Browsing by Author "Gonzalez Martin, O."

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    Constraining X-ray reflection in the low-luminosity AGN NGC3718 using NuSTAR and XMM-Newton
    (2020) Diaz, Y.; Arevalo, P.; Hernandez Garcia, L.; Bassani, L.; Malizia, A.; Gonzalez Martin, O.; Ricci, Claudio; Matt, G.; Stern, D.; Bauer, Franz Erik; May, D.; Zezas, A .
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    Infrared polarimetry of Mrk 231: scattering off hot dust grains in the central core
    (OXFORD UNIV PRESS, 2017) Lopez Rodriguez, E.; Packham, C.; Jones, T. J.; Siebenmorgen, R.; Roche, P. F.; Levenson, N. A.; Alonso Herrero, A.; Perlman, E.; Ichikawa, K.; Ramos Almeida, C.; Gonzalez Martin, O.; Nikutta, R.; Martinez Paredez, M.; Shenoy, D.; Gordon, M. S.; Telesco, C. M.
    We present high-angular (0.17-0.35 arcsec) resolution imaging polarimetric observations of Mrk 231 in the 3.1 mu m filter using MMT-Pol on the 6.5-m MMT, and in the 8.7, 10.3, and 11.6 mu m filters using CanariCam on the 10.4-m Gran Telescopio CANARIAS. In combination with already published observations, we compile the 1-12 mu m total and polarized nuclear spectral energy distribution (SED). The total flux SED in the central 400 pc is explained as the combination of (1) a hot (731 +/- 4 K) dusty structure, directly irradiated by the central engine, which is at 1.6 +/- 0.1 pc away and attributed to be in the pc-scale polar region, (2) an optically-thick, smooth and disc-like dusty structure ('torus') with an inclination of 48 degrees +/- 23 degrees surrounding the central engine, and (3) an extinguished (A(V) = 36 +/- 5 mag) starburst component. The polarized SED decreases from 0.77 +/- 0.14 per cent at 1.2 mu m to 0.31 +/- 0.15 per cent at 11.6 mu m and follows a power-law function, lambda(similar to 0.57). The polarization angle remains constant (similar to 108 degrees) in the 1-12 mu m wavelength range. The dominant polarization mechanism is explained as scattering-off hot dust grains in the pc-scale polar regions.