cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Overview of the university-based addiction studies programs in the United States
Creators: name: Pavlovská, Amalie
name: Peters, Roger H.
name: Gabrhelík, Roman
name: Miovský, Michal
name: Zili Sloboda
name: Babor, Thomas F.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy

description: Background: The field of addiction studies (AS) has grown in the last several decades. However, little is known about the structure and conditions of current academic programs. Only two studies have examined AS programs in the U.S., and both were conducted almost 15 years ago. The current study was designed to identify AS programs existing in the U.S. universities. Methods: We conducted an Internet search to identify university-based programs according to defined key words. The university program websites were then subjected to content analysis. Results: A total of 333 U.S. universities were identified that offered 392 different academic programs in AS of which 302 were degree programs. Out of these, 161 (53%) programs were offered at the associate degree level, 48 (15,9%) at the bachelor’s level, 55 (18.2%) at the master’s level, and 5 (1.6%) at the doctorate level. The largest number of programs was in California. Two states in the U.S. had no identifiable programs. Only one university located in the state of New York offered comprehensive academic programs across the educational spectrum. Many of the academic programs offered certificates. The most common phrases used in program titles were “substance abuse”, “addiction studies/counseling”, and “chemical dependency”. Conclusions: There is a wide range of academic AS programs in the U.S., although their focus is mostly on clinical training rather than on research or drug policy. Future surveys such as this one would benefit from greater attention to issues related to certification, licensing, and academic curricula.
Determination of Leptoquark Properties in Polarized $eγ$ Collisions
Creators: name: Doncheski, M. A.
name: Godfrey, S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study leptoquark production using polarized $eγ$ colliders for the center of mass energies $\sqrt s=500$~GeV and 1~TeV. We show that using polarization asymmetries the ten different types of leptoquarks listed by Buchmüller, Rückl and Wyler can be distinquished from one another for leptoquark masses essentially up to the kinematic limit of the respective colliders. Thus, if a leptoquark were discovered an $eγ$ collider could play a crucial role in determining its origins.
description: 10 pages (plus 10 postscript figures submitted separately), OCIP/C 94-7
Fe intercalation under graphene and hexagonal boron nitride in-plane heterostructure on Pt(111)
Creators: name: Píš, Igor
name: Nappini, Silvia
name: Bondino, Federica
name: Menteş, Tevfik Onur
name: Sala, Alessandro
name: Locatelli, Andrea
name: Magnano, Elena
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Metal nanostructures confined between sp2 hybridized 2D materials and solid supports are attracting attention for their potential application in new nanotechnologies. Model studies under well-defined conditions are valuable for understanding the fundamental aspects of the phenomena under 2D covers. In this work we investigate the intercalation of iron atoms through a single layer of mixed graphene and hexagonal boron nitride on Pt(111) using a combination of spectroscopic and microscopic techniques. Thermally activated diffusion of iron proceeds preferentially under graphene and only partially under hexagonal boron nitride areas. When oxygen is coadsorbed with iron, the intercalation rate is higher, and formation of B2O3 and oxygenated B-C species is observed. Our results suggest the possibility of confining ferromagnetic layers under heterostructures of graphene and hexagonal boron nitride with potential technological implications in the fields of spintronics, magnetic data storage or chemistry under 2D covers.
Topological Magnons in Kitaev Magnets at High Fields
Creators: name: McClarty, P. A.
name: Dong, X. -Y.
name: Gohlke, M.
name: Rau, J. G.
name: Pollmann, F.
name: Moessner, R.
name: Penc, K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We study the Kitaev-Heisenberg-$Γ$-$Γ'$ model that describes the magnetism in strong spin-orbit coupled honeycomb lattice Mott insulators. In strong $[111]$ magnetic fields that bring the system into the fully polarized paramagnetic phase, we find that the spin wave bands carry nontrivial Chern numbers over large regions of the phase diagram implying the presence of chiral magnon edge states. In contrast to other topological magnon systems, the topological nontriviality of these systems results from the presence of magnon number non-conserving terms in the Hamiltonian. Since the effects of interactions are suppressed by $J/h$, the validity of the single particle picture is tunable making paramagnetic phases particularly suitable for the exploration of this physics. Using time dependent DMRG and interacting spin wave theory, we demonstrate the presence of the chiral edge mode and its evolution with field.
description: 16 pages (main text + supplementary material), 10 figures
The Galactic Lithium Evolution Revisited
Creators: name: Romano, D.
name: Matteucci, F.
name: Molaro, P.
name: Bonifacio, P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The evolution of the 7Li abundance in the Galaxy has been computed by taking into account several 7Li sources: novae, massive AGB stars, C-stars, Type II SNe and GCRs. The theoretical predictions for the evolution of the 7Li abundance in the solar neighborhood have been compared to a new compilation of data. A critical analysis of extant observations revealed a possible extension of the Li plateau towards higher metallicities (up to [Fe/H] = -0.5 or even -0.3) with a steep rise afterwards. We conclude that 1) the 7Li contribution from novae is required in order to reproduce the shape of the growth of A(Li) versus [Fe/H], 2) the contribution from Type II SNe should be lowered by at least a factor of two, and 3) the 7Li production from GCRs is probably more important than previously estimated, in particular at the highest metallicities.
description: 23 pages, LaTeX, 8 figures, accepted for publication in Astronomy and Astrophysics (Main Journal)
Testing J/psi Production and Decay Properties in Hadronic Collisions
Creators: name: Kim, C. S.
name: Mirkes, E.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The polar and azimuthal angular distributions for the lepton pair arising from the decay of a J/psi meson produced at transverse momentum p_T balanced by a photon [or gluon] in hadronic collisions are calculated in the color singlet model (CSM). It is shown that the general structure of the decay lepton distribution is controlled by four invariant structure functions, which are functions of the transverse momentum and the rapidity of the J/psi. We found that two of these structure functions [the longitudinal and transverse interference structure functions] are identical in the CSM. Analytical and numerical results are given in the Collins-Soper and in the Gottfried-Jackson frame. We present a Monte Carlo study of the effect of acceptance cuts applied to the leptons and the photon for J/psi+ gamma production at the Tevatron.
description: 22 pages (LaTeX) plus 11 postscript figures, MAD/PH/822, YUMS94-11. Figures are available from the authors or as a compressed tar file via anonymous ftp at phenom.physics.wisc.edu in directory {}~pub/preprints/madph-94-822-figs.tar.Z
A Tower Weak Gravity Conjecture from Infrared Consistency
Creators: name: Andriolo, Stefano
name: Junghans, Daniel
name: Noumi, Toshifumi
name: Shiu, Gary
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We analyze infrared consistency conditions of 3D and 4D effective field theories with massive scalars or fermions charged under multiple $U(1)$ gauge fields. At low energies, one can integrate out the massive particles and thus obtain a one-loop effective action for the gauge fields. In the regime where charge-independent contributions to higher-derivative terms in the action are sufficiently small, it is then possible to derive constraints on the charge-to-mass ratios of the massive particles from requiring that photons propagate causally and have an analytic S-matrix. We thus find that the theories need to contain bifundamentals and satisfy a version of the weak gravity conjecture known as the convex-hull condition. Demanding self-consistency of the constraints under Kaluza-Klein compactification, we furthermore show that, for scalars, they imply a stronger version of the weak gravity conjecture in which the charge-to-mass ratios of an infinite tower of particles are bounded from below. We find that the tower must again include bifundamentals but does not necessarily have to occupy a charge (sub-)lattice.
description: 52 pages
MOESM1 of SH2B1 promotes NSCLC cell proliferation through PI3K/Akt/mTOR signaling cascade
Creators: name: Wang, Shaoqiang
name: Zheng, Yingying
name: He, Zhiwei
name: Zhou, Wolong
name: Cheng, Yuanda
name: Zhang, Chunfang
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Pharmacology
subject: Developmental Biology
subject: Cancer

