We propose to observe with XMM-Newton a set of 10 AGN from a complete sample of88 INTEGRAL selected objects, for which no or limited spectral information areavailable below 10 keV. This is the continuation of 5 previous successful XMMproposals, which have so far provided X-ray observations for a large fraction ofour AGNs; the present proposal will conclude the observational phase of thisproject providing good quality X-ray coverage for the entire INTEGRAL completeAGN sample. Based on our past experience, we estimate that an exposure of 15-20ks for each source (depending on the strength) for a total time of 180 ks issufficient to reach the scientific goals of this proposal. All objects requestedhere have been graded C targets in AO9 but have not been observed yet.
A comprehensive analysis of the hard X-ray spectra of bright Seyfert galaxies |Lubinski, P., Beckmann, V., et al. | MNRAS | 458-2454 | 2016 | 2016MNRAS.458.2454L | http://ui.adsabs.harvard.edu/#abs/2016MNRAS.458.2454L
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
The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions |Pan, Zeyang, Qu, Zhijie, et al. | ApJS | 271-62 | 2024 | 2024ApJS..271...62P | http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P
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
2011-05-06T07:06:21Z/2012-01-21T04:57:53Z
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.
European Space Agency, Dr Loredana Bassani, 2013, 'XMM-Newton observations of a complete sample of INTEGRAL detected AGN', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-smqqtz7
