Proposal ID | 084080 |
Title | Outbursts of radio-quiet AGN |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0840800401 |
DOI | https://doi.org/10.5270/esa-fh4y2rr |
Principal Investigator, PI | Dr Norbert Schartel |
Abstract | Recent XMM-Newton observations of Seyfert galaxies establish outbursts ofradio-quiet AGNs as a poorly explored discovery space for AGN physics with anenormous potential to learn: GSN 069 is most likely a high Eddington-ratio trueSeyfert 2 galaxy with no broad line region and no X-ray continuum. NGC 1566,HE1136-2304 and NGC 2617 are rare changing look AGNs with the latter possiblyshowing absorption by in-falling matter. We propose two 80ks simultaneousXMMNewton/NuSTAR observations accompanied by optical spectroscopy of the nextsuited AGN outburst(s). They will allow tracing accretion physics, spectralcomplexity connected with dramatic emission-line changes and possibly elusivetidal disruption events probing an even more extreme accretion regime. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2019-06-05T07:53:14Z/2019-11-08T23:51:54Z |
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 | "xmm newton", "agn physics", "spectral complexity connected", "accretion regime", "optical spectroscopy", "ngc 2617", "ngc 1566", "eddington ratio", "tracing accretion physics", "xray continuum", "emission line", "NGC 1566", "radio quiet agns", "XMM-Newton", "broad line region", "NuSTAR", "suited agn outburst", "seyfert galaxy", "he1136 2304", "radio quiet agn", "XMM" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Norbert Schartel, 2020, 'Outbursts of radio-quiet AGN', 18.00_20191217_1110, European Space Agency, https://doi.org/10.5270/esa-fh4y2rr |