cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The extreme chemistry of multiple stellar populations in the metal-poor globular cluster NGC 4833
Creators: name: Carretta, E.
name: Bragaglia, A.
name: Gratton, R. G.
name: D'Orazi, V.
name: Lucatello, S.
name: Momany, Y.
name: Sollima, A.
name: Bellazzini, M.
name: Catanzaro, G.
name: Leone, F.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Our FLAMES survey of Na-O anticorrelation in globular clusters (GCs) is extended to NGC 4833, a metal-poor GC with a long blue tail on the horizontal branch (HB). We present the abundance analysis for a large sample of 78 red giants based on UVES and GIRAFFE spectra acquired at the ESO-VLT. We derived abundances of Na, O, Mg, Al, Si, Ca, Sc, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, Y, Ba, La, Nd. This is the first extensive study of this cluster from high resolution spectroscopy. On the scale of our survey, the metallicity of NGC 4833 is [Fe/H]=-2.015+/-0.004+/-0.084 dex (rms=0.014 dex) from 12 stars observed with UVES, where the first error is from statistics and the second one refers to the systematic effects. The iron abundance in NGC 4833 is homogeneous at better than 6%. On the other hand, the light elements involved in proton-capture reactions at high temperature show the large star-to-star variations observed in almost all GCs studied so far. The Na-O anticorrelation in NGC 4833 is quite extended, as expected from the high temperatures reached by stars on the HB, and NGC 4833 contains a conspicuous fraction of stars with extreme [O/Na] ratios. More striking is the finding that large star-to-star variations are seen also for Mg, which spans a range of more than 0.5 dex in this GC. Depletions in Mg are correlated to the abundances of O and anti-correlated with Na, Al, and Si abundances. This pattern suggests the action of nuclear processing at unusually high temperatures, producing the extreme chemistry observed in the stellar generations of NGC 4833. This extreme changes are also seen in giants of the much more massive GCs M 54 and omega Cen, and our conclusion is that NGC 4833 has probably lost a conpicuous fraction of its original mass due to bulge shocking, as also indicated by its orbit.
description: 18 pages, 16 figures, 11 tables; accepted for publication on Astronomy and Astrophysics
Additional file 7 of The low-copy nuclear gene Agt1 as a novel DNA barcoding marker for Bromeliaceae
Creators: name: Bratzel, Fabian
name: Heller, Sascha
name: Cyrannek, Nadine
name: Paule, Juraj
name: Leme, Elton M. C.
name: Loreth, Anna
name: Nowotny, Annika
name: Kiefer, Markus
name: Till, Walter
name: Barfuss, Michael H. J.
name: Lexer, Christian
name: Koch, Marcus A.
name: Zizka, Georg
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 7. Supplementary_Material_S7_Agt1_genmodels_Acomosus_Athaliana.
Freezing and melting of vortex ice
Creators: name: Trastoy, J.
name: Malnou, M.
name: Ulysse, C.
name: Bernard, R.
name: Bergeal, N.
name: Faini, G.
name: Lesueur, J.
name: Briatico, J.
name: Villegas, Javier E.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We report on the realization of artificial ice using superconducting vortices in geometrically frustrated pinning arrays. This vortex ice shows two unique properties among artificial ice systems. The first comes from the possibility to switch the array geometric frustration on/off through temperature variations, which allows "freezing" and "melting" the vortex ice. The second is that the depinning and dynamics of the frozen vortex ice are insensitive to annealing, which implies that the ordered ground state is spontaneously approached. The major role of thermal fluctuations and the strong vortex-vortex interactions are at the origin of this unusual behavior.
Sapromyza trispina Rondani 1868
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Lauxaniidae
Sapromyza
Sapromyza trispina

description: Sapromyza trispina Rondani, 1868
ORIGINAL DESCRIPTION: 1868c: 235 (key), 241 (description).
TYPE LOCALITY: “ in montuosis agri parmensis [Parmese mountains (Italy)]”.
TYPE MATERIAL: 3 ♀♀, syntypes (one missing right fore-leg) (MZUF: Box 29): Sapromyza Fall. / trispina Rndn., Gall., Apenn. [= Apennines] / 1548.
CURRENT STATUS: junior synonym of Minettia tubifer (Meigen, 1826) (Papp 1984a: 202, Nartshuk et al. 1995: 5).
REMARKS: Rondani (1868c: 241) described Sapromyza trispina without specifying the number, the sex or the length of the specimens. We found three syntypes in this study.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 135, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Epidius ganxiensis Yin, Peng & Kim 1999, new combination
Creators: name: Tang, Guo
name: Yin, Changmin
name: Peng, Xianjin
name: Griswold, Charles
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Thomisidae
Epidius
Epidius ganxiensis

