cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
MOESM2 of Glucose associated NETosis in patients with ST-elevation myocardial infarction: an observational study
Creators: name: Helseth, Ragnhild
name: Knudsen, Eva
name: Eritsland, Jan
name: Opstad, Trine
name: Arnesen, Harald
name: Andersen, Geir
name: IngebjĂ¸Rg Seljeflot
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified

description: Additional file 2: Table S2. dsDNA and MPO-DNA related to the glucometabolic status in the acute phase. Values are given as median (25, 75 pencentiles). p values are based on the Mann-Whitney U test. dsDNA: double-stranded deoxyribonucleic acid. IFG: impaired fasting glucose. IGT: impaired glucose tolerance. MPO-DNA: myeloperoxidase deoxyribonucleic acid. OD: optical density units. T2DM: type 2 diabetes mellitus. pa: NGR vs. IFG. pb: NGR vs. IGT. pc: NGR vs. T2DM.
Hard exclusive meson production at next-to-leading order
Creators: name: Belitsky, A. V.
name: Müller, D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We evaluate perturbative next-to-leading order corrections to the hard exclusive leptoproduction of pi+ mesons on a transversely polarized proton target. A model dependent study shows that these corrections can be large. We analyze the scale dependence and explore the Brodsky-Lepage-Mackenzie scale setting procedure. Although the predictions for the cross section suffer from theoretical uncertainties, the transverse nucleon single spin asymmetry turns out to be a rather stable observable since higher order effects approximately cancel there.
description: 14 pages, LaTeX, 3 figures
Developing Innovative Students Through Cohort Innovation Programs
Creators: name: Mehlhorn, Joey
name: Tewari, Rachna
name: Parrott, Scott
name: Pruitt, Ross
name: Mehlhorn, Joey
name: Tewari, Rachna
name: Parrott, Scott
name: Pruitt, Ross
Publisher: name: Unknown
Year: 2016
Subjects: subject: Teaching/Communication/Extension/Profession
subject: innovation
subject: student learning outcomes
subject: agribusiness

description: In the fall 2014, a cohort innovation program was developed for undergraduate students to increase business skills and entrepreneurial capacity. The program focused on three primary areas: soft skills, critical thinking skills, and work experience. Students were pre-screened and selected based on an interview process related to potential, not GPA. The program utilized several unique teaching environments including the use of industry mentors, flipped classrooms, internships, video blogs, and student led program development. Students participated in innovation pitch sessions throughout the program to help develop entrepreneurial skills. Post participation surveys revealed that the program improved soft skills and the ability to work effectively in unfamiliar environments. Major improvements were seen in teamwork skills, project management leadership, and business and communication skills. Participants stated that the program motivated and empowered them to become industry ready innovators.
Random network models with variable disorder of geometry
Creators: name: Klümper, Andreas
name: Nuding, Win
name: Sedrakyan, Ara
Publisher: name: arXiv
Year: 2019
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: Recently it was shown (I.A.Gruzberg, A. Klümper, W. Nuding and A. Sedrakyan, Phys.Rev.B 95, 125414 (2017)) that taking into account random positions of scattering nodes in the network model with $U(1)$ phase disorder yields a localization length exponent $2.37 \pm 0.011$ for plateau transitions in the integer quantum Hall effect. This is in striking agreement with the experimental value of $2.38 \pm 0.06$. Randomness of the network was modeled by replacing standard scattering nodes of a regular network by pure tunneling resp.reflection with probability $p$ where the particular value $p=1/3$ was chosen. Here we investigate the role played by the strength of the geometric disorder, i.e. the value of $p$. We consider random networks with arbitrary probability $0
description: arXiv admin note: text overlap with arXiv:1604.06844
Soesilarishius Makhan 2007
Creators: name: Ruiz, Gustavo Rodrigo Sanches
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Salticidae
Soesilarishius

description: Soesilarishius Makhan, 2007
 Soesilarishius Makhan, 2007: 2 (Type species: S. amrishi Makhan, 2007 — holotype not examined).
 Diagnosis. Species included in this genus are small South American ground dwelling euophryines easily distinguishable from other lineages of this subfamily from the Neotropics by having reduced spiraled emboli. The morphology of these emboli, as described below, seems to be not so constrained when compared to the typical spiraled embolus present in almost all euophryine genera. The typical euophryine spiraled embolus has also been lost in Anasaitis Bryant, another group of ground dwellers typically found in the Caribbean Islands. However, DNA data place Anasaitis and Soesilarishius in very distant clades (J. Zhang, pers. comm.), which suggests the independence of these two events. Additionally, most Anasaitis species have iridescent scales on the body and ventral tibial bumps on the male palp (J. Zhang, pers. comm.), contrasting to the brownish-whitish known species of Soesilarishius.
