cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Hamiltonian Frenet-Serret dynamics
Creators: name: Capovilla, Riccardo
name: Guven, Jemal
name: Rojas, Efrain
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The Hamiltonian formulation of the dynamics of a relativistic particle described by a higher-derivative action that depends both on the first and the second Frenet-Serret curvatures is considered from a geometrical perspective. We demonstrate how reparametrization covariant dynamical variables and their projections onto the Frenet-Serret frame can be exploited to provide not only a significant simplification of but also novel insights into the canonical analysis. The constraint algebra and the Hamiltonian equations of motion are written down and a geometrical interpretation is provided for the canonical variables.
description: Latex file, 14 pages, no figures. Revised version to appear in Class. Quant. Grav
Eulimneria rufifemur var. nigrotibialis KISS 1926
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Eulimneria
Eulimneria rufifemur
Eulimneria rufifemur (thomson) var. nigrotibialis kiss 1926

description: Eulimneria rufifemur (THOMSON) var. nigrotibialis KISS 1926
 Eulimneria rufifemur (THOMSON) var. nigrotibialis KISS 1926b: 107 – Holotypus (3): "Sz. Kézd Silbernagel" (= Szászkézd = Saschiz/ Rumänien), Budapest.
 G ü l t i g e r N a m e Sinophorus fuscicarpus (THOMSON 1887) (syn.nov.).
description: Published as part of Horstmann, K., 2009, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae III. Verschiedene Unterfamilien (Hymenoptera, Ichneumonidae), pp. 673-689 in Linzer biologische Beiträge 41 (1) on page 676, DOI: 10.5281/zenodo.5276253
Fourier Synthesization of Optical Pulses and "Polar'' Light
Creators: name: Zapasskii, V. S.
name: Alexandrov, E. B.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: It is shown that the direct Fourier synthesization of light beams allows one to create polarity-asymmetric waves, which are able, in the process of nonlinear interaction with a medium, to break its inversion symmetry. As a result, these "polar" waves may show the effect of optical rectification in nonlinear centrosymmetric media by generating light-induced dc electric polarization. At the same time, the waves of this type, due to their unusual symmetry properties, can be used for detecting the direction and sign of a dc electric field applied to the medium. The prospects of application of polar waves to data recording and processing are discussed.
description: to be published in May issue of Optics and Spectroscopy
Quantum Seiberg-Witten curve and Universality in Argyres-Douglas theories
Creators: name: Ito, Katsushi
name: Koizumi, Saki
name: Okubo, Takafumi
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the quantum Seiberg-Witten (SW) curves for $(A_1, G)$-type Argyres-Douglas (AD) theory by taking the scaling limit of the quantum SW curve of $N=2$ gauge theory with gauge group $G$. For $G=A_r$, the quantum SW curve of the AD theory is consistent with the scaling limit of the curve of the gauge theory. For $G=D_r$, we need the quantum correction to the SW curve of the AD theory, which depends on the quantization condition of the original SW curve. We also study the universality of the quantum SW curves for $(A_1, A_3)$ and $(A_1, D_4)$-type AD theories.
description: 16 pages
Spectral variability in transonic discs around black holes
Creators: name: Zampieri, L.
name: Turolla, R.
name: Szuszkiewicz, E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Transonic discs with accretion rates relevant to intrinsically bright Galactic X-ray sources ($L\approx 10^{38}$-$10^{39} {\rm erg s}^{-1}$) exhibit a time dependent cyclic behaviour due to the onset of a thermal instability driven by radiation pressure. In this paper we calculate radiation spectra emitted from thermally-unstable discs to provide detailed theoretical predictions for observationally relevant quantities. The emergent spectrum has been obtained by solving self-consistently the vertical structure and radiative transfer in the disc atmosphere. We focus on four particular stages of the disc evolution, the maximal evacuation stage and three intermediate stages during the replenishment phase. The disc is found to undergo rather dramatic spectral changes during the evolution, emitting mainly in the 1-10 keV band during outburst and in the 0.1-1 keV band off-outburst. Local spectra, although different in shape from a blackbody at the disc effective temperature, may be characterized in terms of a hardening factor $f$. We have found that $f$ is rather constant both in radius and in time, with a typical value $\sim 1.65$.
description: 10 pages Latex with 11 ps figures. Accepted for publication in MNRAS
High-Energy Neutrinos from Photomeson Processes in Blazars
Creators: name: Atoyan, A.
name: Dermer, C. D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: An important radiation field for photomeson neutrino production in blazars is shown to be the radiation field external to the jet. Assuming that protons are accelerated with the same power as electrons and injected with a -2 number spectrum, we predict that km^2 neutrino telescopes will detect about 1-to-several neutrinos per year from flat spectrum radio quasars (FSRQs) such as 3C 279. The escaping high-energy neutron and photon beams transport inner jet energy far from the black-hole engine, and could power synchrotron X-ray jets and FR II hot spots and lobes.
description: revised paper (minor revisions), accepted for publication in PRL
Additional file 1 of Epidemiology, antifungal susceptibility, risk factors, and mortality of persistent candidemia in adult patients in China: a 6-year multicenter retrospective study
Creators: name: Li, Yanping
name: Gu, Chenghong
name: Yang, Yuling
name: Ding, Yinhuan
name: Ye, Caihong
name: Tang, Min
name: Liu, Jinbo
name: Zeng, Zhangrui
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Environmental Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Plant Biology
subject: FOS: Biological sciences

