bluuebunny/crossref_metadata_2025_split huggingface dataset:
Perbedaan Makna Novel dan Film Ayat-Ayat Cinta: Kajian Ekranisasi
Authors: Karkono Karkono 
Published: April 2017

Proses adaptasi dari novel ke bentuk film disebut ekranisasi. Perbedaan yang sering muncul dalam proses ekranisasi selama ini lebih sering disebabkan oleh perbedaan sistem sastra (dalam hal ini novel) dan sistem film. Hal-hal teknis seperti media novel yang berupa kata- kata dan bahasa sementara media utama film adalah audio visual (suara dan gambar) memang menjadi kewajaran jika antara novel dan film menjadi berbeda. Dalam kasus novel dan film
Ayat-Ayat Cinta (AAC), perbedaan yang ada bukan sebatas karena masalah teknis tersebut, tetapi adalah perbedaan yang disengaja. Hasil dari penelitian ini adalah menguraikan perbedaan-perbedaan antara novel dan film AAC yang kemudian bisa terdeskripsikan sebab- sebab perbedaan itu terjadi dan juga makna perbedaan tersebut. Dari penelitian ini dapat disimpulkan bahwa perbedaan yang ada antara novel dan film AAC bukan sebatas karena perbedaan sistem sastra dan sistem film, tetapi perbedaan yang disengaja oleh tim produksi film dengan maksud tertentu. Dari pengayaan dan berdasar pada fakta yang diungkap, peneliti menyimpulkan bahwa film AAC lebih menekankan pada persoalan poligami, ini terlihat dengan banyaknya penambahan adegan di dalam film yang menampilkan kehidupan poligami yang tidak ada di novel, sementara novel AAC lebih berisi. penggambaran perjuangan seorang mahasiswa Indonesia yang kuliah di Mesir beserta perjalanan kisah asmaranya.

Abstract
Adaptation process from novel to film is called ecranization. The differences often show up in the process of ecranization all this time is more regularly because of the difference of art
system (in this case novel) and the film system. Technical things as media or novel which consist of words and language, meanwhile film main media is audio visual (sow1d and picture) becomes a common thing if between novel and film become different. In the case of AAC's novel and film, the difference is not only because of that technical problem, but this is an intentional difference. From this research can be concluded that difference among AAC's novel and film is not one bounds because an system difference and film system, but intentional difference by film production team for the specific purposes. From enrichment and based on fact that revealing, researcher concludes that AAC's film more emphasizes on polygamy problem, this appears on many added scenes in film that feature polygamy life that is not tell in the novel, while AAC'S novel more consist of the struggle of an Indonesian college student that study at Egypt there with his love story.

Keywords: ecranization, novel and film, struggle of an Indonesian college student, polygamy
Karakter Masysrakat Madura dalam Syair-Syair Lagu Daerah Madura
Authors: Azhar Iqbal Nurul 
Published: April 2017

Lagu dan syair Madura merupakan salah satu wujud kebudayaan masyarakat Madura. Sayangnya, faktor keterbatasan pemahaman tcntang syair lagu Madura menjadikan syair-syair itu kurang bermakna. Akibatnya, masyarakat. Madura kurang bisa menghargai syair-syair tersebut dan hanya menempatkannya sebagai karya budaya yang tidak memiliki peran signifikan dalam membangun masyarakat Madura. Padahal apabila dikaji lebih jauh, syair- syair dalam lagu-lagu Madura memiliki makna yang dalam karena mampu memberikan gambaran tentang jati diri masyarakat dan simbol-simbol sosial mcrcka yang dapat dipakai sebagai acuan dan pegangan hidup. Artikel ini berusaha memberikan gambaran tcntang jari diri masyarakat Madura yang tergambar dalam syair-syair lagu Madura.

Abstract
Madurese traditional songs and the traditional songs' lyrics are two of Madurese cultures. But, because Madurese people lack understanding of the Madurese Lyrics values, this makes the lyrics meaningless. Because of that, Madurese pay little attentions to the lyrics and consider them as ordinary cultural works which play no role towards their society. In fact, when they study further the values behind the lyrics, they will realize that, actually, the lyrics contain a lot of wisdoms and are able to give them a picture that shows them who they really are. This picture can become a form of guidance in their society. This article informs the reader the truth portrait about the real Madurese characters that are reflected from Madurese traditional songs' lyrics.

