papers

Publications (14)

astro-ph2006

The 2dF-SDSS LRG and QSO (2SLAQ) Luminous Red Galaxy Survey

R. Cannon, M. Drinkwater, A. Edge +29

We present a spectroscopic survey of almost 15,000 candidate intermediate-redshift Luminous Red Galaxies (LRGs) brighter than i=19.8, observed with 2dF on the Anglo-Australian Tele…

astro-ph.CO2011

Evolution in the clustering strength of radio galaxies

S. Fine, T. Shanks, N. Nikoloudakis +1

We cross match the NVSS and FIRST surveys with three large photometric catalogues of luminous red galaxies (LRGs) to define radio-loud samples. These have median redshifts 0.35, 0.…

astro-ph2006

The evolution of host mass and black hole mass in QSOs from the 2dF QSO Redshift Survey

S. Fine, S. M. Croom, L. Miller +9

We investigate the relation between the mass of super-massive black holes (Mbh) in QSOs and the mass of the dark matter halos hosting them (Mdh). We measure the widths of broad emi…

astro-ph.CO2011

Measuring BAO and non-Gaussianity via QSO clustering

U. Sawangwit, T. Shanks, S. M. Croom +4

Our goals are (i) to search for BAO and large-scale structure in current QSO survey data and (ii) to use these and simulation/forecast results to assess the science case for a new,…

astro-ph.CO2010

The Civ line width distribution for quasars and its implications for broad-line region dynamics and virial mass estimation

S. Fine, S. M. Croom, J. Bland-Hawthorn +4

We perform an extensive analysis of the Civ line in three large spectroscopic surveys of quasars. Differing approaches for fitting the Civ line can be found in the literature, and…

astro-ph.CO2013

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…

astro-ph.GA2018

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

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

Galaxy And Mass Assembly (GAMA): The 325 MHz Radio Luminosity Function of AGN and Star Forming Galaxies

Matthew Prescott, T. Mauch, M. J. Jarvis +16

Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies underpins our understanding of galaxy evolution over cosmic time. Radio continuum o…

astro-ph.GA2015

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…

astro-ph.CO2012

Composite reverberation mapping

S. Fine, T. Shanks, S. M. Croom +7

Reverberation mapping offers one of the best techniques for studying the inner regions of QSOs. It is based on cross-correlating continuum and emission-line light curves. New time-…

astro-ph.CO2013

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-ph2008

Constraining the quasar population with the broad-line width distribution

S. Fine, S. M. Croom, P. F. Hopkins +12

We measure the width of the MgII line in quasar spectra from the SDSS, 2QZ and 2SLAQ surveys and, by invoking an unnormalised virial mass estimator, relate the scatte…

astro-ph.CO2011

Do all QSOs have the same black hole mass?

T. Shanks, S. M. Croom, S. Fine +2

QSOs from SDSS, 2QZ and 2SLAQ covering an order of magnitude in luminosity at fixed redshift exhibit similar amplitudes of clustering. In addition, QSO clustering evolution at z>0.…