description: Supplementary Material 1
Paulianidia proxima Lecoq 2008, n. sp.
Creators: name: Lecoq, Jean-Claude
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Paulianidia
Paulianidia proxima

description: Paulianidia proxima n. sp.
(Fig. 6D)
HOLOTYPE. — Madagascar Centre, S Ambositra, R. N. km 295,5, Ambatofitorahana, 1700 m, 5-6.I.1999, J. Janák, 1 ♂ (MNHUB).
PARATYPES. — Mêmes données que l’holotype, R. N. km 295,5 et 293, 1 ♂ (coll. Janák); 1 ♂ (MNHN).
Madagascar Est, Maromitza pr. Périnet, 8-10.I.1995, 950- 1150 m, tamisages en forêt humide, J. Janák, 1 ♂ (coll. Janák); 1 ♂ (MNHN).
 ÉTYMOLOGIE. — Du latin proximus, -a, -um (très proche). Par ses caractères cette espèce est très proche de P. brunnea.
DESCRIPTION
 Cette espèce est très semblable extérieurement à P. brunnea Jarrige,1978. Elle s’en distingue par la longueur des élytres, la courbure des tempes et la forme de l’édéage.
 Les élytres chez P. proxima n. sp. sont nettement plus longs que le pronotum (R = 1,35-1,40). Chez P. brunnea ils sont seulement un peu plus longs que le pronotum (R = 1,15). Longueur mesurée de l’angle huméral à l’apex. La courbure des tempes est plus accentuée chez P. brunnea alors qu’elles sont fuyantes chez P. proxima n. sp. L’édéage en vue ventrale chez P. proxima n. sp. présente un rebord à l’apex évasé latéralement en forme d’aile à peine rabattue. L’édéage en vue ventrale chez P. brunnea présente un évasement plus accentué, large et rabattu vers l’avant. Une vue axiale de l’orifice apical montre un évasement approximativement rectangulaire chez P. brunnea et approximativement ovale chez P. proxima n. sp.
Le sternite du propygidium du mâle est largement mais très peu profondément échancré. Le sternite du pygidium est largement et profondément échancré en U à fond subplat.
description: Published as part of Lecoq, Jean-Claude, 2008, Révision du genre Paulianidia Jarrige, 1978 de Madagascar (Insecta, Coleoptera, Staphylinidae, Paederinae), pp. 579-603 in Zoosystema 30 (3) on pages 602-603, DOI: 10.5281/zenodo.5390906
Additional file 1: of Changing prescribing behaviours with educational outreach: an overview of evidence and practice
Creators: name: Kunstler, Breanne
name: Lennox, Alyse
name: Bragge, Peter
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
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: Developmental Biology
subject: Cancer
subject: Science Policy

description: Search Strategy. (DOCX 13 kb)
Exochus notatus var. nigroscutellatus KISS 1926
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Curculionidae
Exochus
Exochus notatus
Exochus notatus holmgren var. nigroscutellatus kiss 1926

description: Exochus notatus HOLMGREN var. nigroscutellatus KISS 1926
 Exochus notatus HOLMGREN var. nigroscutellatus KISS 1926b: 118 – Holotypus (♀): "Oroszmezö Dr. Kiss" (= Rus/ Rumänien), Budapest. Das Weibchen trägt kein Typenetikett, weshalb BAJÁRI (1961: 437) angegeben hat, dass der Typus verloren sei. Es stimmt aber mit der Beschreibung überein und stammt vom Typenfundort.
 G ü l t i g e r N a m e Exochus lentipes GRAVENHORST 1829 (syn.nov.) (vgl. TOLKANITZ 2007: 665).
description: Published as part of Horstmann, K., 2009, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae III. Verschiedene Unterfamilien (Hymenoptera, Ichneumonidae), pp. 673-689 in Linzer biologische Beiträge 41 (1) on page 676, DOI: 10.5281/zenodo.5276253
Eutrombicula Ewing 1938
Creators: name: Bassini-Silva, Ricardo
name: Jacinavicius, Fernado de Castro
name: Muñoz-Leal, Sebastián
name: Maturano, Ralph
name: Welbourn, W. Calvin
name: Ochoa, Ronald
name: Bauchan, Gary R.
name: Barros-Battesti, Darci M.
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Trombiculidae
Eutrombicula

description: Eutrombicula Ewing, 1938
 Eutrombicula Ewing, 1938: 293; Loomis & Wrenn, 1984: 152; Domrow & Lester, 1985: 8; Hoffmann, 1990: 42; Stekolnikov & González-Acuña, 2015: 3.
 Type species: Microthrombidium alfreddugesi Oudemans, 1910
description: Published as part of Bassini-Silva, Ricardo, Jacinavicius, Fernado de Castro, Muñoz-Leal, Sebastián, Maturano, Ralph, Welbourn, W. Calvin, Ochoa, Ronald, Bauchan, Gary R. & Barros-Battesti, Darci M., 2018, A new species of the genus Eutrombicula Ewing, 1938 (Trombidiformes: Trombiculidae) and new records for the species Eutrombicula batatas (Linnaeus, 1758) in Brazil, pp. 976-986 in Acarologia 1938 (4) on page 978, DOI: 10.24349/acarologia/20184304, http://zenodo.org/record/5390982
MOESM1 of Severe hypoglycemia and the risk of cardiovascular disease and mortality in type 2 diabetes: a nationwide population-based cohort study
Creators: name: Jae-Seung Yun
name: Yong-Moon Park
name: Kyungdo Han
name: Seon-Ah Cha
name: Yu-Bae Ahn
name: Ko, Seung-Hyun
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy
subject: Computational Biology

