Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Dante J Paz"'
Autor:
Agustín M Rodríguez-Medrano, Dante J Paz, Federico A Stasyszyn, Facundo Rodríguez, Andrés N Ruiz, Manuel Merchán
Galaxies in cosmic voids have been reported with properties related to a delayed evolution with respect to the Universe in general. These characteristics reflect the interaction of galaxies with the environment. However, it is not clear the degree of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ed868079b7d34a242e4dff381337dc8b
http://arxiv.org/abs/2212.10594
http://arxiv.org/abs/2212.10594
Autor:
Dante J Paz, Carlos M Correa, Sebastiín R Gualpa, Andres N Ruiz, Carlos S Bederián, R Dario Graña, Nelson D Padilla
We present a new definition of cosmic void and a publicly available code with the algorithm that implements it. Underdense regions are defined as free-form objects, called popcorn voids, made from the union of spheres of maximum volume with a given j
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aad1e28b8228a82426338decbe7e06ed
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 502, 5528-5545. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 502(4), 5528-5545
Monthly Notices of the Royal Astronomical Society, 502(4), 5528-5545
The alignment between halo spins and the cosmic web is still poorly understood despite being a widely studied topic. Here, we study this alignment within the context of tidal torque theory (TTT) and deviations from it. To this end, we analyze the evo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d36307c1d4387aa209027425c4a0f6b5
https://hdl.handle.net/1887/3250927
https://hdl.handle.net/1887/3250927
Autor:
Raul E. Angulo, Carlos M. Correa, Dante J. Paz, Ariel G. Sánchez, Nelson Padilla, Andrés N. Ruiz
This is the second part of a thorough investigation of the redshift-space effects that affect void properties and the impact they have on cosmological tests. Here, we focus on the void-galaxy cross-correlation function, specifically, on the projected
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c8cdcdb48b5a3ec76da5823009077d3f
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
In this work, we identify and analyse the properties of cluster-cluster filaments within a cosmological simulation assuming that they are structures connecting maxima of the density field defined by dark matter halos with masses $M \, \ge 10^{14}\, h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f0bb343e78e47e62212c77c43df57250
Autor:
Raul E. Angulo, Andrés N. Ruiz, Dante J. Paz, Carlos M. Correa, Ariel G. Sánchez, Nelson Padilla
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Monthly Notices of the Royal Astronomical Society
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Monthly Notices of the Royal Astronomical Society
We present a new cosmological test using the distribution of galaxies around cosmic voids without assuming a fiducial cosmology. The test is based on a physical model for the void-galaxy cross-correlation function projected along and perpendicular to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5a5c1cacdc780933a4cc2cfd3170c788
http://arxiv.org/abs/1811.12251
http://arxiv.org/abs/1811.12251
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The tidal torque theory (TTT) relates the origin and evolution of angular momentum with the environment in which dark matter (DM) haloes form. The deviations introduced by late non-linearities are commonly thought as noise in the model. In this work,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e6f9bbd02f18a4f95c26ceeb3d4e6424
http://arxiv.org/abs/1811.09487
http://arxiv.org/abs/1811.09487
Autor:
Heliana E. Luparello, Marcelo Lares, Diego G. Lambas, Andrés N. Ruiz, Victoria E. Maldonado, Laura Ceccarelli, Dante J. Paz
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 455:L99-L103
We compute the bulk motions of cosmic voids, using a $\Lambda$CDM numerical simulation considering the mean velocities of the dark matter inside the void itself and that of the haloes in the surrounding shell. We find coincident values of these two m
Autor:
Dante J. Paz, Ariel G. Sánchez
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The estimation of cosmological constraints from observations of the large scale structure of the Universe, such as the power spectrum or the correlation function, requires the knowledge of the inverse of the associated covariance matrix, namely the p
Autor:
Andrés N. Ruiz, Heliana E. Luparello, Dante J. Paz, Diego G. Lambas, Marcelo Lares, Laura Ceccarelli
We analyse the clustering of cosmic voids using a numerical simulation and the main galaxy sample from the Sloan Digital Sky Survey. We take into account the classification of voids into two types that resemble different evolutionary modes: those wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::51a7139ea302b299959f5e4a0ff8818d
https://academic.oup.com/mnras/article-abstract/468/4/4822/3098196
https://academic.oup.com/mnras/article-abstract/468/4/4822/3098196