cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 2 of The PI3K/AKT/mTOR signaling pathway is aberrantly activated in primary central nervous system lymphoma and correlated with a poor prognosis
Creators: name: Zhang, Xiaowei
name: Wu, Yuchen
name: Sun, Xuefei
name: Cui, Qu
name: Bai, Xueyan
name: Dong, Gehong
name: Gao, Zifen
name: Wang, Yaming
name: Gao, Chunji
name: Sun, Shengjun
name: Ji, Nan
name: Liu, Yuanbo
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 2: Supplementary Table S2. Clinical characteristics and prognosis of PCNSL patients and their correlations with the protein expression of p-AKT, p-mTOR, p-S6, p-4E-BP1 and the loss of PTEN.
Electronic States and Anomalous Hall Effect in Strongly Correlated Topological Systems
Creators: name: Irkhin, V. Yu.
name: Skryabin, Yu. N.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: We treat elementary excitations, the spin-liquid state, and the anomalous Hall effect (including the quantum one in purely 2D situation) in layered highly correlated systems. The mechanisms of the formation of a topological state associated with bare flat energy bands, correlations, and spin-orbit interactions, including the appearance of correlated Chern bands, are analyzed. A two-band picture of the spectrum in metallic kagome lattices is proposed, which involves a transition from the ferromagnetic state, a flat strongly correlated band, and a band of light Dirac electrons. In this case, the effect of separation of the spin and charge degrees of freedom turns out to be significant. The application of the representations of the Kotliar-Rukenstein auxiliary bosons and the Ribeiro-Wen dopons to this problem is discussed.
description: Review paper, 8 pages
Lattice Calculations and Hadron Physics
Creators: name: Aoki, Sinya
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We review progress in lattice QCD, focusing on efforts to calculate weak matrix elements relevant for the determination of the Cabibbo-Kobayashi-Maskawa matrix. Topics we discuss include light hadron spectrum and quark masses, CP-violation in K meson decays and weak matrix elements of heavy-light mesons.
description: 26 pages, latex, 12 figures, Talk presented at the 19th International Symposium on Lepton and Photon Interactions at High Energies, Stanford, August 9 - 14, 1999 ; corrections, references and one figure added
Mass Segregation and Equipartition of Energy in Two Globular Clusters with Central Density Cusps
Creators: name: Sosin, Craig
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We begin by presenting the analysis of a set of deep B- and V-band images of the central density cusp of the globular cluster M30 (NGC 7099), taken with the Faint Object Camera aboard the Hubble Space Telescope. These images are the first to resolve lower-mass main-sequence stars in the cluster's central 10''. From the positions of individual stars, we measure an improved position for the cluster center; this new position is 2.6'' from the previously known position. We find no evidence of a ``flat'', constant-surface-density core; however, the data do not rule out the presence of a core of radius up to 1.9'' (95% confidence level). We measure a logarithmic cusp slope (d \log σ/ d \log r$) of -0.76 +- 0.07 (1-sigma) for stars with masses between 0.69 and 0.76 \Msun, and -0.82 +- 0.11 for stars with masses between 0.57 and 0.69 \Msun. We also compare the overall mass function (MF) of the cluster cusp with the MF of a field at r = 4.6' (near the cluster half-mass radius). The observed degree of mass segregation is well matched by the predictions of an isotropic, multimass King model. We then use the Jeans equation to compare the structure of M30 with that of M15, another cusped cluster, using data from this and a previous paper. We find that M30 is very close to achieving equipartition of energy between stellar species, at least over the observed range in mass and radius, while M15 is not. This difference may be a result of the longer relaxation time in the observed field in M15. The data also suggest that the degree of mass segregation within the two cluster cusps is smaller than one would expect from the measurements at larger radius. If so, this phenomenon might be the result of gravothermal oscillations, of centrally-concentrated populations of binaries, or of a ~10^3 \Msun black hole in one or more clusters.
Generalized inequalities for ratio functions of trigonometric and hyperbolic functions
Creators: name: Kostić, Marko
name: Bagul, Yogesh J.
name: Chesneau, Christophe
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Mathematics (math.GM)
subject: FOS: Mathematics

description: The main aim of this note, which can be viewed as a certain addendum to the paper \cite{2019}, is to propose several generalized inequalities for the ratio functions of trigonometric and hyperbolic functions. We basically follow the approach obeyed in this paper.
Euclidean TSP in Narrow Strips
Creators: name: Alkema, Henk
name: de Berg, Mark
name: van der Hofstad, Remco
name: Kisfaludi-Bak, Sándor
Publisher: name: arXiv
Year: 2020
Subjects: subject: Computational Geometry (cs.CG)
subject: FOS: Computer and information sciences

