bluuebunny/crossref_metadata_2025_split huggingface dataset:
Designing a CRM Framework for online & offline sports footwear retailers
Authors: Cueva Rodrigo , Rufian Guillem , Valdes Maria Gabriela 
Published: July 2019

The use of Customer Relationship Managers to foster customers loyalty has become one of the most common business strategies in the past years. However, CRM solutions do not fill the abundance of happily ever-after relationships that business needs, and each client’s perception is different in the buying process. Therefore, the experience must be precise, in order to extend the loyalty period of a customer as much as possible. One of the economic sectors in which CRM’s have improved this experience is retailing, where the personalized attention to the customer is a key factor. However, brick and mortar experiences are not enough to be aware in how environmental changes could affect the industry trends in the long term. A base unified theoretical framework must be taken into consideration, in order to develop an adaptable model for constructing or implementing CRMs into companies. Thanks to this approximation, the information is complemented, and the outcome will increment the quality in any Marketing/Sales initiative. The goal of this article is to explore the different factors grouped by three main domains within the impact of service quality, from a consumer’s perspective, in both on-line and off-line retailing sector. Secondly, we plan to go a step further and extract base guidelines about previous analysis for designing CRM’s solutions focused on the loyalty of the customers for a specific retailing sector and its product: Sports Running Shoes.
Mekanisme Koping Stres Penderita Tuberkulosis
Authors: Fadhilah Nur 
Published: July 2019

Tuberkulosis (TB) menimbulkan berbagai masalah kesehatan diantaranya perubahan psikologis. Psikologis pada penderita TB dipengaruhi oleh dukungan keluarga yang membuat penderita TB mempunyai koping yang adaptif atau maladaptif.. Tujuan penelitian ini adalah Diketahuinya hubungan dukungan keluarga dengan mekanisme koping stress pasien Tuberkulosis di Wilayah Kerja Puskesmas Gadingrejo Kabupaten Pringsewu Tahun 2014. Penelitian ini merupakan penelitian survei dengan jenis penelitian analitik, dan pendekatan cross sectional. Populasi dalam penelitian ini adalah seluruh keluarga yang mempunyai penderita TB berjumlah 32 orang. Teknik pengamnilan sampel enggunakan non probabilitas (Purposive sampling). Teknik pengumpulan data menggunakan kuesioner dengan memodifikasi kuesioner multidimensional scale of perceved social support. Analisis data univariat dan bivariat . Untuk menguji variabel bebas dan variabel terkait dilakukan dengan uji statistic Chi Squere (X2). Hasil uji statistic menunjukkan P Value = 0,003 < 0,05 dan OR = 3,929. Hal ini membuktikan bahwa Ha diterima dan Ho ditolak. artinya ada hubungan yang signifikan antara dukungan keluarga dengan mekanisme koping stress pasien TB. Diharapkan kepada petugas Puskesmas Gadingrejo dapat melibatkan keluarga dalam memberikan dukungan terhadap proses penyembuhan /pengobatan pasien TB
Faktor Determinan Ispa Pada Daerah Home Industri
Authors: Nuryati Elmi 
Published: July 2019

