bluuebunny/crossref_metadata_2025_split huggingface dataset:
TEKNOLOGI PEMBUATAN ALAT DAN PERHIASAN DI GUA KIDANG, BLORA
Authors: Nurani Indah Asikin 
Published: March 2018

Gua Kidang is a prehistoric settlement that provides a complete description on the life pattern and the development of technology, as well as the adaptation strategy of the dwellers to survive. The development of technology was supported by the intelligence of the artist and the raw material provided in its neighbourhood. The manufacturing technique of tools and jewellery, found in Gua Kidang, demonstrated the effectivity aspect and unique innovation. Artifacts made from clamshell and bone, along with dental remains provide the insight on the variety of tools type and advance manufacturing technique compared to the type found in other prehistoric cave dwelling in Java as well asIndonesial. Based on the analysis of the manufacturing technique and geoarchaeological aspect, the cultural character of Gua Kidang’s dwellers was shown through the development of technology. This paper uses descriptive methods - explanatory with inductive reasoning.GuaKidang merupakan hunian prasejarah yang memberikan gambaran secara lengkap pola hidup dan pengembangan teknologi, serta pola adaptasi manusia dalam mempertahankan hidupnya. Pengembangan teknologi, didasarkan pada kecerdasan artisan pembuatnya, serta bahanbaku yang tersedia di lingkungan alam sekitarnya. Teknik pengerjaan alat dan perhiasan temuan di Gua Kidang, menunjukkan adanya aspek efektivitas dan inovasi tersendiri. Selain itu, temuan artefak kerang dan tulang, serta gigi memberikan kontribusi pengetahuan tentang ragam tipe alat dan teknik pengerjaan yang tinggi dibandingkan tipe alat temuan dari gua-gua hunian prasejarah di Jawa khususnya, dan Indonesia umumnya. Berdasarkan kajian teknik pembuatan dan aspek geoarkeologi, menunjukkan karakter budaya penghuni Gua Kidang dalam pengembangan teknologi. Tulisan ini menggunakan metode deskriptif – eksplanatif dengan penalaran induktif.
TRADISI BERLANJUT BUDAYA AUSTRONESIA DI LIMA PULUH KOTO, SUMATERA BARAT
Authors: Triwurjani Triwurjani 
Published: March 2018

Austronesian diaspora shows that around 60% of Austronesian-speaking people live in Indonesia. Among the locations with traces of Austronesian cultural remains is the information about the diaspora of Research reveals that the continuing megalithic tradition. The problem is: if megalithic culture was brought by migrants in which Austronesian period did the menhirs should be placed, the proto-historic or recent Austronesian; how is the dispersal pattern of the menhirs; and who were the bearers of the culture. Therefore we have to reveal the form and dispersal of the megalithic culture and Austronesian migration in Lima Puluh Koto Area. The aim of this research is revealing cultural history through the migrant's adaptation within the perspective of Austronesian diaspora. Thus information about the diaspora of the Austronesians and the ethnogenesis of Indoneisan nation can be recognized. Research reveals that the continuing megalithic tradition which is used the qualitative method and assumed base on archaeological remains at Lima Puluh Koto area is a distribution of menhirs, that forms clusters in accordance with nagari (state) at certain area, and they are dispersed up to the hilly area. Some of these menhirs have sacred function but there are also those with profane functions like marks of village, house yard, or street boundaries, as well as the marker of village or hamlet roads.Diaspora Austronesia menunjukkan kurang lebih 60% penutur tinggal di Indonesia. Salah satu lokasi jejak Austronesia adalah di Kabupaten Lima Puluh Koto, Sumatera Barat, yaitu sebaran menhir yang mencapai ratusan jumlahnya. Bentuk budaya Austronesia dikenal sebagai budaya yang meneruskan tradisi-tradisi masa prasejarah dan berlanjut pada masa sejarah, seperti tradisi megalitik. Permasalahannya adalah, apabila budaya megalitik dibawa oleh para migran, pada periode Austronesia protosejarah ataukah Austronesia masa kini menhir-menhir tersebut berada?, bagaimana pola sebaran menhir-menhir tersebut? dan siapa pendukungnya?. Penelitian ini berusaha mengungkapkan bentuk dan persebaran budaya megalitik dan migrasi Austronesia di Kawasan Lima Puluh Koto. Maksud dan tujuan penelitian ini adalah untuk mengungkapkan sejarah kebudayaan dan adaptasi kaum migran dalam perpekstif diaspora Austronesia, sehingga memperkaya informasi tentang diaspora Austronesia dan asal-usul etnogenesis bangsa Indoensia. Hasil penelitian yang dilakukan dengan metode kualitatif ini menunjukkan bahwa tradisi megalitik di kawasan Lima Puluh Koto adalah sebaran menhir yang membentuk kelompok-kelompok berdasarkan nagari pada area tertentu. Sebaran menhir ini selain mempunyai fungsi sakral juga mempunyai fungsi profan antara lain sebagai batas kampung, batas halaman, maupun batas jalan raya desa, atau jalan-jalan di kampung.
The Discrepancy between Einstein Mass and Dynamical Mass for SIS and Power-law Mass Models
Authors: Li Rui , Wang Jiancheng , Shu Yiping , Xu Zhaoyi 
Published: March 2018

