cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Secular Evolution of Hierarchical Triple Star Systems
Creators: name: Ford, Eric B.
name: Kozinsky, Boris
name: Rasio, Frederic A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We derive octupole-level secular perturbation equations for hierarchical triple systems, using classical Hamiltonian perturbation techniques. By extending previous work done to leading (quadrupole) order to octupole level (i.e., including terms of order alpha^3, where alpha = a_1/a_2 < 1 is the ratio of semimajor axes) we obtain expressions that are applicable to a much wider range of parameters. For triple systems containing a close inner binary, we also discuss the possible interaction between the classical Newtonian perturbations and the general relativistic precession of the inner orbit. In some cases we show that this interaction can lead to resonances and a significant increase in the maximum amplitude of eccentricity perturbations. We establish the validity of our analytic expressions by providing detailed comparisons with the results of direct numerical integrations of the three-body problem obtained for a large number of representative cases. We also discuss applications of the theory in the context of several observed triple systems of current interest, including the millisecond pulsar PSR B1620-26 in M4, the giant planet in 16 Cygni, and the protostellar binary TMR-1. [short version]
description: 47 pages, including 17 figures, to appear in ApJ, May 20, 2000; revised version with some minor additions and clarifications
Photoproduction of Very Light Gluinos
Creators: name: Carlson, Carl
name: Sher, Marc
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Current experiments allow the possibility of gluino masses below about 600 MeV if the lifetime of the gluino is longer than 100 picoseconds. If the mass and lifetime are in this window, then photoproduction of pairs of gluino-gluon bound states can provide a means to observe them. The cross section is large enough that the window can be fully explored, up to lifetimes exceeding a microsecond, at high luminosity electron accelerators.
description: 9 pages, in Latex, 2 figures will be faxed on request. WM-93-114
Amiota (Amiota) ratnae Chen and Toda
Creators: name: Chen, Hong-Wei
name: Toda, Masanori J.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Drosophilidae
Amiota
Amiota ratnae

description: Amiota (Amiota) ratnae Chen and Toda
(figure 3G, H)
 Amiota (Amiota) ratnae Chen and Toda, 1998b: 412.
 Diagnosis. Surstylus not expanded ventrally; paramere at distally, roundly dilated apically, without any acute projections basally; apical plate of ejaculatory apodeme with two pits per side.
 Description. Female: Seventh tergite not separated mid-dorsally; eighth sternite lacking pubescence, with long setae on distal one-third (figure 3G); pregenital lamella unsclerotized.
 Specimens ex amined. Indonesia: Paratypes 5 2, Bogor, Java, 27–30 N ovember 1996, M. J. Toda leg. (EH U).
 Distribution. Indonesia (West Kalimantan, Java).
description: Published as part of Chen, Hong-Wei & Toda, Masanori J., 2001, A revision of the Asian and European species in the subgenus Amiota Loew (Diptera, Drosophilidae) and the establishment of species-groups based on phylogenetic analysis, pp. 1517-1563 in Journal of Natural History 35 (10) on page 1528, DOI: 10.1080/002229301317067665, http://zenodo.org/record/10683624
การปนเปื้อนของ laryngoscope และการทำความสะอาดที่เหมาะสม
Creators: name: กัลยาณี ศุระศรางค์
Publisher: name: สถาบันวิจัย จัดการความรู้ และมาตรฐานการควบคุมโรค
Year: 2559
Subjects: การปนเปื้อน
การทำความสะอาด

