![Foto de Pablo](/img/uploaded/AB42DBD222704EDA38F810F80D86EA4B.jpg)
Pablo
Rodríguez Gil
Professeur Associé
Publications (138) Publications de Pablo Rodríguez Gil
2024
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The donor star radial velocity curve in the cataclysmic variable GY Cnc confirms white dwarf eclipse modelling mass
Monthly Notices of the Royal Astronomical Society, Vol. 527, Núm. 2, pp. 4353-4358
2023
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Dynamical mass of the white dwarf in XY Ari: A test for intermediate polar X-ray spectral models
Monthly Notices of the Royal Astronomical Society, Vol. 524, Núm. 3, pp. 3314-3323
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Systematic uncertainties in the characterization of helium-dominated metal-polluted white dwarf atmospheres
Monthly Notices of the Royal Astronomical Society, Vol. 520, Núm. 2, pp. 2843-2866
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The orbital period of the recurrent nova V2487 Oph revealed
Monthly Notices of the Royal Astronomical Society, Vol. 526, Núm. 4, pp. 4961-4975
2022
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A 62-minute orbital period black widow binary in a wide hierarchical triple
Nature, Vol. 605, Núm. 7908, pp. 41-45
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A Tentative 114 minute Orbital Period Challenges the Ultracompact Nature of the X-Ray Binary 4U 1812-12
Astrophysical Journal Letters, Vol. 931, Núm. 1
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A dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary
Nature, Vol. 610, Núm. 7932, pp. 467-471
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A refined dynamical mass for the black hole in the X-ray transient XTE J1859+226
Monthly Notices of the Royal Astronomical Society, Vol. 517, Núm. 1, pp. 1476-1482
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MUSE spectroscopy of planetary nebulae with high abundance discrepancies
Monthly Notices of the Royal Astronomical Society, Vol. 510, Núm. 4, pp. 5444-5463
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Optimising rapid autonomous transient classifications with the New Robotic Telescope
Proceedings of SPIE - The International Society for Optical Engineering
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The post-common-envelope binary central star of the planetary nebula Ou 5: A doubly eclipsing post-red-giant-branch system
Monthly Notices of the Royal Astronomical Society, Vol. 510, Núm. 2, pp. 3102-3110
2021
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A transmission spectrum of the planet candidate WD 1856+534 b and a lower limit to its mass
Astronomy and Astrophysics, Vol. 649
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BG Tri: An example of a low-inclination RW Sex-type nova-like
Monthly Notices of the Royal Astronomical Society, Vol. 503, Núm. 1, pp. 1431-1441
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Bow shocks, nova shells, disc winds and tilted discs: The nova-like V341 Ara has it all
Monthly Notices of the Royal Astronomical Society, Vol. 501, Núm. 2, pp. 1951-1969
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GD 424 - A helium-atmosphere white dwarf with a large amount of trace hydrogen in the process of digesting a rocky planetesimal
Monthly Notices of the Royal Astronomical Society, Vol. 501, Núm. 3, pp. 4276-4288
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HiPERCAM: A quintuple-beam, high-speed optical imager on the 10.4-m Gran Telescopio Canarias
Monthly Notices of the Royal Astronomical Society, Vol. 507, Núm. 1, pp. 350-366
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The intermediate polar cataclysmic variable GK Persei 120 years after the nova explosion: A first dynamical mass study
Monthly Notices of the Royal Astronomical Society, Vol. 507, Núm. 4, pp. 5805-5819
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Velocity-imaging the rapidly precessing planetary disc around the white dwarf HE 1349-2305 using Doppler tomography
Monthly Notices of the Royal Astronomical Society, Vol. 508, Núm. 4, pp. 5657-5670
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White dwarfs with planetary remnants in the era of Gaia - I. Six emission line systems
Monthly Notices of the Royal Astronomical Society, Vol. 504, Núm. 2, pp. 2707-2726
2020
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A Systematic Search of Zwicky Transient Facility Data for Ultracompact Binary LISA-detectable Gravitational-wave Sources
Astrophysical Journal, Vol. 905, Núm. 1