cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Standard and non-standard neutrino-antineutrino oscillation analyses and event reconstruction studies using Markov chain Monte Carlo methods at T2K
Creators: name: Sztuc, Artur
Publisher: name: Imperial College London
Year: 2020

description: T2K (from Tokai-to-Kamioka) is a long-baseline neutrino experiment using an off-axis neutrino beam to produce a narrow neutrino energy spectrum. T2K uses a near detector (ND280) to constrain the neutrino cross-section and beam flux systematics for the neutrino oscillation analyses, and provides some of the world's leading cross-section measurements. The neutrino beam is directed to, and detected at, Super-Kamiokande, a large 50\,kT Water Cherenkov detector that is also being used to study atmospheric, cosmic, supernovae neutrinos and more. We describe the oscillation analysis for the T2K experiment that uses both near and far detector data, using Markov Chain Monte Carlo techniques to construct the Bayesian posterior probability distributions for the oscillation parameters. The analysis of the full T2K run 1–9 data with the reactor constraint on $sin^2\theta_{13}$ show that the CP conserving values of $\delta_{CP}$ are rejected with at least 2\,$\sigma$ confidence and intervals between -2.95 and -0.50 with the best fit point -1.82\,rad, whereas the 3\,$\sigma$ intervals are -$\pi$ – 0.13 \& 2.80 – $\pi$. The Normal Mass hierarchy has 88.9\% of the total Markov Chain Monte Carlo steps, corresponding to the likelihood-ratio of the two hypotheses, Bayes Factor, of 8.0. This can be considered as “substantial” on the Jeffreys scale, which is an interpretation the strength of Bayes Factors. The best fit point of $sin^2\theta_{23}$ is 0.537, preferring higher octant with 79.5\% Markov Chain Monte Carlo steps. This corresponds to the Bayes Factor of 3.4, again “substantial” on the Jeffreys scale. Neither run 1–9c nor full run 1–9d data are incompatible with the PMNS model. The 1\,$\sigma$ intervals for $P(\nu_{\mu} \rightarrow \nu_e)$ and $P(\bar{\nu}_{\mu} \rightarrow \bar{\nu}_e)$ posterior probability distributions for both PMNS and non-PMNS analyses comfortably overlap. Far more data from the T2K's far detector, Super-K, is needed to see any potential deviations; we are currently statistically limited. We also describe the development of a novel neutrino event reconstruction method for large Water Cherenkov detectors using similar Bayesian methods as in the oscillation analysis.
Turbulent magnetic pressure instability in stratified turbulence
Creators: name: Kemel, Koen
name: Brandenburg, Axel
name: Kleeorin, Nathan
name: Rogachevskii, Igor
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: A reduction of total mean turbulent pressure due to the presence of magnetic fields was previously shown to be a measurable effect in direct numerical simulations. However, in the studied parameter regime the formation of large-scale structures, as anticipated from earlier mean-field simulations, was not found. An analysis of the relevant mean-field parameter dependency and the parameter domain of interest is conducted in order to clarify this apparent discrepancy.
description: 3 pages, 2 figures, proceedings of IAU Symp. 274, Advances in Plasma Astrophysics, ed. A. Bonanno, E. de Gouveia dal Pino and A. Kosovichev
The Radio-FIR correlation in the Milky Way
Creators: name: Zhang, J.
name: Hopkins, A.
name: Barnes, P. J.
name: Cagnes, M.
name: Yonekura, Y.
name: Fukui, Y.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate the scale on which the correlation arises between the 843 MHz radio and the 60 micron far-infrared (FIR) emission from star forming regions in the Milky way. The correlation, which exists on the smallest scales investigated (down to ~4 pc), becomes noticeably tight on fields of size 30', corresponding to physical scales of ~20-50 pc. The FIR to radio flux ratio on this scale is consistent with the radio emission being dominated by thermal emission. We also investigate the location dependence of q_mean, a parameter measuring the mean FIR to radio flux ratio, of a sample of star forming regions. We show that q_mean displays a modest dependence on galactic latitude. If this is interpreted as a dependence on the intensity of star formation activity, the result is consistent with studies of the Large Magellanic Cloud (LMC) and other nearby galaxies that show elevated values for q in regions of enhanced star formation.
description: 7 pages, 4 figures, accepted for publication by PASA
Additional file 1: of Arginine does not rescue p.Q188R mutation deleterious effect in classic galactosemia
Creators: name: Haskovic, Minela
name: Derks, Britt
name: van der Ploeg, Liesbeth
name: Trommelen, Jorn
name: Nyakayiru, Jean
name: van Loon, Luc
name: Mackinnon, Sabrina
name: Yue, Wyatt
name: Peake, Roy
name: Zha, Li
name: Demirbas, Didem
name: Qi, Wanshu
name: Huang, Xiaoping
name: Berry, Gerard
name: Achten, Jelle
name: Bierau, Jörgen
name: Estela Rubio-Gozalbo, M.
name: Coelho, Ana
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology

description: Figure S1. Expired breath 13CO2 enrichments. Expired breath 13CO2 enrichments of the four galactosemia patients, before and after arginine aspartate supplementation. Results are expressed as mean ± SEM. (PDF 95 kb)
XMM-Newton observations of the X-ray soft polar QS Telescopii
Creators: name: Traulsen, I.
name: Reinsch, K.
name: Schwope, A. D.
name: Burwitz, V.
name: Dreizler, S.
name: Schwarz, R.
name: Walter, F. M.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. On the basis of XMM-Newton observations, we investigate the energy balance of selected magnetic cataclysmic variables, which have shown an extreme soft-to-hard X-ray flux ratio in the ROSAT All-Sky Survey. Aims. We intend to establish the X-ray properties of the system components, their flux contributions, and the accretion geometry of the X-ray soft polar QS Tel. In the context of high-resolution X-ray analyses of magnetic cataclysmic variables, this study will contribute to better understanding the accretion processes on magnetic white dwarfs. Methods. During an intermediate high state of accretion of QS Tel, we have obtained 20 ks of XMM-Newton data, corresponding to more than two orbital periods, accompanied by simultaneous optical photometry and phase-resolved spectroscopy. We analyze the multi-wavelength spectra and light curves and compare them to former high- and low-state observations. Results. Soft emission at energies below 2 keV dominates the X-ray light curves. The complex double-peaked maxima are disrupted by a sharp dip in the very soft energy range (0.1-0.5 keV), where the count rate abruptly drops to zero. The EPIC spectra are described by a minimally absorbed black body at 20 eV and two partially absorbed MEKAL plasma models with temperatures around 0.2 and 3 keV. The black-body-like component arises from one mainly active, soft X-ray bright accretion region nearly facing the mass donor. Parts of the plasma emission might be attributed to the second, virtually inactive pole. High soft-to-hard X-ray flux ratios and hardness ratios demonstrate that the high-energy emission of QS Tel is substantially dominated by its X-ray soft component.
description: Accepted for publication in Astronomy and Astrophysics. 7 pages, 4 figures, 2 tables
Additional file 2: of Arginine does not rescue p.Q188R mutation deleterious effect in classic galactosemia
Creators: name: Haskovic, Minela
name: Derks, Britt
name: van der Ploeg, Liesbeth
name: Trommelen, Jorn
name: Nyakayiru, Jean
name: van Loon, Luc
name: Mackinnon, Sabrina
name: Yue, Wyatt
name: Peake, Roy
name: Zha, Li
name: Demirbas, Didem
name: Qi, Wanshu
name: Huang, Xiaoping
name: Berry, Gerard
name: Achten, Jelle
name: Bierau, Jörgen
name: Estela Rubio-Gozalbo, M.
name: Coelho, Ana
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Table S1. Concentration of arginine in the cell culture supernatant. The concentration of arginine was measured at day 0 and 3 of incubation in two wildtype (Control line 1 and 2) and two classic galactosemic fibroblasts derived from two p.Q188R/p.Q188R patients (cell lines CG1 and CG2) in the absence and in the presence of supplemental arginine (0.1 mM and 1 mM arginine). Results are expressed as μM. (PDF 16 kb)
Chemical evolution during gas-rich galaxy interactions
Creators: name: Perez, Josefa
name: Michel-Dansac, Leo
name: Tissera, Patricia
Publisher: name: arXiv
Year: 2011
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We analyse a set of galaxy interactions performed by using a self-consistent chemo-hydrodynamical model which includes star formation, Supernova feedback and chemical evolution. In agreement with previous works, we find that tidally-induced low-metallicity gas inflows dilute the central oxygen abundance and contribute to the flattening of the metallicity gradients. The tidally-induced inflows trigger starbursts which increase the impact of SN II feedback injecting new chemical elements and driving galactic winds which modulate the metallicity distribution. Although $α$-enhancement in the central regions is detected as a result of the induced starbursts in agreement with previous works, our simulations suggest that this parameter can only provide a timing of the first pericentre mainly for non-retrograde encounters. In order to reproduce wet major mergers at low and high redshifts, we have run simulations with respectively 20 and 50 percent of the disc in form of gas. We find that the more gas-rich encounters behave similarly to the less rich ones, between the first and second pericentre where low-metallicity gas inflows are triggered. However, the higher strength of the inflows triggered in the more gas-rich interactions produces larger metal dilutions factors which are afterward modulated by the new chemical production by Supernova. We find that the more gas-rich interaction develops violent and clumpy star formation triggered by local instabilities all over the disc before the first pericentre, so that if these galaxies were observed at these early stages where no important tidally-induced inflows have been able to develop yet, they would tend to show an excess of oxygen. We find a global mean correlation of both the central abundances and the gradients with the strength of the star formation activity. [abridged]
description: 13 pages, 13 figures, accepted for publication in MNRAS
Additional file 14: of Transcriptome analysis reveals a composite molecular map linked to unique seed oil profile of Neocinnamomum caudatum (Nees) Merr
Creators: name: Gan, Yi
name: Song, Yu
name: Chen, Yadong
name: Liu, Hongbo
name: Yang, Dongdong
name: Xu, Qianyu
name: Zheng, Zhifu
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Space Science
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Computational Biology