description: วารสารควบคุมโรค, 42, 3, 176-183
A Na I Absorption Map of the Small-Scale Structure in the Interstellar Gas Toward M15
Creators: name: Meyer, David M.
name: Lauroesch, J. T.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using the DensePak fiber optic array on the KPNO WIYN telescope, we have obtained high S/N echelle spectra of the Na I D wavelength region toward the central 27" x 43" of the globular cluster M15 at a spatial resolution of 4". The spectra exhibit significant interstellar Na I absorption at LSR velocities of +3 km/s (LISM component) and +68 km/s (IVC component). Both components vary appreciably in strength on these scales. The derived Na I column densities differ by a factor of 4 across the LISM absorption map and by a factor of 16 across the IVC map. Assuming distances of 500 pc and 1500 pc for the LISM and IVC clouds, these maps show evidence of significant ISM structure down to the minimum scales of 2000 AU and 6000 AU probed in these absorbers. The smallest-scale N(Na I) variations observed in the M15 LISM and IVC maps are typically comparable to or higher than the values found at similar scales in previous studies of interstellar Na I structure toward binary stars. The physical implications of the small and larger-scale Na I features observed in the M15 maps are discussed in terms of variations in the H I column density as well as in the Na ionization equilibrium.
description: 11 pages, 3 figures, accepted for publication in ApJ Letters
On multi-solitons for the energy-critical wave equation in dimension 5
Creators: name: Yuan, Xu
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: In this paper, we construct $K$-solitons of the focusing energy-critical nonlinear wave equation in five-dimensional space, i.e. solutions $u$ of the equation such that \begin{equation*} \|\nabla_{t,x}u(t)-\nabla_{t,x}\big(\sum_{k=1}^{K}W_{k}(t)\big)\|_{L^{2}}\to 0\quad \mathrm{as}\ t\to \infty, \end{equation*} where for any $k\in \{1,\dots,K\}$, $W_{k}$ is Lorentz transform of the explicit standing soliton $W(x)=(1+|x|^{2}/15)^{-3/2}$, with any speed $\boldsymbol{\ell}_{k}\in \mathbb{R}^{5}$ ,$|\boldsymbol{\ell}_{k}|<1$ ($\boldsymbol{\ell}_{k'}\ne \boldsymbol{\ell}_{k}$ for $k'\ne k$) satisfying an explicit smallness condition.
description: 30 pages. minor revisions. arXiv admin note: substantial text overlap with arXiv:1708.09712, arXiv:1504.01595 by other authors
The Dilated Chiral Quark Model
Creators: name: Beane, S. R.
name: van Kolck, U.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is argued that constituent quarks live in an effective theory that possesses an approximate conformal invariance. An effective lagrangian is constructed which in the large-$\nc$ approximation incorporates Regge asymptotic constraints. The resulting picture explains why linear-sigma models provide successful constituent quark descriptions, both at zero and finite temperature. Our analysis suggests an interesting relation between non-linearly realized conformal invariance and the completion of chiral multiplets in the broken symmetry phase.
description: 8 pages, uses TeXsis or mTeXsis.tex,CPP-94-2,DOE/ER/40427-01-N94
title: Конструктивное моделирование трикотажных изделий
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2017

description: В учебном пособии изложен материал по конструктивному моделированию трикотажных изделий для проектирования новой объемной формы моделей и внесения модельных особенностей в основу конструкции приближенными или шаблонными методами. Рассмотрены особенности моделирования трикотажных изделий в зависимости от способа их изготовления, приведены способы построения чертежей конструкции и внесения модельных линий в соответствии с эскизом плечевых и поясных изделий из трикотажа. Предназначено для студентов, обучающихся по направлениям подготовки 29.03.02 «Технологии и проектирование текстильных изделий», 54.03.03 «Искусство костюма и текстиля», 54.04.01 «Дизайн» (профиль «Дизайн трикотажа»), и может быть использовано в подготовке студентов других направлений, а также в системе повышения квалификации работников трикотажных и швейных предприятий.
title: Dossiers documentaires de Bouvard et Pécuchet. Recueil g226, volume 6
Creators: name: Flaubert, Gustave
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2022

description: Descriptif matériel du dossier préparatoire selon le catalogue de la Bibliothèque municipale de Rouen : "XIXe s. Papier. 329 folios numérotés de 1 à 328 (n° 63 bissé). Cartonné, dos toile noire", et de son contenu, avec des compléments donnés entre crochets droits :
 F. 1. Titre : Philosophie ; 
F. 2. Liste de 41 ouvrages relatifs à la philosophie ; 
F. 3-66. Notes sur chacun de ces ouvrages ; 
F. 67-76. Notes sur des questions de philosophie ; 
F. 77. Titre : Poésies et Chansons ; 
F. 76-63. Recueil de Chansons nouvelles vendues par Perrier ; 
F. 64-68. Recueil de Chansons nouvelles pour 1845 ; 
F. 69-90. Poèmes publiés par le Figaro ; 
F. 91-92. Justice, poème ; 
F. 93-94. Bal du 26 septembre, poème par Eugène Moreau ; 
F. 95-100. Clair de Lune, poème ; 
F. 101. Le Voyage [poème de Baudelaire dédié à Maxime du Camp] ; 
F. 102. L'Albatros [poème], par Baudelaire ; 
F. 103-110. Poèmes d’Eustache Bérat : Boutade misanthropique et familière ; Conseils d'une veuve à sa fille ; Mes adieux à Rouen ; 
F. 111. Le bon Ange des Napolitains [poème] de V. Chammas ; 
F. 112-117. Poèmes d’Eustache Bérat : Conseils d'une mère à sa fille - A M. Paillette qui critiquait... ; Les Lampions et le soleil ; A M. P. Mathieu, poète... ; A E. Deschamps ; Épître familière à plusieurs membres d'une société littéraire ; Le Rendez-vous d'honneur ; Lettre familière à Lachambaudie ; 
F. 118. Ceux qui ne s’en vont pas [poème], par Z. Papaver ; 
F. 119. Sonnet de René de la Ferté [publié par L'Epoque] ; 
F. 120. La Transalpine, chant national pour l'Italie, par V. Chammas ; 
F. 121. Le Géant vaincu par le Hanneton [chanson] ; 
F. 122-123. Le Canon d'Alarme [n° de septembre 1848], publiant Hodie par Raymond Brucker ; 
F. 124. Titre : Politique ; 
F. 125. Notes de Flaubert sur le socialisme de Montesquieu ; 
F. 126. Liste de 31 ouvrages relatifs au sujet ci-dessus ; 
F. 127-177. Notes sur chacun de ces ouvrages ; 
F. 178. Titre : Religion - Mysticisme - Prophéties ; 
F. 179-197. Citations empruntées à divers auteurs pour illustrer les titres ci-dessus ; 
F. 198.Titre : Religion ; 
F. 199-200. Liste de 76 ouvrages relatifs au sujet ci-dessus ; 
F. 201-314. Notes sur chacun de ces ouvrages ; 
F. 315-328. Résumés de notes sur la religion [chapitre IX de 
Bouvard et Pécuchet].
Evaluation of Malathion, Synergized Pyrethrum, and Diatomaceous Earth as Wheat Protectants ... In Small Bins
Creators: name: La Hue, Delmon W.
name: La Hue, Delmon W.
Publisher: name: Unknown
Year: 1965
Subjects: Crop Production/Industries
Research and Development/Tech Change/Emerging Technologies

