cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Dirichlet process mixtures under affine transformations of the data
Creators: name: Arbel, Julyan
name: Corradin, Riccardo
name: Nipoti, Bernardo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Methodology (stat.ME)
subject: FOS: Computer and information sciences
subject: 62G07, 62F15, 62G35

description: Location-scale Dirichlet process mixtures of Gaussians (DPM-G) have proved extremely useful in dealing with density estimation and clustering problems in a wide range of domains. Motivated by an astronomical application, in this work we address the robustness of DPM-G models to affine transformations of the data, a natural requirement for any sensible statistical method for density estimation and clustering. First, we devise a coherent prior specification of the model which makes posterior inference invariant with respect to affine transformations of the data. Second, we formalise the notion of asymptotic robustness under data transformation and show that mild assumptions on the true data generating process are sufficient to ensure that DPM-G models feature such a property. Our investigation is supported by an extensive simulation study and illustrated by the analysis of an astronomical dataset consisting of physical measurements of stars in the field of the globular cluster NGC 2419.
description: 36 pages, 7 Figures
Morphology of the 12-micron Seyfert Galaxies: II. Optical and Near-Infrared Image Atlas
Creators: name: Hunt, L. K.
name: Malkan, M. A.
name: Rush, B.
name: Bicay, M. D.
name: Nelson, B. O.
name: Stanga, R. M.
name: Webb, W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present 263 optical and near-infrared (NIR) images for 42 Seyfert 1s and 48 Seyfert 2s, selected from the Extended 12-micron Galaxy Sample. Elliptically-averaged profiles are derived from the images, and isophotal radii and magnitudes are calculated from these. We also report virtual aperture photometry, that judging from comparison with previous work, is accurate to roughly 0.05mag in the optical, and 0.07mag in the NIR. Our B-band isophotal magnitude and radii, obtained from ellipse fitting, are in good agreement with those of RC3. When compared with the B band, V, I, J, and K isophotal diameters show that the colors in the outer regions of Seyferts are consistent with the colors of normal spirals. Differences in the integrated isophotal colors and comparison with a simple model show that the active nucleus+bulge is stronger and redder in the NIR than in the optical. Finally, roughly estimated Seyfert disk surface brightnesses are significantly brighter in B and K than those in normal spirals of similar morphological type.
description: 17 pgs including figures; Table 2 is a separate file. Complete Figure 1 is available by contacting the authors. Accepted for publication in ApJS
The VLT-FLAMES Tarantula Survey: XXVIII. Nitrogen abundances for apparently single dwarf and giant B-type stars with small projected rotational velocities
Creators: name: Dufton, P. L.
name: Thompson, A.
name: Crowther, P. A.
name: Evans, C. J.
name: Schneider, F. R. N.
name: de Koter, A.
name: de Mink, S. E.
name: Garland, R.
name: Langer, N.
name: Lennon, D. J.
name: McEvoy, C. M.
name: Ramírez-Agudelo, O. H.
name: Sana, H.
name: Díaz, S. Símon
name: Taylor, W. D.
name: Vink, J. S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Previous analyses of the spectra of OB-type stars in the Magellanic Clouds have identified targets with low projected rotational velocities and relatively high nitrogen abundances. The VFTS obtained spectroscopy for B-type 434 stars. We have estimated atmospheric parameters and nitrogen abundances using TLUSTY model atmospheres for 54 B-type targets that appear to be single, have projected rotational velocities <80 \kms and were not classified as supergiants. In addition, nitrogen abundances for 34 similar stars from a previous survey have been re-evaluated. Approximately 75-80% of the targets have nitrogen enhancements of less than 0.3 dex, consistent with them having experienced only small amounts of mixing. However, stars with low projected rotational velocities <40 \kms and significant nitrogen enrichments are found in both our samples and simulations imply that these cannot all be rapidly rotating objects observed near pole-on. Adopting an enhancement threshold of 0.6 dex, we observed five stars, yet stellar evolution models with rotation predict only 1.25$\pm$1.11 for random stellar viewing inclinations. The excess of such objects is estimated to be 20-30% of all stars with current rotational velocities of less than 40 \kms and 2-4% of the total single B-type sample. These estimates constitute lower limits for stars that appear inconsistent with current grids of stellar evolutionary models. Including targets with smaller nitrogen enhancements of greater than 0.2 dex implies larger percentages of targets that are inconsistent with current evolutionary models, viz. 70% of the stars with rotational velocities less than 40 \kms and 6-8% of the total single stellar population. We consider possible explanations of which the most promising would appear to be breaking due to magnetic fields or stellar mergers with subsequent magnetic braking.
description: Accepted in Astronomy and Astrophyics. Abstract significantly shortened - see paper for full abstract
Possible Long-Lived Asteroid Belts in the Inner Solar System
Creators: name: Evans, Wyn
name: Tabachnik, Serge
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The recent years have witnessed a carnival of discoveries in the Outer Solar System. Here we provide evidence from numerical simulations of orbital stability to suggest the possible existence of two long lived belts of primordial planetesimals in the Solar System. The first is the domain of the Vulcanoids (between 0.09 - 0.21 AU) between the Sun and Mercury, where remnant planetesimals may survive on dynamically stable orbits provided they possess a characteristic radius greater than 0.1 km. The second is a belt between the Earth and Mars (1.08 -1.28 AU) on which an initial population of particles on circular orbits may survive for the age of the Solar System. A search through the catalogues of Near-Earth Objects reveals an excess of asteroids with low eccentricities and inclinations occupying this belt, such as the recently discovered objects 1996 XB27, 1998 HG49 and 1998 KG3.
description: 10 pages, 1 figure, appearing in 6th May issue of Nature
Dynamical Phase Transition of two-component Bose-Einstein condensate with nonlinear tunneling in an optomechanical cavity-mediated double-well system
Creators: name: Li, Qing
name: Tan, Lei
name: Ma, Jin-Lou
name: Gu, Huai-Qiang
name: Shi, Yun-Xia
name: Liu, Wu-Ming
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We investigate the dynamical phase transition of two-component Bose-Einstein condensate with nonlinear tunneling, which is trapped inside a double-well and dispersively coupled to a single mode of a high-finesse optical cavity with one moving end mirror driven by a single mode standing field. The nonlinear tunneling interaction leads to an increase of stability points and riches the phase diagram of the system. It is shown that the appearance of the moving end mirror speeds up the tunneling of Bose-Einstein condensates, which makes population difference between two wells and regulates the number of the stability points of the system.
description: 9 pages, 7 figures
Filter-linkedness and its effect on preservation of cardinal characteristics
Creators: name: Brendle, Jörg
name: Cardona, Miguel A.
name: Mejía, Diego A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Logic (math.LO)
subject: FOS: Mathematics
subject: 03E17, 03E15, 03E35, 03E40

