activity
20062019
most citedNarrow-line region gas kinematics of 24,264 optically-selected AGN: the radio connection

303 citations · 945 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.GA2019★ 29 cited

A new sample of southern radio galaxies: Host galaxy masses and star-formation rates

Takalani Marubini, Matt J. Jarvis, Stephen Fine +3

In this study we define a new sample of distant powerful radio galaxies in order to study their host-galaxy properties and provide targets for future observations of HI absorption…

astro-ph.GA2018★ 26 cited

The Stripe 82 1-2 GHz Very Large Array Snapshot Survey: Multiwavelength Counterparts

Matthew Prescott, I. H. Whittam, M. J. Jarvis +6

We have combined spectrosopic and photometric data from the Sloan Digital Sky Survey (SDSS) with GHz radio observations, conducted as part of the Stripe 82 GHz Snapshot…

astro-ph.GA2016★ 29 cited

The 2QDES Pilot : The luminosity and redshift dependence of quasar clustering

Ben Chehade, T. Shanks, J. Findlay +10

We present a new redshift survey, the 2dF Quasar Dark Energy Survey pilot (2QDESp), which consists of quasars from deg of the southern sky, base…

astro-ph.GA2015★ 2 cited

Counting quasar--radio source pairs to derive the millijansky radio luminosity function and clustering strength to z=3.5

S. Fine, T. Shanks, R. Johnston +2

We apply a cross-correlation technique to infer the mJy radio luminosity function (RLF) from the NRAO VLA sky survey (NVSS) to . We measure the over density of r…

astro-ph.CO2013★ 8 cited

Stacked reverberation lags at high redshift

S. Fine, T. Shanks, P. Green +9

Over the past 20years reverberation mapping has proved one of the most successful techniques for studying the local (<1pc) environment of super-massive black holes that drive activ…

astro-ph.CO2013★ 303 cited

Narrow-line region gas kinematics of 24,264 optically-selected AGN: the radio connection

J. R. Mullaney, D. M. Alexander, S. Fine +3

Using a sample of 24264 optically selected AGNs from the SDSS DR7 database, we characterise how the profile of the [OIII] emission line relates to bolometric luminosity (L_Bol), Ed…