bluuebunny/crossref_metadata_2025_split huggingface dataset:
The Influence of Motor Skills on Measurement Accuracy
Authors: Brychta Petr , Sadílek Marek , Brychta Josef 
Published: November 2016

Abstract
This innovative study trying to do interdisciplinary interface at first view different ways fields: kinantropology and mechanical engineering. A motor skill is described as an action which involves the movement of muscles in a body. Gross motor skills permit functions as a running, jumping, walking, punching, lifting and throwing a ball, maintaining a body balance, coordinating etc. Fine motor skills captures smaller neuromuscular actions, such as holding an object between the thumb and a finger. In mechanical inspection, the accuracy of measurement is most important aspect. The accuracy of measurement to some extent is also dependent upon the sense of sight or sense of touch associated with fine motor skills. It is therefore clear that the level of motor skills will affect the precision and accuracy of measurement in metrology. Aim of this study is literature review to find out fine motor skills level of individuals and determine the potential effect of different fine motor skill performance on precision and accuracy of mechanical engineering measuring.
Application of Thermal Tool Holder in Mechanical Engineering
Authors: Kunstfeld Jaroslav , Hajnyš Jiří , Brychta Josef , Hemžský Pavel , Nicielnik Henryk 
Published: November 2016

Abstract
The paper is focused on testing the thermal tool holder during milling operation from the point of view shimmy and roughness machined surface of the equipped tool. Experimental work will include testing of surface roughness parameters of the machined surface structural steel 1.0553 (Fe510C1) in combination with the monolith three-lips cutter Kennametal F3AU177BDK38 from cemented carbide coated with TiAIN PVD coating. Experimental machining will distinguish the climb milling and conventional milling and will be done under predetermined conditions, always at 15 cycles and in relation to other types of fixture devices. All testing will be done at a sufficiently rigid machine CNC FGS 40/50. During machining will be measured and subsequently evaluated power machine during the milling process, shimmy and selected parameters of the roughness of the machined surface.
Dry Eye Disease and Allergic Conditions: A Korean Nationwide Population-Based Study
Authors: Kim Minkyeong , Oh Jong-Hyun , Park Choul Yong , Lee Sang Wha 
Published: November 2016

Background Dry eye disease (DED) is a multifactorial disease of the tears and ocular surface. No epidemiologic reports have yet been published about the relationship between DED and allergic rhinitis or sensitization to allergens. Objective To investigate the association between DED and allergic conditions in the general adult Korean population. Methods This population-based cross-sectional study included 17,542 individuals (ages a 19 years) who participated in the Korea National Health and Nutrition Examination Survey (KNHANES) from 2010 to 2012. Data for total serum immunoglobulin E (IgE) and allergen-specific IgE levels were available for 1857 subjects. Data were analyzed by using logistic regression to determine the association of DED with allergy or allergic conditions, including allergic rhinitis, atopic dermatitis, asthma, increased total serum IgE, and sensitization to house-dust mite (Dermatophagoides farinae), dog, and cockroach allergens. Results The prevalence of DED, allergic rhinitis, atopic dermatitis, and asthma was 10.4,13.1, 2.2, and 3.3%, respectively. The prevalence of the increased total serum IgE level and sensitization to D. farinae, dog, and cockroach allergens was 34.6, 15.7, 1.0, and 2.8%, respectively. After adjusting for general characteristics, DED was significantly associated with allergic rhinitis (odds ratio 1.58 [95% confidence interval, 1.38–1.81]) and D. farinae sensitization (odds ratio 1.80 [95% confidence interval, 1.17–2.79]). Conclusion This study demonstrated a close association between DED and both allergic rhinitis and D. farinae sensitization in Korean adults. Further studies are warranted to establish temporal relationships between DED and allergic rhinitis.
Open versus Endoscopic Septoplasty Techniques: A Systematic Review and Meta-Analysis
Authors: Hong Chris J. , Monteiro Eric , Badhiwala Jetan , Lee John , de Almeida John R. , Vescan Allan , Witterick Ian J. 
Published: November 2016

