bluuebunny/crossref_metadata_2025_split huggingface dataset:
Prisión preventiva, una mirada desde la lógica jurídica
Authors: López Aquino Miguel Rolando , Torres Toledo Christian Hanesh 
Published: May 2023

La exposición de motivos del presente ensayo tiene como objetivo identificar una visión epistemológica de la prueba conducente al dictamen de prisión preventiva para lo cual se requiere contar con estándares que respondan a la lógica jurídica, asi como también ponderar la libertad del individuo que no se ha comprobado fehacientemente el hecho punible que se le imputa.
Asumiendo que el mejor modelo para evaluar la prueba en el proceso judicial es el de la probabilidad lógica, es necesario reconocer que el razonamiento judicial en materia de hechos será siempre probabilístico y que ningún conjunto de prueba, por rico y completo que sea, permitirá certezas racionales.
Precisamente las normas de prueba ofrecen criterios para la fase de decisión, al no haber lugar a automatismos, la decisión sobre medidas cautelares personales en el proceso penal debe contener partes internas predefinidas con preceptiva explicación judicial y capítulos para el fumus comissi delicti y el periculum libertatis.
PROSPECTS FOR THE APPLICATION OF MACHINE LEARNING IN LOGISTICS
Authors: Михов О.М. 
Published: May 2023

В статье рассмотрены направления использования такого инструмента как машинное обучение в современном логистическом менеджменте. Цель исследования заключается в выявлении перспективных направлений применения машинного обучения в логистике. В статье рассматриваются различные возможности использования современных цифровых технологий как основы для методов машинного обучения и будущие направления применения полученных алгоритмов в управлении логистическими процессами. В результате исследования формируется концепция управления транспортными потоками в городской среде посредством использования машинного обучения.
The article discusses the directions of using such a tool as machine learning in modern logistics management. The purpose of the study is to identify promising areas for the application of machine learning in logistics. The article discusses various possibilities of using modern digital technologies as the basis for machine learning methods and future directions of using the obtained algorithms in the management of logistics processes. As a result of the research, the concept of traffic management in an urban environment is formed through the use of machine learning.
IMPROVING THE METHODOLOGY FOR ASSESSING THE SOCIO-ECONOMIC DEVELOPMENT OF THE REGION BASED ON THE ASSESSMENT OF ITS INNOVATIVE POTENTIAL (ON THE EXAMPLE OF THE KRASNODAR TERRITORY)
Authors: Рыбалко А.Н. 
Published: May 2023

В данной статье на базе ранее разработанной автором методики оценки социально-экономического развития региона представлена усовершенствованная методика с учетом инновационной составляющей. По мнению автора, развитие рассматриваемого направления призвано обеспечить переход от сырьевой модели развития региона к инновационной, тем самым обеспечив его устойчивое развитие. Представленные показатели подобраны при помощи методов логического и корреляционно-регрессионного анализа региональных инновационных процессов. В статье пошагово рассмотрен процесс вычисления каждого из предложенных автором показателей. Адекватность применения данной методики с предложенным автором набором показателей для оценки социально-экономического развития региона была подтверждена проведенным корелляционным анализом, показавшим, что усовершенствованная методика оценки выгодно отличается от предыдущей своей инновационной составляющей и наиболее подробно раскрывает весь потенциал региона для инвестора.
In this article, on the basis of the methodology developed earlier by the author for assessing the socio-economic development of the region, an improved methodology for assessing this region, taking into account the innovative component, is presented. According to the author, the development of the considered direction is designed to ensure the transition from the raw material model of the region's development to an innovative model, thereby ensuring its sustainable development. The presented indicators are selected using the methods of logical and correlation-regression analysis of regional innovation processes. The article step-by-step discusses the process of calculating each of the indicators proposed by the author. The adequacy of the application of this methodology with the set of indicators proposed by the author to assess the socio-economic development of the region was confirmed by a correlation analysis, which showed that the improved calculation method compares favorably with its previous innovative component and will reveal in the most detail the full potential of the region for the investor when choosing an investment region.
Aneurysmal Bone Cyst presenting Incidentally as a Traumatic Foot Injury
Authors: Jose Tom , Mathew Thomas , Oguntade Ayotunde , Tripathy Rajinder , Iqbal Awais 
Published: May 2023