Abstract
We investigate the discrepancy between the two-dimensional projected lensing mass and the dynamical mass for an ensemble of 97 strong gravitational lensing systems discovered by the Sloan Lens ACS Survey, the BOSS Emission-Line Lens Survey (BELLS), and the BELLS for GALaxy-Lyα EmitteR sYstems Survey. We fit the lensing data to obtain the Einstein mass and use the velocity dispersion of the lensing galaxies provided by the Sloan Digital Sky Survey to get the projected dynamical mass within the Einstein radius by assuming the power-law mass approximation. The discrepancy is found to be obvious and quantified by Bayesian analysis. For the singular isothermal sphere mass model, we obtain that the Einstein mass is 20.7% more than the dynamical mass, and the discrepancy increases with the redshift of the lensing galaxies. For the more general power-law mass model, the discrepancy still exists within a 1σ credible region. We suspect the main reason for this discrepancy is mass contamination, including all invisible masses along the line of sight. In addition, the measurement errors and the approximation of the mass models could also contribute to the discrepancy.
Observations of Upward Propagating Waves in the Transition Region and Corona above Sunspots
Authors: Hou Zhenyong , Huang Zhenghua , Xia Lidong , Li Bo , Fu Hui 
Published: March 2018

Abstract
We present observations of persistent oscillations of some bright features in the upper-chromosphere/transition region above sunspots taken by IRIS SJ 1400 Å and upward propagating quasi-periodic disturbances along coronal loops rooted in the same region taken by the AIA 171 Å passband. The oscillations of the features are cyclic oscillatory motions without any obvious damping. The amplitudes of the spatial displacements of the oscillations are about 1″. The apparent velocities of the oscillations are comparable to the sound speed in the chromosphere, but the upward motions are slightly larger than that of the downward. The intensity variations can take 24%–53% of the background, suggesting nonlinearity of the oscillations. The FFT power spectra of the oscillations show a dominant peak at a period of about 3 minutes, which is consistent with the omnipresent 3 minute oscillations in sunspots. The amplitudes of the intensity variations of the upward propagating coronal disturbances are 10%–15% of the background. The coronal disturbances have a period of about 3 minutes, and propagate upward along the coronal loops with apparent velocities in a range of 30 ∼ 80 km s−1. We propose a scenario in which the observed transition region oscillations are powered continuously by upward propagating shocks, and the upward propagating coronal disturbances can be the recurrent plasma flows driven by shocks or responses of degenerated shocks that become slow magnetic-acoustic waves after heating the plasma in the coronal loops at their transition-region bases.
Color Variabilities of Spectrally Defined Red QSOs at z = 0.3–1.2
Authors: Chen I-Chenn , Hwang Chorng-Yuan , Kaiser Nick , Magnier Eugene A. , Metcalfe Nigel , Waters Christopher 
Published: March 2018

