MagAO-X and HST High-contrast Imaging of the AS209 Disk at Hα
The detection of emission lines associated with accretion processes is a direct method for studying how and where gas giant planets form, how young planets interact with their natal protoplanetary disk, and how volatile delivery to their atmosphere takes
Gabriele Cugno +24 more
doaj +1 more source
Detecting Multiplanetary Systems with Gravitational Microlensing and the Roman Space Telescope
It is plausible that most of the Stars in the Milky Way Galaxy, like the Sun, consist of planetary systems, instead of a single planet. Out of the estimately discovered 3980 planet-hosting stars, about 860 of them are known to be multiplanetary systems ...
Hossein Fatheddin, Sedighe Sajadian
doaj +1 more source
Exoplanet detection in starshade images [PDF]
A starshade suppresses starlight by a factor of 1011 in the image plane of a telescope, which is crucial for directly imaging Earth-like exoplanets.
M. Hu, A. Harness, He Sun, N. Kasdin
semanticscholar +1 more source
A Six Year, Low-resolution, Multibroadband Transit Photometry Study of HD 189733b
Transmission spectroscopy offers an invaluable opportunity to characterize the atmospheres of exoplanets. We present new ground-based optical transmission spectra of the hot Jupiter HD 189733b, derived from nine transits observed over a six year time ...
Cristilyn N. Gardner-Watkins +15 more
doaj +1 more source
Three Warm Jupiters around Solar-analog Stars Detected with TESS
We report the discovery and characterization of three giant exoplanets orbiting solar-analog stars, detected by the TESS space mission and confirmed through ground-based photometry and radial velocity measurements taken at La Silla observatory with FEROS.
Jan Eberhardt +34 more
doaj +1 more source
The Exoplanet Population Observation Simulator. II -- Population Synthesis in the Era of Kepler [PDF]
The collection of planetary system properties derived from large surveys such as Kepler provides critical constraints on planet formation and evolution.
Apai, Daniel +5 more
core +3 more sources
Speckle noise reduction techniques for high-dynamic range imaging [PDF]
High-dynamic range imaging from space in the visible, aiming in particular at the detection of terrestrial exoplanets, necessitates not only the use of a coronagraph, but also of adaptive optics to correct optical defects in real time.
Belikov +23 more
core +3 more sources
Variability of Known Exoplanet Host Stars Observed by TESS
Both direct and indirect methods of exoplanet detection rely upon detailed knowledge of the potential host stars. Such stellar characterization allows for accurate extraction of planetary properties, as well as contributing to our overall understanding ...
Emilie R. Simpson +5 more
doaj +1 more source
Assessing telluric correction methods for Na detections with high-resolution exoplanet transmission spectroscopy [PDF]
ABSTRACT Using high-resolution ground-based transmission spectroscopy to probe exoplanetary atmospheres is difficult due to the inherent telluric contamination from absorption in Earth’s atmosphere. A variety of methods have previously been used to remove telluric features in the optical regime and calculate the planetary transmission ...
Adam B Langeveld +3 more
openaire +2 more sources
Optimal method for exoplanet detection by spectral and angular differential imaging [PDF]
ABSTRACT In the context of the SPHERE planet nder project, we further develop and characterize a recently proposedmethod for the ecient direct detection of exoplanets f rom the ground using spectral and angular dierentialimaging. The method, called ANDROMEDA, combines images appropriately into pseudo-data, then uses allof them in a Maximum ...
Cornia, A. +11 more
openaire +3 more sources

