bluuebunny/crossref_metadata_2025_split huggingface dataset:
Dyslipidemia in patients with arterial hypertension and extrasystoles
Authors: Didyc N. V. 
Published: December 2016

The significant incidence of hypertensive disease among the Ukrainian population makes the search for new methods of management and treatment of patients suffering from this pathology a matter of high priority. Our research is focused on study of changes of some biochemical parameters in patients suffering from hypertensive disease as well as patients suffering from hypertensive disease and coexistent extrasystoles. Arterial hypertension leads to different structural and functional changes in the cardiovascular system. In many patients these changes may result in rhythm disorders. 120 patients have been examined (42 men and 78 women) between the ages of 27 to 81 (average 59.8) suffering from hypertensive disease of the II stage as defined by the Ukrainian Association of Cardiologists and from extrasystoles (more than 30 episodes per hour of research) of different topography and 30 persons (13 men and 17 women) suffering from hypertensive disease of the II stage between the ages 30 to 76 (average 56.4) without rhythm disturbance). The first clinical group was formed by 54 (45%) patients suffering from repeated supraventricular extrasystoles (SE) (average 62 ± 2 SE per hour of research). The second clinical group was formed by 42 (35%) patients suffering from repeated ventricular arhythmia (VA) (average 37 ± 2 VA per hour of research). The third group was formed by 24 (20%) patients suffering from both repeated SE and VA (average 48 ± 3 SE and 32 ± 3 VA per hour of research). We conducted 24 hours’ monitoring of blood pressure and electrocardiography using the “Dia Card”-system (“Solvaig”, Ukraine) for all patients. This revealed that ventricle extrasystoles and combined extrasystoles in patients with essential hypertension, II stage are associated with more unfavourable changes in 24 hours’ profile of blood pressure. The paper analyses the cardiac arhythmia structure of heart rate variability in patients with arterial hypertension (AH) and extrasystoles. The findings confirmed the presence of desynchronization in the activity of the neurohnmoral system. Thus, different mechanisms of arhythmogenesis were revealed in patients with arterial hypertension. In the results, frequent ventricular and combined extrasystoles were associated with an unfavourable blood pressure profile during 24-hours monitoring as well as higher end-diastolic left ventricular volume, diastolic dysfunction, aortic valve fibrosis, aorta remodeling, endothelial dysfunction and more prominent lipid disorders. Supraventricular extrasystoles were associated with hypertriglyceridemia, left ventricular diastolic dysfunction and left atrium enlargement.
Association of group erythrocyte antigens and B-cell non-Hodgkin lymphoma
Authors: Tymoshenko U. V. , Sivkovych S. O. , Garkava K. G. , Pavlyuk R. P. , Myronenko G. A. 
Published: December 2016

We analyzed the frequency distribution of blood groups AB0, Rhesus and Kell in patients with B-cell non-Hodgkin lymphoma. An increase of D− patients (31.0%) among ill in comparison to healthy individuals (16.5%) was found. Based on published data, we exclude weakening or alteration of the D antigen for this pathology. We found an association of B-cell non-Hodgkin lymphoma and D− phenotype. It is established that the chances of developing the disease in D− individuals is 2 times higher than for D+ individuals. However, we did not find a significant association of frequency of minor antigens Rhesus (C, c, E, e, CW), K antigen Kell system, A and B antigens AB0 system and the development of B-cell non-Hodgkin lymphoma. We have analyzed the statistics of incidence of non-Hodgkin lymphoma inWestern Europeand Asian countries. We noticed a roughly twofold increase in the incidence of non-Hodgkin lymphoma inWestern Europecompared to Asian countries, where the proportion of D− individuals is almost zero. Parallel with the results of our study, it has been found that the chances of D– persons developing B-cell non-Hodgkin lymphoma are twice as high as for D+ individuals. InUkraine,BelarusandRussiathe incidence of non-Hodgkin lymphoma is almost at the level of Asian countries even though the percentage of D– individuals corresponds to Western European countries (15–16%). This can be explained by other genetic factors, or reduction in quality of care and diagnostics in post-Soviet countries compared toWestern Europe. Thus, D antigen may have a protective role in the morbidity of non-Hodgkin lymphoma.
On \(m\)-polar fuzzy groups
Authors: Farooq Adeel , Ali Ghous , Akram Muhammad 
Published: December 2016

