110 research outputs found

    Exploratory Study of Predicted Indirectly ReCognizable HLA Epitopes in Mismatched Hematopoietic Cell Transplantations

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    HLA-mismatches in hematopoietic stem-cell transplantation are associated with an impaired overall survival (OS). The aim of this study is to explore whether the Predicted Indirectly ReCognizable HLA-Epitopes (PIRCHE) algorithm can be used to identify HLA-mismatches that are related to an impaired transplant outcome. PIRCHE are computationally predicted peptides derived from the patient’s mismatched-HLA molecules that can be presented by donor-patient shared HLA. We retrospectively scored PIRCHE numbers either presented on HLA class-I (PIRCHE-I) or class-II (PIRCHE-II) for a Dutch multicenter cohort of 103 patients who received a single HLA-mismatched (9/10) unrelated donor transplant in an early phase of their disease. These patients were divided into low and high PIRCHE-I and PIRCHE-II groups, based on their PIRCHE scores, and compared using multivariate statistical analysis methods. The high PIRCHE-II group had a significantly impaired OS compared to the low PIRCHE-II group and the 10/10 reference group (HR: 1.86, 95%-CI: 1.02–3.40; and HR: 2.65, 95%-CI: 1.53–4.60, respectively). Overall, PIRCHE-II seem to have a more prominent effect on OS than PIRCHE-I. This impaired OS is probably due to an increased risk for severe acute graft-vs.-host disease. These data suggest that high PIRCHE-II scores may be used to identify non-permissible HLA mismatches within single HLA-mismatched hematopoietic stem-cell transplantations

    Design concept for composite members subjected to impact and blast loads

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    Erratum: "Orbital Gyrocompassing Heading Reference"

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    Flutter of infinitely long plates and shells. I - Plate.

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    New Modelling Of

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    d the same chemical composition but we have no indication neither on their age, t, nor on their helium content, Y . In models using the mixinglength theory (Bohm-Vitense, 1958), the convection parameters are also unknown. These quantities can nevertheless be derived through a calibration of the system. The calibrations have been performed for different fixed Z-values and for a fixed mass for each star (Fernandes & Neuforge, 1995). The mixinglength parameters ff A and ff B may vary independently. Moreover, the chemical composition of the calibrated models must lead to [Z=X] values compatible with the observations. To calculate [Z=X], we have used (Z=X) fi =0.0245 (Grevesse & Noels, 1993). The calibrations were performed with the Li`ege stellar evolution code originally developed by Henyey et al. (1964). The Debye-Huckel corrections (
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