bluuebunny/crossref_metadata_2025_split huggingface dataset:
Pengaruh Pendidikan Kesehatan Tentang Latihan Range of Motion (ROM) Terhadap Keterampilan Keluarga Dalam Melakukan ROM Pada Pasien Stroke Di Bangsal Syaraf RSUP Dr M.Jamil Padang Tahun 2013
Authors: Agonwardi Agonwardi , Budi Hendri 
Published: March 2017

<p><em>Pasien stroke membutuhkan latihan ROM akibat kelemahan atau kelumpuhan yang dialami. Dari survei awal 10 orang keluarga pasien stroke yang di wawancarai di bangsal bedah saraf, (100%) mengatakan tidak bisa melakukan ROM. Hasil wawancarai 3 dari 5 perawat didapatkan bahwa perawat mengajarkan keluarga hanya dalam tahap mobilisasi miring kiri dan kanan.Tujuan penelitian u</em><em>ntuk mengetahui </em><em>pengaruh pendidikan kesehatan tentang ROM </em><em> terhadap ketrampilan keluarga dalam melakukan latihan ROM </em><em>di bangsal saraf RSUP Dr. M. Djamil Padang</em><em> tahun 2013</em><em>.</em><em> </em><em>Penelitian </em><em>dimulai bulan Mei sampai November 2013 m</em><em>enggunakan desain quasi-eksperimen rancangan one group pre-post test dengan intervensi pendidikan kesehatan tentang </em><em>latihan </em><em>ROM. </em><em>Populasi </em><em>seluruh </em><em>keluarga </em><em>pasien </em><em>stroke</em><em>.</em><em> </em><em>Sampel </em><em>berjumlah 15 orang</em><em>.</em><em> Analisis </em><em>data </em><em>secara univariat dan bivariat</em><em>, analisis secara bivariat </em><em>menggunakan uji </em><em>Wilcoxon.</em><em>.</em><em> </em><em>Hasil penelitian keterampilan rata-rata sebelum melakukan pendidikan ROM mempunyai skor 16,27. Setelah dilakukan skor menjadi 77,67. Pendidikan kesehatan tentang latihan ROM berpengaruh terhadap keterampilan keluarga yang dilakukan di RSUP Dr.Mdjamil tahun 2013 ( nilai P = 0,001) . Disarankan kepada kepala ruangan rawat inap bangsal saraf RSUP Dr.Mdjamil Padang dapat menjadikan pendidikan latihan ROM sebagai salah satu intervensi didalam pemberian pelyanan asuhan keperawatan dan pendidikan kesehatan tentang ROM sebagai protap dan standar asuhan keperawatan pasien stroke dan keluarganya.</em></p>
PERENCANAAN STRATEGIS SISTEM INFORMASI (Studi kasus : LEMIGAS)
Authors: Siswipraptini Puji Catur 
Published: March 2017

Perencanaaan Strategis Sistem Informasi menjadi begitu penting ketika isu competitive advantage dan pencapaian target LEMIGAS menjadi fokus bagi manajemen organisasi. LEMIGAS sebagai institusi pemerintah yang bergerak di bidang penelitian dan pengembangan (litbang) kemigasan merasa perlu mengimplementasikan sistem informasi yang baik dengan tujuan untuk meningkatkan efisiensi, efektivitas, dan produktivitas organisasi. Selain itu, kurangnya integrasi data di organisasi, prioritas pengadaan Teknologi Informasi (TI) yang tidak berdasarkan kebutuhan bisnis, serta strategi teknologi yang tidak selaras menjadi isu yang mendasari kebutuhan LEMIGAS akan perencanaan strategis Sistem Informasi/Teknologi Informasi (SI/TI). Tulisan ini dibuat agar dapat menghasilkan suatu usulan Perencanaan Strategis Sistem Informasi bagi LEMIGAS yang mendukung rencana strategis (strategic plan) dan rencana bisnis (business plan) mereka. Deliverables dari proses ini adalah strategi manajemen SI/TI (IS/IT management Strategy), strategi SI bisnis (business IS strategy), dan strategi TI (IT strategy). Manajemen Strategi SI/TI mencakup usulan struktur organisasi unit TI yang baru dan beberapa prinsip penerapan TI. Sedangkan strategi SI bisnis (business IS strategy) berisi usulan aplikasi-aplikasi yang sebaiknya diimplementasikan. Selanjutnya, strategi TI menjelaskan rencana inftrastruktur TI dan strategi implementasi IS/IT di LEMIGAS.
EFFECTS OF THE INQUIRY TRAINING AND MOTIVATION LEARNING AGAINST LEARNING OUTCOMES IN HIGH SCHOOL PHYSICS STUDENTS
Authors: Andini Vika 
Published: March 2017