Abstract
We study the brightness and the color variabilities of 34 red and 122 typical quasi-stellar objects (QSOs) at z = 0.3–1.2 using data from the Pan-STARRS Medium Deep Survey. The red and the typical QSOs are selected based on the ratios of the flux densities at 3000 Å to those at 4000 Å in the rest frame. We find that 16 out of 34 red QSOs are identified as extended sources, which exhibit strong brightness and color variabilities at shorter wavelengths due to the contamination of the emission from their host galaxies. Some point-like QSOs with significant color variabilities are able to change their color classification according to our spectral definition. The timescales of the color variabilities for these point-like QSOs are within 4 years, suggesting that the size scales of the mechanisms producing the color variabilities are less than a few light years. The spectra of some extended and point-like red QSOs can be well fitted with the dust-reddened spectra of a typical QSO, while others are difficult to explain with dust reddening.
Massive Stars in the SDSS-IV/APOGEE SURVEY. I. OB Stars
Authors: Roman-Lopes A. , Román-Zúñiga C. , Tapia Mauricio , Chojnowski Drew , Gómez Maqueo Chew Y. , García-Hernández D. A. , Borissova Jura , Minniti Dante , Covey Kevin R. , Longa-Peña Penélope , Fernandez-Trincado J. G. , Zamora Olga , Nitschelm Christian 
Published: March 2018

Abstract
In this work, we make use of DR14 APOGEE spectroscopic data to study a sample of 92 known OB stars. We developed a near-infrared semi-empirical spectral classification method that was successfully used in case of four new exemplars, previously classified as later B-type stars. Our results agree well with those determined independently from ECHELLE optical spectra, being in line with the spectral types derived from the “canonical” MK blue optical system. This confirms that the APOGEE spectrograph can also be used as a powerful tool in surveys aiming to unveil and study a large number of moderately and highly obscured OB stars still hidden in the Galaxy.
The UV Emission of Stars in the LAMOST Survey. I. Catalogs
Authors: Bai Yu , Liu JiFeng , Wicker James , Wang Song , Guo JinCheng , Qin YuXiang , He Lin , Wang JianLing , Wu Yue , Dong YiQiao , Zhang Yong , Hou Yonghui , Wang Yuefei , Cao Zihuang 
Published: March 2018

Abstract
We present the ultraviolet magnitudes for over three million stars in the LAMOST survey, in which 2,202,116 stars are detected by GALEX. For 889,235 undetected stars, we develop a method to estimate their upper limit magnitudes. The distribution of (FUV − NUV) shows that the color declines with increasing effective temperature for stars hotter than 7000 K in our sample, while the trend disappears for the cooler stars due to upper atmosphere emission from the regions higher than their photospheres. For stars with valid stellar parameters, we calculate the UV excesses with synthetic model spectra, and find that the (FUV − NUV) versus

can be fitted with a linear relation and late-type dwarfs tend to have high UV excesses. There are 87,178 and 1,498,103 stars detected more than once in the visit exposures of GALEX in the FUV and NUV, respectively. We make use of the quantified photometric errors to determine statistical properties of the UV variation, including intrinsic variability and the structure function on the timescale of days. The overall occurrence of possible false positives is below 1.3% in our sample. UV absolute magnitudes are calculated for stars with valid parallaxes, which could serve as a possible reference frame in the NUV. We conclude that the colors related to UV provide good criteria to distinguish between M giants and M dwarfs, and the variability of RR Lyrae stars in our sample is stronger than that of other A and F stars.
Evaluation of facial artery perforator-based flaps in reconstruction of facial defects
Authors: Guha Goutam , Chatterjee Dipmalya , Biswas Siddhartha , Das Kaushik , Bhattacharya Rupnarayan , Sarkar Tapan 
Published: March 2018

