activity
19952009
most citedSupermassive black hole formation during the assembly of pre-galactic discs

490 citations · 5.3k across the 84 of their papers we have counts for

collaborators
Showing 2006Show all

15 papers · 1 filter

astro-ph200632 cited

The Optical and Near-Infrared Properties of 2837 Quasars in the UKIRT Infrared Deep Sky Survey (UKIDSS)

Kuenley Chiu, Gordon T. Richards, Paul C. Hewett +1

The UKIRT Infrared Deep Sky Survey (UKIDSS) is the first of a new generation of hemispheric imaging projects to extend the work of the Two Micron All Sky Survey (2MASS) by reaching…

astro-ph200636 cited

The role of the energy equation in the fragmentation of protostellar discs during stellar encounters

G. Lodato, F. Meru, C. Clarke +1

In this paper, we use high-resolution smoothed particle hydrodynamics (SPH) simulations to investigate the response of a marginally stable self-gravitating protostellar disc to a c…

astro-ph2006103 cited

New brown dwarfs in Upper Sco using UKIDSS Galactic Cluster Survey science verification data

N. Lodieu, N. C. Hambly, R. F. Jameson +3

We present first results from a deep (J = 18.7), wide-field (6.5 square degrees) infrared (ZYJHK) survey in the Upper Sco association conducted within the science verification phas…

astro-ph2006201 cited

Protoclusters associated with z > 2 radio galaxies. I. Characteristics of high redshift protoclusters

B. P. Venemans, H. J. A. Rottgering, G. K. Miley +8

[Abridged] We present the results of a large program conducted with the Very Large Telescope and Keck telescope to search for forming clusters of galaxies near powerful radio galax…

astro-ph200610 cited

Probing the growth of supermassive black holes at z>6 with LOFAR

Kirsty J. Rhook, Martin G. Haehnelt

HII regions surrounding supermassive black holes (BHs) in an otherwise still neutral intergalactic medium (IGM) are likely to be the most easily detectable sources by future 21cm e…

astro-ph200639 cited

Using Radio Bubbles to Constrain the Matter Content of AGN Jets

R. J. H. Dunn, A. C. Fabian, A. Celotti

We revisit a method to obtain upper limits on the jet matter content combining synchrotron self-absorption constraints and the large scale bubble energy. We use both X-ray observat…