We introduce the concept of \(m\)-polar fuzzy subgroup, and investigate some of its properties. We describe the concept of an $m$-polar fuzzy coset and \(m\)-polar fuzzy quotient subgroup. We also present an \(m\)-polar fuzzy analog of Lagrange's theorem.
Morel-Lavallée Lesion: Presenting Etiology of Chronic Myelogenous Leukemia in an Adolescent Athlete
Authors: Hadley Christopher , Wowkanech Charles , Eck Brandon , Austin Luke , Sankar Wudbhav , Tjoumakaris Fotios 
Published: December 2016

Case:
A 16-year-old boy presented with a concealed degloving lesion of the knee, a Morel-Lavallée lesion, 3 weeks after an injury to the right knee while playing basketball. An incidental hematologic finding led to the additional diagnosis of chronic myelogenous leukemia.

Conclusion:
Morel-Lavallée lesions often can be overlooked and appear to be subcutaneous hematomas. This case was complicated further by a leukemic condition that was likely the causative mechanism for the recalcitrant nature of the lesion in this athlete.
PENCITRAAN PASANGAN JOKO WIDODO – BASUKI TJAHAJA PURNAMA DALAM IKLAN KAMPANYE VERSI “JAKARTA BARU” (Studi Analisis Semiotik Iklan Televisi)
Authors: Yunita Irmania , Rochmaniah Ainur , Aesthetika Nur Maghfirah 
Published: December 2016

The objective of this study is to analyze the meaning contained in communication symbols in the version of "New Jakarta" campaign advertisement of Joko Widodo - Tjahaja Basuki Purnama in television, how the messages conveyed through the advertisement sets the image of Joko Widodo - Tjahaja Basuki Purnama at Jakarta election 2012, and the perception of some viewers from the author point of view. This type of study is a qualitative descriptive using communication semiology analysis approach. As a descriptive study, it only describes the situation or discourse, does not look for a relationship, tests hypotheses or makes predictions. This study uses qualitative data so the data are substantive categories which are then interpreted by scientific references. In the data analysis, the author uses Roland Barthes' semiotic system with the concept of denotation and connotation as the first level, mythologies (myth) as the second level, as well as metonymy and metaphor as the concept of intertextual. The result of study show that the image of Joko Widodo - Tjahaja Basuki Purnama is found in the couple’s self-claim that they are agents of change who can bring people's expectations about the city of Jakarta into real, namely for a better condition of the road in the city, regular city planning, cleanness and flood prevention.
Modeling Copper and Cadmium Mobility in an Albeluvisol Amended with Urban Waste Composts
Authors: Filipović Vilim , Cambier Philippe , Filipović Lana , Coquet Yves , Pot Valérie , Bodineau Guillaume , Jaulin Anne , Mercier Vincent , Houot Sabine , Benoit Pierre 
Published: December 2016

Core Ideas
Mobility of Cu and Cd in compost‐amended soil was estimated using HYDRUS‐2D.
Cu and Cd mobility was controlled by sorption in the tilled layer.
Different sorption estimations were used to model trace metal leaching.
EDTA/CaCl2 extracts ratio gave reliable Kd estimates for Cu but not for Cd.
Most of the Cu and Cd mass remained in the tilled layer.
Two experimental plots amended with a co‐compost of sewage sludge and green wastes (SGW) or with a municipal solid waste compost (MSW) were compared with a control plot without organic amendment (CONT) in terms of trace metals mobility. These plots were equipped with wick lysimeters, time‐domain reflectometry probes and tensiometers for 6 yr (2004–2010). Different soil structures due to tillage and compost incorporation were identified in the tilled layers and reproduced in HYDRUS‐2D for simulating water, Cu, and Cd transport. Two sorption estimation approaches were used, either assuming equilibrium between CaCl2 and ethylenediaminetetraacetic acid (EDTA) extractable metals (Kd‐1) or using equations based on pedotransfer functions assuming nonlinear sorption for Cu (Kf) and linear sorption for Cd (Kd‐2). Lysimeter data on Cu leaching were successfully reproduced with the Kd‐1 approach for the SGW and CONT plots (model efficiency coefficient ESGW = 0.97, ECONT = 0.95), while the MSW plot showed better fitting with the Kf approach (EMSW = 0.77), which could be explained by the less stable organic matter of the MSW compost because it takes into account organic matter components (dissolved organic C and soil organic matter). The Cd leaching was reproduced with the Kd‐2 approach for the two amended plots (ESGW = 0.12, EMSW = 0.80), while CONT simulation overestimated leaching. The percentage of measured Cu and Cd leached in reference to input mass was 0.6 and 2.7%, respectively, in the SGW plot compared with 5% for both metals in the MSW plot. Trace metal mobility appeared to be limited in the tilled layer by sorption to organic matter.
Surgical management of dorsal scapular luxation in three dogs
Authors: Tinga Selena , Porter Erin , Lewis Daniel , Jones Stephen 
Published: December 2016

