cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1 of Addition of chemoradiotherapy to palliative chemotherapy in de novo metastatic nasopharyngeal carcinoma: a real-world study
Creators: name: Zheng, Shuo-Han
name: Wang, Yu-Tong
name: Liu, Song-Ran
name: Huang, Zi-Lu
name: Wang, Guan-Nan
name: Lin, Jin-Tao
name: Ding, Shi-Rong
name: Chen, Chen
name: Xia, Yun-Fei
Publisher: name: figshare
Year: 2022
Subjects: Medicine
Biotechnology
Cancer
Hematology

description: Additional file 1: Description of the radiotherapy. Figure S1. Patient selection diagram. Figure S2. Overall Survival (OS) for patients treated with chemoradiotherapy (CRT) or palliative chemotherapy (PCT) in de novo metastatic nasopharyngeal carcinoma. Table S1. Details of common chemotherapy regimens. Table S2. Summary of studies related to locoregional radiotherapy in de novo metastatic nasopharyngeal carcinoma. Table S3. Adverse effects. References.
MOESM2 of Withaferin A ameliorates ovarian cancer-induced cachexia and proinflammatory signaling
Creators: name: Straughn, Alex
name: Kakar, Sham
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer

description: Additional file 2: Table S2. Primary and secondary antibody list.
MOESM1 of Withaferin A ameliorates ovarian cancer-induced cachexia and proinflammatory signaling
Creators: name: Straughn, Alex
name: Kakar, Sham
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: Pharmacology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: 60506 Virology

description: Additional file 1: Table S1. Human and mouse gene specific primer sequences.
Dirty Fireballs and Orphan Afterglows: A Tale of Two Transients
Creators: name: Rhoads, James E.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Orphan afterglows are transient events that are produced by cosmological fireballs and resemble gamma ray burst (GRB) afterglows, yet are not accompanied by gamma rays. Such transients may be produced by jetlike GRBs observed off-axis, and therefore hold great promise as a test of gamma ray burst collimation. However, orphans may also be produced by "dirty fireballs," i.e., cosmological fireballs whose ejecta carry too many baryons to produce a GRB. A well designed orphan afterglow search can distinguish between on-axis dirty fireballs and off-axis orphans in at least two ways. First, by combining real-time triggers from a wide area, multicolor search with deeper followup observations, the light curve can be tracked for a time exceeding 2*t_1, where t_1 is the age of the event at first observation. Such a light curve allows simultaneous fits to t_1 and the time decay slope alpha with sufficient accuracy to distinguish on- and off-axis orphans. Second, radio followup of orphan afterglows will show whether the radio flux is falling in time (as expected for an off-axis orphan) or not (as expected for on-axis events). Additional tests involving multi-band monitoring of the cooling, self-absorption, and f_nu peak frequencies are also possible, although much more observationally demanding. A further complication in orphan searches is that dirty fireballs are likely to also be collimated, and that collimated dirty fireballs viewed off-axis will individually be practically indistinguishable from off-axis GRB afterglows. To recognize their presence, orphan afterglow surveys must be sufficiently extensive to catch at least some dirty fireballs on-axis.
description: 17 pages, 4 figures, accepted for publication in The Astrophysical Journal (April 2003)
Physiotherapy interventions to improve mobility outcomes in adults with moderate to severe traumatic brain injury: a scoping review protocol
Creators: name: Gilfillan, Izel
name: Mothabeng, Diphale
name: van Heerden, Annelie
Publisher: name: figshare
Year: 2022
Subjects: subject: 110317 Physiotherapy
subject: FOS: Clinical medicine

description: This scoping review protocol will outline the planned stages prior to conducting the full scoping study to identify relevant existing literature. The scoping review described in this protocol aims to map the body of literature associated with physiotherapeutic intervention to improve mobility outcomes in adults with moderate to severe traumatic brain injury.
Spinning test particles in the $γ$ spacetime
Creators: name: Toshmatov, Bobir
name: Malafarina, Daniele
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We consider the motion of spinning particles in the field of a well known vacuum static axially-symmetric spacetime, known as $γ$ metric, that can be interpreted as a generalization of the Schwarzschild manifold to include prolate or oblate deformations. We derive the equations of motion for spinning test particles by using the Mathisson-Papapetrou-Dixon equations together with the Tulczyjew spin-supplementary condition, and restricting the motion to the equatorial plane. We determine the limit imposed by super-luminal velocity for the spin of the particle located at the innermost stable circular orbits (ISCO). We show that the particles on ISCO of the prolate $γ$ spacetime are allowed to have nigher spin than the corresponding ones in the the oblate case. We determine the value of the ISCO radius depending on the signature of the spin-angular momentum, ${\rm s-L}$ relation, and show that the value of the ISCO with respect to the non spinning case is bigger for ${\rm sL}<0$ and smaller for ${\rm sL}>0$. The results may be relevant for determining the properties of accretion disks and constraining the allowed values of quadrupole moments of astrophysical black hole candidates.