description: We introduce the property ``$F$-linked'' of subsets of posets for a given free filter $F$ on the natural numbers, and define the properties ``$μ$-$F$-linked'' and ``$θ$-$F$-Knaster'' for posets in a natural way. We show that $θ$-$F$-Knaster posets preserve strong types of unbounded families and of maximal almost disjoint families. Concerning iterations of such posets, we develop a general technique to construct $θ$-$\mathrm{Fr}$-Knaster posets (where $\mathrm{Fr}$ is the Frechet ideal) via matrix iterations of ${
description: 30 pages, 7 figures
Cultivation of autotrophic nitrifying granular sludge for simultaneous removal of ammonia nitrogen and Tl(I)
Creators: name: Zeng, Yu
name: Zeng, Mingjing
name: Cheng, Yuanyuan
name: Long, Bei
name: Wu, Junfeng
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Infectious Diseases
subject: FOS: Health sciences

description: Autotrophic nitrifying granular sludge (ANGS) was cultivated for the simultaneous removal of ammonia nitrogen and Tl(I) from inorganic wastewater. The chemical oxygen demand (COD) in the influent gradually decreased to approximately zero in four parallel sequencing batch reactors (B1: blank controller, B2: 10 mL of added nitrifying bacteria concentrate in each cycle, B3: 1 mg/L Tl(I) added in each cycle and B4: 10 mL of added nitrifying bacteria concentrate and 1 mg/L Tl(I) in each cycle) within 15 days. The main properties, such as the granulation rate and specific oxygen uptake rate (SOUR) of the ANGS in B1, B2, B3 and B4 tended to be stable within 40, 33, 30 and 33 days, the removal efficiencies of Tl(I) were 59.5%–82.9% and 57.1%–88.6% in B3 and B4 after Day 30, the removal efficiencies of ammonia nitrogen in B1, B2, B3 and B4 were usually above 90% after Day 33, and the total inorganic nitrogen (TIN) in the effluent of B1, B2, B3 and B4 gradually stabilized after Day 36, 32, 32 and 36, indicating that mature ANGS was successfully cultivated in B1, B2, B3 and B4 within 40, 33, 33 and 36 days. The nitrogen degradation kinetic parameters of ANGS indicated that B3 had the strongest ability to remove ammonia and nitrite, suggesting that Tl(I) stress was beneficial to ammonia nitrogen removal and nitrite oxidation. The adsorption of Tl(I) can be described by the Freundlich equation, and the addition of external nitrifying bacteria improved the adsorption ability of ANGS.
Cumulant to Factorial Moment Ratio and Multiplicity Data
Creators: name: Dremin, I. M.
name: Arena, V.
name: Boca, G.
name: Gianini, G.
name: Malvezzi, S.
name: Merlo, M.
name: Ratti, S. P.
name: Riccardi, C.
name: Salvadori, G.
name: Viola, L.
name: Vitulo, P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The ratio of cumulant to factorial moments of experimental multiplicity distributions has been calculated for $e^{+}e^{-}$ and $hh$ interactions in a wide range of energies. As a function of the rank it exhibits an initial steep decrease and a series of oscillations around zero. Those features cannot be reproduced by the Negative Binomial Distribution. A comparable behaviour is instead predicted in high-energy perturbative QCD. The presence of a qualitatively similar behaviour for different processes and in wide energy intervals suggests speaking of an approximate scaling of the cumulant to factorial moment ratio.
description: Submitted to Phys.Lett.B; Latex document, 11 pages, 4 PostScript figures appended. Preprint number FIAN/TD-15/93 also FNT/AE 93-25
Individual project on theme "Corvus L." (MOOC: CompTech in biology)
Creators: name: Kuryan, Ekaterina
Publisher: name: Zenodo
Year: 2025

