Oscar Barragán
Also known as: Oscar Barragan, O Barragan, O Barragán
University of Warwick, University of Oxford, Universita degli Studi di Torino Scuola di Scienze della Natura, Universidad de Guanajuato
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research · History and Developments in Astronomy
About
I am an astrophysicist specialising in the detection, characterisation, and evolution of exoplanets, with a particular interest in young planetary systems and the physical processes that shape planetary populations.
My research combines precision radial velocity measurements, space- and ground-based photometry, and advanced statistical modelling to measure planetary properties and disentangle planetary signals from stellar variability. I develop and apply Gaussian Process methods for the analysis of stellar activity and planetary signals, enabling robust characterisation of planets orbiting active stars.
A central focus of my research is understanding how planetary masses, radii, densities, and atmospheres evolve during the first stages of planetary evolution. By connecting observations of young planets with older planetary populations, I aim to distinguish the physical mechanisms responsible for shaping the diversity of planetary systems observed in the Galaxy.
I contribute to international exoplanet collaborations and observing programmes, including the PLATO mission. Alongside my research, I contribute to scientific software development, international training activities, public outreach, and the wider exoplanet community.
Employment
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University of Warwick Warwick Prize Fellow2024 - Present
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University of Oxford Postdoctoral Researcher, Overcoming stellar activity in radial velocities2021 - 2026
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University of Oxford Postdoctoral Researcher, Exoplanet Discovery with the PLATO Mission2019 - 2021
Education
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Universita degli Studi di Torino Scuola di Scienze della Natura PhD in physics and astrophysics2015 - 2018
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Universidad de Guanajuato Master of Science (Astrophysics)2013 - 2015
- 2008 - 2013
Projects & Funding
Projects & funding information is unavailable.
Publications (139)
- Two extremely irradiated volatile-rich sub-Neptunes with companions in the TOI-426 and TOI-1839 systems Save
- A model selection criterion for multidimensional Gaussian processes: application to radial velocities Save
- Mass estimates of the young TOI-451 transiting planets: multidimensional Gaussian Process on stellar spectroscopic and photometric signals Save
- Atmospheric characterization of HIP 67522 b with VLT/CRIRES+ VLT/CRIRES+ suggests a heavier planet and hints at deuterium fractionation Save
- The Discovery of Five Hot Jupiters by TESS Save
- Stellar Rotation in an Old Solar Twin Using ESPRESSO/VLT Validates Gyrochronology Save
- Using Doppler imaging to model stellar activity and search for planets around Sun-like stars Save
- Homogeneous planet masses Save
- A four-planet system orbiting the old thick disk star TOI-1203 Save
- A possible misaligned orbit for the young planet AU Mic c Save
- Precise Masses Reveal that TOI-700 c is Low Density and TOI-700 d is Rocky Save
- TOI-1685 b Is a Hot Rocky Super-Earth: Updates to the Stellar and Planet Parameters of a Popular JWST Cycle 2 Target Save
- A non-zero Doppler amplitude is not enough: Revisiting the putati v e radial velocity detection of sub-Venus exoplanet L 98-59b Save
- An ultra-short-period super-Earth with an extremely high density and an outer companion Save
- HD152843 b & c: the masses and orbital periods of a sub-Neptune and a superpuff Neptune Save
- Homogeneous planet masses I: Reanalysis of archival HARPS radial velocities Save
- Investigating stellar activity through eight years of Sun-as-a-star observations Save
- K2-399 b is not a planet: The Saturn that wandered through the Neptune desert is actually a hierarchical eclipsing binary Save
- Mass determination of two Jupiter-sized planets orbiting slightly evolved stars: TOI-2420 b and TOI-2485 b Save
- Modelling stellar variability in archival HARPS data: I - Rotation and activity properties with multi-dimensional Gaussian Processes Save