bluuebunny/crossref_metadata_2025_split huggingface dataset:
‘Smart Museum’ in China: From technology labs to sustainable knowledgescapes
Authors: Wang Siyi , Duan Yong , Yang Xiaofei , Cao Chenxing , Pan Shouyong 
Published: January 2023

Abstract
Technology has played an instrumental role as a catalyst for museum digitization. Museums are enhancing their methods of management, interpretation, and representation with digitalization, networking, and intelligentization, suggesting a move toward seamless integration, presentation, and delivery of cultural heritage resources. China’s Smart Museum Project, launched in 2014, does not foster digital museums or virtual museums but a new kind of museum composed of dynamic perceptual systems for and between people (online and offline visitors, museum staff, and board) and objects (artifacts, storage areas, galleries, and facilities) through new technologies, including cloud computing, big data, and artificial intelligence. This article advocates the kind of museum digitization seen in the Smart Museum Project, which promotes a digital museum-based paradigm that integrates new technologies with comprehensive perception, ubiquitous interconnection, and syncretic applications. Here, we provide historical context for its development and its impact on museum activities, with further elaboration on the definition, connotation, framework, and outreach of the smart museum. We believe that museums should embrace digital opportunities to evolve from a computer-based technology lab to sustainable, synergistic, and smart knowledgescapes.
Quantitative Microstructural Analysis by Correlative EPMA/EBSD/BSE Electron Microscopies Applied to Nuclear Ceramic
Authors: Delville Rémi , Verwerft Marc 
Published: January 2023

Abstract
Electron microscopy maps were acquired in a mixed-oxide nuclear ceramic to probe independently and optimally grain structure [by Electron BackScattered Diffraction (EBSD)], porosity [by high-resolution BackScattered Electron imaging (BSE)], and elemental distributions [by Electron Probe MicroAnalysis (EPMA) in a separate instrument]. The maps were programmatically correlated spatially and integrated into a single multi-dimensional dataset allowing a correlative approach to assess the interdependence of key ceramic microstructural properties. Through the extraction of statistically representative non-random quantitative correlations between grain size, elemental enrichment, and intra-granular porosity that can be related to solid-state processes, the potency of the method is illustrated. The multi-layered hybrid maps produced by fusing data from the different acquisitions offer novel and unique insights into contiguous crystallographic, microstructural, and chemical features.
Ultrastructural characterization of the scale cover of crypticAspidiotusspp. (Hemiptera: Diaspididae) and the ovipositor of their parasitoids
Authors: Serrana Joeselle M , Almarinez Billy Joel M , Barrion Alberto T , Amalin Divina M 
Published: January 2023

AbstractCorrectly identifying target insect pests and their natural enemies is important in biological control management programs. In the scale insect outbreak that devastated the coconut industry of the Philippines in 2009, the misidentification of the destructive pest population resulted in an unsuccessful biological control application. The scale cover has been proposed as a diagnostic feature to identify the cryptic Aspidiotus species from one another. Here, we examined the scale cover of three Aspidiotus species at higher magnification using scanning electron microscopy (SEM) to validate the observed difference in scale cover characteristics reported in previous literature. SEM observations revealed that the cryptic species A. destructor and A. rigidus scale covers are ultrastructurally similar, having irregularly arranged and highly agglutinated wax ribbons, whereas A. nerii has highly agglutinated wax ribbons arranged in an overlapping concentric pattern. Additionally, a comparative observation of the ovipositor of the hymenopteran parasitoids directly associated with the two cryptic Aspidiotus species, A. rigidus and A. destructor, was done to provide structural evidence that links ovipositor structure to host specificity. The structure of the ovipositor tip of the hymenopteran parasitoids directly associated with the two Aspidiotus species examined under SEM is congruent with their mode of parasitization.
General- and Oral-Health-Related Predisposing Factors for Interrupting Military Service in the Finnish Defence Forces
Authors: Patinen Pertti , Tanner Tarja , Honkanen Jesse , Tjäderhane Leo , Päkkilä Jari , Anttonen Vuokko , Kämppi Antti 
Published: January 2023

ABSTRACT

Introduction
Finland’s security policy relies heavily on its own independent national defense, which is based on conscription. In 2011, 26,492 conscripts started their military service in Finland. Of these, 1,706 interrupted their military service and 191 changed to civilian service. Conscripts who interrupt their service seem to have an increased tendency to smoking, alcohol consumption, and taking snuff, which previous studies suggest to have strong associations with the need for restorative dental treatment and with lower socioeconomic status. The aim of this study was to compare the general and oral health habits between Finnish conscripts who interrupt their service and those who completed their military service and to find out what general- and oral-health-related factors could be used in predicting interruption of service.

