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TLUSTY OSTAR2002
TLUSTY OSTAR2002 Grid: O-type stars, Teff = 27500K - 55000 K (Lanz, T., & Hubeny, I. 2003, ApJS, 146, 417) -
TLUSTY OSTAR2002+BSTAR2006
TLUSTY OSTAR2002+BSTAR2006 Grid, The merged files use the BSTAR2006 models for effective temperatures up to 30,000 K and the OSTAR2002 models for higher temperatures. -
TLUSTY BSTAR2006
TLUSTY BSTAR2006 Grid: Early B-type stars, Teff = 15000K - 30000 K (Lanz, T., Hubeny, I. 2007, ApJS, 169, 83) -
Allard, DUSTY 2000
The DUSTY00 Model grid of theoretical spectra (Lyon group) -
Allard, COND 2000
The COND00 Model grid of theoretical spectra (Lyon group) -
DRIFT-PHOENIX models
Drift-Phoenix is a computer code that simulates the structure of an atmosphere including the formation of clouds. The code is part of the Phoenix-code family. Drift describes... -
Effects of Architecture on Polymer Diffusion
As part of a wider study we are studying the effects of polymer architecture between cyclic and linear polymers. From ATR-FTIR measurements we observe clear differences between... -
Effect of Polymer Architecture on Solution Interactions with CTAB/SDS micelles
Dr Edler¿s group has recently been studying the interactions between polymers and surfactant micelles in solution in order to understand how this drives film formation at the... -
IMAT - neutron tomography using modular phantom objects (tests for samples fr...
This dataset has no description
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Accurate damage localization in concrete using Acoustic Emission, Gutenberg R...
This dataset has no description
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Understanding root architecture and water uptake of water use efficient wheat...
Water scarcity is a serious problem bedevilling crop production in the vast majority of the agricultural ecosystem in the world. This is set to worsen in forthcoming decades as... -
Applying neutron tomography to exceptionally preserved fossils with poor X-ra...
Over the last three decades, methods for visualizing fossils digitally and in 3D have revolutionized the study of past life. X-ray CT scanning, in particular, is widely used,...
