A dataset provided by the European Space Agency

Name 015294
Title XMM-Newton and Chandra to study the ionization cones of the Seyfert 2 NGC5252
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0152940101

DOI 10.5270/esa-uicmrdm
Author Dr Mauro Dadina
Description A 70 ks observation of the Seyfert 2 galaxy NGC 5252, to be performed both by XMM-Newton and Chandra, is requested. X-ray observation of Seyfert galaxies have highlighted that 40% of these objects show extended emission probably due to an outflowing gas. We choose NGC 5252 to test this scenario. for its remarkable optical ionization cones. Goal of this proposal is to disentangle the following issues: 1)to firmly demonstrate that the diffuse emission is due to an AGN driven outflow; 2)to understand if the outflowing gas is confined by gravity; 3)to study the past history of the AGN activity; 4)to observe the shadow of the dusty torus. Even if only one of the above mentioned point is achieved, this would represent a significant step in the comprehension of AGN.
Publication X-ray imaging of the ionisation cones in NGC 5252 . Dadina, M., Guainazzi, M., et all. . A&A . 516-9 . 2010 . 2010A&A...516A...9D ,
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Exploring X-ray and radio emission of type 1 AGN up to z ~ 2.3 . Ballo, L., Heras, F. J. H., et all. . A&A . 545-66 . 2012 . 2012A&A...545A..66B ,
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Uncovering obscured luminous AGN with WISE . Mateos, S., Alonso-Herrero, A., et all. . MNRAS . 434-941 . 2013 . 2013MNRAS.434..941M ,
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Evidence for radiation pressure compression in the X-ray narrow-line region of Seyfert galaxies . Bianchi, Stefano, Guainazzi, Matteo, et all. . MNRAS . 485-416 . 2019 . 2019MNRAS.485..416B ,
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Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
Hot corona properties of Swift-BAT-detected AGNs . Wang, Chan, Yu, Li-Ming, et all. . MNRAS . 487-2463 . 2019 . 2019MNRAS.487.2463W ,
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline . Hollowood, Devon L., Jeltema, Tesla, et all. . ApJS . 244-22 . 2019 . 2019ApJS..244...22H ,
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters . Palmese, A., Annis, J., et all. . MNRAS . 493-4591 . 2020 . 2020MNRAS.493.4591P ,
X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation . Molham, Mona, Clerc, Nicolas, et all. . MNRAS . 494-161 . 2020 . 2020MNRAS.494..161M ,
The Variable and Non-variable X-Ray Absorbers in Compton-thin Type II Active Galactic Nuclei . Laha, Sibasish, Markowitz, Alex G., et all. . ApJ . 897-66 . 2020 . 2020ApJ...897...66L ,
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A Hard Look at Local, Optically Selected, Obscured Seyfert Galaxies . Kammoun, E. S., Miller, J. M., et all. . ApJ . 901-161 . 2020 . 2020ApJ...901..161K ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-07-18T02:16:34Z/2003-07-18T20:58:27Z
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 2004-09-02T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-09-02T00:00:00Z, 015294, 17.56_20190403_1200. https://doi.org/10.5270/esa-uicmrdm