Introduction: Aneurysmal bone cyst is a rare, non-neoplastic lesion affecting the metaphysis of long bones and vertebrae, characterized by blood-filled spaces separated by fibrous septae.
Aims and objectives: In this study, we present a case of an aneurysmal bone cyst in a 7-year-old child with characteristic X-ray findings to increase awareness as early diagnosis and treatment can limit disability.
An aneurysmal bone cyst is a rare, benign neoplastic lesion affecting the metaphysis of long bones and vertebrae, characterized by blood-filled spaces separated by fibrous septae.[1] Diagnosis depends on typical features of magnetic resonance imaging, and confirmation by biopsy is essential before surgery is considered.
We present an aneurysmal bone cyst in a 7-year-old child with characteristic X-ray findings. Diagnosis of ABC should be suspected in young patients presenting with limb pain or swelling, and pain disproportionate to the mechanism of injury could indicate pathologic fracture. Early detection of ABC is possible as an incidental finding by closely examining routine X-rays so that appropriate treatment can be instituted early and complications like pathologic fractures can be avoided. This case will help to increase awareness as early diagnosis and treatment can limit disability.
Obscuring Environment and X-Ray Variability of Compact Symmetric Objects Unveiled with XMM-Newton and NuSTAR
Authors: Sobolewska Małgosia , Siemiginowska Aneta , Migliori Giulia , Ostorero Luisa , Stawarz Łukasz , Guainazzi Matteo 
Published: May 2023

Abstract
Compact symmetric objects (CSOs) show radio features such as jets, lobes, and hot spots, which are contained within their host galaxies, and likely represent a recent radio activity. A subpopulation of CSOs with high intrinsic X-ray column densities has been inferred from shallow, soft X-ray band exposures, and observed to cluster in the linear radio size versus 5 GHz radio power plane, which suggests that a dense circumnuclear medium may dramatically influence the growth of compact radio structures. Here, we report on the first detection of two CSOs, 2021+614 and J1511+0518, at energies above 10 keV with NuSTAR. We model the NuSTAR data jointly with the new XMM-Newton data of J1511+0518, and with the archival XMM-Newton data of 2021+614. A toroidal reprocessor model fits the data well and allows us to robustly confirm the X-ray properties of the CSO absorbers and continuum. In both sources, we find intrinsic X-ray absorbing column densities in excess of 1023 cm−2, hard photon indices of the primary emission, Γ ∼ 1.4–1.7, Fe Kα line emission, and variability of the intrinsic X-ray flux density on the timescale of years. The studied X-ray continua are dominated by the primary power-law emission at energies above 3 keV, and by the scattered component at energies below 3 keV. An additional soft X-ray component, modeled with a hot, collisionally ionized plasma with temperature kT ∼ 1 keV, is required by the XMM-Newton data in J1511+0518, which is corroborated by the tentative evidence for the extension in the archival Chandra image of the source.
The Fast X-Ray Transient XRT 210423 and Its Host Galaxy
Authors: Eappachen D. , Jonker P. G. , Levan A. J. , Quirola-Vásquez J. , Torres M. A. P. , Bauer F. E. , Dhillon V. S. , Marsh T. , Littlefair S. P. , Ravasio M. E. , Fraser M. 
Published: May 2023

Abstract
Fast X-ray Transients (FXTs) are X-ray flares with durations ranging from a few hundred seconds to a few hours. Possible origins include the tidal disruption of a white dwarf by an intermediate-mass black hole, a supernova shock breakout, or a binary neutron star merger. We present the X-ray light curve and spectrum as well as deep optical imaging of the FXT XRT 210423, which has been suggested to be powered by a magnetar produced in a binary neutron star merger. Our Very Large Telescope and Gran Telescopio Canarias (GTC) observations began on 2021 May 6, thirteen days after the onset of the flare. No transient optical counterpart is found in the 1.″ (3σ) X-ray uncertainty region of the source to a depth g

s
= 27.0 AB mag. (We use the word “counterpart” for any transient light in a wave band other than the original X-ray detection wave band, whereas the word “host” refers to the host galaxy.) A candidate host lies within the 1.″ X-ray uncertainty region with a magnitude of 25.9 ± 0.1 in the GTC/HiPERCAM g

s
filter. Due to its faintness, it was not detected in other bands, precluding a photometric redshift determination. We detect two additional candidate host galaxies: one with z
spec = 1.5082 ± 0.0001 and an offset of 4.″2 ± 1.″ (37 ± 9 kpc) from the FXT, and another one with

z

phot

=

1.04

−
0.14

+
0.22

and an offset of 3.″6 ± 1.″ (30 ± 8 kpc). Based on the properties of all the prospective hosts, we favor a binary neutron star merger, as previously suggested in the literature, as the explanation for XRT 210423.
A Statistical Search for a Uniform Trigger Threshold in Solar Flares from Individual Active Regions
Authors: Carlin Julian B. , Melatos Andrew , Wheatland Michael S. 
Published: May 2023

