., Wang, L., Penzo, C., Gutcke, T. A., Buck, T., Kang, X., Brook, C. B., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2856 · Cited by 344
Small Scale Problems of the ΛCDM Model: A Short Review
Popolo, A. D., & Delliou, M. L. (2017) · Galaxies · doi:10.3390/galaxies5010017 · Cited by 316
fire in the field: simulating the threshold of galaxy formation
Fitts, A., Boylan-Kolchin, M., Elbert, O. D., Bullock, J. S., Hopkins, P. F., Oñorbe, J., Wetzel, A. R., Wheeler, C., Faucher‐Giguère, C., Kereš, D., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1757 · Cited by 275
Halo mass function: baryon impact, fitting formulae, and implications for cluster cosmology
Bocquet, S., Saro, A., Dolag, K., & Mohr, J. J. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2657 · Cited by 270
Dark Energy Survey Year 1 results: weak lensing mass calibration of redMaPPer galaxy clusters
McClintock, T., Varga, T., Gruen, D., Rozo, E., Rykoff, E., Shin, T., Melchior, P., DeRose, J., Seitz, S., Dietrich, J., et al. (2018) · Monthly notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2711 · Cited by 145
The Frontier Fields lens modelling comparison project
Meneghetti, M., Natarajan, P., Coe, D., Contini, E., Lucia, G. D., Giocoli, C., Acebrón, A., Borgani, S., Bradač, M., Diego, J. M., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx2064 · Cited by 251
Cui, W., Knebe, A., Yepes, G., Pearce, F. R., Power, C., Davé, R., Arth, A., Borgani, S., Dolag, K., Elahi, P. J., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2111 · Cited by 256
The eagle simulations of galaxy formation: the importance of the hydrodynamics scheme
Schaller, M., Vecchia, C. D., Schaye, J., Bower, R. G., Theuns, T., Crain, R. A., Furlong, M., & McCarthy, I. G. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2169 · Cited by 229
Self-citationThe Hydrangea simulations: galaxy formation in and around massive clusters
Bahé, Y. M., Barnes, D. J., Vecchia, C. D., Kay, S. T., White, S. D. M., McCarthy, I. G., Schaye, J., Bower, R. G., Crain, R. A., Theuns, T., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1403 · Cited by 228
Self-citationStott, J. P., Swinbank, A. M., Johnson, H. L., Tiley, A. L., Magdis, G., Bower, R. G., Bunker, A. J., Bureau, M., Harrison, C. M., Jarvis, M. J., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw129 · Cited by 223
Self-citationSize evolution of normal and compact galaxies in the EAGLE simulation
Furlong, M., Bower, R. G., Crain, R. A., Schaye, J., Theuns, T., Trayford, J. W., Qu, Y., Schaller, M., Berthet, M., & Helly, J. C. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2740 · Cited by 216
Self-citationNext generation cosmology: constraints from theEuclidgalaxy cluster survey
Sartoris, B., Biviano, A., Fedeli, C., Bartlett, J. G., Borgani, S., Costanzi, M., Giocoli, C., Moscardini, L., Weller, J., Ascaso, B., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw630 · Cited by 218
AN OVERMASSIVE DARK HALO AROUND AN ULTRA-DIFFUSE GALAXY IN THE VIRGO CLUSTER
Beasley, M. A., Romanowsky, A. J., Pota, V., Martín-Navarro, I., Delgado, D. M., Neyer, F., & Deich, A. L. (2016) · The Astrophysical Journal Letters · doi:10.3847/2041-8205/819/2/l20 · Cited by 192
A chronicle of galaxy mass assembly in the EAGLE simulation
Qu, Y., Helly, J. C., Bower, R. G., Theuns, T., Crain, R. A., Frenk, C. S., Furlong, M., McAlpine, S., Schaller, M., Schaye, J., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2437 · Cited by 186
Self-citationWeak lensing measurement of the mass–richness relation of SDSS redMaPPer clusters
Simet, M., McClintock, T., Mandelbaum, R., Rozo, E., Rykoff, E. S., Sheldon, E. S., & Wechsler, R. H. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw3250 · Cited by 196
DarkSUSY 6: an advanced tool to compute dark matter properties numerically
Bringmann, T., Edsjö, T., Paolo Gondolo, A., Ullio, P., & Bergström, L. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/07/033 · Cited by 169
The mass of the Milky Way from satellite dynamics
Callingham, T. M., Cautun, M., Deason, A. J., Frenk, C. S., Wang, W., Gómez, F. A., Grand, R. J. J., Marinacci, F., & Pakmor, R. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz365 · Cited by 166
“For each satellite, we calculate the energy by assuming that the host halo is well described by an NFW profile with concentration given by the fits from Schaller et al. (2015).”
