bluuebunny/crossref_metadata_2025_split huggingface dataset:
Bloodstream infection by candida in patients with hematologic neoplasia: polyphasic taxonomy and antifungal susceptibility / Infecção sanguínea por candida em pacientes com neoplasia hematológica: taxonomia polifásica e suscetibilidade antifúngica
Authors: Diniz Madi Veiga , De Araújo Paulo Sérgio Ramos , Barbosa Rodrigo Niskier Ferreira , Neto Reginaldo Gonçalves de Lima , Inácio Cícero Pinheiro , Gimino Nadja Maria Rocha , De Assis Reijane Alves , Lima Kledoaldo , Neves Rejane Pereira 
Published: March 2022

Bloodstream infection (BSI) by species of Candida has been identified as an important cause of death in patients with neutropenia who undergo chemotherapy for the treatment of hematologic malignancies This study aimed to verify the occurrence of bloodstream infections by Candida species in patients admitted to the haematology-oncology service of a public hospital specialized in the treatment of cancer in Northeast Brazil. A total of 105 clinical samples from 62 patients with haematological malignancies were analyzed at the Laboratory of Medical Mycology at the Federal University of Pernambuco. Only 7 of 105 individuals were in the ICU environment. The mycological diagnosis was performed through automation (BACTEC 9120 / PHOENIX™), proteomic identification (MALDI-TOF MS) and molecular analysis (PCR). The antifungal susceptibility test followed the bloodstream infection recommendations of Clinical Laboratory Standards Institute. Among the samples studied, nine strains (8,57%) were of the genus Candida, being six C. tropicalis and three C. albicans. The isolates were completely susceptible to the antifungal agents tested. Deaths occurred in 66,6% of the cases. Patients with hematologic malignancies hospitalized in intensive care and the state of septic shock present a higher risk of occurrence of BSI by Candida and death by this opportunistic pathogen.
Highly efficient voltage-controlled magnetism in HfZrO/CoFeB hybrid film and Hall device
Authors: Chen Jia , Zhao Lei , Tian Guoliang , Yang Tengzhi , Cao Wei , Xu Jing , Gao Jianfeng , Li Junfeng , Wang Wenwu , Kang Jin , Bu Weihai , Zheng Kai , Yang Bingjun , Yue Lei , Cui Yan , Luo Jun 
Published: March 2022

Abstract
We investigate the voltage-controlled magnetism effect of HfZrO/CoFeB hybrid film and a Hall device with perpendicular magnetic anisotropy. The magnetization versus magnetic field experiments and anomalous Hall experiments before and after applying voltage are performed. The results exhibit that the coercive field of samples remain unchanged while the saturation magnetization shows a permanent increase (more than 60%), which is regardless of the direction of applied voltage. Different from conventional voltage-controlled magnetic anisotropy, in our work, only the saturation magnetization is enhanced by the applied voltage without trading off other magnetic parameters of CoFeB. Thus, such a finding proposes a more efficient voltage-controlled method to achieve a magnetic memory device with high thermal stability, high tunnel magnetoresistance and low switching current for magneto-resistive random-access memory under scaling beyond 2X nm.
Pola Komunikasi Orang Tua dalam Pengelolaan Siswa Berkebutuhan Khusus di Sekolah Luar Biasa
Authors: Syah Alif Arfian 
Published: March 2022

