Miracle-dz/UniFAR-FTUs huggingface dataset:
Psychological Interventions for Patients with Coronary Heart Disease and Their Partners: A Systematic Review

Objectives Despite evidence that patients with coronary heart disease (CHD) and their partners report significant psychological distress, and suggestions that involving partners in interventions alleviates such distress, no systematic reviews have examined this. The objective of this study was to systematically review evidence on the effectiveness of psychological interventions for patients with CHD and their partners. Methods CENTRAL, Medline, EMBASE, CINAHL and PsycINFO databases were searched through October 2012. Randomized controlled trials evaluating psychological interventions for patients with CHD and their partners were included. Selection of studies, study appraisal, data extraction and analysis were undertaken using standard methods. Results Seven studies comprising 673 dyads (patient and partner) were included. Psychological interventions result in modest improvements in patients' health-related quality of life, blood pressure, knowledge of disease and treatment, and satisfaction with care, and in partners' anxiety, knowledge and satisfaction. There was a non-significant trend for improvements in anxiety for patients, and depressive symptoms for both patients and partners. There was no evidence of a significant effect on mortality, morbidity or other cardiovascular risk factors for patients, or social support for patients and partners. Conclusions Psychological interventions for patients with CHD and their partners were found to improve health-related quality of life, blood pressure, knowledge, and satisfaction with care for patients, and anxiety, knowledge, and satisfaction with care for partners. However, as the overall quality of the evidence was low, these results should be interpreted with caution.
Relationships Between Social Networks and Mental Health: An Exponential Random Graph Model Approach Among Romanian Adolescents

Social networks have an important effect on health, and social network analysis has become essential for understanding human behavior and vulnerability. Using exponential random graph models (ERGM), this study explores the associations between mental health and network structure (or more specifically, mental health homophily) and the association between poor mental health and social isolation. Two classes of Romanian adolescents aged 12–14 years participated in the study (n = 26 in each class). We assessed school network, sociodemographic covariates, and mental health using the Strengths and Difficulties Questionnaire (SDQ). ERGM was first used to test the presence of sex and mental health homophily and then to test whether mental health was a predictor of social isolation. The results showed homophily patterns regarding sex and mental health. Moreover, participants with a higher SDQ score had a lower probability of a tie. Overall, this study showed how social networks are structured with different forms of homophily and that adolescents with poor mental health are more likely to be social isolates. Thus, prevention and interventions should focus on these vulnerable adolescents. Methodological advances like ERGM constitute a promising avenue for further research.
Parameter properties and stellar population of the old open cluster NGC 3960

We present a $BV\! I$ photometric and astrometric catalogue of the open cluster NGC 3960, down to limiting magnitude $V\sim22$, obtained from observations taken with the Wide Field Imager camera at the MPG/ESO 2.2 m Telescope at La Silla. The photometry of all the stars detected in our field of view has been used to estimate a map of the strong differential reddening affecting this area. Our results indicate that, within the region where the cluster dominates, the $E(V-I)$ values range from 0.21 up to 0.78, with $E(V-I)=0.36$ ($E(B-V)=0.29$) at the nominal cluster centroid position; color excesses $E(V-I)$ up to 1 mag have been measured in the external regions of the field of view where field stars dominate. The reddening-corrected color-magnitude diagram (CMD) allows us to conclude that the cluster has an age between 0.9 and 1.4 Gyr and a distance modulus of $(V-M_V)_0=11.35$. In order to minimize field star contamination, their number has been statistically subtracted based on the surface density map. The empirical cluster main sequence has been recovered in the V vs. $V-I$ and in the J vs. $J-K_{\rm S}$ planes, using optical and infrared data, respectively. From these empirical cluster main sequences, two samples of candidate cluster members were derived in order to obtain the luminosity distributions as functions of the V and J magnitudes. The Luminosity Functions have been transformed into the corresponding Mass Functions; for $M>1~M_\odot$, the two distributions have been fitted with a power law of index $\alpha_V=2.95\pm0.53$ and $\alpha_J=2.81\pm0.84$ in V and in J , respectively, while the Salpeter Mass Function in this notation has index $\alpha=2.35$.
On index coding with side information

Building communication schemes which allow participants to communicate efficiently has always been a challenging yet intriguing problem for communication theorists. Index Coding with Side Information (ICSI) (Birk and Kol (1998)) is a communication scheme dealing with broadcast channels in which receivers have prior side information about the messages to be broadcast. Exploiting the knowledge about the side information, the sender may significantly reduce the number of required transmissions compared with the naive approach. As a consequence, the efficiency of the communication over this type of broadcast channels could be dramatically improved. Apart from being a special case of the well-known (nonmulticast) Network Coding problem (Alhswede et al. (2000), Koetter and Médard (2003)), the ICSI problem has also found various potential applications on its own, such as audioand video-on-demand, daily newspaper delivery, data pushing, and oppoturnistic wireless networks. While most of the known works on ICSI focus on the performances of index codes of various kinds, the security and error correction aspects of those codes have never been examined. Although similar issues have been thoroughly investigated in multicast Network Coding, on the side of non-multicast Network Coding, where ICSI is one example, things are much less understood. In this work, we make an attempt to fill in this gap. We first analyze the block security level of the linear index code based on a
2 A Contingency Model for Requirements Development

