The temperature of the diffuse HI in the Milky Way I: High resolution HI
  21 cm absorption studies
  We have carried out deep, high velocity resolution, interferometric Galactic
HI 21 cm absorption spectroscopy towards 32 compact extra-galactic radio
sources with the Giant Metrewave Radio Telescope (GMRT) and the Westerbork
Synthesis Radio Telescope (WSRT). The optical depth spectra for most sources
have root mean square noise values \lesssim 10^{-3} per 1 km/s velocity channel
and are thus sufficiently sensitive to detect absorption by warm neutral
hydrogen with HI column densities N_HI \gtrsim 10^{20} cm^{-2}, spin
temperatures T_s \leq 5000 K, and line widths equal to the thermal width (20
km/s). HI 21 cm absorption was detected against all background sources but one,
B0438-436. The spectra of sources observed separately with GMRT and WSRT show
excellent agreement, indicating that spectral baseline problems and
contamination from HI 21 cm emission are negligible. This paper presents the
absorption spectra, the emission spectra along neighbouring sightlines from the
Leiden-Argentine-Bonn survey, and the derived spin temperature spectra. On
every sightline, the maximum spin temperature detected (at \ge 3 sigma
significance) even at a velocity resolution of 1 km/s is \gtrsim 1000 K,
indicating that we are detecting the warm neutral medium along most sightlines.
This is by far the largest sample of Galactic HI 21 cm absorption spectra of
this quality, providing a sensitive probe of physical conditions in the neutral
atomic ISM.