description: Additional file 1: Table S1. Baseline characteristics according to the number of severe hypoglycemia events of sensitivity analysis from the sub-cohort which included only the participants who had regular standardized medical checkups. Table S2. Crude and adjusted HRs of cardiovascular outcomes and all-cause mortality from the sub-cohort which included only the participants who had regular standardized medical checkup. Table S3. Crude and adjusted HRs of cardiovascular outcomes and all-cause mortality from the sub-cohort with exclusion of patients who experienced SH at least two years before the occurrence of main outcomes. Table S4. Competing risk analysis including mortality as a competing risk.
Additional file 3 of Epidemiology, antifungal susceptibility, risk factors, and mortality of persistent candidemia in adult patients in China: a 6-year multicenter retrospective study
Creators: name: Li, Yanping
name: Gu, Chenghong
name: Yang, Yuling
name: Ding, Yinhuan
name: Ye, Caihong
name: Tang, Min
name: Liu, Jinbo
name: Zeng, Zhangrui
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Environmental Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Plant Biology
subject: FOS: Biological sciences

description: Supplementary Material 3
Evaluating Variable-Length Multiple-Option Lists in Chatbots and Mobile Search
Creators: name: Atanasova, Pepa
name: Karadzhov, Georgi
name: Kiprov, Yasen
name: Nakov, Preslav
name: Sebastiani, Fabrizio
Publisher: name: arXiv
Year: 2019
Subjects: subject: Information Retrieval (cs.IR)
subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: In recent years, the proliferation of smart mobile devices has lead to the gradual integration of search functionality within mobile platforms. This has created an incentive to move away from the "ten blue links'' metaphor, as mobile users are less likely to click on them, expecting to get the answer directly from the snippets. In turn, this has revived the interest in Question Answering. Then, along came chatbots, conversational systems, and messaging platforms, where the user needs could be better served with the system asking follow-up questions in order to better understand the user's intent. While typically a user would expect a single response at any utterance, a system could also return multiple options for the user to select from, based on different system understandings of the user's intent. However, this possibility should not be overused, as this practice could confuse and/or annoy the user. How to produce good variable-length lists, given the conflicting objectives of staying short while maximizing the likelihood of having a correct answer included in the list, is an underexplored problem. It is also unclear how to evaluate a system that tries to do that. Here we aim to bridge this gap. In particular, we define some necessary and some optional properties that an evaluation measure fit for this purpose should have. We further show that existing evaluation measures from the IR tradition are not entirely suitable for this setup, and we propose novel evaluation measures that address it satisfactorily.
description: 4 pages, in Proceeding of SIGIR 2019
Eustra japonica Bates 1892
Creators: name: Deuve, Thierry
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Carabidae
Eustra
Eustra japonica

