A dataset provided by the European Space Agency

Name 020104
Title X-RAY EMISSION FROM THE GRAVITATIONALLY-LENSED HIDDEN QSO IRAS F10214+4724
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201040101

DOI 10.5270/esa-pd9t0kz
Author Dr KAZUSHI IWASAWA
Description We propose a 45 ks XMM-Newton observation of the high redshift (z=2.3) hyperluminous infrared galaxy IRAS F10214+4724. The first X-ray detection from this gravitationally-lensed object will be aimed. Previous observations strongly suggest that this object harbours a Compton-thick AGN. Weak reflected X-ray emission is expected. The inherent source-size dependency of lensing: differential magnification, offes a possible way to constrain the size of the X-ray reflection region and the contribution of the AGN to the great bolometric luminosity.
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 ,
On the origin of soft X-rays in obscured AGN: answers from high-resolution spectroscopy with XMM-Newton . Guainazzi, Matteo, Bianchi, Stefano, . MNRAS . 374-1290 . 2007 . 2007MNRAS.374.1290G ,
The X-ray Energy Dependence of the Relation Between Optical and X-ray Emission in Quasars . Young, M., Elvis, M., . ApJ . 708-1388 . 2010 . 2010ApJ...708.1388Y ,
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 ,
An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120 and l = 240 . Henley, David B., Shelton, Robin L., . ApJS . 187-388 . 2010 . 2010ApJS..187..388H ,
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, ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-10-22T23:08:56Z/2004-10-23T14:19:45Z
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 2005-11-27T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-11-27T00:00:00Z, 020104, 17.56_20190403_1200. https://doi.org/10.5270/esa-pd9t0kz