bluuebunny/crossref_metadata_2025_split huggingface dataset:
المسؤولية الجنائية للطبيب المُمتنع عن معالجة مصابي فيروس كورونا في القوانين الصحيّة - دراسة تحليلية مقارنة بين القانونين الأردني والإماراتي
Authors: احجيله عبد الله , الفقير رائد 
Published: April 2023

يتمحور موضوع هذه الدراسة حول بيان مدى المسؤولية الجنائية للطبيب الممتنع عن معالجة مصابي فيروس كورون، وذلك في ضوء أحكام قانوني المسؤولية الطبية في الأردن ودولة الإمارات العربية المتحدة، وأمر الدفاع الأردني (23/ 2020 ) ،وتثير الدراسة عدة إشكاليات، أبرزها أن قانون المسؤولية الطبية والصحية الأردني وقانون المسؤولية الطبية الإماراتي عاقبا على جريمة امتناع الطبيب عن تقديم الخدمة الطبية للحالات الخطرة، ومن ضمنها الإصابة بفيروس كورونا، بعقوبة مخففة، وهي عقوبة الغرامة، كما حظرت المادة(5/3) من قانون المسؤولية الطبية الإماراتي على الطبيب الامتناع عن تقديم الخدمة الطبية للحالات المرضية غير الخطرة ، ولكن دون أن يُقر القانون الإماراتي عقوبةٍ جزائية لمخالفة هذا الحظر ،كما تثير الدراسة تساؤلاً جوهرياً هو - ما مدى المسؤولية الجنائية عن امتناع الطبيب عن تقديم الخدمة الطبية لمصابي فيروس كورونا في القوانين الصحية الأردنية والإماراتية؟
وقد أُتبع في هذه الدراسة المنهج التحليلي، لتحليل نصوص القوانين الصحيّة الإماراتية والأردنية المتعلقة بموضوع الدراسة ، وكذلك أُتبع المنهج المقارن، للمقارنة بين نصوص القوانين السالفة الذكر، وبيان أوجه الاتفاق والتباين بينها بشأن موضوع الدراسة.
وتوصلت الدراسة إلى عدة نتائج أهمها- أنه وعلى الرغم من خطورة جريمة امتناع الطبيب عن تقديم الخدمة الطبية للحالات الخطرة، إلا أن المشرعين الأردني والإماراتي تبنيا في قانوني المسؤولية الطبية، منهجاً مُخففاً لعقوبة هذه الجريمة التي اقتصرت على الغرامة، وذلك بخلاف المنهج المتشدد الذي جاء في أمر الدفاع الأردني (23/ 2020 ) ، الذي يتجلى بتشديد عقوبة الحبس على الطبيب الذي يمتنع عن تقديم الخدمة الطبية لمرضى كورونا، وأوصت الدراسة المشرعين الأردني والإماراتي بعدة توصيات، أهمها، النص في قانوني المسؤولية الطبية، على عقوبة الحبس لجريمة امتناع الطبيب عن تقديم الخدمة الطبية للحالات الخطرة.
Leonardo e la navigabilità dei corsi d’acqua milanesi
Authors: Candia Claudia 
Published: April 2023

The paper analyses Leonardo’s main studies concerning the navigability of Milan waterways in order to contextualize and highlight his original contributions. Not only do Leonardo’s studies outline the actual situation of such waterways, they also include new projects and innovations. Even though these are not always ascribable to Leonardo, he certainly drew and examined them himself. The analysis is based on the study of the main transformations of Milan water system and territory over the centuries.
Look into my eyes: a “faceless” avatar interviewer lowers reporting threshold for adult eyewitnesses
Authors: Hsu Che-Wei , Gross Julien , Colombo Marea , Hayne Harlene 
Published: April 2023