Methods
The study population consisted of 13,819 conscripts taking an oral examination during the service. Of these, 8,449 answered a computer-based anamnestic questionnaire and 264 interrupted their service.
Predisposing factors on the anamnestic questionnaire for interrupting military service were evaluated by using a binary logistic regression model. The statistically significant factors were selected to form a sum variable which finally consisted of seven predisposing questions. Odds ratio (OR) values and 95% confidence intervals were calculated for each question and for the sum variable. Predictive accuracy was assessed by area under the receiver-operating curve.

Results
The most obvious predisposing factor among those who interrupted their service compared to the reference group was lack of weekly physical exercise (OR = 5.80). The risk for interruption of military service was 68.6 times higher in cases where a subject exhibited six predisposing factors out of seven compared to those who had none.

Conclusion
As a conclusion, a set of statistically chosen anamnestic questions could help identify conscripts who have an increased risk of interruption of military service in addition to a risk of dental problems.
A Review of Verbal and Written Patient Handoffs Applicable to the U.S. Military’s Expeditionary Care System
Authors: Kunce Nicholas E , Lyon Arthur , Carlton Duncan , Jeyarajah Theepica , Strayhorn Catherine M , Lopreiato Joseph , Wilson Ramey 
Published: January 2023

ABSTRACT

Introduction
Long considered a danger point in patient care, handoffs and patient care transitions contribute to medical errors and adverse events. Without standardization of patient handoffs, communication breakdowns arise and critical patient information is lost. Minimal training and informal learning have led to a lack of understanding the process involved in this vital aspect of patient care. In 2017, the U.S. Army commissioned a report to study the process of patient handoffs and identify training gaps. Our report summarizes that process and makes recommendations for implementation.

Materials and Methods
Scoping literature review of 139 articles published between 1999 and 2017 using PubMed, CINAHL, Cochrane, and Medline databases. Verbal tools for handoffs were evaluated against 12 criteria including patient ID, history, current situation, contingency planning, ability to ask questions, ownership, and read back. Written tools were evaluated against a matrix of 126 casualty/treatment attributes.

Results
Among verbal communication protocols, the highest scoring handoff mnemonics were HAND ME AN ISOBAR, IPASS the BATON, and I-SBARQ. Among written handoff tools, the highest scoring documents were the Special Operations Forces (SOF) Mechanism, Injuries, Signs, and Treatment (MIST) Casualty Treatment Card and the Department of Defense (DD) Form 1380 Tactical Combat Casualty Care (TCCC) Card. Four critical process elements for patient handoffs and transfers were identified: (1) interactive communications, (2) limited interruptions, (3) a process for verification, and (4) an opportunity to review any relevant historical data.

Conclusions
The findings in this review highlight the need for standardized tools and techniques for patient handoffs in the U.S. Military’s expeditionary care system. Future research is needed to trial verbal and nonverbal handoffs under field conditions to gather observational data to assess effectiveness. The results of our gap analyses may provide researchers insight for determining which handoffs to study. If standardized handoffs are utilized, training programs should incorporate the four critical elements into their curricula.
The Source of Normativity
Authors: Bengson John , Cuneo Terence , Shafer-Landau Russ 
Published: January 2023

AbstractThis paper seeks to clarify one of the deepest questions about the source or ground of normativity, while also presenting an essence-based approach to answering it. We call it the ‘Arché Question.’ Though all metanormative theories must address this question, very few realists have explicitly grappled with the challenge it poses; those who have appear to deny any need to give an answer. After critically discussing extant realist responses, this paper outlines an essence-based approach to answering the Arché Question that draws on theoretical resources forged in recent advances in post-modal metaphysics.
Nystatin is commonly prescribed as prophylaxis in children beyond the neonatal age
Authors: Jayawardena-Thabrew Harshani , Warris Adilia ,   The PASOAP Group, Ferreras-Antolin Laura 
Published: January 2023