description: Данный кейс является результатом реализации индивидуального проекта Курьян Екатерины по теме "Corvus L." в рамках онлайн курса "Компьютерные технологии в биологии" (автор – А.В. Ваганов) (https://stepik.org/course/60859/promo)
The contribution of faint AGNs to the ionizing background at z~4
Creators: name: Grazian, A.
name: Giallongo, E.
name: Boutsia, K.
name: Cristiani, S.
name: Vanzella, E.
name: Scarlata, C.
name: Santini, P.
name: Pentericci, L.
name: Merlin, E.
name: Menci, N.
name: Fontanot, F.
name: Fontana, A.
name: Fiore, F.
name: Civano, F.
name: Castellano, M.
name: Brusa, M.
name: Bonchi, A.
name: Carini, R.
name: Cusano, F.
name: Faccini, M.
name: Garilli, B.
name: Marchetti, A.
name: Rossi, A.
name: Speziali, R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Finding the sources responsible for the hydrogen reionization is one of the most pressing issues in cosmology. Bright QSOs are known to ionize their surrounding neighborhood, but they are too few to ensure the required HI ionizing background. A significant contribution by faint AGNs, however, could solve the problem, as recently advocated on the basis of a relatively large space density of faint active nuclei at z>4. We have carried out an exploratory spectroscopic program to measure the HI ionizing emission of 16 faint AGNs spanning a broad U-I color interval, with I~21-23 and 3.6~4. The LyC escape fraction has been detected with S/N ratio of ~10-120 and is between 44 and 100% for all the observed faint AGNs, with a mean value of 74% at 3.6
description: Accepted for publication on A&A, 16 pages, 22 figures
A Precise Measurement of the Weak Mixing Angle in Neutrino-Nucleon Scattering
Creators: name: Arroyo, C. G.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We report a precise measurement of the weak mixing angle from the ratio of neutral current to charged current inclusive cross-sections in deep-inelastic neutrino-nucleon scattering. The data were gathered at the CCFR neutrino detector in the Fermilab quadrupole-triplet neutrino beam, with neutrino energies up to 600 GeV. Using the on-shell definition, ${\rm sin ^2θ_W} \equiv 1 - \frac{{\rm M_W} ^2}{{\rm M_Z} ^2}$, we obtain ${\rm sin ^2θ_W} = 0.2218 \pm 0.0025 ({\rm stat.}) \pm 0.0036 ({\rm exp.\: syst.}) \pm 0.0040 ({\rm model})$.
description: 10 pages, Nevis Preprint #1498 (Submitted to Phys. Rev. Lett.)
The Quantum Gravity Dynamics of Near Extremal Black Holes
Creators: name: Yang, Zhenbin
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study the quantum effects of Near-Extremal black holes near their horizons. The gravitational dynamics in such backgrounds are closely connected to a particle in $AdS_2$ with constant electric field. We use this picture to solve the theory exactly. We will give a formula to calculate all correlation functions with quantum gravity backreactions as well as the exact Wheeler-DeWitt wavefunction. Using the WdW wavefunction, we investigate the complexity growth in quantum gravity.
description: 38 pages, 10 figures/ v2: published version in JHEP
Förderung des Wortschatzes im Sprachheilkindergarten. Ein Stationenbetrieb mithilfe Unterstützter Kommunikation
Creators: name: Redding, Samantha
Publisher: name: Interkantonale Hochschule für Heilpädagogik
Year: 2024
Subjects: Sonderpädagogik
Masterarbeit
Förderung
Wortschatz
Sprachheilkindergarten
Stationenbetrieb
Unterstützte Kommunikation
Sprachentwicklungsstörung

description: Diese Arbeit untersucht, wie die individuelle Arbeitszeit im Kindergarten an einer Sprachheilschule für Kinder mit Sprachentwicklungsstörungen gestaltet werden kann, um sprachhandelndes und interaktives Lernen zu fördern. Mit einem qualitativen Ansatz wurde der Einfluss didaktischer Konzepte sowie der Einsatz von unterstützter Kommunikation auf die Wortschatzentwicklung der Kinder analysiert. Besonders die Förderung des Kern- und Randvokabulars stand im Fokus.Die Ergebnisse zeigen, dass eine gezielte, interaktive Gestaltung der Lernzeit zu einer Verbesserung des Wortschatzes führt. Die Arbeit hebt hervor, dass Kinder durch das Lernen am gemeinsamen Gegenstand (Stationenbetrieb) besonders profitieren.
Cancer spinifer Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer spinifer