This study aims to: determine the significance of differences in physics learning outcomes of students with learning models Inquiry Training and conventional models, knowing the significance of differences in physics learning outcomes of students who have learning motivation high and low, low motivation, the interaction model of learning and motivation to learn physics in improving student learning outcomes. The sample in this study conducted in a cluster random sampling of two classes, where the first class as a class experiment applied learning models and Inquiry Training as a second grade class learning model Conventional control applied. The instrument used in this study is the result of learning physics instruments in the form of 20 multiple-choice questions and motivation questionnaire by 25 statements has been declared valid and reliable. From the results of this study concluded that the learning outcomes of students who are taught by Training Inquiry learning model is better than conventional models of learning outcomes. Learning outcomes of students who have high motivation to learn is better than the learning outcomes of students who have a low learning motivation. Inquiry learning model training and motivation interact in affecting student learning outcomes.
ANALISIS PENGARUH MODEL PEMBELAJARAN PROBLEM SOLVING DAN SIKAP ILMIAH TERHADAP HASIL BELAJAR FISIKA
Authors: Purwanti Sri , Manurung Sondang 
Published: March 2017

Penelitian ini bertujuan: Untuk mengetahui apakah ada perbedaanhasil belajar fisika siswa yang diajarkan menggunakan model pembelajaranProblem Solving dengan yang diajarkan menggunakan model pembelajaranDirect Instruction, untuk mengetahui apakah ada perbedaan hasil belajarfisika siswa yang memiliki sikap ilmiah rendah dan sikap ilmiah tinggi,untuk mengetahui apakah ada Interaksi antara model pembelajaran ProblemSolving dengan tingkat sikap ilmiah siswa dalam mempengaruhi hasilbelajar siswa. Sampel dalam penelitian ini dilakukan secara cluster randomsampling sebanyak dua kelas, dimana kelas pertama sebagai kelas eksperimen diterapkan model pembelajaran Problem Solving dan kelas keduasebagai kelas kontrol diterapkan model pembelajaran Direct Instruction.Instrumen yang digunakan dalam penelitian ini yaitu instrumen tes hasilbelajar fisika dalam bentuk uraian sebanyak 8 soal dan insrumen angketsikap ilmiah sebanyak 22 soal yang telah dinyatakan valid dan reliabel. Darihasil penelitian dapat disimpulkan bahwa terdapat perbedaan hasil belajarfisika siswa dengan model pembelajaran Problem Solving dan modelpembelajaran Direct Instruction. Terdapat perbedaan hasil belajar fisikaantara sikap ilmiah rendah dan sikap ilmiah tinggi. Terdapat interaksi antaramodel pembelajaran Problem Solving dengan sikap ilmiah siswa dalammempengaruhi hasil belajar siswa. Kata kunci: problem solving, sikap ilmiah, hasil belajar
THE INFLUENCE LEARNING MODEL GUIDED INQUIRY AND CREATIVITY ON HIGHER COGNITIVE
Authors: T. M. Ambarita Pretti , . Sahyar , A.Sani Ridwan 
Published: March 2017

