bluuebunny/crossref_metadata_2025_split huggingface dataset:
SPITZER SPACE TELESCOPE MID-IR LIGHT CURVES OF NEPTUNE
Authors: Stauffer John , Marley Mark S. , Gizis John E. , Rebull Luisa , Carey Sean J. , Krick Jessica , Ingalls James G. , Lowrance Patrick , Glaccum William , Kirkpatrick J. Davy , Simon Amy A. , Wong Michael H. 
Published: October 2016

ABSTRACT
We have used the Spitzer Space Telescope in 2016 February to obtain high cadence, high signal-to-noise, 17 hr duration light curves of Neptune at 3.6 and 4.5 μm. The light curve duration was chosen to correspond to the rotation period of Neptune. Both light curves are slowly varying with time, with full amplitudes of 1.1 mag at 3.6 μm and 0.6 mag at 4.5 μm. We have also extracted sparsely sampled 18 hr light curves of Neptune at W1 (3.4 μm) and W2 (4.6 μm) from the Wide-feld Infrared Survey Explorer (WISE)/NEOWISE archive at six epochs in 2010–2015. These light curves all show similar shapes and amplitudes compared to the Spitzer light curves but with considerable variation from epoch to epoch. These amplitudes are much larger than those observed with Kepler/K2 in the visible (amplitude ∼0.02 mag) or at 845 nm with the Hubble Space Telescope (HST) in 2015 and at 763 nm in 2016 (amplitude ∼0.2 mag). We interpret the Spitzer and WISE light curves as arising entirely from reflected solar photons, from higher levels in Neptune’s atmosphere than for K2. Methane gas is the dominant opacity source in Neptune’s atmosphere, and methane absorption bands are present in the HST 763 and 845 nm, WISE W1, and Spitzer 3.6 μm filters.
THE LYMAN CONTINUUM ESCAPE FRACTION OF THE COSMIC HORSESHOE: A TEST OF INDIRECT ESTIMATES*

†
Authors: Vasei Kaveh , Siana Brian , Shapley Alice E. , Quider Anna M. , Alavi Anahita , Rafelski Marc , Steidel Charles C. , Pettini Max , Lewis Geraint F. 
Published: October 2016

ABSTRACT
High-redshift star-forming galaxies are likely responsible for the reionization of the universe, yet direct detection of their escaping ionizing (Lyman continuum [LyC]) photons has proven to be extremely challenging. In this study, we search for escaping LyC of the Cosmic Horseshoe, a gravitationally lensed, star-forming galaxy at z = 2.38 with a large magnification of ∼24. Transmission at wavelengths of low-ionization interstellar absorption lines in the rest-frame ultraviolet suggests a patchy, partially transparent interstellar medium. This makes it an ideal candidate for direct detection of the LyC. We obtained a 10-orbit Hubble near-UV image using the Wide Field Camera 3 (WFC3)/UVIS F275W filter that probes wavelengths just below the Lyman limit at the redshift of the Horseshoe in an attempt to detect escaping LyC radiation. After fully accounting for the uncertainties in the opacity of the intergalactic medium (IGM) and accounting for the charge transfer inefficiency in the WFC3 CCDs, we find a

upper limit for the relative escape fraction of

. This value is a factor of five lower than the value (0.4) predicted by the 40% transmission in the low-ion absorption lines. Though possible, it is unlikely that the nondetection is due to a high-opacity line of sight through the IGM (

% chance). We discuss several possible causes for the discrepancy between the escape fraction and the covering fraction and consider the implications for future attempts at both direct LyC detection and indirect estimates of the escape fraction.
ON THE EVOLUTION OF THE INNER DISK RADIUS WITH FLUX IN THE NEUTRON STAR LOW-MASS X-RAY BINARY SERPENS X-1
Authors: Chiang Chia-Ying , Morgan Robert A. , Cackett Edward M. , Miller Jon M. , Bhattacharyya Sudip , Strohmayer Tod E. 
Published: October 2016

