activity
20182026
most citedAstrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects: A Millimetre/Submillimetre Probe of the Warm and Hot Universe

216 citations · 734 across the 38 of their papers we have counts for

collaborators
Showing 2022Show all

8 papers · 1 filter

astro-ph.GA2022★ 18 cited

To see or not to see a galaxy, that is the question

Melanie Kaasinen, Joshiwa van Marrewijk, Gergö Popping +7

Determining when the first galaxies formed remains an outstanding goal of modern observational astronomy. Theory and current stellar population models imply that the first galaxies…

astro-ph.GA2022★ 38 cited

Radio fossils, relics, and haloes in Abell 3266: cluster archaeology with ASKAP-EMU and the ATCA

C. J. Riseley, E. Bonnassieux, T. Vernstrom +21

Abell 3266 is a massive and complex merging galaxy cluster that exhibits significant substructure. We present new, highly sensitive radio continuum observations of Abell 3266 perfo…

astro-ph.GA2022★ 18 cited

High-resolution, High-sensitivity, Low-frequency uGMRT View of Coma Cluster of Galaxies

D. V. Lal, N. Lyskova, C. Zhang +12

We present high-resolution, high-sensitivity upgraded Giant Metrewave Radio Telescope observations of the Coma cluster (A1656) at 250-500 MHz and 550-850 MHz. At 250-500 MHz, 135 s…

astro-ph.GA2022★ 18 cited

The Spiderweb proto-cluster is being magnetized by its central radio jet

Craig S. Anderson, Christopher L. Carilli, Paolo Tozzi +10

We present deep broadband radio polarization observations of the Spiderweb radio galaxy (J1140-2629) in a galaxy proto-cluster at . These yield the most detailed polarimetr…

astro-ph.HE2022★ 3 cited

The strongest cool core in REXCESS: Missing X-ray cavities in RXC J2014.8-2430

Tony Mroczkowski, Megan Donahue, Joshiwa van Marrewijk +8

We present a multiwavelength study of RXC J2014.8-2430, the most extreme cool-core cluster in the Representative Cluster Structure Survey (REXCESS), using X-…

astro-ph.HE2022★ 13 cited

GBT/MUSTANG-2 9" resolution imaging of the SZ effect in MS0735.6+7421: Confirmation of the SZ Cavities through direct imaging

John Orlowski-Scherer, Saianeesh K. Haridas, Luca Di Mascolo +14

Mechanical feedback from active galactic nuclei (AGN) is thought to be the dominant feedback mechanism quenching cooling flows and star formation in galaxy cluster cores. However,…

astro-ph.GA2022★ 48 cited

The 700 ks Chandra Spiderweb Field I: evidence for widespread nuclear activity in the Protocluster

P. Tozzi, L. Pentericci, R. Gilli +21

(Abridged) We present an analysis of the 700 ks Chandra ACIS-S observation of the field around the Spiderweb Galaxy at z=2.156, focusing on the nuclear activity in the associated l…

astro-ph.HE2022★ 12 cited

X-ray Emission and Radio Emission from the Jets and Lobes of the Spiderweb Radio Galaxy

Christopher L. Carilli, Craig S. Anderson, Paolo Tozzi +12

Deep Chandra and VLA imaging reveals a clear correlation between X-ray and radio emission on scales ~kpc in the Spiderweb radio galaxy at z=2.16. The X-ray emission assoc…