425 research outputs found

    Does bad company corrupt good morals? Social bonding and academic cheating among French and Chinese teens.

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    A well-known common wisdom asserts that strong social bonds undermine delinquency. However, there is little empirical evidence to substantiate this assertion regarding adolescence academic cheating across cultures. In this study, we adopt social bonding theory and develop a theoretical model involving four social bonds (parental attachment, academic commitment, peer involvement, and moral values) and adolescence self-reported academic cheating behavior and cheating perception. Based on 913 adolescents (average age = 15.88) in France (n = 429) and China (n = 484), we show that parental attachment, academic commitment, and moral values curb academic cheating; counter-intuitively, peer involvement contributes to cheating. We test our theoretical model across culture and gender, separately, using multi-group analyses. For French teens, peer involvement encourages and moral values undermine cheating; for Chinese adolescents, all four social bonds contribute to cheating, similar to the whole sample. For girls, parental attachment deters, but peer involvement enhances cheating. For boys, parental attachment is the only social bond that does not affect cheating. We treat social integration (popularity) as a mediator of the relationship between peer involvement and cheating and ask: Considering popularity, who are likely to cheat? Our answers provide an interesting paradox: Popularity matters, yet popular French girls and unpopular Chinese boys are likely to cheat. Social sharing is a positive pro-social behavior in consumer behavior. We shed new lights on both the bright and dark sides of social bonds on cheating, demonstrate bad company corrupts good morals, differently, across culture and gender, and provide practical implications to social bonding, business ethics, and cheating. Keywords: Social bond, Classroom cheating, Adolescent, Cross-cultural, France, China, Gender, Moderator, Mediator, Sharing, Social Integration, Dishonesty, Massacr

    Abundance ratios of OH/CO and HCO+/CO as probes of the cosmic ray ionization rate in diffuse clouds

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    The cosmic-ray ionization rate (CRIR, ζ2\zeta_2) is one of the key parameters controlling the formation and destruction of various molecules in molecular clouds. However, the current most commonly used CRIR tracers, such as H3+_3^+, OH+^+, and H2_2O+^+, are hard to detect and require the presence of background massive stars for absorption measurements. In this work, we propose an alternative method to infer the CRIR in diffuse clouds using the abundance ratios of OH/CO and HCO+^+/CO. We have analyzed the response of chemical abundances of CO, OH, and HCO+^+ on various environmental parameters of the interstellar medium in diffuse clouds and found that their abundances are proportional to ζ2\zeta_2. Our analytic expressions give an excellent calculation of the abundance of OH for ζ2\zeta_2 \leq1015^{-15} s1^{-1}, which are potentially useful for modelling chemistry in hydrodynamical simulations. The abundances of OH and HCO+^+ were found to monotonically decrease with increasing density, while the CO abundance shows the opposite trend. With high-sensitivity absorption transitions of both CO (1--0) and (2--1) lines from ALMA, we have derived the H2_2 number densities (nH2n_{\rm H_2}) toward 4 line-of-sights (LOSs); assuming a kinetic temperature of Tk=50KT_{\rm k}=50\,{\rm K}, we find a range of (0.14±\pm0.03--1.2±\pm0.1)×\times102^2 cm3^{-3}}. By comparing the observed and modelled HCO+^+/CO ratios, we find that ζ2\zeta_2 in our diffuse gas sample is in the { range of 1.01.0+14.81.0_{-1.0}^{+14.8} ×\times10162.52.4+1.4^{-16}- 2.5_{-2.4}^{+1.4} ×\times1015^{-15} s1^{-1}. This is \sim2 times higher than the average value measured at higher extinction, supporting an attenuation of CRs as suggested by theoretical models.Comment: 22 pages, 9 figures, accepted by Ap

    Dependence of Chemical Abundance on the Cosmic Ray Ionization Rate in IC 348

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    Ions (e.g., H3+_3^+, H2_2O+^+) have been used extensively to quantify the cosmic-ray ionization rate (CRIR) in diffuse sightlines. However, measurements of CRIR in low-to-intermediate density gas environments are rare, especially when background stars are absent. In this work, we combine molecular line observations of CO, OH, CH, and HCO+^+ in the star-forming cloud IC~348, and chemical models to constrain the value of CRIR and study the response of the chemical abundances distribution. The cloud boundary is found to have an AVA_{\rm V} of approximately 4 mag. From the interior to the exterior of the cloud, the observed 13^{13}CO line intensities drop by an order of magnitude. The calculated average abundance of 12^{12}CO (assuming 12^{12}C/13^{13}C = 65) is (1.2±\pm0.9) ×\times104^{-4}, which increases by a factor of 6 from the interior to the outside regions. The average abundance of CH (3.3±\pm0.7 ×\times 108^{-8}) is in good agreement with previous findings in diffuse and translucent clouds (AVA_{\rm V} << 5 mag). However, we did not find a decline in CH abundance in regions of high extinction (AVA_{\rm V}\simeq8 mag) as previously reported in Taurus. By comparing the observed molecular abundances and chemical models, we find a decreasing trend of CRIR as AVA_{\rm V} increases. The inferred CRIR of ζcr\zeta_{cr} = (4.7±\pm1.5) ×\times 1016^{-16} s1^{-1} at low AVA_{\rm V} is consistent with H3+^+_3 measurements toward two nearby massive stars.Comment: 21 pages, 11 figures. Submitted to Ap

