VLBI: Arrays & Techniques Arrays: a brief tour Model / delay constituents Difference phase – the key to astrometry Applications / Calibrations Wide-field mapping Geodesy…

Spectral Line VLBI Chris Phillips JIVE The Netherlands Spectral Line Sources VLBI  High brightness temperatures Masers: Galactic OH, H2O, SiO, CH3OH Extragalactic OH,…

VLBI: Arrays & Techniques Arrays: a brief tour Model / delay constituents Difference phase – the key to astrometry Applications / Calibrations Wide-field mapping Geodesy…

Deep, wide-field global VLBI observations of HDF-N Seungyoup Chi Kapteyn Institute (RuG) / JIVE Collaborators : M. A. Garrett, P. D. Barthel et al. 8th EVN Symposium 2006…

Iván Agudo with the collaboration of: S.N. Molina, J. L. Gómez (IAA-CSIC) T. P. Krichbaum, A. Roy, U. Bach (MPIfR) I. Martí Vidal (Chalmers) B. Campbell (JIVE) Signs of…