description: 11 pages, 4 figures, 2 tables
Multi-photon transitions between energy levels in a current-biased Josephson tunnel junction
Creators: name: Wallraff, A.
name: Duty, T.
name: Lukashenko, A.
name: Ustinov, A. V.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The escape of a small current-biased Josephson tunnel junction from the zero voltage state in the presence of weak microwave radiation is investigated experimentally at low temperatures. The measurements of the junction switching current distribution indicate the macroscopic quantum tunneling of the phase below a cross-over temperature of $T^{\star} \approx 280 \rm{mK}$. At temperatures below $T^{\star}$ we observe both single-photon and \emph{multi-photon} transitions between the junction energy levels by applying microwave radiation in the frequency range between $10 \rm{GHz}$ and $38 \rm{GHz}$ to the junction. These observations reflect the anharmonicity of the junction potential containing only a small number of levels.
description: 4 pages, 5 figures
Phloeodes LeConte 1862
Creators: name: Foley, Ian A.
name: Ivie, Michael A.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Zopheridae
Phloeodes

description: Key to the species of Phloeodes
 1 Prothoracic hypomera with deep antennal cavities that are clearly limited posteriorly, and completely contains the antennae while in repose (Figs. 39, 41); elytra usually with at least partially visible velvety arcuate patches; elytra with elevated sculpture reduced, at most to single weak median nodule at start of apical declivity. California Floristic Province. Figs. 35–36 ............................................................................................................... P. diabolicus (LeConte)
- Prothoracic hypomera with deep antennal cavities that are incomplete and not limited posteriorly (Fig. 40), or broad shallow depression (Fig. 42); elytral vestiture variable; elytra with three distinct nodules at start of declivity, two offset medially, and one laterally....................................................................................................................................... 2
 2 Prothoracic hypomera with deep antennal cavity that is not limited posteriorly (Fig. 40); elytral vestiture uniform in coloration from dark red to black; with only three nodules in area of declivity; length rarely over 20mm. California Floristic Province. Fig. 37 ............................................................................................................. P. plicatus (LeConte)
 - Prothoracic hypomera with shallow depression, lacking distinct cavity (Fig. 42); elytral vestiture mottled whitish to black, with velvety spots along suture and on ridges; with three nodules in declivity area and fourth nodule near apex of elytra; length usually over 20mm. Central America. Fig. 38 ............................................... P. venustus (Champion)
description: Published as part of Foley, Ian A. & Ivie, Michael A., 2008, A phylogenetic analysis of the tribe Zopherini with a review of the species and generic classification (Coleoptera: Zopheridae), pp. 1-72 in Zootaxa 1928 (1) on page 42, DOI: 10.11646/zootaxa.1928.1.1, http://zenodo.org/record/5230727
Heavy-Quark Expansion for $\bar{B}_s\to D^{(*)}_s$ Form Factors and Unitarity Bounds beyond the $SU(3)_F$ Limit
Creators: name: Bordone, Marzia
name: Gubernari, Nico
name: Jung, Martin
name: van Dyk, Danny
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We carry out a comprehensive analysis of the full set of $\bar{B}_q \to D_q^{(*)}$ form factors for spectator quarks $q=u,d,s$ within the framework of the Heavy-Quark Expansion (HQE) to order $\mathcal{O}(α_s, 1/m_b, 1/m_c^2)$. In addition to the available lattice QCD calculations we make use of two new sets of theoretical constraints: we produce for the first time numerical predictions for the full set of $\bar{B}_s \to D_s^{(*)}$ form factors using Light-Cone Sum Rules with $B_s$-meson distribution amplitudes. Furthermore, we reassess the QCD three-point sum rule results for the Isgur-Wise functions entering all our form factors for both $q=u,d$ and $q=s$ spectator quarks. These additional constraints allow us to go beyond the commonly used assumption of $SU(3)_F$ symmetry for the $\bar B_s\to D_s^{(*)}$ form factors, especially in the unitarity constraints which we impose throughout our analysis. We find the coefficients of the IW functions emerging at $\mathcal{O}(1/m_c^2)$ to be consistent with the naive $\mathcal{O}(1)$ expectation, indicating a good convergence of the HQE. While we do not find significant $SU(3)$ breaking, the explicit treatment of $q=s$ as compared to a simple symmetry assumption renders the unitarity constraints more effective. We find that the (pseudo)scalar bounds are saturated to a large degree, which affects our theory predictions. We analyze the phenomenological consequences of our improved form factors by extracting $|V_{cb}|$ from $\bar B\to D^{(*)}\ellν$ decays and producing theoretical predictions for the lepton-flavour universality ratios $R(D)$, $R(D^*)$, $R(D_s)$ and $R(D_s^*)$, as well as the $τ$- and $D_q^*$ polarization fractions for the $\bar B_q\to D_q^{(*)}τν$ modes.
