# "SZ spectroscopy" in the coming decade: Galaxy cluster cosmology and   astrophysics in the submillimeter

**Authors:** Kaustuv Basu (Bonn), Jens Erler (Bonn), Jens Chluba (Manchester),, Jacques Delabrouille (APC Paris), J. Colin Hill (IAS/Flatiron Institute),, Tony Mroczkowski (ESO), Michael D. Niemack (Cornell), Mathieu Remazeilles, (Manchester), Jack Sayers (Caltech), Douglas Scott (UBC), Eve M. Vavagiakis, (Cornell), Michael Zemcov (RIT), Manuel Aravena (UDP), James G. Bartlett (APC, Paris/JPL), Nicholas Battaglia (Cornell), Frank Bertoldi (Bonn), Maude, Charmetant (Bonn), Sunil Golwala (Caltech), Terry L. Herter (Cornell), Pamela, Klaassen (UK ATC), Eiichiro Komatsu (MPA), Benjamin Magnelli (Bonn), Adam B., Mantz (KIPAC/Stanford), P. Daniel Meerburg (KICC/Groningen), Jean-Baptiste, Melin (IRFU Saclay), Daisuke Nagai (Yale), Stephen C. Parshley (Cornell),, Etienne Pointecouteau (IRAP Toulouse), Miriam E. Ramos-Ceja (Bonn), Mateusz, Ruszkowski (Michigan), Neelima Sehgal (Stony Brook), Gordon G. Stacey, (Cornell), Rashid Sunyaev (MPA/IKI)

arXiv: 1903.04944 · 2019-03-13

## TL;DR

This paper discusses the potential of submillimeter SZ spectroscopy to advance galaxy cluster studies and astrophysics, emphasizing recent developments and future opportunities in the coming decade.

## Contribution

It highlights the importance of systematic SZ spectral analysis in the submillimeter range and advocates for its role in future galaxy cluster and astrophysics research.

## Key findings

- Recent advancements in CMB instrumentation enable detailed SZ spectral studies.
- Multi-wavelength SZ spectra can reveal new astrophysical insights.
- The coming decade offers a golden era for SZ spectral measurements.

## Abstract

Sunyaev-Zeldovich (SZ) effects were first proposed in the 1970s as tools to identify the X-ray emitting hot gas inside massive clusters of galaxies and obtain their velocities relative to the cosmic microwave background (CMB). Yet it is only within the last decade that they have begun to significantly impact astronomical research. Thanks to the rapid developments in CMB instrumentation, measurement of the dominant thermal signature of the SZ effects has become a routine tool to find and characterize large samples of galaxy clusters and to seek deeper understanding of several important astrophysical processes via high-resolution imaging studies of many targets. With the notable exception of the Planck satellite and a few combinations of ground-based observatories, much of this "SZ revolution" has happened in the photometric mode, where observations are made at one or two frequencies in the millimeter regime to maximize the cluster detection significance and minimize the foregrounds. Still, there is much more to learn from detailed and systematic analyses of the SZ spectra across multiple wavelengths, specifically in the submillimeter (>300 GHz) domain. The goal of this Science White Paper is to highlight this particular aspect of SZ research, point out what new and potentially groundbreaking insights can be obtained from these studies, and emphasize why the coming decade can be a golden era for SZ spectral measurements.

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1903.04944/full.md

## References

96 references — full list in the complete paper: https://tomesphere.com/paper/1903.04944/full.md

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Source: https://tomesphere.com/paper/1903.04944