cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Ficus artocarpoides Warburg 1904
Creators: name: Rasplus, Jean-Yves
name: Harry, Myriam
name: Perrin, Hélène
name: Chassagnard, Marie-Thérèse
name: Lachaise, Daniel
Publisher: name: Zenodo
Year: 2003
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Moraceae
Ficus
Ficus artocarpoides

description: Ficus artocarpoides Warburg, 1904
710 m, 860 m.
Galerie forestière Nimba 1250 m, 1200 m, 1160 m, 1090 m, 1050 m, 1020 m, 1000 m; Bord de torrent 935 m, 915 m; Galerie forestière niveau Cité-2 Base Technique 850 m; Galerie forestière Nimba 825 m, 800 m, 750 m, 740 m, 710 m; savane Zougué 750 m; lisière galerie forestière du Gba niveau Mifergui 725 m, 700 m; chantier Gbakoré 725 m, 705 m; Bossou 550 m; Ziéla 525 m; galerie forestière du Cavally 500 m; savane à buttes 500 m; Zouguépo 500 m; zone bambou 500 m; forêt mésophile et secondarisée zone tampon 500 m.
description: Published as part of Rasplus, Jean-Yves, Harry, Myriam, Perrin, Hélène, Chassagnard, Marie-Thérèse & Lachaise, Daniel, 2003, Les Ficus (Moraceae) et l'entomofaune des figues (Hym. Agaonidae, Pteromalidae, Torymidae, Eurytomidae; Dipt. Drosophilidae; Col. Curculionidae) du mont Nimba en Guinée, pp. 107-182 in Mémoires du Muséum national d'Histoire naturelle 190 on page 118, DOI: 10.5281/zenodo.10683835
The most metal-poor Galactic globular cluster: the first spectroscopic observations of ESO280-SC06
Creators: name: Simpson, Jeffrey D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the first spectroscopic observations of the very metal-poor Milky Way globular cluster ESO280-SC06. Using spectra acquired with the 2dF/AAOmega spectrograph on the Anglo-Australian Telescope, we have identified 13 members of the cluster, and estimate from their infrared calcium triplet lines that the cluster has a metallicity of $\mathrm{[Fe/H]}=-2.48\substack{+0.06 \\ -0.11}$. This would make it the most metal-poor globular cluster known in the Milky Way. This result was verified with comparisons to three other metal-poor globular clusters that had been observed and analyzed in the same manner. We also present new photometry of the cluster from EFOSC2 and SkyMapper and confirm that the cluster is located $22.9\pm2.1$ kpc from the Sun and $15.2\pm2.1$ kpc from the Galactic centre, and has a radial velocity of $92.5\substack{+2.4 \\ -1.6}$ km s$^{-1}$. These new data finds the cluster to have a radius about half that previously estimated, and we find that the cluster has a dynamical mass of the cluster of $(12\pm2)\times10^3$ solar masses. Unfortunately, we lack reliable proper motions to fully characterize its orbit about the Galaxy. Intriguingly, the photometry suggests that the cluster lacks a well-populated horizontal branch, something that has not been observed in a cluster so ancient or metal-poor.
description: 12 pages, 12 figures. Accepted for publication in MNRAS
The complete radiative corrections to the gaugino and Higgsino masses in the Minimal Supersymmetric Model
Creators: name: Pierce, Damien
name: Papadopoulos, Aris
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We determine the radiative corrections to the masses of the gauginos and Higgsinos in the MSSM, including all sectors of the theory in a one-loop calculation in the on-mass-shell renormalization scheme. We find that a gluino which is massless at tree level receives a mass of between 0 and 3 GeV, primarily due to the top/stop contribution. This radiatively generated mass depends directly on the off-diagonal element of the squark mass matrix. In the case of a massive gluino, its mass receives typically large corrections, as large as 40\% for a 125 GeV gluino. We find that the contributions to the neutralino and chargino mass corrections from the gauge/Higgs/gaugino/Higgsino sector are typically +-1%. The lightest neutralino, which can receive corrections larger than 25%, receives 5% corrections over most of the parameter space. We combine our results with the results of LEP and CDF searches to obtain the lower bounds on the neutralino and chargino masses at one-loop. We also demonstrate how the radiative corrections affect the presently excluded region of parameter space.
description: 16 pages, JHU-TIPAC-940001, PURD-TH-94-04. 6 uuencoded postscript figures included. Uncomment the line "%\input epsf" to embed the figures in the text
On stability of blow up solutions for the critical co-rotational Wave Maps problem
Creators: name: Krieger, Joachim
name: Miao, Shuang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: We show that the finite time blow up solutions for the co-rotational Wave Maps problem constructed in [7,15] are stable under suitably small perturbations within the co-rotational class, provided the scaling parameter $λ(t) = t^{-1-ν}$ is sufficiently close to $t^{-1}$, i. e. the constant $ν$ is sufficiently small and positive. The method of proof is inspired by [3,12], but takes advantage of geometric structures of the Wave Maps problem already used in [1,21] to simplify the analysis. In particular, we heavily exploit that the resonance at zero satisfies a natural first order differential equation.
description: 66 pages
Linking Entanglement Detection and State Tomography via Quantum 2-Designs
Creators: name: Bae, Joonwoo
name: Hiesmayr, Beatrix C.
name: McNulty, Daniel
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present an experimentally feasible and efficient method for detecting entangled states with measurements that extend naturally to a tomographically complete set. Our detection criterion is based on measurements from subsets of a quantum 2-design, e.g., mutually unbiased bases or symmetric informationally complete states, and has several advantages over standard entanglement witnesses. First, as more detectors in the measurement are applied, there is a higher chance of witnessing a larger set of entangled states, in such a way that the measurement setting converges to a complete setup for quantum state tomography. Secondly, our method is twice as effective as standard witnesses in the sense that both upper and lower bounds can be derived. Thirdly, the scheme can be readily applied to measurement-device-independent scenarios.
description: 16 pages, 4 figures
Dynamical analysis on $f(R,\mathcal{G})$ cosmology
Creators: name: da Costa, Simony Santos
name: Roig, Fernando V.
name: Alcaniz, Jailson S.
name: Capozziello, Salvatore
name: de Laurentis, Mariafelicia
name: Benetti, Micol
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We use a dynamical system approach to study the cosmological viability of $f(R,\mathcal{G})$ gravity theories. The method consists of formulating the evolution equations as an autonomous system of ODEs, using suitable variables. The formalism is applied to a class of models in which $f(R,\mathcal{G})\propto R^{n}\mathcal{G}^{1-n}$ and its solutions and corresponding stability are analysed in detail. New accelerating solutions that can be attractors in the phase space are found. We also find that this class of models does not exhibit a matter-dominated epoch, a solution which is inconsistent with current cosmological observations.
description: 12 pages, 4 figures. Accepted for publication in Classical and Quantum Gravity
$A_{LR}$, Negative $S$, and Extended Gauge Models
Creators: name: Rizzo, Thomas G.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The implications of the recent measurement of the left-right asymmetry, $A_{LR}$, by the SLD Collaboration for theories with extended gauge sectors is examined. We show that it is possible to arrange for large, negative values of $S$, based on an analysis of leptonic data, without serious side effects for other observables in certain classes of models. The implications of such scenarios for future measurements on the $Z$ peak, at the Tevatron, and for atomic parity violation experiments are examined.
description: 19 pages, 9 Figs, LaTex, figures available upon request, SLAC-PUB-6455
Ostrea pes felis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Ostreoida
Ostreidae
Ostrea
Ostrea pes felis