ABSTRACT
Introduction: Several flaps have been described for reconstructing facial or oral defects. Flaps such as forehead and pectoralis major are often too bulky for small-to-moderate-sized defects, for which nasolabial flaps are often ideal. However, nasolabial flaps have limited mobility and reach and may need two stages, particularly for intraoral defects. According to recent literatures, facial artery provides numerous small cutaneous perforators, based on which skin flaps can be islanded, with greater mobility and reach for reconstruction of small-to-moderate-sized intraoral and facial defects in one stage. Our study aims to evaluate the reliability and versatility of facial artery perforator-based flaps in the reconstruction of such defects. Materials and Methods: A ethical committee-approved retrospective study was conducted on data of the patients attending our outpatient department between February 2014 and October 2015 with small-to-moderate-sized facial/oral lesions. The total sample size was 23. We studied the relation of flap survival with size of flap, route of inset and neck dissection, functional and aesthetic outcomes and feasibility of adjuvant therapy in cases of malignancies. Results and Analysis: A wide range of facial defects, especially intraoral defects, could be reconstructed in one stage using facial artery perforator-based flaps. The flaps were reliable. Complications included only partial skin loss of the flaps in a few cases. Complications were directly related to the length of the flaps and the route of inset. Functional and aesthetic outcomes were satisfactory and none of the flaps showed any significant post-radiotherapy changes. Conclusions: We concluded that facial artery perforator flap can be a simple, safe, versatile and one-stage alternative to the traditional flaps in the reconstruction of small-to-moderate-sized facial defects. Neck dissection can be safely done in the same sitting.
Evaluation of stratospheric age of air from CF4, C2F6, C3F8, CHF3, HFC-125, HFC-227ea and SF6; implications for the calculations of halocarbon lifetimes, fractional release factors and ozone depletion potentials
Authors: Leedham Elvidge Emma C. , Bönisch Harald , Brenninkmeijer Carl A. M. , Engel Andreas , Fraser Paul J. , Gallacher Eileen , Langenfelds Ray , Mühle Jens , Oram David E. , Ray Eric A. , Ridley Anna R. , Röckmann Thomas , Sturges William T. , Weiss Ray F. , Laube Johannes C. 
Published: March 2018

Abstract. In a changing climate, potential stratospheric circulation changes require long-term monitoring. Stratospheric trace gas measurements are often used as a proxy for stratospheric circulation changes via the mean age of air values derived from them. In this study, we investigated five potential age of air tracers – the perfluorocarbons CF4, C2F6 and C3F8 and the hydrofluorocarbons CHF3 (HFC-23) and HFC-125 – and compare them to the traditional tracer SF6 and a (relatively) shorter-lived species, HFC-227ea. A detailed uncertainty analysis was performed on mean ages derived from these new tracers to allow us to confidently compare their efficacy as age tracers to the existing tracer, SF6. Our results showed that uncertainties associated with the mean age derived from these new age tracers are similar to those derived from SF6, suggesting that these alternative compounds are suitable in this respect for use as age tracers. Independent verification of the suitability of these age tracers is provided by a comparison between samples analysed at the University of East Anglia and the Scripps Institution of Oceanography. All five tracers give younger mean ages than SF6, a discrepancy that increases with increasing mean age. Our findings qualitatively support recent work that suggests that the stratospheric lifetime of SF6 is significantly less than the previous estimate of 3200 years. The impact of these younger mean ages on three policy-relevant parameters – stratospheric lifetimes, fractional release factors (FRFs) and ozone depletion potentials – is investigated in combination with a recently improved methodology to calculate FRFs. Updates to previous estimations for these parameters are provided.
Working Towards a Culturally Competent Practice with Mexican Immigrants
Authors: Laser-Maira Julie Anne , Campos Elsa 
Published: March 2018

In this politically charged times, the plight of Mexican immigrants have been incorrectly characterized and ridiculed. We believe clinicians need to better understand who they are and how to become culturally competent to work effectively with Mexican immigrants. The United Nations High Commissioner for Refugees (1951) defines a political refugee as “a person who owing to a well-founded fear of being persecuted for reasons of race, religion, nationality, membership of a particular social group, or political opinion, is outside the country of his nationality, and is unable to or, owing to such fear, is unwilling to avail himself of the protection of that country…” In contrast, an economic refugee is a person seeking refugee status in another country for economic reasons. With political refugee status comes both legal and financial support by the U.S. government. However, an economic refugee is not afforded such opportunities. In the United States, there are 660,477 political refugees (Dovidio & Esses, 2001), additionally, it is estimated that there are five to eight million economic refugees who are without legal documents (Yakushko & Chronister, 2005). It is believed that of this five to eight million economic refugees, 95% are from Mexico (Yakushko & Chronister). This translates to 4,750,000 to 7,600,000 Mexican economic refugees. Though U.S. legislation has tried to control the number of economic refugees entering the country and expel economic refugees already living within its borders, the reality is that great majority of the 4,750,000 to 7,600,000 individuals are gainfully employed and will probably stay in the United States until they have earned sufficient money to be able to return to Mexico and survive economic deprivation. With such staggering numbers of economic refugees seeking the opportunity to make a living within the United States, it is becoming increasingly important to address the mental health needs of such individuals. Although federal policy often dictates the exclusion of funding opportunities for services to economic refugees, the reality is that there is an ethical responsibility to provide services to all individuals despite legal status or country of origin.
Vertrouwen in het ontslag
Authors: Beltzer Ronald 
Published: March 2018

