bluuebunny/crossref_metadata_2025_split huggingface dataset:
DAMPAK PENERAPAN TEKNOLOGI INFORMASI ELECTRONIC DATA INTERCHANE TERHADAP KINERJA PERUSAHAAN FORWARDING
Authors: Sunaryo Agus 
Published: February 2017

Electronic Data Interchane (EDI) is combination of computer technologogy and electronic which com help us to communication and serving document trafficbetween two side or more with the same time in fast and accurate. Mi – Trans Logistic corporation who starting to use EDI in its business operation, received a lot gains, Al thought in start its needed great investment and the up grade of the human resources. The gains are: repare the data lack; less paper and loose the face to face amount with customer because the document manufactured by the electronic so that be data will received efficiency and time efectivy, increase serving to consument beside that. The EDI impact are the custom document serving is easier and faste,. where before EDI it need stime 4 – 5 days, now can served only less 3 days, and the important thing is the image from the customer if the company are developed and bonafide and prestice.
Toward the complete control of brain metastases using surveillance screening and stereotactic radiosurgery
Authors: Wolf Amparo , Kvint Svetlana , Chachoua Abraham , Pavlick Anna , Wilson Melissa , Donahue Bernadine , Golfinos John G. , Silverman Joshua , Kondziolka Douglas 
Published: February 2017

OBJECTIVEThe incidence of brain metastases is increasing with improved systemic therapies, many of which have a limited impact on intracranial disease. Stereotactic radiosurgery (SRS) is a first-line management option for brain metastases. The purpose of this study was to determine if there is a threshold tumor size below which local control (LC) rates approach 100%, and to relate these findings to the use of routine surveillance brain imaging.METHODSFrom a prospective registry, 200 patients with 1237 brain metastases were identified who underwent SRS between December 2012 and May 2015. The median imaging follow-up duration was 7.9 months, and the median margin dose was 18 Gy. The maximal diameter and volume of tumors were measured. Histological analysis included 96 patients with non–small cell lung cancers (NSCLCs), 40 with melanoma, 35 with breast cancer, and 29 with other histologies.RESULTSAlmost 50% of brain metastases were NSCLCs and commonly measured less than 6 mm in maximal diameter or 70 mm3 in volume. Thirty-three of 1237 tumors had local progression at a median of 8.8 months. The 1- and 2-year actuarial LC rates were 97% and 93%, respectively. LC of 100% was achieved for all intracranial metastases less than 100 mm3 in volume or 6 mm in diameter. Patients whose tumors at first SRS were less than 10 mm maximal diameter or a volume of 250 mm3 had improved overall survival.CONCLUSIONSSRS can achieve LC rates approaching 100% for subcentimeter metastases. The earlier initial detection and prompt treatment of small intracranial metastases may prevent the development of neurological symptoms and the need for resection, and improve overall survival. To identify tumors when they are small, routine surveillance brain imaging should be considered as part of the standard of care for lung, breast, and melanoma metastases.■ CLASSIFICATION OF EVIDENCE Type of question: prognostic; study design: retrospective cohort; evidence: Class II.
The first formulation of image-based stereotactic principles: the forgotten work of Gaston Contremoulins
Authors: Giller Cole A. , Mornet Patrick , Moreau Jean-François 
Published: February 2017

Although image-based human stereotaxis began with Spiegel and Wycis in 1947, the major principles of radiographic stereotaxis were formulated 50 years earlier by the French scientific photographer Gaston Contremoulins. In 1897, frustrated by the high morbidity of bullet extraction from the brain, the Parisian surgeon Charles Rémy asked Contremoulins to devise a method for bullet localization using the then new technology of x-rays. In doing so, Contremoulins conceived of many of the modern principles of stereotaxis, including the use of a reference frame, radiopaque fiducials for registration, images to locate the target in relation to the frame, phantom devices to locate the target in relation to the fiducial marks, and the use of an adjustable pointer to guide the surgical approach.Contremoulins' ideas did not emerge from science or medicine, but instead were inspired by his training in the fine arts. Had he been a physician instead of an artist, he might have never discovered his extraordinary methods.Contremoulins' “compass” and its variants enjoyed great success during World War I, but were abandoned by 1920 for simpler methods. Although Contremoulins was one of the most eminent radiographers in France, he was not a physician, and his personality was uncompromising. By 1940, both he and his methods were forgotten. It was not until 1988 that he was rediscovered by Moreau while reviewing the history of French radiology, and chronicled by Mornet in his extensive biography.The authors examine Contremoulins' stereotactic methods in historical context, describe the details of his devices, relate his discoveries to his training in the fine arts, and discuss how his prescient formulation of stereotaxis was forgotten for more than half a century.
Risk of failure in pediatric ventriculoperitoneal shunts placed after abdominal surgery
Authors: Burks Joshua D. , Conner Andrew K. , Briggs Robert G. , Glenn Chad A. , Bonney Phillip A. , Cheema Ahmed A. , Chen Sixia , Gross Naina L. , Mapstone Timothy B. 
Published: February 2017

