A dataset provided by the European Space Agency

Name 030091
Title A hunt for X-ray absorbed Narrow Line Seyfert 1s using the FeII/Hbeta ratio
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300910101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300910201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300910301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300910401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300910601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300910701

DOI https://doi.org/10.5270/esa-24k3f4t
Author Dr Enrico Piconcelli
Description We propose to observe a sample of four Narrow Line Seyfert 1 galaxies with
strong Fe II emission (FeNLS1s) for a total allocation time of 115 ks. The goal
of this proposal is to test how common is the spectral hard X-ray (Evirgul7-8 keV)
absorption feature in FeNLS1s, recently observed in two objects of this class.
This feature appears as a clear signature of dense matter outflowing from the
nucleus. If our optically-based criterion (i.e. Fe II4570/Hbeta higher than 1.5)
would be efficient in selecting objects with deep sharp X-ray edges, the origin
of this feature in outflowing clouds would be supported. A frequent occurrence
of this spectral drop will therefore provide clues of an intimate link between
NLS1s and BAL QSOs phenomena.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-06-17T13:14:34Z/2006-01-24T21:13:25Z
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 2008-01-10T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Enrico Piconcelli, 2008, 030091, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-24k3f4t