bluuebunny/crossref_metadata_2025_split huggingface dataset:
Role of Local Press in Conflicts: A Case Study of Editorial’ Contents of Daily Chand and Daily Shamal during Militancy in district Swat, Pakistan
Authors: Ud Din Jamal , Ul Amin Khan Rooh , Khan Khalid 
Published: September 2017

The study "Role of Local Press in Conflict: A Case Study of Editorial' Contents of Daily Chand and Daily Shamal during Militancy in district Swat, Pakistan" is basically a comparison of editorials, being published on the issue of militancy in both the local dailies of Swat to analyze that how these dailies treated government and militants’ agendas in their editorials. This study was conducted by content analysis of editorials of Daily Chand and Daily Shamal, publishing from district Swat while the media hegemony theory was applied as theoretical frame work for conducting the study. The findings made it clear that both the dailies had been given more coverage to militants' agenda, the ruling class during the unrest, than government agenda. Daily Chand had written total 84 editorials on the issue of militancy, it wrote 12 (14 percent) editorials against government but not a single editorial had been written against militants. Besides the daily had given only 06 percent supportive coverage to government agenda by publishing 05 editorials while the paper had, however, given more supportive coverage to militants by publishing 17 editorials in favor of their agenda with 20 percent of its total editorials, being published on the issue of militancy. Similarly daily Shamal had written 61 editorials on issue of militancy and of them only three editorials had been written with percentage of 05 percent in support of government agenda while it published two editorials in favor of militants' agenda, which reflect 03 percent of the total editorials, being written on the issue of militancy. Daily Shamal wrote o8 editorials (13 percent) against the provincial government, but it did not write even a single editorial to oppose militants' agenda or their any kind of act, meant to challenge writ of the government in district Swat, Pakistan.
Digital Engagement, Political and Civic Participation
Authors: Samsuddin Jamali , Hasan Hamisah , Ching Lai Che 
Published: September 2017

Objective: This paper examines the digital engagement, political and civic participation among Malaysian youth in marginalized communities. It also studies the relationship between digital engagement and two participation constructs. The framework of the study was based on mobilization theories, which suggested that previously unavailable technologies such as the Internet could mobilize members of underprivileged or underrepresented groups who lack socioeconomic resources. Methodology: The data were obtained through a self-administered survey completed by 4,107 youths, aged from 15 to 25 years old, living in marginalized communities in six regions, namely Central, Eastern, Northern, Southern, Sabah, and Sarawak. Descriptive and factor analyses were used to analyze the data. Pearson correlation was also run to test the hypothesis that digital engagement is positively related to political and civic participation. Results: The study found that while youths were digitally engaged, their engagement was still characterized by basic use of the Internet, such as communicating with friends. The study also found that their civic and political participation is low. However, the research found that digital engagement had a significant and positive impact on the youths' political and civic participation. Implication: This research provides empirical data on the level of digital engagement, political and civic participation among Malaysian youths. The study expands on current literatures by examining the effects of Internet on youth participation. This paper offers insights to policy makers on implementing strategies and programs that promote participation among youth in marginalized communities. Its practical implication also includes contributing towards the development of specific policy and good practices on media to encourage youth participation in Malaysia.
Frontal and occipital horn ratio is associated with multifocal intraparenchymal hemorrhages in neonatal shunted hydrocephalus
Authors: Oushy Soliman , Parker Jonathon J. , Campbell Kristen , Palmer Claire , Wilkinson Corbett , Stence Nicholas V. , Handler Michael H. , Mirsky David M. 
Published: September 2017

