bluuebunny/crossref_metadata_2025_split huggingface dataset:
Penyelesaian Tindak Pidana Pemerkosaan di Kecamatan Kelam Tengah Kabupaten Kaur Menurut Hukum Adat Pasemah
Authors: Khairil Ririn 
Published: December 2020

Fakta menunjukan bahwa kasus pemerkosaan yang terjadi di Kecamatan Kelam Tengah Kabupaten Kaur terjadi 6 kasus pemerkosaan.yang di lakukan oleh 4 orang laki-laki yang sudah beristri, sebagiannya 2 orang yang belum beristri. Menurut hukum adat Pasemah perbuatan tindak pidana pemerkosaan merupakan perbuatan yang dipandang oleh masyarakat sebagai perbuatan yang sangat tercela dan merusak sistem kemasyarakatan. Adapun permasalahan yang akan diteliti dalam penelitian ini adalah dapat di rumuskan sebagai berikut, Faktor-faktor apakah yang menyebabkan terjadinya tindak pidana pemerkosaan di Kecamatan Kelam Tengah Kabupaten Kaur? Bagaimana proses penyelesaian tindak pidana pemerkosaan menurut adat Pasemah? Bagaimanakah peranan pemuka adat Pasemahdalam menyelesaikan kasus pemerkosaan? Untuk menjawab permasalahan tersebut, penelitian ini menggunakan metode penelitian hukum Empiris. Berdasarkan Hasil penelitian, disimpulkan bahwa faktor penyebab terjadinya pemerkosaan di Kecamatan Kelam Tengah, yaitu karena sering melihat film porno melalui Hp, vcd, dan internet, melihat kemontokan wanita yang berpakaian seksi, mudahnya kaum perempuan percaya kepada kaum laki-laki,pesta perkawinan muda-mudidimalam hari. Peranan pemuka adat Pasemah dalam menyelesaikan masalah pidana seperti pemerkosaan lebih mengutamakan penyelesaian secara kekeluargaan,artinya lembaga adat tidak akan melanjutkan perkara pidana tersebut kepada pihak yang berwajib, tetapi ada juga yang di lanjutkan sampai ke pengadilan. Kata kunci : Pemerkosaan adalah perbuatan yang tidak bermoral
OPTIMIZATION OF ARTERIAL HYPERTENSION TREATMENT IN DIABETIC PATIENTS
Authors: Бабкин Андрей Петрович 
Published: December 2020

Достижение целевого уровня артериального давления у больных сахарным диабетом является такой же важной задачей, как и коррекция метаболических нарушений. Проведен анализ эффективности комбинированной антигипертензивной терапии у больных сахарным диабетом с диабетической нефропатией на основе динамики гемодинамических и метаболических параметров у больных с различной реакцией артериального давления на нагрузку поваренной солью. Выяснено, что больные с данной патологией не одинаково реагируют на нагрузку поваренной солью - у 23 (53,3 %) пациентов выявлено повышение систолического АД на 10 и более мм рт. ст. (солечувствительные пациенты), а у 21 (46,7%) повышение АД было менее 10 мм рт. ст. или отсутствовало (солерезистентные пациенты). Солечувствительные пациенты имели более высокие исходные значения показателей суточного мониторирования АД - САД ср. у солечувствительных пациентов равнялось 157,4 ± 1,0 мм рт. ст. против 150,7 ± 0,8 мм рт. ст. у солерезистентных пациентов, р<0,01. Обе комбинации лекарственных препаратов показали сопоставимый антигипертензивный эффект. Установлено, что у больных, принимавших комбинацию периндоприла и индапамида и вальсартана и индапамида, более выраженный антигипертензивный эффект был отмечен у больных с солечувствительным характером артериальной гипертонии в каждой группе лечения. Определение солечувствительности АД позволяет прогнозировать индивидуальную эффективность антигипертензивной терапии на основе использования теста с нагрузкой поваренной солью
Reaching the target blood pressure level in diabetic patients is as important as correcting metabolic disorders. The analysis of the effectiveness of combined antihypertensive therapy in patients with diabetes mellitus with diabetic nephropathy based on the dynamics of hemodynamic and metabolic parameters in patients with different reactions of blood pressure to the load of table salt. It was found that patients with this pathology do not equally respond to the load of table salt - 23 (53.3%) patients showed an increase in systolic blood pressure by 10 mm Hg or more. Art. (salt-sensitive patients), and in 21 (46.7%) the increase in blood pressure was less than 10 mm Hg. Art. or absent (salt-resistant patients. Salt-sensitive patients had higher baseline values of 24-hour BP monitoring - SBP mean in salt-sensitive patients was 157.4 ± 1.0 mm Hg versus 150.7 ± 0.8 mm Hg in salt-resistant patients, p <0.01. Both drug combinations showed a comparable antihypertensive effect. Determination of blood pressure salt sensitivity makes it possible to predict the individual effectiveness of antihypertensive therapy based on the use of a salt load test
Determination of the Local Hubble Constant from Virgo Infall Using TRGB Distances
Authors: Kim Yoo Jung , Kang Jisu , Lee Myung Gyoon , Jang In Sung 
Published: December 2020