Abstract
The indications for nystatin as prophylaxis or treatment are limited. In the PASOAP (Pediatric Antifungal Stewardship Optimizing Antifungal Prescription) study, high use of nystatin in hospitalized children beyond the neonatal age was observed. In this report, we present the data on nystatin use in infants and children ≥ 3 months who participated in the PASOAP study. Nystatin was prescribed mainly for prophylaxis. Congenital heart disease, cystic fibrosis, and chronic renal disease were the most commonly reported conditions in children receiving prophylactic nystatin. There is sparse evidence supporting the use of nystatin prophylaxis beyond neonates; trials in specific pediatric patient groups are required.
Orthopedic infections due to Trichosporon species: Case series and literature review
Authors: Mello López Andrés , da Silva Neto Luiz Alves , de Oliveira Vítor Falcão , de Carvalho Vladimir Cordeiro , de Oliveira Priscila Rosalba Domingos , Lima Ana Lúcia Lei Munhoz 
Published: January 2023

Abstract
Reports of orthopedic fungal infections caused by Trichosporon species are extremely scarce, thus we aimed to describe a case series and review the cases published in the literature. Patients were retrospectively included if a previous culture of bone, joint, or soft tissues had resulted positive for Trichosporon species along with a clinical diagnosis of an orthopedic infection. Eight patients were included with diverse orthopedic conditions, most of them cases of osteomyelitis. The main isolated species was Trichosporon asahii. All patients were treated with antifungals, mainly voriconazole, and surgical management, resulting in high rates of clinical improvement and low associated mortality.
Solar plasma characterization in Kappa (κ)-modified polytropic turbomagnetic GES-model perspective
Authors: Sarma Pankaj , Karmakar Pralay Kumar 
Published: January 2023

ABSTRACT
The gravitoelectrostatic sheath (GES) model for exploring the surface emission mechanism of the solar wind plasma (SWP), transformed from the solar interior plasma (SIP) via the solar surface boundary (SSB), has recently been reformulated in different conditions. It considers the realistic plasma key factors previously remaining unaddressed. This continued study elaborately explores the diverse GES-microphysical features influenced mainly by the plasma non-thermality, bulk polytropicity, magneto-activity, logatropicity, etc. It shows that, in the SIP (SWP), the electric potential is κ-insensitive, the Mach number is κ-sensitive, and the current density is κ-sensitive (insensitive). The Mach number is insensitive and the current density is insensitive (sensitive) to the relative temperature, Te/Ti, in the SIP (SWP). The inhomogeneity-induced GES properties are illuminated with the gradient-scale behaviours of the relevant physical variables on both SIP and SWP scales. The self-organization of the bi-scaled solar plasma system is well confirmed by mapping the electric and gravity field gradients in a defined colour phase space illustratively alongside reliability check-ups. A judicious application of the newly derived model-structuring equations results in a non-thermally modified form of the equivalent κ-Bohm sheath criterion featuring the GES formation alongside electric current-flow analyses. Its reliability is validated with a sensible comparison with the extremal cases in fair corroboration with the previous sheath scenarios extensively reported elsewhere. The relevancy of our investigation on the solar multiparametric variations in the GES fabric is lastly bolstered in light of the recent solar astronomic scenarios, such as SolO and PSP.
The shocked molecular layer in RCW 120
Authors: Kirsanova M S , Pavlyuchenkov Ya N , Olofsson A O H , Semenov D A , Punanova A F 
Published: January 2023

