cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Comparative study of the internal and external evaluation of the University of Patras designating its strategic planning by a SWOT analysis (full text in Greek)
Creators: name: Kouremenou, Aggeliki
name: Spyropoulou, Dimitra
name: Fertaki, Theodora
Publisher: name: Academia
Year: 2019
Subjects: Quality assurance, SWOT analysis, strategic plan

description: The internal evaluation at institutional level is carried out in accordance with the legal provisions in forceunder the supervision of MODIP (the Quality Assurance Unit –at institutional level-). It reflects the institution's “physiognomy”and all the features of its operation. Τhe external evaluation is carried out by a Committee of Independent Experts under the supervision of ADIP (Hellenic Quality Assurance and Accreditation Agency), that analyzes and examines the results of the internal report. After an on-site visit by the external evaluation committee to the Institution, which has a specific program, an external evaluation report is being prepared, which is made public. The purpose of this paper is to compare the main points of the internal and external evaluation reports of the University of Patras through a critical view as well as its strategic planning through a SWOT analysis. Through the SWOT analysis, an Institution can effectively identify and reclaim its strengths, exploit future opportunities and avoid threats and dangers that may arise. Adopting strategic planning is the key to the smooth Institution’s cooperation and development and its ability to respond effectively to changes in continuing academic competition in higher education area. In the present paper, after the comparative analysis of the above-mentioned reports, a strategic planning for some of the University’s actions is proposed, based on its "Strengths" and "Opportunities".
description: Academia, No 15 (2019)
Exploring helical dynamos with machine learning
Creators: name: Nauman, Farrukh
name: Nättilä, Joonas
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Machine Learning (cs.LG)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: We use ensemble machine learning algorithms to study the evolution of magnetic fields in magnetohydrodynamic (MHD) turbulence that is helically forced. We perform direct numerical simulations of helically forced turbulence using mean field formalism, with electromotive force (EMF) modeled both as a linear and non-linear function of the mean magnetic field and current density. The form of the EMF is determined using regularized linear regression and random forests. We also compare various analytical models to the data using Bayesian inference with Markov Chain Monte Carlo (MCMC) sampling. Our results demonstrate that linear regression is largely successful at predicting the EMF and the use of more sophisticated algorithms (random forests, MCMC) do not lead to significant improvement in the fits. We conclude that the data we are looking at is effectively low dimensional and essentially linear. Finally, to encourage further exploration by the community, we provide all of our simulation data and analysis scripts as open source IPython notebooks.
description: accepted by A&A, 11 pages, 6 figures, 3 tables, data + IPython notebooks: https://github.com/fnauman/ML_alpha2
Does the plasma composition affect the long term evolution of relativistic jets?
Creators: name: Scheck, L.
name: Aloy, M. A.
name: Marti, J. M.
name: Gomez, J. L.
name: Mueller, E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the influence of the matter content of extragalactic jets on their morphology, dynamics and emission properties. For this purpose we consider jets of extremely different compositions including pure leptonic and baryonic plasmas. Our work is based on two-dimensional relativistic hydrodynamic simulations of the long-term evolution of powerful extragalactic jets propagating into a homogeneous environment. The equation of state used in the simulations accounts for an arbitrary mixture of electrons, protons and electron-positron pairs. Using the hydrodynamic models we have also computed synthetic radio maps and the thermal Bremsstrahlung X-ray emission from their cavities. Although there is a difference of about three orders of magnitude in the temperatures of the cavities inflated by the simulated jets, we find that both the morphology and the dynamic behaviour are almost independent on the assumed composition of the jets. Their evolution proceeds in two distinct epochs. During the first one multidimensional effects are unimportant and the jets propagate ballistically. The second epoch starts when the first larger vortices are produced near the jet head causing the beam cross section to increase and the jet to decelerate. The evolution of the cocoon and cavity is in agreement with a simple theoretical model. The beam velocities are relativistic ($Γ\simeq 4$) at kiloparsec scales supporting the idea that the X-ray emission of several extragalactic jets may be due to relativistically boosted CMB photons. The radio emission of all models is dominated by the contribution of the hot spots. All models exhibit a depression in the X-rays surface brightness of the cavity interior in agreement with recent observations.
description: 41 pages, 12 png figures. See also high quality versions of the figures and several movies under http://www.mpa-garching.mpg.de/~maa/JETS/LongTermEv/index.html
Exploration of the bright and dark exciton landscape and fine structure of MoS$_2$ (using G$_0$W$_0$-BSE)
Creators: name: Yu, Hongyu
name: Laurien, Magdalena
name: Hu, Zhenpeng
name: Rubel, Oleg
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Spectral ordering between dark and bright excitons in transition metal dichalcogenides is of increasing interest for optoelectronic applications. However, little is known about dark exciton energies and their binding energies. We report the exciton landscape including momentum-forbidden dark excitons of MoS$_{2}$ monolayer using single shot GW-Bethe Salpeter equation (G$_{0}$W$_{0}$-BSE) calculations. We find the lowest-energy exciton to be indirect at ($\textrm K'_{v} \rightarrow \textrm K_{c}$) in agreement with recent GdW-BSE calculations [2D Mater. 6, 035003 (2019)]. We also find that by large, dark exciton binding energies ($E_b$) scale with the quasiparticle energies ($E_g$) according to the $E_b/E_g=0.25$ rule. Differences in exciton binding energies are explained using an orbital theory.
description: 19 pages, 7 figs
Microlens Parallaxes of Binary Lenses Measured from a Satellite
Creators: name: Graff, David S.
name: Gould, Andrew
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Caustic-crossing binary lenses make up about 5% of all detected microlenses. The relative proper motion of a caustic-crossing binary lens can be measured with observations from a single terrestrial telescope. Thus, uniquely, binary lenses can be completely solved with only the addition of a measurement of the microlensing parallax. This solution will yield the mass, distance, and transverse velocity of the lens relative to the source. To date, only one of the $\sim 1000$ observed microlensing events has been so solved. We examine the ability of a parallax satellite combined with ground-based observations to solve these events. To measure both components of the vector parallax, the lens must be observed near two different caustics. Thus, the final accuracy is determined mostly by whether one can intensively monitor part of the first caustic crossing, by the magnification pattern, and by the path of the source with respect to the lens geometry. We find that vector parallaxes can be measured far more easily for binary lenses than single lenses, requiring 1-3 orders of magnitude fewer photons. They may thus yield a large number of completely solved lenses relatively cheaply.
description: 8 pages emulateapj style, 4 figures, Submitted to ApJ
The impact of mode of drug administration on medication adherence
Creators: name: Böhm, Anna-Katharina
name: Schneider, Udo
name: Stargardt, Tom
Publisher: name: Zenodo
Year: 2018