OBJECTIVEPlacement of a cerebrospinal fluid diversion device (i.e., shunt) is a routine pediatric neurosurgical procedure, often performed in the first weeks of life for treatment of congenital hydrocephalus. In the postoperative period, shunt placement may be complicated by subdural, catheter tract, parenchymal, and intraventricular hemorrhages. The authors observed a subset of infants and neonates who developed multifocal intraparenchymal hemorrhages (MIPH) following shunt placement and sought to determine any predisposing perioperative variables.METHODSA retrospective review of the electronic medical record at a tertiary-care children’s hospital was performed for the period 1998–2015. Inclusion criteria consisted of shunt placement, age < 30 days, and available pre- and postoperative brain imaging. The following data were collected and analyzed for each case: ventricular size ratios, laboratory values, clinical presentation, shunt and valve type, and operative timing and approach.RESULTSA total of 121 neonates met the inclusion criteria for the study, and 11 patients (9.1%) had MIPH following shunt placement. The preoperative frontal and occipital horn ratio (FOR) was significantly higher in the patients with MIPH than in those without (0.65 vs 0.57, p < 0.001). The change in FOR (∆FOR) after shunt placement was significantly greater in the MIPH group (0.14 vs 0.08, p = 0.04). Among neonates who developed MIPH, aqueductal stenosis was the most common etiology (45%). The type of shunt valve was associated with incidence of MIPH (p < 0.001). Preoperative clinical parameters, including head circumference, bulging fontanelle, and coagulopathy, were not significantly associated with development of MIPH.CONCLUSIONSMIPH represents an underrecognized complication of neonatal shunted hydrocephalus. Markers of severity of ventriculomegaly (FOR) and ventricular response to CSF diversion (∆FOR) were significantly associated with occurrence of MIPH. Choice of shunt and etiology of hydrocephalus were also significantly associated with MIPH. After adjusting for corrected age, etiology of hydrocephalus, and shunt setting, the authors found that ∆FOR after shunting was still associated with MIPH. A prospective study of MIPH prevention strategies and assessment of possible implications for patient outcomes is needed.
Harnessing rhetorical figures for argument mining
Authors: Lawrence John , Visser Jacky , Reed Chris 
Published: September 2017

The generalised, automated reconstruction of the reasoning structures underlying persuasive communication is an enormously challenging task. While this work in argument mining is increasingly informed by the rich tradition of argumentation studies outside the computational field, the rhetorical perspective on argumentation is thus far largely ignored. To explore the application of rhetorical insights in argument mining, we conduct a pilot study on the connection between rhetorical figures and argumentation structure. Rhetorical figures are linguistic devices that perform a variety of functions in argumentative discourse. The textual form of some of these figures is easy to identify automatically, such that an established connection between the figure and a preponderance of argumentative content would improve the performance of argument mining techniques. Furthermore, the automated mining of rhetorical figures could be used as an empirical, corpus-based testing ground for the claims made about these figures in the rhetorical literature. In the pilot study, we explore the connection between eight rhetorical figures the forms of which we expect to be relatively easy to identify computationally, and argumentation structure (concretely, we consider the six schemes ‘anadiplosis’, ‘epanaphora’, ‘epistrophe’, ‘epizeuxis’, ‘eutrepismus’, and ‘polyptoton’, and the two tropes ‘antithesis’ and ‘dirimens copulatio’, and relate their occurrences to relations of inference and conflict). The data of the study is collected in the MM2012c corpus of 39,694 words of argumentatively annotated transcripts from the BBC Radio 4’s Moral Maze discussion program. We show that some of the figures indeed correspond to passages of high argumentative density, relative to the text as a whole.
MALT90 Kinematic Distances to Dense Molecular Clumps
Authors: Whitaker J. Scott , Jackson James M. , Rathborne J. M. , Foster J. B. , Contreras Y. , Sanhueza Patricio , Stephens Ian W. , Longmore S. N. 
Published: September 2017

Abstract
Using molecular-line data from the Millimetre Astronomy Legacy Team 90 GHz Survey (MALT90), we have estimated kinematic distances to 1905 molecular clumps identified in the ATLASGAL 870 μm continuum survey over the longitude range 295° < l < 350°. The clump velocities were determined using a flux-weighted average of the velocities obtained from Gaussian fits to the HCO+, HNC, and N2H+ (1–0) transitions. The near/far kinematic distance ambiguity was addressed by searching for the presence or absence of absorption or self-absorption features in 21 cm atomic hydrogen spectra from the Southern Galactic Plane Survey. Our algorithm provides an estimation of the reliability of the ambiguity resolution. The Galactic distribution of the clumps indicates positions where the clumps are bunched together, and these locations probably trace the locations of spiral arms. Several clumps fall at the predicted location of the far side of the Scutum–Centaurus arm. Moreover, a number of clumps with positive radial velocities are unambiguously located on the far side of the Milky Way at galactocentric radii beyond the solar circle. The measurement of these kinematic distances, in combination with continuum or molecular-line data, now enables the determination of fundamental parameters such as mass, size, and luminosity for each clump.
Multi-frequency Scatter Broadening Evolution of Pulsars. I
Authors: Krishnakumar M. A. , Joshi Bhal Chandra , Manoharan P. K. 
Published: September 2017

