bluuebunny/crossref_metadata_2025_split huggingface dataset:
Criminal legal means for the glorification of the armed aggression of the russian federation in Ukraine
Authors: NOVIKOVA K. 
Published: September 2024

The article is devoted to the study of criminal law sanctions for glorification of the armed aggression of the russian federation in Ukraine (Article 4362 of the Criminal Code of Ukraine (hereinafter – the CC of Ukraine)). The author establishes that the current version of Article 4362 of the CC of Ukraine in terms of sanctions regulation has a number of shortcomings which require legislative resolution. In particular, it is necessary to exclude from Part 2 of this Article such an additional type of punishment as confiscation of property due to its inconsistency with the provisions of the General Part of the CC of Ukraine, or to increase the upper limit of the punishment in the form of imprisonment to six years in order to turn this criminal offense into a grave one. It would also be advisable to supplement the sanction of Part 1 of this Article with such a type of punishment as restriction of liberty. This would eliminate the legislative “vacuum” between probationary supervision and imprisonment. It would also be logical to synchronize the upper limit of imprisonment under Part 1 of Article 4362 of the CC of Ukraine and the lower limit of the same type of punishment under Part 3 of Article 4362 of the CC of Ukraine by setting the amount of imprisonment in Part 3 of Article 4362 of the CC of Ukraine as “three years” instead of “five years”. In addition, the analysis of judicial practice has also shown the need to rethink the types and amounts of punishment for glorification. After all, in 88 % of cases, convicts were released from serving their sentences with probation. This indicates that courts do not always perceive glorification as an offense with a high degree of social danger, and therefore, in their minds, there is an opinion that the types and amounts of punishment for glorification established by law do not correspond to the real degree of social danger. In this regard, it is advisable to reduce the amount of punishment for glorification or to move to less severe types of punishment. This will allow judges to impose real punishment instead of exemption from serving a sentence, which will increase the effectiveness of criminal law measures for glorification.
A Data-driven Search For Mid-infrared Excesses Among Five Million Main-sequence FGK Stars
Authors: Contardo Gabriella , Hogg David W. 
Published: September 2024

Abstract
Stellar infrared excesses can indicate various phenomena of interest, from protoplanetary disks to debris disks, or (more speculatively) techno-signatures along the lines of Dyson spheres. In this paper, we conduct a large search for “extreme” infrared excesses, designed as a data-driven contextual anomaly detection pipeline. We focus our search on FGK stars close to the main sequence to favor nonyoung host stars. We look for excess in the mid-infrared, unlocking a large sample to search in while favoring extreme IR excess akin to the ones produced by extreme debris disks (EDDs) and/or planetary collision events. We combine observations from ESA Gaia Data Release 3, the Two Micron All-Sky Survey, and the unWISE version of NASA’s Wide-field Infrared Survey Explorer (WISE), and create a catalog of 4,898,812 stars with G < 16 mag. We consider a star to have an excess if it is substantially brighter in the W1 and W2 bands than what is predicted from an ensemble of machine learning models trained on the data, taking optical and near-infrared information as input features. We apply a set of additional cuts (derived from the machine learning models and the objects’ astronomical features) to avoid false positives and identify a set of 53 objects, including one previously identified EDD candidate. The typical infrared-excess fractional luminosities we find are in the range 0.005–0.1, consistent with previous EDD candidates and potential planetary collision events.
A Data-constrained Analysis for Joule Heating as a Solar Active Region Atmosphere Heating Mechanism. I. Sunspot Umbral Light Bridge
Authors: Yalim M. S. , Frisse M. , Beck C. , Choudhary D. P. , Prasad A. , Nayak S. S. , Zank G. P. 
Published: September 2024

