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Autor Pérez González, Pablo Guillermo |
Documentos disponibles escritos por este autor (144)
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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 1.4![]()
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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[...]![]()
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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[...]![]()
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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[...]![]()
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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[...]![]()
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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[...]![]()
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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[...]![]()
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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 [...]![]()
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We present measurements of the mean mid-infrared to submillimetre flux densities of massive (M_*? 10^11 M_?) galaxies at redshifts 1.7![]()
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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[...]![]()
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Gil de Paz, Armando ; Gallego Maestro, Jesús ; Castillo Morales, África ; Eliche Moral, María del Carmen ; Marino, Raffaella Anna ; Pascual Ramírez, Sergio ; Zamorano Calvo, Jaime ; Cardiel López, Nicolás ; Pérez González, Pablo Guillermo ; ..., otros | Universidad Nacional Autónoma Mexico, Inst. de Astronomía | 2013In these proceedings we summarize the characteristics and current status of MEGARA, the future optical IFU and MOS for the 10.4 m GTC. MEGARA is being built by a Consortium led by the UCM (Spain) that also includes the INAOE (Mexico), the IAA-CS[...]![]()
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Gil de Paz, Armando ; Gallego Maestro, Jesús ; Castillo Morales, África ; Eliche Moral, María del Carmen ; Pascual, S. ; Sánchez Penim, A. ; Villar, V. ; Zamorano Calvo, Jaime ; Cardiel López, Nicolás ; Cava, A. ; Pérez González, Pablo Guillermo | Spie-Int Soc Optical Engineering | 2012In these proceedings we give a summary of the characteristics and current status of the MEGARA instrument, the future optical IFU and MOS for the 10.4-m Gran Telescopio Canarias (GTC). MEGARA is being built by a Consortium of public research ins[...]![]()
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MEGARA, the new intermediate-resolution optical IFU and MOS for GTC: getting ready for the telescope
Gil de Paz, Armando ; Gallego Maestro, Jesús ; Cardiel López, Nicolás ; Castillo Morales, África ; Cruz García, Jesús Manuel de la ; Esteban San Román, Segundo ; López Orozco, José Antonio ; Pascual, S. ; Picazo, P. ; Sánchez-Penim, A. ; Zamorano Calvo, Jaime ; Pérez González, Pablo Guillermo ; otros, ... | Spie-Int Soc Optical Engineering | 2016MEGARA (Multi-Espectrografo en GTC de Alta Resolucion para Astronomia) is an optical Integral-Field Unit (IFU) and Multi-Object Spectrograph (MOS) designed for the GTC 10.4m telescope in La Palma that is being built by a Consortium led by UCM (S[...]![]()
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Rigby, J. R. ; Marcillac, D. ; Egami, E. ; Rieke, G. H. ; Richard, J. ; Kneib, J. P. ; Fadda, D. ; Willmer, C. N. A. ; Borys, C. ; van der Werf, P. P. ; Pérez González, Pablo Guillermo ; Knudsen, K. K. ; Papovich, C. | American Astronomical Society | 2008-03-01We present Spitzer IRS mid-infrared spectra for 15 gravitationally lensed, 24 ?m-selected galaxies, and combine the results with four additional very faint galaxies with IRS spectra in the literature. The median intrinsic 24 ?m flux density of t[...]![]()
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Ultraviolet (UV) nonionizing continuum and mid-infrared (IR) emission constitute the basis of two widely used star formation (SF) indicators at intermediate and high redshifts. We study 2430 galaxies with z![]()