description: 16 pages, 3 figures, 7 tables, includes ancillary files; v2: minor changes to the text, conclusions unchanged, 2 missing files added, as accepted for publication in EPJC
The State of the Universe: Cosmological Parameters 2002
Creators: name: Krauss, Lawrence M.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In the past decade, observational cosmology has had one of the most exciting periods in the past century. The precision with which we have been able to measure cosmological parameters has increased tremendously, while at the same time, we have been surprised beyond our wildest dreams by the results. I review here recent measurements of the expansion rate, geometry, age, matter content, and equation of state of the universe, and discuss the implications for our understanding of cosmology.
description: 20 pages, To appear in Proceedings, ESO-CERN-ESA Symposium on Astronomy, Cosmology and Fundamental Physics, March 2002. Typo in final table fixed
Mutual Information is not a Reliable Measure for Variations in Total Correlations
Creators: name: Alipour, S.
name: Tuohino, S.
name: Rezakhani, A. T.
name: Ala-Nissila, T.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Correlations disguised in various forms underlie a host of important phenomena in classical and quantum systems, such as information and energy exchanges. The quantum mutual information and the norm of the correlation matrix are both considered as proper measures of total correlations. We demonstrate that, when applied to the same system, these two measures can actually show significantly different behavior except at least in two limiting cases: when there are no correlations and when there is maximal quantum entanglement. We further quantify the discrepancy by providing analytic formulas for time derivatives of the measures for an interacting bipartite system evolving unitarily. We argue that to properly account for correlations, one should consider the full information provided by the correlation matrix (and reduced states of the subsystems). Scalar quantities such as the norm of the correlation matrix or the quantum mutual information can only capture a part of the complex features of correlations. As a concrete example, we show that in describing heat exchange associated with correlations, neither of these quantities can fully capture the underlying physics.
description: 4+2 pages
Logistic Regression Models for Aggregated Data
Creators: name: T. Whitaker
name: B. Beranger
name: S. A. Sisson
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Logistic regression models are a popular and effective method to predict the probability of categorical response data. However, inference for these models can become computationally prohibitive for large datasets. Here we adapt ideas from symbolic data analysis to summarize the collection of predictor variables into histogram form, and perform inference on this summary dataset. We develop ideas based on composite likelihoods to derive an efficient one-versus-rest approximate composite likelihood model for histogram-based random variables, constructed from low-dimensional marginal histograms obtained from the full histogram. We demonstrate that this procedure can achieve comparable classification rates to the standard full data multinomial analysis and against state-of-the-art subsampling algorithms for logistic regression, but at a substantially lower computational cost. Performance is explored through simulated examples, and analyses of large supersymmetry and satellite crop classification datasets. Supplementary materials for this article are available online.
Quasinormal modes of dilatonic Reissner-Nordström black holes
Creators: name: Blázquez-Salcedo, Jose Luis
name: Kahlen, Sarah
name: Kunz, Jutta
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We calculate the quasinormal modes of static spherically symmetric dilatonic Reissner-Nordström black holes for general values of the electric charge and of the dilaton coupling constant. The spectrum of quasinormal modes is composed of five families of modes: polar and axial gravitational-led modes, polar and axial electromagnetic-led modes, and polar scalar-led modes. We make a quantitative analysis of the spectrum, revealing its dependence on the electric charge and on the dilaton coupling constant. For large electric charge and large dilaton coupling, strong deviations from the Reissner-Nordström modes arise. In particular, isospectrality is strongly broken, both for the electromagnetic-led and the gravitational-led modes, for large values of the charge.
description: 17 pages, 8 figures; v3: refs added, matches published version
Finite temperature dynamics near quantum phase transitions
Creators: name: Sachdev, Subir
Publisher: name: arXiv
Year: 2001
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We review the non-zero temperature relaxational dynamics of quantum systems near a zero temperature, second-order phase transition. We begin with the quantum Ising chain, for which universal and exact results for the relaxation rates can be obtained in all the distinct limiting regimes of the phase diagram. Next, we describe the crossovers in the electron spectral function near a transition involving a change in the pairing symmetry of BCS superconductors in two dimensions. Finally, we consider dynamic spin models which may provide a mean-field description of magnetic ordering transitions in the heavy fermion compounds.
