cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1: of Understanding the importance of key risk factors in predicting chronic bronchitic symptoms using a machine learning approach
Creators: name: Huiyu Deng
name: Urman, Robert
name: Gilliland, Frank
name: Sandrah Eckel
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Table S1. Comparison of gradient boosting models fit for all participants and all predictors, for 50 different random training sets. Table S2. Accuracy, sensitivity, and specificity of models fit separately with groups of risk factors for all participants, asthmatics, and non-asthmatics, for 50 different random holdout test datasets. Table S3. Average AUC of models trained on various groups of risk factors using data from all participants and validated separately by asthma status, for 50 random training sets. Table S4. Average area under the receiver operating characteristic curve (AUC), accuracy, sensitivity, and specificity of models fit separately with groups of risk factors for non-asthmatics, non-asthmatics (rhinitis), and non-asthmatics (no rhinitis), for 50 different across- and within- participants holdout test datasets. Table S5. Comparison of gradient boosting models vs. logistic regression for all participants, asthmatics, and non-asthmatics averaged across 50 training sets. Table S6. Logistic regression results for all participants, asthmatics, and non-asthmatics for a random training set. Figure S1. Boxplot of relative influence, for 50 different random training sets, of the top 10 risk factors in models fit using all predictor variables for non-asthmatics, non-asthmatics (rhinitis), and non-asthmatics (no rhinitis). Figure S2. Area under the receiver operating characteristic curve (AUC) of the gradient boosting models and logistic regression model models fit separately with all risk factors and top 10 most important risk factors for 50 different random across-participant holdout test datasets. Figure S3. Area under the receiver operating characteristic curve (AUC) of the gradient boosting models and logistic regression models fit separately with all risk factors and top 10 most important risk factors for 50 different random within-participant holdout test datasets. (DOCX 3711 kb)
Sound Propagation in Elongated Bose-Einstein Condensed Clouds
Creators: name: Kavoulakis, G. M.
name: Pethick, C. J.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We consider propagation of sound pulses along the long axis of a Bose-Einstein condensed cloud in a very anisotropic trap. In the linear regime, we demonstrate that the square of the velocity of propagation is given by the square of the local sound velocity, $c^2=nU_0/m$, averaged over the cross section of the cloud. We also carry out calculations in the nonlinear regime, and determine how the speed of the pulse depends on its amplitude.
description: 4 pages, revtex, 3 eps figures
Additional file 1 of A methylation-based nomogram for predicting survival in patients with lung adenocarcinoma
Creators: name: Wang, Xuelong
name: Zhou, Bin
name: Xia, Yuxin
name: Zuo, Jianxin
name: Liu, Yanchao
name: Bi, Xin
name: Luo, Xiong
name: Zhang, Chengwei
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Additional file 1: Table S1. Clinical information analyzed in present study.
The Changing-Look Quasar Mrk 590 is Awakening
Creators: name: Mathur, S.
name: Denney, K. D.
name: Gupta, A.
name: Vestergaard, M.
name: De Rosa, G.
name: Krongold, Y.
name: Nicastro, F.
name: Collinson, J.
name: Goad, M.
name: Korista, K.
name: Pogge, R. W.
name: Peterson, B. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Mrk 590 was originally classified as a Seyfert 1 galaxy, but then it underwent dramatic changes: the nuclear luminosity dropped by over two orders of magnitude and the broad emission lines all but disappeared from the optical spectrum. Here we present followup observations to the original discovery and characterization of this "changing look" active galactic nucleus (AGN). The new Chandra and HST observations from 2014 show that Mrk 590 is awakening, changing its appearance again. While the source continues to be in a low state, its soft excess has re-emerged, though not to the previous level. The UV continuum is brighter by more than a factor of two and the broad MgII emission line is present, indicating that the ionizing continuum is also brightening. These observations suggest that the soft excess is not due to reprocessed hard X-ray emission. Instead, it is connected to the UV continuum through warm Comptonization. Variability of the Fe K-alpha emission lines suggests that the reprocessing region is within about 10 light years or 3 pc of the central source. The AGN type change is neither due to obscuration, nor due to one-way evolution from type-1 to type-2, as suggested in literature, but may be related to episodic accretion events.
description: ApJ, in press
Controllable coupled-resonator-induced transparency in a dual-recycled Michelson interferometer
Creators: name: Yu, Xudong
name: Li, Wei
name: Jin, YuanBin
name: Zhang, Jing
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We theoretically and experimentally study the effect of the coupled-resonator-induced transparency in the Michelson interferometer with the dual-recycled configuration, which is equivalent to the adjustable coupled resonator. The coupling strength, corresponding to the splitting of the reflection spectrum and associated with the width of the coupled-resonator-induced transparent window,can be controlled by adjusting the arm lengths, i.e., the relative phase of the interference arms on the 50/50 beam splitter. Thus, this tunability of the coupling strength can be very fast, and the absorptive and dispersive properties can be effectively controlled. This work provides a new system to coherently control and storage optical field.
