Pith. sign in

REVIEW

Mapping the intracluster medium temperature in the era of NIKA2 and MUSTANG-2

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2111.01446 v1 pith:7OIHXQIR submitted 2021-11-02 astro-ph.CO

Mapping the intracluster medium temperature in the era of NIKA2 and MUSTANG-2

F. Ruppin , R. Adam , P. Ade , H. Ajeddig , P. Andr\'e , E. Artis , H. Aussel , A. Beelen
show 45 more authors
A. Beno\^it S. Berta L. Bing O. Bourrion M. Brodwin M. Calvo A. Catalano B. Decker M. De Petris F.-X. D\'esert S. Doyle E. F. C. Driessen P. R. M. Eisenhardt A. Gomez A. H. Gonzalez J. Goupy F. K\'eruzor\'e C. Kramer B. Ladjelate G. Lagache S. Leclercq J.-F. Lestrade J.-F. Mac\'ias-P\'erez A. Maury P. Mauskopf F. Mayet M. McDonald A. Monfardini E. Moravec M. Mu\~noz-Echeverr\'ia L. Perotto G. Pisano N. Ponthieu V. Rev\'eret A. J. Rigby A. Ritacco C. Romero H. Roussel K. Schuster S. Shu A. Sievers S. A. Stanford D. Stern C. Tucker R. Zylka
This is my paper
classification astro-ph.CO
keywords highmappingnika2temperatureaimsangulargalaxyintracluster
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

We present preliminary results from an on-going program that aims at mapping the intracluster medium (ICM) temperature of high redshift galaxy clusters from the MaDCoWS sample using a joint analysis of shallow X-ray data obtained by $Chandra$ and high angular resolution Sunyaev-Zel'dovich (SZ) observations realized with the NIKA2 and MUSTANG-2 cameras. We also present preliminary results from an on-going Open Time program within the NIKA2 collaboration that aims at mapping the ICM temperature of a galaxy cluster at $z=0.45$ from the resolved detection of the relativistic corrections to the SZ spectrum. These studies demonstrate how high angular resolution SZ observations will play a major role in the coming decade to push the investigation of ICM dynamics and non-gravitational processes to high redshift before the next generation X-ray observatories come into play.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.