    Gene-body hypermethylation of ATM in peripheral blood DNA of bilateral breast cancer patients

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    Bilaterality of breast cancer is an indicator of constitutional cancer susceptibility; however, the molecular causes underlying this predisposition in the majority of cases is not known. We hypothesize that epigenetic misregulation of cancer-related genes could partially account for this predisposition. We have performed methylation microarray analysis of peripheral blood DNA from 14 women with bilateral breast cancer compared with 14 unaffected matched controls throughout 17 candidate breast cancer susceptibility genes including BRCA1, BRCA2, CHEK2, ATM, ESR1, SFN, CDKN2A, TP53, GSTP1, CDH1, CDH13, HIC1, PGR, SFRP1, MLH1, RARB and HSD17B4. We show that the majority of methylation variability is associated with intragenic repetitive elements. Detailed validation of the tiled region around ATM was performed by bisulphite modification and pyrosequencing of the same samples and in a second set of peripheral blood DNA from 190 bilateral breast cancer patients compared with 190 controls. We show significant hypermethylation of one intragenic repetitive element in breast cancer cases compared with controls (P = 0.0017), with the highest quartile of methylation associated with a 3-fold increased risk of breast cancer (OR 3.20, 95% CI 1.78–5.86, P = 0.000083). Increased methylation of this locus is associated with lower steady-state ATM mRNA level and correlates with age of cancer patients but not controls, suggesting a combined age–phenotype-related association. This research demonstrates the potential for gene-body epigenetic misregulation of ATM and other cancer-related genes in peripheral blood DNA that may be useful as a novel marker to estimate breast cancer risk

    Genomic monitoring of SARS-CoV-2 uncovers an Nsp1 deletion variant that modulates type I interferon response

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    The SARS-CoV-2 virus, the causative agent of COVID-19, is undergoing constant mutation. Here, we utilized an integrative approach combining epidemiology, virus genome sequencing, clinical phenotyping, and experimental validation to locate mutations of clinical importance. We identified 35 recurrent variants, some of which are associated with clinical phenotypes related to severity. One variant, containing a deletion in the Nsp1-coding region (D500-532), was found in more than 20% of our sequenced samples and associates with higher RT-PCR cycle thresholds and lower serum IFN-beta levels of infected patients. Deletion variants in this locus were found in 37 countries worldwide, and viruses isolated from clinical samples or engineered by reverse genetics with related deletions in Nsp1 also induce lower IFN-beta responses in infected Calu-3 cells. Taken together, our virologic surveillance characterizes recurrent genetic diversity and identified mutations in Nsp1 of biological and clinical importance, which collectively may aid molecular diagnostics and drug design.Peer reviewe

    The neck-region polymorphism of DC-SIGNR in peri-centenarian from Han Chinese Population

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    <p>Abstract</p> <p>Background</p> <p>DC-SIGNR (also called CD209L) has been extensively studied on its role in host genetic predisposition to viral infection. In particular, variable number tandem repeat (VNTR) of the neck-region of DC-SIGNR is highly polymorphic and the polymorphism has been investigated for genetic predisposition to various infectious diseases, though conflicting results had been reported. As infection is a major cause of human death and a mechanism of natural selection, we hypothesized that VNTR polymorphism of DC-SIGNR might have an effect on human life span.</p> <p>Methods</p> <p>Here we collected 361 peri-centenarian individuals (age ≥94 for female and age ≥90 for male) and 342 geographically matched controls (age 22-53, mean 35.0 ± 12.0) from Han Chinese. The VNTR polymorphism of the neck region was determined by PCR and genotype was called by separating the PCR products in agarose gel.</p> <p>Results</p> <p>A total of 11 genotypes and 5 alleles were found in our population. The genotype distribution, allele frequencies and homozygote proportion did not show a significant difference between peri-centenarian and control group. As gender differences in lifespan are ubiquitously observed throughout the animal kingdom, we then stratified the samples by gender. There was more 6/7 genotypes in female peri-centenarian group than that in female control group, at a marginal level of significance (5.56 vs. 1.28%, p = 0.041). The difference was not significant after correction by Bonferroni method. It suggests a possible differential effect of DC-SIGNR VNTR genotypes between sexes. Further studies are warranted to confirm our preliminary findings and investigate the mechanisms of the underlying functions.</p> <p>Conclusions</p> <p>Our study indicated that there was absence of association between the neck region polymorphism of DC-SIGNR and longevity in Han Chinese population. But the question of whether the DC-SIGNR could affect longevity in a gender-specific pattern remains open.</p