AbstractEvidential interviewing is often used to gather important information, which can determine the outcome of a criminal case. An interviewer’s facial features, however, may impact reporting during this task. Here, we investigated adults’ interview performance using a novel tool—a faceless avatar interviewer—designed to minimize the impact of an interviewer’s visual communication signals, potentially enhancing memory performance. Adults were interviewed about the details of a video by (1) a human-appearing avatar or a human interviewer (Experiment 1;N= 105) or (2) a human-appearing avatar or a faceless avatar interviewer (Experiment 2;N= 109). Participants assigned to the avatar interviewer condition were (1) asked whether they thought the interviewer was either computer or human operated (Experiment 1) or (2) explicitly told that the interviewer was either computer or human operated (Experiment 2). Adults’ memory performance was statistically equivalent when they were interviewed by a human-appearing avatar or a human interviewer, but, relative to the human-appearing avatar, adults who were interviewed by a faceless avatar reported more correct (but also incorrect) details in response to free-recall questions. Participants who indicated that the avatar interviewer was computer operated—as opposed to human operated—provided more accurate memory reports, but specifically telling participants that the avatar was computer operated or human operated had no influence on their memory reports. The present study introduced a novel interviewing tool and highlighted the possible cognitive and social influences of an interviewer’s facial features on adults’ report of a witnessed event.
The structure and expression of clinical questions in guidelines for most traditional Chinese medicine were poor standardized: a systematic review
Authors:   Author Affiliation:                  Centre for Evidence-Based Chinese Medicine, Beijing University of Chinese Medicine, Beijing, China, Gao Yicheng , Cao Rui , Liu Zhihan , Liu Meijun , Liao Yidi , Feng Yuting , Gaun Xinmiao , Su Chengyuan , Wang Yaqi , Fang Rui , Xiang Wenyuan , Xiang Wenyuan , Fei Yutong 
Published: April 2023

Review question / Objective: To systematically investigate the clinical question reporting of the Grading of Recommendations Assessment, Development, and Evaluation (GRADE) clinical practice guidelines (CPGs) and traditional Chinese medicine (TCM) CPGs. Eligibility criteria: The inclusion of TCM CPGs adopts the following approach: 15 CPGs were randomly selected from six authoritative Chinese medicine societies (China Association of Chinese Medicine, China Association of Traditional Chinese Medicine, Chinese Association of Integrative Medicine, China Association for Acupuncture and Moxibustion, World federation of Chinese medicine societies, Doctor Society of integrative Medicine, Chinese Medical Doctor Association) and guidelines published by other societies, less than 15 are included. We discarded older versions and duplicate published guidelines.
Nature of Intense Magnetism and Differential Rotation in Convective Dynamos of M-dwarf Stars with Tachoclines
Authors: Bice Connor P. , Toomre Juri 
Published: April 2023

