Results 161 to 170 of about 478,002 (271)

TOI-4504: Exceptionally Large Transit Timing Variations Induced by Two Resonant Warm Gas Giants in a Three-planet System

open access: yesThe Astrophysical Journal Letters
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

Benefits of Ground-Based Photometric Follow-Up for Transiting Extrasolar Planets Discovered with Kepler and CoRoT

open access: yes, 2009
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 TESS–Keck Survey. XIX. A Warm Transiting Sub-Saturn-mass Planet and a Nontransiting Saturn-mass Planet Orbiting a Solar Analog

open access: yesThe Astronomical Journal
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

open access: yesThe Astronomical Journal
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]

open access: bronze, 2008
J. M. Fernández   +2 more
openalex   +1 more source

Quantifying the Effect of Short-timescale Stellar Activity Upon Transit Detection in M Dwarfs

open access: yesThe Astronomical Journal
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]

open access: yesInnovation (Camb), 2022
Ge J   +4 more
europepmc   +1 more source

Improved Orbital Parameters And Transit Monitoring For HD 156846b [PDF]

open access: yes, 2013
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]

open access: bronze, 2009
J. Southworth   +22 more
openalex   +1 more source

A Search for Refraction in Kepler Photometry of Gas Giants [PDF]

open access: yesarXiv, 2018
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  

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