bluuebunny/crossref_metadata_2025_split huggingface dataset:
Factors Associated With A Ruptured Perineum On A Vaginal Birth At The Clinic Niar The Terrain Of The Year 2018
Authors: Pemiliana Putri Diah , Sarumpaet Irma Handayani , Ziliwu Dan Sanak 
Published: June 2019

Introduction: Ruptured perineum due to pregnancy, parity, age of mother, baby weight, vacuum extraction, trauma tools and episiotomy. Based on data of the World HealthOrganization(WHO) going on 2.7 million cases of rupturperineum in the mother birthing. This figure is expected to reach 6.3 million by the year 2050. The purpose of : this research is to know the factors which Fotor associated with Ruptured Perineum At vaginal birth at the clinic Pratama Medan Tahun2018 N. Method: the research design used in this research is a survey of the analytic approach of using CrossSectional , sampling using the total populationwith the techniques of medical record data collection by using the statiscttestChi Square. Results: the research on test by Chi Square, the data obtained with the data of skunder test results statistc showed no relationship age mom with ruptured perineum with p =0.037 value (p = 0.04), the relationship of the weight of the baby with a ruptured perineum with p =0.041 value (p = 0,041) and the relationship of parity with ruptured perineum with p =0.003value (p = 0.003). at the clinic the year 2018 Pratama Medan N. Based on logistic regression test variable BBL has close relationship ruptured perineum against value of sig 0.61, the value of the Exp (B)/OR largest 2.510 meaning likely or highly influential BBL 2.510 times can cause the occurrence of ruptured the perineum. Conclusion : the results of data analysis and discussion that there is a relationship of maternal Age, Parity and infant's Weight with a Ruptured Perineum in vaginal birth.
Análise comparativa dos sistemas construtivos alvenaria convencional e light steel framing: um estudo de caso em residência uniifamiliar em Teófilo Otoni, MG
Authors: Salomão Pedro Emílio Amador , Soares Alan Deivid Alves , Lorentz Larissa Petrini Alves , Paula Larissa Tatiane Gonçalves de 
Published: June 2019

A busca por alternativas construtivas mais eficientes, sustentáveis e rápidas de modo a aumentar a produtividade e atender a demanda crescente do mercado tem sido um dos grandes desafios para a construção civil. A fim de atender esta demanda, um novo método de construção conhecido como Light Steel Framing (LSF) vem sendo uma ótima alternativa, embora seja mais conhecido em países mais desenvolvidos, no Brasil, sua prática vem sendo difundida e utilizada ganhando ainda mais espaço no setor, proporcionando uma construção rápida e com qualidade. Neste trabalhando foi realizado uma analise comparativa entre o sistema Light Steel Framing e Alvenaria Convencional através de um projeto de uma residência modelo de um pavimento com objetivo de apresentar os principais diferenciais entre estes sistemas construtivos em residências unifamiliares. Com os projetos definidos é feito o levantamento quantitativo dos materiais utilizados e são montadas as composições dos principais elementos que diferem entre ambos os sistemas estudados. Através das pesquisas foi possível identificar os custos unitários de cada item e realizar uma análise dos resultados obtidos destacando as principais diferenças. Os resultados mostraram que o sistema LSF como um sistema industrializado apresenta maior produtividade, possuindo uma construção limpa, seca, e sustentável, além de apresentar baixo peso, porém em relação ao custo da obra o estudo apresentou o sistema LSF como menos vantajoso quando comparado à alvenaria convencional, apresentando ser 18,09% mais caro. Sabendo-se que o sistema Light Steel Framing tem várias vantagens técnicas com maior viabilidade de execução sobre o sistema de alvenaria convencional já comprovado com este estudo. Conclui-se que os profissionais da área da construção civil devem incentivar mais os empresários e construtores a usar este tipo de construção.
On the nature of ultraluminous X-ray sources
Authors: Fabrika S N , Atapin K E , Vinokurov A S 
Published: June 2019