Abstract
Understanding the mechanisms underlying the heating of the solar atmosphere is a fundamental problem in solar physics. The lower atmosphere of the Sun (i.e., photosphere and chromosphere) is composed of weakly ionized plasma. This results in anisotropic dissipation of electric currents by Coulomb and Cowling resistivities. Joule heating due to dissipation of currents perpendicular to the magnetic field by Cowling resistivity has been demonstrated to be the main mechanism for the heating of a sunspot umbral light bridge located in NOAA AR 12002 on 2014 March 13. Here, we focus on the same target region and demonstrate the importance of further constraining our Joule heating model using observational data in addition to magnetic field, namely plasma temperature calculated from the inversion of spectroscopic data obtained from the Interferometric BI-dimensional Spectrometer instrument of the ground-based Dunn Solar Telescope. As a parameter in our analysis, temperature is demonstrated to have the highest sensitivity after magnetic field. We show that the heating of the light bridge is a highly dynamic event that necessitates utilization of 3D spatially resolved observational data for temperature rather than a 1D temperature stratification based on theoretical/semiempirical solar atmosphere models. Our improved data-constrained analysis using spatially resolved temperatures shows that the entire light bridge is heated by the proposed mechanism, and yields heating rate values that are consistent with our previous study.
A New Deep Learning Model to Detect Gamma-Ray Bursts in the AGILE Anticoincidence System
Authors: Parmiggiani N. , Bulgarelli A. , Castaldini L. , De Rosa A. , Di Piano A. , Falco R. , Fioretti V. , Macaluso A. , Panebianco G. , Ursi A. , Pittori C. , Tavani M. , Beneventano D. 
Published: September 2024

Abstract
The AGILE space mission was launched in 2007 to study X-ray and gamma-ray astrophysics. AGILE operated in spinning mode from 2009 until 2024 February 14, when it re-entered the Earth’s atmosphere. This work uses data acquired from the AGILE anticoincidence system (ACS) from 2019 January 1 to 2022 December 31. The ACS is designed to reject charged background particles. It also detects X-ray photons in the 50–200 KeV energy range and saves each panel count rate in the telemetry as ratemeter data, a time series with a resolution of 1.024 s. We developed a method that uses a deep learning model to predict the background count rates of the AGILE ACS top panel (perpendicular to the pointing direction of the payload detectors) using the satellite’s orbital parameters as input. Then, we use the difference between predicted and acquired count rates to detect gamma-ray bursts (GRB). We trained the model with a background-only data set. After the training, the model can predict the ACS count rates with a mean reconstruction error of 3.8%. We used the GRBs listed in the GRBweb catalog to search for significant anomalies in the ACS data. We extracted light curves of 140 bins of 1.024 s for each GRB from the AGILE ACS to cover the trigger time of the GRBs. The model detected 39 GRBs with a significance of σ ≥ 3. The results contain four GRBs detected for the first time in the AGILE data.
Shocking and Mass Loss of Compact Donor Stars in Type Ia Supernovae
Authors: Wong Tin Long Sunny , White Christopher J. , Bildsten Lars 
Published: September 2024

Abstract
Type Ia supernovae arise from thermonuclear explosions of white dwarfs accreting from a binary companion. Following the explosion, the surviving donor star leaves at roughly its orbital velocity. The discovery of the runaway helium subdwarf star US 708, and seven hypervelocity stars from Gaia data, all with spatial velocities ≳900 km s−1, strongly support a scenario in which the donor is a low-mass helium star or a white dwarf. Motivated by these discoveries, we perform three-dimensional hydrodynamical simulations with the Athena++ code, modeling the hydrodynamical interaction between a helium star or helium white dwarf and the supernova ejecta. We find that ≈0.01–0.02 M
⊙ of donor material is stripped, and explain the location of the stripped material within the expanding supernova ejecta. We continue the postexplosion evolution of the shocked donor stars with the MESA code. As a result of entropy deposition, they remain luminous and expanded for ≈105–106 yr. We show that the postexplosion properties of our helium white dwarf donor agree reasonably with one of the best-studied hypervelocity stars, D6-2.
General Relativistic Radiation Magnetohydrodynamics Simulations of Precessing Tilted Super-Eddington Disks
Authors: Asahina Yuta , Ohsuga Ken 
Published: September 2024

