cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Baryon-Number Nonconservation and the Stability of Strange Matter
Creators: name: Keith, E.
name: Ma, Ernest
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: If baryon-number nonconservation exists in the form of an effective six-quark operator which also changes strangeness by four units, it could have a tremendous impact on the absolute stability of strange quark matter. We show that such an operator is negligible in the supersymmetric standard model with $λ_{ijk} u_i^c d_j^c d_k^c$ terms in the superpotential, but may be of importance in models with exotic particle content. From the experimental lower limit of $10^{25}$ years on the stability of nuclei, we find a model-independent lower limit of the order $10^5$ years on the stability of strange matter against such decays.
description: 14 pages, LaTex, 2 figures available upon request from evan@ucrph0.ucr.edu
The SAMI Galaxy Survey: Global stellar populations on the size-mass plane
Creators: name: Scott, Nicholas
name: Brough, S.
name: Croom, Scott M.
name: Davies, Roger L.
name: van de Sande, Jesse
name: Allen, J. T.
name: Bland-Hawthorn, Joss
name: Bryant, Julia J.
name: Cortese, Luca
name: D'Eugenio, Francesco
name: Federrath, Christoph
name: Ferreras, Ignacio
name: Goodwin, Michael
name: Groves, Brent
name: Konstantopoulos, Iraklis
name: Lawrence, Jon S.
name: Medling, Anne M.
name: Moffett, Amanda J.
name: Owers, Matt S.
name: Richards, Samuel
name: Robotham, A. S. G.
name: Tonini, Chiara
name: Yi, Sukyoung K.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present an analysis of the global stellar populations of galaxies in the SAMI Galaxy Survey. Our sample consists of 1319 galaxies spanning four orders of magnitude in stellar mass and includes all morphologies and environments. We derive luminosity-weighted, single stellar population equivalent stellar ages, metallicities and alpha enhancements from spectra integrated within one effective radius apertures. Variations in galaxy size explain the majority of the scatter in the age--mass and metallicity--mass relations. Stellar populations vary systematically in the plane of galaxy size and stellar mass, such that galaxies with high stellar surface mass density are older, more metal-rich and alpha-enhanced than less dense galaxies. Galaxies with high surface mass densities have a very narrow range of metallicities, however, at fixed mass, the spread in metallicity increases substantially with increasing galaxy size (decreasing density). We identify residual correlations with morphology and environment. At fixed mass and size, galaxies with late-type morphologies, small bulges and low Sersic n are younger than early-type, high n, high bulge-to-total galaxies. Age and metallicity both show small residual correlations with environment; at fixed mass and size, galaxies in denser environments or more massive halos are older and somewhat more metal rich than those in less dense environments. We connect these trends to evolutionary tracks within the size--mass plane.
description: 25 pages, 18 figures, MNRAS in press Corrected typo in author list
title: ADCO, Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Cart. 172 (11 H 69), 115 folios, f. 0180
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: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Archives départementales de la Côte-d'Or, Cart. 172 (11 H 69), 115 folios, f. 0180, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Archives départementales de la Côte-d'Or, Cart. 172 (11 H 69), 115 folios, f. 0180, 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
An Improved Age-Activity Relationship for Cool Stars older than a Gigayear
Creators: name: Booth, R. S.
name: Poppenhaeger, K.
name: Watson, C. A.
name: Aguirre, V. Silva
name: Wolk, S. J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Stars with convective envelopes display magnetic activity, which decreases over time due to the magnetic braking of the star. This age-dependence of magnetic activity is well-studied for younger stars, but the nature of this dependence for older stars is not well understood. This is mainly because absolute stellar ages for older stars are hard to measure. However, relatively accurate stellar ages have recently come into reach through asteroseismology. In this work we present X-ray luminosities, which are a measure for magnetic activity displayed by the stellar coronae, for 24 stars with well-determined ages older than a gigayear. We find 14 stars with detectable X-ray luminosities and use these to calibrate the age-activity relationship. We find a relationship between stellar X-ray luminosity, normalized by stellar surface area, and age that is steeper than the relationships found for younger stars, with an exponent of $-2.80 \pm 0.72$. Previous studies have found values for the exponent of the age-activity relationship ranging between -1.09 to -1.40, dependent on spectral type, for younger stars. Given that there are recent reports of a flattening relationship between age and rotational period for old cool stars, one possible explanation is that we witness a strong steepening of the relationship between activity and rotation.
description: 16 pages, 5 figures, 5 tables, Accepted for publication in MNRAS
Cosmography from well-localized Fast Radio Bursts
Creators: name: Fortunato, Jéferson A. S.
name: Hipólito-Ricaldi, Wiliam S.