Abstract
Ultraluminous X-ray sources (ULXs) that are located in external galaxies exhibit X-ray luminosities exceeding those of the brightest black holes in the Milky Way and the Local Group galaxies by hundreds or even thousands of times. New classes of objects have been discovered: ultraluminous X-ray pulsars (ULXPs) and high-velocity outflows whose X-ray-range speed is up to 0.2c. The ULXs and ULXPs fully correspond to concepts of super-Eddington accretion. Five ULXs exhibit quasiperiodic oscillations and a flat-topped noise in the X-ray range power spectrum. Optical spectra of ULXs are very similar to those of SS433, late nitrogen stars (WNL/WR), or LBV (luminous blue variable) stars. The results obtained suggest that ULXs are systems that contain supercritical accretion disks.
High-energy ball milling of nonstoichiometric compounds
Authors: Gusev A I 
Published: June 2019

Abstract
The preparation of nanocrystalline powders of nonstoichiometric compounds such as carbides and oxides by high-energy milling is considered. The modern state of milling models for nonstoichiometric compounds is described. The influence of nonstoichiometry on the particle size of the produced nanopowders is discussed. The model dependences of the size of nanopowder particles on the duration of milling and the composition of nonstoichiometric compounds are compared with the literature experimental results on the milling of nonstoichiometric carbides and oxides. Diffraction methods for the certification of nanopowders according to the size of the nanoparticles, the magnitude of microstrains, and the uniformity of the microstructure are considered in detail. The importance of taking into account the anisotropy of microstrains in milled nanopowders is shown.
RANCANGAN INSTRUMEN PENGUKURAN KINERJA PEGAWAI DENGAN MENGGUNAKAN PENDEKATAN HUMAN RESOURCES SCORECARD DALAM RANGKA MENINGKATKAN KINERJA ORGANISASI (Studi Kasus pada Taman Lalu Lintas – Ade Irma Suryani Nasution Bandung)
Authors: Achmad Asep Zulkifli 
Published: June 2019

Penelitian ini bertujuan untuk memperoleh bukti empiris mengenai ”Rancangan Instrumen Pengukuran Kinerja Pegawai Dengan Menggunakan Pendekatan Human Resources Scorecard dalam rangka meningkatkan Kinerja Organisasi (Studi Kasus pada Taman Lalu Lintas – Ade Irma Suryani Nasution Bandung)”. Penelitian ini diharapkan juga memberikan sumbangan dalam aspek praktis (daya guna) yaitu masukan kepada pihak manajemen Taman Lalu Lintas AISN Bandung, atau institusi lain yang sejenis dalam melakukan implementasi dan kebijakan serta pengambilan keputusan terutama yang berkaitan dengan masalah kinerja sumber daya manusia dalam rangka peningkatan citra dan peningkatan fungsi lembaga / perusahaan.Metode penelitian yang digunakan adalah analisis deskriptif kualitatif. Pengumpulan data yang digunakan adalah wawancara, observasi, dan dokumentasi. Pengumpulan data di lapangan dilaksanakan pada tahun 2016.Hasil penelitian menunjukan bahwa pencapaian kinerja pegawai Taman Lalu Lintas berada dalam kriteria kinerja kurang baik. Faktor penghambat pengukuran kinerja pegawai di Taman Lalu Lintas Bandung yaitu pelatihan, pengalaman, pendapatan, kepemimpinan, supervisi, pengembangan karir, uraian tugas, dan metode penilaian kinerja. Faktor penting dalam implementasi Human Resources Scorecard yaitu rekrutmen karyawan yang memiliki kompetensi yang sesuai, meningkatkan kualitas pelayanan internal. Kata Kunci : Human Resources Scorecard, Kinerja pegawai, Kinerja Organisasi
CONSULTA DE NUTRICIÓN Una parte del quehacer diario.
Authors: Zúñiga Quesada Jeannette 
Published: June 2019

Cuando trabajamos en comunidad es difícil olvidar las atenciones de la gente y el arraigo que hay en nuestro país por el ofrecer un “bocadito“o un “gallito “al visitante, dejando latente que mostramos amor por medio de la alimentación. De ahí que en ocasiones nuestra labor de fomentar buenos hábitos de alimentación se veaobstaculizada por ese afán de las abuelitas de ver cachetones a sus nietos, con la falsa idea que el niño gordito es el niño saludable. O de darle caldo de frijol con guineo, para quitarles la anemia.
Pausas Activas
Authors: Alfaro Gurrola Silvia 
Published: June 2019

