bluuebunny/crossref_metadata_2025_split huggingface dataset:
Monitoring of the Listeria spp. identification from the poultry products in the Dnipropetrovsk region
Authors: Zazharska N. M. , Borovuk I. V. 
Published: May 2019

Due to high mortality, listeriosis is one of the most common causes of death from illnesses associated with food, taking the second place after salmonellosis. Listeriosis, as a rule, arises as a result of consumption of contaminated products, including meat products, cheese, ready-to-eat foods. L. monocytogenes belongs to the third group of pathogenicity. Contamination by L. monocytogenes in processing of products is a constant problem in food plants. Food contamination Listeria leads to a withdrawal of products that produces economic losses. Analysis of the dynamic detection and of the differential identification of Listeria spp. in the meat products of poultry processing enterprises in Dnipropetrovsk region was conducted. The research was carried out by Dnipropetrovsk regional state laboratory of the state service of Ukraine for food safety and consumer protection. The results of bacteriological researches of meat samples which poultry plants gave for microbiological analysis during period 2008–2018 were used for monitoring. Microbiological research was carried out in accordance with valid international normative documents. The fluorescence analyzer Mini Vidas, France, the CAMP test were used for analysis. The biochemical properties of isolated microorganisms were established using BioMerieux API tests, France. Analyzing the number of researches and identification of microorganisms in the Dnipropetrovsk region for the period of 11 years, 3001 positive results out of 8172 analyzed samples were found (36.7%). Herewith, part of positive samples goes up from 8.5% in 2008 to 77.9% in 2018. L. ivanovii was isolated in 1523 samples (18.6%), L. inocua – 833 (10.2%), L. monocytogenes – 493 (6%), L. seeliger – 97 (1.2%), L. grayi – 36 (0.4%), L. welshimeri in 19 samples of meat products (0.2%) out of the 8172 microbiological studies conducted over 11 years. Of the six types of identified Listeria, more than half were L. ivanovii, which is twice as high as cases with L. incocua and thrice compared to L. monocytogenes.
Urgensi Maintainability Software e-SPT dan Faktor-faktor yang Berpengaruh terhadap Alokasi Penerimaan Pajak Penghasilan (PPh) Pasal 25 Badan di KPP Madya Malang – Jawa Timur
Authors: Alamsyah Agus Rahman 
Published: May 2019

Penelitian ini bertujuan untuk mengetahui urgensi maintainability software e-SPT dan faktor-faktor yang berpengaruh terhadap alokasi penerimaan Pajak Penghasilan (PPh) Pasal 25 Badan, dasar pemilihan Pajak Penghasilan (PPh) Pasal 25 Badan karena total penerimaan pajak tertinggi dari semua kompenen pajak berasal dari penghasilan (PPh) dan ditemukan bahwa pemasukan dari penerimaan PPh Pasal 25 Badan merupakan jenis pajak penghasilan yang tertinggi diantara pajak penghasilan lainnya, selain itu untuk memaintenance sumber pemasukan tersebut maka Direktorat Jenderal Pajak (Dirjen Pajak) sebagai salah satu institusi pemerintah menerapkan sistem informasi perpajakan untuk kemudahan dan efektivitas kelancaran aktivitas penerimaan negara dari sektor pajak khususnya Pajak Penghasilan (PPh). Berdasarkan hasil penelitian maka dapat ditarik kesimpulan bahwa Urgensi Maintainability Software e-SPT, Surat Ketetapan Pajak, dan Kepatuhan Wajib Pajak berpengaruh secara positif dan mampu meningkatkan Penerimaan PPh Pasal 25 di KPP Madya Malang – Jawa Timur, sedangkan Jumlah Wajib Pajak berdampak negatif terhadap kenaikan Penerimaan PPh Pasal 25 di KPP Madya Malang – Jawa Timur.
PENGARUH SISTEM PEMASARAN DIGITAL MARKETING TERHADAP PENINGKATAN VOLUME PENJUALAN HASIL INDUSTRI RUMAHAN
Authors: Pradiani Theresia 
Published: May 2019