Asap yang dihasilkan dari pembakaran kayu itu ternyata berbahaya bagi kesehatan seperti layaknya polutan dari pembakaran mineral dan mesin kendaraan bermotor. Polutan dari kayu bakar dalam industry pembakaran genteng dapat menjadi salah satu penyebab infeksi saluran pernafasan akut (ISPA). Tujuan penelitian ini untuk mengetahui hubungan penggunaan kayu bakar dalam industry pembekaran genteng dengan kejadian ISPA pada daerah home industri Desa Pandansari Selatan Kecamatan Sukoharjo Kabupaten Pringsewu Tahun 2017. Jenis penelitian adalah analitik komparatif dengan desain crosectional. Populasi dalam penelitian ini semua warga desa Pandansari Selatan kecamatan sukoharjo dengan jumlah sampel 80 responden. Teknik sampling yang digunakan consecutive sampling. Pengumpulan data dilakukan dengan kuesioner dan wawancara. Analisis data dilakukan secara bivariat dengan menggunaka uji chi square dan multivariate menggunakan regresi logistic. Hasil penelitian menunjukkan ada hubungan antara penggunaan cerobong asap dalam industry pembakaran genteng dengan kejadian ispa dengan p value 0,033 (<0,05), nilai OR 2,682. Hal tersebut menunjukkan bahwa cerobong pembakaran genteng beresiko meningkatkan infeksi saluran pernafasan akut sebesar 2,682 kali. Industri pemkaran genteng diharapkan mampu meminimalisasi sisa – sisa pembakaran denga menggunakan tekonologi tepat guna sehingga akan mengurangi pencemaran lingkungan
Media Pornografi Dengan Perilaku Seksual Pranikah Pada Remaja Di Smk Patria
Authors: Vellyana Diny , Ardina Rani , Ernawati Indah 
Published: July 2019

Masa remaja adalah masa transisi dari anak anak menuju dewasa dan masa ini juga masa penuh gejolak. Hal ini menyebabkan remaja berprilaku menyimpang, melakukan tindak kriminal, seperti penyalahgunaan obat dan melakukan perilaku seksual pranikah. Faktor pemungkin dengan perilaku seksusal remaja adalah paparan media pornografi. Perkembangan teknologi dan arus globalisasi memudahkan remaja melakukan akses informasi pornografi melalui berbagai media masa. Penelitian ini bertujuan untuk mengetahui distribusi frekuensi responden, distribusi frekuensi media pornografi, distribusi frekuensi perilaku seksual pranikah dan Hubungan media pornografi dengan perilaku seksual pranikah remaja di SMK Patria Gadingrejo Pringsewu Lampung tahun 2017. Penelitian ini menggunakan Metode Cross Sectional dilakukan dengan teknik deskriptif Analitik menggunakan uji Chi squre. Subjek penelitian ini adalah remaja di SMK Patria Gadingrejo Pringsewu Lampung. Besarnya sampel dalam penelitian ini adalah 132 remaja dengan menggunakan teknik Stratified Random Sampling. Hasil analisis bivariat pada penelitian ini menunjukkan bahwa ada Hubungan media pornografi dengan perilaku seksual pranikah remaja di SMK Patria Gadingrejo Pringsewu Lampung tahun 2017 dengan tingkat kemaknaan p<0,05 diperoleh nilai (p=0,00).
Direct Comparison of the Thickness of the Parietal Peritoneum Using Peritoneal Biopsy and Ultrasonography of the Abdominal Wall in Patients Treated with Peritoneal Dialysis
Authors: Abrahams Alferso C. , Dendooven Amélie , van der Veer Jan Willem , Wientjes Rens , Toorop Raechel J. , Bleys Ronald L.A.W. , Hendrickx Antoni P.A. , van Leeuwen Maarten S. , de Lussanet Quido G. , Verhaar Marianne C. , Stapper Gerard , Nguyen Tri Q. 
Published: July 2019

