Stellar obliquities in exoplanetary systems

SH Albrecht, RI Dawson, JN Winn - Publications of the …, 2022 - iopscience.iop.org
The rotation of a star and the revolutions of its planets are not necessarily aligned. This
article reviews the measurement techniques, key findings, and theoretical interpretations …

Tidal dissipation in stars and giant planets

GI Ogilvie - Annual Review of Astronomy and Astrophysics, 2014 - annualreviews.org
Astrophysical fluid bodies that orbit close to one another induce tidal distortions and flows
that are subject to dissipative processes. The spin and orbital motions undergo a coupled …

AstroImageJ: image processing and photometric extraction for ultra-precise astronomical light curves

KA Collins, JF Kielkopf, KG Stassun… - The Astronomical …, 2017 - iopscience.iop.org
ImageJ is a graphical user interface (GUI) driven, public domain, Java-based, software
package for general image processing traditionally used mainly in life sciences fields. The …

Accurate empirical radii and masses of planets and their host stars with Gaia parallaxes

KG Stassun, KA Collins, BS Gaudi - The Astronomical Journal, 2017 - iopscience.iop.org
We present empirical measurements of the radii of 116 stars that host transiting planets.
These radii are determined using only direct observables—the bolometric flux at Earth, the …

[HTML][HTML] Optimized transit detection algorithm to search for periodic transits of small planets

M Hippke, R Heller - Astronomy & Astrophysics, 2019 - aanda.org
We present a new method to detect planetary transits from time-series photometry, the transit
least squares (TLS) algorithm. TLS searches for transit-like features while taking the stellar …

Five key exoplanet questions answered via the analysis of 25 hot-Jupiter atmospheres in eclipse

Q Changeat, B Edwards, AF Al-Refaie… - The Astrophysical …, 2022 - iopscience.iop.org
Population studies of exoplanets are key to unlocking their statistical properties. So far, the
inferred properties have been mostly limited to planetary, orbital, and stellar parameters …

Fundamental parameters and spectral energy distributions of young and field age objects with masses spanning the stellar to planetary regime

JC Filippazzo, EL Rice, J Faherty, KL Cruz… - The Astrophysical …, 2015 - iopscience.iop.org
We combine optical, near-infrared, and mid-infrared spectra and photometry to construct
expanded spectral energy distributions for 145 field age (> 500 Myr) and 53 young (lower …

A giant planet undergoing extreme-ultraviolet irradiation by its hot massive-star host

BS Gaudi, KG Stassun, KA Collins, TG Beatty, G Zhou… - Nature, 2017 - nature.com
The amount of ultraviolet irradiation and ablation experienced by a planet depends strongly
on the temperature of its host star. Of the thousands of extrasolar planets now known, only …

Exploring the ability of Hubble Space Telescope WFC3 G141 to uncover trends in populations of exoplanet atmospheres through a homogeneous transmission survey …

B Edwards, Q Changeat, A Tsiaras… - The Astrophysical …, 2023 - iopscience.iop.org
We present analysis of the atmospheres of 70 gaseous extrasolar planets via transit
spectroscopy with Hubble's Wide Field Camera 3 (WFC3). For over half of these, we …

MuSCAT2: four-color simultaneous camera for the 1.52-m Telescopio Carlos Sánchez

N Narita, A Fukui, N Kusakabe… - Journal of …, 2019 - spiedigitallibrary.org
We report the development of a four-color simultaneous camera for the 1.52-m Telescopio
Carlos Sánchez in the Teide Observatory, Canaries, Spain. The instrument, named …