cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Developments in Cosmic Growth and Gravitation
Creators: name: Linder, Eric V.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Cosmic surveys of large scale structure have imaged hundreds of millions of galaxies and mapped the 3D positions of over a million. Surveys starting over the next few years will increase these numbers more than tenfold. Simultaneously, developments in extracting information on dark energy, dark matter, neutrinos, and gravity on cosmic scales have advanced greatly, with many important works from Asia Pacific institutions.
description: 7 pages; overview for Association of Asia Pacific Physical Societies
The photoionization effect of the ultraviolet background on the colour-magnitude relation of elliptical galaxies
Creators: name: Nagashima, M.
name: Gouda, N.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examined effects of the ultraviolet background radiation (UVB) on the colour--magnitude relation (CMR) of elliptical galaxies in clusters of galaxies in the hierarchical clustering scenario by using a semi-analytic model of galaxy formation. In our model the UVB photoionizes gas in dark haloes and suppresses the cooling of the diffuse hot gas onto galaxy discs. By using a semi-analytic model without the effect of the UVB, Kauffmann & Charlot found that the CMR can be reproduced by strong supernova heating because such supernova feedback suppresses the chemical enrichment in galaxies especially for small galaxies. We find that the CMR also becomes bluer because of the UVB, in a different way from the effect of supernova feedback. While the supernova feedback suppresses the chemical enrichment by a similar mechanism to galactic wind, the UVB suppresses the cooling of the hot gas. This fact induces the suppression of the metallicity of the intracluster medium (ICM). In our model we find that the existence of the UVB can plausibly account for an observed ICM metallicity that is equal to nearly 0.3 times the solar value, and that in this case we can reproduce the CMR and the metallicity of the ICM simultaneously.
description: 5 pages, 3 figures, LaTeX, MNRAS pink pages in press
Syscia persimilis Longino & Branstetter 2021, New Species
Creators: name: Longino, John T.
name: Branstetter, Michael G.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Syscia
Syscia persimilis

description: Syscia persimilis, New Species
Figure 10 (map, worker), S44 (holotype worker), S45 (queen), S46 (intercaste female)
 Holotype: 1 worker, NICARAGUA, Jinotega: RN Cerro Kilambé, 13.57028 −85.69737 ± 20m, 1500m, 23-May-2011, cloud forest, ex sifted leaf litter (LLAMA, Wa-D-05-1-26) [CASC, unique specimen identifier CASENT0630852]. PARATYPES: same data as holotype [worker: MCZC]; same data except 13.56924 −85.69746 ± 10m, 1500m, 23-May-2011, cloud forest, ex sifted leaf litter (LLAMA, Wa-D-05-1-03) [intercaste female: CASC; worker: USNM]; same data except 13.56726 −85.69782 ± 15m, 1400m, 23-May-2011, cloud forest, ex sifted leaf litter (LLAMA, Wa-D-05-2-27) [worker: UCD].
description: Published as part of Longino, John T. & Branstetter, Michael G., 2021, Integrating UCE Phylogenomics With Traditional Taxonomy Reveals a Trove of New World Syscia Species (Formicidae: Dorylinae), pp. 1-51 in Insect Systematics and Diversity 5 (2) on page 31, DOI: 10.1093/isd/ixab001, http://zenodo.org/record/5384404
Synoicum georgianum Sluiter 1932
Creators: name: Sanamyan, K. E.
name: Sanamyan, N. P.
Publisher: name: Zenodo
Year: 2002
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Ascidiacea
Aplousobranchia
Polyclinidae
Synoicum
Synoicum georgianum

description: Synoicum georgianum Sluiter, 1932
(®gure 1A)
 Synoicum georgianum Sluiter, 1932: 11; Millar, 1960: 47; 1968: 9; Monniot, 1970: 333; Vasseur, 1974: 615; Monniot and Gaill, 1978: 155; Monniot and Monniot, 1983: 32.
 Aplidiopsis georgianum: Kott, 1969: 73; 1971: 32.
description: Published as part of Sanamyan, K. E. & Sanamyan, N. P., 2002, Deep-water ascidians from the south-western Atlantic (RV Dmitry Mendeleev, cruise 43 and Academic Kurchatov, cruise 11), pp. 305-359 in Journal of Natural History 36 (3) on page 307, DOI: 10.1080/00222930010004232, http://zenodo.org/record/5299679
Additional file 4: of What do healthcare professionals need to turn risk models for type 2 diabetes into usable computerized clinical decision support systems? Lessons learned from the MOSAIC project
Creators: name: Fico, Giuseppe
name: Hernanzez, Liss
name: Cancela, Jorge
name: Dagliati, Arianna
name: Sacchi, Lucia
name: Martinez-Millana, Antonio
name: Posada, Jorge
name: Manero, Lidia
name: VerdĂş, Jose
name: Facchinetti, Andrea
name: Ottaviano, Manuel
name: Zarkogianni, Konstantia
name: Nikita, Konstantina
name: Groop, Leif
name: Gabriel-Sanchez, Rafael
name: Chiovato, Luca
name: Traver, Vicente
name: Merino-Torres, Juan
name: Cobelli, Claudio
name: Bellazzi, Riccardo
name: Arredondo, Maria
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy

description: AHP Questionnaire - Solution 2.2. (DOCX 836 kb)
Extended Red Emission in the "Evil Eye" Galaxy (NGC4826)
Creators: name: Pierini, D.
name: Majeed, A.
name: Boroson, T. A.
name: Witt, A. N.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We obtained low-resolution, long-slit 5300--9100 A spectroscopy of NGC4826 (a nearby galaxy with an absorbing dust lane (DL) asymmetrically placed across its bulge, associated with several HII regions) with a slit encompassing its bulge, positioned across its nucleus. The wavelength-dependent effects of absorption and scattering by dust in the lane are evident when comparing the observed stellar SEDs of pairs of positions symmetrically located with respect to the nucleus, one on the DL side and one on the opposite side of the bulge, by assuming that the intrinsic ISRF is axi-symmetric. We analyzed these SED ratios through the multiple-scattering radiative transfer model of Witt and Gordon and we discovered strong residual Extended Red Emission (ERE) from a region of the DL within a distance of 13 arcsec from the nucleus, adjacent to a broad, bright HII region. ERE is an established phenomenon in the literature interpreted as originating from photoluminescence by nanometer-sized clusters, illuminated by UV/optical photons. The complex radial variation of the ERE band-integrated intensity and of the ERE-to-scattered light band-integrated intensity ratio with the optical depth of the model derived for the DL and with the strength and hardness of the illuminating ISRF is reproduced consistently through the theoretical interpretation of the photophysics of the ERE carrier by Smith and Witt. When examined within the context of ERE observations in a variety of Galactic dusty environments (e.g. the diffuse ISM, reflection nebulae, planetary nebulae and the Orion Nebula), we conclude that the ERE photon conversion efficiency in NGC4826 is as high as found elsewhere, but that the size of the actively luminescing nanoparticles there is about twice as large as those thought to exist in the Galactic diffuse ISM.
description: 57 pages, 11 Postscript figures, accepted for publication in ApJ
title: Ochrona danych osobowych w wybranych państwach Azji
Creators: name: Abu Gholeh, Magdalena
name: Kuźnicka-Błaszkowska, Dominika
Publisher: name: E-Wydawnictwo. Prawnicza i Ekonomiczna Biblioteka Cyfrowa. Wydział Prawa, Administracji i Ekonomii Uniwersytetu Wrocławskiego
Year: 2019

description: Personal data protection and individual’s right to privacy are one of the most important issues in recent years. In order to ensure the informational autonomy of individuals the European Parliament and the Council have introduced the Regulation 2016/679 of the European Parliament and of the Council of 27 April 2016 on the protection of natural persons with regard to the processing of personal data and on the free movement of such data, and repealing Directive 95/46/EC (General Data Protection Regulation). The basic aim of this legislation is to ensure the effective protection of personal data, as well as to harmonize and enhance the EU’s internal market. However the regulation would not be able to achieve those goals without adequate provisions applicable to processors and controllers from countries outside the Union that offer goods and services to data subjects who are in the EU. This monograph aims at examining whether the use of services provided by Asian entrepreneurs ensures the security of personal data processing.

description: Ochrona danych osobowych i prawa do prywatności jednostki to jeden z najbardziej istotnych problemów ostatnich lat. W celu zapewnienia szerokich gwarancji autonomii informacyjnej jednostki, Parlament Europejski i Rada przyjęły rozporządzenie Parlamentu Europejskiego i Rady (UE) 2016/679 z dnia 27 kwietnia 2016 r. w sprawie ochrony osób fizycznych w związku z przetwarzaniem danych osobowych i w sprawie swobodnego przepływu takich danych oraz uchylenia dyrektywy 95/46/WE (ogólne rozporządzenie o ochronie danych, RODO). Jego celem oprócz zapewnienia efektywnej i skutecznej ochrony danych osobowych jest również harmonizacja i wzmocnienie rynku wewnętrznego UE. Jednocześnie regulacja nie osiągnie swoich celów, jeśli nie zagwarantuje się ochrony prawa do prywatności i danych osobowych przez podmioty, które pochodząc z poza Unii Europejskiej dostarczają towary i usługi jej obywatelom i instytucjom.Prezentowana monografia ma na celu zbadanie, czy korzystanie z usług dostarczanych przez przedsiębiorców pochodzących z państw azjatyckich gwarantuje bezpieczeństwo przetwarzanych danych osobowych.
Embedded nonlinear model predictive control for obstacle avoidance using PANOC
Creators: name: Sathya, Ajay
name: Sopasakis, Pantelis
name: Van Parys, Ruben
name: Themelis, Andreas
name: Pipeleers, Goele
name: Patrinos, Panagiotis
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optimization and Control (math.OC)
subject: FOS: Mathematics

