cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Physical and anthropometric analysis in students with and without menarche at Tucuruí/Pará region of Brazil
Creators: name: Valente, Fredson André Nunes
name: Aidar, Felipe José
name: Boaretto, Sabrina Mondadori
name: Gomes, Adriane Aline Batista
name: Alejo, Andres Armas
name: De Matos, Dihogo Gama
name: Barros, Natalie De Almeida
name: De Souza, Rodrigo Poderoso
name: De Souza, Raphael Fabrício
name: Fernandes Filho, José
Publisher: name: Motricidade
Year: 2017

description: It was our objective to evaluate the anthropometric variables and the physical qualities in girls with menarche and without menarche from public school of Tucuruí - PA, with 11 to 12 years old. Ninety-eight girls aged 11 and 105 aged 12 years were evaluated girls and divided into two groups: girls with menarche and girls without menarche. Weight and height, body mass index (BMI), body composition of two skinfolds (triceps and subscapular) were registered. Also, were assessed the performance in shuttle Run, horizontal jump, 1609 meters running, a 30 meters’ sprint run and a 3kg medicine ball throwing. After normality testing with the Kolmogorov Smirnov a t test for independent samples was computed or the Mann-Whitney test. Alpha value was set at 0.05. All calculations were computed using SPSS for Windows 15.0. It was found significant differences in body mass (44.05 and 37.85 kg) and height (1.48 and 1.42m) between groups among 11 years old girls. In the12 years old girls no significant differences were found between groups in relation to height (1.51 and 1.44m), BMI (19.86 and 18.49 kg/m2), horizontal jump (135.49 and 129.40cm), medicine ball throwing (238.29 and 207.42cm), 1.609 meters running (11.30 and 10.37m) and predicted VO2max (33.67 and 36.055 ml.kg-1.min-1). Girls with menstrual cycle had higher values than their counterparts in anthropometric measurements and in the medicine ball throwing.
description: Motricidade, Vol 12 No 4 (2016)
title: Collaboration on the Social Semantic Desktop
Creators: name: Groza, Tudor
name: Handschuh, Siegfried
Publisher: name: University of Galway
Year: 2007
Subjects: subject: Semantic Web

description: To accomplish the daily work people use several desktop applications to collaborate with co-workers. Each application is specialized on a specific domain, such as document management, email, or time planning. Although the data is distributed over several applications the data is highly interlinked from the user¿s point of view. The Social Semantic Desktop aims to take advantage of Semantic Web technologies on the computer¿s desktop to better support the user¿s mental working model and to enable collaboration over enterprise boundaries. In this paper we present our ongoing work on the Social Semantic Desktop as collaboration environment. We present the intended usage scenarios, discuss the required services and give an outlook on the architecture we envision for the Social Semantic Desktop.
Adaptação Humana ao Stress em Contextos Desportivos: Teoria, Avaliação, Investigação e Intervenção
Creators: name: Gomes, Rui
Publisher: name: Motricidade
Year: 2017

description: Não existem dúvidas acerca do facto dos fatores psicológicos desempenharem um papel fundamental no modo como os atletas se adaptam ao contexto desportivo bem como acerca da influência destes fatores no rendimento desportivo que os atletas obtêm ao longo das suas carreiras. No entanto, existem muitas dúvidas acerca do modo como o “lado mental” interfere nesta adaptação e no sucesso desportivo final obtido em cada competição disputada. Uma das razões que justifica este facto prende-se com a grande dificuldade em estudar, de um modo integrado, os fatores que podem influenciar a adaptação dos atletas a situações stressantes no desporto e que podem, no final, condicionar o rendimento desportivo.
description: Motricidade, Vol 13 No 1 (2017)
Adaptation and validation of the Portuguese version of Basic Psychological Needs Exercise Scale (BPNESp) to the sport domain and invariance across football and swimming
Creators: name: Monteiro, Diogo
name: Marinho, Daniel Almeida
name: Moutão, João
name: Couto, Nuno
name: Antunes, Raúl
name: Cid, Luis
Publisher: name: Motricidade
Year: 2017