Keywords: traditional songs' lyrics, Madurese, life characters
Safety of Annona muricata Extract Supplementation for Colorectal Cancer Patients
Authors: Indrawati Lili , Purwantyastuti Purwantyastuti , Abdullah Murdani , Surono Ingrid S , Basir Ibrahim 
Published: April 2017

Background: People have used Annona muricata leaves traditionally as tea drinks. Traditional use of A. muricata leaves is as an infusion which is closed to water extract. The potential health benefit of A. muricata tea leaves that is traditionally used for maintaining health which lately is being used by cancer patients. Therefore it is urgent to verify the safety of A. muricata leaves extract. Method: A randomized double blind placebo controlled trial was conducted on 30 colorectal cancer out patients who had undergone primary tumor resection. Twenty eight subjects completed the study, divided into two groups, namely ethanol-soluble fraction of A. muricata leaves water extract (ESFAM) (n = 14), and placebo (n = 14) for 8 weeks. Peripheral blood samples were withdrawn from subjects by venipuncture at baseline and at the end of the study period.Results: The effect on bone marrow can be considered to be safe. The measure in indices of organs function, i.e liver and kidney also showed similar results and within normal range after supplementation. The dose given to the subjects is safe and highly tolerable, as shown by very few (6.7%) of patients complained intolerable adverse effects. Conclusion: This study indicates the safety of ESFAM supplementation.
Serologic and Urine Diagnostic Tests to Detect Helicobacter pylori Infection in Functional Dyspepsia Patients
Authors: Wardhana Agasjtya Wisjnu , Syam Ari Fahrial , Sanityoso Andri , Rumende Cleopas Martin 
Published: April 2017

Background: Dyspepsia is a collection of symptoms in the forms of discomfort, pain, nausea, vomiting, bloating, and early satiety in the stomach. This condition can be caused by various problems; one of them is Helicobacter pylori infection. Dyspepsia without organic problem is known as functional dyspepsia. H. pylori examination is recommended in functional dyspepsia patients.Method: In this study, we performed a diagnostic test study in dyspepsia patients in Community Health Centre of Koja District, North Jakarta, from February to April 2015. Samples were obtained through consecutive sampling method; 74 patients were included. The data was gathered by distributing questionnaires to patients, performing urea breath test (UBT) examination, serologic test, and urine test using rapid urine test (RAPIRUN). Results: Prevalence of H. pylori infection by using UBT examination reached up to 36.5%; meanwhile serologic and RAPIRUN tests showed positive results in 32.4% and 24.3% patients, respectively. Serologic test has sensitivity of 74% (95% CI: 55-87%), specificity 91% (95% CI: 80-97%), positive predictive value (PPV) 83% (95% CI: 64-93%), and negative predictive value (NPV) 86% (95% CI: 74-93%). Meanwhile, RAPIRUN has sensitivity of 63% (95% CI: 44-78%), specificity 98% (95% CI: 89-100%), PPV 94% (95% CI: 74-99%), and NPV 82% (95% CI: 70-90%).Conclusion: Sensitivity of serologic and RAPIRUN tests are still inadequate to be alternative to UBT examination. However, they have high specificity. Further studies are required with larger sample size and consideration of factors which may influence the results of both tests.
Accurate Recovery of H i Velocity Dispersion from Radio Interferometers
Authors: Ianjamasimanana R. , Blok W. J. G. de , Heald George H. 
Published: April 2017

Abstract
Gas velocity dispersion measures the amount of disordered motion of a rotating disk. Accurate estimates of this parameter are of the utmost importance because the parameter is directly linked to disk stability and star formation. A global measure of the gas velocity dispersion can be inferred from the width of the atomic hydrogen (H i) 21 cm line. We explore how several systematic effects involved in the production of H i cubes affect the estimate of H i velocity dispersion. We do so by comparing the H i velocity dispersion derived from different types of data cubes provided by The H i Nearby Galaxy Survey. We find that residual-scaled cubes best recover the H i velocity dispersion, independent of the weighting scheme used and for a large range of signal-to-noise ratio. For H i observations, where the dirty beam is substantially different from a Gaussian, the velocity dispersion values are overestimated unless the cubes are cleaned close to (e.g., ∼1.5 times) the noise level.
Observations of Binary Stars with the Differential Speckle Survey Instrument. VII. Measures from 2010 September to 2012 February at the WIYN Telescope
Authors: Horch Elliott P. , Casetti-Dinescu Dana I. , Camarata Matthew A. , Bidarian Akbar , Altena William F. van , Sherry William H. , Everett Mark E. , Howell Steve B. , Ciardi David R. , Henry Todd J. , Nusdeo Daniel A. , Winters Jennifer G. 
Published: April 2017