description: We employ the proximal averaged Newton-type method for optimal control (PANOC) to solve obstacle avoidance problems in real time. We introduce a novel modeling framework for obstacle avoidance which allows us to easily account for generic, possibly nonconvex, obstacles involving polytopes, ellipsoids, semialgebraic sets and generic sets described by a set of nonlinear inequalities. PANOC is particularly well-suited for embedded applications as it involves simple steps, its implementation comes with a low memory footprint and its fast convergence meets the tight runtime requirements of fast dynamical systems one encounters in modern mechatronics and robotics. The proposed obstacle avoidance scheme is tested on a lab-scale autonomous vehicle.
An alternative search for the electron capture of Te-123
Creators: name: Muenstermann, D.
name: Zuber, K.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: A search for the electron capture of Te-123 has been performed using CdZnTe detectors. After a measuring time of 195 h no signal could be found resulting in a lower half-life limt of $T_{1/2} > 3.2 \cdot 10^{16}$ yrs (95 % CL) for this process. This clearly discriminates between existing experimental results which differ by six orders of magnitude and our data are in strong favour of the result with longer half-lifes.
description: 2 pages, 2 eps-figures, reanalysis of data sets
van der Waals forces stabilize low-energy polymorphism in B2O3: Implications for the crystallization anomaly
Creators: name: Ferlat, Guillaume
name: Hellgren, Maria
name: Coudert, François-Xavier
name: Hay, Henri
name: Mauri, Francesco
name: Casula, Michele
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: The cohesive energies and structural properties of recently predicted, and never synthesized, B$_2$O$_3$ polymorphs are investigated from first principles using density functional theory and high-accuracy many-body methods, namely, the random phase approximation and quantum Monte Carlo. We demonstrate that the van der Waals forces play a key role in making the experimentally known polymorph (B$_2$O$_3$-I) the lowest in energy, with many competing metastable structures lying only a few kcal/mol above. Remarkably, all metastable crystals are comparable in energy and density to the glass, while having anisotropic and mechanically soft structures. Furthermore, the best metastable polymorph according to our stability criteria has a structural motif found in both the glass and a recently synthesized borosulfate compound. Our findings provide new perspectives for understanding the B$_2$O$_3$ anomalous behavior, namely, its propensity to vitrify in a glassy structure drastically different from the known crystal.
Syscia pervagata Longino & Branstetter 2021, New Species
Creators: name: Longino, John T.
name: Branstetter, Michael G.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Syscia
Syscia pervagata

description: Syscia pervagata, New Species
Figure 9 (map, worker), S47 (holotype worker), S48 (alate queen), S49 (dealate queen), S50 (male)
 Holotype: 1 worker, HONDURAS, Atlántida: 12km SW La Ceiba, 15.69449 −86.86307 ± 20m, 200m, 19-Jun-2010, tropical rainforest, ex sifted leaf litter (LLAMA, Wa-C-09-1-32) [CASC, unique specimen identifier CASENT0644356]. PARATYPES: same data as holotype [male: CASC; worker: CASC, DZUP, JTLC, MCZC, UCD, UNAM, USNM].
description: Published as part of Longino, John T. & Branstetter, Michael G., 2021, Integrating UCE Phylogenomics With Traditional Taxonomy Reveals a Trove of New World Syscia Species (Formicidae: Dorylinae), pp. 1-51 in Insect Systematics and Diversity 5 (2) on page 32, DOI: 10.1093/isd/ixab001, http://zenodo.org/record/5384404
Gap Size Effects for the Kelvin-Helmholtz Instability in a Hele-Shaw Cell
Creators: name: Meignin, Laurent
name: Ern, Patricia
name: Gondret, Philippe
name: Rabaud, Marc
Publisher: name: arXiv
Year: 2001
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We report experimental results for the Kelvin-Helmholtz instability between two immiscible fluids in parallel flow in a Hele-Shaw cell. We focus our interest on the influence of the gap size between the walls on the instability characteristics. Experimental results show that the instability threshold, the critical wavelength, the phase velocity and the spatial growth rate depend on this gap size. These results are compared to both the previous two-dimensional analysis of Gondret and Rabaud (1997) and the three-dimensional analysis recently derived by Plourabou=E9 and Hinch (2001), showing that the agreement is still not complete especially when gap size increases.
description: 22 pages, 9 figures, accepted in Physical Review E
Data availability - Silicon isotopic fractionation under water stress in Sorghum bicolor: evidence from in situ morphotype-specific phytolith analysis - version 1
Creators: name: D'Agostini, Francesca
name: Frick, Daniel A.
name: Varalli, Alessandra
name: Ruiz Giralt, Abel
name: Madella, Marco
name: Lancelotti, Carla
Publisher: name: Zenodo
Year: 2025
Subjects: subject: Sorghum/chemistry
subject: Sorghum/physiology
subject: Sorghum/growth & development
subject: Sorghum/anatomy & histology
subject: phytoliths
subject: Water stress
subject: Silicon Dioxide
subject: silicon isotopes
subject: fsLA-MC-ICP-MS

description: Data availability for Silicon isotopic fractionation under water stress in Sorghum bicolor: evidence from in situ morphotype-specific phytolith analysis 

Authors: Francesca D’Agostini, Daniel A. Frick, Alessandra Varalli, Abel Ruiz-Giralt, Marco Madella, Carla Lancelotti 

This repository contains all the supplementary information cited in the manuscript and the original dataset. 

Contents:

File S1 - Si_isotopes.xlsx: excel file including silicon isotopical values of each phytolith measured, physiological data (weekly transpiration rate and water added and biomass values for each sample analysed) soil elemental composition, and associated metadata.

File S2 - SiliconISO.R:  R code that includes all the scripts used for statistics and data visualisation.

File S3 - Model Metrics and raw data: supplementary material
Data availability - Silicon isotopic fractionation under water stress in Sorghum bicolor: evidence from in situ morphotype-specific phytolith analysis
Creators: name: D'Agostini, Francesca
name: Frick, Daniel A.
name: Varalli, Alessandra
name: Ruiz Giralt, Abel
name: Madella, Marco
name: Lancelotti, Carla
Publisher: name: Zenodo
Year: 2025
Subjects: subject: Sorghum/chemistry
subject: Sorghum/physiology
subject: Sorghum/growth & development
subject: Sorghum/anatomy & histology
subject: phytoliths
subject: Water stress
subject: Silicon Dioxide
subject: silicon isotopes
subject: fsLA-MC-ICP-MS

description: Data availability for Silicon isotopic fractionation under water stress in Sorghum bicolor: evidence from in situ morphotype-specific phytolith analysis 

Authors: Francesca D’Agostini, Daniel A. Frick, Alessandra Varalli, Abel Ruiz-Giralt, Marco Madella, Carla Lancelotti 

This repository contains the original dataset and the R script cited in the manuscript. 