description: Epidius ganxiensis (Yin, Peng & Kim, 1999), new combination (Figs. 3 A–J, 7) Philodromus ganxiensis Yin, Peng & Kim, 1999: 356, Fig. 2 A–G (types in HNU, examined)  Material examined. – 2 males, 3 females (HNU), Ganxi Township, Tongdao County (26°03'N 109°17'E), Hunan Province, China, coll. C. Yin, X. Peng and Y. Zhang, 1 Jun.1996.  Description. – Male palp with a spatulate VTA and 6 macrosetae in a row at tibial apex, conductor transparent, twisted and concave at apex; embolus slender, apically hidden under the conductor. Epigyne with a pair of spatulate sclerotized plates posteriorly; copulatory openings slit like, copulatory ducts complexly twisted; spermathecae curved in n-shape.  Diagnosis. – This species can be separated from E. gongi (Song & Kim, 1992) by: the atrium slit-shaped laterally (pit like medially); the ratio of length of palpal tibia to palp = 1.2 (5.0 in E. gongi).  Distribution. – China (Hunan).  Remarks. – The species was firstly placed under the spider family Philodromidae. However, the male palp has a spatulate VTA and a row of macrosetae, which are the typical diagnostic characters of the genus Epidius of family Thomisidae. Philodromus ganxiensis Yin, Peng & Kim, 1999, should be transferred to the genus Epidius as E. ganxiensis (Yin, Peng & Kim, 1999), new combination.
description: Published as part of Tang, Guo, Yin, Changmin, Peng, Xianjin & Griswold, Charles, 2009, Six Crab Spiders Of The Subfamily Stephanopinae From Southeast Asia (Araneae: Thomisidae), pp. 39-50 in Raffles Bulletin of Zoology 57 (1) on page 44, DOI: 10.5281/zenodo.4508210
Signatures of very massive stars: supercollapsars and their cosmological rate
Creators: name: Maio, Umberto
name: Barkov, Maxim V.
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We compute the rate of supercollapsars by using cosmological, N-body, hydro, chemistry simulations of structure formation, following detailed stellar evolution according to proper yields (for He, C, N, O, Si, S, Fe, Mg, Ca, Ne, etc.) and lifetimes for stars having different masses and metallicities, and for different stellar populations (population III and population II-I). We find that supercollapsars are usually associated to dense, collapsing gas with little metal pollution and with abundances dominated by oxygen. The resulting supercollapsar rate is about $10^{-2}\,\rm yr^{-1} sr^{-1}$ at redshift $z=0$, and their contribution to the total rate is $ < 0.1 $ per cent, which explains why they have never been detected so far. Expected rates at redshift $z\simeq 6$ are of the order of $\sim 10^{-3}\,\rm yr^{-1} sr^{-1}$ and decrease further at higher $z$. Because of the strong metal enrichment by massive, short-lived stars, only $\sim 1$ supercollapsar generation is possible in the same star forming region. Given their sensitivity to the high-mass end of the primordial stellar mass function, they are suitable candidates to probe pristine population III star formation and stellar evolution at low metallicities.
description: 6 pages; accepted, MNRAS. "Apri la mente a quel ch'io ti paleso" (Par. V, 40)
Additional file 4 of Copy number gain of pro-inflammatory genes in patients with HBV-related acute-on-chronic liver failure
Creators: name: Fengming Sun
name: Wenting Tan
name: Yunjie Dan
name: Xiuhua Wang
name: Yanzhi Guo
name: Deng, Guohong
Publisher: name: figshare
Year: 2020
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: 60506 Virology

description: Additional file 4. Genes locating in the significant lost genomic regions (rare CNVs with the size of 100-200 kb).
Nighttime average and dipping blood pressure can differ based on the temporal distribution of ambulatory measurements at nighttime
Creators: name: Brito, Leandro C.
name: Bowles, Nicole P.
name: McHill, Andrew W.
name: Rice, Sean P.M.
name: Butler, Matthew P.
name: Rueda, Jose
name: Emens, Jonathan S.
name: Shea, Steven A.
name: Thosar, Saurabh S.
Publisher: name: Oregon Health and Science University
Year: 2023
Subjects: subject: Health Services
subject: Sleep
subject: Blood Pressure
subject: Cardiovascular System
subject: Heart, Lung, & Blood
subject: Nocturnal Dipping
subject: Nighttime Blood Pressure
subject: Blood Pressure Monitoring

