bluuebunny/crossref_metadata_2025_split huggingface dataset:
PERAWATAN BAYI BARU LAHIR (BBL) PADA IBU USIA PERKAWINAN KURANG DARI 18 TAHUN (Di Wilayah Puskesmas Tiron Kabupaten Kediri)
Authors: Rahmawati Dian , Meiferina Delialika Ady 
Published: September 2019

Bayi baru lahir (BBL) sangat rentan terhadap infeksi yang disebabkan oleh paparan virus dan kuman selama proses persalinan maupun beberapa saat setelah lahir. Perawatan BBL yang tidak tepat dapat menimbulkan masalah kesehatan pada bayi sampai kematian. Kesalahan tersebut dikarenakan kurangnya pengetahuan dan kesiapan ibu dalam perawatan BBL. Usia perkawinan ibu yang terlalu muda (kurang dari 18 tahun) memungkinkan kurangnya pengetahuan dan kesiapan ibu dalam perawatan BBL. Di Jawa Timur (2015), remaja yang menikah di usia dini sebanyak 53 per 1000 pernikahan dan angka rata-rata nasional 48 per 1000 pernikahan. Hasil wawancara terhadap 3 ibu BBL dengan usia kurang dari 18 tahun diketahui bahwa 2 orang (66,67%) belum mengetahui cara merawat bayinya yang benar. Perawatan BBL yang dimaksud antara lain perawatan tali pusat, memandikan bayi, memberi minum, membersihkan telinga, membersihkan alat kelamin, mengganti popok bayi, dan menggunting kuku. Untuk itu penelitian ini bertujuan untuk mengetahui bagaimana perawatan BBL pada ibu usia perkawinan kurang dari 18 tahun di wilayah Puskesmas Tiron kabupaten Kediri.
Desain penelitian ini adalah deskriptif dengan pendekatan cross sectional. Populasi dalam penelitian ini adalah seluruh ibu dengan usia perkawinan ≤ 18 tahun yang mempunyai BBL di wilayah puskesmas Tiron kabupaten Kediri. Dengan tehnik total sampling didapatkan sampel sebanyak 30 respoden ibu dengan usia perkawinan ≤ 18 tahun yang mempunyai BBL di wilayah puskesmas Tiron kabupaten Kediri. Pengumpulan data dengan kuesioner, wawancara dan observasi, kemudian dilakukan editing, coding,scoring, dan tabulating, selanjutnya data dianalisis dengan persentase.
Penelitian menunjukkan bahwa sebanyak 5 responden (17%) melakukan perawatan BBL dengan kriteria baik, 19 responden (63%) melakukan perawatan BBL dengan kriteria cukup, dan 6 responden (20%) melakukan perawatan BBL dengan kriteria kurang.di Wilayah Puskesmas Tiron Kecamatan Banyakan Kabupaten Kediri.
Perawatan BBL pada ibu usia perkawinan ≤ 18 Tahun di wilayah Puskesmas Tiron kabupaten Kediri secara keseluruhan menunjukkan sebagian besar cara perawatannya cukup sebanyak 19 responden (63%).
Educación inclusiva: una teoría sin disciplina. legados y recuperación de saberes diaspóricos para una epistemología pluritópica
Authors: Ocampo González Aldo 
Published: September 2019