SummaryScapular luxation is an uncommon cause of forelimb lameness in dogs and cats. Traumatic rupture of the serratus ventralis muscle allows the scapula to displace dorsally during weight-bearing. Specific documentation regarding clinical presentation and surgical techniques is limited, with no medium- to long-term results of surgical intervention in dogs described. Presented here are three cases of scapular luxation in dogs, treated with a modified surgical technique. Clinical outcome was considered good to excellent, with resolution of lameness and abnormal scapular motion in all three dogs. Medium-and long-term outcomes were assessed in two of the dogs, with an excellent outcome in both cases.Supplementary Material to this article is available online at https://doi.org/10.3415/VCOT-16-05-0066
OGLE-2012-BLG-0950Lb: THE FIRST PLANET MASS MEASUREMENT FROM ONLY MICROLENS PARALLAX AND LENS FLUX
Authors: Koshimoto N. , Udalski A. , Beaulieu J. P. , Sumi T. , Bennett D. P. , Bond I. A. , Rattenbury N. , Fukui A. , Batista V. , Marquette J. B. , Brillant S. , and  , Abe F. , Asakura Y. , Bhattacharya A. , Donachie M. , Freeman M. , Hirao Y. , Itow Y. , Li M. C. A. , Ling C. H. , Masuda K. , Matsubara Y. , Matsuo T. , Muraki Y. , Nagakane M. , Ohnishi K. , Oyokawa H. , Saito To. , Sharan A. , Shibai H. , Sullivan D. J. , Suzuki D. , Tristram P. J. , Yonehara A. ,   (MOA Collaboration), Kozłowski S. , Pietrukowicz P. , Poleski R. , Skowron J. , Soszyński I. , Szymański M. K. , Ulaczyk K. , Wyrzykowski Ł. ,   (OGLE Collaboration)
Published: December 2016

ABSTRACT
We report the discovery of a microlensing planet OGLE-2012-BLG-0950Lb with a planet/host mass ratio of

. A long term distortion detected in both MOA and OGLE light curve can be explained by the microlens parallax due to the Earth’s orbital motion around the Sun. Although the finite source effect is not detected, we obtain the lens flux by the high resolution Keck AO observation. Combining the microlens parallax and the lens flux reveal the nature of the lens: a planet with mass of

is orbiting around an M-dwarf with mass of

with a planet-host projected separation of

au located at

kpc from us. This is the first mass measurement from only microlens parallax and the lens flux without the finite source effect. In the coming space observation-era with Spitzer, K2, Euclid, and WFIRST, we expect many such events for which we will not be able to measure any finite source effect. This work demonstrates an ability of mass measurements in such events.
CONSTRAINTS ON COMET 332P/IKEYA-MURAKAMI
Authors: Hui (許文韜) Man-To , Ye (葉泉志) Quan-Zhi , Wiegert Paul 
Published: December 2016

ABSTRACT
Encke-type comet 332P/Ikeya-Murakami is experiencing cascading fragmentation events during its 2016 apparition. It is likely the first splitting Encke-type comet ever observed. A nongravitational solution to the astrometry reveals a statistical detection of the radial and transverse nongravitational parameters,

au day−2 and

au day−2, respectively, which implies a nucleus erosion rate of

‰ per orbital revolution. The mass-loss rate likely has to be supported by a much larger fraction of an active surface area than known cases of short-period comets; it may be relevant to the ongoing fragmentation. We failed to detect any serendipitous pre-discovery observations of the comet in archival data from major sky surveys, whereby we infer that 332P used to be largely inactive, and is perhaps among the few short-period comets that have been reactivated from weakly active or dormant states. We therefore constrain an upper limit to the nucleus size as 2.0 ± 0.2 km in radius. A search for small bodies in similar orbits to that of 332P reveals comet P/2010 B2 (WISE) to be the best candidate. From an empirical generalized Jupiter-family (Encke-type included) comet population model, we estimate the likelihood of a chance alignment of the 332P–P/2010 B2 pair to be 1 in 33, a small number indicative of a genetic linkage between the two comets on a statistical basis. The pair possibly originated from a common progenitor, which underwent a disintegration event well before the twentieth century.
A NEW 3D MULTI-FLUID MODEL: A STUDY OF KINETIC EFFECTS AND VARIATIONS OF PHYSICAL CONDITIONS IN THE COMETARY COMA
Authors: Shou Y. , Combi M. , Toth G. , Tenishev V. , Fougere N. , Jia X. , Rubin M. , Huang Z. , Hansen K. , Gombosi T. , Bieler A. 
Published: December 2016