description: Ostrea pes felis [spec. nov.]
O. testa radiis 7 striatis scabris, auricula altera minuta.
Habitat in O. Africano.
Testa parva, pellucida, novem radiis senfim undata.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 697, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
A Unified Model for the Evolution of Galaxies and Quasars
Creators: name: Kauffmann, Guinevere
name: Haehnelt, Martin
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We incorporate a simple scheme for the growth of supermassive black holes into semi-analytic models that follow the formation and evolution of galaxies in a cold dark matter dominated Universe. We assume that supermassive black holes are formed and fuelled during major mergers. If two galaxies of comparable mass merge, their central black holes coalesce and a few percent of the gas in the merger remnant is accreted by the new black hole over a timescale of a few times 10^7 years. With these simple assumptions, our model not only fits many aspects of the observed evolution of galaxies, but also reproduces quantitatively the observed relation between bulge luminosity and black hole mass in nearby galaxies, the strong evolution of the quasar population with redshift and the relation between the luminosities of nearby quasars and those of their host galaxies. The strong decline in the number density of quasars from z=2 to z=0 is due to the combination of three effects: i) a decrease in the merging rate, ii) a decrease in the amount of cold gas available to fuel black holes, and iii) an increase in the timescale for gas accretion. In a LCDM cosmology the predicted decline in the total content of cold gas in galaxies is consistent with that inferred from observations of damped Lyman-alpha systems. Our results strongly suggest that the evolution of supermassive black holes, quasars and starbursts is inextricably linked to the hierarchical build-up of galaxies.
description: 30 pages, Latex, 18 figures included, submitted to MNRAS
Kinks in higher derivative scalar field theory
Creators: name: Zhong, Yuan
name: Guo, Rong-Zhen
name: Fu, Chun-E
name: Liu, Yu-Xiao
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study static kink configurations in a type of two-dimensional higher derivative scalar field theory whose Lagrangian contains second-order derivative terms of the field. The linear fluctuation around arbitrary static kink solutions is analyzed. We find that, the linear spectrum can be described by a supersymmetric quantum mechanics problem, and the criteria for stable static solutions can be given analytically. We also construct a superpotential formalism for finding analytical static kink solutions. Using this formalism we first reproduce some existed solutions and then offer a new solution. The properties of our solution is studied and compared without those preexisted. We also show the possibility in constructing twinlike model in the higher derivative theory, and give the consistency conditions for twinlike models corresponding to the canonical scalar field theory.
description: 14 pages, 5 figures
Additional file 1: of Comparison of cervical cancer screening among women with and without hysterectomies: a nationwide population-based study in Korea
Creators: name: Shin, Ji-Yeon
name: Choi, Kui
name: Suh, Mina
name: Boyoung Park
name: Jun, Jae
Publisher: name: figshare
Year: 2018
Subjects: subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Questionnaire hysterectomy and Pap screening. (DOCX 18 kb)
Ficus asperifolia Miquel 1849
Creators: name: Rasplus, Jean-Yves
name: Harry, Myriam
name: Perrin, Hélène
name: Chassagnard, Marie-Thérèse
name: Lachaise, Daniel
Publisher: name: Zenodo
Year: 2003
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Moraceae
Ficus
Ficus asperifolia