El presente trabajo ofrece un examen analítico-metodológico exhaustivo acerca de las dimensiones de configuración del obstáculo epistemológico de la Educación Inclusiva. Se propone avanzar en la comprensión de un conjunto de elementos post-disciplinarios que explican la ausencia de una teoría clara y oportuna en la materia. Todo ello, demuestra la incapacidad de la investigación de pensar la inclusión desde sistemas de razonamientos alternativos, más amplios y heterológicos, capaces de responder a la pregunta: ¿en qué medida la Educación Inclusiva es para todo el mundo? La hibridez de su racionalidad débilmente construida, se basa, en cierta medida, en la imposición del paradigma tradicional de Educación Especial y en la recurrencia semántica, ideológica y gramatical de la zona de abyección, espacialidad a través de la cual la multiplicidad de diferencias es abordada desde el esencialismo –conceptual, liberal y estratégico–, implantando procesos con referencia a la ‘inclusión a lo mismo’, es decir, estructuras sociales y educativas gobernadas por los formatos del poder. En un primer momento, se analizan los dispositivos de construcción del conocimiento de la Educación Inclusiva, determinando los ejes de configuración de su objeto de conocimiento y el tipo de ideas que forman en un período particular del pensamiento educativo. En un segundo momento, se presentan los axiomas y principios fundamentales de la epistemología de la Educación Inclusiva, las características de la naturaleza de su conocimiento, avanzado hacia la reconstrucción de los nuevos fundamentos de la inclusión en el siglo XXI. Se concluye identificando que los saberes epistémicos de la Educación Inclusiva viajan y se movilizan diaspóricamente por múltiples campos del conocimiento, tales como: los estudios post-coloniales, el feminismo, el marxismo, etc.
Korelasi Kadar Bilirubin Total Dengan Estimasi Laju Filtrasi Glomerolus Pada Penderita Penyakit Ginjal Kronik
Authors: Hidayah Nuraddiyani , Triwardhani Ria 
Published: September 2019

Latar belakang: Penyakit Ginjal Kronik (PGK) merupakan gangguan fungsi renal yang progresif dan ireversibel. Estimasi laju filtrasi glomerolus (eLFG) merupakan indeks untuk menilai fungsi ginjal. Stress oksidatif sebagai salah satu penyebab terjadinya disfungsi renal pada PGK. Bilirubin merupakan antioksidan dan mempunyai kemampuan renoprotektif. Tujuan penelitian untuk menganalisis korelasi kadar bilirubin total serum dengan eLFG pada penderita PGK.Â Metode: Penelitian belah lintang berdasarkan rekam medik penderita PGK di RSUP Dr. Kariadi pada Agustus 2015 â€“ Juli 2016. Analisis statistik untuk korelasi kadar bilirubin total serum dengan eLFG menggunakan uji korelasi Spearman.Hasil: Lima puluh dua penderita PGK dengan median (min-maks) kadar bilirubin total serum 0,55(0,22-2,10) mg/dl dan eLFG 11,75(3,4-112,60) ml/menit/1,73m2. Uji korelasi Spearman kadar bilirubin total serum dengan eLFG didapatkan r = 0,419; p = 0,002. Â Simpulan: Terdapat korelasi positif sedang yang bermakna antara kadar bilirubin total serum dengan eLFG. Bilirubin mempunyai kemampuan renoprotektif sehingga dengan mengetahui kadar bilirubin total serum dapat membantu mengetahui derajat progresifitas PGK.Â Kata kunci : penyakit ginjal kronik, bilirubin total serum, eLFGÂ
Acute kidney injury due to multiple bee stings in a 3 years old girl
Authors: Mellyana Omega , Adelina Dessy , Kusuma Jati 
Published: September 2019

Background:
Bee stings can lead to mild to severe allergic reaction . Serious complications of bee stings include hypersensitivity to the venom, which can develop after a single sting, and acute renal failure which has been reported mostly secondary of intravascular hemolysis developing after multiple bee stings. We report here a child who developed multiorgan system involvement.
Case presentation: A-3 years-old-girl was admitted to Kariadi Hospital with multiple bee stings and referred due to acute kidney injury stage failure by local hospital. Clinical finding were anasarca edema, gastrointestinal bleeding, oliguria (0.8ml/kgBW/hours), stage II hypertension (124/99mmHg), flaccid paraparesis inferior. Laboratory finding were hypoalbuminemia (2.4g/dL), anemia (6g/dl), leukocytosis (35.800/mm3), electrolyte imbalance (hypocalsemia:1.66mg/dL) and estimated glomerular filtration rate (eGFR) 8.09 ml/min/1.73m2. Chest-X ray showed pulmonary edema and duplex pleural effusion. The renal function recovered with supportive management including four sessions of haemodialysis. Patient discharged from the hospital on the nineteenth day.
Conclusions: Multiple bee stings can lead multiorgan system involvement
Keyword: Bee sting, acute kidney injury, hemodialisys
A Data Reduction Pipeline for Gemini-North’s Near-infrared Integral Field Spectrometer
Authors: Lemoine-Busserolle Marie , Comeau Nathaniel , Kielty Collin , Klemmer Kerry , Schwamb Megan E. 
Published: September 2019

