bluuebunny/crossref_metadata_2025_split huggingface dataset:
SHAPING OF SECURITY POLICY IN AN INDONESIAN BANK: INTERPRETING INSTITUTIONALIZATION AND STRUCTURATION
Authors: Nasution M. Faisal , Dhillon Gurpreet , Akyuwen Roberto 
Published: February 2017

Studi ini meneliti pembentukan kebijakan keamanan pada sebuah bank di Indonesia dengan menggunakanÂ teori institusional dan struktural sebagai kerangka teoritis. Penelitian mengenai keamanan sistem informasipada umumnya kurang memperhatikan aspek-aspek sosial dalam perancangan dan pelaksanaan kebijakanÂ keamanan. Penelitian ini menggunakan studi kasus dengan sebuah bank pemerintah di Indonesia sebagaiÂ unit analisis. Kasus ini dipilih karena terjadinya peristiwa penjebolan sistem keamanan pada saat penelitianÂ ini dilakukan. Studi kasus ini membahas mengenai bagaimana kebijakan keamanan dibentuk dan pelajaranÂ penting apa saja yang dapat ditarik dari sudut pandang teori institusional dan stukturasi. Hasil penelitian iniÂ menunjukkan peranan penting dari sebuah desain sistem yang baik dan bagaimana faktor-faktor sosial dan politikÂ dipertimbangkan ketika merencanakan kebijakan keamanan. Kontribusi yang diberikan oleh hasil penelitian ini,antara lain adalah, menunjukkan bagaimana teori institusional dapat digunakan untuk menjelaskan bagaimanaÂ kekuatan institusional mempengaruhi desain dan penggunaan kebijakan keamanan.Kata Kunci: keamanan dan privasi sistem informasi, kebijakan keamanan, teori institusional, teori strukturasi
Measuring Disease Severity in Duchenne and Becker Muscular Dystrophy
Authors: Davis Melinda F. , Scherer Katalin H. , Miller Timothy M. , Meaney F. John 
Published: February 2017

Medical investigations use a wide variety of outcome indicators that are often not comparable. It can be challenging to integrate results across multiple studies that do not share a common metric. Some conditions such as Duchenne and Becker muscular dystrophy have a predictable course of disease progression. Severity can be inferred from a patient's medical history. This paper describes the development of a disease severity measure using common markers of disease progression. Rasch modeling was used to estimate severity using dichotomous events that indicate disease progression. Caregivers of 34 young men with Duchenne or Becker muscular dystrophy completed structured interviews about their care and medical history. Interview questions included surgeries (tendon release, scoliosis, tracheostomy), respiratory equipment (assisted ventilation, cough assist devices), and the use of other medical equipment (e.g., braces, walkers, wheelchairs, transfer boards, hospital beds). The resulting measure had a reliability of .83. The correlation between the severity measure and the Amyotrophic Lateral Sclerosis Functional Rating Scale (ALSFRS) was .68. Preliminary results and item calibrations are provided for the severity measure that can be estimated from caregiver reports or administrative data. DOI:10.2458/azu_jmmss_v1i1_davis
Pharmacokinetics of meloxicam after intramuscular and oral administration of a single dose to American flamingos (Phoenicopertus ruber)
Authors: Boonstra Jennifer L. , Cox Sherry K. , Martin-Jimenez Tomas 
Published: February 2017

