bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGARUH QUALITY OF WORK LIFE TERHADAP WORK ENGAGEMENT PADA PEGAWAI NEGERI SIPIL (PNS) YANG BELUM MENIKAH
Authors: Pertiwi Nisa Indah , Harding Diana , Yanuarti Nurul 
Published: May 2021

ABSTRAK. Work engagement diketahui sebagai sumber bagi keberhasilan performa kerja individu dalam organisasi. Dalam hal ini, quality of work life menjadi salah satu topik yang menarik sebagai dasar dalam membentuk work engagement. Penelitian ini bertujuan untuk mengetahui pengaruh quality of work life terhadap work engagement pada Pegawai Negeri Sipil (PNS) yang belum menikah. Penelitian ini menggunakan metode kuantitatif non-eksperimental yang dilakukan kepada 63 orang PNS yang belum menikah. Alat ukur quality of work life menggunakan adaptasi kuesioner quality of work life dari Timossi dan work engagement menggunakan adaptasi alat ukur the Utrecht Work Engagement Scale (UWES-17). Teknik analisis data menggunakan uji regresi linier sederhana. Hasil penelitian menunjukkan bahwa quality of work life berpengaruh terhadap work engagement pada PNS yang belum menikah. Aspek development using human capacity memiliki kontribusi terbesar bagi quality of work life dalam mempengaruhi work engagement.

ABSTRACT. Work engagement has been known as a source for the succes of individual work performance in the organization. In this case, quality of work life is an interesting topic as a basis for forming work engagement. This study aimed determine the effect of quality of work life on work engagement among unmarried Civil Servants (PNS). This study used non-experimental quantitative method which was conducted on 63 unmarried Civil Servants. Quality of work life instrument was adapted from quality of life questionnaire from Timossi and work engagement instrument was adapted from the Utrecht Work Engagement Scale (UWES-17). The data was analyzed through simple linear regression analysis. The results of this study showed the quality of work life has an effect on work engagement of unmarried Civil Servants. Development using human capacity has the greatest contribution to the quality of work life in effecting work engagement.
Abordaje de diagnóstico y terapéutico de la toxoplasmosis congénita
Authors: Ollos Méndez Jessica , Ruiz Plúas Génesis , Roca Castillo Hugo , Olvera Morán Yamel 
Published: May 2021

La toxoplasmosis es una zoonosis que representa la segunda causa de infección congénita, se adquiere por primera vez cuando la infección por el parasito toxoplasma gondii infecta a una mujer embarazada, es importante detener las trasmisiones y el tratamiento oportuno para disminuir el riesgo de la trasmisión vertical, así como el desarrollo de manifestaciones clínicas en el feto. El diagnóstico de toxoplasmosis congénita puede no ser concluyente en muchos casos. A pesar de las diversas pruebas serológicas desarrolladas, la literatura sobre biomarcadores que pueden ayudar en el diagnóstico de toxoplasmosis congénita y aguda es limitada. El objetivo de este estudio fue analizar el perfil inmunorreactivo de las bandas proteicas de T. gondii con potencial de ser biomarcadores para el diagnóstico y pronóstico de la toxoplasmosis congénita y aguda. El objetivo de este estudio es actualizar los referentes teóricos sobre los métodos diagnósticos para determinar la infección de toxoplasmosis congénita. Se realizó una búsqueda sistemática de investigaciones recientes en bases de datos de Elsevier, Pubmed y Scopus de articulos publicados entre el 2016 al 2020, de idioma inglés y español. Se excluyeron artículos de reportes de casos. La finalidad de esta revisión es ofrecer a los médicos una información y orientación actualizada para optimizar su métodos diagnósticos y terapéuticos y error e la práctica de la atención primaria de salud, sobre todo, por las diferencias entre infección aguda y crónica de la toxoplasmosis congénita.
Luxación recidivante de tendones peroneos: clínica y tratamiento quirúrgico
Authors: Jiménez Plaza Wilson , Soto Viera Paola , Vega Sandoval Michelle , Macías Dumes Alfonso 
Published: May 2021