Abstract
We present multi-wavelength scatter broadening observations of 47 pulsars made with the Giant Metre-wave Radio Telescope (GMRT), Ooty Radio Telescope (ORT), and Long Wavelength Array (LWA). The GMRT observations were made in the phased array mode at 148, 234, and 610 MHz and the ORT observations at 327 MHz. The LWA data sets were obtained from the LWA pulsar data archive. The broadening of each pulsar as a function of observing frequency provides the frequency scaling index, α. The estimations of α have been obtained for 39 pulsars and include entirely new estimates for 31 pulsars. This study increases the total sample of pulsars available with α estimates by ∼50%. The overall distribution of α with the dispersion measure (DM) of the pulsar shows interesting variations, which are consistent with earlier studies. However, for a given value of DM, a range of α values are observed, indicating the characteristic turbulence along each line of sight. For each pulsar, the estimated level of turbulence,

, has also been compared with α and DM. Additionally, we compare the distribution of α with the theoretically predicted model to infer the general characteristics of the ionized interstellar medium. Nearly 65% of the pulsars show a flatter index (i.e.,

) than that expected from the Kolmogorov turbulence model. Moreover, the group of pulsars with flatter indices is typically associated with an enhanced value of

compared to those with steeper indices.
The Relationship Between Brightest Cluster Galaxy Star Formation and the Intracluster Medium in CLASH
Authors: Fogarty Kevin , Postman Marc , Larson Rebecca , Donahue Megan , Moustakas John 
Published: September 2017

Abstract
We study the nature of feedback mechanisms in the 11 CLASH brightest cluster galaxies (BCGs) that exhibit extended ultraviolet and nebular line emission features. We estimate star formation rates (SFRs), dust masses, and starburst durations using a Bayesian photometry-fitting technique that accounts for both stellar and dust emission from the UV through far-IR. By comparing these quantities to intracluster medium (ICM) cooling times and freefall times derived from X-ray observations and lensing estimates of the cluster mass distribution, we discover a tight relationship between the BCG SFR and the ICM cooling time to freefall time ratio,

, with an upper limit on the intrinsic scatter of 0.15 dex. Furthermore, starburst durations may correlate with ICM cooling times at a radius of

, and the two quantities converge upon reaching the gigayear regime. Our results provide a direct observational link between the thermodynamical state of the ICM and the intensity and duration of BCG star formation activity, and appear consistent with a scenario where active galactic nuclei induce condensation of thermally unstable ICM overdensities that fuel long-duration (>1 Gyr) BCG starbursts. This scenario can explain (a) how gas with a low cooling time is depleted without causing a cooling flow and (b) the scaling relationship between SFR and

. We also find that the scaling relation between SFR and dust mass in BCGs with SFRs

yr−1 is similar to that in star-forming field galaxies; BCGs with large (

yr−1) SFRs have dust masses comparable to extreme starbursts.
Emission Line Properties of Seyfert Galaxies in the 12 μm Sample
Authors: Malkan Matthew A. , Jensen Lisbeth D. , Rodriguez David R. , Spinoglio Luigi , Rush Brian 
Published: September 2017

