A dataset provided by the European Space Agency

Name 010606
Title A Detailed Study of the ICM of the Virgo Cluster North of M87
URL

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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0106060201
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DOI 10.5270/esa-i9mg5bp
Author Dr Bernd Aschenbach
Description All cosmologically interesting measurements on galaxy clusters based on X-ray observations like the masses, the Dark Matter and gas mass fractions, the metal abundances, etc. are dependent on how the intracluster medium is modelled. The degree of observationally unresolved temperature and density fluctuations present versus assumed in the analysis modify the results obtained. Therefore it is important to study the structure of the intracluster medium to the highest possible resolution. The key object for this study is the nearby Virgo cluster. To cover at least a representative cross section through part of the cluster a string of 13 pointings is proposed.
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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 ,
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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 ,
Are X-Ray Emitting Coronae around Supermassive Black Holes Outflowing? . Liu, Teng, Wang, Jun-Xian, et all. . ApJ . 783-106 . 2014 . 2014ApJ...783..106L ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Confirming the thermal Comptonization model for black hole X-ray emission in the low-hard state . Castro, M., D.Amico, F., et all. . A&A . 569-82 . 2014 . 2014A&A...569A..82C ,
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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 ,
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Distant clusters of galaxies in the 2XMM-SDSS footprint: follow-up observations with the LBT . Rabitz, A., Lamer, G., et all. . A&A . 607-56 . 2017 . 2017A&A...607A..56R ,
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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 ,
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 ,
Accretion History of AGNs. II. Constraints on AGN Spectral Parameters Using the Cosmic X-Ray Background . Ananna, Tonima Tasnim, Treister, Ezequiel, et all. . ApJ . 889-17 . 2020 . 2020ApJ...889...17A ,
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies . Ojha, Vineet, Chand, Hum, et all. . ApJ . 896-95 . 2020 . 2020ApJ...896...95O ,
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 2001-07-12T03:42:52Z/2002-07-08T08:16:10Z
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 2003-08-23T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-08-23T00:00:00Z, 010606, 17.56_20190403_1200. https://doi.org/10.5270/esa-i9mg5bp