Abstract
We present a python package, called Nifty4Gemini, and its associated Pyraf/Python based pipeline for processing Gemini-North Near-Infrared Integral Field Spectrometer (NIFS) observations. Built on the Gemini IRAF package’s capabilities, Nifty4Gemini's associated NIFS pipeline is a data reduction package which reduces NIFS raw data and produces a flux and wavelength calibrate science cube with the full signal-to-noise ratio, ready for science analysis. It utilizes tasks from the Gemini IRAF package, PyRAF, and packages from the Gemini AstroConda environment. Nifty4Gemini is a configuration-based pipeline framework written in python which is easily extensible to integrate additional pipelines and user-defined scripts. Nifty4Gemini is open source and available for download at https://github.com/mrlb05/Nifty4Gemini with its documentation available at https://nifty4gemini.readthedocs.io/en/latest/. A permanent version of the software described in this paper is archived at https://zenodo.org/record/1000413.
Two Long-period Cataclysmic Variable Stars: ASASSN-14ho and V1062 Cyg
Authors: Gasque L. Claire , Hening Callum A. , Hviding Raphael E. , Thorstensen John R. , Paterson Kerry , Breytenbach Hannes , Motsoaledi Mokhine , Woudt Patrick A. 
Published: September 2019

Abstract
We report spectroscopy and photometry of the cataclysmic variable stars ASASSN-14ho and V1062 Cyg. Both are dwarf novae with spectra dominated by their secondary stars, which we classify approximately as K4 and M0.5, respectively. Their orbital periods, determined mostly from the secondary stars’ radial velocities, proved to be nearly identical, respectively 350.14 ± 0.15 and 348.25 ± 0.60 minutes. The Hα emission line in V1062 Cyg displays a relatively sharp emission component that tracks the secondary’s motion, which may arise on the irradiated face of the secondary; this is not often seen and may indicate an unusually strong flux of ionizing radiation. Both systems exhibit double-peaked orbital modulation consistent with ellipsoidal variation from the changing aspect of the secondary. We model these variations to constrain the orbital inclination i, and estimate approximate component masses based on i and the secondary velocity amplitude K
2.
The Origin of the Late-time Luminosity of Supernova 2011dh
Authors: Maund Justyn R. 
Published: September 2019

Abstract
Due to the small amount of hydrogen (≤0.1 M
⊙) remaining on the surface of their progenitors, SNe IIb are sensitive probes of the mass-loss processes of massive stars toward the ends of their lives, including the role of binarity. We report late-time Hubble Space Telescope observations of SN 2011dh in M51, and a brief period of rebrightening and plateau in the photometric light curve, from 1.8 to 6.2 yr after the explosion. These observations exclude the role of circumstellar interaction, however, a slow rotating magnetar, a significant quantity of radioactive elements, or a light echo could be responsible for the late-time luminosity observed at t > 1000 days. If the late-time light curve is powered by the decay of radioactive elements, SN 2011dh is required to have produced ∼2.6 × 10−3
M
⊙ of 44Ti, which is significantly in excess of the amount inferred from earlier nebular spectra of SN 2011dh itself or measured in the Cas A SN remnant. The evolution of the brightness and the color of the late-time light curve also supports the role of a light echo originating from dust with a preferred geometry of a disk of extent ∼1.8 to ∼2.7 pc from the SN, consistent with a wind-blown bubble. Accounting for the long-term photometric evolution due to a light echo, the flux contribution from a surviving binary companion at ultraviolet wavelengths can be isolated and corresponds to a star of ∼9–10 M
⊙.
On the Occurrence of Crossings between the Angular Distributions of Electron Neutrinos and Antineutrinos in the Supernova Core
Authors: Shalgar Shashank , Tamborra Irene 
Published: September 2019

