bluuebunny/crossref_metadata_2025_split huggingface dataset:
trend Angka kematian Ibu (AKI) Dan Angka Kematian Bayi (AKB) Di Propinsi Jawa Timur Tahun 2011-2015
Authors: Sumiasih Sumiasih 
Published: January 2019

Kematian ibu adalah kasus kematian selama kehamilan atau dalam periode 42 hari setelah berakhirnya kehamilan, akibat semua sebab yang terkait dengan atau diperberat oleh kehamilan atau penanganannya, tetapi bukan disebabkan oleh kecelakaan/ cedera. Sedangkan kasus kematian bayi adalah kasus kematian bayi yang terjadi antara saat setelah bayi lahir sampai bayi belum berusia tepat satu tahun. Rendahnya kesadaran masyarakat tentang kesehatan saat kehamilan, persalinan, masa nifas dan komplikasinya menjadi faktor penentu angka kematian ibu di Provinsi Jawa Timur. Program kesehatan ibu yang telah dilaksanakan untuk menurunkan AKI di provinsi Jawa Timur yaitu dengan memperhatikan kesehatan saat ibu hamil, saat ibu bersalin, saat ibu nifas. Meningkatnya AKB di Provinsi Jawa Timur dapat terjadi karena faktor pelayanan neonatal. Penelitian ini bertujuan adalah untuk mengetahui trend angka kematian ibu (AKI) dan angka kematian bayi (AKB) di Provinsi Jawa Timur pada tahun 2011-2015. Desain penelitian ini merupakan cross sectional, analisis menggunakan data laporan kesehatan ibu Provinsi Jawa Timur. Hasil yang diperoleh trend angka kematian ibu (AKI) di Provinsi dari tahun 2011-2015 adalah menurun, hal ini dapat terjadi karena capaian program kesehatan ibu terjadi peningkatan. Begitu juga dengan trend angka kematian bayi (AKB) menurun dari tahun 2011-2015.
Efektivitas Penggunaan Metode Preseptorship Pada Mahasiswa Keperawatan STIKES Widyagama Husada
Authors: Qodir Abdul 
Published: January 2019

Instalasi Gawat Darurat (IGD) memiliki karakteristik ruangan unik yang dimana beban kerja cukup tinggi dan memerlukan tindakan penanganan yang cepat, tepat dan trampil. Sehingga membutuhkan strategi metode pembelajaran yang tepat agar kompetensi mahasiswa dapat dicapai dengan baik. Tujuan dari penelitian ini adalah membuktikan efektifitas penggunaan metode preseptorship pada mahasiswa keperawatan STIKES Widyagama Husada di Instalasi Gawat Darurat (IGD). Metode penelitian yang digunakan adalah pre-eksperimen dengan pendekatan One group pretest-posttest design dengan jumlah sampel 40 Mahasiswa keperawatan yang di ambil secara consecutive sampling. Luaran dari penelitian ini adalah model pembelajaran yang tepat untuk mahasiswa keperawatan STIKES Widyagama Husada di Instalasi Gawat Darurat, pengayaan dan pengembangan bahan ajar dalam mata kuliah Keperawatan gawat darurat. Selain itu, hasil penelitian ini akan dipublikasikan dalam jurnal lokal ber-ISSN atau jurnal nasional terakreditasi dan Prosiding pada seminar ilmiah baik yang berskala lokal, regional maupun nasional. Hasil analisis bivariat menggunkan uji t berpasangan didapatkan Metode pembelajaran klinik preseptorship efektif dalam meningkatkan pengetahuan dan keterampilan mahasiswa (p=0,009); (p=0,000). Metode pembelajaran preceptorship agar diterpakan untuk meningkatkan kompetensi mahasiswa mahasiswa.
Analisis Penerimaan Penggunaan Aplikasi Grab di Kabupaten Sumedang
Authors: Yuniarto Dwi 
Published: January 2019