BackgroundMethodInfluentialSelf-citationDavies, J. J., Crain, R. A., Oppenheimer, B. D., & Schaye, J. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz3201 · Cited by 167
Self-citationGravitational probes of dark matter physics
Buckley, M. R., & Peter, A. H. G. (2018) · Physics Reports · doi:10.1016/j.physrep.2018.07.003 · Cited by 189
Subhalo abundance matching and assembly bias in the EAGLE simulation
Chaves-Montero, J., Angulo, R. E., Schaye, J., Schaller, M., Crain, R. A., Furlong, M., & Theuns, T. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1225 · Cited by 164
Self-citationThe EAGLE simulations: atomic hydrogen associated with galaxies
Crain, R. A., Bahé, Y. M., Lagos, C. D. P., Rahmati, A., Schaye, J., McCarthy, I. G., Marasco, A., Bower, R. G., Schaller, M., Theuns, T., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2586 · Cited by 157
Self-citationQuantifying the impact of mergers on the angular momentum of simulated galaxies
Lagos, C. D. P., Stevens, A. R. H., Bower, R. G., Davis, T. A., Contreras, S., Padilla, N. D., Obreschkow, D., Croton, D., Trayford, J. W., Welker, C., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx2667 · Cited by 167
Self-citationThe fraction of dark matter within galaxies from the IllustrisTNG simulations
Lovell, M. R., Pillepich, A., Genel, S., Nelson, D., Springel, V., Pakmor, R., Marinacci, F., Weinberger, R., Torrey, P., Vogelsberger, M., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2339 · Cited by 149
“For example, the simulations of Schaller et al. (2015), Wang et al. (2015b), Grand et al. (2017) and Remus et al. (2017) predict Milky Wayanalogue (MW-analogue) rotation curves that are flat outside a few kpc from the centre and in qualitatively good agreement with observations, whereas those of…”
ResultCreasey, P. E., Sameie, O., Sales, L. V., Yu, H.-B., Vogelsberger, M., & Zavala, J. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx522 · Cited by 150
Dark Matter Haloes and Subhaloes
Zavala, J., & Frenk, C. S. (2019) · Galaxies · doi:10.3390/galaxies7040081 · Cited by 164
Self-citationPeirani, S., Dubois, Y., Volonteri, M., Devriendt, J., Bundy, K. A., Silk, J. I., Pichon, C., Kaviraj, S., Gavazzi, R., & Habouzit, M. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx2099 · Cited by 145
Matthee, J., Schaye, J., Crain, R. A., Schaller, M., Bower, R. G., & Theuns, T. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2884 · Cited by 149
Self-citationRahmati, A., Schaye, J., Bower, R. G., Crain, R. A., Furlong, M., Schaller, M., & Theuns, T. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1414 · Cited by 141
Self-citationThe Copernicus Complexio: statistical properties of warm dark matter haloes
Bose, S., Hellwing, W. A., Frenk, C. S., Jenkins, A. R., Lovell, M. R., Helly, J. C., & Li, B. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2294 · Cited by 136
Self-citationKruijssen, J. M. D., Pfeffer, J., Crain, R. A., & Bastian, N. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz968 · Cited by 139
Self-citationThe Extended Distribution of Baryons around Galaxies
Bregman, J. N., Anderson, M. E., Miller, M. J., Hodges-Kluck, E., Dai, X., Li, J.-T., Li, Y., & Qu, Z. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aacafe · Cited by 157
Hydrodynamical Simulations of the Galaxy Population: Enduring Successes and Outstanding Challenges
Crain, R. A., & van de Voort, F. (2023) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-041923-043618 · Cited by 138