description: 15 pages, 4 figures; talk at the 11th International Conference on Recent Progress in Many Body Theories, Manchester, UK; Discussion mainly for T>0, which complements review in cond-mat/0109419 for T=0
Logistic regression models for aggregated data
Creators: name: T. Whitaker
name: B. Beranger
name: S. A. Sisson
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Logistic regression models are a popular and effective method to predict the probability of categorical response data. However inference for these models can become computationally prohibitive for large datasets. Here we adapt ideas from symbolic data analysis to summarise the collection of predictor variables into histogram form, and perform inference on this summary dataset. We develop ideas based on composite likelihoods to derive an efficient one-versus-rest approximate composite likelihood model for histogram-based random variables, constructed from low-dimensional marginal histograms obtained from the full histogram. We demonstrate that this procedure can achieve comparable classification rates to the standard full data multinomial analysis and against state-of-the-art subsampling algorithms for logistic regression, but at a substantially lower computational cost. Performance is explored through simulated examples, and analyses of large supersymmetry and satellite crop classification datasets.
A large deviation perspective on ratio observables in reset processes: robustness of rate functions
Creators: name: Coghi, Francesco
name: Harris, Rosemary J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study large deviations of a ratio observable in discrete-time reset processes. The ratio takes the form of a current divided by the number of reset steps and as such it is not extensive in time. A large deviation rate function can be derived for this observable via contraction from the joint probability density function of current and number of reset steps. The ratio rate function is differentiable and we argue that its qualitative shape is 'robust', i.e. it is generic for reset processes regardless of whether they have short- or long-range correlations. We discuss similarities and differences with the rate function of the efficiency in stochastic thermodynamics.
description: 17 pages, 15 figures
Non-Equilibrium Transport through a Kondo-Dot in a Magnetic Field: Perturbation Theory and Poor Man's Scaling
Creators: name: Rosch, A.
name: Paaske, J.
name: Kroha, J.
name: Wölfle, P.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We consider electron transport through a quantum dot described by the Kondo model in the regime of large transport voltage V in the presence of a magnetic field B with max(V,B) >> T_K. The electric current I and the local magnetization M are found to be universal functions of V/T_K and B/T_K, where T_K is the equilibrium Kondo temperature. We present a generalization of the perturbative renormalization group to frequency dependent coupling functions, as necessitated by the structure of bare perturbation theory. We calculate I and M within a poor man's scaling approach and find excellent agreement with experiment.
description: version accepted in PRL, notations changed, parts rewritten, figures modified, references and some corrections added
Economic Growth: The Role of Institutions and Political Economy
Creators: name: Freebairn, John
name: Freebairn, John
Publisher: name: Unknown
Year: 1995
Subjects: Political Economy

description: Economic growth is a complex process involving many dimensions, causal forces and transmission mechanisms. In order to avoid spurious correlations and serious specification errors, it is necessary to place any empirical analysis of growth in a general equilibrium model framework. The institutional framework is just one of many potential causal forces, and institutions may, themselves, be shaped by economic growth. This paper reviews papers published in the mainstream economics journals over the last ten years which have estimated regression equations to explain differences in long-term rates of economic growth across countries. The review focuses on the role of institutions in growth, and it comments on methodological strengths and weaknesses of these types of empirical studies for better understanding the growth process. The scope of the study is narrowed in three main ways. First, reviewed studies apply to the whole economy. However, the implications could easily be applied to individual sectors or commodities. Second, the studies consider longer-term average growth rates. This enables cyclical and seasonal influences to be ignored. Third, most of the reviewed studies have drawn on the well recognized data banks reported by Summers and Heston (1984, 1988, 1991) which have a high degree of comparability from country to country and over time.
$γN \to N^*(1535)$ transition in soft-wall AdS/QCD
Creators: name: Gutsche, Thomas
name: Lyubovitskij, Valery E.
name: Schmidt, Ivan
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present a study of the $N^*(1535)$ resonance electroexcitation in a soft-wall AdS/QCD model. Both the transverse $A_{1/2}^p$ and longitudinal $S_{1/2}^p$ helicity amplitudes are calculated resulting in good agreement with data and with the MAID parametrization.
description: arXiv admin note: text overlap with arXiv:1906.08641
A Search for Stellar Obscuration Events due to Dark Clouds
Creators: name: Drake, A. J.
name: Cook, K. H.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The recent detections of a large population of faint submillimetre sources, an excess halo gamma-ray background, and the extreme scattering events observed for extragalactic radio sources have been explained as being due to baryonic dark matter in the form of small, dark, gas clouds. In this paper we present the results of a search for the transient stellar obscurations such clouds are expected to cause. We examine the Macho project light curves of 48 x 10^6 stars toward the Galactic bulge, LMC and SMC for the presence of dark cloud extinction events. We find no evidence for the existence of a population of dark gas clouds with Av > 0.2 and masses between ~ 10^-4 and 10^-2 M_solar in the Galactic disk or halo. However, it is possible that such dark cloud populations could exist if they are clustered in regions away from the observed lines of sight.
