Science

This table lists some observing programmes that I am or have been involved in:

Programme TitleTelescope, InstrumentPI, CoIObservations started in
Is there an abundance gradient in the Inner Galactic Bulge?VLT-UT1 and UT3, ISAAC and CRIRESCoIJune 2012
Dust production and the close circumstellar environment of the exceptional C-star BH CruVLT-UT3, VISIRPIMarch 2012
CRIRES-POP: A library of high resolution spectra in the near-infrared, see also here!VLT-UT1, CRIRESCoIOctober 2009
The evolutionary state of Miras with changing pulsation periodsMercator, HermesPIJuly 2009
Confining lithium-rich phases on the RGBVLT-UT2, FLAMES-GiraffeCoIJune 2009
Cool Bottom Processing in Li-rich Galactic bulge AGB stars?VLT-UT1, CRIRESPIJune 2009
The variability of the lithium line in C-type AGB starsMercator, HermesPIApril 2009
Technetium and Cool Bottom Processing in the Galactic S-star V441 Cyg (DDT) 2.2m on Calar Alto, FOCESPIJune 2008
Tracing the AGB evolution and dust formation through high resolution near-infrared spectroscopyVLT-UT1, CRIRESCoIJune 2008
The mass dependence of Fluorine synthesis in massive Galactic AGB starsVLT-UT1, CRIRESPIMay 2008

To conduct science with these observations, I collaborate with several scientists, spread over this planet:

With other scientists, I have more informal contacts, which are not (yet) manifested in common observing projects or papers.

Instrumentation

I am involved in a few instrumentation projects, with varying intensity. During my PhD thesis, partly carried out at ESO headquarters, I was involved in the CRIRES spectrograph project, in particular during commissioning and science verification runs. See also Chapter 6 of my PhD thesis for my contribution to this spectrograph. At the moment, I contribute to improving the understanding and reduction of CRIRES data via the CRIRES-POP project.

During my post-doc at the Instituut voor Sterrenkunde at the University of Leuven, Belgium, I became involved in the Phase A study of METIS (Mid-infrared ELT Imager and Spectrograph), the proposed mid-IR instrument for ESO's E-ELT. The documents of the Phase A study have been submitted to ESO on 17 November 2009. In particular, I contributed to the Operational Concepts definition document (calibration of the instrument and correction of observed spectra for telluric absorption lines, etc.). The Department of Astrophysics in Vienna is an official member in the METIS consortium as of May 2012. Our department will contribute to METIS in the science pipeline work package.

Stefan Uttenthaler - last update June 13, 2012.