Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
ESA / ESTEC, Research and Scientific Support Department, Noordwijk, 2200 AG Netherlands
ESTEC / RSSD Planetary Mission Division, Keplerlaan 1, Norordwijk, 2200 AG Netherlands / ESTEC / RSSD, Keplerlaan 1, Postbus 299, Noordwijk, 2201 AG Netherlands / RSSD, Keplerlaan 1, Postbus 299, Noordwijk, 2201 AG Netherlands / ESTEC, Research and Scientific Support Dept., Noordwijk, MD 20771 Netherlands
ESA / ESTEC, Research and Scientific Support Dept., Noordwijk, Netherlands
ESA, Keplerlaan 1, Noordwijk, Netherlands
ESA / ESTEC, Research and Scientific Support Department, Noordwijk, Netherlands and Scientific Support department, ESA / ESTEC, Keplerlaan 1, Noordwijk, 2200 AG, Netherlands / ESTEC, Keplerlaan 1, Noordwijk, 2201 AZ, Netherlands ESA, Noordwijk, Netherlands
Laboratoire d'Astrophysique de l'Observatoire de Grenoble
ESA / ESTEC, Postbus 299, Noordwijk, 2200, Netherlands / ESTEC, Postbus 299, Noordwjk, 2200, Netherlands / ESTEC, Keplerlaan 1, Nordwijk, 2200, Netherlands Science Department of ESA, ESTEC, Keplerlaan 1 Postbus 299, Noordwijk, 2200 AG Netherlands
ESA / ESTEC, Netherlands
ESA, European Space Research & Technology Centre Keplerlaan 1 Postbus 299, Noordwijk, 2200 AG, Netherlands / ESTEC, SCI-SM, Keplerlaan 1, Noordwijk, 2200 AG, Netherlands
ESA / ESTEC, Postbus 299, Noordwijk, 2200 AG Netherlands ESA, Netherlands
Research and Scientific Support Department, European Space & Technology Centre Keplerlaan 1 Postbus 299, Noordwijk, 2200 AG Netherlands
RSSD, ESA, Noordwijk, Net
A Herschel resolved far-infrared dust ring around HD 207129
A peculiar class of debris disks from Herschel/DUNES - A steep fall off in the far infrared
A VLTI/AMBER closure-phase search for low-mass companions around nearby young stars: first results on beta Pictoris
An icy Kuiper-Belt around the young solar-type star HD 181327
Automated analysis of Current-Voltage Characteristics for the ISL experiment of DEMETER
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