Hirofumi Noda

1 ta ish

Astronomical Institute, Tohoku University, Miyagi 980-8578, Japan

1. XRISM Constraints on Unidentified X-Ray Emission Lines, Including the 3.5 keV Line, in the Stacked Spectrum of 10 Galaxy Clusters

   M. Audard, Hisamitsu Awaki, Ralf Ballhausen +97

   MaqolaGalaxies: Formation, Evolution, PhenomenaThe Astrophysical Journal Letters20250 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.002537