Zobrazeno 1 - 10
of 17
pro vyhledávání: '"large scale structure of the universe cosmology"'
Autor:
Zaninetti Lorenzo
Publikováno v:
Open Astronomy, Vol 27, Iss 1, Pp 335-340 (2018)
The intersections between a spherical shell and the faces of Voronoi polyhedrons are numerically evaluated. The nodes of these intersections are the points that share the same distances from three nuclei. The nodes are assumed to be the places where
Externí odkaz:
https://doaj.org/article/ef5bf4e7d6104e85affbc6a86fdafe29
Autor:
Lemos, P., Weaverdyck, N., Rollins, R. P., Muir, J., Ferté, A., Liddle, A. R., Campos, A., Huterer, D., Raveri, M., Zuntz, J., Di Valentino, E., Fang, X., Hartley, W. G., Aguena, M., Allam, S., Annis, J., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Choi, A., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., Dietrich, J. P., Everett, S., Ferrero, I., Frieman, J., García-Bellido, J., Gatti, M., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lima, M., March, M., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Palmese, A., Paz-Chinchón, F., Pieres, A., Malagón, A. A. Plazas, Porredon, A., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J., DES Collaboration
Recent cosmological analyses rely on the ability to accurately sample from high-dimensional posterior distributions. A variety of algorithms have been applied in the field, but justification of the particular sampler choice and settings is often lack
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ed806b5f951a0a9eeaf687af157daed8
https://hdl.handle.net/11368/3037672
https://hdl.handle.net/11368/3037672
Autor:
Marco De Petris, Chris Power, Matías Gámez-Marín, Alexander Knebe, Roan Haggar, Kai Hoffmann, Weiguang Cui, Frazer R. Pearce, Robert Mostoghiu
Using 324 numerically modelled galaxy clusters we investigate the radial and galaxy-halo alignment of dark matter subhaloes and satellite galaxies orbiting within and around them. We find that radial alignment depends on distance to the centre of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7f52c3f57e67bb18a53b6899a35ac1e5
http://hdl.handle.net/11573/1417899
http://hdl.handle.net/11573/1417899
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 463 (4), pp.3783-3798. ⟨10.1093/mnras/stw2243⟩
Monthly Notices of the Royal Astronomical Society, 2016, 463 (4), pp.3783-3798. ⟨10.1093/mnras/stw2243⟩
Bianchi, D, Percival, W & Bel, J 2016, ' Improving the modelling of redshift-space distortions-II. A pairwise velocity model covering large and small scales ', Monthly Notices of the Royal Astronomical Society, vol. 463, no. 4, pp. 3783-3798 . https://doi.org/10.1093/mnras/stw2243
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 463 (4), pp.3783-3798. ⟨10.1093/mnras/stw2243⟩
Monthly Notices of the Royal Astronomical Society, 2016, 463 (4), pp.3783-3798. ⟨10.1093/mnras/stw2243⟩
Bianchi, D, Percival, W & Bel, J 2016, ' Improving the modelling of redshift-space distortions-II. A pairwise velocity model covering large and small scales ', Monthly Notices of the Royal Astronomical Society, vol. 463, no. 4, pp. 3783-3798 . https://doi.org/10.1093/mnras/stw2243
We develop a model for the redshift-space correlation function, valid for both dark matter particles and halos on scales $>5\,h^{-1}$Mpc. In its simplest formulation, the model requires the knowledge of the first three moments of the line-of-sight pa
Autor:
Lorenzo Zaninetti
Publikováno v:
Open Astronomy, Vol 27, Iss 1, Pp 335-340 (2018)
The intersections between a spherical shell and the faces of Voronoi's polyhedrons are numerically evaluated. The nodes of these intersections are the points that share the same distances from three nuclei. The nodes are assumed to be the places wher
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::efa38ce7e31aedfed3e8965308e9dc5f
http://arxiv.org/abs/1901.06640
http://arxiv.org/abs/1901.06640
Publikováno v:
Fonseca, J, Maartens, R & Santos, M G 2017, ' Probing the primordial Universe with MeerKAT and DES ', Monthly Notices of the Royal Astronomical Society, vol. 466, no. 3, pp. 2780-2786 . https://doi.org/10.1093/mnras/stw3248
It is usually assumed that we will need to wait until next-generation surveys like Euclid, LSST and SKA, in order to improve on the current best constraints on primordial non-Gaussianity from the Planck experiment. We show that two contemporary surve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a9bcd8d9598e4f23715d33a52dbc8f1c
Autor:
Edward Macaulay, D. Scovacricchi, Tamara M. Davis, David Bacon, Robert C. Nichol, Thomas E. Collett
Publikováno v:
Macaulay, E R M, Davis, T M, Scovacricchi, D, Bacon, D, Collett, T & Nichol, B 2017, ' The effects of velocities and lensing on moments of the Hubble diagram ', Monthly Notices of the Royal Astronomical Society, vol. 467, no. 1, pp. 259-272 . https://doi.org/10.1093/mnras/stw3339
We consider the dispersion on the supernova distance-redshift relation due to peculiar velocities and gravitational lensing, and the sensitivity of these effects to the amplitude of the matter power spectrum. We use the MeMo lensing likelihood develo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::28b505e64412bd65743ee7dbfa337c3b
Autor:
Alonso, David, Salvador, Ana Isabel, S��nchez, Francisco Javier, Bilicki, Maciej, Garc��a-Bellido, Juan, S��nchez, Eusebio
Publikováno v:
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Biblos-e Archivo: Repositorio Institucional de la UAM
Universidad Autónoma de Madrid
instname
Biblos-e Archivo: Repositorio Institucional de la UAM
Universidad Autónoma de Madrid
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved
También aparece con
También aparece con
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d6575cc8aaf77f0eac8d5c68b306abad
http://hdl.handle.net/10486/684499
http://hdl.handle.net/10486/684499
Autor:
Simona Ghizzardi, M. Arnaud, T. P. Sasseen, W. T. Vestrand, R. Gastaud, Jonathan P. D. Mittaz, Doris M. Neumann, Bruno Altieri, David H. Lumb, Ulrich G. Briel, Nabila Aghanim
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2001, 365, pp.L67-L73
Astronomy and Astrophysics-A&A, 2001, 365, pp.L67-L73
Astronomy & Astrophysics : a European journal, Vol. 365, no. 1, p. L67-L73 (2001)
Astronomy and Astrophysics-A&A, EDP Sciences, 2001, 365, pp.L67-L73
Astronomy and Astrophysics-A&A, 2001, 365, pp.L67-L73
Astronomy & Astrophysics : a European journal, Vol. 365, no. 1, p. L67-L73 (2001)
We present a temperature map and a temperature profile of the central part (r < 20' or 1/4 virial radius) of the Coma cluster. We combined 5 overlapping pointings made with XMM/EPIC/MOS and extracted spectra in boxes of 3.5' X 3.5'. The temperature d
Publikováno v:
Astroparticle Physics. 5:53-68
We discuss the scaling analysis of CDM and CHDM simulations. We show that on scales larger than about 4–5 h −1 Mpc the two models behave quite differently. In particular, CDM simulations with bias b = 1.5 reveal a smooth transition from small-sca