ABSTRACT
We analyze the latest Suzaku observation of the bright neutron star (NS) low-mass X-ray binary Serpens X-1 taken in 2013 October and 2014 April. The observation was taken using the burst mode and only suffered mild pile-up effects. A broad iron line is clearly detected in the X-ray spectrum. We test different models and find that the iron line is asymmetric and best interpreted by relativistic reflection. The relativistically broadened iron line is generally believed to originate from the innermost regions of the accretion disk, where strong gravity causes a series of special and general relativistic effects. The iron line profile indicates an inner radius of ∼8 R
G, which gives an upper limit on the size of the NS. The asymmetric iron line has been observed in a number of previous observations, which gives several inner radius measurements at different flux states. We find that the inner radius of Serpens X-1 does not evolve significantly over the range of L/L
Edd ∼ 0.4–0.6, and the lack of flux dependence of the inner radius implies that the accretion disk may be truncated outside of the innermost stable circular orbit by the boundary layer, rather than the stellar magnetic field.
THE DETACHED ECLIPSING BINARY KV 29 AND THE AGE OF THE OPEN CLUSTER M11
Authors: Bavarsad Ernest A. , Sandquist Eric L. , Shetrone Matthew D. , Orosz Jerome A. 
Published: October 2016

ABSTRACT
We present an extensive set of photometry and radial velocities for the detached eclipsing binary KV 29 in the intermediate-aged open cluster M11 (NGC 6705). Spectroscopy shows that the system is double lined, and all available evidence (proper motion, photometry, and position on the color–magnitude diagram) indicates that it is a member of the cluster. We find the period of the binary to be 4.64276 ± 0.00001 days. We find masses

and

and radii

and

for the primary and secondary stars, respectively. Because the primary star in the binary is rapidly evolving and is brighter than the cluster turnoff in a color–magnitude diagram, the measurement of its mass leads to a strong constraint on the cluster age. We find the age of M11 to be

Myr, where the quoted uncertainties come from statistical errors in the calculated masses and radii, and systematic uncertainties due to the ambiguity of the metallicity of the open cluster and variations within the isochrone models concerning heavy elements and convective overshooting.
A COMPARISON OF GALAXY COUNTING TECHNIQUES IN SPECTROSCOPICALLY UNDERSAMPLED REGIONS
Authors: Specian Mike A. , Szalay Alex S. 
Published: October 2016

ABSTRACT
Accurate measures of galactic overdensities are invaluable for precision cosmology. Obtaining these measurements is complicated when members of one’s galaxy sample lack radial depths, most commonly derived via spectroscopic redshifts. In this paper, we utilize the Sloan Digital Sky Survey’s Main Galaxy Sample to compare seven methods of counting galaxies in cells when many of those galaxies lack redshifts. These methods fall into three categories: assigning galaxies discrete redshifts, scaling the numbers counted using regions’ spectroscopic completeness properties, and employing probabilistic techniques. We split spectroscopically undersampled regions into three types—those inside the spectroscopic footprint, those outside but adjacent to it, and those distant from it. Through Monte Carlo simulations, we demonstrate that the preferred counting techniques are a function of region type, cell size, and redshift. We conclude by reporting optimal counting strategies under a variety of conditions.
TWO ECLIPSING ULTRALUMINOUS X-RAY SOURCES IN M51
Authors: Urquhart R. , Soria R. 
Published: October 2016

ABSTRACT
We present the discovery, from archival Chandra and XMM-Newton data, of X-ray eclipses in two ultraluminous X-ray sources (ULXs), located in the same region of the galaxy M51: CXOM51 J132940.0+471237 (ULX-1, for simplicity) and CXOM51 J132939.5+471244 (ULX-2). Three eclipses were detected for ULX-1 and two for ULX-2. The presence of eclipses puts strong constraints on the viewing angle, suggesting that both ULXs are seen almost edge-on and are certainly not beamed toward us. Despite the similar viewing angles and luminosities (

erg s−1 in the 0.3–8 keV band for both sources), their X-ray properties are different. ULX-1 has a soft spectrum, well fitted by Comptonization emission from a medium with electron temperature

. ULX-2 is harder, well fitted by a slim disk with

–1.8 keV and normalization consistent with a ∼10 M
⊙ black hole. ULX-1 has a significant contribution from multi-temperature thermal-plasma emission (

erg s−1). About 10% of this emission remains visible during the eclipses, proving that the emitting gas comes from a region slightly more extended than the size of the donor star. From the sequence and duration of the Chandra observations in and out of eclipse, we constrain the binary period of ULX-1 to be either

days, or ≈12.5–13 days. If the donor star fills its Roche lobe (a plausible assumption for ULXs), both cases require an evolved donor, most likely a blue supergiant, given the young age of the stellar population in that Galactic environment.
Les gangs de motards criminalisés : une menace internationale parfois négligée
Authors: Codron Étienne 
Published: October 2016