description: Abstract and poster presentation for the EuHEA 2018 conference in Maastricht about the impact of fixed dose versus loose dose combination drugs on adherence and other outcomes in the treatment of type 2 diabetes mellitus in Germany. Preliminary results.
Threticus lucifugus
Creators: name: Ježek, Jan
name: Hájek, Josef
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psychodidae
Threticus
Threticus lucifugus

description: Threticus lucifugus (Walker, 1856)
 Published record. JEŽEK (1985b): Plasnice.
 Unpublished records. Bartošovice v Orlických horách, Rašeliniště pod Předním vrchem peatbog [2], J, 14.- 24.ix.1993, J + H, YPT; Bedřichovka [4], J, 20.viii.1993, J; Bukačka NNR [7], 4 JJ, 16.-24.ix.1993, 28.vi.- 18.vii. and 18.vii.-5.viii.1994, H + V, H + V + J, J + H, MT and YPT; Čertův důl valley [13], J, 30.viii.1994, J; Hradisko [36], J, 1.viii.1996, J; Jamné [37], J, 11.vii.1981, J; Rašeliniště Kačerov NR peatbog [42], 2 JJ, 26.v.- 13.vi.1994 and 1.viii.1993, H, J, YPT and sweeping; Kamenec [43], J, 31.viii.1994, J; Klášterec nad Orlicí [46], J, 19.ix.1993, J; Kouty [50], J, 18.viii.1993, J; Kovárna hostel near Rampuše [51], J, 1.viii.1993, J; Mezivrší [62], J, 18.viii.1993, J; Mýto [67], J, 3.viii.1993, J; Nová Ves, Divoká Orlice river meander [72], J, 18.v.1994, J + H; Olešnice v Orlických horách, Číhalka hostel [75], J, 12.viii.1993, J; Olešnice v Orlických horách, Panský vrch hill [77], 3 JJ, 21.v., 17.-24.v., 24.v.-9.vi.1994, H, H + J, J, YPT and sweeping; Olešnice v Orlických horách, Polish border [78], J, 11.ix.1997, J; Olešnice v Orlických horách, Ruské údolí valley [79], J, 14.viii.1993, J; between Pěčín and Rokytnice v Orlických horách, Suchá brook [87], J, 29.viii.1994, J; Petrovičky [89], J, 23.vii.1996, J; Podolí [93], J, 17.viii.1994, J; Rokytnice v Orlických horách, Polův kopec hill [94], J, 23.viii.1995, J; Sedloňov – Polom [100], 2 JJ, 24.v.1994 and 11.ix.1997, J; Svatý Matouš church between Jedlová v Orlických horách and Staré Hutě [107], 2 JJ, 22.v.1994 and 15.viii.1993, J; Šerlišské louky meadows [111], J, 16.-24.ix.1993, J + H, YPT; Trčkov env., Velká louka NM meadow [118], J, 9.ix.1997, J; Trčkov NNR [119], 3 JJ, 16.-25. v. and 26.v.- 9.vi.1994, H, H + J, YPT; Vrchní Orlice [125], J, 6.viii.1997, J; Zdobnice, Zdobnice river [132], J, 9.viii.1993, J; Zelenka [134], J, 9.ix.1997, J; Zvonkové údolí valley [139], 2 JJ, 18.viii.1993, 15.-24.ix.1993, J, J + H, YPT and sweeping; Zvonkové údolí valley, Kuní vrch hill [138], 2 JJ, 15.ix.1993, J.
 Vegetation. 1, 2, 5-6, 8, 12, 14-17, 19-20, 22-26, 29-35, 37-38, 40-41, 44-47, 49-53, 55-56, 59-63, 65-68, 70-81, 83-91, 94-102; 110-114, 116-117, 119, 121, 123-126.
European species, common; see JEŽEK (1985b, 2006a) and WAGNER (1990, 2007) for more data on its distribution.
description: Published as part of Ježek, Jan & Hájek, Josef, 2007, Psychodidae (Diptera) of the Orlické hory Protected Landscape Area and neighbouring areas with descriptions of two new species from the Czech Republic, pp. 237-285 in Acta Entomologica Musei Nationalis Pragae 47 on pages 260-261, DOI: 10.5281/zenodo.5328353
On Drum Brake Squeal—Assessment of Damping Measures by Time Series Data Analysis of Dynamometer Tests and Complex Eigenvalue Analyses
Creators: name: Gräbner, Nils
name: Schmid, Dominik
name: Von Wagner, Utz
Publisher: name: MDPI AG
Year: 2023
Subjects: subject: 600 Technik, Medizin, angewandte Wissenschaften::620 Ingenieurwissenschaften::620 Ingenieurwissenschaften und zugeordnete Tätigkeiten
subject: brake squeal
subject: drum brake
subject: shim
subject: dynamometer
subject: finite-element analysis
subject: big data analysis
subject: machine learning

