bluuebunny/crossref_metadata_2025_split huggingface dataset:
Work-life Balance a Strategic Human Resource Policies and Practices followed by Indian Organizations
Authors: Barik Pratibha , Pandey B.B. 
Published: December 2016

<em><span>The study examines the innovative work-life balance policies and practices implemented by various Indian Companies. As with the increase of women workforce, dual earner families and increase in nuclear families have generated the need for the employees to balance their work and personal life. Further to provide better quality of life and to retain their talented employees companies are providing various Work Life programmes. The present paper has made an effort to reveal the present status of work-life balance programs and benefits offered by various well reputed Indian organizations and its prospect and future challenges. The study is based on the extent of literature review, empirical study and secondary data. It was found that many organizations have started taking initiative to overcome work-life conflicts. Practices like flexi-time, parental leaves, childcare assistance and counseling etc. have improved and these supports enhance the performance and behavior of an employee towards their organization. This holistic view of this paper will contribute to the work-life balance literature and discuss the implication for future research. </span></em>
PENGONTROLAN GERAK MOBILE ROBOT MENGGUNAKAN SENSOR ACCELEROMETER PADA PERANGKAT BERGERAK ANDROID
Authors: Hermanto Dedy 
Published: December 2016

<p>Smartphone merupakan perangkat bergerak saat ini yang sering digunakan oleh setiap orang. Didalam ponsel smartphone salah satunya android, ditanamkan beberapa sensor yang digunakan untuk mendukung proses yang berjalan dalam kegiatan yang berjalan dalam ponsel smartphone. Salah satu sensor yang ditanamkan didalam smartphone terdapat sensor accelerometer, accelerometer ini <br />digunakan untuk mengukur percepatan dari sudut X, Y dan Z. sensor yang tertanam didalam smartphone digunakan untuk menggerakkan mobile robot sesuai dengan perubahan sensor yang terjadi pada smartphone. Penerapan komunikasi yang digunakan berupa serial komunikasi dengan teknologi wireless. Teknologi ini menggunakan teknologi bluetooth. Penerapan pergerakan yang digunakan yaitu dengan mengambil nilai perubahan X dan Y.</p>
WATERMARKING CITRA DIGITAL DENGAN INFORMATION DISPERSAL ALGORITHM (IDA) DAN ALGORITMA HUFFMAN
Authors: Hutagalung Bambang T.J. , Syahputra Andrian 
Published: December 2016

<p><em>Penelitian ini memaparkan bagaimana menunjukkan keaslian citra digital dari tindakan klaim kepemilikan citra digital oleh pihak yang tidak bertanggung jawab. Hal tersebut dapat dilakukan dengan proses watermaking menggunakan Information Dispersal Algorithm (IDA). Untuk menjaga </em><em>kerahasiaan parameter pembangkit proses watermarking dapat dilakukan dengan proses encoding dan decoding dengan algoritma Huffman. Pembuktian keaslian citra digital ter-watermark dilakukan dengan proses deteksi dan ekstraksi watermark pada citra digital ter-watermark yang memiliki ukuran yang sama dengan citra digital asli, maupun yang telah mengalami perubahan ukuran. Citra yang telah disisipi data akan mengalami penurunan kualitas. Untuk engevaluasi </em><em>kualitas citra hasil steganografi adalah dengan penilaian secara obyektif yaitu menghitung nilai Mean Square Error (MSE) dan Peak Signal to Noise Ratio (PSNR). Dari hasil pengujian pada citra digital asli dan citra digital watermark tidak mengalami perubahan yang signifikan. Hal ini </em><em>menunjukkan bahwa perbandingan kualitas antara citra asli dan citra watermark tidak jauh berbeda. Sehingga dapat disimpulkan bahwa kualitas citra pada steganografi mengalami penurunan namun sangat kecil, atau dapat dikatakan bahwa kualitas citra tetap baik.</em></p>
Sistem Rekomendasi Pembelian Barang Pada Toko Bangunan Menggunakan Fuzzy Tsukamoto
Authors: Kurniawan July , Haryanto Hanny 
Published: December 2016