La subluxación del tendón peroneo es un trastorno relativamente raro que a menudo se diagnostica erróneamente como un esguince de tobillo. Afecta principalmente a adultos jóvenes, generalmente durante la actividad deportiva. Se debe principalmente a la avulsión del retináculo peroneo superior de su inserción peronea, que requiere intervención quirúrgica, especialmente en los casos de subluxación y/o luxación crónica sintomática del tendón peroneo. El objetivo de la presente revisión es discutir los aspectos fundamentales del tratamiento quirúrgico de la luxación recidivante de los tendones peroneos. La finalidad de esta revisión es proporcionar las herramientas y claves diagnósticas para la identificación oportuna de la patología. Se seleccionó literatura científica relevante con un enfoque en el manejo quirúrgico, de un total de 34 artículos seleccionados de enero del 2010 a marzo del 2021, se excluyeron los estudios de ensayos clínicos y metaanálisis, quedando para el análisis 15 artículos. La finalidad de esta revisión es proporcionar una actualización de la enfermedad para ampliar los conocimientos y mejorar la calidad de atención.
An Asymmetric Dust Ring around a Very Low Mass Star ZZ Tau IRS
Authors: Hashimoto Jun , Dong Ruobing , Muto Takayuki 
Published: May 2021

Abstract
We present Atacama Large Millimeter/submillimeter Array (ALMA) gas and dust observations at band 7 (339 GHz: 0.89 mm) of the protoplanetary disk around a very low mass star ZZ Tau IRS with a spatial resolution of 025. The 12CO J = 3 → 2 position–velocity diagram suggests a dynamical mass of ZZ Tau IRS of ∼0.1–0.3 M
☉. The disk has a total flux density of 273.9 mJy, corresponding to an estimated mass of 24–50 M
⊕ in dust. The dust emission map shows a ring at r = 58 au and an azimuthal asymmetry at r = 45 au with a position angle of 135°. The properties of the asymmetry, including radial width, aspect ratio, contrast, and contribution to the total flux, were found to be similar to the asymmetries around intermediate mass stars (∼2 M
☉) such as MWC 758 and IRS 48. This implies that the asymmetry in the ZZ Tau IRS disk shares a similar origin with others, despite the star being ∼10 times less massive. Our observations also suggest that the inner and outer parts of the disk may be misaligned. Overall, the ZZ Tau IRS disk shows evidence of giant planet formation on a ∼10 au scale at a few megayears. If confirmed, it will challenge existing core accretion models in which such planets have been predicted to be extremely hard to form around very low mass stars.
The Thermal Reprocessing of Reflected Radiation in the AGN Accretion Disk
Authors: Zhong Xiaogu , Wang Jiancheng 
Published: May 2021

Abstract
We present a reflected reprocessing model to study the thermal lag–wavelength relationship in the AGN accretion disk. The main radiation produced from the corona assumed with the lamppost geometry on the axis of the black hole irradiates the accretion disk to affect the temperature structure via reflection processes. Considering the thermal emission of the disk responded to coronal irradiation, we obtain the lag–wavelength relationship of the disk emission by calculating the response function. We then fit the observed data of four Seyfert 1–1.5 galaxies, NGC4151 , Mrk509, NGC5548, and NGC4593, to test the reflected reprocessing model compared with the X-ray spectrum fitting, and the main results present as follows: (I) The actual geometry of the disk corona is more complex than the lamppost. (II) The option of the reference band is sensitive to fitting the observed time lags. (III) The intrinsic bolometric luminosity is larger than the observed luminosity.
Puffed-up Edges of Planet-opened Gaps in Protoplanetary Disks. I. Hydrodynamic Simulations
Authors: Bi 毕 Jiaqing 嘉擎 , Lin 林 Min-Kai 明楷 , Dong 董 Ruobing 若冰 
Published: May 2021

