bluuebunny/crossref_metadata_2025_split huggingface dataset:
KONTRIBUSI SEKTOR PERTANIAN PADA PERTUMBUHAN EKONOMI DI PROVINSI JAWA BARAT
Authors: Widianingsih Wiwin , Suryantini Any , Irham Irham 
Published: December 2016

This study aims to know the trend of GDRP of agricultural sector in West Java Province, sector and sub-sector of agriculture which has a role as a leading sector in West Java Province and each district in this province, the factors that affect the economic growth of agriculture sector in the West Java Province, and the growth typology of the agricultural sector in West Java Province. The method that used for this study are Trend analysis, Location Quotient (LQ), Dynamic Location Quotient (DLQ), Shift-Share, and Klassen Typology. Theresults showed that the trend of agriculture sector/sub-sectors’ GDRP value were significantly increased and the trend of agriculture sector/sub-sectors’ GDRP contribution were significantly decreased over the period year 2003-2012. The agricultural sector is a leading sector for West Java Province and most of its districts. Food crop and the horticultural sub-sector is a leading sector for West Java Province and some districts in this province. The growth of the national economy is the dominant factor affecting the growth of the sector/subsector of agriculture in West Java Province. The competitive advantage (competitiveness) of forestry sub-sector was higher than the same sub-sector in other areas at national level. Food crops and horticultural sub-sector and livestock sub-sector were advanced ut depressed sub-sector. Forestry sub-sectors was categorized in developing sub-sector. The agriculture sector, plantation and fisheries sub-sector were categorized in lagging development. Based on LQ, DLQ and Klassen Typology analysis, the results showed that there was a consistent result that were the forestry sub-sector categorized in a leading sub-sector in the future, f ood crops and horticulture sub-sector categorized in leading sub-sector along year 2003-2012. While sector of agriculture, plantation and fisheries sub-sector categorized in the lagged development sectors.
Perpustakaan Sebagai Organisasi Pembelajar: Studi Perpustakaan Universitas Gadjah Mada
Authors: Wahyuni Nur Cahyati , Uki Martina 
Published: December 2016

A university library as a learning space should put learning as a major issue. As the organization itself, university library needs to measure its quality as a learning organization for members of the organization and as a learning space for the academic community, in order to live sustainably in the process of changing learning trends. The quantitative method was applied in this study using benchmarking model of Garvin's learning organization. The results show that UGM Library has transformed to be a learning organization. Most of the indicators have reached, whereas some others are still below the standard of benchmark. Meanwhile there was difference in score based on level of education. The study was the first time conducted at UGM Library within a certain period of time; therefore there is no description of comparison process between the past and now. In the future its is expected there is further measurement to identify the development of preparedness of UGM Library as a learning organization.
Pemanfaatan E-journal oleh Mahasiswa: Kajian Analisis Sitasi Terhadap Tesis Mahasiswa Klaster Saintek Universitas Gadjah Mada
Authors: Istiana Purwani , Purwaningsih Sri 
Published: December 2016

Universitas Gadjah Mada Library provides various information resources either in printed or electronic formats. The Library has subscribed to electronic information resources in the form of ejournal databases. The availability and utilization of these resources need to be evaluated. This study is a citation analysis of theses of the students from science and technology cluster of Universitas Gadjah Mada in 2015. It is aimed at identifying: 1) types of information resources used by the students in thesis writing, 2)intensity of the utilization of e-journal information resources by the students, and 3) the availability of the required information in the databases subscribed by UGM Library. The object of the study consisted of 7,925 citation derived from 222 theses of the students from science and technology cluster UGM. Data were obtained from documentation. This study used citation analysis to analyze all citations. The result of the study showed types of information resources used by the students in thesis writing were books, journals, theses, websites, proceedings, government regulations/acts, others (maps, learning materials, guides to laboratory practice), research reports and dissertations and papers. Books were information resources mostly used. Journals utilized in thesis writing comprised as much as 25% (1,997 citations) and 84% (1,685 citations) of the journals were English. As many as 1,078 citations (64%) were available and 607 citations (36%) unavailable in the journals subscribed by UGM Library.
Diagnóstico de la oferta privada en la conciliación extrajudicial en derecho, como mecanismo de solución de conflictos intersubjetivo en el municipio de El Espinal -Tolima
Authors: Gaitán Reyes Julián Andrés , Forero Garzón Manuel Ernesto 
Published: December 2016