<p><em>Bisnis ritel mengalami perkembangan yang sangat pesat, terutama di Indonesia.Salah satunya adalah toko bangunan yang belum menerapkan teknologi dan masih bersifat manual.Di era serba modern ini konsumen membutuhkan jual beli secara efektif dan cepat maka diperlukan sistem untuk membantu dalam mengatasi permasalahan dalam hal rekomendasikan barang berdasarkan kebutuhan konsumen. Tujuan yang ingin dicapai dari penelitian ini adalah menentukan kebutuhan konsumen untuk merekomendasikan barang yang dibutuhkan konsumen. Sistem ini akan lebih menyederhanakan proses-proses tersebut, dengan memanfaatkan teknologi informatika fuzzy logic tsukamoto. Sehingga diharapkan kebutuhan konsumen akan lebih cepat dan akurat dalam merekomendasikan barang. Penelitian ini menguraikan apa saja yang dibutuhkan untuk mengatasi masalah yang selama ini dialami oleh konsumen dengan minimnya informasi. Hasil rekomendasi dari penelitian ini adalah berupa persentase barang yang mengacu dari hasil prediksi yang telah diteliti sebelumnya.</em></p>
Sistem Informasi Nilai Siswa SMA Negeri 1 Tegal Berbasis Short Message Service
Authors: Arif Zaenul , Afandi Muhammad 
Published: December 2016

<p>Nilai Siswa pada instansi sekolah merupakan salah satu tolok ukur keberhasilan siswa dalam mempelajari materi yang disampaikan. Pada sistem yang lama orang tua belum mendapatkan nilai secara langsung dari pihak sekolah kecuali pada setiap akhir semester, sehingga mereka kesulitan untuk mengetahui perkembangan nilai anak mereka selama di sekolah. Untuk memberikan transparasi nilai kepada para siswa dan orang tua diperlukan sebuah sistem informasi nilai yang mudah dan cepat dalam pengaksesan data. Dengan mengidentifikasi masalah tersebut dilakukan analisis terhadap sistem lama untuk mengetahui kelemahan sistem. Dengan demikian sistem baru akan mengalami peningkatan. Analisis kelemahan sistem lama dengan menggunakan kategori PIECES (Performance, Information, Economy, Control, Eficiency, dan Service). Dalam memenuhi hal tersebut maka dibangun sebuah sistem informasi nilai siswa berbasis Short Message Service (SMS) Gateway. Sistem ini dibangun menggunakan software Gammu dan dengan menggunakan bahasa pemrograman PHP. Dengan menggunakan SMS untuk memperoleh data nilai bisa memberikan kemudahan bagi orang tua untuk memantau hasil belajar putra putrinya di sekolah.</p>
Implementasi Metode SAW Dan AHP Pada Sistem Informasi Penilaian Kinerja Dosen
Authors: Ari Jayanti Ni Ketut Dewi 
Published: December 2016

<p>Dosen adalah tenaga pendidik profesional yang memiliki tugas menjalankan fungsi Tri Darma Perguruan Tinggi dalam mencerdaskan kehidupan bangsa. Selain itu, agar fungsi dan tugas yang melekat pada jabatan fungsional dosen dilaksanakan sesuai dengan aturan yang berlaku, maka diperlukan penilaian kinerja dosen yang menjamin terjadinya proses pembelajaran yang berkualitas di jenjang pendidikan tinggi. Pelaksanaan penilaian kinerja dosen dimaksudkan bukan untuk menyulitkan dosen, tetapi sebaliknya penilaian kinerja dosen dilaksanakan untuk mewujudkan dosen yang profesional, karena harkat dan martabat suatu profesi ditentukan oleh kualitas layanan profesi yang bermutu. Untuk dapat menghasilkan laporan kinerja dosen yang akurat, tentu saja dibutuhkan suatu metode yang dapat melibatkan banyak komponen atau kriteria yang dinilai (multi kriteria), sehingga dalam penyelesaiannya diperlukan sebuah sistem pendukung keputusan dengan multikriteria. Metode sistem pendukung keputusan yang multikriteria antara lain yaitu Analytical Hierarchy Process (AHP) dan Simple Additive Weighting (SAW), namun keduanya mempunyai metode pengukuran yang berbeda-beda. Hasil yang didapat dari penelitian ini adalah menerapkan metode SAW dan metode AHP dimana pada penilaian kinerja dosen ini melibatkan kriteria dan sub-kriteria serta sistem penilaian kinerja dosen. Kriteria serta sub-kriteria tersebut dapat ditambah ataupun dikurangi sesuai dengan peraturan yang berlaku. Disamping itu, pada masing-masing kriteria tersebut dapat ditentukan jumlah bobotnya sehingga penilai dapat memprioritaskan bobot yang dirasa penting.</p>
Pesquisa de Clima Organizacional: ferramenta de modelo de Gestão na promoção de melhorias contínuas no Ambiente Institucional Financeiro
Authors: Silva Alex Amancio da , Oliveira Maria Do Carmo , Rosini Alessandro Marco , Silva Gislaine Souza dos Santos Amancio da 
Published: December 2016

