bluuebunny/crossref_metadata_2025_split huggingface dataset:
Peningkatan Kualitas Sumber Daya Manusia (SDM) Petani Jagung Melalui Metode Penyuluhan Pertanian
Authors: Ermawati Elly , Akhmad Akhmad , Idhan Abubakar 
Published: April 2023

Penelitian ini bertujuan untuk mengetahui metode penyuluhan pertanian yang efektif dan tepat untuk meningkatkan kualitas sumber daya manusia (SDM) petani jagung serta faktor pendukung dan penghambat dalam meningkatkan kualitas sumber daya manusia (SDM) petani jagung. Metode penelitian ini yaitu kualitatif yang bersifat deskriptif dengan teknik pengumpulan data melalui observasi, wawancara, dokumentasi dan FGD. Hasil penelitian menunjukkan bahwa Metode penyuluhan pertanian yang paling tepat dan efektif yaitu Demplot dan Anjangsana karena petani didatangi langsung oleh penyuluh ke lahan pertanian, kemudian penyuluh memberikan contoh-contoh dan dilakukan oleh petani secara langsung. Faktor pendukung peningkatan kualitas SDM petani yaitu pelatihan, tingkat pendidikan, Kerjasama yang baik penyuluh dan petani serta faktor penghambatnya yaitu kurangnya tenaga penyuluh, partisipasi petani yang kurang dan komunikasi yang tidak berjalan dengan baik.Kata kunci: Kualitas, Metode Penyuluhan Pertanian, Kelompok Tani
Pengaruh Gaya Kepemimpinan Dan Motivasi Terhadap Kinerja Karyawan Pada Pt Bank Tabungan Pensiunan Nasional (Btpn) Kantor Cabang Makassar Tbk
Authors: Larazati Larazati 
Published: April 2023

Penelitian ini bertujuan untuk meneliti secara empiris Pengaruh Gaya Kepemimpinan dan Motivasi terhadap Kinerja Karyawan pada PT Bank Tabungan Pensiunan Nasional (BTPN) Kc Makassar Tbk, Populasi yang digunakan adalah Karyawan pada PT Bank Tabungan Pensiunan Nasional (BTPN) Kc Makassar Tbk yang telah bekerja selama 15 tahun, dengan jumlah Populasi 85 Orang Karyawan, kemudian di tarik sampel berdasarkan rumus slovin akhirnya di dapat 46 orang Karyawan yang dijadikan responden. Penelitian ini merupakan Penelitian Kuantitatif yang diperoleh dari koesioner yang dibagikan dan berhubungan dengan masalah yang diteliti. Pengumpulan data dilakukan dengan pembagian koesioner. Teknik analisis data yang dipakai yaitu analisis Deskriptif. Uji Validasi, Uji Reabilitas, Uji Normalitas, Uji Multikolinearitas, Uji Heteroskedastisitas, Uji Regresi Linier Berganda, Uji Parsial (t-test), dan Uji Simultan (F-test). Instrumen penelitian yang digunakan dalam penelitian ini menggunakan metode skala Likert. Hasil penelitian ini menunjukkan bahwa gaya kepemimpinan dan motivasi berpengaruh secara positif dan signifikan terhadap kinerja karyawan pada PT Bank Tabungan Pensiunan Nasional (BTPN) Kc Makassar Tbk. Kata kunci: Gaya Kepemimpinan; Motivasi; Kinerja Karyawan
Paciente de 54 años con Leishmaniasis Cutánea en Pabellón Auricular Derecho. Reporte de Caso
Authors: Maita Zambrano Alvaro Israel , López Sanmartín Cristina Isabel , Choez Abendaño Yoselyn Isabel , Arroyo Chugcho Pablo Andrés , Alvarez Saltos Miguel David 
Published: April 2023

