cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Variable Very High Energy Gamma-ray Emission from the Microquasar LS I +61 303
Creators: name: MAGIC Collaboration
name: Albert, J.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Microquasars are binary star systems with relativistic radio-emitting jets. They are potential sources of cosmic rays and laboratories for elucidating the physics of relativistic jets. Here we report the detection of variable gamma-ray emission above 100 gigaelectron volts from the microquasar LS I +61 303. Six orbital cycles were recorded. Several detections occur at a similar orbital phase, suggesting the emission is periodic. The strongest gamma-ray emission is not observed when the two stars are closest to one another, implying a strong orbital modulation of the emission or the absorption processes.
description: 11 pages with 4 figures
Analysis of Dark Matter Axion Clumps with Spherical Symmetry
Creators: name: Schiappacasse, Enrico D.
name: Hertzberg, Mark P.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Recently there has been much interest in the spatial distribution of light scalar dark matter, especially axions, throughout the universe. When the local gravitational interactions between the scalar modes are sufficiently rapid, it can cause the field to re-organize into a BEC of gravitationally bound clumps. While these clumps are stable when only gravitation is included, the picture is complicated by the presence of the axion's attractive self-interactions, which can potentially cause the clumps to collapse. Here we perform a detailed stability analysis to determine under what conditions the clumps are stable. In this paper we focus on spherical configurations, leaving aspherical configurations for future work. We identify branches of clump solutions of the axion-gravity-self-interacting system and study their stability properties. We find that clumps that are (spatially) large are stable, while clumps that are (spatially) small are unstable and may collapse. Furthermore, there is a maximum number of particles that can be in a clump. We map out the full space of solutions, which includes quasi-stable axitons, and clarify how a recent claim in the literature of a new ultra-dense branch of stable solutions rests on an invalid use of the non-relativistic approximation. We also consider repulsive self-interactions that may arise from a generic scalar dark matter candidate, finding a single stable branch that extends to arbitrary particle number.
description: 32 pages, 8 figures. V2: Fixed figure 8 and equation 71. Added clarifications regarding spherical symmetry. Added references
A palynological zonation for the Neogene of the Solimões/Amazon Basin, northwestern Amazonia
Creators: name: Jaramillo, Carlos A.
name: D'Apolito, Carlos
name: da Silva-Caminha, Silane A. F.
name: Caballero-Rodríguez, Dayenari
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Biochemistry
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: The tropical rainforests of northwestern Amazonia possess the highest plant diversity of any biome in the world. Understanding their origin, development, maintenance, and future in the face of ongoing global warming requires study of the plant fossil record and a predictive time framework. In this region, palynology is the best biostratigraphic tool because palynomorphs are the most abundant fossils. To construct a biostratigraphic zonation for the Neogene of the Solimões/Amazon basin in northwestern Amazonia, we analyzed palynological information from 25 sections, a total of 143,411 palynomorph grains from 622 samples. Using graphic correlation, we propose seven palynological zones that comprise the Miocene and a portion of the Pleistocene—the Pliocene is absent in the region. We then calibrated these zones against the geological timescale through correlation with a previously calibrated zonation and U/Pb geochronology.
Additional file 3 of Identification and functional characterisation of a locus for target site integration in Fusarium graminearum
Creators: name: Darino, Martin
name: Urban, Martin
name: Kaur, Navneet
name: Machado Wood, Ana
name: Grimwade-Mann, Mike
name: Smith, Dan
name: Beacham, Andrew
name: Hammond-Kosack, Kim
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology
subject: Computational Biology

