31 research outputs found

    Clinical Research - Past, Present & Future

    Get PDF
    Clinical pharmacology/research has a very interesting history. It started in the 40’s of the 20th century through the pioneering work of Harry Gold at Cornell University New York. Clinical research is an integral part of drug development. Drug development can be hastened by a number of new techniques with reduction in cost. In addition reverse pharmacology approaches for drug discovery have come to occupy a special place. 85% of the neutral antagonists act as inverse agonists. Inverse agonists have a distinct effect on receptor regulation as opposed to neutral antagonists.Orphan receptors constitute about 50% of the GPCRs. It is estimated that now there are nearly 175 orphan receptors after 125 having been deorphanised. Targeting these orphan receptors can lead to about the same number of ligands and antagonists thereof. Polymorphism of cytochrome P450 provides the basis for the use of predictive pharmacogenomics to yield drug therapies that are more efficient and safer. It is estimated that such personalized P450 gene-based treatment would be relevant for 10-20% of all drug therapy.Key Words:  Clinical Pharmacology (a facet of clinical research) - Human experiments for safety and efficacy; G-protein coupled receptors (GPCRs) – some orphan receptors ;Strategies for drug discovery – Deorphanisation of orphan receptors, allosteric receptor sites, in-silico drug screenin

    The population of merging compact binaries inferred using gravitational waves through GWTC-3

    Get PDF
    We report on the population properties of 76 compact binary mergers detected with gravitational waves below a false alarm rate of 1 per year through GWTC-3. The catalog contains three classes of binary mergers: BBH, BNS, and NSBH mergers. We infer the BNS merger rate to be between 10 Gpc3yr1\rm{Gpc^{-3} yr^{-1}} and 1700 Gpc3yr1\rm{Gpc^{-3} yr^{-1}} and the NSBH merger rate to be between 7.8 Gpc3yr1\rm{Gpc^{-3}\, yr^{-1}} and 140 Gpc3yr1\rm{Gpc^{-3} yr^{-1}} , assuming a constant rate density versus comoving volume and taking the union of 90% credible intervals for methods used in this work. Accounting for the BBH merger rate to evolve with redshift, we find the BBH merger rate to be between 17.9 Gpc3yr1\rm{Gpc^{-3}\, yr^{-1}} and 44 Gpc3yr1\rm{Gpc^{-3}\, yr^{-1}} at a fiducial redshift (z=0.2). We obtain a broad neutron star mass distribution extending from 1.20.2+0.1M1.2^{+0.1}_{-0.2} M_\odot to 2.00.3+0.3M2.0^{+0.3}_{-0.3} M_\odot. We can confidently identify a rapid decrease in merger rate versus component mass between neutron star-like masses and black-hole-like masses, but there is no evidence that the merger rate increases again before 10 MM_\odot. We also find the BBH mass distribution has localized over- and under-densities relative to a power law distribution. While we continue to find the mass distribution of a binary's more massive component strongly decreases as a function of primary mass, we observe no evidence of a strongly suppressed merger rate above 60M\sim 60 M_\odot. The rate of BBH mergers is observed to increase with redshift at a rate proportional to (1+z)κ(1+z)^{\kappa} with κ=2.91.8+1.7\kappa = 2.9^{+1.7}_{-1.8} for z1z\lesssim 1. Observed black hole spins are small, with half of spin magnitudes below χi0.25\chi_i \simeq 0.25. We observe evidence of negative aligned spins in the population, and an increase in spin magnitude for systems with more unequal mass ratio

    Neoadjuvant treatment of pancreatic adenocarcinoma: a systematic review and meta-analysis of 5520 patients

    Full text link

    Search for gravitational waves associated with gamma-ray bursts detected by Fermi and Swift during the LIGO–Virgo run O3b

    Get PDF
    We search for gravitational-wave signals associated with gamma-ray bursts (GRBs) detected by the Fermi and Swift satellites during the second half of the third observing run of Advanced LIGO and Advanced Virgo (2019 November 1 15:00 UTC–2020 March 27 17:00 UTC). We conduct two independent searches: a generic gravitational-wave transients search to analyze 86 GRBs and an analysis to target binary mergers with at least one neutron star as short GRB progenitors for 17 events. We find no significant evidence for gravitational-wave signals associated with any of these GRBs. A weighted binomial test of the combined results finds no evidence for subthreshold gravitational-wave signals associated with this GRB ensemble either. We use several source types and signal morphologies during the searches, resulting in lower bounds on the estimated distance to each GRB. Finally, we constrain the population of low-luminosity short GRBs using results from the first to the third observing runs of Advanced LIGO and Advanced Virgo. The resulting population is in accordance with the local binary neutron star merger rate

    Levels of circulating endothelial cells and colony forming units are influenced by age and dyslipidaemia

    Get PDF
    Background: The balance between endothelial injury and repair in childhood is poorly understood. We examined this relationship in healthy children, in adults, and in children with familial hypercholesterolemia (FH). Methods: Circulating endothelial cells (CECs) were measured as a marker of vascular injury, with vascular repair assessed by counting colony-forming units (CFUs), also known as endothelial progenitor cells. Results: CEC number increased with age. Children with FH had elevated CECs as compared with healthy children, with similar levels numerically to those found in healthy adults. CFU numbers were higher in healthy children than either healthy adults or children with FH. Endothelium-dependent vascular function, measured by flow-mediated dilatations, was positively associated with CFU number, even after adjustment for confounding risk variables. Conclusion: Levels of CECs increase and CFUs decrease with age. In childhood, before the onset of clinically detectable cardiovascular dysfunction, children with a major risk factor for atherosclerotic disease have levels of these indexes of vascular injury and repair approaching those seen in adults

    Isolation and characterization of mouse bone marrow-derived Lin-/VEGF-R2 + progenitor cells

    Full text link
    Circulating endothelial progenitor cells (EPCs) in the peripheral blood (PB) have physiological roles in the maintenance of the existing vascular beds and rescue of vascular injury. In this study, we have evaluated the properties of Lin-/VEGF-R2+ progenitor cells isolated from the mouse bone marrow (BM) and further studied their distribution and integration in an animal model of laser-induced retinal vascular injury. Lin-/VEGF-R2+ cells were enriched from C57BL/6 mice BM using magnetic cell sorting with hematopoietic lineage (Lin) depletion followed by VEGF-R2 positive selection. Lin-/VEGF-R2+ BM cells were characterized using flow cytometry and immunocytochemistry and further tested for colony formation during culture and tube formation on Matrigel®. Lin-/VEGF-R2+ BM cells possessed typical EPC properties such as forming cobble-stone shaped colonies after 3 to 4 weeks of culture, CD34+ expression, take up of Dil-acLDL and binding to Ulex europaeus agglutinin. However, they did not form tube-like structures on Matrigel®. The progenitor cells retained their phenotype over extended period of culture. After intravitreal transplantation in eyes subjected to the laser-induced retinal vascular injury, some Lin-/VEGF-R2+ cells were able to integrate into the damaged retinal vasculature but the level of cell integration seemed less efficient when compared with previous reports in which EPCs from the human PB were employed. Our results indicate that Lin-/VEGF-R2+ cells isolated from the mouse BM share some similarities to EPCs from the human PB but most of them are at a very early stage of maturation and remain quiescent during culture and after intravitreal transplantation
    corecore