Resolving the Merging Planck Cluster PLCK G147.3-16.6 with GISMO

@article{Mroczkowski2015ResolvingTM,
  title={Resolving the Merging Planck Cluster PLCK G147.3-16.6 with GISMO},
  author={Tony Mroczkowski and Attila Kov'acs and E. Bulbul and Johannes G. Staguhn and Dominic J. Benford and Tracy E. Clarke and R. J. van Weeren and Huib T. Intema and S. W. Randall},
  journal={arXiv: Cosmology and Nongalactic Astrophysics},
  year={2015}
}
The $Planck$ satellite has recently completed an all-sky galaxy cluster survey exploiting the thermal Sunyaev-Zel'dovich (SZ) effect to locate some of the most massive systems observable. With a median redshift of $\left =0.22$, the clusters found by $Planck$ at $z>0.3$ are proving to be exceptionally massive and/or disturbed systems. One notable $Planck$ discovery at $z=0.645$, PLCK G147.3-16.6, has a dual core and hosts a radio halo, indicating it is likely in the process of merging. We… 

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References

SHOWING 1-10 OF 33 REFERENCES
The discovery of a radio halo in PLCK G147.3-16.6 at Z = 0.65
Recent X-ray and Sunyaev-Zel'dovich (SZ) observations have dramatically increased the number of known distant galaxy clusters. In some merging, low-redshift (z < 0.4) clusters, centrally located,
Exploring Cluster Physics with High-Resolution Sunyaev-Zel'dovich Effect Images and X-Ray Data
Foreseeing the era of high spatial resolution measurements of the Sunyaev–Zel’dovich effect (SZE) in clusters of galaxies, we present a prototype analysis of this sort combined with Chandra X-ray
Pressure distribution of the high-redshift cluster of galaxies CL J1226.9+3332 with NIKA ?
The thermal Sunyaev-Zel’dovich (tSZ) e ect is expected to provide a low scatter mass proxy for galaxy clusters since it is directly proportional to the cluster thermal energy. The tSZ observations
The Atacama Cosmology Telescope: Sunyaev-Zel'dovich selected galaxy clusters at 148 GHz from three seasons of data
We present a catalog of 68 galaxy clusters, of which 19 are new discoveries, detected via the Sunyaev-Zel'dovich effect (SZ) at 148 GHz in the Atacama Cosmology Telescope (ACT) survey on the
Galaxy clusters discovered via the Sunyaev-Zel'dovich effect in the 2500-square-degree SPT-SZ survey
We present a catalog of galaxy clusters selected via their Sunyaev-Zel'dovich (SZ) effect signature from 2500 deg^2 of South Pole Telescope (SPT) data. This work represents the complete sample of
Planck intermediate results - X. Physics of the hot gas in the Coma cluster
We present an analysis of Planck satellite data on the Coma cluster observed via the Sunyaev-Zeldovich effect. Thanks to its great sensitivity, Planck is able, for the first time, to detect SZ
Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources
We describe the all-sky Planck catalogue of clusters and cluster candidates derived from Sunyaev-Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite observations. The
A MULTI-WAVELENGTH STUDY OF THE SUNYAEV-ZEL'DOVICH EFFECT IN THE TRIPLE-MERGER CLUSTER MACS J0717.5+3745 WITH MUSTANG AND BOLOCAM
We present 90, 140, and 268 GHz subarcminute resolution imaging of the Sunyaev-Zel'dovich effect (SZE) in the disturbed, intermediate-redshift (z = 0.5458) galaxy cluster MACS J0717.5+3745, a
First observation of the thermal Sunyaev-Zel’dovich effect with kinetic inductance detectors
Clusters of galaxies provide precious informations on the evolution of the Universe and large scale structures. Recent cluster observations via the thermal Sunyaev-Zel'dovich (tSZ) effect have proven
Implications of a High Angular Resolution Image of the Sunyaev-Zel'Dovich Effect in RXJ1347–1145
The most X-ray luminous cluster known, RXJ1347–1145 (z = 0.45), has been the object of extensive study across the electromagnetic spectrum. We have imaged the Sunyaev-Zel'dovich effect (SZE) at 90
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4
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