Penelitian ini memiliki tujuan untuk mendeskripsikan strategi sekolah dalam mengkomunikasikan pengelolaan siswa berkebutuhan khusus. Metode yang digunakan adalah dengan metode kualitatif, dengan rencana penelitian studi kasus. Tempat penelitian ini di SLB Negeri Cendono Kudus. Teknik pengumpulan data dalam penelitian ini adalah menggunakan metode wawancara secara mendalam, observasi dan dokumentasi. Teknik analisis data yang digunakan adalah reduksi data, display data, dan penarikan kesimpulan. Hasil penelitian ini menunjukkan bahwa strategi sekolah dalam mengkomunikasikan pengelolaan siswa berkebutuhan khusus adalah melalui kelas orang tua berkomunikasi dengan guru bayangan, dan wali kelas berkomunikasi langsung dengan siswa orang tua. Strategi menggunakan pemanfaatan media elektronik seperti media sosial, buku penghubung serta pertemuan langsung dengan orang tua siswa, pemberdayaan guru bayangan dan perantara antara sekolah dengan orang tua, dan penggunaan beberapa media sebagai penghubung orang tua dengan sekolah.
Catatan Editor : Langkah-langkah agar tulisan di terima
Authors: Aiyuda Nurul , Syakarofath Nandy Agustin , Adwitiya Asti B , Mujahid Dhestina Religia 
Published: March 2022

Assalamualaikum wr wb.
Salam Sejahtera
Dear rekan-rekan peneliti, kolega dan teman-teman pembaca yang tertarik dengan penelitian psikologi.
Psychopolytan : Jurnal Psikologi merupakan salah satu jurnal dengan open journal system (ojs) yang diterbitkan sejak Agustus 2018. Sejak pengajuan akreditasi di tahun 2019, Psychopolytan lolos evaluasi dan mendapat akreditasi sinta 4. Beriringan dengan akreditasi tersebut, peningkatan artikel masuk terus terjadi. Mengingat banyak kebutuhan penerbitan yang diperlukan untuk kebutuhan kululusan mahasiswa, kepangkatan dosen, maupun sebagai bagian dari Tri Dharma Perguruan Tinggi. Namun demikian beberapa artikel masuk masih belum mengalami peningkatan kualitas, beberapa diantaranya masih tinggi angka plagiasi, minim sitasi dan tidak menonjolkan novelty dalam penulisan naskah. Mengatasi hal ini kami bersama editor berusaha merangkum beberapa langkah agar artikel diterima di psychopolytan : jurnal psikologi. Hal ini dilakukan untuk menguraikan prosedur penulisan maupun tips untuk penulis sebelum melakukan submission. Tentu saja hal ini tidak bisa dianggap sebagai hal yang baku dan akan berbeda pada setiap jurnal. Sehingga beberapa hal mungkin tidak sejalan dengan kondisi jurnal lainnya dalam langkah penerimaan.
Tulisan ini tidak hanya berangkat dari pengalaman tim editor dalam menerima naskah yang masuk, tapi juga mendapat masukan dari para editor dari beberapa jurnal ojs dan terakreditasi lainnya, serta masukan para reviewer. Dengan adanya tulisan ini, diharapkan bisa menjadi masukan dan perbaikan untuk peningkatan kualitas penulisan artikel di psychpolytan ke depan.
Editor In Chief Psychopolytan : Jurnal Psikologi
Nurul Aiyuda
أسباب العنف لدى تلاميذ المرحلة المتوسطة حسب أراء المدرّسين دراسة ميدانية ببعض متوسطات ولاية مسيلة
Authors: حمود أ.م.د. طه , العمري م.م. واضح 
Published: March 2022

تعدّ ظاهرة العنف مشكلة عالمية تعاني منها العديد من الدول، وتتجلى مظاهر هذه الظاهرة في أشكال متعددّة: حروب، تحرشات، أفعال التهديد وغير ذلك. ويشكّل العنف في الوسط المدرسي مشكلة خطيرة لها انعكاسات كبيرة على شركاء النظام التربوي وكذا على المجتمع برمته.
نرمي من هذا البحث إلى التعرّف على الأسباب المؤديّة إلى العنف لدى تلاميذ مرحلة التعليم المتوسط في بعض المؤسسات بولاية مسيلة من خلال الإجابة عن السؤالين الآتيين:

ماهي أسباب العنف في الوسط المدرسي حسب أراء الأساتذة؟
ماهي أنواع الحلول التي يمكن تقديمها للوقاية والحد من هذه الظاهرة في الوسط المدرسي؟
Edukasi Identifikasi Masa Kadaluarsa Obat dan Perhitungan Beyond Use Date pada Pasien Instalasi Farmasi Rawat Jalan di RSUD dr. R. Koesma Kabupaten Tuban
Authors: Iskandar Iskandar , Meida Byba , Octavia Devi Ristian 
Published: March 2022

Public knowledge about health, especially medicine is still very limited. One of the terms of health in medicine that is less known by the public is BUD (Beyond Use Date). BUD is time limit for the use of medicinal products after being prepared/formulated or after the primary packaging is opened /tampered with. While ED (Expiration Date) is the time limit for the use of medicinal products after being produced by the manufacturer before the packaging is opened. ED is listed by the manufacturer on the packaging while BUD is not always listed. Providing correct information about BUD becomes the needs of the community to avoid negative impacts that may arise,such as: the occurrence of medication error, the target therapy is not optimal and decreases the effectiveness of the medicinal products. For this reason, an effort is needed to increase public knowledge about BUD, namely through counseling activities with lecture, discussion and Q&A methods. Counseling on BUD (Beyond Use Date) in patients of Hospital Outpatient Pharmacy Installationt dr.R.Koesma Tuban Regency, aims to find out the level of public knowledge of BUD. Based on the evaluation results of the pre test question sheet (before counseling) and post test question sheet (after counseling) most of the participants increased their knowledge,its means that the participants understood the definition and the difference between BUD and ED solid, semi-solid, liquid, eye drops and insulin preparations.
PELAYANAN MULTIFUNGSI PROFESIONAL KRISTEN DALAM KONTEKS ERA REVOLUSI INDUSTRI 4.0
Authors: Haryono Timotius 
Published: March 2022

ABSTRAK – Semua orang percaya memiliki tanggung jawab untuk melayani. Namun kaum profesional Kristen masih enggan untuk melayani karena munculnya istilah pelayanan penuh waktu dan paruh waktu. Istilah ini secara tidak langsung menganggap kegiatan pelayanan di luar gereja bukanlah pelayanan Kristen yang sesungguhnya. Era Revolusi Industri 4.0 menuntut pelayanan Kristen yang tidak hanya menguasai kerohanian saja tetapi holistik. Keterlibatan profesional Kristen dalam pelayanan menjadi penting dalam menjawab tantangan ini karena kemampuan multifungsinya. Penelitian ini bertujuan untuk mengembangkan suatu strategi pelayanan multifungsi bagi profesional Kristen di Era Revolusi Industri 4.0. Penelitian ini menggunakan paradigma fenomenologi teologia dengan pendekatan kualitatif. Metode penelitian yang digunakan dalam penelitian ini adalah Grounded Theory. Cara mengumpulkan data melalui studi pustaka. Penelitian ini menemukan peran pelayanan multifungsi profesional Kristen untuk memperluas dan meningkatkan kualitas pelayanan gereja di era Revolusi Industri 4.0.Kata kunci: Profesional Kristen, Pelayanan Multifungsi, Era Revolusi Industri 4.0. ABSTRACT – All believer has responsibility to serve God and others. But christian professional people reluctant because term of full time and part time ministry is appear. This terms indirectly means that service activity in outside of church isn’t the real christian service. The era of Industrial Revolution 4.0 demand christian ministry had not only spirituality but holistic. The involvement of Christian professional people in ministry become important to answer this challenge because they had multi-function ability. This research aims to develop a multi-function ministry strategy for Christian professional people in the era of Industrial Revolution 4.0. This research use phenomenology theology with qualitative approach. This research uses grounded theory method. This research use literature study to data collection process. This research found role of Christian professional people in multi-function ministry to expand and increase the quality of church service in the era of Industrial Revolution 4.0Keyword: Christian Professional People, Multi-function Ministry, The Era of Industrial Revolution 4.0
A Systematic Analysis of Stellar Populations in the Host Galaxies of Changing-look AGNs
Authors: Jin Jun-Jie , Wu Xue-Bing , Feng Xiao-Tong 
Published: March 2022