Abstract
An independent determination of H
0 is crucial given the growing tension between the Hubble constant, H
0, derived locally and that determined from the modeling of the cosmic microwave background (CMB) originating in the early universe. In this work, we present a new determination of H
0 using velocities and tip of the red giant branch (TRGB) distances to 33 galaxies located between the Local Group and the Virgo cluster. We use a model of the infall pattern of the local Hubble flow modified by the Virgo mass, which is given as a function of the cosmological constants (H
0, ΩΛ), the radius of the zero-velocity surface R
0, and the intrinsic velocity dispersion, σ

v
. Fitting velocities and TRGB distances of 33 galaxies to the model, we obtain H
0 = 65.8 ± 3.5 (stat) ± 2.4 (sys) km s−1 Mpc−1 and R
0 = 6.76 ± 0.35 Mpc. Our local H
0 is consistent with the global H
0 determined from CMB radiation, showing no tension. In addition, we present new TRGB distances to NGC 4437 and NGC 4592, which are located near the zero-velocity surface: D = 9.28 ± 0.39 Mpc and D = 9.07 ± 0.27 Mpc, respectively. Their spatial separation is 0.29

Mpc, suggesting that they form a physical pair.
A Large Massive Quiescent Galaxy Sample at z ∼ 1.2
Authors: Xu Hai , Dai 戴 Y. Sophia 昱 , Huang Jia-Sheng , Wang Zhaoyu , Cheng Cheng , Shao Xu , Wu Shumei , Yang Xiaohu , Jing Yipeng , Sawicki Marcin , Liu Feng-Yuan 
Published: December 2020

Abstract
In this paper we present a simple color–magnitude selection and obtain a large sample of 33,893 massive quiescent galaxies at intermediate redshifts (1 < z < 1.5). We choose the longest wavelength available in the Hyper-Supreme-Cam (HSC) deep survey, the Y band and i − Y color, to select the 4000 Å Balmer jump in passive galaxies to the highest redshift possible within the survey. With the rich multiwavelength data in the HSC deep fields, we then confirm that the selected galaxies are in the targeted redshift range of 1 < z < 1.5, lie in the passive region of the UVJ diagram, and have high stellar masses at log(M
*/M
⊙) > 10.5, with a median of log(M
*/M
⊙) = 11.0. A small fraction of our galaxies is also covered by the HST CANDELS. Morphological analysis in the observed H band shows that the majority of this subsample are early-type galaxies. As massive early-type galaxies trace the high-density regions in the large-scale structure in the universe, our study provides a quick and simple way to obtain a statistically significant sample of massive galaxies in a relatively narrow redshift range. Our sample is 7–20× larger at the massive end (log(M
*/M
⊙) > 10.5) than any existing samples obtained in previous surveys. This is a pioneer study, and the technique introduced here can be applied to a future wide-field survey to study large-scale structure and to identify high-density regions and clusters.
Transition Probabilities and Collision Strengths for Fine-structure Levels Excitation of Ti II
Authors: Tayal S. S. , Zatsarinny O. 
Published: December 2020

Abstract
Several spectral features from the stellar and nebular objects arise due to the iron-peak Ti II fine-structure excitations. Transition probabilities and electron excitation collision strengths of iron-peak elements are important for a meaningful interpretation and analysis of the observed astrophysical spectra. Accurate description of atomic structure with open 3d-shell elements is the key to the reliable and accurate computation of radiative and collision rates. The term-dependent one-electron orbitals in the multiconfiguration Hartree–Fock approach with adjustable configuration expansions and semi-empirical fine-tuning for energy corrections have been used in achieving highly accurate target description. A total of 314 Ti II fine-structure levels of the ground 3d
24s and excited 3d
3, 3d4s
2, 3d
24p, 3d
25s, 3d4s4p, 3d
24d, 3d
25p, and 3d
24f configurations have been included in the calculations of these atomic parameters. The present calculation of collision strengths has been performed in a close-coupling approximation based on the B-spline Breit–Pauli R-matrix method with inclusion of spin–orbit interaction term in the Hamiltonian matrices. Effective collision strengths over a Maxwellian distribution of electron velocities at temperatures in the range from 103 to 105 K have been reported for transitions between the 314 fine-structure levels. These wide array of transitions give rise to many main Ti II infrared, optical, and ultraviolet lines from a variety of astrophysical objects. Our calculated parameters are compared with the available other theoretical and experimental results, and through this comparison likely uncertainties in our results have been estimated, especially for transitions among the low-lying fine-structure levels of astrophysical importance.
Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium
Authors: Carmo Lorena , González-Casanova Diego F. , Falceta-Gonçalves Diego , Lazarian Alex , Jablonski Francisco , Zhang Jian-Fu , Ferreira Ivan , Castro Manuel , Yang Bo 
Published: December 2020