description: Additional file 1: Figure S1. Cell cycle analysis by propidium iodide (PI) staining showed that (A) SH2B1-knockdown slow down the S phase of A549 cell cycle progression (P = 0.0023, n = 3); (B) SH2B1 overexpression accelerated the S phase of H1299 cell cycle progression (P = 0.0110, n = 3). Figure S2. CCK8 assays were performed in H1299 cells with different treatment at 24 h, 48 h, 72 h, 96 h. Rapamycin impaired the effect of SH2B1 on cell proliferation (both P < 0.001). n = 3, bar: SD. Figure S3. Clinical relevance of SH2B1 and its targets in NSCLC. (A–C) Correlation between SH2B1 and expression of p-Akt, p-mTOR and PTEN with liner regression and Pearson’s significance. SH2B1 has a significant positive correlation with p-Akt (r = 0.614, P < 0.001), p-mTOR (r = 0.523, P < 0.001) expression and negative correlation with PTEN level (r = 0.406, P < 0.001) by IHC staining.
Stellar winds, dead zones, and coronal mass ejections
Creators: name: Keppens, R.
name: Goedbloed, J. P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Axisymmetric stellar wind solutions are presented, obtained by numerically solving the ideal magnetohydrodynamic (MHD) equations. Stationary solutions are critically analysed using the knowledge of the flux functions. These flux functions enter in the general variational principle governing all axisymmetric stationary ideal MHD equilibria. The magnetized wind solutions for (differentially) rotating stars contain both a `wind' and a `dead' zone. We illustrate the influence of the magnetic field topology on the wind acceleration pattern, by varying the coronal field strength and the extent of the dead zone. This is evident from the resulting variations in the location and appearance of the critical curves where the wind speed equals the slow, Alfven, and fast speed. Larger dead zones cause effective, fairly isotropic acceleration to super-Alfvenic velocities as the polar, open field lines are forced to fan out rapidly with radial distance. A higher field strength moves the Alfven transition outwards. In the ecliptic, the wind outflow is clearly modulated by the extent of the dead zone. The combined effect of a fast stellar rotation and an equatorial `dead' zone in a bipolar field configuration can lead to efficient thermo-centrifugal equatorial winds. Such winds show both a strong poleward collimation and some equatorward streamline bending due to significant toroidal field pressure at mid-latitudes. We discuss how coronal mass ejections are then simulated on top of the transonic outflows.
description: scheduled for Astrophys. J. 530 #2, Febr.20 2000 issue. 9 figures (as 6 jpeg and 8 eps files)
Sequential superconductor-Bose insulator-Fermi insulator phase transitions in two-dimensional a-WSi
Creators: name: Zhang, Xiaofu
name: Schilling, Andreas
Publisher: name: arXiv
Year: 2018
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: A zero-temperature magnetic-field-driven superconductor to insulator transition (SIT) in quasi-two-dimensional superconductors is expected to occur when the applied magnetic-field crosses a certain critical value. A fundamental question is whether this transition is due to the localization of Cooper pairs or due to the destruction of them. Here we address this question by studying the SIT in amorphous WSi. Transport measurements reveal the localization of Cooper pairs at a quantum critical field B_c^1 (Bose-insulator), with a product of the correlation length and dynamical exponents zv~4/3 near the quantum critical point (QCP). Beyond B_c^1, superconducting fluctuations still persist at finite temperatures. Above a second critical field B_c^2>B_c^1, the Cooper pairs are destroyed and the film becomes a Fermi-insulator. The different phases all merge at a tricritical point at finite temperatures with zv=2/3. Our results suggest a sequential superconductor to Bose insulator to Fermi insulator phase transition, which differs from the conventional scenario involving a single quantum critical point.
title: ADCO, Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402) (11 H 1160), f. 00350
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2017
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160), f. 00350, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
title: Capturing the hot and violent Universe: Multiwavelength studies of Galactic TeV-discovered Supernova remnant shells and of optically-selected galaxy clusters
Creators: name: Stamer, Nhàn Thanh
Publisher: name: Universität Tübingen
Year: 2025
Subjects: subject: 530
subject: Supernova remnants
subject: cosmic rays
subject: galaxy clusters

