bluuebunny/crossref_metadata_2025_split huggingface dataset:
A jsPsych touchscreen extension for behavioral research on touch-enabled interfaces
Authors: Strittmatter Younes , Spitzer Markus W. H. , Ging-Jehli Nadja , Musslick Sebastian 
Published: July 2024

AbstractOnline experiments are increasingly gaining traction in the behavioral sciences. Despite this, behavioral researchers have largely continued to use keyboards as the primary input devices for such online studies, overlooking the ubiquity of touchscreens in everyday use. This paper presents an open-source touchscreen extension for jsPsych, a JavaScript framework designed for conducting online experiments. We additionally evaluated the touchscreen extension assessing whether typical behavioral findings from two distinct perceptual decision-making tasks – the random-dot kinematogram and the Stroop task – can similarly be observed when administered via touchscreen devices compared to keyboard devices. Our findings indicate similar performance metrics for each paradigm between the touchscreen and keyboard versions of the experiments. Specifically, we observe similar psychometric curves in the random-dot kinematogram across the touchscreen and keyboard versions. Similarly, in the Stroop task, we detect significant task, congruency, and sequential congruency effects in both experiment versions. We conclude that our open-source touchscreen extension serves as a promising tool for data collection in online behavioral experiments on forced-choice tasks.
Sağlık Hukukunda Tartışmalı Konular
Authors: Keçeligil Hasan Tahsin , Cantürk Gürol , Dalcı Özdoğan Nurcihan , Arda Berna , Kıvrak Nasibe , Emiral Emrah , Baysal Dilek , Fırat Ahmet , Özel Yeşilyurt Aysun , Gürbüz Aslıhan , Gündüz Bestami , Nehir Türkü Yağmur , Kılınç Bahar , İyigün Ufuk , Güney Tunalı Işıl , Varman Alper , Almbaidheen Mahmut , Altın Gökçe , Güneş Deniz Yağmur , Çobanoğlu Nesrin , Atalan Mustafa 
Published: July 2024

Tıp Hukuku Dersleri: Samsun Deneyimi
Hasan Tahsin KEÇELİGİL
Ankara Üniversitesi Adli Bilimler Enstitüsü Sağlık Hukuku Tezli Yüksek Lisans Programı
Gürol CANTÜRK
Öğreti ve Yargı Kararları Işığında Zorunlu Aşı Uygulaması
Nurcihan DALCI ÖZDOĞAN
Biyoetik Bakış Açısıyla Kadın Hakları
Berna ARDA
Ceza ve Tutuk Evi Hemşireliği
Nasibe KIVRAK
Emrah EMİRAL
Dilek BAYSAL
Önerilen Tedavinin ve Yoğun Bakım Taburculuğunun Reddedilmesi: Olgu Sunumu
Ahmet FIRAT
Aysun ÖZEL YEŞİLYURT
Dilek ÖZCENGİZ
Olay Yeri İnceleme Hemşireliği
Nasibe KIVRAK Aslıhan GÜRBÜZ
Sağlık Teşkilatlanması İçerisinde Aile Hekiminin Yeri
Bestami GÜNDÜZ
Aile Hekimliği Pratiğinde Hukuki Sorunlar
Türkü Yağmur NEHİR
Özel Hastanede Çalışan Hekimlerin Sosyal Güvenlik Hakları
Bahar KILINÇ
Tıp Bilişimi Hukuku Kapsamında KVKK’nın Değerlendirilmesi
Ufuk İYİGÜN
Yüksek Yargıya Yansıyan Doğumsal Anomali Olgularının İrdelenmesi
Işıl GÜNEY TUNALI
Komplikasyon- Malpraktis Ayrımına Genel Cerrahi Penceresinden Bakış
Alper VARMAN
Çocuk İstismarı ve İhmalinin Adli Bildirimi ve Hekimlerin Rolü
Mahmut ALMBAİDHEEN
Bilirkişi Hemşireliği
Nasibe KIVRAK
Emrah EMİRAL
Dilek BAYSAL
Karşılaştırmalı Hukukta Malpraktis ve Arabuluculuk Uygulamaları
Neval YILMAZ
Güncel Tartışmalar Işığında Eczacının Cezai Sorumluluğu
Gökçe ALTIN
Yaşam Sonu Kararlarda Bilgilendirme ve Rıza
Neval YILMAZ
Yaşamın Sonuna Dair Sorunlar ve Tıbbi Talimatname
Dilek ÖZCENGİZ
Sağlık Politikaları Bağlamında Nadir Hastalıklar ve Yetim İlaçlar
Deniz Yağmur GÜNEŞ
İnsan Hakları ve İnsan Haysiyeti Penceresinden Biyotıp Sözleşmesi
Mete Salih AKER
Tıp Alanında Yapay Zeka Kullanımının Hukuki Boyutu
Ufuk İYİGÜN
Sağlıkta Şiddet: Hukuki Koruma ve Hak Arama Yolları
Hasan Tahsin KEÇELİGİL
Yaşam Sonu Kararlarının Etik Boyutları
Nesrin ÇOBANOĞLU
Adli Olaylara Müdahalede Hekimin Rolü ve Sorumluluğu
Mustafa ATALAN
Factores Socioemocionales que Intervienen en Niños y Niñas Migrantes de Retorno de los Estado Unidos a Localidades de Tlaxcala
Authors: Vázquez Vázquez José Dionicio , Pérez Velázquez Karina 
Published: July 2024

