activity
19982022
most citedThe Planck clusters in the LOFAR sky. I. LoTSS-DR2: new detections and sample overview

97 citations · 291 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2022★ 97 cited

The Planck clusters in the LOFAR sky. I. LoTSS-DR2: new detections and sample overview

A. Botteon, T. W. Shimwell, R. Cassano +23

Relativistic electrons and magnetic fields permeate the intra-cluster medium (ICM) and manifest themselves as diffuse sources of synchrotron emission observable at radio wavelength…

astro-ph.CO2021★ 10 cited

Deep Chandra observations of merging galaxy cluster ZwCl 2341+0000

X. Zhang, A. Simionescu, C. Stuardi +9

Knowledge of X-ray shock and radio relic connection in merging galaxy clusters has been greatly extended in terms of both observation and theory over the last decade. ZwCl 2341+000…

astro-ph.HE2021★ 27 cited

A 3.5 Mpc-long radio relic in the galaxy cluster ClG 0217+70

D. N. Hoang, X. Zhang, C. Stuardi +14

Mega-parsec scale radio sources in the form of halos and relics are often detected in dynamically disturbed galaxy clusters. Although they are associated with merger-induced turbul…

astro-ph.HE2020★ 9 cited

ClG 0217+70: A massive merging galaxy cluster with a large radio halo and relics

X. Zhang, A. Simionescu, J. S. Kaastra +7

We present an analysis of archival Chandra data of the merging galaxy cluster ClG 0217+70. The Fe XXV He X-ray emission line is clearly visible in the 25 ks observation, allowin…

astro-ph.HE2020★ 11 cited

X-ray study of the merging galaxy cluster Abell 3411-3412 with XMM-Newton and Suzaku

X. Zhang, A. Simionescu, H. Akamatsu +3

Context: Chandra observations of the Abell 3411-3412 merging system have revealed an outbound bullet-like sub-cluster in the northern part and many surface brightness (SB) edges at…

astro-ph.HE2013★ 5 cited

Variability and spectral variation of 3C 66A

Shao Ming Hu, Jianghua Wu, H. Y. Guo +3

3C 66A was monitored by the BATC(Beijing-Arizona-Taipei-Connecticut) telescope from 2005 to 2008,1994 observations were obtained on 89 nights. Detailed research and analysis was pe…