bluuebunny/crossref_metadata_2025_split huggingface dataset:
Relationship Between Primary Care Providers’ Perceptions of Alcohol Use Disorder And Pharmacotherapy Prescribing Rates
Authors: Bernstein Eden Y , Pfoh Elizabeth R , Le Phuc , Rothberg Michael B 
Published: October 2022

Abstract

Aims
Acamprosate, naltrexone and disulfiram are underprescribed for alcohol use disorder (AUD) with marked variability among primary care providers (PCPs). We aimed to identify differences between high and low prescribers of medications for AUD (MAUD) with regard to knowledge, experiences, prioritization and attitudes.

Methods
We surveyed PCPs from a large healthcare system with at least 20 patients with AUD. Prescribing rates were obtained from the electronic health record (EHR). Survey responses were scored from strongly disagree (1) to strongly agree (5). Multiple imputation was used to generate attitude scores for 7 missing subjects. PCPs were divided into groups by the median prescribing rate and attitude. Comparisons were made using Wilcoxon rank-sum and regression.

Results
Of the 182 eligible PCPs, 68 (37.4%) completed the survey. Most indicated willingness to attend an educational course (57.4%). Compared with low prescribers, high prescribers viewed the effectiveness of medications more favorably (short term 4.0 vs 3.7, P = 0.02; long term 3.5 vs 3.2, P = 0.04) and were more likely to view prescribing as part of their job (3.9 vs 3.4, P = 0.04). PCPs with positive attitudes (72.4%, CI 60.9–83.8%) had a prescribing rate of 5.0% (CI 3.5–6.5%) compared to 1.9% (CI 0.5–3.4%) among those with negative attitudes (P = 0.028). When stratified by attitude, belief in effectiveness was associated with higher prescribing among PCPs with positive attitudes but not those with negative attitudes.

Conclusions
PCPs indicated an interest in learning to prescribe MAUD. However, education alone may not be effective unless physicians have positive attitudes towards patients with AUD.
DeepLncPro: an interpretable convolutional neural network model for identifying long non-coding RNA promoters
Authors: Zhang Tianyang , Tang Qiang , Nie Fulei , Zhao Qi , Chen Wei 
Published: October 2022

Abstract
Long non-coding RNA (lncRNA) plays important roles in a series of biological processes. The transcription of lncRNA is regulated by its promoter. Hence, accurate identification of lncRNA promoter will be helpful to understand its regulatory mechanisms. Since experimental techniques remain time consuming for gnome-wide promoter identification, developing computational tools to identify promoters are necessary. However, only few computational methods have been proposed for lncRNA promoter prediction and their performances still have room to be improved. In the present work, a convolutional neural network based model, called DeepLncPro, was proposed to identify lncRNA promoters in human and mouse. Comparative results demonstrated that DeepLncPro was superior to both state-of-the-art machine learning methods and existing models for identifying lncRNA promoters. Furthermore, DeepLncPro has the ability to extract and analyze transcription factor binding motifs from lncRNAs, which made it become an interpretable model. These results indicate that the DeepLncPro can server as a powerful tool for identifying lncRNA promoters. An open-source tool for DeepLncPro was provided at https://github.com/zhangtian-yang/DeepLncPro.
The end of the golden age: on growing challenges for male workers and their partners to secure a family income
Authors: Gerlitz Jean-Yves 
Published: October 2022

AbstractThanks to the male breadwinner model with wages sufficient to support a family, working-class families used to be financially secure. The transformation towards the adult worker model (AWM) saw an accumulation of adverse employment characteristics—especially among manual and non-manual routine occupations—and a rise in poverty risks. However, there is a lack of research that combines these strands. I ask to what extent male Western German workers and their partners’ ability to secure labour earnings that support a family has changed, and to what degree this was hampered by various adverse employment characteristics. Focusing on service and production workers with cohabiting partners, I analyse whether their individual and combined labour income is sufficient to support a family. Performing descriptive trend analysis and linear probability models with German Socio-Economic Panel data for 1985–2013, I compare class effects of four periods. I find that since the end of the 1990s, male service and production workers increasingly struggle to secure a family income—mainly driven by low wages and low work intensity, while partners’ labour market participation has gained relevance. The transformation towards the AWM coincided with a devaluation of the most privileged group among workers and thus the working class as a whole.
The political determinants of housing benefits
Authors: Nelson Kenneth , Borg Ida , Nieuwenhuis Rense , Alm Susanne 
Published: October 2022