Abstract
Solar flares result from the sudden release of energy deposited by subphotospheric motions into the magnetic field of the corona. The deposited energy accumulates secularly between events. One may interpret the observed event statistics as resulting from a state-dependent Poisson process in which the instantaneous flare rate is a function of the stress in the system and a flare becomes certain as the stress approaches a threshold set by the microphysics of the flare trigger. If the system is driven fast, and if the threshold is static and uniform globally, a cross-correlation is predicted between the size of a flare and the forward waiting time to the next flare. This cross-correlation is broadly absent from the Geostationary Operational Environmental Satellite (GOES) soft X-ray flare database. One also predicts higher cross-correlations in active regions where the shapes of the waiting time and size distributions match. Again, there is no evidence for such an association in the GOES data. The data imply at least one of the following: (i) the threshold at which a flare is triggered varies in time; (ii) the rate at which energy is driven into active regions varies in time; (iii) historical flare catalogs are incomplete; or (iv) the description of solar flares as resulting from a buildup and release of energy, once a threshold is reached, is incomplete.
The Magnetic Sensitivity of the (250–278 nm) Fe ii Polarization Spectrum
Authors: Afonso Delgado David , del Pino Alemán Tanausú , Trujillo Bueno Javier 
Published: May 2023

Abstract
This paper presents a theoretical investigation of the polarization and magnetic sensitivity of the near-ultraviolet (near-UV) solar spectral lines of Fe ii between 250 and 278 nm. In recent years, UV spectropolarimetry has become key to uncovering the magnetism of the upper layers of the solar chromosphere. The unprecedented data obtained by the CLASP2 suborbital space experiment across the Mg ii h and k lines around 280 nm are a clear example of the capabilities of near-UV spectropolarimetry for magnetic field diagnostics throughout the whole solar chromosphere. Recent works have pointed out the possible complementary diagnostic potential of the many Fe ii lines in the unexplored spectral region between 250 and 278 nm, but no quantitative analysis of the polarization and magnetic sensitivity of those spectral lines has been carried out yet. To study the polarization signals in these spectral lines, we create a comprehensive atomic model including all the atomic transitions resulting in strong spectral lines. We then study the magnetic sensitivity of the linear and circular polarization profiles in a semiempirical model representative of the quiet Sun. We present a selection of Fe ii spectral lines with significant linear and circular polarization signals and evaluate their diagnostic capabilities by studying their formation heights and magnetic sensitivity through the action of the Hanle and Zeeman effects. We conclude that when combined with the CLASP2 spectral region these Fe ii lines are of interest for the inference of magnetic fields throughout the solar chromosphere, up to near the base of the corona.
Early Results from GLASS-JWST. XIX. A High Density of Bright Galaxies at z ≈ 10 in the A2744 Region
Authors: Castellano Marco , Fontana Adriano , Treu Tommaso , Merlin Emiliano , Santini Paola , Bergamini Pietro , Grillo Claudio , Rosati Piero , Acebron Ana , Leethochawalit Nicha , Paris Diego , Bonchi Andrea , Belfiori Davide , Calabrò Antonello , Correnti Matteo , Nonino Mario , Polenta Gianluca , Trenti Michele , Boyett Kristan , Brammer G. , Broadhurst Tom , Caminha Gabriel B. , Chen Wenlei , Filippenko Alexei V. , Fortuni Flaminia , Glazebrook Karl , Mascia Sara , Mason Charlotte A. , Menci Nicola , Meneghetti Massimo , Mercurio Amata , Metha Benjamin , Morishita Takahiro , Nanayakkara Themiya , Pentericci Laura , Roberts-Borsani Guido , Roy Namrata , Vanzella Eros , Vulcani Benedetta , Yang Lilan , Wang Xin 
Published: May 2023