Background Long-term treatment with peritoneal dialysis (PD) results in peritoneal fibrosis. Peritoneal biopsies have been used to determine the severity of fibrosis. Ultrasonography (US) of the abdominal wall has been used to measure peritoneal thickness non-invasively. However, direct comparison of both methods in the same patient has never been done. Furthermore, the validity of US to measure peritoneal thickness has not been investigated. Methods We performed 3 studies: 1) a human biopsy study to compare US measurement of peritoneal thickness with histological examination; 2) a human cadaver study to investigate the effect of removing the peritoneum on US results; and 3) a phantom study in which we used US to measure the thickness of membrane-like structures with a known thickness to investigate the influence of different US settings. Results The median thickness in biopsies of the peritoneum was 113 μm (interquartile range [IQR] 72 –129 μm), while this was 370 μm (IQR 324 – 458 μm) when measured by US ( p < 0.0001). The mean difference between the 2 measures was -257 μm (limits of agreement -4.6 and -511 μm). In the cadaver study, removal of the peritoneum did not have an effect on the presence or thickness of the hyperechoic line reported to represent the peritoneum. In the phantom study, results were highly dependent on frequency of the transducer, scan depth, and gain settings. Conclusions Ultrasonography results differ markedly from histological measurement using peritoneal biopsies. However, the hyperechoic line generated by US represents the interface between 2 neighboring tissues and not a separate morphological structure. Moreover, its thickness is greatly influenced by user-defined US settings.
Remote Patient Monitoring Program in Automated Peritoneal Dialysis: Impact on Hospitalizations
Authors: Sanabria Mauricio , Buitrago Giancarlo , Lindholm Bengt , Vesga Jasmin , Nilsson Lars-Göran , Yang Dongyan , Bunch Alfonso , Rivera Angela 
Published: July 2019

Background Automated peritoneal dialysis (APD) is a growing PD modality but as with other home dialysis methods, the lack of monitoring of patients’ adherence to prescriptions is a limitation with potential negative impact on clinical outcome parameters. Remote patient monitoring (RPM) allowing the clinical team to have access to dialysis data and adjust the treatment may overcome this limitation. The present study sought to determine clinical outcomes associated with RPM use in incident patients on APD therapy. Methods A retrospective cohort study included 360 patients with a mean age of 57 years (diabetes 42.5%) initiating APD between 1 October 2016 and 30 June 2017 in 28 Baxter Renal Care Services (BRCS) units in Colombia. An RPM program was used in 65 (18%) of the patients (APD-RPM cohort), and 295 (82%) were treated with APD without RPM. Hospitalizations and hospital days were recorded over 1 year. Propensity score matching 1:1, yielding 63 individuals in each group, was used to evaluate the association of RPM exposure with numbers of hospitalizations and hospital days. Results After propensity score matching, APD therapy with RPM ( n = 63) compared with APD-without RPM ( n = 63) was associated with significant reductions in hospitalization rate (0.36 fewer hospitalizations per patient-year; incidence rate ratio [IRR] of 0.61 [95% confidence interval (CI) 0.39 – 0.95]; p = 0.029) and hospitalization days (6.57 fewer days per patient-year; IRR 0.46 [95% CI 0.23 – 0.92]; p = 0.028). Conclusions The use of RPM in APD patients is associated with lower hospitalization rates and fewer hospitalization days; RPM could constitute a tool for improvement of APD therapy.
TESS Reveals that the Nearby Pisces–Eridanus Stellar Stream is only 120 Myr Old
Authors: Curtis Jason L. , Agüeros Marcel A. , Mamajek Eric E. , Wright Jason T. , Cummings Jeffrey D. 
Published: July 2019

Abstract
Pisces–Eridanus (Psc–Eri), a nearby (d ≃ 80–226 pc) stellar stream stretching across ≈120° of the sky, was recently discovered with Gaia data. The stream was claimed to be ≈1 Gyr old, which would make it an exceptional discovery for stellar astrophysics, as star clusters of that age are rare and tend to be distant, limiting their utility as benchmark samples. We test this old age for Psc–Eri in two ways. First, we compare the rotation periods for 101 low-mass members (measured using time-series photometry from the Transiting Exoplanet Survey Satellite) to those of well-studied open clusters. Second, we identify 34 new high-mass candidate members, including the notable stars λ Tauri (an Algol-type eclipsing binary) and HD 1160 (host to a directly imaged object near the hydrogen-burning limit). We conduct an isochronal analysis of the color–magnitude data for these highest-mass members, again comparing our results to those for open clusters. Both analyses show that the stream has an age consistent with that of the Pleiades, i.e., ≈120 Myr. This makes the Psc–Eri stream an exciting source of young benchmarkable stars and, potentially, exoplanets located in a more diffuse environment that is distinct from that of the Pleiades and of other dense star clusters.
ALMA Spectral Imaging of Titan Contemporaneous with Cassini's Grand Finale
Authors: Cordiner M. A. , Teanby N. A. , Nixon C. A. , Vuitton V. , Thelen A. E. , Charnley S. B. 
Published: July 2019

