bluuebunny/crossref_metadata_2025_split huggingface dataset:
Analisa pengaruh sakit tenggorokan terhadap perubahan spektrum suara
Authors: Sutono Sutono , Setiawan Hendra , Amrullah Yusuf Aziz 
Published: September 2018

ABSTRACTBackground: Voice is a kind of sound produced by friction or vibration of objects. In humans vocal cords in throat are used to produce voice and the produced voice may have different frequency. Human voice in a kind of a sound created by several organ, such as lungs, laryngs, pharynx, nasal cavity, moulth cavity, moulth and tongue. The existence of those organs will inluance the produced voice. Pharingitis is one of upper channel infection. Objective: To condact a analysis on the human voice because of sore throat, get a list of alphabeth that experience the biggest caused by sore throat, and to recognise the possibility of throat disorder seen by the analysis of frequency spectrum. Method: The research is conducted by comparing the voice result post paryngistis and after being recoved. The research uses fourier transformation to compare the produced pattern by using MSE ( Mean Square Error). The researcher tested 7 respondents. Result: The result shows that there is influence towards the resulted voice. The Alphabeths that experiances the biggest disorder are A (MSE:0,094677), M (MSE:0,072883), L (MSE:0,095975), Z (MSE:0,07552), X (MSE:0,07602) dan K (MSE:0,119209), it can be concluded that each respondent has different alphabeth disorder.
Pemetaan Ergonomi pada Proses Pembuatan Batik
Authors: Rofiatun Rofiatun , Hasanbasri Mubasysyir 
Published: September 2018

The use of non-standard work equipment, inadequate working environment, and health conditions that are poorly monitored by health services are a problem experienced by workers in the informal sector. Ergonomic risks arising from faulty work positions, unsafe workplaces and low knowledge of occupational safety and health. The process of making batik done manually, with long working hours and work postures that are not safe and comfortable. This study aimed to analyze the work posture with the level of ergonomic risk in the batik home-based worker as well as preventive and promotive efforts made by health workers. The research was conducted qualitatively, with in-depth interview method and observation. Triangulation is done to obtain objective information. The ergonomic risk level analysis is done using the Rapid Entire Body Assessment (REBA) method. measurement of work posture done in batik making process obtained REBA score as follows, score 2-4 for waxing or nyanthing, score 7 for coloring process, score 4 and 8 for rinsing process and score 5 for process wax release. Ergonomic risk in the process of batik in the category of medium, medium category for colouring, medium and high category for rinsing process, and medium category for wax release, and still low preventive and promotive efforts made by health workers.
Radioterapi pada Tatalaksana Tumor Wilms
Authors: Sutedja Tirawan , Supriana Nana 
Published: September 2018

Wilms’ tumor atau nefroblastoma merupakan keganasan ginjal tersering pada anak. Insidensinya mencapai 6% dari seluruh kasus keganasan pada anak. Gejala klinis pada mayoritas kasus Wilms’ tumor berupa asimtompatik massa pada abdomen, namun 20-30 persen dari kasus memberikan gejala nyeri abdomen, malaise, atau hematuria mikroskopik ataupun makroskopik. Gambaran umum dari Wilms’ tumor adalah adanya pseudocapsule yang mengelilingi tumor. Modalitas terapi untuk Wilms’ tumor adalah pembedahan, kemoterapi, dan terapi radiasi. Pembedahan merupakan tatalaksana terpenting dan prosedur operasi yang dijalankan dengan akurat dapat menentukan staging Wilms’ tumor dengan tepat serta rencana tatalaksana selanjutnya. Kemoterapi merupakan terapi ajuvan utama pasca radiasi ataupun terapi preoperatif. Radiasi eksterna merupakan terapi ajuvan pada Wilms’ tumor dengan stadium lanjut. Gabungan kemoterapi dan radiasi eksterna memberikan hasil yang lebih baik. Namun demikian patut diperhatikan efek samping kombinasi kedua modalitas terapi tersebut. Mengingat toksisitas jangka panjang, peran radiasi eksterna masih terbatas dan hanya diberikan dengan dosis yang relatif rendah.
Co-Immobilization of pullulanase, glucoamylase and glucose isomerase together with cross-linked enzyme aggregates: Fructose conversion from three enzymes and starch in one step
Authors: AKKOÇ Yakup , TÜKEL S. Seyhan 
Published: September 2018