ABSTRACT
Physics-based numerical coma models are desirable whether to interpret the spacecraft observations of the inner coma or to compare with the ground-based observations of the outer coma. In this work, we develop a multi-neutral-fluid model based on the BATS-R-US code of the University of Michigan, which is capable of computing both the inner and outer coma and simulating time-variable phenomena. It treats H2O, OH, H2, O, and H as separate fluids and each fluid has its own velocity and temperature, with collisions coupling all fluids together. The self-consistent collisional interactions decrease the velocity differences, re-distribute the excess energy deposited by chemical reactions among all species, and account for the varying heating efficiency under various physical conditions. Recognizing that the fluid approach has limitations in capturing all of the correct physics for certain applications, especially for very low density environment, we applied our multi-fluid coma model to comet 67P/Churyumov–Gerasimenko at various heliocentric distances and demonstrated that it yields comparable results to the Direct Simulation Monte Carlo (DSMC) model, which is based on a kinetic approach that is valid under these conditions. Therefore, our model may be a powerful alternative to the particle-based model, especially for some computationally intensive simulations. In addition, by running the model with several combinations of production rates and heliocentric distances, we characterize the cometary H2O expansion speeds and demonstrate the nonlinear dependencies of production rate and heliocentric distance. Our results are also compared to previous modeling work and remote observations, which serve as further validation of our model.
DISK–WIND CONNECTION DURING THE HEARTBEATS OF GRS 1915+105
Authors: Zoghbi Abderahmen , Miller J. M. , King A. L. , Miller M. C. , Proga D. , Kallman T. , Fabian A. C. , Harrison F. A. , Kaastra J. , Raymond J. , Reynolds C. S. , Boggs S. E. , Christensen F. E. , Craig W. , Hailey C. J. , Stern D. , Zhang W. W. 
Published: December 2016

ABSTRACT
Disk and wind signatures are seen in the soft state of Galactic black holes, while the jet is seen in the hard state. Here we study the disk–wind connection in the ρ class of variability in GRS 1915+105 using a joint NuSTAR–Chandra observation. The source shows 50 s limit cycle oscillations. By including new information provided by the reflection spectrum and using phase-resolved spectroscopy, we find that the change in the inner disk inferred from the blackbody emission is not matched by reflection measurements. The latter is almost constant, independent of the continuum model. The two radii are comparable only if the disk temperature color correction factor changes, an effect that could be due to the changing opacity of the disk caused by changes in metal abundances. The disk inclination is similar to that inferred from the jet axis, and oscillates by ∼10°. The simultaneous Chandra data show the presence of two wind components with velocities between 500 and 5000 km s−1, and possibly two more with velocities reaching 20,000 km s−1 (∼0.06 c). The column densities are ∼5 × 1022 cm−2. An upper limit to the wind response time of 2 s is measured, implying a launch radius of <6 × 1010 cm. The changes in wind velocity and absorbed flux require the geometry of the wind to change during the oscillations, constraining the wind to be launched from a distance of 290–1300 r

g
from the black hole. Both data sets support fundamental model predictions in which a bulge originates in the inner disk and moves outward as the instability progresses.
THE PAndAS VIEW OF THE ANDROMEDA SATELLITE SYSTEM. II. DETAILED PROPERTIES OF 23 M31 DWARF SPHEROIDAL GALAXIES
Authors: Martin Nicolas F. , Ibata Rodrigo A. , Lewis Geraint F. , McConnachie Alan , Babul Arif , Bate Nicholas F. , Bernard Edouard , Chapman Scott C. , Collins Michelle M. L. , Conn Anthony R. , Crnojević Denija , Fardal Mark A. , Ferguson Annette M. N. , Irwin Michael , Mackey A. Dougal , McMonigal Brendan , Navarro Julio F. , Rich R. Michael 
Published: December 2016

