A dataset provided by the European Space Agency

Proposal ID 084022
Title Discovering the X-ray Broad Line Region in AGN
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840220701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840220801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840220901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840221001

DOI https://doi.org/10.57780/esa-vzjq1gu
Principal Investigator, PI Dr Elisa Costantini
Abstract Thanks to high resolution spectroscopy, the X-ray emitting broad line region hasbeen recently discovered and studied in few bright type 1 Seyferts. We proposeto observe for 120 ks the bright AGN Mrk110, simultaneously with HST-COS. Thegoal is to model for the first time the panchromatic broad line region emissionin a Narrow Line Seyfert~1 galaxy. We will use the broad lines from the optical,UV and X-rays in a global modeling that will characterize the stratification,extend and ionization of the broad line emitting region, whose X- ray extensionstill awaits a full characterization.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2019-11-03T08:51:40Z/2019-11-07T20:27:46Z
Version 18.00_20191217_1110
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 2020-12-19T23:00:00Z
Last Update 2025-01-27
Keywords "resolution spectroscopy", "hst cos", "broad lines", "x ray extension", "narrow line seyfert", "bright type", "bright agn mrk110", "global modeling", "HST"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Elisa Costantini, 2020, 'Discovering the X-ray Broad Line Region in AGN', 18.00_20191217_1110, European Space Agency, https://doi.org/10.57780/esa-vzjq1gu