Abstract
“Changing-look” active galactic nuclei (CL-AGNs) are a newly discovered class of AGNs that show the appearance (or disappearance) of broad emission lines within short timescales (months to years), and are often associated with dramatic changes in their continuum emissions. They provide us with an unprecedented chance to directly investigate the host galaxy properties with minimal contamination from the luminous central engine during the turn-off state, which is difficult for normal luminous AGNs. In this work, for the first time, we systematically characterize the stellar populations and star formation histories of host galaxies for 26 turn-off CL-AGNs using the stellar population synthesis code STARLIGHT. We find that the stellar populations of CL-AGNs are similar to those of normal AGNs, except that the intermediate stellar populations contribute more fractions. We estimate their stellar velocity dispersions (σ
⋆) and black hole masses (M
BH,vir), and find that CL-AGNs also follow the overall M
BH–σ
⋆ relationship. We also confirm the previous claims that CL-AGNs tend to be biased toward lower Eddington ratios, and that their extreme variabilities are more likely due to the intrinsic changes of the accretion rates. In addition, CL-AGNs with recent star formations tend to have higher Eddington ratios. Compared with previous studies, our analysis suggests that there may be a correlation between CL-AGN host galaxy properties and their CL phenomena.
Self-similar Solution of Hot Accretion Flow with Thermal Conduction and Anisotropic Pressure
Authors: Mosallanezhad Amin , Zeraatgari Fatemeh Zahra , Mei Liquan , Bu De-Fu 
Published: March 2022

Abstract
We explore the effects of anisotropic thermal conduction, anisotropic pressure, and magnetic field strength on the hot accretion flows around black holes by solving the axisymmetric, steady-state magnetohydrodynamic equations. The anisotropic pressure is known as a mechanism for transporting angular momentum in weakly collisional plasmas in hot accretion flows with extremely low mass accretion rates. However, anisotropic pressure does not extensively impact the transport of the angular momentum, it leads to shrinkage of the wind region. Our results show that the strength of the magnetic field can help the Poynting energy flux overcome the kinetic energy flux. This result may be applicable to the understanding of the hot accretion flow in the Galactic Center Sgr A* and the M87 galaxy.
Long-term Photometric and Low-resolution Spectroscopic Analysis of Five Contact Binaries
Authors: Panchal A. , Joshi Y. C. , De Cat Peter , Tiwari S. N. 
Published: March 2022

Abstract
A photometric and spectroscopic investigation is performed on five W Ursae Majoris eclipsing binaries J015818.6+260247 (hereinafter as J0158b), J073248.4+405538 (hereinafter as J0732), J101330.8+494846 (hereinafter as J1013), J132439.8+130747 (hereinafter as J1324), and J152450.7+245943 (hereinafter as J1524). The photometric data are collected with the help of the 1.3 m Devasthal Fast Optical Telescope, the 1.04 m Sampurnanand Telescope, and the Transiting Exoplanet Survey Satellite space mission. The low-resolution spectra of the 4 m Large Sky Area Multi-Object Fiber Spectroscopic Telescope are used for spectroscopic analysis. The orbital period change of these systems is determined using our photometric data and previously available photometric data from different surveys. The orbital period of J1013 and J1524 is changing at a rate of −2.552 (±0.249) × 10−7 days yr−1 and −6.792( ±0.952) × 10−8 days yr−1, respectively, while others do not show any orbital period change. The orbital period change of J1013 and J1524 corresponds to a mass transfer rate of 2.199 × 10−7
and 6.151 × 10−8
M
⊙ yr−1 from the primary to the secondary component in these systems. It is likely that angular momentum loss via magnetic braking may also be responsible for the observed orbital period change in the case of J1524. All systems have a mass ratio lower than 0.5, except J0158b with a mass ratio of 0.71. All the systems are shallow-type contact binaries. J0158b and J1524 are subtype A while others are subtype W. The H
α
emission line region is compared with template spectra prepared using two inactive stars with the help of the STARMOD program. The J0158, J1324, and J1524 systems show excess emission in the residual spectra after subtraction of the template.
New Tests of Milli-lensing in the Blazar PKS 1413 + 135
Authors: Peirson A. L. , Liodakis I. , Readhead A. C. S , Lister M. L. , Perlman E. S. , Aller M. F. , Blandford R. D. , Grainge K. J. B. , Green D. A. , Gurwell M. A. , Hodges M. W. , Hovatta T. , Kiehlmann S. , Lähteenmäki A. , Max-Moerbeck W. , Mcaloone T. , O’Neill S. , Pavlidou V. , Pearson T. J. , Ravi V. , Reeves R. A. , Scott P. F. , Taylor G. B. , Titterington D. J. , Tornikoski M. , Vedantham H. K. , Wilkinson P. N. , Williams D. T. , Zensus J. A. 
Published: March 2022