Self-citationGLOBULAR CLUSTERS INDICATE THAT ULTRA-DIFFUSE GALAXIES ARE DWARFS
Beasley, M. A., & Trujillo, I. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/830/1/23 · Cited by 134
Robertson, A., Harvey, D., Massey, R. J., Eke, V. R., McCarthy, I. G., Jauzac, M., Li, B., & Schaye, J. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz1815 · Cited by 151
Self-citationBaryonic impact on the dark matter distribution in Milky Way-sized galaxies and their satellites
Zhu, Q., Marinacci, F., Maji, M., Li, Y., Springel, V., & Hernquist, L. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw374 · Cited by 124
Galactic outflow rates in the EAGLE simulations
Mitchell, P., Schaye, J., Bower, R. G., & Crain, R. A. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa938 · Cited by 128
Self-citationIt is not easy being green: the evolution of galaxy colour in the EAGLE simulation
Trayford, J. W., Theuns, T., Bower, R. G., Crain, R. A., Lagos, C. D. P., Schaller, M., & Schaye, J. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1230 · Cited by 128
Self-citationFeedback from Active Galactic Nuclei in Galaxy Groups
Eckert, D., Gaspari, M., Gastaldello, F., Brun, A. M. C. L., & O’Sullivan, E. (2021) · Universe · doi:10.3390/universe7050142 · Cited by 129
Shaken and stirred: the Milky Way's dark substructures
Sawala, T., Pihajoki, P., Johansson, P. H., Frenk, C. S., Navarro, J. F., Oman, K. A., & White, S. D. M. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx360 · Cited by 122
Self-citationModelling the line-of-sight contribution in substructure lensing
Despali, G., Vegetti, S., White, S. D. M., Giocoli, C., & van den Bosch, F. C. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty159 · Cited by 124
Baryon-induced dark matter cores in the eagle simulations
Benítez-Llambay, A., Frenk, C. S., Ludlow, A. D., & Navarro, J. F. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz1890 · Cited by 133
Self-citationPontzen, A., Tremmel, M., Roth, N., Peiris, H. V., Saintonge, A., Volonteri, M., Quinn, T., & Governato, F. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2627 · Cited by 125
Astraeus I: the interplay between galaxy formation and reionization
Hutter, A., Dayal, P., Yepes, G., Gottlöber, S., Legrand, L., & Ucci, G. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab602 · Cited by 122
Deep Search for Decaying Dark Matter with XMM-Newton Blank-Sky Observations
Foster, J. W., Kongsore, M., Dessert, C., Park, Y., Rodd, N. L., Cranmer, K. S., & Safdi, B. R. (2021) · Physical Review Letters · doi:10.1103/physrevlett.127.051101 · Cited by 160
Shape of dark matter haloes in the Illustris simulation: effects of baryons
Chua, K. T. E., Pillepich, A., Vogelsberger, M., & Hernquist, L. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty3531 · Cited by 120
The origin of scatter in the star formation rate–stellar mass relation
Matthee, J., & Schaye, J. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz030 · Cited by 117
Self-citationThe impact of assembly bias on the halo occupation in hydrodynamical simulations
Artale, M. C., Zehavi, I., Contreras, S., & Norberg, P. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2110 · Cited by 116
The local high-velocity tail and the Galactic escape speed
Deason, A. J., Fattahi, A., Belokurov, V., Evans, N. W., Grand, R. J. J., Marinacci, F., & Pakmor, R. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz623 · Cited by 114
