The Astronomical Journal · 2023 · 22 citations · 86 references
Natural SciencesAstronomyAstrophysicsPlanetary AstronomyPlanetary ScienceExoplanet Host StarsPlanetary SatellitesStellar StructureGround-based PhotometryHigh-precision PhotometryPhotometryRadial VelocitiesSpace VelocitiesSpectroscopic CharacterizationSpectroscopic DiagnosticsTransit Timing Variations
Abstract We present the spectroscopic confirmation and precise mass measurement of the warm giant planet TOI-199 b. This planet was first identified in TESS photometry and confirmed using ground-based photometry from ASTEP in Antarctica including a full 6.5 hr long transit, PEST, Hazelwood, and LCO; space photometry from NEOSSat; and radial velocities (RVs) from FEROS, HARPS, CORALIE, and CHIRON. Orbiting a late G-type star, TOI-199 b has a <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msubsup> <mml:mrow> <mml:mn>104.854</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.002</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.001</mml:mn> </mml:mrow> </mml:msubsup> <mml:mspace width="0.25em"/> <mml:mrow> <mml:mi mathvariant="normal">day</mml:mi> </mml:mrow> </mml:math> period, a mass of 0.17 ± 0.02 M J , and a radius of 0.810 ± 0.005 R J . It is the first warm exo-Saturn with a precisely determined mass and radius. The TESS and ASTEP transits show strong transit timing variations (TTVs), pointing to the existence of a second planet in the system. The joint analysis of the RVs and TTVs provides a unique solution for the nontransiting companion TOI-199 c, which has a period of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msubsup> <mml:mrow> <mml:mn>273.69</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.22</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.26</mml:mn> </mml:mrow> </mml:msubsup> <mml:mspace width="0.25em"/> <mml:mrow> <mml:mi mathvariant="normal">days</mml:mi> </mml:mrow> </mml:math> and an estimated mass of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msubsup> <mml:mrow> <mml:mn>0.28</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.01</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.02</mml:mn> </mml:mrow> </mml:msubsup> <mml:mspace width="0.25em"/> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="normal">J</mml:mi> </mml:mrow> </mml:msub> </mml:math> . This period places it within the conservative habitable zone.
86
The Two Micron All Sky Survey (2MASS)
Michael F. Skrutskie, R. M. Cutri, R. Stiening et al. · The Astronomical Journal · 2006 · 12.2K citations · Full text
<tt>emcee</tt>: The MCMC Hammer
Publications of the Astronomical Society of the Pacific · 2013 · 11.9K citations · Full text
Computing, Computer Science, Physics +14
T. Prusti, J. H. J. de Bruijne, A. G. A. Brown et al. · Astronomy and Astrophysics · 2016 · 7K citations · Full text
Kepler Planet-Detection Mission: Introduction and First Results
W. J. Borucki, David Koch, Gibor Basri et al. · Science · 2010 · 4.1K citations
Natural Sciences, Astronomy, Physics +11