description: Eustra japonica Bates, 1892
 Eustra plagiata Schmidt-Goebel – Bates 1873: 237.
 Eustra plagiata var. japonica Bates, 1892: 270.
 Eustra batesi Lewis, 1896: 330.
 Eustra japonica Bates – Andrewes 1919: 299. — Uéno 1985: 4.
 TYPES. — L’espèce E. japonica Bates, 1892, étant faiblement variable et ayant donné lieu à la création de deux taxons du groupe-espèce que je considère comme synonymes, il est souhaitable de désigner des lectotypes pour mieux fixer la nomenclature et éviter toute équivoque.
 Lectotype de japonica Bates (présente désignation): 1, Japon, « Lectotype [étiquette rouge] / Nagasaki [étiquette blanche écrite de la main de H. W. Bates] / Ex Musaeo H. W. Bates, 1892 [étiquette blanche imprimée de R. Oberthür] / Muséum Paris, coll. H. W. Bates, 1952 [étiquette blanche] / Eustra japonica Bates, Lectotype, Th. Deuve dés. 1996 [étiquette blanche] » (MNHN).
 Lectotype de batesi Lewis (présente désignation): 1, Japon, « Nagasaki, 13. II. -21. IV.1981 / Japan, G. Lewis. 1910-320 / Eustra Batesi Lewis, Type / Lectotype [étiquette rouge imprimée] / Eustra batesi Lewis, Lectotype, Th. Deuve des. 1998 [étiquette blanche] » (BMNH).
 DISTRIBUTION. — Japon, Honshu. Yokohama, G. Lewis (MNHN). — Osaka, Kibune, A. Nobuchi, 9.III.1951 (MNHN, coll. J. Nègre). — Osaka, Mont Iwawaki, Y. Shibata, 19.V.1957 (NIAS). — Osaka, Nose-Hattani, 250 mètres, M. Gotô, 4.IX.1949 (ETH). — Okayama, Kurashiki, Kamogatsuji, T. Aono, 10.X.1975 (NIAS).
 Japon, Kyushu. Nagasaki, G. Lewis, 13.XI.1880 - 21. IV.1881 (BMNH, MCZC).
 Japon, Ryu-Kyu. Île Iriomote, Kanpira, H. Irie, 1.V.1974 (NSMNH).
DIAGNOSE
Longueur: 3,2-3,7 mm. Coloris jaune testacé, la tête à peine plus foncée, les élytres avec une tache discale de rembrunissement localisée sur la moitié postérieure. Yeux plus convexes que les tempes. Pronotum 1,6 à 1,7 fois plus large que long, les angles antérieurs bien acuminés, les côtés denticulés, faiblement sinués avant les angles basaux qui sont subdroits ou un peu obtus, mais vifs. Édéage (Fig. 5A) petit et étroit, allongé, la lame apicale non incurvée, l’apex brusquement rétréci et infléchi. Endophallus sans sclérites dentiformes, mais une pièce copulatrice arrondie. Paramère gauche en tigette étroite et régulière, l’apex assez large, émoussé. Genitalia femelles orthotopiques, les coxostyles fusiformes, assez allongés, avec un gonostyle terminal porteur d’une longue soie apicale (Fig. 9A); la spermathèque membraneuse, large et plissée, annelée (Fig. 11A).
description: Published as part of Deuve, Thierry, 2001, Le genre Eustra Schmidt-Goebel, 1846, insectes (Coleoptera, Paussidae, Ozaeninae) à genitalia femelles orthotopiques, pp. 547-578 in Zoosystema 23 (3) on pages 565-566, DOI: 10.5281/zenodo.5391021
Analysis and test of the central-blue-spot infall hallmark
Creators: name: Estalella, R.
name: Anglada, G.
name: Díaz-Rodríguez, A. K.
name: Mayen-Gijon, J. M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The infall of material onto a protostar, in the case of optically thick line emission, produces an asymmetry in the blue- and red-wing line emission. For an angularly resolved emission, this translates in a blue central spot in the first-order moment (intensity weighted velocity) map. An analytical expression for the first-order moment intensity as a function of the projected distance was derived, for the cases of infinite and finite infall radius. The effect of a finite angular resolution, which requires the numerical convolution with the beam, was also studied. This method was applied to existing data of several star-forming regions, namely G31.41+0.31 HMC, B335, and LDN 1287, obtaining good fits to the first-order moment intensity maps, and deriving values of the central masses onto which the infall is taking place (G31.41+0.31 HMC: 70-120 $M_\odot$; B335: 0.1 $M_\odot$; Guitar Core of LDN 1287: 4.8 $M_\odot$). The central-blue-spot infall hallmark appears to be a robust and reliable indicator of infall.
description: Accepted for publication in A&A
Coloured conical emission via second-harmonic generation
Creators: name: Trillo, S.
name: Conti, C.
name: Di Trapani, P.
name: Jedrkiewicz, O.
name: Trull, J.
name: Valiulis, G.
name: Bellanca, G.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Optics (physics.optics)
subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: We predict that the combination of space and time modulational instabilities occuring via parametric wave-mixing in quadratic media leads to coloured conical emission. This phenomenon should be observed under conditions usually employed in second-harmonic generation experiments.
description: 10 pages, 4 figures, submitted to Optics Letters
Additional file 3: of Action 3:30R: process evaluation of a cluster randomised feasibility study of a revised teaching assistant-led extracurricular physical activity intervention for 8 to 10â year olds
Creators: name: Tibbitts, Byron
name: Porter, Alice
name: Sebire, Simon
name: Bird, Emma
name: Sanderson, Emily
name: Metcalfe, Chris
name: Powell, Jane
name: Jago, Russell
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Cell Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental 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: Developmental Biology

description: Potential improvements for the maintenance of Action 3:30. (DOCX 14 kb)
Additional file 1 of Association of cardiovascular health score trajectory and risk of subsequent cardiovascular disease in non-diabetic population: a cohort study
Creators: name: Zhou, Hui
name: Ding, Xiong
name: Wu, Shouling
name: Yan, Jin
name: Cao, Jianyun
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified

description: Supplementary Material 1
Glypta bugaczensis KISS 1926
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Glypta
Glypta bugaczensis

description: Glypta bugaczensis KISS 1926
 Glypta bugaczensis KISS 1926a: 243 f. – Holotypus (3): "Bugacz Com. Pest, Szilády, 924.VII.15" (in Ungarn), Budapest. Der Kopf des Typus ist angeklebt.
 G ü l t i g e r N a m e Glypta bugaczensis KISS 1926. Der Typus ist G. monoceros GRAVENHORST sehr ähnlich, er weicht ab durch: Schläfen hinter den Augen kaum verengt; Clypeus apical-median mit einem kleinen Zahn; Mandibeln rotbraun, nur Zähne dunkel. Da diese Unterschiede alle am Kopf anzutreffen sind, besteht die Möglichkeit, dass der Kopf einer anderen Art an den Thorax geklebt worden ist. Ohne zusätzliches Material lässt sich das Problem nicht lösen.
description: Published as part of Horstmann, K., 2009, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae III. Verschiedene Unterfamilien (Hymenoptera, Ichneumonidae), pp. 673-689 in Linzer biologische Beiträge 41 (1) on page 676, DOI: 10.5281/zenodo.5276253
Plato's Dialectic Method and Relevance to Modernity.docx
Creators: name: Dzneladze, Ivliane
Publisher: name: figshare
Year: 2021
Subjects: Uncategorized