description: Excerpts from the report: The primary objective of this study was to compare the effectiveness of malathion and synergized pyrethrum emulsions and a diatomaceous earth dust as wheat protectants in small bins—a method that is intermediate between large field-scale applications and small jar tests in the laboratory. This work is a part of a broad program of research to improve the quality of food that reaches the consumer by preventing damage in marketing channels.
Asterias equestris Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Forcipulatida
Asteriidae
Asterias
Asterias equestris

description: Asterias equestris [spec. nov.]
A. stellata disco reticulato punctis pertuso, tuberculis 5, margine subarticulato subtus simplici serie tentaculato.
Barr. icon. 1285.
Link. stell. t. 6. f. 13; t. 12. f. 21; t. 13. f. 22; t. 23. f. 37; t. 24. f. 39; t. 27. f. 45; t. 33. f. 53.
Habitat in M. Mediterraneo.
Haec etiam subtus disco gaudet, non prior.
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 662, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Quantum Spectral Curve of $γ$-twisted ${\cal N}=4$ SYM theory and fishnet CFT
Creators: name: Kazakov, Vladimir
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We review the quantum spectral curve (QSC) formalism for anomalous dimensions of planar ${\cal\ N}=4$ SYM, including its $γ$-deformation. Leaving aside its derivation, we concentrate on formulation of the "final product" in its most general form: a minimal set of assumptions about the algebraic structure and the analyticity of the $Q$-system -- the full system of Baxter $Q$-functions of the underlying integrable model. The algebraic structure of the $Q$-system is entirely based on (super)symmetry of the model and is efficiently described by Wronskian formulas for $Q$-functions organized into the Hasse diagram. When supplemented with analyticity conditions on $Q$-functions, it fixes completely the set of physical solutions for spectrum of an integrable model. First we demonstrate the spectral equations on the example of $gl(N)$ and $gl(K|M)$ Heisenberg (super)spin chains. Supersymmetry $gl(K|M)$ occurs as a "rotation" of the Hasse diagram for a $gl(K+M)$ system. This picture helps us to construct the QSC formalism for spectrum of AdS$_5$/CFT$_4$-duality, with more complicated analyticity constraints on $Q$-functions which involve an infinitely branching Riemann surface and a set of Riemann-Hilbert conditions. As an example of application of QSC, we consider a special double scaling limit of $γ$-twisted ${\cal\ N}=4$ SYM, combining weak coupling and strong imaginary twist. This leads to a new type of non-unitary CFT dominated by particular integrable, and often computable, 4D fishnet Feynman graphs. For the simplest of such models -- the bi-scalar theory -- the QSC degenerates into the $Q$-system for integrable non-compact Heisenberg spin chain with conformal, $SU(2,2)$ symmetry. We apply the QSC for derivation of Baxter equation and the quantization condition for particular, "wheel" fishnet graphs, and review numerical and analytic results for them.
description: 52 pages
Stellar Populations at the Center of IC 1613
Creators: name: Cole, Andrew A.
name: Tolstoy, Eline
name: Gallagher, John S.
name: Hoessel, John G.
name: Mould, Jeremy R.
name: Holtzman, Jon A.
name: Saha, Abhijit
name: Ballester, Gilda E.
name: Burrows, Christopher J.
name: Clarke, John T.
name: Crisp, David
name: Griffiths, Richard E.
name: Grillmair, Carl J.
name: Hester, Jeff J.
name: Krist, John E.
name: Meadows, Vikki
name: Scowen, Paul A.
name: Stapelfeldt, Karl R.
name: Trauger, John T.
name: Watson, Alan M.
name: Westphal, James R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have observed the center of the Local Group dwarf irregular galaxy IC 1613 with WFPC2 aboard the Hubble Space Telescope in the F439W, F555W, and F814W filters. We find a dominant old stellar population (aged ~7 Gyr), identifiable by the strong red giant branch (RGB) and red clump populations. From the (V-I) color of the RGB, we estimate a mean metallicity of the intermediate-age stellar population [Fe/H] = -1.38 +/- 0.31. We confirm a distance of 715 +/- 40 kpc using the I-magnitude of the RGB tip. The main-sequence luminosity function down to I ~25 provides evidence for a roughly constant SFR of approximately 0.00035 solar masses per year across the WFPC2 field of view (0.22 square kpc) during the past 250-350 Myr. Structure in the blue loop luminosity function implies that the SFR was ~50% higher 400-900 Myr ago than today. The mean heavy element abundance of these young stars is 1/10th solar. The best explanation for a red spur on the main-sequence at I = 24.7 is the blue horizontal branch component of a very old stellar population at the center of IC 1613. We have also imaged a broader area of IC 1613 using the 3.5-meter WIYN telescope under excellent seeing conditions. The AGB-star luminosity function is consistent with a period of continuous star formation over at least the age range 2-10 Gyr. We present an approximate age-metallicity relation for IC 1613, which appears similar to that of the Small Magellanic Cloud. We compare the Hess diagram of IC 1613 to similar data for three other Local Group dwarf galaxies, and find that it most closely resembles the nearby, transition-type dwarf galaxy Pegasus (DDO 216).
description: To appear in the September 1999 Astronomical Journal. LaTeX, uses AASTeX v4.0, emulateapj style file, 19 pages, 12 postscript figures, 2 tables. 5 of the figures available separately via the WWW
title: Конструирование и выполнение в материале изделий из кожи. Курс лекций
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2018

