Search Results - "Asensio Ramos, A."

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  1. 1

    Evidence for Quasi-Isotropic Magnetic Fields from Hinode Quiet-Sun Observations by Asensio Ramos, A

    Published in The Astrophysical journal (20-08-2009)
    “…Some recent investigations of spectropolarimetric observations of the Zeeman effect in the Fe I lines at 630 nm carried out with the Hinode solar space…”
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    Journal Article
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    Advanced Forward Modeling and Inversion of Stokes Profiles Resulting from the Joint Action of the Hanle and Zeeman Effects by Asensio Ramos, A, Trujillo Bueno, J, Landi Degl’Innocenti, E

    Published in The Astrophysical journal (10-08-2008)
    “…A big challenge in solar and stellar physics in the coming years will be to decipher the magnetism of the solar outer atmosphere (chromosphere and corona)…”
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    The Magnetic Response of the Solar Atmosphere to Umbral Flashes by Houston, S. J., Jess, D. B., Ramos, A. Asensio, Grant, S. D. T., Beck, C., Norton, A. A., Prasad, S. Krishna

    Published in The Astrophysical journal (10-06-2018)
    “…Chromospheric observations of sunspot umbrae offer an exceptional view of magnetoacoustic shock phenomena and the impact they have on the surrounding…”
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    X-RAY ABSORPTION, NUCLEAR INFRARED EMISSION, AND DUST COVERING FACTORS OF AGNs: TESTING UNIFICATION SCHEMES by Mateos, S., Carrera, F. J., Alonso-Herrero, A., Hernán-Caballero, A., Barcons, X., Ramos, A. Asensio, Watson, M. G., Blain, A., Caccianiga, A., Ballo, L., Braito, V., Almeida, C. Ramos

    Published in The Astrophysical journal (10-03-2016)
    “…ABSTRACT We present the distributions of the geometrical covering factors of the dusty tori (f2) of active galactic nuclei (AGNs) using an X-ray selected…”
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    Upholding the unified model for active galactic nuclei: VLT/FORS2 spectropolarimetry of Seyfert 2 galaxies by Ramos Almeida, C., Martínez González, M. J., Asensio Ramos, A., Acosta-Pulido, J. A., Hönig, S. F., Alonso-Herrero, A., Tadhunter, C. N., González-Martín, O.

    “…The origin of the unification model for active galactic nuclei (AGN) was the detection of broad hydrogen recombination lines in the optical polarized spectrum…”
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    The Infrared Nuclear Emission of Seyfert Galaxies on Parsec Scales: Testing the Clumpy Torus Models by Ramos Almeida, C, Levenson, N. A, Rodríguez Espinosa, J. M, Alonso-Herrero, A, Asensio Ramos, A, Radomski, J. T, Packham, C, Fisher, R. S, Telesco, C. M

    Published in The Astrophysical journal (10-09-2009)
    “…We present subarcsecond resolution mid-infrared (mid-IR) photometry in the wavelength range from 8 to 20 Delta *mm of 18 Seyfert galaxies, reporting high…”
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    Testing the Unification Model for Active Galactic Nuclei in the Infrared: Are the Obscuring Tori of Type 1 and 2 Seyferts Different? by Ramos Almeida, C, Levenson, N. A, Alonso-Herrero, A, Asensio Ramos, A, Rodríguez Espinosa, J. M, Pérez García, A. M, Packham, C, Mason, R, Radomski, J. T, Díaz-Santos, T

    Published in The Astrophysical journal (20-04-2011)
    “…We present new mid-infrared imaging data for three Type-1 Seyfert galaxies obtained with T-ReCS on the Gemini-South Telescope at subarcsecond resolution. Our…”
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    A substantial amount of hidden magnetic energy in the quiet Sun by Bueno, J. Trujillo, Shchukina, N, Ramos, A. Asensio

    Published in Nature (15-07-2004)
    “…Deciphering and understanding the small-scale magnetic activity of the quiet solar photosphere should help to solve many of the key problems of solar and…”
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    Investigating the sensitivity of observed spectral energy distributions to clumpy torus properties in Seyfert galaxies by Ramos Almeida, C., Alonso-Herrero, A., Levenson, N. A., Asensio Ramos, A., Rodríguez Espinosa, J. M., González-Martín, O., Packham, C., Martínez, M.

    “…We present nuclear spectral energy distributions (SEDs) from 1 to 18 μm of a small sample of nearby, nearly face-on and undisturbed Seyfert galaxies without…”
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    Analysis of spatially deconvolved polar faculae by Quintero Noda, C., Suematsu, Y., Ruiz Cobo, B., Shimizu, T., Asensio Ramos, A.

    “…Polar faculae are bright features that can be detected in solar limb observations and they are related to magnetic field concentrations. Although there are a…”
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    Inferring the 3D Shapes of Extremely Metal-poor Galaxies from Sets of Projected Shapes by Putko, J., Almeida, J. Sánchez, Muñoz-Tuñón, C., Ramos, A. Asensio, Elmegreen, B. G., Elmegreen, D. M.

    Published in The Astrophysical journal (20-09-2019)
    “…The three-dimensional (3D) shape of a galaxy inevitably is tied to how it has formed and evolved and to its dark matter halo. Local extremely metal-poor…”
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    Bayesclumpy: Bayesian Inference with Clumpy Dusty Torus Models by Asensio Ramos, A, Ramos Almeida, C

    Published in The Astrophysical journal (10-05-2009)
    “…Our aim is to present a fast and general Bayesian inference framework based on the synergy between machine learning techniques and standard sampling methods…”
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    Bayesian Magnetohydrodynamic Seismology of Coronal Loops by Arregui, I, Asensio Ramos, A

    Published in The Astrophysical journal (10-10-2011)
    “…We perform a Bayesian parameter inference in the context of resonantly damped transverse coronal loop oscillations. The forward problem is solved in terms of…”
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    ACTIVE REGION FILAMENTS MIGHT HARBOR WEAK MAGNETIC FIELDS by Díaz Baso, C. J., Martínez González, M. J., Asensio Ramos, A.

    Published in The Astrophysical journal (01-05-2016)
    “…ABSTRACT Recent spectropolarimetric observations of active region filaments have revealed polarization profiles with signatures typical of the strong field…”
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    ON THE MAGNETISM AND DYNAMICS OF PROMINENCE LEGS HOSTING TORNADOES by Martínez González, M. J., Ramos, A. Asensio, Arregui, I., Collados, M., Beck, C., Rodríguez, J. de la Cruz

    Published in The Astrophysical journal (10-07-2016)
    “…ABSTRACT Solar tornadoes are dark vertical filamentary structures observed in the extreme ultraviolet associated with prominence legs and filament barbs. Their…”
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    Constraining clumpy dusty torus models using optimized filter sets by Asensio Ramos, A., Ramos Almeida, C.

    “…Recent success in explaining several properties of the dusty torus around the central engine of active galactic nuclei has been gathered with the assumption of…”
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