Add to ORKGThe Space mission DWARFS is designed to determine atmospheric composition and physical properties of rocky extrasolar planets in the habitable zone around M-Type stars. Most importantly, we want to research the atmospheric composition with a special emphasize on O3, H2O, CH, CH4, CO2, CH3Cl lines, as well as the evolution of the planetary systems. For some of the stars DWARFS will be able to detect in addition surface features, moons or further planets in the system. All this will be done with two spectrographs in the NIR/MIR and a photometer (r, i SDSS) in a 4m space telescope
M dwarf stars have emerged as ideal targets for exoplanet observations. Their small radii aids plane...
M dwarfs have proven to be fascinating targets for exoplanetary search, from the growing evidence fr...
Aims The SHINE program is a high-contrast near-infrared survey of 600 young, nearby stars aimed at s...
The Space mission DWARFS is designed to determine atmospheric composition and physical properties of...
Thesis (Ph.D.)--University of Washington, 2020In the next few years, the launch of the James Webb Sp...
We model the atmospheres and spectra of Earth-like planets orbiting the entire grid of M dwarfs for...
We model the atmospheres and spectra of Earth-like planets orbiting the entire grid of M dwarfs for ...
Thesis (Ph.D.)--University of Washington, 2017-08As the technology behind instrumentation in astrono...
The authors acknowledge support from DFG funding ENP KA 3142/1-1 and the Simons Foundation (290357, ...
Context. The characterisation of the atmosphere of exoplanets is one of the main goals of exoplanet ...
The first atmospheres to be characterized on potentially habitable, rocky exoplanets will likely be ...
M dwarfs are the most numerous type of stars in the Universe. Their low masses and their large plane...
Coupled one-dimensional photochemical-climate calculations have been performed for hy-pothetical Ear...
We present design considerations for a ground-based survey for transiting exoplanets around L and T ...
Ph.D. University of Hawaii at Manoa 2013.Includes bibliographical references.M dwarfs have become at...
M dwarf stars have emerged as ideal targets for exoplanet observations. Their small radii aids plane...
M dwarfs have proven to be fascinating targets for exoplanetary search, from the growing evidence fr...
Aims The SHINE program is a high-contrast near-infrared survey of 600 young, nearby stars aimed at s...
The Space mission DWARFS is designed to determine atmospheric composition and physical properties of...
Thesis (Ph.D.)--University of Washington, 2020In the next few years, the launch of the James Webb Sp...
We model the atmospheres and spectra of Earth-like planets orbiting the entire grid of M dwarfs for...
We model the atmospheres and spectra of Earth-like planets orbiting the entire grid of M dwarfs for ...
Thesis (Ph.D.)--University of Washington, 2017-08As the technology behind instrumentation in astrono...
The authors acknowledge support from DFG funding ENP KA 3142/1-1 and the Simons Foundation (290357, ...
Context. The characterisation of the atmosphere of exoplanets is one of the main goals of exoplanet ...
The first atmospheres to be characterized on potentially habitable, rocky exoplanets will likely be ...
M dwarfs are the most numerous type of stars in the Universe. Their low masses and their large plane...
Coupled one-dimensional photochemical-climate calculations have been performed for hy-pothetical Ear...
We present design considerations for a ground-based survey for transiting exoplanets around L and T ...
Ph.D. University of Hawaii at Manoa 2013.Includes bibliographical references.M dwarfs have become at...
M dwarf stars have emerged as ideal targets for exoplanet observations. Their small radii aids plane...
M dwarfs have proven to be fascinating targets for exoplanetary search, from the growing evidence fr...
Aims The SHINE program is a high-contrast near-infrared survey of 600 young, nearby stars aimed at s...