A dataset provided by the European Space Agency

Name: EXPLORING THE CORONA OF MRK 926
Published: 2017-12-02T23:00:00Z

Proposal ID	079064
Title	EXPLORING THE CORONA OF MRK 926
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790640101
DOI	https://doi.org/10.5270/esa-c8fdymj
Principal Investigator, PI	Dr Anne Maria Lohfink
Abstract	We propose to observe Mrk 926 for 35 ks with XMM and 100 ks with NuSTAR toexplore the Comptonization spectrum of this bright Seyfert 1 galaxy. Previousanalyses of non-simultaneous observations have found a lower limit of the highenergy cut-off of 510 keV, bringing it in disagreement by the temperature limitset by run-away pair production. With the proposed observations we will test,whether Mrk 926.s spectrum is consistent with thermal Comptonization or not. Ifit is, we can study its Comptonization spectrum from the UV to the hard X-raysand would obtain key information on the properties of coronae typical forSeyferts. However, if we find that the temperature is inconsistent with thermalComptonization, we can use this dataset to understand which other process could be responsible.
Publications	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 A Weakening Compton Hump and Soft X-Ray Excess Detected in the Seyfert 1 Galaxy MCG -02-58-22 \|Laha, Sibasish, Ghosh, Ritesh, \| ApJ \| 915-93 \| 2021 \| 2021ApJ...915...93L \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...915...93L Fundamental X-ray corona parameters of Swift/BAT AGN \|Hinkle, Jason T., Mushotzky, Richard, \| MNRAS \| 506-4960 \| 2021 \| 2021MNRAS.506.4960H \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.506.4960H X-Ray Coronal Properties of Swift/BAT-selected Seyfert 1 Active Galactic Nuclei \|Kamraj, Nikita, Brightman, Murray, et al. \| ApJ \| 927-42 \| 2022 \| 2022ApJ...927...42K \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...927...42K Broad-band spectral analysis of Mrk 926 using multi-epoch X-ray observations \|Chalise, S., Lohfink, A. M., et al. \| MNRAS \| 517-4788 \| 2022 \| 2022MNRAS.517.4788C \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517.4788C A Multiwavelength Study of Active Galactic Nuclei in Post-merger Remnants \|Li, Wenhao, Nair, Preethi, et al. \| ApJ \| 944-168 \| 2023 \| 2023ApJ...944..168L \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...944..168L 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	2016-11-21T10:42:37Z/2016-11-22T03:05:57Z
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	2017-12-02T23:00:00Z
Keywords	"thermal comptonization", "NuSTAR", "hard xray", "temperature limit set", "coronae typical", "XMM", "energy cut", "lower limit", "key information", "mrk 926", "comptonization spectrum", "510 kev", "bright seyfert", "pair production"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Anne Maria Lohfink, 2017, 'EXPLORING THE CORONA OF MRK 926', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-c8fdymj