description: 13 pages, 9 figures, submitted to ApJ
Science Case of a Scintillator and Radio Surface Array at IceCube
Creators: name: Schröder, Frank G.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The upgrade of IceTop, the surface array of IceCube, by a hybrid array of scintillation and radio detectors is motivated by a rich science case. The scintillators will lower the threshold for the measurement of air showers to about 100 TeV, provide a more efficient veto of air showers for neutrino measurements, and improve the separation of the electromagnetic and muonic shower components due to the different responses of scintillators and ice-Cherenkov tanks. Furthermore, the scintillators will enable the calibration and compensation of the effect of snow accumulation above IceTop. The radio antennas will provide a calorimetric measurement of the electromagnetic shower component and a direct sensitivity to the shower maximum. Consequently, the combination of the existing ice-Cherenkov detectors in the ice and at the surface with the new scintillation and radio detectors at the surface will enable unprecedented accuracy for event-by-event mass classification in the PeV to EeV range. This will transform IceCube into the most accurate instrument for high-energy Galactic cosmic rays in the Southern Hemisphere. Hence, the hybrid array will make an important contribution to the main science case of IceCube of understanding the origin of cosmic rays. In addition to its cosmic-ray science goals, the hybrid array provides essential R&D for IceCube-Gen2 which will feature a larger surface array, sophisticated timing and communication technology, and elevated surface structures. Moreover, the hybrid array will improve the understanding of the atmospheric background to the neutrino measurements and opens new scientific opportunities, such as the searches for PeV gamma rays from the Galactic Center and for mass-dependent anisotropies.
description: Presented at the 36th International Cosmic Ray Conference (ICRC 2019). See arXiv:1907.11699 for all IceCube contributions
Amyttacta Beier 1965
Creators: name: Naskrecki, Piotr
name: Bazelet, Corinna S.
name: Spearman, Lauren A.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Orthoptera
Tettigoniidae
Amyttacta

description: Amyttacta Beier, 1965
 Type species: Amyttacta rhodesica Beier, 1965: 225.
 This southern African genus of the Amytta -group has been recorded previously from Angola (A. angolensis Beier) and Zimbabwe (A. rhodesica Beier), but never south of the Limpopo River, and thus the two species described below are the southernmost records for representatives of the Amytta- group.
 All species of Amyttacta are characterized by relatively simple cerci in the male, which are armed with small, basal hooks or spines. The 10 th in the male is well sclerotized, but not overhanging the epiproct (the posterior edge of the 10 th tergite bears two elongated processes in A. angolensis), and the subgenital plate has a pair of small, but distinct styli. None of the known species has sclerotized titillators. The ovipositor is long (about as long as the hind femur) and nearly straight (only the male is known in A. angolensis.)
 Nothing is known about the biology of the previously described species, except for the fact that adults of A. rhodesica are used by wasps Sphex pelopoeiformis (Dahlbom) as larval food (Beier 1965.) A. farrelli described below, was found to be exceptionally abundant in Limpopo at grassy sites dominated by common Guinea grass Urochloa maxima (Jacq.) R.D. Webster. The density of individuals at some sites was 10–15 individuals/m 2, and often multiple individuals were seen feeding on the same grass inflorescence. These katydids were also seen on other species of plants, but no feeding on plants other than Guinea grass was observed.
 Males of A. farrelli produce long, ultrasonic calls, in the range of 31–100 kHz (see below). While no mating was observed, we saw several females carrying or eating large spermatophylaxes, suggesting a significant paternal investment in this species (Fig. 3D).
description: Published as part of Naskrecki, Piotr, Bazelet, Corinna S. & Spearman, Lauren A., 2008, New species of flightless katydids from South Africa (Orthoptera: Tettigoniidae: Meconematinae), pp. 19-32 in Zootaxa 1933 (1) on page 21, DOI: 10.11646/zootaxa.1933.1.3, http://zenodo.org/record/5230922
title: Opinions of adult children from multi-child families on their family of origin
Creators: name: Sobczyk- Gąsiorek, Anna
name: Gąsiorek, Przemysław
name: Wanda
Publisher: name: EDUsfera. Ewa Jurczyk-Romanowska
Year: 2020

description: Badania nad rodzinami wielodzietnymi są prowadzone przede wszystkim, ze względu na zainteresowanie sytuacją dzieci, które się rozwijają w tych szczególnych warunkach. Wyniki ukazują rodziny wielodzietne w bardzo spolaryzowany sposób. od bardzo negatywnych, eksponujących niewydolność wychowawczą, trudności materialne i różnego rodzaju zaniedbania do bardzo pozytywnych, podkreślających korzystny wpływ licznego rodzeństwa na rozwój dzieci. Przedstawione w artykule wyniki badań ukazują wielodzietność z perspektywy niepodejmowanej dotychczas, a mianowicie analizując opinię dorosłych, którzy wychowywali się w rodzinie wielodzietnej.