Contents:

File S1 - Si_isotopes.xlsx: excel file including silicon isotopical values of each phytolith measured, physiological data (weekly transpiration rate and water added and biomass values for each sample analysed) soil elemental composition, and associated metadata.

File S2 - SiliconISO.R:  R code that includes all the scripts used for statistics and data visualisation.
Additional file 3: of What do healthcare professionals need to turn risk models for type 2 diabetes into usable computerized clinical decision support systems? Lessons learned from the MOSAIC project
Creators: name: Fico, Giuseppe
name: Hernanzez, Liss
name: Cancela, Jorge
name: Dagliati, Arianna
name: Sacchi, Lucia
name: Martinez-Millana, Antonio
name: Posada, Jorge
name: Manero, Lidia
name: VerdĂş, Jose
name: Facchinetti, Andrea
name: Ottaviano, Manuel
name: Zarkogianni, Konstantia
name: Nikita, Konstantina
name: Groop, Leif
name: Gabriel-Sanchez, Rafael
name: Chiovato, Luca
name: Traver, Vicente
name: Merino-Torres, Juan
name: Cobelli, Claudio
name: Bellazzi, Riccardo
name: Arredondo, Maria
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy

description: AHP Questionnaire - Solution 2.1. (DOCX 836 kb)
Black Holes and Hosts of Active and Quiescent Galaxies: I. The Black Hole-Bulge Relation revisited
Creators: name: Wandel, Amri
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Massive Black Holes detected in the centers of many nearby galaxies show an approximately linear relation with the luminosity of the host bulge, with the black hole mass being 0.001-0.002 of the bulge mass. Previous work suggested that black holes of active (Seyfert 1) galaxies follow a similar relation, but apparently with a significantly lower value of $M_{\rm BH}/M_{\rm bulge}$ (Wandel 1999). New data show that this difference was mainly due to overestimating the black hole mass in quiescent galaxies and overestimating the bulge magnitude of Seyfert galaxies. Using new and updated data we show that AGNs (Seyfert galaxies and quasars) follow the same BH-bulge relation as ordinary (inactive) galaxies. We derive the BH-bulge relation for a sample of 55 AGNs and 35 quiescent galaxies, finding that broad line AGNs have an average black hole/bulge mass fraction of $\sim 0.0015$ with a strong correlation (Mbh ~ Lbulge^{0.9\pm 0.16}). This BH-bulge relation is consistent with the BH-bulge relation of quiescent galaxies and much tighter than previous results. Narrow line AGNs appear to have a lower ratio, Mbh/Mbulge ~ 10^{-4}-10^{-3}. We find this to be a more general feature, the BH/bulge ratio in AGNs being inversely correlated with the emission-line width, implying a strong linear relation between the size of the broad emission line region and the luminosity of the bulge. Finally, combining AGNs with observed and estimated stellar velocity dispersion, we find a significant correlation (Mbh ~ v^{3.5-5}), consistent with that of quiescent galaxies.
description: 11 pages, 7 figures, accepted for publication in the Astrophysical Journal, submitted July 11
Additional file 2: of What do healthcare professionals need to turn risk models for type 2 diabetes into usable computerized clinical decision support systems? Lessons learned from the MOSAIC project
Creators: name: Fico, Giuseppe
name: Hernanzez, Liss
name: Cancela, Jorge
name: Dagliati, Arianna
name: Sacchi, Lucia
name: Martinez-Millana, Antonio
name: Posada, Jorge
name: Manero, Lidia
name: VerdĂş, Jose
name: Facchinetti, Andrea
name: Ottaviano, Manuel
name: Zarkogianni, Konstantia
name: Nikita, Konstantina
name: Groop, Leif
name: Gabriel-Sanchez, Rafael
name: Chiovato, Luca
name: Traver, Vicente
name: Merino-Torres, Juan
name: Cobelli, Claudio
name: Bellazzi, Riccardo
name: Arredondo, Maria
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy

description: AHP Questionnaire - Solution 1. (DOCX 836 kb)
Uncertainty-aware demand management of water distribution networks in deregulated energy markets
Creators: name: Sopasakis, Pantelis
name: Sampathirao, Ajay K.
name: Bemporad, Alberto
name: Patrinos, Panagiotis
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optimization and Control (math.OC)
subject: FOS: Mathematics

