The Physik von stark bestrahlten Thermosphären extrasolarer Planeten

• Antragsteller: Professor Dr. Jürgen H.M.M. Schmitt
• Fachliche Zuordnung: Astrophysik und Astronomie
• Förderung: Förderung von 2016 bis 2021
• Projektkennung: Deutsche Forschungsgemeinschaft (DFG) - Projektnummer 314569934

• Erstellungsjahr: 2022

Zusammenfassung der Projektergebnisse

The work carried out in this project yielded two ”firsts”: First, the demonstration that planetary transit observations can be carried out with SWIFT in the UV, thus opening a new observational window in addition to the HST; and second, the demonstration that planetary transits in He I 10830 can be studied from the ground with suitable instrumentation (such as CARMENES). The only previous detection had been made with HST!

Projektbezogene Publikationen (Auswahl)

• 2018, A&A, 620 A97: Detection of He I λ 10830 Å absorption on HD 189733 b with CARMENES high-resolution transmission spectroscopy
  Salz, M., Czesla, S., Schneider, P. C., Nagel, E., Schmitt, J. H. M. M., et al.
  
• A&A, 2018, 618, A98: ”The atmosphere of WASP-17b: Optical high-resolution transmission spectroscopy”
  Khalafinejad, S., Salz, M., Cubillos, P. E. et al.
  
• Science, 2018, 362, 1388: Ground-based detection of an extended helium atmosphere in the Saturn-mass exoplanet WASP-69b
  Nortmann, L., Pallé, E., Salz, M. et al.
  
• 2019, A&A, 623 A57: ”Swift UVOT near-UV transit observations of WASP-121 b”
  Salz, M., Schneider, P. C., Fossati, L., Czesla, S., France, K., Schmitt, J. H. M. M.
  
• A&A, 2019, 619, A96: HD 189733 b: bow shock or no shock?
  Kohl, S. , Salz, M., Czesla, S., Schmitt, J.H.M.M.
  
• A&A, 2019, 629, A5: X-ray emission in the enigmatic CVSO 30 system
  Czesla, S., Schneider, P. C., Salz, M., et al.