bluuebunny/crossref_metadata_2025_split huggingface dataset:
A Systematic Review of Instruments to Assess Guilt in Children and Adolescents
Authors: Zaccari Vittoria , Aceto Marianna , Mancini Francesco 
Published: December 2020

Background: Guilt feelings have received considerable attention in past psychological theory and research. Several studies have been conducted that represent a range of views and propose various implications of guilt in children and adolescents. Variations in theoretical definitions of guilt, emphasizing a lack of measurement convergence, make it difficult to derive a comprehensive definition of the construct in childhood and adolescence. Research shows substantial variability in instruments used to measure guilt in children and adolescents.Purpose: The aim is to discuss existing contributions, illustrating the empirical validity of the available instruments used to measure guilt and identifying the nature of their theoretical backgrounds among children and adolescents.Methods: A systematic search was conducted using the following databases: PsycINFO, PsycARTICLES, MEDLINE, Scopus, Web of Science, and PubMed (all years up to February 19, 2020). Search terms were compiled into three concepts for all databases: “measure,” “guilt,” and “childhood/adolescence.” In addition, a search was conducted to detect the gray literature.Results: After removing the duplicates, a total of 1,408 records were screened, resulting in the identification of 166 full-text articles to be further scrutinized. Upon closer examination, there was consensus that 148 of those studies met the study inclusion criteria or were not retrieved. Twenty-five studies were included in the quality assessment. The data were organized on three main categories: (1) interpersonal or prosocial guilt; (2) intrapunitive guilt or that referring to an excessive sense of responsibility; (3) not specifying a theoretical construct. A great heterogeneity in psychometric evaluations and substantial variability in guilt construct emerged. The construct most represented and supported by valid instruments was interpersonal or prosocial guilt. Analysis of the gray literature showed that some instruments were not immediately available to the clinical and scientific communities.Conclusions: The studies analyzed and selected for qualitative review employed various instruments to measure guilt. Results confirmed what is widely documented in the literature about substantial variability in instruments used to measure guilt. We argue the need to develop measures that assess currently overlooked dimensions of guilt and to provide further additional information about the psychometric proprieties of the available developed instruments.
Prescribing patterns and costs associated with erectile dysfunction drugs in England: a time trend analysis
Authors: Bell Colette , Hadi Muhammad Abdul , Khanal Saval , Paudyal Vibhu 
Published: December 2020

BackgroundSildenafil and tadalafil are recommended firstline treatments for erectile dysfunction (ED). Sildenafil was legally reclassified to a ‘pharmacy’ medicine in the UK in 2018.AimTo assess the prescribing patterns and costs associated with prescribing of ED drugs in England, and to investigate the link between prescribing and deprivation, regional demography, and legal reclassification.Design & settingAnalyses were conducted of publicly available government data from various sources pertaining to primary care prescribing and demographics in England.MethodPrescribing and cost data from January 2009 to November 2019 were extracted and adjusted for inflation, male populations, and regional deprivation.ResultsBetween 2009 and 2019 the rate of prescribing, measured as the number of items per 1000 men, increased by 110%. In 2019, the rate of prescribing of ED medicines in the most deprived areas was 21.0% higher than the rate observed in least deprived areas. The northern regions of England approximately had a 50% higher rate of prescribing compared with London. A 1.3% annual increase in the number of prescription items was observed between 2018 and 2019 for Sildenafil, with a 5.8% increase observed from 2017–2018.ConclusionThe two-fold increase in the rate of primary care prescriptions in the past 10 years suggests that more men are being screened for, or seeking help for, ED. The higher rate of prescribing offers opportunity for monitoring of linked risk factors, such as diabetes mellitus, dyslipidaemia, and vascular disorders, in deprived populations. Reclassification of sildenafil had a modest impact on prescribing practices.
Si no hay tabaco que no se note. Prácticas fumatorias En el fortin La Perra (1883-1885), La Pampa
Authors: Tapia Alicia , Pineau Virginia , Auge Melisa Ayelén 
Published: December 2020

