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ESO 3.6m telescope, Oscar for escale

ESO 3.6m telescope, Oscar for escale.

Credit: Oscar Barragán

Dr. Oscar Barragan Villanueva

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Research theme

  • Astronomy and astrophysics
  • Exoplanets and planetary physics

Sub department

  • Astrophysics

Research groups

  • Exoplanets and Stellar Physics
oscar.barragan@physics.ox.ac.uk
  • About
  • Current projects
  • Publications
logo pyaneti
Pyaneti

pyaneti is a code that allows to fit multi-planet signals in RV and photometric data

K2-99: a subgiant hosting a transiting warm Jupiter in an eccentric orbit and a long-period companion

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 464:3 (2017) 2708-2716

Authors:

AMS Smith, D Gandolfi, O Barragán, B Bowler, Sz Csizmadia, M Endl, MCV Fridlund, S Grziwa, E Guenther, AP Hatzes, G Nowak, S Albrecht, R Alonso, J Cabrera, WD Cochran, HJ Deeg, F Cusano, Ph Eigmüller, A Erikson, D Hidalgo, T Hirano, MC Johnson, J Korth, A Mann, N Narita, D Nespral, E Palle, M Pätzold, J Prieto-Arranz, H Rauer, I Ribas, B Tingley, V Wolthoff

PLANETARY INFLUENCE IN THE GAP OF A PROTOPLANETARY DISK: STRUCTURE FORMATION AND AN APPLICATION TO V1247 ORI

REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA 53:2 (2017) 275-307

Authors:

R Alvarez-Meraz, E Nagel, F Rendon, O Barragan

K2-98b: A 32 M⊕ NEPTUNE-SIZE PLANET IN A 10 DAY ORBIT TRANSITING AN F8 STAR

The Astronomical Journal American Astronomical Society 152:6 (2016) 193

Authors:

Oscar Barragán, Sascha Grziwa, Davide Gandolfi, Malcolm Fridlund, Michael Endl, Hans J Deeg, Manuel P Cagigal, Antonino F Lanza, Pier G Prada Moroni, Alexis MS Smith, Judith Korth, Megan Bedell, Juan Cabrera, William D Cochran, Felice Cusano, Szilard Csizmadia, Philipp Eigmüller, Anders Erikson, Eike W Guenther, Artie P Hatzes, David Nespral, Martin Pätzold, Jorge Prieto-Arranz, Heike Rauer

TWO HOT JUPITERS FROM K2 CAMPAIGN 4

The Astronomical Journal American Astronomical Society 151:6 (2016) 171

Authors:

Marshall C Johnson, Davide Gandolfi, Malcolm Fridlund, Szilard Csizmadia, Michael Endl, Juan Cabrera, William D Cochran, Hans J Deeg, Sascha Grziwa, Ivan Ramírez, Artie P Hatzes, Philipp Eigmüller, Oscar Barragán, Anders Erikson, Eike W Guenther, Judith Korth, Teet Kuutma, David Nespral, Martin Pätzold, Enric Palle, Jorge Prieto-Arranz, Heike Rauer, Joonas Saario

Planet Hunters TESS I: TOI 813, a subgiant hosting a transiting Saturn-sized planet on an 84-day orbit

Authors:

NL Eisner, O Barragán, S Aigrain, C Lintott, G Miller, N Zicher, TS Boyajian, C Briceño, EM Bryant, JL Christiansen, AD Feinstein, LM Flor-Torres, M Fridlund, D Gandolfi, J Gilbert, N Guerrero, JM Jenkins, K Jones, MH Kristiansen, A Vanderburg, N Law, AR López-Sánchez, AW Mann, EJ Safron, ME Schwamb, KG Stassun, HP Osborn, J Wang, A Zic, C Ziegler, F Barnet, SJ Bean, DM Bundy, Z Chetnik, JL Dawson, J Garstone, AG Stenner, M Huten, S Larish, LD Melanson, T Mitchell, C Moore, K Peltsch, DJ Rogers, C Schuster, DS Smith, DJ Simister, C Tanner, I Terentev, A Tsymbal

Abstract:

We report on the discovery and validation of TOI 813b (TIC 55525572 b), a transiting exoplanet identified by citizen scientists in data from NASA's Transiting Exoplanet Survey Satellite (TESS) and the first planet discovered by the Planet Hunters TESS project. The host star is a bright (V = 10.3 mag) subgiant ($R_\star=1.94\,R_\odot$, $M_\star=1.32\,M_\odot$). It was observed almost continuously by TESS during its first year of operations, during which time four individual transit events were detected. The candidate passed all the standard light curve-based vetting checks, and ground-based follow-up spectroscopy and speckle imaging enabled us to place an upper limit of $2 M_{Jup}$ (99 % confidence) on the mass of the companion, and to statistically validate its planetary nature. Detailed modelling of the transits yields a period of $83.8911_{ - 0.0031 } ^ { + 0.0027 }$ days, a planet radius of $6.71 \pm 0.38$ $R_{\oplus}$, and a semi major axis of $0.423_{ - 0.037 } ^ { + 0.031 }$ AU. The planet's orbital period combined with the evolved nature of the host star places this object in a relatively under-explored region of parameter space. We estimate that TOI-813b induces a reflex motion in its host star with a semi-amplitude of $\sim6$ ms$^{-1}$, making this system a promising target to measure the mass of a relatively long-period transiting planet.

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