Abstract
Synchrotron intensity and polarization gradients (SIG and SPG), proposed by Lazarian et al. and Lazarian & Yuen, present a new way to recover the mean magnetic field direction in the plane of the sky. To measure the magnetization level, Lazarian et al. suggested that the methods used in the context of the “Velocity Gradient Technique” could also be used on the SIG and SPG contexts. In this work we test the two proposed methods, named “top-base” and the circular standard deviation, “S,” to obtain the level of magnetization from synchrotron emission. In order to test the methods, we generate synthetic observations from magnetohydrodynamic computer simulations, with Alfvénic Mach numbers, M
A ∈ [0.2,1.7]. Using a Bayesian analysis we find that the circular standard deviations for the SIG and SPG methods are able to recover the magnetization for cases with signal-to-noise ratio ≳5. We found that for weak Faraday depolarization and different angles between the magnetic field direction and the line of sight the magnetization level can still be estimated.
A HaloSat Analysis of the Cygnus Superbubble
Authors: Bluem Jesse , Kaaret Philip , Fuelberth William , Zajczyk Anna , LaRocca Daniel M. , Ringuette R. , Jahoda Keith M. , Kuntz K. D. 
Published: December 2020

Abstract
The Cygnus Superbubble (CSB) is a region of soft X-ray emission approximately 13 degrees wide in the direction of the local spiral arm. Such a large region might be the result of strong stellar winds and supernovae from nearby stellar nurseries, or it could be the result of a single event—a hypernova. HaloSat observed four nonoverlapping 10 degree diameter fields in the CSB region over the 0.4-7 keV band. The CSB absorption and temperature was found to be consistent over all four fields, with a weighted average of 6.1 × 1021 cm−2 and 0.190 keV, respectively. These observations suggest that the CSB is a cohesive object with a singular origin. The total thermal energy for the CSB is estimated at 4 × 1052 erg, based upon a shell-like physical model of the CSB. Absorption and distance estimates to Cyg OB associations are examined. The CSB absorption is found to be most consistent with the absorption seen in Cyg OB1, implying that the CSB lies at a similar distance of 1.1–1.4 kpc.
Powerful t-SNE Technique Leading to Clear Separation of Type-2 AGN and H ii Galaxies in BPT Diagrams
Authors: Zhang XueGuang , Feng Yanqiu , Chen Huan , Yuan QiRong 
Published: December 2020

Abstract
Narrow emission-line galaxies can be distinguished in the well-known BPT diagrams through narrow emission-line properties. However, there are no boundaries visible to the naked eye between type-2 active galactic nuclei (AGN) and H ii galaxies in BPT diagrams, besides the extreme dividing lines expected by theoretical photoionization models. Here, based on the powerful t-SNE technique applied to the local narrow emission-line galaxies in the Sloan Digital Sky Survey Data Release 15, type-2 AGN and H ii galaxies can be clearly separated in the t-SNE determined two-dimensional projected map, and then the dividing lines can be mathematically determined in BPT diagrams, leading to charming harmonization of the theoretical expectations and the actual results from real observed properties. The results not only provide an interesting and robust method to determine the dividing lines in BPT diagrams through the powerful t-SNE technique, but also lead to further confirmation on previously defined composite galaxies more efficiently classified in the BPT diagram of [O iii]/Hβ versus [N ii]/Hα.
Flare Properties of A-type Stars in Kepler Data
Authors: Bai Jian-Ying , Esamdin Ali 
Published: December 2020

