A dataset provided by the European Space Agency

Name 040496
Title The XMM Large Scale Structure Survey
URL

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DOI 10.5270/esa-xyfomia
Author Dr Marguerite Pierre
Description We propose to complete, by an additional 5 deg2, the XMM-LSS Survey region overlying the Spitzer-SWIRE field. This field already has CFHTLS and Integral coverage, and will encompass about 10 deg2. The resulting multi-wavelength medium-depth survey, which complements XMM and Chandra deep surveys, will provide a unique view of large-scale structure over a wide range of redshift, and will show active galaxies in the full range of environments. The complete coverage by optical and IR surveys provides high-quality photometric redshifts, so that cosmological results can quickly be extracted. In the spirit of a Legacy survey, we will make the raw X-ray data immediately public. Multi-band catalogues and images will also be made available on short time scales.
Publication Identifying XMM-Newton observations affected by solar wind charge exchange - Part II . Carter, J. A., Sembay, S., . A&A . 527-115 . 2011 . 2011A&A...527A.115C ,
Six More Quasars at Redshift 6 Discovered by the Canada-France High-z Quasar Survey . Willott, Chris J., Delorme, Philippe, et all. . AJ . 137-3541 . 2009 . 2009AJ....137.3541W ,
Angular correlation functions of X-ray point-like sources in the full exposure XMM-LSS field . Elyiv, A., Clerc, N., et all. . A&A . 537-131 . 2012 . 2012A&A...537A.131E ,
A Chandra view of the z = 1.62 galaxy cluster IRC-0218A . Pierre, M., Clerc, N., et all. . A&A . 540-4 . 2012 . 2012A&A...540A...4P ,
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 ,
Black Hole Accretion in Low-Mass Galaxies since z ~ 1 . Shi, Yong, Rieke, George, et all. . ApJ . 688-794 . 2008 . 2008ApJ...688..794S ,
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 ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The WIRCAM Deep Infrared Cluster Survey. I. Gr...
Instrument EPN, OM, RGS1, RGS2, EMOS1, EMOS2
Temporal Coverage 2006-07-04T06:25:24Z/2007-01-20T19:29:58Z
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 2008-08-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-08-29T00:00:00Z, 040496, 17.56_20190403_1200. https://doi.org/10.5270/esa-xyfomia