cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Curvature induced magnonic crystal in nanowires
Creators: name: Korniienko, Anastasiia
name: Kravchuk, Volodymyr P.
name: Pylypovskyi, Oleksandr V.
name: Sheka, Denis D.
name: Brink, Jeroen van den
name: Gaididei, Yuri
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: A new type of magnonic crystals, curvature induced ones, is realized in ferromagnetic nanowires with periodically deformed shape. A magnon band structure of such crystal is fully determined by its curvature: the developed theory is well confirmed by simulations. An application to nanoscale spintronic devises with the geometrically tunable parameters is proposed, namely, to filter elements.
description: 21 pages, 6 figures, for submission to SciPost
Paralargulus Stehlík & Brailovsky 2011, gen. nov.
Creators: name: Stehlík, Jaroslav L.
name: Brailovsky, Harry
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Largidae
Paralargulus

description: Paralargulus gen. nov.
(Figs. 2, 15)
 Type species. Largulus refulgens Brailovsky & Barrera, 2008 (here designated) = Paralargulus refulgens (Brailovsky & Barrera, 2008) comb. nov.
 Diagnosis. This genus differs remarkably from any other member of the tribe Largulini by strongly concave ventral rim of pygophore, that reaches deeper than half the height of ventral wall, and has the margins of the concavity strongly thickened, ridge-shaped, and apically subacute (Fig. 14).
For a detailed description see BRAILOVSKY & BARRERA (2008: 256–258).
 Etymology. The name is composed from the Greek prefix para (= close to) and the generic name Largulus; gender masculine.
description: Published as part of Stehlík, Jaroslav L. & Brailovsky, Harry, 2011, Two new genera of the tribe Largulini (Hemiptera: Heteroptera: Largidae) from Greater Antilles, pp. 449-456 in Acta Entomologica Musei Nationalis Pragae 51 (2) on page 453, DOI: 10.5281/zenodo.5328601
Collision of two kinks with inner structure
Creators: name: Zhong, Yuan
name: Du, Xiao-Long
name: Jiang, Zhou-Chao
name: Liu, Yu-Xiao
name: Wang, Yong-Qiang
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this work, we study kink collisions in a scalar field model with scalar-kinetic coupling. This model supports kink/antikink solutions with inner structure in the energy density. The collision of two such kinks is simulated by using the Fourier spectral method. We numerically calculate how the critical velocity and the widths of the first three two bounce windows vary with the model parameters. After that, we report some interesting collision results including two-bion escape final states, kink-bion-antikink intermediate states and kink or antikink intertwined final states. These results show that kinks with inner structure in the energy density have similar properties as those of the double kinks.
description: 20 pages, 11 figures, prepared for publication in JHEP
Deep Learning in Video Multi-Object Tracking: A Survey
Creators: name: Ciaparrone, Gioele
name: Sánchez, Francisco Luque
name: Tabik, Siham
name: Troiano, Luigi
name: Tagliaferri, Roberto
name: Herrera, Francisco
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: The problem of Multiple Object Tracking (MOT) consists in following the trajectory of different objects in a sequence, usually a video. In recent years, with the rise of Deep Learning, the algorithms that provide a solution to this problem have benefited from the representational power of deep models. This paper provides a comprehensive survey on works that employ Deep Learning models to solve the task of MOT on single-camera videos. Four main steps in MOT algorithms are identified, and an in-depth review of how Deep Learning was employed in each one of these stages is presented. A complete experimental comparison of the presented works on the three MOTChallenge datasets is also provided, identifying a number of similarities among the top-performing methods and presenting some possible future research directions.
description: Accepted in Neurocomputing, 2019. New in v4: updated license in compliance with Elsevier policy. Main text: 29 pages, 10 figures, 7 tables. Summary table in appendix at the end of the paper
MOESM9 of Internalization and accumulation of model lignin breakdown products in bacteria and fungi
Creators: name: Barnhart-Dailey, Meghan
name: Dongmei Ye
name: Hayes, Dulce
name: Danae Maes
name: Simoes, Casey
name: Appelhans, Leah
name: Carroll-Portillo, Amanda
name: Kent, Michael
name: Timlin, Jerilyn
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Pharmacology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Inorganic Chemistry
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Additional file 9: Figure S9. A. Representative mass spectra for GGE metabolites (guiacol, protocatechuate, and 2-(2-methoxyphenoxy)-1,3-propanediol) from E. lignolyticus lysates grown in minimal media and incubated with DMSO or GGE for 4 h. Integrated peak for each (from left to right in order listed above) is marked with a red arrow. B. Ion counts for integrated peaks indicated with arrows in A. Gray bars are ion counts of each compound for DMSO lysate, and black bars are ion counts of each compound for GGE lysates. 1 biological replicates is shown. C. Representative mass spectra for GGE metabolics (guiacol, protocatechuate, and 2-(2-methoxyphenoxy)-1,3-propanediol) from E. lignolyticus lysates grown in nutrient broth and incubated with DMSO or GGE for 4 h. Integrated peak for protocatechuate is marked with a red arrows. D. Average ion counts for integrated protocatechuate peak indicated with arrows in C. 3 biological replicates are shown, error bars are standard deviation. Gray bars are ions counts for DMSO lysate and black bars are ion counts for the GGE lysates.