name: Santos, Marcelo V. dos
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Fast Radio Bursts (FRBs) are millisecond-duration pulses occurring at cosmological distances that have emerged as prominent cosmological probes due to their dispersion measure (DM) evolution with redshift. In this work, we use cosmography, a model-independent approach to describe the evolution of the universe, to introduce the cosmographic expansion of the DM-z relation. By fitting two different models for the intergalactic medium and host contributions to a sample of 23 well-localized FRBs, we estimate the kinematic parameters $q_0=-0.59 \substack{+0.20 \\ -0.17}$, $j_0=1.08 \substack{+0.62 \\ -0.56}$, $s_0=-2.1\pm7.0$, and $H_0=69.4\pm4.7$ achieving a precision of $6\%$ and $7\%$ for the Hubble constant depending on the models used for contributions. Furthermore, we demonstrate that this approach can be used as an alternative and complementary cosmological-model independent method to revisit the long-standing "Missing Baryons" problem in astrophysics by estimating that $82\%$ of the baryonic content of the universe resides in the intergalactic medium, within $7\%$ and $8\%$ precision, according to the contribution models considered here. Our findings highlight the potential of FRBs as a valuable tool in cosmological research and underscore the importance of ongoing efforts to improve our understanding of these enigmatic events.
ИСПОЛЗОВАНИЕ АУТЕНТИЧНЫХ МАТЕРИАЛОВ В ПРОЦЕССЕ РАЗВИТИЯ КОММУНИКАТИВНОЙ КОМПЕТЕНЦИИ
Creators: name: Курбанова Дилафруз Шухратовна  Преподаватель кафедры «Методы преподавания английского языка и образовательные технологии» Узбекского государственного университета мировых языков
Publisher: name: Zenodo
Year: 2025

description: В данной статье основное внимание уделяется аутентичной оценке коммуникативной компетенции, указываются основные характеристики аутентичных материалов и сравниваются с традиционными способами оценки и языковых навыков. В частности, аутентичный материал представляет трудности для преподавателей английского языка при планировании знания и содержит сложные и трудные языковые структуры. Описывается история подхода к изучению данного понятия, а также аутентичными и адаптированными материалами и изучаются пути включения аутентичных материалов в процесс обучения английскому языку.

Ключевые слова: аутентичные материалы, аутентичность, изучение иностранного языка, языковая компетенция, реальная языковая ситуация.
Memories of a POW
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: Attached is the account of AB Sidney William Swain's experience of capture by a German ship at the beginning of WW2, in his own written words.
Gypsophila paniculata Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Gypsophila
Gypsophila paniculata

description: Gypsophila paniculata, spec. nov.
 3. Gypsophila foliis lanceolatis scabris, corollis revolutis. Gen. nov. 1108.
 Alsine frutescens, caryophylli folio, flore parvo albo. Gerb. tanais. 15.
 Habitat in Sibiriae , Tatariae desertis sabulosis, Tawrow , Bielogrod . ♃
 Folia margine scabra, acuta. Stamina in fundo floris latent. Petala revoluta, minora quam in congeneribus. Styli longiores corolla, incurvi.
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 407, DOI: 10.5281/zenodo.3931989
Gypsophila altissima Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Gypsophila
Gypsophila altissima

description: Gypsophila altissima, spec. nov.
 4. Gypsophila foliis lanceolatis subtrinerviis rectis. Gen. nov. 1103.
 Saponaria calycibus pentaphyllis, corymbis fastigiatis, foliis lanceolatis, caule adscendente. Hort. ups. 107.
 Habitat in Sibiria . ♃
 Differt a sequente magnitudine dupla vel quadrupla omnium partium; Structura eadem, tamen diversa species.
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 407, DOI: 10.5281/zenodo.3931989
Double-peaked Balmer line emission in the radio-quiet AGN RX J1042+1212
Creators: name: Puchnarewicz, E. M.
name: Mason, K. O.
name: Carrera, F. J.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present optical and X-ray spectra of a radio-quiet X-ray selected AGN, RX J1042+1212 ($z$=0.271). The Halpha and Hbeta emission lines are very broad (with full widths at half maximum of ~10000 km s-1) and have double-peaked profiles. Such features are rarely observed in AGN in general but are even more unusual in radio-quiet objects. The analysis of the ROSAT PSPC data reveals a non-varying, unabsorbed spectrum with an energy spectral index, alphax=1.2 and little or no emission from a soft X-ray excess. The slope of the optical spectrum is similar, alphaopt=1.0, and is consistent with an extrapolation of the X-ray spectrum, suggesting that the same power-law continuum may dominate throughout and that the big blue bump component is relatively weak. We look for a link between these various properties and investigate models of double-peaked Balmer line emission in AGN. An accretion disc origin is unlikely in RX J1042+1212 as this model predicts that lines emitted by a disc should have a net gravitational redshift (both Halpha and Hbeta have a net blueshift). Emission from two broad line regions, each gravitationally bound to one component of a supermassive black hole binary, is a possibility if the two components are similar in size and nature. Alternatively, the lines (or at least the narrow peaks of the lines) may be produced by a double-sided jet or bipolar flow.