La Leishmaniasis es una patología producida por un parásito protozoario intracelular estricto perteneciente a la especie Leishmania. Esta enfermedad es inoculada por un vector hacia los animales o al ser humano. El trasmisor directo son las pequeñas moscas flebótomos, cuyo díptero hembra perteneciente al género Lutzomya es el principal causante de esta patología a nivel de Sudamérica mientras que el género Phlebotumus prolifera en el resto del mundo. El diagnóstico es difícil por la inespecificidad de la clínica y el lento crecimiento del parásito en cultivo. A pesar de aparentar ser una enfermedad con un curso relativamente benigno, causa lesiones que pueden ser causa de estigmatización en poblaciones ya de por sí vulnerables, como lo son las personas que se encuentran en las zonas rurales.
Se Reporta un caso de un paciente de 54 años de edad con antecedentes de Hipertensión arterial, trastornos de ansiedad y trastornos depresivos, se evidencia lesiones ulcerosas localizadas en región de pabellón auricular derecho compatibles con leishmaniasis, se procede a tratamiento utilizando Antimoniato de meglumina con evolución favorable y buen pronóstico.
Incidencia del desarrollo profesional docente y el trabajo colaborativo en la gestión de los directores de las Instituciones Educativas de la Ciudad de Pilar
Authors: Galeano Montiel Milce Marilina 
Published: April 2023

Esta investigación tiene el propósito de analizar la incidencia del desarrollo profesional docente y el trabajo colaborativo en la gestión de los directores de las instituciones educativas de la ciudad de Pilar. Este tema se hizo esencial averiguar para establecer los puntos de vistas de los Docentes, Directivos de las instituciones educativas y la Supervisora Pedagógica de la ciudad de Pilar; con relación al fenómeno de estudio. Este trabajo fue desarrollado mediante una metodología con enfoque cuantitativo de tipo descriptivo. Como técnica de recolección de datos se valió de la encuesta. La población de estudio lo conformaron los Docentes, Directivos y la Supervisora; se tomó una muestra representativa a 30 Docentes, 2 Directivos y 1 Supervisora de la ciudad de Pilar. El estudio comprobó que, la incidencia del desarrollo profesional docente y el trabajo colaborativo en la gestión de los directores de las instituciones educativas de la ciudad de Pilar, se basa en el respeto a la individualidad de cada persona, en la ayuda mutua para comprender la enseñanza y aprender de la experiencia y en la reflexión compartida; lo que posibilita la autonomía profesional del profesorado, así como la interdependencia de los compañeros.
Situación actual, características e importancia de la educación emocional postpandemia. Análisis de su relevancia dentro de los Proyectos Educativos Institucionales en la Localidad de Suba
Authors: Martínez Ruiz Jane Alexandra 
Published: April 2023

El presente artículo pretende identificar qué es la educación emocional, sus características y situación actual. Inicia reconociendo el proceso de transformación de la educación como producto de diversos factores que se han venido dando en los últimos años, centrándose en los cambios que trajo consigo el COVID 19 y específicamente en las consecuencias en la salud mental de la población escolar. Posteriormente, se presentan reflexiones sobre la educación emocional en cuanto a su concepto, objetivos, contenido y pertinencia; para finalmente presentar un pequeño estudio realizado en las instituciones educativas distritales de la localidad de Suba en Bogotá, cuyo propósito fue determinar la pertinencia de la educación emocional dentro de los Proyectos Educativos Institucionales del PEI de dichas escuelas. Los resultados del análisis muestran que existe poco interés en la articulación e implementación de la educación emocional con las políticas educativas.
Solar Wind Magnetic Field Line Dispersal: Multispacecraft Analysis and Comparison with Theoretical Results
Authors: Ragot B. R. 
Published: April 2023

Abstract
The dominance of the global over the relative, cross-field transport of magnetic field lines (MFLs), up to scales of a couple of hours in the solar wind (SW), has been predicted both theoretically and numerically, in the approximation of self-similar, single-level power spectra of magnetic fluctuations. Here the predictions for the MFL relative cross-field transport or dispersal are tested against the results of in situ data analysis, using 23 yr of field and flow measurements on board ACE and Wind. The theoretical results are confirmed/refined by nonlinear theoretical computations and corrected to include the effects of power-level variability or intermittency. Other than confirming earlier theoretical findings at the separation scales ρ between a few ×1010 cm and the large-separation limit, with a ballistic regime followed by decorrelation and transition to diffusion in the