Sebagai aplikasi dalam hal transportasi, kehadiran Grab tentu memberikan dampak yang sangat besar pada kehidupan di masyarakat. Budaya penggunaan teknologi informasi yang kini menjadi paradigma baru, menjadikan beberapa aplikasi di beberapa bidang menjadi primadona. Tentu saja kehadiran aplikasi-aplikasi tersebut perlu dikaji lebih lanjut diterima atau tidaknya.
Untuk mengkaji penerimaan aplikasi Grab di Kabupaten Sumedang ini dimulai dengan menyebar kuesioner sebagai alat untuk mendapatkan data. Dari 120 populasi, diambil hanya 92 sampel (melalui perhitungan Krejcie dan Morgan) yang terdiri dari Dosen dan Mahasiswa STMIK Sumedang, dengan pertanyaan dari beberapa variabel dari Technology Acceptance Model (TAM). Dari hasil pembahasan, dapat dilihat uji statistik memperlihatkan tingkat pengaruh yang lebih tinggi dalam penerimaan Masyarakat terhadap aplikasi Grab adalah kemudahan penggunaan terhadap kegunaan, yakni 4.01. Sedangkan tingkat pengaruh yang lebih rendah dalam penerimaan Masyarakat terhadap aplikasi Grab adalah perilaku pengguna terhadap penggunaan sistem yang aktual, yakni 1.74
PERAN PETUGAS KESEHATAN DAN PENGETAHUAN KELUARGA TERHADAP PENINGKATAN KEMAMPUAN MERAWAT KLIEN GANGGUAN JIWA DI RUMAH
Authors: Purnomo Edi , A. Pulungan Zulhaini Sartika , Milawati Andi 
Published: January 2019

Mental disorder schizophrenia is a disorder psychic who ranks second in diseases that cause the greatest burden after heart disease. Its burden of mental disorders is mainly felt by the families who have family members with mental disorders. Patients with mental disorders who live with the family does not always indicate the best condition for the recovery of the client. The purpose of this study was to determine the effect of the role of the clerk and the knowledge of the family in improving the ability of families caring for clients with mental disorders at home. This research method is descriptive quantitative research design descriptive analytic approach cross sectional study. The samples used were 30 families who have family members experiencing mental disorders withpurposivesampling method. The research was conducted in Puskesmas Ulumanda Majene district. Results showed no effect between family knowledge (p=0.005) and the role of health care workers (p=0.008) with the ability of families in caring for clients with mental disorders at home. Conclusion the role of health workers and knowledge affect the ability of families caring for clients with mental disorders at home. Advised the family to be more active in seeking information about the treatment of people with mental disorders at home and health officials often approach to the family to help care clients with mental disorders.
PENYULUHAN DAN PERUBAHAN PENGETAHUAN CUCI TANGAN PAKAI SABUN DI DESA SUKOWIDI KABUPATEN MAGETAN
Authors: Marsanti Avicena Sakufa 
Published: January 2019

Data from primary health care Panekan showed that incidence of diarrhea was increased. The Cause of Diarrhea is a wrong Hand washing Practice. Based on interview over the last 6 month, 10 people didn’t know the importance of hand washing. The objective of this study was to determine This study was experimental one group pretest and postest design with 100 family for samples and proportionate random sampling technique. This study was analyzed by paired t-test with significance P>0.05. The result showed that there was an effect between counseling and knowledge about hand washing with soap (p<0,001). Before the counseling, the mean of knowledge score was 63,6±7,91 and after counseling was 79,90±7,25. There was an effect of counseling and changes in knowledge about hand washing with soap in Sukowidi, Magetan, the mean of knowledge score was better after counseling.
GANGGUAN FUNGSIONAL MENETAP BERPENGARUH PADA RISIKO DEPRESI LANSIA DM DI WILAYAH KERJA PUSKESMAS JEKAN RAYA KOTA PALANGKA RAYA
Authors: Astuti Agnes Dewi , Sulistyowati Reny , Natalansyah Natalansyah 
Published: January 2019

Aging is a a natural process in life. Aging is characterized by loss of slowly ability organ tissue repair itself and is irreversible. The elderly are the final statge of a person’s life cycle and experience the aging process with change in various physical or physiological, psychological and social aspects (Miller, 2012). Hanges dues to aging eldely comple raises enormous opportunity for the elderly are at risk of depression. The objective of this study was to determine the factors that influence the risk of depression in elderly at Puskesmas Jekan Raya of Palangka Raya City with descriptive correlational research design using cross sectional approach. The sampling technique in this research is by using probability sampling technique that sampling technique giving equal oppurtinity to every individual in the population to be the research sample.The statistical test used was descriptive test and Chi Square test. The result indicate that factors influencing the risk of depression in the elderly is functional impairment were settled with p value= 0,000. Conclusion of the elderly who have other diseases besides DM settle a vulnerable population at risk of depression. The most dominant factor is the functional disturbances persist after controlling the variable of age, live event s and other diseases (other than DM) with OR=39. Recommended in elderly nursing decision making in order to improve the health of elderly family based programs to prevent depression in the elderly and especially carring by elderly family members.
Characterizing and Improving the Data Reduction Pipeline for the Keck OSIRIS Integral Field Spectrograph
Authors: Lockhart Kelly E. , Do Tuan , Larkin James E. , Boehle Anna , Campbell Randy D. , Chappell Samantha , Chu Devin , Ciurlo Anna , Cosens Maren , Fitzgerald Michael P. , Ghez Andrea , Lu Jessica R. , Lyke Jim E. , Mieda Etsuko , Rudy Alexander R. , Vayner Andrey , Walth Gregory , Wright Shelley A. 
Published: January 2019