In this study, in order
to obtain fructose syrup from starch, pullulanase (PUL), glucoamylase (GA) and
glucose isomerase (GI) were immobilized together with cross-linked enzyme
aggregates (CLEAs), and named as 'combi-CLEAs'. The values of Vmaxand Kmfrom
the kinetic parameters of combi-CLEAs [(GA + PUL) + GI] were found as 12 U g-1 and 0.1157 mg ml-1
in optimum conditions, respectively. After
50 uses, it was observed that the remaining activity of combi-CLEAs [GA + PUL +
GI] was preserved at 46%. The thermal stability of combi-CLEAs
[GA + PUL) + GI] was observed to be 44% and 30%, respectively, at 60 and 80 ° C
after 24 hours. At the end of 30 days, the
storage stabilities of combi-CLEAs [(GA + PUL) + GI] was determined as 56% and
13% at the temperatures of 4 and 25°C, respectively.
Aggression towards the GP: can we profile the GP–victim? A cross-section survey among GPs
Authors: Demeur Vince , Devos Sarah , Jans Esther , Schoenmakers Birgitte 
Published: September 2018

BackgroundAggression against GPs has increased in the past decade. Depending on experience, interpretation, and personality, the interpretation of aggressive patient behaviour will differ among doctors.AimTo investigate how often GPs experience aggression in a 1-year time span and what the relationship is between the GP's personality (based on the 'Big Five' personality traits) and the reporting of aggression. Secondly, to investigate how personality is related to feeling safe.Design & settingFlemish (Belgian Federal State) GPs were questioned in a cross-sectional design by online survey. GPs were recruited and questioned in their professional environment.MethodOutcome measures were the 'Big Five' personality traits ('reserved' versus 'outgoing', 'compassionate' versus 'challenging', 'efficient' versus 'careless', 'confident' versus 'nervous', and 'cautious' versus 'innovative', based on Cattel's 'Big Five' model of personality), the type of aggression, the reporting of aggression, and feeling safe.ResultsBoth (n= 247) male and female doctors considered physical contact and verbal intimidation as aggression. Female doctors were more likely to consider sexual harassment as aggression. The majority of GPs were confronted with verbal aggression. More than half considered physical aggression as the most threatening. GPs with 'reserved' and 'careless' personality types were more likely to experience aggression. GPs with 'innovative', 'challenging', or 'confident' personality types were also at increased risk, but to a lesser extent than those with 'reserved' and 'careless' personalities. GPs with 'efficient' and 'innovative' personalities were more likely to report incidents. Male GPs and those with 'efficient' personalities felt safer. GPs with 'confident' and 'cautious' personalities were more likely to feel unsafe.ConclusionThe results of this study might help future interventions and support strategies (designed to prevent aggressive incidents or help GPs cope with them) to target the vulnerable groups. Further research should therefore explore the results of these data in depth and on a larger sample size.
Etude stratigraphique et sédimentologique de l'Aquitanien de la Calanque du Petit Nid (Sausset, Bouches-du-Rhône, France). Découverte d'un squelette d'Halitherium Kaup
Authors: Anglada Roger , Arnaud Michel , Catzigras France , Colomb Emile , Delcourt André , Maurel-Ferrandini Michelle 
Published: September 2018