description: The purpose of this study was to adapt and validate the Basic Psychological Needs Exercise Scale (BPNESp) to the sport domain, and to measure model invariance across football and swimming. Athletes (n=1382; 623 football, 759 swimming) with an average age of 18.77±SD 7.04 years participated in this study. Results supported the suitability of both the first and second order models, showing that the model was well adjusted to the data. In addition, the model showed the discriminant and convergent validity and composite reliability of the factors, and was invariant between football and swimming (∆CFI≤.01).
description: Motricidade, Vol 12 No 4 (2016)
Deep Iterative 2D/3D Registration
Creators: name: Jaganathan, Srikrishna
name: Wang, Jian
name: Borsdorf, Anja
name: Shetty, Karthik
name: Maier, Andreas
Publisher: name: arXiv
Year: 2021
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: Image and Video Processing (eess.IV)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Deep Learning-based 2D/3D registration methods are highly robust but often lack the necessary registration accuracy for clinical application. A refinement step using the classical optimization-based 2D/3D registration method applied in combination with Deep Learning-based techniques can provide the required accuracy. However, it also increases the runtime. In this work, we propose a novel Deep Learning driven 2D/3D registration framework that can be used end-to-end for iterative registration tasks without relying on any further refinement step. We accomplish this by learning the update step of the 2D/3D registration framework using Point-to-Plane Correspondences. The update step is learned using iterative residual refinement-based optical flow estimation, in combination with the Point-to-Plane correspondence solver embedded as a known operator. Our proposed method achieves an average runtime of around 8s, a mean re-projection distance error of 0.60 $\pm$ 0.40 mm with a success ratio of 97 percent and a capture range of 60 mm. The combination of high registration accuracy, high robustness, and fast runtime makes our solution ideal for clinical applications.
description: 10 pages,2 figures, Accepted at MICCAI 2021
Additional file 10 of Phenotype and multi-omics comparison of Staphylococcus and Streptococcus uncovers pathogenic traits and predicts zoonotic potential
Creators: name: Zondervan, Niels A.
name: Vitor A. P. Martins Dos Santos
name: Suarez-Diez, Maria
name: Saccenti, Edoardo
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Additional file 10. Streptococcus PCA
An all-sky sample of intermediate- to high-mass OBA-type eclipsing binaries observed by TESS
Creators: name: IJspeert, Luc W.
name: Tkachenko, Andrew
name: Johnston, Cole
name: Garcia, Stefano
name: De Ridder, Joris
name: Van Reeth, Timothy
name: Aerts, Conny
Publisher: name: arXiv
Year: 2021
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Context. Intermediate- to high-mass stars are the least numerous types of stars and they are less well understood than their more numerous low-mass counterparts in terms of their internal physical processes. Modelling the photometric variability of a large sample of main-sequence intermediate- to high-mass stars in eclipsing binary systems will help to improve the models for such stars. Aims. Our goal is to compose a homogeneously compiled sample of main-sequence intermediate- to high-mass OBA-type dwarfs in eclipsing binary systems from TESS photometry. We search for binaries with and without pulsations and determine their approximate ephemerides. Methods. Our selection starts from a catalogue of dwarfs with colours corresponding to those of OBA-type dwarfs in the TESS Input Catalog. We develop a new automated method aimed at detecting eclipsing binaries in the presence of strong pulsational and/or rotational signal relative to the eclipse depths and apply it to publicly available 30-min cadence TESS light curves. Results. Using targets with TESS magnitudes below 15 and cuts in the 2MASS magnitude bands of $J - H < 0.045$ and $J - K < 0.06$ as most stringent criteria, we arrive at a total of 189 981 intermediate- to high-mass candidates, 91193 of which have light curves from at least one of two data reduction pipelines. The eclipsing binary detection and subsequent manual check for false positives resulted in 3155 unique OBA-type eclipsing binary candidates. Conclusions. Our sample of eclipsing binary stars in the intermediate- to high-mass regime allows for future binary (and asteroseismic) modelling with the aim to better understand the internal physical processes in this hot part of the main sequence.
description: 12 pages, 9 figures, 2 tables, 3 appendices (8 additional figures, 1 additional table). Accepted for publication in A&A
Additional file 12 of Phenotype and multi-omics comparison of Staphylococcus and Streptococcus uncovers pathogenic traits and predicts zoonotic potential
Creators: name: Zondervan, Niels A.
name: Vitor A. P. Martins Dos Santos
name: Suarez-Diez, Maria
name: Saccenti, Edoardo
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Additional file 12. Staphylococcus & Streptococcus combined PCA
Fluid energy cascade rate and kinetic damping: new insight from 3D Landau-fluid simulations
Creators: name: Ferrand, R.
name: Sahraoui, F.
name: Laveder, D.
name: Passot, T.
name: Sulem, P. L.
name: Galtier, S.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Using an exact law for incompressible Hall magnetohydrodynamics (HMHD) turbulence, the energy cascade rate is computed from three-dimensional HMHD-CGL (bi-adiabatic ions and isothermal electrons) and Landau fluid (LF) numerical simulations that feature different intensities of Landau damping over a broad range of wavenumbers, typically $0.05\lesssim k_\perp d_i \lesssim100$. Using three sets of cross-scale simulations where turbulence is initiated at large, medium and small scales, the ability of the fluid energy cascade to "sense" the kinetic Landau damping at different scales is tested. The cascade rate estimated from the exact law and the dissipation calculated directly from the simulation are shown to reflect the role of Landau damping in dissipating energy at all scales, with an emphasis on the kinetic ones. This result provides new prospects on using exact laws for simplified fluid models to analyze dissipation in kinetic simulations and spacecraft observations, and new insights into theoretical description of collisionless magnetized plasmas.
description: 10 pages, 9 figures
On the Halo Occupation of Dark Baryons
Creators: name: Tinker, Jeremy L.
name: Chen, Hsiao-Wen
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We introduce a new technique that adopts the halo occupation framework for understanding the origin of QSO absorption-line systems. Our initial study focuses specifically on MgII absorbers. We construct a model of the gaseous content in which the absorption equivalent width W_r is determined by the the amount of cold gas, in the form of discrete clouds, along a sightline through a halo. The two quantities that we specify per halo in the model are (1) the mean absorption strength per unit surface mass density A_W(M), and (2) the mean covering factor kappa_g(M) of the gaseous clouds. These parameters determine the conditional probability distribution of W_r as a function of halo mass, P(W_r|M). Two empirical measurements are applied to constrain the model: (i) the absorber frequency distribution function and (ii) the W_r-dependent clustering amplitude. We find that the data demand a rapid transition in the gas content of halos at ~10^11.5 Msol/h, below which halos contain predominantly cold gas and beyond which gas becomes predominantly hot. In order to reproduce the observed overall strong clustering of the absorbers and the anti-correlation between W_r and halo mass M, roughly 5% of gas in halos up to 10^14 Msol/h is required to be cold. The gas covering factor is near unity over a wide range of halo mass, supporting that Mg II systems probe an unbiased sample of typical galaxies. We discuss the implications of our study in the contexts of mass assembly of distant galaxies and the origin of QSO absorption line systems.
description: 15 emulateapj pages, 7 figures, replaced with revised version incorporating referee's comments
Studies on the aerobic and anaerobic cytochromes of Escherichia coli
Creators: name: Hackett, Neil Robert
Publisher: name: University of British Columbia
Year: 2010