En este artículo se presentan los resultados obtenidos a partir del análisis de microrrestos vegetales identificados en una pipa artesanal hallada en el Fortín La Perra, departamento Loventue, La Pampa. En dicho sitio se instaló un pequeño asentamiento militar que formó parte de una línea de fortines planteada a partir de 1882, como estrategia para ejercer la vigilancia y el control del territorio del cual fueron expulsados los ranqueles durante la Conquista del Desierto en 1879. El patrón de asentamiento de este sitio así como los materiales vítreos, faunísticos y de metal recuperados han sido objeto de diferentes estudios ya publicados. En este caso, el estudio específico del contenido de la pipa constituye un nuevo aporte a los conocimientos alcanzados sobre la falta de provisiones y el aislamiento al que fueron sometidos los integrantes de las guarniciones militares de fines del siglo XIX, ubicadas en el interior de la pampa seca.
Investigación geofísica en la fosa de Santa Lucía, Uruguay
Authors: De los Santos Gregoraschuk Jorge Eduardo , Araneda Cabrera Manuel , Araneda Avendaño Álvaro , Ramos Cavallo Julián Andrés , Corbo Camargo Fernando , Flaquer Barrios Alfonso Nicolás 
Published: December 2020

En este trabajo se investiga el sector sudeste de la fosa tectónica del río Santa Lucía, ubicada al sur de Uruguay, mediante el empleo de métodos geofísicos de exploración. En particular, gravimetría, sondeos magnetotelúricos y eléctricos (SEV y Tomografía eléctrica). El interés de explorar dicha fosa radica en determinar su geometría, reconocer la posible existencia de acuíferos profundos, su desarrollo y la factibilidad de termalismo debido al gradiente geotérmico (3°C cada 100 m de profundidad). Se adquirieron, procesaron e invirtieron 121 estaciones gravimétricas dispuestas en cuatro perfiles y diez sondeosmagnetotelúricos (MT). Los resultados indican que la fosa se profundiza hacia el SE, alcanzando espesores sedimentarios que superan los 800 m. Por lo tanto, a partir de nuestros resultados se podría extraer agua entre los 800-900m de profundidad en dicha zona (SE). Los episodios arenosos o fracturados en profundidad podrían albergar aguas termales, cuya temperatura sería de aproximadamente 36 to 40°C a partir del gradiente geotérmico del país.
Acesso da criança na atenção primária í saúde: uma revisão integrativa
Authors: Marques Ribeiro Ascenso Adeniane , Saraiva Aguiar Ricardo 
Published: December 2020

Objetivo: Analisar os fatores relacionados a garantia do acesso de crianças na atenção primária í saúde. Método: Trata-se de uma revisão integrativa da literatura realizada a partir das bases de dados ScIELO, LILACS e BDENF. Para a definição da pergunta norteadora utilizou-se a estratégia PICO e quanto ao processo de seleção dos estudos, utilizou-se o fluxograma PRISMA. As buscas abrangeram o perí­odo de 2014 a 2019, sendo selecionados os artigos disponí­veis em português, na í­ntegra e no formato original. Resultados: Identificou-se barreiras relacionadas ao acesso, principalmente organizacional, e fragilidades na articulação entre os diferentes ní­veis e locais de prestação de serviços. Conclusão: Faz-se necessário uma atuação de modo multiprofissional com a participação ativa do enfermeiro. Além disso, entende-se que precisa existir ví­nculo empático, longitudinal e integral entre os profissionais de saúde e as famí­lias.
Materiały kolekcyjne owsa w Krajowym Centrum Roślinnych Zasobów Genowych
Authors: Dziubińska Dorota , Podyma Wiesław 
Published: December 2020