Ce travail, entrepris à la suite de la découverte d'un squelette Halitherium, présente une étude stratigraphique et sédimentologique de l'Aquitanien dans un nouveau secteur du littoral de la Nerthe.
Des corrélations sont proposées avec la coupe de Carry-le-Rouet, qui pourrait être utilisée comme coupe auxiliaire de référence du stratotype de l'Aquitanien.
La plate-forme carbonatée de Gavrovo-Tripolitza (Grèce) : évolution des conditions de sédimentation au cours du Mesozoïque
Authors: Bernier Paul , Fleury Jean-Jacques 
Published: September 2018

Les 3 000 m de carbonates de la période Jurassique supérieur (Kimméridgien-Portlandien) -Crétacé terminal du domaine du Gavrovo font l'objet d'une étude qui précise les conditions de leur dépôt. Dans des faciès constamment peu profonds, on distingue :
-une période d'oscillations régulières (milieux subtidaux à supratidaux) pendant le Jurassique supérieur-Crétacé inférieur ;
-une période "régressive" (milieux intertidaux à supratidaux) cénomano-turonienne ;
-une période d'approfondissement (milieu subtidal) turono-sénonienne ;
-une période régressive (fréquents phénomènes de diagenèse à l'émersion et remaniements) accompagnant un dérèglement de l'équilibre subsidence-sédimentation à la fin du Crétacé. Cette dernière période est annonciatrice de la phase tectonique finicrétacée-éotertiaire qui gouverne la sédimentation éocène.
Cette évolution est comparée à celle du domaine adjacent de Tripolitza qui fut le siège d'une subsidence probablement plus faible sous une tranche d'eau un peu plus forte.
La plate-forme carbonatée de Gavrovo-Tripolitza a connu une évolution de type bahamien qui lui confère une étroite parenté avec les "plates-formes carbonatées périadriatiques" avec lesquelles elle constitue un élément important de la plaque d'Apulie.
Les Diatomées des saumures des marais salants de Salin-de-Giraud (Sud de la France)
Authors: Noël Denise 
Published: September 2018

In this study of Diatoms, brines of the salt works have been examined from sea water at Beauduc pumps to the ultime brines (400 g/1 after halite deposition). Filtrations on millipore filters (or Sartorius membranes) have been used to take stock of Diatoms. 37 taxa have been identified which are illustrated by SEM pictures and for which ecological data from literature are recalled.
From an ecological point of view, the following conclusions can be summarized. 1. Diatoms can thrive up to a salinity of 130 g/1. 2. Marine species found in the sea at the entrance of the salt works disappear as soon as oversalinity increases and do not adjust themselves. 3. There are only Pennales which are epiphytic or benthic forms,' may be because of the shallowness of the pans and the drying of some of them in winter. 4. Most of the Diatoms found in the brines are holoeuryhaline species which can bear salinities over as well as under normal marine salinity. It is worthy to point out that some of these Diatoms are known in Messinian pre-or intra-evaporitic laminites. 5. Diversity is low for the whole salt works and this diversity decreases when salinity increases. There is a tendency for the species to replace each other as the salinity increases and three associations can be mentioned : Cocconeis bardawilensis association (up to 60 g/1) ; Amphora coffeaeformis association (up to 90 g/1) ; Nitzschia sigma association (up to 130 g/1).
From a sedimentological point of view, the data show that the Diatoms play an important role in the cycle of silica both in brines and interstitial waters.
Interactions bryozoaires-sédiment dans les environnements actuels et fossiles
Authors: Moissette Pierre 
Published: September 2018

Parmi les facteurs écologiques qui conditionnent la vie des bryozoaires, la nature du substrat et le taux de sédimentation sont particulièrement importants. Les formes zoariales, ou formes de croissance des colonies, ainsi que le plus ou moins grand développement des assemblages à bryozoaires en dépendent étroitement.
Les bryozoaires agissent à leur tour sur le sédiment en intervenant à titre principal ou accessoire dans divers types de constructions, de concrétions et d'accumulations.
The application of a Late Burdigalian -Early Langhian Highstand Event in correlating complex Tertiary orogenic carbonate successions within the Central Mediterranean
Authors: Grasso M. , Pedley Martyn , Maniscalco R. 
Published: September 2018

