Results 41 to 50 of about 536,227 (395)

A Theory of Exoplanet Transits with Light Scattering [PDF]

open access: yes, 2017
Exoplanet transit spectroscopy enables the characterization of distant worlds, and will yield key results for NASA's James Webb Space Telescope.
T. Robinson
semanticscholar   +1 more source

Exoplanet Nodal Precession Induced by Rapidly Rotating Stars: Impacts on Transit Probabilities and Biases

open access: yesThe Astrophysical Journal, 2023
For the majority of short-period exoplanets transiting massive stars with radiative envelopes, the spin angular momentum of the host star is greater than the planetary orbital angular momentum.
Alexander P. Stephan, B. Scott Gaudi
doaj   +1 more source

A search for transits of GJ 581\lowercase{e} and characterization of the host star variability using MOST space telescope photometry [PDF]

open access: yes, 2012
The GJ 581 system has been amply studied since its discovery in 2005: the number of known planets in the system has increased and their orbital parameters are among the most precisely determined for radial velocity detected exoplanets.
Dragomir, Diana   +9 more
core   +2 more sources

Measuring stellar granulation during planet transits [PDF]

open access: yes, 2016
Stellar activity and convection-related surface structures might cause bias in planet detection and characterization that use these transits. Surface convection simulations help to quantify the granulation signal.
A. Chiavassa   +9 more
semanticscholar   +1 more source

TESS Spots a Super-puff: The Remarkably Low Density of TOI-1420b

open access: yesThe Astronomical Journal, 2023
We present the discovery of TOI-1420b, an exceptionally low-density ( ρ = 0.08 ± 0.02 g cm ^−3 ) transiting planet in a P = 6.96 days orbit around a late G-dwarf star.
Stephanie Yoshida   +53 more
doaj   +1 more source

Circumbinary planets - II. When transits come and go [PDF]

open access: yes, 2016
Circumbinary planets are generally more likely to transit than equivalent single-star planets, but practically the geometry and orbital dynamics of circumbinary planets make the chance of observing a transit inherently time-dependent.
D. Martin
semanticscholar   +1 more source

Transition-type change between an inverted Berezinskii-Kosterlitz-Thouless transition and an abrupt transition in the bond percolation on a random hierarchical small-world network [PDF]

open access: yesPhys. Rev. E 89, 042803 (2014), 2013
We study bond percolation on a one-parameter family of hierarchical small-world network, and find a meta-transition between the inverted BKT transition and the abrupt transition driven by changing the network topology. It is found that the order parameter is continuous and fractal exponent is discontinuous in the inverted BKT transition, and oppositely,
arxiv   +1 more source

Limit shape phase transitions: a merger of arctic circles [PDF]

open access: yes, 2022
We consider a free fermion formulation of a statistical model exhibiting a limit shape phenomenon. The model is shown to have a phase transition that can be visualized as the merger of two liquid regions - arctic circles. We show that the merging arctic circles provide a space-time resolved picture of the phase transition in lattice QCD known as Gross ...
arxiv   +1 more source

A Search for Additional Bodies in the GJ 1132 Planetary System from 21 Ground-based Transits and a 100-hr Spitzer Campaign [PDF]

open access: yes, 2016
We present the results of a search for additional bodies in the GJ 1132 system through two methods: photometric transits and transit timing variations of GJ 1132b. We collected 21 transit observations of GJ 1132b with the MEarth-South array.
J. Dittmann   +4 more
semanticscholar   +1 more source

Prehistory of Transit Searches

open access: yes, 2018
Nowadays the more powerful method to detect extrasolar planets is the transit method. We review the planet transits which were anticipated, searched, and the first ones which were observed all through history. Indeed transits of planets in front of their
A Helden Van   +36 more
core   +2 more sources

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