description: Supernova remnants (SNRs) are the expanding structures left behind by supernova explosions. The explosion drives a shock wave outward, sweeping up and heating the surrounding interstellar medium (ISM). These remnants serve as natural laboratories for studying extreme physics processes, including the origin of cosmic rays (CRs). CRs are relativistic, charged particles which are believed to be effectively accelerated at SNRs' shock fronts. The first part of this thesis focuses on the studies of the SNR HESS J1534-571 and the SNR candidate HESS J1614-518, both identified as strong TeV gamma-ray emitters in the H.E.S.S (High Energy Stereoscopic System) Galactic Plane Survey. We investigate the multiwavelength morphology of these sources and the CR acceleration at their sites. Both HESS J1534-571 and HESS J1614-518 exhibit shell-like structures in radio and/or X-ray wavelengths, correlating with their TeV gamma-ray shells. This correlation confirms the SNR nature of HESS J1614-518 for the first time and suggests that radiation across wavelengths originates from the same CR populations. This allows us to construct spectral energy distributions and constrain high-energy gamma-ray production scenarios. For the two objects presented in this thesis, CR electrons cannot be ruled out as the responsible source for the detected high-energy gamma-rays. In addition, other properties of the SNRs, such as the interaction between shock-induced CRs and localised ambient cool gas, are also presented. Galaxy clusters are the largest gravitationally collapsed objects in the Universe, consisting of thousands of galaxies, hot gas in the intracluster medium (ICM), and dark matter, making them detectable across a wide range of wavelengths. They are valuable probes to constrain cosmological parameters and to study large-scale physics. However, samples selected by different methods based on different wavebands may represent distinct populations of clusters. Therefore, it is crucial to understand the characteristics of cluster samples and the impact of selection methods for further cosmological and astrophysical applications. The second part of this thesis presents the analyses of the optically selected cluster sample CAMIRA from the Subaru-HSC observations overlapping the eFEDS survey of the SRG/eROSITA X-ray telescope. Initially focusing on ~40 high-richness (N > 40) objects, we expanded the study to ~1000 clusters with lower richness cut (N > 15), examining morphology, scaling relations, and selection effects. We conclude that the optically-based method can effectively select a complete cluster population with diverse ICM characteristics. While optical properties remain relatively uniform across the sample, X-ray properties vary, influencing cluster detectability in X-ray surveys.
Galactic Bulges from HST-NICMOS Observations: Ages and Dust
Creators: name: Peletier, Reynier
name: Balcells, Marc
name: Davies, Roger
name: Andredakis, Y.
name: Vazdekis, A.
name: Burkert, A.
name: Prada, F.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present optical and near-infrared colour maps of the central regions of bulges of S0 and spiral galaxies obtained with WFPC2 and NICMOS on the HST. By combined use of HST and ground-based data the colour information spans from a few tens of pc to a few kpc. In almost all galaxies the colour profiles in the central 100-200 pc become more rapidly redder. We attribute the high central colour indices to a central concentration of dust. We infer an average extinction at the center of A_V = 0.6 - 1.0 mag. Several objects show central dust rings or disks at sub-kpc scales similar to those found by others in giant ellipticals. For galactic bulges of types S0 to Sb, the tightness of the B-I vs I-H relation suggests that the age spread among bulges of early type galaxies is small, of at most 2 Gyr. Colours at 1 R_eff, where we expect extinction to be negligible are similar to than those of elliptical galaxies in the Coma cluster, suggesting that these bulges formed at the same time as the bright galaxies in Coma. Furthermore the galaxy ages are found to be independent of their environment. Since it is likely that Coma was formed at redshift z > 3, our bulges, which are in groups and in the field, also must have been formed at this epoch. Bulges of early-type spirals cannot be formed by secular evolution of bars at recent epochs, since such bulges would be much younger. There are three galaxies of type Sbc and later, their bulges are younger and could perhaps arise from secular evolution of transient bars. Our results are in good agreement with semi-analytic predictions (Baugh et al. 1996, 1998, Kauffmann 1996), who also predict that bulges, in clusters and in the field, are as old as giant ellipticals in clusters.
description: 14 pages latex, uses MNRAS-style. Accepted for publication in MNRAS. Includes 5 figures. Fig. 1(a-e) are included as jpeg files. Higher resolution versions of those can be obtained from http://www.nottingham.ac.uk/~ppzrfp/colpaper . See also NASA/STScI press release 99-34 at http://oposite.stsci.edu/pubinfo/pr/1999/34/