Abstract
Many of the M-dwarf stars, though they are tiny and dim, are observed to possess strong surface magnetic fields and exhibit remarkably intense flaring. Such magnetism may severely impact habitability on the exoplanets now discovered nearby. The origin of the magnetism must rest with dynamo action achieved by turbulent convection coupled to rotation within the M-dwarfs. To further explore the nature and diversity of the magnetism that can result, we turn here to an extensive set of 45 global MHD simulations to explore dynamos operating within deep convective envelopes of rapidly rotating M2 (0.4 M
⊙) stars. We observe a wide range of cycle periods present in the convection zones, whose durations we find to scale with the Rossby number as Ro−1.66±0.07 in concurrence with scalings identified in simulations of more massive stars. We find a unifying relationship between the ratio of magnetic to convective kinetic energy (ME/CKE) and the degree to which the differential rotation is quenched by magnetic fields. We show that the presence of a tachocline in these model stars enhances their axisymmetric magnetic field components, leading to a surface dipole fraction on average 78% greater than an equivalent star with only a CZ, potentially shedding light on the nature of the tachocline divide through resultant effects on the spin-down rate.
Overview of the DESI Milky Way Survey
Authors: Cooper Andrew P. , Koposov Sergey E. , Allende Prieto Carlos , Manser Christopher J. , Kizhuprakkat Namitha , Myers Adam D. , Dey Arjun , Gänsicke Boris T. , Li Ting S. , Rockosi Constance , Valluri Monica , Najita Joan , Deason Alis , Raichoor Anand , Wang M.-Y. , Ting Y.-S. , Kim Bokyoung , Carrillo Andreia , Wang Wenting , Beraldo e Silva Leandro , Han Jiwon Jesse , Ding Jiani , Sánchez-Conde Miguel , Aguilar Jessica N. , Ahlen Steven , Bailey Stephen , Belokurov Vasily , Brooks David , Cunha Katia , Dawson Kyle , de la Macorra Axel , Doel Peter , Eisenstein Daniel J. , Fagrelius Parker , Fanning Kevin , Font-Ribera Andreu , Forero-Romero Jaime E. , Gaztañaga Enrique , A Gontcho Satya Gontcho , Guy Julien , Honscheid Klaus , Kehoe Robert , Kisner Theodore , Kremin Anthony , Landriau Martin , Levi Michael E. , Martini Paul , Meisner Aaron M. , Miquel Ramon , Moustakas John , Nie Jundan J. D. , Palanque-Delabrouille Nathalie , Percival Will J. , Poppett Claire , Prada Francisco , Rehemtulla Nabeel , Schlafly Edward , Schlegel David , Schubnell Michael , Sharples Ray M. , Tarlé Gregory , Wechsler Risa H. , Weinberg David H. , Zhou Zhimin , Zou Hu 
Published: April 2023

Abstract
We describe the Milky Way Survey (MWS) that will be undertaken with the Dark Energy Spectroscopic Instrument (DESI) on the Mayall 4 m telescope at the Kitt Peak National Observatory. Over the next 5 yr DESI MWS will observe approximately seven million stars at Galactic latitudes ∣b∣ > 20°, with an inclusive target selection scheme focused on the thick disk and stellar halo. MWS will also include several high-completeness samples of rare stellar types, including white dwarfs, low-mass stars within 100 pc of the Sun, and horizontal branch stars. We summarize the potential of DESI to advance understanding of the Galactic structure and stellar evolution. We introduce the final definitions of the main MWS target classes and estimate the number of stars in each class that will be observed. We describe our pipelines for deriving radial velocities, atmospheric parameters, and chemical abundances. We use ≃500,000 spectra of unique stellar targets from the DESI Survey Validation program (SV) to demonstrate that our pipelines can measure radial velocities to ≃1 km s−1 and [Fe/H] accurate to ≃0.2 dex for typical stars in our main sample. We find the stellar parameter distributions from ≈100 deg2 of SV observations with ≳90% completeness on our main sample are in good agreement with expectations from mock catalogs and previous surveys.
New Velocity Measurements of NGC 5128 Globular Clusters Out to 130 kpc: Outer Halo Kinematics, Substructure, and Dynamics*
Authors: Hughes Allison K. , Sand David J. , Seth Anil , Strader Jay , Lidman Chris , Voggel Karina , Dumont Antoine , Crnojević Denija , Mateo Mario , Caldwell Nelson , Forbes Duncan A. , Pearson Sarah , Guhathakurta Puragra , Toloba Elisa 
Published: April 2023

Abstract
We present new radial velocity measurements from the Magellan and the Anglo-Australian Telescopes for 175 previously known and 121 newly confirmed globular clusters (GCs) around NGC 5128, the nearest accessible massive early-type galaxy at D = 3.8 Mpc. Remarkably, 28 of these newly confirmed GCs are at projected radii