(
ln
ρ
,
θ
)

-space, the new study reveals two new supradiffusive regimes in

ln
ρ

and clock angle θ for the MFL dispersal, distinct from a drift-induced supradiffusion found earlier, and distinct from each other. The first supradiffusion, of the nonlinear computations, is a simple nonlinear effect, which cannot be recovered by data analysis at two spacecraft of fixed separation on the analysis timescale. The second supradiffusion, of the data analysis, is much stronger for ρ < few × 1010 cm than the two previous supradiffusions, and it becomes stronger at shorter separations. It follows the ballistic regime without transition through diffusion and is recovered by multiscale, theoretical estimates. It is a Lévy-type supradiffusion, due to the intermittency observed in the SW.
Unfolding Drift Effects for Cosmic Rays over the Period of the Sun’s Magnetic Field Reversal
Authors: Aslam O. P. M. , Luo 罗 Xi 熙 , Potgieter M. S. , Ngobeni M. D. , Song 宋 Xiaojian 小健 
Published: April 2023

Abstract
A well-established, comprehensive 3D numerical modulation model is applied to simulate galactic protons, electrons, and positrons from 2011 May to 2015 May, including the solar magnetic polarity reversal of Solar Cycle 24. The objective is to evaluate how simulations compare with corresponding Alpha Magnetic Spectrometer observations for 1.0–3.0 GV and what underlying physics follows from this comparison to improve our understanding of how the major physical modulation processes change, especially particle drift, from a negative to a positive magnetic polarity cycle. Apart from their local interstellar spectra, electrons and positrons differ only in their drift patterns, but they differ with protons in other ways such as adiabatic energy changes at lower rigidity. In order to complete the simulations for oppositely charged particles, antiproton modeling results are also obtained. Together, observations and corresponding modeling indicate the difference in the drift pattern before and after the recent polarity reversal and clarify to a large extent the phenomenon of charge-sign dependence during this period. The effect of global particle drift became negligible during this period of no well-defined magnetic polarity. The resulting low values of particles’ mean free paths (MFPs) during the polarity reversal contrast their large values during solar minimum activity and as such expose the relative contributions and effects of the different modulation processes from solar minimum to maximum activity. We find that the drift scale starts recovering just after the polarity reversal, but the MFPs keep decreasing or remain unchanged for some time after the polarity reversal.
Early Results from GLASS-JWST. XVII. Building the First Galaxies—Chapter 1. Star Formation Histories for 5 < z < 7 Galaxies
Authors: Dressler Alan , Vulcani Benedetta , Treu Tommaso , Rieke Marcia , Burns Chris , Calabrò Antonello , Bonchi Andrea , Castellano Marco , Fontana Adriano , Leethochawalit Nicha , Mason Charlotte , Merlin Emiliano , Morishita Takahiro , Paris Diego , Bradac Marusa , Mercurio Amata , Nanayakkara Themiya , Poggianti Bianca M. , Santini Paola , Wang Xin , Misselt Karl , Stark Daniel P. , Willmer Christopher 
Published: April 2023

