bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGARUH MOTIVASI KERJA, KOMPETENSI DAN KOMPENSASI TERHADAP KINERJA GURU DI YAYASAN PENDIDIKAN NURHASANAH MEDAN
Authors: Surya Indra , Kusnady Diding , Naipospos Nova Yesyca 
Published: February 2022

Yayasan Pendidikan Nurhasanah Medan adalah suatu Lembaga Pendidikan Islam, terletak di Jl. Garu I No 28 Medan. Yayasan ini memiliki 90 orang Guru yang bekerja sebagai pengajar dari tingkat TK, SD, SMP, Mts sampai dengan SMK/SMA. Penelitian ini bertujuan untuk mengetahui dan menganalisa pengaruh Motivasi Kerja, Kompetensi, dan Kompensasi terhadap Kinerja karyawan di Yayasan Pendidikan Nurhasanah Medan. Hasil penelitian menggambarkan bahwa variabel Motivasi kerja dan variabel kompetensi berpengaruh terhadap kinerja karyawan sedangkan variabel kompensasi tidak berpengaruh. Gambaran hasil penelitian yang diperoleh dapat digambarkan dengan persamaan Y = 0,271 + 0,714X1 + 0,409X2 - 0.168 X3, di mana X1 = Motivasi Kerja, X2 = Kompetensi, dan X3 = Kompensasi. Artinya konstanta sebesar 0,271 menyatakan bahwa faktor faktor selain variabel X1, X2, dan X3 yang mempengaruhi kinerja karyawan sebesar 0,271. Koefisien Motivasi kerja sebesar 0,714 menyatakan bahwa apabila variabel X1 bertambah satu satuan akan menambah pengaruh kinerja karyawan sebesar 0.714 dengan anggapan variabel kompetensi dan kompensasi adalah konstan. Koefisien regresi X2 sebesar 0,409 adalah bahwa apabila variabel X2 bertambah satu satuan akan menambah kinerja pegawai sebesar 0,409 dengan anggapan variabel motivasi kerja dan kompensasi adalah konstan. Selanjutnya dengan koefisien regresi X3 sebesar -0,168. Ini berarti bahwa dengan faktor lain dianggap konstan, pengaruh kompensasi lebih kecil dibandingkan dengan motivasi kerja dan kompetensi. Hasil penelitian ini dapat menjadi acuan bagi yayasan Pendidikan Nurhasanah Medan untuk meningkatkan kinerja guru guru. Untuk itu perlu adanya perhatian terhadap motivasi kerja dalam yayasan. Selain itu, perlu juga dilakukan pengembangan kemampuan karyawan secara terus menerus melalui kompetensi dan kompensasi terhadap para guru.
Pengaruh kualitas pelayanan, citra merek dan kepuasan pelanggan terhadap loyalitas pelanggan pada kafe di kota Batam.
Authors: Hanny Hanny , Krisyana Krisyana 
Published: February 2022

Pada era globalisasi sekarang, industri jasa seperti usaha makanan dan minuman sedang berkembang pesat di Indonesia. Dari segi penataan makanan dan minuman yang unik, bagus dan kreatif membuat masyarakat ingin mengonsumsinya. Salah satu makanan yang disukai oleh masyarakat adalah makanan penutup. Dengan semua data survei yang diisi oleh peserta survei, maka peneliti dapat meneliti dan mengetahui apakah terdapat pengaruh kualitas pelayanan, citra merek, dan kepuasan pelanggan terhadap loyalitas pelanggan pada kafe di Kota Batam. Data yang telah terkumpul dilakukan dengan menyebarkan kuesioner melalui internet dan di analisa oleh peneliti untuk membuktikan bahwa variabel-variabel yang bersifat independen seperti kualitas pelayanan, citra merek dan kepuasan pelanggan dapat berpengaruh pada variabel dependen yaitu loyalitas pelanggan.

Setiap variabel ini telah diteliti sebelumnya sehingga peneliti dapat memilih keempat variabel ini sebagai bahan penelitian. Populasi pada penelitian ini adalah penduduk yang tinggal di Kota Batam, penduduk yang pernah mengunjungi kafe di Kota Batam, dan penduduk yang pernah memesan makanan penutup di kafe Kota Batam. Isi penelitian ini dapat berguna bagi berbagai pihak organisasi pariwisata.

