activity
20062018
most citedThe Assembly of Supermassive Black Holes at High Redshifts

279 citations · 1.5k across the 20 of their papers we have counts for

collaborators

21 papers

astro-ph.GA2018★ 193 cited

Titans of the Early Universe: The Prato Statement on the Origin of the First Supermassive Black Holes

Tyrone E. Woods, Bhaskar Agarwal, Volker Bromm +30

In recent years, the discovery of massive quasars at z~7 has provided a striking challenge to our understanding of the origin and growth of supermassive black holes in the early Un…

astro-ph.GA2017

Population III X-Ray Binaries

Taeho Ryu, Takamitsu L. Tanaka, Rosalba Perna

Understanding of the role of X-rays for driving the thermal evolution of the intergalactic medium (IGM) at high redshifts is one of important questions in astrophysics. High-mass X…

astro-ph.HE2016★ 122 cited

On the likelihood of detecting gravitational waves from Population III compact object binaries

K. Belczynski, T. Ryu, R. Perna +3

We study the contribution of binary black hole (BH-BH) mergers from the first, metal-free stars in the Universe (Pop III) to gravitational wave detection rates. Our study combines…

astro-ph.HE2016★ 30 cited

Flares in Gamma Ray Bursts: Disc Fragmentation and Evolution

Simone Dall'Osso, Rosalba Perna, Takamitsu L. Tanaka +1

Flaring activity following gamma-ray bursts (GRBs), observed in both long and short GRBs, signals a long-term activity of the central engine. However, its production mechanism has…

astro-ph.GA2016★ 43 cited

Intermediate-mass black holes from Population III remnants in the first galactic nuclei

Taeho Ryu, Takamitsu L. Tanaka, Rosalba Perna +1

We report the formation of intermediate-mass black holes (IMBHs) in suites of numerical -body simulations of Population III remnant black holes (BHs) embedded in gas-rich protog…

astro-ph.GA2015★ 31 cited

Formation, disruption and energy output of Population III X-ray binaries

Taeho Ryu, Takamitsu L. Tanaka, Rosalba Perna

The first astrophysical objects shaped the cosmic environment by reionizing and heating the intergalactic medium (IGM). In particular, X-rays are very efficient at heating the IGM…