Abstract
The Cassini mission performed 127 targeted flybys of Titan during its 13 yr mission to Saturn, culminating in the Grand Finale between 2017 April and September. Here we demonstrate the use of the Atacama Large Millimeter/submillimeter Array (ALMA) to continue Cassini’s legacy for chemical and climatological studies of Titan’s atmosphere. Whole-hemisphere, interferometric spectral maps of HCN, HNC, HC3N, CH3CN, C2H3CN, C2H5CN, and C3H8 were obtained using ALMA in 2017 May at moderate (≈0.″2, or ≈1300 km) spatial resolution, revealing the effects of seasonally variable chemistry and dynamics on the distribution of each species. The ALMA submillimeter observations of HCN and HC3N are consistent with Cassini infrared data on these species, obtained in the same month. Chemical/dynamical lifetimes of a few years are inferred for C2H3CN and C2H5CN, in reasonably close agreement with the latest chemical models incorporating the sticking of C2H5CN to stratospheric aerosol particles. ALMA radial limb flux profiles provide column density information as a function of altitude, revealing maximum abundances in the thermosphere (above 600 km) for HCN, HNC, HC3N, and C2H5CN. This constitutes the first detailed measurement of the spatial distribution of HNC, which is found to be confined predominantly to altitudes above 730 ± 60 km. The HNC emission map shows an east–west hemispheric asymmetry of 13% ± 3%. These results are consistent with very rapid production (and loss) of HNC in Titan’s uppermost atmosphere, making this molecule an effective probe of short-timescale (diurnal) ionospheric processes.
Jet Geometry and Rate Estimate of Coincident Gamma-Ray Burst and Gravitational-wave Observations
Authors: Mogushi Kentaro , Cavaglià Marco , Siellez Karelle 
Published: July 2019

Abstract
Short gamma-ray burst (SGRB) progenitors have long been thought to be coalescing binary systems of two neutron stars (NSNS) or a neutron star and a black hole. The 2017 August 17th detection of the GW170817 gravitational-wave (GW) signal by Advanced LIGO and Advanced Virgo in coincidence with the electromagnetic observation of the SGRB GRB 170817A confirmed this scenario and provided new physical information on the nature of these astronomical events. We use SGRB observations by the Neil Gehrels Swift Observatory Burst Alert Telescope and GW170817/GRB 170817A observational data to estimate the detection rate of coincident GW and electromagnetic observations by a GW detector network and constrain the physical parameters of the SGRB jet structure. We estimate the rate of GW detections coincident with SGRB electromagnetic detections by the Fermi Gamma-ray Burst Monitor to be between ∼0.1 and ∼0.6 yr−1 in the third LIGO-Virgo observing run and between ∼0.3 and ∼1.8 yr−1 for the LIGO-Virgo-KAGRA network at design sensitivity. Assuming a structured model with a uniform ultrarelativistic jet surrounded by a region with power-law decay emission, we find the jet half-opening angle and the power-law decay exponent to be θ

c
∼ 7°–22° and s ∼ 5–30 at a 1σ confidence level, respectively.
Probing the Pulsar Population of Terzan 5 via Spectral Modeling
Authors: Ndiyavala H. , Venter C. , Johnson T. J. , Harding A. K. , Smith D. A. , Eger P. , Kopp A. , van der Walt D. J. 
Published: July 2019

