A dataset provided by the European Space Agency

Proposal ID 055097
Title Unveiling a young quasar: PKS1549-79
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550970101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550970201

DOI https://doi.org/10.5270/esa-cm5q6nx
Principal Investigator, PI Dr Paul OBrien
Abstract Galaxy merger models predict rapid black hole growth and strong outflows late inthe merger as the accretion rate increases. PKS1549-79 is a powerful, lowredshift active galaxy which has undergone a recent merger. It is therefore anideal object to test our understanding of galaxy activity and mergers and forstudying feedback between AGN and their host galaxies. We propose a 75 ksecXMM-Newton observation to: (i) determine the amount and onisation state of thenuclear obscuring material in PKS1549-79 and hence confirm its status as a localproto-quasar; (ii) search for the massive, probably highly ionised, outflowingwind predicted by galaxy evolution models and hence complete a census of outflowcomponents in this object; and (iii) quantify the starburst activity.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-09-21T11:51:51Z/2008-09-22T14:09:42Z
Version 17.56_20190403_1200
Mission Description The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 2009-10-30T00:00:00Z
Keywords "galaxy evolution models", "outflowing wind predicted", "p1549 79", "outflows late", "XMM", "nuclear obscuring material", "galaxy activity", "ideal object", "iii quantify", "local proto quasar", "75 xmm newton", "XMM-Newton", "accretion rate increases", "outflow components", "ii search", "starburst activity"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Paul O'Brien, 2009, 'Unveiling a young quasar: PKS1549-79', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-cm5q6nx