Owies jest jednym z najważniejszych zbóż uprawianych na świecie. Ziarno owsa znajduje zastosowanie w produkcji żywności, pasz oraz w przemyśle. W celu zachowania różnorodności gatunków owsa w Krajowym Centrum Roślinnych Zasobów Genowych powstała kolekcja obejmująca zarówno uprawne jak i dzikie jego formy. Zadaniem kolekcji jest zarówno gromadzenie jak również ocena i charakterystyka zebranych obiektów.
Wartość pokarmowa wybranych mieszanek zbóż jarych z roślinami bobowatymi grubonasiennymi
Authors: Wiśniewska Magdalena , Boros Danuta , Zych Józef 
Published: December 2020

Materiał badawczy obejmował trzy mieszanki dwuskładnikowe form jarych jęczmienia i pszenżyta z łubinem wąskolistnym i jęczmienia z grochem oraz ich komponenty pochodzące z siewu czystego. Wartość pokarmową zbadano na podstawie składu chemicznego ziarna/nasion i wartości odżywczej białka określonej in vitro oraz bezpośrednio w układzie modelowym na szczurach. Zboża jare i rośliny bobowate grubonasienne, jak również mieszanki skomponowane z ich udziałem, różniły się istotnie pod względem zawartości składników odżywczych i antyżywieniowych. Wyniki pokazały znaczący wpływ doboru składników na wartość pokarmową mieszanek zbóż jarych z roślinami bobowatymi. Udział łubinu wąskolistnego w mieszance przyczynił się do wzrostu zawartości białka i poprawy jego jakości, ale jednocześnie zwiększył ilość włókna pokarmowego. Odnosi się to w szczególności do mieszanki z jęczmieniem. Zboża, ze względu na dużą zawartość skrobi, podwyższały wartość energetyczną mieszanki. Na podstawie wskaźników chemicznych i badań bilansowych na zwierzętach stwierdzono większą wartość odżywczą białka mieszanek zbóż z roślinami bobowatymi niż ich komponentów z siewu czystego. Mieszanka jęczmienia jarego, odmiany Radek, z grochem, odmiany Model, charakteryzowała się najlepszym składem chemicznym i najwyższą wartością odżywczą białka, określoną metodami in vitro i in vivo.
Entrepreneurship Keunggulan Bersaing : Identitas Merek, Inovasi Produk dan Orientasi Pasar Study UMKM Hijab di Kabupaten Bekasi
Authors: Junedi Junedi 
Published: December 2020

Perkembangan permintaan busana muslim, tumbuhnya komunitas-komunitas hijab seperti Hijabers Community, Hijabers Mom, dan lain-lain sampai diselenggarakannya beragam bazar, peragaan busana muslim, kegiatan hijab class di kampus, perusahaan, pengajian, ataupun arisan sangat mendukung tumbuhnya bisnis busana muslim.
Secara khusus, topik membangun identitas merek UMKM tampaknya memiliki peran dalam sebuah usaha guna membantu untuk menciptakan ide kreatifitas. Inovasi produk mempunyai peran penting dalam keunggulan bersaing. Menilai peluang pasar membutuhkan pengukuran besar secara keseluruhan dan kondisi persaingan bisnis, oleh karena itu untuk memahami kondisi pasar perlu adanya orientasi pasar dalam dunia usaha. Keunggulan bersaing seolah menjadi ajang kompetisi bagi para pelaku usaha, oleh sebab itu para pelaku usaha harus selalu menciptakan hal-hal yang baru dalam membuat produknya.