description: Escherichia coli can produce several respiratory chains which transfer electrons to oxygen, nitrate or other acceptors. Cytochromes are amongst the electron carriers of these chains, and can be studied by a number of spectroscopic techniques. Of particular interest is the formate-nitrate reductase respiratory pathway which is composed of two complexes, formate dehydrogenase and nitrate reductase each with a cytochrome associated. The cytochromes of E. coli after growth under a variety of conditions have been studied by spectrophotometry redox titration and other spectroscopic methods. These have shown that, contrary to some previous reports, there are at least six cytochromes produced irrespective of the culture conditions used. This emphasizes the need for simplified systems and two of these have been investigated. By fractionation of cytochromes prior to spectroscopic analysis a cytochrome b of redox potential OmV was identified in cells grown 556 aerobically. In addition the association of two cytochromes of potential +20mV and +120mV with nitrate reductase was demonstrated. Secondly the formate-nitrate reductase pathway has been investigated by spectroscopic studies of chi mutants which are defective in this activity. Three phenotypes of cytochrome production were observed. Mutants at loci associated with the production of the cofactor for both nitrate reductase and formate dehydrogenase were shown to produce the same cytochromes as the wild-type. Mutants mapping at the chlC locus and defective in nitrate reductase but not formate dehydrogenase were found to lack only the two cytochromes associated with nitrate reductase. They had high leyels of a cytochrome of redox potential -100mV which was shown to be associated with formate dehydrogenase. A third class of pleiotropic regulatory mutants was identified which was not related with a specific genotype. These produced none of the anaerobic respiratory pathways but overproduced the aerobic respiratory pathway leading to cytochrome d. The second aerobic respiratory pathway leading to cytochrome o was most evident in double mutants lacking both of the cytochromes associated with nitrate reductase and that associated with formate dehydrogenase. On the basis of these results a model for the arrangement of the cytochromes in the respiratory chains of E. coli is proposed.
Alternative formulas for synthetic dual system estimation in the 2000 census
Creators: name: Brown, Lawrence
name: Zhao, Zhanyun
Publisher: name: arXiv
Year: 2008
Subjects: subject: Applications (stat.AP)
subject: FOS: Computer and information sciences
subject: 62D05 (Primary)

description: The U.S. Census Bureau provides an estimate of the true population as a supplement to the basic census numbers. This estimate is constructed from data in a post-censal survey. The overall procedure is referred to as dual system estimation. Dual system estimation is designed to produce revised estimates at all levels of geography, via a synthetic estimation procedure. We design three alternative formulas for dual system estimation and investigate the differences in area estimates produced as a result of using those formulas. The primary target of this exercise is to better understand the nature of the homogeneity assumptions involved in dual system estimation and their consequences when used for the enumeration data that occurs in an actual large scale application like the Census. (Assumptions of this nature are sometimes collectively referred to as the ``synthetic assumption'' for dual system estimation.) The specific focus of our study is the treatment of the category of census counts referred to as imputations in dual system estimation. Our results show the degree to which varying treatment of these imputation counts can result in differences in population estimates for local areas such as states or counties.
description: Published in at http://dx.doi.org/10.1214/193940307000000400 the IMS Collections (http://www.imstat.org/publications/imscollections.htm) by the Institute of Mathematical Statistics (http://www.imstat.org)
Potential correlates and outcomes of active commuting to school among adolescents
Creators: name: Martins, João
name: Sallis, James F
name: Marques, Adilson
name: Diniz, José
name: Carreiro Da Costa, Francisco
Publisher: name: Motricidade
Year: 2017