description: We present an open-source solution for the operational control of drinking water distribution networks which accounts for the inherent uncertainty in water demand and electricity prices in the day-ahead market of a volatile deregulated economy. As increasingly more energy markets adopt this trading scheme, the operation of drinking water networks requires uncertainty-aware control approaches that mitigate the effect of volatility and result in an economic and safe operation of the network that meets the consumers' need for uninterrupted water supply. We propose the use of scenario-based stochastic model predictive control: an advanced control methodology which comes at a considerable computation cost which is overcome by harnessing the parallelization capabilities of graphics processing units (GPUs) and using a massively parallelizable algorithm based on the accelerated proximal gradient method.
description: Drinking water networks, Bid-based energy market, Stochastic model predictive control, Graphics processing units, Scenario trees, Open-source software
Additional file 1: of What do healthcare professionals need to turn risk models for type 2 diabetes into usable computerized clinical decision support systems? Lessons learned from the MOSAIC project
Creators: name: Fico, Giuseppe
name: Hernanzez, Liss
name: Cancela, Jorge
name: Dagliati, Arianna
name: Sacchi, Lucia
name: Martinez-Millana, Antonio
name: Posada, Jorge
name: Manero, Lidia
name: VerdĂş, Jose
name: Facchinetti, Andrea
name: Ottaviano, Manuel
name: Zarkogianni, Konstantia
name: Nikita, Konstantina
name: Groop, Leif
name: Gabriel-Sanchez, Rafael
name: Chiovato, Luca
name: Traver, Vicente
name: Merino-Torres, Juan
name: Cobelli, Claudio
name: Bellazzi, Riccardo
name: Arredondo, Maria
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Neuroscience
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy
subject: Computational Biology

description: Detailed information on Lean Canvas, Focus Groups and Use Cases. (DOCX 20 kb)
Facilitated catalytic ozonation of atrazine over highly stabilized Zn-Al Layered Double Oxides composites: Efficacy and mechanism
Creators: name: Li, Shangkun
name: Li, Yangang
name: Sun, Lei
name: Pan, Fei
name: Yuan, Xiangjuan
name: Xia, Dongsheng
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified

description: A series of Zn-Al Layered Double Oxides (ZnAl-LDO) composites were prepared by the hydrothermal and calcination method via employing the Zn-Al Layered Double Hydroxide (ZnAl-LDH) as the precursors in the present study. The structural properties and the catalytic ozonation activity of ZnrAl-T composites synthesized with different Zn/Al molar ratios and calcination temperatures were systematically investigated. Diversified characterizations were applied to analyze the phase structure and chemical composition of ZnrAl-T composites. As the calcination temperature increased, the layered ZnAl-LDH structure could be entirely destroyed and the crystallinity gradually improved. With the Zn/Al mole ratio of 4.0 and calcination temperature of 500°C, the Zn4Al-500 composite obtained the outstanding catalytic ozonation performance for atrazine (ATZ) degradation with the pseudo-first-order constant of 0.5080 min−1, which was 5 times more than that in O3 alone. Meanwhile, the ATZ degradation efficiency was gradually enhanced from 44.1% to 99.9% within 3.0 min when the solution pH ranged from 3.0 to 10.0. Besides, the Zn4Al-500 composite exhibited splendid stability over multiple reaction cycles. In addition, the radical scavenging test and electron spin resonance measurement demonstrated that superoxide radical and hydroxyl radical are the dominant reactive species in O3/Zn4Al-500 process. Moreover, nineteen and ten transformation products were detected in O3 alone and O3/Zn4Al-500 process, and possible degradation pathways of ATZ were further elucidated. Overall, the Zn4Al-500 composite would provide a potential alternative for pollutants removal due to its high catalytic ozonation efficiency, stability, and reusability.
Detection of white dwarf spin period variability in the intermediate polar V2306 Cygni
Creators: name: Breus, V.
name: Petrik, K.
name: Zola, S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Magnetic cataclysmic variables are close binaries which consist of a compact object - a white dwarf - and a red dwarf filling its Roche Lobe. Such systems are physical laboratories which enable study of the influence of magnetic fields on matter flows. They often exhibit spin-up or spin-down of the white dwarf, while some systems exhibit more complex behaviour of the spin period change. We monitor changes of the spin periods of white dwarfs in a sample of close binary systems to study interaction of the magnetic field and accretion processes as well as evolution of intermediate polars. Within the framework of our intermediate polar monitoring program, we obtained photometric CCD observations at several observatories. Two-period trigonometric polynomial fitting was used for determination of extrema timings. The (O-C) analysis was performed to study the variability of the orbital and spin periods of the systems. Using data taken during 9 years of observations of the magnetic cataclysmic variable V2306 Cygni (formerly known as 1WGA J1958.2+3232), we detected the spin period variability which shows a spin-up of the white dwarf with a characteristic time of $(53\pm5)\cdot10^4$ years. The value of the spin period was $733.33976$ seconds with the formal accuracy of $0.00015$ seconds. We derived an improved value of the orbital period of the system to be $4.371523\pm0.000009$ hours.
description: Accepted to MNRAS 2019 July 23. 5 pages, 3 figures, supporting data online
Syscia pollula Longino & Branstetter 2021, New Species
Creators: name: Longino, John T.
name: Branstetter, Michael G.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Syscia
Syscia pollula