Smith, R. J., Lucey, J. R., & Conroy, C. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv518 · Cited by 114
Barred galaxies in the EAGLE cosmological hydrodynamical simulation
Algorry, D. G., Navarro, J. F., Abadi, M. G., Sales, L. V., Bower, R. G., Crain, R. A., Vecchia, C. D., Frenk, C. S., Schaller, M., Schaye, J., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1008 · Cited by 112
Self-citationkeV sterile neutrino dark matter from singlet scalar decays: the most general case
König, J., Merle, A., & Totzauer, M. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/11/038 · Cited by 110
Johnson, H. L., Harrison, C. M., Swinbank, A. M., Tiley, A. L., Stott, J. P., Bower, R. G., Smail, I. R., Bunker, A. J., Sobral, D., Turner, O. J., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx3016 · Cited by 110
Self-citationZooming in on major mergers: dense, starbursting gas in cosmological simulations
Sparre, M., & Springel, V. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1793 · Cited by 75
Limitations to the ‘basic’ HOD model and beyond
Hadzhiyska, B., Bose, S., Eisenstein, D. J., Hernquist, L., & Spergel, D. N. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa623 · Cited by 109
FIREbox: simulating galaxies at high dynamic range in a cosmological volume
Feldmann, R., Quataert, E., Faucher‐Giguère, C., Hopkins, P. F., Çatmabacak, O., Kereš, D., Bassini, L., Bernardini, M., Bullock, J. S., Cenci, E., et al. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad1205 · Cited by 148
Baryonic clues to the puzzling diversity of dwarf galaxy rotation curves
Santos-Santos, I., Navarro, J. F., Robertson, A., Benítez-Llambay, A., Oman, K. A., Lovell, M. R., Frenk, C. S., Ludlow, A. D., Fattahi, A., & Adam Ritz, A. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa1072 · Cited by 107
Self-citationThe Mira-Titan Universe. III. Emulation of the Halo Mass Function
Bocquet, S., Heitmann, K., Habib, S., Lawrence, E., Uram, T. D., Frontiere, N., Pope, A., & Finkel, H. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abac5c · Cited by 107
Stevens, A. R. H., Diemer, B., Lagos, C. D. P., Nelson, D., Pillepich, A., Brown, T., Catinella, B., Hernquist, L., Weinberger, R., Vogelsberger, M., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty3451 · Cited by 106
Hellwing, W. A., Schaller, M., Frenk, C. S., Theuns, T., Schaye, J., Bower, R. G., & Crain, R. A. (2016) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slw081 · Cited by 105
Self-citationDespali, G., & Vegetti, S. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx966 · Cited by 103
The extended distribution of baryons around galaxies
Bregman, J., Anderson, M., Miller, M., Hodges-Kluck, E., Dai, X., Li, J., Li, Y., & Qu, Z. (2018) · Max Planck Digital Library · Cited by 105
Cosmic distribution of highly ionized metals and their physical conditions in the EAGLE simulations
Rahmati, A., Schaye, J., Crain, R. A., Oppenheimer, B. D., Schaller, M., & Theuns, T. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw453 · Cited by 104
Self-citationThe impact of baryons on massive galaxy clusters: halo structure and cluster mass estimates
Henson, M. A., Barnes, D. J., Kay, S. T., McCarthy, I. G., & Schaye, J. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2899 · Cited by 104
Self-citationSimulated Milky Way analogues: implications for dark matter direct searches
