M
Marios Chatzikos
Researcher at University of Kentucky
Publications - 59
Citations - 1246
Marios Chatzikos is an academic researcher from University of Kentucky. The author has contributed to research in topics: Emission spectrum & Spectral line. The author has an hindex of 15, co-authored 50 publications receiving 1043 citations. Previous affiliations of Marios Chatzikos include University of Virginia.
Papers
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Journal Article
The 2017 release of CLOUDY
Gary J. Ferland,Marios Chatzikos,F. Guzmán,Matt L. Lykins,P. A. M. van Hoof,R. J. R. Williams,N. P. Abel,N. R. Badnell,Francis P. Keenan,R. L. Porter,Phillip C. Stancil +10 more
TL;DR: The 2017 version of Cloudy as mentioned in this paper is the most recent version of the spectral synthesis code, which has made many improvements to the scope and accuracy of the physics which have been made since the previous release.
Journal ArticleDOI
The [CII] 158 micron line emission in high-redshift galaxies
TL;DR: In this paper, the authors used a semi-analytical model of galaxy evolution combined with the code CLOUDY to predict the [CII] luminosity of a large number of galaxies at 4 < z < 8.
Journal ArticleDOI
The [CII] 158 μm line emission in high-redshift galaxies
TL;DR: In this paper, a semi-analytical model of galaxy evolution combined with the photoionisation code CLOUDY was used to predict the [CII] luminosity of a large number of galaxies (25,000 at z ≃ 5) at 4 ≤ z ≤ 8.
Journal ArticleDOI
Deep Chandra, HST-COS, and Megacam Observations of the Phoenix Cluster: Extreme Star Formation and AGN Feedback on Hundred Kiloparsec Scales
Michael McDonald,Brian R. McNamara,Brian R. McNamara,Reinout J. van Weeren,Douglas Applegate,Matthew B. Bayliss,Marshall W. Bautz,Bradford Benson,Bradford Benson,John E. Carlstrom,John E. Carlstrom,Lindsey Bleem,Lindsey Bleem,Marios Chatzikos,Alastair C. Edge,Andrew C. Fabian,Gordon P. Garmire,Julie Hlavacek-Larrondo,Christine Jones-Forman,Adam Mantz,Eric D. Miller,B. Stalder,Sylvain Veilleux,John ZuHone +23 more
TL;DR: In this article, the HST-GO-13456.002A (Hubble) was used for the launch of the first HST satellite in the early 1990s.
Journal ArticleDOI
Deep Chandra, HST-COS, and Megacam Observations of the Phoenix Cluster: Extreme Star Formation and AGN Feedback on Hundred Kiloparsec Scales
Mike McDonald,Brian R. McNamara,R. J. van Weeren,D. Applegate,Matthew B. Bayliss,Marshall W. Bautz,Bradford Benson,John E. Carlstrom,Lindsey Bleem,Marios Chatzikos,Alastair C. Edge,A. C. Fabian,Gordon P. Garmire,Julie Hlavacek-Larrondo,C. Jones-Forman,Adam Mantz,Eric D. Miller,B. Stalder,Sylvain Veilleux,John ZuHone +19 more
TL;DR: In this article, the authors presented new ultraviolet, optical, and X-ray data on the Phoenix galaxy cluster (SPT-CLJ2344-4243) and reported a strong detection of OVI(1032,1038) which appears to originate primarily in shock-heated gas, but may contain a substantial contribution from the cooling ICM.