Showing 1–20 of 35 results
/ Date/ Name
Jan 14, 2025PSZ2 G181.06+48.47 II: radio analysis of a low-mass cluster with exceptionally-distant radio relicsJan 3, 2025Revisiting the Group-Dominant Elliptical NGC 5044 in the Radio Band: Continuum Emission and Detection of HI AbsorptionApr 22, 2020Discovering the most elusive radio relic in the sky: Diffuse Shock Acceleration caught in the act?Aug 7, 2020Spectro-polarimetric observations of the CIZA J2242.8+5301 northern radio relic: no evidence of high-frequency steepeningOct 22, 2021Radio relics radio emission from multi-shock scenarioAug 16, 2021Spectral analysis of spatially-resolved 3C295 (sub-arcsecond resolution) with the International LOFAR TelescopeMay 11, 2023A morphological analysis of the substructures in radio relicsFeb 7, 2024Understanding the Nature of the Ultra-Steep Spectrum Diffuse Radio Source in the Galaxy Cluster Abell 272May 22, 2024A hot core in the group-dominant elliptical galaxy NGC 777Jan 10, 2022On the Polarisation of Radio RelicsNov 3, 2021VLA Radio Study of a Sample of Nearby X-ray and Optically Bright Early-Type GalaxiesDec 4, 2012Dependence of Fanaroff--Riley break of radio galaxies on luminosity and redshiftOct 1, 2025Multiphase gas offsets in the atmospheres of central galaxies and their consequences for SMBH activation I. The hot and warm ionized gas phasesJan 15, 2025PSZ2 G181.06+48.47 III: weak-lensing analysis and merging scenario reconstruction of a low-mass cluster with exceptionally-distant radio relicsNov 1, 2023Weak-Lensing Analysis of the Complex Cluster Merger Abell 746 with Subaru/Hyper Suprime-CamOct 31, 2025The Advanced X-ray Imaging Satellite (AXIS) Community Science BookNov 16, 2021Magnetogenesis and the Cosmic Web: a joint challenge for radio observations and numerical simulationsJun 15, 2021Exploring the spectral properties of radio relics I: Integrated spectral index and Mach numberSep 9, 2024Probing the high frequency variability of NGC 5044: the key to AGN feedbackMay 15, 2014Fanaroff-Riley dichotomy of radio galaxies and the Malmquist bias