bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGARUH MODEL DAN MEDIA PEMBELAJARAN TERHADAP HASIL BELAJAR KEMAMPUAN DASAR SENAM LANTAI PADA MAHASISWA JURUSAN PENJASKESREK UNDIKSHA
Authors: Kadek Yogi Parta Luh Putu Spyana Wati 
Published: February 2017

Penelitian ini bertujuan (1) menjelaskan perbedaan hasil belajar kemampuan dasar senam lantai yang signifikan antara model pembelajaran Think-Pair-Share (TPS) dengan model pembelajaran Student Teams-Achievement Devision (STAD). (2) menjelaskan perbedaan hasil belajar kemampuan dasar senam lantai antara mahasiswa yang belajar dengan media VCD dan media gambar. (3) menjelaskan pengaruh interaktif antara model dan media pembelajaran terhadap hasil belajar. Penelitian ini adalah penelitian eksperimen semu (quasi experiment) menggunakan pretest-posttest non-equivalent control group design. Populasi penelitian berjumlah 6 kelas yang terdiri dari 156 mahasiswa. Sampel diambil 4 kelas dengan cara simple random sampling. Data dikumpulkan dengan tes hasil belajar dan dianalisis dengan ANACOVA faktorial 2×2. Hasil penelitian menunjukkan bahwa, (1) terdapat perbedaan hasil belajar kemampuan dasar senam lantai yang signifikan antara model pembelajaran Think-Pair-Share (TPS) dengan model pembelajaran Student Teams-Achievement Devision (STAD) (F = 64.805; p<0.05), dimana hasil belajar kemampuan dasar senam lantai pada mahasiswa yang mengikuti model pembelajaran Think-Pair-Share (TPS) lebih baik dibandingkan dengan mahasiswa yang mengikuti model pembelajaran Student Teams-Achievement Devision (STAD), (2) terdapat perbedaan hasil belajar yang signifikan antara media pembelajaran VCD dengan media pembelajaran gambar terbukti pada nilai (F= 52.577; p<0.05), (3) terdapat pengaruh interaktif antara media dan model pembelajaran terhadap hasil belajar kemampuan dasar senam lantai terbukti pada nilai (F= 88.185; p<0.005).
WORKING SHIFT DIFFERENCES AND THEIR EFFECTS ON EMPLOYEESâ€™ JOB FATIGUE LEVELS: AN EMPIRICAL EVIDENCE FROM HOTEL INDUSTRY IN SURABAYA
Authors: Alvionita Ch Priscillia , Angelina T Frederica , Wijaya Serli 
Published: February 2017

Bisnis pada sektor jasa memiliki keunikan tersendiri dalam pengelolaan karyawannya. Pembagian jamÂ kerja yang sesuai menentukan tingkat kualitas dari bisnis tersebut. Studi ini meneliti pengaruh perbedaanÂ shift kerja terhadap tingkat kelelahan karyawan pada industri perhotelan di Surabaya. Metode penelitian yangÂ digunakan adalah ANOVA. Hasil analisis memperlihatkan bahwa responden yang bekerja pada shift pagi danÂ siang menunjukkan tingkat kelelahan kerja yang berbeda secara signifikan dibandingkan dengan merekayang bekerja pada shift malam, khususnya dalam hal kelelahan emosional, kelelahan umum dan kelelahanÂ keterampilan.Kata Kunci: shift kerja, kelelahan kerja, hotel, Surabaya.
ANALISIS JUMLAH KENDARAAN BERMOTOR DI DAERAH ISTIMEWA YOGYAKARTA (1990â€“2012)
Authors: Wantara I Agus 
Published: February 2017

In the last few years, traffic congestions are often occurred in Yogyakarta. This situation is caused byÂ the increasing number of vehicles in Yogyakarta.This study evaluates the effect of the gross regional domesticproduct (PDRB), the people of Daerah Istimewa Yogyakarta (JP), and region income (PD) to the number ofÂ vehicles in Daerah Istimewa Yogyakarta (JKB). The model consists of one behavioral equation: the numberÂ of vehicles equation. The estimation technique uses Ordinary Least Squares (OLS). MacKinnon, White, andÂ Davidson test (MWD test) is used to choose between the two models: linear regression model or log-linearregression model.The sample covers observations for 23 years (1990 - 2012). The data are obtained from (1)Â Bank Indonesia (2) Badan Pusat Statistik DIY and various other sources. It is found that individually lnJP andlnPD are statistically significant (positive) except ln PDRB on the basis of (separate) t test. It is also found that onÂ the basis of the F test collectively all the regressors have a significant effect on the regressand lnJKB.Keywords: the number of vehicles, traffic congestion, linear regression model, log-linear regression model.
DAMPAK IMPLEMENTASI RGEC TERHADAP NILAI PERUSAHAAN YANG GO PUBLIC DI BURSA EFEK INDONESIA
Authors: , Wardoyo , Agustini Rizki Muti 
Published: February 2017