ABSTRACT
Expansion of wind-blown bubbles or H ii regions lead to formation of shocks in the interstellar medium, which compress surrounding gas into dense layers. We made spatially and velocity-resolved observations of the RCW 120 photo-dissociation region (PDR) and nearby molecular gas with CO(6–5) and 13CO(6–5) lines and distinguished a bright CO-emitting layer, which we related with the dense shocked molecular gas moving away from the ionizing star due to expansion of H ii region. Simulating gas density and temperature, as well as brightness of several CO and C+ emission lines from the PDR, we found reasonable agreement with the observed values. Analysing gas kinematics, we revealed the large-scale shocked PDR and also several dense environments of embedded protostars and outflows. We observe the shocked layer as the most regular structure in the CO(6–5) map and in the velocity space, when the gas around Young stellar objects (YSOs) is dispersed by the outflows.
The TRAPUM L-band survey for pulsars in Fermi-LAT gamma-ray sources
Authors: Clark C J , Breton R P , Barr E D , Burgay M , Thongmeearkom T , Nieder L , Buchner S , Stappers B , Kramer M , Becker W , Mayer M , Phosrisom A , Ashok A , Bezuidenhout M C , Calore F , Cognard I , Freire P C C , Geyer M , Grießmeier J-M , Karuppusamy R , Levin L , Padmanabh P V , Possenti A , Ransom S , Serylak M , Venkatraman Krishnan V , Vleeschower L , Behrend J , Champion D J , Chen W , Horn D , Keane E F , Künkel L , Men Y , Ridolfi A , Dhillon V S , Marsh T R , Papa M A 
Published: January 2023

ABSTRACT
More than 100 millisecond pulsars (MSPs) have been discovered in radio observations of gamma-ray sources detected by the Fermi Large Area Telescope (LAT), but hundreds of pulsar-like sources remain unidentified. Here, we present the first results from the targeted survey of Fermi-LAT sources being performed by the Transients and Pulsars with MeerKAT (TRAPUM) Large Survey Project. We observed 79 sources identified as possible gamma-ray pulsar candidates by a Random Forest classification of unassociated sources from the 4FGL catalogue. Each source was observed for 10 min on two separate epochs using MeerKAT’s L-band receiver (856–1712 MHz), with typical pulsed flux density sensitivities of $\sim 100\, \mu$Jy. Nine new MSPs were discovered, eight of which are in binary systems, including two eclipsing redbacks and one system, PSR J1526−2744, that appears to have a white dwarf companion in an unusually compact 5 h orbit. We obtained phase-connected timing solutions for two of these MSPs, enabling the detection of gamma-ray pulsations in the Fermi-LAT data. A follow-up search for continuous gravitational waves from PSR J1526−2744 in Advanced LIGO data using the resulting Fermi-LAT timing ephemeris yielded no detection, but sets an upper limit on the neutron star ellipticity of 2.45 × 10−8. We also detected X-ray emission from the redback PSR J1803−6707 in data from the first eROSITA all-sky survey, likely due to emission from an intrabinary shock.
A deep radius valley revealed by Kepler short cadence observations
Authors: Ho Cynthia S K , Van Eylen Vincent 
Published: January 2023

ABSTRACT
The characteristics of the radius valley, i.e. an observed lack of planets between 1.5 and 2 Earth radii at periods shorter than about 100 d, provide insights into the formation and evolution of close-in planets. We present a novel view of the radius valley by refitting the transits of 431 planets using Kepler 1-min short cadence observations, the vast majority of which have not been previously analysed in this way. In some cases, the updated planetary parameters differ significantly from previous studies, resulting in a deeper radius valley than previously observed. This suggests that planets are likely to have a more homogeneous core composition at formation. Furthermore, using support vector machines, we find that the radius valley location strongly depends on orbital period and stellar mass and weakly depends on stellar age, with $\partial \log {\left(R_{\rm p, \text{valley}} \right)}/ \partial \log {P} = -0.096_{-0.027}^{+0.023}$, $\partial \log {\left(R_{\rm p, \text{valley}} \right)}/ \partial \log {M_{\star }} = 0.231_{-0.064}^{+0.053}$, and $\partial \log {\left(R_{\rm p, \text{valley}} \right)}/ \partial \log {\left(\text{age} \right)} = 0.033_{-0.025}^{+0.017}$. These findings favour thermally driven mass-loss models such as photoevaporation and core-powered mass-loss, with a slight preference for the latter scenario. Finally, this work highlights the value of transit observations with a short photometric cadence to precisely determine planet radii, and we provide an updated list of precisely and homogeneously determined parameters for the planets in our sample.
Discovery of a resolved white dwarf–brown dwarf binary with a small projected separation: SDSS J222551.65+001637.7AB
Authors: French Jenni R , Casewell Sarah L , Dupuy Trent J , Debes John H , Manjavacas Elena , Martin Emily C , Xu Siyi 
Published: January 2023