description: Cancer spinifer [spec. nov.]
C. brachyurus, thorace postice uni-aculeato, inaequali, pedibus secundi paris longissimis.
Rumph. mus. t. 8. f. 3?
Habitat in Asia.
* e * Brachyuri thorace inaequali.
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 pages 629-630, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Particle acceleration and relativistic shocks
Creators: name: Kirk, J. G.
name: Duffy, P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Observations of both gamma-ray burst sources and certain classes of active galaxy indicate the presence of relativistic shock waves and require the production of high energy particles to explain their emission. In this paper we review the basic theory of shock waves in relativistic hydrodynamics and magneto-hydrodynamics, emphasising the astrophysically interesting cases. This is followed by an overview of the theory of particle acceleration at such shocks. We summarise the applications to the astrophysics of relativistic jets and fireball models of gamma-ray-bursts.
description: 43 pages, 5 figures, accepted for publication in Journal of Physics G: Nuclear and Particle Physics as a topical review
The determined property of Baire in reverse math
Creators: name: Astor, Eric P.
name: Dzhafarov, Damir
name: Montalbán, Antonio
name: Solomon, Reed
name: Westrick, Linda Brown
Publisher: name: arXiv
Year: 2018
Subjects: subject: Logic (math.LO)
subject: FOS: Mathematics
subject: 03B30

description: We define the notion of a determined Borel code in reverse math, and consider the principle $DPB$, which states that every determined Borel set has the property of Baire. We show that this principle is strictly weaker than $ATR$. Any $ω$-model of $DPB$ must be closed under hyperarithmetic reduction, but $DPB$ is not a theory of hyperarithmetic analysis. We show that whenever $M\subseteq 2^ω$ is the second-order part of an $ω$-model of $DPB$, then for every $Z \in M$, there is a $G \in M$ such that $G$ is $Δ^1_1$-generic relative to $Z$.
description: Greatly expanded introduction as requested by referee
Additional file 6: of Comparison of logistic regression with machine learning methods for the prediction of fetal growth abnormalities: a retrospective cohort study
Creators: name: Kuhle, Stefan
name: Maguire, Bryan
name: Hongqun Zhang
name: Hamilton, David
name: Allen, Alexander
name: K. Joseph
name: Allen, Victoria
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology

description: Figure S3. Receiver operating characteristic curves for the prediction of SGA among multiparous women (pre-pregnancy) using elastic net, classification trees, random forest, gradient boosting, and neural networks. (PDF 188 kb)
Additional file 3 of Sarcopenia predicts adverse outcomes in an elderly population with coronary artery disease: a systematic review and meta-analysis
Creators: name: Xue, Qiqi
name: Wu, Jie
name: Ren, Yan
name: Hu, Jiaan
name: Yang, Ke
name: Cao, Jiumei
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Additional file 3: Supplementary Appendix S3. NOS criteria for quality of cohort studies.
title: ADCO, Grènetier de Cîteaux : comptes (1499-1503) (11 H 1173), f. 00129
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: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: comptes
subject: Corpus Burgundiae Medii Aevi

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. 00129, 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
Characterization of self-injected electron beams from LWFA experiments at SPARC_LAB
Creators: name: Costa, G.
name: Anania, M. P.
name: Bisesto, F.
name: Chiadroni, E.
name: Cianchi, A.
name: Curcio, A.
name: Ferrario, M.
name: Filippi, F.
name: Marocchino, A.
name: Mira, F.
name: Pompili, R.
name: Zigler, A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The plasma-based acceleration is an encouraging technique to overcome the limits of the accelerating gradient in the conventional RF acceleration. A plasma accelerator is able to provide accelerating fields up to hundreds of $GeV/m$, paving the way to accelerate particles to several MeV over a short distance (below the millimetre range). Here the characteristics of preliminary electron beams obtained with the self-injection mechanism produced with the FLAME high-power laser at the SPARC_LAB test facility are shown. In detail, with an energy laser on focus of $1.5\ J$ and a pulse temporal length (FWHM) of $40\ fs$, we obtained an electron plasma density due to laser ionization of about $6 \times 10^{18}\ cm^{-3}$, electron energy up to $350\ MeV$ and beam charge in the range $(50 - 100)\ pC$.
description: 6 pages, 11 figures, conference EAAC2017
The Dyadosphere of Black Holes and Gamma-Ray Bursts
Creators: name: Ruffini, Remo
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent works on the Dyadosphere are reviewed.
description: A&A macros, 4 pages and 3 figures. To appear in the proceedings of 19th Texas Symposium, Dec. 1998
Descent Theory and Mapping Spaces
Creators: name: Meadows, Nicholas
Publisher: name: arXiv
Year: 2018
Subjects: subject: Algebraic Geometry (math.AG)
subject: Algebraic Topology (math.AT)
subject: FOS: Mathematics
subject: 14A20 (Primary), 14F05, 55P42, 18F20