description: Ficus asperifolia Miquel, 1849
Ce figuier dioïque, sarmenteux ou lianescent est une espèce ripicole commune et abondante sur les berges des rivières et des fleuves au contact même de l’eau. Il forme des fourrés denses le long du Cavally à Taï ou du Bandama à Lamto en Côte d’Ivoire. Dans cette région du Sud-Baoulé le nom vernaculaire de ce figuier signifierait ‘‘qui est mangé par les poissons’’ lesquels assureraient la dispersion des graines, d’où sa distribution essentiellement ripicole. Dans la région du Nimba nous ne l’avons pas retrouvé en 1993. Il ne fait cependant pas de doute que l’espèce y est présente. Schnell (1952) la signale dans la brousse secondaire de la région de Nzo au nord-est du Nimba. Il semble ainsi que l’espèce soit mieux représentée dans le bas Cavally que dans le haut Cavally.
 TABLEAU 1. Les 31 espèces de Ficus de la région du mont Nimba en Guinée selon la nomenclature de Berg (Berg 1988, 1989, 1990; Berg & Wiebes 1992). Dans la colonne de gauche et en gras sont mentionnées les 26 espèces recensées pendant la mission avril-mai 1993; les cinq espèces restantes sont celles que nous n’avons pas retrouvées mais qui sont rapportées par Schnell (1952) et Adam (1981). (*) Les sept espèces mentionnées pour la première fois du Nimba.  TABLE 1. The 31 species of  Ficus of the mount Nimba region in Guinea according to Berg’s nomenclatura (Berg 1988, 1989, 1990; Berg & Wiebes 1992). In the left column in bold are mentioned those 26 species recorded during the authors’ April-May 1993 field survey; the 5 remaining species are those which we did not found but were reported by Schnell (1952) and Adam (1981). (*) The 7 species mentioned for the first time from Nimba.
description: Published as part of Rasplus, Jean-Yves, Harry, Myriam, Perrin, Hélène, Chassagnard, Marie-Thérèse & Lachaise, Daniel, 2003, Les Ficus (Moraceae) et l'entomofaune des figues (Hym. Agaonidae, Pteromalidae, Torymidae, Eurytomidae; Dipt. Drosophilidae; Col. Curculionidae) du mont Nimba en Guinée, pp. 107-182 in Mémoires du Muséum national d'Histoire naturelle 190 on pages 112-113, DOI: 10.5281/zenodo.10683835
Infrared spectrum and intermolecular potential energy surface of the CO-O2 dimer
Creators: name: Barclay, A. J.
name: McKellar, A. R. W.
name: Moazzen-Ahmadi, N.
name: Dawes, Richard
name: Wang, Xiao-Gang
name: Carrington, Tucker
Publisher: name: arXiv
Year: 2018
Subjects: subject: Atomic and Molecular Clusters (physics.atm-clus)
subject: FOS: Physical sciences

description: Only a few weakly-bound complexes containing the O2 molecule have been characterized by high resolution spectroscopy, no doubt due to the complications added by the oxygen molecule's unpaired electron spin. Here we report an extensive infrared spectrum of CO-O2, observed in the CO fundamental band region using a tunable quantum cascade laser to probe a pulsed supersonic jet expansion. The rotational energy level pattern derived from the spectrum consists of stacks of levels characterized by the total angular momentum, J, and its projection on the intermolecular axis, K. Five such stacks are observed in the ground vibrational state, and ten in the excited state (v(CO) = 1). They are divided into two groups, with no observed transitions between groups. The groups correspond to different projections of the O2 electron spin, and correlate with the two lowest rotational states of O2, (N, J) = (1, 0) and (1, 2). The rotational constant of the lowest K = 0 stack implies an effective intermolecular separation of 3.82 Angstroms, but this should be interpreted with caution since it ignores possible effects of electron spin. A new high-level 4-dimensional potential energy surface is developed for CO-O2, and rotational energy levels are calculated for this surface, ignoring electron spin. By comparing calculated and observed levels, it is possible to assign detailed quantum labels to the observed level stacks.
description: 35 pages and 8 figures
title: Transcriptions Cisterciens et Ressources #84
Creators: name: Flammarion, Hubert
name: Flammarion, Hubert
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023
Subjects: subject: abbaye de Morimond
subject: Forêt
subject: terre
subject: paturage
subject: Eau
subject: Moulin