description: The codon-optimized sequence of NcFATB. The full-length CDS of NcFATB was codon optimized and chemically synthesized in Genscript Co. Ltd. (China) for further validation of gene function in E. coli BL21 (DE3) cells. (DOCX 14 kb)
Helical Luttinger Liquids and Three Dimensional Black Holes
Creators: name: Balasubramanian, Vijay
name: García-Etxebarria, Iñaki
name: Larsen, Finn
name: Simón, Joan
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Cold interacting fermions in two dimensions form exactly solvable Luttinger liquids, whose characteristic scaling exponents differ from those of conventional Fermi liquids. We use the AdS/CFT correspondence to discuss an equivalence between a class of helical, strongly coupled Luttinger liquids and fermions propagating in the background of a 3D black hole. The microscopic Lagrangian is explicitly known and the construction is fully embeddable in string theory. The retarded Green function at low temperature and energy arises from the geometry very near the black hole horizon. This structure is universal for all cold, charged liquids with a dual description in gravity.
description: 4 pages
Extended Schmidt Law: Role Of Existing Stars In Current Star Formation
Creators: name: Shi, Yong
name: Helou, George
name: Yan, Lin
name: Armus, Lee
name: Wu, Yanling
name: Papovich, Casey
name: Stierwalt, Sabrina
Publisher: name: arXiv
Year: 2011
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We propose an "extended Schmidt law" with explicit dependence of the star formation efficiency (SFE=SFR/Mgas) on the stellar mass surface density. This relation has a power-law index of 0.48+-0.04 and an 1-sigma observed scatter on the SFE of 0.4 dex, which holds over 5 orders of magnitude in the stellar density for individual global galaxies including various types especially the low-surface-brightness (LSB) galaxies that deviate significantly from the Kennicutt-Schmidt law. When applying it to regions at sub-kpc resolution of a sample of 12 spiral galaxies, the extended Schmidt law not only holds for LSB regions but also shows significantly smaller scatters both within and across galaxies compared to the Kennicutt-Schmidt law. We argue that this new relation points to the role of existing stars in regulating the SFE, thus encoding better the star formation physics. Comparison with physical models of star formation recipes shows that the extended Schmidt law can be reproduced by some models including gas free-fall in a stellar-gravitational potential and pressure-supported star formation. By implementing this new law into the analytic model of gas accretion in Lambda CDM, we show that it can re-produce the observed main sequence of star-forming galaxies (a relation between the SFR and stellar mass) from z=0 up to z=2.
description: 18 pages, 9 figures; Accepted for Publication In ApJ
Learning When Training Data are Costly: The Effect of Class Distribution on Tree Induction
Creators: name: Provost, F.
name: Weiss, G. M.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: For large, real-world inductive learning problems, the number of training examples often must be limited due to the costs associated with procuring, preparing, and storing the training examples and/or the computational costs associated with learning from them. In such circumstances, one question of practical importance is: if only n training examples can be selected, in what proportion should the classes be represented? In this article we help to answer this question by analyzing, for a fixed training-set size, the relationship between the class distribution of the training data and the performance of classification trees induced from these data. We study twenty-six data sets and, for each, determine the best class distribution for learning. The naturally occurring class distribution is shown to generally perform well when classifier performance is evaluated using undifferentiated error rate (0/1 loss). However, when the area under the ROC curve is used to evaluate classifier performance, a balanced distribution is shown to perform well. Since neither of these choices for class distribution always generates the best-performing classifier, we introduce a budget-sensitive progressive sampling algorithm for selecting training examples based on the class associated with each example. An empirical analysis of this algorithm shows that the class distribution of the resulting training set yields classifiers with good (nearly-optimal) classification performance.
Laplacian-level density functionals for the exchange-correlation energy of low-dimensional nanostructures
Creators: name: Pittalis, S.
name: Rasanen, E.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In modeling low-dimensional electronic nanostructures, the evaluation of the electron-electron interaction is a challenging task. Here we present an accurate and practical density-functional approach to the two-dimensional many-electron problem. In particular, we show that spin-density functionals in the class of meta-generalized-gradient approximations can be greatly simplified by reducing the explicit dependence on the Kohn-Sham orbitals to the dependence on the electron spin density and its spatial derivatives. Tests on various quantum-dot systems show that the overall accuracy is well preserved, if not even improved, by the modifications.
China's Chang'e-5 Landing Site: An Overview
Creators: name: Qian, Yuqi
Publisher: name: Zenodo
Year: 2021
Subjects: Chang'e-5
Planetary Geology