description: Additional file 3: Genomic sequence analysis of the mCherry expressing strains and PCR amplification of the insertion. A) IGV screenshots displaying genomic regions with low read depth coverage. Regions with low read depth were identified not only in the transformant strains but also in PH-1. Low coverage regions were usually identified at the telomeres (Chr1I, Chr1IV, Chr2, Chr3I, Chr3II and Chr4IV), in the 5’UTRs (Chr1II, Chr1III and Chr4I) or 3’UTRs (Chr4II and Chr4III) of different genes. The red bar above the figure indicates the chromosomic region with read depth values ≤ 1. B) Contigs with evidence of cassette truncations and/or tandem insertions for the mCherry and SP-mCherry strains. Graphs above the contigs represent the read depth for each base of the contig. C) PCR amplification of the insertion at the TSI locus 1 in the mCherry strain. Graph represents the predicted tandem insertion for the mCherry line.
Peering beyond the horizon with standard sirens and redshift drift
Creators: name: Jimenez, Raul
name: Raccanelli, Alvise
name: Verde, Licia
name: Matarrese, Sabino
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: An interesting test on the nature of the Universe is to measure the global spatial curvature of the metric in a model independent way, at a level of $|Ω_k|<10^{-4}$, or, if possible, at the cosmic variance level of the amplitude of the CMB fluctuations $|Ω_k|\approx10^{-5}$. A limit of $|Ω_k|<10^{-4}$ would yield stringent tests on several models of inflation. Further, improving the constraint by an order of magnitude would help in reducing "model confusion" in standard parameter estimation. Moreover, if the curvature is measured to be at the value of the amplitude of the CMB fluctuations, it would offer a powerful test on the inflationary paradigm and would indicate that our Universe must be significantly larger than the current horizon. On the contrary, in the context of standard inflation, measuring a value above CMB fluctuations will lead us to conclude that the Universe is not much larger than the current observed horizon, this can also be interpreted as the presence of large fluctuations outside the horizon. However, it has proven difficult, so far, to find observables that can achieve such level of accuracy, and, most of all, be model-independent. Here we propose a method that can in principle achieve that, this is done by making minimal assumptions and using distance probes that are cosmology-independent: gravitational waves, redshift drift and cosmic chronometers. We discuss what kind of observations are needed in principle to achieve the desired accuracy.
description: Matches version published in JCAP, minor changes, conclusions unchanged
Verification of operational solar flare forecast: Case of Regional Warning Center Japan
Creators: name: Kubo, Yûki
name: Den, Mitsue
name: Ishii, Mamoru
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: Space Physics (physics.space-ph)
subject: Applications (stat.AP)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: In this article, we discuss a verification study of an operational solar flare forecast in the Regional Warning Center (RWC) Japan. The RWC Japan has been issuing four-categorical deterministic solar flare forecasts for a long time. In this forecast verification study, we used solar flare forecast data accumulated over 16 years (from 2000 to 2015). We compiled the forecast data together with solar flare data obtained with the Geostationary Operational Environmental Satellites (GOES). Using the compiled data sets, we estimated some conventional scalar verification measures with 95% confidence intervals. We also estimated a multi-categorical scalar verification measure. These scalar verification measures were compared with those obtained by the persistence method and recurrence method. As solar activity varied during the 16 years, we also applied verification analyses to four subsets of forecast-observation pair data with different solar activity levels. We cannot conclude definitely that there are significant performance difference between the forecasts of RWC Japan and the persistence method, although a slightly significant difference is found for some event definitions. We propose to use a scalar verification measure to assess the judgment skill of the operational solar flare forecast. Finally, we propose a verification strategy for deterministic operational solar flare forecasting.
description: 29 pages, 7 figures and 6 tables. Accepted for publication in Journal of Space Weather and Space Climate (SWSC)
Bocconia frutescens Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Papaveraceae
Bocconia
Bocconia frutescens

description: Bocconia frutescens, spec. nov.
1. Bocconia.
 Bocconia ramosa, sphondylii folio tomentoso. Plum. gen. 55.
 Chelidonium majus arboreum, foliis quercinis. Sloan. jam. 82. hist. 1. p.195. t.125.
 Habitat in Jamaica , Mexico . ♄
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 505, DOI: 10.5281/zenodo.3931989
Sanguinaria canadensis Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Papaveraceae
Sanguinaria
Sanguinaria canadensis

description: Sanguinaria canadensis, spec. nov.
 1. Sanguinaria. Hort. cliff. 202. Gron. virg. 57.
 Sanguinaria minor, flore simplici. Dill. elth. 335. t. 252. f.326.
 Chelidonium majus canadense acaulon. Corn. canad. 212. Moris. hist. 2. p. 257. s.3. t.11. f.1. Raj. hist. 1887.
 β Sanguinaria major, flore simplici. Dill. elth. 335. t. 252. f.325.
 γ. Sanguinaria major, flore pleno. Dill. elth. 335. t. 252. f.326.
 Habitat in America septentrionali. ♃
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 505, DOI: 10.5281/zenodo.3931989
Knowledge Transfer for Out-of-Knowledge-Base Entities: A Graph Neural Network Approach
Creators: name: Hamaguchi, Takuo
name: Oiwa, Hidekazu
name: Shimbo, Masashi
name: Matsumoto, Yuji
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences

description: Knowledge base completion (KBC) aims to predict missing information in a knowledge base.In this paper, we address the out-of-knowledge-base (OOKB) entity problem in KBC:how to answer queries concerning test entities not observed at training time. Existing embedding-based KBC models assume that all test entities are available at training time, making it unclear how to obtain embeddings for new entities without costly retraining. To solve the OOKB entity problem without retraining, we use graph neural networks (Graph-NNs) to compute the embeddings of OOKB entities, exploiting the limited auxiliary knowledge provided at test time.The experimental results show the effectiveness of our proposed model in the OOKB setting.Additionally, in the standard KBC setting in which OOKB entities are not involved, our model achieves state-of-the-art performance on the WordNet dataset. The code and dataset are available at https://github.com/takuo-h/GNN-for-OOKB
description: This paper has been accepted by IJCAI17
Additional file 6: of Characterizing oral microbial communities across dentition states and colonization niches
Creators: name: Mason, Matthew
name: Chambers, Stephanie
name: Shareef Dabdoub
name: Sarat Thikkurissy
name: Purnima Kumar
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Physiology
subject: FOS: Biological sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Supplemental Figure S2: Functional shifts in the core supragingival microbiome during various dentition states. Figure 2a shows a Bland-Altman plot of changes in the relative abundances of core functional genes in the supragingival microbiome between the different dentitions. Each point is a functional gene. Points above and below the red median line represent genes demonstrating higher abundances in the specified dentition. Red points indicate genes with significantly different abundances (p < 0.05, FDR adjusted Wald test). Figure 2b shows the number of functional genes that were different between two subsequent dentitions. For example, the bar “Primary” represents genes that were different between predentate and primary dentitions, while “Mixed” represents number of genes differing between primary and mixed dentitions. Figures 2c and d represent the functions encoded by these genes in the primary and permanent dentitions respectively. (PDF 428 kb)
Monogenic Calculus as an Intertwining Operator
Creators: name: Kisil, Vladimir V.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Functional Analysis (math.FA)
subject: Complex Variables (math.CV)
subject: Spectral Theory (math.SP)
subject: FOS: Mathematics
subject: 47A60; 30G35, 46H30, 47A10, 47B15

description: We revise a monogenic calculus for several non-commuting operators, which is defined through group representations. Instead of an algebraic homomorphism we use group covariance. The related notion of joint spectrum and spectral mapping theorem are discussed. The construction is illustrated by a simple example of calculus and joint spectrum of two non-commuting selfadjoint (n\times n) matrices. Keywords: Functional calculus, spectrum, intertwining operator, spectral mapping theorem, jet spaces, monogenic function, Clifford algebra
description: 16 pages, 3 PS figures
Spin-density wave state in simple hexagonal graphite
Creators: name: Mosoyan, K. S.
name: Rozhkov, A. V.
name: Sboychakov, A. O.
name: Rakhmanov, A. L.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Simple hexagonal graphite, also known as AA graphite, is a metastable configuration of graphite. Using tight-binding approximation it is easy to demonstrate that AA graphite is a metal with well-defined Fermi surface. The Fermi surface consists of two sheets, each shaped like a rugby ball. One sheet corresponds to electron states, another corresponds to hole states. The Fermi surface demonstrates good nesting: a suitable translation in the reciprocal space superposes one sheet onto another. In the presence of the electron-electron repulsion a nested Fermi surface is unstable with respect to spin-density wave ordering. This instability is studied using the mean-field theory at zero temperature, and the spin-density wave order parameter is evaluated.
Equation of State in Numerical Relativistic Hydrodynamics
Creators: name: Ryu, Dongsu
name: Chattopadhyay, Indranil
name: Choi, Eunwoo
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Relativistic temperature of gas raises the issue of the equation of state (EoS) in relativistic hydrodynamics. We study the EoS for numerical relativistic hydrodynamics, and propose a new EoS that is simple and yet approximates very closely the EoS of the single-component perfect gas in relativistic regime. We also discuss the calculation of primitive variables from conservative ones for the EoS's considered in the paper, and present the eigenstructure of relativistic hydrodynamics for a general EoS, in a way that they can be used to build numerical codes. Tests with a code based on the Total Variation Diminishing (TVD) scheme are presented to highlight the differences induced by different EoS's.
description: To appear in the ApJS September 2006, v166n1 issue. Pdf with full resolution figures can be downloaded from http://canopus.cnu.ac.kr/ryu/ryuetal.pdf
Half-life Expectations for Neutrinoless Double Beta Decay in Standard and Non-Standard Scenarios
Creators: name: Ge, Shao-Feng
name: Rodejohann, Werner
name: Zuber, Kai
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We investigate the half-life expectations for neutrinoless double beta decay by applying statistical distributions of neutrino mixing observables, neutrino mass constraints from cosmology and nuclear matrix elements. The analysis is performed in the standard scenario of active Majorana neutrino exchange, when light sterile neutrinos are added, and within TeV-scale left-right symmetric frameworks. The latter two cases correspond to a modified phenomenology of double beta decay for a normal and inverted mass ordering, and thus different discovery potential for future experiments.
description: 18 pages, 10 figures, and 4 tables
Spectral analyses of eighteen hot H-deficient (pre-) white dwarfs from the Sloan Digital Sky Survey Data Release 4
Creators: name: Huegelmeyer, S. D.
name: Dreizler, S.
name: Homeier, D.
name: Krzesinski, J.
name: Werner, K.
name: Nitta, A.
name: Kleinman, S. J.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Context: The Sloan Digital Sky Survey Data Release 4 has provided spectra of several new PG 1159 stars and DO white dwarfs. This increase in known hot H-deficient compact objects significantly improves the statistics and helps to investigate late stages of stellar evolution. Aims: From the optical SDSS spectra, effective temperatures and surface gravities are derived in order to place the observed objects in an evolutionary context. Especially the connection between PG 1159 stars and DO white dwarfs shall be investigated. Method: Using our non-LTE model atmospheres and applying chi^2-fitting techniques, we determine stellar parameters and their errors. We derive total stellar masses for the DO white dwarfs using model evolutionary tracks. Results: We confirm three PG 1159 stars, with one showing ultra-high excitation ion features, and one sdO which we originally classified as a PG 1159 star. Additionally, we re-analysed the known PG 1159 star, PG 1424+535, with our new models. Furthermore, we present the first spectral analyses of thirteen DO white dwarfs, three of which show M-star features in their spectra, while two display ultra-high excitation ion features.
description: 9 pages, 6 figures, accepted for publication in A&A
Additional file 1: of Neural correlates of socio-emotional perception in 22q11.2 deletion syndrome
Creators: name: Dubourg, Lydia
name: Vrticka, Pascal
name: DebbanĂŠ, Martin
name: LĂŠa Chambaz
name: Eliez, Stephan
name: Schneider, Maude
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Table S1. Characteristic of the IAPS images selected. (DOCX 15Â kb)
Podophyllum peltatum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Berberidaceae
Podophyllum
Podophyllum peltatum