Abstract
Neutrino fast pairwise conversions have been postulated to occur in the dense core of a core-collapse supernova (SN), possibly having dramatic consequences on the SN mechanism and the observable neutrino signal. One crucial condition favoring pairwise conversions is the presence of crossings between the electron neutrino and antineutrino angular distributions (i.e., electron neutrino lepton number crossings, ELN crossings). A stationary and spherically symmetric SN toy model is constructed to reproduce the development of the neutrino angular distributions in the dense SN core in the absence of perturbations induced by hydrodynamical instabilities. By iteratively solving the neutrino Boltzmann equations including the collisional term, our model predicts that ELN crossings can develop only in the proximity of the decoupling region and for a sharp radial evolution of the baryon density, when the electron neutrino and antineutrino number densities are comparable. Such conditions are likely to occur only in the late SN stages. Interestingly, flavor instabilities induced by spatial or temporal perturbations are unlikely to generate ELN crossings dynamically within our simplified setup.
Homogeneous Analysis of Hot Earths: Masses, Sizes, and Compositions
Authors: Dai Fei , Masuda Kento , Winn Joshua N. , Zeng Li 
Published: September 2019

Abstract
Terrestrial planets have been found orbiting Sun-like stars with extremely short periods—some as short as 4 hr. These “ultra-short-period planets” or “hot Earths” are so strongly irradiated that any initial H/He atmosphere has probably been lost to photoevaporation. As such, the sample of hot Earths may give us a glimpse at the rocky cores that are often enshrouded by thick H/He envelopes on wider-orbiting planets. However, the mass and radius measurements of hot Earths have been derived from a hodgepodge of different modeling approaches, and include several cases of contradictory results. Here, we perform a homogeneous analysis of the complete sample of 11 known hot Earths with an insolation exceeding 650 times that of the Earth. We combine all available data for each planet, incorporate parallax information from Gaia to improve the stellar and planetary parameters, and use Gaussian process regression to account for correlated noise in the radial-velocity data. The homogeneous analysis leads to a smaller dispersion in the apparent composition of hot Earths, although there does still appear to be some intrinsic dispersion. Most of the planets are consistent with an Earth-like composition (35% iron and 65% rock), but two planets (K2-141b and K2-229b) show evidence for a higher iron fraction, and one planet (55 Cnc e) has either a very low iron fraction or an envelope of low-density volatiles. All of the planets are less massive than 8 M
⊕, despite the selection bias toward more massive planets, suggesting that 8 M
⊕ is the critical mass for runaway accretion.
Time-reversed Gamma-Ray Burst Light-curve Characteristics as Transitions between Subluminal and Superluminal Motion
Authors: Hakkila Jon , Nemiroff Robert 
Published: September 2019