 Monophyly. Similarly to the type species, the species mentioned herein have the typical euophryine loop in the sperm duct but the typical coiled embolus is reduced (the long embolus of S. crispiventer sp. nov. coils to the opposite side and is probably derived from a short embolus). In this paper, this condition, observed in all the species, is interpreted as homologous and they are all described under Soesilarishius. Phylogenetic studies using molecular data could help us clarify whether the genus represents a natural group or if it only gathers similar, but unrelated, euophryines with reduced emboli.
 Redescription. Very small to small sized jumping spiders (1.5–4.0 mm), ground dwellers, generally dark in body color, with pairs of spots or transverse stripes with white scales on the abdomen of both sexes, more conspicuous in males; chelicera with one retromarginal and two promarginal teeth in both sexes; male palp lacking the typical euophryine spiraled embolus, which is generally short and positioned at the distal end of tegulum; generally with legs 4312 in females and 4312 or 4132 in males, claw tufts poorly developed and some species with long ventral spines on front legs of both sexes; epigyne generally only with primary spermathecae, from which fertilization ducts arise (some species may have an additional pair of secondary spermathecae with no connecting fertilization ducts), scent glands (sensu Berry & Prószyṅski 2001) on the beginning of the copulation ducts and pores of nutritive glands on the inner wall of primary spermathecae.
description: Published as part of Ruiz, Gustavo Rodrigo Sanches, 2011, Systematics of the genus Soesilarishius (Araneae: Salticidae: Euophryinae), pp. 22-38 in Zootaxa 3022 (1) on page 23, DOI: 10.11646/zootaxa.3022.1.2, http://zenodo.org/record/5280700
The Corley-Jacobson dispersion relation and trans-Planckian inflation
Creators: name: Martin, Jerome
name: Brandenberger, Robert H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this Letter we study the dependence of the spectrum of fluctuations in inflationary cosmology on possible effects of trans-Planckian physics, using the Corley/Jacobson dispersion relations as an example. We compare the methods used in previous work [1] with the WKB approximation, give a new exact analytical result, and study the dependence of the spectrum obtained using the approximate method of Ref. [1] on the choice of the matching time between different time intervals. We also comment on recent work subsequent to Ref. [1] on the trans-Planckian problem for inflationary cosmology.
description: 6 pages, Revtex4
Strongly interacting $σ$-electrons and MgB$_2$ superconductivity
Creators: name: Ivanov, V. A.
name: Broek, M. van den
name: Peeters, F. M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: MgB$(p^{n_σ}p^{n_π})_{2}$ is classified as a system with strongly interacting $σ$-electrons and non-correlated $π$-electrons of boron ions. The kinematic and Coulomb interaction V between the orbitally degenerated $σ$-electrons provide the superconducting state with an anisotropic gap of s*-wave symmetry. The critical temperature $T_c$ has a non-monotonic dependence on the distance r between the centers of gravity of $σ$- and $π$-bands. MgB$_2$ corresponds to r=0.085 eV and V=0.45 eV in our model with flat bands. The derived superconducting density of electronic states is in good agreement with available experimental and theoretical data. The possibilities for increasing $T_c$ are discussed.
description: 8 pages, 4 figures
Exact non-symmetric closed line vacuum magnetic fields in a topological torus
Creators: name: Weitzner, Harold
name: Sengupta, Wrick
Publisher: name: arXiv
Year: 2019
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Non-symmetric vacuum magnetic fields with closed magnetic field lines are of interest in the construction of stellarator equilibria. Beyond the result of D.Lortz (ZAMP \textbf{21}, 196 (1970)), few results are available. This work presents a closed-form expression for a class of vacuum magnetic fields in a topological torus with closed field lines. We explicitly obtain the invariants of such a field. We finally show that a three-dimensional low beta magnetohydrodynamic (MHD) equilibrium may be constructed in a topological torus starting with these closed line vacuum magnetic fields.
MOESM2 of Mixed method evaluation of Relational Team Development (RELATED) to improve team-based care for complex patients with mental illness in primary care
Creators: name: Loeb, Danielle
name: Monson, Samantha
name: Lockhart, Steven
name: Depue, Cori
name: Ludman, Evette
name: Nease, Donald
name: Binswanger, Ingrid
name: Kline, Danielle
name: Gruy, Frank
name: Good, Dixie
name: Bayliss, Elizabeth
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Medicine
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Additional file 2: PCP survey. Pre- and Post- PCP survey.
