SIMBAD references

We present the discovery of a new extreme high proper motion object (∼3.5arcsec/year) which we classify as an ultracool subdwarf with [M/H]~-0.5. It has a formal spectral type of sdM9 but also shows L-type features: while the VO bands are completely absent, it exhibits extremely strong TiO absorption in its optical spectrum. With a radial velocity of about -160km/s and a rough distance estimate of 16-24pc, it is likely one of the nearest halo members crossing the Solar neighbourhood with a heliocentric space velocity of (U,V,W)=(-244,-256,-100)±(32,77,6)km/s.