description: This is an 2021 NASA Exploration Science Forum & European Lunar Symposium (https://lunarscience.arc.nasa.gov/nesfels2021/) presentation , entitled "China’s Chang’e 5 Landing Site: An Overview" in Session "Destinations (Landing Sites)". The abstract is available through: https://dl.airtable.com/.attachments/183cc4ef1c49d3de46244134264ef2d8/fd27c944/NESF_ELS_2021_Abstract_Chang27e-52028YQ2004-07-2129.pdf 2021 NESF & ELS is a virtual meeting and this presentation happened on July 22, 2021. The corresponding presentation video has been uploaded to Youtube: https://youtu.be/6Sny2KCGRQI Anyone use this presentation anywhere for any purpose should cite this abstract. Questions and comments can be submitted to:
 Yuqi Qian
 School of Earth Sciences
 China University of Geosciences, Wuhan
 yuqii.qian@gmail.com
description: {"references": ["Qian et al., Young lunar mare basalts in the Chang'e-5 sample return region, northern Oceanus Procellarum. Earth Planet. Sci. Lett. 555, 116702 (2021).", "Qian et al., China's Chang'e-5 landing site: Geology, stratigraphy, and provenance of materials. Earth Planet. Sci. Lett. 561, 116855 (2021).", "Qian et al., The Long Sinuous Rille System in Northern Oceanus Procellarum and Its Relation to the Chang'e-5 Returned Samples. Geophys. Res. Lett. 48, e2021GL092663 (2021)."]}
Hydrodynamic modeling of deconfinement phase transition in nuclear collisions
Creators: name: Mishustin, I. N.
name: Merdeev, A. V.
name: Satarov, L. M.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The (3+1)-dimensional ideal hydrodynamics is used to simulate collisions of gold nuclei with bombarding energies from 1 to 160 GeV per nucleon. The initial state is represented by two cold Lorentz-boosted nuclei. Two equations of state: with and without the deconfinement phase transition are used. We have investigated dynamical trajectories of compressed baryon-rich matter as functions of various thermodynamical variables. The parameters of collective flow and hadronic spectra are calculated. It is shown that presence of the deconfinement phase transition leads to increase of the elliptic flow and to flattening of proton rapidity distributions.
description: 11 pages, 6 figures
Characterisation of observability and controllability for nonuniformly sampled discrete systems
Creators: name: Fúster-Sabater, Amparo
name: Guillén, J. M.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Discrete Mathematics (cs.DM)
subject: FOS: Computer and information sciences
subject: F.1.1
subject: 93C55, 93B10

description: A joint characterisation of the observability and controllability of a particular kind of discrete system has been developed. The key idea of the procedure can be reduced to a correct choice of the sampling sequence. This freedom, owing to the arbitrary choice of the sampling instants, is used to improve the sensitivity of system observability and controllability, by exploiting an adequate geometric structure. Some qualitative examples are presented for illustrative purposes.
description: 13 pages; 2 figures
A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
Creators: name: Plionis, M.
name: Terlevich, R.
name: Basilakos, S.
name: Bresolin, F.
name: Terlevich, E.
name: Melnick, J.
name: Chavez, R.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We explore the possibility of setting stringent constraints to the Dark Energy equation of state using alternative cosmic tracers like: (a) the Hubble relation using HII galaxies, which can be observed at much higher redshifts (z~3.5) than those currently traced by SNIa samples, and (b) the large-scale structure using the clustering of X-ray selected AGN,which have a redshift distribution peaking at z~1. We use extensive Monte-Carlo simulations to define the optimal strategy for the recovery of the dark-energy equation of state using the high redshift (z~2) Hubble relation, but accounting also for the effects of gravitational lensing, which for such high redshifts can significantly affect the derived cosmological constraints. Based on a "Figure of Merit" analysis, we provide estimates for the number of 2
description: MNRAS in press, 12 colour figures
Improving finite-volume diffusive fluxes through better reconstruction
Creators: name: Sejekan, Chandan Balachandra
Publisher: name: University of British Columbia
Year: 2016