>
50
′

(≳54 kpc), extending to ∼130 kpc, in the outer halo where few GCs had been confirmed in previous work. We identify several subsets of GCs that spatially trace halo substructures that are visible in red giant branch star maps of the galaxy. In some cases, these subsets of GCs are kinematically cold, and may be directly associated with and originate from these specific stellar substructures. From a combined kinematic sample of 645 GCs, we see evidence for coherent rotation at all radii, with a higher rotation amplitude for the metal-rich GC subpopulation. Using the tracer mass estimator, we measure a total enclosed mass of 2.5 ± 0.3 × 1012
M
⊙ within ∼120 kpc, an estimate that will be sharpened with forthcoming dynamical modeling. The combined power of stellar mapping and GC kinematics makes NGC 5128 an ongoing keystone for understanding galaxy assembly at mass scales inaccessible in the Local Group.
The Ionization and Dynamics of the Makani Galactic Wind
Authors: Rupke David S. N. , Coil Alison L. , Perrotta Serena , Davis Julie D. , Diamond-Stanic Aleksandar M. , Geach James E. , Hickox Ryan C. , Moustakas John , Petter Grayson C. , Rudnick Gregory H. , Sell Paul H. , Tremonti Christy A. , Whalen Kelly E. 
Published: April 2023

Abstract
The Makani galaxy hosts the poster child of a galactic wind on scales of the circumgalactic medium. It consists of a two-episode wind in which the slow, outer wind originated 400 Myr ago (Episode I; R
I = 20 − 50 kpc) and the fast, inner wind is 7 Myr old (Episode II; R
II = 0 − 20 kpc). While this wind contains ionized, neutral, and molecular gas, the physical state and mass of the most extended phase—the warm, ionized gas—are unknown. Here we present Keck optical spectra of the Makani outflow. These allow us to detect hydrogen lines out to r = 30–40 kpc and thus constrain the mass, momentum, and energy in the wind. Many collisionally excited lines are detected throughout the wind, and their line ratios are consistent with 200–400 km s−1 shocks that power the ionized gas, with v
shock = σ
wind. Combining shock models, density-sensitive line ratios, and mass and velocity measurements, we estimate that the ionized mass and outflow rate in the Episode II wind could be as high as those of the molecular gas:

M

II

H
II

∼

M

II

H

2

=
(
1
−
2
)
×

10

9

M

⊙

and

dM

/

dt

II

H
II

∼
dM

/

dt

II

H

2

=
170
−
250

M

⊙

yr−1. The outer wind has slowed, so that

dM

/

dt

I

H
II

∼
10

M

⊙

yr−1, but it contains more ionized gas,

M

I

H
II

=
5
×

10

9

M
⊙. The momentum and energy in the recent Episode II wind imply a momentum-driven flow (p “boost” ∼7) driven by the hot ejecta and radiation pressure from the Eddington-limited, compact starburst. Much of the energy and momentum in the older Episode I wind may reside in a hotter phase, or lie further into the circumgalactic medium.
Flares, Jets, and Quasiperiodic Outbursts from Neutron Star Merger Remnants
Authors: Most Elias R. , Quataert Eliot 
Published: April 2023

Abstract
Using numerical relativity simulations with a subgrid dynamo prescription to generate strong initial magnetic fields, we investigate the possibility of launching a jet-like outflow from the hypermassive neutron star (HMNS) during the early stages of the merger, prior to the remnant’s collapse to a black hole. We demonstrate that buoyant instabilities in the strongly magnetized HMNS can lead to a periodic emission of powerful electromagnetic flares shortly after the merger. These are followed by a collimated mildly relativistic outflow. Both types of outflows feature quasiperiodic kilohertz substructure. These early-time outflows may power precursors to short-duration gamma-ray bursts (sGRBs) or in some cases the entire sGRB. While the overall temporal power spectrum we find broadly agrees with the one recently reported for quasiperiodic oscillations in the sGRB GRB910711, our simulations suggest that the periodic electromagnetic substructure is dominated by magnetohydrodynamic shearing processes rather than correlating with the corresponding postmerger gravitational-wave signal.
A new species of Siamspinops Dankittipakul &amp; Corronca, 2009 from Guizhou, China (Araneae, Selenopidae)
Authors: Wang Cheng , Gan Jiahui , Xiaoqi Mi 
Published: April 2023