Abstract
We analyzed the long-cadence (LC) light curves of 5435 stars with effective temperatures of 7000–10,500 K in Data Release 25 of Kepler to extend the samples of A-type flare stars and study their flare properties. A total of 103 flare stars are detected, of which 72 have the Large Sky Area Multi-Object fiber Spectroscopic Telescope spectral types, resulting in 51 A-type stars, including 17 new and 34 known. A total of 352 flares are detected from the 51 stars. The flare durations, amplitudes, and energies in the Kepler band are calculated, with medians of 2.5 hr, 2.1 mmag, and 1035.8 erg, respectively. We give the flare frequency distribution (FFD) of the A-type stars. Within the same energy range, the flare rates of our FFD are lower than those in previous research, which was also based on Kepler LC data, and the FFD slope is consistent with that in the research. The activity–rotation relation of the A-type flare stars is shown for the first time, in which the flare activity decreases as the rotation period increases. The relation is similar to that of the late-type stars in previous studies. For the two relatively bright A-type flare stars, KIC 5360548 and KIC 9468475, three high-resolution spectra are observed on different nights for each of them, and radial velocities are calculated and compared with that of the previous research. The comparisons suggest that there is no evidence of the KIC 5360548 companion, and KIC 9468475 could have a low-mass companion.
Faint Quasars Live in the Same Number Density Environments as Lyman Break Galaxies at z ∼ 4
Authors: Uchiyama Hisakazu , Akiyama Masayuki , Toshikawa Jun , Kashikawa Nobunari , Overzier Roderik , Nagao Tohru , Ichikawa Kohei , Marinello Murilo , Imanishi Masatoshi , Tanaka Masayuki , Matsuoka Yoshiki , Komiyama Yutaka , Ishikawa Shogo , Onoue Masafusa , Kubo Mariko , Harikane Yuichi , Ito Kei , Namiki Shigeru , Liang Yongming 
Published: December 2020

Abstract
Characterizing high-z quasar environments is key to understanding the coevolution of quasars and the surrounding galaxies. To restrict their global picture, we statistically examine the g-dropout galaxy overdensity distribution around 570 faint quasar candidates at z ∼ 4, based on the Hyper Suprime-Cam Subaru Strategic Program survey. We compare the overdensity significances of g-dropout galaxies around the quasars with those around g-dropout galaxies, and find no significant difference between their distributions. A total of 4 (22) out of the 570 faint quasars,

, are found to be associated with the >4σ overdense regions within an angular separation of 1.8 (3.0) arcmin, which is the typical size of protoclusters at this epoch. This is similar to the fraction of g-dropout galaxies associated with the >4σ overdense regions. This result is consistent with our previous work in which

and

of luminous quasars detected in the Sloan Digital Sky Survey exist in the >4σ overdense regions within 1.′8 and 3.′0 separations, respectively. Therefore, we suggest that the galaxy number densities around quasars are independent of their luminosity, and most quasars do not preferentially appear in the richest protocluster regions at z ∼ 4. The lack of an apparent positive correlation between the quasars and the protoclusters implies that (i) the gas-rich major merger rate is relatively low in the protocluster regions, (ii) most high-z quasars may appear through secular processes, or (iii) some dust-obscured quasars exist in the protocluster regions.
Why Interstellar Ice Dust Grains Should Be Elongated
Authors: Bellan P. M. 
Published: December 2020

Abstract
Models of interstellar dust alignment assume that dust grains are elongated, but none of these models explain why dust grains should be elongated. On the other hand, models of interstellar dust grain growth assume that dust grains are spherical and not elongated. We show that when dusty plasma effects and the dipole moment of water molecules are together taken into account, ice grains in interstellar space should be prolate ellipsoids and not spheres. Dusty plasma analysis shows that an ice grain is charged to a negative potential that has magnitude nearly equal to that of the electron temperature. Several different mechanisms causing deviation from sphericity are identified; these mechanisms involve the interaction of the dipole moment of water molecules with electric fields associated with ice grain charging. These mechanisms include the focusing of water molecule trajectories, the migration of water molecules in a quasi-liquid layer on the grain surface toward regions where the electric field is strongest, the enhancement of this migration by the bombardment of energetic protons that gain energy upon falling into the ice grain negative potential, and mutual repulsion by electric charges having the same sign. The aspect ratio is established shortly after the ice grain is formed, and then is maintained as the grain grows.
A Dust Trap in the Young Multiple System HD 34700
Authors: Benac Peyton , Matrà Luca , Wilner David J. , Jimènez-Donaire Marìa J. , Monnier J. D. , Harries Tim J. , Laws Anna , Rich Evan A. , Zhang Qizhou 
Published: December 2020