description: The overarching goal of CFD is to compute solutions with low numerical error. For finite-volume schemes, this error originates as error in the flux integral. For diffusion problems on unstructured meshes, the diffusive flux (computed from reconstructed gradients) is one order less accurate than the reconstructed solution. Worse, the gradient errors are not smooth, and so no error cancellation accompanies the flux integration, reducing the flux integral to zero order for second-order schemes. Our aim is to compute the gradient and flux more accurately at the cell boundaries and hence obtain a better flux integral for a slight increase in computational cost. We propose a novel reconstruction method and flux discretization to improve diffusive flux accuracy on cell-centred, isotropic unstructured meshes. Our approach uses a modified least-squares system to reconstruct the solution to second-order accuracy in the H₁ norm instead of the prevalent L₂ norm, thus ensuring second-order accurate gradients. Either circumcentres or containment centres are chosen as the control-volume reference points based on a criteria to facilitate calculation of second-order gradients at flux quadrature points using a linear interpolation scheme along with a high-accuracy jump term to enhance stability of the system. Numerical results show a significant improvement in the order of accuracy of the computed diffusive flux as well as the flux integral. When applied to a channel flow advection-diffusion problem, the scheme resulted in an increased order of accuracy for the flux integral along with gains in solution accuracy by a factor of two. The characteristics of the new scheme were studied through stability, truncation error and cost analysis. The increase in computational costs were modest and affordable. The behaviour of the scheme was also tested by implementing a variation of it within the ANSYS Fluent discretization framework.
Generalized Geologic Map for Land-Use Planning: Rowan County, Kentucky
Creators: name: Carey, Daniel I.
name: Dever, Garland R.
name: Flanders, Cam
Publisher: name: Kentucky Geological Survey, University of Kentucky
Year: 2007

description: Abstract:
This map is not intended to be used for selecting individual sites. Its purpose is to inform land-use planners, government officials, and the public in a general way about geologic bedrock conditions that affect the selection of sites for various purposes. The properties of thick soils may supercede those of the underlying bedrock and should be considered on a site-to-site basis. At any site, it is important to understand the characteristics of both the soils and the underlying rock.
Glomus tumour of pulp of 3rd toe
Creators: name: CHARY, DURAIKANNU
Publisher: name: EURORAD
Year: 2013
Subjects: subject: Musculoskeletal soft tissue
subject: MR
subject: MR-Angiography
subject: Ultrasound
subject: Diagnostic procedure
subject: Pathology

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 21 years
description: Clinical History: 21-year-old male patient with severe pain and tenderness and cold hypersensitivity in base of distal phalanx of right 3rd toe for 4 years. On examination no obvious swelling was seen and the overlying skin was normal. Final Diagnosis: Glomus tumour
Generalized Geologic Map for Land-Use Planning: Taylor County, Kentucky
Creators: name: Carey, Daniel I.
name: Pike, Adam
Publisher: name: Kentucky Geological Survey, University of Kentucky
Year: 2007

description: Abstract:
This map is not intended to be used for selecting individual sites. Its purpose is to inform land-use planners, government officials, and the public in a general way about geologic bedrock conditions that affect the selection of sites for various purposes. The properties of thick soils may supercede those of the underlying bedrock and should be considered on a site-to-site basis. At any site, it is important to understand the characteristics of both the soils and the underlying rock.
Type II Shocks Characteristics: Comparison with associated CMEs and Flares
Creators: name: Pothitakis, G.
name: Mitsakou, E.
name: Preka-Papadema, P.
name: Moussas, X.
name: Caroubalos, C.
name: Alissandrakis, C. E.
name: Hillaris, A.
name: Tsitsipis, P.
name: Kontogeorgos, A.
name: Bougeret, J. -L.
name: Dumas, G.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: A number of metric (100-650 MHz) typeII bursts was recorded by the ARTEMIS-IV radiospectrograph in the 1998-2000 period; the sample includes both CME driven shocks and shocks originating from flare blasts. We study their characteristics in comparison with characteristics of associated CMEs and flares.
description: Recent Advances in Astronomy and Astrophysics: 7th International Conference of the Hellenic Astronomical Society. AIP Conference Proceedings, Volume 848, pp. 238-242 (2006)
Additional file 1: of Resilience to cognitive impairment in the oldest-old: design of the EMIF-AD 90+ study
Creators: name: Legdeur, Nienke
name: Badissi, Maryam
name: Carter, Stephen
name: de Crom, Sophie
name: van de Kreeke, Aleid
name: Vreeswijk, Ralph
name: Trappenburg, Marijke
name: Oudega, Mardien
name: Koek, Huiberdina
name: van Campen, Jos
name: Keijsers, Carolina
name: Amadi, Chinenye
name: Hinz, Rainer
name: Gordon, Mark
name: Novak, Gerald
name: Podhorna, Jana
name: SernĂŠ, Erik
name: Verbraak, Frank
name: Yaqub, Maqsood
name: Hillebrand, Arjan
name: Griffa, Alessandra
name: Pendleton, Neil
name: Kramer, Sophia
name: Teunissen, Charlotte
name: Lammertsma, Adriaan
name: Barkhof, Frederik
name: van Berckel, Bart
name: Scheltens, Philip
name: Muller, Majon
name: Maier, Andrea
name: Herholz, Karl
name: Visser, Pieter
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Neuroscience
subject: Biotechnology
subject: Evolutionary Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Mental Health
subject: Hematology

