Add to ORKGIn this thesis, I describe the search for transiting hot Jupiters with a focus on cool dwarfs, low-mass main-sequence stars. I detail the results of our Pan-Planets survey and the necessary follow-up and show a discovered planet in the Beehive cluster M44, a transiting hot Neptune around an M dwarf. Finally, I evaluate our results in the context of planet occurrence rate and demonstrate that we set more precise limits for hot Jupiters in M dwarf systems than other projects before us.Deutsche Übersetzung des Titels: Die Suche nach heißen Jupiter-Transits um kühle Stern
Many current exoplanetary surveys focus on stars thought likely to host detectable habitable rocky p...
For planets with very small semi-major axes, the implications of residing so close to a star can be ...
In this thesis the results of the multifrequency VLBA observations of the GPS 1944+5448 and the HFP ...
In this thesis, I describe the search for transiting hot Jupiters with a focus on cool dwarfs, low-m...
With over 4000 discoveries to date, the field of exoplanets is rapidly expanding. The large numbers ...
The University of North Dakota Space Studies Internet Observatory was used to observe the transits o...
The study of exoplanets has rapidly developed in the last twenty years, and the detailed characteriz...
Circumbinary planets are bodies that orbit both components in a binary star system. This thesis focu...
The characteristics and dynamics of exoplanets are broad and diverse. Detailed analysis of the syste...
Photometric transit surveys on the ground & in space have detected thousands of transiting exoplanet...
This Ph.D. Thesis has as general subject the study of extrasolar planets using the radial velocity t...
The research on exoplanet atmospheres has expanded rapidly over the last two decades since the first...
Jupiter has long been a subject of fascination and curiosity. Recently it has become the focus of nu...
Around a third of the stars in our Galaxy are binary or multiple systems, with triples possibly acco...
This thesis is focused on the photometric analysis of stellar light curves (LCs), to search for vari...
Many current exoplanetary surveys focus on stars thought likely to host detectable habitable rocky p...
For planets with very small semi-major axes, the implications of residing so close to a star can be ...
In this thesis the results of the multifrequency VLBA observations of the GPS 1944+5448 and the HFP ...
In this thesis, I describe the search for transiting hot Jupiters with a focus on cool dwarfs, low-m...
With over 4000 discoveries to date, the field of exoplanets is rapidly expanding. The large numbers ...
The University of North Dakota Space Studies Internet Observatory was used to observe the transits o...
The study of exoplanets has rapidly developed in the last twenty years, and the detailed characteriz...
Circumbinary planets are bodies that orbit both components in a binary star system. This thesis focu...
The characteristics and dynamics of exoplanets are broad and diverse. Detailed analysis of the syste...
Photometric transit surveys on the ground & in space have detected thousands of transiting exoplanet...
This Ph.D. Thesis has as general subject the study of extrasolar planets using the radial velocity t...
The research on exoplanet atmospheres has expanded rapidly over the last two decades since the first...
Jupiter has long been a subject of fascination and curiosity. Recently it has become the focus of nu...
Around a third of the stars in our Galaxy are binary or multiple systems, with triples possibly acco...
This thesis is focused on the photometric analysis of stellar light curves (LCs), to search for vari...
Many current exoplanetary surveys focus on stars thought likely to host detectable habitable rocky p...
For planets with very small semi-major axes, the implications of residing so close to a star can be ...
In this thesis the results of the multifrequency VLBA observations of the GPS 1944+5448 and the HFP ...