Drawing upon the requirements and software development literature, the present study proposes an integrative contingency model for requirements development. Based on 116 quality journal articles, we analyze requirements development risks, requirements development techniques, and heuristics for how they are effectively related. Subsequently, we synthesize the insights from the identified literature into a model for requirements development that relates patterns of risk resolution to archetypical risk profiles. The model integrates the literature on requirements and software development; sets the scene for future research; and, finally proposes how practitioners can manage risks in requirements development projects.
Decreased Levels of Active SMAD2 Correlate with Poor Prognosis in Gastric Cancer

Background TGF-β plays a dual role in the progression of human cancer. During the early stages of carcinogenesis, TGF-β functions as a tumor suppressor. During the late stages of tumor development, however, TGF-β can promote tumor growth and metastasis. A shift in Smad2/3 phosphorylation from the carboxy terminus to linker sites is a key event determining biological function of TGF-β in colorectal and hepatocellular carcinoma. In the present study, we investigated the potential role of differential Smad2/3 phosphorylation in gastric adenocarcinoma. Methodology Immunohistochemical staining with anti-P-Smad2/3C and P-Smad2/3L antibodies was performed on 130 paraffin-embedded gastric adenocarcinoma specimens. The relationship between P-Smad2/3C and P-Smad2/3L immunohistochemical score and clinicopathologic characteristics of patients was analyzed. Real time PCR was used to measure mRNA expression of Smad2 and Smad3 in cancer and surrounding non-tumor tissue. Principal Findings No significant P-Smad2L and/or P-Smad3L positive staining was detected in the majority of specimens (positive staining in 18/130 samples). Positive P-Smad2/3L staining was not associated with a decrease in carboxyterminal phosphorylation staining. Loss of P-Smad2C remarkably correlated with depth of tumor infiltration and poor differentiation of cancer cells in patients with gastric cancer. No correlation was detectable between P-Smad3C and clinicopathologic characteristics of gastric adenocarcinoma. However, co-staining analysis revealed that P-Smad3C co-localised with α-SMA and collagen I in gastric cancer cells, indicating a potential link between P-Smad3C and epithelial-to-mesenchymal transition of cancer. Real time PCR demonstrated reduced mRNA expression of Smad2 in gastric cancer when compared with surrounding non-tumor tissue in 15/16 patients. Conclusions Loss of P-Smad2C tightly correlated with cancer invasion and poor differentiation in gastric cancer. Contrary to colorectal and hepatocellular carcinoma, canonical carboxy-terminal phosphorylation, but not linker phosphorylation, of Smad2 is critical for gastric cancer.
Self-Care Practices among Diabetes Patients in Addis Ababa: A Qualitative Study

Background Self-care practices that include self-monitoring of blood sugar level, diet management, physical exercise, adherence to medications, and foot care are the cornerstones of diabetes management. However, very little is known about self-care in developing countries where the prevalence of diabetes is increasing. Objective The objective of this study was to describe self-care practices among individuals with type II diabetes in Addis Ababa, Ethiopia. Methods A qualitative method was used to gather data from type II diabetes patients. Patients were recruited from the outpatient diabetes clinics of two public hospitals in Addis Ababa. Data were collected using a semi structured interview guide. A thematic analysis approach was used to process the data. Results Overall self-care practices were not adequate. Most patients reported irregular self-monitoring of blood sugar. Dietary and physical exercise recommendations were inadequately practiced by most of the participants. Most patients better adhered to medication prescriptions. Patients generally lack proper information/knowledge regarding the importance of self-care and how it should be implemented. Based on reported behavior we identified three main categories of patients; which are those ‘endeavor to be compliant’, ‘confused’ and ‘negligent’. Conclusion Diabetes patients largely depend on prescribed medications to control their blood sugar level. The importance of proper self-care practices for effective management of diabetes is not adequately emphasized in diabetes care centers and patients lack sufficient knowledge for proper self-care.
An Offset Cancellation Technique for Two-Stage CMOS Operational Amplifiers

An offset cancellation technique for two-stage CMOS operational amplifiers is proposed. The auxiliary amplifiers are employed to cancel the offset voltage. The error voltage is stored on a capacitor during the cancellation phase and is canceled during the normal operation. An experimental prototype amplifier implemented in a 0.35-mum CMOS technology demonstrates that the offset voltage is reduced to 1.898 mV under a clock frequency of 200 KHz.
Auditory perception bias in speech imitation