description: Brake squeal—an audible high-frequency noise phenomenon in the range between 1 kHz and 15 kHz resulting from self-excited vibrations—is one of the main cost drivers while developing brake systems. Increasing damping is often a crucial factor in the context of self-excited vibrations. Countermeasures applied for preventing brake squeal have been investigated particularly for disk brakes in the past. However, in recent years, drum brakes have once again become more important, partly because of the issue of particle emissions. Concerning noise problems, drum brakes have a decisive advantage compared to disk brake systems in that the outer drum surface is freely accessible for applying damping devices. This paper focuses on the fundamental proving and evaluation of passive damping measures on a simplex drum brake system. To obtain a detailed understanding of the influence of additional damping on the squealing behavior of drum brakes, extensive experimental investigations are performed on a brake with an intentionally introduced high squealing tendency in the initial configuration. This made it possible to investigate the influence of different types of damping measures on their effectiveness. Techniques from the field of big data analysis and machine learning are tested to detect squeal in measured time series data. These techniques were remarkably reliable and made it possible to detect squeal efficiently even in data that was not generated on a traditional costly NVH brake dynamometer. To investigate whether the simulation method usually used for the simulation of brake squeal is applicable to depicting the influence of additional damping in drum brakes, a complex eigenvalue analysis was performed with Abaqus, and the results were compared with those from the experiments.
Basking in Their Glory? Expressive Partisanship among People of Color Before and After the 2020 US Election
Creators: name: Maxwell, Rahsaan
name: Pérez, Efrén
name: Zonszein, Stephanie
Publisher: name: Cambridge University Press (CUP)
Year: 2022

description:
As the number of people of color (PoC) grows in the United States, a key question is how partisanship will develop among this important electoral group. Yet many open questions remain about PoC partisanship, due to limited availability of panel data, a lack of sensitive instrumentation, and small samples of PoC in most public opinion surveys. This brief report leverages a unique panel of African American ( N = 650) and Latino ( N = 650) eligible voters, before and after the 2020 Presidential Election between Democrat Joe Biden and Republican Donald Trump. Using measures that tap expressive partisan, racial, and national identity attachments, we find that Biden’s electoral victory significantly intensified partisan identity among his Democratic PoC supporters, relative to PoC who were not Democrats and supported Trump. We do not find significant changes in racial or national identities. Our results advance research on PoC’s partisanship.
Mass Density Profiles of LSB Galaxies
Creators: name: de Blok, W. J. G.
name: McGaugh, Stacy S.
name: Bosma, Albert
name: Rubin, Vera C.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We derive the mass density profiles of dark matter halos that are implied by high spatial resolution rotation curves of low surface brightness galaxies. We find that at small radii, the mass density distribution is dominated by a nearly constant density core with a core radius of a few kpc. For rho(r) ~ r^a, the distribution of inner slopes a is strongly peaked around a = -0.2. This is significantly shallower than the cuspy a < -1 halos found in CDM simulations. While the observed distribution of alpha does have a tail towards such extreme values, the derived value of alpha is found to depend on the spatial resolution of the rotation curves: a ~ -1 is found only for the least well resolved galaxies. Even for these galaxies, our data are also consistent with constant density cores (a = 0) of modest (~ 1 kpc) core radius, which can give the illusion of steep cusps when insufficiently resolved. Consequently, there is no clear evidence for a cuspy halo in any of the low surface brightness galaxies observed.
description: To be published in ApJ Letters. 6 pages. Uses aastex and emulateapj5.sty Typo in Eq 1 fixed
Additional file 2: of The impact of governance in primary health care delivery: a systems thinking approach with a European panel
Creators: name: Espinosa-GonzĂĄlez, Ana
name: Delaney, Brendan
name: Marti, Joachim
name: Darzi, Ara
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Evolution of the framework through three Delphi rounds. (PDF 107 kb)
Tensor-Network Approach for Quantum Metrology in Many-Body Quantum Systems
Creators: name: Chabuda, Krzysztof
name: Dziarmaga, Jacek
name: Osborne, Tobias J.
name: Demkowicz-Dobrzanski, Rafal
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Identification of the optimal quantum metrological protocols in realistic many particle quantum models is in general a challenge that cannot be efficiently addressed by the state-of-the-art numerical and analytical methods. Here we provide a comprehensive framework exploiting matrix product operators (MPO) type tensor networks for quantum metrological problems. Thanks to the fact that the MPO formalism allows for an efficient description of short-range spatial and temporal noise correlations, the maximal achievable estimation precision in such models, as well as the optimal probe states in previously inaccessible regimes can be identified. Moreover, the application of infinite MPO (iMPO) techniques allows for a direct and efficient determination of the asymptotic precision of optimal protocols in the limit of infinite particle numbers. We illustrate the potential of our framework in terms of an atomic clock stabilization (temporal noise correlation) example as well as for magnetic field sensing in the presence of locally correlated magnetic field fluctuations (spatial noise correlations). As a byproduct, the developed methods for calculating the quantum Fisher information via MPOs may be used to calculate the fidelity susceptibility - a parameter widely used in many-body physics to study phase transitions.
description: 24 pages
The Universe Was Reionized Twice
Creators: name: Cen, Renyue
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show the universe was reionized twice, first at z~15-16 and second at z~6. Such an outcome appears inevitable, when normalizing to two well determined observational measurements, namely, the epoch of the final cosmological reionization at z~6 and the density fluctuations at z~6, which in turn are tight ly constrained by Lyman alpha forest observations at z~3. These two observations most importantly fix the product of star formation efficiency and ionizing photon escape fraction from galaxies at high redshift. To the extent that the relative star formation efficiencies in gaseous minihalos with H2 cooling and large halos with atomic cooling at high redshift are still unknown, the primary source for the first reionization could be Pop III stars either in minihalos or in large halos. We show that gas in minihalos can be cooled efficiently by H2 molecules and star formation can continue to take place largely unimpeded throughout the first reionization period, thanks to two new mechanisms for generating a high X-ray background during the Pop III era, put forth here. Moreover, an important process for producing a large number of H2 molecules in relic HII regions of Pop III galaxies, first pointed out by Ricotti, Gnedin, & Shull, is quantified here. It is shown that the Lyman-Werner background may never build up during the Pop III era. The long cosmological reionization and reheating history is complex. We discuss a wide range of implications and possible tests for this new reionization picture. In particular, Thomson scattering optical depth is increased to 0.10 +- 0.03, compared to 0.027 for the case of only one rapid reionization at z=6. Upcoming Microwave Anisotropy Probe observation of the polarization of the cosmic microwave background should be able to distinguish between these two scenarios.
description: submitted to ApJ, 69 pages, substantial revision made and conclusions strengthened
title: One-pot synthesis of mesoporous cobalt phosphate used as a catalase-like nanozyme
Creators: name: Hughes, Davin V.
name: Berstler, Calvin
name: Trewyn, Brian G.
Publisher: name: Colorado School of Mines. Arthur Lakes Library
Year: 2024