description: Nighttime ambulatory (BP) and dipping% (nighttime/daytime BP of <0.9; non-dipping ≥0.9) are independent predictors of adverse cardiovascular events. Standard guidelines recommend at least ≥20/7 daytime/nighttime measurements for reliable ambulatory BP monitoring, but newer reports suggest ≥8/4 daytime/nighttime measurements are sufficient. Considering BP oscillates across the night, the temporal distribution of measurements across the night may impact nighttime BP and dipping%. To test whether this new recommendation holds for extreme examples of temporal distribution, we compared average nighttime BP and dipping% when using BP measurements only in the first (1st-half) vs. only in the second half (2nd-half) of the night.
From Voids to Coma: the prevalence of pre-processing in the local Universe
Creators: name: Cybulski, Ryan
name: Yun, Min S.
name: Fazio, Giovanni G.
name: Gutermuth, Robert A.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We examine the effects of pre-processing across the Coma Supercluster, including 3505 galaxies over 500 sq deg, by quantifying the degree to which star-forming (SF) activity is quenched as a function of environment. We characterise environment using the complementary techniques of Voronoi Tessellation, to measure the density field, and the Minimal Spanning Tree, to define continuous structures, and so we measure SF activity as a function of local density and the type of environment (cluster, group, filament, and void), and quantify the degree to which environment contributes to quenching of SF activity. Our sample covers over two orders of magnitude in stellar mass (10^8.5 to 10^11 Msun), and consequently we trace the effects of environment on SF activity for dwarf and massive galaxies, distinguishing so-called "mass quenching" from "environment quenching". Environmentally-driven quenching of SF activity, measured relative to the void galaxies, occurs to progressively greater degrees in filaments, groups, and clusters, and this trend holds for dwarf and massive galaxies alike. A similar trend is found using g-r colours, but with a more significant disparity between galaxy mass bins driven by increased internal dust extinction in massive galaxies. The SFR distributions of massive SF galaxies have no significant environmental dependence, but the distributions for dwarf SF galaxies are found to be statistically distinct in most environments. Pre-processing plays a significant role at low redshift, as environmentally-driven galaxy evolution affects nearly half of the galaxies in the group environment, and a significant fraction of the galaxies in the more diffuse filaments. Our study underscores the need for sensitivity to dwarf galaxies to separate mass-driven from environmentally-driven effects, and the use of unbiased tracers of SF activity.
description: 23 pages, 17 figures. Accepted to MNRAS. Version with higher-resolution figures available here: https://www.dropbox.com/s/p45wnkl4z2da97p/paper_coma_final.pdf
Default Sensitivity
Creators: name: Lee, David
Publisher: name: Zenodo
Year: 2022
Subjects: Default Sensitivity

description: The default sensitivity test in Scenario Manager is implemented by setting the default time of the perturbed obligor to be the valuation date when the present value of each tranche is calculated, no matter when that obligor defaults in the generated Monte Carlo scenarios. Compared with other models, the implementation of Scenario Manager model is simple, direct, and efficient. However, the joint default events generated in the MC scenarios remain unchanged, which is an approximation of the realistic situation.
description: https://ia601506.us.archive.org/32/items/abs-analytics/AbsAnalytics.pdf
HAL-NeRF: High Accuracy Localization Leveraging Neural Radiance Fields
Creators: name: Reppas, Asterios
name: Cheimariotis, Grigorios-Aris
name: Papadopoulos, Panos K.
name: Frasiolas, Panagiotis
name: Zarpalas, Dimitrios
Publisher: name: arXiv
Year: 2025
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Precise camera localization is a critical task in XR applications and robotics. Using only the camera captures as input to a system is an inexpensive option that enables localization in large indoor and outdoor environments, but it presents challenges in achieving high accuracy. Specifically, camera relocalization methods, such as Absolute Pose Regression (APR), can localize cameras with a median translation error of more than $0.5m$ in outdoor scenes. This paper presents HAL-NeRF, a high-accuracy localization method that combines a CNN pose regressor with a refinement module based on a Monte Carlo particle filter. The Nerfacto model, an implementation of Neural Radiance Fields (NeRFs), is used to augment the data for training the pose regressor and to measure photometric loss in the particle filter refinement module. HAL-NeRF leverages Nerfacto's ability to synthesize high-quality novel views, significantly improving the performance of the localization pipeline. HAL-NeRF achieves state-of-the-art results that are conventionally measured as the average of the median per scene errors. The translation error was $0.025m$ and the rotation error was $0.59$ degrees and 0.04m and 0.58 degrees on the 7-Scenes dataset and Cambridge Landmarks datasets respectively, with the trade-off of increased computational time. This work highlights the potential of combining APR with NeRF-based refinement techniques to advance monocular camera relocalization accuracy.
description: 8 pages, 4 figures
Stellar mass -- halo mass relation and star formation efficiency in high-mass halos
Creators: name: Kravtsov, Andrey
name: Vikhlinin, Alexey
name: Meshscheryakov, Alexander
Publisher: name: arXiv
Year: 2014
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study relation between stellar mass and halo mass for high-mass halos using a sample of galaxy clusters with accurate measurements of stellar masses from optical and IR data and total masses from X-ray observations. We find that stellar mass of the brightest cluster galaxies (BCGs) scales as M*BCG\propto M500^a_BCG with the best fit slope of a_BCG~0.35+-0.1 and scatter of M*BCG at a fixed M500 of ~0.2 dex. We show that M*-M relations from abundance matching or halo modelling reported in recent studies underestimate stellar masses of BCGs by a factor of ~2-4, because these studies used stellar mass functions (SMF) based on photometry that severely underestimates the outer surface brightness profiles of massive galaxies. We show that M*-M relation derived using abundance matching with the recent SMF calibration by Bernardi et al. (2013) based on improved photometry is in a much better agreement with the relation we derive. The total stellar mass of galaxies correlates with total mass M500 with the slope of \approx 0.6+-0.1 and scatter of 0.1 dex. This indicates that efficiency with which baryons are converted into stars decreases with increasing cluster mass. We show that for a fixed choice of the initial mass function (IMF) total stellar fraction in clusters is only a factor of ~3-5 lower than the peak stellar fraction reached in M\approx 10^12 Msun halos, and only a factor of ~1.5-3 if the IMF becomes progressively more bottom heavy with increasing mass in early type galaxies, as indicated by recent observations. The larger normalization and slope of the M*-M relation derived in this study shows that the overall efficiency of star formation in massive halos is suppressed much less than was thought before and that feedback and associated suppression of star formation in massive halos should be weaker than assumed in most of the current semi-analytic models and simulations.
description: 21 pages, 17 figures, submitted to the Astrophysical Journal
Additional file 7 of Copy number gain of pro-inflammatory genes in patients with HBV-related acute-on-chronic liver failure
Creators: name: Fengming Sun
name: Wenting Tan
name: Yunjie Dan
name: Xiuhua Wang
name: Yanzhi Guo
name: Deng, Guohong
Publisher: name: figshare
Year: 2020
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: 60506 Virology

