activity
20022019
most citedThe radio/X-ray domain of black hole X-ray binaries at the lowest radio luminosities

149 citations · 1.3k across the 33 of their papers we have counts for

collaborators

33 papers

astro-ph.HE2019★ 9 cited

Sub-Eddington super-massive black hole activity in Fornax early type galaxies

Nathan Lee, Elena Gallo, Edmund Hodges-Kluck +6

We characterize the incidence and intensity of low-level super-massive black hole activity within the Fornax cluster, through X-ray observations of the nuclei of 29 quiescent early…

astro-ph.HE2018★ 33 cited

Investigating the X-ray enhancements of highly radio-loud quasars at z > 4

Shifu Zhu, William N. Brandt, Jianfeng Wu +2

We have investigated the jet-linked \mbox{X-ray} emission from highly radio-loud quasars (HRLQs; ) at high redshift. We studied the X-ray properties of 15 HRLQs at $z>4…

astro-ph.SR2017

Magnetism and activity of planet hosting stars

Jason T. Wright, Brendan P. Miller

The magnetic activity levels of planet host stars may differ from that of stars not known to host planets in several ways. Hot Jupiters may induce activity in their hosts through m…

astro-ph.HE2017★ 18 cited

AGN Activity in Nucleated Galaxies as Measured by Chandra

Adi Foord, Elena Gallo, Edmund Hodges-Kluck +4

Motivated by theoretical expectations that Nuclear Star Clusters (NSCs) in galactic centers may provide a favorable environment for super-massive black holes to form and/or efficie…

astro-ph.GA2016

The role of galactic cold gas in low-level supermassive black hole activity

Erik D. Alfvin, Brendan P. Miller, Martha P. Haynes +5

The nature of the relationship between low-level supermassive black hole (SMBH) activity and galactic cold gas, if any, is currently unclear. Here, we test whether central black ho…

astro-ph.HE2016★ 14 cited

The X-ray Properties of Million Solar Mass Black Holes

Richard M. Plotkin, Elena Gallo, Francesco Haardt +5

We present new Chandra X-ray observations of seven low-mass black holes (~1e6 Msun) accreting at low Eddington ratios between -2.0<log L/Ledd<-1.5. We compare the X-ray properties…