La Conciliación Extrajudicial en derecho, se ha mostrado como el método indicado para el gran número de conflictos intersubjetivos cualificados, convirtiéndose en una herramienta eficaz, confiable y con todas las ventajas de ser en esencia una justicia que reconstruye tejido social, la cual debe ser entendida como una institución socio-jurídica. El escrito es resultado de la investigación sobre la eficacia de la conciliación extrajudicial en derecho, como mecanismo de solución de conflictos intersubjetivos cualificados, en el Municipio de El Espinal – Tolima. Para ello, se llevó a cabo un estudio minucioso a la oferta privada (notarias, Cámara de Comercio y Universidad Cooperativa de Colombia sede El Espinal) de la conciliación extrajudicial en derecho en el municipio en mención. Se encontró que, la institución de la conciliación extrajudicial en derecho en la oferta privada es la menos conocida, con bajos niveles de utilización; igualmente, se encuentra mal articulada con el resto de la oferta. se concluye que el fortalecimiento de la conciliación debe ser divulgado como instrumento eficaz para la solución de conflictos y su articulación con la oferta pública del Municipio del Espinal.
Estrategias didácticas para la enseñanza de las ciencias naturales en la educación superior
Authors: Colorado Ordoñez Paula , Gutiérrez Gamboa Leidy Adriana 
Published: December 2016

El presente estudio tiene como propósito indagar las estrategias didácticas más pertinentes para la enseñanza en la formación de profesionales del campo de las ciencias naturales; para lo cual se tendrá en cuenta la descripción de cinco estrategias utilizadas en el área de la pedagogía en tres países diferentes, España, Argentina y Colombia. Esta investigación es cualitativa con enfoque descriptivo, ya que la presentación de resultados es una comparación de las estrategias s didácticas adoptadas por tres países diferentes para la enseñanza de las ciencias naturales, con base en estudios realizados y publicados en educación superior. Teniendo en cuenta los aprendizajes y los nuevos avances de la tecnología en general, y más específicamente en el campo de las ciencias naturales, se hace necesario incorporar nuevas estrategias didácticas acorde con los procesos tecnológicos en el aula, para la formación de estudiantes en la educación superior; para que con ello adquieran una visión global de los aprendizajes e incorporen nuevas didácticas que estimulen la construcción de conocimiento. Finalmente, se concluye que las estrategias más utilizadas actualmente, para atraer la atención y centrar la disposición para el aprendizaje, son la interrogación acerca de los conceptos previos que posee el estudiante, su expresión verbal y la utilización de lenguaje apropiado, la construcción de aprendizajes cooperativo en el grupo donde se desarrolle la dinámica de aprender mediante la formulación de problemas en proyectos que sirvan como eje fundamental para el desarrollo de las ciencias naturales.
“The Changing of the Guards”?
Authors: Frieman Catherine. J. , Wilkin Neil 
Published: December 2016

ABSTRACTOver the past 30 years, Britain’s large archaeological museums and collections have shifted their focus away from academic visitors exploring their stores and collections and toward the dynamic presentation of permanent and temporary displays. These are arranged to emphasize compelling and relevant interpretative narratives over the presentation of large numbers of objects. The shift to digitization and the online presentation of collections is a major feature of public engagement activities at many museums but also might open older and less accessible collections up to research. In this article, we consider what role digital platforms may have in the future of British museum-based archaeology, with special reference to initiatives at the British Museum. We suggest that online collections have the potential to mediate between engaging the public and allowing professional archaeologists to develop sophisticated research programs, since these platforms can present multiple narratives aimed at different audiences.
Repatriation as Inspiration
Authors: Beisaw April M. , Duus Penelope H. 
Published: December 2016

ABSTRACTAt the turn of the twentieth century, American museums helped to legitimize archaeology as a scientific discipline. By the next century, repatriation legislation had forced archaeologists to confront the dehumanization that can take place when bodies and sacred objects are treated as scientific specimens. Charting the future(s) of archaeology-museum relationships requires us to (1) recognize where, when, and how harm has been done, (2) confront those harmful precedents, and (3) restructure collections and exhibits in ways that heal wounds and advance research. Current research on the 1916 Susquehanna River Expedition, an archaeology-museum project funded by George Gustav Heye, provides insight into how our predecessors viewed their work. Using the expedition project as backdrop, an archaeology professor and an undergraduate student engage in a dialogue that explores the changing roles of American museums as the public faces of archaeology, training grounds for young professionals, and cultural centers for us all.
Curation as Public Scholarship
Authors: Buchanan Sarah A. 
Published: December 2016