Abstract
We introduce a simple model to explain the time-reversed and stretched residuals in gamma-ray burst (GRB) pulse light curves. In this model an impactor wave in an expanding GRB jet accelerates from subluminal to superluminal velocities, or decelerates from superluminal to subluminal velocities. The impactor wave interacts with the surrounding medium to produce Cerenkov and/or other collisional radiation when traveling faster than the speed of light in this medium, and other mechanisms (such as thermalized Compton or synchrotron shock radiation) when traveling slower than the speed of light. These transitions create both a time-forward and a time-reversed set of light-curve features through the process of relativistic image doubling. The model can account for a variety of unexplained yet observed GRB pulse behaviors, including the amount of stretching observed in time-reversed GRB pulse residuals and the relationship between stretching factor and pulse asymmetry. The model is applicable to all GRB classes since similar pulse behaviors are observed in long/intermediate GRBs, short GRBs, and X-ray flares. The free model parameters are the impactor’s Lorentz factor when moving subluminally, its Lorentz factor when moving superluminally, and the speed of light in the impacted medium.
The Analogous Structure of Accretion Flows in Supermassive and Stellar Mass Black Holes: New Insights from Faded Changing-look Quasars
Authors: Ruan John J. , Anderson Scott F. , Eracleous Michael , Green Paul J. , Haggard Daryl , MacLeod Chelsea L. , Runnoe Jessie C. , Sobolewska Malgosia A. 
Published: September 2019

Abstract
Despite their factor of ∼108 difference in black hole mass, several lines of evidence suggest possible similarities between black hole accretion flows in active galactic nuclei (AGN) and Galactic X-ray binaries. However, it is still unclear whether the geometry of the disk–corona system in X-ray binaries directly scales up to AGN and whether this analogy still holds in different accretion states. We test this AGN/X-ray binary analogy by comparing the observed correlations between the UV–to–X-ray spectral index (α
OX) and Eddington ratio in AGN to those predicted from observations of X-ray binary outbursts. This approach probes the geometry of their disk–corona systems as they transition between different accretion states. We use new Chandra X-ray and ground-based rest-UV observations of faded “changing-look” quasars to extend this comparison to lower Eddington ratios of <10−2, where observations of X-ray binaries predict a softening of α
OX in AGN. We find that the observed correlations between the α
OX and Eddington ratio of AGN displays a remarkable similarity to accretion state transitions in prototypical X-ray binary outbursts, including an inversion of this correlation at a critical Eddington ratio of ∼10−2. Our results suggest that the structures of black hole accretion flows directly scale across a factor of ∼108 in black hole mass and across different accretion states, enabling us to apply theoretical models of X-ray binaries to explain AGN phenomenology.
Forward Modeling of a Pseudostreamer
Authors: Karna Nishu , Savcheva Antonia , Dalmasse Kévin , Gibson Sarah , Tassev Svetlin , Toma Giuliana de , DeLuca Edward E. 
Published: September 2019

Abstract
In this paper, we present an analysis of a pseudostreamer embedding a filament cavity, observed on 2015 April 18 on the solar southwest limb. We use the flux-rope insertion method to construct nonlinear force-free field (NLFFF) models constrained by observed Solar Dynamics Observatory (SDO)/AIA coronal structures and the SDO/Helioseismic Magnetic Imager photospheric magnetogram. The resulting magnetic field models are forward-modeled to produce synthetic data directly comparable to Mauna Loa Solar Observatory/Coronal Multichannel Polarimeter (CoMP) observations of the intensity and linear polarization of the Fe xiii 1074.7 nm infrared coronal emission line using FORWARD. In addition, we determine the location of quasi-separatrix layers in the magnetic models, producing a Q-map from which the signatures of magnetic null points and separatrices can be identified. An apparent magnetic null observed in linear polarization by CoMP is reproduced by the model and appears in the region of the 2D-projected magnetic null in the Q-map. Further, we find that the height of the CoMP null is better reproduced by our NLFFF model than by the synthetic data we produce with potential-field source-surface models, implying the presence of a flux rope in the northern lobe of the pseudostreamer.
Linear Acoustic Waves in a Nonisothermal Atmosphere. II. Photospheric Resonator Model of Three-minute Umbral Oscillations
Authors: Chae Jongchul , Kang Juhyung , Litvinenko Yuri E. 
Published: September 2019

