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19962026
Showing 2018Show all

431 papers · 1 filter

astro-ph.EP2018★ 19 cited

The GTC exoplanet transit spectroscopy survey X. Stellar spots versus Rayleigh scattering: the case of HAT-P-11b

F. Murgas, G. Chen, E. Pallé +2

Rayleigh scattering in a hydrogen-dominated exoplanet atmosphere can be detected from ground or space based telescopes, however, stellar activity in the form of spots can mimic Ray…

astro-ph.EP2018★ 22 cited

Detection and characterization of an ultra-dense sub-Neptune planet orbiting the Sun-like star HD 119130

R. Luque, G. Nowak, E. Pallé +51

We present the discovery and characterization of a new transiting planet from Campaign 17 of the Kepler extended mission K2. HD 119130 b is a warm sub-Neptune on a 17-d orbit aroun…

astro-ph.SR2018★ 18 cited

Height dependence of the penumbral fine-scale structure in the inner solar atmosphere

Mariarita Murabito, I. Ermolli, F. Giorgi +6

We studied the physical parameters of the penumbra in a large and fully-developed sunspot, one of the largest over the last two solar cycles, by using full-Stokes measurements take…

astro-ph.SR2018★ 94 cited

A homogeneous analysis of globular clusters from the APOGEE survey with the BACCHUS code. I. The Northern clusters

T. Masseron, D. A. García-Hernández, Sz. Mészáros +12

We analyze a large sample of 885 GCs giants from the APOGEE survey. We used the Cannon results to separate the red giant branch and the asymptotic giant branch stars, not only allo…

astro-ph.GA2018★ 18 cited

SOFIA/FORCAST resolves 30 - 40 um extended dust emission in nearby active galactic nuclei

Lindsay Fuller, Enrique Lopez-Rodriguez, Chris Packham +7

We present arcsecond-scale observations of the active galactic nuclei (AGNs) of seven nearby Seyfert galaxies observed from the Stratospheric Observatory For Infrared Astronomy (SO…

astro-ph.GA2018★ 17 cited

The Fornax 3D project: dust mix and gas properties in the center of early-type galaxy FCC 167

S. Viaene, M. Sarzi, N. Zabel +15

Galaxies continuously reprocess their interstellar material. One can therefore expect changing dust grain properties in galaxies which have followed different evolutionary pathways…