A study to compare the efficacy of methotrexate alone vs. methotrexate plus pioglitazone in the management of plaque-type psoriasis

Background: Psoriasis is a common skin condition affecting a huge segment of global population. So far, the treatment has been confined to drugs like methotrexate, cyclosporine and oral retinoids which are highly toxic for long term usage and requires a novel drug that is safer.Methods: Cases of plaque type psoriasis are divided into two arms and treated with methotrexate monotherapy in group A and methotrexate plus pioglitazone combination therapy in group B. The outcome of the study is analyzed using PASI score and DLQI scoring systems.Results: Group A and Group B showed significant reduction in the PASI and DLQI scores. Group B was better in terms of efficacy (p<0.05) when compared to Group A. There was no significant difference between the groups in terms of DLQI scoring. Both groups had similar side effect profile.Conclusions: Pioglitazone which acts by sensitizing the cells to insulin poses no risk of hypoglycemia. It is more specific for the treatment of psoriasis as it targets the keratinocytes. Present study suggests a possible role as an adjuvant in the treatment of psoriasis, and could pave way for low dose methotrexate and thereby reducing the potential side effects

A prospective study to evaluate oral iron preparations in antenatal women at a tertiary care hospital

Background: Iron deficiency is the most common cause of anemia in pregnancy worldwide. It can be mild, moderate or severe. Severe anemia can have very serious consequences for mothers and babies. Pregnant women requiring medication represent a challenge to healthcare providers to avoid any teratogenic risk to foetus. The purpose of this study was to provide information about the most effective iron preparations prescribed to pregnant women and to evaluate the haemoglobin status before and after oral iron therapy.Methods: This was a Prospective observational study conducted in the Department of Obstetrics and Gynaecology, Rajarajeswari Medical College and Hospital, between October 2013 and March 2014.This study was conducted by reviewing the antenatal care Outpatient department case papers of 200 pregnant women who were anaemic.Results: Demographic profile, detailed medical history and drug intake in current pregnancy was noted. The prescription pattern was assessed. Of the three common iron preparations prescribed, Ferrous sulphate was the most common preparation. Findings of our study showed that all pregnant anaemic women included in the study were provided with iron and folic acid therapy and the most effective oral iron preparation was Ferrous sulphate.Conclusions: Present study shows that ferrous sulphate is the most common iron preparation prescribed. Ferrous sulphate and ferrous fumarate preparations showed better improvement in Hb levels. Anaemia is common among all pregnant women and therefore it raises the concern about high morbidity and mortality associated with pregnancy outcome. This can be minimized by educating pregnant women about importance of balanced diet and utilization of antenatal facilities even during early pregnancy.

Complete genome sequences of seven Vibrio cholerae phages isolated in China

The complete genome sequences of seven closely related Vibrio cholerae phages isolated from environmental sites in southeastern China are reported here. Phages QH, CJY, H1, H2, H3, J2, and J3 are members of the Podoviridae family and are highly similar to the previously sequenced Vibrio phages VP2, VP5, and phiVC8

Predicting cell types and genetic variations contributing to disease by combining GWAS and epigenetic data

Genome-wide association studies (GWASs) identify single nucleotide polymorphisms (SNPs) that are enriched in individuals suffering from a given disease. Most disease-associated SNPs fall into non-coding regions, so that it is not straightforward to infer phenotype or function; moreover, many SNPs are in tight genetic linkage, so that a SNP identified as associated with a particular disease may not itself be causal, but rather signify the presence of a linked SNP that is functionally relevant to disease pathogenesis. Here, we present an analysis method that takes advantage of the recent rapid accumulation of epigenomics data to address these problems for some SNPs. Using asthma as a prototypic example; we show that non-coding disease-associated SNPs are enriched in genomic regions that function as regulators of transcription, such as enhancers and promoters. Identifying enhancers based on the presence of the histone modification marks such as H3K4me1 in different cell types, we show that the location of enhancers is highly cell-type specific. We use these findings to predict which SNPs are likely to be directly contributing to disease based on their presence in regulatory regions, and in which cell types their effect is expected to be detectable. Moreover, we can also predict which cell types contribute to a disease based on overlap of the disease-associated SNPs with the locations of enhancers present in a given cell type. Finally, we suggest that it will be possible to re-analyze GWAS studies with much higher power by limiting the SNPs considered to those in coding or regulatory regions of cell types relevant to a given disease

