Multiwavelength energy distributions of ultraluminous IRAS galaxies .1. Submillimetre and X-ray observations 由 Rigopoulou, D, Lawrence, A, RowanRobinson, M

An alternative to the cosmological 'concordance model' 由 Blanchard, A, Douspis, M, Rowan-Robinson, M, Sarkar, S

An alternative to the cosmological "concordance model" 由 Blanchard, A, Douspis, M, Rowan-Robinson, M, Sarkar, S

Large-scale galaxy correlations as a test for dark energy 由 Blanchard, A, Douspis, M, Rowan-Robinson, M, Sarkar, S

Sub-millimetre observations of hyperluminous infrared galaxies 由 Farrah, D, Serjeant, S, Efstathiou, A, Rowan-Robinson, M, Verma, A

ISO photometry of hyperluminous infrared galaxies: Implications for the origin of their extreme luminosities 由 Verma, A, Rowan-Robinson, M, McMahon, R, Efstathiou, A

Observations of hyperluminous infrared galaxies with the Infrared Space Observatory: Implications for the origin of their extreme luminosities 由 Verma, A, Rowan-Robinson, M, McMahon, R, Efstathiou, A

HST imaging of hyperluminous infrared galaxies 由 Farrah, D, Verma, A, Oliver, S, Rowan-Robinson, M, McMahon, R

Molecular line CO (2->1) observations of ultraluminous IRAS galaxies 由 Rigopoulou, D, Lawrence, A, White, G, RowanRobinson, M, Church, SE

HST imaging of hyperluminous infrared galaxies 由 Farrah, D, Verma, A, Oliver, S, Rowan-Robinson, M, McMahon, R

Hubble Space Telescope Wide Field Planetary Camera 2 observations of hyperluminous infrared galaxies 由 Farrah, D, Verma, A, Oliver, S, Rowan-Robinson, M, McMahon, R

A spectroscopic study of IRAS F10214+4724 由 Serjeant, S, Rawlings, S, Lacy, M, McMahon, R, Lawrence, A, Rowan-Robinson, M, Mountain, M

The environments of hyperluminous infrared galaxies at 0.44 由 Farrah, D, Geach, J, Fox, M, Serjeant, S, Oliver, S, Verma, A, Kaviani, A, Rowan-Robinson, M

Extreme submillimetre starburst galaxies 由 Rowan-Robinson, M, Wang, L, Farrah, D, Rigopoulou, D, Gruppioni, C, Vaccari, M, Marchetti, L, Clements, D

The star-formation rate density from z = 0-6 由 Rowan-Robinson, M, Oliver, S, Wang, L, Farrah, D, Clements, D, Gruppioni, C, Marchetti, L, Rigopoulou, D, Vaccari, M

Infrared spectroscopy of faint 15 mu m sources in the Hubble Deep Field South: First hints at the properties of the sources of the IR background 由 Franceschini, A, Berta, S, Rigopoulou, D, Aussel, H, Cesarsky, C, Elbaz, D, Genzel, R, Moy, E, Oliver, S, Rowan-Robinson, M, Van der Werf, P

X-ray QSO evolution from a very deep ROSAT survey 由 Jones, L, McHardy, I, Merrifield, MR, Mason, K, Smith, P, Abraham, R, Branduardi-Raymont, G, Newsam, A, Dalton, G, Rowan-Robinson, M, Luppino, G

Meeting of the royal astronomical society: Friday 2007 May 11th at 16h 00m in the Geological Society Lecture Theatre, Burlington House 由 Rowan-Robinson, M, Lintott, C, Fletcher, L, Smith, G, Trotta, R, Barber, G, Hood, A, Stanley, G, Diego, F, Weiss, N, Kollerstrom, N, Murdin, P

The European Large Area ISO Survey - IV. The preliminary 90-mu m luminosity function 由 Serjeant, S, Efstathiou, A, Oliver, S, Surace, C, Heraudeau, P, Linden-Vornle, M, Gruppioni, C, La Franca, F, Rigopoulou, D, Morel, T, Crockett, H, Sumner, T, Rowan-Robinson, M, Graham, M

Very large telescope-ISAAC near-infrared spectroscopy of ISO-selected hubble deep field south galaxies 由 Rigopoulou, D, Franceschini, A, Aussel, H, Genzel, R, van der Werf, P, Cesarsky, C, Dennefeld, M, Oliver, S, Rowan-Robinson, M, Mann, R, Perez-Fournon, I, Rocca-Volmerange, B