description: Being able to conduct multi-step chemoenzymatic catalysis in a one-pot system is a challenging task. A chemoenzymatic reaction represents a reaction where two or more consecutive transformations take place in a single reaction vessel. This process uses both enzymatic and chemical catalysis to more efficiently generate desired products from commercially available starting materials while removing the need to isolate intermediates. With new techniques to support employing enzymes and organic species within single-pot systems, the use of catalytically active mesoporous nanomaterials as enzyme supports has the potential benefits to enhance the performance of chemoenzymatic tandem systems. There are numerous advantages to using enzymes though they are costly and their functionality is limited to a small range of temperatures and pH levels. Because of this, enzyme mimics (Nanozymes) are very sought-after inorganic alternatives that are low-cost, high-stability alternatives. Here I explore a low-cost, high-efficiency method to synthesize a mesoporous cobalt phosphate (mCoPi) with the ability to transform hydrogen peroxide into water and oxygen and to be able to act as a catalase-like nanozyme in a variety of harsh local environments.
Hydrogenation of Carbon Dioxide to Dimethyl Ether on CuO–ZnO/ZSM-5 Catalysts: Comparison of Powder and Electrospun Structures
Creators: name: Nejadsalim, Aidin
name: Godini, Hamid Reza
name: Ramesh Kumar, Sanjay
name: Gallucci, Fausto
name: Kober, Delf
name: Gurlo, Aleksander
name: Görke, Oliver
Publisher: name: MDPI AG
Year: 2023
Subjects: subject: 600 Technik, Medizin, angewandte Wissenschaften::620 Ingenieurwissenschaften::620 Ingenieurwissenschaften und zugeordnete Tätigkeiten
subject: hybrid catalyst
subject: CO2 hydrogenation
subject: dimethyl ether
subject: electrospinning
subject: CuO–ZnO
subject: ZSM-5
subject: characterization

