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Exploring relations between BCG and cluster properties in the SPectroscopic IDentification of eROSITA Sources survey from 0.05 < z < 0.3
Kate E. Furnell
, Chris A. Collins
, Lee S. Kelvin
, Nicolas Clerc
, Ivan K. Baldry
, Alexis Finoguenov
, Ghazaleh Erfanianfar
, Johan Comparat
,
Donald P. Schneider
Astronomy & Astrophysics
Center for Theoretical and Observational Cosmology
Center for Exoplanets & Habitable Worlds
Institute for Gravitation & the Cosmos
Research output
:
Contribution to journal
›
Article
›
peer-review
16
Scopus citations
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Keyphrases
Brightest Cluster Galaxies
100%
Spectroscopic Identification
100%
Galaxy Properties
100%
Clustering Property
100%
Stellar Masses
30%
X-ray
20%
Effective Radius
20%
Visual Inspection
10%
X-ray Data
10%
Luminosity
10%
Halo
10%
Sloan Digital Sky Survey
10%
ROSAT
10%
Spectroscopic Surveys
10%
Finders
10%
Maximum Likelihood
10%
Imaging Data
10%
Velocity Dispersion
10%
Point Spread Function
10%
Structural Evolution
10%
Significant Trend
10%
Galaxy Morphology
10%
Three-band
10%
Random Cluster
10%
Environmental Dependence
10%
Physics
Brightest Cluster Galaxies
100%
Stellar Mass
30%
X Ray
30%
Sky Surveys
10%
Galaxy Classification Systems
10%