description: Additional file 7. Prediction of potential sponging microRNAs between HCG4B and 3’UTR of HLA-A.
Gravitational phase transitions with an exclusion constraint in position space
Creators: name: Chavanis, Pierre-Henri
Publisher: name: arXiv
Year: 2013
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We discuss the statistical mechanics of a system of self-gravitating particles with an exclusion constraint in position space in a space of dimension $d$. The exclusion constraint puts an upper bound on the density of the system and can stabilize it against gravitational collapse. We plot the caloric curves giving the temperature as a function of the energy and investigate the nature of phase transitions as a function of the size of the system and of the dimension of space in both microcanonical and canonical ensembles. We consider stable and metastable states and emphasize the importance of the latter for systems with long-range interactions. For $d\le 2$, there is no phase transition. For $d>2$, phase transitions can take place between a "gaseous" phase unaffected by the exclusion constraint and a "condensed" phase dominated by this constraint. The condensed configurations have a core-halo structure made of a "rocky core" surrounded by an "atmosphere", similar to a giant gaseous planet. For large systems there exist microcanonical and canonical first order phase transitions. For intermediate systems, only canonical first order phase transitions are present. For small systems there is no phase transition at all. As a result, the phase diagram exhibits two critical points, one in each ensemble. There also exist a region of negative specific heats and a situation of ensemble inequivalence for sufficiently large systems. By a proper interpretation of the parameters, our results have application for the chemotaxis of bacterial populations in biology described by a generalized Keller-Segel model including an exclusion constraint in position space. They also describe colloids at a fluid interface driven by attractive capillary interactions when there is an excluded volume around the particles. Connexions with two-dimensional turbulence are also mentioned.
Mesembrina mystacea Rondani 1862
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Mesembrina
Mesembrina mystacea

description: [Mesembrina mystacea] Rondani, 1862d: 210.
REMARKS: name that Rondani (1862d: 210) proposed as a synonym of Mesembrina matutina Rondani, 1862 (from one specimen labeled “ mystacea Macq. ” received from Macquart) and not made available by use as a valid species before 1961. O’Hara et al. (2011: 210) considered this name as unavailable.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 163, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Additional file 5 of Copy number gain of pro-inflammatory genes in patients with HBV-related acute-on-chronic liver failure
Creators: name: Fengming Sun
name: Wenting Tan
name: Yunjie Dan
name: Xiuhua Wang
name: Yanzhi Guo
name: Deng, Guohong
Publisher: name: figshare
Year: 2020
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: 60506 Virology

description: Additional file 5. Key deleted genes in leukocyte transendothelial migration pathway.
Bürger von Frankfurt! Die bedauerlichen Vorfälle, welche vorgestern Abends hier stattgefunden haben, und die durch zahlreiche Zuzüge von Aussen herbeigeführte Bedrohung der Ruhe und Ordnung haben den Senat der freien Stadt Frankfurt veranlaßt, das Reichsministerium aufzufordern, daß es unmittelbar die Pflicht, die Nationalversammlung vor äußerer Gewalt zu schützen, zu erfüllen übernehme. ...; [1848]
Creators: name: Schmerling, Anton von
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: Kopftitel
Universal attractor in a highly occupied non-Abelian plasma
Creators: name: Berges, Juergen
name: Boguslavski, Kirill
name: Schlichting, Soeren
name: Venugopalan, Raju
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We study the thermalization process in highly occupied non-Abelian plasmas at weak coupling. The non-equilibrium dynamics of such systems is classical in nature and can be simulated with real-time lattice gauge theory techniques. We provide a detailed discussion of this framework and elaborate on the results reported in~\cite{Berges:2013eia} along with novel findings. We demonstrate the emergence of universal attractor solutions, which govern the non-equilibrium evolution on large time scales both for non-expanding and expanding non-Abelian plasmas. The turbulent attractor for a non-expanding plasma drives the system close to thermal equilibrium on a time scale $t\sim Q^{-1} α_s^{-7/4}$. The attractor solution for an expanding non-Abelian plasma leads to a strongly interacting albeit highly anisotropic system at the transition to the low-occupancy or quantum regime. This evolution in the classical regime is, within the uncertainties of our simulations, consistent with the ``bottom up'' thermalization scenario~\cite{Baier:2000sb}. While the focus of this paper is to understand the non-equilibrium dynamics in weak coupling asymptotics, we also discuss the relevance of our results for larger couplings in the early time dynamics of heavy ion collision experiments.
description: 49 pages, 21 figures
Hochsensible Kinder und ihre Bedürfnisse in der Tagesschule
Creators: name: Blättler, Veronica
Publisher: name: Zenodo
Year: 2022
Subjects: Sonderpädagogik
Masterarbeit
Hochsensibilität
Tagesschule