description: Syscia pollula, New Species
Figure 8 (map, worker), S53 (holotype worker), S54 (queen), S55 (brachypterous queen)
 Holotype: 1 worker, NICARAGUA, Matagalpa: RN Cerro Musún, 12.96817 −85.23301 ± 20m, 1060m, 2-May-2011, montane wet forest, ex sifted leaf litter (LLAMA, Wm-D-01-1-07) [CASC, unique specimen identifier CASENT0624110]. PARATYPES: NICARAGUA, Matagalpa: RN Cerro Musún, 12.96087 −85.2329 ± 10m, 750m, 1-May-2011, tropical wet forest, ex sifted leaf litter (LLAMA, Wa-D-01-1-10) [worker: MCZC, USNM]; RN Cerro Musún, 12.95884 −85.22486 ± 10m, 700m, 1-May-2011, tropical wet forest, ex sifted leaf litter (LLAMA, Wa-D-01-2-14) [worker: CASC].
description: Published as part of Longino, John T. & Branstetter, Michael G., 2021, Integrating UCE Phylogenomics With Traditional Taxonomy Reveals a Trove of New World Syscia Species (Formicidae: Dorylinae), pp. 1-51 in Insect Systematics and Diversity 5 (2) on page 34, DOI: 10.1093/isd/ixab001, http://zenodo.org/record/5384404
Radioactivities and nucleosynthesis in SN 1987A
Creators: name: Fransson, Claes
name: Kozma, Cecilia
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The nucleosynthesis and production of radioactive elements in SN 1987A are reviewed. Different methods for estimating the masses of 56Ni, 57Ni, and 44Ti are discussed, and we conclude that broad band photometry in combination with time-dependent models for the light curve gives the most reliable estimates.
description: 8 pages, 4 figs. Proceedings of the workshop "Astronomy with Radioactivities III", special issue of the "New Astronomy Reviews"
Proagnesia depressa
Creators: name: Sanamyan, K. E.
name: Sanamyan, N. P.
Publisher: name: Zenodo
Year: 2002
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Ascidiacea
Phlebobranchia
Agneziidae
Proagnesia
Proagnesia depressa

description: Proagnesia depressa (Millar, 1955)
(®gures 15A, 16B)
 Agnesia depressa Millar, 1955: 223.
 Proagnesia depressa: Monniot and Monniot, 1973: 418; 1974: 739.
 Material examined. St. 4077, 3285± 3160 m, one specimen; st. 4104, 5110±5120 m, one specimen.
 Description. The specimens are strongly contracted and are about 1 cm in diameter. The basal half is hemispherical with thin test. The upper surface is ¯attened, oval and covered by thicker and more rigid test. The apertures are on short siphons on the upper disk. The area around and between the siphons is covered by short thick crowded papillae, but the remainder of the upper disk is covered by long outgrowths which are sparse on the lower part of the body (which apparently was immersed in soft mud).
Thin crowded circular muscles are present around the apertures, and a conspicuous band of long thick parallel transverse muscles crosses the dorsal surface between the apertures and posterior to the atrial siphon. They closely resemble those ®gured by Monniot and Monniot (1974). We have not found any tentacles. The prepharyngeal band is composed of a single lamella and the dorsal V is absent. The neural ganglion and oval neural gland are halfway between the siphons. There are four long dorsal languets. The branchial sac has four high transverse vessels without papillae. Some stigmata spiral, but mostly they are irregular and it is not possible to count either the number per row, or the number of rows between two transverse vessels.
The gut loop makes a complete circle and the rectum is directed away from the atrial siphon. The stomach is relatively large, oval and smooth-walled. The anal border has long ®nger-like lobes. The gonad is in the gut loop, but gonoducts were not detected.
 Remarks. The orientation of the rectum is probably an artefact. In previously described specimens the proximal part of the gut forms the usual loop and the rectum is, as usual, directed to the atrial aperture. The other features, especially the structure of the branchial sac and body muscles, are in agreement with existing accounts.
This is the ®rst record of the species from Antarctic waters. It was previously known from numerous records from the northern and central Atlantic, around South Africa and from central and northern parts of the Indian Ocean.
description: Published as part of Sanamyan, K. E. & Sanamyan, N. P., 2002, Deep-water ascidians from the south-western Atlantic (RV Dmitry Mendeleev, cruise 43 and Academic Kurchatov, cruise 11), pp. 305-359 in Journal of Natural History 36 (3) on pages 330-331, DOI: 10.1080/00222930010004232, http://zenodo.org/record/5299679
Multidimensional Poverty Index and Need to Revise the Methodology for Counting Poor
Creators: name: Ahmed, Masood
Publisher: name: figshare
Year: 2021
Subjects: subject: 140201 Agricultural Economics
subject: FOS: Economics and business
subject: 140202 Economic Development and Growth
subject: Economics