En el presente estudio se abordan los efectos socioemocionales en niños y niñas migrantes de retorno en educación básica en localidades del municipio de Tlaxcala, donde el principal objetivo se enfoca en conocer algunos factores sociales, escolares, familiares, de salud mental y emocional que intervienen en la reintegración social, como parte de la calidad de vida familiar de niños y niñas migrantes de retorno, centrándose en sus experiencias en edad escolar básica, abordando cómo se integran en el sistema educativo y a la comunidad de origen luego de su regreso familiar de Estados Unidos a Tlaxcala, México. El trabajo se abordó desde el enfoque cualitativo que permitió comprender en parte la migración de retorno y de la calidad de vida, desde la complejidad de la experiencia de niños migrantes que regresan a su país de origen. Un hallazgo que resalta es que los infantes a menudo no participan en la decisión de retornar, lo que puede generar un deseo de volver al país extranjero en el futuro. Los padres, madres o tutores llegan a tomar la decisión de retorno basada en factores familiares, económicos y personales, provocando ciertos cambios en su nivel de vida, alterando su reinserción escolar.
Decay Timescales of Chromospheric Condensations in Solar Flare Footpoints
Authors: Butler Elizabeth C. , Kowalski Adam F. 
Published: July 2024

Abstract
Chromospheric condensations (CCs) are a prominent feature of flare footpoint heating in the solar flare standard model, yet their timescales and velocities are not well understood. Fisher derived several important analytical relationships, which have rarely been examined with modern spectral observations. The Interface Region Imaging Spectrograph (IRIS) provides a wealth of flare data with a high enough cadence to sufficiently capture CC evolution. We analyzed Doppler shifts in Mg ii 2791 and Fe ii 2814 from a sample of flare footpoint pixels observed by IRIS to compare with Fisher's analytics and recent flare models. We found a detection lifetime of 1 minute occurs in 50% of the sample, with Mg ii showing several pixels with longer values and Fe ii almost categorically shorter, and both growing with the maximum velocity, v
max. The shifts’ half-life is commonly <40 s and is inversely related to v
max, indicating that the first half of the CC evolution has more efficient kinetic energy loss. The lifetime’s wide range and growth with v
max indicate that the footpoint atmospherics and heating scenarios can vary more widely than first postulated in Fisher. Around 90% of the sample had observable acceleration periods, lasting an average of 38 and 32 s for Mg ii and Fe ii, respectively. These acceleration periods, as well as serving as flare model diagnostics themselves, could potentially be used to calculate other model diagnostics such as the initially accelerated mass.
Carbon Cycle Instability for High-CO2 Exoplanets: Implications for Habitability
Authors: Graham R. J. , Pierrehumbert R. T. 
Published: July 2024