Abstract
Dust gaps and rings appear ubiquitous in bright protoplanetary disks. Disk–planet interaction with dust trapping at the edges of planet-induced gaps is one plausible explanation. However, the sharpness of some observed dust rings indicate that sub-millimeter-sized dust grains have settled to a thin layer in some systems. We test whether or not such dust around gas gaps opened by planets can remain settled by performing three-dimensional, dust-plus-gas simulations of protoplanetary disks with an embedded planet. We find planets massive enough to open gas gaps stir small, sub-millimeter-sized dust grains to high disk elevations at the gap edges, where the dust scale height can reach ∼70% of the gas scale height. We attribute this dust “puff up” to the planet-induced meridional gas flows previously identified by Fung & Chiang and others. We thus emphasize the importance of explicit 3D simulations to obtain the vertical distribution of sub-millimeter-sized grains around gas gaps opened by massive planets. We caution that the gas-gap-opening planet interpretation of well-defined dust rings is only self-consistent with large grains exceeding millimeter size.
The GALAH Survey: No Chemical Evidence of an Extragalactic Origin for the Nyx Stream
Authors: Zucker Daniel B. , Simpson Jeffrey D. , Martell Sarah L. , Lewis Geraint F. , Casey Andrew R. , Ting 丁 Yuan-Sen 源森 , Horner Jonathan , Nordlander Thomas , Wyse Rosemary F. G. , Zwitter Tomaž , Bland-Hawthorn Joss , Buder Sven , Asplund Martin , De Silva Gayandhi M. , D’Orazi Valentina , Freeman Ken C. , Hayden Michael R. , Kos Janez , Lin Jane , Lind Karin , Schlesinger Katharine J. , Sharma Sanjib , Stello Dennis 
Published: May 2021

Abstract
The results from the ESA Gaia astrometric mission and deep photometric surveys have revolutionized our knowledge of the Milky Way. There are many ongoing efforts to search these data for stellar substructure to find evidence of individual accretion events that built up the Milky Way and its halo. One of these newly identified features, called Nyx, was announced as an accreted stellar stream traveling in the plane of the disk. Using a combination of elemental abundances and stellar parameters from the GALAH and Apache Point Observatory Galactic Evolution Experiment (APOGEE) surveys, we find that the abundances of the highest likelihood Nyx members are entirely consistent with membership of the thick disk, and inconsistent with a dwarf galaxy origin. We conclude that the postulated Nyx stream is most probably a high-velocity component of the Milky Way’s thick disk. With the growing availability of large data sets including kinematics, stellar parameters, and detailed abundances, the probability of detecting chance associations increases, and hence new searches for substructure require confirmation across as many data dimensions as possible.
The In Situ Exploration of a Relict Ocean World: An Assessment of Potential Landing and Sampling Sites for a Future Mission to the Surface of Ceres
Authors: Scully Jennifer E. C. , Baker Samantha R. , Castillo-Rogez Julie C. , Buczkowski Debra L. 
Published: May 2021

