Outputs (359)

Top-pair forward-backward asymmetry beyond next-to-leading order. (2011)
Journal Article
Ahrens, V., Ferroglia, A., Neubert, M., Pecjak, B. D., & Yang, L. L. (2011). Top-pair forward-backward asymmetry beyond next-to-leading order. Physical Review D, 84(7), Article 074004. https://doi.org/10.1103/physrevd.84.074004

We make use of recent results in effective theory and higher-order perturbative calculations to improve the theoretical predictions of the QCD contribution to the top-quark pair production forward-backward asymmetry at the Tevatron. In particular, we... Read More about Top-pair forward-backward asymmetry beyond next-to-leading order..

Galaxy and Mass Assembly (GAMA): the GAMA galaxy group catalogue (G$^3$Cv1) (2011)
Journal Article
Robotham, A., Norberg, P., Driver, S., Baldry, I., Bamford, S., Hopkins, A., …Wijesinghe, D. (2011). Galaxy and Mass Assembly (GAMA): the GAMA galaxy group catalogue (G$^3$Cv1). Monthly Notices of the Royal Astronomical Society, 416(4), 2640-2668. https://doi.org/10.1111/j.1365-2966.2011.19217.x

The satellite luminosity functions of galaxies in Sloan Digital Sky Survey (2011)
Journal Article
Guo, Q., Cole, S., Eke, V., & Frenk, C. (2011). The satellite luminosity functions of galaxies in Sloan Digital Sky Survey. Monthly Notices of the Royal Astronomical Society, 417(1), 370-381. https://doi.org/10.1111/j.1365-2966.2011.19270.x

The population of Milky Way satellites in the $\Lambda$ cold dark matter cosmology (2011)
Journal Article
Font, A., Benson, A., Bower, R., Frenk, C., Cooper, A., De Lucia, G., …White, S. (2011). The population of Milky Way satellites in the $\Lambda$ cold dark matter cosmology. Monthly Notices of the Royal Astronomical Society, 417, 1260-1279. https://doi.org/10.1111/j.1365-2966.2011.19339.x

Searching for the trigger of the active galactic nucleus quasi-periodic oscillation: 8 years of RE J1034+396 (2011)
Journal Article
Middleton, M., Uttley, P., & Done, C. (2011). Searching for the trigger of the active galactic nucleus quasi-periodic oscillation: 8 years of RE J1034+396. Monthly Notices of the Royal Astronomical Society, 417, 250-260. https://doi.org/10.1111/j.1365-2966.2011.19185.x

New constraints on the X-ray spectral properties of type 1 active galactic nuclei (2011)
Journal Article
Scott, A., Stewart, G., Mateos, S., Alexander, D., Hutton, S., & Ward, M. (2011). New constraints on the X-ray spectral properties of type 1 active galactic nuclei. Monthly Notices of the Royal Astronomical Society, 417, 992-1012. https://doi.org/10.1111/j.1365-2966.2011.19325.x

A Variable Mid-infrared Synchrotron Break Associated with the Compact Jet in GX 339-4. (2011)
Journal Article
Gandhi, P., Blain, A., Russell, D., Casella, P., Malzac, J., Corbel, S., …Mainzer, A. (2011). A Variable Mid-infrared Synchrotron Break Associated with the Compact Jet in GX 339-4. Astrophysical Journal Letters, 740(1), Article L13. https://doi.org/10.1088/2041-8205/740/1/l13

Evidence for a change in the X-ray radiation mechanism in the hard state of Galactic black holes (2011)
Journal Article
Sobolewska, M., Papadakis, I., Done, C., & Malzac, J. (2011). Evidence for a change in the X-ray radiation mechanism in the hard state of Galactic black holes. Monthly Notices of the Royal Astronomical Society, 417, 280-288. https://doi.org/10.1111/j.1365-2966.2011.19209.x

The Milky Way stellar halo out to 40 kpc: squashed, broken but smooth (2011)
Journal Article
Deason, A., Belokurov, V., & Evans, N. (2011). The Milky Way stellar halo out to 40 kpc: squashed, broken but smooth. Monthly Notices of the Royal Astronomical Society, 416, 2903-2915. https://doi.org/10.1111/j.1365-2966.2011.19237.x

X-ray spectral evolution in the ultraluminous X-ray source M33 X-8 (2011)
Journal Article
Middleton, M., Sutton, A., & Roberts, T. (2011). X-ray spectral evolution in the ultraluminous X-ray source M33 X-8. Monthly Notices of the Royal Astronomical Society, 417(1), 464-471. https://doi.org/10.1111/j.1365-2966.2011.19285.x

The bright ultraluminous X-ray source (ULX), M33 X-8, has been observed several times by XMM–Newton, providing us with a rare opportunity to ‘flux bin’ the spectral data and search for changes in the average X-ray spectrum with flux level. The aggreg... Read More about X-ray spectral evolution in the ultraluminous X-ray source M33 X-8.