OBJECTIVEExperience has led us to suspect an association between shunt malfunction and recent abdominal surgery, yet information about this potential relationship has not been explored in the literature. The authors compared shunt survival in patients who underwent abdominal surgery to shunt survival in our general pediatric shunt population to determine whether such a relationship exists.METHODSThe authors performed a retrospective review of all cases in which pediatric patients underwent ventriculoperitoneal shunt operations at their institution during a 7-year period. Survival time in shunt operations that followed abdominal surgery was compared with survival time of shunt operations in patients with no history of abdominal surgery. Univariate and multivariate analyses were used to identify factors associated with failure.RESULTSA total of 141 patients who underwent 468 shunt operations during the period of study were included; 107 of these 141 patients had no history of abdominal surgery and 34 had undergone a shunt operation after abdominal surgery. Shunt surgery performed more than 2 weeks after abdominal surgery was not associated with time to shunt failure (p = 0.86). Shunt surgery performed within 2 weeks after abdominal surgery was associated with time to failure (adjusted HR 3.6, 95% CI 1.3–9.6).CONCLUSIONSUndergoing shunt surgery shortly after abdominal surgery appears to be associated with shorter shunt survival. When possible, some patients may benefit from shunt placement utilizing alternative termini.
Brainstem arteriovenous malformations: lesion characteristics and treatment outcomes
Authors: Madhugiri Venkatesh S. , Teo Mario K. C. , Vavao Joli , Bell-Stephens Teresa , Steinberg Gary K. 
Published: February 2017

OBJECTIVEBrainstem arteriovenous malformations (AVMs) are rare lesions that are difficult to diagnose and treat. They are often more aggressive in their behavior when compared with their supratentorial counterparts. The consequence of a brainstem hemorrhage is often devastating, and many patients are in poor neurological status at presentation. The authors examine the factors associated with angiographically confirmed cure and those affecting management outcomes for these complex lesions.METHODSThis was a retrospective analysis of data gathered from the prospectively maintained Stanford AVM database. Lesions were grouped based on their location in the brainstem (medulla, pons, or midbrain) and the quadrant they occupied. Angiographic cure was dichotomized as completely obliterated or not, and functional outcome was dichotomized as either independent or not independent at last follow-up.RESULTSOver a 23-year period, 39 lesions were treated. Of these, 3 were located in the medulla, 14 in the pons, and 22 in the midbrain. At presentation, 92% of the patients had hemorrhage, and only 43.6% were functionally independent. Surgery resulted in the best radiographic cure rates, with a morbidity rate of 12.5%. In all, 53% of patients either improved or remained stable after surgery. Absence of residual nidus and female sex correlated with better outcomes.CONCLUSIONSBrainstem AVMs usually present with hemorrhage. Surgery offers the best chance of cure, either in isolation or in combination with other modalities as appropriate.
Prometheus: Analyzing WebInject-based information stealers
Authors: Continella Andrea , Carminati Michele , Polino Mario , Lanzi Andrea , Zanero Stefano , Maggi Federico 
Published: February 2017

