A dataset provided by the European Space Agency

Name 008299
Title Searching for Inverse Compton Emission in strong FRII Radio Galaxies
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0082990101

DOI https://doi.org/10.5270/esa-9j3unzb
Author Dr Brunetti Gianfranco
Description We propose relatively deep XMM observations of 3 high redshift radio--galaxies in order to study the origin of their X--ray emission. In particular we want to test if a hot thermal gas possibly associated with high redshift cluster is present or if a Invers Compton emission of the nuclear photons off the relativistic electrons in the radio lobes is responsible of the weak X--ray fluxes observed by ROSAT.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-12-10T21:22:03Z/2002-12-11T11:30:23Z
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 2004-02-02T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-02-02T00:00:00Z, 008299, 17.56_20190403_1200. https://doi.org/10.5270/esa-9j3unzb