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All Outputs (8)

Galaxies Die in Groups: An IRAC Autopsy (2008)
Conference Proceeding
Wilman, D., Pierini, D., Tyler, K., McGee, S., Oemler, A., Morris, S., …Mulchaey, J. (2008). Galaxies Die in Groups: An IRAC Autopsy.

Faint Lyα Emitters, Star-forming Galaxies, and Damped Lyα Systems (2008)
Conference Proceeding
Rauch, M., Haehnelt, M., Bunker, A., Becker, G., Marleau, F., Graham, J., …Theuns, T. (2008). Faint Lyα Emitters, Star-forming Galaxies, and Damped Lyα Systems. In Panoramic Views of Galaxy Formation and Evolution ASP Conference Series, Vol. 399, proceedings of the conference held 11-16 December, 2007, at Shonan Village Center, Hayama, Japan

Science requirements for EAGLE for the E-ELT (2008)
Conference Proceeding
Evans, C., Lehnert, M., Cuby, J., Morris, S., Swinbank, A., Taylor, W., …Paumard, T. (2008). Science requirements for EAGLE for the E-ELT. In Ground-based and Airborne Instrumentation for Astronomy II, Proceedings of the SPIE

EAGLE: an MOAO fed multi-IFU in the NIR on the E-ELT (2008)
Conference Proceeding
Cuby, J., Morris, S., Bryson, I., Lehnert, M., Evans, C., Fusco, T., …Wells, M. (2008). EAGLE: an MOAO fed multi-IFU in the NIR on the E-ELT. In Ground-based and Airborne Instrumentation for Astronomy II. Edited by McLean, Ian S.; Casali, Mark M. Proceedings of the SPIE, Volume 7014

A population of faint extended line emitters and the host galaxies of optically thick QSO absorption systems (2008)
Journal Article
Rauch, M., Haehnelt, M., Bunker, A., Becker, G., Marleau, F., Graham, J., …Theuns, T. (2008). A population of faint extended line emitters and the host galaxies of optically thick QSO absorption systems. Astrophysical Journal, 681(2), 856-880. https://doi.org/10.1086/525846

We have conducted a long-slit search for low surface brightness Lyα emitters at redshift 2.67 < z < 3.75. A 92 hr long exposure with the ESO VLT FORS2 instrument down to a 1 σ surface brightness detection limit of 8 × 10−20 erg cm−2 s−1 arcsec−2 per... Read More about A population of faint extended line emitters and the host galaxies of optically thick QSO absorption systems.