Abstract
We report the detection of a high density of redshift z ≈ 10 galaxies behind the foreground cluster A2744, selected from imaging data obtained recently with NIRCam on board JWST by three programs—GLASS-JWST, UNCOVER, and DDT#2756. To ensure robust estimates of the lensing magnification μ, we use an improved version of our model that exploits the first epoch of NIRCam images and newly obtained MUSE spectra and avoids regions with μ > 5 where the uncertainty may be higher. We detect seven bright z ≈ 10 galaxies with demagnified rest frame −22 ≲ M
UV ≲ −19 mag, over an area of ∼37 arcmin2. Taking into account photometric incompleteness and the effects of lensing on luminosity and cosmological volume, we find that the density of z ≈ 10 galaxies in the field is about 10× (3×) larger than the average at M
UV ≈ −21 ( −20) mag reported so far. The density is even higher when considering only the GLASS-JWST data, which are the deepest and the least affected by magnification and incompleteness. The GLASS-JWST field contains five out of seven galaxies, distributed along an apparent filamentary structure of 2 Mpc in projected length, and includes a close pair of candidates with M
UV < −20 mag having a projected separation of only 16 kpc. These findings suggest the presence of a z ≈ 10 overdensity in the field. In addition to providing excellent targets for efficient spectroscopic follow-up observations, our study confirms the high density of bright galaxies observed in early JWST observations but calls for multiple surveys along independent lines of sight to achieve an unbiased estimate of their average density and a first estimate of their clustering.
M92 (NGC 6341) Is a Metal-complex Globular Cluster with an Atypical Primordial Population
Authors: Lee Jae-Woo 
Published: May 2023

Abstract
We present a multiple stellar population study of the metal-poor globular cluster (GC) M92 (NGC 6341), which is long known for the substantial metallicity dispersion, using our own photometric system. We find two groups with slightly different mean metallicities, the metal-poor (MP) stars with [Fe/H]
hk
= −2.412 ± 0.03 and the metal-rich (MR) ones with −2.282 ± 0.002. The MP constitutes about 23% of the total mass with a more central concentration. Our populational tagging based on the [C/Fe]
ch
and [N/Fe]
nh
provides the mean n(P):n(I):n(E) = 32.2:31.6:36.2 (±2.4), where P, I, and E denote the primordial, intermediate, and extreme populations, respectively. Our populational number ratio is consistent with those of others. However, the MP has a significantly different populational number ratio than the mean value, and the domination of the primordial population in the MP is consistent with observations of Galactic GCs that less massive GCs contain larger fractions of the primordial population. Structural and constituent differences between the MP and MR may indicate that M92 is a merger remnant in a dwarf galaxy environment, consistent with recent suggestions that M92 is a GC in a dwarf galaxy or a remnant nucleus of the progenitor galaxy. Discrepancy between our method and those widely used for the Hubble Space Telescope photometry exists in the primordial population. Significant magnesium and oxygen depletions of −0.8 and −0.3 dex, respectively, and helium enhancement of ΔY ≳ 0.03 are required to explain the presence of this abnormal primordial group. No clear explanation is available with limited information of detailed elemental abundances.
There’s More to Life than O2: Simulating the Detectability of a Range of Molecules for Ground-based, High-resolution Spectroscopy of Transiting Terrestrial Exoplanets
Authors: Currie Miles H. , Meadows Victoria S. , Rasmussen Kaitlin C. 
Published: May 2023