Abstract
OSIRIS is a near-infrared (1.0–2.4 μm) integral field spectrograph operating behind the adaptive optics system at Keck Observatory and one of the first lenslet-based integral field spectrographs. Since its commissioning in 2005, it has been a productive instrument, producing nearly half the laser guide star adaptive optics papers on Keck. The complexity of its raw data format necessitated a custom data reduction pipeline (DRP) delivered with the instrument in order to iteratively assign flux in overlapping spectra to the proper spatial and spectral locations in a data cube. Other than bug fixes and updates required for hardware upgrades, the bulk of the DRP has not been updated since initial instrument commissioning. We report on the first major comprehensive characterization of the DRP using on-sky and calibration data. We also detail improvements to the DRP, including characterization of the flux assignment algorithm, exploration of spatial rippling in the reduced data cubes, and improvements to several calibration files, including the rectification matrix, bad-pixel mask, and wavelength solution. We present lessons learned from over a decade of OSIRIS data reduction that are relevant to the next generation of integral field spectrograph hardware and data reduction software design.
Measuring the Absolute Total Intrinsic Redshifts (Surface Gravity Plus the Convective Blueshift) of the Main-sequence Stars and Red Giants using Gaia Data
Authors: Dai De-Chang , Li ZhiGang , Stojkovic Dejan 
Published: January 2019

Abstract
We analyze the GAIA release II data to demonstrate how one can measure the absolute total intrinsic redshifts of the main-sequence stars and red giants. We remove the relative velocity components of the stars’ motion with respect to the Sun by doing the analysis in the local standard of the rest frame defined by the average stars’ motion. We provide results for four different types of stars. F-, G-, and K-type stars have about the same value of intrinsic redshift, which is, however, much smaller than the expected gravitational redshift. This indicates that GAIA’s data includes a convective blueshift effect of a several hundred m s−1 magnitude. The red giants’ intrinsic redshifts are negative, which implies that their convective blueshift is stronger than the gravitational redshift. This is expected since red giants are far less compact than other types.
Variable Stars in Terzan 5: Additional Evidence of Multi-age and Multi-iron Stellar Populations*
Authors: Origlia L. , Mucciarelli A. , Fiorentino G. , Ferraro F. R. , Dalessandro E. , Lanzoni B. , Rich R. M. , Massari D. , Contreras Ramos R. , Matsunaga N. 
Published: January 2019

Abstract
Terzan 5 is a complex stellar system in the Galactic bulge, harboring stellar populations (SPs) with very different iron content (Δ[Fe/H] ∼ 1 dex) and with ages differing by several gigayears. Here we present an investigation of its variable stars. We report on the discovery and characterization of three RR Lyrae stars. For these newly discovered RR Lyrae and for six Miras of known periods we provide radial velocity (RV) and chemical abundances from spectra acquired with X-SHOOTER at the Very Large Telescope. We find that the three RR Lyrae and the three short-period Miras (P < 300 days) have RV consistent with being Terzan 5 members. They have subsolar iron abundances and enhanced [α/Fe], well matching the age and abundance patterns of the 12 Gyr metal-poor SPs of Terzan 5. Only one, out of the three long-period (P > 300 days) Miras analyzed in this study, has an RV consistent with being a Terzan 5 member. Its super-solar iron abundance and solar-scaled [α/Fe] nicely match the chemical properties of the metal-rich SP of Terzan 5 and its derived mass nicely agrees with being several gigayears younger than the short-period Miras. This young variable is an additional proof of the surprisingly young subpopulation discovered in Terzan 5.
ALMA Observations of the Spatial Distribution of Three C2H4O2 Isomers toward Sgr B2(N)
Authors: Xue Ci , Remijan Anthony J. , Burkhardt Andrew M. , Herbst Eric 
Published: January 2019

