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result(s) for
"Kesebonye, Kabelo C"
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A Multiwavelength Dynamical State Analysis of ACT-CL J0019.6+0336
by
Turner, David J.
,
Knowles, Kenda
,
Moodley, Kavilan
in
Calibration
,
cluster dynamical state
,
Clusters
2021
In our study, we show a multiwavelength view of ACT-CL J0019.6+0336 (which hosts a radio halo), to investigate the cluster dynamics, morphology, and ICM. We use a combination of XMM-Newton images, Dark Energy Survey (DES) imaging and photometry, SDSS spectroscopic information, and 1.16 GHz MeerKAT data to study the cluster properties. Various X-ray and optical morphology parameters are calculated to investigate the level of disturbance. We find disturbances in two X-ray parameters and the optical density map shows elongated and axisymmetric structures with the main cluster component southeast of the cluster centre and another component northwest of the cluster centre. We also find a BCG offset of ∼950 km/s from the mean velocity of the cluster, and a discrepancy between the SZ mass, X-ray mass, and dynamical mass (MX,500 and MSZ,500 lies >3σ away from Mdyn,500), showing that J0019 is a merging cluster and probably in a post-merging phase.
Journal Article
A Multiwavelength Dynamical State Analysis of ACT-CLJ0019.6+0336
2021
In our study, we show a multiwavelength view of ACT-CL J0019.6+0336 (which hosts aradio halo), to investigate the cluster dynamics, morphology, and ICM. We use a combination ofXMM-Newton images, Dark Energy Survey (DES) imaging and photometry, SDSS spectroscopicinformation, and 1.16 GHz MeerKAT data to study the cluster properties. Various X-ray and opticalmorphology parameters are calculated to investigate the level of disturbance. We find disturbancesin two X-ray parameters and the optical density map shows elongated and axisymmetric structureswith the main cluster component southeast of the cluster centre and another component northwest ofthe cluster centre. We also find a BCG offset of∼950 km/s from the mean velocity of the cluster, anda discrepancy between the SZ mass, X-ray mass, and dynamical mass (MX,500andMSZ,500lies>3σaway fromMdyn,500), showing that J0019 is a merging cluster and probably in a post-merging phase.
Journal Article
The MeerKAT Galaxy Clusters Legacy Survey: star formation in massive clusters at 0.15 < z < 0.35
by
Knowles, Kenda
,
Moodley, Kavilan
,
Sikhosana, Sinenhlanhla P
in
Dark energy
,
Galactic clusters
,
Galactic halos
2022
We investigate dust-unbiased star formation rates (SFR) as a function of the environment in 20 massive clusters (\\(M_{200}>4\\times10^{14} {\\rm M}_{\\odot}\\)) between \\(0.15
A Multiwavelength Dynamical State Analysis of ACT-CL J0019.6+0336
2021
In our study, we show a multiwavelength view of ACT-CL J0019.6+0336 (which hosts a radio halo), to investigate the cluster dynamics, morphology, and ICM. We use a combination of XMM-Newton images, Dark Energy Survey (DES) imaging and photometry, SDSS spectroscopic information, and 1.16 GHz MeerKAT data to study the cluster properties. Various X-ray and optical morphology parameters are calculated to investigate the level of disturbance. We find disturbances in two X-ray parameters and the optical density map shows elongated and axisymmetric structures with the main cluster component southeast of the cluster centre and another component northwest of the cluster centre. We also find a BCG offset of \\(\\sim\\)950 km/s from the mean velocity of the cluster, and a discrepancy between the SZ mass, X-ray mass, and dynamical mass (\\(M_{X,500}\\) and \\(M_{SZ,500}\\) lies >3 \\(\\sigma\\) away from \\(M_{\\rm{dyn},500}\\)), showing that J0019 is a merging cluster and probably in a post-merging phase.
A Multiwavelength Dynamical State Analysis of ACT-CLJ0019.6+0336
by
Knowles, Kenda
,
Moodley, Kavilan
,
Mroczkowski, Tony
in
Clusters
,
Dark energy
,
Elongated structure
2021
In our study, we show a multiwavelength view of ACT-CL J0019.6+0336 (which hosts aradio halo), to investigate the cluster dynamics, morphology, and ICM. We use a combination ofXMM-Newton images, Dark Energy Survey (DES) imaging and photometry, SDSS spectroscopicinformation, and 1.16 GHz MeerKAT data to study the cluster properties. Various X-ray and opticalmorphology parameters are calculated to investigate the level of disturbance. We find disturbancesin two X-ray parameters and the optical density map shows elongated and axisymmetric structureswith the main cluster component southeast of the cluster centre and another component northwest ofthe cluster centre. We also find a BCG offset of∼950 km/s from the mean velocity of the cluster, anda discrepancy between the SZ mass, X-ray mass, and dynamical mass (MX,500andMSZ,500lies 3σaway fromMdyn,500), showing that J0019 is a merging cluster and probably in a post-merging phase.
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