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Autor Pérez González, Pablo Guillermo |
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Marino, Raffaella Anna ; Gil de Paz, Armando ; Castillo Morales, África ; Muñoz Mateos, J. C. ; Sánchez, S. F. ; Pérez González, Pablo Guillermo ; Zamorano Calvo, Jaime ; Gallego Maestro, Jesús ; Alonso Herrera, A. ; Kannappan, S. ; Boissier, S. ; Eliche Moral, María del Carmen ; García Vargas, M. L. ; Carrasco, E. ; Vílchez, J. M. ; Sánchez Moreno, F. M. | Universidad Nacional Autónoma México, Instituto Astronomía | 2013MEGARA (Multi-Espectrógrafo en GTC de Alta Resolución para Astronomía) is an optical Integral-Field Unit (IFU) and Multi-Object Spectrograph (MOS) designed for the GTC 10.4 m telescope in La Palma. MEGARA will be a 3rd generation instrument for [...]texto impreso
Marino, Raffaella Anna ; Gil de Paz, Armando ; Castillo Morales, África ; Muñoz Mateos, J. C. ; Sánchez, S. F. ; Pérez González, Pablo Guillermo ; Gallego Maestro, Jesús ; Zamorano Calvo, Jaime ; Alonso Herrero, A. ; Boissier, S. | American Astronomical Society | 2012-07-20We present an analysis of the full bidimensional optical spectral cube of the nearby spiral galaxy NGC 5668, observed with the Pmas fiber PAcK Integral Field Unit (IFU) at the Calar Alto observatory 3.5 m telescope. We make use of broadband imag[...]texto impreso
Georgakakis, A. ; Pérez González, Pablo Guillermo ; Fanidakis, N. ; Salvato, M. ; Aird, J. ; Messias, H. ; Lotz, J. M. ; Barro, Guillermo ; Hsu, Li-Ting ; Nandra, K. ; Rosario, D. ; Cooper, M. C. ; Kocevski, D. D. ; Newman, J. A. | Wiley | 2014-05Chandra data in the COSMOS, AEGIS-XD and 4 Ms Chandra Deep Field South are combined with multiwavelength photometry available in those fields to determine the rest-frame U ? V versus V ? J colours of X-ray AGN hosts in the redshift intervals 0.1[...]texto impreso
Álvarez González, J. ; Colina, L. ; Marqués Chaves, R. ; Pérez González, Pablo Guillermo | EDP Sciencies | 2019-08-23The James Webb Space Telescope (JWST) will provide deep imaging and spectroscopy for sources at redshifts above 6, covering the entire Epoch of Reionization (EoR, 6texto impreso
We present Keck-I MOSFIRE near-infrared spectroscopy for a sample of 13 compact star-forming galaxies (SFGs) at redshift 2 ? z ? 2.5 with star formation rates of SFR ? 100 M yr?1 and masses of log(M/M ) ? 10.8. Their high integrated gas velocit[...]texto impreso
Girard, M. ; Dessauges-Zavadsky, M. ; Schaerer, D. ; Cirasuolo, M. ; Turner, O. J. ; Cava, A. ; Rodríguez Muñoz, L. ; Richard, J. ; Pérez González, Pablo Guillermo | EDP SCIENCES S A | 2018-06-04We present results from the KMOS LENsing Survey (KLENS), which is exploiting gravitational lensing to study the kinematics of 24 star -forming galaxies at 1.4texto impreso
Georgakakis, A. ; Mountrichas, G. ; Salvato, M ; Rosario, D. ; Pérez González, Pablo Guillermo ; Lutz, D. ; Nandra, K. ; Coil, A. ; Cooper, M. C. ; Newman, J. A. ; Berta, S. ; Magnelli, B. ; Popesso, P. ; Pozzi, F. | Wiley | 2014-10-01We combine multi-wavelength data in the AEGIS-XD and C-COSMOS surveys to measure the typical dark matter halo mass of X-ray selected active galactic nuclei (AGN) [L_X(2–10?keV) > 10^42?erg?s^? 1] in comparison with far-infrared selected star-fo[...]texto impreso