Les Gangs de motards criminalisés (GMC) sont parfois considérés comme de simples groupes marginaux, un peu folkloriques et surtout bien éloignés du crime organisé. Cet article est destiné à montrer que ces GMC sont insérés au cœur de la criminalité transnationale, bénéficiant d’un réseau bien établi à travers le monde et ayant de bonnes relations (d’affaires...) avec des organisations criminelles plus classiques. Ces clubs criminels, dont le plus connu est sans nul doute le Hells Angels Motorcycle Club, savent s’implanter dans des lieux stratégiques pour développer leurs activités criminelles : stupéfiants, armes, trafic d’êtres humains. Voici un regard sur ces criminels en uniforme...
Fraude documentaire : explosion d’une criminalité transversale à la jonction de tous les trafics
Authors: Naudin Christophe 
Published: October 2016

La criminalité identitaire est désormais l’une des infractions qui connaît la plus forte croissance mondiale. Elle s’appuie sur notre dispositif d’État-civil, aménagé dans la hâte depuis le XVI e siècle et imposé au reste du monde sans discernement. Tous les États occidentaux sont touchés par ce phénomène criminel, lequel déstabilise fortement le fonctionnement de la société. Une solution existe : copier la nature en revenant à l’identification animale. C’est la fameuse biométrie ou « mesure du vivant ».
De la guerre impensable à la guerre impensée
Authors: Danet Laurent 
Published: October 2016

L’histoire civilo-militaire des États-Unis semble s’ouvrir actuellement sur une disjonction entre la réflexion et l’action militaire. La seconde dans les faits précéderait la première, au moment où la plus grande puissance mondiale paraît s’acheminer vers une attitude plus impériale. À cet égard, entre intérêt de proximité civilisationnelle et divergence de situation stratégique, quelle conduite la France doit-elle choisir ?
Bitcoin : entre économie dangereuse et nouveaux « idéaux »
Authors: Mortier Stéphane 
Published: October 2016

« Bitcoin » est une monnaie virtuelle, électronique, cryptographique disponible en « peer to peer », créée en 2009. Au vu de sa popularité grandissante, le taux de convertibilité de cette monnaie augmente et baisse de façon incontrôlée depuis quelques mois. « Bitcoin », échappant par sa nature à tout contrôle des autorités financières, pourrait devenir un objet de spéculation, un outil utile aux « systèmes d’économie dangereuse » mais aussi constituer le ferment de changements sociétaux d’ampleur. Controversée, elle a fait l’objet de plusieurs tentatives de déstabilisation.
Joint Education Fosters Collaboration and Role Clarity Between Practical and Degree Nursing Students
Authors: Limoges Jacqueline M. , Jagos Kim 
Published: October 2016

Background:
Tensions and hierarchies among nurses who have different educational preparations can hinder effective communication and collaborative practices.

Method:
A 2-year longitudinal cohort study involving 214 participants explored the influences of joint education on Canadian Practical Nursing (PN) and Bachelor of Science in Nursing (BScN) students.

Results:
Joint education helps students dismantle unhelpful power relations, address myths and misconceptions about the other, and develop respect for each other's contributions to patient care.

Conclusion:

Joint education enhances collaboration between nursing designations by placing a focus on the actual knowledge, skill, and judgment rather than on the hierarchies established through credentialing. Joint education also assists students to see overlap in scope of practice and points of intersection requiring collaboration. This understanding promotes safe patient-focused care. Contextualizing the findings within broader discourses, such as the professions, institutions, regulating organizations, and sociopolitical relations within nursing, exposes future possibilities within nursing education. [
J Nurs Educ
. 2016;55(11):623–630.]
Applications of VoiceThread
©
Technology in Graduate Nursing Education
Authors: Donnelly Mary K. , Kverno Karan S. , Belcher Anne E. , Ledebur Lindsay R. , Gerson Linda D. 
Published: October 2016

Background:

Online graduate courses provide opportunities for faculty to use technology and digital applications to enhance student learning and learning environments. In nursing education, as we become increasingly dependent on technology, it is important to ensure that both faculty and students add digital literacy to their repertoire of knowledge and skills. VoiceThread
©
, one type of Web-based digital application tool, allows students and faculty to verbally communicate and collaborate asynchronously.

Method:
This article discusses the use of VoiceThread technology in graduate nursing education and offers four examples of VoiceThread teaching methods: personal introductions, issues discussions, case presentations, and the elevator speech.

Results:
Student participation in VoiceThread assignments is evaluated using leveled rubrics. A poll of the students in one of the graduate courses showed high overall satisfaction with VoiceThread in the online classroom.