ABSTRACTMuseum archaeology offers opportunities to practice artifact storytelling, engaging visitors on the strength of objects that have been conserved and curated. Public appreciation of science and history is bolstered when museums exhibit objects of singular historic significance in a manner that allows visitors to build an experiential understanding of the objects’ provenance. Archaeologists and conservators began reassembling the 330-year-old French ship La Belle as a live-action exhibition on 25 October 2014 in the Bullock Texas State History Museum. The collaboration broke new ground by inviting visitors, in person and via streaming online video, to watch the experts rebuild the ship in full public view. Until, and after, the reconstructed ship hull was moved into its permanent first-floor gallery location on 21 May 2015, the exhibition brought archaeologists and international museum visitors into the same room to learn. The article interprets these events toward reimagining museum object curation as public scholarship.
THE SOLAR NEIGHBORHOOD. XXXVIII. RESULTS FROM THE CTIO/SMARTS 0.9 m: TRIGONOMETRIC PARALLAXES FOR 151 NEARBY M DWARF SYSTEMS
Authors: Winters Jennifer G. , Sevrinsky R. Andrew , Jao Wei-Chun , Henry Todd J. , Riedel Adric R. , Subasavage John P. , Lurie John C. , Ianna Philip A. , Finch Charlie T. 
Published: December 2016

ABSTRACT
We present 160 new trigonometric parallaxes for 151 M dwarf systems from the REsearch Consortium On Nearby Stars (RECONS) group’s long-term astrometry/photometry program at the CTIO/SMARTS 0.9 m telescope. Most systems (124 or 82%) are found to lie within 25 pc. The stars have 119 mas yr

μ

828 mas yr−1 and 3.85

8.47. Among these are 58 systems from the SuperCOSMOS-RECONS search, discovered via our proper motion trawls of the SuperCOSMOS digitized archival photographic plates, while the remaining stars were suspected via photometric distance estimates to lie nearby. Sixteen systems were newly discovered via astrometric perturbations to be binaries, many of which are ideal for accurate mass determinations due to their proximity and orbital periods on the order of a decade. A variability analysis of the stars presented, two-thirds of which are new results, shows six of the stars to vary by more than 20 mmag. This effort brings the total number of parallaxes for M dwarf systems measured by RECONS to nearly 500 and increases by 26% the number of southern M dwarf systems with accurate trigonometric parallaxes placing them within 25 pc.
RESURRECTION OF (3200) PHAETHON IN 2016
Authors: Hui(許文韜) Man-To , Li(李京) Jing 
Published: December 2016

ABSTRACT
We present a study of the active asteroid (3200) Phaethon in the 2016 apparition using the Solar and Terrestrial Relations Observatory (STEREO) spacecraft and compare the results with data from the previous two perihelia in 2009 and 2012. Once again, Phaethon brightened by ∼2 mag soon after its perihelion passage, contradicting expectations from the phase function of a macroscopic monolithic body. Subsequently, a short antisolar tail of ∼0.°1 in length was formed within ∼1 day and quickly disappeared. No trail was seen. Our syndyne-synchrone analysis indicates that the tail was comprised of submicron to micron particles and can be approximated by a synchrone coinciding with the outburst. We estimate that the outburst has released a mass of ∼104–105 kg, comparable to the two mass ejections in 2009 and 2012, and that the average mass-loss rate is ∼0.1–1 kg s−1. The forward-scattering effect hinted at low level activity of Phaethon prior to the outburst, which increased the effective cross section by merely ≲1 km2. Without the forward-scattering enhancement, detecting such activity at side-scattering phase angles is very difficult. The forward-scattering effect also reinforces the idea that the ejected dust grains rather than gas emissions were responsible for the activity of Phaethon. Despite Phaethon's reactivation, it is highly unlikely that the Geminid meteoroid stream can be sustained by similar perihelion mass-loss events.
PROBABILITY OF THE PHYSICAL ASSOCIATION OF 104 BLENDED COMPANIONS TO KEPLER OBJECTS OF INTEREST USING VISIBLE AND NEAR-INFRARED ADAPTIVE OPTICS PHOTOMETRY
Authors: Atkinson Dani , Baranec Christoph , Ziegler Carl , Law Nicholas , Riddle Reed , Morton Tim 
Published: December 2016