Abstract
We present optical and ultraviolet spectroscopic measurements of the emission lines of 81 Seyfert 1 and 104 Seyfert 2 galaxies that comprise nearly all of the IRAS 12 μm AGN sample. We have analyzed the emission-line luminosity functions, reddening, and other diagnostics. For example, the narrow-line regions (NLR) of Seyfert 1 and 2 galaxies do not significantly differ from each other in most of these diagnostics. Combining the Hα/Hβ ratio with a new reddening indicator—the [S ii]6720/[O ii]3727 ratio—we find the average E(B–V) is 0.49 ± 0.35 for type 1 and 0.52 ± 0.26 for type 2 Seyferts. The NLR of Sy 1s has an ionization level insignificantly higher than that of Sy 2s. For the broad-line region (BLR), we find that the C iv equivalent width correlates more strongly with [O iii]/Hβ than with UV luminosity. Our bright sample of local active galaxies includes 22 Seyfert nuclei with extremely weak broad wings in Hα, known as Seyfert 1.9s and 1.8s, depending on whether or not broad Hβ wings are detected. Aside from these weak broad lines, our low-luminosity Seyferts are more similar to the Sy 2s than to Sy 1s. In a BPT diagram, we find that Sy 1.8s and 1.9s overlap the region occupied by Sy 2s. We compare our results on optical emission lines with those obtained by previous investigators, using AGN subsamples from the Sloan Digital Sky Survey. The luminosity functions of forbidden emission lines [O ii]λ3727 Å, [O iii]λ5007 Å, and [S ii]λ6720 Å in Sy 1s and Sy 2s are indistinguishable. They all show strong downward curvature. Unlike the LFs of Seyfert galaxies measured by the Sloan Digital Sky Survey, ours are nearly flat at low luminosities. The larger number of faint Sloan “AGN” is attributable to their inclusion of weakly emitting LINERs and H ii+AGN “composite” nuclei, which do not meet our spectral classification criteria for Seyferts. In an Appendix, we have investigated which emission line luminosities can provide the most reliable measures of the total non-stellar luminosity, estimated from our extensive multi-wavelength database. The hard X-ray or near-ultraviolet continuum luminosity can be crudely predicted from either the [O iii]λ5007 Å luminosity or the combinations of [O iii]+Hβ or [N ii]+Hα lines, with a scatter of

times for Sy 1s and

times for Sy 2s. Although these uncertainties are large, the latter two hybrid (NLR+BLR) indicators have the advantage of predicting the same HX luminosity independent of Seyfert type.
An ALMA Dynamical Mass Estimate of the Proposed Planetary-mass Companion FW Tau C
Authors: Wu Ya-Lin , Sheehan Patrick D. 
Published: September 2017

Abstract
Dynamical mass estimates down to the planet-mass regime can help to understand planet formation. We present Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm observations of FW Tau C, a proposed ∼10 M
Jup planet-mass companion at ∼330 au from the host binary FW Tau AB. We spatially and spectrally resolve the accretion disk of FW Tau C in 12CO (2–1). By modeling the Keplerian rotation of gas, we derive a dynamical mass of ∼0.1 M
☉. Therefore, FW Tau C is unlikely a planet, but rather a low-mass star with a highly inclined disk. This also suggests that FW Tau is a triple system consisting of three ∼0.1 M
☉ stars.
Rickettsia sibirica mongolitimonae infection, Sri Lanka
Authors: Cordier Charlotte , Tattevin Pierre , Leyer Caroline , Cailleaux Marine , Raoult Didier , Angelakis Emmanouil 
Published: September 2017

Introduction. Rickettsia sibirica mongolitimonae was recently reported as a common rickettsiosis in France. Current serological evidence suggests the presence of scrub typhus and spotted fever group rickettsiosis in Sri Lanka. We detected a human case of R. sibirica mongolitimonae in Sri Lanka.
Methodology. A skin biopsy of the eschar was tested for the presence of Rickettsia spp. using qPCR assay targeting a 109-bp fragment of a hypothetical protein and by PCR amplification and sequencing targeting the ompA gene.
Results. A 30-year-old woman who had just returned from travel to a jungle in Sri Lanka was evaluated as an outpatient for fever. Examination revealed an enlarged axillary lymph node, a maculopapular rash and an eschar at her left flank and a skin biopsy of the eschar was performed. The skin biopsy was positive for the presence of Rickettsia spp. by qPCR and PCR amplification and sequencing targeting the ompA gene revealed R. sibirica mongolitimonae. Immunofluorescence assay on an acute serum sample for spotted fever group rickettsial antigens (Rickettsia conorii conorii, R. sibirica mongolitimonae, Rickettsia felis) and typhus group rickettsiae (Rickettsia typhi) was negative. The patient was treated by oral doxycycline (200 mg/day) for one week.
Conclusions. R. sibirica mongolitimonae should be considered in the differential diagnosis of patients with suspected rickettsiosis in, or returning from, Sri Lanka.
Prevalence and antimicrobial resistance profiles of Escherichia coli isolated from free-range pigs
Authors: Zhang Hongna , Zhao Xiaonan , Wang Xuepeng , Chang Weishan 
Published: September 2017