Three new VHS-DES Quasars at 6.7 < z < 6.9 and Emission Line Properties at z > 6.5
Creators: name: Reed, S. L.
name: Banerji, M.
name: Becker, G. D.
name: Hewett, P. C.
name: Martini, P.
name: McMahon, R. G.
name: Pons, E.
name: Rauch, M.
name: Abbott, T. M. C.
name: Allam, S.
name: Annis, J.
name: Avila, S.
name: Bertin, E.
name: Brooks, D.
name: Buckley-Geer, E.
name: Rosell, A. Carnero
name: Kind, M. Carrasco
name: Carretero, J.
name: Castander, F. J.
name: Cunha, C. E.
name: D'Andrea, C. B.
name: da Costa, L. N.
name: De Vicente, J.
name: Desai, S.
name: Diehl, H. T.
name: Doel, P.
name: Evrard, A. E.
name: Flaugher, B.
name: Frieman, J.
name: Garcia-Bellido, J.
name: Gaztanaga, E.
name: Gruen, D.
name: Gschwend, J.
name: Gutierrez, G.
name: Hollowood, D. L.
name: Honscheid, K.
name: Hoyle, B.
name: James, D. J.
name: Kuehn, K.
name: Lahav, O.
name: Lima, M.
name: Maia, M. A. G.
name: Marshall, J. L.
name: Miquel, R.
name: Ogando, R. L. C.
name: Plazas, A. A.
name: Roodman, A.
name: Sanchez, E.
name: Scarpine, V.
name: Schubnell, M.
name: Serrano, S.
name: Sevilla-Noarbe, I.
name: Smith, M.
name: Smith, R. C.
name: Sobreira, F.
name: Suchyta, E.
name: Swanson, M. E. C.
name: Tarle, G.
name: Thomas, D.
name: Tucker, D. L.
name: Vikram, V.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We report the results from a search for z > 6.5 quasars using the Dark Energy Survey (DES) Year 3 dataset combined with the VISTA Hemisphere Survey (VHS) and WISE All-Sky Survey. Our photometric selection method is shown to be highly efficient in identifying clean samples of high-redshift quasars leading to spectroscopic confirmation of three new quasars - VDESJ 0244-5008 (z=6.724), VDESJ 0020-3653 (z=6.834) and VDESJ 0246-5219 (z=6.90) - which were selected as the highest priority candidates in the survey data without any need for additional follow-up observations. The new quasars span the full range in luminosity covered by other z>6.5 quasar samples (J AB = 20.2 to 21.3; M1450 = -25.6 to -26.6). We have obtained spectroscopic observations in the near infrared for VDESJ 0244-5008 and VDESJ 0020-3653 as well as our previously identified quasar, VDESJ 0224-4711 at z=6.50 from Reed et al. (2017). We use the near infrared spectra to derive virial black-hole masses from the full-width-half-maximum of the MgII line. These black-hole masses are ~ 1 - 2 x 10$^9$M$_\odot$. Combining with the bolometric luminosities of these quasars of L$_{\rm{bol}}\simeq$ 1 - 3 x 10$^{47}$implies that the Eddington ratios are high - $\simeq$0.6-1.1. We consider the C\textrm{\textsc{IV}} emission line properties of the sample and demonstrate that our high-redshift quasars do not have unusual C\textrm{\textsc{IV}} line properties when compared to carefully matched low-redshift samples. Our new DES+VHS $z>6.5$ quasars now add to the growing census of luminous, rapidly accreting supermassive black-holes seen well into the epoch of reionisation.
description: 12 pages, 9 figures
Charged neutron stars and observational tests of a dark force weaker than gravity
Creators: name: Fabbrichesi, Marco
name: Urbano, Alfredo
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We discuss the possibility of exploring an unbroken U(1) gauge interaction in the dark sector by means of gravitational waves. Dark sector states charged under the dark force can give a macroscopic charge to astronomical bodies. Yet the requirement of having gravitationally bounded stars limits this charge to negligible values if the force has a sizeable strength. Gravitational tests are only possible if the dark force is weaker than gravity. By solving the Einstein-Maxwell field equations, we study in detail an explicit model for dark charge generation and separation in a neutron star. Charged states originate from the decay of neutrons inside the star into three dark fermions; we show that in this model the equation of state is consistent with limits on neutron star masses and tidal deformability. We find that while the dark force can be observed in binary mergers (making them an optimal observational test even though with limited precision), it is Debye screened in binary pulsars (for which more precise data exist). The emitted radiation in the inspiral phase of a binary system is modified and the dark force tested at the level of the uncertainty of the experimental detection. The test covers a region where current limits on deviations from Newton inverse-squared law come from geophysical and laser-ranging observations.