Abstract
Implicit in the definition of the classical circumstellar habitable zone (HZ) is the hypothesis that the carbonate-silicate cycle can maintain clement climates on exoplanets with land and surface water across a range of instellations by adjusting atmospheric CO2 partial pressure (pCO2). This hypothesis is made by analogy to the Earth system, but it is an open question whether silicate weathering can stabilize climate on planets in the outer reaches of the HZ, where instellations are lower than those received by even the Archean Earth and CO2 is thought likely to dominate atmospheres. Since weathering products are carried from land to ocean by the action of water, silicate weathering is intimately coupled to the hydrologic cycle, which intensifies with hotter temperatures under Earth-like conditions. Here, we use global climate model simulations to demonstrate that the hydrologic cycle responds counterintuitively to changes in climate on planets with CO2-H2O atmospheres at low instellations and high pCO2, with global evaporation and precipitation decreasing as pCO2 and temperatures increase at a given instellation. Within the Maher & Chamberlain (or MAC) weathering formulation, weathering then decreases with increasing pCO2 for a range of instellations and pCO2 typical of the outer reaches of the HZ, resulting in an unstable carbon cycle that may lead to either runaway CO2 accumulation or depletion of CO2 to colder (possibly snowball) conditions. While the behavior of the system has not been completely mapped out, the results suggest that silicate weathering could fail to maintain habitable conditions in the outer reaches of the nominal HZ.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic Star Formation Rate Density 300 Myr after the Big Bang
Authors: Robertson Brant , Johnson Benjamin D. , Tacchella Sandro , Eisenstein Daniel J. , Hainline Kevin , Arribas Santiago , Baker William M. , Bunker Andrew J. , Carniani Stefano , Cargile Phillip A. , Carreira Courtney , Charlot Stephane , Chevallard Jacopo , Curti Mirko , Curtis-Lake Emma , D’Eugenio Francesco , Egami Eiichi , Hausen Ryan , Helton Jakob M. , Jakobsen Peter , Ji Zhiyuan , Jones Gareth C. , Maiolino Roberto , Maseda Michael V. , Nelson Erica , Pérez-González Pablo G. , Puskás Dávid , Rieke Marcia , Smit Renske , Sun Fengwu , Übler Hannah , Whitler Lily , Williams Christina C. , Willmer Christopher N. A. , Willott Chris , Witstok Joris 
Published: July 2024

Abstract
We characterize the earliest galaxy population in the JADES Origins Field, the deepest imaging field observed with JWST. We make use of ancillary Hubble Space Telescope optical images (five filters spanning 0.4–0.9 μm) and novel JWST images with 14 filters spanning 0.8−5 μm, including seven medium-band filters, and reaching total exposure times of up to 46 hr per filter. We combine all our data at >2.3 μm to construct an ultradeep image, reaching as deep as ≈31.4 AB mag in the stack and 30.3–31.0 AB mag (5σ, r = 0.″1 circular aperture) in individual filters. We measure photometric redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts z = 11.5−15. These objects show compact half-light radii of R
1/2 ∼ 50−200 pc, stellar masses of M
⋆ ∼ 107−108
M
☉, and star formation rates ∼ 0.1−1 M
☉ yr−1. Our search finds no candidates at 15 < z < 20, placing upper limits at these redshifts. We develop a forward-modeling approach to infer the properties of the evolving luminosity function without binning in redshift or luminosity that marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the impact of nondetections. We find a z = 12 luminosity function in good agreement with prior results, and that the luminosity function normalization and UV luminosity density decline by a factor of ∼2.5 from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical models for evolution of the dark matter halo mass function.
The Stagger Code for Accurate and Efficient, Radiation-coupled Magnetohydrodynamic Simulations
Authors: Stein Robert F. , Nordlund Åke , Collet Remo , Trampedach Regner 
Published: July 2024