Tujuan dilakukan penelitian pada variabel kualitas pelayanan, citra merek, kepuasan pelanggan dan loyalitas pelanggan untuk menambahkan karya ilmiah dan untuk referensi bagi pembaca. Hasil dari penelitian pada variabel independen terdapat pengaruh positif terhadap variabel dependen.
Mirada, territorio, cuerpo y palabra: a propósito de lo que se cuenta sin contar
Authors: Osorio Yoni Alexander 
Published: February 2022

El texto pretende hacer una reflexión sobre la mirada, que, cuando se cultiva, puede visibilizar historias ocultas en los territorios con el objeto de crear memoria, identidad y conciencia de sí. Es una exploración por las historias ocultas tras lo evidente a los ojos; plantea el ejercicio de ver más allá de lo inmediato a los sentidos para reconocer que es más importante aquello no contado, lo que se dice sin decir, y lo que está detrás de cada acontecimiento, que encierra toda una memoria, sobre el territorio, el cuerpo y la identidad.
Typology of innovative projects and directions of their implementation in modern society
Authors: Самигуллин Ф.Ф. 
Published: February 2022

В настоящее время в России быстрыми темпами развивается инновационная составляющая экономики как средство обеспечения технологического лидерства, позволяющего интегрироваться в открытое пространство глобальной конкурентоспособности. В этих условиях важно понимать с позиций осуществления инновационной деятельности сущность инновационного проекта, его особенности, типы и эффективность осуществления на разных уровнях (от микроуровня до макро- и мегауровня).Целью статьи является рассмотрение характеристик инновационного проекта, приведенных в исследованиях ученых, определение направлений реализации инновационных проектов с учетом традиционной и дополненной типологии (разработанной автором), в связи с открывшимися обстоятельствами современной экономикиВ рамках обоснования классификационных признаков инновационных проектов в работе приведена детализация фазы жизненного цикла инновационного проекта по выделенной типологии.
At present, the innovative component of the economy is rapidly developing in Russia as a means of ensuring technological leadership, allowing it to integrate into the open space of global competitiveness. In these conditions, it is important to understand from the standpoint of the implementation of innovative activities the essence of an innovative project, its features, types and efficiency of implementation at different levels (micro-, meso-, macro-, mega).The purpose of the article is to consider the characteristics of an innovative project, given in the research of scientists, to determine the directions for the implementation of innovative projects, taking into account the traditional and amended typology (developed by the author), in connection with the opening circumstances of the modern economyAs part of the substantiation of the classification features of innovative projects, the work provides a detailing of the phase of the life cycle of an innovative project according to the selected typology.
6.2. ISSUES OF FORMATION OF THE MANAGEMENT MECHANISM INNOVATIVE ACTIVITY OF THE ORGANIZATION
Authors: Мисхожев Э.Р. 
Published: February 2022

В статье рассматриваются вопросы формирования механизма управления инновационной деятельностью организации. Анализируются существующие подходы к понятию механизма в системах различного происхождения. Дается авторская интерпретация сущности механизма управления инновационной деятельностью организации, формируется его теоретическая модель. Делается вывод о многообразии путей его реализации.
The article deals with the formation of the mechanism of management of innovative activity of the organization. The existing approaches to the concept of mechanism in systems of various origins are analyzed. The author's interpretation of the essence of the mechanism of management of innovative activity of the organization is given, its theoretical model is formed. The conclusion is made about the variety of ways to implement it.
Energy Extraction via Magnetic Reconnection in the Ergosphere of a Rotating Non-Kerr Black Hole
Authors: Liu Wenshuai 
Published: February 2022

Abstract
Magnetic reconnection in the ergosphere is investigated for a relativistic plasma around a rotating non-Kerr black hole. For a rotating non-Kerr black hole immersed in a magnetic field generated by an externally material, antiparallel magnetic field line could form in the ergosphere due to frame dragging. Therefore, magnetic reconnection could occur in the ergosphere. This magnetic reconnection may generate negative energy at infinity by redistributing the angular momentum during the process. The results show that, taking into account the effect of the deformed parameter, extraction of energy from a rotating non-Kerr black hole by magnetic reconnection could be enhanced in the presence of a positive deformed parameter.
Dissecting Nearby Galaxies with piXedfit. I. Spatially Resolved Properties of Stars, Dust, and Gas as Revealed by Panchromatic SED Fitting
Authors: Abdurro’uf  , Lin Yen-Ting , Hirashita Hiroyuki , Morishita Takahiro , Tacchella Sandro , Akiyama Masayuki , Takeuchi Tsutomu T. , Wu Po-Feng 
Published: February 2022