ABSTRACT
We determine probabilities of physical association for stars in blended Kepler Objects of Interest (KOIs), and find that

of companions within ∼4″ are consistent with being physically unassociated with their primary. This produces a better understanding of potential false positives in the Kepler catalog and will guide models of planet formation in binary systems. Physical association is determined through two methods of calculating multi-band photometric parallax using visible and near-infrared adaptive optics observations of 84 KOI systems with 104 contaminating companions within ∼4″. We find no evidence that KOI companions with separations of less than 1″ are more likely to be physically associated than KOI companions generally. We also reinterpret transit depths for 94 planet candidates, and calculate that 2.6% ± 0.4% of transits have

, which is consistent with prior modeling work.
THE INCLINATION OF THE PLANETARY SYSTEM RELATIVE TO THE SOLAR EQUATOR MAY BE EXPLAINED BY THE PRESENCE OF PLANET 9
Authors: Gomes Rodney , Deienno Rogerio , Morbidelli Alessandro 
Published: December 2016

ABSTRACT
We evaluate the effects of a distant planet, commonly known as planet 9, on the dynamics of the giant planets of the solar system. We find that the dynamics of the giant planets can be decomposed into a classic Lagrange–Laplace dynamics relative to their own invariant plane and a slow precession of said plane relative to the total angular momentum vector of the solar system, including planet 9. Under specific configurations for planet 9, this precession can explain the current tilt of ∼6° between the invariant plane of the giant planets and the solar equator. An analytical model is developed to map the evolution of the inclination of the inner giant planets’ invariant plane as a function of the planet 9's mass and orbital elements, and numerical simulations of the equations of motion are performed to validate our analytical approach. The longitude of the ascending node of planet 9 is found to be linked to the longitude of the ascending node of the giant planets’ invariant plane, which also constrains the longitude of the node of planet 9 on the ecliptic. Some of the planet 9 configurations that allow the explanation of the current solar tilt are compatible with those proposed to explain the orbital confinement of distant Kuiper Belt objects. This work gives an elegant explanation for the current tilt between the invariant plane of the inner giant planets and the solar equator and also adds new constraints to the orbital elements of planet 9.
HIGH RESOLUTION He i 10830 Å NARROW-BAND IMAGING OF AN M-CLASS FLARE. I. ANALYSIS OF SUNSPOT DYNAMICS DURING FLARING
Authors: Wang Ya , Su Yingna , Hong Zhenxiang , Zeng Zhicheng , Ji Kaifan , Goode Philip R. , Cao Wenda , Ji Haisheng 
Published: December 2016

ABSTRACT
In this paper, we report our first-step results of high resolution He i 10830 Å narrow-band imaging (bandpass: 0.5 Å) of an M1.8 class two-ribbon flare on 2012 July 5. The flare was observed with the 1.6 m aperture New Solar Telescope at Big Bear Solar Observatory. For this unique data set, sunspot dynamics during flaring were analyzed for the first time. By directly imaging the upper chromosphere, running penumbral waves are clearly seen as an outward extension of umbral flashes; both take the form of absorption in the 10830 Å narrow-band images. From a space–time image made of a slit cutting across a flare ribbon and the sunspot, we find that the dark lanes for umbral flashes and penumbral waves are obviously broadened after the flare. The most prominent feature is the sudden appearance of an oscillating absorption strip inside the ribbon when it sweeps into the sunspot’s penumbral and umbral regions. During each oscillation, outwardly propagating umbral flashes and subsequent penumbral waves rush out into the inwardly sweeping ribbon, followed by a return of the absorption strip with similar speed. We tentatively explain the phenomena as the result of a sudden increase in the density of ortho-helium atoms in the area of the sunspot being excited by the flare’s extreme ultraviolet illumination. This explanation is based on the observation that 10830 Å absorption around the sunspot area gets enhanced during the flare. Nevertheless, questions are still open and we need further well-devised observations to investigate the behavior of sunspot dynamics during flares.
DOES A DIFFERENTIATED, CARBONATE-RICH, ROCKY OBJECT POLLUTE THE WHITE DWARF SDSS J104341.53+085558.2?
Authors: Melis Carl , Dufour P. 
Published: December 2016

