CSF1R inhibitor JNJ-40346527 attenuates microglial proliferation and neurodegeneration in P301S mice

Neuroinflammation and microglial activation are significant processes in Alzheimer's disease pathology. Recent genome-wide association studies have highlighted multiple immune-related genes in association with Alzheimer's disease, and experimental data have demonstrated microglial proliferation as a significant component of the neuropathology. In this study, we tested the efficacy of the selective CSF1R inhibitor JNJ-40346527 (JNJ-527) in the P301S mouse tauopathy model. We first demonstrated the anti-proliferative effects of JNJ-527 on microglia in the ME7 prion model, and its impact on the inflammatory profile, and provided potential CNS biomarkers for clinical investigation with the compound, including pharmacokinetic/pharmacodynamics and efficacy assessment by TSPO autoradiography and CSF proteomics. Then, we showed for the first time that blockade of microglial proliferation and modification of microglial phenotype leads to an attenuation of tau-induced neurodegeneration and results in functional improvement in P301S mice. Overall, this work strongly supports the potential for inhibition of CSF1R as a target for the treatment of Alzheimer's disease and other tau-mediated neurodegenerative diseases

Inflammatory biomarkers in Alzheimer's disease plasma

Introduction: Plasma biomarkers for Alzheimer's disease (AD) diagnosis/stratification are a \u201cHoly Grail\u201d of AD research and intensively sought; however, there are no well-established plasma markers. Methods: A hypothesis-led plasma biomarker search was conducted in the context of international multicenter studies. The discovery phase measured 53 inflammatory proteins in elderly control (CTL; 259), mild cognitive impairment (MCI; 199), and AD (262) subjects from AddNeuroMed. Results: Ten analytes showed significant intergroup differences. Logistic regression identified five (FB, FH, sCR1, MCP-1, eotaxin-1) that, age/APO\u3b54 adjusted, optimally differentiated AD and CTL (AUC: 0.79), and three (sCR1, MCP-1, eotaxin-1) that optimally differentiated AD and MCI (AUC: 0.74). These models replicated in an independent cohort (EMIF; AUC 0.81 and 0.67). Two analytes (FB, FH) plus age predicted MCI progression to AD (AUC: 0.71). Discussion: Plasma markers of inflammation and complement dysregulation support diagnosis and outcome prediction in AD and MCI. Further replication is needed before clinical translation

Erratum: "A Gravitational-wave Measurement of the Hubble Constant Following the Second Observing Run of Advanced LIGO and Virgo" (2021, ApJ, 909, 218)

[no abstract available

GW190814: gravitational waves from the coalescence of a 23 solar mass black hole with a 2.6 solar mass compact object

We report the observation of a compact binary coalescence involving a 22.2–24.3 Me black hole and a compact object with a mass of 2.50–2.67 Me (all measurements quoted at the 90% credible level). The gravitational-wave signal, GW190814, was observed during LIGO’s and Virgo’s third observing run on 2019 August 14 at 21:10:39 UTC and has a signal-to-noise ratio of 25 in the three-detector network. The source was localized to 18.5 deg2 at a distance of - + 241 45 41 Mpc; no electromagnetic counterpart has been confirmed to date. The source has the most unequal mass ratio yet measured with gravitational waves, - + 0.112 0.009 0.008, and its secondary component is either the lightest black hole or the heaviest neutron star ever discovered in a double compact-object system. The dimensionless spin of the primary black hole is tightly constrained to �0.07. Tests of general relativity reveal no measurable deviations from the theory, and its prediction of higher-multipole emission is confirmed at high confidence. We estimate a merger rate density of 1–23 Gpc−3 yr−1 for the new class of binary coalescence sources that GW190814 represents. Astrophysical models predict that binaries with mass ratios similar to this event can form through several channels, but are unlikely to have formed in globular clusters. However, the combination of mass ratio, component masses, and the inferred merger rate for this event challenges all current models of the formation and mass distribution of compact-object binaries

Open data from the third observing run of LIGO, Virgo, KAGRA, and GEO

The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in 2019 April and lasting six months, O3b starting in 2019 November and lasting five months, and O3GK starting in 2020 April and lasting two weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org. The main data set, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages

Pesquisa de alguns microrganismos em saladas com maionese adquiridas em restaurantes, lanchonetes e "rotisseries" Research into microrganisms in mayonnaise salad obtained in restaurants, snack bars and "rotisseries"

Em vinte amostras de saladas com maionese foram efetuadas as contagens de bactérias mesófilas e psicrófilas, Staphylococcus aureus, Bacillus cereus, bolores e leveduras, a determinação do Número Mais Provável (NMP) de bactérias coliforme totais de Escherichia coli e de estreptococos fecais, bem como a pesquisa de salmonelas. A contagem de bactérias mesófilas variou de 2,64 x 10(4) a <FONT FACE=Symbol>&sup3;</FONT>3 x 10(7)/g do produto. Quanto às bactérias psicrófilas, as contagens variaram de < 10 a <FONT FACE=Symbol>&sup3;</FONT> 3 x 10(7)/g. Para S. aureus, as contagens oscilaram de < 10² a 4 x 10(5)/g do alimento, enquanto que para B. cereus os números mínimo e máximo foram < 10² e <FONT FACE=Symbol>&sup3;</FONT> 3 x 10(4)/g, respectivamente. Para bolores e leveduras, as contagens variaram de 7,1 x 10² a 3,7 x 10(6)/g. Com relação ao NMP de coliformes totais e estreptococos fecais, os resultados obtidos mostraram-se compreendidos entre < 0,03 e <FONT FACE=Symbol>&sup3;</FONT> 4,3 x 10(5)/g. Quanto ao NMP de E. coli os números mínimo e máximo obtidos foram respectivamente de < 0,03 e <FONT FACE=Symbol>&sup3;</FONT> 2,4 x 10(4)/g de salada com maionese. Tais constatações indicam a ocorrência de contaminação inclusive por microrganismos de origem fecal. Todas as amostras revelaram-se negativas para bactérias do gênero Salmonella.<br>Twenty samples of mayonnaise salads obtained in restaurants, snack bars and "rotisseries" were analysed for total plate count of mesophilic and psichrophilic bacteria, yeasts and molds, enumeration and isolation of Staphylococcus aureus, Bacillus cereus, the MPN of totally coliform bacteria, Escherichia coli and fecal streptococci as well as for investigation into the occurrence of Salmonella. It was found, in total counts, of coliform and streptococci, that numbers were high in many samples, showing the occurrence of contamination probably during the handling of the food. All the analysed samples were positive to total coliforms as well as to Escherichia coli and fecal streptococci showing that the food had, at some point, suffered pollution of fecal origi n. Staphylococcus aureus and Bacillus cereus in varying proportions were found in different samples. All the samples were showed to be negative for Salmonella