scholarly journals Galaxy Cluster Mass Reconstruction Project – IV. Understanding the effects of imperfect membership on cluster mass estimation

2018 ◽  
Vol 481 (1) ◽  
pp. 324-340 ◽  
Author(s):  
R Wojtak ◽  
L Old ◽  
G A Mamon ◽  
F R Pearce ◽  
R de Carvalho ◽  
...  
2015 ◽  
Vol 449 (2) ◽  
pp. 1897-1920 ◽  
Author(s):  
L. Old ◽  
R. Wojtak ◽  
G. A. Mamon ◽  
R. A. Skibba ◽  
F. R. Pearce ◽  
...  

2014 ◽  
Vol 441 (2) ◽  
pp. 1513-1536 ◽  
Author(s):  
L. Old ◽  
R. A. Skibba ◽  
F. R. Pearce ◽  
D. Croton ◽  
S. I. Muldrew ◽  
...  

2016 ◽  
Vol 460 (4) ◽  
pp. 3900-3912 ◽  
Author(s):  
Arya Farahi ◽  
August E. Evrard ◽  
Eduardo Rozo ◽  
Eli S. Rykoff ◽  
Risa H. Wechsler

2019 ◽  
Vol 884 (1) ◽  
pp. 33 ◽  
Author(s):  
Sheridan B. Green ◽  
Michelle Ntampaka ◽  
Daisuke Nagai ◽  
Lorenzo Lovisari ◽  
Klaus Dolag ◽  
...  

2019 ◽  
Vol 486 (4) ◽  
pp. 4863-4879 ◽  
Author(s):  
Ali Takey ◽  
Florence Durret ◽  
Isabel Márquez ◽  
Amael Ellien ◽  
Mona Molham ◽  
...  

ABSTRACT We present X-ray and optical properties of the optically confirmed galaxy cluster sample from the 3XMM/SDSS Stripe 82 cluster survey. The sample includes 54 galaxy clusters in the redshift range of 0.05–1.2, with a median redshift of 0.36. We first present the X-ray temperature and luminosity measurements that are used to investigate the X-ray luminosity–temperature relation. The slope and intercept of the relation are consistent with those published in the literature. Then, we investigate the optical properties of the cluster galaxies including their morphological analysis and the galaxy luminosity functions (GLFs). The morphological content of cluster galaxies is investigated as a function of cluster mass and distance from the cluster centre. No strong variation of the fraction of early- and late-type galaxies with cluster mass is observed. The fraction of early-type galaxies as a function of cluster radius varies as expected. The individual GLFs of red sequence galaxies were studied in the five ugriz bands for 48 clusters. The GLFs were then stacked in three mass bins and two redshift bins. Twenty clusters of the present sample are studied for the first time in X-rays, and all are studied for the first time in the optical range. Altogether, our sample appears to have X-ray and optical properties typical of ‘average’ cluster properties.


2006 ◽  
Vol 368 (2) ◽  
pp. 518-533 ◽  
Author(s):  
L. M. Voigt ◽  
A. C. Fabian

2007 ◽  
Vol 467 (2) ◽  
pp. 427-436 ◽  
Author(s):  
S. Paulin-Henriksson ◽  
V. Antonuccio-Delogu ◽  
C. P. Haines ◽  
M. Radovich ◽  
A. Mercurio ◽  
...  

2016 ◽  
Vol 2016 (04) ◽  
pp. 023-023 ◽  
Author(s):  
L. Pizzuti ◽  
B. Sartoris ◽  
S. Borgani ◽  
L. Amendola ◽  
K. Umetsu ◽  
...  

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