The Sunyaev–Zel'dovich effect at 5″: RX J1347.5−1145 imaged by ALMA

@article{Kitayama2016TheSE,
  title={The Sunyaev–Zel'dovich effect at 5″: RX J1347.5−1145 imaged by ALMA},
  author={Tetsu Kitayama and Shutaro Ueda and Shigehisa Takakuwa and Takahiro Tsutsumi and Eiichiro Komatsu and Takuya Akahori and Daisuke Iono and Takuma Izumi and Ryohei Kawabe and Kotaro Kohno and Hiroshi Matsuo and Naomi Ota and Yasushi Suto and Motokazu Takizawa and Kohji Yoshikawa},
  journal={Publications of the Astronomical Society of Japan},
  year={2016},
  volume={68},
  pages={88}
}
We present the first image of the thermal Sunyaev-Zel'dovich effect (SZE) obtained by the Atacama Large Millimeter/submillimeter Array (ALMA). Combining 7-m and 12-m arrays in Band 3, we create an SZE map toward a galaxy cluster RXJ1347.5-1145 with 5 arc-second resolution (corresponding to the physical size of 20 kpc/h), the highest angular and physical spatial resolutions achieved to date for imaging the SZE, while retaining extended signals out to 40 arc-seconds. The 1-sigma statistical… 

A joint ALMA–Bolocam–Planck SZ study of the pressure distribution in RX J1347.5−1145

We report the joint analysis of single-dish and interferometric observations of the Sunyaev–Zeldovich (SZ) effect from the galaxy cluster RX J1347.5−1145. We have developed a parametric fitting

Pressure Profiles and Mass Estimates Using High-resolution Sunyaev–Zel’dovich Effect Observations of Zwicky 3146 with MUSTANG-2

The galaxy cluster Zwicky 3146 is a sloshing cool core cluster at z = 0.291 that in X-ray imaging does not appear to exhibit significant pressure substructure in the intracluster medium (ICM). The

Measurement of the Relativistic Sunyaev–Zeldovich Correction in RX J1347.5-1145

We present a measurement of the relativistic corrections to the thermal Sunyaev–Zel’dovich (SZ) effect spectrum, the rSZ effect, toward the massive galaxy cluster RX J1347.5-1145 by combining

ATCA 16 cm Observation of CIZA J1358.9-4750: Implication of Merger Stage and Constraint on Non-Thermal Properties

We report the Australia Telescope Compact Array 16 cm observation of CIZA J1358.9-4750. Recent X-ray studies imply that this galaxy cluster is composed of merging, binary clusters. Using the EW367

Sunyaev–Zel’dovich profile fitting with joint AMI-Planck analysis

We develop a Bayesian method of analysing Sunyaev–Zel’dovich measurements of galaxy clusters obtained from the Arcminute Microkelvin Imager (AMI) radio interferometer system and from the Planck

Unveiling the Merger Dynamics of the Most Massive MaDCoWS Cluster at z = 1.2 from a Multiwavelength Mapping of Its Intracluster Medium Properties

The characterization of the Intracluster Medium (ICM) properties of high-redshift galaxy clusters is fundamental to our understanding of large-scale structure formation processes. We present the

A High-resolution SZ View of the Warm-Hot Universe

The Sunyaev-Zeldovich (SZ) effect was first predicted nearly five decades ago, but has only recently become a mature tool for performing high resolution studies of the warm and hot ionized gas in and

Galaxy Cluster Pressure Profiles as Determined by Sunyaev Zel’dovich Effect Observations with MUSTANG and Bolocam. II. Joint Analysis of 14 Clusters

We present pressure profiles of galaxy clusters determined from high-resolution Sunyaev–Zel’dovich (SZ) effect observations of 14 clusters, which span the redshift range of . The procedure

The role of XMM-Newton for present and next-generation Sunyaev–Zeldovich experiments

A strong synergy exists between observations of the hot gas trapped in the potential well of galaxy clusters at X-ray wavelengths and through the Sunyaev–Zeldovich (SZ) effect. XMM-Newton has been a

First detection of a virial shock with SZ data: implication for the mass accretion rate of Abell 2319

Shocks produced by the accretion of infalling gas in the outskirts of galaxy clusters are expected in the hierarchical structure formation scenario, as found in cosmological hydrodynamical

References

SHOWING 1-10 OF 61 REFERENCES

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

Imaging Simulations of the Sunyaev-Zel'dovich Effect for ALMA

We present imaging simulations of the Sunyaev-Zel’dovich effect of galaxy clusters for the Atacama Large Millimeter/submillimeter Array (ALMA) including the Atacama Compact Array (ACA). In its most

MUSTANG HIGH ANGULAR RESOLUTION SUNYAEV–ZEL'DOVICH EFFECT IMAGING OF SUBSTRUCTURE IN FOUR GALAXY CLUSTERS

We present resolved images of four massive clusters of galaxies through the Sunyaev–Zel'dovich effect (SZE). These measurements, made at 90 GHz with the MUSTANG receiver on the Green Bank Telescope

CARMA MEASUREMENTS OF THE SUNYAEV–ZEL'DOVICH EFFECT IN RX J1347.5−1145

We demonstrate the Sunyaev–Zel'dovich (SZ) effect imaging capabilities of the Combined Array for Research in Millimeter-wave Astronomy (CARMA) by presenting an SZ map of the galaxy cluster RX

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

Extended Sunyaev-Zeldovich Map of the Most Luminous X-Ray Cluster, RX J1347–1145

We present a high-resolution (22'' FWHM) extended map at 2.1 mm of the Sunyaev-Zeldovich effect toward the most luminous X-ray cluster, RX J1347-1145. These observations have been performed with the

A Sunyaev-Zeldovich Map of the Massive Core in the Luminous X-Ray Cluster RX J1347–1145

We have mapped the Sunyaev-Zeldovich (SZ) decrement in the direction of the most luminous X-ray cluster known to date, RX J1347-1145, at z = 0.451. This has been achieved with an angular resolution

Substructures Revealed by the Sunyaev–Zel’dovich Effect at 150 GHz in a High-Resolution Map of RX J1347$-$1145

We report on mapping observations toward the region of the most luminous X-ray cluster RXJ1347-1145 (z=0.45) through the Sunyaev-Zel'dovich effect at 21GHz and 150GHz with the Nobeyama 45-m

MEASUREMENTS OF THE SUNYAEV–ZEL’DOVICH EFFECT IN MACS J0647.7+7015 AND MACS J1206.2–0847 AT HIGH ANGULAR RESOLUTION WITH MUSTANG

We present high resolution (9″) imaging of the Sunyaev–Zel’dovich Effect (SZE) toward two massive galaxy clusters, MACS J0647.7+7015 (z = 0.591) and MACS J1206.2–0847 (z = 0.439). We compare these 90

Interferometric Imaging of the Sunyaev-Zeldovich Effect at 30 GHz

We present high signal-to-noise ratio images of the Sunyaev-Zeldovich effect toward the clusters CL 0016+16 and Abell 773. A null result is reported for Abell 1704. The data were obtained with the
...