Bozorgnia, N., Calore, F., Schaller, M., Lovell, M., Bertone, G., Frenk, C. S., Crain, R. A., Navarro, J. F., Schaye, J., & Theuns, T. (2016) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2016/05/024 · Cited by 103
Self-citationThe link between galaxy and black hole growth in the eagle simulation
McAlpine, S., Bower, R. G., Harrison, C. M., Crain, R. A., Schaller, M., Schaye, J., & Theuns, T. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx658 · Cited by 102
Self-citationDutton, A. A., Macciò, A. V., Dekel, A., Wang, L., Stinson, G., Obreja, A., Di Cintio, A., Brook, C., Buck, T., & Kang, X. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1537 · Cited by 100
Stevens, A. R. H., Croton, D., & Mutch, S. J. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1332 · Cited by 102
Davies, J., Crain, R. A., McCarthy, I. G., Oppenheimer, B. D., Schaye, J., Schaller, M., & McAlpine, S. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz635 · Cited by 105
Self-citationThe effect of baryons on the inner density profiles of rich clusters
Schaller, M., Frenk, C. S., Bower, R. G., Theuns, T., Trayford, J. W., Crain, R. A., Furlong, M., Schaye, J., Vecchia, C. D., & McCarthy, I. G. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1341 · Cited by 100
Self-citationThe Nearest Ultra Diffuse Galaxy: UGC 2162
Trujillo, I., Roman, J., Filho, M., & Almeida, J. S. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa5cbb · Cited by 98
Oppenheimer, B., Babul, A., Bahe, Y., Butsky, I. S., & McCarthy, I. (2021) · Universe · doi:10.3390/universe7070209 · Cited by 24
Self-citationGalaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models
Guo, Q., González-Pérez, V., Guo, Q., Schaller, M., Furlong, M., Bower, R. G., Cole, S., Crain, R. A., Frenk, C. S., Helly, J. C., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1525 · Cited by 96
Self-citationDark matter spikes in the vicinity of Kerr black holes
Ferrer, F., da Rosa, A. M., & Will, C. M. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.96.083014 · Cited by 116
The origin of the mass discrepancy–acceleration relation in ΛCDM
Navarro, J. F., Benítez-Llambay, A., Fattahi, A., Frenk, C. S., Ludlow, A. D., Oman, K. A., Schaller, M., & Theuns, T. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1705 · Cited by 93
Self-citationNo cores in dark matter-dominated dwarf galaxies with bursty star formation histories
Bose, S., Frenk, C. S., Jenkins, A. R., Fattahi, A., Gómez, F. A., Grand, R. J. J., Marinacci, F., Navarro, J. F., Oman, K. A., Pakmor, R., et al. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz1168 · Cited by 91
Self-citationSDSS-IV MaNGA: Variation of the Stellar Initial Mass Function in Spiral and Early-type Galaxies
Li, H., Ge, J., Mao, S., Cappellari, M., Long, R. J., Li, R., Emsellem, É., Dutton, A. A., Li, C., Bundy, K., et al. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa662a · Cited by 92
The low-mass end of the baryonic Tully–Fisher relation
Sales, L. V., Navarro, J. F., Oman, K. A., Fattahi, A., Ferrero, I., Abadi, M. G., Bower, R. G., Crain, R. A., Frenk, C. S., Sawala, T., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2461 · Cited by 91
Self-citationThe three phases of galaxy formation
Clauwens, B., Schaye, J., Franx, M., & Bower, R. G. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1229 · Cited by 89
Self-citationAyromlou, M., Nelson, D., & Pillepich, A. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad2046 · Cited by 89
Missing dark matter in dwarf galaxies?