The objective of this research were to produce a lesson plans and worksheets learning instrument design that corresponded to problem based learning models and analyze whether it was can improve student learning outcomes. This research development was done in classroom by using development research methods of Analysis Design Development Implementation and Evaluation (ADDIE). ADDIE method was used as a method for designing a lesson plans and worksheets that corresponded to it. Three stages of development of lesson plans and worksheets such as an assessment by a team of experts, small group, and a field test. Assessment by a team of experts based on theree aspects such as format, content, and language. In small group and field test based on a response of students sheet. The student response sheet contains of teacher's ability to teach. Worksheet assessment based on aspects of the format, content, and language. Assessment of student learning outcomes based on pretest and posttest were analyzed by ngain. The results of development of lesson plans and worksheets were validated by a team of experts on aspects of format, content, and language. The result both of development of lesson plans and worksheets in small group and field test produced good categories. There was an increased student learning outcomes of first to third meeting with categories of low to moderate.
IDENTIFIKASI KAPANG PADA KECAP KEDELAI MANIS PRODUKSI LOKAL KEDIRI DENGAN METODE PENGENCERAN
Authors: Humairoh Durroh 
Published: March 2017

Kecap kedelai merupakan salah satu produk fermentasi yang telah dikenal sejak ribuan tahun yang lalu di berbagai negara termasuk Indonesia. Namun kecap kedelai manis merupakan produk kecap kedelai yang merupakan produk khas Indonesia. Faktor keamanan pangan berkaitan dengan tercemar tidaknya pangan oleh cemaran mikrobiologis, logam berat, dan bahan kimia yang membahayakan kesehatan. Tujuan penelitian ini adalah untuk mengetahui jumlah kapang dan jenis kapang yang ditemukan pada sampel kecap produk lokal Kediri. Penelitian ini menggunakan metode pengenceran hingga 101 dari 10 sampel kecap kedelai manis produksi lokal Kediri dengan merek yang berbeda. Hasil pengamatan menunjukkan bahwa pada sampel kecap kedelai manis ditemukan jumlah kapang sebanyak < 50 koloni/ml pada setiap sampelnya dan jenis kapang yang ditemukan meliputi Penicillium sp., Aspergillus sp., Rhizopus sp., dan Mucor sp. sehingga dapat disimpulkan bahwa kecap produksi Kediri aman dikonsumsi karena sesuai standar yang ditetapkan Pemerintah dalam SNI 3543: 2013.Â Kata kunci: Jumlah koloni, Jenis kapang, Kecap kedelai manis, produk lokal Kediri
Fish Tales: Local fishing in the Kingdom of Tonga
Authors: Brown Pulu Teena 
Published: March 2017

In the small island developing state of Tonga, an archipelago of 176 coral atolls scattered across 664,853 square kilometres of the South Pacific Ocean, power and resourcing differentials dictate which people are permitted to be commercial fishermen and what groups do the subsistence kind, customary fishing. A handful of Native Tongans engage in commercial exporting. The tuna industry is dominated by foreign vessels, by foreign countries, that can afford the state fishing license and the operation costs.
The Government of Tonga has confined coastal communities to customary fishing as the sustainable development model, a solution beset with tension. There is resource scarcity of inshore fishing stock. When local fishermen are denied access to deep sea commercial fishing their chances at exporting and making profit are limited, tempting some to poach undersized stock and pressure the government to remove conservation sanctions on species at risk of depletion. What options for livelihood from the sea do coastal communities have? Related to this, what tensions emerge between the Tongan state and coastal communities wanting to be included in the commercial fishing industry?
Who’s Who in the Zoo: Tonga Election 2014
Authors: Brown Pulu Teena , Pamatatau Richard 
Published: March 2017