description: Laut Studien sind 15 bis 30 Prozent der Kinder hochsensibel. Pro Klasse sind das je nach Schätzungen 3 bis 6 Schüler*innen, die Reize intensiver aufnehmen und verarbeiten. Die Stadt Zürich plant mit dem Projekt «Tagesschule 2025» in den nächsten Jahren alle Schulen der Stadt als Tagesschulen zu führen. Die vorliegende Masterarbeit geht deshalb den Fragen nach, wie Tagesschulen auf die Bedürfnisse hochsensibler Kinder eingehen können und welche Handlungsmöglichkeiten für das Schulteam bestehen. Nach einer Erörterung der Theorie folgt eine qualitative Auswertung von vier Experteninterviews. Die Ergebnisse werden diskutiert und anhand von Empfehlungen für Tagesschulen zusammengefasst. Die Arbeit zeigt, dass eine «hochsensible» Tagesschule auf drei zentrale Bedürfnisse eingehen muss: Rückzugsmöglichkeiten, verlässliche Beziehungen und Strukturen. Die Rücksichtnahme auf diese Bedürfnisse kommt letztlich allen Kindern zugute.
Additional file 6 of Copy number gain of pro-inflammatory genes in patients with HBV-related acute-on-chronic liver failure
Creators: name: Fengming Sun
name: Wenting Tan
name: Yunjie Dan
name: Xiuhua Wang
name: Yanzhi Guo
name: Deng, Guohong
Publisher: name: figshare
Year: 2020
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: 60506 Virology

description: Additional file 6. Genes locating in the significant gained genomic regions (rare CNVs with the size of 100-200 kb).
Poligenia luteiventris Rondani 1868
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Poligenia
Poligenia luteiventris

description: [Poligenia luteiventris] Morge, 1959b: 90.
REMARKS: nomen nudum; Morge (1959b: 90) listed an unpublished Rondani name. O’Hara et al. (2011: 199) consider the genus name as unavailable.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 163, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Evaluation of spectral induced polarization field measurements in time and frequency domain
Creators: name: Martin, Tina
name: Günther, Thomas
name: Orozco, Adrian Flores
name: Dahlin, Torleif
Publisher: name: Amsterdam [u.a.] : Elsevier Science
Year: 2020
Subjects: subject: Comparison
subject: Frequency domain IP (FDIP)
subject: Graptolite shale
subject: Induced polarization (IP)
subject: Spectral bandwidth
subject: Time domain IP (TDIP)
subject: 620
subject: 660
subject: 550

description: Spectral induced polarization (SIP) measurements have been demonstrated to correlate with important parameters in hydrogeological and environmental investigations. Although SIP measurements were often collected in the frequency domain (FDIP), recent developments have demonstrated the capabilities to solve for the frequency-dependence of the complex conductivity through measurements collected in the time domain (TDIP). Therefore, the aim of our field investigations is a comparison of the measured frequency-dependence at a broad frequency range resolved through FDIP and TDIP. In contrast to previous studies, we conducted measurements with different instruments and measuring technologies for both FDIP and TDIP. This allows for investigating the robustness of different measurements and assessing various sources of errors, for the assessment of the advantages and drawbacks from different measuring techniques. Our results demonstrate that data collected through different instruments are consistent. Apparent resistivity measurements as well as the inversion results revealed quantitatively the same values for all instruments. The measurements of the IP effect are also comparable, particularly FDIP readings in the low frequencies (< 10 Hz) revealed to be quantitatively the same for different instruments. TDIP measurements are consistent for data collected with both devices. As expected, the spatial distribution of the values is also consistent for low frequency data (in FDIP) and late times measurements in TDIP (> 0.1 s). However, data quality for higher frequencies in FDIP (i.e., early times in TDIP) show larger variations, which reflects the differences between the instruments to deal with the electromagnetic contamination of the IP data. Concluded in general, the different instruments and measuring techniques can provide consistent responses for varying signal-to-noise ratio and measuring configurations. © 2020 The Authors
Power of poetry
Creators: name: Brown, Audrey Alexandra, 1904-1998
Publisher: name: University of Victoria Libraries
Year: 2020
Subjects: subject: Canadian poetry
valueUri: http://id.worldcat.org/fast/845173
subject: Authors, Canadian
valueUri: http://id.worldcat.org/fast/821870
subject: Brown, Audrey Alexandra, 1904-1998
valueUri: http://id.worldcat.org/fast/409826
subject: Canadian literature
valueUri: http://id.worldcat.org/fast/845111