Las pausas activas son una serie de actividades y acciones que les permiten a diferentes partes delcuerpo un cambio en su rutina habitual. Debemos descartarlas como interrupciones laborales y por el contrario verlas como períodos de recuperación que se hacen durante la jornada de trabajo; para recuperar la energía, disminuir el estrés y mejorar el desempeño y eficiencia en las labores. Está comprobado que la inactividad física aumentael número de incapacidades, no sólo en cuanto a su frecuencia sino también en cuanto a su duración; alterando la dinámica para el trabajador y la empresa
ANALISIS PENERAPAN PERATURAN PEMERINTAH NO.96 TAHUN 2012 TENTANG PELAYAAN PUBLIK DI PEMERINTAHAN KECAMATAN PASARWAJO KABUPATEN BUTON SULAWESI TENGGARA (STUDI PERBANDINGAN KUALITAS PELAYANAN PUBLIK SEBELUM DAN SESUDAH PENERAPANYA)
Authors: Gazalin Junaid 
Published: June 2019

Penelitian ini bertujuan untuk : (1). Untuk mengetahui Penerapan Peraturan Pemerintah No.96 Tahun 2012 Tentang Pelayaan Publik di Pemerintahan Kecamatan Pasarwajo. Untuk mengidentifikasi faktor-faktor yang mempengaruhi Penerapan Peraturan Pemerintah No.96 Tahun 2012 Tentang Pelayaan Publik di Pemerintahan Kecamatan Pasarwajo.
Penelitian menjelaskan bahwa proses serta kualitas pelayanan publik, dalam hal ini pengurusan pengantar admnistrasi, KK, Akta Jual Beli Tanah, Akte Lahir, IMB dan SIU bagi warga masyarakat di Kantor Kecamatan Pasarwajo Kabupaten Buton sebelum diterapkan PP 96 Tahun 2012, pada umumnya kurang memuaskan dan masih perlu untuk ditingkatkan. Setelah peraturan tersebut diterapkan dengan menata kembali sistem pelayanan sesuai dengan standar operasional pelayanan publik, maka proses dan mekanisme pelayanan publik bagi warga masyarakat setempat telah berjalan lancar. kualitas pelayanan publik menjadi lebih baik. Terutama mengenai kemudahan pelayanan, kecepatan waktu pelayanan, keramah-tamahan aparat, transparansi biaya, tingkat produktivitas pelayanan, efisiensi dan efektivitas pelayanan publik. Hal ini dicapai karena camat membenahi persyaratan berkas yang disiapkan, kejelasan informasi prosedur, mekanisme dan alur yang harus dilalui, tranparansi biaya dan waktu pengurusan. Penyelesaian pelayanan publik yang cepat seringkali beriringan dengan beban biaya pelayanan, untuk itu proses ini perlu dirubah pelan-pelan melalui pembiasaan oleh aparat untuk bekerja profesional.
Pengaruh Perkawinan Usia Muda Terhadap Pola Asuh Keluarga Di Kota Baubau
Authors: Nurbaena Wa Ode Wati 
Published: June 2019

Tujuan penelitian ini menaruh pokok kajian pada dinamika perkawinan usia muda dan implikasi yang sering menjadi keluhan dan masalah yang ditemui beberapa tahun ini. Disisi lain, kajian ini juga menaruh perhatian lebih pada peran dari pemerintah daerah dalam memberikan pengawasan dan pembinaan pada kejadian pernikahan usia muda khususnya di Kota Baubau. Penelitian menggunakan metode kualitatif dengan pendekatan deskriptif. Hal ini menjadi alasan untuk menggunakan metode kualitatif adalah sejalan dengan tujuan penelitian ini yang ingin mendapatkan data deskriptif berupa lisan atau kata-kata dari gejala yang diamati atau diteliti. Berdasarkan hasil penelitian di atas, mengenai faktor-faktor pendorong, dampak-dampak dan bentuk pola asuh keluarga dalam pasangan yang menikah pada usia muda, dipengaruhi oleh adanya tekanan pada beberapa faktor diantaranya adalah faktor ekonomi, faktor orang tua, faktor pendidikan, faktor diri sendiri dan faktor adat setempat.
TRANSFORMASI UPAYA ADMINISTRATIF DALAM PENYELESAIAN SENGKETA KEPEGAWAIAN
Authors: Marbun Robinsar 
Published: June 2019