description: Podophyllum peltatum, spec. nov.
1. Podophyllum foliis peltatis lobatis.
 Podophyllum. Hort. cliff. 202. Hort. ups. 137. Gron. virg. 57. Roy. lugdb. 480.
 Anapodophyllum canadense. Catesb. car. 1. p. 24. t. 24.
 Aconitifolia humilis, flore albo unico campanulato, fructu cynosbati. Mentz. pug. t.11.
 Habitat in America septentrionali. ♃
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 505, DOI: 10.5281/zenodo.3931989
Podophyllum diphyllum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Berberidaceae
Podophyllum
Podophyllum diphyllum

description: Podophyllum diphyllum, spec. nov.
2. Podophyllum foliis binatis semicordatis.
 Habitat in Virginia . Collinson. ♃
 Folia radicalia, petiolata, binata ut in Hymenea, glabra, integerrima, semicordata, absque pedicellis. Scapus radicalis, uniflorus, fructu antecedentis. Flos mihi non visus.
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 505, DOI: 10.5281/zenodo.3931989
Additional file 5: of Comparative effectiveness of angiotensin-converting enzyme inhibitors and angiotensin II receptor blockers in chemoprevention of hepatocellular carcinoma: a nationwide high-risk cohort study
Creators: name: Cheng-Maw Ho
name: Chih-Hsin Lee
name: Ming-Chia Lee
name: Zhang, Jun-Fu
name: Jann-Yuan Wang
name: Rey-Heng Hu
name: Po-Huang Lee
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Table S3. Duration and amount of HBV medications and interferons in patients who received them in the study period, as grouped according to the use of ACEIs or ARBs within 6Â months after the index date. (DOCX 17Â kb)
Newton's method's basins of attraction revisited
Creators: name: Susanto, H.
name: Karjanto, N.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Numerical Analysis (math.NA)
subject: Complex Variables (math.CV)
subject: FOS: Mathematics
subject: 65B99, 28A10, 28A80, 30D05

description: In this paper, we revisit the chaotic number of iterations needed by Newton's method to converge to a root. Here, we consider a simple modified Newton method depending on a parameter. It is demonstrated using polynomiography that even in the simple algorithm the presence and the position of the convergent regions, i.e. regions where the method converges nicely to a root, can be complicatedly a function of the parameter.
description: 9 pages, 3 figures
Chelidonium majus Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Papaveraceae
Chelidonium
Chelidonium majus