In an experimental study, we explored the role of auditory perception bias in vocal pitch imitation. Psychoacoustic tasks involving a missing fundamental indicate that some listeners are attuned to the relationship between all the higher harmonics present in the signal, which supports their perception of the fundamental frequency (the primary acoustic correlate of pitch). Other listeners focus on the lowest harmonic constituents of the complex sound signal which may hamper the perception of the fundamental. These two listener types are referred to as fundamental and spectral listeners, respectively. We hypothesized that the individual differences in speakers' capacity to imitate F0 found in earlier studies, may at least partly be due to the capacity to extract information about F0 from the speech signal. Participants' auditory perception bias was determined with a standard missing fundamental perceptual test. Subsequently, speech data were collected in a shadowing task with two conditions, one with a full speech signal and one with high-pass filtered speech above 300 Hz. The results showed that perception bias toward fundamental frequency was related to the degree of F0 imitation. The effect was stronger in the condition with high-pass filtered speech. The experimental outcomes suggest advantages for fundamental listeners in communicative situations where F0 imitation is used as a behavioral cue. Future research needs to determine to what extent auditory perception bias may be related to other individual properties known to improve imitation, such as phonetic talent.
A gas-rich nuclear bar fuelling a powerful central starburst in NGC 2782

We present evidence that the peculiar interacting starburst galaxy NGC 2782 (Arp 215) harbors a gas-rich nuclear stellar bar feeding an M82-class powerful central starburst, from a study based on OVRO CO (J=1->0) data, WIYN BVR&Halpha observations, along with available NIR images, a 5 GHz RC map and HST images. NGC 2782 harbors a clumpy, bar-like CO feature of radius ~ 7.5'' (1.3 kpc) which leads a nuclear stellar bar of similar size. The nuclear CO bar is massive: it contains ~2.5x10**9 M_sun of molecular gas, which makes up ~ 8 % of the dynamical'mass present within a 1.3 kpc radius. Within the CO bar, emission peaks in two extended clumpy lobes which lie on opposite sides of the nucleus, separated by ~ 6'' (1 kpc). Between the CO lobes, in the inner 200 pc radius, resides a powerful central starburst which is forming stars at a rate of 3 to 6 M_sun yr-1. While circular motions dominate the CO velocity field, the CO lobes show weak bar-like streaming motions on the leading side of the nuclear stellar bar, suggestive of gas inflow. We estimate semi-analytically the gravitational torque from the nuclear stellar bar on the gas, and suggest large gas inflow rates from the CO lobes into the central starburst. These observations, which are amongst the first ones showing a nuclear stellar bar fuelling molecular gas into an intense central starburst, are consistent with simulations and theory which suggest that nuclear bars provide an efficient way of transporting gas closer to the galactic center to fuel central activity. Furthermore, several massive clumps are present at low radii, and dynamical friction might produce further gas inflow. We suggest that the nuclear molecular gas bas and central activity will be very short-lived, likely disappearing within 5x10**8 years.
Optimal population coding by noisy spiking neurons

In retina and in cortical slice the collective response of spiking neural populations is well described by “maximum-entropy” models in which only pairs of neurons interact. We asked, how should such interactions be organized to maximize the amount of information represented in population responses? To this end, we extended the linear-nonlinear-Poisson model of single neural response to include pairwise interactions, yielding a stimulus-dependent, pairwise maximum-entropy model. We found that as we varied the noise level in single neurons and the distribution of network inputs, the optimal pairwise interactions smoothly interpolated to achieve network functions that are usually regarded as discrete—stimulus decorrelation, error correction, and independent encoding. These functions reflected a trade-off between efficient consumption of finite neural bandwidth and the use of redundancy to mitigate noise. Spontaneous activity in the optimal network reflected stimulus-induced activity patterns, and single-neuron response variability overestimated network noise. Our analysis suggests that rather than having a single coding principle hardwired in their architecture, networks in the brain should adapt their function to changing noise and stimulus correlations.
DIRECTION GÉNÉRALE DES ÉTUDES ET DES RELATIONS INTERNATIONALES DOES THE VOLATILITY OF COMMODITY PRICES REFLECT MACROECONOMIC UNCERTAINTY?