A pesquisa de clima organizacional tem sido uma ferramenta importante no mundo corporativo, modo pelo qual as instituições podem avaliar e apurar por meio dos resultados obtidos, o grau de satisfação de seus colaboradores e buscar por meio de plano de ação, alcançar melhores resultados tanto em desempenho quanto em produção. Através de uma investigação empírica, de linha de pesquisa qualitativa exploratória, com coleta de dados secundários, verificou-se que a implementação da pesquisa de clima organizacional, “Fale Francamente” do banco Itaú Unibanco, possibilitou analisar dados e efetuar um plano de ação eficaz almejando melhorias contínuas no ambiente organizacional, servindo como modelo de gestão de pessoas. Os resultados obtidos foram favoráveis no período compreendido do ano de 2012 a 2014 com elevação do grau de satisfação em quatro 4% e mantida ótima aderência dos funcionários em responder as perguntas chegando a atingir 90% o número de colaboradores.
Sur les propriétés optiques de l'appareil stomatique. Absorption des rayonnements de 662, 530 et 440 nm par les cellules stomatiques et leurs plastes chez quelques espèces du midi méditerranéen au cours de la saison sèche
Authors: Mouravieff Igor 
Published: December 2016

On a mesuré par microphotométrie et en fluorescence chez une vingtaine d'espèces des terrains ensoleillés et secs, au cours de la saison sèche, l'absorption des rayonnements de 662, 530 et 440 nm par les cellules stomatiques et leurs plastes.
Les plastes stomatiques, de petite taille absorbent la lumière rouge à peine plus que la verte : 1 à 2 % seulement. Ils sont pauvres en chlorophylle et l'observation en fluorescence le confirme.
Pour les cellules stomatiques entières, l'absorption de la lumière verte dépasse parfois celle de la lumière rouge, la masse chlorophyllienne de l'ensemble des plastes de ces cellules étant trop faible par rapport aux pigments vacuolaires, qui retiennent une partie des radiations vertes.
Récolte de Coléoptères Dryopidae dans la région éthiopienne
Authors: Bertrand Henri 
Published: December 2016

L'auteur donne la liste complète des récoltes de Coléoptères Dryopides, effectuées par lui dans l'ensemble de l'Afrique au sud du Sahara, de la Guinée au Cap et à Madagascar durant les années 1957-1960, récoltes intéressant successivement l'Afrique occidentale et équatoriale française, l'Angola, le Congo belge, l'Afrique orientale, l'Afrique du Sud et les Rhodésies et Madagascar.
Les déterminations ont été faites par J. Delève, un spécialiste de l'Institut Royal des Sciences naturelles de Belgique qui procède à une révision complète de tous les Dryopides de la région éthiopienne.
Le nombre des espèces recueillies s'élève à 93, plus 3 sous-espèces, réparties en 25 genres différents ; sur ce nombre on compte 28 espèces ou sous-espèces nouvelles pour la science.
Ces insectes ont été tous capturés dans les eaux courantes depuis le niveau de la mer jusqu'à 2 000 mètres et plus, tous les grands massifs montagneux ayant été visités.
Étant donnée l'étendue des territoires parcourus, l'auteur donne un nouvel aperçu biogéographique sur les Dryopides de la région éthiopienne, très différent de celui reposant sur des connaissances systématiques insuffisantes ; c'est ainsi qu'il apparaît que trois genres seulement sont communs à l'Europe et à l'Afrique éthiopienne. Parmi les nouveaux genres créés par J. Delève, certains sont des endémiques propres à l'Afrique australe ou à Madagascar.
Qu'est-ce que Harpalus decipiens Dejean ?
Authors: Nicolas Jean-Pierre 
Published: December 2016