Nowadays Information stealers are reaching high levels of sophistication. The number of families and variants observed increased exponentially in the last years. Furthermore, these trojans are sold on underground markets along with automatic frameworks that include web-based administration panels, builders and customization procedures. From a technical point of view such malware is equipped with a functionality, called WebInject, that exploits API hooking techniques to intercept all sensitive data in a browser context and modify web pages on infected hosts. In this paper we propose Prometheus, an automatic system that is able to analyze trojans that base their attack technique on DOM modifications. Prometheus is able to identify the injection operations performed by malware, and generate signatures based on the injection behavior. Furthermore, it is able to extract the WebInject targets by using memory forensic techniques. We evaluated Prometheus against real-world, online websites and a dataset of distinct variants of financial trojans. In our experiments we show that our approach correctly recognizes known variants of WebInject-based malware and successfully extracts the WebInject targets.
Virtual and augmented reality in the treatment of phantom limb pain: A literature review
Authors: Dunn Justin , Yeo Elizabeth , Moghaddampour Parisah , Chau Brian , Humbert Sarah 
Published: February 2017

BACKGROUND: Phantom limb pain (PLP), the perception of discomfort in a limb no longer present, commonly occurs following amputation. A variety of interventions have been employed for PLP, including mirror therapy. Virtual Reality (VR) and augmented reality (AR) mirror therapy treatments have also been utilized and have the potential to provide an even greater immersive experience for the amputee. However, there is not currently a consensus on the efficacy of VR and AR therapy. OBJECTIVE: The aim of this review is to evaluate and summarize the current research on the effect of immersive VR and AR in the treatment of PLP. METHODS: A comprehensive literature search was conducted utilizing PubMed and Google Scholar in order to collect all available studies concerning the use of VR and/or AR in the treatment of PLP using the search terms “virtual reality,” “augmented reality,” and “phantom limb pain.” Eight studies in total were evaluated, with six of those reporting quantitative data and the other two reporting qualitative findings. RESULTS: All studies located were of low-level evidence. Each noted improved pain with VR and AR treatment for phantom limb pain, through quantitative or qualitative reporting. Additionally, adverse effects were limited only to simulator sickness occurring in one trial for one patient. CONCLUSIONS: Despite the positive findings, all of the studies were confined purely to case studies and case report series. No studies of higher evidence have been conducted, thus considerably limiting the strength of the findings. As such, the current use of VR and AR for PLP management, while attractive due to the increasing levels of immersion, customizable environments, and decreasing cost, is yet to be fully proven and continues to need further research with higher quality studies to fully explore its benefits.
La propriété immobilière est-elle un obstacle pour sortir du chômage ?
Authors: Brunet Carole , Havet Nathalie , Lesueur Jean-Yves 
Published: February 2017

Does Homeownership Hinder Exits from Unemployment ?
This study uses microeconomic data to test “ Oswald’s hypothesis”, which postulates a link between rising homeownership rates and longer unemployment spells. We contribute to the existing literature by contrasting econometric results for France and the United States, whose labour and housing markets function and interact in very different ways. Using unemployment-spell samples from the French part of the European Community Household Panel and the Panel Study of Income Dynamics, both covering 1994-2001, we estimate mixed proportional hazard models incorporating simultaneous behaviours in the housing and labour markets. Ourmain results indicate that homeownership is not significantly related to longer unemployment spells in the United States, while French homeowners exhibit faster re-employment rates than renters.
A Principal Component Analysis of the Diffuse Interstellar Bands
Authors: Ensor T. , Cami J. , Bhatt N. H. , Soddu A. 
Published: February 2017

Abstract
We present a principal component (PC) analysis of 23 line-of-sight parameters (including the strengths of 16 diffuse interstellar bands, DIBs) for a well-chosen sample of single-cloud sightlines representing a broad range of environmental conditions. Our analysis indicates that the majority (∼93%) of the variations in the measurements can be captured by only four parameters The main driver (i.e., the first PC) is the amount of DIB-producing material in the line of sight, a quantity that is extremely well traced by the equivalent width of the λ5797 DIB. The second PC is the amount of UV radiation, which correlates well with the λ5797/λ5780 DIB strength ratio. The remaining two PCs are more difficult to interpret, but are likely related to the properties of dust in the line of sight (e.g., the gas-to-dust ratio). With our PCA results, the DIBs can then be used to estimate these line-of-sight parameters.
Formation and Assembly History of Stellar Components in Galaxies as a Function of Stellar and Halo Mass
Authors: Lee Jaehyun , Yi Sukyoung K. 
Published: February 2017