description: В пособии нашли отражение важные вопросы проектирования обуви. Качество проектирования моделей обуви во многом зависит от умения разработчика получать точное отображение развертки боковой поверхности колодки, по которой проводится проектирование наружных деталей заготовки верха обуви, на плоскости. В связи с этим методикам получения усредненной развертки боковой поверхности колодки (УРК) уделено пристальное внимание. Освещено несколько подходов к получению УРК, дано обоснование приемлемости той или иной методики для работы над проектом конкретной модели обуви. Обобщены достоинства и недостатки того или иного подхода, разработан специальный раздел, поясняющий обучающимся, как правильно комбинировать приемы работы из разных методик для достижения точности проектных работ. Основные положения отечественной графо-копировальной системы моделирования, основывающиеся на проектировании базовых моделей обуви с использованием базисных и вспомогательных линий, обновлены с учетом изменений, касающихся исходных размеров родовых групп. Сопоставлению размеров обуви метрической и штихмассовой систем нумерации уделено особое внимание. Нормативная документация не дает полного представления о сопоставимости размеров двух систем, одна из которых лежит в основе положений отечественных методик проектирования, а вторая является господствующей на рынке сбыта. Разночтения положений нормативной документации нуждаются в констатации и обсуждении в рамках курса конструирования и изготовления изделий из кожи. В пособии обновлен и дополнен материал методики ОДМО по проектированию конструктивных основ ботинок. Изменения в исходных размерах родовых групп нашли отражение и в представленных в соответствующем разделе таблицах. Предназначено для использования в учебном процессе.
Herramientas de apoyo a la actividad científica
Creators: name: Pallares, César
Publisher: name: Zenodo
Year: 2019
Subjects: Open science
Open Access
Visibility
Zenodo

description: Esta presentación da un breve resumen de herramientas que apoyan a la actividad científica en pro de la visibilidad y de ajustar a los investigadores a las nuevas dinámicas de la ciencia abierta
description: {"references": ["Universidad de Navarra (2017). Como usar Mendeley. En l\u00ednea: https://www.youtube.com/watch?v=5Uc4e6ULzI4"]}
Asterias ophiura Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Forcipulatida
Asteriidae
Asterias
Asterias ophiura

description: Asterias ophiura [spec. nov.]
A. radiata radiis quinque, corpore orbiculato quinquelobo.
Rumph. mus. 40. t. 15. f. B. C.
Pet. amb. t. 3. f. C. Stella marina V. scolopendroides.
Barr. rar. 131. t. 1295. Stella marina ophiocnemos s. ophiurus.
Sloan. jam. 2. p. 272. t. 244. f. 8, 9. Stella marina minor echinata purpurea.
Martens. spitzb. t. P. f. D.
Link. stell. t. 2. f. 4; t. 11. f. 17; t. 22. f. 35. Stella marina.
Habitat in Oceano.
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 662, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title: Консалтинг в связях с общественностью
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2017

