A dataset provided by the European Space Agency

Name 055097
Title Unveiling a young quasar: PKS1549-79
URL

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

DOI 10.5270/esa-cm5q6nx
Author Dr Paul O.Brien
Description Galaxy merger models predict rapid black hole growth and strong outflows late in the merger as the accretion rate increases. PKS1549-79 is a powerful, low redshift active galaxy which has undergone a recent merger. It is therefore an ideal object to test our understanding of galaxy activity and mergers and for studying feedback between AGN and their host galaxies. We propose a 75 ksec XMM-Newton observation to: (i) determine the amount and onisation state of the nuclear obscuring material in PKS1549-79 and hence confirm its status as a local proto-quasar; (ii) search for the massive, probably highly ionised, outflowing wind predicted by galaxy evolution models and hence complete a census of outflow components in this object; and (iii) quantify the starburst activity.
Publication X-ray variability of 104 active galactic nuclei. XMM-Newton power-spectrum density profiles . Gonzalez-Martin, O., Vaughan, S., . A&A . 544-80 . 2012 . 2012A&A...544A..80G ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
Ultrafast outflows in radio-loud active galactic nuclei . Tombesi, F., Tazaki, F., et all. . MNRAS . 443-2154 . 2014 . 2014MNRAS.443.2154T ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Star Formation Suppression Due to Jet Feedback in Radio Galaxies with Shocked Warm Molecular Gas . Lanz, Lauranne, Ogle, Patrick M., et all. . ApJ . 826-29 . 2016 . 2016ApJ...826...29L ,
The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo . Miller, Matthew J., Bregman, Joel N., . ApJ . 829-9 . 2016 . 2016ApJ...829....9M ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The close environments of accreting massive black holes are shaped by radiative feedback . Ricci, Claudio, Trakhtenbrot, Benny, et all. . Natur . 549-488 . 2017 . 2017Natur.549..4...,
BAT AGN Spectroscopic Survey (BASS) - VI. The GammaX-L-LEdd relation . Trakhtenbrot, Benny, Ricci, Claudio, et all. . MNRAS . 470-800 . 2017 . 2017MNRAS.470..800T ,
BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift-BAT 70-month AGN Catalog . Ricci, C., Trakhtenbrot, B., et all. . ApJS . 233-17 . 2017 . 2017ApJS..233...17R ,
The Swift-BAT AGN Spectroscopic Survey. IX. The Clustering Environments of an Unbiased Sample of Local AGNs . Powell, M. C., Cappelluti, N., et all. . ApJ . 858-110 . 2018 . 2018ApJ...858..110P ,
Hot corona properties of Swift-BAT-detected AGNs . Wang, Chan, Yu, Li-Ming, et all. . MNRAS . 487-2463 . 2019 . 2019MNRAS.487.2463W ,
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 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 2009-10-30T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-10-30T00:00:00Z, 055097, 17.56_20190403_1200. https://doi.org/10.5270/esa-cm5q6nx