A dataset provided by the European Space Agency

Name 008802
Title XMM Observations of HyLIRGs at z~1


DOI 10.5270/esa-05gi68x
Author Dr Guido DiCocco
Description Recent deep FIR, sub-mm and X-ray observations of the cosmic background all point to the importance of HyLIRGs in a cosmological context. XMM offers for the first time the opportunity to study these objects in the X-ray band at redshift 1. IRAS F21243-4501 and IRAS F15307+3252, two HyLIRGs at z sim 0.9, are proposed for observation with XMM. Our goals are to obtain the first X-ray spectra of high-z HyLIRGs and measure both absorption and FeK line parameters precisely. To achieve these goals, we will take advantage of the redshift which shifts the expected strong absorption and FeK lines where the XMM sensitivity is greatest.
Publication Exploring the X-ray sky with the XMM-Newton bright serendipitous survey . Della Ceca, R., Maccacaro, T., et all. . A&A . 428-383 . 2004 . 2004A&A...428..383D ,
High-precision multi-band measurements of the angular clustering of X-ray sources . Ebrero, J., Mateos, S., et all. . A&A . 500-749 . 2009 . 2009A&A...500..749E ,
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 ,
The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project . Fassbender, R., Bohringer, H., et all. . NJPh . 13-125014 . 2011 . 2011NJPh...13l5014F ,
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 ,
The XMM-Newton HBS28 sample: Studying the obscuration in hard X-ray selected AGNs . Caccianiga, A., Severgnini, P., et all. . A&A . 416-901 . 2004 . 2004A&A...416..901C ,
High precision X-ray log N - log S distributions: implications for the obscured AGN population . Mateos, S., Warwick, R. S., et all. . A&A . 492-51...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-04-29T10:41:54Z/2001-04-29T19:38:55Z
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 2002-09-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-09-17T00:00:00Z, 008802, 17.56_20190403_1200. https://doi.org/10.5270/esa-05gi68x