A dataset provided by the European Space Agency

Name 067190
Title X-ray vs. H2O maser emission in AGN
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671900101

DOI https://doi.org/10.5270/esa-wc9dbxw
Author Dr Paola Castangia
Description Water megamaser radio emission originates from the innermost parsec(s) of active
galactic nuclei (AGN). X-ray photons are produced in regions even closer to the
supermassive central object. Combining the information provided by these two
tracers has the potential to substantially improve our understanding of the AGN
physics. Correlations between X-ray and water maser emission in AGN have been
reported, however, the lack of systematic studies affects the confidence level
of these results. Here we propose to complete the approved XMM project with
Proposal ID 065480, aimed at measuring column densities in a sample of five AGN
hosting H2O maser emission, thus shedding light on the physics of their active
nuclei and improving the statistics of the aforementioned studies.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-09-08T22:42:42Z/2011-09-09T07:19:40Z
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 2012-09-30T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Paola Castangia, 2012, 067190, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-wc9dbxw