A dataset provided by the European Space Agency

Name 060069
Title Compton-thick luminous AGNs at the heart of bright [OIII] emitters
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600690101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600690201

DOI https://doi.org/10.5270/esa-2i78soy
Author European Space Agency
Description We propose the observation of two narrow-line, [O III] luminous AGNs (z<virgul0.05)
aimed at discovering clearcut examples of local Compton-thick (CT) quasars, that
are still lacking so far. Previous low-quality observations provided strong, but
not definitive, indications of a reflection-dominated X-ray spectrum in both
sources. The large [OIII] luminosities should ensure an intrinsic X-ray
luminosity typical of quasars. Thanks to the expected photon statistics the
proposed observations will shed definitive light on the CT nature of the
absorber in these sources. Our program is designed to miminize the risks of
non-detection of the target and/or ambiguous results that have affected several
blind searches for CT luminous AGNs performed to date.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-05-22T17:09:34Z/2010-01-31T14:00:09Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2011-03-03T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011, Compton-Thick Luminous Agns At The Heart Of Bright Square_Bracket_Openoiiisquare_Bracket_Close Emitters, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2i78soy