Abstract
We perform a three-dimensional general relativistic radiation magnetohydrodynamics simulation of a tilted super-Eddington accretion disk around a spinning black hole (BH). The disk, which tilts and twists as it approaches the BH, precesses while maintaining its shape. The gas is mainly ejected around the rotation axis of the outer part of the disk rather than around the spin axis of the BH. The disk precession changes the ejection direction of the gas with time. The radiation energy is also released in approximately the same direction as the outflow, so the precession is expected to cause a quasiperiodic time variation of the observed luminosity. The timescale of the precession is about 10 s for a 10 M
⊙ BH and for the radial extent of a disk of several tens of gravitational radii, where M
⊙ is the solar mass. This timescale is consistent with the frequency of the low-frequency quasiperiodic oscillation (0.01–1 Hz) observed in some ultraluminous X-ray sources.
The Chandra Source Catalog Release 2 Series
Authors: Evans Ian N. , Evans Janet D. , Martínez-Galarza J. Rafael , Miller Joseph B. , Primini Francis A. , Azadi Mojegan , Burke Douglas J. , Civano Francesca M. , D’Abrusco Raffaele , Fabbiano Giuseppina , Graessle Dale E. , Grier John D. , Houck John C. , Lauer Jennifer , McCollough Michael L. , Nowak Michael A. , Plummer David A. , Rots Arnold H. , Siemiginowska Aneta , Tibbetts Michael S. 
Published: September 2024

Abstract
The Chandra Source Catalog (CSC) is a virtual X-ray astrophysics facility that enables both detailed individual source studies and statistical studies of large samples of X-ray sources detected in Advanced CCD Imaging Spectrometer and High Resolution Camera-I imaging observations obtained by the Chandra X-ray Observatory. The catalog provides carefully curated, high-quality, and uniformly calibrated and analyzed tabulated positional, spatial, photometric, spectral, and temporal source properties, as well as science-ready X-ray data products. The latter includes multiple types of source- and field-based FITS format products that can be used as a basis for further research, significantly simplifying follow-up analysis of scientifically meaningful source samples. We discuss in detail the algorithms used for the CSC Release 2 Series, including CSC 2.0, which includes 317,167 unique X-ray sources on the sky identified in observations released publicly through the end of 2014, and CSC 2.1, which adds Chandra data released through the end of 2021 and expands the catalog to 407,806 sources. Besides adding more recent observations, the CSC Release 2 Series includes multiple algorithmic enhancements that provide significant improvements over earlier releases. The compact source sensitivity limit for most observations is ∼5 photons over most of the field of view, which is ∼2× fainter than Release 1, achieved by coadding observations and using an optimized source detection approach. A Bayesian X-ray aperture photometry code produces robust fluxes even in crowded fields and for low-count sources. The current release, CSC 2.1, is tied to the Gaia-CRF3 astrometric reference frame for the best sky positions for catalog sources.
Metrics of Astrometric Variability in the International Celestial Reference Frame. I. Statistical Analysis and Selection of the Most Variable Sources
Authors: Cigan Phil , Makarov Valeri V. , Secrest Nathan J. , Gordon David , Johnson Megan C. , Lambert Sebastien 
Published: September 2024

Abstract
Using very long baseline interferometry data for the sources that comprise the third International Celestial Reference Frame (ICRF3), we examine the quality of the formal source-position uncertainties of ICRF3 by determining the excess astrometric variability (unexplained variance) for each source as a function of time. We also quantify multiple qualitatively distinct aspects of astrometric variability seen in the data, using a variety of metrics. Average position offsets, statistical dispersion measures, and coherent trends over time as explored by smoothing the data are combined to characterize the most and least positionally stable ICRF3 sources. We find a notable dependence of the excess variance and statistical variability measures on decl., as is expected for unmodeled ionospheric delay errors and the Northern Hemisphere–dominated network geometries of most astrometric and geodetic observing campaigns.
The review of the genus Coccinella (Coleoptera, Coccinellidae) from Pakistan
Authors: Iqbal Zafar , Azad Rashid , Jin Xu , Nasir Muhammad , Bodlah Imran , Abbas Munawar , Hassan Muhammad Asghar , Ali Muhammad , Szawaryn Karol , Nie Rui-E 
Published: September 2024