Abstract
We study spatially resolved properties (on spatial scales of ∼1–2 kpc out to at least 3 effective radii) of the stars, dust, and gas in 10 nearby spiral galaxies. The properties of the stellar population and dust are derived by fitting the spatially resolved spectral energy distribution (SED) with more than 20 photometric bands ranging from far-ultraviolet to far-infrared. Our newly developed software piXedfit performs point-spread function matching of images, pixel binning, and models the stellar light, dust attenuation, dust emission, and emission from a dusty torus heated by an active galactic nucleus simultaneously through the energy-balance approach. With this self-consistent analysis, we present the spatially resolved version of the IRX–β relation, finding that it is consistent with the relationship from the integrated photometry. We show that the old stellar populations contribute to the dust heating, which causes an overestimation of the star formation rate (SFR) derived from the total ultraviolet and infrared luminosities on kiloparsec scales. With archival high-resolution maps of atomic and molecular gas, we study the radial variation of the properties of the stellar populations (including stellar mass, age, metallicity, and SFR), dust (including dust mass, dust temperature, and abundance of polycyclic aromatic hydrocarbon), and gas, as well as dust-to-stellar mass and dust-to-gas mass ratios. We observe a depletion of the molecular gas mass fraction in the central region of the majority of the galaxies, suggesting that the lack of available fuel is an important factor in suppressing the specific SFR at the center.
The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High Redshift
Authors: Garg Prerak , Narayanan Desika , Byler Nell , Sanders Ryan L. , Shapley Alice E. , Strom Allison L. , Davé Romeel , Hirschmann Michaela , Lovell Christopher C. , Otter Justin , Popping Gergö , Privon George C. 
Published: February 2022

Abstract
The Baldwin, Philips, & Terlevich diagram of [O iii]/Hβ versus [N ii]/Hα (hereafter N2-BPT) has long been used as a tool for classifying galaxies based on the dominant source of ionizing radiation. Recent observations have demonstrated that galaxies at z ∼ 2 reside offset from local galaxies in the N2-BPT space. In this paper, we conduct a series of controlled numerical experiments to understand the potential physical processes driving this offset. We model nebular line emission in a large sample of galaxies, taken from the simba cosmological hydrodynamic galaxy formation simulation, using the cloudy photoionization code to compute the nebular line luminosities from H ii regions. We find that the observed shift toward higher [O iii]/Hβ and [N ii]/Hα values at high redshift arises from sample selection: when we consider only the most massive galaxies M
* ∼ 1010–11
M
⊙, the offset naturally appears, due to their high metallicities. We predict that deeper observations that probe lower-mass galaxies will reveal galaxies that lie on a locus comparable to z ∼ 0 observations. Even when accounting for samples-selection effects, we find that there is a subtle mismatch between simulations and observations. To resolve this discrepancy, we investigate the impact of varying ionization parameters, H ii region densities, gas-phase abundance patterns, and increasing radiation field hardness on N2-BPT diagrams. We find that either decreasing the ionization parameter or increasing the N/O ratio of galaxies at fixed O/H can move galaxies along a self-similar arc in N2-BPT space that is occupied by high-redshift galaxies.
Hubble Space Telescope Observations of NGC 253 Dwarf Satellites: Three Ultra-faint Dwarf Galaxies*
Authors: Mutlu-Pakdil Burçin , Sand David J. , Crnojević Denija , Jones Michael G. , Caldwell Nelson , Guhathakurta Puragra , Seth Anil C. , Simon Joshua D. , Spekkens Kristine , Strader Jay , Toloba Elisa 
Published: February 2022

Abstract
We present deep Hubble Space Telescope (HST) imaging of five faint dwarf galaxies associated with the nearby spiral NGC 253 (D ≈ 3.5 Mpc). Three of these are newly discovered dwarf galaxies, while all five were found in the Panoramic Imaging Survey of Centaurus and Sculptor, a Magellan+Megacam survey to identify faint dwarfs and other substructures in resolved stellar light around massive galaxies outside of the Local Group. Our HST data reach ≳3 magnitudes below the tip of the red giant branch for each dwarf, allowing us to derive their distances, structural parameters, and luminosities. All five systems contain mostly old, metal-poor stellar populations (age ∼12 Gyr, [M/H] ≲ −1.5) and have sizes (r

h
∼ 110–3000 pc) and luminosities (M

V
∼ −7 to −12 mag) largely consistent with Local Group dwarfs. The three new NGC 253 satellites are among the faintest systems discovered beyond the Local Group. We also use archival H i data to place limits on the gas content of our discoveries. Deep imaging surveys such as our program around NGC 253 promise to elucidate the faint end of the satellite luminosity function and its scatter across a range of galaxy masses, morphologies, and environments in the decade to come.
Frequency Evolution Behavior of Pulse Profile of PSR B1737+13 with the Inverse Compton Scattering Model
Authors: Zhi Q. J. , Xu X. , Shang L. H. , Qiao G. J. , Bai J. T. , Dang S. J. , Zhao R. S. , Dong A. J. , Zhang D. D. , Lin Q. W. , Yang H. 
Published: February 2022

