Zobrazeno 1 - 10
of 12
pro vyhledávání: '"J. M. Colberg"'
Autor:
Riccardo Brunino, Lorne Nelson, Michael S. Vogeley, Volker Mueller, J. M. Colberg, Hume A. Feldman, Oliver Hahn, Erwin Platen, Mark C. Neyrinck, Caroline Foster, Sergei F. Shandarin, Rien van de Weygaert, F. Hoyle, Cristiano Porciani, Stefan Gottloeber, Frazer R. Pearce, Manolis Plionis, A. P. Fairall, Spyros Basilakos
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 387 (2)
Monthly Notices of the Royal Astronomical Society, 387(2), 933-944. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 387(2), 933-944. Oxford University Press
Despite a history that dates back at least a quarter of a century studies of voids in the large--scale structure of the Universe are bedevilled by a major problem: there exist a large number of quite different void--finding algorithms, a fact that ha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fcf994d8c0c60b44b22e7e7de573eee1
http://doc.rero.ch/record/298665/files/mnras0387-0933.pdf
http://doc.rero.ch/record/298665/files/mnras0387-0933.pdf
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 360:216-226
We study the formation and evolution of voids in the dark matter distribution using various simulations of the popular $\Lambda$ Cold Dark Matter cosmogony. We identify voids by requiring them to be regions of space with a mean overdensity of -0.8 or
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c571e4e71dcc5b161ae6b715ebafc4c7
https://doi.org/10.1111/j.1365-2966.2005.09064.x
https://doi.org/10.1111/j.1365-2966.2005.09064.x
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 359:272-282
The large--scale structure (LSS) in the Universe comprises a complicated filamentary network of matter. We study this network using a high--resolution simulation of structure formation of a $\Lambda$ Cold Dark Matter cosmology. We investigate the dis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::eaa20ca2c9c7ffcfde3619797ec5c85d
https://doi.org/10.1111/j.1365-2966.2005.08897.x
https://doi.org/10.1111/j.1365-2966.2005.08897.x
Autor:
J. M. Colberg, S. D. M. White, N. Yoshida, T. J. MacFarland, A. Jenkins, C. S. Frenk, F. R. Pearce, A. E. Evrard, H. M. P. Couchman, G. Efstathiou, J. A. Peacock, P. A. Thomas, null the Virgo Consortium
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 319:209-214
We use very large cosmological N--body simulations to obtain accurate predictions for the two-point correlations and power spectra of mass-limited samples of galaxy clusters. We consider two currently popular cold dark matter (CDM) cosmogonies, a cri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a1746da64bbf4c26e982e161da361126
https://doi.org/10.1046/j.1365-8711.2000.03832.x
https://doi.org/10.1046/j.1365-8711.2000.03832.x
Autor:
Carlos S. Frenk, August E. Evrard, Frazer R. Pearce, Adrian Jenkins, John A. Peacock, Stephen White, T. J. MacFarland, George Efstathiou, Peter A. Thomas, Naoki Yoshida, H. M. P. Couchman, J. M. Colberg
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 325:803-816
We create mock pencil-beam redshift surveys from very large cosmological $N$-body simulations of two Cold Dark Matter cosmogonies, an Einstein-de Sitter model ($\tau$CDM) and a flat model with $\Omega_0 =0.3$ and a cosmological constant ($\Lambda$CDM
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4ac94513defd27387d5e48a26407664f
https://doi.org/10.1046/j.1365-8711.2001.04499.x
https://doi.org/10.1046/j.1365-8711.2001.04499.x
Autor:
Simon D. M. White, Naoki Yoshida, J. M. Colberg, Shaun Cole, Hugh M. P. Couchman, Adrian Jenkins, Carlos S. Frenk, August E. Evrard
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2001, Vol.321(2), pp.372-384 [Peer Reviewed Journal]
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::339e07e450529a9d45a015c36d02a24d
https://doi.org/10.1046/j.1365-8711.2001.04029.x
https://doi.org/10.1046/j.1365-8711.2001.04029.x
Autor:
J. M. Colberg, Adi Nusser
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 294:457-464
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::188f1ef2a85ea45729d4f87c4cddd4ec
https://doi.org/10.1046/j.1365-8711.1998.01218.x
https://doi.org/10.1046/j.1365-8711.1998.01218.x
Autor:
Simon D. M. White, Carlos S. Frenk, Adrian Jenkins, Peter A. Thomas, Frazer R. Pearce, George Efstathiou, John A. Peacock, J. M. Colberg, Hugh M. P. Couchman
Publikováno v:
High-Performance Computing ISBN: 9781461372110
Computer simulations have played a central role in defining the modern approach to physical cosmology. Simulations provide the means to calculate the formation history of cosmic structure, given a set of assumptions regarding the physics of the early
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f9490ea89e5d7f724124feaf76c262fa
https://doi.org/10.1007/978-1-4615-4873-7_54
https://doi.org/10.1007/978-1-4615-4873-7_54
We introduce a new technique for following the formation and evolution of galaxies in cosmological N-body simulations. Dissipationless simulations are used to track the formation and merging of dark matter halos as a function of redshift. Simple pres
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e5a9b71ba03876f17f8821282f192aec
Autor:
G. P. Efstathiou, Carlos S. Frenk, John A. Peacock, Peter A. Thomas, Adrian Jenkins, J. M. Colberg, Simon D. M. White, Frazer R. Pearce, A. H. Nelson, Roger M. Hutchings, Hugh M. P. Couchman
Publikováno v:
Astrophysics and Space Science Library ISBN: 9789401060820
We report on work done by the Virgo consortium, an international collaboration set up in order to study the formation and evolution of Large-Scale Structure using N-body simulations on the latest generation of parallel supercomputers. We show results
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cdc6c8383308e8a13d3ec8d0787c443a
https://doi.org/10.1007/978-94-011-4960-0_30
https://doi.org/10.1007/978-94-011-4960-0_30