This study comprehensively reviews the genus Coccinella in Pakistan and highlights Coccinella luteopicta as a new country record. The prey, host plants, distribution, and identification key of the genus Coccinella species in Pakistan were provided. Additionally, the COI (cytochrome-c-oxidase subunit I) sequence data of C. luteopicta and C. marussii were provided firstly, to identify their position.
The genus Coccinella includes seven species in Pakistan, namely, C. marussii Kapur, C. iranica Dobzhansky, C. transversalis Fabricius, C. septempunctata Linnaeus, C. transversoguttata transversoguttata Faldermann, and C. undecimpunctata Linnaeus was reviewed. Morphological features of adults, including male genital characters, and an identification key to known species in Pakistan, were presented. Also, the prey, host plants, and distribution were provided. The new data (COI-barcode) shows that C. luteopicta (Mulsant, 1866) was recorded first in Pakistan.
A brief summary of the WHO 2021 classification of adult diffuse gliomas
Authors: Lan Tien-Li , Lin Shih-Chieh , Chen Yi-Wei , Lee Yi-Yen 
Published: September 2024

Abstract
The World Health Organization (WHO) classification system for central nervous system (CNS) tumors provides a distinct framework for differentiating these tumors from other types. Notably, gliomas are the most common and clinically significant primary brain tumors. The 2021 update of the WHO classification system (WHO CNS5), building upon the 2016 edition, integrates molecular genetics with histopathological insights to enhance diagnostic precision. This update advocates a multi-layered diagnostic strategy, combining histopathology, WHO grading, and molecular genetics into a unified diagnosis, thus refining the basis for clinical research, trials, and therapeutic interventions. In WHO CNS5, gliomas are categorized into three main groups based on IDH mutation and 1p/19q codeletion status: Diffuse astrocytoma with IDH-mutant, oligodendroglioma with IDH-mutant and 1p/19q-codeletion, and glioblastoma with IDH-wildtype. The diagnostic criteria for adult diffuse gliomas include detailed descriptions of the updated classification, focusing on the molecular markers and histopathological characteristics.
Radiological and Anthropometrical Analysis of the Hip Joint Using Computed Tomography Scan in North Indian Population
Authors: Pandey Divya Nand , Garg Ravi , Kumar Chandan , Singh Chetan , Gautam Nayank 
Published: September 2024

Abstract

Background:
Anthropometric research on the hip joint has significant clinical implications, including (1) implant design and (2) avoiding implant mismatch complications, such as aseptic loosening and incorrect load distribution, which are mainly unknown in North India. The aim of this research is to ascertain the anatomical differences in the normal hip joint across individuals in North India and to statistically compare the results with global data.

Materials and Methods:
We used one hip topogram and one axial segment of the femoral head to analyze 100 people (35 females and 65 males) with normal hips between the ages of 20 and 65. In both sexes and on both sides, we determined the means of the following measurements: femoral head diameter (HD), femoral neck width (NW), femoral neck length, acetabular angle of sharp, femoral version, horizontal offset, acetabular version, and vertical offset.

Results:
The following are the mean parameters that were observed: (a) neck shaft angle (NSA) - 128.93°, (b) femoral HD = 4.29 cm, (c) femoral NW = 2.97 cm, (d) femoral neck length = 3.61 cm, (e) Acetabular angle of Sharp - 33.01°, (f) Acetabular version = 20.44°, (g) femoral Version = 21.57°, (h) horizontal offset = 3.62 cm, and (i) Vertical offset = 4.43 cm.

Conclusion:
The NSA and acetabular angle of sharp were 5°–6° more when compared to the western population while horizontal and vertical offset is comparatively less than Western population and in the Indian NSA was higher for North Eastern population than the North Indian population. The residual parameters were comparable to those found in Western literature.
Medical appraisal of Chinese military aircrew with abnormal results of coronary computed tomographic angiography
Authors: Zeng Jia , Zhao Yao , Gao Di , Lu Xiang , Dong Jing-Jing , Liu Yan-Bing , Shen Bin 
Published: September 2024