Abstract
The radio radiation mechanism is one of the open questions in pulsar physics. Multiband observations are very important for constraining the pulsar radiation mechanism. In this paper, we investigate the pulse profiles of PSR B1737+13 and its evolution with the frequency. The integrated pulse profiles are obtained from the European Pulsar Network and the Australia Telescope National Facility data, together with recent observations from the largest dish Five-hundred-meter Aperture Spherical radio Telescope. The radiation components are separated with the squared hyperbolic secant functions, and the radiation altitudes of each radiation component at different frequencies are calculated. It is found that the radio radiation at different frequencies comes from different altitudes. The frequency evolutions of separations for the inner and outer cone components are studied. It is found that the separations of the inner and outer cone components have opposite frequency dependence. We simulate the RFM of PSR B1737+13 with the inverse Compton scattering (ICS) model and find that the RFM can be naturally described by the ICS model. Through the simulation, the radio radiation region of PSR B1737+13 is determined, and the result shows that the radio radiation of this pulsar may be generated in the annular gap region.
Large Binocular Telescope Search for Companions and Substructures in the (Pre)transitional Disk of AB Aurigae
Authors: Jorquera Sebastián , Bonnefoy Mickaël , Betti Sarah , Chauvin Gaël , Buenzli Esther , Pérez Laura M. , Follette Katherine B. , Hinz Philip M. , Boccaletti Anthony , Bailey Vanessa , Biller Beth , Defrère Denis , Eisner Josh , Henning Thomas , Klahr Hubert , Leisenring Jarron , Olofsson Johan , Schlieder Joshua E. , Skemer Andrew J. , Skrutskie Michael F. , Van Boekel Roy 
Published: February 2022

Abstract
Multiwavelength high-resolution imaging of protoplanetary disks has revealed the presence of multiple, varied substructures in their dust and gas components, which might be signposts of young, forming planetary systems. AB Aurigae bears an emblematic (pre)transitional disk showing spiral structures observed in the inner cavity of the disk in both the submillimeter (Atacama Large Millimeter/submillimeter Array (ALMA); 1.3 mm, 12CO) and near-infrared (Spectro-polarimetric High-contrast Exoplanet Research; 1.5–2.5 μm) wavelengths, which have been claimed to arise from dynamical interactions with a massive companion. In this work, we present new deep K
s (2.16 μm) and L′ (3.7 μm) band images of AB Aurigae obtained with the L/M-band Infrared Camera on the Large Binocular Telescope, aimed for the detection of both planetary companions and extended disk structures. No point source is recovered, in particular at the outer regions of the disk, where a putative candidate (ρ = 0.″681, PA = 7.°6) had been previously claimed. The nature of a second innermost planet candidate (ρ = 0.″16, PA = 203.°9) cannot be investigated by the new data. We are able to derive 5σ detection limits in both magnitude and mass for the system, going from 14 M
Jup at 0.″3 (49 au) down to 3–4 M
Jup at 0.″6 (98 au) and beyond, based on the ATMO 2020 evolutionary models. We detect the inner spiral structures (<0.″5) resolved in both CO and polarimetric H-band observations. We also recover the ring structure of the system at larger separation (0.″5–0.″7) showing a clear southeast/northwest asymmetry. This structure, observed for the first time at L′ band, remains interior to the dust cavity seen at ALMA, suggesting an efficient dust trapping mechanism at play in the disk.
Faut-il brûler les règles budgétaires ? Leçons de l’expérience américaine (1988-2017)
Authors: Farvaque Étienne , Joanis Marcelin , Ooghe Nicolas 
Published: February 2022

L’étude des règles budgétaires en vigueur dans les États américains, pour la plupart depuis très longtemps, permet de juger si leur effet est pro ou contra-cyclique face à un choc. Nous analysons les ajustements budgétaires mis en œuvre, non seulement en étudiant les variations des dépenses et des impôts, mais aussi en intégrant la volatilité de l’emploi public. Nous utilisons une classification des règles budgétaires plus détaillée que celle couramment utilisée dans la littérature et intégrons également les fonds de stabilisation (Rainy Day Funds), qui offrent un instrument de lissage de la conjoncture, pour les États en possédant. Nous montrons que, pour les États américains en cycle budgétaire annuel, les règles budgétaires ne sont pas neutres : le nombre de règles budgétaires dans la phase de mise en œuvre du budget exerce une fonction limitative sur le budget, notamment si elles sont de nature constitutionnelle. Ce sont ces règles qui contraignent les gouverneurs à opérer des ajustements budgétaires, et ce avec un effet amplifié en fonction de la force d’un choc non anticipé (générant donc un comportement procyclique).
Could the Public Debt Management via ECB’s QE Create a Surge of Inflation in the Euro Area?
Authors: Papadamou Stephanos , Sidiropoulos Moïse , Vidra Aristea 
Published: February 2022

