A search for HI 21cm absorption toward the highest redshift radio loud objects
arXiv:astro-ph/0703797 · doi:10.1086/518436
Abstract
We have searched for HI 21cm absorption toward the two brightest radio AGN at high redshift, J0924--2201 at , and J0913+5919 at , using the Giant Meter Wave Radio Telescope (GMRT). These data set a 3 upper limit to absorption of at 40 km s resolution for the 30 mJy source J0913+5919, and for the 0.55 Jy source J0924--2201 at 20 km s resolution. For J0924--2201, limits to broader lines at the few percent level are set by residual spectral baseline structure. For J0924--2201 the column density limit per 20 km s channel is: N(HI) cm over a velocity range of -700 km s to km s centered on the galaxy redshift determined through CO emission, assuming a covering factor of one. For J0913+5919 the column density limit per 40 km s channel is: N(HI) cm within km s of the optical redshift. These data rule out any cool, high column density HI clouds within roughly km s of the galaxies, as are often seen in Compact Steep Spectrum radio AGN, or clouds that might correspond to residual gas left over from cosmic reionization.
arXiv commentaccepted to the Astronomical Journal; 7 figures; 9 pages aastex format
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