Abstract
OBJECTIVE To determine pharmacokinetics after IM and oral administration of a single dose of meloxicam to American flamingos (Phoenicopertus ruber).
ANIMALS 14 adult flamingos.
PROCEDURES Flamingos were allocated to 2 groups. Each group received a dose of meloxicam (1 mg/kg) by the IM or oral route. After a 4-week washout period, groups received meloxicam via the other route of administration. Plasma meloxicam concentrations were measured with high-performance liquid chromatography. Data for each bird were analyzed. Estimated values of selected pharmacokinetic parameters were compared by use of a linear mixed-effects ANOVA. Pooled concentration-time profiles for each route of administration were analyzed to examine the influence of body weight on pharmacokinetics.
RESULTS Mean ± SD maximum plasma concentration was 1.00 ± 0.88 μg/mL after oral administration. This was approximately 15% of the mean maximum plasma concentration of 5.50 ± 2.86 μg/mL after IM administration. Mean time to maximum plasma concentration was 1.33 ± 1.32 hours after oral administration and 0.28 ± 0.17 hours after IM administration. Mean half-life of the terminal phase after oral administration (3.83 ± 2.64 hours) was approximately twice that after IM administration (1.83 ± 1.22 hours).
CONCLUSIONS AND CLINICAL RELEVANCE Results indicated that the extent and rate of meloxicam absorption were less after oral administration than after IM administration. Intramuscular administration resulted in a short period during which mean plasma concentrations met or exceeded reported efficacious analgesic concentrations in other species, whereas oral administration did not. These results suggested that higher doses may be required for oral administration.
Effect of cold storage on immediate graft function in an experimental model of renal transplantation in cats
Authors: Csomos Rebecca A. , Hardie Robert J. , Schmiedt Chad W. , Delaney Fern A. , McAnulty Jonathan F. 
Published: February 2017

Abstract
OBJECTIVE To assess the effect of cold storage (CS) on immediate posttransplantation function of renal autografts in cats.
ANIMALS 15 healthy 1-year-old cats.
PROCEDURES Cats were assigned to 2 groups and underwent autotransplantation of the left kidney followed by nephrectomy of the right kidney. The left kidney was autotransplanted either immediately (IT group; n = 6) or after being flushed with a cold sucrose phosphate solution and stored on ice while the implant site was prepared (CS group; 9). Serum creatinine and BUN concentrations were monitored daily and autografts were ultrasonographically examined intermittently for 14 days after surgery.
RESULTS Mean duration of CS was 24 minutes for the CS group. Posttransplantation serum creatinine and BUN concentrations for the CS group had lower peak values, returned to the respective reference ranges quicker, and were generally significantly lower than those for the IT group. Mean posttransplantation autograft size for the CS group was smaller than that for the IT group.
CONCLUSIONS AND CLINICAL RELEVANCE Results indicated that immediate posttransplantation function of renal autografts following a short period of CS was better than that of renal autografts that did not undergo CS, which suggested CS protected grafts from ischemic injury and may decrease perioperative complications, speed recovery, and improve the long-term outcome for cats with renal transplants.
IMPACT FOR HUMAN MEDICINE Cats metabolize immunosuppressive drugs in a manner similar to humans; therefore, renal transplantation in cats may serve as a desirable model for investigating the effects of renal transplantation in human patients.
Cardiorespiratory function in Thoroughbreds during locomotion on a treadmill at an incline or decline
Authors: Ohmura Hajime , Mukai Kazutaka , Takahashi Toshiyuki , Aida Hiroko , Jones James H. 
Published: February 2017