Abstract
The

isomers have been previously investigated primarily via disparate sets of observations involving single-dish and array measurements. The only attempt at using a uniform set of observations was performed with the IRAM 30 m observation in 2013. In this study, we present an intensive and rigorous spectral and morphological analysis of the

isomers toward Sgr B2(N) with interferometers, Atacama Large Millimeter/submillimeter Array Band 3 observations. We propose a quantitative selection method, which automates the determination of the most uncontaminated transitions and allows us to report the discovery of previously undetected transitions of the three isomers. With the least contaminated transitions, the high spatial-resolution millimeter (mm) maps of the

isomers reveal that

and

each display two different velocity components, while only one velocity component of

is resolved. Moreover, the distribution of

is extended and offset from the continuum emission, unlike

and

, for which the low-velocity component is found to be compact and concentrated toward the continuum emission peak of Sgr B2(N). The distinct morphologies of these

isomeric species indicate that

have significant differences in chemical processes compared to

and

, which display similar spatial distributions.
Shock-generating Planetesimals Perturbed by a Giant Planet in a Gas Disk
Authors: Nagasawa M. , Tanaka K. K. , Tanaka H. , Nomura H. , Nakamoto T. , Miura H. 
Published: January 2019

Abstract
We examined the excitations of planetesimals caused by the resonances of a giant planet in a protoplanetary gas disk. The highly excited planetesimals generate bow shocks, the mechanism of which results in chondrule formation, crystallization of silicate dust, and evaporation of icy planetesimals. The planetesimals beyond 2:1 resonance migrate owing to the gas drag and obtain the maximum eccentricity around 3:1 resonance, which is located at approximately half the planetary distance. The eccentricity depends on the parameters of the planetesimals and the Jovian planet, such as size and location, and the gas density of the disk. The maximum relative velocity of a 100 km sized planetesimal with respect to the gas disk reaches up to ∼12 km s−1 in the case of Jupiter owing to secular resonance, which occurs because of the disk’s gravity. We find that if a Jovian-mass planet is located within 10 au, the planetesimals larger than 100 km gain sufficient velocity to cause the melting of chondrule precursors and crystallization of the silicate. The maximum velocity is higher for large planetesimals and eccentric planets. Planetesimals are trapped temporarily in the resonances and continue to have high speed over ≳1 Myr after the formation of a Jovian planet. This duration fits into the timescale of chondrule formation suggested by the isotopic data. The evaporation of icy planetesimals occurs when a Jovian planet is located within 15 au. This mechanism can be a new indicator of planet formation in exosystems if some molecules ejected from icy planetesimals are detected.
Multiband Optical and Near-Infrared Properties of Faint Submillimeter Galaxies with Serendipitous ALMA Detections
Authors: Patil Pallavi , Nyland Kristina , Lacy Mark , Farrah Duncan , Afonso José , Barkhouse Wayne , Surace Jason 
Published: January 2019

Abstract
We present a catalog of 26 faint submillimeter galaxies (SMGs) in the XMM Large Scale Structure (XMM-LSS) field identified by cross-matching serendipitously detected sources in archival pre–Atacama Large Millimeter Array (ALMA) band 6 and 7 data with multiband near-infrared (NIR) and optical data from the Spitzer Extragalactic Representative Volume Survey, the VISTA Deep Extragalactic Survey, the Canada–France–Hawaii Telescope Legacy Large Survey, and the Hyper Suprime-Cam Subaru Strategic Program. Of the 26 SMGs in our sample, 15 are identified here for the first time. The majority of the sources in our sample (16/26) have faint submillimeter fluxes (0.1 mJy < S
1mm < 1 mJy). In addition to the 26 SMGs with multiband optical and NIR detections, there are 60 highly reliable (>5σ) ALMA sources with no counterpart in any other band down to an Infrared Array Camera (IRAC) [4.5] AB magnitude of ≈23.7. To further characterize the 26 galaxies with both ALMA and optical/NIR counterparts, we provide 13-band forced photometry for the entire catalog using the Tractor and calculate photometric redshifts and rest-frame colors. The median redshift of our sample is

. We find that our sample galaxies have bluer colors compared to bright SMGs, and the UVJ color plot indicates that their colors are consistent with main-sequence star-forming galaxies. Our results provide new insights into the nature of the faint population of SMGs and also highlight opportunities for galaxy evolution studies based on archival ALMA data.
Transition from Circular-ribbon to Parallel-ribbon Flares Associated with a Bifurcated Magnetic Flux Rope
Authors: Zhong Z. , Guo Y. , Ding M. D. , Fang C. , Hao Q. 
Published: January 2019

