INTEGRAL chases obscured active galaxies in the deepest
55 of 236

INTEGRAL chases obscured active galaxies in the deepest extragalactic hard X-ray survey to date

January 8, 2013
A large fraction of active galactic nuclei (AGN) is thought to be hidden behind a vast quantity of gas and dust that absorbs low-energy X-rays. Thanks to its hard X-ray imager IBIS, INTEGRAL is able to pierce this opaque layer and uncover the full population of AGN. A new study exploited this capability to perform in the 20-60 keV band the deepest extragalactic hard X-ray survey to date. The survey is centred around the quasar 3C 273 and the Coma cluster, uses a total of 4 million seconds of exposure time from 1660 different pointings and covers 12% of the sky. Thanks to the very large exposure time, the faintest sources detected in this survey are much fainter than those in previous extragalactic hard X-ray surveys. The figure on the left shows the effective exposure time map, with contours indicating the survey border and the regions exposed more than 10 000, 100 000, 300 000 and 500 000 seconds respectively. The positions of the 34 AGN candidates which have been detected in this survey are also marked with green dots. Coordinates are right ascension and declination. The figure on the right shows the cumulative source counts as a function of minimum hard X-ray flux, separately for absorbed (blue) and non-absorbed (red) sources. The number of absorbed sources is about three times larger than that of non-absorbed sources, while the numbers for sources selected in the medium X-rays are approximately equal at these flux levels. This highlights the importance of pushing the sensitivity limit of hard X-ray surveys to its absolute minimum if we want to understand the population of AGN. Related publication Paltani S., et al., "A deep INTEGRAL hard X-ray survey of the 3C 273/Coma region", A&A Volume 485, Issue 3, 2008, pp.707-718 Date: 01 Aug 2008 Satellite: INTEGRAL Depicts: IBIS deep hard X-ray survey around quasar 3C 273 and the Coma cluster Copyright: Adapted from Paltani, S. et al. [2008]

comments powered by Disqus