Abstract
The JWST observations of high-redshift galaxies are used to measure their star formation histories—the buildup of stellar mass in the earliest galaxies. Here we use a novel analysis program, SEDz*, to compare near-IR spectral energy distributions for galaxies with redshifts 5 < z < 7 to combinations of stellar population templates evolved from z = 12. We exploit NIRCam imaging in seven wide bands covering 1–5 μm taken in the context of the GLASS-JWST-ERS program and use SEDz* to solve for well-constrained star formation histories for 24 exemplary galaxies. In this first look, we find a variety of histories, from long, continuous star formation over 5 < z < 12 to short but intense starbursts, sometimes repeating, and, most commonly, contiguous mass buildup lasting ∼0.5 Myr, possibly the seeds of today’s typical M* galaxies.
Early Results from GLASS-JWST. XIV. A Spectroscopically Confirmed Protocluster 650 Million Years after the Big Bang
Authors: Morishita Takahiro , Roberts-Borsani Guido , Treu Tommaso , Brammer Gabriel , Mason Charlotte A. , Trenti Michele , Vulcani Benedetta , Wang Xin , Acebron Ana , Bahé Yannick , Bergamini Pietro , Boyett Kristan , Bradac Marusa , Calabrò Antonello , Castellano Marco , Chen Wenlei , De Lucia Gabriella , Filippenko Alexei V. , Fontana Adriano , Glazebrook Karl , Grillo Claudio , Henry Alaina , Jones Tucker , Kelly Patrick L. , Koekemoer Anton M. , Leethochawalit Nicha , Lu Ting-Yi , Marchesini Danilo , Mascia Sara , Mercurio Amata , Merlin Emiliano , Metha Benjamin , Nanayakkara Themiya , Nonino Mario , Paris Diego , Pentericci Laura , Rosati Piero , Santini Paola , Strait Victoria , Vanzella Eros , Windhorst Rogier A. , Xie Lizhi 
Published: April 2023

Abstract
We present the spectroscopic confirmation of a protocluster at z = 7.88 behind the galaxy cluster Abell 2744 (hereafter A2744-z7p9OD). Using JWST NIRSpec, we find seven galaxies within a projected radius of 60 kpc. Although the galaxies reside in an overdensity around ≳20× greater than a random volume, they do not show strong Lyα emission. We place 2σ upper limits on the rest-frame equivalent width <16–28 Å. Based on the tight upper limits to the Lyα emission, we constrain the volume-averaged neutral fraction of hydrogen in the intergalactic medium to be x
HI > 0.45 (68% C i). Using an empirical M
UV–M
halo relation for individual galaxies, we estimate that the total halo mass of the system is ≳4 × 1011
M
⊙. Likewise, the line-of-sight velocity dispersion is estimated to be 1100 ± 200 km s−1. Using an empirical relation, we estimate the present-day halo mass of A2744-z7p9OD to be ∼2 × 1015
M
⊙, comparable to the Coma cluster. A2744-z7p9OD is the highest redshift spectroscopically confirmed protocluster to date, demonstrating the power of JWST to investigate the connection between dark-matter halo assembly and galaxy formation at very early times with medium-deep observations at <20 hr total exposure time. Follow-up spectroscopy of the remaining photometric candidates of the overdensity will further refine the features of this system and help characterize the role of such overdensities in cosmic reionization.
Early Results from GLASS-JWST. XV. Properties of the Faintest Red
Sources in the NIRCAM Deep Fields
Authors: Glazebrook K. , Nanayakkara T. , Jacobs C. , Leethochawalit N. , Calabrò A. , Bonchi A. , Castellano M. , Fontana A. , Mason C. , Merlin E. , Morishita T. , Paris D. , Trenti M. , Treu T. , Santini P. , Wang X. , Boyett K. , Bradac Marusa , Brammer G. , Jones T. , Marchesini D. , Nonino M. , Vulcani B. 
Published: April 2023