description: History has shown numerous philosophers who claim original ideas and try to establish new ways of thinking. Starting from spiritualism and concluded up to rationalism idealism philosophy became the abstract discipline and therefore popular interest towards it has been lost. Especially antique philosophy has become subject of a critique from rationalist school of thought by imputing argument that metaphysics is unable to cover the problem of a material world which places the limitation on a broader development of rational reason
Host Galaxies of Gamma-ray Bursts: Spectral Energy Distributions and Internal Extinction
Creators: name: Sokolov, V. V.
name: Fatkhullin, T. A.
name: Castro-Tirado, A. J.
name: Fruchter, A. S.
name: Komarova, V. N.
name: Kasimova, E. R.
name: Dodonov, S. N.
name: Afanasiev, V. L.
name: Moiseev, A. V.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present BVRcIc broad-band flux spectra for the host galaxies of GRB970508, GRB980613, GRB980703, GRB990123 and GRB991208 obtained with the 6-m telescope of SAO RAS. The BVRcIc of these hosts are best fitted by the spectral properties of template SEDs of starburst galaxies and that there is a significant internal extinction in these host galaxies. We derived the absolute magnitudes of the GRB host galaxies making use of SEDs for the starburst galaxies. We performed the population synthesis modeling of the continuum spectral energy distribution of the host galaxies of GRB970508 and GRB980703 using different extinction laws and assuming burst and exponential scenarios of star formation. The comparison of BVRcIc broad-band flux spectra with the local starburst galaxies templates and theoretical templates as well as direct estimates (using Balmer emission lines) of the internal extinction shows that it is likely to be of great importance to take into account effects of the internal extinction in the host galaxies. From the SED of the host galaxy of GRB991208 and from the intensity of their spectral lines it follows that this is a GRB galaxy with the highest massive star-formation rate of all known GRB galaxies. The reduced luminosity of these dusty galaxies (e.g. for the host of GRB970508 A_V\sim 2 mag, for the host of GRB980703 A_V\sim 0.6 mag and for the host of GRB991208 A_V\sim 2 mag) could explain the observational fact: none of the observed GRB host galaxies with known distances is brighter than the local galaxies with the luminosity L_*.
description: Added acknowledgements
Plato's dialectic method and relevenace to modernity.docx
Creators: name: Dzneladze, Ivliane
Publisher: name: figshare
Year: 2021
Subjects: Uncategorized

description: History has shown numerous philosophers who claim original ideas and try to establish new ways of thinking. Starting from spiritualism and concluded up to rationalism idealism philosophy became the abstract discipline and therefore popular interest towards it has been lost. Especially antique philosophy has become subject of a critique from rationalist school of thought by imputing argument that metaphysics is unable to cover the problem of a material world which places the limitation on a broader development of rational reason
Sugar, organic acid, and MS-e-nose properties of non-centrifugal cane sugars from Japan and ASEAN countries
Creators: name: Ayustaningwarno, Fitriyono
name: ASIKIN, Yonathan
name: Wada, Koji
name: Tsuchida, Eito
name: MAEDA, Goki
name: NAM, Vu Tuan
name: HAJAR-AZHARI, Siti
Publisher: name: figshare
Year: 2021
Subjects: subject: 90805 Food Processing
subject: FOS: Other engineering and technologies

description: Sugar, organic acid, and MS-e-nose properties of non-centrifugal cane sugars from Japan and ASEAN countries2021 Japan Society for Bioscience, Biotechnology, and Agrochemistry Annual conference
High-resolution spectroscopic analysis of a large sample of Li-rich giants found by LAMOST
Creators: name: Zhou, Yutao
name: Yan, Hongliang
name: Shi, Jianrong
name: Blanco-Cuaresma, S.
name: Gao, Qi
name: Pan, K.
name: Xu, Xiaodong
name: Zhang, Junbo
name: Zhao, Gang
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The discovery of Li-rich giant has cast a new challenge for the standard stellar evolution models, and to resolve this issue, the number of this type object has been rapidly increased because of the development of worldwide surveys these days. Taking advantage of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope survey, 44 newly Li-rich giants are reported, which are confirmed with high-resolution observations. Based on the high-resolution and high signal-to-noise spectra, we derived the atmospheric parameters and elemental abundances with the spectral synthesis method. We performed a detailed analysis of their evolutionary stages, infrared excess, projected rotational velocity (v sin i), and the stellar population. We find that (1) The Li-rich giants concentrate at the evolutionary status of the red giant branch bump, red clump, and asymptotic giant branch; (2) Three of them are fast rotators and none exhibit infrared excess. Our results imply that the origins of Li enrichment are most likely to be associated with the extra mixing in the stellar interior, and the external sources maybe only make a minor contribution. Moreover, various Li-rich episodes take place at different evolutionary stages.
description: 13 pages, 5 figures, accepted for publication in ApJ
Eustra hammondi Deuve 2001, n. sp.
Creators: name: Deuve, Thierry
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Carabidae
Eustra
Eustra hammondi