Conclusion:

Strategies for effective use of VoiceThread technology to enhance student engagement and learning are recommended. [
J Nurs Educ
. 2016;55(11):655–658.]
Response of adult Colorado potato beetles (Coleoptera: Chrysomelidae) to water in the landscape
Authors: Boiteau Gilles , MacKinley Pamela 
Published: October 2016

AbstractThis laboratory study confirmed that the strategy of adult terrestrial Colorado potato beetle (Leptinotarsa decemlineata(Say); Coleoptera Chrysomelidae) to survive the threat of drowning in water is based on avoidance of water crossings. It also showed that beetles at the surface of a body of water after failing to avoid it, long considered limited to passive floating and phoretic transport were in fact likely to rely on a complex fight or flee response. Beetles showed capacity to swim in a pattern similar to land foraging beetles. Beetles also tolerated submergence and walked underwater. These active behaviours should improve their probability of finding shore or refuge for longer survival. Results confirmed that Colorado potato beetles are likely to accumulate near water features in the potato agro-ecosystem landscape but suggest that successful crossings and colonisation of crops on the other side are more likely than previously expected. On a larger scale, new information provided by this study combined with our knowledge of dominant winds and currents should make it possible for future research to better predict the probability of surviving encounters with water and the orientation of invasive Colorado potato beetle colonisers dispersing at the surface of bodies of water.
Improving Individual Acceptance of Health Clouds through Confidentiality Assurance
Authors: Fabian Benjamin , Zarnekow Rüdiger , Ermakova Tatiana 
Published: October 2016

SummaryBackground Cloud computing promises to essentially improve healthcare delivery performance. However, shifting sensitive medical records to third-party cloud providers could create an adoption hurdle because of security and privacy concerns.ObjectivesThis study examines the effect of confidentiality assurance in a cloud-computing environment on individuals’ willingness to accept the infrastructure for inter-organizational sharing of medical data.MethodsWe empirically investigate our research question by a survey with over 260 full responses. For the setting with a high confidentiality assurance, we base on a recent multi-cloud architecture which provides very high confidentiality assurance through a secret-sharing mechanism: Health information is cryptographically encoded and distributed in a way that no single and no small group of cloud providers is able to decode it.ResultsOur results indicate the importance of confidentiality assurance in individuals’ acceptance of health clouds for sensitive medical data. Specifically, this finding holds for a variety of practically relevant circumstances, i.e., in the absence and despite the presence of conventional offline alternatives and along with pseudonymization. On the other hand, we do not find support for the effect of confidentiality assurance in individuals’ acceptance of health clouds for non-sensitive medical data. These results could support the process of privacy engineering for health-cloud solutions.Citation: Ermakova T, Fabian B, Zarnekow R. Improving individual acceptance of health clouds through confidentiality assurance.
Assessment of Oral Status in Pediatric Patients with Special Health Care Needs receiving Dental Rehabilitation Procedures under General Anesthesia: A Retrospective Analysis
Authors: Awasthi Neha , Solanki Neeraj , Kundu Anjali , Mathur Suveet , Bidhumadhav Suresh 
Published: October 2016

ABSTRACT

Introduction
Dental problems serve as additional burden on the children with special health care needs (CSHCN) because of additional hospitalization pressure, they face for the treatment of various serious medical problems. These patients have higher incidence of dental caries due to increased quantity of sugar involved in the drug therapies and lower salivary flow in the oral cavity. Such patients are difficult to treat with local anesthesia or inhaled sedatives. Single-sitting dental treatment is possible in these patients with general anesthesia. Therefore, we conducted this retrospective analysis of oral health status of CSHCN receiving various dental treatments in a given population.

Materials and methods
A total of 200 CSHCN of age 14 years or less reporting in the pediatric wing of the general hospital from 2005 to 2014 that underwent comprehensive dental treatment under general anesthesia were included in the study. Patients with history of any additional systemic illness, any malignancy, any known drug allergy, or previous history of any dental treatment were excluded from the study. Complete mouth rehabilitation was done in these patients under general anesthesia following standard protocols. Data regarding the patient's disability, type, duration, and severity of disability was collected and analyzed. All the results were analyzed by Statistical Package for the Social Sciences (SPSS) software. Chi-square test, Student's t-test, and one-way analysis of variance were used to assess the level of significance.

Results
Statistically significant results were obtained while analyzing the subject's decayed missing filled/decayed extracted filled teeth indices divided based on age. Significant difference was observed only in cases where patients underwent complete crown placement even when divided based on type of disability. While analyzing the prevalence, statistically significant results were observed in patients when divided based on their age.