AbstractHousing benefits differ substantially across countries. In this paper, we apply power resource theory, developed primarily in relation to the emergence and subsequent expansion of social citizenship, to housing policy. The purpose is to analyse the political determinants of housing benefits, and particularly the role of left parties and the partisan mobilization of labour. The empirical analyses are based on new housing benefit data for 31 affluent democracies from the period 2001–2018. The results of a series of fixed effects pooled time-series regressions show that the strength of left government is positively associated with the size of housing benefits. However, the positive influence of left cabinets is conditional on the relative size of rental housing and the fractionalization of the party system. Our findings highlight the need to combine actor-oriented explanations of the welfare state with theories about the corporatist power structures of society.
Gender and mathematics achievement: the role of gender stereotypical beliefs of classroom peers
Authors: Smith Emil , Farkas George 
Published: October 2022

AbstractWe tested the relationship between gender-stereotypical beliefs (GSBs) of female and male classroom peers and female achievement in mathematics. Complete-class student survey data merged with family register data from 1,047 Danish 6th-grade students, nested in 50 classrooms within 28 schools, were analysed using multilevel linear regressions including controls for parental education and income, the percentage of females in the classroom, prior math test scores, and the parental education, income, and prior test scores of female and male peers. We found that the GSBs of female peers were negatively associated with girls’ math achievement. Similar variables were not related to the math achievement of boys.
Hybrid balancing as classical realist statecraft: China's balancing behaviour in the Indo-Pacific
Authors: Ito Ryuta 
Published: October 2022

Abstract
Hybrid warfare has recently attracted scholarly attention. Despite its importance, hybrid warfare research remains underdeveloped, as it sometimes falls into the trap of ‘simplistic hypothesis testing’, which focuses on narrowly defined military factors while downplaying the fundamentals of international politics (e.g. balancing and diplomacy). This article fills this gap by constructing a new theoretical concept called ‘hybrid balancing’ by introducing the essence of hybrid warfare into classical realism, based on the scientific realism in the philosophy of science as a meta-theoretical foundation. ‘Hybrid balancing’ consists of three ideal types of balancing beyond the traditional hard one: political, economic and informational balancing. As a plausibility probe to show that the argument is sufficiently grounded in evidence to justify further research, I illustrate the new concept by examining China's hybrid warfare in the Indo-Pacific, an arena of geopolitical competition between China and the United States. The implications of the research are that it (1) shows the significance of ‘agency’ over ‘structure’ to solve the agent–structure debate, (2) develops a new theoretical concept explaining non-military aspects of balancing, (3) overcomes ‘simplistic hypothesis testing’, and (4) sheds new light on the Indo-Pacific, which had been overlooked in previous research around hybrid warfare.
Evaluation of Torula yeast as a protein source in extruded feline diets
Authors: Holt Dalton A , Aldrich Charles G 
Published: October 2022