description: The promising direct dimethyl ether (DME) production through CO2 hydrogenation was systematically analyzed in this research by synthesizing, characterizing, and testing several catalytic structures. In doing so, various combinations of precipitation and impregnation of copper- and zinc-oxides (CuO–ZnO) over a ZSM-5 zeolite structure were applied to synthesize the hybrid catalysts capable of hydrogenating carbon dioxide to methanol and dehydrating it to DME. The resulting catalytic structures, including the co-precipitated, sequentially precipitated, and sequentially impregnated CuO–ZnO/ZSM-5 catalysts, were prepared in the form of particle and electrospun fibers with distinguished chemical and structural features. They were then characterized using XRD, BET, XPS, ICP, TGA, SEM, and FIB-SEM/EDS analyses. Their catalytic performances were also tested and analyzed in light of their observed characteristics. It was observed that it is crucial to establish relatively small-size and well-distributed zeolite crystals across a hybrid catalytic structure to secure a distinguished DME selectivity and yield. This approach, along with other observed behaviors and the involved phenomena like catalyst particles and fibers, clusters of catalyst particles, or the whole catalytic bed, were analyzed and explained. In particular, the desired characteristics of a CuO–ZnO/ZSM-5 hybrid catalyst, synthesized in a single-pot processing of the precursors of all involved catalytically active elements, were found to be promising in guiding the future efforts in tailoring an efficient catalyst for this system.
On scalar radiation
Creators: name: Fiol, Bartomeu
name: Martínez-Montoya, Jairo
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss radiation in theories with scalar fields. Our key observation is that even in flat spacetime, the radiative fields depend qualitatively on the coupling of the scalar field to the Ricci scalar: for non-minimally coupled scalars, the radiative energy density is not positive definite, the radiated power is not Lorentz invariant and it depends on the derivative of the acceleration. We explore implications of this observation for radiation in conformal field theories. First, we find a relation between two coefficients that characterize radiation, that holds in all the conformal field theories we consider. Furthermore, we find evidence that for a $1/2$-BPS probe coupled to ${\cal N}=4$ super Yang-Mills, and following an arbitrary trajectory, the spacetime dependence of the one-point function of the energy-momentum tensor is independent of the Yang-Mills coupling.
description: 14 pages. v2: important typo fixed in equation (25). Minor edits. v3: Expanded version with a new section. A new computation has been added, showing that the full one-point function of the energy density in ${\cal N}=4$ SYM in the presence of a 1/2-BPS probe, displays the same spacetime dependence at weak and strong 't Hooft coupling. v4: tiny typo fixed
Chandra observtaion of A2256 - a cluster at the early stage of merging
Creators: name: Sun, M.
name: Murray, S. S.
name: Markevitch, M.
name: Vikhlinin, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present here \chandra observations of the rich cluster of galaxies A2256. In addition to the known cool subcluster, a new structure was resolved 2$'$ east of the peak of the main cluster. Its position is roughtly at the center of a low-brightness radio halo. Spectral analysis shows that the "shoulder" has high iron abundance ($\sim$ 1). We suggest that this structure is either another merging component or an internal structure of the main cluster. The X-ray redshifts of several regions were measured. The results agree with the optical ones and suggest that the main cluster, the subcluster and the "shoulder" are physically associated and interacting. The subcluster has low temperature ($\sim$ 4.5 keV) and high iron abundance ($\sim$ 0.6) in the central 150 kpc. The \chandra image shows a relatively sharp brightness gradient at the south of the subcluster peak running south-south-east (SSE). A temperature jump was found across the edge, with higher temperature ahead of the edge in the low density region. This phenomenon is qualitatively similar to the "cold fronts" found in A2142 and A3667. If the "shoulder" is ignored, the temperature map resembles those simulations at the early stage of merging while the subcluster approached the main cluster from somewhere west. This fact and the observed edge, in combination with the clear iron abundance contrast between the center of the subcluster ($\sim$ 0.6) and the main cluster ($\sim$ 0.2), all imply that the ongoing merger is still at the early stage. At least three member galaxies, including a radio head-tail galaxy, were found to have corresponding X-ray emission.
description: The revised version. The shown abstract is shrunk. Accepted by ApJ. If it is possible, please try to look at the high-resolution version is http://cfa160.harvard.edu/~sunm/a2256.tar.gz
Trichopsychoda hirtella
Creators: name: Ježek, Jan
name: Hájek, Josef
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psychodidae
Trichopsychoda
Trichopsychoda hirtella