Additional file 1 of Development of a composite hydrogel incorporating anti-inflammatory and osteoinductive nanoparticles for effective bone regeneration
Creators: name: Byun, Hayeon
name: Jang, Gyu Nam
name: Jeong, Hyewoo
name: Lee, Jinkyu
name: Huh, Seung Jae
name: Lee, Sangmin
name: Kim, Eunhyung
name: Shin, Heungsoo
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Supplementary material 1
Lectures on the functional renormalization group method
Creators: name: Polonyi, Janos
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: These introductory notes are about functional renormalization group equations and some of their applications. It is emphasised that the applicability of this method extends well beyond critical systems, it actually provides us a general purpose algorithm to solve strongly coupled quantum field theories. The renormalization group equation of F. Wegner and A. Houghton is shown to resum the loop-expansion. Another version, due to J. Polchinski, is obtained by the method of collective coordinates and can be used for the resummation of the perturbation series. The genuinely non-perturbative evolution equation is obtained in a manner reminiscent of the Schwinger-Dyson equations. Two variants of this scheme are presented where the scale which determines the order of the successive elimination of the modes is extracted from external and internal spaces. The renormalization of composite operators is discussed briefly as an alternative way to arrive at the renormalization group equation. The scaling laws and fixed points are considered from local and global points of view. Instability induced renormalization and new scaling laws are shown to occur in the symmetry broken phase of the scalar theory. The flattening of the effective potential of a compact variable is demonstrated in case of the sine-Gordon model. Finally, a manifestly gauge invariant evolution equation is given for QED.
description: 47 pages, 11 figures, final version
Population dynamics of Xylella fastidiosa subsp. pauca indicate that coffee strains are the founding populations for the olive-Xylella infections in Brazil
Creators: name: Sardinha, Francisco Carolina
name: Nagela, Safady
name: Augusto, Dos Santos Pereira Danilo
name: Rodrigo, Almeida
name: Helvecio, Coletta-Filho
Publisher: name: Zenodo
Year: 2021
Subjects: subject: plant health
subject: xylella
subject: http://id.agrisemantics.org/gacs/C20262
subject: http://id.agrisemantics.org/gacs/C764
subject: http://id.agrisemantics.org/gacs/C13089

description: Xylella fastidiosa subsp. pauca (X.f. pauca) is a multi-host pathogen responsible for significant disease outbreaks in the agro-ecosystem worldwide. In Brazil, the species causes severe economic losses in coffee and sweet orange productions and was recently identified as causing the olive quick syndrome decline (OQSD), a newly emerging disease. We lack information on the evolutionary potential of this new olive-infecting population, and its relationship with established populations from other hosts. We showed that X.f. pauca strains were widely spread through olive orchards and 75% of the diseased plants were infected by a single sequence type (ST16) that was firstly reported infecting coffee orchards. Based on the epidemiological characteristics of X.f. pauca and its ancient infections in coffee plants in Brazil, we then hypothesized that coffee populations are the source of inoculum of X.f. pauca for olive trees under natural conditions. To test this hypothesis, we analyzed the genetic diversity and population dynamics of all 584 isolates (n=82 from olive, n=170 from coffee, and n=237 from citrus) of X.f. pauca using 12 microsatellites (SSR) loci. We observed that the coffee-infecting population had the highest genetic diversity and lowest clonal fraction among the three hosts. Based on a discriminant analysis of principal components and Bayesian clustering analysis, we found evidence for two major genetic groups of isolates. The first group is formed by isolates from olive and coffee and the second and more distant by isolates from citrus. A minimum spanning network analysis provided further evidence for the proximity between olive and coffee populations, maintaining citrus haplotypes further isolated. Coffee and olive crops occur sympatrically in São Paulo and Minas Gerais states, which may favor the exchange of the genetic material between these two hosts. Our results corroborate the importance of monitoring the population structure of multi-host pathogens to elaborate strategies for pathogen control and reduction of pathogen transmission.