While there exists numerous studies on the macroeconomic e§ects of oil and commodity shocks, the literature is quite silent on the impact of macroeconomic uncertainty on oil and commodity prices and, especially, on their volatility. This paper tackles this issue through the estimation of a threshold vector autoregressive (TVAR) model on a sample of 19 commodity markets. We aim at (i) assessing whether the e§ect of macroeconomic uncertainty shocks on commodity price returns depends on the degree of uncertainty, and (ii) investigating the transfer from macroeconomic uncertainty to price uncertainty using a newly developed measure of commodity price uncertainty. Our Öndings show that both agricultural and industrial markets are highly sensitive to the variability and the level of macroeconomic uncertainty, while the impact on precious metals is more parsimonious given their well-identiÖed safe-haven role in time of economic turmoil. In addition, we Önd evidence that the recent 2007-09 recession has generated an unprecedented episode of high uncertainty in numerous commodity prices. Interestingly, our analysis further reveals that volatility and uncertainty in prices can be disconnected. This is especially true for the oil market as most important shocks in the 1990s and the beginning of the 2000s that lead to price volatility do not generate price uncertainty, highlighting the relevance of our uncertainty measure in linking uncertainty to predictability rather than to
Developmental Trends in Children's Internal Body Knowledge

Literature on children's internal body knowledge has consistently indicated that knowledge about the body develops in an orderly sequence with increasing age. How much children currently know about their internal organs, however, may be influenced by the increase in health and body information available through school education programmes. As there is little recent research in this area, the present study aimed to provide an update on what Australian children currently understand about their anatomy, and to corroborate the developmental trends found in previous research. One hundred and eighty-nine school children aged 7 to 12 years were asked to draw the interior of the body in a body outline provided, with a subset of 54 children also being interviewed about their understanding of their anatomy. The developmental trends found in this study were broadly consistent with those reported in the existing literature on children's inside body knowledge, and are similar to those documented with children's human figure drawing; namely, that children's body knowledge and understanding increased with age. Although awareness of the integration of internal body parts amongst children in the present study seemed more developed than suggested in previous studies, the availability of educational resources influencing children's knowledge about their internal organs remains equivocal. Nevertheless, this research has relevance for those involved in children's health awareness and education, as well as direct implications for paediatric health care procedures.
Influence of a stellar cusp on the dynamics of young stellar discs and the origin of the S‐stars in the Galactic Centre

Observations of the Galactic Centre show evidence of one or two disc-like structures of very young stars orbiting the central supermassive black hole within a distance of a few 0.1 pc. A number of analyses have been carried out to investigate the dynamical behaviour and consequences of these discs, including disc thickness and eccentricity growth as well as mutual interaction and warping. However, most of these studies have neglected the influence of the stellar cusp surrounding the black hole, which is believed to be one to two orders of magnitude more massive than the disc(s). By means of N-body integrations using our BHINT code, we study the impact of stellar cusps of different compositions. We find that although the presence of a cusp does have an important effect on the evolution of an otherwise isolated flat disc, its influence on the evolution of disc thickness and warping is rather mild in a two-disc configuration. However, we show that the creation of highly eccentric orbits strongly depends on the graininess of the cusp (i.e. the mean and maximum stellar masses). While Chang recently found that full cycles of Kozai resonance are prevented by the presence of an analytic cusp, we show that relaxation processes play an important role in such highly dense regions and support short-term resonances. We thus find that young disc stars on initially circular orbits can achieve high eccentricities by resonant effects also in the presence of a cusp of stellar remnants, yielding a mechanism to create S-stars and hypervelocity stars. Furthermore, we discuss the underlying initial mass function (IMF) of the young stellar discs and find no definite evidence for a non-canonical IMF.
Contextual modulation of primary visual cortex by auditory signals

Early visual cortex receives non-feedforward input from lateral and top-down connections (Muckli & Petro 2013 Curr. Opin. Neurobiol. 23, 195–201. (doi:10.1016/j.conb.2013.01.020)), including long-range projections from auditory areas. Early visual cortex can code for high-level auditory information, with neural patterns representing natural sound stimulation (Vetter et al. 2014 Curr. Biol. 24, 1256–1262. (doi:10.1016/j.cub.2014.04.020)). We discuss a number of questions arising from these findings. What is the adaptive function of bimodal representations in visual cortex? What type of information projects from auditory to visual cortex? What are the anatomical constraints of auditory information in V1, for example, periphery versus fovea, superficial versus deep cortical layers? Is there a putative neural mechanism we can infer from human neuroimaging data and recent theoretical accounts of cortex? We also present data showing we can read out high-level auditory information from the activation patterns of early visual cortex even when visual cortex receives simple visual stimulation, suggesting independent channels for visual and auditory signals in V1. We speculate which cellular mechanisms allow V1 to be contextually modulated by auditory input to facilitate perception, cognition and behaviour. Beyond cortical feedback that facilitates perception, we argue that there is also feedback serving counterfactual processing during imagery, dreaming and mind wandering, which is not relevant for immediate perception but for behaviour and cognition over a longer time frame. This article is part of the themed issue ‘Auditory and visual scene analysis’.