description: Geoffroy, évêque de Langres, notifie un certain nombre de donations à l'abbaye de Morimond pour la grange des Gouttes.
description: Source: abbaye de Morimond
description: Source: A. Original perdu, scellé de cire rouge à queue pendant en fil de soye verte (d'après C.)
description: Source: B. Copie partielle, Cartulaire de Morimond (1476-1480), Bibl. Bourbonne-les-Bains, ms 1, p. 59.
description: Source: C. Copie sur papier, XVIIIe siècle, coll. Jolibois, A. D. Haute-Marne, 19 J 10, fol. 201-202.
description: Source: a. H. FLAMMARION, Recueil des chartes de l’abbaye de Morimond au XIIe siècle, Brepols ARTEM, n° 21, 2014, 558 p., (d'ap. C.), n° 34.
description: Bibliographic citation: Transcription CIS#84, Hubert Flammarion, in Projet Cisterciens et Ressources [Ressource en ligne], https://cisterciensetressources.lamop.fr/
description: Transcriptions Cisterciens et Ressources #84
description: date: 1150-1162
Ostrea pellucens Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Ostreoida
Ostreidae
Ostrea
Ostrea pellucens

description: Ostrea pellucens [spec. nov.]
O. testa radiis 9, laevi: fornice squamis cochlearihemisphaericis.
Argenv. conch. t. 27. f. H. Pecten semiauritus.
Habitat in O. australiore.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 698, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Thermonuclear Burning Regimes and the Use of SNe Ia in Cosmology
Creators: name: Sorokina, E. I.
name: Blinnikov, S. I.
name: Bartunov, O. S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The calculations of the light curves of thermonuclear supernovae are carried out by a method of multi-group radiation hydrodynamics. The effects of spectral lines and expansion opacity are taken into account. The predictions for UBVI fluxes are given. The values of rise time for B and V bands found in our calculations are in good agreement with the observed values. We explain why our results for the rise time have more solid physical justification than those obtained by other authors. It is shown that small variations in the chemical composition of the ejecta, produced in the explosions with different regimes of nuclear burning, can influence drastically the light curve decline in the B band and, to a lesser extent, in the V band. We argue that recent results on positive cosmological constant Lambda, found from the high redshift supernova observations, could be wrong in the case of possible variations of the preferred mode of nuclear burning in the earlier Universe.
description: 20 pages, 5 figures, presented at the conference "Astronomy at the Eve of the New Century", Puschino, May 17-22, 1999. A few references and a table added, typos corrected
How to measure the intercept of the BFKL pomeron at HERA
Creators: name: Nikolaev, N. N.
name: Zakharov, B. G.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Determination of the intercept of the BFKL pomeron is one of the pressing issues in the high energy physics. Earlier we have shown that, at the dipole size $r=r_Δ=(0.1-0.2)$f, the dipole cross section $σ(x,r)$ which is a solution of the generalized BFKL equation, exhibits a precocious asymptotic behavior $σ(x,r)\propto \left({1\over x}\right)^{Δ_{\Pom}}$. In this paper we discuss how measuring $F_{L}(x,Q^{2})$ and $\partial F_{T}(x,Q^{2})/\partial \log Q^{2}$ at $Q^{2}= (10-40)$GeV$^{2}$ and $Q^{2}=(2-10)$GeV$^{2}$, respectively, one can probe $σ(x,r_Δ)$ and directly determine the intercept $Δ_{\Pom}$ of the BFKL pomeron in the HERA experiments.
description: 10 pages, 2 figures upon the request from kph154@zam001.zam.kfa-juelich.de, Juelich preprint KFA-IKP(Th)-1994-10, 28 February 1994
VLA Observations of H2O Masers in the Class 0 Protostar S106 FIR: Evidence for a 10 AU-Scale Accelerating Jet-like Flow
Creators: name: Furuya, R. S.
name: Kitamura, Y.
name: Saito, M.
name: Kawabe, R.
name: Wootten, H. A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We conducted VLA observations at 0".06 resolution of the 22 GHz water masers toward the Class 0 source S106 FIR (d=600 pc; 15" west of S106-IRS4) on two epochs separated by ~3 months. Two compact clusters of the maser spots were found in the center of the submillimeter core of S106 FIR. The separation of the clusters was ~80 mas (48 AU) along P. A. = 70 degrees and the size of each cluster was ~20 mas x 10 mas. The western cluster, which had three maser components, was 7.0 km/s redshifted with respect to the ambient cloud velocity. Each component was composed of a few spatially localized maser spots and was aligned on a line connecting the clusters. We found relative proper motions of the components with ~30 mas/yr (18 AU/yr) along the line. In addition, a series of single-dish observations show that the maser components drifted with a radial acceleration of ~1 km/s/yr. These facts indicate that the masers could be excited by a 10 AU-scale jet-like accelerating flow ejected from an assumed protostar located between the two clusters. The outflow size traced by the masers was 50 AU x 5 AU after correction for an inclination angle of 10 degrees which was derived from the relative proper motions and radial velocities of the maser components. The three-dimensional outflow velocity ranged from 40 to 70 km/s assuming symmetric motions for the blue and red components. Since no distinct CO molecular outflows have been detected so far, we suggest that S106 FIR is an extremely young protostar observed just after the onset of outflowing activity.
description: 24 pages, 6 figures, No. 5 color. Accepted, Astrophysical Journal
On determination of the large-${1\over x}$ gluon distribution at HERA
Creators: name: Nikolaev, N. N.
name: Zakharov, B. G.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We discuss corrections to the Leading-Log$Q^{2}$ relationships between the gluon density $g(x,Q^{2})$ and $F_{L}(x,Q^{2}),\,\partial F_{T}(x,Q^{2}) /\partial \log Q^{2}$ in the HERA range of large ${1\over x}$. We find that the above quantities probe the gluon density $g(x,Q_{T,L}^{2})$ at $Q_{T,L}^{2}=C_{T,L}Q^{2}$, with the $Q^{2}$-rescaling factors $C_{T}\approx 2.2$ and $C_{L}\approx 0.42$. The possibility of treating charm as an active flavour is critically re-examined.
description: 12 pages, 4 figures upon the request from kph154@zam001.zam.kfa-juelich.de, J\"ulich preprint KFA-IKP(TH)-1994-12. Some misprints and ordering of references corrected
Extending the Cybercrime Incident Architecture with a feature-­based Cybercrime Classification System (CCS)
Creators: name: Vavatsioulas, Dimitrios
Publisher: name: figshare
Year: 2021
Subjects: Applied Computer Science