description: We investigate how the complexity of Euclidean TSP for point sets $P$ inside the strip $(-\infty,+\infty)\times [0,δ]$ depends on the strip width $δ$. We obtain two main results. First, for the case where the points have distinct integer $x$-coordinates, we prove that a shortest bitonic tour (which can be computed in $O(n\log^2 n)$ time using an existing algorithm) is guaranteed to be a shortest tour overall when $δ\leq 2\sqrt{2}$, a bound which is best possible. Second, we present an algorithm that is fixed-parameter tractable with respect to $δ$. Our algorithm has running time $2^{O(\sqrtδ)} n + O(δ^2 n^2)$ for sparse point sets, where each $1\timesδ$ rectangle inside the strip contains $O(1)$ points. For random point sets, where the points are chosen uniformly at random from the rectangle $[0,n]\times [0,δ]$, it has an expected running time of $2^{O(\sqrtδ)} n$. These results generalise to point sets $P$ inside a hypercylinder of width $δ$. In this case, the factors $2^{O(\sqrtδ)}$ become $2^{O(δ^{1-1/d})}$.
description: To appear in Discrete & Computational Geometry. See also earlier version in Proceedings 36th International Symposium on Computational Geometry (SoCG 2020)
The bridge number of surface links and kei colorings
Creators: name: Sato, Kouki
name: Tanaka, Kokoro
Publisher: name: arXiv
Year: 2020
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 57K45 (Primary) 57K12 (Secondary)

description: Meier and Zupan introduced bridge trisections of surface links in $S^4$ as a 4-dimensional analogue to bridge decompositions of classical links, which gives a numerical invariant of surface links called the bridge number. We prove that there exist infinitely many surface knots with bridge number $n$ for any integer $n \geq 4$. To prove it, we use colorings of surface links by keis and give lower bounds for the bridge number of surface links.
description: 11 pages, 2 figures, v2: typos corrected and there are some minor revisions
Field distributions in heavy mesons and baryons
Creators: name: Kuzmenko, D. S.
name: Simonov, Yu. A.
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: Field distributions generated by static quark-antiquark and QQQ sources are calculated analytically in the framework of the Field Correlator Method (FCM) using Gaussian (bilocal) correlator. In both cases the string consists mostly of longitudinal color electric field, while transverse electric field contributes locally less then 3%, in agreement with earlier lattice studies. In the QQQ case the profile of the Y shape was calculated for the first time and found to have a complicated structure with a deep well at the string junction position. Possible consequences of this form for the baryon structure are discussed.
description: LaTeX2e, 11 pages, 4 Postscript figures, 2 GIF images, version to appear in Physics Letters B
Preliminary Results from the Sick Childcare Needs Assessment Study
Creators: name: Ahmeti, Shpresa
Publisher: name: Zenodo
Year: 2024
Subjects: public health
sick chilcare
needs assessment
child health
school based health centers
parent survey
sick childcare needs assessment

description: Abstract

Working parents face a challenging predicament when their child falls ill at school or daycare. They must consider factors like the cost of sick childcare, transportation challenges, and potential loss of a day's pay when deciding whether to take time off work. To better understand these challenges and explore parents' needs, preferences, and behaviors related to sick childcare, the "Sick Childcare Needs Assessment Parent Survey" was conducted via social media from January 22 to February 28, 2024. Nineteen employed parents participated (n=19) in the survey. The study examined parents' likely actions if their child became ill, the maximum distance they would travel for sick childcare, interest in home-based sick childcare, perceptions of healthcare access, and the influence of sick childcare subsidies on employment decisions, along with demographic data. Analysis was performed using SPSS, with Chi-Square tests investigating correlations between staying home and factors like income, marital status, gender, and child illness frequency. Results showed no significant association between parents' actions and gender, income, or child illness frequency, nor between income and travel distance for sick childcare. However, a significant association was found between parents' actions and marital status. Overall, parents showed interest in home-based sick childcare and indicated that sick childcare subsidies might influence their decision to remain with an employer. Given the small sample size, these findings should be interpreted with caution. Future research with a larger sample is needed to better understand parents' sick childcare needs and decision-making challenges in accommodating sick childcare.
OILADA E'TIQOD TARBIYASI, UNING PSIXOLOGIK MOHIYATI VA SOG'LOM RUHIYATNI SHAKLLANTIRISHDAGI O'RNI
Creators: name: Axmedova Shahnoza Ismatovna  Buxoro Viloyati G'ijduvon tumani 4-umumta'lim maktabi amaliyotchi psixologi
Publisher: name: Zenodo
Year: 2024

description:  

Annotatsiya: Ushbu maqola oilada iymonni tarbiyalashning psixologik mohiyatini va uning sog'lom psixikani shakllantirishdagi muhim ro`lini o'rganadi. Keng qamrovli adabiyotlarni tahlil qilish orqali tadqiqot iymonning turli o'lchovlarini, uning psixologik rivojlanishiga ta'sirini va e'tiqodga asoslangan tarbiyani tarbiyalashda qo'llaniladigan usullarni o'rganadi. Natijalar oiladagi iymon va bardoshli va muvozanatli psixikani shakllantirish o'rtasidagi ijobiy bog'liqlikni ta'kidlaydi. Muhokama bo'limi ushbu topilmalarning oqibatlari to'g'risida tushuncha beradi, bu esa oilaviy dinamikada iymonni rivojlantirish bo'yicha yakuniy mulohazalar va amaliy takliflarga olib keladi.

