Search Results - Stu Hart*

A new method for classifying galaxy SEDs from multiwavelength photometry by Wild, Vivienne, Almaini, Omar, Cirasuolo, Michele, Dunlop, Jim, McLure, Ross, Bowler, Rebecca, Ferreira, Joao, Bradshaw, Emma, Chuter, Robert, Hartley, Will

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Why z > 1 radio-loud galaxies are commonly located in protoclusters by Hatch, Nina A., Wylezalek, D., Kurk, J.D., Stern, D., De Breuck, C., Jarvis, M.J., Galametz, A., Gonzalez, A.H., Hartley, W.G., Mortlock, A., Seymour, N., Stevens, J.A.

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Why z > 1 radio-loud galaxies are commonly located in protoclusters by Hatch, N., Wylezalek, D., Kurk, J., Stern, D., Breuck, C.D., Jarvis., M., Galametz, A., Gonzalez, A., Hartley, W., Mortlock, A., Seymour, Nick, Stevens, J.

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Detailed afterglow modelling and host galaxy properties of the dark GRB 111215A by van der Horst, A., Levan, A., Pooley, G., Wiersema, K., Kruhler, T., Perley, D., Starling, R., Curran, Peter, Tanvir, N., Wijers, R., Strom, R., Kouveliotou, C., Hartoog, O., Xu, D., Fynbo, J., Jakobsson, P.

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