 Support: Horizon 2020 (XF Actors 727987), Fapesp (Proc. 2016/02176-7)
description: BR; PDF; hdcoletta@ccsm.br
Nuclear Inelastic X-Ray Scattering of FeO to 48 GPa
Creators: name: Struzhkin, Viktor V.
name: Mao, Ho-kwang
name: Hu, Jingzhu
name: Schwoerer-Böhning, Markus
name: Shu, Jinfu
name: Hemley, Russell J.
name: Sturhahn, Wolfgang
name: Hu, Michael Y.
name: Alp, Ercan E.
name: Eng, Peter
name: Shen, Guoyin
Publisher: name: arXiv
Year: 2001
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The partial density of vibrational states has been measured for Fe in compressed FeO (wüstite) using nuclear resonant inelastic x-ray scattering. Substantial changes have been observed in the overall shape of the density of states close to the magnetic transiton around 20 GPa from the paramagnetic (low pressure) to the antiferromagnetic (high pressure) state. Our data indicate a substantial softening of the aggregate sound velocities far below the transition, starting between 5 and 10 GPa. This is consistent with recent radial x-ray diffraction measurements of the elastic constants in FeO. The results indicate that strong magnetoelastic coupling in FeO is the driving force behind the changes in the phonon spectrum of FeO.
description: 4 pages, 4 figures
Additional file 1 of Coding quality of deaths and its impact on elderly unintentional fall mortality data from 1990 to 2019: a retrospective analysis of the WHO Mortality Database
Creators: name: Hua, Junjie
name: Ning, Peishan
name: Cheng, Peixia
name: Rao, Zhenzhen
name: He, Jieyi
name: Xiao, Wangxin
name: Li, Li
name: Fu, Yanhong
name: Li, Ruotong
name: Li, Jie
name: Wang, Wanhui
name: Schwebel, David C.
name: Hu, Guoqing
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified

description: Additional file 1: Appendix 1. Coding quality by county/territory income. Appendix 2. Country-specific coding quality. Appendix 3. Crude and corrected age-adjusted unintentional fall mortality. Appendix 4. Flow chart of selection of eligible countries/territories. Appendix 5. GATHER checklist
Fusion systems of blocks of finite groups over arbitrary fields
Creators: name: Boltje, Robert
name: Karagüzel, Çisil
name: Yılmaz, Deniz
Publisher: name: arXiv
Year: 2019
Subjects: subject: Representation Theory (math.RT)
subject: Group Theory (math.GR)
subject: Rings and Algebras (math.RA)
subject: FOS: Mathematics
subject: 20C20

description: To any block idempotent $b$ of a group algebra $kG$ of a finite group $G$ over a field $k$ of characteristic $p>0$, Puig associated a fusion system and proved that it is saturated if the $k$-algebra $kC_G(P)e$ is split, where $(P,e)$ is a maximal $kGb$-Brauer pair. We investigate in the non-split case how far the fusion system is from being saturated by describing it in an explicit way as being generated by the fusion system of a related block idempotent over a larger field together with a single automorphism of the defect group.
description: 11 pages
Evidence for coupling between the Sagittarius dwarf galaxy and the Milky Way warp
Creators: name: Bailin, Jeremy
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using recent determinations of the mass and orbit of Sagittarius, I calculate its orbital angular momentum. From the latest observational data, I also calculate the angular momentum of the Milky Way's warp. I find that both angular momenta are directed toward l=270, b=0, and have magnitude 2-8x10^12 M_Sun kpc km s^-1, where the range in both cases reflects uncertainty in the mass. The coincidence of the angular momenta is suggestive of a coupling between these systems. Direct gravitational torque of Sgr on the disk is ruled out as the coupling mechanism. Gravitational torque due to a wake in the halo and the impulsive deposition of momentum by a passage of Sgr through the disk are still both viable mechanisms pending better simulations to test their predictions on the observed Sgr-MW system.
description: 11 pages, to appear in the February 1 issue of ApJL
Energy Spectrum of Neutral Collective Excitations in Striped Hall States
Creators: name: Aoyama, T.
name: Ishikawa, K.
name: Ishizuka, Y.
name: Maeda, N.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate neutral collective excitations in the striped Hall state. In the striped Hall state, the magnetic translation and rotation symmetries are spontaneously broken. Using the commutation relation between charges and currents corresponding to the broken and unbroken symmetry, the existence of the gapless neutral excitation is proved. The spectrum of the neutral collective excitation at the half-filled third Landau level is obtained in the single mode approximation. We find the periodic line nodes in the spectrum. The spectrum is compared with the particle-hole excitation spectrum in the Hartree-Fock approximation.
description: 8 pages, 5 figures, some comments, appendix, and references added
Current profiles and AC losses of a superconducting strip with elliptic cross-section in perpendicular magnetic field
Creators: name: Gomory, F.
name: Tebano, R.
name: Sanchez, A.
name: Pardo, E.
name: Navau, C.
name: Husek, I.
name: Strycek, F.
name: Kovac, P.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The case of a hard type II superconductor in the form of strip with elliptic cross-section when placed in transverse magnetic field is studied. We approach the problem in two steps, both based on the critical-state model. First we calculate numerically the penetrated current profiles that ensure complete shielding in the interior, without assuming an a priori form for the profiles. In the second step we introduce an analytical approximation that asumes that the current profiles are ellipses. Expressions linking the sample magnetization to the applied field are derived covering the whole range of applied fields. The theoretical predictions are tested by the comparison with experimental data for the imaginary part of AC susceptibility.