description: The present study analysed the prevalence, potential correlates and physical activity (PA), body mass index (BMI), and academic performance outcomes, of active commuting to and from school (ACS), considering the home-to-school distance. A total of 391 Portuguese adolescents (189 boys, aged 14-18 years) completed a questionnaire about their active and passive commuting behaviours; potential correlates and perceived barriers of ACS; PA, BMI and academic performance. Multinomial regressions analyses were performed for ‘no walk/cycle’, ‘one-way commuters’ and for ‘both-ways commuters’ living near (<2 miles) school. The prevalence of one-way and both-ways active commuters decreased as the distance to school increased to more than two miles (66.5% to 23.5%). For the ‘near group’, walking to (47.8%) and from (55.5%) school was much more common than cycling (< 1%). The barrier with the greatest effect for one-way and both-ways active commuters was ‘distance’, followed by ‘stuff to carry’, ‘don’t enjoy walking/cycling’. No significant relations were found between walking or cycling one-way or both-ways and total PA, BMI and academic performance. To increase ACS, results suggest interventions promoting bicycling use and addressing multiple perceived barriers, such as ‘PA and ACS attitudes’, ‘stuff to carry’, perceptions of ‘hot and sweaty’ and ‘distance’.
description: Motricidade, Vol 12 No 4 (2016)
Comparison of Polish and Portuguese hospital cost accounting methods
Creators: name: Da Silva, Amélia Cristina Ferreira
name: Cyganska, Malgorzata
Publisher: name: Motricidade
Year: 2017

description: Dissemination of New Public Management ideology has motivated numerous studies about changes to management accounting practices in public healthcare organizations. However, few studies compare these practices on an international basis. The aim of the paper is to explore the differences and similarities in cost accounting practices within hospitals in different countries within the European Union. We follow a multiple comparative case-study approach. Qualitative data about the accounting practices of five hospitals, three from Poland and two from Portugal, are compared and discussed. Results show fairly similar models of cost accounting and an increasing need for accurately determined costs at hospitals in both countries. However, the data suggest some important differences in the way overhead is allocated. This study highlights the benefits of cross-country comparison practices. Moreover, this study points to the need for more qualitative cross-country research within management accounting topics.
description: Motricidade, Vol 12 No 4 (2016)
Euprenolepis echinata Lapolla, 2009, sp. nov.
Creators: name: Lapolla, John S.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Euprenolepis
Euprenolepis echinata

description: Euprenolepis echinata, sp. nov.
(Figures 3A–D)
Holotype worker, MALAYSIA: Borneo, Sabah, Poring Hot Spring, East Ridge, N 06°02’ E 116°42’, 600 m, 2.iv.1996 (A. Malsch) (USNM); paratype worker, same locality as holotype (ANIC).
 Worker. Measurements (n=1): TL: 3.11; HW: 0.68; HL: 0.77; SL: 1.1; WL: 1.2; GL: 1.14. Indices: CI: 89; SI: 161.
 Head brownish-yellow, with lighter mandibles and funiculi; head longer than broad. Cuticular surface dull and weakly rugoreticulate, with scattered distinctly thick erect setae, no pubescence underneath. Posterior margin complete. Eyes notably convex and more round in shape than observed in other Euprenolepis. Scapes surpass posterior margin by about length of the first four funicular segments; with scattered erect setae and no pubescence underneath. Mesosoma brownish-yellow, dull, legs slightly lighter. Pronotum elongate, very gently rises towards mesonotum (less than 30º angle); mesonotum and metanotal area flat; propodeum dorsum rounded, dome-like; declivity steep. Only a few erect setae present on notum, concentrated on posterior pronotum and anterior mesonotum. Petiole triangular with posterior face longer than anterior face. Gaster brownish-yellow with scattered long, erect setae and no pubescence underneath; cuticular surface dull and faintly rugoreticulate.
 Etymology: The species epithet is Latin for hedgehog, in reference to the unique setae of this species.
 Discussion: This is an easily recognized species with distinctly long and thick erect setae scattered across its entire body. The setal bases are especially noteworthy because they are clearly defined: large and darker than the surrounding cuticle. The pronotum is lower in profile and more elongated than is seen in other species except E. negrosensis. While the presence of long erect setae and an elongated pronotum might indicate a close relationship with E. negrosensis, it is worth noting that the erect setae are different between the two species with E. negrosensis possessing setae that are much thinner than in E. echinata.
description: Published as part of Lapolla, John S., 2009, Taxonomic Revision of the Southeast Asian Ant Genus Euprenolepis, pp. 1-25 in Zootaxa 2046 on pages 6-8, DOI: 10.5281/zenodo.186449
BitTrain: Sparse Bitmap Compression for Memory-Efficient Training on the Edge
Creators: name: Hosny, Abdelrahman
name: Neseem, Marina
name: Reda, Sherief
Publisher: name: arXiv
Year: 2021
Subjects: subject: Machine Learning (cs.LG)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: FOS: Computer and information sciences