Abstract
We present a first look at the reddest 2–5 μm
sources found in deep images from the GLASS Early Release Science program. We
undertake a general search, i.e., not looking for any particular spectral
signatures, for sources detected only in bands redder than is reachable with the
Hubble Space Telescope, and which would likely not have been identified in
pre-JWST surveys. We search for sources down to AB ∼27 (corresponding to
>10σ detection threshold) in any of the F200W to F444W filters, with a >1
magnitude excess relative to F090W to F150W bands. Fainter than F444W >25 we
find 56 such sources of which 37 have reasonably constrained spectral energy
distributions to which we can fit photometric redshifts. We find the majority of
this population (∼65%) as 2 < z < 6
star-forming low-attenuation galaxies that are faint at rest-frame
ultraviolet-optical wavelengths, have stellar masses
108.5–109.5
M
⊙, and have observed fluxes at >2 μm
boosted by a combination of the Balmer break and emission lines. The typical
implied rest equivalent widths are ∼200 Å with some extreme objects up to ∼1000
Å. This is in contrast with brighter magnitudes where the red sources tend to be
z < 3 quiescent galaxies and dusty
star-forming objects. Our general selection criteria for red sources allow us to
independently identify other phenomena as diverse as extremely low-mass
(∼108
M
⊙) quiescent galaxies at z < 1,
recovering recently identified z > 11 galaxies
and a very cool brown dwarf.
Early Results from GLASS-JWST. XVI. Discovering a Bluer z ∼ 4–7 Universe through UV Slopes
Authors: Nanayakkara Themiya , Glazebrook Karl , Jacobs Colin , Bonchi Andrea , Castellano Marco , Fontana Adriano , Mason Charlotte , Merlin Emiliano , Morishita Takahiro , Paris Diego , Trenti Michele , Treu Tommaso , Calabrò Antonello , Boyett Kristan , Bradac Marusa , Leethochawalit Nicha , Marchesini Danilo , Santini Paola , Strait Victoria , Vanzella Eros , Vulcani Benedetta , Wang Xin , Yang Lilian 
Published: April 2023

Abstract
We use the GLASS-JWST Early Release Science NIRCam parallel observations to provide a first view of the UV continuum properties of NIRCam/F444W selected galaxies at 4 < z < 7. By combining multiwavelength NIRCam observations, we constrain the UV continuum slope for a sample of 401 galaxies with stringent quality controls. We find that >99% of the galaxies are blue star-forming galaxies with very low levels of dust (Av

β
∼ 0.01 ± 0.33). We find no statistically significant correlation for UV slope with redshift or UV magnitude. However, we find that in general galaxies at higher redshifts and fainter UV magnitudes have steeper UV slopes. We find a statistically significant correlation for UV slope with stellar mass, with galaxies with higher stellar mass showing shallower UV slopes. Individual fits to some of our galaxies reach the bluest UV slopes of β ∼ −3.1 allowed by stellar population models used in this analysis. Therefore, it is likely that stellar population models with a higher amount of Lyman continuum leakage, active galactic nucleus effects, and/or Population III contributions are required to accurately reproduce the rest-UV and optical properties of some of our bluest galaxies. This dust-free early view confirms that our current cosmological understanding of gradual mass + dust buildup of galaxies with cosmic time is largely accurate to describe the ∼0.7–1.5 Gyr age window of the universe. The abundance of a large population of UV faint dust-poor systems may point to a dominance of low-mass galaxies at z > 6 playing a vital role in cosmic reionization.
Improved Clinic Flow and Satisfaction After Lean Implementation in a Pediatric Ophthalmology Clinic
Authors: Bradfield Yasmin , Suneja Aneesh , Coullard Darla , Anderson Kristin 
Published: April 2023

Purpose:
To report outcomes using Lean concepts (FlowOne Lean Consulting, LLC) and implemented changes in a single academic pediatric ophthalmology practice.

Methods:
Lean principles such as patient flow, wasted movement, and non-value added visit time were taught to clinic staff. Spaghetti maps to document patient and staff movement during examinations, patient simulation, and clinic flow exercises were performed prior to implementing clinic changes. Clinic changes included maximizing easily reachable equipment and standardizing equipment in each examination room, physician-controlled doorbells to notify staff for help, and implementing a visual real-time electronic board of patients throughout the entirety of their examination. Patient surveys before and after Lean and staff feedback were obtained.

Results:
Four years of data were collected of patient examination visits after Lean principles were introduced. Prior to Lean implementation, mean pediatric ophthalmology clinic visit times were 120 minutes. Within 3 months of Lean clinic changes, mean visit times reduced to 75 minutes. Four years later, this was sustained at 69 minutes. Clinic templates were modified and increased by 17%. Patient satisfaction surveys before and after demonstrated improved scores from 6.5 to 9.0. Patient survey comments included satisfaction with shorter patient examination visits, less shuffling between examination rooms, less non-value added time, and perception of happier clinic staff. Staff survey comments included receiving fewer parent complaints, feeling less disorganized, being able to troubleshoot in real time, and leaving at an earlier time at the end of the clinic day.