description: Chelidonium majus, spec. nov.
1. Chelidonium pedunculis umbellatis.
 Chelidonium pedunculis multifloris umbellatis. Hort. cliff. 201. Fl. suec. 430. Hort. ups. 137. Mat. med. 252. Roy. lugdb. 478. Dalib. paris. 152.
 Chelidonium majus vulgare. Bauh. pin. 144.
 Chelidonium majus. Fuchs. hist. 865.
 β. Chelidonium majus, foliis quernis. Bauh. pin. 144.
 Chelidonium majus, folio laciniato. Clus. hist. 2. p. 203.
 Habitat in Europae ruderatis. ♃
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on pages 505-506, DOI: 10.5281/zenodo.3931989
title: Préface_L'art ogival en France et principalement en Champagne, suivi des comptes de la cathédrale de Troyes au XIIIe siècle et d'un voyage de saint Bernard en 1147
Creators: name: AmateurS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021

description: Préface
description: ID_PARA_01013
Better Actions
Creators: name: Cahill, Kevin
name: Herling, Gary
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We explain why compact U(1) confines and how to fix it. We show that plaquettes of negative trace carry most of the confinement signal in compact SU(2). We show how to perform noncompact gauge-invariant simulations without auxiliary fields. We suggest a way to simulate fermions without doublers.
description: Talk presented at LATTICE96(algorithms), 4 pages, Latex, espcrc2, pictex
Nectar sources of Asian honeybees (Apis cerana Fabricius) in West Bengal: determining by pollen analysis of honey and bee’s crop-nectar
Creators: name: Das, Nandita
name: Mondal, Rajib
name: Layek, Ujjwal
name: Karmakar, Prakash
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology

description: Understanding nectar sources is crucial for sustainable apiculture with Apis cerana, yet information on these sources remains limited. We conducted pollen analysis of honey and bees’ ingested nectar (mainly crop content) to determine the nectar sources of this honeybee species in West Bengal, India. Diverse pollen types were obtained from honey (33) and crop-nectar samples (47). A few pollen types came from non-nectariferous plants, and most came from actual nectariferous plants. Predominant pollen types in honey samples were Calendula officinalis, Eucalyptus tereticornis, and Peltophorum pterocarpum. The very frequent pollen types obtained from crop-nectar were Eucalyptus tereticornis, Peltophorum pterocarpum, and Tridax procumbens. In conclusion, versatile pollen types (that were obtained from honey and bee’s crop-nectar), indicating that the Asian honeybee (Apis cerana) is a generalist visitor, collect nectar from a large number of plant species. Our results also conclude that pollen analysis of bees’ crop-nectar can provide vital information about their nectar sources (excluding a few pollen types of non-nectariferous plants) in addition to the traditional honey analysis.
Additional file 2: of Transcriptomic analysis reveals vacuolar Na+ (K+)/H+ antiporter gene contributing to growth, development, and defense in switchgrass (Panicum virgatum L.)
Creators: name: Yanhua Huang
name: Cui, Xin
name: Huifang Cen
name: Kehua Wang
name: Yunwei Zhang
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: Figure S1. Total mapped and unmapped RNA-seq clean reads for transgenic lines and WT plants. (PDF 119Â kb)
Chelidonium glaucium Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Papaveraceae
Chelidonium
Chelidonium glaucium