Abstract
We report on speckle observations of binary stars carried out at the WIYN Telescope over the period from 2010 September through 2012 February, providing relative astrometry for 2521 observations of 883 objects, 856 of which are double stars and 27 of which are triples. The separations measured span a range of 0.01–1.75 arcsec. Wavelengths of 562, 692, and 880 nm were used, and differential photometry at one or more of these wavelengths is presented in most cases. 66 components were resolved for the first time. We also estimate detection limits at 0.2 and 1.0 arcsec for high-quality observations in cases where no companion was seen, a total of 176 additional objects. Detection limits vary based on observing conditions and signal-to-noise ratio, but are approximately 4 mag at 0.2 arcsec and 6 mag at 1.0 arcsec on average. Analyzing the measurement precision of the data set, we find that the individual separations obtained have linear measurement uncertainties of approximately 2 mas, and photometry is uncertain to approximately 0.1 mag in general. This work provides fundamental, well-calibrated data for future orbit and mass determinations, and we present three first orbits and total mass estimates of nearby K-dwarf systems as examples of this potential.
Radiative Grain Alignment in Protoplanetary Disks: Implications for Polarimetric Observations
Authors: Tazaki Ryo , Lazarian Alexandre , Nomura Hideko 
Published: April 2017

Abstract
We apply the theory of radiative torque (RAT) alignment for studying protoplanetary disks around a T-Tauri star and perform 3D radiative transfer calculations to provide the expected maps of polarized radiation to be compared with observations, such as with ALMA. We revisit the issue of grain alignment for large grains expected in the protoplanetary disks and find that mm-sized grains at the midplane do not align with the magnetic field since the Larmor precession timescale for such large grains becomes longer than the gaseous damping timescale. Hence, for these grains the RAT theory predicts that the alignment axis is determined by the grain precession with respect to the radiative flux. As a result, we expect that the polarization will be in the azimuthal direction for a face-on disk. It is also shown that if dust grains have superparamagnetic inclusions, magnetic field alignment is possible for (sub-)micron grains at the surface layer of disks, and this can be tested by mid-infrared polarimetric observations.
The SCUBA-2 Cosmology Legacy Survey: Multi-wavelength Properties of ALMA-identified Submillimeter Galaxies in UKIDSS UDS
Authors: Simpson J. M. , Smail Ian , Swinbank A. M. , Ivison R. J. , Dunlop J. S. , Geach J. E. , Almaini O. , Arumugam V. , Bremer M. N. , Chen Chian-Chou , Conselice C. , Coppin K. E. K. , Farrah D. , Ibar E. , Hartley W. G. , Ma C. J. , Michałowski M. J. , Scott D. , Spaans M. , Thomson A. P. , Werf P. P. van der 
Published: April 2017

Abstract
We present a multi-wavelength analysis of 52 submillimeter galaxies (SMGs), identified using ALMA 870 μm continuum imaging in a pilot program to precisely locate bright SCUBA-2-selected submillimeter sources in the UKIDSS Ultra Deep Survey (UDS) field. Using the available deep (especially near-infrared) panoramic imaging of the UDS field at optical-to-radio wavelengths we characterize key properties of the SMG population. The median photometric redshift of the bright ALMA/SCUBA-2 UDS (AS2UDS) SMGs that are detected in a sufficient number of wavebands to derive a robust photometric redshift is z = 2.65 ± 0.13. However, similar to previous studies, 27% of the SMGs are too faint at optical-to-near-infrared wavelengths to derive a reliable photometric redshift. Assuming that these SMGs lie at z ≳ 3 raises the median redshift of the full sample to z = 2.9 ± 0.2. A subset of 23 unlensed, bright AS2UDS SMGs have sizes measured from resolved imaging of their rest-frame far-infrared emission. We show that the extent and luminosity of the far-infrared emission are consistent with the dust emission arising from regions that are, on average, optically thick at a wavelength of

(1σ dispersion of 55–90 μm). Using the dust masses derived from our optically thick spectral energy distribution models, we determine that these galaxies have a median hydrogen column density of N
H = 9.8

× 1023 cm−2, or a corresponding median V-band obscuration of A
v = 540

mag, averaged along the line of sight to the source of their rest-frame ∼200 μm emission. We discuss the implications of this extreme attenuation by dust for the multi-wavelength study of dusty starbursts and reddening-sensitive tracers of star formation.
Radiation Hydrodynamic Simulations of Dust-driven Winds
Authors: Zhang Dong , Davis Shane W. 
Published: April 2017