Civil Service dispute is a dispute/dispute arising as a result of the stipulation of a State Administrative Decision in the field of personnel by the Authorized Body or Official regarding the position, obligation, right and guidance of Civil Servants. While Administrative Efforts is a procedure that can be taken by Civil Servants who are not satisfied with disciplinary punishment imposed on him in the form of objection or administrative appeal. The objection itself is an administrative effort that can be taken by the Disgruntled Civil Servant against disciplinary punishment imposed by the competent authority to punish the superior officer in charge of punishment. For Administrative Appeals alone it is an administrative undertaking that a disgruntled Civil Servant may take with respect to disciplinary punishment in the form of dismissal with respect not on his own request or dismissal with respect as a Civil Servant imposed by a punitive authority to the Employment Advisory Board
CHIPS: THE COSMOLOGICAL H i POWER SPECTRUM ESTIMATOR
Authors: Trott C. M. , Pindor B. , Procopio P. , Wayth R. B. , Mitchell D. A. , McKinley B. , Tingay S. J. , Barry N. , Beardsley A. P. , Bernardi G. , Bowman Judd D. , Briggs F. , Cappallo R. J. , Carroll P. , Oliveira-Costa A. de , Dillon Joshua S. , Ewall-Wice A. , Feng L. , Greenhill L. J. , Hazelton B. J. , Hewitt J. N. , Hurley-Walker N. , Johnston-Hollitt M. , Jacobs Daniel C. , Kaplan D. L. , Kim H. S. , Lenc E. , Line J. , Loeb A. , Lonsdale C. J. , Morales M. F. , Morgan E. , Neben A. R. , Thyagarajan Nithyanandan , Oberoi D. , Offringa A. R. , Ord S. M. , Paul S. , Pober J. C. , Prabu T. , Riding J. , Shankar N. Udaya , Sethi Shiv K. , Srivani K. S. , Subrahmanyan R. , Sullivan I. S. , Tegmark M. , Webster R. L. , Williams A. , Williams C. L. , Wu C. , Wyithe J. S. B. 
Published: June 2019

ABSTRACT
Detection of the cosmological neutral hydrogen signal from the Epoch of Reionization (EoR) and estimation of its basic physical parameters are principal scientific aims of many current low-frequency radio telescopes. Here we describe the Cosmological H i Power Spectrum Estimator (CHIPS), an algorithm developed and implemented with data from the Murchison Widefield Array, to compute the two-dimensional and spherically-averaged power spectrum of brightness temperature fluctuations. The principal motivations for CHIPS are the application of realistic instrumental and foreground models to form the optimal estimator, thereby maximizing the likelihood of unbiased signal estimation, and allowing a full covariant understanding of the outputs. CHIPS employs an inverse-covariance weighting of the data through the maximum likelihood estimator, thereby allowing use of the full parameter space for signal estimation (“foreground suppression”). We describe the motivation for the algorithm, implementation, application to real and simulated data, and early outputs. Upon application to a set of 3 hr of data, we set a 2σ upper limit on the EoR dimensionless power at

Mpc−1 of

mK2 in the redshift range z = [6.2–6.6], consistent with previous estimates.
THE H i CONTENT OF GALAXIES IN GROUPS AND CLUSTERS AS MEASURED BY ALFALFA
Authors: Odekon Mary Crone , Koopmann Rebecca A. , Haynes Martha P. , Finn Rose A. , McGowan Christopher , Micula Adina , Reed Lyle , Giovanelli Riccardo , Hallenbeck Gregory 
Published: June 2019