Background Septal deviation is a condition of high prevalence, which ranges from 22% in newborns to 90% in adults. Surgical intervention is frequently considered in the management of patients with symptoms. Although many surgeons prefer either the endoscopic or the open approach to septoplasty, there is an ongoing debate regarding comparative outcomes between the two approaches. Objective The purpose of this study was to systematically review the literature and provide pooled summary estimates to evaluate the efficacy and safety of open versus endoscopic septoplasty techniques. Methods This study was registered with PROSPERO (CRD42014010730). MEDLINE, EMBASE, Google Scholar, CINAHL, Web of Science, and The Cochrane Central Registry for Randomized Trials were searched for relevant studies by using the following keywords in varying combinations: “nasal septum,” “nasal obstruction,” “nasal cartilages,” “nose,” “nose diseases,” “surgery,” “nasal/septal deviation,” and “septoplasty.” All the studies that compared open versus endoscopic septoplasty techniques for the management of symptomatic septal deviation were considered. Two reviewers independently extracted data by using a preestablished extraction form and performed quality assessment by using the Jadad and Newcastle Ottawa Scales. Weighted pooled estimates were calculated and reported, along with relative risks and 95% confidence intervals. Results Fourteen studies met our inclusion criteria. When comparing open versus endoscopic septoplasty techniques, there was significant improvement in postoperative symptoms (i.e., nasal obstruction, headaches) (p ≤ 0.05) in the endoscopic septoplasty group. There also were significantly fewer complications associated with the endoscopic septoplasty technique (p ≤ 0.05). Based on the quality assessment, included studies were deemed at a moderate-to-high risk of bias. Conclusion Our analysis indicated that endoscopic septoplasty may have some advantages over open septoplasty. However, our findings should be taken with caution given the poor quality of included studies.
Local Allergic Rhinitis to Pollens is Underdiagnosed in Young Patients
Authors: Krajewska-Wojtys Anna , Jarzab Jerzy , Gawlik Radoslaw , Bozek Andrzej 
Published: November 2016

Background Local allergic rhinitis (LAR) has been observed in patients without atopy. However, LAR is still underdiagnosed in patients with perennial or seasonal nasal symptoms. Objective The aim of this study was to determine the prevalence of LAR in young patients with a previous diagnosis of nonallergic rhinitis or suspicion of allergy. Methods A total of 121 patients, ages 12–18 years old, with confirmed nonallergic rhinitis and typical seasonal nasal symptoms were examined. Skin-prick tests; serum and nasal specific immunoglobulin E (IgE) measurements; and nasal provocation tests by using grass (Phleum partense), Artemisia, and birch pollens were performed. A control group of age-matched patients with a diagnosis of seasonal allergic rhinitis underwent the same procedures as the test group. Results LAR to grass pollen (P. partense), Artemisia, and birch was confirmed in 17 (16.6%), 6 (5.9%), and 9 (8.9%) of patients, respectively. Polyvalent allergy was established in 21 subjects (20.8%): grass and Artemisia, 11 patients (10.9%); and grass and birch, 10 patients (9.9%). The remaining 48 patients (47.5%) were diagnosed with nonallergic rhinitis. The results of the nasal provocation tests and the concentrations of nasal IgE were similar among the analyzed groups. Furthermore, the concentration of nasal IgE increased faster in patients with LAR than in patients with allergic rhinitis; however, this difference was not statistically significant. Conclusion LAR is a serious problem in young patients; however, its significance is still unappreciated.
Outcomes of Endoscopic Repair of Cerebrospinal Fluid Rhinorrhea without Lumbar Drains
Authors: Adams Austin S. , Russell Paul T. , Duncavage James A. , Chandra Rakesh K. , Turner Justin H. 
Published: November 2016

