| Selection of highly obscured quasars by mid-infrared SED fitting |
| Bonfield, Rawlings et al., 2009, MNRAS, submitted |
| Modelling the orientation of accretion disks in quasars from Halpha emission |
| Down,Rawlings, Sivia & Baker 2009, MNRAS, submitted (MN-08-2251-MJ), moderate revision requested (resubmitted) |
| The discovery of a typical radio galaxy at z=4.88 |
| Jarvis, Teimourian, Simpson, Smith, Rawlings & Bonfield, 2009, MNRAS, submitted |
| Compactness of Cold Gas in High-redshift Galaxies |
| Obreschkow & Rawlings, 2009, ApJL, submitted |
| A Heuristic Prediction of the Cosmic Evolution of the CO-Luminosity Functions |
| Obreschkow, Heywood, Kloeckner & Rawlings, 2009, ApJ, submitted |
| A Virtual Sky with Extragalactic HI- and CO-line for the SKA and ALMA |
| Obreschkow, Heywood, Kloeckner & Rawlings, 2009, ApJ, submitted |
| The TEXOX-1000 redshift survey of radio sources I": the TOOT00 region |
| Vardoulaki, Rawlings et al., 2008, MNRAS, submitted, MN-09-0374-MJ |
| Cosmology with the SKA |
| Blake C.A., Abdalla F.B., Bridle S.L., Rawlings S., |
| Using radio galaxies to find super-structures |
| Brand K., Rawlings S., Hill, G.J., Lacy M. |
| High-redshift clusters from NVSS: the TexOx Cluster (TOC) survey |
| Croft S., Rawlings S., Hill G.J. |
| The Receding Torus Model - evidence from emission-line luminosities and the quasar fraction |
| Grimes J.A., Rawlings S., Willott C.J. |
| The TOOT survey: status and early results |
| Hill G.J., Rawlings S. |
| High-redshift radio galaxies: at the crossroads |
| Rawlings S. |
| Simple applications of Bayesian methods |
| Sivia D. & Rawlings S., |
| Radio galaxy host properties spanning three dex in radio luminosity |
| Willott C.J., McLure R.J., Jarvis M.J., Rawlings S., Hill G.J., Mitchell E., Dunlop J.S |