Abstract
OBJECTIVE To determine cardiorespiratory responses of Thoroughbreds to uphill and downhill locomotion on a treadmill at identical gradients.
ANIMALS 5 highly trained Thoroughbred geldings.
PROCEDURES Thoroughbreds were exercised for 2-minute intervals on a treadmill at 1.7, 3.5, 6.0, 8.0, and 10.0 m/s at a 4% incline, 0% incline (horizontal plane), and 4% decline in random order on different days. Stride frequency, stride length, and cardiopulmonary and O2-transport variables were measured and analyzed by means of repeated-measures ANOVA and Holm-Šidák pairwise comparisons.
RESULTS Horses completed all treadmill exercises with identical stride frequency and stride length. At identical uphill speeds, they had higher (vs horizontal) mass-specific O2 consumption (mean increase, 49%) and CO2 production (mean increase, 47%), cardiac output (mean increase, 21%), heart rate (mean increase, 11%), and Paco2 (mean increase, 1.7 mm Hg), and lower Pao2 (mean decrease, 5.8 mm Hg) and arterial O2 saturation (mean decrease, 1.0%); tidal volume was not higher. Downhill locomotion (vs horizontal) reduced mass-specific O2 consumption (mean decrease, 24%), CO2 production (mean decrease, 23%), and cardiac output (mean decrease, 9%). Absolute energy cost during uphill locomotion increased linearly with speed at approximately twice the rate at which it decreased during downhill locomotion.
CONCLUSIONS AND CLINICAL RELEVANCE Findings suggested that for Thoroughbreds, downhill locomotion resulted in a lower energy cost than did horizontal or uphill locomotion and that this cost changed with speed. Whether eccentric training induces skeletal muscle changes in horses similar to those in humans remains to be determined.
EPIC 219388192b—An Inhabitant of the Brown Dwarf Desert in the Ruprecht 147 Open Cluster
Authors: Nowak Grzegorz , Palle Enric , Gandolfi Davide , Dai Fei , Lanza Antonino F. , Hirano Teruyuki , Barragán Oscar , Fukui Akihiko , Bruntt Hans , Endl Michael , Cochran William D. , Moroni Pier G. Prada , Prieto-Arranz Jorge , Kiilerich Amanda , Nespral David , Hatzes Artie P. , Albrecht Simon , Deeg Hans , Winn Joshua N. , Yu Liang , Kuzuhara Masayuki , Grziwa Sascha , Smith Alexis M. S. , Guenther Eike W. , Eylen Vincent Van , Csizmadia Szilard , Fridlund Malcolm , Cabrera Juan , Eigmüller Philipp , Erikson Anders , Korth Judith , Narita Norio , Pätzold Martin , Rauer Heike , Ribas Ignasi 
Published: February 2017

Abstract
We report the discovery of EPIC 219388192b, a transiting brown dwarf in a 5.3 day orbit around a member star of Ruprecht 147, the oldest nearby open cluster association, which was photometrically monitored by K2 during its Campaign 7. We combine the K2 time-series data with ground-based adaptive optics imaging and high-resolution spectroscopy to rule out false positive scenarios and determine the main parameters of the system. EPIC 219388192b has a radius of

R
Jup and mass of

M
Jup, yielding a mean density of

. The host star is nearly a solar twin with mass

M
⊙, radius

R
⊙, effective temperature T
eff = 5850 ± 85 K, and iron abundance [Fe/H] = 0.03 ± 0.08 dex. Its age, spectroscopic distance, and reddening are consistent with those of Ruprecht 147, corroborating its cluster membership. EPIC 219388192b is the first mature brown dwarf with precise determinations of mass, radius, and age, and serves as benchmark for evolutionary models in the substellar regime.
K2-60b and K2-107b. A Sub-Jovian and a Jovian Planet from the K2 Mission
Authors: Eigmüller Philipp , Gandolfi Davide , Persson Carina M. , Donati Paolo , Fridlund Malcolm , Csizmadia Szilard , Barragán Oscar , Smith Alexis M. S. , Cabrera Juan , Korth Judith , Grziwa Sascha , Prieto-Arranz Jorge , Nespral David , Saario Joonas , Cochran William D. , Cusano Felice , Deeg Hans J. , Endl Michael , Erikson Anders , Guenther Eike W. , Hatzes Artie P. , Pätzold Martin , Rauer Heike 
Published: February 2017

Abstract
We report the characterization and independent detection of K2-60b, as well as the detection and characterization of K2-107b, two transiting hot gaseous planets from the K2 space mission. We confirm the planetary nature of the two systems and determine their fundamental parameters combining the K2 time-series data with FIES@NOT and HARPS-N@TNG spectroscopic observations. K2-60b has a radius of 0.683 ± 0.037 R
Jup and a mass of 0.426 ± 0.037 M
Jup and orbits a G4 V star with an orbital period of 3.00267 ± 0.00006 days. K2-107b has a radius of 1.44 ± 0.15 R
Jup and a mass of 0.84 ± 0.08 M
Jup and orbits an F9 IV star every 3.31392 ± 0.00002 days. K2-60b is among the few planets at the edge of the so-called “desert” of short-period sub-Jovian planets. K2-107b is a highly inflated Jovian planet orbiting an evolved star about to leave the main sequence.
Seven-year Collection of Well-monitored Fermi-LAT Gamma-Ray Burst Afterglows
Authors: Panaitescu A. 
Published: February 2017