Radiation drag driven mass accretion in clumpy interstellar medium: implications for the supermassive black hole-to-bulge relation
Creators: name: Kawakatu, Nozomu
name: Umemura, Masayuki
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We quantitatively scrutinize the effects of the radiation drag arising from the radiation fields in a galactic bulge in order to examine the possibility that the radiation drag could be an effective mechanism to extract angular momentum in a spheroidal system like a bulge and allow plenty of gas to accrete onto the galactic center. For this purpose, we numerically solve the relativistic radiation hydrodynamical equation coupled with the accurate radiative transfer and quantitatively assess the radiation drag efficiency. As a result, we find that in an optically thick regime the radiation drag efficiency is sensitively dependent on the density distributions of interstellar medium (ISM). The efficiency drops according to $τ_{\rm T}^{-2}$ in an optically thick {\it uniform} ISM, where $τ_{\rm T}$ is the total optical depth of the dusty ISM, whereas the efficiency remains almost constant at a high level if the ISM is {\it clumpy}. Hence, if the bulge formation begins with a star formation event in a clumpy ISM, the radiation drag will effectively work to remove the angular momentum and the accreted gas may form a supermassive black hole. As a natural consequence, this mechanism reproduces a putative linear relation between the mass of a supermassive black hole and the mass of a galactic bulge, although further detailed modeling for stellar evolution is required for the more precise prediction.
description: 7pages,4figures, accepted for publication
Coelogyne edentula M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne edentula

description: Coelogyne edentula (Blume) M.W.Chase & Schuit., comb. nov.
 Basionym: Dendrochilum edentulum Blume, Bijdr. Fl. Ned. Ind.: 399 (1825).
 Homotypic synonyms: Platyclinis edentula (Blume) Benth. ex Hemsl., Gard. Chron., n.s., 16: 656 (1881). Acoridium edentulum (Blume) Rolfe, Orchid Rev. 12: 220 (1904).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 109, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
Porocallus insignis SHARP 1888
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Porocallus
Porocallus insignis

description: Porocallus insignis SHARP 1888 (Map 1)
M a t e r i a l e x a m i n e d: Russia: 1 ex., 70 km E Vladivostock, Anisimovka, 43°11'N, 132°41'E, 200 m, 7.VI.1993, leg. Zerche (SDEI).
 C o m m e n t: The above record is within the known range of P. insignis.
description: Published as part of Assing, V., 2012, A revision of Porocallus SHARP. III. A new species from China and an additional record (Coleoptera: Staphylinidae: Aleocharinae), pp. 1011-1016 in Linzer biologische Beiträge 44 (2) on page 1012, DOI: 10.5281/zenodo.5328670
Additional file 1: of Linked read technology for assembling large complex and polyploid genomes
Creators: name: Ott, Alina
name: Schnable, James
name: Yeh, Cheng-Ting
name: Wu, Linjiang
name: Liu, Chao
name: Hu, Heng-Cheng
name: Dalgard, Clifton
name: Sarkar, Soumik
name: Schnable, Patrick
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Figure S1. Pulsed field gel electrophoresis image of B73 high molecular weight DNA after extraction and before LR library preparation. Figure S2. Length distributions of A) LR scaffolds (N = 171,932), B) distances between contig pairs (two contigs that comprise a scaffold) which align to the same chromosome (N = 6566), C) LR contigs (N = 234,153), D) LR contig tails (N = 64,704), E) trimmed LR contigs (N = 233,095), and F) trimmed LR contig tails (N = 39,237). Figure S3. Estimated percent reduction in assembly error (A) and percent bases remaining following contig trimming (B). Figure S4. Repeat content at the junction of the aligned portion of a representative LR contig with a tail and its tail. Figure S5. Length of A) trimmed LR (N = 234,153), B) MAGI (N = 114,173), and C) ABySS contigs (N = 10,787,574). Means ( x ¯ $$ \overline{x} $$ ) and medians ( X ~ $$ \overset{\sim }{X} $$ ) are indicated by vertical lines with the values reported on each plot. Figure S6. Comparisons of LR, MAGI, and REF contigs. MAGI and LR contigs were aligned to REF contigs. Figure S7. Coverage of debarcoded reads uniquely aligned to the reference genome in regions where LR contigs align (N = 244,649) or do not align (N = 1,324,967). Figure S8. Genomic overlap of LR assemblies. A) Percent of bases shared between aligned regions of fully aligned contigs from all LR assemblies. Figure S9. Relationship between contig length in bins of 1 kb and contig quality for LR and ABySS assemblies. Figure S10. Genome-wide distribution of maize and proso millet LR contigs. Table S1. Summary of assemblies. Table S2. Categorization of trimmed simulation contig alignment. (DOCX 789 kb)
The Pattern Speed of the OH/IR Stars in the Milky Way
Creators: name: Debattista, Victor P.