Abstract
Magnetic flux ropes play a key role in triggering solar flares in the solar atmosphere. In this paper, we investigate the evolution of NOAA Active Region 12268 within 36 hr from 2015 January 29 to 30, during which a flux rope was formed and three M-class and three C-class flares were triggered without coronal mass ejections. During the evolution of the active region, the flare emission seen in the Hα and ultraviolet wavebands changed from a circular shape (plus an adjacent conjugated ribbon and a remote ribbon) to three relatively straight and parallel ribbons. Based on a series of reconstructed nonlinear force-free fields, we find sheared or twisted magnetic field lines and a large-scale quasi-separatrix layer (QSL) associated with 3D null points in a quadrupolar magnetic field. These features always existed and constantly evolved during the 2 days. The twist of the flux rope was gradually accumulated, eventually leading to its instability. Around the flux rope, there were some topological structures, including a bald patch, a hyperbolic flux tube, and a torus QSL. We discuss how the particular magnetic structure and its evolution produce the flare emission. In particular, the bifurcation of the flux rope can explain the transition of the flares from circular to parallel ribbons. We propose a two-stage evolution of the magnetic structure and its associated flares. In the first stage, sheared arcades under the dome-like large-scale QSL were gradually transformed into a flux rope through magnetic reconnection, which produced the circular-ribbon flare. In the second stage, the flux rope bifurcated to form the three relatively straight and parallel flare ribbons.
TESS Discovery of an Ultra-short-period Planet around the Nearby M Dwarf LHS 3844
Authors: Vanderspek Roland , Huang Chelsea X. , Vanderburg Andrew , Ricker George R. , Latham David W. , Seager Sara , Winn Joshua N. , Jenkins Jon M. , Burt Jennifer , Dittmann Jason , Newton Elisabeth , Quinn Samuel N. , Shporer Avi , Charbonneau David , Irwin Jonathan , Ment Kristo , Winters Jennifer G. , Collins Karen A. , Evans Phil , Gan Tianjun , Hart Rhodes , Jensen Eric L. N. , Kielkopf John , Mao Shude , Waalkes William , Bouchy François , Marmier Maxime , Nielsen Louise D. , Ottoni Gaël , Pepe Francesco , Ségransan Damien , Udry Stéphane , Henry Todd , Paredes Leonardo A. , James Hodari-Sadiki , Hinojosa Rodrigo H. , Silverstein Michele L. , Palle Enric , Berta-Thompson Zachory , Crossfield Ian , Davies Misty D. , Dragomir Diana , Fausnaugh Michael , Glidden Ana , Pepper Joshua , Morgan Edward H. , Rose Mark , Twicken Joseph D. , Villaseñor Jesus Noel S. , Yu Liang , Bakos Gaspar , Bean Jacob , Buchhave Lars A. , Christensen-Dalsgaard Jørgen , Christiansen Jessie L. , Ciardi David R. , Clampin Mark , Lee Nathan De , Deming Drake , Doty John , Jernigan J. Garrett , Kaltenegger Lisa , Lissauer Jack J. , McCullough P. R. , Narita Norio , Paegert Martin , Pal Andras , Rinehart Stephen , Sasselov Dimitar , Sato Bun’ei , Sozzetti Alessandro , Stassun Keivan G. , Torres Guillermo 
Published: January 2019

Abstract
Data from the newly commissioned Transiting Exoplanet Survey Satellite has revealed a “hot Earth” around LHS 3844, an M dwarf located 15 pc away. The planet has a radius of

R
⊕ and orbits the star every 11 hr. Although the existence of an atmosphere around such a strongly irradiated planet is questionable, the star is bright enough (I = 11.9, K = 9.1) for this possibility to be investigated with transit and occultation spectroscopy. The star’s brightness and the planet’s short period will also facilitate the measurement of the planet’s mass through Doppler spectroscopy.
Dynamo Wave Patterns inside of the Sun Revealed by Torsional Oscillations
Authors: Kosovichev Alexander G. , Pipin Valery V. 
Published: January 2019

Abstract
Torsional oscillations represent bands of fast and slow zonal flows around the Sun, which extend deep into the convection zone and migrate during solar cycles toward the equator following the sunspot “butterfly” diagram. Analysis of helioseismology data obtained in 1996–2018 for almost two solar cycles reveals zones of deceleration of the torsional oscillations inside of the Sun due to dynamo-generated magnetic field. The zonal deceleration originates near the bottom of the convection zone at high latitudes, and migrates to the surface revealing patterns of magnetic dynamo waves predicted by Parker’s dynamo theory. The analysis reveals that the primary seat of the solar dynamo is located in a high-latitude zone of the tachocline. It suggests a dynamo scenario that can explain “extended solar cycles” previously observed in the evolving shape of the solar corona. The results show a substantial decrease of the zonal acceleration in the current solar cycle and indicate a further decline of activity in the next solar cycle. Although the relationship between the magnitude of zonal deceleration and the amount of emerged toroidal field that leads to formation of sunspots is not yet established, the results reveal a new perspective for solar cycle modeling and prediction using helioseismology data.