description: Chelidonium glaucium, spec. nov.
2. Chelidonium pedunculis unifloris, foliis amplexicaulibus sinuatis, caule glabro.
 Chelidonium glabrum, pedunculis unifloris. Hort. ups. 137. Roy. lugdb. 478. Dalib. paris. 152.
 Chelidonium pedunculis unifloris. Hort. cliff. 201. Gron. virg.57.
 Papaver corniculatum luteum. Bauh. pin. 171.
 Papaver corniculatum, flavo flore. Clus. hist. 2. p. 91.
 Habitat in Angliae , Helvetiae , Galliae , Italiae , Virginiae arenosis. ☉
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 506, DOI: 10.5281/zenodo.3931989
The planets capture model of V838 Monocerotis: conclusions for the penetration depth of the planet/s
Creators: name: Retter, Alon
name: Zhang, Bing
name: Siess, Lionel
name: Levinson, Amir
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: V838 Mon is the prototype of a new class of objects. Understanding the nature of its multi-stage outburst and similar systems is challenging. So far, several scenarios have been invoked to explain this group of stars. In this work, the planets-swallowing model for V838 Mon is further investigated, taking into account the findings that the progenitor is most likely a massive B type star. We find that the super-Eddington luminosity during the eruption can explain the fast rising times of the three peaks in the optical light curve. We used two different methods to estimate the location where the planets were consumed. There is a nice agreement between the values obtained from the luminosities of the peaks and from their rising time scale. We estimate that the planets were stopped at a typical distance of one solar radius from the center of the host giant star. The planets-devouring model seems to give a satisfying explanation to the differences in the luminosities and rising times of the three peaks in the optical light curve of V838 Mon. The peaks may be explained by the consumption of three planets or alternatively by three steps in the terminal falling process of a single planet. We argue that only the binary merger and the planets-swallowing models are consistent with the observations of the new type of stars defined by V838 Mon.
description: 8 pages, 2 figures, MNRAS, accepted
Correlations in the three-dimensional Lyman-alpha forest contaminated by high column density absorbers
Creators: name: Rogers, Keir K.
name: Bird, Simeon
name: Peiris, Hiranya V.
name: Pontzen, Andrew
name: Font-Ribera, Andreu
name: Leistedt, Boris
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Correlations measured in three dimensions in the Lyman-alpha forest are contaminated by the presence of the damping wings of high column density (HCD) absorbing systems of neutral hydrogen (HI; having column densities $N(\mathrm{HI}) > 1.6\times10^{17}\,\mathrm{atoms}\,\mathrm{cm}^{-2}$), which extend significantly beyond the redshift-space location of the absorber. We measure this effect as a function of the column density of the HCD absorbers and redshift by measuring 3D flux power spectra in cosmological hydrodynamical simulations from the Illustris project. Survey pipelines exclude regions containing the largest damping wings. We find that, even after this procedure, there is a scale-dependent correction to the 3D Lyman-alpha forest flux power spectrum from residual contamination. We model this residual using a simple physical model of the HCD absorbers as linearly biased tracers of the matter density distribution, convolved with their Voigt profiles and integrated over the column density distribution function. We recommend the use of this model over existing models used in data analysis, which approximate the damping wings as top-hats and so miss shape information in the extended wings. The simple 'linear Voigt model' is statistically consistent with our simulation results for a mock residual contamination up to small scales ($|k| < 1\,h\,\mathrm{Mpc}^{-1}$). It does not account for the effect of the highest column density absorbers on the smallest scales (e.g., $|k| > 0.4\,h\,\mathrm{Mpc}^{-1}$ for small damped Lyman-alpha absorbers; HCD absorbers with $N(\mathrm{HI}) \sim 10^{21}\,\mathrm{atoms}\,\mathrm{cm}^{-2}$). However, these systems are in any case preferentially removed from survey data. Our model is appropriate for an accurate analysis of the baryon acoustic oscillations feature. It is additionally essential for reconstructing the full shape of the 3D flux power spectrum.
description: 13 pages, 11 figures. Minor changes to match version published in MNRAS
Complete Weight Enumerators of Generalized Doubly-Even Self-Dual Codes
Creators: name: Nebe, Gabriele
name: Quebbemann, H. -G.
name: Rains, E. M.
name: Sloane, N. J. A.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Number Theory (math.NT)
subject: Information Theory (cs.IT)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: 94B05, 13A50, 94B60

description: For any q which is a power of 2 we describe a finite subgroup of the group of invertible complex q by q matrices under which the complete weight enumerators of generalized doubly-even self-dual codes over the field with q elements are invariant. An explicit description of the invariant ring and some applications to extremality of such codes are obtained in the case q=4.
The structure of accretion flows in nova-like cataclysmic variables: RW Sextantis and 1RXS J064434.5+334451
Creators: name: Hernandez, M. S.
name: Zharikov, S.
name: Neustroev, V.
name: Tovmassian, G.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: New time-resolved optical spectroscopic echelle observations of the nova-like cataclysmic variable RW Sextantis were obtained, with the aim to study the properties of emission features in the system. The profile of the H_alpha emission line can be clearly divided into two (`narrow' and `wide') components. Similar emission profiles are observed in another nova-like system, 1RXS~J064434.5+33445, for which we also reanalysed the spectral data and redetermined the system parameters. The source of the `narrow', low-velocity component is the irradiated face of the secondary star. We disentangled and removed the `narrow' component from the H_alpha profile to study the origin and structure of the region emitting the wide component. We found that the `wide' component is not related to the white dwarf or the wind from the central part of the accretion disc, but is emanated from the outer side of the disc. Inspection of literature on similar systems indicates that this feature is common for some other long-period nova-like variables. We propose that the source of the `wide' component is an extended, low-velocity region in the outskirts of the opposite side of the accretion disc, with respect to the collision point of the accretion stream and the disc.
description: 11 pages, 7 figures, accepted for publication in MNRAS
Topology in 4D simplicial quantum gravity
Creators: name: Bilke, S.
name: Burda, Z.
name: Petersson, B.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We simulate 4d simplicial gravity for three topologis S4, S3xS1, (S1)^4 and show that the free energy for these three fixed topology ensembles is the same in the thermodynamic limit. We show, that the next-to-leading order corrections, at least away from the critical point, can be described by kinematic sources.
description: 12 pages, 5 figures
MOESM1 of KRDS: a web server for evaluating drug resistance mutations in kinases by molecular docking
Creators: name: Aeri Lee
name: Seungpyo Hong
name: Dongsup Kim
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Computational Biology