ABSTRACT
We present spectroscopic observations of the dust- and gas-enshrouded, polluted, single white dwarf star SDSS J104341.53+085558.2 (hereafter SDSS J1043+0855). Hubble Space Telescope Cosmic Origins Spectrograph far-ultraviolet spectra combined with deep Keck HIRES optical spectroscopy reveal the elements C, O, Mg, Al, Si, P, S, Ca, Fe, and Ni and enable useful limits for Sc, Ti, V, Cr, and Mn in the photosphere of SDSS J1043+0855. From this suite of elements we determine that the parent body being accreted by SDSS J1043+0855 is similar to the silicate Moon or the outer layers of Earth in that it is rocky and iron-poor. Combining this with comparison to other heavily polluted white dwarf stars, we are able to identify the material being accreted by SDSS J1043+0855 as likely to have come from the outermost layers of a differentiated object. Furthermore, we present evidence that some polluted white dwarfs (including SDSS J1043+0855) allow us to examine the structure of differentiated extrasolar rocky bodies. Enhanced levels of carbon in the body polluting SDSS J1043+0855 relative to the Earth–Moon system can be explained with a model where a significant amount of the accreted rocky minerals took the form of carbonates; specifically, through this model the accreted material could be up to 9% calcium-carbonate by mass.
EQUATION OF STATE FOR NUCLEONIC AND HYPERONIC NEUTRON STARS WITH MASS AND RADIUS CONSTRAINTS
Authors: Tolos Laura , Centelles Mario , Ramos Angels 
Published: December 2016

ABSTRACT
We obtain a new equation of state for the nucleonic and hyperonic inner core of neutron stars that fulfils the 2 M
⊙ observations as well as the recent determinations of stellar radii below 13 km. The nucleonic equation of state is obtained from a new parameterization of the FSU2 relativistic mean-field functional that satisfies these latest astrophysical constraints and, at the same time, reproduces the properties of nuclear matter and finite nuclei while fulfilling the restrictions on high-density matter deduced from heavy-ion collisions. On the one hand, the equation of state of neutron star matter is softened around saturation density, which increases the compactness of canonical neutron stars leading to stellar radii below 13 km. On the other hand, the equation of state is stiff enough at higher densities to fulfil the 2 M
⊙ limit. By a slight modification of the parameterization, we also find that the constraints of 2 M
⊙ neutron stars with radii around 13 km are satisfied when hyperons are considered. The inclusion of the high magnetic fields present in magnetars further stiffens the equation of state. Hyperonic magnetars with magnetic fields in the surface of ∼1015 G and with values of ∼1018 G in the interior can reach maximum masses of 2 M
⊙ with radii in the 12–13 km range.
X-RAY/GeV EMISSIONS FROM CRAB-LIKE PULSARS IN THE LMC
Authors: Takata J. , Cheng K. S. 
Published: December 2016

ABSTRACT
We discuss X-ray and gamma-ray emissions from Crab-like pulsars, PSRs J0537-6910 and J0540-6919, in the Large Magellanic Cloud. Fermi-LAT observations have resolved the gamma-ray emissions from these two pulsars and found pulsed emissions from PSR J0540-6919. The total pulsed radiation in the X-ray/gamma-ray energy bands of PSR J0540-6919 is observed with efficiency

(in 4π sr), which is about a factor of ten larger than

of the Crab pulsar. Although PSR J0537-6910 has the highest spin-down power among currently known pulsars, the efficiency of the observed X-ray emissions is about two orders of magnitude smaller than that of PSR J0540-6919. This paper mainly discusses what causes the difference in the radiation efficiencies of these three energetic Crab-like pulsars. We discuss electron/positron acceleration and high-energy emission processes within the outer gap model. By solving the outer gap structure with the dipole magnetic field, we show that the radiation efficiency decreases as the inclination angle between the magnetic axis and the rotation axis increases. To explain the difference in the pulse profile and in the radiation efficiency, our model suggests that PSR J0540-6919 has an inclination angle much smaller than that of the Crab pulsar (here we assume the inclination angles of both pulsars are

). On the other hand, we speculate that the difference in the radiation efficiencies between PSRs J0537-6910 and J0549-6919 is mainly caused by the difference in the Earth viewing angle, and that we see PSR J0537-6910 with an Earth viewing angle

(or

) measured from the spin axis, while we see PSR J0540-6919 with

.