name: Gerhard, Ortwin
name: Sevenster, Maartje N.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show how the continuity equation can be used to determine pattern speeds in the Milky Way Galaxy (MWG). This method, first discussed by Tremaine & Weinberg in the context of external galaxies, requires projected positions, $(l,b)$, and line-of-sight velocities for a spatially complete sample of relaxed tracers. If the local standard of rest (LSR) has a zero velocity in the radial direction ($u_{\rm LSR}$), then the quantity that is measured is $ΔV \equiv Ω_p R_0 - V_{\rm LSR}$, where $Ω_p$ is the pattern speed of the non-axisymmetric feature, $R_0$ is the distance of the Sun from the Galactic centre and $V_{\rm LSR}$ is the tangential motion of the LSR, including the circular velocity. We use simple models to assess the reliability of the method for measuring a single, constant pattern speed of either a bar or spiral in the inner MWG. We then apply the method to the OH/IR stars in the ATCA/VLA OH 1612 MHz survey of Sevenster et al, finding $ΔV = 252 \pm 41$ km/s, if $u_{\rm LSR} = 0$. Assuming further that $R_0 = 8$ kpc and $V_{\rm LSR} = 220$ \kms, this gives $Ω_p = 59\pm 5$ km/s/kpc with a possible systematic error of perhaps 10 km/s/kpc. The non-axisymmetric feature for which we measure this pattern speed must be in the disc of the MWG.
description: 15 pages, 13 figures. Accepted to MNRAS
Chemical evolution of Elliptical Galaxies and the ICM
Creators: name: Pipino, Antonio
name: Matteucci, Francesca
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a new model for the chemical evolution of elliptical galaxies taking into account SN feedback, detailed nucleosynthesis and galactic winds. We discuss the effect of galactic winds on the chemical enrichment of the ICM and compute the energy per particle injected by the galaxies into the ICM.
description: 4 pages, 2 figures, to appear in the ''Proceedings of The evolution of galaxies III. From simple approaches to self-consistent models'', Kiel (Germany), 2002
Signals of primordial phase transitions on CMB maps
Creators: name: Corasaniti, P. S.
name: Amendola, L.
name: Occhionero, F.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The analysis of the CMB anisotropies is a rich source of cosmological informations. In our study, we simulated the signals produced by the relics of a first order phase transition occured during an inflationary epoch in the early Universe. These relics are bubbles of true vacuum that leave a characteristic non-Gaussian imprint on the CMB. We use different statistical estimators in order to evaluate this non-Gaussianity. We obtain some limits on the allowed values of the bubble parameters comparing our results with the experimental data. We also predict the possibility to detect this signal with the next high resolution experiments.
description: 2 pages, submitted to Proceedings of 9th Marcel Grossmann meeting
MOESM8 of Internalization and accumulation of model lignin breakdown products in bacteria and fungi
Creators: name: Barnhart-Dailey, Meghan
name: Dongmei Ye
name: Hayes, Dulce
name: Danae Maes
name: Simoes, Casey
name: Appelhans, Leah
name: Carroll-Portillo, Amanda
name: Kent, Michael
name: Timlin, Jerilyn
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Additional file 8: Figure S8. A. Representative mass spectra (QToF-MS) for each uptake compound (4-HBA, VA, SA, CA, and GGE) in E. coli lysates. Integrated peak for internalization experiments is marked with a red arrow. DMSO vehicle control mass spectra are shown at the retention time for each compound of interest for peak comparison. E. lignolyticus spectra look similar (data not shown). B. ion counts for each compound in E. coli vs. E. lignolyticus cell lysates from 3 biological replicates. Error bars are standard deviation. C. Ion counts for spiked E. coli or E. lignolyticus lysate with indicated compounds at a concentration of 0.005Â mM. Spikes were used to calculate the relative intracellular concentrations in Fig.Â 5.
