A dataset provided by the European Space Agency

Name 006460
Title Exploring New Inverse-Compton Sources in Radio Galaxies
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0064600101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0064600301

DOI https://doi.org/10.5270/esa-fiztlmb
Author Prof Kazuo Makishima
Description Observations are proposed for two radio galaxies with medium radio fluxes, 3C 98 and 3C 386. A 30 ks exposure onto each will enable detections of diffuse inverse-Compton X-rays from their radio lobes. This will yield accurate estimates of the lobe magnetic field strength and the relativisitic electron energy density.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-09-07T05:02:58Z/2003-02-05T22:20:35Z
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 2004-03-02T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-03-02T00:00:00Z, 006460, 17.56_20190403_1200. https://doi.org/10.5270/esa-fiztlmb