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: Instrument, Mission, Data, and First Results
The SUNRISE balloon-borne solar observatory consists of a 1 m aperture Gregory telescope, a UV filter imager, an imaging vector polarimeter, an image...
Super-Earth of 8 M⊕ in a 2.2-day orbit around the K5V star K2-216
Context. Although thousands of exoplanets have been discovered to date, far fewer have been fully characterised, in particular super-Earths. The KESPRINT...
Superluminal non-ballistic jet swing in the quasar NRAO 150 revealed by mm-VLBI
Context: NRAO 150, a compact and bright radio to mm source showing core/jet structure, has been recently identified as a quasar at redshift z = 1.52 through a...
Surface composition and dynamical evolution of two retrograde objects in the outer solar system: 2008 YB3 and 2005 VD
Most of the objects in the trans-Neptunian belt (TNb) and related populations move in prograde orbits with low eccentricity and inclination. However, the list...
Surface Rotation and Photometric Activity for Kepler Targets. I. M and K Main-sequence Stars
Brightness variations due to dark spots on the stellar surface encode information about stellar surface rotation and magnetic activity. In this work, we analyze...
Survey of Surveys. I. The largest compilation of radial velocities for the Galaxy
Context. In the present-day panorama of large spectroscopic surveys, the amount, diversity, and complexity of the available data continuously increase. The...
Surveys for low-mass stars and brown dwarfs: Solar Neighbourhood and intermediate-age clusters Alpha Per and Collinder 359
Lipid bilayers are key components of biomembranes; they are self-assembled two-dimensional structures, primarily serving as barriers to the leakage of cell's...
SWEET-Cat update and FASMA. A new minimization procedure for stellar parameters using high-quality spectra
Context. Thanks to the importance that the star-planet relation has to our understanding of the planet formation process, the precise determination of stellar...