Utilisation d'un Haut-Niveau Marin du Burdigalien supérieur-Langhien inférieur pour correler des successions carbonatées cenozoïques en contexte orogénique, en Méditerranée centrale.
Les rampes carbonatées tertiaires du SE de la Sicile contiennent un remarquable niveau durci, phosphaté, dans les rampes externes autour des villes de Donnalucata et Sampieri. Dans les autres secteurs les phosphorites apparaissent seulement en grains allochtones associées latéralement à des packstones et des grainstones à stratifications obliques et structures de tempêtes. Les phosphorites sont contenues dans un ensemble tabulaire de wackestones de milieu pélagique. Le banc situé au dessous est daté du Burdigalien terminal alors que le banc du dessus contient un assemblage de Foraminifères planctoniques du Burdigalien terminal-Langhien inférieur. Cet exemple d'événement eustatique et bien d'autres marqués sur le plateau ibléen par des onlaps illustrent un signal eustatique global tant en mer profonde qu'en domaine littoral de plate-forme stable. A une plus grande échelle, les événements eustatiques, peuvent influencer la sédimentation marine même dans les légions à tectonique active. C'est le cas des calcarénites de Floresta dans les Monts Péloritains au NE de la Sicile. Le même événement eustatique est également reconnu dans le Sud des Apennines sur la bordure calabro-lucanienne et dans le Nord des Apennines. Nous interprétons tous ces événements en terme de offlap-onlap en relation avec l'événement eustatique mondial TE 2.3 (HAQ et al., 1987 ; HAQ 1991) nouvellement reconnu en Méditerranée. La reconnaissance de cet événement offlap-onlap un peu partout en Méditerranée en fait un outil performant non seulement pour la compréhension lithostratigraphique des régions à tectonique complexe mais aussi pour le calibrage des événements tectoniques.
Les séries du Dogger moyen du Haut Adas au Nord d'Errachidia (Maroc) : lithostratigraphie et sédimentologie d'une nouvelle formation : la formation Tazigzaout
Authors: Ait Addi A. 
Published: September 2018

L'étude stratigraphique et sédimentologique des faciès du Dogger moyen du Haut Atlas marocain au Nord d'Errachidia permet d'individualiser une nouvelle formation nommée formation Tazigzaout. Ses équivalents, dans le Haut Atlas central, sont les formations Bin el Ouidane 2 et 3, Ait Abdi 2 et Assoul 1. Une révision des corrélations stratigraphiques (locales et régionales) en relation avec l'évolution géodynamique du bassin s'avérait nécessaire.
Dans le domaine distal septentrional de notre zone d'étude, la formation Tazigzaout attribuée au Bajocien-Bathonien pp., est bien individualisée et empli le synclinal de Tazigzaout formant l'axe du grand synclinal perché du jebel Boukendil formé par les termes sommitaux de la formation Agoudim sous-jacente. Chacune de ces deux formations montre une évolution de type "shallowing-upward" et apparaît coiffée par des barres carbonatées à monticules bioconstruits. Leurs équivalents latéraux en domaine de plate-forme sud sont très délicats à déterminer. Toutefois, sur la base de données sédimentologiques et paléontologiques nous avons pu distinguer ces deux formations et établir de proche en proche des corrélations entre les faciès qui les composent.
Medium-sized Satellites of Large Kuiper Belt Objects
Authors: Brown Michael E. , Butler Bryan J. 
Published: September 2018

