by SK Heftel
2019
Cited by 7
In their method, Liao et al. reported that the photometric transit signals were detectable with ground-based telescopes.
We use 3.6 years of follow-up data from the SuperWASP-North and SuperWASP-South in Australia and six years of data from the SIDE-WASP network in Italy to estimate the frequencies of transits and eclipses in the WASP planet population.
by EA Gomes
2017
Cited by 10
We performed a theoretical analysis of the linear and quadratic transit timing variations of transiting exoplanets, .
by M Madhusudhan
2020
Cited by 30
Observation of magnetic fields and geometry in the chromosphere using spectropolarimetry. .
by J Scharmer
2018
Cited by 4
We investigate the inversion of vertical magnetic fields using spectropolarimetry in the cores of sunspots. .
by J Wang
2019
Cited by 5
We model 3D, time-dependent disk-driven jet driven by the accretion disk with a highly collimated flow. .
by M Shadmehri
2019
Cited by 4
We show that the efficient fractionation of H$_2$O along the hot disk midplane is dominated by the gravitational settling and the effect of H$_2$O photodissociation,.
by H Kataoka
2020
Cited by 17
A study of the enrichment of the gas-phase SiO in the atmospheres of hot Jupiters. .
by A Tokunaga
2020
Cited by 2
A Combined Spectroscopic and Photometric Investigation of the Transiting Exoplanet WASP-24b
As a second target, we chose 47UMa, a planet with an orbital period of 2.5 days that was discovered by Pont et al. (2010) and confirmed by the team. Both the host star and the planet are young with an age of $ be359ba680
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