The grand tradition v007
Kepler 413b a_slightly_misaligned_neptune_size_transiting_circumbinary_planet
Lessons for STEREO - learned from Helios Presented at the STEREO/Solar B Workshop, 17.11.2005 Rainer Schwenn, MPS Lindau [email protected] The Helios.
Polarization 2005, Orsay, 13/09/2005 Depolarization canals in Milky Way radio maps Anvar Shukurov and Andrew Fletcher School of Mathematics and Statistics,
KBO Workshop, DPS 2003 - Stellar occultations are diffracting phenomena - A powerful tool to accede to invisible small KBO - First results of the Pic du.
Wijnholds 2006 The potential for Galactic Plane Surveys with LOFAR Glenn White – The Open University UK, and The Rutherford Appleton Laboratory UK On behalf.
The mass ratio of the stellar components of a spectroscopic binary can be directly computed from their ratio in radial velocities. To derive the total.
03/000 Cosmologic astrometry Australian Government Geoscience Australia Yonsei University, Seoul 18 October 2010.
Submillimeter ( l < 1 mm) Continuum Imaging at CSO: a Retrospective C. Darren Dowell (Caltech),
Controlling Field-of-View of Radio Arrays using Weighting Functions MIT Haystack FOV Group: Lynn D. Matthews,Colin Lonsdale, Roger Cappallo, Sheperd Doeleman,
ESO
Preparing for STEREO – revisit Helios