8 research outputs found
Effects of red grape, wild grape and black raspberry wines on ground pork during refrigerated storage
The effects of red grape, wild grape and black raspberry wines on the quality of ground pork during a 15 days refrigerated storage period were investigated. The levels of phenolic compounds were the highest in black raspberry wine (P0.05). The addition of 5% and 10% wine influenced the quality of ground pork by decreasing pH, inhibiting the progression of lipid oxidation and the formation of total volatile basic nitrogen (TVB-N), and stabilizing the red colour of the ground pork compared to control samples to which no wine was added. In ground pork, addition of red grape wine led to lower concentrations of thiobarbituric acid reactive substances (TBARS, 0.19–0.39 mg kg−1) and TVB-N values (69.1–119.9 mg kg−1) than wild grape (0.16–0.43 mg kg−1 and 72.0–194.1 mg kg−1, respectively) or black raspberry wine (0.33–0.58 mg kg−1 and 81.7–225.4 mg kg−1, respectively) up to 10 days of storage. Results from the present study suggested that the quality of ground pork was affected by wine type and storage period. These effects could be due to phenolic compounds as well as other chemical components of the wines
Latitudinal Variation in Sedimentary Processes in the Peru-Chile Trench off Central Chile
Dynamics of the α6β4 Integrin in Keratinocytes
The integrin α6β4 has been implicated in two apparently contrasting processes, i.e., the formation of stable adhesions, and cell migration and invasion. To study the dynamic properties of α6β4 in live cells two different β4-chimeras were stably expressed in β4-deficient PA-JEB keratinocytes. One chimera consisted of full-length β4 fused to EGFP at its carboxy terminus (β4-EGFP). In a second chimera the extracellular part of β4 was replaced by EGFP (EGFP-β4), thereby rendering it incapable of associating with α6 and thus of binding to laminin-5. Both chimeras induce the formation of hemidesmosome-like structures, which contain plectin and often also BP180 and BP230. During cell migration and division, the β4-EGFP and EGFP-β4 hemidesmosomes disappear, and a proportion of the β4-EGFP, but not of the EGFP-β4 molecules, become part of retraction fibers, which are occasionally ripped from the cell membrane, thereby leaving “footprints” of the migrating cell. PA-JEB cells expressing β4-EGFP migrate considerably more slowly than those that express EGFP-β4. Studies with a β4-EGFP mutant that is unable to interact with plectin and thus with the cytoskeleton (β4(R1281W)-EGFP) suggest that the stabilization of the interaction between α6β4 and LN-5, rather than the increased adhesion to LN-5, is responsible for the inhibition of migration. Consistent with this, photobleaching and recovery experiments revealed that the interaction of β4 with plectin renders the bond between α6β4 and laminin-5 more stable, i.e., β4-EGFP is less dynamic than β4(R1281W)-EGFP. On the other hand, when α6β4 is bound to laminin-5, the binding dynamics of β4 to plectin are increased, i.e., β4-EGFP is more dynamic than EGFP-β4. We suggest that the stability of the interaction between α6β4 and laminin-5 is influenced by the clustering of α6β4 through the deposition of laminin-5 underneath the cells. This clustering ultimately determines whether α6β4 will inhibit cell migration or not
Stochastic Partial Differential Equations in Neurobiology: Linear and Nonlinear Models for Spiking Neurons
A demonstration of improved constraints on primordial gravitational waves with delensing
International audienceWe present a constraint on the tensor-to-scalar ratio, r, derived from measurements of cosmic microwave background (CMB) polarization B-modes with “delensing,” whereby the uncertainty on r contributed by the sample variance of the gravitational lensing B-modes is reduced by cross-correlating against a lensing B-mode template. This template is constructed by combining an estimate of the polarized CMB with a tracer of the projected large-scale structure. The large-scale-structure tracer used is a map of the cosmic infrared background derived from Planck satellite data, while the polarized CMB map comes from a combination of South Pole Telescope, bicep/Keck, and Planck data. We expand the bicep/Keck likelihood analysis framework to accept a lensing template and apply it to the bicep/Keck dataset collected through 2014 using the same parametric foreground modeling as in the previous analysis. From simulations, we find that the uncertainty on r is reduced by ∼10%, from σ(r)=0.024 to 0.022, which can be compared with a ∼26% reduction obtained when using a perfect lensing template or if there were zero lensing B-modes. Applying the technique to the real data, the constraint on r is improved from r0.05<0.090 to r0.05<0.082 (95% C.L.). This is the first demonstration of improvement in an r constraint through delensing