Harpalus decipiens Dej. se sépare morphologiquement assez nettement de rufitarsis Duft. par son pronotum non sinué, et nettement par son apex pénien de forme différente. Les ♀ ♀ que l'on est tenté d'attribuer au premier ont un pronotum non sinué et un apex élytral simple.
Ces deux formes ne sont nullement géographiques. Les sacs internes des ♂ ♂ sont identiques ; il n'est pas prouvé qu'elles soient spécifiquement distinctes bien que morphologiquement reconnaissables. Connaissant d'autres cas analogues (deux formes distinctes au regard de tel ou tel caractère ou couple de caractères, mais vraisemblablement conspécifiques), nous préférons y voir une seule espèce présentant un mélange de deux formes, et nous pensons que l'étude approfondie de phénomènes de ce genre pourrait avoir une certaine portée sur les connaissances relatives aux modalités de l'évolution si l'on sait se garder de les interpréter hâtivement.
OBLIQUITIES OF EXOPLANET HOST STARS FROM PRECISE DISTANCES AND STELLAR ANGULAR DIAMETERS
Authors: Quinn Samuel N. , White Russel J. 
Published: December 2016

ABSTRACT
The next generation of exoplanet space photometry missions proposed by both NASA and ESA promise to discover small transiting planets around the nearest and brightest main-sequence stars. The physical and rotational properties of these stars, in conjunction with Gaia-precision distances, can be used to determine the inclination of the stellar rotation axis. Given edge-on orbital paths for transiting planets, stellar inclinations can be interpreted as obliquities projected into the line of sight, which can be used to more clearly reveal the system architectures of small planets and the factors that drive their orbital evolution. To demonstrate the method, we use a sample of simulated target stars for the NASA Transiting Exoplanet Survey Satellite (TESS) mission. Based on predicted characteristics of these stars and likely measurement uncertainties, we show that the expected TESS discoveries will allow us to finely differentiate the true underlying obliquity distribution. Under conservative assumptions in our illustrative example—in which the true distribution is assumed to contain systems drawn from both well-aligned and isotropic distributions (e.g., due to multiple migration channels)—the correct fractions can be determined to within 0.15, thus enabling constraints on the evolutionary processes that shape system architectures. Moreover, because of the excellent astrometric precision expected from Gaia, this technique will also be applicable to the large number of planets already discovered by Kepler orbiting much more distant stars.
A VERSATILE TECHNIQUE TO ENABLE SUB-MILLI-KELVIN INSTRUMENT STABILITY FOR PRECISE RADIAL VELOCITY MEASUREMENTS: TESTS WITH THE HABITABLE-ZONE PLANET FINDER*
Authors: Stefansson Gudmundur , Hearty Frederick , Robertson Paul , Mahadevan Suvrath , Anderson Tyler , Levi Eric , Bender Chad , Nelson Matthew , Monson Andrew , Blank Basil , Halverson Samuel , Henderson Chuck , Ramsey Lawrence , Roy Arpita , Schwab Christian , Terrien Ryan 
Published: December 2016

ABSTRACT
Insufficient instrument thermomechanical stability is one of the many roadblocks for achieving 10 cm s−1 Doppler radial velocity precision, the precision needed to detect Earth-twins orbiting solar-type stars. Highly temperature and pressure stabilized spectrographs allow us to better calibrate out instrumental drifts, thereby helping in distinguishing instrumental noise from astrophysical stellar signals. We present the design and performance of the Environmental Control System (ECS) for the Habitable-zone Planet Finder (HPF), a high-resolution (R = 50,000) fiber-fed near-infrared (NIR) spectrograph for the