Abstract
We study dusty winds driven by radiation pressure in the atmosphere of a rapidly star-forming environment. We apply the variable Eddington tensor algorithm to re-examine the two-dimensional radiation hydrodynamic problem of a column of gas that is accelerated by a constant infrared radiation flux. In the absence of gravity, the system is primarily characterized by the initial optical depth of the gas. We perform several runs with different initial optical depths and resolutions. We find that the gas spreads out along the vertical direction, as its mean velocity and velocity dispersion increase. In contrast to previous work using the flux-limited diffusion algorithm, we find little evolution in the trapping factor. The momentum coupling between radiation and gas in the absence of gravity is similar to that with gravity. For Eddington ratio increasing with the height in the system, the momentum transfer from the radiation to the gas is not merely

, but amplified by a factor of

, where

is the integrated infrared optical depth through the system, and

, decreasing with the optical depth. We apply our results to the atmosphere of galaxies and conclude that radiation pressure may be an important mechanism for driving winds in the most rapidly star-forming galaxies and starbursts.
Accurate Orbital Solution for the New and Metal-poor Eclipsing Binary Tycho 5227-1023-1
Authors: Traven G. , Munari U. , Dallaporta S. , Zwitter T. 
Published: April 2017

Abstract
The orbit and physical parameters of the previously unsolved double-lined eclipsing binary Tyc 5227-1023-1, discovered during the search for RR Lyr variable candidate members of the Aquarius stream, are derived using high-resolution échelle spectroscopy and

photometry. A synthetic spectral analysis of both components has been performed, yielding metallicity [M/H] = −0.63 ± 0.11 for both stars and a temperature for the secondary that is in close agreement with the one from the orbital solution, while the temperature of the primary is determined from photometry (

). The masses and radii (

) reveal that both stars have already slightly evolved away from the main-sequence band, having an age of about 7 Gyr, and the results of the synthetic spectral analysis support the claim of corotation with the orbital motion. The radial velocity of the system is

, while its distance, computed from orbital parameters and the derived reddening

, is 496 ± 35 pc. Even though Tyc 5227-1023-1 was initially treated as a possible member of the Aquarius stream, the results presented here disagree with reported values for this ancient structure and suggest a likely membership of the thick disk.
Intraocular Pressure After Implantation of a Phakic Collamer Intraocular Lens With a Central Hole
Authors: Rodríguez-Una Ignacio , Rodríguez-Calvo Pedro Pablo , Cueto Luis Fernández-Vega , Lisa Carlos , Cueto Andrés Fernández-Vega , Alfonso José F. 
Published: April 2017

PURPOSE:
To investigate the middle-term intraocular pressure (IOP) results after implantation of a posterior chamber collagen copolymer phakic intraocular lens (IOL) (V4c Visian; STAAR Surgical Co., Nidau, Switzerland) with a central hole in patients with myopia.

METHODS:
This retrospective study enrolled patients who had implantation of a phakic IOL with a central hole. IOP, central vault, and adverse events were evaluated 1, 3, 6, 12, and 24 months postoperatively.

RESULTS:
The study enrolled 763 eyes (384 patients, 128 men and 256 women). Mean follow-up was 7.0 ± 7.2 months (range: 1 to 24 months). The mean IOP was 13.2 ± 2.1 mm Hg preoperatively. Postoperatively, the mean IOP was 12.4 ± 1.7 mm Hg at 1 month, 12.5 ± 1.8 mm Hg at 3 months, 12.6 ± 1.3 mm Hg at 6 months, 12.6 ± 1.4 mm Hg at 12 months, and 12.7 ± 1.1 mm Hg at 24 months. Only one case (0.13%) presented an increased IOP (> 21 mm Hg) during the observation period. No pupillary block or acute angle closure was recorded. IOP at the final follow-up visit was 12.8 ± 1.3 mm Hg.

CONCLUSIONS:
Implantation of central hole phakic IOL in myopic patients provided good and safe IOP outcomes throughout the 24-month observation period.