Thermal Desorption of Water-Ice in the Interstellar Medium
Creators: name: Fraser, Helen J.
name: Collings, Mark P.
name: McCoustra, Martin R. S.
name: Williams, David A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Water (H2O) ice is an important solid constituent of many astrophysical environments. To comprehend the role of such ices in the chemistry and evolution of dense molecular clouds and comets, it is necessary to understand the freeze-out, potential surface reactivity, and desorption mechanisms of such molecular systems. Consequently, there is a real need from within the astronomical modelling community for accurate empirical molecular data pertaining to these processes. Here we give the first results of a laboratory programme to provide such data. Measurements of the thermal desorption of H2O ice, under interstellar conditions, are presented. For ice deposited under conditions that realistically mimic those in a dense molecular cloud, the thermal desorption of thin films (~50 molecular layers) is found to occur with zero order kinetics characterised by a surface binding energy, E_{des}, of 5773 +/- 60 K, and a pre-exponential factor, A, of 10^(30 +/- 2) molecules cm^-2 s^-1. These results imply that, in the dense interstellar medium, thermal desorption of H2O ice will occur at significantly higher temperatures than has previously been assumed.
description: 9 pages, 4 figures, accepted for publication in MNRAS
Road Scene Understanding by Occupancy Grid Learning from Sparse Radar Clusters using Semantic Segmentation
Creators: name: Sless, Liat
name: Cohen, Gilad
name: Shlomo, Bat El
name: Oron, Shaul
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Occupancy grid mapping is an important component in road scene understanding for autonomous driving. It encapsulates information of the drivable area, road obstacles and enables safe autonomous driving. Radars are an emerging sensor in autonomous vehicle vision, becoming more widely used due to their long range sensing, low cost, and robustness to severe weather conditions. Despite recent advances in deep learning technology, occupancy grid mapping from radar data is still mostly done using classical filtering approaches.In this work, we propose learning the inverse sensor model used for occupancy grid mapping from clustered radar data. This is done in a data driven approach that leverages computer vision techniques. This task is very challenging due to data sparsity and noise characteristics of the radar sensor. The problem is formulated as a semantic segmentation task and we show how it can be learned using lidar data for generating ground truth. We show both qualitatively and quantitatively that our learned occupancy net outperforms classic methods by a large margin using the recently released NuScenes real-world driving data.
title: Factors Affecting SMEs Decision-Makers Risk Perceptions Associated with Exporting: A Comparison Study of Emerging and Advanced Markets
Creators: name: Al-Rashidi, Yousif Abdullah
Publisher: name: Griffith University
Year: 2012
Subjects: subject: International trade
subject: Exports
subject: Multinational enterprises
subject: Business risk
subject: Multinational enterprises decision making

description: International trade is vital to a country’s economic survival (Al-Aali, 1995; Asiedu & Lien, 2004). Currently, exporting represents one of the most common international trade activities and entry modes to international markets. Multinational-enterprises (MNEs) have enacted a dominant role in global markets for a substantial time. However, more recently, small and medium-seized enterprises (SMEs) have come to play an increasingly important role in the global economy. In fact, SMEs have been reported to contribute between 25 to 35 percent of world exports (Chen, 2006) and manufacturing, thus, emphasising their importance in the global marketplace. This being the case, significant research attention in the area of SMEs and their exporting performance, international activities and barriers to new market entry has resulted. However, little attention has been given to the decision-making processes associated with exporting (Anderson & Floren, 2004). Moreover, little is known about SME decision-makers and, in particular, the level of perceived risk they associate with international business activities. This represents a significant gap in the literature. Given this, there is a need to understand how individual characteristics (for example demographic characteristics and management style) and cultural characteristics (for example uncertainty avoidance and long-term orientation) together with exporting motivations and barriers influence SMEs decision-makers’ risk perception associated with exporting and how these may differ within emerging and advanced markets. In doing so, important theoretical and practical implications will result.
Polarization surveys of the Galaxy
Creators: name: Reich, W.
name: Fuerst, E.
name: Reich, P.
name: Wielebinski, R.
name: Wolleben, M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on sensitive 21cm and 11cm polarization surveys of the Galactic plane carried out with the Effelsberg 100-m telescope at arcmin angular resolution and some related work. Highly structured polarized emission is seen along the Galactic plane as well as up to very high Galactic latitudes. These observations reflect Faraday effects in the interstellar medium. Polarized foreground and background components along the line of sight, modified by Faraday rotation and depolarization, add in a complex way. The amplitudes of polarized emission features are highly frequency dependent. Small-scale components decrease in amplitude rapidly with increasing frequency. We stress the need for sensitive absolutely calibrated polarization data. These are essential for baseline setting and a correct interpretation of small-scale structures. Absolutely calibrated data are also needed to estimate the high-frequency polarized background. A recent study of polarized emission observed across the local Taurus-Auriga molecular cloud complexes indicates excessive synchrotron emission within a few hundred parsecs. These results suggest that possibly a large fraction of the Galactic high latitude total intensity and polarized emission is of local origin.
description: 6 pages with 2 PS figures. To be published in "Astrophysical Polarized Backgrounds", eds. S. Cecchini, S. Cortiglioni, R. Sault and C. Sbarra, AIP Conf. Proc
Coelogyne erectilabia M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne erectilabia

description: Coelogyne erectilabia (H.A.Pedersen) M.W.Chase & Schuit., comb. nov.