description: Cybercrime is an evolving and growing threat that heavily bothers Internet users and the relevant authorities. Due to the rapid adoption of technology, Cybercrime Incidents have been increasing at an enormous rate. Cybercrime has several types and various targets, depending on what the offender wants to achieve. It is well-established that the prevention and confrontation of such incidents is a challenging problem since they have a highly complex nature that is constantly developing. This thesis aims to propose a Cybercrime Classification System (CCS) that automatically classifies Cybercrimes into a specific type/class. This process will help to group similar incidents together, propose appropriate counter-measures, design an effective response policy and find recurring patterns between the incidents. The CCS consists of three Components and each serves a different purpose. In order to classify Cybercrime Incidents, the Cybercrime Classification System uses a feature-based approach, which means that each incident is characterized by some specific, distinctive features. These features will determine the Cybercrime Class that the incident falls into. Machine Learning techniques, such as Data Mining, are used by the CCS for the Classification process. The results of the presented system are decent and prove that a practical and real-world system which uses the proposed approach could be developed, and it could be proven critical for mitigating Cybercrime. The CCS could be extended in order to provide more functionalities, such as automatically assess threat severity or automatically apply the respective counter-actions.
Direct Analysis of Spectra of the Type Ic Supernova 1994I
Creators: name: Millard, J.
name: Branch, D.
name: Baron, E.
name: Hatano, K.
name: Fisher, A.
name: Filippenko, A.
name: Kirshner, R.
name: Challis, P.
name: Fransson, C.
name: Panagia, N.
name: Phillips, M.
name: Sonneborn, G.
name: Suntzeff, N.
name: Wagoner, R.
name: Wheeler, J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Synthetic spectra generated with the parameterized supernova synthetic-spectrum code SYNOW are compared to observed photospheric-phase spectra of the Type Ic supernova 1994I. The observed optical spectra can be well matched by synthetic spectra that are based on the assumption of spherical symmetry. We consider the identification of the infrared absorption feature observed near 10,250 Å, which previously has been attributed to He I $\lambda10830$ and regarded as strong evidence that SN 1994I ejected some helium. We have difficulty accounting for the infrared absorption with He I alone. It could be a blend of He I and C I lines. Alternatively, we find that it can be fit by Si I lines without compromising the fit in the optical region. In synthetic spectra that match the observed spectra, from 4 days before to 26 days after the time of maximum brightness, the adopted velocity at the photosphere decreases from 17,500 to 7000 \kms. Simple estimates of the kinetic energy carried by the ejected mass give values that are near the canonical supernova energy of $10^{51}$ ergs. The velocities and kinetic energies that we find for SN 1994I in this way are much lower than those that we find elsewhere for the peculiar Type Ic SNe 1997ef and 1998bw, which therefore appear to have been hyper-energetic.
description: 18 pages, 12 figures, ApJ, in press
The Planes of Satellite Galaxies Problem, Suggested Solutions, and Open Questions
Creators: name: Pawlowski, Marcel S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Satellite galaxies of the Milky Way and of the Andromeda galaxy have been found to preferentially align in significantly flattened planes of satellite galaxies, and available velocity measurements are indicative of a preference of satellites in those structures to co-orbit. There is increasing evidence that such kinematically correlated satellite planes are also present around more distant hosts. Detailed comparisons show that similarly anisotropic phase-space distributions of sub-halos are exceedingly rare in cosmological simulations based on the $Λ$CDM paradigm. Analogs to the observed systems have frequencies of $\leq 0.5$ per cent in such simulations. In contrast to other small-scale problems, the satellite planes issue is not strongly affected by baryonic processes because the distribution of sub-halos on scales of hundreds of kpc is dominated by gravitational effects. This makes the satellite planes one of the most serious small-scale problem for $Λ$CDM. This review summarizes the observational evidence for planes of satellite galaxies in the Local Group and beyond, and provides an overview of how they compare to cosmological simulations. It also discusses scenarios which aim at explaining the coherence of satellite positions and orbits, and why they all are currently unable to satisfactorily resolve the issue.
description: Invited review for MPLA, accepted for publication. 26 pages, 3 figures
Ostrea sanguinea Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Ostreoida
Ostreidae
Ostrea
Ostrea sanguinea

