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 J-statistic, and by analyzing data from Advanced LIGO's second observing run. In the frequency range searched, from 60 to 650 Hz, we find no evidence of gravitational radiation. At 194.6 Hz, the most sensitive search frequency, we report an upper limit on gravitational wave strain (at 95% confidence) of h095%=3.47×10-25 when marginalizing 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. © 2019 American Physical Society

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

Internalized stigma in pediatric psoriasis: A comparative multicenter study

Background: Internalized stigma, adoption of negative attitudes and stereotypes of the society regarding persons' illness, has not been studied previously in pediatric psoriasis patients. Objective: We aimed to investigate the internalized stigma in pediatric psoriasis patients and to determine differences according to factors affecting internalized stigma compared to adult psoriasis patients. Methods: This multicenter, cross-sectional, comparative study included 125 pediatric (55 female, 70 male; mean age±standard deviation [SD], 14.59±2.87 years) and 1,235 adult psoriasis patients (577 female, 658 male; mean age±SD, 43.3±13.7 years). Psoriasis Internalized Stigma Scale (PISS), Dermatology Life Quality Index (DLQI), Perceived Health Status (PHS), and the General Health Questionnaire (GHQ)-12 were the scales used in the study. Results: The mean PISS was 58.48±14.9 in pediatric group. When PISS subscales of groups were compared, the pediatric group had significantly higher stigma resistance (p=0.01) whereas adult group had higher scores of alienation (p=0.01) and stereotype endorsement (p=0.04). There was a strong correlation between mean values of PISS and DLQI (r=0.423, p=0.001). High internalized stigma scores had no relation to either the severity or localization of disease in pediatric group. However, poor PHS (p=0.007) and low-income levels (p=0.03) in both groups, and body mass index (r=0.181, p=0.04) in the pediatric group were related to high PISS scores. Conclusion: Internalized stigma in pediatric patients is as high as adults and is related to poor quality of life, general health, and psychological illnesses. Unlike adults, internalized stigma was mainly determined by psoriasis per se, rather than disease severity or involvement of visible body parts, genitalia or folds. Copyright © The Korean Dermatological Association and The Korean Society for Investigative Dermatology

Estudo do crescimento, desempenho, rendimento de carcaça e qualidade de carne de três linhagens de frango de corte Growth, performance, carcass yield and meat quality of three broiler chickens strains

O objetivo nesta pesquisa foi avaliar o potencial de crescimento, desempenho zootécnico e as características de rendimento da carcaça, das partes e dos órgãos e a qualidade da carne de três linhagens de frango de corte: Cobb (CB), Paraíso Pedrês (PP) e ISA Label (IL). O delineamento foi inteiramente casualizado, com cinco repetições de 29 aves por tratamento. Semanalmente, com os dados obtidos para peso corporal médio, foi descrito o crescimento das aves, utilizando-se a equação de Gompertz e, com sua derivada, foi obtida a taxa de crescimento das aves. Três aves de cada repetição foram selecionadas e abatidas para análises do rendimento da carcaça, das partes e dos órgãos. As características físico-químicas da carne foram avaliadas utilizando-se o peito de duas destas aves. As aves CB apresentaram maior potencial de crescimento e, entre as caipiras o maior potencial foi observado para PP. Quanto ao desempenho, observou-se que a linhagem CB apresentou maior ganho de peso e consumo de ração, seguida pelas aves PP e IL. Maiores rendimentos de carcaça, de peito, sobrecoxa, fígado, intestinos e proventrículo foram obtidos com as aves CB em relação às caipiras, que não diferiram entre si. As aves CB apresentaram carne de peito com maior pH e maior capacidade de retenção de água que as de linhagens caipiras, que apresentaram carne de peito menos macia e com maior intensidade da cor vermelha. Maior potencial de crescimento e maiores rendimentos de pés, coxa, coxa+sobrecoxa e de coração foram verificados nos machos, enquanto, nas fêmeas, maiores rendimentos de peito, porcentagem de gordura abdominal, fígado, moela e proventrículo. As aves CB em relação às caipiras possuíram maior potencial de crescimento e maior rendimento de partes nobres, mas as caipiras apresentaram atributos diferenciados que justificam sua criação.<br>This is study aimed to compare growth performance, meat quality, and carcass yield of three broiler chicken strains: Cobb, Paraiso Pedrês and ISA Label. The experiment was analyzed according to a randomized design, with five replicates of 29 birds per treatment. Weight gain, feed intake, and feed conversion were evaluated weekly. Adjustments performed according to Gompertz model to describe the birds growth were based on mean weight gain. The birds growth rate was obtained by the Gompertz derivative model. When the males of each strain reached body weight of 2.5 kg, three broilers of replicate were slaughtered for carcass analyses. Samples of breast samples of two birds were taken for physical-chemical characteristics analyses. Cobb birds had higher weight gain and feed intake, followed by Paraíso Pedrês and ISA Label. Cobb birds exhibited higher values of growth potential, according to Gompertz equation. Cobb birds showed higher values of carcass yield, breast, drumstick, liver, intestines, and proventricule than the other strains, that did not differ between them. Cobb birds presented higher values of pH and water retention capacity of breast meat. Paraíso Pedrês and ISA Label exhibited stronger red color intensity. Sex did not influence meat quality but influenced feet, drumisticks + upper drumstick, and heart, that were higher in males. Females exhibited higher values of breast, abdominal fat, liver, gizzard, and proventricule yield. Therefore, Cobb strain showed greater capacity to reach higher growth rates and meat quality, and Paraíso Pedrês and ISA Label birds exhibited colors that satisfy consumers demand

GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M o

On 2019 April 25, the LIGO Livingston detector observed a compact binary coalescence with signal-to-noise ratio 12.9. The Virgo detector was also taking data that did not contribute to detection due to a low signal-to-noise ratio, but were used for subsequent parameter estimation. The 90% credible intervals for the component masses range from to if we restrict the dimensionless component spin magnitudes to be smaller than 0.05). These mass parameters are consistent with the individual binary components being neutron stars. However, both the source-frame chirp mass and the total mass of this system are significantly larger than those of any other known binary neutron star (BNS) system. The possibility that one or both binary components of the system are black holes cannot be ruled out from gravitational-wave data. We discuss possible origins of the system based on its inconsistency with the known Galactic BNS population. Under the assumption that the signal was produced by a BNS coalescence, the local rate of neutron star mergers is updated to 250-2810. © 2020. The Author(s). Published by the American Astronomical Society.

Model comparison from LIGO-Virgo data on GW170817's binary components and consequences for the merger remnant

GW170817 is the very first observation of gravitational waves originating from the coalescence of two compact objects in the mass range of neutron stars, accompanied by electromagnetic counterparts, and offers an opportunity to directly probe the internal structure of neutron stars. We perform Bayesian model selection on a wide range of theoretical predictions for the neutron star equation of state. For the binary neutron star hypothesis, we find that we cannot rule out the majority of theoretical models considered. In addition, the gravitational-wave data alone does not rule out the possibility that one or both objects were low-mass black holes. We discuss the possible outcomes in the case of a binary neutron star merger, finding that all scenarios from prompt collapse to long-lived or even stable remnants are possible. For long-lived remnants, we place an upper limit of 1.9 kHz on the rotation rate. If a black hole was formed any time after merger and the coalescing stars were slowly rotating, then the maximum baryonic mass of non-rotating neutron stars is at most 3.05M⊙, and three equations of state considered here can be ruled out. We obtain a tighter limit of 2.67M⊙ for the case that the merger results in a hypermassive neutron star. © 2020 IOP Publishing Ltd

A guide to LIGO–Virgo detector noise and extraction of transient gravitational-wave signals

The LIGO Scientific Collaboration and the Virgo Collaboration have cataloged eleven confidently detected gravitational-wave events during the first two observing runs of the advanced detector era. All eleven events were consistent with being from well-modeled mergers between compact stellar-mass objects: black holes or neutron stars. The data around the time of each of these events have been made publicly available through the gravitational-wave open science center. The entirety of the gravitational-wave strain data from the first and second observing runs have also now been made publicly available. There is considerable interest among the broad scientific community in understanding the data and methods used in the analyses. In this paper, we provide an overview of the detector noise properties and the data analysis techniques used to detect gravitational-wave signals and infer the source properties. We describe some of the checks that are performed to validate the analyses and results from the observations of gravitational-wave events. We also address concerns that have been raised about various properties of LIGO–Virgo detector noise and the correctness of our analyses as applied to the resulting data