activity
20042022
most citedSpectacular X-ray tails, intracluster star formation and ULXs in A3627

163 citations · 429 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2022★ 18 cited

Multiple shock fronts in RBS 797: the Chandra window on shock heating in galaxy clusters

F. Ubertosi, M. Gitti, F. Brighenti +11

Using 427 ks of Chandra observations, we present a study of shock heating and ICM cooling in the galaxy cluster RBS 797. We discover three nested pairs of weak shocks at roug…

astro-ph.GA2022★ 40 cited

Gas condensation in Brightest Group Galaxies unveiled with MUSE

V. Olivares, P. Salome, S. L. Hamer +18

The origin of the cold gas in central galaxies in groups is still a matter of debate. We present Multi-Unit Spectroscopic Explorer (MUSE) observations of 18 optically selected loca…

astro-ph.GA2015★ 26 cited

The discovery of lensed radio and X-ray sources behind the Frontier Fields cluster MACS J0717.5+3745 with the JVLA and Chandra

R. J. van Weeren, G. A. Ogrean, C. Jones +24

We report on high-resolution JVLA and Chandra observations of the HST Frontier Cluster MACS J0717.5+3745. MACS J0717.5+3745 offers the largest contiguous magnified area of any know…

astro-ph.IM2012★ 131 cited

Wide-Field InfraRed Survey Telescope (WFIRST) Final Report

J. Green, P. Schechter, C. Baltay +51

In December 2010, NASA created a Science Definition Team (SDT) for WFIRST, the Wide Field Infra-Red Survey Telescope, recommended by the Astro 2010 Decadal Survey as the highest pr…

astro-ph.CO2009★ 163 cited

Spectacular X-ray tails, intracluster star formation and ULXs in A3627

M. Sun, M. Donahue, E. Roediger +5

We present the discovery of spectacular double X-ray tails associated with ESO137-001 and a possibly heated X-ray tail associated with ESO137-002, both late-type galaxies in the cl…

astro-ph2004★ 51 cited

The nature of a gravitationally lensed sub-millimetre arc in MS0451.6-0305: two interacting galaxies at z~2.9?

C. Borys, S. C. Chapman, M. Donahue +6

We present a new SCUBA image of the cluster MS0451.6-0305, which exhibits strong, extended sub-mm flux at 850 microns. The most striking feature in the map is an elongated region o…