description: Ostrea sanguinea [spec. nov.]
O. testa radiis 22 scabris, semiaurita.
Gvalt. test. t. 74. f. N.
Habitat in O. australiore.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 698, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
АНАЛИЗ ЗАКОНОДАТЕЛЬНЫХ АКТОВ ПО РЕГУЛИРОВАНИЮ ПРОИЗВОДСТВА ЛЕКАРСТВЕННЫХ СРЕДСТВ НА ФАРМАЦЕВТИЧЕСКОМ РЫНКЕ РЕСПУБЛИКИ УЗБЕКИСТАН
Creators: name: Азлярова, Г.У.
name: Ибрагимова, М.Я.
name: Абдураимова, О.А.
Publisher: name: Zenodo
Year: 2024

description: В данной работе рассмотрены, влияние нормативно-правовых норм на фармацевтическом рынке. Фармацевтические рынки являются самыми быстрорастущими и сложными с точки зрения их социальной значимости в обеспечении населения лекарственными средствами. В связи с этим одной из важнейших задач в развитии общества и государства является изучение вопросов управления лекарственными средствами. Таким образом, в Республике Узбекистан реализован ряд организационных мероприятий, направленных на создание условий для повышения качества и эффективности лекарственных средств, медицинской техники и изделий медицинского назначения. Создание экономических и фармацевтических свободных зон, развитие предпринимательства в государственных и частных секторах.
Next Generation of Phonon Tests of Lorentz Invariance using Quartz BAW Resonators
Creators: name: Goryachev, Maxim
name: Kuang, Zeyu
name: Ivanov, Eugene N.
name: Haslinger, Philipp
name: Muller, Holger
name: Tobar, Michael E.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Nuclear Experiment (nucl-ex)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: We demonstrate technological improvements in phonon sector tests of Lorentz Invariance that implement quartz Bulk Acoustic Wave oscillators. In this experiment, room temperature oscillators with state-of-the-art phase noise are continuously compared on a platform that rotates at a rate of order a cycle per second. The discussion is focused on improvements in noise measurement techniques, data acquisition and data processing. Preliminary results of the second generation of such tests are given, and indicate that SME coefficients in the matter sector can be measured at a precision of order $10^{-16}$ GeV after taking a years worth of data. This is equivalent to an improvement of two orders of magnitude over the prior acoustic phonon sector experiment.
Additional file 1: of LncRNA DLEU1 contributes to colorectal cancer progression via activation of KPNA3
Creators: name: Tianyou Liu
name: Zhiyang Han
name: Huanyu Li
name: Yuekun Zhu
name: Ziquan Sun
name: Anlong Zhu
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: 60506 Virology