description: An address given by Brown at a 1951 Canadian Author's Association Convention in Banff. Published in Canadian author& bookman, v. 27, no. 3-4, winter 1951. p. 14-15
Simulation of a two-dimensional shot in a closed contour with dispersers in the center
Creators: name: Sabogal, Miguel
Publisher: name: Zenodo
Year: 2018

description: It was simulated the bidimensional launching of a particle of mass m in a closed circular environment, with four equal dispersers located in the center, using the computational language of phyton and the runge kutta of order 4, to describe the trajectory of the particle from the initial conditions ( vecro, vecvo). Then, using the Lyapunov coefficients, it was observed that the system presents chaos, and the chaotic region was observed for a set of specific parameters. It was also shown that the degree of dispersion of the particles depends on the impact parameter and of the initial energy of launching, and in a similar way the effective section was determined, from the distribution of impact on the contour of the circular region.
description: College project
Galaxy and Mass Assembly (GAMA): Fine filaments of galaxies detected within voids
Creators: name: Alpaslan, Mehmet
name: Robotham, Aaron S. G.
name: Obreschkow, Danail
name: Penny, Samantha
name: Driver, Simon
name: Norberg, Peder
name: Brough, Sarah
name: Brown, Michael
name: Cluver, Michelle
name: Holwerda, Benne
name: Hopkins, Andrew M.
name: van Kampen, Eelco
name: Kelvin, Lee S.
name: Lara-Lopez, Maritza A.
name: Liske, Jochen
name: Loveday, Jon
name: Mahajan, Smriti
name: Pimbblet, Kevin
Publisher: name: arXiv
Year: 2014
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Based on data from the Galaxy and Mass Assembly (GAMA) survey, we report on the discovery of structures that we refer to as `tendrils' of galaxies: coherent, thin chains of galaxies that are rooted in filaments and terminate in neighbouring filaments or voids. On average, tendrils contain 6 galaxies and span 10 $h^{-1}$ Mpc. We use the so-called line correlation function to prove that tendrils represent real structures rather than accidental alignments. We show that voids found in the SDSS-DR7 survey that overlap with GAMA regions contain a large number of galaxies, primarily belonging to tendrils. This implies that void sizes are strongly dependent on the number density and sensitivity limits of a survey. We caution that galaxies in low density regions, that may be defined as `void galaxies,' will have local galaxy number densities that depend on such observational limits and are likely higher than can be directly measured.
description: 6 pages, 3 figures, accepted for publication in MNRAS Letters on Tue 28 Jan 2014
Mythicomyiidae
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Mythicomyiidae

description: Mythicomyiidae
This family, proposed by Melander in 1902, contains 421 predominantly Nearctic and Palaearctic species (Evenhuis & Pape 2020) and is considered to be the sister group of Bombyliidae (Marshall 2012). Zaitzev (1989) and Pape et al. (2011) considered it as a subfamily of Bombyliidae. Rondani (1863) described two Palaearctic species in Mythicomyiidae, both considered as valid (Zaitzev 1989, Contini et al. 1995, Evenhuis 2002). The type material was not found in this study and is presumed lost.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 165, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Zwischen individueller Förderung und gemeinsamen Lernsituationen. Entwicklung eines Kapitels für einen heilpädagogischen Kommentar zum Lehrmittel Mathematik 5 Primarstufe zum Thema Proportionalität
Creators: name: Feusi, Noemi
Publisher: name: Zenodo
Year: 2022
Subjects: Sonderpädagogik
Masterarbeit
individuelle Förderung
gemeinsame Lernsituation