Hobby–Eberly Telescope at McDonald Observatory. HPF will operate at

, driven by the choice of an H2RG NIR detector array with a

cutoff. This ECS has demonstrated

rms stability over 15 days at both 180 and

, and maintained high-quality vacuum (

) over months, during long-term stability tests conducted without a planned passive thermal enclosure surrounding the vacuum chamber. This control scheme is versatile and can be applied as a blueprint to stabilize future NIR and optical high-precision Doppler instruments over a wide temperature range from ∼77

to elevated room temperatures. A similar ECS is being implemented to stabilize NEID, the NASA/NSF NN-EXPLORE spectrograph for the

WIYN telescope at Kitt Peak, operating at

. A [full SolidWorks 3D-CAD model] and a comprehensive parts list of the HPF ECS are included with this manuscript to facilitate the adaptation of this versatile environmental control scheme in the broader astronomical community.
IMPACT OF NEW GAMOW–TELLER STRENGTHS ON EXPLOSIVE TYPE IA SUPERNOVA NUCLEOSYNTHESIS
Authors: Mori Kanji , Famiano Michael A. , Kajino Toshitaka , Suzuki Toshio , Hidaka Jun , Honma Michio , Iwamoto Koichi , Nomoto Ken’ichi , Otsuka Takaharu 
Published: December 2016

ABSTRACT
Recent experimental results have confirmed a possible reduction in the Gamow–Teller (GT+) strengths of pf-shell nuclei. These proton-rich nuclei are of relevance in the deflagration and explosive burning phases of SNe Ia. While prior GT strengths result in nucleosynthesis predictions with a lower-than-expected electron fraction, a reduction in the GT+ strength can result in a slightly increased electron fraction compared to previous shell model predictions, though the enhancement is not as large as previous enhancements in going from rates computed by Fuller, Fowler, and Newman based on an independent particle model. A shell model parametrization has been developed that more closely matches experimental GT strengths. The resultant electron-capture rates are used in nucleosynthesis calculations for carbon deflagration and explosion phases of SNe Ia, and the final mass fractions are compared to those obtained using more commonly used rates.
SPECIAL RELATIVISTIC HYDRODYNAMICS WITH GRAVITATION
Authors: Hwang Jai-chan , Noh Hyerim 
Published: December 2016

ABSTRACT
Special relativistic hydrodynamics with weak gravity has hitherto been unknown in the literature. Whether such an asymmetric combination is possible has been unclear. Here, the hydrodynamic equations with Poisson-type gravity, considering fully relativistic velocity and pressure under the weak gravity and the action-at-a-distance limit, are consistently derived from Einstein’s theory of general relativity. An analysis is made in the maximal slicing, where the Poisson’s equation becomes much simpler than our previous study in the zero-shear gauge. Also presented is the hydrodynamic equations in the first post-Newtonian approximation, now under the general hypersurface condition. Our formulation includes the anisotropic stress.
CONSTRAINTS OF THE PHYSICS OF LOW-MASS AGB STARS FROM CH AND CEMP STARS
Authors: Cristallo S. , Karinkuzhi D. , Goswami A. , Piersanti L. , Gobrecht D. 
Published: December 2016