description: 24 pages, 13 figures
Fairleigh Dickinson University Poll: New Jersey September 2018
Creators: name: Fairleigh Dickinson University
Publisher: name: Roper Center for Public Opinion Research
Year: 2019

description: Registered to vote (1); upcoming November elections (2); how often do you vote (1); President Donald Trump job approval (1); country right direction/wrong track (1); New Jersey Governor Phil Murphy job approval (1); New Jersey right direction/wrong track (1); Senator Robert Menendez vs. Bob Hugin for U.S. Senate (1); favorability of public figures (5); Supreme Court nominee Brett Kavanaugh (2); minimum wage (4); source for news about politics and public affairs (1); current Speaker of the House (1); name of individual leading investigation into President Trump (1); which candidate in 2016 presidential election won the popular vote (1); current events (4); prescription pain killers (1); Alzheimer's disease (5).
Edge-driven transition in surface structure of nanoscale silicon
Creators: name: Ismail-Beigi, Sohrab
name: Arias, T. A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We present an ab initio exploration of the phenomena which will become important for freestanding structures of silicon as they are realized on the nanoscale. We find that not only surface but also edge effects are important considerations in structures of dimensions on the order of 3 nm. Specifically, for long nanoscale silicon bars, we find two competing low-energy reconstructions with a transition from one to the other as the cross section of the bar decreases. We predict that this size-dependent phase transition has a signature in the electronic structure of the bar but little effect on elastic properties.
title: Revisited phylogeny of Scleroderminae (Hymenoptera: Bethylidae) reveals a plastic evolutionary history
Creators: name: Vargas R., Juan M.
name: Colombo, Wesley D.
name: Azevedo, Celso O.
Publisher: name: Senckenberg Gesellschaft für Naturforschung
Year: 2020

description: The first comprehensive phylogenetic study of Scleroderminae with all 30 valid genera is presented. It is based on 138 morphological characters. Phylogenetic analyses support the monophyly of the subfamily Scleroderminae. All genus-level clades are monophy-letic, except Cephalonomia. The extensive homoplasy across the topology is regarded as evidence of the high morphological diversity in the subfamily. Thlastepyris marquisensis stat. et comb.n. are transferred from the bethyline subspecies Sierola depressa marquisensis with species status. The traditional characters historically used in the taxonomy of Scleroderminae were mapped onto the new topology, such as body flatness, number of flagellomeres, size shape of wings and the length of 2r-rs&Rs vein of the forewing, and were shown to be highly homoplastic. Five new genera and their respective type-species are proposed, described, and illustrated as follows: Decemnoxus infrequens gen. et sp.n., Longinoxus inusitatus gen. et sp.n., Madanoxus patulus gen. et sp.n., Mutatio mutata gen. et sp.n., and Pilocutis mollis gen. et sp.n., the former four from Madagascar and the latter from Thailand. Madagascar plays an important role in the evolutionary history of Scleroderminae by having several odd morphological pattern and endemic fauna.
Confinement in 3d $\mathcal{N}=2$ $Spin(N)$ gauge theories with vector and spinor matters
Creators: name: Nii, Keita
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present various confinement phases of three-dimensional $\mathcal{N}=2$ $Spin(N)$ gauge theories with vector and spinor matters. The quantum Coulomb branch of the moduli space of vacua is drastically changed when the rank of the gauge group and the matter contents are changed. In many examples, the Coulomb branch is one- or two-dimensional but its interpretation varies. In some examples, the Coulomb branch becomes three-dimensional and we need to introduce a "dressed" Coulomb branch operator.
description: 33 pages
Additional file 2: of The role of the intra-abdominal view in complicated intra-abdominal infections
Creators: name: Tolonen, Matti
name: Sallinen, Ville
name: LeppĂ¤Niemi, Ari
name: BĂ¤Cklund, Minna
name: Mentula, Panu
Publisher: name: figshare
Year: 2019
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Cancer
subject: Plant Biology
subject: Computational Biology

description: Bootstrapping. Legend: Distribution of AUC value in the bootstrap sample (auc.boot) and the distribution of the AUC value deriving from the model fitted to the bootstrap samples and evaluated on the original sample (auc.orig). The blue line represents apparent AUC and the red line AUC adjusted for optimism. (DOCX 65 kb)
Non-Universal Quasi-Long Range Order in the Glassy Phase of Impure Superconductors
Creators: name: Emig, Thorsten
name: Bogner, Simon
name: Nattermann, Thomas
Publisher: name: arXiv
Year: 1999
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The structural correlation functions of a weakly disordered Abrikosov lattice are calculated for the first time in a systematic RG-expansion in d=4-εdimensions. It is shown, that in the asymptotic limit the Abrikosov lattice exhibits still quasi long range translational order described by a non-universal exponent \barη_{\bf G} which depends on the ratio of the renormalized elastic constants κ=\tilde c_{66}/\tilde c_{11} of the flux line (FL) lattice. Our calculations show clearly three distinct scaling regimes corresponding to the Larkin, the manifold and the asymptotic Bragg glass regime. On a wide range of intermediate length scales the FL displacement correlation function increases as a power law with twice of the manifold roughness exponent ζ_{rm}(κ), which is also non-universal. Our results, in particular the κ-dependence of the exponents, are in variance with those of the variational treatment with replica symmetry breaking which allows in principle an experimental discrimination between the two approaches.
description: 4 pages, 3 figures
Disclosing connections between black holes and naked singularities: Horizon remnants, Killing throats and bottlenecks
Creators: name: Pugliese, D.
name: Quevedo, H.
