  By 2000 there were only 10 established Galactic pulsar-supernova remnant
associations. Two years later there are 16 such associations known. I discuss
the work leading to this substantial increase. In particular I summarize an
ongoing search project that has resulted in the detection of several young
pulsars with a very low radio luminosity of about 1 mJy kpc^2 at 1.4 GHz, and
comment on future prospects.