description: Учебное издание соответствует содержанию федеральной дисциплины базовой части Б1.Б.31 Консалтинг в связях с общественностью направления подготовки 42.03.01 Реклама и связи с общественностью профиль Реклама и связи с общественностью в коммерческой сфере.
Emergence of Topological insulator and Nodal line semi-metal states in XX'Bi (X=Na, K, Rb, Cs; X'=Ca, Sr)
Creators: name: Mondal, Chiranjit
name: Barman, C. K.
name: Kumar, Sourabh
name: Alam, Aftab
name: Pathak, Biswarup
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: In this letter, we predict the emergence of non-trivial band topology in the family of XX'Bi compounds having $P\overline{6}2m$ (\# 189) space group. Using first principles calculations within hybrid functional framework, we demonstrate that NaSrBi and NaCaBi are strong topological insulator under controlled band engineering. Here, we propose three different ways to engineer the band topology to get a non-trivial order: (i) hydrostatic pressure, (ii) biaxial strain (due to epitaxial mismatch), and (iii) doping. Non-triviality is confirmed by investigating bulk band inversion, topological Z$_2$ invariant, surface dispersion and spin texture. Interestingly, some of these compounds also show a three dimensional topological nodal line semi-metal (NLS) state in the absence of spin orbit coupling (SOC). In these NLS phases, the closed loop of band degeneracy in the Brillouin zone lie close to the Fermi level. Moreover, a drumhead like flat surface state is observed on projecting the bulk state on the [001] surface. The inclusion of SOC opens up a small band gap making them behave like a topological insulator.
Asterias multiradiata Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Forcipulatida
Asteriidae
Asterias
Asterias multiradiata

description: Asterias multiradiata [spec. nov.]
A. radiata radiis palmato-multiplicatis pinnatis: inferioribus filiformibus.
Link. stell. t. 21. f. 33, t. 22. f. 34. Stella marina.
Habitat in M. Indico.
Valde affinis A. pectinatae, si non sola varietas.
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 663, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
A High-Order Weighted Compact High Resolution Scheme with Boundary Closures for Compressible Turbulent Flows with Shocks
Creators: name: Subramaniam, A.
name: Wong, M. L.
name: Lele, S. K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We present an improved high-order weighted compact high resolution (WCHR) scheme that extends the idea of weighted compact nonlinear schemes (WCNS's) using nonlinear interpolations in conjunction with compact finite difference schemes for shock-capturing in compressible turbulent flows. The proposed scheme has better resolution property than previous WCNS's. This is achieved by using a compact (or spatially implicit) form instead of the traditional fully explicit form for the nonlinear interpolation. Since compact interpolation schemes tend to have lower dispersion errors compared to explicit interpolation schemes, the proposed scheme has the ability to resolve more fine-scale features while still having the ability to provide sufficiently localized dissipation to capture shocks and discontinuities robustly. Approximate dispersion relation characteristics of this scheme are analyzed to show the superior resolution properties of the scheme compared to other WCNS's of similar orders of accuracy. Conservative and high-order accurate boundary schemes are also proposed for non-periodic problems. Further, a new conservative flux-difference form for compact finite difference schemes is derived and allows for the use of positivity-preserving limiters for improved robustness. Different test cases demonstrate the ability of this scheme to capture discontinuities in a robust and stable manner while also localizing the required numerical dissipation only to regions containing discontinuities and very high wavenumber features and hence preserving smooth flow features better in comparison to WCNS's.
title: Компьютерная графика и дизайн художественных изделий. Теория и практика
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2019

description: Целью учебного пособия является предоставление студентам систематически изложенной информации об управлении программным комплексом 3Ds MAX, а также практикума с пояснениями и упражнениями, которые понадобятся студентам в подготовке курсовых проектов, реализации творческих задач, а также в условиях самостоятельной работы обучающихся. Учебное пособие разработано на основе многолетней практической и учебно-методической работы сотрудников кафедры ТХОМиЮИ. Предназначено для студентов всех форм обучения направления подготовки 29.03.04 – Технология художественной обработки материалов и может использоваться при изучении дисциплин «Компьютерная графика и дизайн художественных изделий», «Компьютерная графика и дизайн ювелирных изделий».
CN and CH Band Strengths of Bright Giants in M3
Creators: name: Lee, Sang-Gak
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: CN and CH band strengths for ten bright red giants in M3 have been measured from archival spectra obtained with the MMT. A CN-CH band strength anticorrelation is confirmed for the program stars together with other stars for which there is published data. This suggests an anticorrelation between carbon and nitrogen abundances with a constant total abundance of carbon plus nitrogen. However, stars which do not follow the CN-CH anticorrelation are also found. The star III-77, which is found to have both strong CN and CH bands, is the most peculiar among them. While three other stars, VZ194, VZ352, and VZ1420, which show both weak CN and CH band strengths could be AGB stars.
description: 10 pages, 5 figures, 1 table
Additional file 1 of Reading activities compensate for low education-related cognitive deficits
Creators: name: Wang, Yue
name: Wang, Shinan
name: Zhu, Wanlin
name: Liang, Na
name: Zhang, Chen
name: Pei, Yuankun
name: Wang, Qing
name: Li, Shiping
name: Shi, Jiong
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Neuroscience
subject: Pharmacology
subject: Science Policy
subject: Sociology
subject: FOS: Sociology
subject: Mental Health