Introduction: Numerous studies about antimicrobial resistant Escherichia coli (E. coli) of animal origins have been conducted around the world, most of them focus on bacteria from animals raised in intensive breeding farms, but systematic studies on antimicrobial resistance in E. coli of free range animals are still lacking.
Methodology: This study aimed to investigate the prevalence and antimicrobial resistance profiles of E. coli from free-range pigs in Laiwu mountainous areas, eastern China.
Results: Among 123 fecal samples, 123 non-duplicate E. coli were obtained with an isolation rate of 100.0％ (123/123). These E. coli showed the highest resistance rate to tetracycline (77/123, 62.6％), but all were sensitive to amoxicillin/clavulanic acid. Thirty-eight E. coli (38/123, 30.9％) showed multidrug resistance (MDR). Among 123 E. coli isolates, only 39 carried antimicrobial resistant genes detected in this study. Of these 39 isolates, blaTEM-1, blaCTX-M-14, blaCTX-M-15, qnrB, qnrD, qnrS1, floR and cfr genes were detected in 13, 9, 4, 7, 10, 7, 20, and 7 isolates, respectively. blaTEM-1 and blaCTX-M-14 genes were concomitantly detected in 6 isolates, and blaTEM, qnrB, qnrS and qnrD genes were concomitantly detected in 7 isolates.
Conclusions: Free-ranging pigs may be regarded as a potential reservoir for antibiotic resistant genes.
Factors Associated With First-Time NCLEX-RN Success: A Descriptive Research Study
Authors: Johnson Tanya , Sanderson Bonnie , Wang Chih-hsuan , Parker Francine 
Published: September 2017

Background:

The purpose of this study was to identify variables associated with scores achieved on the Health Education Systems, Inc. (HESI) exit examination and successful first-time NCLEX-RN
®
pass rates.

Method:
A retrospective descriptive study examined the administrative data of 211 baccalaureate nursing students.

Results:
Students who completed the program in sequence and scored higher in certain HESI course examinations were more likely to have a better performance on the HESI exit examination. The higher the scores students achieved on the HESI exit examination, the more likely they were to pass the NCLEX-RN on their first attempt.

Conclusion:

These findings add to the growing body of literature seeking to identify variables associated with success in first-time NCLEX-RN success. Further research is needed to identify strategies that can be implemented to ensure timely progression, program completion, and licensure examination success. [
J Nurs Educ.
2017;56(9):542–545.]
Mask-Ed: Breaking the Barrier of Fear of Intimate Care for Nursing Students
Authors: Reid-Searl Kerry , O'Neill Barbara 
Published: September 2017

Background:
Nursing students learn to toilet, shower, and dress patients in the clinical laboratory with simulation modalities that lack the realism necessary to address the fears, values, and beliefs of nudity and intimate contact with patients.

Method:

A high-fidelity Mask-Ed™ (KRS [
K
nowledgeable,
R
ealistic,
S
pontaneous] simulation) intervention was developed and piloted with first-year nursing students around patient showering to increase confidence and skills around intimate care.

Results:
Students initially felt intimidated, awkward, nervous, and anxious about showering patients; however, after the Mask-Ed simulation, 93% reported feeling more confident and having insight into the patient experience. The realism of the scenario was a contributing factor.

Conclusion:

Mask-Ed provides a platform for the educator to create realistic scenarios around intimate care that help students prepare, on many levels, for their initial clinical experiences. [
J Nurs Educ.
2017;56(9):572–574.]