Abstract
We present the light curves and spectra of 24 afterglows that have been monitored by Fermi-LAT at 0.1–100 GeV over more than a decade. All light curves (except 130427) are consistent with a single power law starting from their peaks, which occur in most cases before the burst end. The light curves display a brightness–decay rate correlation, with all but one (130427) of the bright afterglows decaying faster than the dimmer afterglows. We attribute this dichotomy to the quick deposition of relativistic ejecta energy in the external shock for the brighter/faster-decaying afterglows and to an extended energy injection in the afterglow shock for the dimmer/slower-decaying light curves. The spectra of six afterglows (090328, 100414, 110721, 110731, 130427, 140619B) indicate the existence of a harder component above a spectral dip or ankle at energies of 0.3–3 GeV, offering evidence for inverse-Compton emission at higher energies and suggesting that the harder power-law spectra of five other LAT afterglows (130327B, 131231, 150523, 150627, 160509) could also be inverse-Compton, while the remaining, softer LAT afterglows should be synchrotron emission. Marginal evidence for a spectral break and softening at higher energies is found for two afterglows (090902B and 090926).
Dust Radiative Transfer Modeling of the Infrared Ring around the Magnetar SGR 1900+14
Authors: Natale G. , Rea N. , Lazzati D. , Perna R. , Torres D. F. , Girart J. M. 
Published: February 2017

Abstract
A peculiar infrared ring-like structure was discovered by Spitzer around the strongly magnetized neutron star SGR 1900+14. This infrared (IR) structure was suggested to be due to a dust-free cavity, produced by the Soft Gamma-ray Repeaters (SGRs) Giant Flare occurring in 1998, and kept illuminated by surrounding stars. Using a 3D dust radiative transfer code, we aimed to reproduce the emission morphology and the integrated emission flux of this structure assuming different spatial distributions and densities for the dust, and different positions for the illuminating stars. We found that a dust-free ellipsoidal cavity can reproduce the shape, flux, and spectrum of the ring-like IR emission, provided that the illuminating stars are inside the cavity and that the interstellar medium has high gas density (n
H ∼ 1000 cm−3). We further constrain the emitting region to have a sharp inner boundary and to be significantly extended in the radial direction, possibly even just a cavity in a smooth molecular cloud. We discuss possible scenarios for the formation of the dustless cavity and the particular geometry that allows it to be IR-bright.
Propagation Characteristics of Two Coronal Mass Ejections from the Sun Far into Interplanetary Space
Authors: Zhao Xiaowei , Liu Ying D. , Hu Huidong , Wang Rui 
Published: February 2017

Abstract
Propagation of coronal mass ejections (CMEs) from the Sun far into interplanetary space is not well understood, due to limited observations. In this study we examine the propagation characteristics of two geo-effective CMEs, which occurred on 2005 May 6 and 13, respectively. Significant heliospheric consequences associated with the two CMEs are observed, including interplanetary CMEs (ICMEs) at the Earth and Ulysses, interplanetary shocks, a long-duration type II radio burst, and intense geomagnetic storms. We use coronagraph observations from SOHO/LASCO, frequency drift of the long-duration type II burst, in situ measurements at the Earth and Ulysses, and magnetohydrodynamic propagation of the observed solar wind disturbances at 1 au to track the CMEs from the Sun far into interplanetary space. We find that both of the CMEs underwent a major deceleration within 1 au and thereafter a gradual deceleration when they propagated from the Earth to deep interplanetary space, due to interactions with the ambient solar wind. The results also reveal that the two CMEs interacted with each other in the distant interplanetary space even though their launch times on the Sun were well separated. The intense geomagnetic storm for each case was caused by the southward magnetic fields ahead of the CME, stressing the critical role of the sheath region in geomagnetic storm generation, although for the first case there is a corotating interaction region involved.
Connection between Stellar Mass Distributions within Galaxies and Quenching Since z = 2
Authors: Mosleh Moein , Tacchella Sandro , Renzini Alvio , Carollo C. Marcella , Molaeinezhad Alireza , Onodera Masato , Khosroshahi Habib G. , Lilly Simon 
Published: February 2017