 Basionym: Dendrochilum erectilabium H.A.Pedersen, Nordic J. Bot. 15: 394 (1995 publ. 1996).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 110, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
A morphological comparison between the central region in AGN and normal galaxies using HST data
Creators: name: Xilouris, E. M.
name: Papadakis, I. E.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the morphology of the central region of a sample of Active Galactic Nuclei (AGN) and a ``control'' sample of normal galaxies using archival observations of the WFPC2 instrument onboard the Hubble Space Telescope (HST). We use the ellipse fitting technique in order to get a good description of the inner ``smooth'' light distribution of the galaxy. We then divide the observed galaxy image by the artificial image from the fitted ellipses in order to detect morphological signatures in the central region around the nucleus of the galaxy. We perform quantitative comparisons of different subgroups of our sample of galaxies (according to the Hubble type and the nuclear activity of the galaxies) by calculating the average amplitude of the structures that are revealed with the ellipse fitting technique. Our main conclusions are as follows: 1) All AGNs show significant structure in their inner 100 pc and 1 kpc regions whose amplitude is similar in all of them, independent of the Hubble type of the host galaxy. 2) When considering early-type galaxies, non-AGN galaxies show no structure at all, contrary to what we find for AGN. 3) When considering late-type galaxies, both AGN and non-AGN galaxies show significant structure in their central region. Our results are consistent with the hypothesis that all early-type galaxies host a supermassive black hole, but only those that have enough material in the central regions to fuel it show an active nucleus. The situation is more complicated in late-type galaxies. Either not all of them host a central black hole, or, in some of them, the material inside the innermost 100 pc region is not transported to the scales of the central engine for some reason, or the large amount of gas and dust hides the active nucleus from our sight.
description: Accepted for publication in A&A. A gziped ps file with high resolution figures is available at http://armonia.physics.uoc.gr/~xilouris/publications/pub.html
Additional results and discussion. from Profile likelihood analysis for a stochastic model of diffusion in heterogeneous media
Creators: name: Simpson, Matthew J.
name: Browning, Alexander P.
name: Drovandi, Christopher
name: Carr, Elliot J.
name: Maclaren, Oliver J.
name: Baker, Ruth E.
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: Biophysics
subject: 10299 Applied Mathematics not elsewhere classified
subject: FOS: Mathematics
subject: 19999 Mathematical Sciences not elsewhere classified

description: We compute profile likelihoods for a stochastic model of diffusive transport motivated by experimental observations of heat conduction in layered skin tissues. This process is modelled as a random walk in a layered one-dimensional material, where each layer has a distinct particle hopping rate. Particles are released at some location, and the duration of time taken for each particle to reach an absorbing boundary is recorded. To explore whether this data can be used to identify the hopping rates in each layer, we compute various profile likelihoods using two methods: first, an exact likelihood is evaluated using a relatively expensive Markov chain approach; and, second, we form an approximate likelihood by assuming the distribution of exit times is given by a Gamma distribution whose first two moments match the moments from the continuum limit description of the stochastic model. Using the exact and approximate likelihoods, we construct various profile likelihoods for a range of problems. In cases where parameter values are not identifiable, we make progress by re-interpreting those data with a reduced model with a smaller number of layers.
Coelogyne ewae M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne ewae

description: Coelogyne ewae (R.Boos, Cootes & W.Suarez) M.W.Chase & Schuit., comb. nov.
 Basionym: Dendrochilum ewae R.Boos, Cootes & W.Suarez, OrchideenJ. 21: 125 (2014).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 110, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
Porocallus sinensis PACE 2012
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Porocallus
Porocallus sinensis

description: Porocallus sinensis PACE 2012 (Map 1)
 Porocallus sinensis PACE 2012: 140.
 C o m m e n t: In the original description of P. sinensis, which is based on a single female from " China: Guangxi, Da Ming Shan" (Map 1), PACE (2012) compares the species with P. insignis, but there is no reference whatsoever to other species of the genus. The spermatheca is similar to that of P. ligo ASSING 2006 from Guizhou, but the illustration of the habitus of P. sinensis provided by PACE (2012) suggests that the pronotum is more transverse.