ABSTRACT
We present a comprehensive analysis of the structural properties and luminosities of the 23 dwarf spheroidal galaxies that fall within the footprint of the Pan-Andromeda Archaeological Survey (PAndAS). These dwarf galaxies represent the large majority of Andromeda’s known satellite dwarf galaxies and cover a wide range in luminosity (

or

) and surface brightness (

mag arcsec−2). We confirm most previous measurements, but we find And XIX to be significantly larger than before (

,

) and cannot derive parameters for And XXVII as it is likely not a bound stellar system. We also significantly revise downward the luminosities of And XV and And XVI, which are now

or

. Finally, we provide the first detailed analysis of Cas II/And XXX, a fairly faint system (

) of typical size (

), located in close proximity to the two bright elliptical dwarf galaxies NGC 147 and NGC 185. Combined with the set of homogeneous distances published in an earlier contribution, our analysis dutifully tracks all relevant sources of uncertainty in the determination of the properties of the dwarf galaxies from the PAndAS photometric catalog. We further publish the posterior probability distribution functions of all the parameters we fit for in the form of MCMC chains available online; these inputs should be used in any analysis that aims to remain truthful to the data and properly account for covariance between parameters.
SUPRATHERMAL ELECTRON STRAHL WIDTHS IN THE PRESENCE OF NARROW-BAND WHISTLER WAVES IN THE SOLAR WIND
Authors: Kajdič P. , Alexandrova O. , Maksimovic M. , Lacombe C. , Fazakerley A. N. 
Published: December 2016

ABSTRACT
We perform the first statistical study of the effects of the interaction of suprathermal electrons with narrow-band whistler mode waves in the solar wind (SW). We show that this interaction does occur and that it is associated with enhanced widths of the so-called strahl component. The latter is directed along the interplanetary magnetic field away from the Sun. We do the study by comparing the strahl pitch angle widths in the SW at 1 AU in the absence of large scale discontinuities and transient structures, such as interplanetary shocks, interplanetary coronal mass ejections, stream interaction regions, etc. during times when the whistler mode waves were present and when they were absent. This is done by using the data from two Cluster instruments: Spatio Temporal Analysis of Field Fluctuations experiment (STAFF) data in the frequency range between ∼0.1 and ∼200 Hz were used for determining the wave properties and Plasma Electron And Current Experiment (PEACE) data sets at 12 central energies between ∼57 eV (equivalent to ∼10 typical electron thermal energies in the SW, E

T
) and ∼676 eV (∼113 E

T
) for pitch angle measurements. Statistical analysis shows that, during the intervals with the whistler waves, the strahl component on average exhibits pitch angle widths between 2° and 12° larger than during the intervals when these waves are not present. The largest difference is obtained for the electron central energy of ∼344 eV (∼57 E

T
).
ACCURATE OH MASER POSITIONS FROM THE SPLASH PILOT REGION
Authors: Qiao Hai-Hua , Walsh Andrew J. , Green James A. , Breen Shari L. , Dawson J. R. , Ellingsen Simon P. , Gómez José F. , Jordan Christopher H. , Shen Zhi-Qiang , Lowe Vicki , Jones Paul A. 
Published: December 2016

ABSTRACT
We report on high spatial resolution observations, using the Australia Telescope Compact Array (ATCA), of ground-state OH masers. These observations were carried out toward 196 pointing centers previously identified in the Southern Parkes Large-Area Survey in Hydroxyl (SPLASH) pilot region, between Galactic longitudes of 334° and 344° and Galactic latitudes of −2° and +2°. Supplementing our data with data from the MAGMO (Mapping the Galactic Magnetic field through OH masers) survey, we find maser emission toward 175 of the 196 target fields. We conclude that about half of the 21 nondetections were due to intrinsic variability. Due to the superior sensitivity of the followup ATCA observations, and the ability to resolve nearby sources into separate sites, we have identified 215 OH maser sites toward the 175 fields with detections. Among these 215 OH maser sites, 111 are new detections. After comparing the positions of these 215 maser sites to the literature, we identify 122 (57%) sites associated with evolved stars (one of which is a planetary nebula), 64 (30%) with star formation, two sites with supernova remnants, and 27 (13%) of unknown origin. The infrared colors of evolved star sites with symmetric maser profiles tend to be redder than those of evolved star sites with asymmetric maser profiles, which may indicate that symmetric sources are generally at an earlier evolutionary stage.