Abstract
We study the history from

to

of the stellar mass assembly of quiescent and star-forming galaxies in a spatially resolved fashion. For this purpose, we use multi-wavelength imaging data from the Hubble Space Telescope (HST) over the GOODS fields and the Sloan Digital Sky Survey (SDSS) for the local population. We present the radial stellar mass surface density profiles of galaxies with

, corrected for mass-to-light ratio (

/L) variations, and derive the half-mass-radius (R

m
), central stellar mass surface density within 1 kpc (

) and surface density at R

m
(

) for star-forming and quiescent galaxies and study their evolution with redshift. At fixed stellar mass, the half-mass sizes of quiescent galaxies increase from

to

by a factor of

, whereas the half-mass sizes of star-forming galaxies increase only slightly, by a factor of ∼2. The central densities

of quiescent galaxies decline slightly (by a factor of

) from

to

, while for star-forming galaxies

increases with time, at fixed mass. We show that the central density

has a tighter correlation with specific star-formation rate (sSFR) than

and for all masses and redshifts galaxies with higher central density are more prone to be quenched. Reaching a high central density (

) seems to be a prerequisite for the cessation of star formation, though a causal link between high

and quenching is difficult to prove and their correlation can have a different origin.
Broad-lined Supernova 2016coi with a Helium Envelope
Authors: Yamanaka Masayuki , Nakaoka Tatsuya , Tanaka Masaomi , Maeda Keiichi , Honda Satoshi , Hanayama Hidekazu , Morokuma Tomoki , Imai Masataka , Kinugasa Kenzo , Murata Katsuhiro L. , Nishimori Takefumi , Hashimoto Osamu , Gima Hirotaka , Hosoya Kensuke , Ito Ayano , Karita Mayu , Kawabata Miho , Morihana Kumiko , Morikawa Yuto , Murakami Kotone , Nagayama Takahiro , Ono Tatsuharu , Onozato Hiroki , Sarugaku Yuki , Sato Mitsuteru , Suzuki Daisuke , Takahashi Jun , Takayama Masaki , Yaguchi Hijiri , Akitaya Hiroshi , Asakura Yuichiro , Kawabata Koji S. , Kuroda Daisuke , Nogami Daisaku , Oasa Yumiko , Omodaka Toshihiro , Saito Yoshihiko , Sekiguchi Kazuhiro , Tominaga Nozomu , Uemura Makoto , Watanabe Makoto 
Published: February 2017

Abstract
We present the early-phase spectra and the light curves of the broad-lined (BL) supernova (SN) 2016coi from t = 7 to 67 days after the estimated explosion date. This SN was initially reported as a BL Type SN Ic (SN Ic-BL). However, we found that spectra up to t = 12 days exhibited the He i
λ5876, λ6678, and λ7065 absorption lines. We show that the smoothed and blueshifted spectra of normal SNe Ib are remarkably similar to the observed spectrum of SN 2016coi. The line velocities of SN 2016coi were similar to those of SNe Ic-BL and significantly faster than those of SNe Ib. Analyses of the line velocity and light curve suggest that the kinetic energy and the total ejecta mass of SN 2016coi are similar to those of SNe Ic-BL. Together with BL SNe 2009bb and 2012ap, for which the detection of He i was also reported, these SNe could be transitional objects between SNe Ic-BL and SNe Ib, and be classified as BL Type “Ib” SNe (SNe “Ib”-BL). Our work demonstrates the diversity of the outermost layer in BL SNe, which should be related to the variety of the evolutionary paths.
Telaprevir-Containing Triple Therapy in Acute HCV Coinfection: The CHAT Study
Authors:   the CHAT study group, Boesecke Christoph , Singh Gurmit K Jagjit , Scholten Stefan H-A , Lutz Thomas , Baumgarten Axel , Schneeweiss Stephan M , Trein Andreas , Rausch Michael , Ingiliz Patrick , Rockstroh Jürgen K , Nelson Mark 
Published: February 2017

