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A. Gil de Paz
Researcher at Complutense University of Madrid
Publications - 210
Citations - 14408
A. Gil de Paz is an academic researcher from Complutense University of Madrid. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 56, co-authored 200 publications receiving 13290 citations. Previous affiliations of A. Gil de Paz include Carnegie Learning & Jet Propulsion Laboratory.
Papers
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Mapping the star formation history of Mrk 86 ? I. Data and models
TL;DR: In this paper, the authors presented optical near-infrared colors and emission-line fluxes for the currently star-forming regions, intermediate aged starburst and underlying stellar population.
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Palomar/Las Campanas Imaging Atlas of Blue Compact Dwarf galaxies: I. Images and integrated photometry
TL;DR: In this paper, B, R, and Halpha images for a total of 114 nearby galaxies (v_helio -21mag), peak surface brightness (mu_B, peak-mu_R, peak<~1).
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On the Optimization of Broadband Photometry for Galaxy Evolution Studies
TL;DR: In this article, the uncertainties to be expected in the derivation of galaxy physical properties (star formation history, age, metallicity, and reddening) when comparing broadband photometry to the predictions of evolutionary synthesis models are derived.
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On the nature of the extragalactic number counts in the K-band
Guillermo Barro,Jesús Gallego,Pablo G. Pérez-González,C. Eliche-Moral,Marc Balcells,Víctor Villar,Nicolás Cardiel,David Cristóbal-Hornillos,A. Gil de Paz,Rafael Guzman,Roser Pello,Mercedes Prieto,Jaime Zamorano +12 more
TL;DR: In this paper, a near-infrared imaging survey was conducted at the 3.5 m telescope of the Calar Alto Spanish-German Astronomical Center (CAHA), covering two separated fields centered on the HFDN and the Groth field, with a total combined area of similar to 0.27 deg(2) to a depth of K similar to 19 (3 sigma, Vega).
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A multi-wavelength analysis of M 81: insight on the nature of Arp's loop
Antonio Sollima,A. Gil de Paz,David Martínez-Delgado,David Martínez-Delgado,R. J. Gabany,J. Gallego-Laborda,T. Hallas +6 more
TL;DR: In this article, the authors identify the sources of optical and infrared emission observed in Arp's loop using deep wide-field optical images and measured its colors using IRAS and Spitzer-MIPS infrared images and compared them with those of the disk of M81 and Galactic dust cirrus.