 Kalit so'zlar: Iymon, oila, tarbiya, psixologik rivojlanish, sog'lom ruhiyat, e'tiqod tizimlari.
Quark Orbital Angular Momentum from Lattice QCD
Creators: name: Mathur, N.
name: Dong, S. J.
name: Liu, K. F.
name: Mankiewicz, L.
name: Mukhopadhyay, N. C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We calculate the quark orbital angular momentum of the nucleon from the quark energy-momentum tensor form factors on the lattice. The disconnected insertion is estimated stochastically which employs the $Z_2$ noise with an unbiased subtraction. This reduced the error by a factor of 4 with negligible overhead. The total quark contribution to the proton spin is found to be $0.30 \pm 0.07$. From this and the quark spin content we deduce the quark orbital angular momentum to be $0.17 \pm 0.06$ which is $\sim 34$% of the proton spin. We further predict that the gluon angular momentum to be $0.20 \pm 0.07$, i. e. $\sim$ 40% of the proton spin is due to the glue.
description: 4 pages, 7 figures
SHOIR TILAK JO`RA IJODIDA LIRIK QAHRAMON VA TABIAT TASVIRI UYG`UNLIGI
Creators: name: Giyazova, Shahnoza
Publisher: name: Zenodo
Year: 2024

description: Ushbu maqolada shoir Tilak Jo`ra ijodining o’ziga xos xususiyatlari, ifoda uslublari, lirik qahramon holatining tabiat bilan uyg`unligi haqida fikr yuritiladi. Ijodkorning badiiy mahorati,  tasviriy vositalardan foydalanishdagi ijodiy kashfiyotlari she’riy parchalar orqali tahlil qilingan. Tilak Jo`ra ijodining mavzu jihatdan rang-barangligi, sodda va xalqonaligi yoritilgan.
The Large N Limit of ${\cal N}=1$ Field Theories from F Theory
Creators: name: Ahn, Changhyun
name: Oh, Kyungho
name: Tatar, Radu
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study AdS/CFT correspondence in four dimensional N=1 field theories realized on the worldvolume of D3 branes near the intersections between D7 and D7' branes in F theory studied by Aharony et al. We consider the compactification of F theory on elliptically fibered Calabi-Yau threefolds corresponding to two sets of parallel D7 branes sharing six spacetime directions. This can be viewed as orbifolds of six torus T^6 by Z_p x Z_q (p, q=2, 3, 4, 6). We find the large N spectrum of chiral primary operators by exploiting the property of AdS/CFT correspondence. Moreover, we discuss supergravity solutions for D3 branes in D7 and D7' branes background.
description: 12 pages, latex, v2: reference on eq. (4.3) added, v3: corrected the discussion on chiral primary field and its analysis in page 7, v4: corrected the statement between (3.3) and (3.4)
On the balanced condition for the Eguchi-Hanson metric
Creators: name: Aghedu, Francesco Cannas
Publisher: name: arXiv
Year: 2018
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 53C55, 58C25, 58F06

description: Let $g_{EH}$ be the Eguchi-Hanson metric on the blow-up of $\mathbb{C}^2$ at the origin. In this paper we show that $mg_{EH}$ is not balanced for any positive integer $m$.
description: 9 pages, 1 figure, to appear in Journal of Geometry and Physics
Wilker and Huygens type inequalities for mixed trigonometric-hyperbolic functions
Creators: name: Bagul, Yogesh J.
name: Dhaigude, Ramkrishna M.
name: Bhayo, Barkat A.
name: Raut, Vinay M.
Publisher: name: arXiv
Year: 2020
Subjects: subject: General Mathematics (math.GM)
subject: FOS: Mathematics

description: Motivated by the work of J. Sándor [19], in this paper we establish a new Wilker type and Huygens type inequalities involving the trigonometric and hyperbolic functions. Moreover, in terms of hyperbolic functions, the upper and lower bounds of sin(x)/x and tan(x)/x are given.
title: 01_1247
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Additional file 8: of Whole genome sequencing of Trypanosoma cruzi field isolates reveals extensive genomic variability and complex aneuploidy patterns within TcII DTU
Creators: name: Reis-Cunha, João
name: Baptista, Rodrigo
name: Rodrigues-Luiz, Gabriela
name: Coqueiro-Dos-Santos, Anderson
name: Valdivia, Hugo
name: Almeida, Laila De
name: Cardoso, Mariana
name: D’Ávila, Daniella
name: Dias, Fernando
name: Fujiwara, Ricardo
name: Galvão, Lúcia
name: Egler Chiari
name: Cerqueira, Gustavo
name: Bartholomeu, Daniella
Publisher: name: figshare
Year: 2018
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified

description: Table S5. T. cruzi read libraries description. (DOCX 14 kb)
Influence of Earth-Directed Coronal Mass Ejections on the Sun's Shadow Observed by the Tibet-III Air Shower Array
Creators: name: Amenomori, M.
name: Bi, X. J.
name: Chen, D.
name: Chen, T. L.
name: Chen, W. Y.
name: Cui, S. W.
name: Danzengluobu
name: Ding, L. K.
name: Feng, C. F.
name: Feng, Zhaoyang
name: Feng, Z. Y.
name: Gou, Q. B.
name: Guo, Y. Q.
name: He, H. H.
name: He, Z. T.
name: Hibino, K.
name: Hotta, N.
name: Hu, Haibing
name: Hu, H. B.
name: Huang, J.
name: Jia, H. Y.
name: Jiang, L.
name: Kajino, F.
name: Kasahara, K.
name: Katayose, Y.
name: Kato, C.
name: Kawata, K.
name: Kozai, M.
name: Labaciren
name: Le, G. M.
name: Li, A. F.
name: Li, H. J.
name: Li, W. J.
name: Liu, C.
name: Liu, J. S.
name: Liu, M. Y.
name: Lu, H.
name: Meng, X. R.
name: Miyazaki, T.
name: Munakata, K.
name: Nakajima, T.
name: Nakamura, Y.
name: Nanjo, H.
name: Nishizawa, M.
name: Niwa, T.
name: Ohnishi, M.
name: Ohta, I.
name: Ozawa, S.
name: Qian, X. L.
name: Qu, X. B.
name: Saito, T.
name: Saito, T. Y.
name: Sakata, M.
name: Sako, T. K.
name: Shao, J.
name: Shibata, M.
name: Shiomi, A.
name: Shirai, T.
name: Sugimoto, H.
name: Takita, M.
name: Tan, Y. H.
name: Tateyama, N.
name: Torii, S.
name: Tsuchiya, H.
name: Udo, S.
name: Wang, H.
name: Wu, H. R.
name: Xue, L.
name: Yamamoto, Y.
name: Yamauchi, K.
name: Yang, Z.
name: Yuan, S. A. F.
name: Zhai, L. M.
name: Zhang, H. M.
name: Zhang, J. L.
name: Zhang, X. Y.
name: Zhang, Y.
name: Zhang, Yi
name: Zhang, Ying
name: Zhaxisangzhu
name: Zho, X. X.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We examine the possible influence of Earth-directed coronal mass ejections (ECMEs) on the Sun's shadow in the 3~TeV cosmic-ray intensity observed by the Tibet-III air shower (AS) array. We confirm a clear solar-cycle variation of the intensity deficit in the Sun's shadow during ten years between 2000 and 2009. This solar-cycle variation is overall reproduced by our Monte Carlo (MC) simulations of the Sun's shadow based on the potential field model of the solar magnetic field averaged over each solar rotation period. We find, however, that the magnitude of the observed intensity deficit in the Sun's shadow is significantly less than that predicted by MC simulations, particularly during the period around solar maximum when a significant number of ECMEs is recorded. The $χ^2$ tests of the agreement between the observations and the MC simulations show that the difference is larger during the periods when the ECMEs occur, and the difference is reduced if the periods of ECMEs are excluded from the analysis. This suggests the first experimental evidence of the ECMEs affecting the Sun's shadow observed in the 3~TeV cosmic-ray intensity.
description: 11 pages, 3 figures, accepted for publication in the ApJ
Supplementary Material 1: from The source of microbial transmission influences niche colonization and microbiome development
Creators: name: Tanger, Isabel S.
name: Stefanschitz, Julia
name: Schwert, Yannick
name: Roth, Olivia
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 310499
subject: Evolutionary biology not elsewhere classified
classificationCode: 310799
subject: Microbiology not elsewhere classified
classificationCode: 320499
subject: Immunology not elsewhere classified

description: Sampling protocol
A Determination of the Spectral Index of Galactic Synchrotron Emission in the 1-10 GHz range
Creators: name: Platania, P.
name: Bensadoun, M.
name: Bersanelli, M.
name: De Amici, G.
name: Kogut, A.
name: Levin, S.
name: Maino, D.
name: Smoot, G. F.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present an analysis of simultaneous multifrequency measurements of the Galactic emission in the 1-10 GHz range with 18 degrees, angular resolution taken from a high altitude site. Our data yield a determination of the synchrotron spectral index between 1.4 GHz and 7.5 GHz of 2.81 +/- 0.16. Combining our data with the maps from Haslam et al. (1982) and Reich & Reich (1986) we find 2.76 +/- 0.11 in the 0.4 - 7.5 GHz range. These results are in agreement with the few previously published measurements. The variation of spectral index with frequency based on our results and compared with other data found in the literature suggests a steepening of the synchrotron spectrum towards high frequencies as expected from theory, because of the steepening of the parent cosmic ray electron energy spectrum. Comparison between the Haslam data and the 19 GHz map (Cottingham 1987) also indicates a significant spectral index variation on large angular scale. Addition quality data are necessary to provide a serious study of these effects.
description: 12 pages, 8 figures
Neural Networks-Based Automatic Audio Classification for Al-Quran Chapters
Creators: name: Radwan, Wael
Publisher: name: Manara - Qatar Research Repository
Year: 2025
Subjects: classificationCode: 40
subject: Engineering