description: Additional file 1: Table S1. Re-docking of five ligands co-crystalized with CDK2 to the five RosettaBackrub generated CDK2 conformations. Table S2. RMSD values after re-docking of co-crystals into native structures. Table S3. The list of pdb ids of DFG-in and its corresponding DFG-out structures to perform docking in ABL1, BRAF, EGFR, FGFR4, and IGF1R. Table S4. The averaged docking values of DFG-in and its corresponding DFG-out structures. Table S5. The maximum docking values obtained among ensembles. Table S6. The docking results of ABL1 and EGFR using GOLD. Table S7. The docking results of ABL1 and EGFR using AutoDock Vina. Table S8. Comparison of docking scores and kinase activity data in ABL1 and EGFR. Table S9. Tanimoto coefficient scores between two drugs. Figure S1. Re-docking of imatinib and erlotinib in ABL1 and EGFR. Figure S2. The results of re-docking ligands on different DFG states.
The Second Data Release of the KODIAQ Survey
Creators: name: O'Meara, John M.
name: Lehner, Nicolas
name: Howk, J. Christopher
name: Prochaska, J. Xavier
name: Fox, Andrew J.
name: Peeples, Molly S.
name: Tumlinson, Jason
name: O'Shea, Brian W.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present and make publicly available the second data release (DR2) of the Keck Observatory Database of Ionized Absorption toward Quasars (KODIAQ) survey. KODIAQ DR2 consists of a fully-reduced sample of 300 quasars at 0.07 < z_em < 5.29 observed with HIRES at high resolution (36,000 <= R <= 103,000). DR2 contains 831 spectra available in continuum normalized form, representing a sum total exposure time of ~4.9 megaseconds on source. These co-added spectra arise from a total of 1577 individual exposures of quasars taken from the Keck Observatory Archive (KOA) in raw form and uniformly processed. DR2 extends DR1 by adding 130 new quasars to the sample, including additional observations of QSOs in DR1. All new data in DR2 were obtained with the single-chip Tektronix TK2048 CCD configuration of HIRES in operation between 1995 and 2004. DR2 is publicly available to the community, housed as a higher level science product at the KOA and in the igmspec database (v03).
description: Accepted for publication in the Astronomical Journal. 4 pages, 3 tables, 7 figures
Asteroseismic signatures of helium gradients in late F-type stars
Creators: name: Castro, M.
name: Vauclair, S.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Element diffusion is expected to occur in all kinds of stars : according to the relative effect of gravitation and radiative acceleration, they can fall or be pushed up in the atmospheres. Helium sinks in all cases, thereby creating a gradient at the bottom of the convective zones. This can have important consequences for the sound velocity, as has been proved in the sun with helioseismology. We investigate signatures of helium diffusion in late F-type stars by asteroseismology. Stellar models were computed with different physical inputs (with or without element diffusion) and iterated in order to fit close-by evolutionary tracks for each mass. The theoretical oscillation frequencies were computed and compared for pairs of models along the tracks. Various asteroseismic tests (large separations, small separations, second differences) were used and studied for the comparisons. The results show that element diffusion leads to changes in the frequencies for masses larger than 1.2 Msun. In particular the helium gradient below the convective zone should be detectable through the second differences.
description: 8 pages, 11 figures, 2 tables Accepted for publication in Astronomy and Astrophysics. The official date of acceptance is 03/05/2006
Hopf algebras of dimension 2p
Creators: name: Ng, Siu-Hung
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Algebra (math.QA)
subject: Rings and Algebras (math.RA)
subject: FOS: Mathematics
subject: 16W30