description: Table S1. Brain MRI scan analyses in the EMIF-AD 90+ Study. (DOCX 26 kb)
Very‑high resolution earth observation data and open‑source solutions for mapping urban areas in sub-Saharan Africa. Implementation of an operational framework for production of geoinformation: Application on Ouagadougou (Burkina Faso) and Dakar (Senegal)
Creators: name: Grippa, Taïs
Publisher: name: Zenodo
Year: 2019
Subjects: Remote sensing
Geomatics
Thesis
ULB
African cities
Urban areas
Land cover
Land use
Population estimation

description: Nowadays, in sub-Saharan Africa (SSA), about 40% of the population is urban and this region is expected to face the highest growth rates during the next decades. By 2100, the three most populated cities in the world will be located in SSA. As a consequence of the extremely fast transformations experienced during the last decades, SSA cities are facing social and environmental issues combined with a lack of financial means and capacity in urban planning and management. The poorest often constitute a large part of the urban population that is extremely vulnerable to health and disaster risks.

In SSA cities, up-to-date and spatially detailed geographic information is often missing. This lack of information is an important issue for many scientific studies focusing on different urban issues and there is a real need to improve the availability of geoinformation for these cities in order to support urban planning, urban management, environment monitoring, epidemiology or risk assessment, etc. . . The work presented in this thesis aims to develop different frameworks for the production of geoinformation. For this purpose, advantage is taken of Very-High Resolution Remote Sensing imagery (0.5 meters) and open-source software. These frameworks implement cutting-edge methods and can handle a large amount of data in a semi-automated fashion to produce maps covering very large areas of interest. In the spirit of open science, the processing chains are entirely based on open-source software and are released publicly in open-access for any interested researchers, in order to make the methods developed completely transparent and in order to contribute to the creation of a pool of common tools and scientific knowledge. These frameworks are used to produce very detailed land-cover and land-use maps that provide essential information such as the built-up density, or the fact that a neighborhood is residential or not. This detailed geoinformation is then used as indicators of presence of populated places to improve existing population models at the intra-urban level.
BioExcel Webinar #75: VIAMD: A Software for Visual Analysis of Molecular Dynamics
Creators: name: Skånberg, Robin
name: Linares, Mathieu
Publisher: name: Zenodo
Year: 2024
Subjects: webinar

description: The typical workflow in molecular dynamics (MD) analysis requires several separate tools, often resulting in a lack of synergy and interaction between the individual analysis steps. In this seminar, we will present VIAMD [1] (https://github.com/scanberg/viamd) , an application designed to address this issue by integrating a 3D visualization of molecular trajectories with flexible analysis components. VIAMD uses an interactive scripting interface, allowing for property definition and evaluation. The application provides context-aware suggestions and expression feedback through information and visualizations. The user-defined properties can be explored and analyzed through the various components. This enables correlation with spatial conformations, statistical analysis of distributions, and powerful aggregation of multidimensional properties such as spatial distribution functions. We would be happy to use data from the participants for the webinar, so contact us if you are willing to share your data with us.

[1] Skånberg et al., J. Chem. Inf. Model. 2023, 63, 23, 7382–7391 (2023)
Large-N_c operator analysis of 2-body meson-baryon counterterms in the chiral Lagrangian
Creators: name: Lutz, M. F. M.
name: Semke, A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The chiral SU(3) Lagrangian with the baryon octet and decuplet fields is considered. The Q^2 counterterms involving the decuplet fields are constructed. We derive the correlation of the chiral parameters implied by the 1/N_c expansion at leading order in QCD.
description: 20 pages, 3 figures
Additional file 1: of Development and validation of the Ulcerative Colitis patient-reported outcomes signs and symptoms (UC-pro/SS) diary
Creators: name: Higgins, Peter
name: Harding, Gale
name: Revicki, Dennis
name: Globe, Gary
name: Patrick, Donald
name: Fitzgerald, Kristina
name: Viswanathan, Hema
name: Donelson, Sarah
name: Ortmeier, Brian
name: Chen, Wen
name: Leidy, Nancy
name: DeBusk, Kendra
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Pharmacology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences

description: UC-PRO/SS Supplementary Material. (DOCX 130 kb)
Low temperature properties of the infinite-dimensional attractive Hubbard model
Creators: name: Koga, Akihisa
name: Werner, Philipp
Publisher: name: arXiv
Year: 2011
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We investigate the attractive Hubbard model in infinite spatial dimensions by combining dynamical mean-field theory with a strong-coupling continuous-time quantum Monte Carlo method. By calculating the superfluid order parameter and the density of states, we discuss the stability of the superfluid state. In the intermediate coupling region above the critical temperature, the density of states exhibits a heavy fermion behavior with a quasi-particle peak in the dense system, while a dip structure appears in the dilute system. The formation of the superfluid gap is also addressed.
description: 8 pages, 9 figures
Additional file 1: of Transcriptome analysis reveals a composite molecular map linked to unique seed oil profile of Neocinnamomum caudatum (Nees) Merr
Creators: name: Gan, Yi
name: Song, Yu
name: Chen, Yadong
name: Liu, Hongbo
name: Yang, Dongdong
name: Xu, Qianyu
name: Zheng, Zhifu
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Lipid analysis of N. caudatum tissue samples. The total lipid content and FA compositions of leaves, flowers and developing fruits (20, 52, 81, 96, 126 and 146 days after flowering, DAF) were quantified with GC-FID. Data are means Âą SD of three biological replications. (DOCX 19 kb)
Additional file 3: of Identification and validation of NOLC1 as a potential target for enhancing sensitivity in multidrug resistant non-small cell lung cancer cells
Creators: name: Huang, Huaping
name: Li, Tangying
name: Chen, Mingjing
name: Liu, Feng
name: Wu, Haifeng
name: Wang, Jie
name: Chen, Jialiang
name: Li, Xi
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Table S3. Classification of upregulated DEGs between A549/MDR cells and A549/DDP cells according to GO terms with p value <â 0.05. DEGs: differentially expressed genes; GO, Gene Ontology. (DOCX 15 kb)
Landau-Zener-Stückelberg Spectroscopy of a Superconducting Flux Qubit
Creators: name: Xu, Shuang
name: Sun, Guozhu
name: Yu, Yang
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We proposed a new method to measure the energy spectrum of a superconducting flux qubit. Different from the conventional frequency spectroscopy, a short triangle pulse is used to drive the qubit through the anticrossing and generates Landau-Zener-Stückelberg interference patterns, from which the information of the energy spectrum can be extracted. Without installing microwave lines one can simplify the experimental setup and reduce the unwanted effects of noise. Moreover, the method can be applied to other quantum systems, opening the possibility of calibrating and manipulating qubits with linear pulses.
description: 7 pages, 5 figures
The atoll sign
Creators: name: Oreste, Donato
Publisher: name: EURORAD
Year: 2013
Subjects: subject: Lung
subject: CT
subject: Diagnostic procedure
subject: Infection
subject: Inflammation

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 74 years
description: Clinical History: An elderly man with non-productive cough and slight fever for three months was sent to our institute to undergo a thoracic CT. No drug consumption was reported nor were there any blood count changes. Final Diagnosis: Cryptogenic organizing pneumonia
Switching Casimir forces with Phase Change Materials
Creators: name: Torricelli, G.
name: van Zwol, P. J.
name: Shpak, O.
name: Binns, C.
name: Palasantzas, G.
name: Svetovoy, B. J. Kooi V. B.
name: Wuttig, M.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We demonstrate here a controllable variation in the Casimir force. Changes in the force of up to 20% at separations of ~100 nm between Au and AgInSbTe (AIST) surfaces were achieved upon crystallization of an amorphous sample of AIST. This material is well known for its structural transformation, which produces a significant change in the optical properties and is exploited in optical data storage systems. The finding paves the way to the control of forces in nanosystems, such as micro- or nanoswitches by stimulating the phase change transition via localized heat sources.
description: 7 pages, 3 figures The AFM images for the inset in Fig.2 were replaced with new ones as obtained with tips having high aspect ratio
Perforated appendicitis with an associated mucinous tumour
Creators: name: Gariani, Joanna
Publisher: name: EURORAD
Year: 2013
Subjects: subject: Abdomen
subject: CT
subject: Contrast agent-intravenous
subject: Inflammation
subject: Lymphoma

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 82 years
description: Clinical History: 82-year-old female patient institutionalised in the context of advanced dementia, Parkinson's disease and ischaemic stroke was referred to the emergency department for abdominal pain and sepsis. History and physical examination were extremely limited. Lab... Final Diagnosis: 1. Acute perforated appendicitis with low-grade mucinous neoplasm2. Lymphoma
Tailored bright illumination attack on distributed-phase-reference protocols
Creators: name: Lydersen, Lars
name: Skaar, Johannes
name: Makarov, Vadim
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Detector control attacks on quantum key distribution systems exploit the linear mode of avalanche photodiode in single photon detectors. So far, the protocols under consideration have been the BB84 protocol and its derivatives. Here we present how bright tailored illumination exploiting the linear mode of detectors can be used to eavesdrop on distributed-phase-reference protocols, such as differential-phase-shift and coherent-one-way.
description: 5 pages, 3 figures
Medial transposition of the carotid arteries mimicking retropharyngeal collection
Creators: name: Durran, Alexandra
Publisher: name: EURORAD
Year: 2013
Subjects: subject: Head and neck
subject: CT-Angiography
subject: Conventional radiography
subject: Image manipulation / Reconstruction
subject: Normal variants
subject: Abscess