description: Published as part of Assing, V., 2012, A revision of Porocallus SHARP. III. A new species from China and an additional record (Coleoptera: Staphylinidae: Aleocharinae), pp. 1011-1016 in Linzer biologische Beiträge 44 (2) on page 1012, DOI: 10.5281/zenodo.5328670
Additional file 1: of Plant geographic phenotypic variation drives diversification in its associated community of a phytophagous insect and its parasitoids
Creators: name: Yu, Hui
name: Liang, Dan
name: Tian, Enwei
name: Zheng, Linna
name: Kjellberg, Finn
Publisher: name: figshare
Year: 2018
Subjects: subject: Molecular Biology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Hematology
subject: Plant Biology
subject: Virology

description: Figure S1. Neighbour joining COI phylogeny of 75 Sycoscapter individuals collected from Ficus hirta. Figure S2. Neighbour joining COI phylogeny of 70 Philotrypesis individuals collected from Ficus hirta. Figure S3. Assignation of microsatellite multilocus genotypes to cluster using STRUCTURE. Figure S4. Spatial genetic structure in Ficus hirta and its associated wasps. (PDF 252 kb)
Universal scaling of conserved charge in the stochastic diffusion dynamics
Creators: name: Wu, Shanjin
name: Song, Huichao
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: In this paper, we explore the Kibble-Zurek scaling of the conserved charge, using the stachastic diffusion dynamics. After determining the characteristic scales $τ_{kz}$ and $l_{kz}$ and properly rescaling the traditional correlation function and cumulant, we construct universal functions for both the two-point correlation function $C(y_1-y_2;τ)$ and second-order cumulant $K(Δy,τ)$ of the conserved charge in the critical regime, which are insensitive to the initial temperature and a parameter in the mapping between 3D Ising model and the hot QCD system near the critical point.
Childhood adversity and its effects on military members’ health and readiness : the mediating and moderating effects of social support
Creators: name: Paine, Christopher Michael
name: 0000-0002-8407-7130
Publisher: name: The University of Texas at Austin
Year: 2019
Subjects: Adverse childhood experience
ACE
Military
Army
Veteran
Deploy
Social support
Military cohesion
Vertical cohesion
Horizontal cohesion
Leadership
Moderation
Mediation
Mental health
Structural equation model
Regression

description: This cross-sectional study examined (a) the mediating role of several social pathways (i.e., unit cohesion, task cohesion, organizational support, positive and negative perceptions of officer and noncommissioned officer support, and anxiety in experiencing close relationships) on the relationship between adverse childhood experiences (ACEs) and service members’ mental health, and (b) the moderating effect of the aformentioned social support types on ACEs’ effect on service members’ mental health. A secondary analysis of data through structural equation modeling (SEM) and linear regression was conducted using responses from 1,285 active duty Army soldiers (1,137 males and 148 females) from a single brigade combat team (BCT) six months post-deployment. The Walter Reed Army Institute of Research (WRAIR) provided the data. SEM demonstrated that the effects of ACEs on several mental health outcomes were consistently mediated by the perceptions of poor officer and noncommissioned officer leader support and positive officer leader support, and anxiety in experiencing close relationships, but buffered by organizational support. Linear regression analyses also demonstrated that ACE’s effects on various mental health outcomes was positively or negatively moderated by distinct types of military cohesion (e.g., positive and negative officer and noncommissioned officer leadership, organizational support, anxiety in experiencing close relationships) and military cohesion appears to have a more important moderating effect among women than for men (e.g., among women, the effect of ACE on aggressive behavior and PTSD decreased as positive NCO leader support increased; and the effect of ACE on alcohol problems increased as poor NCO leader support increased). These findings broaden knowledge about ACEs as a growing antecedent for mental health problems among service members, elucidate key mechanisms through which ACEs are linked to service members’ mental health risk, and demonstrate that distinct types of vertical cohesion (i.e., organizational and supportive leader support behaviors) appear to be robust health capacity builders and military strength-multipliers.
An optical bow shock around the nearby millisecond pulsar J2124-3358
Creators: name: Gaensler, Bryan
name: Jones, Heath
name: Stappers, Ben
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of an H-alpha-emitting bow-shock nebula powered by the nearby millisecond pulsar J2124-3358. The bow shock is very broad, and is highly asymmetric about the pulsar's velocity vector. This shape is not consistent with that expected for the case of an isotropic wind interacting with a homogeneous ambient medium. Models which invoke an anisotropy in the pulsar wind, a bulk flow of the surrounding gas, or a density gradient in the ambient medium either perpendicular or parallel to the pulsar's direction of motion also fail to reproduce the observed morphology. However, we find an ensemble of good fits to the nebular morphology when we consider a combination of these effects. In all such cases, we find that the pulsar is propagating through an ambient medium of mean density 0.8-1.3 cm^(-3) and bulk flow velocity ~15-25 km/s and that the star has recently encountered an increase in density by 1-10 cm^(-3) over a scale ~<0.02 pc. The wide variety of models which fit the data demonstrate that in general there is no unique set of parameters which can be inferred from the morphology of a bow-shock nebula.
