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Markus Schöller

Researcher at European Southern Observatory

Publications -  286
Citations -  8581

Markus Schöller is an academic researcher from European Southern Observatory. The author has contributed to research in topics: Stars & Magnetic field. The author has an hindex of 43, co-authored 281 publications receiving 7737 citations. Previous affiliations of Markus Schöller include Max Planck Society.

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Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole

Roberto Abuter, +108 more
TL;DR: Eisenhauer et al. as mentioned in this paper detect the combined gravitational redshift and relativistic transverse Doppler effect for S2 of z = Δλ / λ ≈ 200 km s−1/c with different statistical analysis methods.
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Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole.

TL;DR: In this article, the authors detect the combined gravitational redshift and relativistic transverse Doppler effect for S2 of z ~ 200 km/s / c with different statistical analysis methods.
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AMBER, the near-infrared spectro-interferometric three-telescope VLTI instrument

Romain Petrov, +98 more
TL;DR: AMBER as mentioned in this paper is one of the VLTI instruments that combines up to three beams with low, moderate and high spectral resolutions in order to provide milli-arcsecond spatial resolution for compact astrophysical sources in the near-infrared wavelength domain.
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First Light for GRAVITY: Phase Referencing Optical Interferometry for the Very Large Telescope Interferometer

R. Abuter, +131 more
TL;DR: GRAVITY as mentioned in this paper is a new instrument to coherently combine the light of the European Southern Observatory Very Large Telescope Interferometer to form a telescope with an equivalent 130 m diameter angular resolution and a collecting area of 200 m$^2$.
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The building blocks of planets within the ‘terrestrial’ region of protoplanetary disks

TL;DR: Sp spatially resolved detections and compositional analyses of dust building blocks in the innermost two astronomical units of three proto-planetary disks imply that silicates crystallize before any terrestrial planets are formed, consistent with the composition of meteorites in the Solar System.