A dataset provided by the European Space Agency

Name: ESO511-G030: THE ULTIMATE TEST BENCH FOR THE TWO-CORONA MODEL
Published: 2020-09-02T22:00:00Z

Proposal ID	085201
Title	ESO511-G030: THE ULTIMATE TEST BENCH FOR THE TWO-CORONA MODEL
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852010101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852010201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852010301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852010401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852010501
DOI	https://doi.org/10.5270/esa-gps51j3
Principal Investigator, PI	Mr Riccardo Middei
Abstract	We propose a nustar/xmm monitoring of 5x30ks observations spaced by 3-4 days ofthe bright Radio-Quiet Seyfert 1 ESO511-G030. Its spectrum is characterised by arelativistic Fe Kalpha line (significance >5sig) and a strong soft excess, thusmaking ESO511-G030 the ideal candidate for testing the warm Comptonisationorigin of soft excess in AGN. In fact, warm corona has been proved to be aviable physical model in sources without a relativistic reflection component,but it has never been properly tested in a source hosting a relativistic ironline where the soft excess is reproduced via relativistic reflection. Theproposed monitoring will allow us to test the general validity of the warmComptonisation by breaking its spectral degeneracy with relativistic reflection.
Publications	The Low-temperature Corona in ESO 511-G030 Revealed by NuSTAR and XMM-Newton \|Zhang, Zuobin, Jiang, Jiachen, et al. \| ApJ \| 949-4 \| 2023 \| 2023ApJ...949....4Z \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...949....4Z Tracking the spectral properties of ESO 511-G030 across different epochs \|Middei, R., Petrucci, P. -O., et al. \| A&A \| 672-101 \| 2023 \| 2023A&A...672A.101M \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A.101M 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2019-07-20T16:51:38Z/2019-08-10T02:44:28Z
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	2020-09-02T22:00:00Z
Keywords	"spectral degeneracy", "eso511 g030", "ideal candidate", "viable physical model", "test bench", "soft excess", "warm comptonisation", "warm comptonisation origin", "relativistic reflection", "corona model", "relativistic reflection component", "relativistic iron line", "properly tested", "G030.", "warm corona"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Riccardo Middei, 2020, 'ESO511-G030: THE ULTIMATE TEST BENCH FOR THE TWO-CORONA MODEL', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gps51j3