Abstract
Terzan 5 is the only Galactic globular cluster that has plausibly been detected at very high energies by the High Energy Stereoscopic System. It has an unexpectedly asymmetric very high energy morphology that is offset from the cluster center, in addition to a large-scale, offset radio structure and compact diffuse X-ray emission associated with this cluster. We present new data from the Fermi Large Area Telescope on this source. We model the updated broadband spectral energy distribution, attributing this to cumulative pulsed emission from a population of embedded millisecond pulsars, as well as unpulsed emission from the interaction of their leptonic winds with the ambient magnetic and soft-photon fields. In particular, our model invokes unpulsed synchrotron and inverse Compton components to model the radio and TeV data and cumulative pulsed curvature radiation to fit the Fermi data, and it explains the hard Chandra X-ray spectrum via a “new” cumulative synchrotron component from electron–positron pairs within the pulsar magnetospheres that has not been implemented before. We find reasonable spectral fits for plausible model parameters. We also derive constraints on the millisecond pulsar luminosity function using the diffuse X-ray data and the Chandra sensitivity. Future higher-quality spectral and spatial data will help discriminate between competing scenarios (such as dark matter annihilation, white dwarf winds, or hadronic interactions) proposed for the broadband emission, as well as constraining degenerate model parameters.
New Probe of Gravity: Strongly Lensed Gravitational-wave Multimessenger Approach
Authors: Yang Tao , Hu Bin , Cai Rong-Gen , Wang Bin 
Published: July 2019

Abstract
Strong gravitational lensing by galaxies provides us with a unique opportunity to understand the nature of gravity on galactic and extra-galactic scales. In this paper, we propose a new multimessenger approach using data from both the gravitational wave (GW) and the corresponding electromagnetic (EM) counterpart to infer the constraint of the modified gravity (MG) theory denoted by the scale dependent phenomenological parameter. To demonstrate the robustness of this approach, we calculate the time-delay predictions by choosing various values of the phenomenological parameters and then compare them with that from general relativity (GR). For the third generation ground-based GW observatory, with one typical strongly lensed GW+EM event, and assuming that the dominated error from the stellar velocity dispersions is 5%, the GW time-delay data can distinguish an 18% MG effect on a scale of tens of kiloparsecs with a 68% confidence level. Assuming GR and a Singular Isothermal Sphere mass model, there exists a simplified consistency relationship between time-delay and imaging data. This relationship does not require the velocity dispersion measurement, and hence can avoid major uncertainties. By using this relationship, the multimessenger approach is able to distinguish an 8% MG effect. Our results show that the GW multimessenger approach can play an important role in revealing the nature of gravity on galactic and extra-galactic scales.
A Giant Lyα Nebula and a Small-scale Clumpy Outflow in the System of the Exotic Quasar J0952+0114 Unveiled by MUSE∗
Authors: Marino Raffaella Anna , Cantalupo Sebastiano , Pezzulli Gabriele , Lilly Simon J. , Gallego Sofia , Mackenzie Ruari , Matthee Jorryt , Brinchmann Jarle , Bouché Nicolas , Feltre Anna , Muzahid Sowgat , Schroetter Ilane , Johnson Sean D. , Nanayakkara Themiya 
Published: July 2019