Background No published randomized controlled data on the use of direct-acting antivirals (DAA) in acute hepatitis C (AHC) coinfection exist. However, with the AHC epidemic ongoing among men who have sex with men (MSM) these are urgently needed. Methods The CHAT study is a randomized controlled trial of pegylated interferon + ribavirin (PR) plus telaprevir (TVR) for 12–24 weeks versus PR alone for 24–48 weeks in the response-guided treatment of patients with AHC genotype (GT) 1 infection and HIV-1 coinfection in Germany and Great Britain. Results 34 patients were included: 15 were randomized to the PR arm (arm 1), 19 to the TVR + PR arm (arm 2). All patients were MSM, median age was 40 years. 55% had IL28B C/C GT. Median baseline HCV RNA was 291,227 IU/ml, median alanine aminotransferase was 105 U/l. 85% received cART, all had baseline HIV RNA <40 copies/ml. Overall sustained virological response (SVR12) rate was 79.4% (27/34). SVR12 was seen in 12/15 (80%) in arm 1 and in 15/19 (79.8%) in arm 2. Of the four patients without SVR in arm 2, one experienced viraI breakthrough, two were non-responders; in one case HCV protease inhibitor (PI)-associated mutations were selected under TVR (V36M, R155K). Conclusions Due to moderate response rates and additional toxicities 1st generation HCV PIs should not be used in treating acute HCV. While not being licensed, recent study data and guidelines support the use of dual DAA therapy but optimal treatment duration in acute HCV needs further investigation.
Correlation between Soil Transmitted Helminth Infection and Eosinophil Levels among Primary School Children in Medan
Authors: Darlan Dewi Masyithah , Tala Zaimah Z. , Amanta Cellya , Warli Syah Mirsya , Arrasyid Nurfida Khairina 
Published: February 2017

BACKGROUND: Soil Transmitted Helminth infection is one of most prevalent health problems worldwide, especially in environments with poor sanitation. Based on World Health Organisation (WHO) data, more than 2 billion people, or 24% of the world's population, are infected with intestinal parasite. The highest prevalence is located in areas of poor sanitation and unsafe water supplies. In Indonesia, the prevalence of parasite infections is 15% of the entire population.AIM: The purpose of this study was to determine the relationship between Soil Transmitted Helminth infection on levels of eosinophils among primary school children. In addition, this study also aimed to determine the prevalence of different types of worm infections and the levels of eosinophils in children infected with worms.MATERIAL AND METHODS: This study was analytic observational using a cross-sectional method. The sampling technique was consecutive and in total 132 samples was obtained. The study involved primary school children in Amplas Medan and Hamparan Perak, Deli Serdang through May to October 2016. Univariate analysis was performed to determine STH infection prevalence and bivariate analysis was used to find the correlation between STH infection and eosinophil levels through a Chi square (X2) test. Â RESULTS: The results showed that the prevalence of Soil Transmitted Helminth was 7.6%. The most common types of STH infection were 3.8% with Trichuris trichiura and 3% with Ascaris lumbricoides. A significant correlation was found between Parasite infection and eosinophil levels (Contingency Coefficient (C) = 0.2, X2 = 5.3, p = 0.021) and the risk of STH infection that caused eosinophilia or increased eosinophil levels in the children with a Prevalence Ratio (PR) of 1.56 (Confidence Interval (CI) 95%: 1.10-2.22).CONCLUSION: It is recommended that schools at similar risk improve and maintain hygiene and healthy behaviour in the school environment and that parents and teachers pay greater attention to the cleanliness of their children.