description: Eustra hammondi n. sp.
TYPE. — Holotype 1, Philippines, Île de Mindanao, Province de Davao, versant oriental du Mont McKinley, 3300 pieds, H. Hoogstraal, 1.X.1946 (MCZC).
ÉTYMOLOGIE. — Cette espèce est très cordialement dédiée à Mr Peter Hammond, du Muséum d’Histoire naturelle de Londres.
 DISTRIBUTION. — Philippines, Mindanao. Seul l’holotype est connu.
DIAGNOSE
 Petite espèce (long. 3,0 mm), morphologiquement proche de E. japonica, mais le pronotum plus allongé (lp/Lp = 1,50). Coloris entièrement testacé jaune, le disque élytral avec toutefois une faible aire rembrunie dans la moitié apicale, mais peu distincte. Yeux plus convexes que les tempes. Côtés du pronotum très peu mais régulièrement denticulés, à peine sinués avant les angles basaux qui sont subdroits ou obtus, mais vifs. Édéage (Fig. 5B) petit, de forme allongée mais un peu incurvé, l’apex court et étroit, lobulaire. Pas de sclérites dentiformes dans l’endophallus, mais une pièce copulatrice en forme de cuilleron, son extrémité arrondie. Paramère gauche court, l’apex un peu sinueux. Femelle inconnue.
description: Published as part of Deuve, Thierry, 2001, Le genre Eustra Schmidt-Goebel, 1846, insectes (Coleoptera, Paussidae, Ozaeninae) à genitalia femelles orthotopiques, pp. 547-578 in Zoosystema 23 (3) on page 566, DOI: 10.5281/zenodo.5391021
The distance, supernova rate and supernova progenitors of NGC 6946
Creators: name: Eldridge, J. J.
name: Xiao, Lin
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The distance to the fireworks galaxy NGC 6946 is highly uncertain. Recent distance estimates using the tip of the red giant branch of 7.7 to 7.8 Mpc are larger than the distance commonly assumed for studying supernovae in this galaxy of 5.9 Mpc. Here we use the high supernova rate of the galaxy to derive the star-formation rate and predict the galaxy's FUV flux. We also account for dust extinction by different methods to derive a distance of 7.9+/-4.0 Mpc for NGC 6946. We then use the new distance to re-evaluate the understanding of the supernova progenitors 2002hh, 2004et, 2017eaw, the possible electron capture event 2008S and the possible black-hole forming event N6946-BH1. For the latter two exotic events the new distance improves the consistency between the observed progenitors and the stellar models that give rise to these events. From our findings we strongly recommend that all future studies of NGC~6946 must use the greater distance to the galaxy of 7.72+/-0.32 Mpc of Anand et al. (2018).
description: Accepted for publication in MNRAS letters, 5 pages, 1 figure, 1 table
Additional file 3: of Does the national dental scaling policy reduce inequalities in dental scaling usage? A population-based quasi-experimental study
Creators: name: Kim, Eun-Soo
name: Baek-Il Kim
name: Jung, Hoi In
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Table S2. Characteristics of people stratified by policy implementation using the Community Health Survey 2010â 2016 (weighted %). Changes in demographics, socioeconomics variables, and health conditions between pre- and post-policy periods. (DOCX 21 kb)
The pH-dependent electrostatic interaction of a metal nanoparticle with the MS2 virus-like particles
Creators: name: Phan, Anh D.
name: Hoang, Trinh X.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Other Condensed Matter (cond-mat.other)
subject: Biological Physics (physics.bio-ph)
subject: Quantitative Methods (q-bio.QM)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: The electrostatic interaction of metal nanoparticles with viruses is attracting great interest due to their antiviral activity and their role in enhancing the detection of viruses at ultra-low concentrations. We model the MS2 virus devoid of its single strand RNA core using a core-shell model. The dependence of the inner and outer surface charge density on the pH is taken into account in our model of the interaction. Varying the pH causes a change in the sign of the outer surface charge leading to the attractive-repulsive transition in the electrostatic interaction between the MS2 virus and metal nanoparticle at pH = 4.
description: 6 pages, 4 figures, accepted for publication on Chemical Physics Letter
Symmetry properties of the large-scale solar magnetic field
Creators: name: Galitski, Victor
name: Kuzanyan, K. M.
name: Sokoloff, D. D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate symmetry properties of the solar magnetic field in the framework of the linear Parker's migratory dynamo model. We show that the problem can be mapped onto the well-known quantum-mechanical double-well problem. Using the WKB approximation, we construct analytical solutions for the dipole and quadrupole configurations of the generated magnetic field. Our asymptotic analysis within the equatorial region indicates the existence of an additional weak dynamo wave which violates the Hale's polarity law. We estimate the spatial decay decrement of this wave. We also calculate explicitly the splitting of the eigenvalues corresponding to the dipole and quadrupole modes. The real part of the dipole eigenvalue is shown to exceed the quadrupole one. A sufficiently long time after generation the dipole mode should dominate the quadrupole one. The relevant observational evidences of the properties obtained are discussed.
description: 18 pages; slightly differs from published version, all results are the same
Additional file 4: of Does the national dental scaling policy reduce inequalities in dental scaling usage? A population-based quasi-experimental study
Creators: name: Kim, Eun-Soo
name: Baek-Il Kim
name: Jung, Hoi In
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Computational Biology

