A dataset provided by the European Space Agency

Name 090337
Title XMM/HST monitoring of the ultra soft Narrow Line Seyfert 1 RX J1355.2+5612
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903370201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903370301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903370401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903370501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903370601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903370701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903370801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903370901

DOI https://doi.org/10.57780/esa-xt4dut9
Author European Space Agency
Description Ultra soft Narrow Line Seyfert 1 are characterized by a large spectral
variability, a very steep X-ray primary continuum (> 2.5) and a strong soft
excess. This remarkable spectral shape questions the origin of their broad-band
UV-X-ray continuum compared to standard Seyfert galaxies. We propose to perform
a monitoring composed of 5 x 26 ks XMM observations (total: 130 ks), spaced by
2-3 days and coordinated with HST, to probe the FUV, of RX J1355.2+5612. The
proposed monitoring will allow us to 1) disentangle the different spectral
components present from the UV/FUV to X-ray energy range and 2) investigate the
nature of the soft X-ray excess and discriminate between the theoretical models
that have been heavily discussed in the past decade
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-11-06T07:15:32Z/2022-11-18T19:56:49Z
Version 20.09_20221024_1724
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 2023-12-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2023, Xmm/Hst Monitoring Of The Ultra Soft Narrow Line Seyfert 1 Rx J1355.2+5612, 20.09_20221024_1724, European Space Agency, https://doi.org/10.57780/esa-xt4dut9