This research aims to find and analyze influence risk profile, good corporate governance, earnings, andÂ capital on the banking sector companies in Indonesia public company. Based on the completeness of data, thereÂ are only 14 banks to the period observation in 2009-2011 that able to be analyzed. The analysis used is multipleÂ regression. The research results show that risk market and risks reputation impact on value of enterprise, whileÂ credit risk, risk liquidity, operational risk, risk law, and risks compliance have not been affecting the value ofÂ enterprise. Size of the board of commissioners, independence of the board of commissioners, size of the boardÂ of directors, and the number of audit committee have not been affecting the value of enterprise. While, ROEÂ impacts on value of enterprise. In the other hands, ROA, BOPO, and CAR values have not been affecting theÂ value of enterprise.Keywords: corporate value, tobinâ€™s Q, risk profile, good corporate governance, earnings.
DAMPAK STRUKTUR PASAR DAN EFSIENSI TERHADAP KINERJA BANK PEMBANGUNAN DAERAH
Authors: Yudaruddin Rizky 
Published: February 2017

Conditions Regional Development Bank (BPD) in terms of Business Growth, Markets and CompetitivenessÂ within the last three years shows an alarming condition. The study aims to assess the impact of market structureÂ and efficiency of the performance of the BPD in Indonesia. The data used is secondary data in the form of financialÂ statements of banks BPD in 2004-2013. The analytical tool used in this research is panel data regression. TheÂ results found that the banking industry in particular BPD in Indonesia supports the traditional hypothesis thatÂ assumes that the concentration is a proxy of market power (market power). Variable efficiency is not significantÂ positive effect on the performance.Keywords: market structure, efficiency, performance, regional development banks
IMPLEMENTASI PERDA 8 TAHUN 2010 TENTANG PENGALIHAN BPHTB UNTUK MENINGKATKAN PAD KABUPATEN JOMBANG
Authors: Ermayanti Dwi 
Published: February 2017

AbstrakBea Perolehan Hak Atas Tanah Dan Bangunan (BPHTB) merupakan salah satu sumber pendapatan daerah. Pengalihan BPHTB menjadi pajak daerah diawali dengan perumusan kebijakan yang dituangkan dalam UU Nomor 28 Tahun 2009 tentang Pajak Daerah dan Retribusi Daerah. Penelitian ini bertujuan untukmengetahui implementasi UU NO. 8 Tahun 2010 serta mengetahui faktor-faktor yang mempengaruhi untuk meningkatkan PAD Kabupaten Jombang. Kesimpulan penelitian adalah Implementasi Perda No. 8 tahun 2010 tentang Pengalihan BPHTB, berhasil mencapai tujuannya yaitu meningkatkan PAD di Kabupaten Jombang. Peneliti berharap selanjutnya Pemerintah Kabupaten Jombang lebih menekankan lagi Peraturan Daerah BPHTB dan membuat kebijakan bagi wajib pajak yang melanggar peraturan yang ada.Kata kunci: BPHTB, PBB, Pajak dan Retribusi DaerahAbstractRegional autonomy has broad implications on the regional authority to explore and manage local revenue sources. Tax on Acquisition of Land and Building (BPHTB) is one source of local revenue. The BPHTB diversion becomes the local tax started by the policies formulation that set forth in Law No. 28, 2009 on Taxes and Retribution Regional. This study aims to determine the implementation of Law NO. 8 of 2010 on BPHTB to increase Jombang district PAD and determine the factors that affect the implementation of Law NO. 8 of 2010 on BPHTB, to improve Jombang district PAD. The conclusion of the study is the implementation of Regulation No. 8, 2010 on BPHTB diversion, succeeded in achieving its goal of increasing PAD in Jombang. The researchers hope to the Jombang District Government to emphasizes again the BPHTB Regional Regulation and create taxpayers policies for anyone violate the rulesKeywords: Tax on Acquisition of Land and Building, Taxes and Retribution Regional
Pacific Media Watch and protest in Oceania: An investigative free media case study
Authors: Robie David 
Published: February 2017