Lobe Advance Velocities in the Extragalactic Compact Symmetric Object 4C 31.04
Creators: name: Giroletti, M.
name: Giovannini, G.
name: Taylor, G. B.
name: Conway, J. E.
name: Lara, L.
name: Venturi, T.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on the results of a two epoch study of the low power Compact Symmetric Object 4C 31.04. Observations performed with the VLBA at 5 GHz in 1995 and 2000 have yielded images of this source at milliarcsecond angular resolution. A central core is detected, with bright compact hot spots and extended lobes on both sides. Model-fitting and other analysis of the data (brightness profile, difference map) clearly indicate that the source is expanding. We estimate the velocity of this expansion to be (0.085 +/- 0.016) mas/yr, i.e. (0.33 +/- 0.06) c in both hot spots. Assuming a constant expansion velocity, we estimate the kinematic age of the source at 550 yrs. We also study the spectral index using VLBA observations at 1.3 GHz and MERLIN at 22 GHz. The derived spectral age is 3000-5000 years in equipartition conditions. The two estimates are discussed and found to be in agreement, given present uncertainties.
description: 9 pages, 8 .eps figures; accepted for publication in Astronomy & Astrophysics
SNR Enhancement in Brillouin Microspectroscopy using Spectrum Reconstruction
Creators: name: Xiang, YuChen
name: Foreman, Matthew R.
name: Török, Peter
Publisher: name: arXiv
Year: 2019
Subjects: subject: Signal Processing (eess.SP)
subject: Optics (physics.optics)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Physical sciences

description: Brillouin imaging suffers from intrinsically low signal-to-noise ratios (SNR). Such low SNRs can render common data analysis protocols unreliable, especially for SNRs below $\sim10$. In this work we exploit two denoising algorithms, namely maximum entropy reconstruction (MER) and wavelet analysis (WA), to improve the accuracy and precision in determination of Brillouin shifts and linewidth. Algorithm performance is quantified using Monte-Carlo simulations and benchmarked against the Cramér-Rao lower bound. Superior estimation results are demonstrated even at low SNRS ($\geq 1$). Denoising was furthermore applied to experimental Brillouin spectra of distilled water at room temperature, allowing the speed of sound in water to be extracted. Experimental and theoretical values were found to be consistent to within $\pm1\%$ at unity SNR.
Observability of the Lightest CMSSM Higgs Boson at Hadron Colliders
Creators: name: Ellis, J.
name: Heinemeyer, S.
name: Olive, K. A.
name: Weiglein, G.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We discuss the observability of the lightest neutral Higgs boson in the constrained MSSM (CMSSM), with universal soft supersymmetry-breaking parameters, at hadron colliders such as the Tevatron and the LHC. We take account of the constraints on parameter space provided by LEP, the measured rate of b to s gamma decay, the cosmological relic density Omega h^2, and the recent measurement of g_mu - 2. We normalize products of the expected CMSSM Higgs production cross sections and decay branching ratios (sigma B)_CMSSM relative to those expected for a Standard Model Higgs boson of the same mass. In the h to gamma gamma channel, we find that (sigma B)_CMSSM > 0.85 (sigma B)_SM. In the W/t tbar + h, h to b bbar channels, we find that (sigma B)_CMSSM \~ 1.05 (sigma B)_SM. We conclude that the lightest CMSSM Higgs boson should be almost as easy to see as the Standard Model Higgs boson: in particular, it should be discoverable with about 15/fb of luminosity at the Tevatron or 10/fb of luminosity at the LHC.
description: 13 pages, 4 eps figures, typos corrected, more references
title: 01_2027
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Inside Job: Diagnosing Bluetooth Lower Layers Using Off-the-Shelf Devices
Creators: name: Classen, Jiska
name: Hollick, Matthias
Publisher: name: arXiv
Year: 2019
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: Bluetooth is among the dominant standards for wireless short-range communication with multi-billion Bluetooth devices shipped each year. Basic Bluetooth analysis inside consumer hardware such as smartphones can be accomplished observing the Host Controller Interface (HCI) between the operating system's driver and the Bluetooth chip. However, the HCI does not provide insights to tasks running inside a Bluetooth chip or Link Layer (LL) packets exchanged over the air. As of today, consumer hardware internal behavior can only be observed with external, and often expensive tools, that need to be present during initial device pairing. In this paper, we leverage standard smartphones for on-device Bluetooth analysis and reverse engineer a diagnostic protocol that resides inside Broadcom chips. Diagnostic features include sniffing lower layers such as LL for Classic Bluetooth and Bluetooth Low Energy (BLE), transmission and reception statistics, test mode, and memory peek and poke.