description: 12 pages; 3 figures
Impact Factor volatility to a single paper: A comprehensive analysis
Creators: name: Antonoyiannakis, Manolis
Publisher: name: arXiv
Year: 2019
Subjects: subject: Digital Libraries (cs.DL)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: We study how a single paper affects the Impact Factor (IF) by analyzing data from 3,088,511 papers published in 11639 journals in the 2017 Journal Citation Reports of Clarivate Analytics. We find that IFs are highly volatile. For example, the top-cited paper of 381 journals caused their IF to increase by more than 0.5 points, while for 818 journals the relative increase exceeded 25%. And one in 10 journals had their IF boosted by more than 50% by their top three cited papers. Because the single-paper effect on the IF is inversely proportional to journal size, small journals are rewarded much more strongly than large journals for a highly-cited paper, while they are penalized more for a low-cited paper, especially if their IF is high. This skewed reward mechanism incentivizes high-IF journals to stay small, to remain competitive in rankings. We discuss the implications for breakthrough papers appearing in prestigious journals. We question the reliability of IF rankings given the high IF sensitivity to a few papers for thousands of journals.
description: Quantitative Science Studies (accepted). arXiv admin note: text overlap with arXiv:1906.02660
Photometric Survey of the Irregular Satellites
Creators: name: Grav, Tommy
name: Holman, Matthew J.
name: Gladman, Brett
name: Aksnes, Kaare
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present BVRI colors of 13 Jovian and 8 Saturnian irregular satellites obtained with the 2.56m Nordic Optical Telescope on La Palma, the 6.5m Magellan Baade Telescope on La Campanas, and the 6m MMT on Mt. Hopkins. The observations were performed between December 2001 to March 2002. Nearly all of the known irregular satellites can be divided into two distinct classes based on their colors. One, the grey color class, has the similar colors to the C-type asteroid, and the other, the light red color class, has colors similar to P/D-type asteroids. We also find at least one object, the Jovian irregular J XXIII Kalyke, that has colors similar to the red colored Centaurs/TNOs, although its classification is unsecure. We also find that there is a correlation between the physical properties and dynamical properties of the irregular satellites. Most of the dynamical clusters have homogeneous colors, which points to single homogeneous progenitors being cratered or fragmented as the source of each individual cluster. The heterogeneous colored clusters are most easily explained by assuming that there are several dynamical clusters in the area, rather than just one.
description: Submitted to Icarus, 43 pages including 5 figures
title: Editions of Lycian Inscriptions not Included in Melchert’s Corpus from 2001
Creators: name: Adiego (Ed.), Ignasi-Xavier
name: García Trabazo (Ed.), José Virgilio
name: Vernet (Ed.), Mariona
name: Obrador-Cursach (Ed.), Bartomeu
name: Martínez Rodríguez (Ed.), Elena
Publisher: name: Universitat de  Barcelona Ediciones
Year: 2019

description: The purpose of the paper is to provide editions of all Lycian inscriptions and fragments of inscriptions that are neither included in Neumann 1979 nor the online corpus published by Melchert in 2001. 1 As far as possible or appropriate, the texts will be presented in transliteration, translation, and commentaries. This applies both to the inscriptions that have already been published by other scholars and to those that I have been entrusted with for publication.
Amyttacta Beier 1965
Creators: name: Naskrecki, Piotr
name: Bazelet, Corinna S.
name: Spearman, Lauren A.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Orthoptera
Tettigoniidae
Amyttacta

description: Key to known species of Amyttacta (males)
1. Macropterous, wings extending well past the tip of the abdomen...............................................................2
- Brachypterous, wings completely hidden under the pronotum...................................................................3
 2. Tenth abdominal tergite with a pair of elongated median lobes; cercus straight ........... A. angolensis Beier
 - Tenth abdominal tergite without a pair of median lobes; cercus slightly bent inwards ... A. rhodesica Beier
 3. Cercus bent downwards when seen from the side (Fig. 1D), its basal part with a small, hook-like lobe (Fig. 1E) ............................................................................................................................... A. farrelli n. sp.
 - Cercus straight when seen from the side (Fig. 1L), its basal part with a multi-lobed projection at the base (Fig. 1J) ...................................................................................................................... A. marakelensis n. sp.
description: Published as part of Naskrecki, Piotr, Bazelet, Corinna S. & Spearman, Lauren A., 2008, New species of flightless katydids from South Africa (Orthoptera: Tettigoniidae: Meconematinae), pp. 19-32 in Zootaxa 1933 (1) on page 21, DOI: 10.11646/zootaxa.1933.1.3, http://zenodo.org/record/5230922