    The Love of Money and Pay Level Satisfaction: Measurement and Functional Equivalence in 29 Geopolitical Entities around the World

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    Demonstrating the equivalence of constructs is a key requirement for cross-cultural empirical research. The major purpose of this paper is to demonstrate how to assess measurement and functional equivalence or invariance using the 9-item, 3-factor Love of Money Scale (LOMS, a second-order factor model) and the 4-item, 1-factor Pay Level Satisfaction Scale (PLSS, a first-order factor model) across 29 samples in six continents (N = 5973). In step 1, we tested the configural, metric and scalar invariance of the LOMS and 17 samples achieved measurement invariance. In step 2, we applied the same procedures to the PLSS and nine samples achieved measurement invariance. Five samples (Brazil, China, South Africa, Spain and the USA) passed the measurement invariance criteria for both measures. In step 3, we found that for these two measures, common method variance was non-significant. In step 4, we tested the functional equivalence between the Love of Money Scale and Pay Level Satisfaction Scale. We achieved functional equivalence for these two scales in all five samples. The results of this study suggest the critical importance of evaluating and establishing measurement equivalence in cross-cultural studies. Suggestions for remedying measurement non-equivalence are offered

    Fine Mapping of the NRG1 Hirschsprung's Disease Locus

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    The primary pathology of Hirschsprung's disease (HSCR, colon aganglionosis) is the absence of ganglia in variable lengths of the hindgut, resulting in functional obstruction. HSCR is attributed to a failure of migration of the enteric ganglion precursors along the developing gut. RET is a key regulator of the development of the enteric nervous system (ENS) and the major HSCR-causing gene. Yet the reduced penetrance of RET DNA HSCR-associated variants together with the phenotypic variability suggest the involvement of additional genes in the disease. Through a genome-wide association study, we uncovered a ∼350 kb HSCR-associated region encompassing part of the neuregulin-1 gene (NRG1). To identify the causal NRG1 variants contributing to HSCR, we genotyped 243 SNPs variants on 343 ethnic Chinese HSCR patients and 359 controls. Genotype analysis coupled with imputation narrowed down the HSCR-associated region to 21 kb, with four of the most associated SNPs (rs10088313, rs10094655, rs4624987, and rs3884552) mapping to the NRG1 promoter. We investigated whether there was correlation between the genotype at the rs10088313 locus and the amount of NRG1 expressed in human gut tissues (40 patients and 21 controls) and found differences in expression as a function of genotype. We also found significant differences in NRG1 expression levels between diseased and control individuals bearing the same rs10088313 risk genotype. This indicates that the effects of NRG1 common variants are likely to depend on other alleles or epigenetic factors present in the patients and would account for the variability in the genetic predisposition to HSCR

    A ring-like accretion structure in M87 connecting its black hole and jet

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    The nearby radio galaxy M87 is a prime target for studying black hole accretion and jet formation^{1,2}. Event Horizon Telescope observations of M87 in 2017, at a wavelength of 1.3 mm, revealed a ring-like structure, which was interpreted as gravitationally lensed emission around a central black hole^3. Here we report images of M87 obtained in 2018, at a wavelength of 3.5 mm, showing that the compact radio core is spatially resolved. High-resolution imaging shows a ring-like structure of 8.4_{-1.1}^{+0.5} Schwarzschild radii in diameter, approximately 50% larger than that seen at 1.3 mm. The outer edge at 3.5 mm is also larger than that at 1.3 mm. This larger and thicker ring indicates a substantial contribution from the accretion flow with absorption effects in addition to the gravitationally lensed ring-like emission. The images show that the edge-brightened jet connects to the accretion flow of the black hole. Close to the black hole, the emission profile of the jet-launching region is wider than the expected profile of a black-hole-driven jet, suggesting the possible presence of a wind associated with the accretion flow.Comment: 50 pages, 18 figures, 3 tables, author's version of the paper published in Natur
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