Abstract
The Dawn orbiter’s exploration of Ceres, the most water-rich body in the inner solar system after Earth, revealed the dwarf planet to be a relict ocean world of great interest to the astrobiology and ocean worlds communities. Evidence for an early global subsurface ocean is preserved in Ceres’ surface minerals. While most of the subsurface ocean froze billions of years ago, its liquid (preserved in a deep brine reservoir) and solid remnants are responsible for spectacular surface features such as the faculae in the Occator crater, Ahuna Mons, and Haulani crater. Therefore, the next step in Ceres exploration is an in situ mission to the surface, with these three features being among the most scientifically compelling targets. Here we demonstrate the process of identifying potential landing/sampling sites. Using the highest resolution data obtained by Dawn (up to ∼5 m/pixel in Occator and up to ∼35 m/pixel elsewhere), we identify safe and scientifically compelling potential landing/sampling sites in these three regions. For future landing/sample return, higher spatial resolution data (a few decimeters per pixel to ∼1 m/pixel) than are currently available are needed to identify hazards on the scale of a ∼1–5 m lander. Such data could be obtained in an orbital reconnaissance phase prior to landing/sampling. Orbital reconnaissance, in combination with terrain relative navigation/hazard avoidance, and the ability to land within a ≦100 m diameter circle (>800,000 of which fit within Occator), makes it highly likely that safe and scientifically compelling landing/sampling sites could be reached by a future in situ mission.
Posterior Chamber Phakic Intraocular Lens Implantation for Refractive Correction in Corneal Ectatic Disorders: A Review
Authors: Kalra Nidhi , Asif Mohamed Ibrahime , Bafna Rahul Kumar , Sharma Namrata , Sinha Rajesh 
Published: May 2021

PURPOSE:
To summarize the indications and outcomes of posterior chamber phakic intraocular lens (PIOL) implantation in corneal ectasias including keratoconus, pellucid marginal degeneration (PMD), post-refractive surgery, and post-keratoplasty ectasias.

METHODS:
A review of the literature was conducted using the relevant keywords from various databases up to August 15, 2020. All pertinent studies were reviewed, and the relevant articles were studied in detail for efficacy, stability, predictability, and safety outcomes. In addition, visual quality, corneal biomechanical outcomes, complications, the role of posterior chamber PIOL in combination treatment, and comparison of posterior chamber PIOL with other PIOLs for ectasias were also evaluated.

RESULTS:
A total of 30 relevant studies (13 prospective, 13 retrospective, 4 case reports) on the subject were studied and summarized. All studies showed a favorable refractive outcome. Quality of vision remained unaffected and no significant complications were reported in any of the studies.

CONCLUSIONS:
Posterior chamber PIOLs represent a viable option in the treatment of mild to moderate and stable corneal ectasia in patients with contact lens intolerance who have low irregular astigmatism, a clear central cornea, and good preoperative corrected distance visual acuity.

[
J Refract Surg
. 2021;37(5):351–359.]
The Relationship Between the Change of Intraocular Lens Position and Capsular Bend After Cataract Surgery
Authors: Chang Pingjun , Li Xiuyuan , Chen Dongjie , Xu Zhizi , Ding Xixia , Zhao Yun-e 
Published: May 2021

PURPOSE:
To explore the relationship between the change in intraocular lens (IOL) position and capsular bend after cataract surgery.

METHODS:
Patients underwent phacoemulsification and IOL implantation (Alcon Laboratories, Inc). Patients were divided into two groups based on preoperative axial length: long axial length group (axial length ⩾ 26 mm) and normal axial length group (axial length > 22 but < 26 mm). Swept-source optical coherence tomography was performed at 1 day, 1 week, 1 month, and 3 months after mydriasis to obtain postoperative aqueous depth (PAD) and capsular bend index (CBI). The relationship between CBI and PAD changes was analyzed.

RESULTS:

Eighty patients (80 eyes) were included in the study. PAD decreased gradually from 1 day to 1 week and increased from 1 week to 3 months. Mean CBI was moderately positively correlated with PAD changes (
r
= 0.586,
P
< .001). The IOL moved forward gradually when the CBI was less than 2.30 and the IOL gradually moved backward when the CBI was 2.30 or greater. The root mean square of the change in PAD was smaller in the long axial length group (0.08 ± 0.04 mm) than in the normal axial length group (0.09 ± 0.05 mm) during the 3 months after surgery (
P
= .036).

CONCLUSIONS:
The position of the IOL was almost stable 1 month after operation, and postoperative capsule adhesion mainly occurred within 1 month. The change in PAD was related to capsule adhesion. The postoperative position of the IOL was relatively stable and capsular bend was relatively slow for the long axial length group over 3 months.