description: TeX file and eps figures, .sty files included. Accepted in MNRAS
Time-resolved purification of photon pairs from ultrasmall sources
Creators: name: Sultanov, Vitaliy
name: Chekhova, Maria
Publisher: name: arXiv
Year: 2023
Subjects: subject: Quantum Physics (quant-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Generation of entangled photons through spontaneous parametric down-conversion (SPDC) from ultrasmall sources like thin films, metasurfaces, or nanoantennas, offers unprecedented freedom in quantum state engineering. However, as the source of SPDC gets smaller, the role of photoluminescence increases, which leads to the contamination of two-photon states with thermal background. Here we propose and implement a solution to this problem: by using pulsed SPDC and time distillation, we increase the purity and the heralding efficiency of the photon pairs. In the experiment, we increase the purity of two-photon states generated in a 7 $μ$m film of lithium niobate from 0.002 to 0.99. With the higher purity, we were able to observe and characterize different polarization states of photon pairs generated simultaneously due to relaxed phase matching. In particular, we showed the presence of orthogonally polarized photons, potentially usable for the generation of polarization entanglement.
Additional file 1: of INSIGHT responsive parenting intervention reduces infantâ s screen time and television exposure
Creators: name: Adams, Elizabeth
name: Marini, Michele
name: Stokes, Jennifer
name: Birch, Leann
name: Paul, Ian
name: Savage, Jennifer
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences

description: INSIGHT study CONSORT diagram. Flow diagram detailing the number of participants who were screened, enrolled, randomized, and completed study visits up to infant age 1 year. (PDF 234Â kb)
The integrable quantum group invariant A_{2n-1}^(2) and D_{n+1}^(2) open spin chains
Creators: name: Nepomechie, Rafael I.
name: Pimenta, Rodrigo A.
name: Retore, Ana L.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mathematical Physics (math-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Algebra (math.QA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: A family of A_{2n}^(2) integrable open spin chains with U_q(C_n) symmetry was recently identified in arXiv:1702.01482. We identify here in a similar way a family of A_{2n-1}^(2) integrable open spin chains with U_q(D_n) symmetry, and two families of D_{n+1}^(2) integrable open spin chains with U_q(B_n) symmetry. We discuss the consequences of these symmetries for the degeneracies and multiplicities of the spectrum. We propose Bethe ansatz solutions for two of these models, whose completeness we check numerically for small values of n and chain length N. We find formulas for the Dynkin labels in terms of the numbers of Bethe roots of each type, which are useful for determining the corresponding degeneracies. In an appendix, we briefly consider D_{n+1}^(2) chains with other integrable boundary conditions, which do not have quantum group symmetry.
description: 47 pages; v2: two references added and minor changes
Additional file 1: of Whole-genome sequencing of Aspergillus tubingensis G131 and overview of its secondary metabolism potential
Creators: name: Choque, Elodie
name: Klopp, Christophe
name: Valiere, Sophie
name: Raynal, José
name: Mathieu, Florence
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Table S1. BUSCO analysis of A. tubingensis G131 scaffolds assembly. Figure S1. Dot Plot analysis between A. tubingensis G131 and A. tubingensis CBS 148.33 to order the scaffold assembly. Table S2. Accession number (NCBI) of sequences used for phylogenetic analysis. Figure S2. Phylogenetic tree produced from Rpb2 partial gene sequence of 38 strains of black aspergilli. Figure S3. Phylogenetic tree produced from Cam1 partial gene sequence of 38 strains of black aspergilli. Figure S4. Phylogenetic tree produced from BenA partial gene sequence of 38 strains of black aspergilli. Figure S5. Blast2GO statistics summary. Table S3. KOG analysis of A. tubingensis G131, A. tubingensis CBS 134.48, A. kawachii IFO 4308 and A. niger CBS 513.88. Figure S6. Venn Diagram of secretome analysis obtained through SignalP and OrthoMCL analysis. Table S4. SM Clusters coordinates of the scaffolds assembly. Figure S7. Genes similarity between SM cluster 44 from A. tubingensis G131 and others known fungal biosynthetic cluster. (Results obtained with AntiSMASH software). Figure S8. AntiSMASH schematic representation of the conserved domains in SM clusters unique in A. tubingensis G131 and their similarities with other SM clusters identified in various fungi (AntiSMASH results). Table S5. Blast results for Ochratoxin A, Fumonisins and asperazine biosynthesis in A. tubingensis. Figure S9. Schematic representation of Cluster 4 presenting small homology with fumonisin cluster. Figure S10. Repartition of conserved domains in predictive enzymes coding genes of the asperazine cluster obtained with CD search. Figure S11. Conserved domain (CD-Search) and Distance tree results obtained from NCBI BlastP analysis of predicted PKS of A. tubingensis G131 putatively involved in NGPs synthesis. Figure S12. Clustal Omega Alignment of predicted PKS from SM Clusters 54 and 16 of A. tubingensis G131. Figure S13. Genes similarity between Cluster 16 from A. tubingensis G131 with other known fungal genomes assembly. (PDF 2680 kb)
The particle in a box in PT quantum mechanics and an electromagnetic analog
Creators: name: Dasarthy, Anirudh
name: Isaacson, Joshua P.