Abstract
We describe the Stagger code for simulations of magnetohydrodynamic (MHD) systems. This is a modular code with a variety of physics modules that will let the user run simulations of deep stellar atmospheres, sunspot formation, stellar chromospheres and coronae, proto-stellar disks, star formation from giant molecular clouds, and even galaxy formation. The Stagger code is efficiently and highly parallelizable, enabling such simulations with large ranges of both spatial and temporal scales. We describe the methodology of the code and present the most important of the physics modules, as well as its input and output variables. We show results of a number of standard MHD tests to enable comparison with other, similar codes. In addition, we provide an overview of tests that have been carried out against solar observations, ranging from spectral line shapes, spectral flux distribution, limb darkening, intensity and velocity distributions of granulation, to seismic power spectra and the excitation of p-modes. The Stagger code has proven to be a high-fidelity code with a large range of uses.
First Constraints on the Interstellar Medium Conditions of a Low-mass, Highly Obscured z = 4.27 Main-sequence Galaxy
Authors: Mizener Andrew , Pope Alexandra , McKinney Jed , Kamieneski Patrick , Whitaker Katherine E. , Battisti Andrew , Murphy Eric 
Published: July 2024

Abstract
We present the molecular gas content and interstellar medium conditions of MACS J0717_Az9, a strong gravitationally lensed z = 4.273, M
* ≃ 2 × 109
M
⊙ star-forming galaxy with an unusually high (∼80%) obscured star formation fraction. We detect CO (4–3) in two independent lensed images, as well as [N ii] 205 μm, with the Atacama Large Millimeter Array. We derive a molecular gas mass of log

10

[

M

H

2

(

M

⊙

)
]
=
9.77

, making it moderately deficient in molecular gas compared to the lower-redshift gas fraction scaling relation. Leveraging photodissociation region (PDR) models, we combine our CO (4–3) measurements with existing measurements of the [C ii] 158 μm line and total infrared luminosity to model the PDR conditions. We find PDR conditions similar to those in local star-forming galaxies, with a mean hydrogen density log10[n
H cm−3] = 4.80 ± 0.39 and a mean radiation field strength log10[G
0 Habing] = 2.83 ± 0.26. Based on Band 3 continuum data, we derive an upper limit on the intrinsic dust mass of log10[M
dust(M
⊙)] < 7.73, consistent with existing estimates. We use the 3D tilted-ring model fitting code 3D-Barolo to determine the kinematic properties of the CO (4–3) emitting gas. We find that it is rotationally dominated, with a V/σ = 4.6 ± 1.7, consistent with the kinematics of the [C ii]. With PDR conditions remarkably similar to those in normal dusty star-forming galaxies at z < 0.2 and a stable molecular disk, our observations of Az9 suggest that the dust-obscured phase for a low-mass galaxy at z ∼ 4 is relatively long. Thus, Az9 may be representative of a more widespread population that has been missed owing to insufficiently deep existing millimeter surveys.
MIDIS: The Relation between Strong (Hβ + [O iii]) Emission, Star Formation, and Burstiness around the Epoch of Reionization
Authors: Caputi K. I. , Rinaldi P. , Iani E. , Pérez-González P. G. , Östlin G. , Colina L. , Greve T. R. , Nørgaard-Nielsen H. U. , Wright G. S. , Álvarez-Márquez J. , Eckart A. , Hjorth J. , Labiano A. , Le Fèvre O. , Walter F. , van der Werf P. , Boogaard L. , Costantin L. , Crespo Gómez A. , Gillman S. , Jermann I. , Langeroodi D. , Melinder J. , Peissker F. , Güdel M. , Henning Th. , Lagage P. O. , Ray T. P. 
Published: July 2024

Abstract
We investigate the properties of strong (Hβ + [O iii]) emitters before and after the end of the “Epoch of Reionization” from z = 8 to z = 5.5. We make use of ultradeep JWST/NIRCam imaging in the parallel field (P2) of the MIRI Deep Imaging Survey (MIDIS) in the Hubble eXtreme Deep Field (H-XDF), in order to select prominent (Hβ + [O iii]) emitters (with rest-frame equivalent width (EW0) ≳ 100 Å) at z = 5.5–7, based on their flux density enhancement in the F356W band with respect to the spectral energy distribution continuum. We complement our selection with other (Hβ + [O iii]) emitters from the literature at similar and higher (z = 7−8) redshifts. We find (nonindependent) anticorrelations between EW0(Hβ + [O iii]) and both galaxy stellar mass and age, in agreement with previous studies, and a positive correlation with specific star formation rate (sSFR). On the SFR–M
⋆ plane, the (Hβ + [O iii]) emitters populate both the star formation main sequence and the starburst region, which become indistinguishable at low stellar masses (

log
10

(

M
⋆

)

