A dataset provided by the European Space Agency

Name 050111
Title Are fossil groups a challenge of the CDM paradigm?


DOI 10.5270/esa-offpf58
Author Dr Gabriel Pratt
Description Fossil groups may have up to two orders of magnitude less substructure than predicted in CDM simulations. The significance of this lack of substructure depends on the depth of the galaxy luminosity function and on the mass of the group. We have initiated a project to determine the substructure distribution function (SDF) for the members of a representative sample of 4 REFLEX fossil groups down to M^* + 6 within a large fraction of the infall region. We will obtain X-ray observations of two fossil groups to complete the X-ray sample, to complement the optical observations and to compare with new simulations. We will compare the SDF from optical and X-ray mass estimates with theoretical predictions. We will establish if fossil groups do challenge the CDM paradigm.
Publication Testing adiabatic contraction of dark matter in fossil group candidates . Democles, J., Pratt, G. W., et all. . A&A . 517-52 . 2010 . 2010A&A...517A..52D ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive . Clerc, N., Sadibekova, T., et all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
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 ,
An XMM-Newton Survey of the Soft X-Ray Background. III. The Galactic Halo X-Ray Emission . Henley, David B., Shelton, Robin L., . ApJ . 773-92 . 2013 . 2013ApJ...773...92H ,
A volume-limited sample of X-ray galaxy groups and clusters - I. Radial entropy and cooling time profiles . Panagoulia, E. K., Fabian, A. C., . MNRAS . 438-2341 . 2014 . 2014MNRAS.438.2341P ,
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 ,
Scaling properties of a complete X-ray selected galaxy group sample . Lovisari, L., Reiprich, T. H., . A&A . 573-118 . 2015 . ...,
The Origin of the Hot Gas in the Galactic Halo: Testing Galactic Fountain Models. X-Ray Emission . Henley, David B., Shelton, Robin L., et all. . ApJ . 800-102 . 2015 . 2015ApJ...800..102H ,
A New Sample of Obscured AGNs Selected from the XMM-Newton and AKARI Surveys . Terashima, Yuichi, Hirata, Yoshitaka, et all. . ApJ . 814-11 . 2015 . 2015ApJ...814...11T ,
A volume-limited sample of X-ray galaxy groups and clusters - II. X-ray cavity dynamics . Panagoulia, E. K., Fabian, A. C., et all. . MNRAS . 444-1236 . 2014 . 2014MNRAS.444.1236P ,
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 ,
SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV . Clerc, N., Merloni, A., et all. . MNRAS . 463-4490 . 2016 . 2016MNRAS.463.4490C ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
XMM-Newton view of X-ray overdensities from nearby galaxy clusters: the environmental dependencies . Caglar, Turgay, Hudaverdi, Murat, . MNRAS . 471-4990 . 2017 . 2017MNRAS.471.4990C ,
The non-uniformity of galaxy cluster metallicity profiles . Lovisari, L., Reiprich, T. H., . MNRAS . 483-540 . 2019 . 2019MNRAS.483..540L ,
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 ,
Probing cosmic isotropy with a new X-ray galaxy cluster sample through the LX-T scaling relation . Migkas, K., Schellenberger, G., et all. . A&A . 636-15 . 2020 . 2020A&A...636A..15M ,
Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks . Kosiba, Matej, Lieu, Maggie, et all. . MNRAS . 496-4141 . 2020 . 2020MNRAS.496.4141K ,
SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release . Clerc, N., Kirkpatrick, C. C., et all. . MNRAS . 497-3976 . 2020 . 2020MNRAS.497.3976C ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-05-29T23:28:09Z/2007-11-23T09:19:27Z
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 2009-01-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-01-01T00:00:00Z, 050111, 17.56_20190403_1200. https://doi.org/10.5270/esa-offpf58