Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Marcelo Lares"'
Autor:
Germán Alfaro, Ingrid Vanessa Daza Perilla, José Benavides Blanco, Marcelo Lares, Victoria Santucho, Juan Cabral, Ana Laura O’mill, Facundo Rodríguez, Mauricio Koraj
Publikováno v:
SciComm Report. :1-9
Muchos temas de la Astronomía moderna se caracterizan por la identificación de características en imágenes. Si bien esta es una tarea fácil para un ojo entrenado, es difícil obtener la misma calidad al realizarse mediante modelos o métodos num
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 506:4667-4675
All estimators of the two-point correlation function are based on a random catalogue, a set of points with no intrinsic clustering following the selection function of a survey. High-accuracy estimates require the use of large random catalogues, which
Autor:
T. Ribeiro, Richard Camuccio, C. Quiñones, José Franco, Antonio Kanaan, Americo F Hinojosa, R. Vrech, Amelia Cristina Ramirez Rivera, Omar López-Cruz, Darren L. DePoy, William Schoenell, Rodolfo Artola, Emmanuel Ríos-López, Adam Zadrożny, Manuel Starck, Horacio Rodriguez, José Luis Nilo Castellón, Marina Tornatore, Wahltyn Rattray, Diego G. Lambas, B. Sanchez, Ervin Vilchis, Darío Graña, H. Cuevas, Moises Castillo, D. Fernández, C. Girardini, Alejandro F Hinojosa, Andrea Hinojosa, S. Torres-Flores, Jennifer L. Marshall, Marcelo Lares, M. Schneiter, Antonio Chiavassa Ferreyra, Aldo Fonrouge, V. H. Chavushyan, Nelson Padilla, Deborah Dultzin, Sebastián Gurovich, Luis Tapia, V. Renzi, Wendy Mendoza, Mario C. Díaz, Victor Haber Perez, T. Penuela, M. Beroiz, Lucas M. Macri, C. Colazo, Raul Melia, Mariano Dominguez, Juan B. Cabral
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 493:2207-2214
We present the results of the optical follow-up, conducted by the TOROS collaboration, of gravitational wave events detected during the Advanced LIGO-Virgo second observing run (Nov 2016 -- Aug 2017). Given the limited field of view ($\sim100\arcmin$
Using a new statistical approach we study the alignment signal of galactic spins with respect to the center of voids identified in the TNG-300 simulation. We explore this signal in different samples of galaxies, varying their distance from the void c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0336aa41e583f639017a300e50ee91db
We report and analyse the presence of foregrounds in the cosmic microwave background (CMB) radiation associated to extended galactic halos. Using the cross correlation of Planck and WMAP maps and the 2MRS galaxy catalogue, we find that the mean tempe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::194bce8b50cc7ca5552d0dd4b88fe221
Context. As most of the modern astronomical sky surveys produce data faster than humans can analyse it, machine learning (ML) has become a central tool in astronomy. Modern ML methods can be characterised as highly resistant to some experimental erro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6f79022ec37b474b6fc61ee7f5fa0e14
http://arxiv.org/abs/2105.01714
http://arxiv.org/abs/2105.01714
Publikováno v:
Theology and Science Vol.17, No.3, 2019
Repositorio Institucional (UCA)
Pontificia Universidad Católica Argentina
instacron:UCA
Repositorio Institucional (UCA)
Pontificia Universidad Católica Argentina
instacron:UCA
The Search for Extraterrestrial Intelligence (SETI) research assumes that we live in an intelligence-friendly universe. But do we live in a spiritual-friendly universe? We include the spiritual quest in a new multidisciplinary approach to SETI. In a
Autor:
Heliana E. Luparello, Santucho, Marcelo Lares, Andrés N. Ruiz, Diego G. Lambas, Mario Agustín Sgró
Studies of large-scale structures in the Universe, such as superstructures or cosmic voids, have been widely used to characterize the properties of the cosmic web through statistical analyses. On the other hand, the 2-point correlation function of la
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::561da0e28a5275e22f9dfec539e1f0e6
http://arxiv.org/abs/2005.00053
http://arxiv.org/abs/2005.00053
Publikováno v:
Lares, Marcelo, Funes, José Gabriel ORCID: https://orcid.org/0000-0003-4304-2094 and Gramajo, Luciana (2020) Monte Carlo estimation of the probability of causal contacts between communicating civilizations. International Journal of Astrobiology, 19 (5). pp. 393-405. ISSN 1473-5504
Lares, Marcelo, Funes, José Gabriel and Gramajo, Luciana (2020) Monte Carlo estimation of the probability of causal contacts between communicating civilizations. International Journal of Astrobiology, 19 (5). pp. 393-405. ISSN 1473-5504
Producción Académica (UCC)
Universidad Católica de Córdoba
instacron:UCC
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Lares, Marcelo, Funes, José Gabriel and Gramajo, Luciana (2020) Monte Carlo estimation of the probability of causal contacts between communicating civilizations. International Journal of Astrobiology, 19 (5). pp. 393-405. ISSN 1473-5504
Producción Académica (UCC)
Universidad Católica de Córdoba
instacron:UCC
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
In this work we address the problem of estimating the probabilities of causal contacts between civilizations in the Galaxy. We make no assumptions regarding the origin and evolution of intelligent life. We simply assume a network of causally connecte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0aeb04c4647125b0d6bcdefe28544328
Autor:
M. C. Díaz, Sebastián Gurovich, Bruno Sanchez, J. L. Nilo Castellón, Marcelo Lares, Rodolfo Artola, C. Quiñones, D. García Lambas, C. Girardini, Juan B. Cabral, Martin Beroiz, C. Colazo, M. Schneiter, M. Tornatore
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We present a comparison of several Difference Image Analysis (DIA) techniques, in combination with Machine Learning (ML) algorithms, applied to the identification of optical transients associated with gravitational wave events. Each technique is asse
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4ce2e2ba97a335f3c8bdccf55226e5ae
http://arxiv.org/abs/1812.10518
http://arxiv.org/abs/1812.10518