description: Trichopsychoda hirtella (Tonnoir, 1919)
 Unpublished records. Deštné v Orlických horách, Bělá brook [16], ♀, 14.viii.1993, J; Dolní Čermná, Orlice Nature Park [24], 3 JJ, 27.vii.-11.viii. and 12.-26.viii.1995, J, LT, yellow and red ST; Kamenec [43], J, 31.viii.1994, J; Neratov [70], J, 23.vii.1993, J; Olešnice v Orlických horách [74], ♀, 26.vi.1996, J; Vysoké Žibřidovice [128], J, 2.viii.1997, J.
 Vegetation. 1, 3, 14, 17, 23, 25, 29, 32, 37, 44, 56, 60, 67, 71, 80, 86, 88, 98; 111, 113-114, 121, 124.
European species, common; for more information see JEŽEK (1985b, 2006a).
description: Published as part of Ježek, Jan & Hájek, Josef, 2007, Psychodidae (Diptera) of the Orlické hory Protected Landscape Area and neighbouring areas with descriptions of two new species from the Czech Republic, pp. 237-285 in Acta Entomologica Musei Nationalis Pragae 47 on page 261, DOI: 10.5281/zenodo.5328353
Additional file 1 of Bilateral asymmetrical herpes-zoster with Ramsay hunt syndrome in an immunocompetent adult
Creators: name: Dai, Siqi
name: Huang, Xiaowen
name: Chen, Yuxiang
name: Wang, Menglei
name: Zheng, Huanxin
name: Zeng, Kang
name: Li, Li
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Additional file 1. Supplement 1. References for 40 cases in the Table 1.
Impact of secukinumab on patient-reported outcomes in biologic-naive patients with psoriasis in a US real-world setting
Creators: name: Strober, Bruce
name: Patil, Dhaval
name: McLean, Robert R.
name: Moore-Clingenpeel, Melissa
name: Guo, Ning
name: Levi, Eugenia
name: Lebwohl, Mark
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Science Policy
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: To describe real-world baseline characteristics and patient-reported outcomes (PROs) at 6-month and 12-month follow-up visits among patients with psoriasis who initiated and maintained secukinumab, stratified by prior exposure to biologics. This real-world study included patients enrolled in the CorEvitas (formerly Corrona) Psoriasis Registry who initiated and maintained secukinumab through 6-month and/or 12-month follow-up. Demographics, clinical characteristics, and PROs were collected. PROs included Dermatology Life Quality Index (DLQI); itch, skin pain, fatigue, and EuroQol visual analog scales; and Work Productivity and Activity Impairment. Mean (SD) differences between baseline and follow-up visits were calculated for all outcomes. Overall, 652 patients had a 6-month follow-up visit, 460 (70.6%) were biologic experienced and 192 (29.4%) were biologic naive. Biologic-experienced and biologic-naive patients reported mean (SD) improvements in all PROs measured at 6-month follow-up. Similar improvements were seen among patients with a 12-month follow-up visit (n = 390) and both 6-month and 12-month follow-up visits (n = 326). Biologic-experienced and biologic-naive patients with psoriasis who initiated and maintained secukinumab treatment reported improvements in PROs at 6-month and/or 12-month follow-up visits. These findings suggest that secukinumab is a potential biologic for psoriasis at any point along the patient treatment journey.
The Lense-Thirring timing-accretion plane for ULXs
Creators: name: Middleton, M.
name: Fragile, P. C.
name: Ingram, A.
name: Roberts, T. P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Identifying the compact object in ultraluminous X-ray sources (ULXs) has to-date required detection of pulsations or a cyclotron resonance scattering feature (CRSF), indicating a magnetised neutron star. However, pulsations are observed to be transient and it is plausible that accretion onto the neutron star may have suppressed the surface magnetic field such that pulsations and CRSFs will be entirely absent. We may therefore lack direct means to identify neutron star systems whilst we presently lack an effective means by which to identify black hole ULXs. Here we present a possible method for separating the ULX population by assuming the X-ray, mHz quasi-periodic oscillations (QPOs) and day timescale periods/QPOs are associated with Lense-Thirring precession of the inflow and outflowing wind respectively. The precession timescales combined with the temperature of the soft X-ray component produce planes where the accretor mass enters as a free parameter. Depending on the properties of the wind, use of these planes may be robust to a range in the angular momentum (spin) and, for high accretion rates, essentially independent of the neutron star's surface dipole field strength. Our model also predicts the mHz QPO frequency and magnitude of the phase-lag imprinted due to propagation through the optically thick wind; in the case of NGC 5408 X-1 we subsequently infer a black hole mass and high spin. Finally, we note that observing secular QPO evolution over sufficient baselines may indicate a neutron star, as the precession responds to spin-up which is not readily observable for black hole primaries.
description: 17 pages, accepted to MNRAS (updated, pre-epoof)
Additional file 1: of The impact of governance in primary health care delivery: a systems thinking approach with a European panel
Creators: name: Espinosa-GonzĂĄlez, Ana
name: Delaney, Brendan
name: Marti, Joachim
name: Darzi, Ara
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: List of variables and categories used in the study. (PDF 97 kb)
Gallup Poll # 704
Creators: name: Gallup
Publisher: name: Roper Center for Public Opinion Research
Year: 2021

description: Lyndon Johnson job performance (1); predictions for 1965 (5); intentions for 1965 (3); death penalty (2); Vietnam (20); establishing a government in Vietnam (1); outcome of Vietnam war (1); U.S. involvement in Vietnam (1); gun control (4); gun ownership (4); job satisfaction (3).
MPEC 2024-C164 : 2021 CM7
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Fano weighted complete intersections of large codimension
Creators: name: Przyjalkowski, Victor
name: Shramov, Constantin
Publisher: name: arXiv
Year: 2019
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics

description: We classify smooth Fano weighted complete intersections of large codimension.
description: 8 pages
Additional file 1: of Subgrouping patients with sciatica in primary care for matched care pathways: development of a subgrouping algorithm
Creators: name: Konstantinou, Kika
name: Dunn, Kate
name: Windt, Danielle
name: Ogollah, Reuben
name: Jasani, Vinay
name: Foster, Nadine
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Factors considered for their potential association with referral to spinal specialist services. (DOCX 24 kb)
Prävalenz von potenziellen Medikamenteninteraktionen und deren Einschätzung mithilfe verschiedener Interaktionssoftwares bei Patienten mit Multipler Sklerose
Creators: name: Bachmann, Paula
Publisher: name: Universität Rostock
Year: 2022
Subjects: subject: 610 Medical sciences Medicine

description: Die Multiple Sklerose (MS) ist eine immunmediierte, chronisch neurologische Erkrankung. Es war Gegenstand dieser Arbeit, die Prävalenz sowie Schwere von potentiellen Medikamenteninteraktionen und von Polypharmazie bei Patienten mit MS einzuschätzen und drei verschiedene, dafür verwendete Interaktionssoftwares zu vergleichen. Mithilfe der drei Interaktionssoftwares MediQ, Stockley’s und Drugs.com wurden in der vorliegenden Arbeit die Medikationsdaten von 627 Patienten mit MS auf pDDIs analysiert. .
Chodopsycha lobata
Creators: name: Ježek, Jan
name: Hájek, Josef
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psychodidae
Chodopsycha
Chodopsycha lobata