Conclusion
In CSHCN, dental pathologies and caries indices are increased regardless of the type or extent of disability.

Clinical significance
Children with special health care needs should be given special oral health care, and regular dental checkup should be conducted as they are more prone to have dental problems.

How to cite this article
Solanki N, Kumar A, Awasthi N, Kundu A, Mathur S, Bidhumadhav S. Assessment of Oral Status in Pediatric Patients with Special Health Care Needs receiving Dental Rehabilitation Procedures under General Anesthesia: A Retrospective Analysis. J Contemp Dent Pract 2016;17(6):476-479.
Fundamentos para la Elaboración de Manuscritos Científicos en Trauma y Cuidado Agudo de Emergencias (Parte 1): Cómo Elaborar y Cómo Presentar un Resúmen para Una Reunión Científica
Authors: Rubiano Andres Mariano 
Published: October 2016

RESUMEN

Objetivo
Los resúmenes científicos son la forma más frecuente de dar a conocer la información relevante en avances en investigación. Existen metodologías recomendadas para elaborar resúmenes de alta calidad que permitan una comprensión rápida y óptima por parte de evaluadores y de la comunidad científica en general. El objetivo de esta revisión, es discutir y presentar elementos fundamentales para la elaboración y presentación de resúmenes científicos en el área de trauma y cuidados agudos de emergencia.

Antecedentes
Más de diez millones de artículos científicos del área biomédica son publicados anualmente; estos proceden regularmente de resúmenes presentados de manera oral o escrita en reuniones científicas. Muchos resúmenes presentan fallas en el proceso de elaboración y no permiten generar una comunicación efectiva entre el investigador y los jurados. Muchos de estos resúmenes de investigación no llegan con éxito a ser un artículo completo.

Resultados
Una de las metodologías estandarizadas para la elaboración de artículos científicos se conoce como el principio IMRaD. Este principio es un acrónimo que surge de las palabras: Introducción, Métodos, Resultados y (and) Discusión. Con la difusión de este tipo de metodologías, se ha logrado mejorar la calidad de elaboración de los resúmenes. Aún así, solo entre un 15 a un 45% de los resúmenes elaborados por los diferentes proponentes llegan a convertirse en una publicación completa. Los dos motivos más frecuentes para la nó elaboración del documento definitivo, incluyen la poca disponibilidad de tiempo por parte del investigador principal y la dificultad en generar el documento completo en un idioma diferente al nativo.

Conclusione
Existen metodologías estandarizadas para elaborar resúmenes científicos de alta calidad. Es deber de las asociaciones científicas de las diferentes especialidades y subespecialidades, difundir los lineamientos para la mejor elaboración de estos resúmenes.

How to cite this article
Rubiano AM, Echeverri RA, Puyana JC. Fundamentos para la Elaboración de Manuscritos Científicos en Trauma y Cuidado Agudo de Emergencias (Parte 1): Cómo Elaborar y Cómo Presentar un Resúmen para Una Reunión Científica. Panam J Trauma Crit Care Emerg Surg 2016;5(1):52-57.
A High Resolution SEM Study of the Effects Supplementation Different Ratio Of n-6:n-3 on the Endometrial Pregnant Rat
Authors: Kassem Amira , Abu Bakar Md Zuki , Meng Goh Yong , Mohamed Mustapha Noordin 
Published: October 2016

This study, therefore, aims to investigate the effects of dietary fatty acids onendometrial pinopode expression. Twenty eight rats were randomly divided into four groups (seven rat per treatment).Treatment diets were rat chow only control diet ( con ), rat chow containing 0.9 ml soybean oil (SO) + 0.9 ml cod liver oil (CLO) the ratio 1:1, rat chow added with 1.5 ml SO + 0 .3 ml CLO the ratio 6:1 and rat chow added with 1.74 ml SO + 0.06 ml CLO the ratio 30:1 ,feeds of 15g/ day were given and water was available ad libitum .. The endometrial samples were evaluated under SEM. developing pinopodes were seen during increasing progesterone concentrations especially in Diet 1:1 group, and regressing pinopodes were found with decreasing progesterone in Diet 30:1 groups. In both Diet 1:1 treated and control animals, on days 15 of pregnancy, scanning electron micros copy revealed the microvilli of the uterine epithelial cells in the treated animals were more dense than those in the Diet 30:1 treated animals.