Disturbed galaxy clusters are more abundant in an X-ray volume-limited sample
A&A, 606 (2017) L4
Published online: 2017-10-05
Articles citing this article
The Citing articles tool gives a list of articles citing the current article.
The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
Cited article:
This article has been cited by the following article(s):
Beyond MACS: physical properties of extremely X-ray luminous clusters at z > 0.5
H Ebeling, J Richard, B Beauchesne, Q Basto, A C Edge and I SmailMonthly Notices of the Royal Astronomical Society 537 (3) 2662 (2025)
https://doi.org/10.1093/mnras/staf063
The FLAMINGO project: a comparison of galaxy cluster samples selected on mass, X-ray luminosity, Compton-Y parameter, or galaxy richness
Roi Kugel, Joop Schaye, Matthieu Schaller, Ian G McCarthy, Joey Braspenning, John C Helly, Victor J Forouhar Moreno and Robert J McGibbonMonthly Notices of the Royal Astronomical Society 534 (3) 2378 (2024)
https://doi.org/10.1093/mnras/stae2218
Hydrostatic mass profiles of galaxy clusters in the eROSITA survey
Dominik Scheck, Jeremy S. Sanders, Veronica Biffi, et al.Astronomy & Astrophysics 670 A33 (2023)
https://doi.org/10.1051/0004-6361/202244582
Dynamical state of galaxy clusters evaluated from X-ray images
Z S Yuan, J L Han and Z L WenMonthly Notices of the Royal Astronomical Society 513 (2) 3013 (2022)
https://doi.org/10.1093/mnras/stac1037
XMM-Newton study of six massive, X-ray luminous galaxy cluster systems in the redshift range z = 0.25–0.5
H. Böhringer, G. Chon, R. S. Ellis, R. Barrena and N. LaporteAstronomy & Astrophysics 664 A57 (2022)
https://doi.org/10.1051/0004-6361/202243424
Why are we still using 3D masses for cluster cosmology?
Stijn N B Debackere, Henk Hoekstra, Joop Schaye, Katrin Heitmann and Salman HabibMonthly Notices of the Royal Astronomical Society 515 (3) 3383 (2022)
https://doi.org/10.1093/mnras/stac1687
How baryons can significantly bias cluster count cosmology
Stijn N B Debackere, Joop Schaye and Henk HoekstraMonthly Notices of the Royal Astronomical Society 505 (1) 593 (2021)
https://doi.org/10.1093/mnras/stab1326
The Three Hundred project: dynamical state of galaxy clusters and morphology from multiwavelength synthetic maps
Federico De Luca, Marco De Petris, Gustavo Yepes, et al.Monthly Notices of the Royal Astronomical Society 504 (4) 5383 (2021)
https://doi.org/10.1093/mnras/stab1073
ENISALA. II. Distinct Star Formation and Active Galactic Nucleus Activity in Merging and Relaxed Galaxy Clusters
Andra Stroe and David SobralThe Astrophysical Journal 912 (1) 55 (2021)
https://doi.org/10.3847/1538-4357/abe7f8
X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field
Naomi Ota, Ikuyuki Mitsuishi, Yasunori Babazaki, Hiroki Akamatsu, Yuto Ichinohe, Shutaro Ueda, Nobuhiro Okabe, Masamune Oguri, Ryuichi Fujimoto, Takashi Hamana, Keita Miyaoka, Satoshi Miyazaki, Hanae Otani, Keigo Tanaka, Ayumi Tsuji and Atsushi YoshidaPublications of the Astronomical Society of Japan 72 (1) (2020)
https://doi.org/10.1093/pasj/psz118
The impact of the observed baryon distribution in haloes on the total matter power spectrum
Stijn N B Debackere, Joop Schaye and Henk HoekstraMonthly Notices of the Royal Astronomical Society 492 (2) 2285 (2020)
https://doi.org/10.1093/mnras/stz3446
How frequent are close supermassive binary black holes in powerful jet sources?
Martin G H Krause, Stanislav S Shabala, Martin J Hardcastle, et al.Monthly Notices of the Royal Astronomical Society 482 (1) 240 (2019)
https://doi.org/10.1093/mnras/sty2558
The Most Massive galaxy Clusters (M2C) across cosmic time: link between radial total mass distribution and dynamical state
I. Bartalucci, M. Arnaud, G. W. Pratt, J. Démoclès and L. LovisariAstronomy & Astrophysics 628 A86 (2019)
https://doi.org/10.1051/0004-6361/201935984
Interaction of the massive cluster system Abell 3016/3017 embedded in a cosmic filament
Gayoung Chon, Hans Böhringer, Sarthak Dasadia, et al.Astronomy & Astrophysics 621 A77 (2019)
https://doi.org/10.1051/0004-6361/201833068
Optical substructure and BCG offsets of Sunyaev–Zel’dovich and X-ray-selected galaxy clusters
Paulo A A Lopes, M Trevisan, T F Laganá, et al.Monthly Notices of the Royal Astronomical Society 478 (4) 5473 (2018)
https://doi.org/10.1093/mnras/sty1374
Evolution of the degree of substructures in simulated galaxy clusters
Cristiano De Boni, Hans Böhringer, Gayoung Chon and Klaus DolagMonthly Notices of the Royal Astronomical Society 478 (2) 2086 (2018)
https://doi.org/10.1093/mnras/sty1200