  The afterglow of a gamma ray burst (GRB) can give us valuable insight into
the properties of its host galaxy. To correctly interpret the spectra of the
afterglow we need to have a good understanding of the foreground interstellar
medium (ISM) in our own Galaxy. The common practice to correct for the
foreground is to use neutral hydrogen (HI) data from the Leiden/Argentina/Bonn
(LAB) survey. However, the poor spatial resolution of the single dish data may
have a significant effect on the derived column densities. To investigate this,
we present new high-resolution HI observations with the Australia Telescope
Compact Array (ATCA) towards 4 GRBs. We combine the interferometric ATCA data
with single dish data from the Galactic All Sky Survey (GASS) and derive new
Galactic HI column densities towards the GRBs. We use these new foreground
column densities to fit the Swift XRT X-ray spectra and calculate new intrinsic
hydrogen column density values for the GRB host galaxies. We find that the new
ATCA data shows higher Galactic HI column densities compared to the previous
single dish data, which results in lower intrinsic column densities for the
hosts. We investigate the line of sight optical depth near the GRBs and find
that it may not be negligible towards one of the GRBs, which indicates that the
intrinsic hydrogen column density of its host galaxy may be even lower. In
addition, we compare our results to column densities derived from far-infrared
data and find a reasonable agreement with the HI data.