In the past three decades, global and regional media freedom advocacy and activist groups have multiplied as risks to journalists and media workers have escalated. Nowhere has this trend been so marked as in the Oceania region where some four organisations have developed a media freedom role. Of these, one is unique in that while it has had a regional mission for almost two decades, it has been continuously based at four university journalism schools in Australia, Fiji, New Zealand and Papua New Guinea. Pacific Media Watch was founded as an independent, non-profit and non-government network by two journalism academics in the Australian Centre for Independent Journalism (ACIJ) at the University of Technology, Sydney. Its genesis was the jailing of two Taimi ‘o Tonga journalists, ‘Ekalafi Moala and Filokalafi ‘Akau’ola, and a ‘whistleblowing’ pro-democracy member of Parliament in Tonga, ‘Akilisi Pohiva, for alleged contempt in September 1996. PMW played a role in the campaign to free the three men. Since then, the agency has developed an investigative journalism strategy to challenge issues of ethics, media freedom, industry ownership, cross-cultural diversity and media plurality. One of PMW’s journalists won the 2013 Dart Asia-Pacific Centre for Journalism and Trauma Prize for an investigation into torture and social media in Fiji. This article presents a case study of the PMW project and examines its history and purpose as a catalyst for independent journalists, educator journalists, citizen journalists and critical journalists in a broader trajectory of Pacific protest.Figure 1: A Pacific Media Watch Fiji torture and social media investigation series won the Dart Asia-Pacific Centre trauma journalism prize in 2013.
Interictal diffusion and perfusion magnetic resonance imaging features of cats with familial spontaneous epilepsy
Authors: Mizoguchi Shunta , Hasegawa Daisuke , Hamamoto Yuji , Yu Yoshihiko , Kuwabara Takayuki , Fujiwara-Igarashi Aki , Fujita Michio 
Published: February 2017

Abstract
OBJECTIVE To evaluate the usefulness of diffusion and perfusion MRI of the cerebrum in cats with familial spontaneous epilepsy (FSECs) and identify microstructural and functional deficit zones in affected cats.
ANIMALS 19 FSECs and 12 healthy cats.
PROCEDURES Diffusion-weighted, diffusion tensor, and perfusion-weighted MRI of the cerebrum were performed during interictal periods in FSECs. Imaging findings were compared between FSECs and control cats. Diffusion (apparent diffusion coefficient and fractional anisotropy) and perfusion (relative cerebral blood volume [rCBV], relative cerebral blood flow [rCBF], and mean transit time) variables were measured bilaterally in the hippocampus, amygdala, thalamus, parietal cortex gray matter, and subcortical white matter. Asymmetry of these variables in each region was also evaluated and compared between FSECs and control cats.
RESULTS The apparent diffusion coefficient of the total amygdala of FSECs was significantly higher, compared with that of control cats. The fractional anisotropy of the right side and total hippocampus of FSECs was significantly lower, compared with that of control cats. The left and right sides and total hippocampal rCBV and rCBF were significantly lower in FSECs than in control cats. The rCBV and rCBF of the parietal cortex gray matter in FSECs were significantly lower than in control cats.
CONCLUSIONS AND CLINICAL RELEVANCE In FSECs, diffusion and perfusion MRI detected microstructural changes and hypoperfusion (lowered function) in the cerebrum during interictal periods from that of healthy cats. These findings indicated that diffusion and perfusion MRI may be useful for noninvasive evaluation of epileptogenic foci in cats.
Relating Complexity and Error Rates of Ontology Concepts
Authors: Zheng Ling , Perl Yehoshua , Halper Michael , Coronado Sherri de , Ochs Christopher , Min Hua 
Published: February 2017

SummaryObjectives: Ontologies are knowledge structures that lend support to many health-information systems. A study is carried out to assess the quality of ontological concepts based on a measure of their complexity. The results show a relation between complexity of concepts and error rates of concepts.Methods: A measure of lateral complexity defined as the number of exhibited role types is used to distinguish between more complex and simpler concepts. Using a framework called an area taxonomy, a kind of abstraction network that summarizes the structural organization of an ontology, concepts are divided into two groups along these lines. Various concepts from each group are then subjected to a two-phase QA analysis to uncover and verify errors and inconsistencies in their modeling. A hierarchy of the National Cancer Institute thesaurus (NCIt) is used as our test- bed. A hypothesis pertaining to the expected error rates of the complex and simple concepts is tested.Results: Our study was done on the NCIt’s Biological Process hierarchy. Various errors, including missing roles, incorrect role targets, and incorrectly assigned roles, were discovered and verified in the two phases of our QA analysis. The overall findings confirmed our hypothesis by showing a statistically significant difference between the amounts of errors exhibited by more laterally complex concepts vis-à-vis simpler concepts.Conclusions: QA is an essential part of any ontology’s maintenance regimen. In this paper, we reported on the results of a QA study targeting two groups of ontology concepts distinguished by their level of complexity, defined in terms of the number of exhibited role types. The study was carried out on a major component of an important ontology, the NCIt. The findings suggest that more complex concepts tend to have a higher error rate than simpler concepts. These findings can be utilized to guide ongoing efforts in ontology QA.
The H i Chronicles of LITTLE THINGS BCDs. III. Gas Clouds in and around Mrk 178, VII Zw 403, and NGC 3738
Authors: Ashley Trisha , Simpson Caroline E. , Elmegreen Bruce G. , Johnson Megan , Pokhrel Nau Raj 
Published: February 2017