description: Al-Quran Audio classification is one example of content-based analysis of audio signals. This study aims to design a neural network that is able to classify Al-Quran audio files to the correct chapter [special characters omitted] and this requires implementing state of the art Convolutional Neural Network (CNN) to train Al-Quran Dataset and predict the correct chapter (سورة ). In order to achieve this aim, a critical evaluation of the current state of the automatic based reciting classification of Al-Quran was conducted, and the principles, assumptions and methods at the field were used to present a prototype based on this evaluation. Special focus is placed upon creating a suitable robust Quranic dataset and on discovering the features of that dataset that make it possible for an automated recognition of Al-Quran chapters and recitation. In addition, it sets out principles that should be kept in mind when designing Al-Quran reciting recognition and learning systems, and a prototype based on these features is presented. The thesis provides a framework for the auditory classification of Al-Quran chapters, as the final results shows that the use of a newly created IQRA-15 dataset and CNN as a model architecture produced in excess of 90% accuracy on unseen data. This is a proof of concept that deep learning can achieve good results when applied to Al-Quran. This knowledge can be used to design an AI based system for self-correcting Al-Quran recitation for Arabs and non-native Arabic speakers.
title: 20_F_ROUSSET_LeFilsDeSatan_FR_GAD
Creators: name: Rousset, Pierre
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2024
Subjects: subject: Horizon 2020
subject: Plassard, Didier
subject: Guignol (personnage fictif)
subject: PuppetPlays
subject: Horizon 2020
subject: Plassard, Didier
subject: Guignol (personnage fictif)

description: MAM - Musée des Arts de la Marionnette (Musée Gadagne). B84 D86. Acquis de Durafour, 69 rue Cuvier Lyon le 1er mai 1927
Numérisé dans le cadre du projet ERC PuppetPlays, financé par le Programme de recherche et d'innovation Horizon 2020 de l'Union européenne (Grant Agreement 835193).
description: Digitized by the ERC project PuppetPlays, receiving funding from the European Union's Horizon 2020 research and innovation programme under Grant Agreement ERC 835193.
Discovery of stable surfaces with extreme work functions by high-throughput density functional theory and machine learning
Creators: name: Schindler, Peter
name: Antoniuk, Evan R.
name: Cheon, Gowoon
name: Zhu, Yanbing
name: Reed, Evan J.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Computational Physics (physics.comp-ph)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: The work function is the key surface property that determines how much energy is required for an electron to escape the surface of a material. This property is crucial for thermionic energy conversion, band alignment in heterostructures, and electron emission devices. Here, we present a high-throughput workflow using density functional theory (DFT) to calculate the work function and cleavage energy of 33,631 slabs (58,332 work functions) that we created from 3,716 bulk materials, including up to ternary compounds. The number of materials for which we calculated surface properties surpasses the previously largest database, the Materials Project, by a factor of $\sim$27. On the tail ends of the work function distribution we identify 34 and 56 surfaces with an ultra-low (<2 eV) and ultra-high (>7 eV) work function, respectively. Further, we discover that the $(100)$-Ba-O surface of BaMoO$_3$ and the $(001)$-F surface of Ag$_2$F have record-low (1.25 eV) and record-high (9.06 eV) steady-state work functions without requiring coatings, respectively. Based on this database we develop a physics-based approach to featurize surfaces and use supervised machine learning to predict the work function. We find that physical choice of features improves prediction performance far more than choice of model. Our random forest model achieves a mean absolute test error of 0.09 eV, which is more than 6 times better than the baseline and comparable to the accuracy of DFT. This surrogate model enables rapid predictions of the work function ($\sim 10^5$ faster than DFT) across a vast chemical space and facilitates the discovery of material surfaces with extreme work functions for energy conversion, electronic applications, and contacts in 2-dimensional devices.
description: 13 pages, 5 figures
Nodal Loop and Nodal Surface States in Ti3Al Family Materials
Creators: name: Zhang, Xiaoming
name: Yu, Zhi-Ming
name: Zhu, Ziming
name: Wu, Weikang
name: Wang, Shan-Shan
name: Sheng, Xian-Lei
name: Yang, Shengyuan A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Topological metals and semimetals are new states of matter which attract great interest in current research. Here, based on first-principles calculations and symmetry analysis, we propose that the family of titanium-based compounds Ti3X (X=Al, Ga, Sn, Pb) are unexplored topological semimetals. These materials feature the coexistence of a nodal loop and a nodal surface in their low-energy band structure. Taking Ti3Al as an example, we show that the material has an almost ideal nodal loop in the sense that the loop is close to the Fermi level and it is nearly flat in energy with energy variation <0.25 meV. The loop is protected by either one of the two independent symmetries: the combined spacetime inversion symmetry and the mirror reflection symmetry. The nodal surface at the k_z=πplane is guaranteed by the nonsymmorphic screw rotational symmetry and the time reversal symmetry. We discuss the effect of spin-orbit coupling and construct an effective model for describing the nodal loop. Our findings indicate that the Ti3Al family compounds can serve as an excellent material platform for studying new topological phases and particularly the interplay between nodal-loop and nodal-surface fermions.
Supplementary Material 3: from The source of microbial transmission influences niche colonization and microbiome development
Creators: name: Tanger, Isabel S.
name: Stefanschitz, Julia
name: Schwert, Yannick
name: Roth, Olivia
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 310499
subject: Evolutionary biology not elsewhere classified
classificationCode: 310799
subject: Microbiology not elsewhere classified
classificationCode: 320499
subject: Immunology not elsewhere classified

