A dataset provided by the European Space Agency

Name 015149
Title NGC 1132: A Fully-Merged Optically Dark Group
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0151490101

DOI 10.5270/esa-ypgdk4w
Author Prof William Mathews
Description We propose to observe NGC 1132, an isolated E galaxy surrounded by an ensemble of faint dwarf galaxies. Evidently, all of the more luminous original group members merged to form NGC 1132. It has a remarkably high total mass to light ratio suggesting that star formation in the group is unusually inefficient. XMM temperature measurements will provide an accurate dark mass profile out to half the virial radius. The radial variation of the Fe abundance in the hot gas will define the total number of supernova that have occurred over time. The simplicity of this fully merged system is ideal for gas dynamical calculations, which, when compared to XMM observations, afford a unique opportunity to learn about galaxy evolution.
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 ,
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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 ,
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 . ...,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
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 ,
Variability and the X-ray-UV ratio of active galactic nuclei . Vagnetti, F., Turriziani, S., et all. . A&A . 519-17 . 2010 . 2010A&A...519A..17V ,
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 ,
The XMM-Newton serendipitous ultraviolet source survey catalogue . Page, M. J., Brindle, C., et all. . MNRAS . 426-903 . 2012 . 2012MNRAS.426..903P ,
Properties of the integrated spectrum of serendipitous 2XMM catalog sources . Chaudhary, P., Brusa, M., et all. . A&A . 518-58 . 2010 . 2010A&A...518A..58C ,
Rest-frame stacking of 2XMM catalog sources. Properties of the Fe Kalpha line . Chaudhary, P., Brusa, M., et all. . A&A . 537-6 . 2012 . 2012A&A...537A...6C ,
Using the Bright Ultrahard XMM-Newton survey to define an IR selection of luminous AGN based on WISE colours . Mateos, S., Alonso-Herrero, A., et all. . MNRAS . 426-3271 . 2012 . 2012MNRAS.426.3271M ,
Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey . Pineau, F.-X., Motch, C., et all. . A&A . 527-126 . 2011 . 2011A&A...527A.126P ,
A systematic cross-search for radio-infrared counterparts of XMM- Newton sources . Combi, J. A., Albacete Colombo, J. F., et all. . Ap&SS . 331-53 . 2011 . 2011Ap&SS.331...53C ,
Exploring X-ray and radio emission of type 1 AGN up to z ~ 2.3 . Ballo, L., Heras, F. J. H., et all. . A&A . 545-66 . 2012 . 2012A&A...545A..66B ,
The Fifth Data Release Sloan Digital Sky Survey-XMM-Newton Quasar Survey . Young, M., Elvis, M., . ApJS . 183-17 . 2009 . 2009ApJS..183...17Y ,
A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys . Brightman, M., Silverman, J. D., et all. . MNRAS . 433-2485 . 2013 . 2013MNRAS.433.2485B ,
Uncovering obscured luminous AGN with WISE . Mateos, S., Alonso-Herrero, A., et all. . MNRAS . 434-941 . 2013 . 2013MNRAS.434..941M ,
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 . 2015A&A...573A.118L ,
Revisiting the relationship between 6 mum and 2-10 keV continuum luminosities of AGN . Mateos, S., Carrera, F. J., et all. . MNRAS . 449-1422 . 2015 . 2015MNRAS.449.1422M ,
ERRATUM: "The Fifth Data Release Sloan Digital Sky Survey-XMM-Newton Quasar Survey" (2009, ApJS, 183, 17) . Young, M., Elvis, M., . ApJS . 185-250 . 2009 . 2009ApJS..185..250Y ,
Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
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 ,
A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 . Pons, E., Watson, M. G., . A&A . 594-72 . 2016 . 2016A&A...594A..72P ,
Studying Cosmic Evolution with the XMM-Newton Distant Cluster Project: X-ray Luminous Galaxy Clusters at z>~1 and their Galaxy Populations . Fassbender, Rene, . PhDT . 0-116 . 2008 . 2008PhDT.......116F ,
AGNs with discordant optical and X-ray classification are not a physical family: diverse origin in two AGNs . Ordovas-Pascual, I., Mateos, S., et all. . MNRAS . 469-693 . 2017 . 2017MNRAS.469..693O ,
Disturbed Fossil Group Galaxy NGC 1132 . Kim, Dong-Woo, Anderson, Craig, et all. . ApJ . 853-129 . 2018 . 2018ApJ...853..129K ,
Anisotropy of the galaxy cluster X-ray luminosity-temperature relation . Migkas, Konstantinos, Reiprich, Thomas H., . A&A . 611-50 . 2018 . 2018A&A...611A..50M ,
Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals . Sibeck, David G., Allen, R., et all. . SSRv . 214-79 . 2018 . 2018SSRv..214...79S ,
The XMM Cluster Survey: Present status and latest results . Viana, P. T. P., Mehrtens, N., et all. . AN . 334-462 . 2013 . 2013AN....334..462V ,
The non-uniformity of galaxy cluster metallicity profiles . Lovisari, L., Reiprich, T. H., . MNRAS . 483-540 . 2019 . 2019MNRAS.483..540L ,
The Massive and Distant Clusters of WISE Survey. I. Survey Overview and a Catalog of >2000 Galaxy Clusters at z ~= 1 . Gonzalez, Anthony H., Gettings, Daniel P., et all. . ApJS . 240-33 . 2019 . 2019ApJS..240...33G ,
A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). II. Physical Properties Derived from the SED Fitting with Optical, Infrared, and Radio Data . Toba, Yoshiki, Yamashita, Takuji, et all. . ApJS . 243-15 . 2019 . 2019ApJS..243...15T ,
Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline . Hollowood, Devon L., Jeltema, Tesla, et all. . ApJS . 244-22 . 2019 . 2019ApJS..244...22H ,
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters . Palmese, A., Annis, J., et all. . MNRAS . 493-4591 . 2020 . 2020MNRAS.493.4591P ,
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 ,
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 2003-07-16T08:28:01Z/2003-07-16T21:34:45Z
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 2004-09-10T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-09-10T00:00:00Z, 015149, 17.56_20190403_1200. https://doi.org/10.5270/esa-ypgdk4w