  We present the results of the first multiwavelength observing campaign on the
high-mass X-ray binary LS I +61 303 comprising observations at the TeV regime
with the MAGIC telescope, along with X-ray observations with Chandra, and radio
interferometric observations with the MERLIN, EVN and VLBA arrays, in October
and November 2006. From our MERLIN observations, we can exclude the existence
of large scale (~100 mas) persistent radio-jets. Our 5.0 GHz VLBA observations
display morphological similarities to previous 8.4 GHz VLBA observations
carried out at the same orbital phase, suggesting a high level of periodicity
and stability of the processes behind the radio emission. This makes it
unlikely that variability of the radio emission is due to the interaction of an
outflow with variable wind clumps. If the radio emission is produced by a
milliarcsecond scale jet, it should also show a stable, periodic behavior. It
is then difficult to reconcile the absence of a large scale jet (~100 mas) in
our observations with the evidence of a persistent relativistic jet reported
previously. We find a possible hint of temporal correlation between the X-ray
and TeV emissions and evidence for radio/TeV non-correlation, which points to
the existence of one population of particles producing the radio emission and a
different one producing the X-ray and TeV emissions. Finally, we present a
quasi-simultaneous energy spectrum including radio, X-ray and TeV bands.