description: Summary of Indicator species analysis transfer during pregnancy
Estimating Mixed-Memberships Using the Symmetric Laplacian Inverse Matrix
Creators: name: Qing, Huan
name: Wang, Jingli
Publisher: name: arXiv
Year: 2020
Subjects: subject: Machine Learning (stat.ML)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Mixed membership community detection is a challenging problem. In this paper, to detect mixed memberships, we propose a new method Mixed-SLIM which is a spectral clustering method on the symmetrized Laplacian inverse matrix under the degree-corrected mixed membership model. We provide theoretical bounds for the estimation error on the proposed algorithm and its regularized version under mild conditions. Meanwhile, we provide some extensions of the proposed method to deal with large networks in practice. These Mixed-SLIM methods outperform state-of-art methods in simulations and substantial empirical datasets for both community detection and mixed membership community detection problems.
Four-fermion production with RACOONWW
Creators: name: Denner, A.
name: Dittmaier, S.
name: Roth, M.
name: Wackeroth, D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: RACOONWW is an event generator for e+e- --> WW --> 4fermions(+gamma) that includes full tree-level predictions for e+e- --> 4f and e+e- --> 4f+gamma as well as O(alpha) corrections to e+e- --> 4f in the so-called double-pole approximation. We briefly sketch the concept of the calculation on which this generator is based and present some numerical results.
description: 9 pages, latex, 6 postscript files, to appear in the proceedings of the UK Phenomenology Workshop on Collider Physics, Durham, UK, 19-24 September, 1999
The Hyades: distance, structure, dynamics, and age
Creators: name: Perryman, M. A. C.
name: Brown, A. G. A.
name: Lebreton, Y.
name: Gomez, A.
name: Turon, C.
name: de Strobel, G. Cayrel
name: Mermilliod, J. C.
name: Robichon, N.
name: Kovalevsky, J.
name: Crifo, F.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use absolute trigonometric parallaxes from the Hipparcos Catalogue to determine individual distances to members of the Hyades cluster, from which the 3-dimensional structure of the cluster can be derived. Inertially-referenced proper motions are used to rediscuss distance determinations based on convergent-point analyses. A combination of parallaxes and proper motions from Hipparcos, and radial velocities from ground-based observations, are used to determine the position and velocity components of candidate members with respect to the cluster centre, providing new information on cluster membership: 13 new candidate members within 20 pc of the cluster centre have been identified. Farther from the cluster centre there is a gradual merging between certain cluster members and field stars, both spatially and kinematically. Within the cluster, the kinematical structure is fully consistent with parallel space motion of the component stars with an internal velocity dispersion of about 0.3 km/s. The spatial structure and mass segregation are consistent with N-body simulation results, without the need to invoke expansion, contraction, rotation, or other significant perturbations of the cluster. The quality of the individual distance determinations permits the cluster zero-age main sequence to be accurately modelled. The helium abundance for the cluster is determined to be Y=0.26+/-0.02 which, combined with isochrone modelling including convective overshooting, yields a cluster age of 625+/-50 Myr. The distance to the observed centre of mass is 46.34+/-0.27 pc, corresponding to a distance modulus m-M=3.33+/-0.01 mag for the objects within 10 pc of the cluster centre (roughly corresponding to the tidal radius). Discrepancies with previous distance estimates are investigated and explained.
description: Accepted for publication in Astronomy and Astrophysics, 40 pages, including 35 PS -figures, uses AA tex-macros, PS-version available at http://www.strw.leidenuniv.nl/~brown/hyades.html
Anchor Cascade for Efficient Face Detection
Creators: name: Yu, Baosheng
name: Tao, Dacheng
