A dataset provided by the European Space Agency

Name 055412
Title An XMM-Newton investigation of AGN feedback modes across cosmological time
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554120101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554120701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554121001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554121101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0554121301

DOI 10.5270/esa-gdodpuf
Author Dr Mari Polletta
Description We request a deep (250 ksec) XMM-Newton observation of a field that benefits from the deepest multi-frequency radio observations currently possible to study the AGN bright and radio feedback modes across cosmological times. The selected field also benefits from deep Spitzer, near-infrared, and optical data and moderate X-ray data from Chandra. With the proposed observations we will discriminate between cold and hot gas accretors among radio and X-ray selected AGNs to constrain the evolution of the two AGN feedback processes. A series of additional topics will be also addressed: X-ray variability vs radio, infrared, and optical spectral properties; the X-ray properties of various extreme and rare sources; and we will search for heavily absorbed radio-selected AGNs.
Publication The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive . Clerc, N., Sadibekova, T., et all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
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 ,
An XMM-Newton Survey of the Soft X-Ray Background. III. The Galactic Halo X-Ray Emission . Henley, David B., Shelton, Robin L., . ApJ . 773-92 . 2013 . 2013ApJ...773...92H ,
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 ,
The Origin of the Hot Gas in the Galactic Halo: Testing Galactic Fountain Models. X-Ray Emission . Henley, David B., Shelton, Robin L., et all. . ApJ . 800-102 . 2015 . 2015ApJ...800..102H ,
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function . Vagnetti, F., Middei, R., et all. . A&A . 593-55 . 2016 . 2016A&A...593A..55V ,
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 ,
SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV . Clerc, N., Merloni, A., et all. . MNRAS ....
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-10-11T20:29:36Z/2009-04-11T21:22:20Z
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 2010-05-12T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-05-12T00:00:00Z, 055412, 17.56_20190403_1200. https://doi.org/10.5270/esa-gdodpuf