Abstract
While satellites of mid- to small-Kuiper Belt objects tend to be similar in size and brightness to their primaries, the largest Kuiper Belt objects preferentially have satellites with small fractional brightness. In the two cases where the sizes and albedos of the small faint satellites have been measured, these satellites are seen to be small icy fragments consistent with collisional formation. Here, we examine Dysnomia and Vanth, the satellites of Eris and Orcus, respectively. Using the Atacama Large Millimeter Array, we obtain the first spatially resolved observations of these systems at thermal wavelengths. Vanth is easily seen in individual images, and we find a 3.5σ detection of Dysnomia by stacking all of the data on the known position of the satellite. We calculate a diameter for Dysnomia of 700 ± 115 km and for Vanth of 475 ± 75 km, with albedos of

and 0.08 ± 0.02, respectively. Both Dysnomia and Vanth are indistinguishable from typical Kuiper Belt objects of their size. Potential implications for the formation of these types of satellites are discussed.
The Location and Environments of Neutron Star Mergers in an Evolving Universe
Authors: Wiggins Brandon K. , Fryer Christopher L. , Smidt Joseph M. , Hartmann Dieter , Lloyd-Ronning Nicole , Belcynski Chris 
Published: September 2018

Abstract
The simultaneous detection of gravitational and electromagnetic waves from a binary neutron star merger has both solidified the link between neutron star mergers and short-duration gamma-ray bursts (GRBs), and demonstrated the ability of astronomers to follow-up the gravitational wave detection to place constraints on the ejecta from these mergers, as well as the nature of the GRB engine and its surroundings. As the sensitivity of aLIGO and VIRGO increases, it is likely that a growing number of such detections will occur in the next few years, leading to a sufficiently large number of events to constrain the populations of these GRB events. While long-duration GRBs originate from massive stars and thus are located near their stellar nurseries, binary neutron stars may merge on much longer timescales, and thus may have had time to migrate appreciably. The strength and character of the electromagnetic afterglow emission of binary neutron star mergers is a sensitive function of the circum-merger environment. Though the explosion sites of short GRBs have been explored in the literature, the question has yet to be fully addressed in its cosmological context. We present cosmological simulations following the evolution of a galaxy cluster, including star formation combined with binary population synthesis models, to self-consistently track the locations and environmental gas densities of compact binary merger sites throughout the cosmic web. We present probability distributions for densities as a function of redshift and discuss model sensitivity to population synthesis model assumptions.
Probing Star Formation in Galaxies at z ≈ 1 via a Giant Metrewave Radio Telescope Stacking Analysis
Authors: Bera Apurba , Kanekar Nissim , Weiner Benjamin J. , Sethi Shiv , Dwarakanath K. S. 
Published: September 2018

Abstract
We report deep Giant Metrewave Radio Telescope (GMRT) 610 MHz continuum imaging of four subfields of the DEEP2 Galaxy Redshift Survey. We stacked the radio emission in the GMRT images from a near-complete (absolute blue magnitude M
B ≤ −21) sample of 3698 blue star-forming galaxies with redshifts 0.7 ≲ z ≲ 1.45 to detect (at ≈17σ significance) the median rest-frame 1.4 GHz radio continuum emission of the sample galaxies. The stacked emission is unresolved, with a rest-frame 1.4 GHz luminosity of L
1.4GHz = (4.13 ± 0.24) × 1022 W Hz−1. We used the local relation between total star formation rate (SFR) and 1.4 GHz luminosity to infer a median total SFR of (24.4 ± 1.4) M
⊙ yr−1 for blue star-forming galaxies with M
B ≤ −21 at 0.7 ≲ z ≲ 1.45. We detect the main-sequence relation between SFR and stellar mass, M
⋆, obtaining SFR = (13.4 ± 1.8) × [(M
⋆/1010
M
⊙)]0.73±0.09
M
⊙ yr−1; the power-law index shows no change over z ≈ 0.7–1.45. We find that the nebular line emission suffers less extinction than the stellar continuum, contrary to the situation in the local universe; the ratio of nebular extinction to stellar extinction increases with decreasing redshift. We obtain an upper limit of 0.87 Gyr to the atomic gas depletion time of a subsample of DEEP2 galaxies at z ≈ 1.3; neutral atomic gas thus appears to be a transient phase in high-z star-forming galaxies.
The Hard State of the Highly Absorbed High Inclination Black Hole Binary Candidate Swift J1658.2–4242 Observed by NuSTAR and Swift
Authors: Xu Yanjun , Harrison Fiona A. , Kennea Jamie A. , Walton Dominic J. , Tomsick John A. , Miller Jon M. , Barret Didier , Fabian Andrew C. , Forster Karl , Fürst Felix , Gandhi Poshak , García Javier A. 
Published: September 2018