Objective Lumbar drains (LD) are commonly used during endoscopic repair of cerebrospinal fluid (CSF) rhinorrhea, either to facilitate graft healing or to monitor CSF fluid dynamics. However, the indications and necessity of LD placement remains controversial. The current study sought to evaluate endoscopic CSF leak repair outcomes in the setting of limited LD use. Methods Patients who underwent endoscopic repair of CSF rhinorrhea between 2004 and 2014 were identified by a review of medical records. Demographic and clinical data were extracted and compared between patients who had surgery with and patients who had surgery without a perioperative LD. A univariate analysis was performed to identify factors predictive of recurrence. Results A total of 107 patients (116 surgical procedures) were identified, with a mean follow-up of 15.8 months. Eighty-eight of 107 patients (82.2%) had surgery without an LD. The mean hospital stay was 4.48 days in the LD group versus 1.03 days in the non-LD group (p ≤ 0.00001). There was no difference in recurrence rate between the LD and non-LD groups. Predictors of recurrence included repair technique (p = 0.04) and size of defect (p = 0.005). Body mass index, leak site (ethmoid, sphenoid, frontal), and etiology (spontaneous, iatrogenic, traumatic) were not predictive of leak recurrence. Conclusion Use of LDs in endoscopic CSF leak repair was not associated with reduced recurrence rates, regardless of leak etiology, and resulted in a significant increase in hospital length of stay. Although the use of perioperative LDs to monitor CSF dynamics may have some therapeutic and diagnostic advantages, it may not be associated with clinically significant improvements in patient outcomes or recurrence rates.
Le palais de Iolkos et sa destruction
Authors: Adrymi-Sismani Vassiliki 
Published: November 2016

Vassiliki ADRYMI-SISMANI
The palace at Iolkos and its destruction.
p.1-54
Since 1977 an important Mycenaean settlement (ca. 10 ha) has been excavated at Dimini east of the hill occupied by the well-known prehistoric site, in the plain near the sea. Eleven houses have been brought to light, built on top of Middle Helladic megara and Early Bronze age levels, lining a central street that traverses the settlement, and also a large pottery kiln.
An architectural complex comprising two megara (A and B), a central court, workshops and magazines has been excavated since 1997, where the central street traversing the settlement terminates. The destruction of the complex, dating to the transition LH III B2-LH III C Early, brought about the collapse of the roughcast in Megaron A and a violent conflagration in Megaron B. Some rooms in Megaron A were reoccupied after being cleared and small repairs were made ; Megaron B, on the other hand, was not reoccupied. The reoccupied rooms in Megaron A produced Mycenaean pottery of the LH II C Early phase, wheel-made pseudo Grey Minyan pottery and burnished handmade ware ; this pottery is completely absent from Megaron B. The pottery shows that the reoccupation occurred immediately after the destruction and lasted a very short time.
Le dépôt archaïque du rempart Nord d'Amathonte III. Les petits objets
Authors: Fourrier Sabine , Louca E. , Meeks Dimitri , Olivier Jean-Pierre , Sznycer Maurice 
Published: November 2016

Sabine Fourrier et al.
The Archaic Deposit by the North Wall at Amathus, III. The Small Finds
p. 67-118
The small finds discovered in a fill of the Archaic period deposited against the North Wall of the lower town at Amathus are described. The rich and varied material reflects the different functions of the palace that it came from. Many types are unknown or only attested among the finds from the palace on the acropolis. Certain categories, like the terracotta figurines or the marks incised on the vases, are especially well represented. In spite of their often fragmentary condition, these objects give an overall picture of the finds contained in the Archaic palace of Amathus.
Deux décrets inédits de Larissa
Authors: Tziafalias Athanasios , Helly Bruno 
Published: November 2016

