Zobrazeno 1 - 10
of 50
pro vyhledávání: '"Moreno, Víctor J."'
Autor:
Broxterman, Jeger C., Schaller, Matthieu, Hoekstra, Henk, Schaye, Joop, McGibbon, Robert J., Moreno, Victor J. Forouhar, Kugel, Roi, Elbers, Willem
Weak gravitational lensing (WL) convergence peaks contain valuable cosmological information in the regime of non-linear collapse. Using the FLAMINGO suite of cosmological hydrodynamical simulations, we study the physical origin and redshift distribut
Externí odkaz:
http://arxiv.org/abs/2412.02736
Autor:
McCarthy, Ian G., Amon, Alexandra, Schaye, Joop, Schaan, Emmanuel, Angulo, Raul E., Salcido, Jaime, Schaller, Matthieu, Bigwood, Leah, Elbers, Willem, Kugel, Roi, Helly, John C., Moreno, Victor J. Forouhar, Frenk, Carlos S., McGibbon, Robert J., Ondaro-Mallea, Lurdes, van Daalen, Marcel P.
Energetic feedback processes associated with accreting supermassive black holes can expel gas from massive haloes and significantly alter various measures of clustering on ~Mpc scales, potentially biasing the values of cosmological parameters inferre
Externí odkaz:
http://arxiv.org/abs/2410.19905
Autor:
Kugel, Roi, Schaye, Joop, Schaller, Matthieu, Moreno, Victor J. Forouhar, McGibbon, Robert J.
Galaxy cluster counts have historically been important for the measurement of cosmological parameters and upcoming surveys will greatly reduce the statistical errors. To exploit the potential of current and future cluster surveys, theoretical uncerta
Externí odkaz:
http://arxiv.org/abs/2408.17217
Autor:
Moreno, Victor J. Forouhar, Fattahi, Azadeh, Deason, Alis J., Henstridge, Fergus, Benítez-Llambay, Alejandro
Galactic stellar haloes are largely composed of the remnants of galaxies accreted during the assembly of their host galaxies, and hence their properties reflect the mass spectrum and post-accretion evolution of their satellites. As the nature of dark
Externí odkaz:
http://arxiv.org/abs/2407.05899
Autor:
Kugel, Roi, Schaye, Joop, Schaller, Matthieu, McCarthy, Ian G., Braspenning, Joey, Helly, John C., Moreno, Victor J. Forouhar, McGibbon, Robert J.
Galaxy clusters provide an avenue to expand our knowledge of cosmology and galaxy evolution. Because it is difficult to accurately measure the total mass of a large number of individual clusters, cluster samples are typically selected using an observ
Externí odkaz:
http://arxiv.org/abs/2406.03180
We investigate the population of bright satellites ($M_{*} \geq 10^{5} \mathrm{M}_{\odot}$) of haloes of mass comparable to that of the Milky Way in cosmological simulations in which the dark matter (DM) is either cold, warm or self-interacting (CDM,
Externí odkaz:
http://arxiv.org/abs/2208.07376
We select a sample of Milky Way (MW) mass haloes from a high-resolution version of the EAGLE simulation to study their inner dark matter (DM) content and how baryons alter it. As in previous studies, we find that all haloes are more massive at the ce
Externí odkaz:
http://arxiv.org/abs/2107.14245
Autor:
Miglioranza, Karina S.B., Gonzalez, Mariana, Ondarza, Paola M., Shimabukuro, Valeria M., Isla, Federico I., Fillmann, Gilberto, Aizpún, Julia E., Moreno, Víctor J.
Publikováno v:
In Science of the Total Environment 1 May 2013 452-453:275-285
Autor:
Gerpe, Marcela S., de León, Alberto Ponce, Bastida, Ricardo, Moreno, Víctor J., Rodríguez, Diego H.
Publikováno v:
Marine Ecology Progress Series, 2009 Jan . 375, 239-245.
Externí odkaz:
https://www.jstor.org/stable/24872984
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