Stenzel, O.: Alkali Metals in Cometary Particles what is the Chemical Context? 50th ESLAB Symposium: From Giotto to Rosetta, Leiden, Netherlands (2016)
Stenzel, O. J.; Paquette, J.; the Cosima Team: Boron and Oxygen in Cometary Particles. 79th Annual Meeting of the Meteoritical Society, Berlin, Germany (2016)
Stenzel, O. J.; Varmuza, K.; Engrand, C.; Ferriere, L.; Brandstätter, F.; Koeberl, C.; Filzmoser, P.; Paquette, J.; Hilchenbach, M.: Using Meteorite Samples as a Test for Correlation Based Analysis of SIMS Data from Cometary Grains. 46th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2015)
Stenzel, O. J.; Varmuza, K.; Engrand, C.; Ferrière, L.; Brandstätter, F.; Koeberl, C.; Filzmoser, P.; Paquette, J.; Hilchenbach, M.: Correlation Based analysis of SIMS Data from Meteorite Samples for Comparison with Cometary Grains. European Planetary Science Congress, Nantes, France (2015)
Paquette, J.; Engrand, C.; Stenzel, O.; Hilchenbach, M.: Measuring Oxygen Isotopes with COSIMA. American Geophysical Union Fall Meeting, San Francisco, USA (2014)
Paquette, J. A.; Stenzel, O.: The Effects of Sputtering Yields on the Rosetta/COSIMA Instrument Efficiency. Asteroids Comets Meteors 2014, Helsinki, Finland (2014)
Reiss, D.; Hoekzema, N. M.; Stenzel, O. J.: Dust Deflation by Dust Devils on Mars Derived from Optical Depth Measurements Using the Shadow Method in HiRISE Images. 45th Lunar and Planetary Science Conference, The Woodlands, Texas (2014)
Stenzel, O. J.; Hoekzema, N. M.; Markiewicz, W. J.: Mars' Atmospheric Optical Depth from Mars Express HRSC and Mars Exploration Rovers A Comparison. 45th Lunar and Planetary Science Conference, The Woodlands, Texas (2014)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
For PhD students whose project is already funded and who are applying for admission to the IMPRS, or for applicants who want to bring their own funding and their own project idea to the IMPRS.