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An interferometric CO survey of luminous submm galaxies
(2005-05)
In this paper we present results from an IRAM Plateau de Bure millimetre-wave Interferometer (PdBI) survey for CO emission towards radio-detected submillimetre galaxies (SMGs) with known optical and near-infrared spectroscopic ...
New algorithms for MODIS sun-induced chlorophyll fluorescence and a comparison with present data products
(2005-02)
We discuss important sources of variability in sun-induced chlorophyll fluorescence and examine difficulties in deriving fluorescence data products from satellite imagery, with a focus on the MODerate-resolution Imaging ...
The vertical structure of tropical convection and its impact on the budgets of water vapor and ozone
(American Meteorological Society, 2005)
Convective clouds in the Tropics that penetrate the boundary layer inversion preferentially detrain into a shallow outflow layer (2-5 km) or a deep outflow layer (10-17 km). The properties of these layers are diagnosed ...
Rest-frame optical and far-infrared observations of extremely bright Lyman-break galaxy candidates at z ~ 2.5
(2005-09)
We have investigated the rest-frame optical and far-infrared properties of a sample of extremely bright candidate Lyman-break galaxies (LBG) identified in the Sloan Digital Sky Survey. Their high ultraviolet luminosities ...
Maximally fast coarsening algorithms
(2005-11)
We present maximally fast numerical algorithms for conserved coarsening systems that are stable and accurate with a growing natural time step Deltat=At2/3s. We compare the scaling structure obtained from our maximally fast ...
A Redshift Survey of the Submillimeter Galaxy Population
(2005-04)
We have obtained spectroscopic redshifts using the Keck-I telescope for a sample of 73 submillimeter (submm) galaxies for which precise positions are available. The galaxies lie at redshifts out to z=3.6, with a median ...
Optical and Near-Infrared Integral Field Spectroscopy of the SCUBA Galaxy N2-850.4
(2005-05-11)
We present optical and near-infrared integral field spectroscopy of the SCUBA galaxy SMM J163650.43+405734.5 (ELAIS N2 850.4) at z=2.385. We combine Ly-alpha and H-alpha emission line maps and velocity structure with high ...
An upper limit to [C II] emission in a z ~= 5 galaxy
(2005-05-01)
Low-ionization-state far-infrared (FIR) emission lines may be useful diagnostics of star-formation activity in young galaxies, and at high redshift may be detectable from the ground. In practice, however, very little is ...
Field Trip B5: Geology and environmental geochemistry of lode gold deposits in Nova Scotia
(Atlantic Geoscience Society, 2005)
Stable isotopic composition of deep-sea gorgonian corals Primnoa spp.: a new archive of surface processes
(2005)
The deep-sea gorgonian coral Primnoa spp. live in the Atlantic and Pacific Oceans at depths of 65 to 3200 m. They have an arborescent growth form with a skeletal axis composed of annual rings made from calcite and gorgonin. ...