Pereira Santaella, Miguel ; Alonso Herrero, Almudena ; Rieke, George H. ; Colina, Luis ; Diaz Santos, Tanio ; Smith, J. D. T. ; Pérez González, Pablo Guillermo ; Engelbracht, Charles W. | University Chicago Press | 2010-06We present results from the Spitzer Infrared Spectrograph spectral mapping observations of 15 local luminous infrared galaxies (LIRGs). In this paper, we investigate the spatial variations of the mid-IR emission which includes fine structure lin[...]texto impreso
Alonso Herrero, Almudena ; Pereira Santaella, Miguel ; Rieke, George H. ; Colina, Luis ; Engelbracht, Charles W. ; Pérez González, Pablo Guillermo ; Diaz Santos, Tanio ; Smith, J. D. T. | Elsevier | 2010-01-04Luminous Infrared (IR) Galaxies (LIRGs, L_IR=10^11-10 L_?) are an important cosmological class of galaxies as they are the main contributors to the co-moving star formation rate density of the universe at z=1. In this paper we present a guarant[...]texto impreso
Caballero, J. A. ; Valdivielso, L. ; Martín, E. L. ; Montes Gutiérrez, David ; Pascual, S. ; Pérez González, Pablo Guillermo | EDP Sciencies | 2008-11Aims. We study in detail nine sources in the direction of the young ? Orionis cluster, which is considered to be a unique site for studying stellar and substellar formation. The nine sources were selected because of their peculiar properties, su[...]texto impreso
Pérez González, Pablo Guillermo ; Gallego Maestro, Jesús ; Zamorano Calvo, Jaime ; Alonso Herrero, A. ; Gil de Paz, Armando ; Aragón Salamanca, A. | American Astronomical Society | 2003-04-10We present the optical and near-infrared luminosity and mass functions of the local star-forming galaxies in the Universidad Complutense de Madrid (UCM) Survey. A bivariate method that explicitly deals with the H? selection of the survey is used[...]texto impreso
The rate of major galaxy-galaxy merging is theoretically predicted to steadily increase with redshift during the peak epoch of massive galaxy development (1 1.5. Instead, if we use an evolving T-obs,T-pair(z) alpha (1 + z)- 2 from Snyder et a[...]texto impreso
Huertas Company, M. ; Bernardi, M. ; Pérez González, Pablo Guillermo ; Ashby, M. L. N. ; Barro, G. ; Conselice, C. ; Daddi, E. ; Dekel, A. ; Dimauro, P. ; Faber, S. M. ; Grogin, N. A. ; Kartaltepe, J. S. ; Kocevski, D. D. ; Koekemoer, A. M. ; Koo, D. C. ; Mei, S. ; Shankar, F. | Wiley | 2016-11-11We quantify the evolution of the stellar mass functions (SMFs) of star-forming and quiescent galaxies as a function of morphology from z ? 3 to the present. Our sample consists of ?50?000 galaxies in the CANDELS fields (?880 arcmin^2), which we [...]texto impreso
We present measurements of the mean mid-infrared to submillimetre flux densities of massive (M_*? 10^11 M_?) galaxies at redshifts 1.7texto impreso
Gil de Paz, Armando ; Gallego Maestro, Jesús ; Castillo Morales, África ; Eliche Moral, María del Carmen ; Marino, Raffaella Anna ; Pascual, S. ; Sánchez Penim, A. ; Zamorano Calvo, Jaime ; Cardiel López, Nicolás ; Pérez González, Pablo Guillermo ; Villar, V. | SPIE, the international society for optics and photonics | 2014MEGARA (Multi-Espectrógrafo en GTC de Alta Resolución para Astronomía) is an optical Integral-Field Unit (IFU) and Multi-Object Spectrograph (MOS) designed for the GTC 10.4m telescope in La Palma. MEGARA offers two IFU fiber bundles, one coverin[...]