description: The purpose of this paper is to develop a theory of $(\infty, 1)$-stacks, in the sense of Hirschowitz-Simpson's `Descent Pour Les n-Champs', using the language of quasi-category theory and the author's local Joyal model structure. The main result is a characterization of $(\infty, 1)$-stacks in terms of mapping space presheaves. An important special case of this theorem gives a sufficient condition for the presheaf of quasi-categories associated to a presheaf of model categories to be a higher stack. In the final section, we apply this result to construct the higher stack of unbounded complexes associated to a ringed site.
description: This is a pre copy-edited, post accceptance. Jour. Homotopy Rel. Struct (2020)
Cancer cruentatus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer cruentatus

description: Cancer cruentatus [spec. nov.]
C. brachyurus, thorace tuberculoso sanguineo, rostro lineari truncato.
Habitat in M. Mediterraneo. E. Brander.
Testa statura & magnitudine C. Aranei, supra admodum nodosa tuberibus inaequalibus: apice maculis albis. Rostrum lineare, truncatum, cum dente utrinque ad ejus basin. Chelae lineares ad carpos utrinque dente retrospectante obtuso. Pedes acuti.
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 630, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Supernova Remnants in the Magellanic Clouds III: An X-ray Atlas of LMC Supernova Remnants
Creators: name: Williams, Rosa Murphy
name: Chu, You-Hua
name: Dickel, John R.
name: Petre, Robert
name: Smith, R. Chris
name: Tavarez, Maritza
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have used archival ROSAT data to present X-ray images of thirty-one supernova remnants (SNRs) in the Large Magellanic Cloud (LMC). We have classified these remnants according to their X-ray morphologies, into the categories of Shell-Type, Diffuse Face, Centrally Brightened, Point-Source Dominated, and Irregular. We suggest possible causes of the X-ray emission for each category, and for individual features of some of the SNRs.
description: 27 pages, 6 figures (9 figure files). To appear in the Supplement Series of the Astrophysical Journal, August 1999 Vol. 123 #2
Additional file 5: of Comparison of logistic regression with machine learning methods for the prediction of fetal growth abnormalities: a retrospective cohort study
Creators: name: Kuhle, Stefan
name: Maguire, Bryan
name: Hongqun Zhang
name: Hamilton, David
name: Allen, Alexander
name: K. Joseph
name: Allen, Victoria
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology

description: Figure S2. Receiver operating characteristic curves for the prediction of SGA among primiparous women (26Â weeks) using elastic net, classification trees, random forest, gradient boosting, and neural networks. (PDF 186 kb)
Supersymmetry at the DiTevatron
Creators: name: Kamon, T.
name: Lopez, J.
name: McIntyre, P.
name: White, J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We study the signals for supersymmetry at the Tevatron and DiTevatron ($\sqrt{s}=4\TeV$) in various well-motivated supersymmetric models. We consider the trilepton signature in the decay of pair-produced charginos and neutralinos, the missing energy signature in gluino and squark production, and the $b\bar b$ signal in the decay of the lightest supersymmetric Higgs boson produced in association with a $W$ or $Z$ boson. In each case we perform signal and background studies, using Monte Carlo and/or real data to estimate the sensitivity to these signals at the Tevatron and DiTevatron with the Main Injector, for short- and long-term integrated luminosities of ${\cal L}=10$ and $25\ifb$, and $5σ$ statistical significance. We conclude that one could probe chargino masses as high as $m_{χ^\pm_1}\sim180\,(200)\GeV$, gluino masses as high as $m_{\tilde g}\sim450\,(750)\GeV$, and lightest Higgs boson masses as high as $m_h\sim110\,(120)\GeV$ at the Tevatron (DiTevatron). A high-luminosity option at the Tevatron ($10^{33}\cm^{-2}\s^{-1}$) may compensate somewhat for the higher reach of the DiTevatron, but only in the trilepton and Higgs signals. However, these gains may be severely compromised once the multiple-interaction environment of the high-luminosity Tevatron is accounted for.
description: 38 pages, Latex, 12 figures (not included). Figures are available via anonymous ftp from hplaa02.cern.ch (/pub/lopez) as one uuencoded file (DiTevFigs.uu, 0.731MB). CTP-TAMU-19/94
The Proper Motion of SgrA*: I. First VLBA Results
Creators: name: Reid, M. J.
name: Readhead, A. C. S.
name: Vermeulen, R. C.
name: Treuhaft, R. N.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We observed Sgr A* and two extragalactic radio sources nearby in angle with the VLBA over a period of two years and measured relative positions with an accuracy approaching 0.1 mas. The apparent proper motion of Sgr A* relative to J1745-283 is 5.90 +/- 0.4 mas/yr, almost entirely in the plane of the Galaxy. The effects of the orbit of the Sun around the Galactic Center can account for this motion, and any residual proper motion of Sgr A*, with respect to extragalactic sources, is less than about 20 km/s. Assuming that Sgr A* is at rest at the center of the Galaxy, we estimate that the circular rotation speed in the Galaxy at the position of the Sun is 219 +/- 20 km/s, scaled by Ro/8.0 kpc. Current observations are consistent with Sgr A* containing all of the nearly 2.6 x 10^6 solar masses, deduced from stellar proper motions, in the form of a massive black hole. While the low luminosity of Sgr A*, for example, might possibly have come from a contact binary containing of order 10 solar masses, the lack of substantial motion rules out a "stellar" origin for Sgr A*. The very slow speed of Sgr A* yields a lower limit to the mass of Sgr A* of about 1,000 solar masses. Even for this mass, Sgr A* appears to be radiating at less than 0.1 percent of its Eddington limit.
Cancer hepaticus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Cancridae
Cancer
Cancer hepaticus

