activity
20082023
most citedCRIRES on sky at the ESO Very Large Telescope

84 citations · 115 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.IM2023★ 84 cited

CRIRES on sky at the ESO Very Large Telescope

R. J. Dorn, P. Bristow, J. V. Smoker +49

The CRyogenic InfraRed Echelle Spectrograph (CRIRES) Upgrade project CRIRES extended the capabilities of CRIRES. It transformed this VLT instrument into a cross-dispersed spe…

astro-ph.IM2014★ 10 cited

Concept and optical design of the cross-disperser module for CRIRES+

E. Oliva, A. Tozzi, D. Ferruzzi +31

CRIRES, the ESO high resolution infrared spectrometer, is a unique instrument which allows astronomers to access a parameter space which up to now was largely uncharted. In its cur…

astro-ph.SR2011

MIDI interferometry of massive YSOs: Updates on the MPIA programme

Hendrik Linz, Roman Follert, Paul A. Boley +4

Information about the inner structure of young stellar objects is crucial for understanding how the central forming stars gain their mass. However, especially for observations of (…

astro-ph.SR2010★ 12 cited

Mid - infrared interferometry of massive young stellar objects II Evidence for a circumstellar disk surrounding the Kleinmann - Wright object

R. Follert, H. Linz, B. Stecklum +5

The formation scenario for massive stars is still under discussion. To further constrain current theories, it is vital to spatially resolve the structures from which material accre…

astro-ph.IM2009★ 4 cited

An active fiber sensor for mirror vibration metrology in astronomical interferometers

S. Minardi, A. Chipouline, S. Krämer +4

We present a fiber sensor based on an active integrated component which could be effectively used to measure the longitudinal vibration modes of telescope mirrors in an interferome…

astro-ph2008★ 4 cited

Mid-infrared interferometry of massive young stellar objects

H. Linz, B. Stecklum, R. Follert +5

The very inner structure of massive young stellar objects (YSOs) is difficult to trace. With conventional observational methods we identify structures still several hundreds of AU…