A dataset provided by the European Space Agency

Name 083055
Title NUSTAR/XMM MONITORING OF THE EXTREME NARROW LINE SEYFERT MRK 359
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0830550801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0830550901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0830551001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0830551101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0830551201

DOI https://doi.org/10.5270/esa-zog6mur
Author Dr pierre-olivier petrucci
Description We propose to perform a unique NuSTAR/XMM monitoring with 5 repeated
observations of 50 ks spaced by a 2-3 days of the extreme Radio-Quiet Narrow
line Seyfert 1 galaxy Mrk 359. This will permit 1) to correctly disentangle the
different spectral components present in this energy band, and 2) to reveal
their complex interdependences and variability behavior. This study will allow
us i) to constrain the physical parameters of the Comptonizing coronae
responsible for the bulk of the X-ray emission ; ii) to investigate the nature
of the soft X-ray excess and differentiate between multiple origins; iii) to put
firm conclusions on the distance, nature and geometry of the reflecting
material(s). Such monitorings appear as the best strategy to reach these goals.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2019-01-25T03:06:39Z/2019-02-02T18:56:47Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2020-02-28T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr pierre-olivier petrucci, 2020, 083055, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zog6mur