description: Additional file 1: Supplemental Table 1. Cognitive performance of participants having different reading years.
LeMMINGs. I. The eMERLIN legacy survey of nearby galaxies. 1.5-GHz parsec-scale radio structures and cores
Creators: name: Baldi, R. D.
name: Williams, D. R. A.
name: McHardy, I. M.
name: Beswick, R. J.
name: Argo, M. K.
name: Dullo, B. T.
name: Knapen, J. H.
name: Brinks, E.
name: Muxlow, T. W. B.
name: Aalto, S.
name: Alberdi, A.
name: Bendo, G. J.
name: Corbel, S.
name: Evans, R.
name: Fenech, D. M.
name: Green, D. A.
name: Klöckner, H. -R.
name: Körding, E.
name: Kharb, P.
name: Maccarone, T. J.
name: Martí-Vidal, I.
name: Mundell, C. G.
name: Panessa, F.
name: Peck, A. B.
name: Pérez-Torres, M. A.
name: Saikia, D. J.
name: Saikia, P.
name: Shankar, F.
name: Spencer, R. E.
name: Stevens, I. R.
name: Uttley, P.
name: Westcott, J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the first data release of high-resolution ($\leq0.2$ arcsec) 1.5-GHz radio images of 103 nearby galaxies from the Palomar sample, observed with the eMERLIN array, as part of the LeMMINGs survey. This sample includes galaxies which are active (LINER and Seyfert) and quiescent (HII galaxies and Absorption line galaxies, ALG), which are reclassified based upon revised emission-line diagrams. We detect radio emission $\gtrsim$ 0.2 mJy for 47/103 galaxies (22/34 for LINERS, 4/4 for Seyferts, 16/51 for HII galaxies and 5/14 for ALGs) with radio sizes typically of $\lesssim$100 pc. We identify the radio core position within the radio structures for 41 sources. Half of the sample shows jetted morphologies. The remaining half shows single radio cores or complex morphologies. LINERs show radio structures more core-brightened than Seyferts. Radio luminosities of the sample range from 10$^{32}$ to 10$^{40}$ erg s$^{-1}$: LINERs and HII galaxies show the highest and the lowest radio powers respectively, while ALGs and Seyferts have intermediate luminosities. We find that radio core luminosities correlate with black hole (BH) mass down to $\sim$10$^{7}$ M$_{\odot}$, but a break emerges at lower masses. Using [O III] line luminosity as a proxy for the accretion luminosity, active nuclei and jetted HII galaxies follow an optical fundamental plane of BH activity, suggesting a common disc-jet relationship. In conclusion, LINER nuclei are the scaled-down version of FR I radio galaxies; Seyferts show less collimated jets; HII galaxies may host weak active BHs and/or nuclear star-forming cores; and recurrent BH activity may account for ALG properties.
description: accepted for publication on MNRAS (45 pages, 10 figures with reduced image quality)
Asterias aranciaca Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Forcipulatida
Asteriidae
Asterias
Asterias aranciaca

description: Asterias aranciaca [spec. nov.]
A. stellata disco tentaculis hispidis muricato, margine articulato, varie aculeato.
Mus. Tess. 114. t. 9. f. 3.
Barr. ic. 1281.
Link. stell. t. 4. f. 14; t. 5. f. 6; t. 8. f. 12; t. 23. f. 38; t. 27. f. 44; t. 36. f. 63.
Habitat in M. Mediterraneo.
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 662, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Two-Loop Radiative Corrections to the Lightest Higgs Boson Mass in the Minimal Supersymmetric Model
Creators: name: Hempfling, Ralf
name: Hoang, Andre H.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the minimal supersymmetric model (MSSM), the upper limit of the lightest Higgs boson mass, $\mhl$, depends strongly on the top quark mass, $m_t$. We have computed the dominant two-loop radiative corrections to this upper limit of $\mhl$ in order to eliminate large uncertainties due to QCD and $m_t^6$ corrections. It is shown that the QCD corrections significantly reduce the one-loop corrections. As a result, the SUSY parameter space accessible to LEP experiments is significantly increased.
description: 14 pages using PHYZZX, 4 figs. are appended as PS-files
title: ADCO, Ordre cistercien : comptes (1499-1515) (11 H 1162), f. 00316
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: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes

