Jaime Zamorano
Jaime Zamorano
Dirección de correo verificada de fis.ucm.es
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Citado por
The stellar mass assembly of galaxies from z= 0 to z= 4: analysis of a sample selected in the rest-frame near-infrared with spitzer
PG Pérez-González, GH Rieke, V Villar, G Barro, M Blaylock, E Egami, ...
The Astrophysical Journal 675 (1), 234, 2008
The current star formation rate of the local universe
J Gallego, J Zamorano, A Aragon-Salamanca, M Rego
The Astrophysical Journal Letters 455 (1), L1, 1995
Radial distribution of stars, gas, and dust in sings galaxies. II. Derived dust properties
JC Muñoz-Mateos, AG De Paz, S Boissier, J Zamorano, DA Dale, ...
The Astrophysical Journal 701 (2), 1965, 2009
Specific star formation rate profiles in nearby spiral galaxies: quantifying the inside-out formation of disks
JC Muñoz-Mateos, A Gil de Paz, S Boissier, J Zamorano, T Jarrett, ...
Astrophysical Journal 658 (2), 1006-1026, 2007
Radial distribution of stars, gas and dust in SINGS galaxies. I. Surface photometry and morphology
JC Munoz-Mateos, AG de Paz, J Zamorano, S Boissier, DA Dale, ...
The Astrophysical Journal 703 (2), 1569, 2009
Estadística básica para estudiantes deficiencias
J Gorgas, N Cardiel, J Zamorano
Madrid. Universidad Complutense. 258p.[Consultado 30 agosto 2018] Disponible …, 2011
High-resolution imagery of earth at night: New sources, opportunities and challenges
C Kyba, S Garz, H Kuechly, AS De Miguel, J Zamorano, J Fischer, ...
Remote sensing 7 (1), 1-23, 2015
Worldwide variations in artificial skyglow
CCM Kyba, KP Tong, J Bennie, I Birriel, JJ Birriel, A Cool, A Danielsen, ...
Scientific reports 5, 8409, 2015
UV-to-FIR analysis of Spitzer/IRAC sources in the extended groth strip. I. Multi-wavelength photometry and spectral energy distributions
G Barro, PG Pérez-González, J Gallego, MLN Ashby, M Kajisawa, ...
The Astrophysical Journal Supplement Series 193 (1), 13, 2011
UV-to-FIR analysis of Spitzer/IRAC sources in the extended groth strip. II. Photometric redshifts, stellar masses, and star formation rates
G Barro, PG Pérez-González, J Gallego, MLN Ashby, M Kajisawa, ...
The Astrophysical Journal Supplement Series 193 (2), 30, 2011
Spectroscopic Properties and Luminosity Distribution of the Universidad Complutense de Madrid Survey Galaxies
J Gallego, J Zamorano, M Rego, AG Vitores
The Astrophysical Journal 475 (2), 502, 1997
Survey of emission-line galaxies: Universidad Complutense de Madrid list
J Zamorano Calvo, M Rego Fernández, J Gallego Maestro, AG Vitores, ...
Astrophysical journal supplement series 95 (2), 387-399, 1994
The Hα-based Star Formation Rate Density of the Universe at z= 0.84
V Villar, J Gallego, PG Pérez-González, S Pascual, K Noeske, DC Koo, ...
The Astrophysical Journal 677 (1), 169, 2008
Observations of a complete sample of Halpha emission-line galaxies. Long-slit spectroscopy of galaxies in UCM lists 1 and 2.
J Gallego, J Zamorano, M Rego, O Alonso, AG Vitores
Astronomy and Astrophysics Supplement Series 120, 323-356, 1996
SHARDS: an optical spectro-photometric survey of distant galaxies
PG Perez-Gonzalez, A Cava, G Barro, V Villar, N Cardiel, I Ferreras, ...
The Astrophysical Journal 762 (1), 46, 2012
Spatial analysis of the Hα emission in the local star-forming UCM galaxies
PG Pérez-González, J Zamorano, J Gallego, A Aragón-Salamanca, ...
The Astrophysical Journal 591 (2), 827, 2003
The galaxy major merger fraction to~ 1
C López-Sanjuan, M Balcells, PG Pérez-González, G Barro, ...
Astronomy & Astrophysics 501 (2), 505-518, 2009
Exploring the evolutionary paths of the most massive galaxies since z~ 2
PG Pérez-González, I Trujillo, G Barro, J Gallego, J Zamorano, ...
The Astrophysical Journal 687 (1), 50, 2008
Hα emitting galaxies and the star formation rate density at 0.24
S Pascual, J Gallego, A Aragón-Salamanca, J Zamorano
Astronomy & Astrophysics 379 (3), 798-806, 2001
A minor merger origin for stellar inner discs and rings in spiral galaxies
MC Eliche-Moral, AC González-García, M Balcells, JAL Aguerri, J Gallego, ...
Astronomy & Astrophysics 533, A104, 2011
El sistema no puede realizar la operación en estos momentos. Inténtalo de nuevo más tarde.
Artículos 1–20