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We study the properties of black holes and naked singularities by considering stationary observers and light surfaces in Kerr spacetimes. We reconsider the notion of Killing horizons from a special perspective by exploring the entire family of Kerr metrics. To this end, we introduce the concepts of extended plane, Killing throats and bottlenecks for weak (slowly spinning) naked singularities. Killing bottlenecks (or horizon remnants in analogy with the corresponding definition of throats in black holes) are restrictions of the Killing throats appearing in special classes of slowly spinning naked singularities. Killing bottlenecks appear in association with the concept of pre-horizon regime introduced in [1, 2]. In the extended plane of the Kerr spacetime, we introduce particular sets, metric bundles, of metric tensors which allow us to reinterpret the concept of horizon and to find connections between black holes and naked singularities throughout the horizons. To evaluate the effects of frame-dragging on the formation and structure of Killing bottlenecks and horizons in the extended plane, we consider also the Kerr-Newman and the Reissner-Norstrom spacetimes. We argue that these results might be significant for the comprehension of processes that lead to the formation and eventually destruction of Killing horizons.
description: 33 pages, 32 multi-panels figures, 3 Tables
Additional file 1 of A novel mechanism for C1GALT1 in the regulation of gastric cancer progression
Creators: name: Dong, Xiaoxia
name: Chen, Chunli
name: Deng, Xinzhou
name: Liu, Yongyu
name: Duan, Qiwen
name: Peng, Zhen
name: Luo, Zhiguo
name: Shen, Li
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Figure S1. Scatter diagrams for C1GALT1 expression versus transcription factors expression in GC samples based on the TCGA and GTEx databases. Figure S2. Effect of SP1 on C1GALT1 expression. C1GALT1 mRNA levels were detected by qRT-PCR. siNC, cells transfected with negative control siRNA; si1, cells transfected with SP1 siRNA1; si2, cells transfected with SP1 siRNA2; Ctrl, cells transfected with control plasmid; SP1, cells transfected with SP1 plasmid. *p < 0.05, **p < 0.01 compared with the siNC or Ctrl group (Student’s t-test). Figure S3. Correlation of miR-148b and C1GALT1 expression in GC tissues (Spearman’s rank correlation test). Table S1. PNA-binding proteins identified by the proteomic analysis. Table S2. The sequence of shRNAs and siRNAs. Table S3. Primer sequences used in the qRT-PCR analysis.
Adversarial Inpainting of Medical Image Modalities
Creators: name: Armanious, Karim
name: Mecky, Youssef
name: Gatidis, Sergios
name: Yang, Bin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Numerous factors could lead to partial deteriorations of medical images. For example, metallic implants will lead to localized perturbations in MRI scans. This will affect further post-processing tasks such as attenuation correction in PET/MRI or radiation therapy planning. In this work, we propose the inpainting of medical images via Generative Adversarial Networks (GANs). The proposed framework incorporates two patch-based discriminator networks with additional style and perceptual losses for the inpainting of missing information in realistically detailed and contextually consistent manner. The proposed framework outperformed other natural image inpainting techniques both qualitatively and quantitatively on two different medical modalities.
description: To be submitted to ICASSP 2019
D3.1 TOPOS Declaration
Creators: name: Spanidis Pavlos
name: Bardi Alessia
name: Garcia Clara
name: Giannakari Olga
name: Tromaras Alkiviadis
Publisher: name: Zenodo
Year: 2020
Subjects: Be open
Transport
Transport research
Open science
Open access
Project

description: This deliverable contributes towards the development of new schemes for membership and governance scheme of the Transport Observatory/fOrum for Promoting Open Science (TOPOS observatory and forum) in order to implement and transition FAIR principles.