description: Cancer hepaticus [spec. nov.]
C. brachyurus, thorace verrucoso gibbo semiorbiculato: margine serrato.
Habitat in Indiis.
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 630, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Optimal Control of Networks in the presence of Attackers and Defenders
Creators: name: Kafle, Ishan
name: Bartaula, Sudarshan
name: Shirin, Afroza
name: Klickstein, Isaac
name: Das, Pankaz
name: Sorrentino, Francesco
Publisher: name: arXiv
Year: 2018
Subjects: subject: Systems and Control (eess.SY)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: We consider the problem of a dynamical network whose dynamics is subject to external perturbations (`attacks') locally applied at a subset of the network nodes. We assume that the network has an ability to defend itself against attacks with appropriate countermeasures, which we model as actuators located at (another) subset of the network nodes. We derive the optimal defense strategy as an optimal control problem. We see that the network topology, as well as the distribution of attackers and defenders over the network affect the optimal control solution and the minimum control energy. We study the optimal control defense strategy for several network topologies, including chain networks, star networks, ring networks, and scale free networks.
Physiological assessment of water deficit in soybean using midday leaf water potential and spectral features
Creators: name: Wijewardana, Chathurika
name: Alsajri, Firas A.
name: Irby, J. Trenton
name: Krutz, L. Jason
name: Golden, Bobby
name: Henry, W. Brien
name: Gao, Wei
name: Reddy, K. Raja
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Plant Biology

description: Drought is one of the major abiotic stresses that limit soybean production worldwide. This study was conducted to determine whether soybean cultivars with divergent growth habits respond differently to drought stress at the vegetative growth stage regarding canopy reflectance, physiological, and gas exchange traits under controlled conditions. Soil moisture content was positively correlated with mid-day leaf water potential. Pooled over cultivar, photosynthesis and stomatal conductance were highly correlated with mid-day leaf water potential, while Ci/Ca exhibited a weak positive correlation. These data indicate that, regardless of cultivar, the decrease in net photosynthesis is mainly due to stomatal closure. For both cultivars, drought stress increased soybean canopy reflectance in the visible range of the spectrum but decreased reflectance in the near-infrared region. The quantified physiological traits would be useful to understand plant water relations and canopy structure to help soybean growers to make field management decisions during the growing season.
A subarcsecond resolution near-infrared study of Seyfert and `normal' galaxies: I. Imaging data
Creators: name: Peletier, R. F.
name: Knapen, J. H.
name: Shlosman, I.
name: Perez-Ramirez, D.
name: Nadeau, D.
name: Doyon, R.
name: Rodriguez-Espinosa, J. M.
name: Garcia, A. M. Perez -
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present new high-resolution near-infrared observations in the J,H and K bands, obtained to study the properties of Seyfert host galaxies. The dataset consists of images in the three bands of practically the entire CfA sample of Seyfert galaxies, and K-band images of a control sample of non-active, `normal', galaxies, matched to the Seyfert sample in the distribution of type and inclination. The spatial resolution and sampling of the new images is a factor 2 better than previously published K-band data. In this paper, we present the data in the form of profiles of surface brightness and color, ellipticity and major axis position angle, as well as greyscale maps of surface brightness in H or K and both J-H and H-K colors. We compare our surface brightness and color profiles with the literature, and find good agreement. Our data are discussed in detail in three subsequent publications, where we analyze the morphologies of Seyfert and normal hosts, quantify the strength of nonaxisymmetric features in disks and their relationship to nuclear activity, address the question of bar fraction in Seyferts and normal galaxies, and analyze the color information in the framework of emission mechanisms in Seyfert 1s and 2s, and in non-active galaxies.
description: 17 pages + 2 figures + data tables. Accepted for publication in the Astrophysical Journal Supplement. Figure 1, together with much more information about the Cfa sample of Seyfert galaxies, can be found at http://star-www.dur.ac.uk/~peletier/SEYFERT and http://www.pa.uky.edu/~shlosman/gals/SEYFERT
title: ADCO, Ordre cistercien : comptes (1403-1423) (11 H 1161), f. 00072
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
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes
subject: LaMOP