description: Table S3. Medians of each income category in pre- or post-policy periods using the Community Health Surveys 2010–12 and 2014–16 (weighted %). Table S4. Percentage and cut-off of per capita and equivalized monthly household income in pre- or post-policy periods using the Community Health Surveys 2010–12 and 2014–16 (weighted %). Table S5. Relative ratio and absolute differences of dental scaling non-user prevalence using equivalized household income levels in pre- or post-policy periods, Community Health Surveys 2010–12 and 2014–16 (weighted %). Table S6. Relative ratio and absolute differences of dental scaling non-user prevalence using per capita household income levels in pre- or post-policy periods, Community Health Surveys 2010–12 and 2014–16 (weighted %). Sensitivity analysis using equivalized and per-capita household income. (DOCX 32 kb)
A Spectroscopic Analysis of the California-Kepler Survey Sample: I. Stellar Parameters, Planetary Radii and a Slope in the Radius Gap
Creators: name: Martinez, Cintia F.
name: Cunha, Katia
name: Ghezzi, Luan
name: Smith, Verne V.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present results from a quantitative spectroscopic analysis conducted on archival Keck/HIRES high-resolution spectra from the California-$Kepler$ Survey (CKS) sample of transiting planetary host stars identified from the $Kepler$ mission. The spectroscopic analysis was based on a carefully selected set of Fe I and Fe II lines, resulting in precise values for the stellar parameters of effective temperature (T$_{\rm eff}$) and surface gravity (log $g$). Combining the stellar parameters with $Gaia$ DR2 parallaxes and precise distances, we derived both stellar and planetary radii for our sample, with a median internal uncertainty of 2.8$\%$ in the stellar radii and 3.7$\%$ in the planetary radii. An investigation into the distribution of planetary radii confirmed the bimodal nature of this distribution for the small radius planets found in previous studies, with peaks at: $\sim$1.47 $\pm$ 0.05 R$_{\oplus}$ and $\sim$2.72 $\pm$ 0.10 R$_{\oplus}$, with a gap at $\sim$ 1.9R$_{\oplus}$. Previous studies that modeled planetary formation that is dominated by photo-evaporation predicted this bimodal radii distribution and the presence of a radius gap, or photo-evaporation valley. Our results are in overall agreement with these models. The high internal precision achieved here in the derived planetary radii clearly reveal the presence of a slope in the photo-evaporation valley for the CKS sample, indicating that the position of the radius gap decreases with orbital period; this decrease was fit by a power law of the form R$_{pl}$ $\propto$ P$^{-0.11}$, which is consistent with photo-evaporation and Earth-like core composition models of planet formation.
description: 33 pages, 13 figures
Structure and evolution of the photospheric magnetic field in 2010 - 2017: comparison of SOLIS/VSM vector field and $B_{LOS}$ potential field
Creators: name: Virtanen, Ilpo I.
name: Pevtsov, Alexei A.
name: Mursula, Kalevi
Publisher: name: arXiv
Year: 2019
Subjects: subject: Space Physics (physics.space-ph)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The line-of-sight (LOS) component of the large-scale photospheric magnetic field has been observed since the 1950s, but the daily full-disk observations of the full vector magnetic field started only in 2010 using the SOLIS Vector Stokes Magnetograph (VSM) and the SDO helioseismic and magnetic imager (HMI). Traditionally, potential field extrapolations are based on the assumption that the magnetic field in the photosphere is approximately radial. The validity of this assumption has not been tested yet. We investigate here the structure and evolution of the three components of the solar large-scale magnetic field in 2010 - 2017, covering the ascending to mid-declining phase of solar cycle 24, using SOLIS/VSM vector synoptic maps of the photospheric magnetic field. We compare the observed VSM vector magnetic field to the potential vector field derived using the VSM LOS magnetic field observations as an input. The new vector field data allow us to derive the meridional inclination and the azimuth angle of the magnetic field and to investigate their solar cycle evolution and latitudinal profile of these quantities. SOLIS/VSM vector data show that the photospheric magnetic field is in general fairly non-radial. In the meridional plane the field is inclined toward the equator, reflecting the dipolar structure of the solar magnetic field. Rotationally averaged meridional inclination does not have significant solar cycle variation. While the vector radial component $B_r$ and the potential radial component $B_r^{PFSS}$ are fairly similar, the meridional and zonal components do not agree very well. We find that SOLIS/VSM vector observations are noisy at high latitudes and suffer from the vantage point effect more than LOS observations. This is due to different noise properties in the LOS and transverse components of the magnetic field, which needs to be addressed in future studies.
Quantum invariants of Seifert 3-manifolds and their asymptotic expansions
Creators: name: Hansen, Soren Kold
name: Takata, Toshie
Publisher: name: arXiv
Year: 2002
Subjects: subject: Geometric Topology (math.GT)
subject: Quantum Algebra (math.QA)
subject: FOS: Mathematics
subject: 57M27, 17B37, 18D10, 41A60

