Zobrazeno 1 - 10
of 584
pro vyhledávání: '"González, Elizabeth"'
Autor:
Palumbo III, Michael L., Ford, Eric B., Gonzalez, Elizabeth B., Wright, Jason T., Moulla, Khaled Al, Schlichenmaier, Rolf
Publikováno v:
AJ 168, 46 (2024)
We present an updated version of GRASS (the GRanulation And Spectrum Simulator, Palumbo et al. 2022) which now uses an expanded library of 22 solar lines to empirically model time-resolved spectral variations arising from solar granulation. We show t
Externí odkaz:
http://arxiv.org/abs/2405.07945
Autor:
Torres-Sánchez, Pablo, Steiger, Hans Th. J., Mastinu, Pierfrancesco, Wyss, Jeffery L., Kayser, Lennard, Silvestrin, Luca, Musacchio-González, Elizabeth, Stock, Matthias Raphael, Dörflinger, David, Fahrendholz, Ulrike, Prete, Gianfranco, Carletto, Osvaldo, Oberauer, Lothar, Porras, Ignacio
Fast neutron beams are of relevance for many scientific and industrial applications. This paper explores fast neutron production using a TANDEM accelerator at the Legnaro National Laboratories, via an energetic ion beam (90 MeV $^{14}N$) onto a lithi
Externí odkaz:
http://arxiv.org/abs/2311.06143
The aim of this work is to study the anisotropic weak lensing signal associated with the mass distribution of massive clusters of galaxies using the Cosmic Microwave Background (CMB) data. For this purpose, we stack patches of the Planck Collaboratio
Externí odkaz:
http://arxiv.org/abs/2310.04387
Autor:
Gonzalez, Elizabeth Johana, Rodriguez-Medrano, Agustín, Pereyra, Luis Alberto, Lambas, Diego García
Self-interacting dark matter (SIDM) is an alternative to the standard collisionless cold dark matter model (CDM), allowing for interactions between the dark matter particles through the introduction of a self-scattering cross-section. However, the ob
Externí odkaz:
http://arxiv.org/abs/2308.13461
Autor:
Gonzalez, Elizabeth J., Hoffmann, Kai, Gaztañaga, Enrique, Lambas, Diego R. García, Fosalba, Pablo, Crocce, Martin, Castander, Francisco J., Makler, Martín
Shape estimates that quantify the halo anisotropic mass distribution are valuable parameters that provide information on their assembly process and evolution. Measurements of the mean shapes for a sample of cluster-sized halos can be used to test hal
Externí odkaz:
http://arxiv.org/abs/2207.09482
Autor:
Gonzalez, Elizabeth J., Hoffmann, Kai, Lambas, Diego R. García, Gaztañaga, Enrique, Graña, Dario, Tallada-Crespí, Pau, Carretero, Jorge, Santucho, M. Victoria, Fosalba, Pablo, Crocce, Martin, Castander, Francisco J., Rodriguez, Facundo, Makler, Martín
Constraints on dark matter halo masses from weak gravitational lensing can be improved significantly by using additional information about the morphology of their density distribution, leading to tighter cosmological constraints derived from the halo
Externí odkaz:
http://arxiv.org/abs/2205.06827
Autor:
Musacchio-González, Elizabeth, Mastinu, Pierfrancesco, Martín-Hernández, Guido, Porras, Ignacio, Centofante, Lisa, Arias de Saavedra, Fernando, Maran, Luca, Ruzzon, Alberto, Lideo, Daniele
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A June 2024 1063
Autor:
Cascio González, Elizabeth
Publikováno v:
Journal of Research in Innovative Teaching & Learning, 2022, Vol. 16, Issue 2, pp. 226-238.
Externí odkaz:
http://www.emeraldinsight.com/doi/10.1108/JRIT-05-2022-0023
Autor:
Zuntz, Joe, Lanusse, François, Malz, Alex I., Wright, Angus H., Slosar, Anže, Abolfathi, Bela, Alonso, David, Bault, Abby, Bom, Clécio R., Brescia, Massimo, Broussard, Adam, Campagne, Jean-Eric, Cavuoti, Stefano, Cypriano, Eduardo S., Fraga, Bernardo M. O., Gawiser, Eric, Gonzalez, Elizabeth J., Green, Dylan, Hatfield, Peter, Iyer, Kartheik, Kirkby, David, Nicola, Andrina, Nourbakhsh, Erfan, Park, Andy, Teixeira, Gabriel, Heitmann, Katrin, Kovacs, Eve, Mao, Yao-Yuan
This paper presents the results of the Rubin Observatory Dark Energy Science Collaboration (DESC) 3x2pt tomography challenge, which served as a first step toward optimizing the tomographic binning strategy for the main DESC analysis. The task of choo
Externí odkaz:
http://arxiv.org/abs/2108.13418
Autor:
Gonzalez, Elizabeth J., Ragone-Figueroa, Cinthia, Donzelli, Carlos J., Makler, Martín, Lambas, Diego García, Granato, Gian Luigi
We present a detailed study of the shapes and alignments of different galaxy cluster components using hydrodynamical simulations. We compute shape parameters from the Dark Matter (DM) distribution, the galaxy members and the intra-cluster light (ICL)
Externí odkaz:
http://arxiv.org/abs/2107.03418