description: 6 pages, uses emulateapj, ApJ Letters, in press
Superintendents’ decision making for funding full day prekindergarten programs in schools that serve low-income families
Creators: name: Hill, Elena Sue
name: 0000-0001-6657-9084
Publisher: name: The University of Texas at Austin
Year: 2019
Subjects: Prekindergarten
Pre-kindergarten
Decision making
Low-income families
School superintendents
Superintendent decision making
Low-income schools
Prekindergarten program funding
Prekindergarten funding decisions
Low-income prekindergarten

description: While abundant literature exists that outlines the benefits of investing in prekindergarten programs for children as well as the advantages of children attending prekindergarten, attention is needed to identify how decisions are actually made to fund full day prekindergarten programs. Most studies have focused on decision making in general and some studies have focused on the decision making process regarding implementing prekindergarten. Few studies, however, have focused on decision making for funding full day prekindergarten programs for low-income families. Additional research is needed to identify decision making factors and considerations that superintendents use to make decisions to fund full day prekindergarten programs. Therefore, this study identified characteristics superintendents use to describe their decision making processes and factors that were considered when making decisions for funding prekindergarten. Three questions guided the study: 1) How do superintendents characterize their decision making processes for funding full day prekindergarten programs serving low-income families? 2) What factors do superintendents consider to make full day prekindergarten funding decisions? 3) How do superintendents’ decision making practices, regarding funding for full day prekindergarten reflect rational decision making? A purposeful sampling method was used to select three superintendents for this study who had experience with decision making regarding funding for full day prekindergarten programs at the district level, had a minimum of two years in their role as superintendent, and who serve in large public school systems of at least 25,000 students. Face to face interviews, document analysis and observations were the primary data collection protocols. Findings suggest that superintendents characterize their decision making as collaborative, data-driven, and priority based. This study also found that superintendents appear to consider accessibility to high-quality education, benefit to community and sources of funding as factors when making decisions to fund full day prekindergarten. Further, a comparative analysis of the rational decision making framework and the decision making practices of superintendents suggest that the steps of a rational decision making process are completed to some extent. This study provides insight and information for practicing superintendents who attempt to make decisions for funding full day prekindergarten. Finally, given the nature and findings of the present study, recommendations for practice and further research are offered
Energy and Flavor Discrimination Using Precision Time Structure in On-Axis Neutrino Beams
Creators: name: Angelico, Evan
name: Eisch, Jonathan
name: Elagin, Andrey
name: Frisch, Henry
name: Nagaitsev, Sergei
name: Wetstein, Matthew
Publisher: name: arXiv
Year: 2019
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We propose to use a higher-frequency RF bunch structure for the primary proton beam on target and precision timing to select different energy and flavor spectra from a wide-band neutrino beam, based on the relative arrival times of the neutrinos with respect to the RF bunch structure. This `stroboscopic' approach is complementary to techniques that select different neutrino energy spectra based on the angle with respect to the beam axis. A timing-based approach allows for the selection of varying energy spectra from the same on-axis detector, and applies equally to both the near and far detectors in an oscillation experiment. Energy and flavor discrimination of neutrinos produced by hadrons in-flight will require proton bunch lengths on the order of 100 ps and commensurate time resolution in the detector. Correlating neutrino events with the parent proton interaction is currently limited by the nanosecond-scale width of the proton bunches impinging on the target. We show that these limitations can be addressed by using a superconducting RF cavity to rebunch the present 53.1 MHz RF bunch structure with a factor of 10 higher RF frequency, thus attaining the required shorter bunch length.
description: 12 pages, 11 figures
Additional file 1 of Evaluation of home detection algorithms on mobile phone data using individual-level ground truth
Creators: name: Pappalardo, Luca
name: Ferres, Leo
name: Sacasa, Manuel
name: Cattuto, Ciro
name: Bravo, Loreto
Publisher: name: figshare
Year: 2021
Subjects: subject: Information Systems
subject: FOS: Computer and information sciences

description: The pdf file entitled “Supplementary material for Evaluation of Home Detection Algorithms on Mobile Phone Datausing Individual-Level Ground Truth” contains extra details about the computation carried out in the main text. (PDF 1.1 MB)
X-Ray Beaming due to Resonance Scattering in the Accretion Column of Magnetic Cataclysmic Variables
Creators: name: Terada, Yukikatsu.
name: Ishida, M.
name: Makishima, K.
name: Imanari, T.
name: Fujimoto, R.
name: Matsuzaki, K.