Color-Neutral Superconducting Quark Matter
Creators: name: Steiner, Andrew W.
name: Reddy, Sanjay
name: Prakash, Madappa
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We investigate the consequences of enforcing local color neutrality on the color superconducting phases of quark matter by utilizing the Nambu-Jona-Lasinio model supplemented by diquark and the t'Hooft six-fermion interactions. In neutrino free matter at zero temperature, color neutrality guarantees that the number densities of u, d, and s quarks in the Color-Flavor-Locked (CFL) phase will be equal even with physical current quark masses. Electric charge neutrality follows as a consequence and without the presence of electrons. In contrast, electric charge neutrality in the less symmetric 2-flavor superconducting (2SC) phase with ud pairing requires more electrons than the normal quark phase. The free energy density cost of enforcing color and electric charge neutrality in the CFL phase is lower than that in the 2SC phase, which favors the formation of the CFL phase. With increasing temperature and neutrino content, an unlocking transition occurs from the CFL phase to the 2SC phase with the order of the transition depending on the temperature, the quark and lepton number chemical potentials. The astrophysical implications of this rich structure in the phase diagram, including estimates of the effects from Goldstone bosons in the CFL phase, are discussed.
description: 20 pages, 4 figures; version to appear in Phys. Rev. D
Non periodic Ishibashi states: the su(2) and su(3) affine theories
Creators: name: Ruelle, Philippe
name: Verhoeven, Olivier
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider the su(2) and su(3) affine theories on a cylinder, from the point of view of their discrete internal symmetries. To this end, we adapt the usual treatment of boundary conditions leading to the Cardy equation to take the symmetry group into account. In this context, the role of the Ishibashi states from all (non periodic) bulk sectors is emphasized. This formalism is then applied to the su(2) and su(3) models, for which we determine the action of the symmetry group on the boundary conditions, and we compute the twisted partition functions. Most if not all data relevant to the symmetry properties of a specific model are hidden in the graphs associated with its partition function, and their subgraphs. A synoptic table is provided that summarizes the many connections between the graphs and the symmetry data that are to be expected in general.
description: 19 pages, 3 figures
Anomaly in the stability limit of liquid helium 3
Creators: name: Caupin, Frederic
name: Balibar, Sebastien
name: Maris, Humphrey J
Publisher: name: arXiv
Year: 2001
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We propose that the liquid-gas spinodal line of helium 3 reaches a minimum at 0.4 K. This feature is supported by our cavitation measurements. We also show that it is consistent with extrapolations of sound velocity measurements. Speedy [J. Phys. Chem. 86, 3002 (1982)] previously proposed this peculiar behavior for the spinodal of water and related it to a change in sign of the expansion coefficient alpha, i. e. a line of density maxima. Helium 3 exhibits such a line at positive pressure. We consider its extrapolation to negative pressure. Our discussion raises fundamental questions about the sign of alpha in a Fermi liquid along its spinodal.
description: 5 pages, 3 figures
Electronic excitation of transition metal nitrides by light ions with keV energies
Creators: name: Bruckner, Barbara
name: Hans, Marcus
name: Nyberg, Tomas
name: Greczynski, Grzegorz
name: Bauer, Peter
name: Primetzhofer, Daniel
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We investigated the specific electronic energy deposition by protons and He ions with keV energies in different transition metal nitrides of technological interest. Data were obtained from two different time-of-flight ion scattering setups and show excellent agreement. For protons interacting with light nitrides, i.e. TiN, VN and CrN, very similar stopping cross sections per atom were found, which coincide with literature data of N2 gas for primary energies <= 25 keV. In case of the chemically rather similar nitrides with metal constituents from the 5th and 6th period, i.e. ZrN and HfN, the electronic stopping cross sections were measured to exceed what has been observed for molecular N2 gas. For He ions, electronic energy loss in all nitrides was found to be significantly higher compared to the equivalent data of N2 gas. Additionally, deviations from velocity proportionality of the observed specific electronic energy loss are observed. A comparison with predictions from density functional theory for protons and He ions yields a high apparent efficiency of electronic excitations of the target for the latter projectile. These findings are considered to indicate the contributions of additional mechanisms besides electron hole pair excitations, such as electron capture and loss processes of the projectile or promotion of target electrons in atomic collisions.
Determination of absolute neutrino masses from Z-bursts
Creators: name: Fodor, Z.
name: Katz, S. D.
name: Ringwald, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Ultrahigh energy neutrinos (UHEν) scatter on relic neutrinos (Rν) producing Z bosons, which can decay hadronically producing protons (Z-burst). We compare the predicted proton spectrum with the observed ultrahigh energy cosmic ray (UHECR) spectrum and determine the mass of the heaviest Rνvia a maximum likelihood analysis. Our prediction depends on the origin of the power-like part of the UHECR spectrum: m_ν=2.75^{+1.28}_{-0.97} eV for Galactic halo and 0.26^{+0.20}_{-0.14} eV for extragalactic (EG) origin. The necessary UHEνflux should be detected in the near future.
description: slight rewording, revised neutrino fluxes, conclusions unchanged, version to appear in Phys. Rev. Lett
Economic Modelling of Dryland Salinity in Western Australia
Creators: name: Gomboso, J.
name: Gomboso, J.
