A dataset provided by the European Space Agency

Name 060359
Title The Evolution of Galaxies in Groups


DOI 10.5270/esa-3fnc2cx
Author Dr John Mulchaey
Description We propose to observe two fields from the CNOC2 redshift survey to study the evolution of galaxies in groups. The proposed observations will allow typical X-ray groups to be discovered out to z=0.8. The unique aspect of our program is that we have already identified a large sample of optically-selected groups in these fields over the same redshift interval. The combination of the X-ray and optically-selected samples will allow the construction of a sample spanning the full range of dynamical states of groups.
Publication Exploring the Diversity of Groups at 0.1 < z < 0.8 with X-Ray and Optically Selected Samples . Connelly, J. L., Wilman, David J., et all. . ApJ . 756-139 . 2012 . 2012ApJ...756..139C ,
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 ,
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 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 ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
A sensitive search for unknown spectral emission lines in the diffuse X-ray background with XMM-Newton . Gewering-Peine, A., Horns, D., . JCAP . 6-36 . 2017 . 2017JCAP...06..036G ,
AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton . Svoboda, J., Guainazzi, M., . A&A . 603-127 . 2017 . 2017A&A...603A.127S ,
A luminous X-ray outburst from an intermediate-mass black hole in an off-centre star cluster . Lin, Dacheng, Strader, Jay, et all. . NatAs . 2-656 . 2018 . 2018N...,
Tidal Disruption of a Main-sequence Star by an Intermediate-mass Black Hole: A Bright Decade . Chen, Jin-Hong, Shen, Rong-Feng, . ApJ . 867-20 . 2018 . 2018ApJ...867...20C ,
Multiwavelength Follow-up of the Hyperluminous Intermediate-mass Black Hole Candidate 3XMM J215022.4-055108 . Lin, Dacheng, Strader, Jay, et all. . ApJ . 892-25 . 2020 . 2020ApJ...892L..25L ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-06-01T07:54:25Z/2009-06-08T06:22:24Z
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 2010-06-24T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-06-24T00:00:00Z, 060359, 17.56_20190403_1200. https://doi.org/10.5270/esa-3fnc2cx