Conclusions:
Lean improved clinic efficiency, reduced patient visit times, and improved patient and staff satisfaction. These improvements were sustained 4 years after Lean principles were implemented.

[
J Pediatr Ophthalmol Strabismus
. 2024;61(1):14–19.]
The Role of Social Media in Strabismus Surgical Experience
Authors: Eatz Tiffany A. , Kalavar Meghana , Birnhak Michael , Al-Khersan Hasenin , Sridhar Jayanth , Cavuoto Kara M. 
Published: April 2023

Purpose:
To understand patients' strabismus surgery experience, including its impact on patients' appearance and psychosocial factors such as anxiety and depression, via trends on popular social media platforms.

Methods:
TikTok and Instagram were searched for the following post hashtags: “#strabismus,” “#strabismussurgery,” “#crosseyed,” and “#lazyeye.” Data regarding date of post, username, gender, city, state, United States or international location, surgical status (preoperative, perioperative, or postoperative), tone (positive or negative), place of treatment, type of post (photo or video), number of likes/views, and number of followers were recorded for statistical analysis.

Results:

A total of 790 posts (400 TikTok, 390 Instagram) were included. The majority (87.8%) had a positive tone, particularly for Instagram (Instagram = 97.7%, TikTok = 78.3%,
P
< .01). TikTok had significantly more likes/follower (
P
< .01), as did negative posts (
P
< .01). #Lazyeye gained significantly more traction than other hashtags (range:
P
< .001 to .006). There were no differences in likes/follower for treatment phase (preoperative/perioperative/postoperative), gender, or relative age of poster (adult/parent/child).

Conclusions:
These findings demonstrated that TikTok and Instagram users tend to share positive strabismus surgical experiences; however, negative posts were associated with more interactive responses from viewers. Colloquial hashtags (eg, #lazyeye) were more likely to gain traction than medical terms. TikTok posts were associated with more engagement than Instagram, which suggests TikTok may be a better platform going forward for patient outreach.

[
J Pediatr Ophthalmol Strabismus
. 2023;60(6):402–405.]
Effectiveness of a Novel Video Game Platform in the Treatment of Pediatric Amblyopia
Authors: Poltavski Dmitri , Adams Richard J. , Biberdorf David , Patrie James T. 
Published: April 2023

Purpose:
To test the non-inferiority of a novel game platform for the treatment of pediatric amblyopia compared to standard eye patching.

Methods:
Forty participants (ages 4 to 18 years) across seven optometric clinics in the United States diagnosed as having amblyopia associated with anisometropia were randomly assigned to either 12 weeks of eye patching therapy (n = 19) or Barron Vision (Barron Associates, Inc) video game treatment (n = 21). Participants in the eye patching group with best corrected visual acuity (BCVA) worse than 20/200 in their amblyopic eye were prescribed 6 hours of patching daily, whereas those whose BCVA was 20/200 (1.00 logarithm of the minimum angle of resolution [logMAR]) or better were instructed to patch for 2 hours daily. Participants in the video game group, irrespective of the severity of their amblyopia, were instructed to play four different 5-minute mini-games five times a week for a total of 20 minutes a day.

Results:
A mixed linear modeling analysis of before and after BCVA differences after 12 weeks showed the non-inferiority of video game treatment to eye patching using a 0.10 logMAR threshold while adjusting for the participant's age, sex, and baseline BCVA.

Conclusions:
The results of the study suggest that a 12-week home-based video game vision therapy intervention can provide equivalent treatment outcomes to eye patching for amblyopia in children ages 5 to 18 years. Video game–based vision therapy may be a more acceptable and time-efficient alternative to existing approaches. By incorporating elements of perceptual learning, approaches such as Barron Vision video game treatment may have additional long-term therapeutic benefits and may improve treatment compliance.

[
J Pediatr Ophthalmol Strabismus
. 2024;61(1):20–29.]