Abstract
The velocity oscillations observed in the chromosphere of sunspot umbrae resemble a resonance in that their power spectra are sharply peaked around a period of about three minutes. In order to describe the resonance that leads to the observed 3-minute oscillations, we propose the photospheric resonator model of acoustic waves in the solar atmosphere. The acoustic waves are driven by the motion of a piston at the lower boundary, and propagate in a nonisothermal atmosphere that consists of the lower layer (photosphere), where temperature rapidly decreases with height, and the upper layer (chromosphere), where temperature slowly increases with height. We have obtained the following results: (1) The lower layer (photosphere) acts as a leaky resonator of acoustic waves. The bottom end is established by the piston, and the top end by the reflection at the interface between the two layers. (2) The temperature minimum region partially reflects and partially transmits acoustic waves of frequencies around the acoustic cutoff frequency at the temperature minimum. (3) The resonance occurs in the photospheric layer at one frequency around this cutoff frequency. (4) The waves escaping the photospheric layer appear as upward-propagating waves in the chromosphere. The power spectrum of the velocity oscillation observed in the chromosphere can be fairly well reproduced by this model. The photospheric resonator model was compared with the chromospheric resonator model and the propagating wave model.
Réinterprétation sociale locale et mémoires familiales de l’immigration aveyronnaise à Pigüé (Province de Buenos Aires, Argentine)
Authors: Albaladejo Christophe , Sassone Susana , Bustos Cara Roberto 
Published: September 2019

Résumé Cet article analyse un cas de revalorisation locale récente d’un passé d’immigration marginale (l’immigration française) dans un pays marqué par l’immigration massive : l’Argentine. Ce cas est constitué par la petite ville pampéenne de Pigüé qui a été fondée par des colons aveyronnais à la fin du xix e siècle. À travers 17 entretiens approfondis conduits auprès d’acteurs locaux en 2016 et 2017, et 4 entretiens menés en France auprès de responsables de la coopération avec Pigüé, nous analysons dans cet article les formes de distinction des lieux, les expressions culturelles, les moments particuliers (festivités), les pratiques culinaires et l’usage de la langue française. L’article met en évidence deux processus qui ne sont pas portés par les mêmes sujets et institutions : une patrimonialisation fondée sur la famille et l’identité individuelle, et une patrimonialisation établie sur l’appartenance au territoire local ainsi qu’une appropriation par ses habitants d’un passé de migrants qui permet d’aborder la question du processus socioculturel par lequel un habitant de Pigüé non descendant de Français peut sentir que le patrimoine de l’immigration aveyronnaise lui appartient également.
L’archéologisation des imaginaires. La mise en valeur des vestiges au nord du Pérou entre injonction et appropriation
Authors: Canghiari Emanuela 
Published: September 2019

Résumé Au Pérou, dans les années 1990, un champ patrimonial émerge sur la côte nord du pays. Cela se produit dans une conjoncture particulière. En effet, les importantes découvertes archéologiques conduisent l’élite régionale à reformuler un récit identitaire du Norte Grande basé sur un glorieux passé commun (la civilisation Moche ou Mochica). Cette « renaissance », impulsée par la décentralisation administrative et les politiques multiculturelles, s’inscrit dans un contexte de concurrence des mémoires. En effet, entre l’hégémonie culturelle de Cuzco d’une part et le centralisme économique de Lima de l’autre, la revalorisation de la région est amorcée à partir d’une injonction patrimoniale faisant coïncider l’identité Moche avec le nouveau découpage territorial et la recherche de dynamisme économique. L’authenticité, la filiation et la connexion avec le passé préhispanique deviennent ainsi des enjeux fondamentaux dans la production de légitimités au plan local. Ce processus sera analysé à partir de la comparaison de données ethnographiques recueillies à Túcume et à Huaca Rajada-Sipán (Lambayeque). Ces deux communautés ont adopté des stratégies d’appropriation des vestiges et des positionnements très divers, afin de faire reconnaître la concordance entre identité et territoire, et de devenir ainsi des acteurs dignes de patrimonialisation.