 For the industry stakeholders of transport research, long-term learning with an emphasis on sustainability constitutes necessity and as such, they will confirm their continuous engagement with scientific stakeholders. The proposed membership and governance scheme will be built upon recognizing the challenges of data-driven transport research in pursuing excellent science and granting that the vision of Open Science in transport research is an iterative process based on constant learning and mutual alignment. Hence, the proposed schemes will encompass some key elements, such as data culture and management, services and architecture and funding mechanisms.
description: {"references": ["Spanidis Pavlos, Bardi Alessia, Garcia Clara, Giannakari Olga & Tromaras Alkiviadis. (2020). D3.1 TOPOS Declaration. Zenodo."]}
#EsLey. Lessons on the Legalisation of Abortion in Argentina
Creators: name: Slep, Melisa Tatiana
Publisher: name: Zenodo
Year: 2021
Subjects: abortion
Argentina
feminism
advocacy
legalisation of abortion
activism
sexual and reproductive rights
rights-based approach
framing
social movements
social mobilisation
collective action
strategic behaviour

description: The paper focuses on the passing of an abortion bill in Argentina, from the perspective of the multi-stakeholder front that mobilised in its favour the National Campaign for the Right to Abortion. Using frame analysis, the paper goes into three main aspects of feminist activism that have been deemed crucial in guaranteeing the success of such mobilisation efforts: i) the stakeholders coalition that formed around this Campaign; ii) the multitude of strategies designed to reach targeted objectives; and iii) the use of storytelling to shift the narrative and centre the debate in terms of the Campaign. The paper concludes with reflections around the success of the Campaign and its meaning in the Argentinean context, the Latin American context – if not the Global South in general; and some questions regarding potential research avenues for further discussion.
description: {"references": ["Pazmi\u00f1o, S. (2013). El proceso de politizaci\u00f3n de la sexualidad: Identificaciones y marcos de sentido de la acci\u00f3n colectiva / The politicization of sexuality: Identities and frameworks that lend meaning to collective action. Revista Mexicana De Sociolog\u00eda, 75(2), 173-200. Retrieved June 17, 2021, from http://www.jstor.org/stable/43495653", "Ruibal, Alba & Fernandez Anderson, Cora (2018). Legal obstacles and social change: strategies of the abortion rights movement in Argentina, Politics, Groups, and Identities, 8:4, 698-713, DOI: 10.1080/21565503.2018.1541418", "DAWN (22/06/2021). Making history in Argentina: the fight for legal abortion. Available at https://dawnnet.org/publication/making-history-in-argentina-the-fight-for-legal-abortion/", "Motta, S.C. (2019). Feminising our revolutions: New movements in Latin America offer inspiration and re-enchantment. Soundings: A journal of politics and culture 71(71), 15-27. https://www.muse.jhu.edu/article/723166.", "Socorristas en Red (2019). \u00abArchivo Rosa\u00bb. Available at https://archivorosa.socorristasenred.org/ [date accessed 15.06.2021]", "REDAAS (08/06/2021). El camino a la legalizaci\u00f3n del aborto en Argentina. Available at https://youtu.be/q95JglDlM1c"]}
Carbon nanotube-copper fibers produced by electrospinning: electrical conductivity measurements
Creators: name: Daneshvar, Farhad
name: Sue, Hung-Jue
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: Recent advances in nanotechnology have provided new materials which have the potential to surpass copper and aluminum alloys in electrical conductivity, weight and ampacity [2-6]. Among these carbon nanotubes (CNTs) stand out due to their remarkable thermal and electrical conductivity and ampacity (103 times of copper), low density, abundance of precursor materials and supreme mechanical properties. However, making these materials into a continuous fiber or macrostructures has remained the main obstacle. A promising approach to tackle this issue is employing CNTs as nanofillers in copper matrixes. Subramaniam et al. [5] combined several simple fabrication to produce high density CNT (45 vol%)-Cu composite films with specific conductivity 26% greater than copper. These results show that by improving the interfacial interactions between the CNTs and the copper matrix strong and highly conductive nanocomposites can be made. In this research continuous CNT-Cu nanocomposite is produced using electrospinning method. For improving the interfacial interaction the surface of the CNTs were first coated with a thin layer of copper using electroless deposition methods (the process is explained in details in [7]).
description: Presented at PTIC meeting on October 2018
Additional file 1: of The role of the intra-abdominal view in complicated intra-abdominal infections
Creators: name: Tolonen, Matti
name: Sallinen, Ville
name: LeppĂ¤Niemi, Ari
name: BĂ¤Cklund, Minna
name: Mentula, Panu
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Molecular Biology
subject: Ecology
subject: FOS: Biological sciences
subject: Marine Biology
subject: Science Policy
subject: 60506 Virology

description: Paper sheet for the collection of the intra-abdominal findings (DOCX 468 kb)
Acoustically regulated optical emission dynamics from quantum dot-like emission centers in GaN/InGaN nanowire heterostructures
Creators: name: Lazic, S.
name: Chernysheva, E.
name: Hernández-Mínguez, A.
name: Santos, P. V.