<
7.5

). We find tentative evidence for a nonmonotonic relation between EW0(Hβ + [O iii]) and SFR, such that both parameters correlate with each other at SFR ≳ 1 M
⊙ yr−1, while the correlation flattens out at lower SFRs. This suggests that low metallicities producing high EW0(Hβ + [O iii]) could be important at low SFR values. Interestingly, the properties of the strong emitters and other galaxies (33% and 67% of our z = 5.5–7 sample, respectively) are similar, including, in many cases, high sSFR. Therefore, it is crucial to consider both emitters and nonemitters to obtain a complete picture of the cosmic star formation activity around the Epoch of Reionization.
Millimeter to THz Spectroscopy of HC18O+ and HC17O+: Accurate Rest Frequencies for Astrophysical Studies
Authors: Bizzocchi Luca , Tonolo Francesca , Giuliano Barbara M. , Caselli Paola , Melosso Mattia , Dore Luca , Alessandrini Silvia , Puzzarini Cristina , Pietropolli Charmet Andrea 
Published: July 2024

Abstract
Heavy oxygen isotopic species of HCO+ are important optically thin astrophysical tracers. The ground-state rotational spectrum of HC18O+, DC18O+, HC17O+, and DC17O+ has been recorded in the laboratory in the frequency range from 85 GHz to 1.3 THz. The ions have been produced in the negative column of a glow-discharge plasma, and their spectrum has been recorded in absorption using a frequency-modulation submillimeter-wave spectrometer. Various sources of systematic error have been carefully accounted for in order to obtain highly accurate line-position measurements. Theoretical estimates of the molecular parameters and of the collision effects on the line shape have been obtained by high-level ab initio calculations. The analysis yielded much improved rotational and centrifugal distortion constants, thus bringing the spectroscopic characterization of these rare isotopic variants to the same level of the parent species. Also, the first experimental rotational data for DC17O+ have been provided. These results allow for the calculation of an updated set of rest frequencies to support current and future astrophysical studies. The derived data set for the widely used HC18O+ tracer reaches an accuracy of a few parts in 109 up to 1.5 THz. Such accuracy is important for the analysis of astrophysical objects targeted by Atacama Large Millimeter/submillimeter Array observations at the submillimeter regime.
Hadrianic Echoes in the Work of Synesius of Cyrene
Authors: Gordillo Hervás Rocío 
Published: July 2024

Résumé Résumé : Synésios de Cyrène, l’un des auteurs les plus représentatifs des iv e - v e siècles après J.-C., est l’un des rares exemples où l’on trouve encore, dans l’Antiquité tardive, des traces de la politique menée par l’empereur Hadrien dans le monde grec. L’objectif de cet article est d’analyser les références possibles à la politique d’Hadrien dans l’œuvre de Synésios de Cyrène, en se concentrant particulièrement sur l’importance donnée par ce dernier à ses racines grecques, et les échos possibles du modèle culturel d’Hadrien qui a été établi avec la création de la ligue du Panhellénion. En outre, Synésios est la seule source existante dans laquelle un groupe d’intellectuels de Constantinople est désigné par le terme Panhellénion, ce qui représenterait un autre élément de l’impact culturel de la politique culturelle hadrienne.
Les partis populistes de droite radicale et la démocratie face à la pandémie de COVID-19 : Analyse comparée de la communication du Rassemblement national et du Vlaams Belang
Authors: Ricotta Anthony 
Published: July 2024