[
J Refract Surg
. 2021;37(5):324–330.]
Predictability of Refractive Outcome of a Small-Aperture Intraocular Lens in Eyes With Irregular Corneal Astigmatism
Authors: Langer Julian , Shajari Mehdi , Kreutzer Thomas , Priglinger Siegfried , Mayer Wolfgang J. , Mackert Marc J. 
Published: May 2021

PURPOSE:
To compare different new-generation biometric formulas and ray-tracing for small-aperture intraocular lens (IOL) (IC-8; Acufocus, Inc) implantation in patients undergoing cataract and refractive lens exchange surgery with highly irregular corneas.

METHODS:
This monocenter study included 17 eyes of 17 patients with highly irregular corneas of different genesis. Biometric and topographic corneal data were assessed using the IOLMaster 700 (Carl Zeiss Meditec) and Pentacam (Oculus Optkigeräte GmbH). Prediction and absolute error were compared after 3 months based on manifest refraction. Furthermore, change of total corneal refractive power in different corneal pathologies was also evaluated. For IOL power calculation, three fourth-generation IOL formulas were compared (Haigis, SRK-T, and Barrett Universal II). The dataset was then checked against ray-tracing and analyzed to improve prediction error in these highly irregular corneas.

RESULTS:
All patients showed an improvement in visual acuity postoperatively with a mean spherical equivalent of −1.22 ± 0.49 diopters (D). Overall comparison of the three formulas showed the Haigis formula to be superior in terms of the smallest deviation of predictive and absolute error. IOL calculations with ray-tracing were possible in all eyes, but showed inaccurate results with keratometric values of 48.00 D and greater.

CONCLUSIONS:
The IC-8 IOL is well suited for patients with lens exchange in highly irregular corneas. The Haigis formula seemed to be the most accurate in the patient group. Ray-tracing confirmed the results of biometric formulas up to a keratometric value of 48.00 D and should be compared with standard biometric formulas to address corneal irregularities and to minimize refractive surprises after surgery. A comparison with ray-tracing in eyes with a keratometric value of greater than 48.00 D should not be considered due to the inaccurate results.

[
J Refract Surg
. 2021;37(5):312–317.]
Vegetation and flora of the river-basin of the Gačnik stream (Vojsko, Spodnja Trebuša) – a contribution for its nature protection evaluation / Rastje in rastlinstvo povodja Gačnika na Vojskem in v Trebuši – prispevek za njegovo naravovarstveno vrednotenje
Authors: Dakskobler Igor , Čar Jože , Rudolf Anka , Terpin Rafael , Vreš Branko 
Published: May 2021

We have summarized results of our research of vegetation and flora in the river-basin of the Gačnik (Vojsko, Dolenja Trebuša) in western Slovenia. We enumerate most frequent and characteristic plant communities, which belong to seven habitat types of European conservation importance. In their stands grow two Natura 2000 species (Primula carniolica, Cypripedium calceolus) and almost 60 vascular plant species, which are protected and (or) on the red list. Among communities and plants are the most threatened fens and moist grasslands and their characteristic species: Drosera rotundifolia, Dactylorhiza lapponicasubsp. rhaetica, D. traunsteineri, Eleocharis quinqueflora,Eriophorum angustifolium, E. latifolium, Pinguicula vulgaris and Trichophorum alpinum.
Key words: vegetation, flora, wetlands, fens, Natura 2000, Slovenia