description: Ordre cistercien : comptes (1499-1515), Archives départementales de la Côte-d'Or, (11 H 1162). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien : comptes (1499-1515), Archives départementales de la Côte-d'Or, (11 H 1162), f. 00316, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Dust Properties of NGC4753
Creators: name: Dewangan, G. C.
name: Singh, K. P.
name: Bhat, P. N.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report BVR surface photometry of a lenticular galaxy, NGC4753 with prominent dust lanes. We have used the multicolor broadband photometry to study dust-extinction as a function of wavelength and derived the extinction curve. We find the extinction curve of NGC 4753 to be similar to the Galactic extinction curve in the visible region which implies that the sizes of dust grains responsible for optical extinction are similar to those in our Galaxy. We derive dust mass from optical extinction as well as from the far infrared fluxes observed with IRAS. The ratio of the two dust masses, $\frac{M_{d,IRAS}}{M_{d,optical}}$, is 2.28 for NGC 4753, which is significantly lower than the value of 8.4 \pm 1.3 found previously for a large sample of elliptical galaxies. The total mass of the observed dust within NGC4753 is about a factor of 10 higher than the mass of dust expected from loss of mass from red giant stars and destruction by sputtering and grain-grain collisions in low velocity shocks, and sputtering in supernova driven blast waves. We find evidence for the coexistence of dust and H$α$ emitting gas within NGC4753. The current star formation rate of NGC4753, averaged over past $2\times10^{6} yr$, is estimated to be less than $0.21M_{\sun}yr^{-1}$. A substantial amount of dust within NGC4753 exists in the form of cirrus.
description: 15 pages, 8 jpeg figures, 5 tables in one file, AASTEX style, Accepted for publication in the Astronomical Journal, 1999 August
Satellites of Infinite Rank in the Smooth Concordance Group
Creators: name: Hedden, Matthew
name: Pinzon-Caicedo, Juanita
Publisher: name: arXiv
Year: 2018
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 57M25, 57N70, 57M27

description: We conjecture that satellite operations are either constant or have infinite rank in the concordance group. We reduce this to the difficult case of winding number zero satellites, and use $SO(3)$ gauge theory to provide a general criterion sufficient for the image of a satellite operation to generate an infinite rank subgroup of the smooth concordance group $\mathcal{C}$. Our criterion applies widely; notably to many unknotted patterns for which the corresponding operators on the topological concordance group are zero. We raise some questions and conjectures regarding satellite operators and their interaction with concordance.
description: Significant changes and improvements to exposition. Numerous minor corrections and updates
The Two-mass Contribution to the Three-Loop Gluonic Operator Matrix Element $A_{gg,Q}^{(3)}$
Creators: name: Ablinger, J.
name: Blümlein, J.
name: De Freitas, A.
name: Goedicke, A.
name: Schneider, C.
name: Schönwald, K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We calculate the two-mass QCD contributions to the massive operator matrix element $A_{gg,Q}$ at $\mathcal{O} (α_s^3)$ in analytic form in Mellin $N$- and $z$-space, maintaining the complete dependence on the heavy quark mass ratio. These terms are important ingredients for the matching relations of the variable flavor number scheme in the presence of two heavy quark flavors, such as charm and bottom. In Mellin $N$-space the result is given in the form of nested harmonic, generalized harmonic, cyclotomic and binomial sums, with arguments depending on the mass ratio. The Mellin inversion of these quantities to $z$-space gives rise to generalized iterated integrals with square root valued letters in the alphabet, depending on the mass ratio as well. Numerical results are presented.
description: 99 pages LATEX, 2 Figures
Asterias caputmedusae Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Forcipulatida
Asteriidae
Asterias
Asterias caputmedusae

description: Asterias caputmedusae [spec. nov.]
A. radiata radiis dichotomis.
Mus. Ad. Fr. 1. p. 95.
Rumph. mus. 41. t. 16. Caput Medusae.
Martens. spitzb. t. P. f. E.
Link. stell. t. 18. f. 29; t. 19. f. 30, 31; t. 20. f. 32; t. 29. f. 48; t. 30. f. 49.
Habitat in omni Oceano, imprimis Pelagico.
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 663, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title: Коммуникационный менеджмент
Creators: name: ELS IPR BOOKS
Publisher: name: Санкт-Петербургский государственный университет промышленных технологий и дизайна
Year: 2019

description: Учебное издание соответствует содержанию дисциплины Б1.В.ДВ.5 Коммуникационный менеджмент направления подготовки 42.03.01 Реклама и связи с общественностью профиль Реклама и связи с общественностью в коммерческой сфере.
Amiota (Amiota) okinawana Okada 1971
Creators: name: Chen, Hong-Wei
name: Toda, Masanori J.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Drosophilidae
Amiota
Amiota okinawana