description: Training on the Edge enables neural networks to learn continuously from new data after deployment on memory-constrained edge devices. Previous work is mostly concerned with reducing the number of model parameters which is only beneficial for inference. However, memory footprint from activations is the main bottleneck for training on the edge. Existing incremental training methods fine-tune the last few layers sacrificing accuracy gains from re-training the whole model. In this work, we investigate the memory footprint of training deep learning models, and use our observations to propose BitTrain. In BitTrain, we exploit activation sparsity and propose a novel bitmap compression technique that reduces the memory footprint during training. We save the activations in our proposed bitmap compression format during the forward pass of the training, and restore them during the backward pass for the optimizer computations. The proposed method can be integrated seamlessly in the computation graph of modern deep learning frameworks. Our implementation is safe by construction, and has no negative impact on the accuracy of model training. Experimental results show up to 34% reduction in the memory footprint at a sparsity level of 50%. Further pruning during training results in more than 70% sparsity, which can lead to up to 56% reduction in memory footprint. BitTrain advances the efforts towards bringing more machine learning capabilities to edge devices. Our source code is available at https://github.com/scale-lab/BitTrain.
description: 12 pages, 13 figures, to appear in the proceedings of The Sixth ACM/IEEE Symposium on Edge Computing (SEC 2021)
Optically-detected galaxy cluster candidates in the $AKARI$ North Ecliptic Pole field based on photometric redshift from Subaru Hyper Suprime-Cam
Creators: name: Huang, T. -C.
name: Matsuhara, H.
name: Goto, T.
name: Santos, D. J. D.
name: Ho, S. C. -C.
name: Kim, S. J.
name: Hashimoto, T.
name: Ikeda, Hiroyuki
name: Oi, Nagisa
name: Malkan, M. A.
name: Pearson, W. J.
name: Pollo, A.
name: Serjeant, S.
name: Shim, H.
name: Miyaji, T.
name: Hwang, H. S.
name: Durkalec, A.
name: Poliszczuk, A.
name: Greve, T. R.
name: Pearson, C.
name: Toba, Y.
name: Lee, D.
name: Kim, H. K.
name: Toft, S.
name: Jeong, W. -S.
name: Enokidani, U.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Galaxy clusters provide an excellent probe in various research fields in astrophysics and cosmology. However, the number of galaxy clusters detected so far in the $AKARI$ North Ecliptic Pole (NEP) field is limited. In this work, we provide galaxy cluster candidates in the $AKARI$ NEP field with the minimum requisites based only on coordinates and photometric redshift (photo-$z$) of galaxies. We used galaxies detected in 5 optical bands ($g$, $r$, $i$, $z$, and $Y$) by the Subaru Hyper Suprime-Cam (HSC), assisted with $u$-band from Canada-France-Hawaii Telescope (CFHT) MegaPrime/MegaCam, and IRAC1 and IRAC2 bands from the $Spitzer$ space telescope for photo-$z$ estimation. We calculated the local density around every galaxy using the 10$^{th}$-nearest neighbourhood. Cluster candidates were determined by applying the friends-of-friends algorithm to over-densities. 88 cluster candidates containing 4390 member galaxies below redshift 1.1 in 5.4 deg$^2$ have been detected. The reliability of our method was examined through false detection tests, redshift uncertainty tests, and applications on the COSMOS data, giving false detection rates of 0.01 to 0.05 and recovery rate of 0.9 at high richness. 3 X-ray clusters previously observed by $ROSAT$ and $Chandra$ were recovered. The cluster galaxies show higher stellar mass and lower star formation rate (SFR) compared to the field galaxies in two-sample Z-tests. These cluster candidates are useful for environmental studies of galaxy evolution and future astronomical surveys in the NEP, where $AKARI$ has performed unique 9-band mid-infrared photometry for tens of thousands of galaxies.
description: 19 pages, 16 figures, has been accepted for publication in MNRAS
Additional file 13 of Phenotype and multi-omics comparison of Staphylococcus and Streptococcus uncovers pathogenic traits and predicts zoonotic potential
Creators: name: Zondervan, Niels A.
name: Vitor A. P. Martins Dos Santos
name: Suarez-Diez, Maria
name: Saccenti, Edoardo
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Additional file 13. Staphylococcus & Streptococcus combined t-SNE
High-Level Data Flow Description of FPGA Firmware Components for Online Data Preprocessing
Creators: name: Engel, H.
name: Grüll, F.
name: Kebschull, U.
Publisher: name: GSI Helmholtzzentrum fuer Schwerionenforschung, Darmstadt
Year: 2014
Subjects: Physics

description: GSI Scientific Report 2013 - GSI Report 2014-1
Interstellar planetesimals: potential seeds for planet formation?
Creators: name: Moro-Martín, Amaya
name: Norman, Colin
Publisher: name: arXiv
Year: 2021
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We investigate the trapping of interstellar objects during the early stages of star and planet formation. Our results show a very wide range of possible values that will be narrowed down as the population of interstellar objects becomes better characterized. When assuming a background number density of 2$\cdot$10$^{15}$ pc$^{-3}$ (based on 1I/'Oumuamua detection), a velocity dispersion of 30 km/s and an equilibrium size distribution, the number of interstellar objects captured by a molecular cloud and expected to be incorporated to each protoplanetary disk during its formation is O(10$^{9}$) (50 cm-5 m), O(10$^{5}$) (5 m-50 m), O(10$^{2}$) (50 m-500 m), O(10$^{-2}$) (500 m-5 km). After the disk formed, the number of interstellar objects it could capture from the ISM during its lifetime is 6$\cdot$10$^{11}$ (50 cm-5 m), 2$\cdot$10$^{8}$ (5 m-50 m), 6$\cdot$10$^{4}$ (50 m-500 m), 20 (500 m-5 km); in an open cluster where 1% of stars have undergone planet formation, these values increase by a factor of O(10$^{2}$-10$^{3}$). These trapped interstellar objects might be large enough to rapidly grow into larger planetesimals via the direct accretion of the sub-cm sized dust grains in the protoplanetary disk before they drift in due to gas drag, helping overcome the meter-size barrier, acting as "seeds" for planet formation. They should be considered in future star and planet formation models and in the potential spread of biological material across the Galaxy.
description: Accepted to ApJ. 32 pages, 10 figures
Simulations for position-sensitive tracking of $\gamma$ rays in scintillators Approach for source reconstruction
Creators: name: Lalovic, N.
name: Gerl, J.
name: Rudolph, D.
name: Hoischen, R.
name: Golubev, P.
Publisher: name: GSI Helmholtzzentrum fuer Schwerionenforschung, Darmstadt
Year: 2014
Subjects: Physics