Izvleček
V članku smo povzeli rezultate naših raziskav rastja in rastlinstva v povodja Gačnika na Vojskem in v Trebuši v zahodni Sloveniji. Naštevamo najbolj pogoste in najbolj značilne rastlinske združbe, zavarovane in redke rastline in naravovarstveno vredne habitatne tipe. Slednjih je vsaj sedem. V njihovih združbah uspevata dve Natura 2000 vrsti (Primula carniolica, Cypripedium calceolus) in skoraj 60 zavarovanih in (ali) redkih cevnic (rdeči seznam). Med združbami so najbolj ogrožena mokrišča (nizka barja in mokrotni travniki) in njihove značilne vrste: Drosera rotundifolia, Dactylorhiza lapponicasubsp. rhaetica, D. traunsteineri, Eleocharis quin­queflora,Eriophorum angustifolium, E. latifolium, Pinguicula vulgaris in Trichophorum alpinum.
Ključne besede: vegetacija, flora, mokrišča, nizka barja, Natura 2000, Slovenija
Stratégie-cadre d’éducation relative à l’environnement auprès des adultes pour la construction de systèmes agroalimentaires socialement équitables et écologiquement responsables
Authors: Bisquert i Pérez Kylyan Marc , Agundez-Rodriguez Adolfo 
Published: May 2021

L’évolution des systèmes agroalimentaires a été déterminant pour le développement des sociétés humaines. Ainsi, de nos jours, le système hégémonique en place induit des modes de production, de distribution et de consommation alimentaires qui participent de façon majeure à la crise socio-environnementale. Dans un tel contexte, un changement de paradigme agroalimentaire s’impose afin de promouvoir les transformations nécessaires à la transition écosociale. La création d’espaces de réflexion collective et de co-construction de systèmes agroalimentaires alternatifs apparaît comme un contexte privilégié pour contribuer à un tel changement. À cet égard, l’éducation peut jouer un rôle de premier ordre : elle peut stimuler la mise en place de tels espaces, accompagner l’apprentissage qui s’y réalise et inviter à l’analyse, à la discussion et à la diffusion d’initiatives porteuses. Cet article propose en ce sens des éléments essentiels à l’élaboration d’une stratégie-cadre d’action socio-éducative auprès des adultes, inspirée du courant écologiste de l’éducation relative à l’environnement et basée sur les principes de l’agroécologie.
De l’intérêt au savoir : le processus de l’apprentissage chez Dewey et Bachelard
Authors: Charbonnier Sébastien 
Published: May 2021

Il s’agit, dans cet article, de rapprocher les pensées, a priori opposées, de Dewey et Bachelard concernant le rôle et le fonctionnement de l’apprentissage. Les thèmes abordés correspondent à l’ordre génétique de production de la connaissance. Se pose d’abord le problème de la dialectique entre l’intérêt et l’effort. Comment susciter le désir d’apprendre chez les élèves ? En même temps, comment gérer les impulsions premières qui sont autant d’obstacles à la connaissance ? Les deux auteurs partagent une même défiance vis-à-vis de la paresse intellectuelle des explications du sens commun, mais savent prendre en compte la nécessité d’« intéresser » les élèves pour autoriser un effort qui ne soit pas une souffrance. Une fois l’amorce du processus d’apprentissage établie, se pose le problème de la nature du savoir offert à l’apprentissage. Celui-ci n’est plus contemplation passive mais expérimentation active. La connaissance n’est plus un état, elle est un devenir – elle se situe « dans » le passage. Il s’agit donc de partir de ce que les élèves savent pour travailler dessus. L’épistémologie suit la psychologie : de même qu’il faut partir des intérêts actuels des élèves pour les réformer, de même il faut partir des connaissances des élèves pour les rectifier. Quelle est alors la conception de la relation enseignante qui découle d’un savoir conçu de cette sorte ? Le cogito se dédouble dans les deux figures du maître et de l’élève, désormais interchangeables alternativement. On ne corrige plus l’élève, on se corrige les uns les autres. Le savoir se construit comme la perspective générale des erreurs rectifiées. Il en résulte une pédagogie relationnelle en un sens non seulement intersubjectif mais transcendantal. Le maître et l’élève sont moins des personnes physiques que des « personnages conceptuels » qui correspondent à des moments de la pensée.