description: Chodopsycha lobata (Tonnoir, 1940)
 Published record. JEŽEK (1990a): Sedloňov.
 Unpublished records. Bartošovice v Orlických horách, Rašeliniště pod Předním vrchem peatbog [2], J, 14.- 24.ix.1993, J + H, YPT; Bedřichovka [4], J, 29.vii.-20.viii.1993, J, YPT; Bukačka NNR [7], J ♀, 16.-24.ix.1993 and 18.vii.-5.viii.1994, H + V, J + H, MT, YPT; Homole Mt. [32], ♀, 9.viii.1993, J; Rašeliniště Kačerov NR peatbog [42], 2 JJ ♀, 1.viii.1993, 26.v.-13.vi. and 18.vii.-8.viii.1994, H, H+ V, J, MT and sweeping; Kamenec, Strážný hill [44], J, 30.viii.1994, J; Karlův vrch hill (Lubný), Zdobnice river [45], ♀, 31.viii.1994, J; Klášterec nad Orlicí [46], ♀, 19.ix.1993, J; Kouty [50], 2 ♀♀, 29.vii.-20.viii. and 18.viii.1993, J, YPT and sweeping; 1 km NNE of Kunštátská kaple chapel [53], J, 20.viii.1993, J; Luisino Údolí [60], ♀, 14.viii.1993, J; Mezivrší [62], 2 ♀♀, 18.viii.1993, J; Mýto [67], ♀, 3.viii.1993, J; Nebeská Rybná [68], ♀, 1.viii.1993, J; Nepomuky [69], ♀, 12.vii.1981, J; Ruské údolí valley [96], ♀, 14.viii.1993, J; Říčka brook near Strašidelný mlýn mill [98], ♀, 20.viii.1993, J; Sedloňov [99], ♀, 3.viii.1993, J; Sedloňovský vrch Mt. [101], J, 14.viii.1993, J; Svinecký Dvůr [108], ♀, 19.vii.1996, J; Trčkov env., Velká louka NM meadow [118], ♀, 9.ix.1997, J; Trčkov NNR [119], 3 ♀♀, 16.-29.vi., 30.vi.-18.vii., 26.viii.- 15.ix.1994, H + V, H + V + J, MT; Vysoké Žibřidovice [128], ♀, 2.viii.1997, J; Zdobnice, Zdobnice river [132], ♀, 9.viii.1993, J; Zemská brána, Ledříčkova skála rock [136], J, 5.viii.1994, J; Zvonkové údolí valley, chapel [140], 2 ♀♀, 18.viii.1993, J.
 Vegetation. 1-3, 5-6, 8, 12, 14-15, 17-18, 20, 22-35, 40-41, 44-46, 49-53, 55-56, 59-63, 65, 67-68, 70-72, 74-76, 78-81, 83-84, 86-91, 94-96, 98-102; 110-111, 113-114, 117, 119, 121, 124-126, 128.
European and Transcaucasian species, common; for more information on its distribution see JEŽEK (2004b, 2006a).
description: Published as part of Ježek, Jan & Hájek, Josef, 2007, Psychodidae (Diptera) of the Orlické hory Protected Landscape Area and neighbouring areas with descriptions of two new species from the Czech Republic, pp. 237-285 in Acta Entomologica Musei Nationalis Pragae 47 on page 261, DOI: 10.5281/zenodo.5328353
Long-Term RXTE Monitoring of Anomalous X-ray Pulsars
Creators: name: Gavriil, Fotis P.
name: Kaspi, Victoria M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on the long-term monitoring of three anomalous X-ray pulsars using the Rossi X-ray Timing Explorer (RXTE). We present a phase-coherent timing ephemeris for 4U 0142+61, and show that it has rotated with high stability over 4.4 yr, with RMS phase deviations of 7% of the pulse period from a simple fit including only $ν$ and $\dotν$. We report on the continued timing stability of 1E 2259.1+586, for which phase coherence has now been maintained over 4.5 yr, as well as on the detection of a significant $\ddotν$ in 1.4 yr of monitoring of RXS J170849.0-400910, consistent with recovery following a glitch. We note a correlation in which timing stability in AXPs decreases with increasing $\dotν$. The timing stability of soft gamma repeaters in quiescence is consistent with this trend, given their large spin-down rates. This trend is similar to one seen in radio pulsars, suggesting a connection between the three populations. We find no large variability in pulse morphology as a function of time. We present high signal-to-noise ratio average pulse profiles for each AXP, and consider them as a function of energy. We find a variety of different behaviors, and consider possible trends in the data. We also find no large variations in pulsed flux, and set 1 $σ$ upper limits of ~20-30% of the mean. Assuming a constant pulsed fraction, either more than one of the AXPs are coincidentally in a much more quiescent state during our RXTE monitoring than in the past, or past claims of large flux variations are incorrect.
description: 32 pages, 11 figures, accepted in the Astrophysical Journal. Figures 1,2,7,8 have been modified. Slight modifications to text
Additional file 1: of Preoperative CT versus intraoperative hybrid DynaCT imaging for localization of small pulmonary nodules: a randomized controlled trial
Creators: name: Yin-Kai Chao
name: Kuang-Tse Pan
name: Chih-Tsung Wen
name: Hsin-Yueh Fang
name: Ming-Ju Hsieh
Publisher: name: figshare
Year: 2019
Subjects: Medicine
Science Policy

description: SPIRIT 2013 checklist: Recommended items to address in a clinical trial protocol and related documents*. (DOC 121 kb)
Additional file 1 of A clinical-radiomics nomogram for the preoperative prediction of lymph node metastasis in colorectal cancer
Creators: name: Li, Menglei
name: Zhang, Jing
name: Dan, Yibo
name: Yao, Yefeng
name: Dai, Weixing
name: Cai, Guoxiang
name: Yang, Guang
name: Tong, Tong
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer

description: Additional file 1. Additional material about the additional descriptions of the clinical features, model building and statistical for software and Table S1 (Performance of different parameters of model).
Readerielliopsidaceae Abdollahz. & Crous 2020
Creators: name: Haituk, Sukanya
name: Suwannarach, Nakarin
name: Hongsanan, Sinang
name: Senwanna, Chanokned
name: Cheewangkoon, Ratchadawan
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Fungi
Ascomycota
Dothideomycetes
Capnodiales
Readerielliopsidaceae

description: Key to genera of Readerielliopsidaceae
1. Produce a thin superficial network of dense, dark hyphae on leaves.................................................................................................2
- Produce hyphal mass, black, web-like colonies on leaves.................................................................................................................5
2. Pycnidia flask shaped or sub globose to pyriform, brown.................................................................................................................3
 - Pycnidia irregularly cylindrical, straight or flexuous, short or long........................................................................... Scolecoxyphium
 3. Conidia globose to clavate, non-septate..................................................................................................................... Readerielliopsis
- Conidia with septate...........................................................................................................................................................................4
 4. Conidia filiform, fusoid-ellipsoidal, with up to 15-septate......................................................................................... Phaeoxyphiella
 - Conidia oblong or ovoid, with 3–4 transverse septa..................................................................................................... Fumagospora
 5. Ascostromata with stalks, ascospore oblong to saccate, 3-septate, hyaline............................................................................. Scorias
 - Ascostromata without stalks, ascospore fusoid, 3-septate with a mucilaginous sheath, hyaline...................................... Alloscorias
description: Published as part of Haituk, Sukanya, Suwannarach, Nakarin, Hongsanan, Sinang, Senwanna, Chanokned & Cheewangkoon, Ratchadawan, 2021, New genus of epiphytic sooty mold: Alloscorias syngonii (Readerielliopsidaceae) from Thailand, pp. 271-282 in Phytotaxa 507 (4) on page 276, DOI: 10.11646/phytotaxa.507.4.1, http://zenodo.org/record/5425691
WASP-169, WASP-171, WASP-175 and WASP-182: three hot Jupiters and one bloated sub-Saturn mass planet discovered by WASP-south
Creators: name: Nielsen, L. D.
name: Bouchy, F.
name: Turner, O. D.
name: Anderson, D. R.
name: Barkaoui, K.
name: Benkhaldoun, Z.
name: Burdanov, A.
name: Cameron, A. Collier
name: Delrez, L.
name: Gillon, M.
name: Ducrot, E.
name: Hellier, C.
name: Jehin, E.
name: Lendl, M.
name: Maxted, P. F. L.
name: Pepe, F.
name: Pollacco, D.
name: Pozuelos, F. J.
name: Queloz, D.
name: Segransan, D.
name: Smalley, B.
name: Triaud, A. H. M. J.
name: Udry, S.
name: West, R. G.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present the discovery of four new giant planets from \WASP, three hot Jupiters and one bloated sub-Saturn mass planet; WASP-169b, WASP-171b, WASP-175b and WASP-182b. Besides the discovery photometry from \wasp\ we use radial velocity measurements from CORALIE and HARPS as well as follow-up photometry from EulerCam, TRAPPIST-North and -South and SPECULOOS. WASP-169b is a low density Jupiter ($M=0.561 \pm 0.061~\mathrm{M_{Jup}}, R=1.304^{+0.150}_{-0.073} ~\mathrm{R_{Jup}}$) orbiting a V=12.17 F8 sub-giant in a 5.611~day orbit. WASP-171b is a typical hot Jupiter ($M=1.084 \pm 0.094~\mathrm{M_{Jup}}, R=0.98^{+0.07}_{-0.04} ~\mathrm{R_{Jup}}$, $P=3.82~\mathrm{days}$) around a V=13.05 G0 star. We find a linear drift in the radial velocities of WASP-171 spanning 3.5 years, indicating the possibility of an additional outer planet or stellar companion. WASP-175b is an inflated hot Jupiter ($M=0.99 \pm 0.13~\mathrm{M_{Jup}}, R=1.208 \pm 0.081 ~\mathrm{R_{Jup}}$, $P=3.07~\mathrm{days}$) around a V=12.04 F7 star, which possibly is part of a binary system with a star 7.9\arcsec\ away. WASP-182b is a bloated sub-Saturn mass planet ($M=0.148 \pm 0.011~\mathrm{M_{Jup}}, R=0.850\pm 0.030 ~\mathrm{R_{Jup}}$) around a metal rich V=11.98 G5 star ([Fe/H]$=0.27 \pm 0.11$). With a orbital period of $P=3.377~\mathrm{days}$, it sits right in the apex of the sub-Jovian desert, bordering the upper- and lower edge of the desert in both the mass-period and radius-period plane. WASP-169b, WASP-175b and WASP-182b are promising targets for atmospheric characterisation through transmission spectroscopy, with expected transmission signals of 121, 150 and 264 ppm respectively.
description: Published in MNRAS Aug 23, 2019
Additional file 2: of Subgrouping patients with sciatica in primary care for matched care pathways: development of a subgrouping algorithm
Creators: name: Konstantinou, Kika
name: Dunn, Kate
name: Windt, Danielle
name: Ogollah, Reuben
name: Jasani, Vinay
name: Foster, Nadine
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology

description: STarT Back Tool. (DOC 40 kb)