description: We report on recent results of the authors concerning calculations of quantum invariants of Seifert 3-manifolds. These results include a derivation of the Reshetikhin-Turaev invariants of all oriented Seifert manifolds associated with an arbitrary complex finite dimensional simple Lie algebra, and a determination of the asymptotic expansions of these invariants for lens spaces. Our results are in agreement with the asymptotic expansion conjecture due to JE Andersen [The Witten invariant of finite order mapping tori I, to appear in J. Reine Angew. Math.] and [The asymptotic expansion conjecture, from `Problems on invariants of knots and 3--manifolds', edited by T. Ohtsuki, http://www.ms.u-tokyo.ac.jp/~tomotada/proj01/].
description: Published by Geometry and Topology Monographs at http://www.maths.warwick.ac.uk/gt/GTMon4/paper6.abs.html
Origin of $α$-rich young stars: clues from C, N and O
Creators: name: Hekker, Saskia
name: Johnson, Jennifer A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A small set of chemically old stars that appear young by their independently derived masses has been detected. These are so-called $α$-rich young stars. For a sample of 51 red-giant stars, for which spectra are available from SDSS/APOGEE and masses are available from asteroseismic measures based on \textit{Kepler} lightcurves, we derive the C, N and O abundances through an independent analysis. These stars span a wide range of N/C surface number density ratios. We interpret the high-mass stars with low N/C as being products of mergers or mass transfer during or after first dredge up, because the dredge-up features are the same as for low-mass stars. The $α$-rich young stars with high N/C follow the expected trend of N/C for their mass, and could be either genuine young stars (leaving their high [$α$/Fe] unexplained) or the results of mergers on the main sequence.
description: Accepted for publication in MNRAS
Superluminal Tunneling Devices
Creators: name: Nimtz, Günter
Publisher: name: arXiv
Year: 2002
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: Photonic tunneling permits superluminal signal transmission. The principle of causality is not violated but the time duration between cause and effect can be shortened compared with an interaction exchange with velocity of light. This outstanding property can be applied to speed-up photonic signal modulation and transmission as well as to improve micro-electronic devices. Superluminal photonic signal transmission have been presented at microwave and infrared frequencies already. Presumably superluminal photonic and electronic devices can become reality having in mind the experimental evidence of the universal tunneling time of photons and of electrons.
description: Invited talk at the 22nd Solvay Conference in Physics, "The Physics of Communication", European Cultural Center of Delphi, Delphi, 24-29 November 2001
Early formation of moons around large trans-Neptunian objects via giant impacts
Creators: name: Arakawa, Sota
name: Hyodo, Ryuki
name: Genda, Hidenori
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: Recent studies have revealed that all large (over 1000 km in diameter) trans-Neptunian objects (TNOs) form satellite systems. Although the largest Plutonian satellite, Charon, is thought to be an intact fragment of an impactor directly formed via a giant impact, whether giant impacts can explain the variations in secondary-to-primary mass ratios and spin/orbital periods among all large TNOs remains to be determined. Here we systematically perform hydrodynamic simulations to investigate satellite formation via giant impacts. We find that the simulated secondary-to-primary mass ratio varies over a wide range, which overlaps with observed mass ratios. We also reveal that the satellite systems' current distribution of spin/orbital periods and small eccentricity can be explained only when their spins and orbits tidally evolve: initially as fluid-like bodies, but finally as rigid bodies. These results suggest that all satellites of large TNOs were formed via giant impacts in the early stage of solar system formation, before the outward migration of Neptune, and that they were fully or partially molten during the giant impact era.
description: 24 pages, 8 figures. Accepted for publication in Nature Astronomy. The final authenticated version is available online at: https://rdcu.be/bHBXX
Glypta rufoclypeata KISS 1924
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Glypta
Glypta rufoclypeata

description: Glypta rufoclypeata KISS 1924
 Ctenochares slavonicus KISS 1924: 86 – Lectotypus (♀) hiermit festgelegt: "Igenpataka Dr. Szilády" (= Ighiel/ Rumänien), "906.VII.08", Budapest. Der Kopf des Typus ist angeklebt.
 G ü l t i g e r N a m e Glypta sculpturata GRAVENHORST 1829 (AUBERT 1972a: 85).
description: Published as part of Horstmann, K., 2009, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae III. Verschiedene Unterfamilien (Hymenoptera, Ichneumonidae), pp. 673-689 in Linzer biologische Beiträge 41 (1) on pages 676-677, DOI: 10.5281/zenodo.5276253
Properties of the Trans-Neptunian Belt: Statistics From the CFHT Survey
Creators: name: Trujillo, Chadwick A.
name: Jewitt, David C.
name: Luu, Jane X.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of a wide-field survey designed to measure the size, inclination, and radial distributions of Kuiper Belt Objects (KBOs). The survey found 86 KBOs in 73 square degrees observed to limiting red magnitude 23.7 using the Canada-France-Hawaii Telescope and the 12k x 8k CCD Mosaic camera. For the first time, both ecliptic and off-ecliptic fields were examined to more accurately constrain the inclination distribution of the KBOs. The survey data were processed using an automatic moving object detection algorithm, allowing a careful characterization of the biases involved. In this work, we quantify fundamental parameters of the Classical KBOs (CKBOs), the most numerous objects found in our sample, using the new data and a maximum likelihood simulation. Deriving results from our best-fit model, we find that the size distribution follows a differential power law with exponent q = 4.0 (+0.6)(-0.5) (1 sigma, or 68.27% confidence). In addition, the CKBOs inhabit a very thick disk consistent with a Gaussian distribution of inclinations with a Half-Width of i(1/2) = 20 (+6)(-4) deg (1 sigma). We estimate that there are N = 3.8 (+2.0)(-1.5) x 10^4 (1 sigma) CKBOs larger than 100 km in diameter. We also find compelling evidence for an outer edge to the CKBOs at heliocentric distance R = 50 AU.
description: To be published in the Astronomical Journal, July 2001