Kata kunci : Identitas Merek (IM), Inovasi Produk (IP), Orientasi Pasar (OP) dan Keunggulan Bersaing (KB).
How to lose a hand: Sensory updating drives disembodiment
Authors: Pfister Roland , Klaffehn Annika L. , Kalckert Andreas , Kunde Wilfried , Dignath David 
Published: December 2020

AbstractBody representations are readily expanded based on sensorimotor experience. A dynamic view of body representations, however, holds that these representations cannot only be expanded but that they can also be narrowed down by disembodying elements of the body representation that are no longer warranted. Here we induced illusory ownership in terms of a moving rubber hand illusion and studied the maintenance of this illusion across different conditions. We observed ownership experience to decrease gradually unless participants continued to receive confirmatory multisensory input. Moreover, a single instance of multisensory mismatch – a hammer striking the rubber hand but not the real hand – triggered substantial and immediate disembodiment. Together, these findings support and extend previous theoretical efforts to model body representations through basic mechanisms of multisensory integration. They further support an updating model suggesting that embodied entities fade from the body representation if they are not refreshed continuously.
ARES IV: Probing the Atmospheres of the Two Warm Small Planets HD 106315c and HD 3167c with the HST/WFC3 Camera*
Authors: Guilluy Gloria , Gressier Amélie , Wright Sam , Santerne Alexandre , Jaziri Adam Yassin , Edwards Billy , Changeat Quentin , Modirrousta-Galian Darius , Skaf Nour , Al-Refaie Ahmed , Baeyens Robin , Bieger Michelle Fabienne , Blain Doriann , Kiefer Flavien , Morvan Mario , Mugnai Lorenzo V. , Pluriel William , Poveda Mathilde , Zingales Tiziano , Whiteford Niall , Yip Kai Hou , Charnay Benjamin , Leconte Jérémy , Drossart Pierre , Sozzetti Alessandro , Marcq Emmanuel , Tsiaras Angelos , Venot Olivia , Waldmann Ingo , Beaulieu Jean-Philippe 
Published: December 2020

Abstract
We present an atmospheric characterization study of two medium-sized planets bracketing the radius of Neptune: HD 106315c (R
P = 4.98 ± 0.23 R
⊕) and HD 3167c (

R
⊕). We analyze spatially scanned spectroscopic observations obtained with the G141 grism (1.125–1.650 μm) of the Wide Field Camera 3 (WFC3) on board the Hubble Space Telescope. We use the publicly available Iraclis pipeline and TauREx3 atmospheric retrieval code and detect water vapor in the atmosphere of both planets, with an abundance of

(∼5.68σ) and

(∼3.17σ) for HD 106315c and HD 3167c, respectively. The transmission spectrum of HD 106315c also shows possible evidence of ammonia absorption (

, even if it is not significant), while carbon dioxide absorption features may be present in the atmosphere of HD 3167c in the ∼1.1–1.6 μm wavelength range (

, ∼3.28σ). However, the CO2 detection appears significant, and it must be considered carefully and put into perspective. Indeed, CO2 presence is not explained by 1D equilibrium chemistry models, and it could be due to possible systematics. The additional contributions of clouds, CO, and CH4 are discussed. HD 106315c and HD 3167c will be interesting targets for upcoming telescopes such as the James Webb Space Telescope and the Atmospheric Remote-sensing Infrared Exoplanet Large-survey.
Metal-poor Stars Observed with the Southern African Large Telescope
Authors: Rasmussen Kaitlin C. , Zepeda Joseph , Beers Timothy C. , Placco Vinicius M. , Depagne Éric , Frebel Anna , Dietz Sarah , Hartwig Tilman 
Published: December 2020

