We report the discovery of the 1.008-d, ultrashort period (USP) super-Earth HD 213885b (TOI-141b) orbiting the bright (V= 7.9) star HD 213885 (TOI-141, TIC 403224672), detected using photometry from the recently launched TESS mission. Using FEROS, HARPS, and CORALIE radial velocities, we measure a precise mass of 8.8 ±0.6M⊙ for this 1.74±0.05R⊙ exoplanet, which provides enough information to constrain its bulk composition - similar to Earth's but enriched in iron. The radius, mass, and stellar irradiation of HD 213885b are, given our data, very similar to 55 Cancri e, making this exoplanet a good target to perform comparative exoplanetology of short period, highly irradiated super-Earths. Our precise radial velocities reveal an additional 4...
We present the bright (Vmag = 9.12), multiplanet system TOI-431, characterized with photometry and r...
Context. Ultra-short-period (USP) planets are defined as planets with orbital periods shorter than o...
We report the detection of a transiting super-Earth-sized planet (R = 1.39 ± 0.09 R⊕ ) in a 1.4-day ...
© 2019 The Author(s). We report the discovery of the 1.008-d, ultrashort period (USP) super-Earth HD...
We report the discovery of the 1.008-d, ultrashort period (USP) super-Earth HD 213885b (TOI-141b) or...
We report the discovery of the 1.008-d, ultrashort period (USP) super-Earth HD 213885b (TOI-141b) or...
.-- Espinoza, N. et al.We report the discovery of the 1.008-d, ultrashort period (USP) super-Earth H...
We report the discovery of the 1.008-d, ultrashort period (USP) super-EarthHD213885b (TOI141b) orbit...
The future of exoplanet science is bright, as Transiting Exoplanet Survey Satellite (TESS) once agai...
Dynamical histories of planetary systems, as well as the atmospheric evolution of highly irradiated ...
peer reviewedWe present the discovery of TOI-2136b, a sub-Neptune planet transiting every 7.85 days...
ABSTRACT We present the bright (Vmag = 9.12), multiplanet system TOI-431, characterized with photome...
We present the bright (Vmag = 9.12), multiplanet system TOI-431, characterized with photometry and r...
© 2021. The American Astronomical Society. All rights reserved. We report the discovery and validati...
We report the discovery and validation of four extrasolar planets hosted by the nearby, bright, Sun-...
We present the bright (Vmag = 9.12), multiplanet system TOI-431, characterized with photometry and r...
Context. Ultra-short-period (USP) planets are defined as planets with orbital periods shorter than o...
We report the detection of a transiting super-Earth-sized planet (R = 1.39 ± 0.09 R⊕ ) in a 1.4-day ...
© 2019 The Author(s). We report the discovery of the 1.008-d, ultrashort period (USP) super-Earth HD...
We report the discovery of the 1.008-d, ultrashort period (USP) super-Earth HD 213885b (TOI-141b) or...
We report the discovery of the 1.008-d, ultrashort period (USP) super-Earth HD 213885b (TOI-141b) or...
.-- Espinoza, N. et al.We report the discovery of the 1.008-d, ultrashort period (USP) super-Earth H...
We report the discovery of the 1.008-d, ultrashort period (USP) super-EarthHD213885b (TOI141b) orbit...
The future of exoplanet science is bright, as Transiting Exoplanet Survey Satellite (TESS) once agai...
Dynamical histories of planetary systems, as well as the atmospheric evolution of highly irradiated ...
peer reviewedWe present the discovery of TOI-2136b, a sub-Neptune planet transiting every 7.85 days...
ABSTRACT We present the bright (Vmag = 9.12), multiplanet system TOI-431, characterized with photome...
We present the bright (Vmag = 9.12), multiplanet system TOI-431, characterized with photometry and r...
© 2021. The American Astronomical Society. All rights reserved. We report the discovery and validati...
We report the discovery and validation of four extrasolar planets hosted by the nearby, bright, Sun-...
We present the bright (Vmag = 9.12), multiplanet system TOI-431, characterized with photometry and r...
Context. Ultra-short-period (USP) planets are defined as planets with orbital periods shorter than o...
We report the detection of a transiting super-Earth-sized planet (R = 1.39 ± 0.09 R⊕ ) in a 1.4-day ...