Schröder, S. E.; Keller, H. U.: The unusual phase curve of Titan's surface observed by Huygens Descent Imager/Spectral Radiometer. Planetary and Space Science 57, pp. 1963 - 1974 (2009)
Sizemore, H. G.; Mellon, M. T.; Searls, M. L.; Lemmon, M. T.; Zent, A. P.; Heet, T. L.; Arvidson, R. E.; Blaney, D. L.; Keller, H. U.: Rocks of the Phoenix Landing Site. Journal Geophysical Research 115, E00E09 (2009)
Smith, P. H.; Tamppari, L. K.; Arvidson, R. E.; Bass, D.; Blaney, D.; Boynton, W. V.; Carswell, A.; Catling, D. C.; Clark, B. C.; Duck, T.et al.; DeJong, E.; Fisher, D.; Goetz, W.; Gunnlaugsson, H. P.; Hecht, M. H.; Hipkin, V.; Hoffman, J.; Hviid, S. F.; Keller, H. U.; Kounaves, S. P.; Lange, C. F.; Lemmon, M. T.; Madsen, M. B.; Markiewicz, W. J.; Marshall, J.; Mckay, C. P.; Mellon, M. T.; Ming, D. W.; Morris, R. V.; Pike, W. T.; Renno, N.; Staufer, U.; Stoker, C.; Taylor, P.; Whiteway, J. A.; Zent, A. P.: H2O at the Phoenix Landing Site. Science 325 (5936), pp. 58 - 61 (2009)
Hecht, M. H.; Marshall, J.; Pike, W. T.; Staufer, U.; Blaney, D.; Braendlin, D.; Gautsch, S.; Goetz, W.; Hidber, H.-R.; Keller, H. U.et al.; Markiewicz, W. J.; Mazer, A.; Meloy, T. P.; Morookian, J. M.; Mogensen, C.; Parrat, D.; Smith, P.; Sykulska, H.; Tanner, R. J.; Reynolds, R. O.; Tonin, A.; Vijendran, S.; Weilert, M.; Woida, P. M.: Microscopy capabilities of the Microscopy, Electrochemistry, and Conductivity Analyzer. Journal Geophysical Research 113, E00A22 (2008)
Inada, A.; Garcia-Comas, M.; Altieri, F.; Gwinner, K.; Poulet, F.; Bellucci, G.; Keller, H. U.; Markiewicz, W. J.; Richardson, M. I.; Hoekzema, N.et al.; Neukum, G.; Bibring, J.-P.: Dust haze in Valles Marineris observed by HRSC and OMEGA on board Mars Express. Journal Geophysical Research 113, E02004 (2008)
Maltagliati, L.; Titov, D. V.; Encrenaz, T.; Melchiorri, R.; Forget, F.; Garcia-Comas, M.; Keller, H. U.; Langevin, Y.; Bibring, J.-P.: Observations of atmospheric water vapor above the Tharsis volcanoes on Mars with the OMEGA/MEx imaging spectrometer. Icarus 194 (1), pp. 53 - 64 (2008)
Schröder, S. E.; Keller, H.-U.: The reflectance spectrum of Titan's surface at the Huygens landing site determined by the Descent Imager/Spectral Radiometer. Planetary and Space Science 56, pp. 753 - 769 (2008)
Skorov, Y. V.; Keller, H. U.; Rodin, A. V.: Optical properties of aerosols in Titan's atmosphere. Planetary and Space Science 56 (5), pp. 660 - 668 (2008)
Basilevsky, A. T.; Keller, H. U.: Craters, smooth terrains, flows, and layering on the comet nuclei. Solar System Research 41 (2), pp. 109 - 117 (2007)
Jorda, L.; Lamy, P.; Faury, G.; Keller, H. U.; Hviid, S.; Küppers, M.; Koschny, D.; Lecacheux, J.; Gutiérrez, P.; Lara, L. M.: Properties of the dust cloud caused by the Deep Impact experiment. Icarus 187, pp. 208 - 219 (2007)
Küppers, M.; Keller, H. U.; Kührt, E.; the CNSR Team: A comet nucleus sample return (CNSR) mission in ESAs Cosmic Vision program. Geochim. Cosmochim. Acta 71, p. A531 (2007)
Küppers, M.; Mottola, S.; Lowry, S. C.; A'Hearn, M. A.; Barbieri, C.; Barucci, M. A.; Fornasier, S.; Groussin, O.; Gutiérrez, P.; Hviid, S. F.et al.; Keller, H. U.; Lamy, P.: Determination of the light curve of the Rosetta target asteroid (2867) Steins by the OSIRIS cameras onboard Rosetta. Astronomy and Astrophysics 462, pp. L13 - L16 (2007)
The European Space Agency (ESA) has given the green light to build the flight models of the spacecraft and science payload for the PLATO mission to search for extrasolar planets.
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
The longest-serving solar observatory in space has turned 25 and is still making significant contributions to solar research. Its old age has become an important merit.