Efficacy and Safety of Modafinil for Improving Daytime Wakefulness in Patients Treated Previously With Psychostimulants

Objectives: To assess the efficacy and safety of modafinil for improving wakefulness in narcolepsy patients treated previously with psychostimulants. Background: Modafinil has become a standard therapy for improving daytime wakefulness in narcolepsy patients and may be a useful therapeutic alternative to psychostimulants used to improve waking function in other medical conditions. Modafinil is chemically dissimilar to and has a pharmacological profile that differs from the psychostimulants. Modafinil has a low abuse potential and is well tolerated. Methods: Patients (N = 151) with narcolepsy who had been unsatisfactorily treated with dextroamphetamine (N = 48), methylphenidate (N = 66), or pemoline (N = 37) were enrolled in this 6-week, open-label, multicenter study. Following a 2-week washout period, patients received modafinil once daily (Week 1, 200 mg; Weeks 2-6, 200 or 400 mg). Efficacy was evaluated at Weeks 1, 2, and 6 using the Epworth Sleepiness Scale and the Clinical Global Impression of Change. Adverse events were monitored throughout the study. Results: Treatment with modafinil improved daytime wakefulness versus baseline regardless of which psychostimulant was taken previously. Mean ESS scores were improved after 1 week of treatment with modafinil. Improvements were maintained throughout the 6 weeks of treatment (all P \u3c 0.001 versus baseline after washout). At Week 6, 79% of all patients were considered to be clinically improved relative to post-washout baseline. The most frequent adverse events were headache, nausea, and insomnia; the majority of adverse events were mild or moderate in nature. Approximately 70% of patients were receiving 400 mg of modafinil once daily at the end of the study. Conclusion: During this 6-week, open-label study, modafinil was an effective and well-tolerated treatment for improving daytime wakefulness in narcolepsy patients previously treated with psychostimulants. (C) 2002 Elsevier Science B.V. All rights reserved

Evolution of genes and genomes on the Drosophila phylogeny

Comparative analysis of multiple genomes in a phylogenetic framework dramatically improves the precision and sensitivity of evolutionary inference, producing more robust results than single-genome analyses can provide. The genomes of 12 Drosophila species, ten of which are presented here for the first time (sechellia, simulans, yakuba, erecta, ananassae, persimilis, willistoni, mojavensis, virilis and grimshawi), illustrate how rates and patterns of sequence divergence across taxa can illuminate evolutionary processes on a genomic scale. These genome sequences augment the formidable genetic tools that have made Drosophila melanogaster a pre-eminent model for animal genetics, and will further catalyse fundamental research on mechanisms of development, cell biology, genetics, disease, neurobiology, behaviour, physiology and evolution. Despite remarkable similarities among these Drosophila species, we identified many putatively non-neutral changes in protein-coding genes, non-coding RNA genes, and cis-regulatory regions. These may prove to underlie differences in the ecology and behaviour of these diverse species

Search for gravitational waves from Scorpius X-1 with a hidden Markov model in O3 LIGO data

Results are presented for a semicoherent search for continuous gravitational waves from the low-mass x-ray binary Scorpius X-1, using a hidden Markov model (HMM) to allow for spin wandering. This search improves on previous HMM-based searches of Laser Interferometer Gravitational-Wave Observatory data by including the orbital period in the search template grid, and by analyzing data from the latest (third) observing run. In the frequency range searched, from 60 to 500 Hz, we find no evidence of gravitational radiation. This is the most sensitive search for Scorpius X-1 using a HMM to date. For the most sensitive subband, starting at 256.06 Hz, we report an upper limit on gravitational wave strain (at 95% confidence) of h 95 % 0 = 6.16 × 10 − 26 , assuming the orbital inclination angle takes its electromagnetically restricted value ι = 4 4 ° . The upper limits on gravitational wave strain reported here are on average a factor of ∼ 3 lower than in the second observing run HMM search. This is the first Scorpius X-1 HMM search with upper limits that reach below the indirect torque-balance limit for certain subbands, assuming ι = 4 4 °