ABSTRACT
We analyze a set of published elemental abundances from a sample of CH stars which are based on high resolution spectral analysis of ELODIE and SUBARU/HDS spectra. All the elemental abundances were derived from local thermodynamic equilibrium analysis using model atmospheres, and thus they represent the largest homogeneous abundance data available for CH stars to date. For this reason, we can use the set to constrain the physics and the nucleosynthesis occurring in low mass asymptotic giant branch (AGB) s.tars. CH stars have been polluted in the past from an already extinct AGB companion and thus show s-process enriched surfaces. We discuss the effects induced on the surface AGB s-process distributions by different prescriptions for convection and rotation. Our reference theoretical FRUITY set fits only part of the observations. Moreover, the s-process observational spread for a fixed metallicity cannot be reproduced. At [Fe/H] > −1, a good fit is found when rotation and a different treatment of the inner border of the convective envelope are simultaneously taken into account. In order to increase the statistics at low metallicities, we include in our analysis a selected number of CEMP stars and, therefore, we compute additional AGB models down to [Fe/H] = −2.85. Our theoretical models are unable to attain the large [hs/ls] ratios characterizing the surfaces of those objects. We speculate on the reasons for such a discrepancy, discussing the possibility that the observed distribution is a result of a proton mixing episode leading to a very high neutron density (the so-called i-process).
THE THERMAL STATE OF KS 1731−260 AFTER 14.5 YEARS IN QUIESCENCE
Authors: Merritt Rachael L. , Cackett Edward M. , Brown Edward F. , Page Dany , Cumming Andrew , Degenaar Nathalie , Deibel Alex , Homan Jeroen , Miller Jon M. , Wijnands Rudy 
Published: December 2016

ABSTRACT
Crustal cooling of accretion-heated neutron stars provides insight into the stellar interior of neutron stars. The neutron star X-ray transient, KS 1731−260, was in outburst for 12.5 years before returning to quiescence in 2001. We have monitored the cooling of this source since then through Chandra and XMM-Newton observations. Here we present a 150 ks Chandra observation of KS 1731−260 taken in 2015 August, about 14.5 years into quiescence and 6 years after the previous observation. We find that the neutron star surface temperature is consistent with the previous observation, suggesting that crustal cooling has likely stopped and the crust has reached thermal equilibrium with the core. Using a theoretical crust thermal evolution code, we fit the observed cooling curves and constrain the core temperature (T

c
= 9.35 ± 0.25 × 107 K), composition (Q

), and level of extra shallow heating required (Q
sh = 1.36 ± 0.18 MeV/nucleon). We find that the presence of a low thermal conductivity layer, as expected from nuclear pasta, is not required to fit the cooling curve well, but cannot be excluded either.
SUSTAINED TURBULENCE IN DIFFERENTIALLY ROTATING MAGNETIZED FLUIDS AT A LOW MAGNETIC PRANDTL NUMBER
Authors: Nauman Farrukh , Pessah Martin E. 
Published: December 2016

ABSTRACT
We show for the first time that sustained turbulence is possible at a low magnetic Prandtl number in local simulations of Keplerian flows with no mean magnetic flux. Our results indicate that increasing the vertical domain size is equivalent to increasing the dynamical range between the energy injection scale and the dissipative scale. This has important implications for a large variety of differentially rotating systems with low magnetic Prandtl number such as protostellar disks and laboratory experiments.
A SUBMILLIMETER CONTINUUM SURVEY OF LOCAL DUST-OBSCURED GALAXIES
Authors: Lee Jong Chul , Hwang Ho Seong , Lee Gwang-Ho 
Published: December 2016

ABSTRACT
We conduct a 350 μm dust continuum emission survey of 17 dust-obscured galaxies (DOGs) at z = 0.05–0.08 with the Caltech Submillimeter Observatory (CSO). We detect 14 DOGs with S
350 μm = 114–650 mJy and signal-to-noise > 3. By including two additional DOGs with submillimeter data in the literature, we are able to study dust content for a sample of 16 local DOGs, which consist of 12 bump and four power-law types. We determine their physical parameters with a two-component modified blackbody function model. The derived dust temperatures are in the range 57–122 K and 22–35 K for the warm and cold dust components, respectively. The total dust mass and the mass fraction of the warm dust component are 3–34 × 107
M
⊙ and 0.03%–2.52%, respectively. We compare these results with those of other submillimeter-detected infrared luminous galaxies. The bump DOGs, the majority of the DOG sample, show similar distributions of dust temperatures and total dust mass to the comparison sample. The power-law DOGs show a hint of smaller dust masses than other samples, but need to be tested with a larger sample. These findings support that the reason DOGs show heavy dust obscuration is not an overall amount of dust content, but probably the spatial distribution of dust therein.