Athanasios Tziafalias και Bruno Helly
Δύο ανέκδοτα ψηφίσματα από τη Λάρισα
σ. 377-420
Ανάμεσα στις επιγραφικές μαρτυρίες που ανακαλύφθηκαν τα τελευταία χρόνια στη Λάρισα συγκαταλέγονται και δύο ψηφίσματα της πόλης αυτής, που παρουσιάζουν ιδιαίτερο ενδιαφέρον. Το πρώτο από αυτά είναι ένα προξενικό ψήφισμα, γραμμένο σε διάλεκτο, που αφορά έναν Μυτιληναίο και χρονολογείται στις αρχές του 2ου αιώνα π.Χ. Αντικατοπτρίζει τις σχέσεις που δημιουργήθηκαν πριν από την έναρξη του Δεύτερου Μακεδονικού Πολέμου και ανανεώθηκαν, στο πλαίσιο της αποδοχής των Ασκληπιείων της Μυτιλήνης, μεταξύ, αφενός του Κοινού των Θεσσαλών και των πόλεων που το αποτελούσαν και αφετέρου των Μυτιληναίων. Αυτό μας επιτρέπει να δούμε κάτω από νέο πρίσμα ένα πολύ γνωστό έγγραφο, το ψήφισμα της Μυτιλήνης για το Κοινό των Θεσσαλών IG XII Suppl., 3 και να εμπλουτίσουμε την ιστορία των σχέσεων μεταξύ των δύο μερών, σχέσεις οι οποίες διατηρήθηκαν έως την εποχή του Αυγούστου, όπως γνωρίζουμε από τμήματα ψηφισμάτων προς τιμήν του Μυτιληναίου Ποταμώνα, γιου του Λεσβώνακτος. Το δεύτερο ψήφισμα από τη Λάρισα, γραμμένο στην κοινή, αφορούσε δυο πολίτες από τη Χαλκίδα, στην Εύβοια, και θα πρέπει να τοποθετηθεί χρονολογικά πάνω από έναν αιώνα αργότερα, γύρω στο 70 π. Χ.· καταδεικνύει τη διαδικασία σύμφωνα με την οποία ένας ξένος, που είχε την προξενία από το Κοινό των Θεσσαλών, μπορούσε να αποκτήσει, ύστερα από αίτημά του, την ιδιότητα του πολίτη μιας πόλης-μέλους αυτού του Κοινού.
Vers une redéfinition typologique et analytique des céramiques du type Zeuxippus Ware
Authors: Waksman Yona , François Véronique 
Published: November 2016

Yona Waksman, Véronique François
Προς έναν τυπολογικό και αναλυτικό επαναπροσδιορισμό της βυζαντινής κεραμικής του τύπου Zeuxippus Ware
σ. 629-724
Η επιτραπέζια κεραμική του τύπου Zeuxippus Ware είναι θεωρητικά μια από τις καλύτερα γνωστές κατηγορίες βυζαντινής κεραμικής. Έχοντας μεγάλη διάδοση στην επικράτεια της Βυζαντινής αυτοκρατορίας αλλά και σε ολόκληρη τη Μεσόγειο και τη Μαύρη θάλασσα, στα τέλη του 12ου και στις αρχές του 13ου αι., χρησιμεύει συχνά ως σημείο αναφοράς στη στρωματογραφία για την περίοδο αυτή. Τα τελευταία χρόνια, το αυξημένο πλήθος των ευρημάτων και οι δυσκολίες απόδοσης στην αρχική ομάδα φανέρωσαν τα όρια της τυπολογίας, η οποία είχε καθιερωθεί το 1968 από τον A.H.S. Megaw. Κρίθηκε λοιπόν απαραίτητο να επανεξετάσουμε το σύνολο αυτό πραγματοποιώντας χημικές αναλύσεις του πηλού, οι οποίες επιτρέπουν να ομαδοποιήσουμε αγγεία που έχουν την ίδια προέλευση, βασιζόμενοι σε πιο ισχυρά κριτήρια. Αυτή η μελέτη σε μεγάλη κλίμακα προτείνει μια αναθεώρηση του ζητήματος αυτού, συσχετίζοντας τα τυπολογικά και στυλιστικά χαρακτηριστικά, τη χημική και ορυκτολογική σύνθεση του πηλού ενός μεγάλου δείγματος της κεραμικής του τύπου Zeuxippus Ware , καθώς και δείγματα σχετιζόμενης κεραμικής τοπικής παραγωγής, προερχόμενα από αρχαιολογικούς χώρους σε ολόκληρη τη Μεσόγειο και τη Μαύρη θάλασσα.
CHEMICAL ABUNDANCE ANALYSIS OF MOVING GROUP W11450 (LATHAM 1)
Authors: O’Connell Julia E. , Martens Kylee , Frinchaboy Peter M. 
Published: November 2016