ABSTRACT
We present the H i content of galaxies in nearby groups and clusters as measured by the 70% complete Arecibo Legacy Fast-ALFA (ALFALFA) survey, including constraints from ALFALFA detection limits. Our sample includes 22 systems at distances between 70 and 160 Mpc over the mass range

, for a total of 1986 late-type galaxies. We find that late-type galaxies in the centers of groups lack H i at fixed stellar mass relative to the regions surrounding them. Larger groups show evidence of a stronger dependence of H i properties on environment, despite a similar dependence of color on environment at fixed stellar mass. We compare several environment variables to determine which is the best predictor of galaxy properties; group-centric distance r and

are similarly effective predictors, while local density is slightly more effective and group size and halo mass are slightly less effective. While both central and satellite galaxies in the blue cloud exhibit a significant dependence of H i content on local density, only centrals show a strong dependence on stellar mass, and only satellites show a strong dependence on halo mass. Finally, we see evidence that H i is deficient for blue cloud galaxies in denser environments even when both stellar mass and color are fixed. This is consistent with a picture where H i is removed or destroyed, followed by reddening within the blue cloud. Our results support the existence of pre-processing in isolated groups, along with an additional rapid mechanism for gas removal within larger groups and clusters, perhaps ram-pressure stripping.
THE KINEMATICS OF C iv IN STAR-FORMING GALAXIES AT z ∼ 1.2
Authors: Du Xinnan 杜辛楠 , Shapley Alice E. , Martin Crystal L. , Coil Alison L. 
Published: June 2019

ABSTRACT
We present the first statistical sample of rest-frame far-UV spectra of star-forming galaxies at z ∼ 1. These spectra are unique in that they cover the high-ionization C iv
λλ1548, 1550 doublet. We also detect low-ionization features such as Si ii
λ1526, Fe ii
λ1608, Al ii
λ1670, Ni ii
λλ1741, 1751, and Si ii
λ1808, and intermediate-ionization features from Al iii
λλ1854, 1862. Comparing the properties of absorption lines of lower- and higher-ionization states provides a window into the multiphase nature of circumgalactic gas. Our sample is drawn from the DEEP2 survey and spans the redshift range 1.01 ≤ z ≤ 1.35 (

). By isolating the interstellar C iv absorption from the stellar P Cygni wind profile, we find that 69% of the C iv profiles are blueshifted with respect to the systemic velocity. Furthermore, C iv shows a small but significant blueshift relative to Fe ii (offset of the best-fit linear regression −76 ± 26 km s−1). At the same time, the C iv blueshift is on average comparable to that of Mg ii
λλ2796, 2803. At this point, in explaining the larger blueshift of C iv absorption at the ∼3σ level, we cannot distinguish between the faster motion of highly ionized gas relative to gas traced by Fe ii and filling in on the red side from resonant C iv emission. We investigate how far-UV interstellar absorption kinematics correlate with other galaxy properties using stacked spectra. These stacking results show a direct link between C iv absorption and the current star formation rate, though we only observe small velocity differences among different ionization states tracing the outflowing interstellar medium.
THERMAL INFRARED IMAGING AND ATMOSPHERIC MODELING OF VHS J125601.92-125723.9 b: EVIDENCE FOR MODERATELY THICK CLOUDS AND EQUILIBRIUM CARBON CHEMISTRY IN A HIERARCHICAL TRIPLE SYSTEM
Authors: Rich Evan A. , Currie Thayne , Wisniewski John P. , Hashimoto Jun , Brandt Timothy D. , Carson Joseph C. , Kuzuhara Masayuki , Uyama Taichi 
Published: June 2019

ABSTRACT
We present and analyze Subaru/IRCS L′ and M′ images of the nearby M dwarf VHS J125601.92-125723.9 (VHS 1256), which was recently claimed to have an ∼11 M