description: GSI Scientific Report 2013 - GSI Report 2014-1
title: SALT: Semantically Annotated LATEX
Creators: name: Groza, Tudor
name: Handschuh, Siegfried
name: Kim, Hak Lae
Publisher: name: University of Galway
Year: 2006
Subjects: subject: LATEX
subject: Semantic annotation
subject: Semantic document
subject: Authoring
subject: PDF (Computer file format)
subject: Metadata
subject: Authorship
subject: Science publishing

description: Machine-understandable data constitutes the basis for the Semantic Desktop. We provide in this paper means to author and annotate Semantic Documents on the Desktop. In our approach, the PDF file format is the basis for semantic documents, which store both a document and the related metadata in a single file. To achieve this we provide a framework, SALT that extends the Latex writing environment and supports the creation of metadata for scientific publications. SALT lets the scientific author create metadata while putting together the content of a research paper. We discuss some of the requirements one has to meet when developing such an ontology-based writing environment and we describe a usage scenario.
Highly eccentric EMRI waveforms via fast self-forced inspirals
Creators: name: McCart, Jonathan
name: Osburn, Thomas
name: Burton, Justin Y. J.
Publisher: name: arXiv
Year: 2021
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present new developments and comparisons of competing inspiral and waveform models for highly eccentric non-spinning extreme and intermediate mass-ratio inspirals (EMRIs and IMRIs). Starting from our high eccentricity self-force library, we apply the near-identity transform (NIT) technique to rapidly compute highly eccentric self-forced inspirals for the first time. Upon evaluating our approximate NIT results via comparison with full self-force inspirals, we couple our accurate and streamlined inspiral data to potential waveform generation schemes. We find that, although high eccentricity strains the NIT method, NIT inspirals are consistent with full self-force inspirals for EMRIs. However, our NIT implementation (at 1st post-adiabatic order) is not able to achieve LISA-motivated accuracy goals for highly eccentric IMRIs. Our most sophisticated waveforms are devised through a new technique that efficiently connects NIT orbital parameters to Teukolsky amplitudes and phases. We compare these sophisticated Teukolsky waveforms to those with synthesized (summing over harmonics) amplitudes based on a kludge. We find that, assuming identical worldlines (so that dephasing is negligible), kludge waveforms compare favorably to Teukolsky waveforms for non-spinning bodies.
description: 14 pages, 8 figures, updated to more closely match published version
Sphingius Thorell 1890
Creators: name: Feng, Zhang
name: Fu, Jianying
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Liocranidae
Sphingius