Abstract
The well-known quasar SDSS J095253.83+011421.9 (J0952+0114) at z = 3.02 has one of the most peculiar spectra discovered so far, showing the presence of narrow Lyα and broad metal emission lines. Although recent studies have suggested that a proximate damped Lyα absorption (PDLA) system causes this peculiar spectrum, the origin of the gas associated with the PDLA is unknown. Here we report the results of observations with the Multi Unit Spectroscopic Explorer (MUSE) that reveal a new giant (≈100 physical kpc) Lyα nebula. The detailed analysis of the Lyα velocity, velocity dispersion, and surface brightness profiles suggests that the J0952+0114 Lyα nebula shares similar properties with other QSO nebulae previously detected with MUSE, implying that the PDLA in J0952+0144 is covering only a small fraction of the solid angle of the QSO emission. We also detected bright and spectrally narrow C iv
λ1550 and He ii
λ1640 extended emission around J0952+0114 with velocity centroids similar to the peak of the extended and central narrow Lyα emission. The presence of a peculiarly bright, unresolved, and relatively broad He ii
λ1640 emission in the central region at exactly the same PDLA redshift hints at the possibility that the PDLA originates in a clumpy outflow with a bulk velocity of about 500 km s−1. The smaller velocity dispersion of the large-scale Lyα emission suggests that the high-speed outflow is confined to the central region. Lastly, the derived spatially resolved He ii/Lyα and C iv/Lyα maps show a positive gradient with the distance to the QSO, hinting at a non-homogeneous distribution of the ionization parameter.
Imaging the Thermal and Kinematic Sunyaev–Zel’dovich Effect Signals in a Sample of 10 Massive Galaxy Clusters: Constraints on Internal Velocity Structures and Bulk Velocities
Authors: Sayers Jack , Montaña Alfredo , Mroczkowski Tony , Wilson Grant W. , Zemcov Michael , Zitrin Adi , Cibirka Nathália , Golwala Sunil , Hughes David , Nagai Daisuke , Reese Erik D. , Sánchez David , Zuhone John 
Published: July 2019

Abstract
We have imaged the Sunyaev–Zel’dovich (SZ) effect signals at 140 and 270 GHz toward 10 galaxy clusters with Bolocam and AzTEC/ASTE. We also used Planck data to constrain the signal at large angular scales, Herschel–SPIRE images to subtract the brightest galaxies that comprise the cosmic infrared background (CIB), Chandra imaging to map the electron temperature

of the intra-cluster medium, and Hubble Space Telescope imaging to derive models of each galaxy cluster’s mass density. The galaxy clusters gravitationally lens the background CIB, which produced an on-average reduction in brightness toward the galaxy clusters’ centers after the brightest galaxies were subtracted. We corrected for this deficit, which was between 5% and 25% of the 270 GHz SZ effect signal within R
2500. Using the SZ effect measurements, along with the X-ray constraint on

, we measured each galaxy cluster’s average line of sight (LOS) velocity v

z
within R
2500, with a median per-cluster uncertainty of ±700 km s−1. We found an ensemble-mean

v

z

of 430 ± 210 km s−1, and an intrinsic cluster-to-cluster scatter

of 470 ± 340 km s−1. We also obtained maps of v

z
over each galaxy cluster’s face with an angular resolution of 70″. All four galaxy clusters previously identified as having a merger oriented along the LOS showed an excess variance in these maps at a significance of ≃2–4σ, indicating an internal v

z
rms of ≳1000 km s−1. None of the six galaxy clusters previously identified as relaxed or plane-of-sky mergers showed any such excess variance.
Les dispenses d’instruction. De la pertinence et des dangers d’un outil régulateur
Authors: Fardet Christophe 
Published: July 2019

Historiquement, les hypothèses de dispenses d’instruction n’étaient en rien un préjugement parce qu’elles n’étaient pas un refus de jugement. Il ne s’agissait que de décisions insusceptibles de recours aboutissant à un jugement final collégialement délibéré. Or, le droit positif révèle une toute autre logique en y ajoutant les ordonnances susceptibles de recours mais constituant elles-mêmes le jugement. Ainsi, de Juger sans instruire, le mécanisme s’est mué en Refus de juger sans instruire. Ce faisant, les dispenses d’instruction ne portent pas atteinte qu’au principe du contradictoire : elles interdisent au juge de connaître de tous les éléments du dossier. Deux problèmes en résultent. D’une part, l’article L. 5 CJA permet seulement la dérogation à la contradiction et non pas à l’instruction : l’absence de dérogation à l’instruction, n’exclut-elle pas toute dérogation à la nécessaire instruction des affaires ? D’autre part, dans certaines hypothèses, la dispense d’instruction peut s’inscrire dans un cumul de suppression de garanties qui, finalement, peut faire douter du respect dû au droit au recours tel qu’il est constitutionnellement et conventionnellement protégé.