BACKGROUND
Coronary artery diseases can cause myocardial ischemia and hypoxia, angina pectoris, myocardial infarction, arrhythmia, and even sudden death led to inflight incapacitation of aircrew. As the main cause of grounding due to illness, they severe threats to the health and fighting strength of military aircrew. Early warning in an early and accurate manner and early intervention of diseases possibly resulting in inflight incapacitation are key emphases of aeromedical support in clinic.
AIM
To figure out the flight factors and clinical characteristics of military aircrew with abnormal results of coronary artery computed tomographic angiography (CTA), thereby rendering theoretical references for clinical aeromedical support of military flying personnel.
METHODS
The clinical data of 15 flying personnel who received physical examinations in a military medical center from December 2020 to June 2023 and were diagnosed with coronary artery diseases by coronary artery CTA were collected and retrospectively analyzed, and a descriptive statistical analysis was conducted on their onset age, aircraft type and clinical data.
RESULTS
The 15 military flying personnel diagnosed with coronary artery diseases by coronary artery CTA were composed of 9 pilots, 1 navigator and 5 air combat service workers. Multi-vessel disease was detected in 9 flying personnel, among which 8 (88.9%) were pilots. Flying personnel with multi-vessel disease had higher content of cholesterol, low-density lipoprotein cholesterol and apolipoprotein B than those with single-vessel disease.
CONCLUSION
Coronary artery diseases are the major heart disease for the grounding of flying personnel due to illness, which can lead to inflight incapacitation. Coronary artery CTA is conducive to early detection and early intervention treatment of such diseases in clinic.
Intracoronary thrombolysis combined with drug balloon angioplasty in a young ST-segment elevation myocardial infarction patient: A case report
Authors: She Li-Qiong , Gao De-Kui , Hong Le , Tian Yin , Wang Hui-Zhen , Huang Sheng 
Published: September 2024

BACKGROUND
The combination of acute ST-segment elevation myocardial infarction (STEMI) and gastric ulcers poses a challenge to primary percutaneous coronary intervention (PPCI), particularly for young patients. The role of drug-coated balloons (DCBs) in the treatment of de novo coronary artery lesions in large vessels remains unclear, especially for patients with STEMI. Our strategy is to implement drug balloon angioplasty following the intracoronary administration of low-dose prourokinase and adequate pre-expansion.
CASE SUMMARY
A 54-year-old male patient presented to the emergency department due to chest pain on June 24, 2019. Within the first 3 minutes of the initial assessment in the emergency room, the electrocardiogram (ECG) showed significant changes. There was atrial fibrillation with ST-segment elevation. Subsequently, atrial fibrillation terminated spontaneously and reverted to sinus rhythm. Soon after, the patient experienced syncope. The ECG revealed torsades de pointes ventricular tachycardia. A few seconds later, it returned to sinus rhythm. High-sensitivity tropon in I was normal. The diagnosis was acute STEMI. Emergency coronary angiography revealed subtotal occlusion with thrombus formation in the proximal segment of the left anterior descending artery. Considering the patient's age and history of peptic ulcer disease, after the intracoronary injection of prourokinase, percutaneous transluminal coronary angioplasty and cutting balloon angioplasty were conducted for thorough preconditioning, and paclitaxel drug-eluting balloon angioplasty was performed without any stents, achieving favorable outcomes.
CONCLUSION
A PPCI without stents may be a viable treatment strategy for select patients with STEMI, and further research is warranted.
Inquiry for Social Transformation: Black Mother Scholars Redefining Scholarly Inquiry Through Black Artistic Expression
Authors: Fearon Stephanie 
Published: September 2024

Writing, dancing, drawing, spittin’ rhymes, and other artistic expressions have long offered us, Black mother scholars, opportunities to reaffirm our humanity amid oppression (Fearon, 2023). Art offers Black mother scholars space to reconceptualise inquiry in ways that engage our families, challenge injustices, and usher social change within the educational milieu and beyond. The centring of Black artistic expression in educational research invites Black mother scholars to affirm the parts of ourselves, our families, and our communities that dominant forms of inquiry and anti-Blackness have sought to discredit. Educational research grounded in Black artistic expression compels us all to reimagine scholarly inquiry for social transformation. In this paper, I critically reflect on an arts-informed research study I led with a group of Black Canadian mothers who are adult literacy learners. In this reflexive piece, I explore how grounding research practices in Black art allows opportunities for storytelling, story listening, and Black refusal. Specifically, this paper explores the ways Black art supports researchers in addressing power differentials inherent in inquiry processes. The paper concludes with a series of reflective questions challenging scholars, especially Black mother scholars, to redefine traditional academic boundaries and recommit to social transformation through the arts.