name: van der Meulen, H. P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We report on experimental studies of the effects induced by surface acoustic waves on the optical emission dynamics of GaN/InGaN nanowire quantum dots. We employ stroboscopic optical excitation with either time-integrated or time-resolved photoluminescence detection. In the absence of the acoustic wave, the emission spectra reveal signatures originated from the recombination of neutral exciton and biexciton confined in the probed nanowire quantum dot. When the nanowire is perturbed by the propagating acoustic wave, the embedded quantum dot is periodically strained and its excitonic transitions are modulated by the acousto-mechanical coupling. Depending on the recombination lifetime of the involved optical transitions, we can resolve acoustically driven radiative processes over time scales defined by the acoustic cycle. At high acoustic amplitudes, we also observe distortions in the transmitted acoustic waveform, which are reflected in the time-dependent spectral response of our sensor quantum dot. In addition, the correlated intensity oscillations observed during temporal decay of the exciton and biexciton emission suggest an effect of the acoustic piezoelectric fields on the quantum dot charge population. The present results are relevant for the dynamic spectral and temporal control of photon emission in III-nitride semiconductor heterostructures.
description: 14 pages, 5 figures
Qualitative analysis of a scalar-tensor theory with exponential potential
Creators: name: Batista, A. B.
name: Fabris, J. C.
name: Goncalves, S. V. B.
name: Tossa, J.
Publisher: name: arXiv
Year: 2000
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: A qualitative analysis of a scalar-tensor cosmological model, with an exponential potential for the scalar field, is performed. The phase diagram for the flat case is constructed. It is shown that solutions with an initial and final inflationary behaviour appear. The conditions for which the scenario favored by supernova type Ia observations becomes an attractor in the space of the solutions are established.
description: Latex file, 9 pages, 1 figure
Clusterization and deformation of multi-$Λ$ hypernuclei within relativistic mean-field model
Creators: name: Tanimura, Yusuke
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Deformed multi-$Λ$ hypernuclei are studied within a relativistic mean-field model. In this paper, we take some $N=Z$ "hyper isotope" chains, i.e., $^{8+n}_{\ \ nΛ}{\rm Be}$, $^{20+n}_{\ \ \ nΛ}{\rm Ne}$, and $^{28+n}_{\ \ \ nΛ}{\rm Si}$ systems where $n = 2$, $4$ for Be, and $n = 2$, $8$ for Ne and Si. A sign of two-$^6_{2Λ}$He cluster structure is observed in the two-body correlation in $^{12}_{4Λ}$Be. In the Ne hyper isotopes, the deformation is slightly reduced by addition of $Λ$ hyperons whereas it is significantly reduced or even disappears in the Si hyper isotopes.
description: 9 pages, 7 figures, to be submitted to Physical Review C
MOESM2 of Unexpected insertion of carrier DNA sequences into the fission yeast genome during CRISPRâ Cas9 mediated gene deletion
Creators: name: Longmuir, Sophie
name: Akhtar, Nabihah
name: MacNeill, Stuart
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
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
subject: Computational Biology

description: Additional file 2: Methods. Methods for growth and phenotypic analysis of fission yeast, molecular biology and genome editing.
Modelling the spinning dust emission from LDN 1780
Creators: name: Vidal, Matias
name: Dickinson, Clive
name: Harper, S. E.
name: Casassus, Simon
name: Witt, A. N.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study the anomalous microwave emission (AME) in the Lynds Dark Nebula (LDN) 1780 on two angular scales. Using available ancillary data at an angular resolution of 1 degree, we construct an SED between 0.408 GHz to 2997 GHz. We show that there is a significant amount of AME at these angular scales and the excess is compatible with a physical spinning dust model. We find that LDN 1780 is one of the clearest examples of AME on 1 degree scales. We detected AME with a significance > 20$σ$. We also find at these angular scales that the location of the peak of the emission at frequencies between 23-70 GHz differs from the one on the 90-3000 GHz map. In order to investigate the origin of the AME in this cloud, we use data obtained with the Combined Array for Research in Millimeter-wave Astronomy (CARMA) that provides 2 arcmin resolution at 30 GHz. We study the connection between the radio and IR emissions using morphological correlations. The best correlation is found to be with MIPS 70$μ$m, which traces warm dust (T$\sim$50K). Finally, we study the difference in radio emissivity between two locations within the cloud. We measured a factor $\approx 6$ of difference in 30 GHz emissivity. We show that this variation can be explained, using the spinning dust model, by a variation on the dust grain size distribution across the cloud, particularly changing the carbon fraction and hence the amount of PAHs.
description: 14 pages, 11 figures, submitted to MNRAS
Modes of Multiple Star Formation
Creators: name: Adams, Fred C.