Abstract
Symmetric achromatic variability (SAV) is a rare form of radio variability in blazars that has been attributed to gravitational milli-lensing by a ∼102–105
M
⊙ mass condensate. Four SAVs have been identified between 1980 and 2020 in the long-term radio monitoring data of the blazar PKS 1413 + 135. We show that all four can be fitted with the same, unchanging, gravitational lens model. If SAV is due to gravitational milli-lensing, PKS 1413 + 135 provides a unique system for studying active galactic nuclei with unprecedented microarcsecond resolution, as well as for studying the nature of the milli-lens itself. We discuss two possible candidates for the putative milli-lens: a giant molecular cloud hosted in the intervening edge-on spiral galaxy, and an undetected dwarf galaxy with a massive black hole. We find a significant dependence of SAV crossing time on frequency, which could indicate a fast shock moving in a slower underlying flow. We also find tentative evidence for a 989 day periodicity in the SAVs, which, if real, makes possible the prediction of future SAVs: the next three windows for possible SAVs begin in 2022 August, 2025 May, and 2028 February.
Current Challenges in Cepheid Distance Calibrations Using Gaia Early Data Release 3
Authors: Owens Kayla A. , Freedman Wendy L. , Madore Barry F. , Lee Abigail J. 
Published: March 2022

Abstract
Using parallaxes from Gaia Early Data Release 3 (EDR3), we determine multi-wavelength BVI

c
, JHK

s
, and [3.6] and [4.5] micron absolute magnitudes for 37 nearby Milky Way Cepheids, covering the period range between 5 and 60 days. We apply these period–luminosity relations to Cepheids in the Large and Small Magellanic Clouds and find that the derived distances are significantly discrepant with the geometric distances according to detached eclipsing binaries (DEBs). We explore several potential causes of these issues, including reddening, metallicity, and the existence of an additional zero-point offset, but none provide a sufficient reconciliation with both DEB distances. We conclude that the combination of the systematic uncertainties on the EDR3 parallaxes with the uncertainties on the effect of metallicity on the Cepheid distance scale leads to a systematic error floor of approximately 3%. We therefore find that the EDR3 data are not sufficiently accurate in the regime of these bright Cepheids to determine extragalactic distances precise to the 1% level at this time, in agreement with a number of contemporary studies.
First Images of Phosphorus Molecules toward a Protosolar Analog
Authors: Bergner Jennifer B. , Burkhardt Andrew M. , Öberg Karin I. , Rice Thomas S. , Bergin Edwin A. 
Published: March 2022