Abstract
Within the next decade, atmospheric O2 on Earth-like M-dwarf planets may be accessible with visible–near-infrared (NIR), high-spectral-resolution, ground-based extremely large telescope (ELT) instruments. However, the prospects for using ELTs to detect environmental properties that provide context for O2 have not been thoroughly explored. Additional molecules may help indicate planetary habitability, rule out abiotically generated O2, or reveal alternative biosignatures. To understand the accessibility of environmental context using ELT spectra, we simulate high-resolution transit transmission spectra of previously generated evolved terrestrial atmospheres. We consider inhabited preindustrial and Archean Earth–like atmospheres, and lifeless worlds with abiotic O2 buildup from CO2 and H2O photolysis. All atmospheres are self-consistent with M2V–M8V dwarf host stars. Our simulations include explicit treatment of systematic and telluric effects to model high-resolution spectra for Giant Magellan Telescope (GMT), Thirty Meter Telescope (TMT), and European ELT (E-ELT) configurations for systems 5 and 12 pc from Earth. Using the cross-correlation technique, we determine the detectability of major species in these atmospheres: O2, O3, CH4, CO2, CO, H2O, and C2H6. Our results suggest that CH4 and CO2 are the most accessible molecules for terrestrial planets transiting a range of M-dwarf hosts using an E-ELT-, TMT-, or GMT-sized telescope, and that the O2 NIR and H2O 0.9 μm bands may also be accessible with more observation time. Although this technique still faces considerable challenges, the ELTs will provide access to the atmospheres of terrestrial planets transiting earlier-type M-dwarf hosts that may not be possible using JWST.
Le cirque en France à l’épreuve de l’École républicaine : histoire d’une scolarisation différée (1880-1974)
Authors: Froissart Tony , Lemonnier Jean-Marc , Dutheil Frédéric 
Published: May 2023

Si les historiens et sociologues ont relaté les difficultés enseignantes à s’emparer des activités physiques artistiques comme support d’une éducation physique scolaire (EPS) depuis 1980-1990 en France, cette contribution se tourne vers la période précédant ces structurations institutionnelle, professionnelle et scolaire. L’enjeu réside dans le questionnement d’une absence scolaire du cirque de près d’un siècle (1880-1974) et les motifs et valeurs qui y président. Il s’agit d’interroger les tenants et aboutissants d’une pratique physique très ancienne mais durablement absente de l’école française durant le xx e siècle alors qu’elle recouvre certains codes de la gymnastique ou du sport. En centrant nos focales sur l’EPS, l’évolution de la pratique du cirque et la lente structuration de la profession circassienne, notre intention est d’apprécier le procès de non scolarisation du cirque, à l’aune des représentations sociales, des attentes institutionnelles et conceptuelles depuis la fin du xix e aux années 1970. Nous montrerons notamment que le cirque ne peut ou ne doit pas être scolarisé durant ces neuf décennies en croisant plusieurs types de sources, qu’elles relèvent de textes institutionnels, d’ouvrages de concepteurs scolaires, de revues spécialisées ou d’affiches de cirque.
Donner une part de soi. La transférabilité des ressources et dispositions dans l’encadrement des classes de mer
Authors: Guillaud Étienne 
Published: May 2023

Les entretiens et observations menés au sein d’établissements assurant l’encadrement de classes de mer soulignent comment le travail « d’éducation au milieu marin » prend des formes variées selon les propriétés sociales des éducateurs eux-mêmes et de l’organisation plus générale du travail. Occuper un poste d’éducateur de classe de mer est une activité professionnelle peu formalisée, où il est possible pour le travailleur de transférer des savoirs et savoir-faire constitués en dehors de l’espace de travail. L’importation d’un capital social local peut ainsi devenir un élément déterminant dans la constitution d’une offre éducative. La nature comme les modalités de cette transférabilité s’avèrent toutefois variables selon les configurations.
Specializing Within a Prelicensure Nursing Program: An Innovative Clinical Design
Authors: Barnum Leslie , Mutascio Jennifer 
Published: May 2023

Background:
Traditionally, prelicensure nursing programs aim to give students exposure to several different populations in preparation for becoming a registered nurse. Those who begin a career in a specialty such as pediatrics have often had little exposure and experience with the aptitudes and knowledge needed to be workforce ready.

Method:
An innovative clinical cohort program was designed to prepare students better to graduate with a strong specialty foundation already established. Following the American Association of Colleges of Nursing recommendation to seek academic-practice partnerships, this cohort model was established between a university and freestanding children's hospital. Students enrolled in this program complete all required didactic and simulation coursework in the traditional curriculum. In addition, they participate in frequent clinical experiences at the children's hospital throughout the entire program.

Results:
Students graduating from this program have received adequate preparation to graduate, pass NCLEX, and are competent in all necessary general nursing principles. At the same time, they are well versed in pediatric nursing and comfortable caring for this specialty population.

Conclusion:

Prelicensure students can specialize in pediatrics while meeting all general requirements of a traditional Bachelor of Science in Nursing program. This novel clinical cohort design could serve as a model to change standard programming and better meet the needs of our practice partners.

[
J Nurs Educ
. 2023;62(8):475–478.]