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Face detection is essential to facial analysis tasks such as facial reenactment and face recognition. Both cascade face detectors and anchor-based face detectors have translated shining demos into practice and received intensive attention from the community. However, cascade face detectors often suffer from a low detection accuracy, while anchor-based face detectors rely heavily on very large networks pre-trained on large scale image classification datasets such as ImageNet [1], which is not computationally efficient for both training and deployment. In this paper, we devise an efficient anchor-based cascade framework called anchor cascade. To improve the detection accuracy by exploring contextual information, we further propose a context pyramid maxout mechanism for anchor cascade. As a result, anchor cascade can train very efficient face detection models with a high detection accuracy. Specifically, comparing with a popular CNN-based cascade face detector MTCNN [2], our anchor cascade face detector greatly improves the detection accuracy, e.g., from 0.9435 to 0.9704 at 1k false positives on FDDB, while it still runs in comparable speed. Experimental results on two widely used face detection benchmarks, FDDB and WIDER FACE, demonstrate the effectiveness of the proposed framework.
High Resolution Imaging of the Magnetic Field in the central parsec of the Galaxy
Creators: name: Roche, P. F.
name: Lopez-Rodriguez, E.
name: Telesco, C. M.
name: Schodel, R.
name: Packham, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We discuss a high resolution (FWHM~ 0.45 arcsec) image of the emissive polarization from warm dust in the minispiral in the Galactic Centre and discuss the implications for the magnetic field in the dusty filaments. The image was obtained at a wavelength of 12.5 microns with the CanariCam multimode mid-infrared imager on the Gran Telescopio Canarias. It confirms the results obtained from previous observations but also reveals new details of the polarization structures. In particular, we identify regions of coherent magnetic field emission at position angles of ~45 deg to the predominantly north--south run of field lines in the Northern Arm which may be related to orbital motions inclined to the general flow of the Northern Arm. The luminous stars that have been identified as bow-shock sources in the Northern Arm do not disrupt or dilute the field but are linked by a coherent field structure, implying that the winds from these objects may push and compress the field but do not overwhelm it. The magnetic field in the the low surface brightness regions in the East-West Bar to the south of SgrA* lies along the Bar, but the brighter regions generally have different polarization position angles, suggesting that they are distinct structures. In the region of the Northern Arm sampled here, there is only a weak correlation between the intensity of the emission and the degree of polarization. This is consistent with saturated grain alignment where the degree of polarization depends on geometric effects, including the angle of inclination of the field to the line of sight and superposition of filaments with different field directions, rather than the alignment efficiency.
description: 9 pages, 3 figures, Proceedings of Cosmic Dust X, held in Mitaka, Japan in August 2017
Additional file 7: of Whole genome sequencing of Trypanosoma cruzi field isolates reveals extensive genomic variability and complex aneuploidy patterns within TcII DTU
Creators: name: Reis-Cunha, João
name: Baptista, Rodrigo
name: Rodrigues-Luiz, Gabriela
name: Coqueiro-Dos-Santos, Anderson
name: Valdivia, Hugo
name: Almeida, Laila De
name: Cardoso, Mariana
name: D’Ávila, Daniella
name: Dias, Fernando
name: Fujiwara, Ricardo
name: Galvão, Lúcia
name: Egler Chiari
name: Cerqueira, Gustavo
name: Bartholomeu, Daniella
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Figure S3. Read Depth Coverage of the chromosome 11 in the Y strain and clones. In this picture, the blue lines correspond to the normalized RDC of each position of the chromosome 11, estimated by the ratio between the RDC and the genome coverage. The red line corresponds to the 248 kb position in the chromosome. Below, the protein-coding genes are depicted as rectangles drawn as proportional to their length, and their coding strand is indicated by their position above (top strand) or below (bottom strand) the central line. Cyan and black rectangles represent multigene families and hypothetical/housekeeping genes, respectively. The initial 248-kb in this chromosome had a smaller RDC when compared to remaining sequence in the Y strain as well as in all three Y clones evaluated. (DOCX 226 kb)
Additional file 4 of SUPERGNOVA: local genetic correlation analysis reveals heterogeneous etiologic sharing of complex traits
Creators: name: Zhang, Yiliang
name: Lu, Qiongshi
name: Ye, Yixuan
name: Huang, Kunling
name: Liu, Wei
name: Wu, Yuchang
name: Zhong, Xiaoyuan
name: Li, Boyang
name: Yu, Zhaolong
name: Travers, Brittany G.
name: Werling, Donna M.
name: Li, James J.
name: Zhao, Hongyu
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Statistics
subject: FOS: Mathematics

