Multiple inflation by Adams, J, Ross, G, Sarkar, S

“…An observed feature in the power spectrum of galaxy clustering from the APM survey may well be associated with such structure. …”

Observational constraints on f(T) gravity from model-independent data by F. B. M. dos Santos, J. E. Gonzalez, R. Silva

“…In particular, we investigate the restrictions given by the gas mass fraction measurements of galaxy clusters and transversal BAO data. Both data sets are regarded as weakly dependent on a fiducial cosmology. …”
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Searching for a 0.1-1 keV Cosmic Axion Background by Conlon, J, Marsh, M

“…We propose that axion-photon conversion may explain the observed excess emission of soft X-rays from galaxy clusters, and may also contribute to the diffuse unresolved cosmic X-ray background. …”

The <i>κ</i>-Model under the Test of the SPARC Database by Gianni Pascoli

“…The <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi>κ</mi></semantics></math></inline-formula>-model has been tested on a small sample of spiral galaxies and in galaxy clusters. Now, we test this model on a large sample of galaxies issued from the SPARC database.…”
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A machine learning method to infer clusters of galaxies mass radial profiles from mock Sunyaev-Zel’dovich maps with The Three Hundred clusters by Ferragamo A., de Andres D., Sbriglio A., Cui W., De Petris M., Yepes G., Dupuis R., Jarraya M., Lahouli I., De Luca F., Gianfagna G., Rasia E.

“…Our study introduces a new machine learning algorithm for estimating 3D cumulative radial profiles of total and gas mass in galaxy clusters from thermal Sunyaev-Zel’dovich (SZ) effect maps. …”
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Linear structures in the core of the Coma cluster of galaxies. by Sanders, J, Fabian, A, Churazov, E, Schekochihin, A, Simionescu, A, Walker, SA, Werner, N

“…The hot x-ray-emitting plasma in galaxy clusters is predicted to have turbulent motion, which can contribute around 10% of the cluster's central energy density. …”

The galaxy-halo connection in the VIDEO Survey at 0.5 by Hatfield, P, Lindsay, S, Jarvis, M, Haeussler, B, Vaccari, M, Verma, A

“…VIDEO is the only survey currently capable of probing the bulk of stellar mass in galaxies at redshifts corresponding to the peak of star formation on degree scales. Galaxy clustering is measured with the two-point correlation function, which is calculated using a non parametric kernel based density estimator. …”

Are cluster radio relics revived fossil radio cocoons? by Ensslin, T, Gopal-Krishna

“…Such a wave can be caused by merging events in galaxy clusters, or by accretion onto clusters. An implication of this model is the existence of a population of diffuse, ultra-steep spectrum, very low-frequency radio sources located inside and possibly outside of clusters of galaxies, tracing the revival of aged fossil radio plasma by the shock waves associated with large-scale structure formation.…”

Global simulations of heat-flux-driven buoyancy and magnetothermal instabilities, and their astrophysical implications by Kulchoakrungsun, Ekapob

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A novel heterodyne interferometer for millimetre and sub-millimetre astronomy by Grimes, P, Brock, M, Holler, C, Jacobs, K, Jones, M, King, O, Leech, J, Taylor, A, Yassin, G

“…The primary science goal of this instrument is to measure the spectrum of the Sunyaev-Zel'dovich effect in galaxy clusters. In particular we intend to measure the frequency of the S-Z null near 217 GHz, which allows the gas temperature of the cluster to be determined. …”

Projection effects on pressure profiles: A case study of the Virgo replica by Lebeau T., Sorce J.G., Aghanim N.

“…An accurate mass calibration of galaxy clusters is a crucial step towards precise constraints on the cosmological parameters σ8 and Ωm from clusters. …”
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Searching for modified growth patterns with tomographic surveys by Gong-Bo, Zhao, Pogosian, Levon, Silvestri, Alessandra, Zylberberg, Joel

“…We then apply the Fisher matrix technique to forecast the errors on the modified growth parameters from galaxy clustering, weak lensing, CMB, and their cross correlations across multiple photometric redshift bins. …”
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Numerical modeling of laser-driven experiments aiming to demonstrate magnetic field amplification via turbulent dynamo by Tzeferacos, P, Rigby, A, Bott, A, Bell, A, Bingham, R, Casner, A, Cattaneo, F, Churazov, E, Emig, J, Flocke, N, Fiuza, F, Forest, C, Foster, J, Graziani, C, Katz, J, Koenig, M, Li, C, Meinecke, J, Petrasso, R, Park, H, Remington, B, Ross, J, Ryu, D, Ryutov, D, Weide, K, White, T, Reville, B, Miniati, F, Schekochihin, A, Froula, D, Gregori, G, Lamb, D

“…The universe is permeated by magnetic fields, with strengths ranging from a femtogauss in the voids between the filaments of galaxy clusters to several teragauss in black holes and neutron stars. …”

FRIIb radio sources, ambient gas densities, and clusters of galaxies by Daly, R, Guerra, E, Chester, M

“…Typical ambient gas densities and the composite density profile indicate that the sources lie in gaseous environments very much like the cores of galaxy clusters. Some evolution of the core gas density and radius with redshift axe suggested by the data.…”

Some contributions of MAGIC to the physics ofcosmic rays by Gozzini S.R.

“…We will also mention cosmic ray acceleration in galaxy clusters. Other than that, hadron-hadron interactions are supposed to take place in some supernova remnants in interaction with surrounding molecular clouds; we will show some results, in connection with cosmic rays of galactic origin. …”
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Dynamics of stochastic-constrained particles by Tao Guo

“…The predicted density distribution of the particle swarm in the stable aggregation state is consistent with the total mass distribution of massive, relaxed galaxy clusters (at least in the range of $$r<r_{\textrm{s}}$$ r < r s ), preventing cuspy problems in the empirical Navarro–Frenk–White profile. …”
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Towards precision SZ cluster cosmology: From Planck to the Simons Observatory by Zubeldia Í.

“…As demonstrated by Planck, SPT, and ACT, the abundance of Sunyaev-Zeldovich-detected galaxy clusters across mass and redshift is a powerful cosmological probe. …”
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Strong lensing considerations for the LSST observing strategy by Verma, A, Collett, T, Smith, G, on behalf of the Strong Lensing Science Collaboration, in collaboration with the DESC Strong Lensing Science Working Group

“…LSST will drive studies of strongly lensed galaxies, galaxy groups and galaxy clusters into the statistical age. Time variable lensing events, e.g. measuring cosmological time delays from strongly lensed supernovae and quasars, place the strongest constraints on LSST's observing strategy and have been considered in the DESC observing strategy white papers. …”

Turbulence, magnetic fields and plasma physics in clusters of galaxies by Schekochihin, A, Cowley, S

“…Observations of galaxy clusters show that the intracluster medium (ICM) is likely to be turbulent and is certainly magnetized. …”

Analytic marginalization of N(z) uncertainties in tomographic galaxy surveys by Hadzhiyska, B, Alonso, D, Nicola, A, Slosar, A

“…We showcase this method by applying it to the galaxy clustering measurements from the Hyper Suprime-Cam first data release. …”