description: The largest share in Mineral Gross Domestic Product isfrom Jharkhand; it has 33% of Indian mineral reserve.Still, one out every three people is living below thepoverty line; the fact is that 37% state population isbelow the poverty line. The Jharkhand state problemis its poverty decline rate is slowest; growth dependson industrial performance that too shows volatility. Thepaper focuses on critical areas of education, healthand living standard by applying the Alkire-Foster (AF)methodology. The paper covers 24 districts ofJharkhand state with inference stress on rural-urbandivide and population under five categories of wealthindex (poorest, poorer, middle, rich and richest).
Measurement of the lambda and lambda^bar particles in Au+Au Collisions at sqrt(s_NN)=130 GeV
Creators: name: Adcox, K.
name: Collaboration, PHENIX
Publisher: name: arXiv
Year: 2002
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We present results on the measurement of lambda and lambda^bar production in Au+Au collisions at sqrt(s_NN)=130 GeV with the PHENIX detector at RHIC. The transverse momentum spectra were measured for minimum bias and for the 5% most central events. The lambda^bar/lambda ratios are constant as a function of p_T and the number of participants. The measured net lambda density is significantly larger than predicted by models based on hadronic strings (e.g. HIJING) but in approximate agreement with models which include the gluon junction mechanism.
description: 6 pages, RevTeX 3, 4 figures, 2 tables, 310 authors, submitted to Phys. Rev. Lett. on 17 April 2002. Plain text data tables for the points plotted in figures for this and previous PHENIX publications are (will be made) publicly available at http://www.phenix.bnl.gov/phenix/WWW/run/phenix/papers.html
DALI: a large Dataset of synchronized Audio, LyrIcs and notes, automatically created using teacher-student machine learning paradigm
Creators: name: Meseguer-Brocal, Gabriel
name: Cohen-Hadria, Alice
name: Peeters, Geoffroy
Publisher: name: arXiv
Year: 2019
Subjects: subject: Audio and Speech Processing (eess.AS)
subject: Databases (cs.DB)
subject: Machine Learning (cs.LG)
subject: Sound (cs.SD)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: The goal of this paper is twofold. First, we introduce DALI, a large and rich multimodal dataset containing 5358 audio tracks with their time-aligned vocal melody notes and lyrics at four levels of granularity. The second goal is to explain our methodology where dataset creation and learning models interact using a teacher-student machine learning paradigm that benefits each other. We start with a set of manual annotations of draft time-aligned lyrics and notes made by non-expert users of Karaoke games. This set comes without audio. Therefore, we need to find the corresponding audio and adapt the annotations to it. To that end, we retrieve audio candidates from the Web. Each candidate is then turned into a singing-voice probability over time using a teacher, a deep convolutional neural network singing-voice detection system (SVD), trained on cleaned data. Comparing the time-aligned lyrics and the singing-voice probability, we detect matches and update the time-alignment lyrics accordingly. From this, we obtain new audio sets. They are then used to train new SVD students used to perform again the above comparison. The process could be repeated iteratively. We show that this allows to progressively improve the performances of our SVD and get better audio-matching and alignment.
Syscia JTL
Creators: name: Longino, John T.
name: Branstetter, Michael G.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Syscia

description: Syscia JTL 071, Unnamed Morphospecies
Figure 9 (map, worker)
description: Published as part of Longino, John T. & Branstetter, Michael G., 2021, Integrating UCE Phylogenomics With Traditional Taxonomy Reveals a Trove of New World Syscia Species (Formicidae: Dorylinae), pp. 1-51 in Insect Systematics and Diversity 5 (2) on page 44, DOI: 10.1093/isd/ixab001, http://zenodo.org/record/5384404
Hubble Constant at Intermediate Redshift using the CO-Line Tully-Fisher Relation
Creators: name: Tutui, Y.
name: Sofue, Y.
name: Honma, M.
name: Ichikawa, T.
name: Wakamatsu, K.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have determined distances and Hubble ratios for galaxies at intermediate redshifts, cz=about 10,000 to 35,000 km/s, by applying the CO-line Tully-Fisher relation to our 12CO (J=1-0)-line observations using the Nobeyama 45-m telescope, and near-IR (NIR) photometry in the J and H bands using the 1.88-m telescope at Okayama Astrophysical Observatory. By averaging the Hubble ratios from J-band result, we obtain a Hubble constant of H_0 = 60 (+/- 10) km/s/Mpc. We argue that the CO line-NIR TFR can be a complimentary method to the other methods for measuring distances of galaxies at intermediate and high redshifts.
description: PASJ in press
Syscia JTL
Creators: name: Longino, John T.
name: Branstetter, Michael G.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Syscia

description: Syscia JTL 074, Unnamed Morphospecies
(Figure 9)
description: Published as part of Longino, John T. & Branstetter, Michael G., 2021, Integrating UCE Phylogenomics With Traditional Taxonomy Reveals a Trove of New World Syscia Species (Formicidae: Dorylinae), pp. 1-51 in Insect Systematics and Diversity 5 (2) on page 45, DOI: 10.1093/isd/ixab001, http://zenodo.org/record/5384404
title: Η διερεύνηση της αξίας του double product κατά την εξάλεπτη δοκιμασία βάδισης ως δείκτη φυσικής κατάστασης ασθενών με άσθμα διάφορης βαρύτητας
titleType: AlternativeTitle
title: Τhe use of the double product value during 6 minute walk test in evaluation of the physical status of patients with mild-moderate or severe asthma
Creators: name: Γεωργοπούλου, Αθηνούλα Δ.
Publisher: name: University of Thessaly
Year: 2021
Subjects: subject: Άσθμα -- Παθοφυσιολογία
subject: Αναπνευστικές ασκήσεις
subject: Αναπνευστικό σύστημα -- Φυσιολογία
subject: Καρδιά -- Παθοφυσιολογία

description: Σημείωση: διατίθεται συμπληρωματικό υλικό σε ξεχωριστό αρχείο.
ENHANCING CYBERSECURITY: A RULE-BASED APPROACH TO PHISHING SITE DETECTION
Creators: name: Chinedu, Ezechi Nwachukwu
name: Amina Fatimah, Olayemi Adeoye
name: Idris Abdulrahman, Sani
Publisher: name: kEITH jOURNAL
Year: 2025
Subjects: Phishing; Association rule; URL.