The inflated radii of M-dwarfs in the Pleiades
Creators: name: Jackson, R. J.
name: Deliyannis, Constantine P.
name: Jeffries, R. D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Rotation periods obtained with the Kepler satellite have been combined with precise measurements of projected rotation velocity from the WIYN 3.5-m telescope to determine the distribution of projected radii for several hundred low-mass ($0.1 \leq M/M_{\odot} \leq 0.8$), fast-rotating members of the Pleiades cluster. A maximum likelihood modelling technique, that takes account of observational uncertainties, selection effects and censored data, and considers the effects of differential rotation and unresolved binarity, has been used to find that the average radius of these stars is $14 \pm 2$ per cent larger at a given luminosity than predicted by the evolutionary models of Dotter et al. (2008) and Baraffe et al. (2015). The same models are a reasonable match to the interferometric radii of older, magnetically inactive field M-dwarfs, suggesting that the over-radius may be associated with the young, magnetically active nature of the Pleiades objects. No evidence is found for any change in this over-radius above and below the boundary marking the transition to full convection. Published evolutionary models that incorporate either the effects of magnetic inhibition of convection or the blocking of flux by dark starspots do not individually explain the radius inflation, but a combination of the two effects might. The distribution of projected radii is consistent with the adopted hypothesis of a random spatial orientation of spin axes; strong alignments of the spin vectors into cones with an opening semi-angle $<30^{\circ}$ can be ruled out. Any plausible but weaker alignment would increase the inferred over-radius.
description: Accepted version, to appear in MNRAS
Lepton-pair production in association with a $b\bar{b}$ pair and the determination of the $W$ boson mass
Creators: name: Bagnaschi, Emanuele
name: Maltoni, Fabio
name: Vicini, Alessandro
name: Zaro, Marco
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We perform a study of lepton-pair production in association with bottom quarks at the LHC based on the predictions obtained at next-to-leading order in QCD, both at fixed order and matched with a QCD parton shower. We consider a comprehensive set of observables and estimate the associated theoretical uncertainties by studying the dependence on the perturbative QCD scales (renormalisation, factorisation and shower) and by comparing different parton-shower models (Pythia8 and Herwig++) and matching schemes (MadGraph5_aMC@NLO and POWHEG). Based on these results, we propose a simple procedure to include bottom-quark effects in neutral-current Drell-Yan production, going beyond the standard massless approximation. Focusing on the inclusive lepton-pair transverse-momentum distribution $p_{\bot}^{l^+l^-}$, we quantify the impact of such effects on the tuning of the simulation of charged-current Drell-Yan observables and the $W$-boson mass determination.
description: 47 pages, 29 figures, 1 table
On the migration of a system of protoplanets
Creators: name: Kley, Willy
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The evolution of a system consisting of a protoplanetary disc with two embedded Jupiter sized planets is studied numerically. The disc is assumed to be flat and non-self gravitating, which is modeled by the planar (two-dimensional) Navier-Stokes equations. The mutual gravitational interaction of the planets and the star, and the gravitational torques of the disc acting on the planets and the central star are included. The planets have an initial mass of one Jupiter mass $M_{Jup}$ each and the radial distances from the star are one and two semi-major axis of Jupiter, respectively. During the evolution both planets increase their mass due to accretion of gas from the disc; after about 2500 orbital periods of the inner planet it has reached a mass of 2.3 and the outer planet of 3.2~$M_{Jup}$. The net gravitational torques exerted by the disc on the planets result in an inward migration of the outer planet on time-scales comparable to the viscous evolution time of the disc, while the semi-major axis of the inner planet remains constant. When the distance of close approach eventually becomes smaller than their mutual Hill radius the eccentricities increase strongly and the system may turn unstable. The implications for the origin of the solar system and the extrasolar planets are discussed.
description: 5 Pages, 4 eps-figures, uses MN-Latex style file
Analyzing the Digital Traces of Political Manipulation: The 2016 Russian Interference Twitter Campaign
Creators: name: Badawy, Adam
name: Ferrara, Emilio
name: Lerman, Kristina
Publisher: name: arXiv
Year: 2018
Subjects: subject: Social and Information Networks (cs.SI)
subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences

description: Until recently, social media was seen to promote democratic discourse on social and political issues. However, this powerful communication platform has come under scrutiny for allowing hostile actors to exploit online discussions in an attempt to manipulate public opinion. A case in point is the ongoing U.S. Congress' investigation of Russian interference in the 2016 U.S. election campaign, with Russia accused of using trolls (malicious accounts created to manipulate) and bots to spread misinformation and politically biased information. In this study, we explore the effects of this manipulation campaign, taking a closer look at users who re-shared the posts produced on Twitter by the Russian troll accounts publicly disclosed by U.S. Congress investigation. We collected a dataset with over 43 million election-related posts shared on Twitter between September 16 and October 21, 2016, by about 5.7 million distinct users. This dataset included accounts associated with the identified Russian trolls. We use label propagation to infer the ideology of all users based on the news sources they shared. This method enables us to classify a large number of users as liberal or conservative with precision and recall above 90%. Conservatives retweeted Russian trolls about 31 times more often than liberals and produced 36x more tweets. Additionally, most retweets of troll content originated from two Southern states: Tennessee and Texas. Using state-of-the-art bot detection techniques, we estimated that about 4.9% and 6.2% of liberal and conservative users respectively were bots. Text analysis on the content shared by trolls reveals that they had a mostly conservative, pro-Trump agenda. Although an ideologically broad swath of Twitter users was exposed to Russian Trolls in the period leading up to the 2016 U.S. Presidential election, it was mainly conservatives who helped amplify their message.
Supplimentary material from A morphological novelty evolved by co-option of a reduced gene regulatory network and gene recruitment in a beetle
Creators: name: Yonggang Hu
name: Schmitt-Engel, Christian
name: Schwirz, Jonas
name: Nadi Stroehlein
name: Richter, Tobias
name: Upalparna Majumdar
name: Bucher, Gregor
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Developmental Biology

