Zobrazeno 1 - 10
of 67
pro vyhledávání: '"Martinez, Vicent J."'
Autor:
Torralba-Torregrosa, Alberto, Gurung-López, Siddhartha, Arnalte-Mur, Pablo, Spinoso, Daniele, Izquierdo-Villalba, David, Fernández-Soto, Alberto, Angulo, Raúl, Bonoli, Silvia, Delgado, Rosa M. González, Márquez, Isabel, Martínez, Vicent J., Rahna, P. T., Vílchez, José M., Abramo, Raul, Alcaniz, Jailson, Benitez, Narciso, Carneiro, Saulo, Cenarro, Javier, Cristóbal-Hornillos, David, Dupke, Renato, Ederoclite, Alessandro, Hernán-Caballero, Antonio, López-Sanjuan, Carlos, Marín-Franch, Antonio, de Oliveira, Claudia Mendes, Moles, Mariano, Sodré Jr., Laerte, Taylor, Keith, Varela, Jesús, Ramió, Héctor Vázquez
Publikováno v:
A&A 680, A14 (2023)
We present the Lyman-$a$ (Lya) Luminosity Function (LF) at $2.05
Externí odkaz:
http://arxiv.org/abs/2307.10215
Morpho-statistical characterisation of the spatial galaxy distribution through Gibbs point processes
This paper proposes a morpho-statistical characterisation of the galaxy distribution through spatial statistical modelling based on inhomogeneous Gibbs point processes. The galaxy distribution is supposed to exhibit two components. The first one is r
Externí odkaz:
http://arxiv.org/abs/2104.13891
KIC 8462852 stood out among more than 100,000 stars in the Kepler catalogue because of the strange features of its light curve: a wide, asymmetric dimming taking up to 15 per cent of the light at D793 and a period of multiple, narrow dimmings happeni
Externí odkaz:
http://arxiv.org/abs/1705.08427
Autor:
Arnalte-Mur, Pablo, Vielva, Patricio, Martínez, Vicent J., Sanz, José L., Saar, Enn, Paredes, Silvestre
Publikováno v:
JCAP03(2016)005
We present a full description of the N-probability density function of the galaxy number density fluctuations. This N-pdf is given in terms, on the one hand, of the cold dark matter correlations and, on the other hand, of the galaxy bias parameter. T
Externí odkaz:
http://arxiv.org/abs/1506.07794
Autor:
Ascaso, Begoña, Benítez, Narciso, Fernández-Soto, Alberto, Arnalte-Mur, Pablo, López-Sanjuan, Carlos, Molino, Alberto, Schoenell, William, Jiménez-Teja, Yolanda, Merson, Alexander I., Huertas-Company, Marc, Díaz-García, Luis Alberto, Martínez, Vicent J., Cenarro, A. Javier, Dupke, Renato, Márquez, Isabel, Masegosa, Josefa, Nieves-Seoane, Lorena, Povic, Mirjana, Varela, Jesús, Viironen, Kerttu, Aguerri, J. Alfonso L., Del Olmo, Ascensión, Moles, Mariano, Perea, Jaime, Alfaro, Emilio, Aparicio-Villegas, Teresa, Broadhurst, Tom, Cabrera-Caño, Jesús, Castander, Francisco J., Cepa, Jordi, Cerviño, Miguel, González~Delgado, Rosa M., Cristóbal-Hornillos, David, Hurtado-Gil, Lluis, Husillos, Cesar, Infante, Leopoldo, Prada, Francisco, Quintana, Jose María
We present a catalogue of 348 galaxy clusters and groups with $0.2
Externí odkaz:
http://arxiv.org/abs/1506.03823
Autor:
Ballesteros, Fernando J., Martínez, Vicent J., Luque, Bartolo, Lacasa, Lucas, Valor, Enric, Moya, Andrés
The origin and shape of metabolic scaling has been controversial since Kleiber found that basal metabolic rate of animals seemed to vary as a power law of their body mass with exponent 3/4, instead of 2/3, as a surface-to-volume argument predicts. Th
Externí odkaz:
http://arxiv.org/abs/1407.3659
Publikováno v:
Astronomy and Astrophysics, Volume 513, id.A22 (2010)
(abridged) The clustering properties of galaxies belonging to different luminosity ranges or having different morphological types are different. These characteristics or `marks' permit to understand the galaxy catalogs that carry all this information
Externí odkaz:
http://arxiv.org/abs/1001.1294
Autor:
Martinez, Vicent J., Trimble, Virginia
We review the present status of cosmological discoveries and how these confirm our modern cosmological model, but at the same time we try to focus on its weaknesses and inconsistencies with an historical perspective, and foresee how the on-going big
Externí odkaz:
http://arxiv.org/abs/0904.1126
Autor:
Arnalte-Mur, Pablo, Fernández-Soto, Alberto, Martínez, Vicent J., Saar, Enn, Heinämäki, Pekka, Suhhonenko, Ivan
Publikováno v:
Mon. Not. R. Astron. Soc. 394, 1631-1639 (2009)
Measurements of clustering in large-scale imaging surveys that make use of photometric redshifts depend on the uncertainties in the redshift determination. We have used light-cone simulations to show how the deprojection method successfully recovers
Externí odkaz:
http://arxiv.org/abs/0812.4226