Abstract
We present the first release of a large-scale study of relatively bright (V < 13.5) metal-poor stars observed with the Southern African Large Telescope (SALT), based on high-resolution spectra of 50 stars with a resolving power of R ∼ 40,000 and S/N ∼ 20 per pixel at 4300 Å. The elemental abundances of C, Sr, Ba, and Eu are reported, as well as several α-elements (Mg, Ca, Sc, Ti, and V) and iron-peak elements (Mn, Co, Ni, and Zn). We find a diverse array of abundance patterns, including several consistent with the signatures of carbon-enhanced metal-poor CEMP-i and CEMP-r stars. We find that 15 of 50 (30%) are carbon enhanced (with [C/Fe] > +0.70), and that a large fraction (26 of 50, 52%) are enhanced in r-process elements. Among the r-process-enhanced stars, five are strongly enhanced r-II ([Eu/Fe] > +1.0) stars (two of which are newly discovered) and 21 are newly discovered moderately enhanced r-I (+0.3 ≤ [Eu/Fe] ≤ +1.0) stars. There are eight stars in our sample that, on the basis of their abundances and kinematics, are possible members of the metal-weak thick-disk population. We also compare our measured abundances to progenitor-enrichment models, and find that the abundance patterns for the majority of our stars can be attributed to a single (rather than multiple) enrichment event.
Fast Outflows in Hot Dust-obscured Galaxies Detected with Keck/NIRES
Authors: Finnerty Luke , Larson Kirsten , Soifer B. T. , Armus Lee , Matthews Keith , Jun Hyunsung D. , Moon Dae-Sik , Melbourne Jason , Gomez Percy , Tsai Chao-Wei , Díaz-Santos Tanio , Eisenhardt Peter , Cushing Michael 
Published: December 2020

Abstract
We present rest-frame optical spectroscopic observations of 24 Hot Dust-Obscured Galaxies (Hot DOGs) at redshifts 1.7–4.6 with KECK/NIRES. Our targets are selected, based on their extreme red colors, to be the highest-luminosity sources from the WISE infrared survey. In 20 sources with well-detected emission, we fit the key [O iii], Hβ, Hα, [N ii], and [S ii] diagnostic lines to constrain physical conditions. Of the 17 targets with a clear detection of the [O iii]λ5007 Å emission line, 15 display broad blueshifted and asymmetric line profiles, with widths ranging from 1000 to 8000 km s−1 and blueshifts up to 3000 km s−1. These kinematics provide strong evidence for the presence of massive ionized outflows of up to

, with a median of

. As many as eight sources show optical emission line ratios consistent with vigorous star formation. Balmer-line star formation rates, uncorrected for reddening, range from 30 to 1300

, with a median of

. Estimates of the SFR from Spectral Energy Distribution fitting of mid- and far-infrared photometry suggest significantly higher values. We estimate the central black hole masses to be of order

, assuming the present-day

relation. The bolometric luminosities and the estimated masses of the central black holes of these galaxies suggest that many of the active galactic nucleus-dominated Hot DOGs are accreting at or above their Eddington limit. The combination of ongoing star formation, massive outflows, and high Eddington ratios suggest Hot DOGs are a transitional phase in galaxy evolution.
Using SDO/AIA to Understand the Thermal Evolution of Solar Prominence Formation
Authors: Viall Nicholeen M. , Kucera Therese A. , Karpen Judith T. 
Published: December 2020

Abstract
We investigated the thermal properties of prominence formation using time series analysis of Solar Dynamics Observatory's Atmospheric Imaging Assembly (SDO/AIA) data. Here, we report the first time-lag measurements derived from SDO/AIA observations of a prominence and its cavity on the solar limb, made possible by AIA's different wave bands and high time resolution. With our time-lag analysis, which tracks the thermal evolution using emission formed at different temperatures, we find that the prominence cavity exhibited a mixture of heating and cooling signatures. This is in contrast to prior time-lag studies of multiple active regions that chiefly identified cooling signatures and very few heating signatures, which is consistent with nanoflare heating. We also computed time lags for the same pairs of SDO/AIA channels using output from a one-dimensional hydrodynamic model of prominence material forming through thermal nonequilibrium (TNE). We demonstrate that the SDO/AIA time lags for flux tubes undergoing TNE are predicted to be highly complex, changing with time and location along the flux tube, and are consistent with the observed time-lag signatures in the cavity surrounding the prominence. Therefore, the time-lag analysis is a sensitive indicator of the heating and cooling processes in different coronal regions. The time lags calculated for the simulated prominence flux tube are consistent with the behavior deduced from the AIA data, thus supporting the TNE model of prominence formation. Future investigations of time lags predicted by other models for the prominence mass could be a valuable method for discriminating among competing physical mechanisms.
The Catalogue for Astrophysical Turbulence Simulations (CATS)
Authors: Burkhart B. , Appel S. M. , Bialy S. , Cho J. , Christensen A. J. , Collins D. , Federrath C. , Fielding D. B. , Finkbeiner D. , Hill A. S. , Ibáñez-Mejía J. C. , Krumholz M. R. , Lazarian A. , Li M. , Mocz P. , Mac Low M.-M. , Naiman J. , Portillo S. K. N. , Shane B. , Slepian Z. , Yuan Y. 
Published: December 2020