J
companion (VHS 1256 b) at ∼102 au separation. Our adaptive optics images partially resolve the central star into a binary, whose components are nearly equal in brightness and separated by 0.″106 ± 0.″001. VHS 1256 b occupies nearly the same near-infrared position in the color–magnitude diagram as HR 8799 bcde and has a comparable L′ brightness. However, it has a substantially redder H – M′ color, implying a relatively brighter M′ flux density than for the planets of HR 8799 and suggesting that non-equilibrium carbon chemistry may be less significant in VHS 1256 b. We successfully match the entire spectral energy distribution (optical through thermal infrared) for VHS 1256 b to atmospheric models assuming chemical equilibrium, models that failed to reproduce HR 8799 b at 5 μm. Our modeling favors slightly thick clouds in the companion's atmosphere, although perhaps not quite as thick as those favored recently for HR 8799 bcde. Combined with the non-detection of lithium in the primary, we estimate that the system is at least 200 Myr old and the masses of the stars comprising the central binary are at least 58 M

J
each. Moreover, we find that some of the properties of VHS 1256 are inconsistent with the recent suggestion that it is a member of the AB Dor moving group. Given the possible range in distance (12.7 pc versus 17.1 pc), the lower mass limit for VHS 1256 b ranges from 10.5 M

J
to 26.2 M

J
. Our detection limits rule out companions more massive than VHS 1256 b exterior to 6–8 au, placing significant limits on and providing some evidence against a second, more massive companion that may have scattered the wide-separation companion to its current location. VHS 1256 is most likely a very low-mass hierarchical triple system and could be the third such system in which all components reside in the mass regime of brown dwarfs.
Confirmation of the Gaia DR2 Parallax Zero-point Offset Using Asteroseismology and Spectroscopy in the Kepler Field
Authors: Zinn Joel C. , Pinsonneault Marc H. , Huber Daniel , Stello Dennis 
Published: June 2019

Abstract
We present an independent confirmation of the zero-point offset of Gaia Data Release 2 parallaxes using asteroseismic data of evolved stars in the Kepler field. Using well-characterized red giant branch stars from the APOKASC-2 catalog, we identify a Gaia astrometric pseudocolor (

ν

eff

)- and Gaia G-band magnitude-dependent zero-point offset of

ϖ

seis

−

ϖ

Gaia

= 52.8 ± 2.4 (rand.) ± 8.6 (syst.) − (150.7 ± 22.7)(

ν

eff

− 1.5) − (4.21 ± 0.77)(G − 12.2) μas, in the sense that Gaia parallaxes are too small. The offset is found in high- and low-extinction samples, as well as among both shell H-burning red giant stars and core He-burning red clump stars. We show that errors in the asteroseismic radius and temperature scales may be distinguished from errors in the Gaia parallax scale. We estimate systematic effects on the inferred global Gaia parallax offset, c, due to radius and temperature systematics, as well as choices in bolometric correction and the adopted form for Gaia parallax spatial correlations. Because of possible spatially correlated parallax errors, as discussed by the Gaia team, our Gaia parallax offset model is specific to the Kepler field, but broadly compatible with the magnitude- and color-dependent offset inferred by the Gaia team and several subsequent investigations using independent methods.
Long Gamma-Ray Burst Rate at Very High Redshift
Authors: Kinugawa Tomoya , Harikane Yuichi , Asano Katsuaki 
Published: June 2019

Abstract
Future missions for long gamma-ray burst (GRB) observations at high redshift, such as the High-z Gamma-ray bursts for Unraveling the Dark Ages Mission and the Transient High-Energy Sky and Early Universe Surveyor, will provide clues to the star formation history in our universe. In this paper focusing on high-redshift (z > 8) GRBs, we calculate the detection rate of long GRBs by future observations, considering both Population I and II stars and Population III stars as GRB progenitors. For the Population I and II star formation rate (SFR), we adopt an up-to-date model of a high-redshift SFR based on the halo mass function and the dark matter accretion rate obtained from cosmological simulations. We show that the Population I and II GRB rate steeply decreases with redshift. This would rather enable us to detect the different type of GRBs, Population III GRBs, at very high redshift. If 10% or more Population III stars die as an ultra-long GRB, the future missions would detect such GRBs in one year in spite of their low fluence. More luminous GRBs are expected from massive compact Population III stars produced via the binary merger. In our conventional case, the detection rate of such luminous GRBs is 3–20 yr−1 (z > 8). Those future observations contribute to revealing the Population III star formation history.