Perkembangan teknologi informasi yang berkembang sangat pesat saat ini berpengaruh bagi masyarakat dalam mendukung berbagai kegiatan bisnis baik besar maupun kecil agar dapat dikenal secara global. Dampak yang paling nyata adalah selain dikenal juga dapat meningkatkan volume penjualan dan profit. Digital Marketing adalah salah satu media pemasaran yang sangat besar memberikan pengaruh. Dengan menggunakan digital marketing dalam hal ini adalah sosial media, ibu-ibu PKK di RW 02 Randuagung Singosari Malang memasarkan hasil indutri rumahan berupa kerajinan tangan tas dari bungkus minuman instan. Awalnya kegiatan ini hanya sebagai pengisi waktu luang, tetapi saat ini justru menjadi kegiatan utama sebagai penambah perputaran ekonomi dalam rumah tangga. Dahulu kegiatan penjualan hasil industri ini secara konvesional maupun tradisiona, mereka membuat produk hanya berdasarkan pesanan. Tetapi setelah mengenal adanya sosial media ibu-ibu PKK ini sudah mulai menerima banyak pesanan, sehingga volume penjualan semakin meningkat pesat dibandingkan saaat penjualan dengan cara lama. Digital marketing dipandang sebagai media yang paling baik sebagai sarana promosi yang paling efektif dan efisien serta mampu meningkatkan volume penjualan yang signifikan, dari pendapatan perbulan bersih Rp. 1.000.000,- s.d. Rp. 1.500.000,- sekarang bisa mencapai Rp. 2.000.000 s.d. 3.500.000,- (100%).
FAKTOR-FAKTOR YANG MEMPENGARUHI PERKEMBANGAN USAHA KECIL SEKTOR INDUSTRI PENGOLAHAN DI KOTA MALANG
Authors: Cahyanti Mega Mirasa , Anjaningrum Widiya Dewi 
Published: May 2019

This study aims to determine the factors that influence the development of the small business manufacturing sector in Malang town. This research is a kind of field research, where the primary quantitative data through questionnaire was taken directly from small businesses. The sampling technique that was used is purposive sampling, where the sample was selected based on the consideration which the sample could provide some informations that are suitable with the needs of the research. Based on the Slovin formula, a predetermine number of samples that taken was 89 small businesses. Based on the result taken by data processing and factor analysis using SPSS 23, shows that the factors which influence the development of small business manufacturing sector are the quality of human resources, production systems, financial management systems, marketing strategies, the partnership system, the quality of infrastructure and regulation. In this case, the factor which has the higest significant effect is partnership system. Finally, improving the partnership system on small business should be developed not only with suppliers, but also with the government, large business, financial institutions and business centers. Therefore, these small business could be thrive.
STUDI FENOMENOLOGIS TERHADAP PERAN ETIKA DALAM PENDIDIKAN PERPAJAKAN
Authors: Widyaningrum Tri Rahayu 
Published: May 2019

Ethics, has a very important role in all aspects including the aspect of taxation Education. The existence of ethics is absolutely necessary within the framework of a healthy mindset and full balance so that the education process running for this not only focus on improving the capabilities, expertise and intellectual, but also pay attention to morality that comes to fruition ethics in the construction of education completely. This study aims to assess the understanding of the students in terms of knowledge about the role of ethics in education tax.The extent to which their understanding in terms of ethics and critical payloads contained in it. Phenomenology is used as an analytical tool understanding of the role of ethics in education tax. These findings indicate that students understanding the role of ethics that is so important in the educational process of taxation and will be used as stock ethics profession as a career offender taxes. significantly still needed effort for understanding the role of ethics in education taxation can achieve balance by integrating a variety of clever angles and interests as a whole.
PENINGKATAN DAYA SAING USAHA MIKRO PEMPEK IKAN DAN NABATI SAYURAN TROPIS DI KOTA MALANG
Authors: Nugroho Yuni Agung , Sugiarti Untung 
Published: May 2019

Community Development Activities (IbM) is designed to address the problems faced by partner companies. The implementation of IbM will be carried out by the following methods: a) Transfer of Application of Sanitation and Hygiene Standard to Pempek Production, c) Management training, financial management of production and marketing management, d) Monitoring and Evaluation.
The results of IbM activities that have been done is the aid of mixing machine pempek dough dedicated to Partners 2, while for Part 1 in the form of fretrer polytron and vacum sealer. However, the pempping stirrer can be used, after the electric power of partner 2 plus the power to 1300 watts. Mitra 1 (Pempek Maliana) is more open and creative in developing pempek products, while partner 2 (Pempek Sulfat 28) still adheres to pempek that already exist in Malang with the same appearance and hard. Assistance and counseling to open insight and add skills have been done but at Partner 2 is still not able to adopt it. Partner 1 is already more advanced in terms of innovation and creativity in products and marketing.Keywords: competitiveness, micro business, pempek, tropical vegetables
Investigation of Sodium Doped Lanthanum Manganite in Optical, Dielectric and Capacitive Perspective Prepared by Flux Method
Authors: Majumder R. , Sarker M. A. R. , Hossain M. M. , Hossain M. E. , Shen D. , Reza A. K. M. S. , Kabir M. H. 
Published: May 2019

