Acknowledgements We gratefully acknowledge Scott Klakamp & Andy Drake (Abgenix Inc.) and David Myszka (University of Utah) for their invaluable contributions in making this collaboration possible. Figure 1. Biacore® A100 offers both rapid kinetic screening and high resolution kinetic characterization of mAbs direct from crude hybridoma samples in one versatile, high-performance system. APPLICAT...

The Mass Spectrometer Telescope (MAST) on SAMPEX is designed to provide high resolution measurements of the isotopic composition of energetic nuclei from He to Ni (Z = 2 to 28) over the energy range from -10 to several hundred MeV/nuc. During large solar flares MAST will measure the isotopic abundances of solar energetic particles to determine directly the composition of the solar corona, while...

The long term archiving of both Landsat imagery and wheat yield mapping datasets sensed by precision agriculture technology has the potential through the development of statistical relationships to predict high resolution estimates of wheat yield over large areas for multiple seasons. Quantifying past yield performance over different growing seasons can inform agricultural management decisions ...

We present a series of high resolution radio and optical observations of the CLASS gravitational lens system B1152+199 obtained with the Multi-Element Radio-Linked Interferometer Network (MERLIN), Very Long Baseline Array (VLBA) and Hubble Space Telescope (HST). Based on the milliarcsecond-scale substructure of the lensed radio components and precise optical astrometry for the lensing galaxy, w...

It updates the biostratigraphic refinement in the Indian Mesozoics with focus on the Triassic in Spiti, Jurassic in Kachchh, and Cretaceous in Kachchh and Cauvery. As an example, the ammonoid stratigraphic zonation in Kachchh basin inclusive of the new Oxfordian zones, as also the origin of the basin are developed at length. Also are touched upon the salient pre-sequence Paleozoic features as b...

where Qi = eii M − ( ai M ) is the contribution made by community ci. It can be seen easily that after moving vertex v from ci to cj , the only terms that will be changed are Qi and Qj . Therefore, the difference between the new modualarity Q and the original modularity can be computed by: Q − Q = Q′i + Q ′ j − Qi − Qj . After the move, the total degrees within community i and j can be given by...

Table A1: At high resolution (∼ 0.3 ˚ A), T98 indices of BSPs obtained with the fitting functions (FFs) method.