Publisher: name: Unknown
Year: 1990
Subjects: Crop Production/Industries

description: The clearing of land for agricultural purposes in the low rainfall areas of south-west Western Australia has resulted in soluble salts being transported from upslope recharge areas, through groundwater flows, to downslope discharge areas. Dryland salinity is not confined to individual properties. It may disperse among properties and catchments and is thus a common property problem. In an attempt to model the effect of natural resource utilisation and the divergence between private and socially optimal rates of land degradation resulting from the exploitation of common resources, a dynamic optimisation model of soil salinity has been developed. The objective of soil conservation models may not necessarily be to stop future degradation in its entirety, but to ensure that all resources are applied to their highest value combination of end uses, both currently and in the future (Morris et al, 1988). The model is also used to examine the steady-state solution to optimal control. In the case of dryland salinity, a steady-state equilibrium occurs when the hydrological balance is in equilibrium. Salinisation of dryland areas has been caused predominantly by the removal of high water-using, deep-rooted native forest, and its replacement with shallow-rooted annual crops and pastures. Agricultural expansion in the low rainfall areas of south-west Western Australia has modified the natural water balance, thereby affecting the volume and flow of surface and ground water. The resultant change in the hydrological balance of the soil brings rising water tables and stored salts to the surface, and evaporation causes these salts to be left behind.
Multi-wavelength consensus of large-scale linear bias
Creators: name: Pan, Hengxing
name: Obreschkow, Danail
name: Howlett, Cullan
name: Lagos, Claudia del P.
name: Elahi, Pascal J.
name: Baugh, Carlton
name: Gonzalez-Perez, Violeta
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We model the large-scale linear galaxy bias $b_g(x,z)$ as a function of redshift $z$ and observed absolute magnitude threshold $x$ for broadband continuum emission from the far infrared to ultra-violet, as well as for prominent emission lines, such as the H$α$, H$β$, Lya and [OII] lines. The modelling relies on the semi-analytic galaxy formation model GALFORM, run on the state-of-the-art $N$-body simulation SURFS with the Planck 2015 cosmology. We find that both the differential bias at observed absolute magnitude $x$ and the cumulative bias for magnitudes brighter than $x$ can be fitted with a five-parameter model: $b_g(x,z)=a + b(1+z)^e(1 + \exp{[(x-c)d]})$. We also find that the bias for the continuum bands follows a very similar form regardless of wavelength due to the mixing of star-forming and quiescent galaxies in a magnitude limited survey. Differences in bias only become apparent when an additional colour separation is included, which suggest extensions to this work could look at different colours at fixed magnitude limits. We test our fitting formula against observations, finding reasonable agreement with some measurements within $1σ$ statistical uncertainties, and highlighting areas of improvement. We provide the fitting parameters for various continuum bands, emission lines and intrinsic galaxy properties, enabling a quick estimation of the linear bias in any typical survey of large-scale structure.
description: Revised manuscript accepted for publication in MNRAS
An Ultra-High-Resolution Survey of the Interstellar ^7Li-to-^6Li Isotope Ratio in the Solar Neighborhood
Creators: name: Knauth, David C.
name: Federman, S. R.
name: Lambert, David L.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In an effort to probe the extent of variations in the interstellar ^7Li/^6Li ratio seen previously, ultra-high-resolution (R ~ 360,000), high signal-to-noise spectra of stars in the Perseus OB2 and Scorpius OB2 Associations were obtained. These measurements confirm our earlier findings of an interstellar ^7Li/^6Li ratio of about 2 toward o Per, the value predicted from models of Galactic cosmic ray spallation reactions. Observations of other nearby stars yield limits consistent with the isotopic ratio ~ 12 seen in carbonaceous chondrite meteorites. If this ratio originally represented the gas toward o Per, then to decrease the original isotope ratio to its current value an order of magnitude increase in the Li abundance is expected, but is not seen. The elemental K/Li ratio is not unusual, although Li and K are formed via different nucleosynthetic pathways. Several proposals to account for the low ^7Li/^6Li ratio were considered, but none seems satisfactory. Analysis of the Li and K abundances from our survey highlighted two sight lines where depletion effects are prevalent. There is evidence for enhanced depletion toward X Per, since both abundances are lower by a factor of 4 when compared to other sight lines. Moreover, a smaller Li/H abundance is observed toward 20 Aql, but the K/H abundance is normal, suggesting enhanced Li depletion (relative to K) in this direction. Our results suggest that the ^7Li/^6Li ratio has not changed significantly during the last 4.5 billion years and that a ratio ~ 12 represents most gas in the solar neighborhood. In addition, there appears to be a constant stellar contribution of ^7Li, indicating that one or two processes dominate its production in the Galaxy.