Abstract
Galaxy mass assembly is an end product of structure formation in the ΛCDM cosmology. As an extension of Lee & Yi, we investigate the assembly history of stellar components in galaxies as a function of halo environments and stellar mass using semi-analytic approaches. In our fiducial model, halo mass intrinsically determines the formation and assembly of the stellar mass. Overall, the ex situ fraction slowly increases in central galaxies with increasing halo mass but sharply increases for

. A similar trend is also found in satellite galaxies, which implies that mergers are essential to build stellar masses above

. We also examine the time evolution of the contribution of mass growth channels. Mergers become the primary channel in the mass growth of central galaxies when their host halo mass begins to exceed

. However, satellite galaxies seldom reach the merger-dominant phase despite their reduced star-formation activities due to environmental effects.
Molecular Gas Kinematics and Star Formation Properties of the Strongly-lensed Quasar Host Galaxy RXS J1131–1231
Authors: Leung T. K. Daisy , Riechers Dominik A. , Pavesi Riccardo 
Published: February 2017

Abstract
We report observations of CO(J = 2 → 1) and

line emission toward the quadruply-lensed quasar RXS J1131−1231 at z = 0.654 obtained using the Plateau de Bure Interferometer (PdBI) and the Combined Array for Research in Millimeter-wave Astronomy (CARMA). Our lens modeling shows that the asymmetry in the double-horned CO(J = 2 → 1) line profile is mainly a result of differential lensing, where the magnification factor varies from ∼3 to ∼9 across different kinematic components. The intrinsically symmetric line profile and a smooth source-plane velocity gradient suggest that the host galaxy is an extended rotating disk, with a CO size of

kpc and a dynamical mass of

M
⊙. We also find a secondary CO-emitting source near RXS J1131−1231, the location of which is consistent with the optically-faint companion reported in previous studies. The lensing-corrected molecular gas masses are M
gas = (1.4 ± 0.3) × 1010
M
⊙ and (2.0 ± 0.1) × 109
M
⊙ for RXS J1131−1231 and the companion, respectively. We find a lensing-corrected stellar mass of M
* = (3 ± 1) × 1010
M
⊙ and a star formation rate of SFRFIR = (120 ± 63) M
⊙ yr−1, corresponding to a specific SFR and star formation efficiency comparable to z ∼ 1 disk galaxies not hosting quasars. The implied gas mass fraction of ∼18 ± 4% is consistent with the previously observed cosmic decline since z ∼ 2. We thus find no evidence for quenching of star formation in RXS J1131−1231. This agrees with our finding of an elevated

ratio of >0.27

% compared to the local value, suggesting that the bulk of its black hole mass is largely in place while its stellar bulge is still assembling.
Shock–Cloud Interaction in the Solar Corona
Authors: Takahashi Takuya 
Published: February 2017

Abstract
Flare-associated coronal shock waves sometimes interact with solar prominences, leading to large-amplitude prominence oscillations (LAPOs). Such prominence activation gives us a unique opportunity to track the time evolution of shock–cloud interaction in cosmic plasmas. Although the dynamics of interstellar shock–cloud interaction has been extensively studied, coronal shock–solar prominence interaction is rarely studied in the context of shock–cloud interaction. Associated with the X5.4 class solar flare that occurred on 2012 March 7, a globally propagated coronal shock wave interacted with a polar prominence, leading to LAPO. In this paper, we studied bulk acceleration and excitation of the internal flow of the shocked prominence using three-dimensional magnetohydrodynamic (MHD) simulations. We studied eight MHD simulation runs, each with different mass density structure of the prominence, and one hydrodynamic simulation run, and we compared the result. In order to compare the observed motion of activated prominence with the corresponding simulation, we also studied prominence activation by injection of a triangular-shaped coronal shock. We found that the prominence is first accelerated mainly by magnetic tension force as well as direct transmission of the shock, and later decelerated mainly by magnetic tension force. The internal flow, on the other hand, is excited during the shock front sweeps through the prominence and damps almost exponentially. We construct a phenomenological model of bulk momentum transfer from the shock to the prominence, which agreed quantitatively with all the simulation results. Based on the phenomenological prominence activation model, we diagnosed physical parameters of the coronal shock wave. The estimated energy of the coronal shock is several percent of the total energy released during the X5.4 flare.
13CO/C18O Gradients across the Disks of Nearby Spiral Galaxies
Authors: Jiménez-Donaire María J. , Cormier Diane , Bigiel Frank , Leroy Adam K. , Gallagher Molly , Krumholz Mark R. , Usero Antonio , Hughes Annie , Kramer Carsten , Meier David , Murphy Eric , Pety Jérôme , Schinnerer Eva , Schruba Andreas , Schuster Karl , Sliwa Kazimierz , Tomicic Neven 
Published: February 2017

