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The LABOCA survey of the extended Chandra Deep Field South : two modes of star formation in active galactic nucleus hosts? (2010)
Journal Article
Lutz, D., Mainieri, V., Rafferty, D., Shao, L., Hasinger, G., Weiß, A., …Xue, Y. (2010). The LABOCA survey of the extended Chandra Deep Field South : two modes of star formation in active galactic nucleus hosts?. Astrophysical Journal, 712(2), 1287-1301. https://doi.org/10.1088/0004-637x/712/2/1287

We study the co-existence of star formation and active galactic nucleus (AGN) activity in Chandra X-ray-selected AGN by analyzing stacked 870 μm submillimeter emission from a deep and wide map of the Extended Chandra Deep Field South (ECDFS), obtaine... Read More about The LABOCA survey of the extended Chandra Deep Field South : two modes of star formation in active galactic nucleus hosts?.

Modulation-free pump-probe spectroscopy of strontium atoms (2010)
Journal Article
Javaux, C., Hughes, I., Lochead, G., Millen, J., & Jones, M. (2010). Modulation-free pump-probe spectroscopy of strontium atoms. The European Physical Journal D, 57(2), 151-154. https://doi.org/10.1140/epjd/e2010-00029-4

We have performed polarization spectroscopy on the 5s21S0 →5s5p1P1 transition of atomic strontium. The signal is generated by saturation effects, rather than optical pumping, as the ground state is non-degenerate. This technique generated a dispersio... Read More about Modulation-free pump-probe spectroscopy of strontium atoms.

The Herschel ATLAS (2010)
Journal Article
Eales, S., Dunne, L., Clements, D., Cooray, A., de Zotti, G., Dye, S., …White, G. (2010). The Herschel ATLAS. Publications of the Astronomical Society of the Pacific, 122(891), 499-515. https://doi.org/10.1086/653086

The Herschel ATLAS is the largest open-time key project that will be carried out on the Herschel Space Observatory. It will survey 570 deg2 of the extragalactic sky, 4 times larger than all the other Herschel extragalactic surveys combined, in five f... Read More about The Herschel ATLAS.

Optical control of Faraday rotation in hot Rb vapor (2010)
Journal Article
Siddons, P., Adams, C., & Hughes, I. (2010). Optical control of Faraday rotation in hot Rb vapor. Physical Review A, 81(4), Article 043838. https://doi.org/10.1103/physreva.81.043838

We demonstrate controlled polarization rotation of an optical field conditional on the presence of a second field. Induced rotations of greater than π/2 rad are seen with a transmission of 95%, corresponding to a ratio of phase shift to absorption of... Read More about Optical control of Faraday rotation in hot Rb vapor.

Mid-infrared spectroscopy of candidate active galactic nuclei-dominated submillimeter galaxies (2010)
Journal Article
Coppin, K., Pope, A., Menéndez-Delmestre, K., Alexander, D., Dunlop, J., Egami, E., …Yun, M. (2010). Mid-infrared spectroscopy of candidate active galactic nuclei-dominated submillimeter galaxies. Astrophysical Journal, 713(1), 503-519. https://doi.org/10.1088/0004-637x/713/1/503

Spitzer spectroscopy has revealed that sime80% of submm galaxies (SMGs) are starburst (SB)-dominated in the mid-infrared. Here we focus on the remaining sime20% that show signs of harboring powerful active galactic nuclei (AGNs). We have obtained Spi... Read More about Mid-infrared spectroscopy of candidate active galactic nuclei-dominated submillimeter galaxies.

Structure formation by fifth force: power spectrum from N-Body simulations (2010)
Journal Article
Zhao, H., Maccio, A., Li, B., Hoekstra, H., & Feix, M. (2010). Structure formation by fifth force: power spectrum from N-Body simulations. Astrophysical Journal Letters, 712(2), L179-L183. https://doi.org/10.1088/2041-8205/712/2/l179

We lay out the framework to numerically study nonlinear structure formation in the context of scalar-field-coupled cold dark matter models (phivCDM models) where the scalar field phiv serves as dynamical dark energy. Adopting parameters for the scala... Read More about Structure formation by fifth force: power spectrum from N-Body simulations.

Large-scale structure and dynamics of the most X-ray luminous galaxy cluster known - RX J1347-1145 (2010)
Journal Article
Lu, T., Gilbank, D., Balogh, M., Milkeraitis, M., Hoekstra, H., van Waerbeke, L., …Bower, R. (2010). Large-scale structure and dynamics of the most X-ray luminous galaxy cluster known - RX J1347-1145. Monthly Notices of the Royal Astronomical Society, 403(4), 1787-1800. https://doi.org/10.1111/j.1365-2966.2010.16245.x

We present photometric, spectroscopic and weak lensing analysis of the large-scale structure and dynamics of the most X-ray luminous galaxy cluster known, RX J1347−1145, at z= 0.451. We spectroscopically confirmed 47 new members with Low Dispersion S... Read More about Large-scale structure and dynamics of the most X-ray luminous galaxy cluster known - RX J1347-1145.

Obscured star formation at z = 0.84 with HiZELS: the relationship between star formation rate and H$\alpha$ or ultraviolet dust extinction (2010)
Journal Article
Garn, T., Sobral, D., Best, P., Geach, J., Smail, I., Cirasuolo, M., …Farrah, D. (2010). Obscured star formation at z = 0.84 with HiZELS: the relationship between star formation rate and H$\alpha$ or ultraviolet dust extinction. Monthly Notices of the Royal Astronomical Society, 402, 2017-2030. https://doi.org/10.1111/j.1365-2966.2009.16042.x