The wall crab spider genus Siamspinops Dankittipakul & Corronca, 2009 contains eight species restricted to South and Southeast Asia, of which two are recorded from China.
A new species, Siamspinops yejiei sp. n., is diagnosed and described based on both sexes from Foding Mountain National Nature Reserve, Guizhou, China. Diagnostic photos of the habitus and copulatory organs and a distributional map are provided.
Guerre en Ukraine : la paix se construit maintenant
Authors: Desportes Vincent , Bonnéry Stéphane , Darriau Mathilde , Bari Dominique 
Published: April 2023

Le général Vincent Desportes revient dans cet entretien sur les causes profondes du conflit en Ukraine. Les ambitions des États-Unis, affichées à l’issue de la guerre froide, se sont heurtées à celles de Poutine. L’affaiblissement durable de la Russie, la vassalisation de l’Europe, le renforcement de l’OTAN ont été au centre de la grande stratégie américaine. Dans ce conflit à hauts risques, la question fondamentale se fait attendre : comment faire la paix ? L’Europe saura-t-elle s’émanciper du joug américain et devenir un acteur majeur dans un processus de négociation et imaginer son futur avec la Russie ?
Des écoles vitaminées en EPS, pourquoi pas partout ?
Authors: Pontais Claire , Thépaut Antoine , Verscheure Ingrid 
Published: April 2023

L’éducation physique et sportive (EPS) à l’école primaire n’est pas enseignée à la hauteur de ce que les programmes prévoient (3 heures par semaine), alors même que les enjeux de santé sont criants et que des inégalités d’accès à la culture physique, sportive et artistique persistent. Or, même dans un contexte qui n’est pas favorable, certaines écoles réussissent à considérer l’EPS comme une discipline fondamentale et à dynamiser leur projet d’école par l’enseignement d’activités physiques, sportives et artistiques (APSA). Comprendre le fonctionnement de ces « Écoles vitaminées en EPS » a été l’enjeu d’une enquête portée par deux syndicats de la Fédération syndicale unitaire (FSU), enquête que nous présentons ici.
Paul Bourget, l’âme incarnée d’un dandy ? Expressions du corps et de l’âme au travers de ses journaux intimes
Authors: Ancelet-Netter Dominique 
Published: April 2023

Avant d’être l’auteur engagé du Disciple et un académicien honoré, Paul Bourget a été un jeune homme de lettres de la génération fin-de-siècle, oscillant entre dandysme et dilettantisme. Il tenta d’incarner ces « manières d’être » à l’imitation de Barbey d’Aurevilly avant de les théoriser dans ses Essais de psychologie contemporaine . Dans ses journaux intimes conservés à la bibliothèque de Fels, Bourget scrute ses états d’âmes et transcrit son moi déchiré en mots et en images. Dans le manuscrit de la période parisienne et mondaine du 31 février 1879 au 11 décembre 1883 et dans deux récits de voyage en 1893 autour de la Méditerranée et en 1898 aux États-Unis, trois portraits de l’auteur étonnent. Un soir de spleen, dans ses jeunes années, Bourget s’est dessiné allongé dans sa tombe. Dilettante cosmopolite, il fait son autoportrait en costume de berger grec. Une photographie de l’auteur prise lors d’un voyage à Newport le montre avec les attributs du dandy. Mais ce portrait collé à la première page de son récit de voyage américain et curieusement coupé en deux illustrerait-il l’âme incarnée et toujours tourmentée de ce « demi-dandy » qui a été l’un des maîtres du roman psychologique ?
Regards sur le roman « fin-de-siècle » : envois et dédicaces entre Paul Bourget et Eugène-Melchior de Vogüé
Authors: Selle Zoë 
Published: April 2023