Abstract
In most blue compact dwarf (BCD) galaxies, it remains unclear what triggers their bursts of star formation. We study the H i of three relatively isolated BCDs, Mrk 178, VII Zw 403, and NGC 3738, in detail to look for signatures of star formation triggers, such as gas cloud consumption, dwarf–dwarf mergers, and interactions with companions. High angular and velocity resolution atomic hydrogen (H i) data from the Very Large Array (VLA) dwarf galaxy H i survey, Local Irregulars That Trace Luminosity Extremes, The H i Nearby Galaxy Survey (LITTLE THINGS), allow us to study the detailed kinematics and morphologies of the BCDs in H i. We also present high-sensitivity H i maps from the NRAO Green Bank Telescope (GBT) of each BCD to search their surrounding regions for extended tenuous emission or companions. The GBT data do not show any distinct galaxies obviously interacting with the BCDs. The VLA data indicate several possible star formation triggers in these BCDs. Mrk 178 likely has a gas cloud impacting the southeast end of its disk or it is experiencing ram pressure stripping. VII Zw 403 has a large gas cloud in its foreground or background that shows evidence of accreting onto the disk. NGC 3738 has several possible explanations for its stellar morphology and H i morphology and kinematics: an advanced merger, strong stellar feedback, or ram pressure stripping. Although apparently isolated, the H i data of all three BCDs indicate that they may be interacting with their environments, which could be triggering their bursts of star formation.
The Interstellar Medium in High-redshift Submillimeter Galaxies as Probed by Infrared Spectroscopy∗
Authors: Wardlow Julie L. , Cooray Asantha , Osage Willow , Bourne Nathan , Clements David , Dannerbauer Helmut , Dunne Loretta , Dye Simon , Eales Steve , Farrah Duncan , Furlanetto Cristina , Ibar Edo , Ivison Rob , Maddox Steve , Michałowski Michał M. , Riechers Dominik , Rigopoulou Dimitra , Scott Douglas , Smith Matthew W. L. , Wang Lingyu , Werf Paul van der , Valiante Elisabetta , Valtchanov Ivan , Verma Aprajita 
Published: February 2017

Abstract
Submillimeter galaxies (SMGs) at

are luminous in the far-infrared, and have star formation rates, SFR, of hundreds to thousands of solar masses per year. However, it is unclear whether they are true analogs of local ULIRGs or whether the mode of their star formation is more similar to that in local disk galaxies. We target these questions by using Herschel-PACS to examine the conditions in the interstellar medium (ISM) in far-infrared luminous SMGs at

–4. We present 70–160 μm photometry and spectroscopy of the [O iv]26 μm, [Fe ii]26 μm, [S iii]33 μm, [Si ii]34 μm, [O iii]52 μm, [N iii]57 μm, and [O i]63 μm fine-structure lines and the S(0) and S(1) hydrogen rotational lines in 13 lensed SMGs identified by their brightness in early Herschel data. Most of the 13 targets are not individually spectroscopically detected; we instead focus on stacking these spectra with observations of an additional 32 SMGs from the Herschel archive—representing a complete compilation of PACS spectroscopy of SMGs. We detect [O i]63 μm, [Si ii]34 μm, and [N iii]57 μm at

in the stacked spectra, determining that the average strengths of these lines relative to the far-IR continuum are

,

, and

, respectively. Using the [O iii]52 μm/[N iii]57 μm emission line ratio, we show that SMGs have average gas-phase metallicities

. By using PDR modeling and combining the new spectral measurements with integrated far-infrared fluxes and existing [C ii]158 μm data, we show that SMGs have average gas densities, n, of

and FUV field strengths,

(in Habing units:

), consistent with both local ULIRGs and lower luminosity star-forming galaxies.
A Closer Look at the Alpha Persei Coronal Conundrum
Authors: Ayres Thomas R. 
Published: February 2017