name: Kaneda, H.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Extremely strong ionized Fe emission lines, with the equivalent width reaching about 4000 eV, were discovered with ASCA from a few Galactic compact objects, including AX J2315-0592, RX J1802.1+1804 and AX J1842.8-0423. These objects are thought to be binary systems containing magnetized white dwarfs (WDs). A possible interpretation of the strong Fe-K line is the line-photon collimation in the WD accretion column, due to resonance scattering of line photons. The collimation occurs when the accretion column has a flat shape, and the effect is augmented by the vertical velocity gradient there, which reduces the resonant trapping of resonant photons along the magnetic field lines. This effect was quantitatively confirmed with Monte-Carlo simulations. Furthermore, with ASCA observations of the polar V834 Centauri, this collimation effect was clearly detected as a rotational modulation of the equivalent width of the Fe-K emission line. Extremely strong emission lines mentioned above can be explained by our interpretation consistently. Combing this effect with other X-ray information, the geometry and plasma parameters in the accretion column were determined.
description: 16 pages, Postscript, 32 figures, and 4 tables; accepted for MNRAS (Monthly Notices of The Royal Astronomical Society) on July 24, 2001
MOESM7 of Internalization and accumulation of model lignin breakdown products in bacteria and fungi
Creators: name: Barnhart-Dailey, Meghan
name: Dongmei Ye
name: Hayes, Dulce
name: Danae Maes
name: Simoes, Casey
name: Appelhans, Leah
name: Carroll-Portillo, Amanda
name: Kent, Michael
name: Timlin, Jerilyn
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Additional file 7: Figure S6. A. ASAP-MS representative spectra of S. cerevisiae lysates incubated with vanillic acid for 1, 2, 3, or 17 h. Blue arrow indicates integrated peak of interest for results displayed in Fig. 4c. B. ASAP-MS representative chromatogram of P. chrysosporium lysates incubated with vanillic acid for 1, 2, 4, or 24 h. Orange arrow indicates integrated peak of interest for results displayed in Fig. 4b. C. ASAP-MS representative chromatogram of P. chrysosporium lysates incubated with 13C labeled vanillic acid for 1, 2, 4, or 24 h. Red arrow indicates integrated peak of interest for results displayed in Fig. 4b. D. ASAP-MS representative chromatogram of P. chrysosporium lysates incubated with vanillic acid for 5, 15, and 60 min. Orange arrow indicates integrated peak of interest for results displayed in Fig. 4b.
Additional file 6 of Characteristics and interplay of esophageal microbiota in esophageal squamous cell carcinoma
Creators: name: Lin, Zheng
name: Rao, Wenqing
name: Xiang, Zhisheng
name: Zeng, Qiaoyan
name: Liu, Shuang
name: Yu, Kaili
name: Zhou, Jinsong
name: Wang, Jianwen
name: Chen, Weilin
name: Chen, Yuanmei
name: Peng, Xiane
name: Hu, Zhijian
Publisher: name: figshare
Year: 2022
Subjects: Physical Sciences not elsewhere classified
Medicine
Cell Biology
Chemical Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Cancer

description: Additional file 6: Table S4. The corresponding description of the differential MetaCyc metabolic pathways.
Introductory review to the historical development of modern cosmology
Creators: name: Martinez, Vicent J.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This talk introduces the contributions of the lecturers to the international summer school ``Historical Development of Modern Cosmology'' held at the Universidad Internacional Menéndez Pelayo, Valencia, Spain, during September 18-22 2000.
description: 8 pages, 3 eps figures (included in the main file) and 3 separated gif figures. Conference proceedings
Eusarima Yang 1994
Creators: name: Gnezdilov, Vladimir M.
name: Mozaffarian, Fariba
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Issidae
Eusarima

description: Genus Eusarima Yang, 1994
 Eusarima Yang, 1994 in CHAN & YANG (1994): 108. Type species: Eusarima contorta Yang, 1994 in CHAN & YANG (1994), by original designation.
 Nepalius Dlabola, 1997:309. Type species: Nepalius hellerianus Dlabola, 1997, by original designation.Synonymised under Eusarima Yang, 1994 by GNEZDILOV (2009): 84.
 Diagnosis. Metope with complete median and sublateral carinae joining below or at its upper margin. Fore wing with or without hypocostal plate; radius and cubitus anterior bifurcate, media tri- or tetrafurcate (R 2 M 3–4 CuA 2). Hind wing with two clefts; radius and first anal vein bifurcate, media, cubitus posterior, postcubitus, and second anal vein simple, cubitus anterior bi- or trifurcate (R 2, M 1, CuA 2–3, CuP 1, Pcu 1, A 1 2 and A 2 1); cubitus anterior and posterior fused apically. Each dorso-lateral lobe of phallobase with elongate subapical process directed apically. Style with small capitulum.
description: Published as part of Gnezdilov, Vladimir M. & Mozaffarian, Fariba, 2011, A new species of the genus Eusarima (Hemiptera: Fulgoroidea: Issidae) from Iran, pp. 457-462 in Acta Entomologica Musei Nationalis Pragae 51 (2) on page 458, DOI: 10.5281/zenodo.5328684