We report on sulphur abundances in halo stars as derived from near-IR UVES spectra. The importance of removing telluric lines and residual CCD fringing patterns...
Sulphur Abundances in Metal-Poor Stars First Result from CRIRES Science Verification
Sulphur is the tenth most abundant element in the Universe and plays an im-portant role in studies of the chemical enrichment and star formation history of...
Summer 2002 photometric multisite campaign on the open cluster NGC 6633
NGC 6633 is a solar metallicity, young open cluster. In addition to providing useful information from an asteroseismic point of view, it has the additional...
Sun Cities: Thebes, Hattusha, and Petra: A Landscape Story
The sky is a very important component of the landscape that has been lost in our modern, overcrowded, and excessively illuminated cities. However, this was not...
Sunrise Chromospheric Infrared SpectroPolarimeter (SCIP) for sunrise III: system design and capability
The Sunrise balloon-borne solar observatory carries a 1 m aperture optical telescope and provides us a unique platform to conduct continuous seeing-free...
SUNRISE Impressions from a successful science flight
SUNRISE is a balloon-borne telescope with an aperture of one meter. It is equipped with a filter imager for the UV wavelength range between 214 nm and 400 nm...
Sunrise is a light-weight solar telescope with a 1 m aperture for spectro-polarimetric observations of the solar atmosphere. The telescope is planned to be...
SUNRISE: a balloon-borne telescope for high resolution solar observations in the visible and UV
Sunrise is a light-weight solar telescope with a 1 m aperture for spectro-polarimetric observations of the solar atmosphere. The telescope is planned to be...