Abstract
Millimeter observations of disks around young stars reveal substructures indicative of gas pressure traps that may aid grain growth and planet formation. We present Submillimeter Array observations of HD 34700: two Herbig Ae stars in a close binary system (Aa/Ab, ∼0.25 au), surrounded by a disk presenting a large cavity and spiral arms seen in scattered light, and two distant, lower-mass companions. These observations include 1.3 mm continuum emission and the 12CO 2–1 line at ∼05 (178 au) resolution. They resolve a prominent azimuthal asymmetry in the continuum and Keplerian rotation of a circumbinary disk in the 12CO line. The asymmetry is located at a radius of 155+11
−7 au, consistent with the edge of the scattered-light cavity, being resolved in both radius (72 +14
−15 au) and azimuth (FWHM = 64°+8
−7). The strong asymmetry in millimeter continuum emission could be evidence for a dust trap, together with the more symmetric morphology of 12CO emission and small grains. We hypothesize an unseen circumbinary companion responsible for the cavity in scattered light and creating a vortex at the cavity edge that manifests in dust trapping. The disk mass has limitations imposed by the detection of 12CO and nondetection of 13CO. We discuss its consequences for the potential past gravitational instability of this system, likely accounting for the rapid formation of a circumbinary companion. We also report the discovery of resolved continuum emission associated with HD 34700B (projected separation ∼1850 au), which we explain through a circumstellar disk.
Star Formation in Splash Bridges
Authors: Yeager Travis , Struck Curtis 
Published: December 2020

Abstract
Splash bridges are created from the direct collision of two gas-rich disk galaxies. These direct collisions can eject gas masses on the order of 1010
M
⊙ stripped from the stellar disks of each galaxy. The Taffy Galaxy system (UGC 1294/5) is a prototypical example of a splash bridge system. CO observations of the Taffy revealed that its splash bridge contains a mass of H2 equal to the Milky Way’s H2 mass. However, the little visible star formation occurring within the bridge highlights the need for models of direct gas-rich disk collisions. The Arp 194 system displays what may be another splash bridge resulting from the collision between two disk galaxies. The region between the two stellar disks contains bright clumps of active star formation. We aim to better understand the conditions for star formation in splash bridges by employing a Jeans criterion to determine where gravitational instabilities occur in the shocked and cooling gas of gas-rich disk collisions. The splash bridge results are obtained from our previous work using a sticky particle code and post-processed. We find that the inclination between the gas disks and the collision velocity with which the gas collides strongly affects the fraction of gas that will become gravitationally unstable. Low inclinations between gas disks produce starbursts whereas high inclinations result in steady-rate star formation. The offset of the gas disks at impact will determine how many gas elements directly collide but does not strongly affect the resulting star formation.
La Guerra del Paraguay entre líneas. Los proyectos archivísticos y la correspondencia de Juan E. O’Leary y Luis A. de Herrera (1905 – 1926)
Authors: Liliana María Brezzo  , Maria Laura Reali  
Published: December 2020

Resumen
La Guerra del Paraguay es uno de los grandes temas que circulan en el espacio epistolar del historiador paraguayo Juan E. O’Leary y de su par uruguayo Luis A. de Herrera. La extendida correspondencia que cultivaron entre los años 1905 y 1926, que alberga los respectivos archivos personales, es examinada en este trabajo para analizar el pensamiento de los dos historiadores haciéndose, a modo de taller de su escritura sobre la guerra y en tanto estadios eventuales de sus producciones mayores dirigidas a la esfera pública.
Palabras clave: Escritura de la Guerra del Paraguay – Archivos Personales – Redes Epistolares – Revisionismo histórico – Círculos Intelectuales Trasnacionales.
MANAJEMEN STRATEGIK DALAM PENILAIAN KINERJA
Authors: Muzakki Muzakki , Ariyanto Soni Yuda 
Published: December 2020

Setiap organisasi atau instansi dalam melaksanakan program yang diarahkan selalu berdaya guna untuk mencapai tujuan perusahaan. Salah satu caranya adalah meningkatkan kinerja karyawan. kinerja adalah hasil kerja secara kualitas dan kuantitas yang dicapai oleh seorang pegawai dalam melaksanakan tugasnya sesuai dengan tanggung jawab yang diberikan kepadanya. Penilaian kinerja guru pada dasarnya merupakan proses membandingkan antara kinerja actual dengan kinerja ideal untuk mengetahui tingkat keberhasilan guru dalam melaksanakan tugas-tugasnya dalam periode tertentu. Penilaian kinerja guru diartikan sebagai penilaian dari tiap butir kegiatan tugas utama guru dalam kerangka pembinaan karier, kepangkatan, dan jabatannya

Kata kunci: Manajemen Strategik, Penilaian Kinerja