Abstract Background and Aims Continuing medical education (CME) aims at modeling best practice in promoting positive behavior. We hypothesized that participation the case-based “Challenging Cases of Glomerulonephritis: How Would You Diagnose Manage These Patients?” would lead to improved knowledge competence nephrologists diagnosis management glomerulonephritis. Method The online CME activity c...

Objective: The aim of this study was to design and optimize lipid based beads for multiunit floating drug delivery ramipril.
 Methods: prepared by melt-solidification method. In the investigation 32 full factorial used investigate joint influence two formulation variable amount Gelucire (X1) Tween 20 (X2) as independent percentage release in 1 (Y1), 6 (Y2), 12 h (Y3) dependent variable. 43...

We assess the cosmological variability of the fine-structure constant α from the analysis of an ensemble of Fe  λ1608, λ2344, λ2374, λ2383, λ2587, and λ2600 absorption lines at the redshift z = 1.15 toward the QSO HE 0515–4414 by means of the standard many-multiplet (MM) technique and its revision based on linear regression (RMM). This is the first time the MM technique is applied to exceptio...

International Journal of Pharma Sciences and Scientific Research A quantitative in vitro determination of relative phototoxic potential of quinolone antibiotics Reaserch Article Open Access *Corresponding Author Byungse Suh, Section of Infectious Diseases Lewis Katz School of Medicine Temple University, 3401 N. Broad Street, Philadelphia, Pennsylvania 19140 Tel. 215-707-3603; Fax 215-707-4414, ...

We report on detailed Monte Carlo inversion analysis of five Ovi systems from the spectrum of the bright quasar HE 0515–4414 (zem = 1.71). The associated system at zabs = 1.697 with the neutral hydrogen column density N(H i) = 4.4×10 cm shows pronounced absorption from highly ionized transitions of C iii, C iv, Nv, Ovi, Si iv, and probably Svi. We found that only a power law type ionizing spect...

A new molecular hydrogen cloud is found in the sub-damped Lyα absorber [logN(H i) = 19.88± 0.05] at the redshift zabs = 1.15 toward the bright quasar HE 0515–4414 (zem = 1.71). More than 30 absorption features in the Lyman band system of H2 are identified in the UV spectrum of this quasar obtained with the Space Telescope Imaging Spectrograph (STIS) aboard the Hubble Space Telescope. The H2-bea...