AbstractThe objective of this work was to evaluate the use of a Torula yeast (TY) on diet processing, palatability, and total tract nutrient digestibility in extruded feline diets. Four dietary treatments were compared, differing by protein source: TY, pea protein concentrate (PP), soybean meal (SM), and chicken meal (CM). Diets were produced using a single-screw extruder under similar processing conditions. Palatability assessment was conducted as a split plate design where both first choice and intake ratio (IR) were determined. Apparent total tract digestibility (ATTD) of nutrients was estimated using Titanium dioxide as an indigestible marker. During diet production, specific mechanical energy of TY and SM (average of 187 kJ/kg) was greater (P &lt; 0.05) than for PP (138 kJ/kg); however, CM was similar to all treatments (167 kJ/kg). Kibble diameter, piece volume, and sectional expansion ratio were greatest for TY (P &lt; 0.05). Additionally, both bulk and piece density were lowest (P &lt; 0.05) for TY. Kibble hardness was lower for TY and SM (P &lt; 0.05; average of 2.10 Newtons) compared to CM and PP (average of 2.90 Newtons). During the palatability trial, TY was chosen first a greater number of times than CM (P &lt; 0.05; 36 vs. 4, respectively), but differences were not found between TY and PP (25 vs. 15, respectively) or TY and SM (24 vs. 16, respectively). Cats had a greater IR (P &lt; 0.05) of TY compared to CM and PP (0.88 and 0.73, respectively). However, there was no difference in preference between TY and SM. ATTD of dry matter (DM) and organic matter (OM) was greater (P &lt; 0.05) for CM (87.43% and 91.34%, respectively) than other treatments. Both DM and OM ATTD of TY were similar (P &lt; 0.05) to PP and SM (average of 86.20% and average of 89.76%, respectively). Ash ATTD was greater (P &lt; 0.05) for cats fed TY and SM (average of 37.42%), intermediate for PP (32.79%), and lowest for CM (23.97%). Crude protein (CP) ATTD of TY was similar to all other treatments (average of 89.97%), but fat ATTD was lower (P &lt; 0.05; 92.52%) than other treatments (93.76% to 94.82%). Gross energy ATTD was greater (P &lt; 0.05) for CM than TY (90.97% vs. 90.18%, respectively); however, TY was similar to PP and SM (average of 90.22%). Total dietary fiber ATTD was similar between TY and CM (average of 66.20%) and greater (P &lt; 0.05) than PP and SM (average of 58.70%). The TY used in this study facilitated diet formation, increased diet preference, and was highly digestible when fed to cats.
Comparison of Vector Trapping Methods for Outdoor Biting Malaria Vector Surveillance in Thailand and Vietnam
Authors: Ngoenklan Ratchadawan , Thanh Duong Tran , Duc Chinh Vu , Quang Thieu Nguyen , Hii Jeffrey , Bangs Michael J , Aum-Aung Boonserm , Suwonkerd Wannapa , Chareonviriyaphap Theeraphap 
Published: October 2022

Abstract
The performances of the human-baited double net trap (HDNT) and the human-baited host decoy trap (HDT) methods were compared against the outdoor human landing catch (OHLC) method in Thailand and Vietnam. Two study sites were selected in each country: a rural village and a nearby forest setting. The three outdoor trap methods were rotated nightly between three set trapping positions, in a pre-assigned Latin square design. Volunteers were rotated following the trap rotation to avoid bias. The greatest number of adult mosquitoes was collected from the forest sites in both countries, showing Anopheles minimus (s.s.) Theobald (96.54%) and Anopheles dirus (s.s.) Peyton & Harrison (25.71%) as the primary malaria vectors in Thailand and Vietnam, respectively. At the Thai forest site, OHLC collected significantly more anopheline mosquitoes per trap night than HDNT and HDT, with mean ± standard error values of 14.17 ± 4.42, 4.83 ± 1.56, and 4.44 ± 1.45, respectively, whilst HDNT and HDT were significantly less productive at 0.34 times and 0.31 times, respectively, than OHLC in capturing anopheline mosquitoes. However, there were no significant differences among the three methods of trapping malaria vectors for the village site. At the Vietnamese forest site, HDNT achieved the highest performance in collecting Anopheline mosquitoes at 1.54 times compared to OHLC, but there was no significant difference between the two traps. The results suggested HDNT could be a possible alternative trap to OHLC in this area. Although HDT was less efficient at attracting Anopheline mosquitoes, it was highly efficient at trapping culicine mosquitoes.
Do cosmological observations allow a negative Λ?
Authors: Sen Anjan A , Adil Shahnawaz A , Sen Somasri 
Published: October 2022

ABSTRACT
In view of the recent measurement of H0 from the Hubble Space Telescope and Supernova H0 for the Equation of State (SH0ES) team, we explore the possibility of existence of a negative cosmological constant [anti-de Sitter (AdS) vacua in the dark energy sector] in the Universe. In this regard, we consider quintessence fields on top of a negative cosmological constant and compare such construction with Λ cold dark matter (ΛCDM) model using a different combination of cosmic microwave background, Type Ia supernova, baryon acoustic oscillation, and H0 data. Various model comparison estimators show that quintessence models with a negative Λ are either preferred over ΛCDM or perform equally as the ΛCDM model. This suggests that the presence of a negative Λ (AdS ground state) in our Universe, which can naturally arise in string theory, is consistent with cosmological observations.
The Tianlai dish array low-z surveys forecasts
Authors: Perdereau Olivier , Ansari Réza , Stebbins Albert , Timbie Peter T , Chen Xuelei , Wu Fengquan , Li Jixia , Marriner John P , Tucker Gregory S , Cong Yanping , Das Santanu , Li Yichao , Liu Yingfeng , Magneville Christophe , Peterson Jeffrey B , Phan Anh , Robinthal Lily , Sun Shijie , Wang Yougang , Wu Yanlin , Xu Yidong , Yu Kaifeng , Yu Zijie , Zhang Jiao , Zhang Juyong , Zuo Shifan 
Published: October 2022

