J
J. M. Rodríguez Espinosa
Researcher at University of La Laguna
Publications - 70
Citations - 2367
J. M. Rodríguez Espinosa is an academic researcher from University of La Laguna. The author has contributed to research in topics: Galaxy & Luminous infrared galaxy. The author has an hindex of 25, co-authored 68 publications receiving 2243 citations. Previous affiliations of J. M. Rodríguez Espinosa include Spanish National Research Council & European Southern Observatory.
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Journal ArticleDOI
Testing the Unification Model for Active Galactic Nuclei in the Infrared: Are the Obscuring Tori of Type 1 and 2 Seyferts Different?
C. Ramos Almeida,N. A. Levenson,Almudena Alonso-Herrero,A. Asensio Ramos,A. Asensio Ramos,J. M. Rodríguez Espinosa,J. M. Rodríguez Espinosa,A. M. Pérez García,A. M. Pérez García,Chris Packham,Rachel Mason,J. T. Radomski,Tanio Díaz-Santos +12 more
TL;DR: In this paper, the authors compared the properties of Type-1 and Type-2 Seyfert tori using clumpy torus models and a Bayesian approach to fit the infrared nuclear spectral energy distributions (SEDs).
Journal ArticleDOI
The infrared nuclear emission of seyfert galaxies on parsec scales: testing the clumpy torus models
C. Ramos Almeida,Nancy A. Levenson,J. M. Rodríguez Espinosa,Almudena Alonso-Herrero,A. Asensio Ramos,J. T. Radomski,Chris Packham,R. S. Fisher,Charles M. Telesco +8 more
TL;DR: In this paper, the authors presented subarcsecond resolution mid-infrared (mid-IR) photometry in the wavelength range from 8 to 20 μm of 18 Seyfert galaxies, reporting high spatial resolution nuclear fluxes for the entire sample.
Journal ArticleDOI
Testing the Unification Model for AGN in the Infrared: are the obscuring tori of Type 1 and 2 Seyferts different?
C. Ramos Almeida,N. A. Levenson,A. Alonso-Herrero,A. Asensio Ramos,J. M. Rodríguez Espinosa,A. M. Pérez García,Chris Packham,Rachel Mason,J. T. Radomski,Tanio Díaz-Santos +9 more
TL;DR: In this paper, the authors compared the properties of Type-1 and Type-2 Seyfert tori using clumpy torus models and a Bayesian approach to fit the infrared nuclear spectral energy distributions (SEDs).
Journal ArticleDOI
Nuclear star formation activity and black hole accretion in nearby seyfert galaxies
P. Esquej,P. Esquej,A. Alonso-Herrero,Omaira González-Martín,Omaira González-Martín,Sebastian F. Hönig,Sebastian F. Hönig,Antonio Hernán-Caballero,Antonio Hernán-Caballero,Patrick F. Roche,C. Ramos Almeida,C. Ramos Almeida,Rachel Mason,Tanio Díaz-Santos,N. A. Levenson,Itziar Aretxaga,J. M. Rodríguez Espinosa,J. M. Rodríguez Espinosa,Chris Packham +18 more
TL;DR: In this article, the authors used the 11.3 μm polycyclic aromatic hydrocarbon (PAH) feature as a proxy for the star-formation rate (SFR) and active galactic nucleus (AGN) luminosity of Seyfert galaxies.
Journal ArticleDOI
Nuclear star formation activity and black hole accretion in nearby Seyfert galaxies
P. Esquej,A. Alonso-Herrero,O. González-Martín,Sebastian F. Hönig,A. Hernan Caballero,Patrick F. Roche,C. Ramos Almeida,Rachel Mason,Tanio Díaz-Santos,N. A. Levenson,Itziar Aretxaga,J. M. Rodríguez Espinosa,Chris Packham +12 more
TL;DR: In this article, the authors used the 11.3 micron polycyclic aromatic hydrocarbon (PAH) emission in the vicinity of the active galactic nuclei (AGN) and used this feature as a proxy for the star formation rate.