description: 54 pages, accepted for publication in the Astrophysical Journal
Polca SARA - Full polarization, direction-dependent calibration and sparse imaging for radio interferometry
Creators: name: Birdi, Jasleen
name: Repetti, Audrey
name: Wiaux, Yves
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: New generation of radio interferometers are envisaged to produce high quality, high dynamic range Stokes images of the observed sky from the corresponding under-sampled Fourier domain measurements. In practice, these measurements are contaminated by the instrumental and atmospheric effects that are well represented by Jones matrices, and are most often varying with observation direction and time. These effects, usually unknown, act as a limiting factor in achieving the required imaging performance and thus, their calibration is crucial. To address this issue, we develop a global algorithm, named Polca SARA, aiming to perform full polarization, direction-dependent calibration and sparse imaging by employing a non-convex optimization technique. In contrast with the existing approaches, the proposed method offers global convergence guarantees and flexibility to incorporate sophisticated priors to regularize the imaging as well as the calibration problem. Thus, we adapt a polarimetric imaging specific method, enforcing the physical polarization constraint along with a sparsity prior for the sought images. We perform extensive simulation studies of the proposed algorithm. While indicating the superior performance of polarization constraint based imaging, the obtained results also highlight the importance of calibrating for direction-dependent effects as well as for off-diagonal terms (denoting polarization leakage) in the associated Jones matrices, without inclusion of which the imaging quality deteriorates.
Fuzzy-Controlled Scheduling of Route-Request Packets (FSRR) in Mobile Ad Hoc Networks
Creators: name: Sufian, A.
name: Banerjee, A.
name: Dutta, P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: In ad hoc networks, the scheduling of route-request packets should be different from that of message packets, because during transmission of message packets the location of the destination is known whereas in route discovery this is not known in most of the cases. The router has to depend upon the last known location, if any, of the destination to determine the center and radius of the circle that embeds all possible current position of the destination. Route-request packets generated from the source are directed towards this circle i.e., directional route discovery can be applied. Otherwise, when no earlier location of the destination is known the route-requested has to be broadcast in the whole network consuming a significant amount of time than directional route discovery. The present article proposes fuzzy controlled scheduling of route-request packets in particular that greatly reduces the average delay in route discovery in ad hoc networks.
description: 6 pages, 4 figures
Axion Quark Nuggets and how a Global Network can discover them
Creators: name: Budker, Dmitry
name: Flambaum, Victor V.
name: Liang, Xunyu
name: Zhitnitsky, Ariel
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We advocate an idea that the presence of the daily and annual modulations of the axion flux on the Earth surface may dramatically change the strategy of the axion searches. Our computations are based on the so-called Axion Quark Nugget (AQN) dark matter model which was originally put forward to explain the similarity of the dark and visible cosmological matter densities $Ω_{\rm dark}\sim Ω_{\rm visible}$. In our framework, the population of galactic axions with mass $ 10^{-6} {\rm eV}\lesssim m_a\lesssim 10^{-3}{\rm eV}$ and velocity $< v_a>\sim 10^{-3} c$ will be always accompanied by the axions with typical velocities $\sim 0.6 c$ emitted by AQNs. We formulate the broadband detection strategy to search for such relativistic axions by studying the daily and annual modulations. We describe several tests which could effectively discriminate a true signal from noise. These AQN-originated axions can be observed as correlated events which could be recorded by synchronized stations in the global network. The correlations can be effectively studied if the detectors are positioned at distances shorter than a few hundred kilometres.
description: Matches the published version in Phys. Rev. D
MOESM3 of Small RNA and degradome deep sequencing reveal respective roles of cold-related microRNAs across Chinese wild grapevine and cultivated grapevine
Creators: name: Pengfei Wang
name: Yang, Yang
name: Hongmei Shi
name: Yongmei Wang
name: Fengshan Ren
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 3: Table S3. Conseved miRNA orthologous between cultivated grape and Chinese wild grape.
Cost Estimates and Investment Analysis for Muscadine Grapes Production in Georgia
Creators: name: Fonsah, Esendugue Greg
name: Awondo, Sebastian N.
name: Fonsah, Esendugue Greg
name: Awondo, Sebastian N.