ABSTRACT
We present the science case for surveys with the Tianlai dish array interferometer tuned to the [1300, 1400] MHz frequency range. Starting from a realistic generation of mock visibility data according to the survey strategy, we reconstruct maps of the sky and perform foreground subtraction. We estimate the level of residuals from imperfect subtraction, mostly due to mode mixing, i.e. distortions in the reconstructed 3D maps due to frequency-dependent instrument response. We show that a survey of the North Celestial Polar cap during a year of observations, covering an area of $150 \, \mathrm{deg^2}$, would reach a sensitivity of $1.5-2 \, \mathrm{mK}$ per $1 \, \mathrm{MHz} \times 0.25^2 \, \mathrm{deg^2 }$ voxel and be marginally impacted by mode mixing. Tianlai would be able to detect ∼10 nearby massive H i  clumps as well as a very strong cross-correlation signal of 21 cm intensity maps with the North Celestial Cap Survey optical galaxies. We also studied the performance of a mid-latitude survey, covering $\sim 1500 \, \mathrm{deg^2}$ overlapping the SDSS footprint. Despite a higher noise level for the mid-latitude survey, as well as significant distortions due to mode mixing, Tianlai would be able to detect a highly significant cross-correlation between the 21 cm signal and the Sloan spectroscopic galaxy sample. Using the extragalactic signals measured from either or both of these surveys, and comparing them with simulations such as those presented here will make it possible to assess the impact of various instrumental imperfections on the Tianlai dish array performance. This would pave the way for future intensity mapping surveys with higher sensitivity.
Semitransparent shear turbulence in hot Jupiter atmospheres
Authors: Menou Kristen 
Published: October 2022

ABSTRACT
Turbulent transport driven by secular shear instabilities can lead to enhanced vertical mixing in hot Jupiter atmospheres, impacting their cloudiness, chemistry, and overall vertical structure. We discuss the turbulent regime expected and evaluate theoretical uncertainties on the strength of the vertical mixing (i.e. Kzz values). We focus our work on three well-studied hot Jupiters with a hierarchy of atmospheric temperatures: HD189733b (Teq ≃ 1200 K), HD209458b (Teq ≃ 1450 K), and Kepler7b (Teq ≃ 1630 K). Kzz uncertainties are large. They are dominated by (i) the poorly understood magnitude of turbulent transport and (ii) the semitransparent nature of shear turbulence near the planetary photosphere. Using a specific Moore–Spiegel instability threshold, we infer that the cooler HD189733b is not subject to enhanced mixing from semitransparent shear turbulence, while the daysides of the hotter Kepler7b and (marginally so) HD209458b are. Enhanced vertical mixing is generally expected to manifest on hot enough exoplanets, with Teq &gt; 1500–1600 K. On a given planet, day and night Kzz profiles can differ by an order of magnitude or more. Vertical mixing is slightly favoured in equatorial regions, where the atmospheric zonal shear is strongest. In all three planetary cases studied, momentum feedback on the atmospheric mean flow is minor to negligible.
Subaru HSC weak lensing of SDSS redMaPPer cluster satellite galaxies: empirical upper limit on orphan fractions
Authors: Kumar Amit , More Surhud , Rana Divya 
Published: October 2022

ABSTRACT
Weak gravitational lensing directly probes the matter distribution surrounding satellite galaxies in galaxy clusters. We measure the weak lensing signal induced on the shapes of background galaxies around the Sloan Digital Sky Survey (SDSS) redMaPPer cluster satellite galaxies, which have their central galaxies assigned with a probability Pcen &gt; 0.95 in the redshift range, 0.1 ≤ z ≤ 0.33. We use the galaxy shapes from the Subaru Hyper Suprime-Cam (HSC) survey for this purpose. We bin satellite galaxies by their distance from the cluster centre and compare it to the signal around a control sample of galaxies that do not reside in clusters but have similar colours and magnitudes. We explore the effect of environmental processes on the dark matter mass around satellites. We see hints of a difference in the mass of the subhalo of the satellite compared to the halo masses of galaxies in our control sample, especially in the innermost cluster-centric radial bin (0.1 &lt; r &lt; 0.3 [${h^{-1}\,\rm Mpc}$]). For the first time, we put an upper limit on the prevalence of orphan galaxies that have entirely lost their dark matter haloes with cluster-centric distances with the help of our measurements. However, these upper limits could be relaxed if there is substantial contamination in the satellite galaxy sample.
The MOSDEF survey: a new view of a remarkable z = 1.89 merger
Authors: Runco Jordan N , Shapley Alice E , Kriek Mariska , Cappellari Michele , Topping Michael W , Sanders Ryan L , Kokorev Vasily I , Price Sedona H , Reddy Naveen A , Coil Alison L , Mobasher Bahram , Siana Brian , Zick Tom , Magdis Georgios E , Brammer Gabriel , Aird James 
Published: October 2022