Abstract
Turbulence is a key process in many fields of astrophysics. Advances in numerical simulations of fluids over the last several decades have revolutionized our understanding of turbulence and related processes such as star formation and cosmic ray propagation. However, data from numerical simulations of astrophysical turbulence are often not made public. We introduce a new simulation-oriented database for the astronomical community: the Catalogue for Astrophysical Turbulence Simulations (CATS), located at www.mhdturbulence.com. CATS includes magnetohydrodynamic (MHD) turbulent box simulation data products generated by the public codes athena++, arepo, enzo, and flash. CATS also includes several synthetic observational data sets, such as turbulent HI data cubes. We also include measured power spectra and three-point correlation functions from some of these data. We discuss the importance of open-source statistical and visualization tools for the analysis of turbulence simulations such as those found in CATS.
Magnetogenesis by Wave-driven Momentum Exchange
Authors: Ochs Ian E. , Fisch Nathaniel J. 
Published: December 2020

Abstract
When multiple species interact with an electrostatic ion acoustic wave, they can exchange momentum, despite the lack of momentum in the field itself. The resulting force on the electrons can have a curl, and thus give rise to compensating electric fields with curl on magnetohydrodynamic timescales. As a result, a magnetic field can be generated. Surprisingly, in some astrophysical settings, this mechanism can seed magnetic fields with growth rates even larger than through the traditional Biermann battery.
Model Dependence of Bayesian Gravitational-wave Background Statistics for Pulsar Timing Arrays
Authors: Hazboun Jeffrey S. , Simon Joseph , Siemens Xavier , Romano Joseph D. 
Published: December 2020

Abstract
Pulsar timing array (PTA) searches for a gravitational-wave background (GWB) typically include time-correlated “red” noise models intrinsic to each pulsar. Using a simple simulated PTA data set with an injected GWB signal we show that the details of the red noise models used, including the choice of amplitude priors and even which pulsars have red noise, have a striking impact on the GWB statistics, including both upper limits and estimates of the GWB amplitude. We find that the standard use of uniform priors on the red noise amplitude leads to 95% upper limits, as calculated from one-sided Bayesian credible intervals, that are less than the injected GWB amplitude 50% of the time. In addition, amplitude estimates of the GWB are systematically lower than the injected value by 10%–40%, depending on which models and priors are chosen for the intrinsic red noise. We tally the effects of model and prior choice and demonstrate how a “dropout” model, which allows flexible use of red noise models in a Bayesian approach, can improve GWB estimates throughout.
Une expérience communautaire d’entraide
Authors: Fiatte Vincent 
Published: December 2020

L’hôtel social de l’EDVO est une structure d’hébergement pour personnes concernées par l’addiction. Inspirée du Modèle Minnesota, elle s’appuie sur l’entraide des pairs, la responsabilisation et la gestion des émotions. La crise sanitaire liée au Covid-19 et l’annonce du plan de confinement a pris l’équipe et les résidents au dépourvu. Passée la stupeur, l’équipe a fait le choix de garder la structure ouverte et de laisser les 28 résidents en autonomie complète. Cet article relate leur expérience et en tire un bilan.