[
J Refract Surg.
2017;33(4):244–249.]
Megeremaeus cretaceousnew species (Acari: Oribatida), the first oribatid mite from Canadian amber
Authors: Sidorchuk Ekaterina A. , Behan-Pelletier Valerie M. 
Published: April 2017

AbstractCanadian Cretaceous amber belongs to the Taber Coal Zone, and was deposited in beds of coal and shale saturated with organic matter. It is upper Campanian (~76–72 million years ago), and the source of the original resin is predominantly the plant genusParataxodiumArnold and Lowther (Cupressaceae). We describe the first oribatid mite from this amber,Megeremaeus cretaceousnew species(Acari: Oribatida: Megeremaeidae). We provide a key to all described species ofMegeremaeusHiggins and Woolley, 1965, and discuss the advantages that confocal microscopy provides for the study of dark, resin-filled, miniature amber inclusions.
Mucosal IgM Antibody with d-Mannose Affinity in Fugu Takifugu rubripes Is Utilized by a Monogenean Parasite Heterobothrium okamotoi for Host Recognition
Authors: Igarashi Kento , Matsunaga Ryohei , Hirakawa Sachi , Hosoya Sho , Suetake Hiroaki , Kikuchi Kiyoshi , Suzuki Yuzuru , Nakamura Osamu , Miyadai Toshiaki , Tasumi Satoshi , Tsutsui Shigeyuki 
Published: April 2017

Abstract
How parasites recognize their definitive hosts is a mystery; however, parasitism is reportedly initiated by recognition of certain molecules on host surfaces. Fish ectoparasites make initial contact with their hosts at body surfaces, such as skin and gills, which are covered with mucosa that are similar to those of mammalian guts. Fish are among the most primitive vertebrates with immune systems that are equivalent to those in mammals, and they produce and secrete IgM into mucus. In this study, we showed that the monogenean parasite Heterobothrium okamotoi utilizes IgM to recognize its host, fugu Takifugu rubripes. Oncomiracidia are infective larvae of H. okamotoi that shed their cilia and metamorphose into juveniles when exposed to purified d-mannose–binding fractions from fugu mucus. Using liquid chromatography–tandem mass spectrometry analysis, proteins contained in the fraction were identified as d-mannose–specific IgM with two d-mannose–binding lectins. However, although deciliation was significantly induced by IgM and was inhibited by d-mannose or a specific Ab against fugu IgM, other lectins had no effect, and IgM without d-mannose affinity induced deciliation to a limited degree. Subsequent immunofluorescent staining experiments showed that fugu d-mannose–specific IgM binds ciliated epidermal cells of oncomiracidium. These observations suggest that deciliation is triggered by binding of fugu IgM to cell surface Ags via Ag binding sites. Moreover, concentrations of d-mannose–binding IgM in gill mucus were sufficient to induce deciliation in vitro, indicating that H. okamotoi parasites initially use host Abs to colonize host gills.
Assessment of heavy metal contamination in sub-tropical riverine sediments using geoaccumulation index
Authors: Silva Patrícia Pedreira da , Santos Leila Thaise Santana de Oliveira , Jesus Taise Bomfim de 
Published: April 2017

Heavy metal determination in surface sediment allows pollutant assessment when the detection in the water column is not possible. Geoaccumulation Index (Igeo) and the Sediment Quality Guidelines (SQGs) were used to quantitatively evaluate the degree of heavy metal contamination in fluvial sediments. Both of these methods had already been used by several authors and the generated indexes allowed a good comparison parameter. In the present study, heavy metal in sediments (Mn, Zn, Cd, Cr, Cu, Pb and Ni) were analyzed in 14 sampling points, distributed in the upper watercourse of Subaé river, Feira de Santana – BA, in two field campaigns in order to compare dry and wet seasons. The quantification of heavy metal contents was measured by flame atomic absorption spectrometer. The heavy metal levels in the sampling points were low when compared to the global reference values for world sediments. Cadmium concentrations were always below the detection limit of the used spectrometer, and the relative abundance of the studied metals was the following: Mn>Zn>Pb>Cu>Cr>Ni. The variation range of each element concentrations was: Mn 69.3 and 266 mg Kg-1; Zn 30.7 and 426 mg Kg-1; Pb 6.00 and 63.6 mg Kg-1; Cu 4.26 and 66.2 mg Kg-1; Cr 3.24 and 52.9 mg Kg-1; Ni 1.96 and 24.7 mg Kg-1. These results are indicating low contamination risk to biota, despite of the fact that some points presented moderate risk of toxicity. The Igeo ranged from unpolluted (Zn, Mn, Cr, and Ni) to slightly polluted (Pb and Cu) in the assessed sediments. The different approaches to geochemical information treatment allow a wide and coherent debate about the environmental risk of heavy metals from anthropogenic diffuse sources.