Publisher: name: Unknown
Year: 2016
Subjects: subject: Crop Production/Industries
subject: Demand and Price Analysis
subject: Public Economics
subject: muscadine grape
subject: budgets
subject: production costs
subject: net returns
subject: biotechnology

description: Muscadine (Vitis rotundifolia), also known as wild grapes are native to the Southeastern United States and well adapted to the warm and humid conditions of the region. Georgia is the largest producer of mscadine grapes in the United States and has enjoyed a market niche for decades consisting of fresh fruit processed for jams, juice and wine. In recent years, precision breeding using cisgenic technology has allow the development of new disease-resistant and seedless cultivars with potentials to serve different end-use market segments. However, the profitability of muscadine grapes cultivars newly developed with cisgenic technology relative to those developed with traditional transgenic technology is still questionable. This study takes a first step in bridging the gap in the literative with the objective to estimate the costs, revenue and profitability of producing transgenic-bred muscadine grapes in Georgia using a Single Trellis System with drip irrigation. Subsequently, we plan to derive similiar estimates for a new cisgenicbred rot resistant and seedless counterpart, currently in field trials, and compare both estimates to determine which of the two has the highest economic potentials in term of profitability and or net returns to the growers.
Additional file 1 of Patterns of human social contact and mask wearing in high-risk groups in China
Creators: name: Zheng, Bo
name: Zhu, Wenlong
name: Pan, Jinhua
name: Wang, Weibing
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1. Figure S1. The distributions of contacts’ age crossing different occupation. Figure S2. The proportion of reporting physical contacts in different contact durations stratified by province and occupation groups. Figure S3. The proportion of reporting physical contacts in different contact settings stratified by province and occupation groups. Figure S4. The proportion of reporting physical contacts in different contact relations stratified by province and occupation groups. Figure S5. The proportion of reporting physical contacts in different contact frequency stratified by province and occupation groups. Figure S6. Individual contact matrices of different province and occupations. Figure S7. Total contact matrices of different province and occupations. Figure S8. Proportion of always wearing masks in different places stratified by different characteristics. Figure S9. The association of always wearing masks and different characteristics of participants. Figure S10. The proportion of participants who reported always wearing masks in different places, for different contact groups, stratified by occupation group and province (A: Shanghai, B: Qinghai, C: Zhejiang).
MOESM1 of Mixed method evaluation of Relational Team Development (RELATED) to improve team-based care for complex patients with mental illness in primary care
Creators: name: Loeb, Danielle
name: Monson, Samantha
name: Lockhart, Steven
name: Depue, Cori
name: Ludman, Evette
name: Nease, Donald
name: Binswanger, Ingrid
name: Kline, Danielle
name: Gruy, Frank
name: Good, Dixie
name: Bayliss, Elizabeth
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 1: Standards for Reporting Implementation Studies: the StaRI checklist for completion. Reporting standards for implementation.
Perturbative and non-perturbative aspects of the non-abelian Boltzmann-Langevin equation
Creators: name: Bodeker, Dietrich
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the Boltzmann-Langevin equation which describes the dynamics of hot Yang-Mills fields with typical momenta of order of the magnetic screening scale g^2 T. It is transformed into a path integral and Feynman rules are obtained. We find that the leading log Langevin equation can be systematically improved in a well behaved expansion in log(1/g)^-1. The result by Arnold and Yaffe that the leading log Langevin equation is still valid at next-to-leading-log order is confirmed. We also confirm their result for the next-to-leading-log damping coefficient, or color conductivity, which is shown to be gauge fixing independent for a certain class of gauges. The frequency scale g^2T does not contribute to this result, but it does contribute, by power counting, to the transverse gauge field propagator. Going beyond a perturbative expansion we find 1-loop ultraviolet divergences which cannot be removed by renormalizing the parameters in the Boltzmann-Langevin equation.
description: Some discussions and notations clarified
Cavitation pressure in liquid helium
Creators: name: Caupin, Frederic
name: Balibar, Sebastien
Publisher: name: arXiv
Year: 2001
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Recent experiments have suggested that, at low enough temperature, the homogeneous nucleation of bubbles occurs in liquid helium near the calculated spinodal limit. This was done in pure superfluid helium 4 and in pure normal liquid helium 3. However, in such experiments, where the negative pressure is produced by focusing an acoustic wave in the bulk liquid, the local amplitude of the instantaneous pressure or density is not directly measurable. In this article, we present a series of measurements as a function of the static pressure in the experimental cell. They allowed us to obtain an upper bound for the cavitation pressure P_cav (at low temperature, P_cav < -2.4 bar in helium 3, P_cav < -8.0 bar in helium 4). From a more precise study of the acoustic transducer characteristics, we also obtained a lower bound (at low temperature, P_cav > -3.0 bar in helium 3, P_cav > - 10.4 bar in helium 4). In this article we thus present quantitative evidence that cavitation occurs at low temperature near the calculated spinodal limit (-3.1 bar in helium 3 and -9.5 bar in helium 4). Further information is also obtained on the comparison between the two helium isotopes. We finally discuss the magnitude of nonlinear effects in the focusing of a sound wave in liquid helium, where the pressure dependence of the compressibility is large.
description: 11 pages, 9 figures
Wave function of the radion with a bulk scalar field
Creators: name: Brax, P.
name: van de Bruck, C.
name: Davis, A. C.
name: Rhodes, C. S.