description: Im Schulalltag stellen die Mathematiklektionen die Klassenlehrer*innen vor eine grosse Herausforderung, da die Wissensstände der einzelnen Schüler*innen innerhalb einer Klasse sehr heterogen sind. Obwohl Schüler*innen mit besonderem Förderbedarf auf individualisierte Förderung angewiesen sind, darf nicht vergessen werden, dass gemeinsame Lernsituationen vor allem für Schüler*innen mit besonderem Förderbedarf von grosser Bedeutung sind. Das Ziel dieser Arbeit ist es, das Thema «Proportionalität» des Lehrmittels Mathematik 5 Primarstufe so aufzubereiten, dass allen Schüler*innen ein zieldifferentes Lernen am gemeinsamen Gegenstand ermöglicht wird. Um den Entwicklungserfolg zu messen, wird in zwei fünften Klassen ein Quasi-Experiment durchgeführt, welches durch eine teilnehmende Feldbeobachtung und ein qualitatives Interview mit einer Schülerin mit besonderem Förderbedarf ergänzt wird. Methodisch wird das erhaltene Datenmaterial mit Hilfe eines inhaltsanalytischen Kategoriensystems qualitativ analysiert. In dieser Arbeit wird aufgezeigt, mit welchen Differenzierungsansätzen eine hohe Passung zwischen den Anforderungen im Unterricht und dem Leistungsvermögen der Schüler*innen erreicht werden kann, wodurch es allen Schüler*innen möglich ist, im Unterricht zu partizipieren.
Persistent spin currents in an elastic Landau system
Creators: name: Bakke, K.
name: Furtado, C.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We consider a neutral particle with permanent magnetic dipole moment in an elastic medium with the presence of a uniform distribution of screw dislocations interacting with a radial electric field. We show that the uniform distribution of dislocations plays the role of an effective uniform magnetic field, and obtain a spectrum of energy which depends on the Aharonov-Casher geometric phase [Y. Aharonov and A. Casher, Phys. Rev. Lett. 53, 319 (1984)]. Moreover, from the dependence of energy levels on the Aharonov-Casher geometric phase, we calculate the persistent spin currents in this elastic Landau system.
title: Neueste ausführliche Prager Revolutions-Geschichte und der Aufstand der böhmischen Sensenmänner; [1848]
title: 1. Warum rebelliren die Böhmen? 2. Kriegserklärung der Slaven gegen Ungarn. 3. Verrath des Gouverneur Graf Thun. 4. 700 böhmische Amazonen. 5. Alleneueste Berichte aus der Umgebung
titleType: Subtitle
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: Kopftitel
Photometric classification of emission line galaxies with Machine Learning methods
Creators: name: Cavuoti, Stefano
name: Brescia, Massimo
name: D'Abrusco, Raffaele
name: Longo, Giuseppe
name: Paolillo, Maurizio
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In this paper we discuss an application of machine learning based methods to the identification of candidate AGN from optical survey data and to the automatic classification of AGNs in broad classes. We applied four different machine learning algorithms, namely the Multi Layer Perceptron (MLP), trained respectively with the Conjugate Gradient, Scaled Conjugate Gradient and Quasi Newton learning rules, and the Support Vector Machines (SVM), to tackle the problem of the classification of emission line galaxies in different classes, mainly AGNs vs non-AGNs, obtained using optical photometry in place of the diagnostics based on line intensity ratios which are classically used in the literature. Using the same photometric features we discuss also the behavior of the classifiers on finer AGN classification tasks, namely Seyfert I vs Seyfert II and Seyfert vs LINER. Furthermore we describe the algorithms employed, the samples of spectroscopically classified galaxies used to train the algorithms, the procedure followed to select the photometric parameters and the performances of our methods in terms of multiple statistical indicators. The results of the experiments show that the application of self adaptive data mining algorithms trained on spectroscopic data sets and applied to carefully chosen photometric parameters represents a viable alternative to the classical methods that employ time-consuming spectroscopic observations.
description: 10 pages, 1 figure, accepted by MNRAS in October 10, 2013
Additional file 1 of The impact of social insurance on health among middle-aged and older adults in rural China: a longitudinal study using a three-wave nationwide survey
Creators: name: Xinxin Ma
name: Oshio, Takashi
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy

description: Additional file 1.
Phora picta Lehmann 1822
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Phoridae
Phora
Phora picta

description: [Phora picta] Morge, 1959b: 91.
REMARKS: nomen nudum; Morge (1959b: 91) listed an unpublished Rondani name.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 172, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Early X-ray emission from Type Ia supernovae originating from symbiotic progenitors or recurrent novae
Creators: name: Dimitriadis, Georgios
name: Chiotellis, Alexandros
name: Vink, Jacco
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: One of the key observables for determining the progenitor nature of Type Ia supernovae is provided by their immediate circumstellar medium, which according to several models should be shaped by the progenitor binary system. So far, X-ray and radio observations indicate that the surroundings are very tenuous, producing severe upper-limits on the mass loss from winds of the progenitors. In this study, we perform numerical hydro-dynamical simulations of the interaction of the SN ejecta with circumstellar structures formed by possible mass outflows from the progenitor systems and we estimate numerically the expected numerical X-ray luminosity. We consider two kinds of circumstellar structures: a) A circumstellar medium formed by the donor star's stellar wind, in case of a symbiotic binary progenitor system; b) A circumstellar medium shaped by the interaction of the slow wind of the donor star with consecutive nova outbursts for the case of a symbiotic recurrent nova progenitor system. For the hydro-simulations we used well-known Type Ia supernova explosion models, as well as an approximation based on a power law model for the density structure of the outer ejecta. We confirm the strict upper limits on stellar wind mass loss, provided by simplified interpretations of X-ray upper limits of Type Ia supernovae. However, we show that supernova explosions going off in the cavities created by repeated nova explosions, provide a possible explanation for the lack of X-ray emission from supernovae originating from symbiotic binaries. Moreover, the velocity structure of circumstellar medium, shaped by a series of nova explosion matches well with the Na absorption features seen in absorption toward several Type Ia supernovae.
description: 11 pages, 12 figures, submitted to MNRAS
Alltagsintegrierte Sprachförderung für den Zweitspracherwerb im Zyklus 1. Ein Leitfaden für pädagogische Fachkräfte mit Praxistipps für die alltagsintegrierte Sprachförderung abgeleitet von einer systematischen Literaturanalyse
Creators: name: Hess, Claudia
name: Zürcher, Evelyne
Publisher: name: Zenodo
Year: 2022
Subjects: Sonderpädagogik
Masterarbeit
Sprachförderung
Zyklus 1
Zweitspracherwerb