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The cold molecular gas in contemporary galaxies is structured in discrete cloud complexes. These giant molecular clouds (GMCs), with 10^(4) –10^(7) solar masses (M?) and radii of 5–100 parsecs, are the seeds of star formation1 . Highlighting the[...]![]()
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The cold molecular gas in contemporary galaxies is structured in discrete cloud complexes. These giant molecular clouds (GMCs), with 104 –107 solar masses (M?) and radii of 5–100 parsecs, are the seeds of star formation1 . Highlighting the molec[...]![]()
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Zamorano Calvo, Jaime ; Díaz-Guerra Viejo, Carlos ; Gallego Maestro, Jesús ; Pérez González, Pablo Guillermo ; Gil de Paz, Armando ; Pascual, S. ; Villar, V. ; Alonso Herrero, A. ; Aragón Salamanca, A. | Universidad Nacional Autónoma México, Instituto Astronomía | 2005We have studied in detail the properties of local active star-forming galaxies from the UCM survey, and in particular their star-formation histories. We have quantified the relative importance of the current episode of star formation in comparis[...]![]()
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Alonso Herrero, Almudena ; Rieke, George H. ; Rieke, Marcia J. ; Colina, Luis ; Pérez González, Pablo Guillermo ; Ryder, Stuart D. | American Astronomical Society | 2006-10-20We use Hubble Space Telescope (HST) NICMOS continuum and Pa? observations to study the near-infrared and star formation properties of a representative sample of 30 local (d ~ 35-75 Mpc) luminous infrared galaxies (LIRGs, infrared [8-1000 ?m] lum[...]![]()
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Duncan, Kenneth ; Conselice, Christopher J. ; Mundy, Carl ; Bell, Eric ; Donley, Jennifer ; Galametz, Audrey ; Guo, Yicheng ; Grogin, Norman A. ; Hathi, Nimish ; Kartaltepe, Jeyhan ; Kocevski, Dale ; Koekemoer, Anton M. ; Pérez González, Pablo Guillermo ; Mantha, Kameswara B. ; Snyder, Gregory F. ; Stefanon, Mauro | IOP publishing ltd | 2019-05-08Galaxy mergers are expected to have a significant role in the mass assembly of galaxies in the early universe, but there are very few observational constraints on the merger history of galaxies at z > 2. We present the first study of galaxy maj[...]![]()
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Relaño, M. ; Lisenfeld, U. ; Pérez González, Pablo Guillermo ; Vílchez, J. M. ; Battaner, E., E. | American Astronomical Society | 2007-10-01We investigate the use of the rest-frame 24 ?m luminosity as an indicator of the star formation rate (SFR) in galaxies with different metallicities by comparing it to the (extinction-corrected) H? luminosity. We carry out this analysis in two s[...]![]()
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Barro, G. ; Gallego Maestro, Jesús ; Pérez González, Pablo Guillermo ; Eliche Moral, María del Carmen ; Balcells, M. ; Villar, V. ; Cardiel López, Nicolás ; Cristobal Hornillos, D. ; Gil de Paz, Armando ; Guzmán, R. ; Pelló, R. ; Prieto, M. ; Zamorano Calvo, Jaime | EDP Sciencies | 2009-01Context. The galaxy number counts has been traditionally used to test models of galaxy evolution. However, the origin of significant differences in the shape of number counts at different wavelengths is still unclear. By relating the most remark[...]![]()
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We investigate the galaxy quenching process at intermediate redshift using a sample of similar to 4400 galaxies with M-* > 10(9) M-circle dot between redshift 0.5 and 1.0 in all five CANDELS fields. We divide this sample, using the integrated sp[...]![]()
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The Herschel very wide field surveys have charted hundreds of square degrees in multiple far-IR (FIR) bands. While the Sloan Digital Sky Survey (SDSS) is currently the best resource for optical counterpart identifications over such wide areas, i[...]![]()
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Pérez González, Pablo Guillermo ; Zamorano Calvo, Jaime ; Gallego Maestro, Jesús ; Gil de Paz, Armando | EDP Sciences | 2000-02We present Johnson B CCD photometry for the whole sample of galaxies of the Universidad Complutense de Madrid (UCM) Survey Lists I and II. They constitute a well-defined and complete sample of galaxies in the Local Universe with active star form[...]