ABSTRACT
We present the confirmation of SDSS J222551.65+001637.7AB as a closely separated, resolved, white dwarf–brown dwarf binary. We have obtained spectroscopy from GNIRS and seeing-limited Ks-band imaging from NIRI on Gemini North. The target is spatially resolved into its constituent components: a 10926 ± 246 K white dwarf, with log g = 8.214 ± 0.168 and a mass of 0.66$^{+0.11}_{-0.06}$ M⊙, and an L4 brown dwarf companion, which are separated by 0.9498 ± 0.0022 arcsec. We derive the fundamental properties of the companion from the Sonora–Bobcat evolutionary models, finding a mass of 25–53 MJup and a radius of 0.101–0.128 R⊙ for the brown dwarf, at a confidence level of 1σ. We use wdwarfdate to determine the age of the binary as $1.97^{+4.41}_{-0.76}$ Gyr. A kinematic analysis shows that this binary is likely a member of the thick disc. The distance to the binary is 218$^{+14}_{-13}$ pc, and hence the projected separation of the binary is 207$^{+13}_{-12}$ au. Whilst the white dwarf progenitor was on the main sequence the binary separation would have been 69 ± 5 au. SDSS J222551.65+001637.7AB is the third closest spatially resolved white dwarf–brown dwarf binary after GD 165AB and PHL 5038AB.
Detecting the non-Gaussianity of the 21-cm signal during reionization with the wavelet scattering transform
Authors: Greig Bradley , Ting Yuan-Sen , Kaurov Alexander A 
Published: January 2023

ABSTRACT
Detecting the 21-cm hyperfine transition from neutral hydrogen in the intergalactic medium is our best probe for understanding the astrophysical processes driving the Epoch of Reionization (EoR). The primary means for a detection of this 21-cm signal is through a statistical measurement of the spatial fluctuations using the 21-cm power spectrum (PS). However, the 21-cm signal is non-Gaussian meaning the PS, which only measures the Gaussian fluctuations, is suboptimal for characterizing all of the available information. The upcoming Square Kilometre Array (SKA) will perform a deep, 1000 h observation over 100 deg2 specifically designed to recover direct images of the 21-cm signal. In this work, we use the Wavelet Scattering Transform (WST) to extract the non-Gaussian information directly from these 2D images of the 21-cm signal. The key advantage of the WST is its stability with respect to statistical noise for measuring non-Gaussian information, unlike the bispectrum whose statistical noise diverges. In this work, we specifically focus on introducing a novel method to isolate non-Gaussian information from an image and apply this methodology to individual mock 21-cm images to quantify the strength of the non-Gaussian information contained within a single image. For example, at 150 (177) MHz (z ∼ 8.5 and ∼7) for a fiducial reionization model we recover a signal to noise of ∼5 (8) for the non-Gaussian information assuming perfect foreground removal and ∼2 (3) assuming foreground wedge avoidance.
The exoplanetary magnetosphere extension in Sun-like stars based on the solar wind–solar UV relation
Authors: Reda Raffaele , Giovannelli Luca , Alberti Tommaso , Berrilli Francesco , Bertello Luca , Del Moro Dario , Di Mauro Maria Pia , Giobbi Piermarco , Penza Valentina 
Published: January 2023

ABSTRACT
The Earth’s magnetosphere extension is controlled by the solar activity level via solar wind properties. Understanding such a relation in the Solar system is important for predicting the condition of exoplanetary magnetospheres near Sun-like stars. We use measurements of a chromospheric proxy, the Ca ii K index, and solar wind OMNI parameters to connect the solar activity variations, on decennial time-scales, to the solar wind properties. The data span the period 1965–2021, which almost entirely covers the last five solar cycles. Using both cross-correlation and mutual information analysis, we find a 3.2-yr lag of the solar wind speed with respect to the Ca ii K index. Analogously, a 3.6-yr lag is found once we consider the dynamic pressure. A correlation between the solar wind dynamic pressure and the solar ultraviolet emission is found and used to derive the Earth’s magnetopause standoff distance. Moreover, the advantage of using a chromospheric proxy, such as the Ca ii K index, creates the possibility to extend the relation found for the Sun to Sun-like stars, by linking stellar variability to stellar wind properties. The model is applied to a sample of Sun-like stars as a case study, where we assume the presence of an Earth-like exoplanet at 1 au. Finally, we compare our results with previous estimates of the magnetosphere extension for the same set of Sun-like stars.