description: Ordre cistercien : comptes (1403-1423), Archives départementales de la Côte-d'Or, (11 H 1161). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien : comptes (1403-1423), Archives départementales de la Côte-d'Or, (11 H 1161), f. 00072, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
The performances of R GPU implementations of the GMRES method
Creators: name: Oancea, Bogdan
name: Pospisil, Richard
Publisher: name: arXiv
Year: 2018
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: FOS: Computer and information sciences

description: Although the performance of commodity computers has improved drastically with the introduction of multicore processors and GPU computing, the standard R distribution is still based on single-threaded model of computation, using only a small fraction of the computational power available now for most desktops and laptops. Modern statistical software packages rely on high performance implementations of the linear algebra routines there are at the core of several important leading edge statistical methods. In this paper we present a GPU implementation of the GMRES iterative method for solving linear systems. We compare the performance of this implementation with a pure single threaded version of the CPU. We also investigate the performance of our implementation using different GPU packages available now for R such as gmatrix, gputools or gpuR which are based on CUDA or OpenCL frameworks.
Bronze Age and Early Saxon Activity at Dagenham Heathway, London Borough of Barking and Dagenham
Creators: name: P Boyer, Peter
name: F Keith-Lucas, Fiona
name: J Bishop, Barry
name: C Jarrett, Chris
name: L Rayner, Louise
Publisher: name: Archaeology Data Service
Year: 2021

description: Transactions of the London and Middlesex Archaeological Society, 2.65, 103-148
Microwave spectrum of the complex of 3,3,3-trifluoro-2-(trifluoromethyl)propanoic acid and formic acid
Creators: name: Thomas, Javix
name: Carrillo, Michael J.
name: Serrato, Agapito
name: Xie, Fan
name: Jäger, Wolfgang
name: Xu, Yunjie
name: Lin, Wei
Publisher: name: Taylor & Francis
Year: 2018
Subjects: Biophysics
Biochemistry
Pharmacology
Biotechnology
Chemical Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Cancer

description: We report the first high resolution spectroscopic observation of the complex of 3,3,3-trifluoro-2-(trifluoromethyl)propanoic acid (TTPA) and formic acid. The rotational spectra were measured using a broadband chirped pulse and a narrow band cavity-based Fourier transform microwave spectrometer in the 8–10 GHz range. The conformational landscape of the TTPA-formic acid complex was explored at several levels of theory. The two most stable TTPA-formic acid conformers are of similar stability and feature the usual cyclic carboxylic double hydrogen bonded ring. Based on the broadband spectra obtained, only one stable heterodimer conformer was observed. We explain the absence of the second conformer to be a result of a double hydrogen tunnelling motion which converts the less stable heterodimer to the one observed in the jet expansion. Further CCSD(T) relative energy calculations confirm that the heterodimer conformer detected contains the most stable TTPA monomeric subunit. It is interesting to note that hydrogen bonding with formic acid offers a new path to effectively convert the less stable TTPA subunit to the most stable one in the jet expansion, while both TTPA monomeric conformers were detected in the same experiment.
German Morphological Fluency Task
Creators: name: Haase, Astrid
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Education
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology
subject: German Morphological Fluency Task

description: This task measures the ability to produce morphologically complex words based on one’s knowledge on word families.

Implementation: Participants are asked name for every target word within 30s as many words as they can find belonging to the same word family as the target word. Target words are presented both auditorily and in writing. The task consists of eight test target words and one practice item.

Example: For the target word “Tisch” (table), participants could produce “Tischtennis” (table tennis), “Holztisch” (wooden table), or “auftischen” (serve) etc..

Items: Four verb target words from Haase and Steinbrink (2022) were taken and complemented with four nouns to account for the fact that nouns form 50-60% of German vocabulary (cf. Fleischer & Barz, 2012). We matched the nouns as closely as possible to the four verbs regarding word frequency and morphological family size (in how many different words the stem appeared in a lexical database of German read by children “childLex”; Schroeder et al., 2015).

References
Casalis, S., Colé, P., & Sopo, D. (2004). Morphological Awareness in Developmental Dyslex-ia. Annals of Dyslexia, 54(1), 114–138. https://doi.org/10.1007/s11881-004-0006-z

Fleischer, W., & Barz, I. (2012). Wortbildung der deutschen Gegenwartssprache (4th ed.). Studienbuch. De Gruyter.

