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Now showing items 481-490 of 549
A survey of molecular gas in luminous sub-millimetre galaxies
(2012-05-07)
We present the results from a survey for 12CO emission in 40 luminous sub-millimetre galaxies (SMGs), with 850um fluxes of S850 = 4 - 20 mJy, conducted with the Plateau de Bure Interferometer. We detect 12CO emission in ...
Intercomparison of ground-based ozone and NO2 measurements during the MANTRA 2004 campaign
(2007)
No abstract available.
A submillimetre galaxy at z=4.76 in the LABOCA survey of the Extended Chandra Deep Field South
(2009-06-01)
We report on the identification of the highest redshift submm-selected source currently known: LESSJ033229.4-275619. This source was detected in the Large Apex BOlometer CAmera (LABOCA) Extended Chandra Deep Field South ...
A search for the submillimetre counterparts to Lyman break galaxies
(2002-04-04)
We have carried out targetted sub-mm observations as part of a programme to explore the connection between the rest-frame UV and far-IR properties of star-forming galaxies at high redshift, which is currently poorly ...
Infrared measurements in the Arctic using two Atmospheric Emitted Radiance Interferometers
(2012)
No abstract available.
Subcellular Min Oscillations as a Single-Cell Reporter of the Action of Polycations, Protamine, and Gentamicin on Escherichia coli
(2009-09)
No abstract available.
Classical Antiferromagnets on the Kagome Lattice
(1992-04)
No abstract available.
Detection of molecular gas in a distant submillimetre galaxy at z=4.76 with ATCA
(2010-04-22)
We have detected the CO(2-1) transition from the submillimetre galaxy (SMG) LESSJ033229.4-275619 at z=4.755 using the new Compact Array Broadband Backend system on the Australian Telescope Compact Array. These data have ...
Steady-state helices of the actin homolog MreB inside bacteria: dynamics without motors
(2007-09)
Within individual bacteria, we combine force-dependent polymerization dynamics of individual MreB protofilaments with an elastic model of protofilament bundles buckled into helical configurations. We use variational ...