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- C1-esterase inhibitor protein (1)
- HAEGARDA (1)
- Hereditary angioedema (1)
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Background: For the prevention of attacks of hereditary angioedema (HAE), the efficacy and safety of subcutaneous human C1-esterase inhibitor (C1-INH[SC]; HAEGARDA®, CSL Behring) was established in the 16-week COMPACT trial.
Objective: To assess the long-term safety, occurrence of angioedema attacks, and use of rescue medication with C1-INH(SC).
Methods: Open-label, randomised, parallel-arm extension of COMPACT across 11 countries. Patients with frequent angioedema attacks, either study treatment-naïve or who had completed the COMPACT trial, were randomly assigned (1:1) to 40 IU/kg or 60 IU/kg C1-INH(SC) twice per week, with conditional up-titration to optimise prophylaxis. ClinicalTrials.gov registration: NCT02316353.
Results: 126 patients with a monthly attack rate of 4.3 in 3 months prior to entry in the COMPACT program were enrolled and treated for a mean of 1·5 years; 44 patients (34·9%) had >2 years exposure. Median steady-state C1-INH functional activity increased to a maximum of 73.0% with 60 IU/kg. Incidence of adverse events was low and similar in both dose groups (11·3 and 8·5 events per patient-year for 40 IU/kg and 60 IU/kg, respectively). For 40 IU/kg and 60 IU/kg, median annualised attack rates were 1·3 and 1·0, respectively and median rescue medication use was 0.2 and 0.0 times per year, respectively. Of 23 patients receiving 60 IU/kg for >2 years, 19 (83%) were attack-free during months 25–30 of treatment.
Conclusion: In patients with frequent HAE attacks, long-term replacement therapy with C1-INH(SC) is safe and exhibits a substantial and sustained prophylactic effect, with the vast majority of patients becoming free from debilitating disease symptoms.
The idea of slow-neutron capture nucleosynthesis formulated in 1957 triggered a tremendous experimental effort in different laboratories worldwide to measure the relevant nuclear physics input quantities, namely (n,γ) cross sections over the stellar temperature range (from few eV up to several hundred keV) for most of the isotopes involved from Fe up to Bi. A brief historical review focused on total energy detectors will be presented to illustrate how, advances in instrumentation have led, over the years, to the assessment and discovery of many new aspects of s-process nucleosynthesis and to the progressive refinement of theoretical models of stellar evolution. A summary will be presented on current efforts to develop new detection concepts, such as the Total-Energy Detector with γ-ray imaging capability (i-TED). The latter is based on the simultaneous combination of Compton imaging with neutron time-of-flight (TOF) techniques, in order to achieve a superior level of sensitivity and selectivity in the measurement of stellar neutron capture rates.