A comprehensive analysis of optical and dielectric properties of a material is very much essential for the research of device fabrication. From this perception, the sodium (Na) doped lanthanum manganite with 15% substitution of La by Na (La0.85Na0.15MnO3) has been synthesized using the flux method and investigated to observe the optical absorbance, refractive index, capacitance and dielectric constant. In this study, we have reported better optical absorbance for the monovalent Na doping with a slightly lower value of the energy band gap (~ 1.57 eV) compared to the divalent Sr doping on parent LaMnO3. The structural analysis has been accomplished using X-ray diffraction (XRD) and Fourier transform infrared spectroscopy (FTIR) to confirm the ability of the flux method to grow higher order La0.85Na0.15MnO3 crystal satisfactorily. Optical properties of La0.85Na0.15MnO3 have been estimated using UV-Vis spectroscopy and the frequency dependent electronic properties (ac conductivity, dielectric constants and capacitance) have been investigated using a precision impedance analyzer. The capacitance has been reported in Pico farad range for La0.85Na0.15MnO3 crystal with the low value of dielectric constant throughout the high-frequency region.
A Study on Fish Species of Sarıkum Lake in Sinop Province in the Black Sea Region
Authors: Yardım Öztekin 
Published: May 2019

ABSTRACT: This study was carried out between January and December 2009 in order to discover the fish species found in Sarikum Lake of Sinop Province. Sampling activities were done by using multi-filament trammel nets, scoop nets and cast nets. As a result of the sampling, 9 species (Atherina boyeri, Liza aurata, Mugil cephalus, Mugil soiuy, Neogobius melanostomus, Aphanius chantrei, Gasterosteus aculeatus, Cyprinus carpio and Platichthys flesus) were determined. Results were discussed with other studies.
Announcement: First Edition of IASA-TC 06 Online
Authors: Fleischhauer Carl 
Published: May 2019

Archives hold original video recordings in a range of types, from media-dependent, carrier-based analogue videotapes to computer-file-based digital recordings. The appropriate preservation treatments for this array reflect the variation in the source recordings. For analogue videotapes, for example, digitisation is called for. Meanwhile, examples of digital file-based recording may require rewrapping into a fresh file "wrapper" or a combination of digital transcoding and rewrapping.
When complete, IASA-TC 06 will cover the full range of topics in the preceding paragraph, as well as providing advice on shooting ethnographic, documentary, and oral history video footage in a manner that maximizes its "preserve-ability".
Ultra-diffuse Galaxies at Ultraviolet Wavelengths
Authors: Singh Pranjal Rajendra , Zaritsky Dennis , Donnerstein Richard , Spekkens Kristine 
Published: May 2019

Abstract
We measure near-ultraviolet (NUV) aperture magnitudes from Galaxy Evolution Explorer images for 258 ultra-diffuse galaxy (UDG) candidates drawn from the initial Systematically Measuring Ultra-Diffuse Galaxies (SMUDGes) survey of ∼300 square degrees surrounding, and including, the Coma galaxy cluster. For the vast majority, 242 of them, we present flux upper limits due either to a lack of significant flux in the aperture or confusion with other objects projected within the aperture. These limits often place interesting constraints on the UDG candidates, indicating that they are non-star-forming or quiescent. In particular, we identify field, quiescent UDG candidates, which are a challenge for formation models and are, therefore, compelling prospects for spectroscopic follow-up and distance determinations. We present far-ultraviolet (FUV) and NUV magnitudes for 16 detected UDG candidates and compare those galaxies to the local population of galaxies on color–magnitude and specific star formation rate diagrams. The NUV-detected UDG candidates form mostly an extension toward lower stellar masses of the star-forming galaxy sequence, and none of these lie within regions of high local galaxy density. UDG candidates span a range of properties, although almost all are consistent with being quiescent, low surface brightness galaxies, regardless of environment.
A New Mass Determination of (349) Dembowska with Close Encounters
Authors: Li Fan , Fu Yanning , Yuan Ye 
Published: May 2019