description: Sphingius Thorell, 1890 Sphingius Thorell 1890: 284; Gravely 1931: 269; Majumder and Tikader 1991: 147; Deeleman-Reinhold 2001: 488; Tso et al. 2005: 48; Zhang et al. 2009: 32. Thamphilus Thorell 1895: 35. Alaeho Barrion and Litsinger 1995: 170. Scotophaeoides Schenkel 1963: 49. Type species: Sphingius thecatus Thorell, 1890, by original designation. Diagnosis and description: see Zhang et al. 2009.
description: Published as part of Feng, Zhang & Fu, Jianying, 2010, A new species of the genus Sphingius (Araneae, Liocranidae) from China, and first description of the female: Sphingius hainan Zhang, Fu & Zhu, 2009, pp. 23-31 in ZooKeys 49 (49) on page 24, DOI: 10.3897/zookeys.49.391, http://zenodo.org/record/576675
description: {"references": ["Thorell T (1890) Arachnidi di Pinang raccolti nel 1889 dai Signori L. Loria e L. Fea. Annali del Museo Civico di Storia Naturale di Genova 30: 269 - 383.", "Gravely FH (1931) Some Indian spiders of the families Ctenidae, Sparassidae, Selenopidae and Clubionidae. Records of the Indian Museum, Calcutta 33: 211 - 282.", "Majumder SC, Tikader BK (1991) Studies on some spiders of the family Clubionidae from India. Records of the Zoological Survey of India, Ocasional Paper: 1 - 174.", "Deeleman-Reinhold CL (2001) Forest spiders of South East Asia: with a revision of the sac and ground spiders (Araneae: Clubionidae, Corinnidae, Liocranidae, Gnaphosidae, Prodidomidae and Trochanterriidae). Brill, Leiden, 591 pp.", "Tso IM, Zhu MS, Zhang JX, Zhang F (2005) Two new and one newly recorded species of Corinnidae and Liocranidae from Taiwan (Arachnida: Araneae). Acta arachnologica, Tokyo 54: 45 - 49.", "Zhang F, Fu JY, Zhu MS (2009) Spiders of the genus Sphingius (Araneae: Liocranidae) from China, with descriptions of two new species. Zootaxa 2298: 31 - 44.", "Thorell T (1895) Descriptive catalogue of the spiders of Burma. London, 406 pp.", "Barrion AT, Litsinger JA (1995) Riceland Spiders of South and Southeast Asia. CAB International, Wallingford, UK, xix + 700 pp.", "Schenkel E (1963) Ostasiatische Spinnen aus dem Museum d'Histoire naturelle de Paris. Memoires du Museum National d'Histoire Naturelle, Serie A, Zoologie (Paris) 25: 1 - 481."]}
GossiCrypt: Wireless Sensor Network Data Confidentiality Against Parasitic Adversaries
Creators: name: Luo, Jun
name: Papadimitratos, Panos
name: Hubaux, Jean-Pierre
Publisher: name: arXiv
Year: 2008
Subjects: subject: Cryptography and Security (cs.CR)
subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: Resource and cost constraints remain a challenge for wireless sensor network security. In this paper, we propose a new approach to protect confidentiality against a parasitic adversary, which seeks to exploit sensor networks by obtaining measurements in an unauthorized way. Our low-complexity solution, GossiCrypt, leverages on the large scale of sensor networks to protect confidentiality efficiently and effectively. GossiCrypt protects data by symmetric key encryption at their source nodes and re-encryption at a randomly chosen subset of nodes en route to the sink. Furthermore, it employs key refreshing to mitigate the physical compromise of cryptographic keys. We validate GossiCrypt analytically and with simulations, showing it protects data confidentiality with probability almost one. Moreover, compared with a system that uses public-key data encryption, the energy consumption of GossiCrypt is one to three orders of magnitude lower.
Is gravitino still a warm dark matter candidate?
Creators: name: Gorbunov, D.
name: Khmelnitsky, A.
name: Rubakov, V.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We make use of the phase space density approach to discuss gravitino as a warm dark matter candidate. Barring fine tuning between the reheat temperature in the Universe and superparticle masses, we find that \emph{warm} gravitinos have both appropriate total mass density, Omega_{\tilde G} = Ω_{DM} \simeq 0.2, and suitable primordial phase space density at low momenta provided that their mass is in the range 1 keV \lesssim \mg \lesssim 15 keV, the reheat temperature in the Universe is low, T_R \lesssim 10 TeV, and masses of some of the superparticles are sufficiently small, M \lesssim 350 GeV. The latter property implies that the gravitino warm dark matter scenario will be either ruled out or supported by the LHC experiments.
description: 18 pages, 5 figures. Replaced with journal version
The forward masking effect of 2fl-f2 in normal hearing and noise-induced hearing loss subjects
Creators: name: Carson, Arlene Jane
Publisher: name: University of British Columbia
Year: 2010

description: The present study investigated the combination tone 2fl-f2 in normal hearing subjects and subjects with high frequency noise-induced hearing loss by measuring the forward masking effect of 2fl-f2 exerted at its own frequency. Forward masking was plotted as the increase in masked threshold of a brief probe tone located at frequency 2fl-f2 as a function of the intensity of the primary tones, fl and f2. The masking effect of the lower primary alone, fl, was also measured to determine the possible contribution of fl toward the total masking obtained with the fl+f2 stimulus. Results of this investigation showed that 1) a forward-masking effect attributable to 2fl-f2 was seen for each normal-hearing subject, usually beginning at an fl+f2 intensity between 40 and 60 dB SPL. Average slopes of the growth of this masking were 0.8 between 60 and 70 dB SPL and 1.1 between 70 and 80 dB SPL. 2) there was little or no masking effect due to fl+f2 for hearing-loss subjects at intensities between 60 and 70 dB SPL, most likely explained by the fact that the quiet thresholds at the fl, f2, and probe tone frequencies were elevated for these subjects. This finding agreed with published studies by showing that the forward masking effect was strongly and inversely correlated with the quiet thresholds at the fl, f2, and probe tone frequencies (significant to p=.0l). 3) at an fl+f2 intensity of 80 dB SPL, several hearing-loss subjects displayed a masking effect attributable to 2fl-f2. It is not clear why this occurred for some of these subjects, because even at 80 dB SPL, the sensation level of the fl+f2 stimulus was only slightly supra-threshold. 4) for some normal-hearing and hearing-loss subjects a significant masking effect due to fl alone was noted. This finding made it difficult to assess the contribution of 2fl-f2 toward the total masking displayed with the fl+f2 stimulus for these subjects. 5) results with the fl and fl+f2 stimulus were highly variable for both subject groups. 6) the unresolved role of suppression in distortion product generation as well as a limited understanding of noise-induced hearing loss make it difficult to apply the present results toward one particular model of combination tone production.
Euprenolepis maschwitzi Lapolla, 2009, sp. nov.
Creators: name: Lapolla, John S.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Euprenolepis
Euprenolepis maschwitzi