En contexte de crise sanitaire, de multiples mesures – parfois qualifiées de liberticides, voire d’autoritaires – ont été prises par les autorités politiques respectives des États d’Europe et du monde afin de contenir le virus. Dans un contexte caractérisé par une remise en question du caractère démocratique des mesures sanitaires, il apparait pertinent d’étudier les propos que les partis populistes de droite radicale – qui sont habituellement critiques envers la démocratie libérale qu’ils disent être dirigée par des élites intéressées qui ignorent systématiquement les volontés populaires – tiennent sur la démocratie. Cet article s’inscrit dans cet objectif et procède à une analyse thématique comparative des propos tenus par deux partis populistes de droite radicale – le Vlaams Belang et le Rassemblement national – sur Twitter et dans l’enceinte parlementaire. Il en résulte une mise en lumière du caractère antisystème et antiestablishment de ces partis, qui instrumentalisent la défense de la démocratie au service de leur critique du système.
Une évolution des jardins collectifs vers des fonctions de production et d’expérimentation : exemple des jardins partagés lyonnais
Authors: Bally Frédéric 
Published: July 2024

Le jardin collectif a le vent en poupe dans les villes françaises. Porteurs d’enjeux pour les collectivités qui y voient un moyen de retisser du lien social et de permettre à des habitants de produire des légumes, mais aussi pour les habitants qui veulent rencontrer leurs voisins et profiter d’un espace de verdure à proximité de chez eux, ces jardins rencontrent et complètent les problématiques urbaines d’aujourd’hui : participation et inclusion des habitants dans l’aménagement du territoire. Via une étude qualitative menée auprès des participants de jardins partagés de Lyon, nous montrons que ces espaces sont aussi des lieux d’exclusion, s’éloignant de leurs valeurs de départ.
Unlocking the True Power of Additive Manufacturing for EMI Shielding
Authors: Scheibel Markus G. , Kaiser Michael P. , Balasubramaniam Sutharsan , Chernobryvko Mykola , Koszegi Julia-Marie , Dreissigacker Marc , Adler Marius , Braun Tanja , Huang Chuan I. Eric , Li Meng Jason , Thomas Muriel , Vollmann Franz 
Published: July 2024

Miniaturization trends in electronic packaging led to reduced spacing of individual packages on the printed circuit boards and thus increased the overall electromagnetic interference (EMI) levels within a device. State-of-the-art conformal coatings as EMI shielding layers are typically applied via sputter technology and offer design limitations with respect to coating selectivity on individual positions of the overall package. Our new technology of additively Ag layer application via inkjet printing overcomes today’s design limitations and is a key enabler for next-generation packaging designs. In this study, we compare the shielding effectiveness (S.E.) on specifically designed transmission line emitter samples coated with state-of-the-art sputtered conformal layers against silver coatings applied via inkjet printing of particle-free metal-organic decomposition inks to evaluate the new technology for its potential on package-level shielding performance. Mechanical and electrical characterization of the silver coatings indicates appropriate tools to specify layer characteristics and ensure S.E. of 40 dB or higher at frequencies of 800 MHz and higher. The suitability of our well-tailored silver coatings to match typical S.E. requirements is shown with even much thinner layer thickness as compared with state-of-the-art coatings.
Análisis de los servicios preventivos de seguridad y salud en una institución educativa empleando la NOM-030-STPS-2009
Authors: Duarte Beltrán Elizabeth 
Published: July 2024

En México, el instituto mexicano del seguro social registró un total de 78 647 enfermedades ocupacionales, siendo las de mayor incidencia COVID-19 con un 80.6%, dorsopatías 3.6%; hipoacusias 2.7%, lesiones del hombro 1.6%, síndrome del túnel carpiano 1.4% y neumoconiosis 1.3%. El objetivo de la investigación es reducir las enfermedades registradas en el año 2023 de una institución educativa, implementando un programa preventivo de seguridad y salud que contenga las acciones que se deben llevar a cabo con base a la NOM-030-STPS. La metodología que se empleó consta de 5 etapas para profundizar su estudio. En los resultados se observó que el área de enfermería en un año, brindó 2310 consultas a 492 trabajadores, registrando enfermedades como gripes con un 44%, padecimientos gastrointestinales 31%, curaciones e inyecciones 12%, cólicos 8% y otros 5%, para mejorar la asistencia sanitaria a los trabajadores y reducir las enfermedades ocupacionales, se propone implementar un programa de prevención de seguridad y salud, adoptando la inteligencia artificial, como alternativa médica en el área laboral.