name: Myers, Philip C.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This paper argues that star forming environments should be classified into finer divisions than the traditional isolated and clustered modes. Using the observed set of galactic open clusters and theoretical considerations regarding cluster formation, we estimate the fraction of star formation that takes place within clusters. We find that less than 10% of the stellar population originates from star forming regions destined to become open clusters, confirming earlier estimates. The smallest clusters included in the observational surveys (having at least N=100 members) roughly coincide with the smallest stellar systems that are expected to evolve as clusters in a dynamical sense. We show that stellar systems with too few members N < N_\star have dynamical relaxation times that are shorter than their formation times (1-2 Myr), where the critical number of stars N_\star \approx 100. Our results suggest that star formation can be characterized by (at least) three principal modes: I. isolated singles and binaries, II. groups (NN_\star). Many -- if not most -- stars form through the intermediate mode in stellar groups with 10
description: accepted to The Astrophysical Journal
MOESM3 of Unexpected insertion of carrier DNA sequences into the fission yeast genome during CRISPR–Cas9 mediated gene deletion
Creators: name: Longmuir, Sophie
name: Akhtar, Nabihah
name: MacNeill, Stuart
Publisher: name: figshare
Year: 2019
Subjects: 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: Additional file 3: Figures S1–S3. Multiple sequence alignments of Smp1–Smp4 proteins from various Schizosaccharomyces species (Figure S1), basic phenotypic analysis of smp1∆–smp4∆ strains (Figure S2) and insertion sites relative to sgRNA and PAM sequences for all six insertion alleles (Figure S3).
Discovery of Dying Active Galactic Nucleus in Arp 187: Experience of Drastic Luminosity Decline within $10^4$ years
Creators: name: Ichikawa, Kohei
name: Ueda, Junko
name: Bae, Hyun-Jin
name: Kawamuro, Taiki
name: Matsuoka, Kenta
name: Toba, Yoshiki
name: Shidatsu, Megumi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Arp 187 is one of the fading active galactic nuclei (AGN), whose AGN activity is currently decreasing in luminosity. We investigate the observational signatures of AGN in Arp 187, which trace various physical scales from less than 0.1 pc to the nearly 10 kpc, to estimate the longterm luminosity change over $10^{4}$ years. The VLA 5 GHz, 8 GHz, and the ALMA 133 GHz images reveal bimodal jet lobes with $\sim$5 kpc size and the absence of the central radio-core. The 6dF optical spectrum shows that Arp 187 hosts narrow line region with the estimated size of $\sim$1 kpc, and the line strengths give the AGN luminosity of $L_{\rm bol}=1.5 \times 10^{46}$ erg s$^{-1}$. On the other hand, the current AGN activity estimated from the AGN torus emission gives the upper bound of $L_{\rm bol} < 2.2 \times 10^{43}$ erg s$^{-1}$. The absence of the radio-core gives the more strict upper bound of the current AGN luminosity of $L_{\rm bol} < 8.0 \times 10^{40}$ erg s$^{-1}$, suggesting that the central engine is already quenched. These multi-wavelength signatures indicate that Arp 187 hosts a "dying" AGN: the central engine is already dead, but the large scale AGN indicators are still observable as the remnant of the past AGN activity. The central engine has experienced the drastic luminosity decline by a factor of $\sim10^{3-5}$ fainter within $\sim10^{4}$ years, which is roughly consistent with the viscous timescale of the inner part of the accretion disk within $\sim$500 years.
description: 15 pages, 8 figures, accepted for publication in ApJ
What is the central bank of Wikipedia?
Creators: name: Demidov, Denis
name: Frahm, Klaus M.
name: Shepelyansky, Dima L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Social and Information Networks (cs.SI)
subject: Physics and Society (physics.soc-ph)
subject: General Finance (q-fin.GN)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences
subject: FOS: Economics and business

description: We analyze the influence and interactions of 60 largest world banks for 195 world countries using the reduced Google matrix algorithm for the English Wikipedia network with 5 416 537 articles. While the top asset rank positions are taken by the banks of China, with China Industrial and Commercial Bank of China at the first place, we show that the network influence is dominated by USA banks with Goldman Sachs being the central bank. We determine the network structure of interactions of banks and countries and PageRank sensitivity of countries to selected banks. We also present GPU oriented code which significantly accelerates the numerical computations of reduced Google matrix.
Evolution of Magnetic and Superconducting Fluctuations with Doping of High-Tc Superconductors
Creators: name: Blumberg, G.
name: Kang, M.
name: Klein, M. V.
name: Kadowaki, K.
name: Kendziora, C.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Electronic Raman scattering from high- and low-energy excitations was studied as a function of temperature, extent of hole doping, and energy of the incident photons in Bi_2Sr_2CaCu_2O_{8 \pm δ} superconductors. For underdoped superconductors, short range antiferromagnetic (AF) correlations were found to persist with hole doping, and doped single holes were found to be incoherent in the AF environment. Above the superconducting (SC) transition temperature T_c, the system exhibits a sharp Raman resonance of B_{1g} symmetry and energy of 75 meV and a pseudogap for electron-hole excitations below 75 meV, a manifestation of a partially coherent state forming from doped incoherent quasi particles. The occupancy of the coherent state increases with cooling until phase ordering at T_c produces a global SC state.
description: 6 pages, 4 color figures, PDF format
Discovery and Vetting of Exoplanets I: Benchmarking K2 Vetting Tools
Creators: name: Kostov, Veselin B.
