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20172026
most citedThe Hyper Suprime-Cam SSP Survey: Overview and Survey Design

1.1k citations · 1.1k across the 15 of their papers we have counts for

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astro-ph.GA2026

Spiraling into the `snail' cluster MCXC J0157.4-0550

Chao Geng, Chong Ge, Ming Sun +8

We present a deep Chandra (130 ks) study of a striking, tidally induced cold front in a subcluster merging with the galaxy cluster MCXC J0157.4-0550. The subcluster, nicknamed the…

astro-ph.CO2026

Constraints on Nonlinearity of the Mass-Concentration Relation

Nobuhiro Okabe

We develop a Bayesian generalization of the previous method to constrain a wide variety of mass-concentration (M-C) relations motivated by both theoretical and observational studie…

astro-ph.HE2026

Exploring the dynamics of the Coma galaxy cluster by mapping its X-ray emission line profiles with XRISM

Kosei Sakai, Kazuhiro Nakazawa, Maxim Markevitch +17

The intracluster medium (ICM) in merging galaxy clusters exhibits turbulence and bulk flows. Unraveling these components is crucial not only for elucidating the geometry of the clu…

astro-ph.CO2026

Weak-lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: III. A precision cosmological sample enabled by optical confirmation

I-Non Chiu, Kai-Feng Chen, Masamune Oguri +9

We develop fCAMIRA (forced-mode CAMIRA), a tool for optical cluster confirmation, and apply it to a sample of 129 weak-lensing (WL) shear-selected galaxy clusters identified in ape…

astro-ph.CO2026

CHEX-MATE: AMALGAM weak-lensing analysis of 41 Planck Sunyaev-Zel'dovich-selected galaxy clusters

Keiichi Umetsu, Raphael Gavazzi, Mauro Sereno +20

We present a weak-lensing shear analysis of 41 Planck SZ-selected galaxy clusters at from the CHEX-MATE sample, using wide-field Subaru/Suprime-Cam and CFHT/Meg…

astro-ph.CO2026

XMM-Newton observations of ten high-redshift CAMIRA clusters of galaxies

Naomi Ota, Ikuyuki Mitsuishi, Nobuhiro Okabe +9

We present results from XMM-Newton observations of ten high-redshift () galaxy clusters selected from the CAMIRA catalog based on high richness (). These m…