Abstract
We use the IRAM Large Program EMPIRE and new high-resolution ALMA data to measure 13CO(1-0)/C18O(1-0) intensity ratios across nine nearby spiral galaxies. These isotopologues of 12CO are typically optically thin across most of the area in galaxy disks, and this ratio allows us to gauge their relative abundance due to chemistry or stellar nucleosynthesis effects. Resolved 13CO/C18O gradients across normal galaxies have been rare due to the faintness of these lines. We find a mean 13CO/C18O ratio of 6.0 ± 0.9 for the central regions of our galaxies. This agrees well with results in the Milky Way, but differs from results for starburst galaxies (3.4 ± 0.9) and ultraluminous infrared galaxies (1.1 ± 0.4). In our sample, the 13CO/C18O ratio consistently increases with increasing galactocentric radius and decreases with increasing star formation rate surface density. These trends could be explained if the isotopic abundances are altered by fractionation; the sense of the trends also agrees with those expected for carbon and oxygen isotopic abundance variations due to selective enrichment by massive stars.
A Common Origin of Magnetism from Planets to White Dwarfs
Authors: Isern Jordi , García-Berro Enrique , Külebi Baybars , Lorén-Aguilar Pablo 
Published: February 2017

Abstract
Isolated magnetic white dwarfs have field strengths ranging from kilogauss to gigagauss. However, the origin of the magnetic field has not been hitherto elucidated. Whether these fields are fossil, hence the remnants of original weak magnetic fields amplified during the course of the evolution of their progenitor stars, or are the result of binary interactions, or, finally, they are produced by other internal physical mechanisms during the cooling of the white dwarf itself, remains a mystery. At sufficiently low temperatures, white dwarfs crystallize. Upon solidification, phase separation of its main constituents, 12C and 16O, and of the impurities left by previous evolution occurs. This process leads to the formation of a Rayleigh–Taylor unstable liquid mantle on top of a solid core. This convective region, as it occurs in solar system planets like the Earth and Jupiter, can produce a dynamo able to yield magnetic fields of strengths of up to 0.1 MG, thus providing a mechanism that could explain magnetism in single white dwarfs.
The study of customer relationship management in Thai airline industry: A case of Thai travelers in Thailand
Authors: Law Colin 
Published: February 2017

Purpose: This paper offer marketing strategy suggestion to the airlines operating within the Thai aviation market. It identifies the recommended motivational factors that influence the airline customers’ decision to their airline choices. Airlines use different customer relationship management programs to attract returning customers. This paper suggested the most attractive motivation factors for Thailand's air travel market.Design/methodology/approach: This research paper is an attempt to study and identify the factors, including loyalty program, distribution channel, customer services, promotions and other influence causes that affected the customer preference in the airline ticket purchasing behavior in Thailand.A questionnaire survey was conducted with the sample identified through unrestricted non probability sampling technique at four major airports in Thailand. The data collected are analyzed to identify the favorable drivers that lead to customer decision on airline choice.Findings: The result from the study has demonstrated that price, and promotion has a significant impact on customer preference and positively leads to repurchase intention for their future travel. Moreover, flight schedules are also a main factor influencing the travelers’ final decision on airline choice. However, when the promotional strategies and schedule are comparable between airlines, customers are attracted by the airline amenities and services. Loyalty program (frequent-flier program flier program) is showing a less attractive motivator while distribution channel demonstrates the least important affecting the travelers’ choice of airline.Originality/value: The paper begins with an overview of previous research in the area of airlines customer relationship management and then moves on to what is currently being implemented by the airlines. The authors then propose several customer relationship strategies and identify the most attractive one that motivates the Thai consumers.