description: Sprache wird als Schlüssel zur Integration und Teilhabe angesehen. Für Kinder mit Deutsch als Zweitsprache ist es wichtig, die deutsche Sprache möglichst schnell zu erlernen und zu beherrschen, um Bildungsgerechtigkeit zu erleben. Die alltagsintegrierte Sprachförderung hat erwiesenermassen einen positiven Einfluss auf die gesamte Sprachentwicklung eines Kindes. Vor diesem Hintergrund befasst sich diese Masterarbeit mit der Frage, wie pädagogische Fachkräfte alltagsintegrierte Sprachförderung für Zweitsprachlernende im Zyklus 1 positiv beeinflussen können. Die vorliegende Entwicklungsarbeit basiert auf einer systematischen Literaturanalyse. Die Ergebnisse zeigen auf, dass alltagsintegrierte Sprachförderung in der Praxis zu wenig stattfindet. Ein Grund dafür kann fehlendes Fachwissen der pädagogischen Fachkräfte sein. Ausgehend von dieser Hypothese wird ein Weiterbildungsbedarf abgeleitet. Das Produkt dieser Masterarbeit ist ein Leitfaden mit Praxistipps für pädagogische Fachkräfte. Er dient der alltagsintegrierten Sprachförderung mehrsprachiger Kinder und kann deshalb als Schlüssel zur Integration und Teilhabe betrachtet werden.
title: Behavior of branched buried MDPE gas distribution pipes under relative axial ground movements
Creators: name: Chakraborty, Sudipta
Publisher: name: Memorial University of Newfoundland
Year: 2022

description: The performance of medium density polyethylene (MDPE) gas distribution pipes subjected to relative ground movements has been a significant concern to the utility owners and companies. The tee-joints (tapping tee) and the lateral branches, common in gas distribution piping systems, may increase the effects of ground movement caused by various geohazards such as landslides, earthquakes etc. Most ground movement scenarios depict leak/stress concentration near the tapping tee of the branched pipe system. However, limited studies are currently available in the literature on the soil-pipe interaction of branched pipes during ground movement. Thus, the complex interactions of the pipe, the tee-junction, and the branch with surrounding soil are not well-understood. This thesis presents an experimental investigation of different configurations of 42.2-mm and 60.3-mm diameter branched buried MDPE pipes under relative axial ground movement. Tests with different positions of the tee-joint with respect to the pulling end of the pipe and varying densities of sand are conducted using the laboratory facility at Memorial University of Newfoundland. Pipe wall strains and soil pressures around the pipes are measured during the tests to capture the mechanism of soil-pipe interaction. Subsequently, an additional test is done with the tapping tee only (without the branch pipe) to identify the contribution of the branch pipe to soil resistance and pipe wall strain. The study explores the contribution of the trunk pipe, the tapping tee, and the branch pipe separately on the axial pulling force. Test results reveal the possibility of localized strain occurring on the trunk pipe near the tee. The anchoring effects of the tee and the branch significantly affect the soil resistance and the strain distribution on the trunk pipes.
Shared decision making in rheumatoid arthritis: study protocol for a stepped wedge, cluster-randomized trial
Creators: name: Barton, Jennifer L.
name: Kunneman, Marleen
name: Matsumoto, Rachel
name: Larsen, Chris
name: Hughes, Arielle
name: Schmajuk, Gabriela
name: Baker, Joshua
name: Lovejoy, Travis
name: Scholl, Isabelle
Publisher: name: Oregon Health and Science University
Year: 2023
Subjects: subject: Health Services
subject: Arthritis, Rheumatoid
subject: Decision Making, Shared
subject: Communication
subject: Study Protocol
subject: Rheumatology
subject: Patient Education
subject: Clinical Decision-Making
subject: Decision Aids
subject: Patient Participation
subject: Physician-Patient Relations

description: Rheumatoid arthritis (RA) impacts quality of life causing disability and increased mortality. Treatment decisions are complex and require individualized decisions. Shared decision making (SDM) is the first principle of RA treat-to-target guidelines but uptake is suboptimal. We aim to evaluate the effectiveness of a multicomponent SDM intervention on RA disease activity and explore the early implementation of the intervention within three geographically diverse rheumatology services.
Twist-two operators and the BFKL regime - nonstandard solutions of the Baxter equation
Creators: name: Janik, Romuald A.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The link between BFKL physics and twist-two operators involves an analytical continuation in the spin of the operators away from the physical even integer values. Typically this is done only after obtaining an analytical result for integer spin through nested harmonic sums. In this paper we propose analyticity conditions for the solution of Baxter equation which would work directly for any value of complex spin and reproduce results from the analytical continuation of harmonic sums. We carry out explicit contructions up to 2-loop level. These nonstandard solutions of the Baxter equation have rather surprising asymptotics. We hope that these analyticity conditions may be used for incorporating them into the exact TBA/FiNLIE/QSC approaches valid at any coupling.
description: 22 pages, 1 figure, Mathematica notebook with numerical checks included in the source submission