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The behaviour of the distance between two branes (the `radion') in a braneworld model with a bulk scalar field is investigated. We show that the BPS conditions of supergravity ensure that the dynamics of the scalar field and the radion are not independent; we derive the four-dimensional effective action, showing that the effective theory is of scalar--tensor nature, coupling the radion to four-dimensional gravity.
description: 13 pages, LaTeX
Fuzzy Route Switching For Energy Preservation (FEP) in Ad Hoc Networks
Creators: name: Banerjee, A.
name: Dutta, P.
name: Sufian, A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: Nodes in ad hoc networks have limited battery power. Hence they require an energy-efficient technique to improve average network performance. Maintaining energy-efficiency in ad hoc networks is really challenging because highest energy efficiency is achieved if all the nodes are always switched off and energy-efficiency will be minimum if all the nodes are fully operational i.e. always turned-on. Energy preservation requires redirection of data packets through some other routes having good performance. This improves the data packet delivery ratio and the number of alive nodes decreasing the cost of messages.
description: 11 pages, 12 figures, 4 tables
Soesilarishius aurifrons Ruiz 2011, comb. nov.
Creators: name: Ruiz, Gustavo Rodrigo Sanches
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Salticidae
Soesilarishius
Soesilarishius aurifrons

description: Soesilarishius aurifrons (Taczanowski, 1878) comb. nov.
Fig. 1
 Euophrys aurifrons Taczanowski, 1878: 308 (Male and juvenile syntypes from Amable Maria, Peru, 1871–1878, Jelski, Polska Akademia Nauk, Łomna, Poland, examined; male here designated as lectotype).
 Diagnosis. The male palp is similar to that of S. amrishi Makhan, 2007 by the almost straight embolus and a short RTA (Fig. 1); while the embolus arises from the prolateral border of the tegulum in S. amrishi (Makhan 2007, fig. 5), the embolus of S. aurifrons emerges almost from the center of the tegulum (Fig. 1).
 Description. Male. The lectotype has a homogeneous faded brown body color. See Taczanowski (1878) for details. The female is unknown.
description: Published as part of Ruiz, Gustavo Rodrigo Sanches, 2011, Systematics of the genus Soesilarishius (Araneae: Salticidae: Euophryinae), pp. 22-38 in Zootaxa 3022 (1) on page 23, DOI: 10.11646/zootaxa.3022.1.2, http://zenodo.org/record/5280700
LivDet in Action - Fingerprint Liveness Detection Competition 2019
Creators: name: Orrù, Giulia
name: Casula, Roberto
name: Tuveri, Pierluigi
name: Bazzoni, Carlotta
name: Dessalvi, Giovanna
name: Micheletto, Marco
name: Ghiani, Luca
name: Marcialis, Gian Luca
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: The International Fingerprint liveness Detection Competition (LivDet) is an open and well-acknowledged meeting point of academies and private companies that deal with the problem of distinguishing images coming from reproductions of fingerprints made of artificial materials and images relative to real fingerprints. In this edition of LivDet we invited the competitors to propose integrated algorithms with matching systems. The goal was to investigate at which extent this integration impact on the whole performance. Twelve algorithms were submitted to the competition, eight of which worked on integrated systems.
description: Preprint version of a paper accepted at ICB 2019
MOESM1 of Glucose associated NETosis in patients with ST-elevation myocardial infarction: an observational study
Creators: name: Helseth, Ragnhild
name: Knudsen, Eva
name: Eritsland, Jan
name: Opstad, Trine
name: Arnesen, Harald
name: Andersen, Geir
name: Seljeflot, Ingebjørg
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified

description: Additional file 1: Table S1. Correlations between NETs markers and plasma glucose levels. p values are based on the Spearman’s rho. dsDNA: double-stranded deoxyribonucleic acid. MPO-DNA: myeloperoxidase deoxyribonucleic acid. PAD4 mRNA: peptidylarginine deiminase 4 messenger ribonucleic acid. OD: optical density units. r: correlation coefficient. RQ: relative quantification values.