description: including figure S1-S7 and Table S1-S4
Flickering in AGB stars: Probing the nature of accreting companions
Creators: name: Snaid, S.
name: Zijlstra, A A.
name: McDonald, I.
name: Barker, Helen
name: Marsh, T. R.
name: Dhillon, V. S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Binary companions to asymptotic giant branch (AGB) stars are an important aspect of their evolution. Few AGB companions have been detected, and in most cases it is difficult to distinguish between main-sequence and white dwarf companions. Detection of photometric flickering, a tracer of compact accretion disks around white dwarfs, can help identify the nature of these companions. In this work, we searched for flickering in four AGB stars suggested to have likely accreting companions. We found no signs for flickering in two targets: R~Aqr and V1016 Cyg. Flickering was detected in the other two stars: Mira and Y Gem. We investigated the true nature of Mira's companion using three different approaches. Our results for Mira strongly suggest that its companion is a white dwarf.
Supplementary tables from Rapid aggregation of biofilm-covered microplastics with marine biogenic particles
Creators: name: Michels, Jan
name: Stippkugel, Angela
name: Lenz, Mark
name: Wirtz, Kai
name: Engel, Anja
Publisher: name: The Royal Society
Year: 2018
Subjects: Environmental Science

description: This file contains tables showing (a) an overview of the different experiments performed in this study and (b) results of the statistical analyses.
Pion Mass Effects in the Large $N$ Limit of $\chiPT$
Creators: name: Dobado, A.
name: Morales, J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We compute the large $N$ effective action of the $O(N+1)/O(N)$ non-linear sigma model including the effect of the pion mass to order $m^2_π/f_π^2$. This action is more complex than the one corresponding to the chiral limit not only because of the pion propagators but also because chiral symmetry produce new interactions proportional to $m^2_π/f_π^2$. We renormalize the action by including the appropriate counter terms and find the renormalization group equations for the corresponding couplings. Then we estudy the unitarity propierties of the scattering amplitudes. Finally our results are applied to the particular case of the linear sigma model and also are used to fit the pion scattering phase shifts.
description: FT/UCM/18/94
Macroscytus abditus J. A. LIS
Creators: name: Lis, J. A.
Publisher: name: Zenodo
Year: 2000
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Cydnidae
Macroscytus
Macroscytus abditus

description: Macroscytus abditus J.A. LIS
(Figs 8­14)
Macroscytus abditus J.A. LIS, 1993b: 41.
DESCRIPTION
Body 8.05­8.65 mm in length, 4.39­4.55 mm in width, from castaneous to almost black, sometimes corium and apices of pronotal umbones slightly brown or yellowish brown.
Head dorsally with tiny and hardly visible punctures; clypeus subapically without a pair of setigerous punctures, each paraclypeus with a single submarginal preocular puncture bearing hair­like seta (Fig. 9); ocular index 2.19­2.50; interocellar index 3.7­4.6; length of antennal segments (in mm): 0.35­0.38: 0.43­ 0.46: 0.55­0.59: 0.73­0.84: 0.87­0.94.
Pronotal disc weakly punctate, transverse discal impression behind calli absent; each lateral margin with 4­5 submarginal setigerous punctures (Fig. 8). Propleural depression with numerous coarse punctures.
Puncturation of a scutellar disc very weak, better visible only in its median part.
Mesocorium punctate with large punctures basally and the smaller apically; exocorium densely punctate; costa narrow, almost entirely separated from exocorium, bearing no setigerous punctures (Fig. 8).
Hind femora with 1­2 small teeth subapically, hind tibiae with neither denticles nor emargination on inner margins (Fig. 10).
Abdominal sterna smooth and polished; sutures laterally with small punctures, each segment with a patch of punctures posterior to spiracle, and a few punctures lateral and anterior to it; pregenital segment almost impunctate.
Male genitalia as in Figs 11­14.
TYPE DATA
Holotype male: Papua New Guinea, East. High. Prov., Alyura (BMNH).
MATERIAL EXAMINED
Holotype, 3 paratypes, and 3 other specimens: Papua New Guinea: East. High. Prov., Alyura, 3 paratypes (BMNH, UO); Star Range, Sibil, 3 exx. (NNML, UO).
DISTRIBUTION
Papua New Guinea.
description: Published as part of Lis, J. A., 2000, A revision of the burrower-bug genus Macroscytus Fieber, 1860 (Hemiptera: Heteroptera: Cydnidae), pp. 359-509 in Genus (Wrocław) 11 (3) on page 374
title: ADCO, Cartulaire des Dominicains de Dijon (1286), Cart. 221 (H 53), 170 folios, f. 0247
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios, f. 0247, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb15250518p
description: Provenance: http://www.idref.fr/02643413X/id
description: Provenance: https://www.geonames.org/6453767
description: Provenance: Dijon
description: Provenance: http://www.wikidata.org/entity/Q7003
Novel insight into circular RNA HECTD1 in astrocyte activation via autophagy by targeting MIR142-TIPARP: Implications for cerebral ischemic stroke
Creators: name: Han, Bing
name: Zhang, Yuan
name: Zhang, Yanhong
name: Bai, Ying
name: Chen, Xufeng
name: Huang, Rongrong
name: Wu, Fangfang
name: Leng, Shuo
name: Chao, Jie
name: H. Zhang, John
name: Hu, Gang
name: Yao, Honghong
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: Pharmacology
subject: Biological Sciences not elsewhere classified
subject: Mental Health

description: Circular RNAs (circRNAs) are highly expressed in the central nervous system and are involved in the regulation of physiological and pathophysiological processes. However, the potential role of circRNAs in stroke remains largely unknown. Here, using a circRNA microarray, we showed that circular RNA Hectd1 (circHectd1) levels were significantly increased in ischemic brain tissues in transient middle cerebral artery occlusion (tMCAO) mouse stroke models and further validated this finding in plasma samples from acute ischemic stroke (AIS) patients. Knockdown of circHectd1 expression significantly decreased infarct areas, attenuated neuronal deficits, and ameliorated astrocyte activation in tMCAO mice. Mechanistically, circHECTD1 functions as an endogenous MIR142 (microRNA 142) sponge to inhibit MIR142 activity, resulting in the inhibition of TIPARP (TCDD inducible poly[ADP-ribose] polymerase) expression with subsequent inhibition of astrocyte activation via macroautophagy/autophagy. Taken together, the results of our study indicate that circHECTD1 and its coupling mechanism are involved in cerebral ischemia, thus providing translational evidence that circHECTD1 can serve as a novel biomarker of and therapeutic target for stroke.
Poster : The Investigation of IL-1 β and Oxytocin Levels among Teeneger with Primary Dysmenorrhea
Creators: name: Mukhoirotin
name: Kurniawati
name: Fatmawati, Diah Ayu
Publisher: name: Zenodo
Year: 2019
Subjects: Investigation of IL-1 β
Oxytocin Levels
Primary Dysmenorrhea