Abstract
A ROSAT survey of the Alpha Per open cluster in 1993 detected its brightest star, the mid-F supergiant α Persei: the X-ray luminosity and spectral hardness were similar to coronally active late-type dwarf members. Later, in 2010, a Hubble Cosmic Origins Spectrograph SNAPshot of α Per found the far-ultraviolet (FUV) coronal-proxy Si iv unexpectedly weak. This, and a suspicious offset of the ROSAT source, suggested that a late-type companion might be responsible for the X-rays. Recently, a multifaceted program tested that premise. Ground-based optical coronography and near-UV imaging with Hubble Space Telescope (HST) Wide-Field Camera 3 searched for any close-in faint candidate coronal objects, but without success. Then, a Chandra pointing found the X-ray source single and coincident with the bright star. Significantly, the Si iv emissions of α Per, in a deeper FUV spectrum collected by the HST Cosmic Origin Spectrograph as part of the joint program, are aligned well with chromospheric atomic oxygen (which must be intrinsic to the luminous star), within the context of cooler late-F and early-G supergiants, including Cepheid variables. This pointed to the X-rays as the fundamental anomaly. The overluminous X-rays still support the case for a hyperactive dwarf secondary, albeit now spatially unresolved. However, an alternative is that α Per represents a novel class of coronal source. Resolving the first possibility now has become more difficult, because the easy solution—a well-separated companion—has been eliminated. Testing the other possibility will require a broader high-energy census of the early-F supergiants.
Nonlinear Force-free Coronal Magnetic Stereoscopy
Authors: Chifu Iulia , Wiegelmann Thomas , Inhester Bernd 
Published: February 2017

Abstract
Insights into the 3D structure of the solar coronal magnetic field have been obtained in the past by two completely different approaches. The first approach are nonlinear force-free field (NLFFF) extrapolations, which use photospheric vector magnetograms as boundary condition. The second approach uses stereoscopy of coronal magnetic loops observed in EUV coronal images from different vantage points. Both approaches have their strengths and weaknesses. Extrapolation methods are sensitive to noise and inconsistencies in the boundary data, and the accuracy of stereoscopy is affected by the ability of identifying the same structure in different images and by the separation angle between the view directions. As a consequence, for the same observational data, the 3D coronal magnetic fields computed with the two methods do not necessarily coincide. In an earlier work (Paper I) we extended our NLFFF optimization code by including stereoscopic constrains. The method was successfully tested with synthetic data, and within this work, we apply the newly developed code to a combined data set from SDO/HMI, SDO/AIA, and the two STEREO spacecraft. The extended method (called S-NLFFF) contains an additional term that monitors and minimizes the angle between the local magnetic field direction and the orientation of the 3D coronal loops reconstructed by stereoscopy. We find that when we prescribe the shape of the 3D stereoscopically reconstructed loops, the S-NLFFF method leads to a much better agreement between the modeled field and the stereoscopically reconstructed loops. We also find an appreciable decrease by a factor of two in the angle between the current and the magnetic field. This indicates the improved quality of the force-free solution obtained by S-NLFFF.
Diversity of Abundance Patterns of Light Neutron-capture Elements in Very-metal-poor Stars∗
Authors: Aoki Misa , Ishimaru Yuhri , Aoki Wako , Wanajo Shinya 
Published: February 2017

Abstract
We determine the abundances of neutron-capture elements from Sr to Eu for five very-metal-poor stars (

) in the Milky Way halo to reveal the origin of light neutron-capture elements. Previous spectroscopic studies have shown evidence of at least two components in the r-process; one referred to as the “main r-process” and the other as the “weak r-process,” which is mainly responsible for producing heavy and light neutron-capture elements, respectively. Observational studies of metal-poor stars suggest that there is a universal pattern in the main r-process, similar to the abundance pattern of the r-process component of solar-system material. Still, it is uncertain whether the abundance pattern of the weak r-process shows universality or diversity, due to the sparseness of measured light neutron-capture elements. We have detected the key elements, Mo, Ru, and Pd, in five target stars to give an answer to this question. The abundance patterns of light neutron-capture elements from Sr to Pd suggest a diversity in the weak r-process. In particular, scatter in the abundance ratio between Ru and Pd is significant when the abundance patterns are normalized at Zr. Our results are compared with the elemental abundances predicted by nucleosynthesis models of supernovae with parameters such as electron fraction or proto-neutron-star mass, to investigate sources of such diversity in the abundance patterns of light neutron-capture elements. This paper presents that the variation in the abundances of observed stars can be explained with a small range of parameters, which can serve as constraints on future modeling of supernova models.