Abstract
The chemistry of phosphorus in star- and planet-forming regions is poorly understood, despite the central role of phosphorus in terrestrial biochemistry. We present Atacama Large Millimeter/submillimeter Array band 3 and 4 observations of PO and PN toward the Class I protostar B1-a, representing the first spatially resolved observations of phosphorus carriers toward a solar-type star-forming region. The phosphorus molecules emit from two distinct clumps, which coincide with regions where the protostellar outflow (traced by SiO) interacts with a filament of dense gas (traced by CCS). Thus, the gas-phase phosphorus seems to originate from the shocking of dense interstellar clumps. Based on the observed emission patterns, PO and PN appear to be daughter products of a solid phosphorus carrier with an intermediate volatility between ices and silicate grains. Interstellar shocks may therefore play an important role in converting semi-refractory phosphorus to a more volatile form prior to incorporation into cometary ices. Indeed, the (PO+PN)/CH3OH ratio is similar in B1-a and comet 67P, implying a comparable reservoir of volatile phosphorus. The PO/PN ratio ranges from ∼1–8 across B1-a. The northern emission clump exhibits a lower PO/PN ratio and weaker 13CH3OH emission than southern clump, indicating distinct shock physics and chemistry at the two positions. Resolved observations of P carriers toward additional sources are needed to better understand what regulates such variations in the PO/PN ratio in protostellar environments.
Measuring Spin from Relative Photon-ring Sizes
Authors: Broderick Avery E. , Tiede Paul , Pesce Dominic W. , Gold Roman 
Published: March 2022

Abstract
The direct detection of a bright, ring-like structure in horizon-resolving images of M87* by the Event Horizon Telescope (EHT) is a striking validation of general relativity. The angular size and shape of the ring is a degenerate measure of the location of the emission region, mass, and spin of the black hole. However, we show that the observation of multiple rings, corresponding to the low-order photon rings, can break this degeneracy and produce mass and spin measurements independent of the shape of the rings. We describe two potential experiments that would measure the spin. In the first, observations of the direct emission and n = 1 photon ring are made at multiple epochs with different emission locations. This method is conceptually similar to spacetime constraints that arise from variable structures (or hot spots) in that it breaks the near-perfect degeneracy between emission location, mass, and spin for polar observers using temporal variability. In the second, observations of the direct emission and n = 1 and n = 2 photon rings are made during a single epoch. For both schemes, additional observations comprise a test of general relativity. Thus, comparisons of EHT observations in 2017 and 2018 may be capable of producing the first horizon-scale spin estimates of M87* inferred from strong lensing alone. Additional observation campaigns from future high-frequency, Earth-sized, and space-based radio interferometers can produce high-precision tests of general relativity.
FRAMEx. II. Simultaneous X-Ray and Radio Variability in Active Galactic Nuclei—The Case of NGC 2992
Authors: Fernandez Luis C. , Secrest Nathan J. , Johnson Megan C. , Schmitt Henrique R. , Fischer Travis C. , Cigan Phillip J. , Dorland Bryan N. 
Published: March 2022

Abstract
Using simultaneous Very Long Baseline Array and Neil Gehrels Swift Observatory X-ray Telescope observations of the active galactic nucleus (AGN) in NGC 2992 over a six-month observing campaign, we observed a large drop in core 5 cm radio luminosity, by a factor of >3, in tandem with a factor of >5 increase in 2–10 keV X-ray luminosity. While NGC 2992 has long been an important object for studies of X-ray variability, our study is the first simultaneous X-ray and radio variability campaign for this object. We observe that the X-ray spectral index does not change over the course of the flare, consistent with a change in the bulk amount of Comptonizing plasma, potentially due to a magnetic reconnection event in the accretion disk. The drop in apparent radio luminosity can be explained by a change in free–free absorption, which we calculate to correspond to an ionized region with a physical extent and electron density consistent with the broad-line region (BLR). Our results are consistent with magnetic reconnection events in the dynamic accretion disk creating outbursts of ionizing material, increasing Compton up-scattering of UV accretion disk photons and feeding material into the BLR. These findings present an important physical picture for the dynamical relationship between X-ray and radio emission in AGNs.