description: This material presented in 1st ICESE 2019, Kuala Lumpur, Malaysia
Metal Organic Frameworks - I MOF come sensori chimici e adsorbenti di inquinanti
Creators: name: Barbara, Ventura
name: Khaled, Hassanein
Publisher: name: Zenodo
Year: 2019

description: Poster presented at the "European Reserachers' Night 2018", in the frame of the activity "TEC01: I MOF come sensori chimici e adsorbenti di inquinanti", 28 September 2018, Bologna, Italy
Multi-diagnostic imaging of evaporating fuel wall-films in combustion as a source of PAH and soot
Creators: name: Jüngst, Niklas
name: Kaiser, Sebastian
Publisher: name: Zenodo
Year: 2018

description: In direct-injection gasoline engines, evaporating fuel wall-films and the resulting inhomogeneities of the air-fuel mixture near those films make the formation of PAH and soot in subsequent combustion likely. Different optical techniques are needed to visualize the links of this process chain, such as the spray, film formation, evaporation, combustion, and soot formation. In our model experiment, a mixture of isooctane (surrogate fuel) and toluene (fluorescent tracer) is injected by a multi-hole injector into an optically accessible flow channel. Air flows continuously through the channel at room pressure. Combustion is initiated by a spark plug within the fuel/air-mixture cloud. Some of the liquid fuel impinges on the quartz-glass wall on the opposite side and forms wall films. The turbulent flame front propagates along the chamber and ignites pool fires above the wall films, leading to locally sooting combustion. Laser-induced fluorescence (LIF) of the toluene using 266 nm excitation images the fuel-film thickness and visualizes the fuel vapor above the liquid films. Laser-induced incandescence (LII) using 1064 nm excitation visualizes soot. As a complementary visualization of soot, the natural flame luminosity, mainly from soot incandescence, is captured with a high-speed camera. Schlieren imaging combines the visualization of the evaporating liquid and the sooting flame. The LIF images show that indeed the fuel wall-films remain on the surface long after the flame front has passed, leading to subsequent soot formation. In a next step, we will simultaneously visualize the formation of soot precursors (PAH) and soot with LIF and LII, respectively.
title: The effects of social norms and observability on food choice
Creators: name: Dannenberg, Astrid
name: Klatt, Charlotte
name: Weingärtner, Eva
Publisher: name: Universität Kassel
Year: 2024
Subjects: subject: food choice
subject: meat consumption
subject: social norms
subject: observability
subject: experiment
subject: 300
subject: 330
subject: Lebensmittel
subject: Entscheidung
subject: Verbraucherverhalten
subject: Fleischverbrauch
subject: Soziale Norm
subject: Beobachtbarkeit
subject: Experiment