description: Additional file 4. Review history.
Factorization and q-Deformed Algebra of Quantum Anharmonic Oscillator
Creators: name: Bak, Dongsu
name: Kim, Sang Pyo
name: Kim, Sung Ku
name: Soh, Kwang-Sup
name: Yee, Jae Hyung
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We have studied the underlying algebraic structure of the anharmonic oscillator by using the variational perturbation theory. To the first order of the variational perturbation, the Hamiltonian is found to be factorized into a supersymmetric form in terms of the annihilation and creation operators, which satisfy a q-deformed algebra. This algebraic structure is used to construct all the eigenstates of the Hamiltonian.
description: 6 pages, no figures, revtex
Large Deviations for High Minima of Gaussian Processes with Nonnegatively Correlated Increments
Creators: name: Selk, Zachary
Publisher: name: arXiv
Year: 2021
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 60G15, 60G22, 60K25, 60G55, 60F10

description: In this article we prove large deviations principles for high minima of Gaussian processes with nonnegatively correlated increments on arbitrary intervals. Furthermore, we prove large deviations principles for the increments of such processes on intervals $[a,b]$ where $b-a$ is either less than the increment or twice the increment, assuming stationarity of the increments. As a chief example, we consider fractional Brownian motion and fractional Gaussian noise for $H\geq 1/2$.
description: Comments Welcome!
Efficient amplification of superpositions of coherent states using input states with different parities
Creators: name: Oh, Changhun
name: Jeong, Hyunseok
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We investigate an experimentally feasible scheme for amplification of superpositions of coherent states (SCSs) in light fields. This scheme mixes two input SCSs at a 50:50 beam splitter and performs post-selection by a homodyne detection on one output mode. The key idea is to use two different types of SCSs with opposite parities for input states, which results in an amplified output SCS with a nearly perfect fidelity.
description: 10 pages, 8 figures
Collapsing and group growth as obstructions to Einstein metrics on some smooth 4-manifolds
Creators: name: Peruyero, Haydeé Contreras
name: Suárez-Serrato, Pablo
Publisher: name: arXiv
Year: 2021
Subjects: subject: Differential Geometry (math.DG)
subject: Group Theory (math.GR)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 53C25, 53C23, 57R57

description: We show that a combination of collapsing and excessive growth from the fundamental group impedes the existence of Einstein metrics on several families of smooth four-manifolds. These include infrasolvmanifolds whose fundamental group is not virtually nilpotent, most elliptic surfaces of zero Euler characteristic, geometrizable manifolds with hyperbolic factor geometries in their geometric decomposition, and higher graph four-manifolds without purely negatively curved pieces.
description: 13 pages. v2; Final version, corrected typos, added references, streamlined exposition. To appear in the New York Jour. Math
The detection of the lambda 2175 A feature, and further analysis of the BAL line profile structure in the gravitational lens candidate UM425
Creators: name: Michalitsianos, A. G.
name: Falco, E. E.
name: Munoz, J. A.
name: Hintzen, P.
name: Kazanas, D.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We obtained MMT spectra of the gravitational lens candidate UM425 to compare the redshifts and line profile structures of lens components A and B, which are separated by ~6.5". The CIV lambda 1550 A emission in both A and B exhibits Broad Absorption Line (BAL) structure, consistent with the earlier detection of BAL structure in OVI lambda 1033 A and NV lambda 1240 A that was found with the International Ultraviolet Explorer (IUE) in component A. Cross-correlation of the spectra of A and B using emission lines of CIV lambda 1550 A, HeII lambda 1640 A, NIII lambda 1750 A, CIII] lambda 1909 A and MgII lambda 2800 A reveals a difference in the redshifts of A & B. However, the detailed BAL line profile structure found in spectra of A & B are strikingly similar to one another, which suggests the system is lensed. The spectra of A & B also indicate significant dust extinction, which we base on the presence of the lambda 2175 A absorption feature in the rest frame of the QSO (z_{QSO}=1.47). This feature is commonly seen in galactic sources, but is not generally observed in QSO spectra. Our spectra show the presence of the lambda 2175 A absorption feature in spectra of both images associated with the gravitational lens UM425. Based upon the strong similarity of BAL line profile structure exhibited by UM425A&B, particularly the presence of the lambda 2175 dust absorption feature in spectra of both images, we conclude that UM425 is a gravitational lens.
description: 13 pp, 2 figs, Accepted by ApJL
Monte Carlo study of the discontinuous quantum phase transition in the transverse-field Ising model on the pyrochlore lattice
Creators: name: Emonts, Patrick
name: Wessel, Stefan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The antiferromagnetic Ising model on the pyrochlore lattice exhibits a quantum phase transition in an applied transverse field from the low-field quantum spin-ice phase to the high-field polarized regime. Recent field-theoretical analysis and series expansion results indicate this to be a discontinuous, first-order transition. Here, we explore this transition using quantum Monte Carlo simulations in order to assess this scenario and study the thermodynamic properties in the vicinity of the quantum phase transition. For this purpose, we also consider several variants of extended cluster-update schemes for the transverse field Ising antiferromagnet on frustrated lattices and compare their performance to the conventional bond-based algorithm for the transverse field Ising model on the pyrochlore lattice.
description: 13 pages, 15 figures, v2: as published
Supplementary Material 2 from The source of microbial transmission influences niche colonization and microbiome development
Creators: name: Tanger, Isabel S.
name: Stefanschitz, Julia
name: Schwert, Yannick
name: Roth, Olivia
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 310499
subject: Evolutionary biology not elsewhere classified
classificationCode: 310799
subject: Microbiology not elsewhere classified
classificationCode: 320499
subject: Immunology not elsewhere classified

description: DNA Extraction protocol
Additional file 3: of Relationship between volume and outcome for congenital diaphragmatic hernia: a systematic review protocol
Creators: name: Morche, Johannes
name: Mathes, Tim
name: Jacobs, Anja
name: Pietsch, Barbara
name: Wessel, Lucas
name: Gruber, Sabine
name: Neugebauer, Edmund
name: Pieper, Dawid
Publisher: name: figshare
Year: 2018
Subjects: subject: Physiology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: Computational Biology

description: List of conferences. (DOCX 14Â kb)