description: Figure S1. Overexpression of DLEU1 promotes CRC cell proliferation, migration and invasion. a The expression of DLEU1 was measured by qRT-PCR in HCT116 and SW620 cells transfected with DLEU1 ectopic expressing vector or control. b CCK8 assay was used for analysis of cell proliferation. c, d Transwell assay was utilized to determine cell migration and invasion. *P<0.05. All data were collected from three independent experiments. (DOCX 133 kb)
A New Method for Helicity Calculations
Creators: name: Ballestrero, A.
name: Maina, E.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We propose a new helicity formalism based on the formal insertion in spinor lines of a complete set of states build up with unphysical spinors. The method is developed both for massless and massive fermions for which it turns out to be particularly fast. All relevant formulae are given.
description: 14 pages, 2 figs. using feynman.tex
Interactions resolve state-dependence in a toy-model of AdS black holes
Creators: name: Bzowski, Adam
name: Gnecchi, Alessandra
name: Hertog, Thomas
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We show that the holographic description of a class of AdS black holes with scalar hair involves dual field theories with a double well effective potential. Black hole microstates have significant support around both vacua in the dual, which correspond to perturbative degrees of freedom on opposite sides of the horizon. A solvable toy-model version of this dual is given by a quantum mechanical particle in a double well potential. In this we show explicitly that the interactions replace the state-dependence that is needed to describe black hole microstates in a low energy effective model involving the tensor product of two decoupled harmonic oscillators. A naive number operator signals the presence of a firewall but a careful construction of perturbative states and operators extinguishes this.
description: 43 pages, 11 figures
Anharmonicity-induced isostructural phase transition of Zirconium under pressure
Creators: name: Stavrou, Elissaios
name: Yang, Lin H.
name: Soderlind, Per
name: Aberg, Daniel
name: Radousky, Harry B.
name: Armstrong, Michael R.
name: Belof, Jonathan L.
name: Kunz, Martin
name: Greenberg, Eran
name: Prakapenka, Vitali B.
name: Young, David A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We have performed a detailed x-ray diffraction structural study of Zr under pressure and unambiguously identify the existence of a first-order isostructural bcc-to-bcc phase transition near 58 GPa. First-principles quantum molecular dynamics lattice dynamics calculations support the existence of this phase transition, in excellent agreement with experimental results, triggered by anharmonic effects. Our results highlight the potential ubiquity of anharmonically driven isostructural transitions within the periodic table under pressure and calls for follow-up experimental and theoretical studies.
A new mixed isogeometric approach to Kirchhoff-Love shells
Creators: name: Rafetseder, Katharina
name: Zulehner, Walter
Publisher: name: arXiv
Year: 2018
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics

description: For Kichhoff-Love shell problems a new mixed formulation solely based on standard $H^1$ spaces is presented. This allows for flexibility in the construction of discretization spaces, e.g., standard $C^0$-coupling of multi-patch isogeometric spaces is sufficient. In terms of solution strategies, for iterative solvers efficient methods for standard second-order problems like multigrid can be used as building blocks of a preconditioner. Furthermore, a combination of the proposed mixed formulation of the bending part with a popular mixed formulation of the membrane part in order to avoid membrane locking is considered. The performance of both mixed formulations is demonstrated by numerical benchmark studies.
The Shape and Figure Rotation of NGC 2915's Dark Halo
Creators: name: Bureau, M.
name: Freeman, K. C.
name: Pfitzner, D. W.
name: Meurer, G. R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: NGC 2915 is a blue compact dwarf galaxy with a very extended HI disk showing a short central bar and extended spiral arms, both reaching far beyond the optical component. We use Tremaine & Weinberg (1984) method to measure the pattern speed of the bar from HI radio synthesis data. Our measurements yield a pattern speed of 0.21+/-0.06 km/s/arcsec (8.0+/-2.4 km/s/kpc for D=5.3 Mpc), in disagreement with the general view that corotation in barred disks lies just outside the end of the bar, but consistent with recent models of barred galaxies with dense dark matter halos. Our adopted bar semi-length puts corotation at more than 1.7 bar radii. The existence of the pattern is also problematic. Because NGC 2915 is isolated, interactions cannot account for the structure observed in the HI disk. We also demonstrate that the low observed disk surface density and the location of the pseudo-rings make it unlikely that swing amplification or bar-driven spiral arms could explain the bar and spiral pattern. Based on the similarity of the dark matter and HI surface density profiles, we discuss the possibility of dark matter distributed in a disk and following closely the HI distribution. The disk then becomes unstable and can naturally form a bar and spiral pattern. However, this explanation is hard to reconcile with some properties of NGC 2915. We also consider the effect of a massive and extended triaxial dark matter halo with a rotating figure. The existence of such halos is supported by CDM simulations showing strongly triaxial dark halos with slow figure rotation. The observed structure of the HI disk can then arise through forcing by the rotating triaxial figure. We associate the measured pattern speed in NGC 2915 with the figure rotation of its dark halo.
description: 37 pages, including 8 figures and 2 tables (AASTeX, aaspp4.sty). Fig.1 and 2 available as jpg. Accepted for publication in The Astronomical Journal. Online manuscript with PostScript figures available at: http://www.strw.leidenuniv.nl/~bureau/pub_list.html
Political Sophistication, Political Efficacy and Split-Ticket Voting in Mixed-Member Electoral Systems: The Case of Lithuania
Creators: name: Morkevičius, Vaidas
name: Butkevičienė, Eglė
name: Vaidelytė, Eglė
name: Žvaliauskas, Giedrius
Publisher: name: Zenodo
Year: 2021
Subjects: Internal Political Efficacy
Political Sophistication
European Social Survey
Lithuanian National Election Study
Split-Ticket Voting