description: Let $H$ be a finite-dimensional Hopf algebra over an algebraically closed field of characteristic 0. If $H$ is not semisimple and $\dim(H)=2n$ for some odd integer $n$, then $H$ or $H^*$ is not unimodular. Using this result, we prove that if $\dim(H)=2p$ for some odd prime $p$, then $H$ is semisimple. This completes the classification of Hopf algebras of dimension $2p$.
description: 6 pages
V4745 Sgr -- a nova above the period gap and an intermediate polar candidate
Creators: name: Dobrotka, Andrej
name: Retter, Alon
name: Liu, Alex
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A period analysis of CCD unfiltered photometry of V4745 Sgr (Nova Sgr 2003 #1) performed during 23 nights in the years 2003 - 2005 is presented. The photometric data are modulated with a period of 0.20782 +- 0.00003 d ($4.98768 +- 0.00072 h). Following the shape of the phased light curve and the presence of the periodicity in all data sets with no apparent change in its value, we interpret this periodicity as orbital in nature and this is consistent with a cataclysmic variable above the period gap. We found a probable short-term periodicity of 0.017238 +- 0.000037 d (24.82272 +- 0.05328 m) which we interpret as the probable spin period of the white dwarf or the beat period between the orbital and spin period. Therefore, we propose that nova V4745 Sgr should be classified as an intermediate polar candidate, supporting the proposed link between transition-oscillation novae and intermediate polars. The mass-period relation for cataclysmic variables yields a secondary mass of about 0.52 +- 0.05 M_solar.
description: 6 pages, 8 figures, accepted for publication in MNRAS
Light Quenched Hadron Spectrum and Decay Constants on different Lattices
Creators: name: Allton, C. R.
name: Gimenez, V.
name: Giusti, L.
name: Rapuano, F.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this paper we study O(2000) (quenched) lattice configurations from the APE collaboration, for different lattice volumes and for 6.0 \le beta \le 6.4 using both the Wilson and the SW-Clover fermion actions. We determine the light hadronic spectrum and meson decay constants and study the mesonic dispersion relation. We extract the hadronic variable J and the strange quark mass in the continuum at the next-to-leading order obtaining m_s^{MSbar}(mu=2 GeV) = 122 +/- 20 MeV. A study is made of their dependence on lattice spacing. We implement a newly developed technique to extract the inverse lattice spacing using data at the simulated values of the quark mass (i.e. at masses around the strange quark mass).
description: 36 pages, LateX with 20 postscript figures. Small numerical errors corrected, no conclusions changed
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 1006
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
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: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1006, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1006, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Chelidonium corniculatum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Papaveraceae
Chelidonium
Chelidonium corniculatum

description: Chelidonium corniculatum, spec. nov.
3. Chelidonium pedunculis unifloris, foliis sessilibus pinnatifidis, caule hispido.
 Chelidonium hispidum, pedunculis unifloris. Hort. ups. 137. Sauv. monsp. 286.
 Glaucium hirsutum, flore phoeniceo. Tournef. inst. 254.
 Papaver cornutum, phoeniceo flore. Clus. hist. 2. p. 91.
 Habitat in Hungaria , Bohemia , Monspelii . ☉
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 506, DOI: 10.5281/zenodo.3931989
Einstein Metrics on Exotic Spheres in Dimensions 7, 11, and 15
Creators: name: Boyer, Charles P.
name: Galicki, Krzysztof
name: Kollár, János
name: Thomas, Evan
Publisher: name: arXiv
Year: 2003
Subjects: subject: Differential Geometry (math.DG)
subject: High Energy Physics - Theory (hep-th)
subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 53C20, 53C12, 14E30

description: In a recent article the first three authors proved that in dimension $4m+1$ all homotopy spheres that bound parallelizable manifolds admit Einstein metrics of positive scalar curvature which, in fact, are Sasakian-Einstein. They also conjectured that all such homotopy spheres in dimension $4m-1, m\geq2$ admit Sasakian-Einstein metrics \cite{BGK}, and proved this for the simplest case, namely dimension $7.$ In this paper we describe computer programs that show that this conjecture is also true for 11-spheres and 15-spheres. Moreover, a program is given that determines the partition of the 8610 deformation classes of Sasakian-Einstein metrics into the 28 distinct oriented diffomorphism types in dimension $7.$
description: 7 pages
Annotations on letter B moving from Petrucci’s article
Creators: name: Marichal, Robert
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015

description: vue 33
description: Observations on A. PETRUCCI, Per la storia della scrittura romana: i graffiti di Condatomagos, "Bullettino dell'archivio paleografico italiano", III serie , 1 (1962), 85-132.
description: Source: 4MAR_1_1.3.1-3-1
description: created: n. d.