A dataset provided by the European Space Agency

Name 014096
Title The X-ray weakness of GPS radio galaxies:a volume-limited complete sample
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0140960101

DOI 10.5270/esa-co1vvwz
Author Dr Matteo Guainazzi
Description We propose to observe a flux- and volume-limited complete sample of GPS radio galaxies. The goal of the proposals is to determine: a. the presence of hot confining gas around the active nucleus, and its properties, through its optically thin soft X-ray emission; b. the presence of cold environment gas through the measurement of X-ray absorption - in the most extreme case, Compton-thick. These measurements will provide tests for the current scenarios to explain the origin of these objects. We request 4 targets to be observed within the XMM-Newton AO2, for a total allocation time of 80 ks. This list includes 1404+286, the first GPS radio galaxy where a poor quality ASCA observation suggests the above components may have been simultaneously detected.
Publication The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy . Levan, A. J., Tanvir, N. R., et all. . Sci . 333-199 . 2011 . 2011Sci...333..199L ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
XMM-Newton discovery of a Compton-thick AGN in the GPS galaxy Mkn 668 . Guainazzi, M., Siemiginowska, A., et all. . A&A . 421-461 . 2004 . 2004A&A...421..461G ,
X-ray emission from GPS and CSS sources . Siemiginowska, A., . AN . 330-264 . 2009 . 2009AN....330..264S ,
A serendipitous XMM survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z= 0.8 to 0.1 . Georgakakis, Antonis, Nandra, K., . MNRAS . 414-992 . 2011 . 2011MNRAS.414..992G ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Fe Kalpha line profile in AGNs: avera...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-01-31T19:04:50Z/2003-02-01T01:26:46Z
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 2004-02-28T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-02-28T00:00:00Z, 014096, 17.56_20190403_1200. https://doi.org/10.5270/esa-co1vvwz