This paper reflects on fieldwork Teena Brown Pulu and Richard Pamatatau conducted in Tonga on the people’s election and the nobles’ election of November 27th 2014. Who’s who in the zoo?[i] Ethnographically speaking we mean what did voters say of the leadership and government needed, and the country’s priorities for moving forward? Furthermore, how was Tongan “life, liberty and security” made sense of? (United Nations, 1948). With Democratic Party leader ‘Akilisi Pohiva elected prime minister for the 2014 to 2018 term of government, what was different now?
Written by Teena Brown Pulu with Richard Pamatatau’s fieldwork notes woven in the text, the essay probes two critical interstices. Why do ethnic Tongans insist the authors can critique Tongan politics and society in ways they cannot for risk they will be rebuked by established canons exerting authority and control over citizens? Who then in Tonga can disrupt the taken for granted categories of class, culture, and politics, and who cannot?
Endnotes
[i] Who’s who in the zoo is Richard Pamatatau’s Master of Philosophy thesis title at Auckland University of Technology. Richard’s thesis investigates how New Zealand social pages in traditional media, e.g. the weekend pages of The New Zealand Herald newspaper, select, rank, and frame the who’s who of public celebrities.
The suckling pig chronicles Kolonga day in Auckland
Authors: Brown Teena , Pamatatau Richard 
Published: March 2017

The Tongan diaspora of New Zealand, Australia, and the United States has invented the observance of village days. Auckland affiliates to Kolonga, a rural farming settlement in Tonga, held an inaugural village day on October 26th, 2015. The result generated mixed feelings. The greater part wanted Kolonga day made a regular celebration. Others thought the event could be improved. While some saw the maiden Kolonga day as chaos, which should be reworked to resemble a function less costly and showy, and more down-to-earth and practical. Why have Tongan village days taken off in diaspora, and will they continue to be bankrolled by generations born overseas?
Peritonitis as the First Presentation of Disseminated Listeriosis in a Patient on Peritoneal Dialysis—a Case Report
Authors: Beckerleg Weiwei , Keskar Vaibhav , Karpinski Jolanta 
Published: March 2017

Infections with Listeria monocytogenes are uncommon but serious, with mortality rate approaching 30% in cases of systemic involvement despite first-line therapy. They are usually caused by ingestion of contaminated foods, but spontaneous infections have also been described. Listeria monocytogenes is a rare cause of peritonitis, and most of the published cases are in patients with cirrhosis and ascites. There are a few reported cases of Listeria peritonitis associated with peritoneal dialysis (PD), primarily isolated peritonitis. If detected early, Listeria peritonitis can be successfully treated with ampicillin, alone or in combination with gentamicin. Vancomycin has been listed as a second-line agent. However, it has been associated with treatment failure. In this case report, we present a patient who developed disseminated listeriosis, with peritonitis as the first manifestation of disseminated infection. This case illustrates the importance of having a high index of suspicion for L. monocytogenes if patients deteriorate despite empiric therapy for PD-associated peritonitis and serves as a further example demonstrating the inadequate coverage of vancomycin for L. monocytogenes.
The 2.4 μm Galaxy Luminosity Function As Measured Using WISE. I. Measurement Techniques
Authors: Lake S. E. , Wright E. L. , Tsai C.-W. , Lam A. 
Published: March 2017

Abstract
The astronomy community has at its disposal a large back catalog of public spectroscopic galaxy redshift surveys that can be used for the measurement of luminosity functions (LFs). Utilizing the back catalog with new photometric surveys to maximum efficiency requires modeling the color selection bias imposed on the selection of target galaxies by flux limits at multiple wavelengths. The likelihood derived herein can address, in principle, all possible color selection biases through the use of a generalization of the LF,

, over the space of all spectra: the spectro-luminosity functional,

. It is, therefore, the first estimator capable of simultaneously analyzing multiple redshift surveys in a consistent way. We also propose a new way of parametrizing the evolution of the classic Schechter function parameters, L
⋆ and ϕ
⋆, that improves both the physical realism and statistical performance of the model. The techniques derived in this paper are used in a companion paper by Lake et al. to measure the LF of galaxies at the rest-frame wavelength of

using the Widefield Infrared Survey Explorer (WISE).
Observing Exoplanets with High Dispersion Coronagraphy. I. The Scientific Potential of Current and Next-generation Large Ground and Space Telescopes
Authors: Wang Ji , Mawet Dimitri , Ruane Garreth , Hu Renyu , Benneke Björn 
Published: March 2017