Abstract
We present a spectral and timing analysis of the newly reported Galactic X-ray transient Swift J1658.2–4242 observed by Nuclear Spectroscopic Telescope Array (NuSTAR) and Swift. The broadband X-ray continuum is typical of a black hole binary in the bright hard state, with a photon index of Γ = 1.63 ± 0.02 and a low coronal temperature of kT
e = 22 ± 1 keV, corresponding to a low spectral cutoff well constrained by NuSTAR. Spectral modeling of the relativistic disk reflection features, consisting of a broad Fe Kα line and the Compton reflection hump, reveals that the black hole is rapidly spinning with the spin parameter of a* > 0.96, and the inner accretion disk is viewed at a high inclination angle of

(statistical errors, 90% confidence). The high inclination is independently confirmed by dips in the light curves, which can be explained by absorbing material located near the disk plane temporarily obscuring the central region. In addition, we detect an absorption line in the NuSTAR spectra centered at

keV. If associated with ionized Fe K absorption lines, this provides evidence for the presence of outflowing material in the low/hard state of a black hole binary candidate. A timing analysis shows the presence of a type-C quasi-periodic oscillation in the power spectrum, with the frequency increasing from ∼0.14 to ∼0.21 Hz during the single NuSTAR exposure. Our analysis reveals that Swift J1658.2–4242 displays characteristics typical for a black hole binary that is viewed at a high inclination angle, making it a good system for studying the accretion geometry in black hole binaries.
Dark Structures in Sunspot Light Bridges
Authors: Zhang Jingwen , Tian Hui , Solanki Sami K. , Wang Haimin , Peter Hardi , Ahn Kwangsu , Xu Yan , Zhu Yingjie , Cao Wenda , He Jiansen , Wang Linghua 
Published: September 2018

Abstract
We present unprecedented high-resolution TiO images and Fe i 1565 nm spectropolarimetric data of two light bridges taken by the 1.6 m Goode Solar Telescope at Big Bear Solar Observatory. In the first light bridge (LB1), we find striking knot-like dark structures within the central dark lane. Many dark knots show migration away from the penumbra along the light bridge. The sizes, intensity depressions, and apparent speeds of their proper motion along the light bridges of 33 dark knots identified from the TiO images are mainly in the ranges of 80 ∼ 200 km, 30% ∼ 50%, and 0.3 ∼ 1.2 km s−1, respectively. In the second light bridge (LB2), a faint central dark lane and striking transverse intergranular lanes were observed. These intergranular lanes have sizes and intensity depressions comparable to those of the dark knots in LB1 and also migrate away from the penumbra at similar speeds. Our observations reveal that LB2 is made up of a chain of evolving convection cells, as indicated by patches of blueshift surrounded by narrow lanes of redshift. The central dark lane generally corresponds to blueshifts, supporting the previous suggestion of central dark lanes being the top parts of convection upflows. In contrast, the intergranular lanes are associated with redshifts and located at two sides of each convection cell. The magnetic fields are stronger in intergranular lanes than in the central dark lane. These results suggest that these intergranular lanes are manifestations of convergent convective downflows in the light bridge. We also provide evidence that the dark knots observed in LB1 may have a similar origin.