Shaposhnikov, D.; Rodin, A. V.; Medvedev, A. S.; Hartogh, P.: Hydrological cycle in the general circulation model of the Martian atmosphere. Sixth international workshop on the Mars atmosphere: Modelling and observations , Granada, Spain (2017)
Rengel, M.; Reach, W.; Hartogh, P.; Sagawa, H.: Tracing the Composition of Hydrogen Cyanide in the Stratosphere of Titan from Space, Airborne, and Ground-Based Observations. ESA SCI Science Workshop #9, Aklersloot, Netherlands (2016)
Rengel, M.; Sagawa, H.; Hartogh, P.: Venusian Mesospheric thermal structure and winds from May 2009 SMT CO spectral- line observations. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Rezac, L.; de Val-Borro, M.; Hartogh, P.; Cavalié, T.; Jarchow, C.; Rengel, M.; Dobrijevic, M.: New Determination of the HCN Profile in the Stratosphere of Neptune from Millimeter-wave Spectroscopy. Asia Oceania Geosciences Society (AOGS) 11th Annual Meeting, Sapporo, Japan (2014)
Hartogh, P.: Chirptransformations-Spektrometer für die passive Millimeterwellenradiometrie: Messungen der 142 GHz Emissionslinie des atmosphärischen Ozons. Dissertation, Georg-August-Universität Göttingen (1989)
Hartogh, P.: Raumflugtauglicher FM-Pulskompressionsempfänger mit Oberflächenwellenfiltern für die Millimeter- und Submillimeterwellenspektroskopie. Diploma, Georg-August-Universität Göttingen (1985)
Biver, N.; Bockelée-Morvan, D.; Moreno, R.; Crovisier, J.; Hartogh, P.; de Val-Borro, M.; Kidger, M.; Kueppers, M.; Szutowicz, S.; Lis, D. C.et al.; Blake, G. A.; Gonzalez, J. J.; Seargent, D. A. J.; Mattiazzo, M.: Comet C/2011 L4 (Panstarrs). Central Bureau Electronic Telegrams 3230, 1 (2012)
Meister, C.-V.; Hartogh, P.; Villanueva, G.; Berger, U.: Hydrodynamic model of the Martian atmosphere between near-surface layers and an altitude of about 130 km. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (2002)
Gulkis, S.; Forget, F.; Janssen, M.; Riley, L.; Hartogh, P.; Clancy, T.; Allen, M.; Frerking, M.: Microwave Investigation of the Martian Atmosphere and Surface. JPL, California Institute of Technology, Pasadena, CA, USA (2000)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
Data from NASA's Dawn mission, analyzed for the first time, suggest that brine rose from the depths and organic compounds were deposited in Urvara crater.