Abstract
(349) Dembowska is a big R-type main-belt asteroid. A new and more precise determination of its mass, M, is presented. The high precision is achieved, in particular, using our generally applied criterion of selecting model parameters. This criterion takes into account the sensitivity to M of the available observables, i.e., the position of another much smaller body involved in a close encounter with (349) Dembowska. Using this criterion, as well as observations from the Minor Planet Center (MPC) and the ephemeris DE431, M is redetermined to be (4.1 ± 0.4) × 1018 kg, which is a weighted mean of compatible masses independently determined with five encounters. From the most recently determined effective diameter, we get a bulk density of ρ = 2.08 ± 0.24 g cm−3 for (349) Dembowska. A macroporosity of 36 is derived from a grain density of 3.25 g cm−3.
Fermi-GBM GRBs with Characteristics Similar to GRB 170817A
Authors: von Kienlin A. , Veres P. , Roberts O. J. , Hamburg R. , Bissaldi E. , Briggs M. S. , Burns E. , Goldstein A. , Kocevski D. , Preece R. D. , Wilson-Hodge C. A. , Hui C. M. , Mailyan B. , Malacaria C. 
Published: May 2019

Abstract
We present a search for gamma-ray bursts in the Fermi-GBM 10 yr catalog that show similar characteristics to GRB 170817A, the first electromagnetic counterpart to a GRB identified as a binary neutron star (BNS) merger via gravitational wave observations. Our search is focused on a nonthermal pulse, followed by a thermal component, as observed for GRB 170817A. We employ search methods based on the measured catalog parameters and Bayesian Block analysis. Our multipronged approach, which includes examination of the localization and spectral properties of the thermal component, yields a total of 13 candidates, including GRB 170817A and the previously reported similar burst, GRB 150101B. The similarity of the candidates is likely caused by the same processes that shaped the gamma-ray signal of GRB 170817A, thus providing evidence of a nearby sample of short GRBs resulting from BNS merger events. Some of the newly identified counterparts were observed by other space telescopes and ground observatories, but none of them have a measured redshift. We present an analysis of this subsample, and we discuss two models. From uncovering 13 candidates during a time period of 10 yr we predict that Fermi-GBM will trigger on-board on about one burst similar to GRB 170817A per year.
Numerical Simulations on the Deflection of Coronal Mass Ejections in the Interplanetary Space
Authors: Zhuang Bin , Wang Yuming , Hu Youqiu , Shen Chenglong , Liu Rui , Gou Tingyu , Zhang Quanhao , Li Xiaolei 
Published: May 2019

Abstract
Deflection of coronal mass ejections (CMEs) in the interplanetary space, especially in the ecliptic plane, serves as an important factor deciding whether CMEs arrive at the Earth. Observational studies have shown evidence for deflection, whose detailed dynamic processes, however, remain obscure. Here we developed a 2.5D ideal magnetohydrodynamic simulation to study the propagation of CMEs traveling with different speeds in the heliospheric equatorial plane. The simulation confirms the existence of the CME deflection in the interplanetary space, which is related to the difference between the CME speed (v

r
) and the solar wind speed (v
sw): a CME will propagate radially as v

r
is close to v
sw but eastward or westward when v

r
is larger or smaller than v
sw; the greater the difference is, the larger the deflection angle will be. This result supports the model for CME deflection in the interplanetary space (DIPS) proposed by Wang et al., predicting that an isolated CME can be deflected due to the pileup of solar wind plasma ahead of or behind the CME. Furthermore, the deflection angles, which are derived by inputting v

r
and v
sw from the simulation into the DIPS model, are found to be consistent with those in the simulation.
Discovery of a Double Blue Straggler Sequence in M15: New Insight into the Core-collapse Process
Authors: Beccari G. , Ferraro F. R. , Dalessandro E. , Lanzoni B. , Raso S. , Origlia L. , Vesperini E. , Hong J. , Sills A. , Dieball A. , Knigge C. 
Published: May 2019

