Results 161 to 170 of about 478,002 (271)
We present a joint analysis of transit timing variations (TTVs) and Doppler data for the transiting exoplanet system TOI-4504. TOI-4504 c is a warm Jupiter-mass planet that exhibits the largest known TTVs, with a peak-to-node amplitude of ∼2 days, the ...
Michaela Vítková+26 more
doaj +1 more source
Currently, over forty transiting planets have been discovered by ground-based photometric surveys, and space-based missions like Kepler and CoRoT are expected to detect hundreds more.
Bakos+27 more
core +1 more source
The Transiting Exoplanet Survey Satellite (TESS) continues to increase dramatically the number of known transiting exoplanets, and is optimal for monitoring bright stars amenable to radial velocity (RV) and atmospheric follow-up observations. TOI-1386 is
Michelle L. Hill+47 more
doaj +1 more source
Two Earth-size Planets and an Earth-size Candidate Transiting the nearby Star HD 101581
We report the validation of multiple planets transiting the nearby ( d = 12.8 pc) K5V dwarf HD 101581 (GJ 435, TOI–6276, TIC 397362481). This system consists of at least two Earth-size planets whose orbits are near a mutual 4:3 mean-motion resonance, HD ...
Michelle Kunimoto+45 more
doaj +1 more source
Optical Follow up Photometry of the Transiting Extrasolar Planet XO-2 [PDF]
J. M. Fernández+2 more
openalex +1 more source
Quantifying the Effect of Short-timescale Stellar Activity Upon Transit Detection in M Dwarfs
M dwarf stars comprise 70%–80% of the galaxy's stars and host most of its rocky planets. They also differ from Sunlike stars in that they are “active” for billions of years or more: rotating quickly, flaring often, and emitting large amounts of UV and X ...
Dana Clarice Yaptangco+3 more
doaj +1 more source
The ET mission to search for earth 2.0s. [PDF]
Ge J+4 more
europepmc +1 more source
Improved Orbital Parameters And Transit Monitoring For HD 156846b [PDF]
HD 156846b is a Jovian planet in a highly eccentric orbit (e = 0.85) with a period of 359.55 days. The pericenter passage at a distance of 0.16 AU is nearly aligned to our line of sight, offering an enhanced transit probability of 5.4% and a potentially ...
Ciardi, D. R.+12 more
core +2 more sources
High-precision photometry by telescope defocusing - I. The transiting planetary system WASP-5 [PDF]
J. Southworth+22 more
openalex +1 more source
A Search for Refraction in Kepler Photometry of Gas Giants [PDF]
Refraction can lead to a brightening just before ingress and just after egress of a transit, as light passes through the exoplanet's atmosphere and is refracted into our line of sight. Refraction just outside of transit has been seen and modeled in our own solar system during transits of Venus.
arxiv