description: Amiota (Amiota) okinawana Okada
 Amiota (Amiota) okinawana Okada, 1971: 86; Toda and Peng, 1992: 202; Máca and Lin, 1993: 2.
 Diagnosis. Paramere about 1.8 times as long as aedeagus, apically less sclerotized and much narrower than aedeagus.
 Specimens examined. Japan: Holotype, Komi, Iriomote, Ryukyu Is., 9 July 1966, T. Okada and F. H ihara leg. (N SM T); Iriomote, R yukyu Is., 4, 1 July 1998, tree trunks, M. T. Kimura leg. China: Dinghushan, Guangdong, 6, 31 August 6 September 1988, ex banana traps, T. X. Peng leg.
 Distribution. China (Taiwan, G uangdon g), Japan (R yukyu Is.).
description: Published as part of Chen, Hong-Wei & Toda, Masanori J., 2001, A revision of the Asian and European species in the subgenus Amiota Loew (Diptera, Drosophilidae) and the establishment of species-groups based on phylogenetic analysis, pp. 1517-1563 in Journal of Natural History 35 (10) on page 1529, DOI: 10.1080/002229301317067665, http://zenodo.org/record/10683624
Electroweak String Configurations with Baryon Number
Creators: name: Vachaspati, Tanmay
name: Field, George B.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the context of electroweak strings, the baryon number anomaly equation may be reinterpreted as a conservation law for baryon number minus helicity. Since the helicity is a sum of the link and twist numbers, linked or twisted loops of electroweak string carry baryon number. We evaluate the change in the baryon number obtained by delinking loops of electroweak $Z-$string and show that twisted electroweak string segments may be regarded as extended sphalerons. We also suggest an alternative scenario for electroweak baryogenesis.
description: 11 pages, figure available on request. Added discussion of string-sphaleron connection for non-vanishing Weinberg angle and shortened discussion on formation of linked configurations
The Minor-Merger Driven Nuclear Activity in Seyfert Galaxies: A Step toward the Simple Unified Formation Mechanism of Active Galactic Nuclei in the Local Universe
Creators: name: Taniguchi, Yoshiaki
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Seyfert nuclei are typical active galactic nuclei (AGNs) in the local universe, which are thought to be powered by gas accretion onto a supermassive black hole (SMBH). The dynamical effect exerted either by non-axisymmetric gravitational potential (such as a stellar bar) or by interaction with other galaxies has been often considered to cause the efficient gas fueling. However, recent systematic studies for large samples of Seyfert nuclei have shown that; 1) Seyfert nuclei do not prefer barred galaxies as their hosts, and 2) only $\simeq$ 10% of Seyfert galaxies have companion galaxies. These findings raise again a question; "What is important in the fueling of nuclear activity ?" Here we suggest that an alternative fueling mechanism, the minor-merger (i.e., mergers between a gas-rich disk galaxy and a bound, less-massive satellite galaxy) driven fueling appears consistent with almost all important observational properties of Seyfert galaxies. Nucleated (i.e., either a SMBH or a dense nuclear star cluster) galaxies and satellites seem necessary to ensure that the gas in the host disk is surely fueled into the very inner region (e.g., $\ll$ 1 pc). Taking account that local quasars may be formed by major mergers between/among galaxies, we propose that all the AGNs in the local universe were made either by minor or by major mergers.
description: 7 pages, 1 figure. The Astrophysical Journal, Part 1, in press
Bounds on the Error Probability of Raptor Codes under Maximum Likelihood Decoding
Creators: name: Lázaro, Francisco
name: Liva, Gianluigi
name: Bauch, Gerhard
name: Paolini, Enrico
Publisher: name: arXiv
Year: 2018
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: In this paper upper and lower bounds on the probability of decoding failure under maximum likelihood decoding are derived for different (nonbinary) Raptor code constructions. In particular four different constructions are considered; (i) the standard Raptor code construction, (ii) a multi-edge type construction, (iii) a construction where the Raptor code is nonbinary but the generator matrix of the LT code has only binary entries, (iv) a combination of (ii) and (iii). The latter construction resembles the one employed by RaptorQ codes, which at the time of writing this article represents the state of the art in fountain codes. The bounds are shown to be tight, and provide an important aid for the design of Raptor codes.
description: Accepted in IEEE Transactions on Information Theory
title: ADCO, Grènetier de Cîteaux : comptes (1499-1503) (11 H 1173), f. 00598
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
name: Petot, Frédéric
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: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173), f. 00598, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
MPEC 2024-K91 : 2019 WU35
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2019 WU35

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
The Higher Derivative Expansion of the Effective Action by the String-Inspired Method, Part I
Creators: name: Fliegner, D.
name: Schmidt, M. G.
name: Schubert, C.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The higher derivative expansion of the one-loop effective action for an external scalar potential is calculated to order O(T**7), using the string-inspired Bern-Kosower method in the first quantized path integral formulation. Comparisons are made with standard heat kernel calculations and with the corresponding Feynman diagrammatic calculation in order to show the efficiency of the present method.
description: 13 pages, Plain TEX, 1 figure may be obtained from the authors, HD-THEP-93-44