Abstract
Direct imaging of exoplanets presents a formidable technical challenge owing to the small angular separation and high contrast between exoplanets and their host stars. High Dispersion Coronagraphy (HDC) is a pathway to achieve unprecedented sensitivity to Earth-like planets in the habitable zone. Here, we present a framework to simulate HDC observations and data analyses. The goal of these simulations is to perform a detailed analysis of the trade-off between raw star light suppression and spectral resolution for various instrument configurations, target types, and science cases. We predict the performance of an HDC instrument at Keck observatory for characterizing directly imaged gas-giant planets in near-infrared bands. We also simulate HDC observations of an Earth-like planet using next-generation ground-based (TMT) and spaced-base telescopes (HabEx and LUVOIR). We conclude that ground-based ELTs are more suitable for HDC observations of an Earth-like planet than future space-based missions owing to the considerable difference in collecting area. For ground-based telescopes, HDC observations can detect an Earth-like planet in the habitable zone around an M-dwarf star at 10−4 star light suppression level. Compared to the 10−7 planet/star contrast, HDC relaxes the star light suppression requirement by a factor of 103. For space-based telescopes, detector noise will be a major limitation at spectral resolutions higher than 104. Considering detector noise and speckle chromatic noise, R = 400 (1600) is the optimal spectral resolutions for HabEx (LUVOIR). The corresponding star light suppression requirement to detect a planet with planet/star contrast =

is relaxed by a factor of 10 (100) for HabEx (LUVOIR).
Transiting Planets with LSST. III. Detection Rate per Year of Operation
Authors: Jacklin Savannah R. , Lund Michael B. , Pepper Joshua , Stassun Keivan G. 
Published: March 2017

Abstract
The Large Synoptic Survey Telescope (LSST) will generate light curves for approximately 1 billion stars. Our previous work has demonstrated that, by the end of the LSST 10-year mission, large numbers of transiting exoplanetary systems could be recovered using the LSST “deep-drilling” cadence. Here, we extend our previous work to examine how the recoverability of transiting planets over a range of orbital periods and radii evolves per year of LSST operation. As specific example systems, we consider hot Jupiters orbiting solar-type stars and hot Neptunes orbiting K-dwarfs at distances from Earth of several kpc, as well as super-Earths orbiting nearby low-mass M-dwarfs. The detection of transiting planets increases steadily with the accumulation of data over time, generally becoming large (≳10%) after 4–6 years of operation. However, we also find that short-period (≲2 days) hot Jupiters orbiting G-dwarfs and hot Neptunes orbiting K-dwarfs can already be discovered within the first 1–2 years of LSST operation.
Imaging a Central Ionized Component, a Narrow Ring, and the CO Snowline in the Multigapped Disk of HD 169142
Authors: Macías Enrique , Anglada Guillem , Osorio Mayra , Torrelles José M. , Carrasco-González Carlos , Gómez José F. , Rodríguez Luis F. , Sierra Anibal 
Published: March 2017