name: Mullally, Susan E.
name: Quintana, Elisa V.
name: Coughlin, Jeffrey L.
name: Mullally, Fergal
name: Barclay, Thomas
name: Colon, Knicole D.
name: Schlieder, Joshua E.
name: Barentsen, Geert
name: Burke, Christopher J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We have adapted the algorithmic tools developed during the Kepler mission to vet the quality of transit-like signals for use on the K2 mission data. Using the four sets of publicly-available lightcurves on MAST, we produced a uniformly-vetted catalog of 772 transiting planet candidates from K2 as listed at the NASA Exoplanet archive in the K2 Table of Candidates. Our analysis marks 676 of these as planet candidates and 96 as false positives. All confirmed planets pass our vetting tests. 60 of our false positives are new identifications -- effectively doubling the overall number of astrophysical signals mimicking planetary transits in K2 data. Most of the targets listed as false positives in our catalog either show prominent secondary eclipses, transit depths suggesting a stellar companion instead of a planet, or significant photocenter shifts during transit. We packaged our tools into the open-source, automated vetting pipeline DAVE (Discovery and Vetting of Exoplanets) designed to streamline follow-up efforts by reducing the time and resources wasted observing targets that are likely false positives. DAVE will also be a valuable tool for analyzing planet candidates from NASA's TESS mission, where several guest-investigator programs will provide independent lightcurve sets -- and likely many more from the community. We are currently testing DAVE on recently-released TESS planet candidates and will present our results in a follow-up paper.
description: 43 pages, 23 figures, 5 tables
Additional file 1 of Moderating effect of people-oriented public health services on depression among people under mandatory social isolation during the COVID-19 pandemic: a cross-sectional study in China
Creators: name: Cao, Bolin
name: Wang, Dongya
name: Wang, Yifan
name: Hall, Brian J.
name: Wu, Nan
name: Wu, Meimei
name: Ma, Qishan
name: Tucker, Joseph D.
name: Lv, Xing
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Mental Health

description: Additional files 1. Survey questionnaire.
Additional file 1 of RCPred: RNA complex prediction as a constrained maximum weight clique problem
Creators: name: Legendre, Audrey
name: Angel, Eric
name: Fariza Tahi
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Supplementary statistical results. Supplementary Figures showing the sensitivity, PPV and MCC results of RCPred compared to the results of NanoFolder, NUPACK and MultiRNAFold. (PDF 61.8 kb)
Inter-satellite Quantum Key Distribution at Terahertz Frequencies
Creators: name: Wang, Ziqing
name: Malaney, Robert
name: Green, Jonathan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: Cryptography and Security (cs.CR)
subject: Information Theory (cs.IT)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: Terahertz (THz) communication is a topic of much research in the context of high-capacity next-generation wireless networks. Quantum communication is also a topic of intensive research, most recently in the context of space-based deployments. In this work we explore the use of THz frequencies as a means to achieve quantum communication within a constellation of micro-satellites in Low-Earth-Orbit (LEO). Quantum communication between the micro-satellite constellation and high-altitude terrestrial stations is also investigated. Our work demonstrates that THz quantum entanglement distribution and THz quantum key distribution are viable deployment options in the micro-satellite context. We discuss how such deployment opens up the possibility for simpler integration of global quantum and wireless networks. The possibility of using THz frequencies for quantum-radar applications in the context of LEO deployments is briefly discussed.
description: 7 pages, 6 figures
Wetting and Capillary Condensation in Symmetric Polymer Blends: A comparison between Monte Carlo Simulations and Self-Consistent Field Calculations
Creators: name: Mueller, M.
name: Binder, K.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We present a quantitative comparison between extensive Monte Carlo simulations and self-consistent field calculations on the phase diagram and wetting behavior of a symmetric, binary (AB) polymer blend confined into a film. The flat walls attract one component via a short range interaction. The critical point of the confined blend is shifted to lower temperatures and higher concentrations of the component with the lower surface free energy. The binodals close the the critical point are flattened compared to the bulk and exhibit a convex curvature at intermediate temperatures -- a signature of the wetting transition in the semi-infinite system. Investigating the spectrum of capillary fluctuation of the interface bound to the wall, we find evidence for a position dependence of the interfacial tension. This goes along with a distortion of the interfacial profile from its bulk shape. Using an extended ensemble in which the monomer-wall interaction is a stochastic variable, we accurately measure the difference between the surface energies of the components, and determine the location of the wetting transition via the Young equation. The Flory-Huggins parameter at which the strong first order wetting transition occurs is independent of chain length and grows quadratically with the integrated wall-monomer interaction strength. We estimate the location of the prewetting line. The prewetting manifests itself in a triple point in the phase diagram of very thick films and causes spinodal dewetting of ultrathin layers slightly above the wetting transition. We investigate the early stage of dewetting via dynamic Monte Carlo simulations.
description: to appear in Macromolecules