Please use this identifier to cite or link to this item:
|Title:||A search for H I 21 cm absorption toward the highest redshift (z~5.2) radio-loud objects|
van Hoven, M.B.
|Publisher:||The University of Chicago Press for the American Astronomical Society|
|Citation:||The Astronomical Journal, 2007, Vol.133, p2841-2845|
|Abstract:||We have searched for H I 21 cm absorption toward the two brightest radio AGNs at high redshift, J0924-2201 at z=5.20 and J0913+5919 at z=5.11, using the Giant Metrewave Radio Telescope. These data set a 3 σ upper limit to absorption of <30% at 40 km s-1 resolution for the 30 mJy source J0913+5919, and <3% for the 0.55 Jy source J0924-2201 at 20 km s-1 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 -1 channel is N(H I)<2.2×1018Ts cm-2 over a velocity range of -700 to +1180 km s-1 centered on the galaxy redshift determined through CO emission, assuming a covering factor of 1. For J0913+5919 the column density limit per 40 km s-1 channel is N(H I)<2.2×1019Ts cm-2 within +/-2400 km s-1 of the optical redshift. These data rule out any cool, high column density H I clouds within roughly +/-1000 km s-1 of the galaxies, as are often seen in compact steep-spectrum radio AGNs, or clouds that might correspond to residual gas left over from cosmic reionization.|
|Description:||Restricted Access. An open-access version is available at arXiv.org. Articles older than 2 years are open to all at the journal site (alternative location)|
|Copyright:||2007 The American Astronomical Society|
|Appears in Collections:||Research Papers (A&A)|
Files in This Item:
|2007 AJ V133 p2841.pdf|
|Restricted Access||228.34 kB||Adobe PDF||View/Open Request a copy|
Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.