En 1902, le romancier Paul Bourget, auteur du roman Le Disciple (1889), réinvestit la problématique du maître à penser, en publiant L’Étape . Il dédicace ce roman à l’écrivain Eugène-Melchior de Vogüé, célèbre pour son étude Le Roman russe , publiée en 1886, où il retrace l’œuvre des grands auteurs russes au xix e siècle. Depuis leur rencontre au cercle littéraire animé par Juliette Adam en 1883, ces écrivains issus de la même génération, et convaincus de l’attrait psychologique des personnages, nouent une amitié littéraire. De nombreuses dédicaces et correspondances sont conservées de nos jours et témoignent d’un lien d’affection manifeste entre ces deux écrivains et théoriciens du roman. Cet échange invite à comprendre l’influence mutuelle de ces deux auteurs, en regard de leurs contemporains, sur leur appréhension du monde moderne.
Guselkumab More Effectively Neutralizes Psoriasis-Associated Histologic, Transcriptomic, and Clinical Measures than Ustekinumab
Authors: Campbell Kim , Li Katherine , Yang Feifei , Branigan Patrick , Elloso M Merle , Benson Jacqueline , Orlovsky Yevgeniya , Chen Yanqing , Garcet Sandra , Krueger James G 
Published: April 2023

Abstract
Given the key role of the IL-23/Th17 axis in the pathogenesis of moderate-to-severe plaque psoriasis, several specific inhibitors of the p19 subunit of IL-23 have been approved to treat this chronic inflammatory disease. Clinical data indicate that guselkumab, one such selective IL-23 inhibitor, achieves greater clinical efficacy compared with ustekinumab, which inhibits both IL-12 and IL-23 via binding their shared p40 subunit. To understand mechanisms underlying the enhanced efficacy observed with the p19 subunit of IL-23–specific inhibition, we explored cellular and molecular changes in skin of psoriasis patients treated with ustekinumab or guselkumab and in ustekinumab inadequate responders (Investigator’s Global Assessment of psoriasis score ≥ 2) subsequently treated with guselkumab (ustekinumab→guselkumab). Skin biopsies were collected pretreatment and posttreatment to assess histologic changes and molecular responses in ustekinumab- and guselkumab-treated patients. Serum cytokines and skin transcriptomics from the subset of ustekinumab→guselkumab-treated patients were also analyzed to characterize differential treatment effects. Ustekinumab and guselkumab demonstrated differential effects on secretion of pathogenic Th17-related cytokines induced by IL-23 in in vitro assays, which suggest guselkumab is a more potent therapeutic agent. Consistent with these findings, guselkumab elicited a significantly greater reduction in cellular and molecular psoriasis-related disease indicators than ustekinumab. In ustekinumab→guselkumab patients, suppression of serum IL-17A and IL-17F levels and neutralization of molecular scar and psoriasis-related gene markers in skin were significantly greater compared with patients continuing ustekinumab. This comparative study demonstrates that guselkumab inhibits psoriasis-associated pathology, suppresses Th17-related serum cytokines, and normalizes the psoriasis skin gene expression profile more effectively than ustekinumab.
Expression of Concern (RESOLVED). Relationship between body mass index and oral health indicators: a cross-sectional study
Authors: Publisher The 
Published: April 2023

Update to April 27th, 2023: The Publisher is glad to inform the readers that the issue discussed here has been favorably resolved and we have no longer cause of concern regarding this paper.
This is a note of a temporary expression of concern related to the above-mentioned publication, as an occurrence of duplicate publication has been discovered. The Authors, their Institutions and other entities are investigating the issue of possible misconduct by a third entity. Evidence of inappropriate dual publication is available and will remain confidential while the investigation is ongoing; due to various complexities, the investigation will not be complete for a considerable time.
The concern and this note will remain appended to the above-mentioned article, unless the parties provide the editors of the journal and the Publisher with a solution to the dispute.

Reference
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