A dataset provided by the European Space Agency

Name 069009
Title Understanding the gamma-ray loud Narrow-Line Seyfert 1 Galaxies
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690090101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690090201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690090301

DOI https://doi.org/10.5270/esa-birguzy
Author European Space Agency
Description We ask for 41 ks exposure to observe three Narrow-Line Seyfert 1 Galaxies
(NLS1s) that have been detected at high-energy gamma rays (E>100 MeV) with
Fermi/LAT. The selected targets have been poorly or never detected at X-rays and
the requested observations, bringing also optical-to-UV data from the Optical
Monitor, will allow us to build simultaneous optical-to-X-ray spectral energy
distributions (SEDs), which will be complemented with Fermi data. We will
calculate the jet and the accretion power from these data and compare with other
active nuclei with or without jets, in order to better understand both how jets
are generated and the nature of NLS1s.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2012-06-11T06:59:55Z/2012-12-15T01:47:11Z
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 2014-01-15T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014, Understanding The Gamma-Ray Loud Narrow-Line Seyfert 1 Galaxies, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-birguzy