Oman, K. A., Navarro, J. F., Sales, L. V., Fattahi, A., Frenk, C. S., Sawala, T., Schaller, M., & White, S. D. M. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1251 · Cited by 97
Self-citationOn the OVI abundance in the circumgalactic medium of low-redshift galaxies
Suresh, J., Rubin, K. H. R., Kannan, R., Werk, J. K., Hernquist, L., & Vogelsberger, M. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2499 · Cited by 86
Thob, A. C. R., Crain, R. A., McCarthy, I. G., Schaller, M., Lagos, C. D. P., Schaye, J., Talens, G. J., James, P. A., Theuns, T., & Bower, R. G. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz448 · Cited by 83
Self-citationSimulated Milky Way analogues: implications for dark matter indirect searches
Calore, F., Bozorgnia, N., Lovell, M. R., Bertone, G., Schaller, M., Frenk, C. S., Crain, R. A., Schaye, J., Theuns, T., & Trayford, J. W. (2015) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2015/12/053 · Cited by 92
Self-citationLiu, X., Li, B., Zhao, G., Chiu, M., Fang, W., Pan, C., Wang, Q., Du, W., Yuan, S., Fu, L., et al. (2016) · Physical Review Letters · doi:10.1103/physrevlett.117.051101 · Cited by 84
The impact of the observed baryon distribution in haloes on the total matter power spectrum
Debackere, S. N. B., Schaye, J., & Hoekstra, H. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz3446 · Cited by 81
Self-citationThe Tully–Fisher and mass–size relations from halo abundance matching
Desmond, H., & Wechsler, R. H. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1978 · Cited by 79
Newman, A. B., Ellis, R. S., & Treu, T. (2015) · UCL Discovery (University College London) · Cited by 78
Dutton, A. A., Macciò, A. V., Frings, J., Wang, L., Stinson, G. S., Penzo, C., & Kang, X. (2016) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slv193 · Cited by 75
Wegg, C., Gerhard, O., & Portail, M. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1954 · Cited by 78
Metadata
- Authors
- Schaller, M., Frenk, C. S., Bower, R. G., Theuns, T., Jenkins, A., Schaye, J., Crain, R. A., Furlong, M., Dalla Vecchia, C., & McCarthy, I. G.
- Affiliations
- Durham University (GB)
- University of Antwerp (BE)
- Leiden University (NL)
- Liverpool John Moores University (GB)
- Corresponding author
- Schaller, Matthieu
- ORCID
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2015-06-04
- Volume
- 451
- Issue
- 2
- Pages
- 1247-1267
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W1940538082
- Cited by
- 375
- References
- 114
- Citations by year
- 2026: 10 · 2025: 19 · 2024: 27 · 2023: 21 · 2022: 30 · 2021: 31 · 2020: 35 · 2019: 38 · 2018: 40 · 2017: 50 · 2016: 52 · 2015: 22
- FWCI
- 31.11
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Monthly Notices of the Royal Astronomical Society (publishedVersion)
- Durham Research Online (Durham University) (publishedVersion, other-oa)
- arXiv (Cornell University) (acceptedVersion)
- Durham Research Online (Durham University) (acceptedVersion)
- Leiden Repository (Leiden University) (submittedVersion)
- Durham Research Online (Durham University) (submittedVersion, cc-by)
- Liverpool John Moores University (submittedVersion)
- Data Archiving and Networked Services (DANS) (submittedVersion, other-oa)
- HighWire Press Open Archive (submittedVersion)
- arXiv (Cornell University)
- Funders
- European Commission (238356)
- Durham University (ST/K00042X/1, ST/K003267/1, ST/H008519/1)
- Partnership for Advanced Computing in Europe AISBL
- Belgian Federal Science Policy Office (AP P7/08 CHARM)
- Nederlandse Organisatie voor Wetenschappelijk Onderzoek (ST/K00042X/1, ST/H008519/1)
- Science and Technology Facilities Council (ST/H008519, ST/I004459/2, ST/K00042X/1, ST/L00061X/1, ST/I00162X/1, ST/L00075X/1, ST/M007006/1, ST/I004459/1, ST/H008519/1, ST/K003267/1)
- FP7 Ideas: European Research Council (278594, 267291)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- halo density profiles, Navarro-Frenk-White profile, stellar mass fraction, galaxy rotation curves, halo mass, EAGLE simulation
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