description: Gefördert im Rahmen des Projekts DEAL
Radio galaxy evolution: what you can learn from a Brief Encounter
Creators: name: Blundell, Katherine
name: Rawlings, Steve
name: Willott, Chris
name: Kassim, Namir
name: Perley, Rick
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe the pitfalls encountered in deducing from classical double radio source observables (luminosity, spectral index, redshift and linear size) the essential nature of how these objects evolve. We discuss the key role played by hotspots in governing the energy distribution of the lobes they feed, and subsequent spectral evolution. We present images obtained using the new 74 MHz receivers on the VLA and discuss constraints which these enforce on models of the backflow and ages in classical doubles.
description: invited talk at `Lifecycles of Radio Galaxies' workshop; eds John Biretta et al
On the Role of Dissolved Gases in the Atmosphere Retention of Low-Mass Low-Density Planets
Creators: name: Chachan, Yayaati
name: Stevenson, David J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Low-mass low-density planets discovered by Kepler in the super-Earth mass regime typically have large radii for their inferred masses, implying the presence of H$_2$-He atmospheres. These planets are vulnerable to atmospheric mass loss due to heating by the parent star's XUV flux. Models coupling atmospheric mass loss with thermal evolution predicted a bimodal distribution of planetary radii, which has gained observational support. However, a key component that has been ignored in previous studies is the dissolution of these gases into the molten core of rock and iron that constitute most of their mass. Such planets have high temperatures ($>$2000 K) and pressures ($\sim$kbars) at the core-envelope boundary, ensuring a molten surface and a subsurface reservoir of hydrogen that can be 5-10 times larger than the atmosphere. This study bridges this gap by coupling the thermal evolution of the planet and the mass loss of the atmosphere with the thermodynamic equilibrium between the dissolved H$_2$ and the atmospheric H$_2$ (Henry's law). Dissolution in the interior allows a planet to build a larger hydrogen repository during the planet formation stage. We show that the dissolved hydrogen outgasses to buffer atmospheric mass loss. The slow cooling of the planet also leads to outgassing because solubility decreases with decreasing temperature. Dissolution of hydrogen in the interior therefore increases the atmosphere retention ability of super-Earths. The study highlights the importance of including the temperature- and pressure-dependent solubility of gases in magma oceans and coupling outgassing to planetary evolution models.
description: 11 pages, 6 figures, published in ApJ on February 7 2018
Additional file 1 of Ibrutinib combination therapy for advanced gastrointestinal and genitourinary tumours: results from a phase 1b/2 study
Creators: name: Oh, Do-Youn
name: Maqueda, Maria Alsina
name: Quinn, David I.
name: O’Dwyer, Peter J.
name: Chau, Ian
name: Kim, Sun Young
name: Duran, Ignacio
name: Castellano, Daniel
name: Berlin, Jordan
name: Mellado, Begona
name: Williamson, Stephen K.
name: Lee, Keun-Wook
name: Marti, Francisca
name: Mathew, Paul
name: Saif, Muhammad Wasif
name: Wang, Ding
name: Chong, Elizabeth
name: Hilger-Rolfe, Jacqueline
name: Dean, James P.
name: Arkenau, Hendrik-Tobias
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Hematology

description: Additional file 1: Supplementary Methods. Follow-up. Supplementary Methods. Maximum tolerated dose. Supplementary Methods. Dose adjustment guidelines. Supplementary Table S1. Prior therapies
Cosmological Constraints on the Scale of Supersymmetry Breaking
Creators: name: Rangarajan, Raghavan
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider the cosmological and astrophysical constraints on the decay of massive $E_8 \times E_8^\prime$ superstring axions associated with the hidden sector. We find that decay lifetimes greater than 1 s are ruled out by limits from nucleosynthesis, by limits on the distortion of the cosmic microwave and gamma ray backgrounds and by closure arguments. We conclude that $Λ>1.2\times10^{13}\gev$, where $Λ$ is the scale of gaugino condensation in the hidden sector. This implies that the scale of supersymmetry breaking is greater than $10^{10}\gev$. Significantly, our result agrees with the value of $5\times 10^{13}\gev$ for $Ł$ obtained independently by setting supersymmetric scalar masses equal to $m_W$.
description: 14 pages, Constraints on axion decays from limits on photodissociation of light elements revised. No change in final results. Three appendices from companion paper hep-ph/9407323 added. Plain TEX file
File S1. Description of three-compartment model from In silico mouse study identifies tumour growth kinetics as biomarkers for the outcome of anti-angiogenic treatment
Creators: name: Qianhui Wu
name: Arnheim, Alyssa D.
name: Finley, Stacey D.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: 60114 Systems Biology
subject: FOS: Biological sciences
subject: 90399 Biomedical Engineering not elsewhere classified
subject: FOS: Medical engineering

description: Detailed description of the computational model used
Random-cluster correlation inequalities for Gibbs fields
Creators: name: Gandolfi, Alberto
Publisher: name: arXiv
Year: 2018
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 60G60, 60J99, 82B44, 82D30

description: In this note we prove a correlation inequality for local variables of a Gibbs field based on the connectivity by active hyperbonds in a random cluster representation of the non overlap configuration distribution of two independent copies of the field. As a consequence, we show that absence of Machta-Newman-Stein blue bonds percolation implies uniqueness of Gibbs distribution in EA Spin Glasses. In dimension two this could constitute a step towards a proof that the critical temperature is zero.
description: 23 pages
Conference: "Approaches to Multimodal Digital Environments: from theories to practices"
Creators: name: Eu Made 4ll
Publisher: name: Zenodo
Year: 2019
Subjects: multimodality
digital literacy
digital skills
multimodal
language learning
blog
social semiotics
discourse analysis
sociolinguistics
visual communication

description: Approaches to Multimodal Digital Environments: from theories to practices Rome, University of “Tor Vergata”
 20 – 22 June 2019 Multimodal digital communication is the main theme of this conference meant to attract multidisciplinary research on a wide range of issues from teaching and learning to analysing multimodal digital data appearing in multiple communication arenas. More information on a-mode.eumade4ll.eu/ Keynote speakers:
 Marina Bondi
 Carey Jewitt
 Rodney Jones
 Gunther Kress and Jeff Bezemer
 David Machin
 Theo van Leeuwen