Galaxy and Mass Assembly (GAMA): Selection of the Most Massive Clusters
2014 ◽
Vol 11
(S308)
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pp. 215-216
Keyword(s):
AbstractWe have developed a galaxy cluster finding technique based on the Delaunay Tessellation Field Estimator (DTFE) combined with caustic analysis. Our method allows us to recover clusters of galaxies within the mass range of $10^{12}$ to $10^{16}\ \mathcal{M}_{\odot}$. We have found a total of 113 galaxy clusters in the Galaxy and Mass Assembly survey (GAMA). In the corresponding mass range, the density of clusters found in this work is comparable to the density traced by clusters selected by the thermal Sunyaev Zel'dovich Effect; however, we are able to cover a wider mass range. We present the analysis of the two-point correlation function for our cluster sample.
2019 ◽
Vol 490
(2)
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pp. 1693-1696
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Keyword(s):
2005 ◽
Vol 216
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pp. 43-50
2005 ◽
Vol 216
◽
pp. 196-202
Keyword(s):
2020 ◽
Vol 493
(1)
◽
pp. 1120-1129
Keyword(s):
2020 ◽
Vol 496
(3)
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pp. 3169-3181
Keyword(s):
1994 ◽
Vol 73
(2)
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pp. 215-219
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1987 ◽
Vol 124
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pp. 363-366
2010 ◽
Vol 409
(2)
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pp. 867-872
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