Het ontslagrecht in het regeerakkoord
In dit artikel gaat de auteur in op de in het regeerakkoord 2017 voorgestelde maatregelen ten aanzien van ontslag. Voorts gaat hij in op het recent verschenen wetsvoorstel ten aanzien van payrolling.
Constar Plastics: aanzegging of opzegging – overgangsrecht en opvolgend werkgeverschap
Authors: Palm Steven 
Published: March 2018

Constar Plastics: aanzegging of opzegging – overgangsrecht en opvolgend werkgeverschap
Dit artikel bespreekt de uitspraak van de Hoge Raad inzake Constar Plastics. De Hoge Raad beantwoordt twee vragen. (i) Kan een schriftelijke aanzegging als bedoeld in artikel 7:668 lid 1 BW onder omstandigheden als een opzegging van de werkgever worden beschouwd? (ii) Welke maatstaf voor opvolgend werkgeverschap geldt bij een werkgeverswissel die plaatsvond voor 1 juli 2015? Het artikel bevat een nadere analyse van de beslissing van de Hoge Raad en beschrijft de (proces)rechtelijke consequenties van deze uitspraak voor de rechtspraktijk.
Próba uporządkowania polskiego nazewnictwa bambusów przydatnych do uprawy w rodzimych warunkach klimatycznych
Authors: Hoser Szymon , Hoser Wojciech , Nawrocka Katarzyna 
Published: March 2018

Próba uporządkowania polskiego nazewnictwa bambusów przydatnych do uprawy w rodzimych warunkach klimatycznych
W Polsce, w wyniku wzrostu popularności bambusów, zaczynają funkcjonować potoczne nazwy dla najczęściej uprawianych gatunków. W efekcie tego spontanicznie postępującego procesu pojawiają się zarówno liczne nazwy oboczne w odniesieniu do pojedynczych taksonów, jak i błędne formy nazewnicze. Celem niniejszej publikacji jest uporządkowanie powstającego polskiego nazewnictwa bambusów. Opracowanie obejmuje taksony o największym znaczeniu, wybrane na podstawie przydatności do uprawy w warunkach klimatycznych Polski, występowania w polskojęzycznych publikacjach i tematycznych stronach internetowych oraz obecności w ofertach krajowych szkółek i centrów ogrodniczych. Dla omawianych taksonów sformułowano polskie nazwy w oparciu o etymologię, dotychczasowe propozycje nazewnicze i cechy dystynktywne roślin. Zestawienie obejmuje 43 gatunki należące do 9 rodzajów z plemienia <em>Bambuseae</em>, spośród których najliczniej reprezentowane są tu rodzaje <em>Phyllostachys</em> (23 taksony), <em>Fargesia</em> (7 taksonów) i <em>Sasa</em> (4 taksony).
An attempt to settle Polish names for bamboos useful for cultivation in the local climate
As a result of the growing popularity of bamboos in Poland, common names for the most often cultivated species are beginning to be used. As a result of this spontaneous process, many double as well as wrong names appear according to one taxa. The purpose of this publication is to organize Polish names for bamboos. The most important taxa have been chosen. As selection criteria were taken: usefulness for cultivation in the Polish climate conditions, occurrence in Polish language publications and thematic web sites, and presence in offer of Polish nurseries and garden centers. For this selection Polish names have been formulated in consideration of etymology, so far suggested nomenclature and distinctive features. The article includes 43 species belonging to 9 genera from Bambuseae tribe. Most represented are <em>Phyllostachys</em> (23 taxa), <em>Fargesia</em> (7 taxa), and <em>Sasa</em> (4 taxa).