Abstract
We report Very Large Array observations at 7 mm, 9 mm, and 3 cm toward the pre-transitional disk of the Herbig Ae star HD 169142. These observations have allowed us to study the millimeter emission of this disk with the highest angular resolution so far (0.″12 × 0.″09, or 14 au × 11 au, at 7 mm). Our 7 and 9 mm images show a narrow ring of emission at a radius of ∼25 au tracing the outer edge of the inner gap. This ring presents an asymmetric morphology that could be produced by dynamical interactions between the disk and forming planets. Additionally, the azimuthally averaged radial intensity profiles of the 7 and 9 mm images confirm the presence of the previously reported gap at ∼45 au and reveal a new gap at ∼85 au. We analyzed archival DCO+(3–2) and C18O(2–1) ALMA observations, showing that the CO snowline is located very close to this third outer gap. This suggests that growth and accumulation of large dust grains close to the CO snowline could be the mechanism responsible for this proposed outer gap. Finally, a compact source of emission is detected at 7 mm, 9 mm, and 3 cm toward the center of the disk. Its flux density and spectral index indicate that it is dominated by free–free emission from ionized gas, which could be associated with the photoionization of the inner disk, an independent object, or an ionized jet.
The Thermal Proximity Effect: A New Probe of the He ii Reionization History and Quasar Lifetime
Authors: Khrykin I. S. , Hennawi J. F. , McQuinn M. 
Published: March 2017

Abstract
Despite decades of effort, the timing and duration of He ii reionization and the properties of the quasars believed to drive it are still not well constrained. We present a new method to study both via the thermal proximity effect—the heating of the intergalactic medium (IGM) around quasars when their radiation doubly ionizes helium. We post-process hydrodynamical simulations with 1D radiative transfer and study how the thermal proximity effect depends on the He ii fraction,

, which prevailed in the IGM before the quasar turned on, and the quasar lifetime

. We find that the amplitude of the temperature boost in the quasar environment depends on

, with a characteristic value of

for

, whereas the size of the thermal proximity zone is sensitive to

, with typical sizes of

for

. This temperature boost increases the thermal broadening of H i absorption lines near the quasar. We introduce a new Bayesian statistical method based on measuring the Lyα forest power spectrum as a function of distance from the quasar, and demonstrate that the thermal proximity effect should be easily detectable. For a mock data set of 50 quasars at

, we predict that one can measure

to an (absolute) precision

and

to a precision of

dex. By applying our formalism to existing high-resolution Lyα forest spectra, one should be able to reconstruct the He ii reionization history, providing a global census of hard photons in the high-z universe.
Importance of Cross-redistribution in Scattering Polarization of Spectral Lines:The Cases of 3P−3S Triplets of Mg i and Ca i
Authors: Sampoorna M. , Nagendra K. N. 
Published: March 2017

Abstract
Scattering on a multi-level atomic system has dominant contributions from resonance and Raman scattering. While initial and final levels are the same for resonance scattering, they are different for Raman scattering. The frequency redistribution for resonance scattering is described by the usual partial frequency redistribution functions of Hummer, while that for Raman scattering is described by cross-redistribution (XRD) function. In the present paper, we investigate the importance of XRD on linear polarization profiles of 3P−3S triplets of Mg i and Ca i formed in an isothermal one-dimensional atmosphere. We show that XRD produces significant effects on the linear polarization profiles when the wavelength separations between the line components of the multiplet are small, like in the cases of Mg i b and Ca i triplets.
The Geometry and Origin of Ultra-diffuse Ghost Galaxies
Authors: Burkert A. 
Published: March 2017

Abstract
The geometry and intrinsic ellipticity distribution of ultra-diffuse galaxies (UDG) is determined from the line-of-sight distribution of axial ratios q of a large sample of UDGs, detected by Koda et al. in the Coma cluster. With high significance, the data rules out an oblate, disk-like geometry, characterized by major axes a = b > c. The data is, however, in good agreement with prolate shapes, corresponding to a = b < c. This indicates that UDGs are not thickened, rotating, axisymmetric disks, puffed up by violent processes. Instead, they are anisotropic elongated cigar- or bar-like structures, similar to the prolate dwarf spheroidal galaxy population of the Local Group. The intrinsic distribution of axial ratios of the Coma UDGs is flat in the range of 0.4 ≤ a/c ≤ 0.9 with a mean value of

. This might provide important constraints for theoretical models of their origin. Formation scenarios that could explain the extended prolate nature of UDGs are discussed.