description: Paper presented at the 26th IPSA World Congress of Political Science, July 12, 2021, Panel: RC17.10 “New Patterns of Political Participation and Voting: Evidence from Comparative Survey Research”, Research Committee: RC17 Comparative Public Opinion.
Globular Cluster Systems I: V-I Color Distributions
Creators: name: Gebhardt, Karl
name: Kissler-Patig, Markus
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have compiled data for the globular cluster systems of 50 galaxies from the HST WFPC2 archive, of which 43 are type S0 or earlier. In this paper, we present the data set and derive the V-I color distributions. We derive the first four moments of the color distributions, as well as a measure for their non--unimodality. The number of globular clusters in each galaxy ranges from 18 (in NGC 2778) to 781 (NGC 5846). For those systems having more than 100 clusters, seven of sixteen (44%) show significant bimodality. Overall, roughly half of all the systems in our sample show hints of a bimodal color distribution. In general, the distributions of the faint galaxies are consistent with unimodality, whereas those of the brighter galaxies are not. In comparing the moments of the V-I distributions with various galaxy properties for the early-type galaxies, we find the following difference in the correlations between the field and cluster galaxy populations: the peak V-I color of the globular cluster distribution correlates well with the central velocity dispersion---and hence the Mg2 index and total luminosity---for galaxies in cluster environments; there exists no such correlation for field galaxies. This difference between cluster and field galaxies possibly reflects different formation scenarios for their globular cluster systems. Among the explanations for such a correlation, we consider either a larger age spread in the field populations or the possibility that cluster galaxies are always affected by significant accretion whereas some field galaxies could host pure ``in situ'' formed populations.
description: 30 pages, accepted AJ
Scaling Laws in Hierarchical Clustering Models with Poisson Superposition
Creators: name: Hegyi, S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Properties of cumulant- and combinant ratios are studied for multihadron final states composed of Poisson distributed clusters. The application of these quantities to ``detect'' clusters is discussed. For the scaling laws which hold in hierarchical clustering models (void scaling, combinant scaling) a generalization is provided. It is shown that testing hierarchical models is meaningful only for phase-space volumes not larger than the characteristic correlation length introduced by Poisson superposition. Violation of the scaling laws due to QCD effects is predicted.
description: 14 pages, Plain TeX, no figures
Ostrea pusio Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Ostreoida
Ostreidae
Ostrea
Ostrea pusio

description: Ostrea pusio [spec. nov.]
O. testa radiis 40 filiformibus uniaurita.
Habitat in O. australiore.
Testa magnitudine nucis coryli, utrinque aequaliter convexa. Auricula fere unica.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 698, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Top quark polarization as a probe of $t\bar{t}$ threshold dynamics
Creators: name: Fadin, V. S.
name: Khoze, V. A.
name: Kotsky, M. I.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the spin properties of top quarks produced in collisions of polarized photons in the threshold region. For a relatively heavy top quark the influence of non-perturbative effects is small and its polarization parameters can be predicted in perturbative QCD. The measurements of the top polarization may allow a novel test of QCD in the $t\bar{t}$ system. In particular, they may provide a new way to determine the precise value of $α_s$ and to study the properties of the top quark.
description: 21 pages. Figures available upon request
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 1492
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1492, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1492, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Improvement of SVM-based Road Extraction from Remote Sensing Image by using FCM and MRF
Creators: name: Jiawei Xu
Publisher: name: figshare
Year: 2018
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences

description: Master Thesis Submitted to Department of Electronic Engineering, Hallym University.A short version was presented at "Jiawei Xu and Seop Hyeong Park, “Experiments on Road Extraction from Remote Sensing Images using SVM combined with FCM and MRF,” 한국멀티미디어학회 학술발표논문집, 2010, Seoul, Republic of Korea.
TEXNIK OLIY TAʻLIM MUASSASALARIDA MATERIALSHUNOSLIK VA FIZIK FANLARINING INTEGRALLASHUVI
Creators: name: Abdurahmonova, Shohidaxon
name: Jonibekova ., Sayyora
Publisher: name: Zenodo
Year: 2025

description: Ushbu maqolada texnik oliy taʻlim muassasalarida materialshunoslik va fizik fanlarining integrallashgan holda ta'lim berilishi ustozlar va talabalar vaqti va ta'lim sifatini oshishiga , dars soatlarini ko'payishi , bir vaqtning o'zida ikki fandan chuqurroq ta'lim olish imkonini yanada oshishi haqida aytib oʻtilgan.