ABSTRACT
We present a detailed study of a galaxy merger taking place at z = 1.89 in the GOODS-S field. Here, we analyse Keck/MOSFIRE spectroscopic observations from the MOSFIRE Deep Evolution Field (MOSDEF) survey along with multiwavelength photometry assembled by the 3D-HST survey. The combined data set is modelled to infer the past star formation histories (SFHs) of both merging galaxies. They are found to be massive, with log10(M*/M⊙) &gt; 11, with a close mass ratio satisfying the typical major-merger definition. Additionally, in the context of delayed-τ models, GOODS-S 43114, and GOODS-S 43683 have similar SFHs and low star formation rates (log10(SFR(SED)/${\rm M}_{\odot }\,\rm {yr}^{-1}$) &lt; 1.0) compared to their past averages. The best-fitting model SEDs show elevated H δA values for both galaxies, indicating that their stellar spectra are dominated by A-type stars, and that star formation peaked ∼0.5−1 Gyr ago and has recently declined. Additionally, based on SED fitting both merging galaxies turned on and shut off star formation within a few hundred Myr of each other, suggesting that their bursts of star formation may be linked. Combining the SFHs and H δA results with recent galaxy merger simulations, we infer that these galaxies have recently completed their first pericentric passage and are moving apart. Finally, the relatively low second velocity moment of GOODS-S 43114, given its stellar mass suggests a disc-like structure. However, including the geometry of the galaxy in the modelling does not completely resolve the discrepancy between the dynamical and stellar masses. Future work is needed to resolve this inconsistency in mass.
The Pristine Inner Galaxy Survey (PIGS) – IV. A photometric metallicity analysis of the Sagittarius dwarf spheroidal galaxy
Authors: Vitali Sara , Arentsen Anke , Starkenburg Else , Jofré Paula , Martin Nicolas F , Aguado David S , Carlberg Raymond , González Hernández Jonay I , Ibata Rodrigo , Kordopatis Georges , Malhan Khyati , Ramos Pau , Sestito Federico , Yuan Zhen , Buder Sven , Lewis Geraint F , Wan Zhen , Zucker Daniel B 
Published: October 2022

ABSTRACT
We present a comprehensive metallicity analysis of the Sagittarius dwarf spheroidal galaxy (Sgr dSph) using Pristine CaHK photometry. We base our member selection on Gaia EDR3 astrometry, applying a magnitude limit at G0 = 17.3, and our population study on the metallicity-sensitive photometry from the Pristine Inner Galaxy Survey (PIGS). Working with photometric metallicities instead of spectroscopic metallicities allows us to cover an unprecedented large area (∼100 square degrees) of the dwarf galaxy, and to study the spatial distribution of its members as function of metallicity with little selection effects. Our study compares the spatial distributions of a metal-poor population of 9719 stars with [Fe/H] &lt;−1.3 and a metal-rich one of 30 115 stars with [Fe/H] &gt;−1.0. The photometric Sgr sample also allows us to assemble the largest sample of 1150 very metal-poor Sgr candidates ([Fe/H] &lt;−2.0). By investigating and fitting the spatial properties of the metal-rich and metal-poor population, we find a negative metallicity gradient which extends up to 12 degrees from the Sgr centre (or ∼5.5 kpc at the distance of Sgr), the limit of our footprint. We conclude that the relative number of metal-poor stars increases in the outer areas of the galaxy, while the central region is dominated by metal-rich stars. These findings suggest an outside-in formation process and are an indication of the extended formation history of Sgr, which has been affected by the tidal interaction between Sgr and the Milky Way.