A dataset provided by the European Space Agency

Name: IGR J14488--4008 and IGR J17488--2338: two X-ray absorbed BLRG
Published: 2015-07-29T22:00:00Z

Proposal ID	072836
Title	IGR J14488--4008 and IGR J17488--2338: two X-ray absorbed BLRG
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728360101
DOI	https://doi.org/10.5270/esa-7omn2op
Principal Investigator, PI	Dr Manuela Molina
Abstract	We propose to observe with XMM-Newton two radio galaxies, IGR J14488-4008 andIGR J17488-2338, recently discovered by INTEGRAL and for which limited spectralinformation is available below 10 keV. In particular, we aim at assessing thenature of absorption which is at odds with their optical classification as broadline AGN and to probe the presence of reflection features, such as the iron lineand Compton reflection hump. Based on our past experience and simulations, weestimate that an exposure of 20 ks for each source is sufficient to reach thescientific goals of this proposal.
Publications	The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F The close environments of accreting massive black holes are shaped by radiative feedback \|Ricci, Claudio, Trakhtenbrot, Benny, et al. \| Natur \| 549-488 \| 2017 \| 2017Natur.549..488R \| http://ui.adsabs.harvard.edu/#abs/2017Natur.549..488R BAT AGN Spectroscopic Survey (BASS) - VI. The GammaX-L/LEdd relation \|Trakhtenbrot, Benny, Ricci, Claudio, et al. \| MNRAS \| 470-800 \| 2017 \| 2017MNRAS.470..800T \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470..800T BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog \|Ricci, C., Trakhtenbrot, B., et al. \| ApJS \| 233-17 \| 2017 \| 2017ApJS..233...17R \| http://ui.adsabs.harvard.edu/#abs/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 al. \| ApJ \| 858-110 \| 2018 \| 2018ApJ...858..110P \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...858..110P Hot corona properties of Swift/BAT-detected AGNs \|Wang, Chan, Yu, Li-Ming, et al. \| MNRAS \| 487-2463 \| 2019 \| 2019MNRAS.487.2463W \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487.2463W Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
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 Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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
Keywords	"xmm newton radiogalaxy", "broad line agn", "limited spectral information", "XMM", "past experience", "iron line", "igr j14488 4008", "igr j17488 2338", "xray absorbed blrg", "XMM-Newton", "compton reflection hump", "optical classification"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Manuela Molina, 2015, 'IGR J14488--4008 and IGR J17488--2338: two X-ray absorbed BLRG', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7omn2op