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 75 years
description: Clinical History: We present the case of a 75-year-old lady who was referred by her GP for a lateral C-spine X-ray for worsening dysphagia. Final Diagnosis: Medial transposition of the carotid arteries
Resolved photometry of extragalactic young massive star clusters
Creators: name: Larsen, S. S.
name: de Mink, S. E.
name: Eldridge, J. J.
name: Langer, N.
name: Bastian, N.
name: Seth, A.
name: Smith, L. J.
name: Brodie, J.
name: Efremov, Y. N.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present colour-magnitude diagrams (CMDs) for a sample of seven young massive clusters in the galaxies NGC 1313, NGC 1569, NGC 1705, NGC 5236 and NGC 7793. The clusters have ages in the range 5-50 million years and masses of 10^5 -10^6 Msun. Although crowding prevents us from obtaining photometry in the central regions of the clusters, we are still able to measure up to 30-100 supergiant stars in each of the richest clusters, along with the brighter main sequence stars. The resulting CMDs and luminosity functions are compared with photometry of artificially generated clusters, designed to reproduce the photometric errors and completeness as realistically as possible. In agreement with previous studies, our CMDs show no clear gap between the H-burning main sequence and the He-burning supergiant stars, contrary to predictions by common stellar isochrones. In general, the isochrones also fail to match the observed number ratios of red-to-blue supergiant stars, although the difficulty of separating blue supergiants from the main sequence complicates this comparison. In several cases we observe a large spread (1-2 mag) in the luminosities of the supergiant stars that cannot be accounted for by observational errors. This spread can be reproduced by including an age spread of 10-30 million years in the models. However, age spreads cannot fully account for the observed morphology of the CMDs and other processes, such as the evolution of interacting binary stars, may also play a role.
description: 15 pages, 12 figures, accepted for publication in A&A
Ischaemic fasciitis: unusual localisation
Creators: name: Vasselli, Federica
Publisher: name: EURORAD
Year: 2013
Subjects: subject: Musculoskeletal joint
subject: Musculoskeletal soft tissue
subject: Musculoskeletal system
subject: MR
subject: Imaging sequences
subject: Surgery
subject: Ischaemia / Infarction
subject: Pathology

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 65 years
description: Clinical History: We describe a 65-years-old male patient, who came to our department with an asymptomatic mass in the right axilla. On clinical history, the patient reported a previous surgical intervention in the same site, two years before, for lipoma excision. Final Diagnosis: Fasciitis with the characteristics of ischaemic type.
All that grows is not a tumour
Creators: name: Ait Batahar, Salma
Publisher: name: EURORAD
Year: 2013
Subjects: subject: Lung
subject: Mediastinum
subject: CT
subject: Conventional radiography
subject: Computer Applications-Detection, diagnosis
subject: Diagnostic procedure
subject: Infection
subject: Neoplasia
subject: Pathology

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 33 years
description: Clinical History: A 33-year-old female patient with no past medical history presented with chest pain, cough and dyspnoea. The chest radiograph showed a right dense upper lobe opacity and further investigation with CT of the chest was warranted. Final Diagnosis: Pseudo-tumoural pulmonary tuberculosis
An incidental finding: a benign schwannoma
Creators: name: Garcia Barquin, Paula
Publisher: name: EURORAD
Year: 2013
Subjects: subject: Thorax
subject: CT
subject: Plain radiographic studies
subject: Diagnostic procedure
subject: Pathology

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 58 years
description: Clinical History: A 58-year-old woman came to our hospital to undergo a presurgical evaluation for possible kidney donation to her son. She did not have relevant medical history and her physical exploration and laboratory tests were normal. Final Diagnosis: A benign schwannoma
Some additional materials illustrating space stem precursor formation process at the negative lightning leader corona periphery
Creators: name: Syssoev A., A.
Publisher: name: Zenodo
Year: 2020
Subjects: space stem
negative stepped leader

description: These additional files (12 figures and a movie) present several examples of the final stage of our model realization at which a space stem precursor forms at the negative corona streamer burst periphery. Detailed description of these illustrating materials can be found in a separate pdf file.
Intracranial haemorrhage in an infant
Creators: name: Puttagunta, Srikanth
Publisher: name: EURORAD
Year: 2013
Subjects: subject: Haematologic
subject: Head and neck
subject: Paediatric
subject: CT
subject: Decision analysis
subject: Haemorrhage

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 3 months
description: Clinical History: 3-month old twin boy (full term) presented to A&E with fevers, lethargy and was noted to have a bulging fontanelle. A CT scan was requested to exclude possibility of intracerebral abscess. Coagulation studies returned as abnormal at this point. ... Final Diagnosis: Acute Extra-axial haemorrhage / haematoma secondary to haemophilia