We present preliminary results from imaging three Hubble Space Telescope (HST) Wide Field Planetary Camera 2 fields in V and I within the Chandra Deep Field-South (CDF-S). HST Is sensitivity and resolution are sufficient to reveal optical counterparts for 24 of the 26 CDF-S X-ray sources detected in the 300 ks X-ray catalog and determine the morphologies of most of these. We find that the X-ray sources comprise two apparently distinct populations of optical candidates : one optically faint (I greater than or similar to 24), with V-I colors consistent with the I>24 field population, and the other significantly brighter (I less than or similar to 22), with colors redder than the I < 22 field population. More than two-thirds of the X-ray source counterparts are resolved galaxies. The brighter sources are mostly active galactic nuclei (AGNs) based on their high X-ray luminosity. The optically resolved sources in the brighter population have a very narrow range of V-I color and appear to be a mix of both late- and early-type morphologies at low to moderate redshift. We show that the second population, with fainter optical counterparts, can be explained as higher redshift type 2 AGNs.
Hubble Space Telescope imaging in the Chandra Deep Field-South. I. Multiple active galactic nucleus populations
ROSATI, Piero;
2001
Abstract
We present preliminary results from imaging three Hubble Space Telescope (HST) Wide Field Planetary Camera 2 fields in V and I within the Chandra Deep Field-South (CDF-S). HST Is sensitivity and resolution are sufficient to reveal optical counterparts for 24 of the 26 CDF-S X-ray sources detected in the 300 ks X-ray catalog and determine the morphologies of most of these. We find that the X-ray sources comprise two apparently distinct populations of optical candidates : one optically faint (I greater than or similar to 24), with V-I colors consistent with the I>24 field population, and the other significantly brighter (I less than or similar to 22), with colors redder than the I < 22 field population. More than two-thirds of the X-ray source counterparts are resolved galaxies. The brighter sources are mostly active galactic nuclei (AGNs) based on their high X-ray luminosity. The optically resolved sources in the brighter population have a very narrow range of V-I color and appear to be a mix of both late- and early-type morphologies at low to moderate redshift. We show that the second population, with fainter optical counterparts, can be explained as higher redshift type 2 AGNs.I documenti in SFERA sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