description: Phishing is a very serious challenge in web-based security these days. Phishing websites are forge web pages that are designed by noxious individuals to emulate pages of genuine sites. Phishers regularly make website pages that looks outwardly like the authentic and original site pages used in deceiving their victims. An uninformed internet customer is likely to be effortlessly tricked unknowing that this is a scam. Phishing webpages victims may uncover their financial details, secret key, and other sensitive data to the proprietor of phishing webpage. This research work is exceptionally significant in that it aimed at developing a model that will give security to users from phishers fraudulent tricks, and enable the users to distinguish the authenticity of websites. The benefit of this research work is to enable government institutes and financial organization to render variety of secured financial services to their various customers. The proposed model used association rule mining algorithm called Predictive Apriori to address phishing website issues that has been a global threat.  The algorithm is proficient in analyzing and extracting phishing URL features and is able to perform URL feature classification to identify phishing websites. It then flags the website as either legitimate or malicious. Therefore the user will be able to open only legitimate links. Systems Analysis and Design Method and Prototype methodologies were applied during this research. Our results showed that the algorithm used in this research work generates more accurate predictions than that of the existing system
Generalized Aubry-André-Harper model with modulated hopping and $p$-wave pairing
Creators: name: Yahyavi, Mohammad
name: Hetényi, Balázs
name: Tanatar, Bilal
Publisher: name: arXiv
Year: 2019
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We study an extended Aubry-Andr{é}-Harper model with simultaneous modulation of hopping, on-site potential, and $p$-wave superconducting pairing. For the case of commensurate modulation of $β= 1/2$ it is shown that the model hosts four different types of topological states: adiabatic cycles can be defined which pump particles, two types of Majorana fermions, or Cooper pairs. In the incommensurate case we calculate the phase diagram of the model in several regions. We characterize the phases by calculating the mean inverse participation ratio and perform multi-fractal analysis. In addition, we characterize whether the phases found are topologically trivial or not. We find an interesting critical extended phase when incommensurate hopping modulation is present. The rise between the inverse participation ratio in regions separating localized and extended states is gradual, rather than sharp. When, in addition, the on-site potential modulation is incommensurate, we find several sharp rises and falls in the inverse participation ratio. In these two cases all different phases exhibit topological edge states. For the commensurate case we calculate the evolution of the Hofstadter butterfly and the band Chern numbers upon variation of the pairing parameter for zero and finite on-site potential. For zero on-site potential the butterflies are triangular-like near zero pairing, when gap-closure occurs, they are square-like, and hexagonal-like for larger pairing, but with the Chern numbers switched compared to the triangular case. For the finite case gaps at quarter and three-quarters filling close and lead to a switch in Chern numbers.
Chandra and Hubble Space Telescope observations of dark gamma-ray bursts and their host galaxies
Creators: name: Chrimes, A. A.
name: Levan, A. J.
name: Stanway, E. R.
name: Lyman, J. D.
name: Fruchter, A. S.
name: Jakobsson, P.
name: O'Brien, P.
name: Perley, D. A.
name: Tanvir, N. R.
name: Wheatley, P. J.
name: Wiersema, K.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a study of 21 dark gamma-ray burst (GRB) host galaxies, predominantly using X-ray afterglows obtained with the Chandra X-Ray Observatory (CXO) to precisely locate the burst in deep Hubble Space Telescope (HST) imaging of the burst region. The host galaxies are well-detected in F160W in all but one case and in F606W imaging in approx 60 per cent of cases. We measure magnitudes and perform a morphological analysis of each galaxy. The asymmetry, concentration and ellipticity of the dark burst hosts are compared against the host galaxies of optically bright GRBs. In agreement with other studies, we find that dark GRB hosts are redder and more luminous than the bulk of the GRB host population. The distribution of projected spatial offsets for dark GRBs from their host galaxy centroids is comparable to that of optically-bright bursts. The dark GRB hosts are physically larger, more massive and redder, but are morphologically similar to the hosts of bright GRBs in terms of concentration and asymmetry. Our analysis constrains the fraction of high redshift (z greater than 5) GRBs in the sample to approx 14 per cent, implying an upper limit for the whole long-GRB population of less than 4.4 per cent. If dust is the primary cause of afterglow darkening amongst dark GRBs, the measured extinction may require a clumpy dust component in order to explain the observed offset and ellipticity distributions.
description: Accepted for publication in MNRAS
Rapid Formation of Ice Giant Planets
Creators: name: Boss, Alan P.
name: Wetherill, George W.
name: Haghighipour, Nader
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The existence of Uranus and Neptune presents severe difficulties for the core accretion model for the formation of ice giant planets. We suggest an alternative mechanism, namely disk instability leading to the formation of gas giant protoplanets, coagulation and settling of dust grains to form ice/rock cores at their centers, and photoevaporation of their gaseous envelopes by a nearby OB star, as a possible means of forming ice giant planets.
description: TeX file, 20 pages, no figures, 1 table, accepted by Icarus, Preprints available at http://www.ciw.edu/boss/ftp/planets/icaice.ps
Ancognatha Erichson 1847
Creators: name: Paucar-Cabrera, Aura
name: Ratcliffe, Brett C.
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Dynastidae
Ancognatha

description: Ancognatha Erichson, 1847
 Ancognatha Erichson 1847: 97.
 Barotheus Bates 1891: 30 (synonym). Pseudancognatha Otoya 1945: 275 (synonym).
description: Published as part of Paucar-Cabrera, Aura & Ratcliffe, Brett C., 2018, The Ancognatha Erichson (Coleoptera: Scarabaeidae: Dynastinae: Cyclocephalini) of Ecuador, with Description of a New Species, pp. 665-687 in The Coleopterists Bulletin 72 (4) on page 669, DOI: 10.1649/0010-065X-72.4.665, http://zenodo.org/record/5384479