All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run

We present the results of a search for short-duration gravitational-wave transients in the data from the second observing run of Advanced LIGO and Advanced Virgo. We search for gravitational-wave transients with a duration of milliseconds to approximately one second in the 32-4096 Hz frequency band with minimal assumptions about the signal properties, thus targeting a wide variety of sources. We also perform a matched-filter search for gravitational-wave transients from cosmic string cusps for which the waveform is well modeled. The unmodeled search detected gravitational waves from several binary black hole mergers which have been identified by previous analyses. No other significant events have been found by either the unmodeled search or the cosmic string search. We thus present the search sensitivities for a variety of signal waveforms and report upper limits on the source rate density as a function of the characteristic frequency of the signal. These upper limits are a factor of 3 lower than the first observing run, with a 50% detection probability for gravitational-wave emissions with energies of ∼10-9 Mc2 at 153 Hz. For the search dedicated to cosmic string cusps we consider several loop distribution models, and present updated constraints from the same search done in the first observing run

Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during Their First and Second Observing Runs

When formed through dynamical interactions, stellar-mass binary black holes (BBHs) may retain eccentric orbits (e &gt; 0.1 at 10 Hz) detectable by ground-based gravitational-wave detectors. Eccentricity can therefore be used to differentiate dynamically formed binaries from isolated BBH mergers. Current template-based gravitational-wave searches do not use waveform models associated with eccentric orbits, rendering the search less efficient for eccentric binary systems. Here we present the results of a search for BBH mergers that inspiral in eccentric orbits using data from the first and second observing runs (O1 and O2) of Advanced LIGO and Advanced Virgo. We carried out the search with the coherent WaveBurst algorithm, which uses minimal assumptions on the signal morphology and does not rely on binary waveform templates. We show that it is sensitive to binary mergers with a detection range that is weakly dependent on eccentricity for all bound systems. Our search did not identify any new binary merger candidates. We interpret these results in light of eccentric binary formation models. We rule out formation channels with rates ⪆100 Gpc-3 yr-1 for e &gt; 0.1, assuming a black hole mass spectrum with a power-law index ≲2

Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network

Gravitational-wave astronomy has been firmly established with the detection of gravitational waves from the merger of ten stellar-mass binary black holes and a neutron star binary. This paper reports on the all-sky search for gravitational waves from intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network. The search uses three independent algorithms: two based on matched filtering of the data with waveform templates of gravitational-wave signals from compact binaries, and a third, model-independent algorithm that employs no signal model for the incoming signal. No intermediate mass black hole binary event is detected in this search. Consequently, we place upper limits on the merger rate density for a family of intermediate mass black hole binaries. In particular, we choose sources with total masses M=m1+m2ϵ[120,800] M and mass ratios q=m2/m1ϵ[0.1,1.0]. For the first time, this calculation is done using numerical relativity waveforms (which include higher modes) as models of the real emitted signal. We place a most stringent upper limit of 0.20 Gpc-3 yr-1 (in comoving units at the 90% confidence level) for equal-mass binaries with individual masses m1,2=100 M and dimensionless spins χ1,2=0.8 aligned with the orbital angular momentum of the binary. This improves by a factor of ∼5 that reported after Advanced LIGO's first observing run

Search for gravitational waves from Scorpius X-1 in the second Advanced LIGO observing run with an improved hidden Markov model

We present results from a semicoherent search for continuous gravitational waves from the low-mass X-ray binary Scorpius X-1, using a hidden Markov model (HMM) to track spin wandering. This search improves on previous HMM-based searches of LIGO data by using an improved frequency domain matched filter, the $\mathcal{J}$-statistic, and by analysing data from Advanced LIGO's second observing run. In the frequency range searched, from $60$ to $650\,\mathrm{Hz}$, we find no evidence of gravitational radiation. At $194.6\,\mathrm{Hz}$, the most sensitive search frequency, we report an upper limit on gravitational wave strain (at 95\% confidence) of $h_0^{95\%} = 3.47 \times 10^{-25}$ when marginalising over source inclination angle. This is the most sensitive search for Scorpius X-1, to date, that is specifically designed to be robust in the presence of spin wandering