Abstract
In this paper we report the discovery of a double blue straggler star (BSS) sequence in the core of the core-collapsed cluster M15 (NGC 7078). We performed a detailed photometric analysis of the extremely dense core of the cluster using a set of images secured with the Advanced Camera for Survey in the High Resolution Channel mode on board the Hubble Space Telescope. The proper combination of the large number of single frames in the near-UV (F220W), and blue (F435W) filters allowed us to perform a superb modeling of the point-spread function and an accurate deblending procedure. The color–magnitude diagram revealed the presence of two distinct parallel sequences of blue stragglers. In particular, the blue BSS sequence is characterized by the intriguing presence of two different branches. The first branch appears extremely narrow, it extends up to 2.5 mag brighter than the cluster main-sequence turnoff (MS-TO) point, and it is nicely reproduced by a 2 Gyr old collisional isochrone. The second branch extends up to 1.5 mag from the MS-TO and it is reproduced by a 5.5 Gyr old collisional isochrone. Our observations suggest that each of these branches is mainly constituted by a population of nearly coeval collisional BSSs of different masses generated during two episodes of high collisional activity. We discuss the possibility that the oldest episode corresponds to the core-collapse (CC) event (occurred about 5.5 Gyr ago), while the most recent one (occurred about 2 Gyr ago) is associated with a core oscillation in the post-CC evolution. The discovery of these features provides further strong evidence in support of the connection between the BSS properties and globular cluster dynamical evolution, and it opens new perspectives on the study of CC and post-CC evolution.
A Novel Statistical Method for Measuring the Temperature–Density Relation in the IGM Using the b–NH i Distribution of Absorbers in the Lyα Forest
Authors: Hiss Hector , Walther Michael , Oñorbe Jose , Hennawi Joseph F. 
Published: May 2019

Abstract
We present a new method for determining the thermal state of the intergalactic medium based on Voigt profile decomposition of the Lyα forest. The distribution of Doppler parameter and column density (b–N
H i
distribution) is sensitive to the temperature–density relation T = T
0(ρ/ρ
0)
γ−1, and previous work has inferred T
0 and γ by fitting its low-b cutoff. This approach discards the majority of available data and is susceptible to systematics related to cutoff determination. We present a method that exploits all information encoded in the b
–N
H i
distribution by modeling its entire shape. We apply kernel density estimation to discrete absorption lines to generate model probability density functions, and then we use principal component decomposition to create an emulator that can be evaluated anywhere in thermal parameter space. We introduce a Bayesian likelihood based on these models enabling parameter inference via Markov Chain Monte Carlo. The method’s robustness is tested by applying it to a large grid of thermal history simulations. By conducting 160 mock measurements, we establish that our approach delivers unbiased estimates and valid uncertainties for a 2D (T
0, γ) measurement. Furthermore, we conduct a pilot study applying this methodology to real observational data at z = 2. Using 200 absorbers, equivalent in path length to a single Lya forest spectrum, we measure

and

in excellent agreement with cutoff fitting determinations using the same data. Our method is far more sensitive than cutoff fitting, enabling measurements of log T
0 and γ with precision on

(γ) nearly two (three) times higher for current data set sizes.
Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM
Authors: Riess Adam G. , Casertano Stefano , Yuan Wenlong , Macri Lucas M. , Scolnic Dan 
Published: May 2019

Abstract
We present an improved determination of the Hubble constant from Hubble Space Telescope (HST) observations of 70 long-period Cepheids in the Large Magellanic Cloud (LMC). These were obtained with the same WFC3 photometric system used to measure extragalactic Cepheids in the hosts of SNe Ia. Gyroscopic control of HST was employed to reduce overheads while collecting a large sample of widely separated Cepheids. The Cepheid period–luminosity relation provides a zero-point-independent link with 0.4% precision between the new 1.2% geometric distance to the LMC from detached eclipsing binaries (DEBs) measured by Pietrzyński et al. and the luminosity of SNe Ia. Measurements and analysis of the LMC Cepheids were completed prior to knowledge of the new DEB LMC distance. Combined with a refined calibration of the count-rate linearity of WFC3-IR with 0.1% precision, these three improved elements together reduce the overall uncertainty in the geometric calibration of the Cepheid distance ladder based on the LMC from 2.5% to 1.3%. Using only the LMC DEBs to calibrate the ladder, we find H
0 = 74.22 ± 1.82 km s−1 Mpc−1 including systematic uncertainties, 3% higher than before for this particular anchor. Combining the LMC DEBs, masers in NGC 4258, and Milky Way parallaxes yields our best estimate: H
0 = 74.03 ± 1.42 km s−1 Mpc−1, including systematics, an uncertainty of 1.91%–15% lower than our best previous result. Removing any one of these anchors changes H
0 by less than 0.7%. The difference between H
0 measured locally and the value inferred from Planck CMB and ΛCDM is 6.6 ± 1.5 km s−1 Mpc−1 or 4.4σ (P = 99.999% for Gaussian errors) in significance, raising the discrepancy beyond a plausible level of chance. We summarize independent tests showing that this discrepancy is not attributable to an error in any one source or measurement, increasing the odds that it results from a cosmological feature beyond ΛCDM.