description: Euprenolepis maschwitzi, sp. nov.
(Figures 4A–D)
Holotype worker, MALAYSIA: Borneo, Sabah, Poring Hot Spring, East Ridge, N 06°02’ E 116°42’, 980 m, 31.v.1997 (A. Malsch) (USNM); 2 paratype workers, same locality as holotype (USNM; ANIC); 1 paratype worker, MALAYSIA: Borneo, Sabah, Tawau Nat. Park, N 04°23.8', E 117°53.5, 13.iii.2001 (M. Pfeiffer) (USNM).
 Worker. Measurements (n=3): TL: 3.41–4.02; HW: 0.84–0.89; HL: 0.84–0.93; SL: 1.03–1.14; WL: 1.21–1.36; GL: 1.32–1.73. Indices: CI: 96–100; SI: 116–125.
Head yellowish-brown, with lighter mandibles and funiculi; head about as long as broad. Cuticular surface shiny, weakly rugoreticulate, with scattered erect setae and sparse, scattered pubescence. Posterior margin complete. Scapes surpass posterior margin by about length of the first three funicular segments. Scapes with erect setae and a layer of pubescence, becoming denser distally. Mesosoma brownish-yellow, smooth and slightly dull, legs lighter, especially tarsi. Scattered erect setae of varying length concentrated on posterior pronotum and anterior mesonotum. Pronotum rises gently towards mesonotum (about 30º angle). Propodeum dorsum rounded, dome-like; declivity short, but steep. Petiole triangular, inclined forward, with posterior face longer than anterior face; gaster yellowish-brown with scattered erect setae and no pubescence underneath; cuticular surface slightly dull and weakly rugoreticulate.
 Etymology: The species epithet is given to honor Ulrich Maschwitz for his insightful contributions to Euprenolepis natural history.
 Discussion: This species is most likely to be confused with E. variegata and E. wittei. It can be separated most easily from E. wittei by the scapes, which on E. wittei possess a thick layer of pubescence distally, and by a flatter, more elongated pronotum. Its separation from E. variegata can be more difficult, but E. variegata possesses longer gastral setae overall (majority of setae greater than 0.1 mm in length). Also, E. maschwitzi is lighter in color, being more yellow than either E. variegata or E. wittei, and this species possesses a duller cuticle, especially on the head and gaster.
description: Published as part of Lapolla, John S., 2009, Taxonomic Revision of the Southeast Asian Ant Genus Euprenolepis, pp. 1-25 in Zootaxa 2046 on page 8, DOI: 10.5281/zenodo.186449
Form factors in finite volume I: form factor bootstrap and truncated conformal space
Creators: name: Pozsgay, B.
name: Takacs, G.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Other Condensed Matter (cond-mat.other)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We describe the volume dependence of matrix elements of local fields to all orders in inverse powers of the volume (i.e. only neglecting contributions that decay exponentially with volume). Using the scaling Lee-Yang model and the Ising model in a magnetic field as testing ground, we compare them to matrix elements extracted in finite volume using truncated conformal space approach to exact form factors obtained using the bootstrap method. We obtain solid confirmation for the form factor bootstrap, which is different from all previously available tests in that it is a non-perturbative and direct comparison of exact form factors to multi-particle matrix elements of local operators, computed from the Hamiltonian formulation of the quantum field theory. We also demonstrate that combining form factor bootstrap and truncated conformal space is an effective method for evaluating finite volume form factors in integrable field theories over the whole range in volume.
description: 43 pages, 31 eps figures, LaTeX2e file. v2: main theoretical argument substantially expanded and clarified, typos and references corrected
Broadband Modeling of Low Luminosity Active Galactic Nuclei Detected in Gamma Rays
Creators: name: Tomar, Gunjan
name: Gupta, Nayantara
name: Prince, Raj
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Low luminosity active galactic nuclei are more abundant and closer to us than the luminous ones but harder to explore as they are faint. We have selected the four sources NGC 315, NGC 4261, NGC 1275, and NGC 4486, which have been detected in gamma rays byFermi-LAT. We have compiled their long-term radio, optical, X-ray data from different telescopes, analysed XMM-Newton data for NGC 4486, XMM-Newton and Swift data for NGC 315. We have analysed the Fermi-LAT data collected over the period of 2008 to 2020 for all of them. Electrons are assumed to be accelerated to relativistic energies in sub-parsec scale jets, which radiate by synchrotron and synchrotron self-Compton emission covering radio to gamma-ray energies. This model can fit most of the multi-wavelength data points of the four sources. However, the gamma-ray data points from NGC 315 and NGC 4261 can be well fitted only up to 1.6 GeV and 0.6 GeV, respectively in this model. This motivates us to find out the origin of the higher energy γ-rays detected from these sources. Kilo-parsec scale jets have been observed previously from these sources in radio and X-ray frequencies. If we assume γ-rays are also produced in kilo-parsec scale jets of these sources from inverse Compton scattering of starlight photons by ultra-relativistic electrons, then it is possible to fit the gamma-ray data at higher energies. Our result also suggests that strong host galaxy emission is required to produce GeV radiation from kilo-parsec scale jets.
description: Accepted for publication in ApJ
PEDAGOGICAL FOUNDATIONS OF DEVELOPING SOCIAL AND CULTURAL COMPETENCE IN STUDENTS BASED ON JALALUDDIN RUMI'S MORAL VIEWS
Creators: name: Bayjanova, Sadokat
Publisher: name: Zenodo
Year: 2023

description: This article discusses the characteristics of the moral views of Jalaluddin Rumi, one of the great philosophers of the East, and thus the pedagogical foundations of the development of social competence in students.