A dataset provided by the European Space Agency

Name 072836
Title IGR J14488--4008 and IGR J17488--2338: two X-ray absorbed BLRG


DOI 10.5270/esa-7omn2op
Author Dr Manuela Molina
Description We propose to observe with XMM-Newton two radio galaxies, IGR J14488-4008 and IGR J17488-2338, recently discovered by INTEGRAL and for which limited spectral information is available below 10 keV. In particular, we aim at assessing the nature of absorption which is at odds with their optical classification as broad line AGN and to probe the presence of reflection features, such as the iron line and Compton reflection hump. Based on our past experience and simulations, we estimate that an exposure of 20 ks for each source is sufficient to reach the scientific goals of this proposal.
Publication The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The close environments of accreting massive black holes are shaped by radiative feedback . Ricci, Claudio, Trakhtenbrot, Benny, et all. . Natur . 549-488 . 2017 . 2017Natur.549..488R ,
BAT AGN Spectroscopic Survey (BASS) - VI. The GammaX-L-LEdd relation . Trakhtenbrot, Benny, Ricci, Claudio, et all. . MNRAS . 470-800 . 2017 . 2017MNRAS.470..800T ,
BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift-BAT 70-month AGN Catalog . Ricci, C., Trakhtenbrot, B., et all. . ApJS . 233-17 . 2017 . 2017ApJS..233...17R ,
The Swift-BAT AGN Spectroscopic Survey. IX. The Clustering Environments of an Unbiased Sample of Local AGNs . Powell, M. C., Cappelluti, N., et all. . ApJ . 858-110 . 2018 . 2018ApJ...858..110P ,
Hot corona properties of Swift-BAT-detected AGNs . Wang, Chan, Yu, Li-Ming, et all. . MNRAS . 487-2463 . 2019 . 2019MNRAS.487.2463W ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-07-19T06:53:18Z/2014-07-19T13:08:18Z
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 2015-07-29T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015-07-29T22:00:00Z, 072836, 17.56_20190403_1200. https://doi.org/10.5270/esa-7omn2op