ABSTRACT
We present elemental abundances for all seven stars in Moving Group W11450 (Latham 1) to determine if they may be chemically related. These stars appear to be both spatially and kinematically related, but no spectroscopic abundance analysis exists in literature. Abundances for eight elements were derived via equivalent width analyses of high-resolution (R ∼ 60,000), high-signal-to-noise ratio (

) spectra obtained with the Otto Struve 2.1 m telescope and the Sandiford Echelle Spectrograph at McDonald Observatory. The large star-to-star scatter in metallicity, −0.55 ≤ [Fe/H]

0.06 dex (σ = 0.25), implies these stars were not produced from the same chemically homogeneous molecular cloud, and are therefore not part of a remnant or open cluster as previously proposed. Prior to this analysis, it was suggested that two stars in the group, W11449 and W11450, are possible wide binaries. The candidate wide binary pair show similar chemical abundance patterns with not only iron but with other elements analyzed in this study, suggesting the proposed connection between these two stars may be real.
HAT-P-65b AND HAT-P-66b: TWO TRANSITING INFLATED HOT JUPITERS AND OBSERVATIONAL EVIDENCE FOR THE REINFLATION OF CLOSE-IN GIANT PLANETS*
Authors: Hartman J. D. , Bakos G. Á. , Bhatti W. , Penev K. , Bieryla A. , Latham D. W. , Kovács G. , Torres G. , Csubry Z. , Val-Borro M. de , Buchhave L. , Kovács T. , Quinn S. , Howard A. W. , Isaacson H. , Fulton B. J. , Everett M. E. , Esquerdo G. , Béky B. , Szklenar T. , Falco E. , Santerne A. , Boisse I. , Hébrard G. , Burrows A. , Lázár J. , Papp I. , Sári P. 
Published: November 2016

ABSTRACT
We present the discovery of the transiting exoplanets HAT-P-65b and HAT-P-66b, with orbital periods of

and

days, masses of

and

, and inflated radii of

and

, respectively. They orbit moderately bright (

and

) stars of mass

and

. The stars are at the main-sequence turnoff. While it is well known that the radii of close-in giant planets are correlated with their equilibrium temperatures, whether or not the radii of planets increase in time as their hosts evolve and become more luminous is an open question. Looking at the broader sample of well-characterized close-in transiting giant planets, we find that there is a statistically significant correlation between planetary radii and the fractional ages of their host stars, with a false-alarm probability of only 0.0041%. We find that the correlation between the radii of planets and the fractional ages of their hosts is fully explained by the known correlation between planetary radii and their present-day equilibrium temperatures; however, if the zero-age main-sequence equilibrium temperature is used in place of the present-day equilibrium temperature, then a correlation with age must also be included to explain the planetary radii. This suggests that, after contracting during the pre-main-sequence, close-in giant planets are reinflated over time due to the increasing level of irradiation received from their host stars. Prior theoretical work indicates that such a dynamic response to irradiation requires a significant fraction of the incident energy to be deposited deep within the planetary interiors.
DIFFERENCES IN HALO-SCALE ENVIRONMENTS BETWEEN TYPE 1 AND TYPE 2 AGNs AT LOW REDSHIFT
Authors: Jiang Ning , Wang Huiyuan , Mo Houjun , Dong Xiao-Bo , Wang Tinggui , Zhou Hongyan 
Published: November 2016

ABSTRACT
Using low-redshift (

) samples of active galactic nuclei (AGNs), normal galaxies and groups of galaxies selected from the Sloan Digital Sky Survey, we study the environments of Type 1 and Type 2 AGNs, both on small and large scales. Comparisons are made for galaxy samples matched in redshift, r-band luminosity, [O iii] luminosity, and also the position in groups (central or satellite). We find that Type 2 AGNs and normal galaxies reside in similar environments. Type 1 and Type 2 AGNs have similar clustering properties on large scales (