Haase, A., & Steinbrink, C. (2022). Associations between morphological awareness and litera-cy skills in German primary school children: the roles of grade level, phonological pro-cessing and vocabulary. Reading and Writing, 35(7), 1675–1709. https://doi.org/10.1007/s11145-021-10247-1

Schroeder, S., Würzner, K. M., Heister, J., Geyken, A., & Kliegl, R. (2015). Childlex: A lexi-cal database of German read by children. Behavior Research Methods, 47(4), 1085–1094. https://doi.org/10.3758/s13428-014-0528-1
A light stop and its consequences at the Tevatron and LEPII
Creators: name: Lopez, J.
name: Nanopoulos, D.
name: Zichichi, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: An interesting prediction of a string-inspired {\em one-parameter} $SU(5)\times U(1)$ supergravity model, is the fact that the lightest member ($\tilde t_1$) of the top-squark doublet $(\tilde t_1,\tilde t_2)$, may be substantially lighter than the top quark. This sparticle ($\tilde t_1$) may be readily pair-produced at the Tevatron and, if $m_{\tilde t_1}\lsim130\GeV$, even be observed at the end of Run IB. Top-squark production may also be an important source of sought-for top-quark signatures in the dilepton and $\ell$+jets channels. Therefore, a re-analysis of the top data sample in the presence of a possibly light top-squark appears necessary before definitive statements concerning the discovery of the top quark can be made. Such a light top-squark is linked with a light supersymmetric spectrum, which can certainly be searched for at the Tevatron through trilepton and squark-gluino searches, and at LEPII through direct $\tilde t_1$ pair-production (for $m_{\tilde t_1}\lsim100\GeV$) and via chargino and Higgs-boson searches.
description: CERN-TH.7296/94, 9 pages, LaTeX, 3 figures (included as uuencoded file)
On the extensions of the De Giorgi approach to nonlinear hyperbolic equations
Creators: name: Tentarelli, Lorenzo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35L70, 35L71, 35L75, 35L76, 35L90, 35L15, 49J45

description: In this talk we present an overview on the extensions of the De Giorgi approach to general second order nonlinear hyperbolic equations. We start with an introduction to the original conjecture by E. De Giorgi (De Giorgi '96) and to its solution by E. Serra and P. Tilli (Serra&Tilli '12). Then, we discuss a first extension of this idea (Serra&Tilli '16) aimed at investigating a wide class of homogeneous equations. Finally, we announce a further extension to nonhomogeneous equations, obtained by the author in collaboration with P. Tilli (Tentarelli&Tilli '17).
description: 9 pages, proceeding of conference Bruxelles-Torino Talks in PDEs, Turin, May 2-5, 2016
Additional file 4: of Comparison of logistic regression with machine learning methods for the prediction of fetal growth abnormalities: a retrospective cohort study
Creators: name: Kuhle, Stefan
name: Maguire, Bryan
name: Hongqun Zhang
name: Hamilton, David
name: Allen, Alexander
name: K. Joseph
name: Allen, Victoria
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology

description: Figure S1. Receiver operating characteristic curves for the prediction of SGA among primiparous women (pre-pregnancy) using elastic net, classification trees, random forest, gradient boosting, and neural networks. (PDF 176 kb)
Discovery of Radio Outbursts in the Active Nucleus of M81
Creators: name: Ho, Luis C.
name: Van Dyk, Schuyler D.
name: Pooley, Guy G.
name: Sramek, Richard A.
name: Weiler, Kurt W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The low-luminosity active galactic nucleus of M81 has been monitored at centimeter wavelengths since early 1993 as a by-product of radio programs to study the radio emission from Supernova 1993J. The extensive data sets reveal that the nucleus experienced several radio outbursts during the monitoring period. At 2 and 3.6 cm, the main outburst occurred roughly in the beginning of 1993 September and lasted for approximately three months; at longer wavelengths, the maximum flux density decreases, and the onset of the burst is delayed. These characteristics qualitatively resemble the standard model for adiabatically expanding radio sources, although certain discrepancies between the observations and the theoretical predictions suggest that the model is too simplistic. In addition to the large-amplitude, prolonged variations, we also detected milder changes in the flux density at 3.6 cm and possibly at 6 cm on short (less than 1 day) timescales. We discuss a possible association between the radio activity and an optical flare observed during the period that the nucleus was monitored at radio wavelengths.
description: To appear in The Astronomical Journal. Latex, 18 pages including embedded figures and tables
Renormalization Group Effects in Dark Matter Interactions
Creators: name: Bishara, Fady
name: Brod, Joachim
name: Grinstein, Benjamin
name: Zupan, Jure
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present a renormalization-group (RG) analysis of dark matter interactions with the standard model, where dark matter is allowed to be a component of an electroweak multiplet, and has a mass at or below the electroweak scale. We consider, in addition to the gauge interactions, the complete set of effective operators for dark matter interactions with the standard model above the weak scale, up to and including mass dimension six. We calculate the RG evolution of these operators from the high scale Lambda down to the weak scale, and perform the matching to the tower of effective theories below the weak scale. We also summarize the RG evolution below the weak scale and the matching to the nonrelativistic nuclear interactions. We present several numerical examples and show that in certain cases the dark matter - nucleus scattering rate can change by orders of magnitude when the electroweak running is included.
description: 62 pages, 16 figures. Updated references; version published in JHEP