Sur la base de l’expérience récente des programmes d’assouplissement quantitatif (QE) avec des taux d’intérêt négatifs adoptés par la BCE après la crise de la dette publique dans la zone euro (2010-2011) et face à la pandémie en 2020, nous étudions les effets de sa récente politique monétaire non conventionnelle sur la poussée de l’inflation dans la zone euro via le mécanisme des marges de crédit des banques. En utilisant la méthodologie des modèles « Panel Vector Autoregressive » (PVAR) sur huit États membres de la zone euro, cette étude suggère qu’une expansion du bilan de la BCE due à la monétisation de la dette publique génère un faible effet positif sur l’inflation de la zone euro lorsqu’elle s’accompagne aussi d’une politique de taux négatifs. Ceci valide le résultat selon lequel « la crainte exprimée par certains que l’excédent monétaire résultant des injections massives de liquidités via l’assouplissement quantitatif puisse conduire à de l’inflation dans la zone euro ne résiste pas à l’épreuve » (De Grauwe [2021]) ainsi que la proposition de Christine Lagarde [2021] réitérant que le programme de QE de la BCE se poursuivra et qu’il n’est pas envisagé de relever les taux d’intérêt en 2022.
Characterisation of seriousness and outcome of adverse drug reactions in patients received cancer chemotherapy drugs – A prospective observational study
Authors: Fatmi Syed Meraj , Bagati Kavita Dhar , Dutta Shaktibala , Sharma Jyotsna 
Published: February 2022

Background:
Cancer chemotherapeutic drugs are commonly associated with serious adverse effect which contributes to increase in the duration of hospitalisation and economic burden.

Aim:
The aim of this study was to characterise the seriousness and outcome of adverse drug reactions (ADRs) produced by chemotherapy drugs in cancer patients.

Materials and Methods:
Patient's demographic characteristics and ADRs due to chemotherapeutic drugs were documented inpatient case report form. Frequencies of the seriousness of the ADRs, its outcome and preventability were studied using descriptive statistics. Proportion of life-threatening ADRs and ADRs linked to increase in duration of hospitalisation were studied. Factors associated with serious ADRs and patient characteristics were studied using calculation of odds ratio (OR) at 95% confidence interval (P < 0.5).

Results:
A total of 412 ADRs were noted in selected 120 patients received chemotherapy drugs. Majority of ADRs (61%) were linked to increase in duration of hospital admission. Some ADRs (12%) were noted as life-threatening to the patients. OR 1.58 was found on the association between patient age group and serious ADRs (P = 0.02). Association of preventability of ADRs and serious ADRs shows OR of 3.65 (P = 0.0001). Common serious ADRs were noted as anaemia, neutropenia, fever, thrombocytopenia, diarrhoea, mucositis and nausea and vomiting.

Conclusion:
The incidence of serious ADRs due to chemotherapy drugs amongst cancer patients is high. Studies on the nature of seriousness of ADRs, outcome and its triggering factors may help to prevent them. Early identification of serious ADRs may support to reduce hospital stay and economic burden.
Multifocal Unilateral Wilms’ Tumor: Radiopathological Correlation
Authors: Reddy Ravikanth 
Published: February 2022

Abstract
Wilms’ tumor constitutes majority of malignant primary renal tumors in children. Outcomes of treatment are excellent in Wilms’ tumor, with a cumulative survival rate of 87%. A combination of imaging and histopathology is needed for confirmation of Wilms’ tumor. However, imaging alone can be used for screening, diagnostic workup, assessment of response to treatment, preoperative evaluation, and follow-up for recurrence. In malignant primary tumors such as Wilms’ tumor, where the outcomes following treatment are excellent, management strategies are aimed at risk-based stratification approach, thereby improving the quality of life in children with high-grade tumors while maintaining extremely good outcomes in the pediatric age group with low-grade tumors. This case report describes a rare sonological appearance of multifocal unilateral Wilms’ tumor in a 4-month-old infant.