), but at scales smaller than

, Type 2s have significantly more neighbors than Type 1s (3.09 ± 0.69 times more for central AGNs at

). These results suggest that Type 1 and Type 2 AGNs are hosted by halos of similar masses, as can also be seen directly from the mass distributions of their host groups (

for centrals and

for satellites). Type 2s have significantly more satellites around them, and the distribution of their satellites is also more centrally concentrated. The host galaxies of both types of AGNs have similar optical properties, but their infrared colors are significantly different. Our results suggest that the simple unified model based solely on torus orientation is not sufficient, but that galaxy interactions in dark matter halos must have played an important role in the formation of the dust structure, which obscures AGNs.
GRS 1739-278 OBSERVED AT VERY LOW LUMINOSITY WITH XMM-NEWTON AND NuSTAR
Authors: Fürst F. , Tomsick J. A. , Yamaoka K. , Dauser T. , Miller J. M. , Clavel M. , Corbel S. , Fabian A. , García J. , Harrison F. A. , Loh A. , Kaaret P. , Kalemci E. , Migliari S. , Miller-Jones J. C. A. , Pottschmidt K. , Rahoui F. , Rodriguez J. , Stern D. , Stuhlinger M. , Walton D. J. , Wilms J. 
Published: November 2016

ABSTRACT
We present a detailed spectral analysis of XMM-Newton and NuSTAR observations of the accreting transient black hole GRS 1739−278 during a very faint low hard state at ∼0.02% of the Eddington luminosity (for a distance of 8.5 kpc and a mass of 10

). The broadband X-ray spectrum between 0.5 and 60 keV can be well-described by a power-law continuum with an exponential cutoff. The continuum is unusually hard for such a low luminosity, with a photon index of Γ = 1.39 ± 0.04. We find evidence for an additional reflection component from an optically thick accretion disk at the 98% likelihood level. The reflection fraction is low, with

. In combination with measurements of the spin and inclination parameters made with NuSTAR during a brighter hard state by Miller et al., we seek to constrain the accretion disk geometry. Depending on the assumed emissivity profile of the accretion disk, we find a truncation radius of 15–35

(5–12

) at the 90% confidence limit. These values depend strongly on the assumptions and we discuss possible systematic uncertainties.
HIGH-WAVENUMBER SOLAR f-MODE STRENGTHENING PRIOR TO ACTIVE REGION FORMATION
Authors: Singh Nishant K. , Raichur Harsha , Brandenburg Axel 
Published: November 2016

ABSTRACT
We report a systematic strengthening of the local solar surface or fundamental f-mode one to two days prior to the emergence of an active region (AR) in the same (corotating) location. Except for a possibly related increase in the kurtosis of the magnetic field, no indication can be seen in the magnetograms at that time. Our study is motivated by earlier numerical findings of Singh et al., which showed that, in the presence of a nonuniform magnetic field that is concentrated a few scale heights below the surface, the f-mode fans out in the diagnostic

diagram at high wavenumbers. Here we explore this possibility using data from the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory and show for six isolated ARs, 11130, 11158, 11242, 11105, 11072, and 11768, that at large latitudinal wavenumbers (corresponding to horizontal scales of around

), the f-mode displays strengthening about two days prior to AR formation and thus provides a new precursor for AR formation. Furthermore, we study two ARs, 12051 and 11678, apart from a magnetically quiet patch lying next to AR 12529, to demonstrate the challenges in extracting such a precursor signal when a newly forming AR emerges in a patch that lies in close proximity to one or several already existing ARs, which are expected to pollute neighboring patches. We then discuss plausible procedures for extracting precursor signals from regions with crowded environments. The idea that the f-mode is perturbed days before any visible magnetic activity occurs at the surface can be important in constraining dynamo models aimed at understanding the global magnetic activity of the Sun.