name: Jones-Smith, Katherine
name: Tabachnik, Jason
name: Mathur, Harsh
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In PT quantum mechanics a fundamental principle of quantum mechanics, that the Hamiltonian must be hermitian, is replaced by another set of requirements, including notably symmetry under PT, where P denotes parity and T denotes time reversal. Here we study the role of boundary conditions in PT quantum mechanics by constructing a simple model that is the PT symmetric analog of a particle in a box. The model has the usual particle in a box Hamiltonian but boundary conditions that respect PT symmetry rather than hermiticity. We find that for a broad class of PT-symmetric boundary conditions the model respects the condition of unbroken PT-symmetry, namely that the Hamiltonian and the symmetry operator PT have simultaneous eigenfunctions, implying that the energy eigenvalues are real. We also find that the Hamiltonian is self-adjoint under the PT inner product. Thus we obtain a simple soluble model that fulfils all the requirements of PT quantum mechanics. In the second part of this paper we formulate a variational principle for PT quantum mechanics that is the analog of the textbook Rayleigh-Ritz principle. Finally we consider electromagnetic analogs of the PT-symmetric particle in a box. We show that the isolated particle in a box may be realized as a Fabry-Perot cavity between an absorbing medium and its conjugate gain medium. Coupling the cavity to an external continuum of incoming and outgoing states turns the energy levels of the box into sharp resonances. Remarkably we find that the resonances have a Breit-Wigner lineshape in transmission and a Fano lineshape in reflection; by contrast in the corresponding hermitian case the lineshapes always have a Breit-Wigner form in both transmission and reflection.
description: Published in 2013, previously unavailable on arxiv
Confinement-Induced Nonlocality and Casimir Force in Transdimensional Systems
Creators: name: Bondarev, Igor V.
name: Pugh, Michael D.
name: Rodriguez-Lopez, Pablo
name: Woods, Lilia M.
name: Antezza, Mauro
Publisher: name: arXiv
Year: 2023
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study within the framework of the Lifshitz theory the long-range Casimir force for in-plane isotropic and anisotropic free-standing transdimensional material slabs. In the former case, we show that the confinement-induced nonlocality not only weakens the attraction of ultrathin slabs but also changes the distance dependence of the material-dependent correction to the Casimir force to go as $\sim\!1/\!\sqrt{l}$ contrary to the $\sim\!1/l$ dependence of that of the local Lifshitz force. In the latter case, we use closely packed array of parallel aligned single-wall carbon nanotubes in a dielectric layer of finite thickness to demonstrate strong orientational anisotropy and crossover behavior for the inter-slab attractive force in addition to its reduction with decreasing slab thickness. We give physical insight as to why such a pair of ultrathin slabs prefers to stick together in the perpendicularly oriented manner, rather than in the parallel relative orientation as one would customarily expect.
description: 20 pages, 4 figures, 52 references
Supersymmetric Scenarios with Dominant Radiative Neutralino Decay
Creators: name: Ambrosanio, Sandro
name: Mele, Barbara
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The radiative decay of the next-to-lightest neutralino into a lightest neutralino and a photon is analyzed in the MSSM. We find that significant regions of the supersymmetric parameter space with large radiative BR's (up to about 100%) do exist. The radiative channel turns out to be enhanced when the neutralino tree-level decays are suppressed either "kinematically" or "dynamically". In general, in the regions allowed by LEP data and not characterized by asymptotic values of the SuSy parameters, the radiative enhancement requires tan beta ~= 1 and/or M_1 ~= M_2, and negative values of μ. We present typical specific scenarios where these "necessary" conditions are fulfilled, relaxing the usual relation M_1=(5/3)*tan^2(th_W)*M_2. The influence of varying the stop masses and mixing angle when the radiative decay is enhanced is also considered. Some phenomenological consequences of the above picture are discussed.
description: 32 pages, LaTeX file + 23 figures embedded with epsf.sty. In this revised version, Eq.(3) plus some related notations and text passages have been changed. Minor error corrected in Fig.12(a). The numerical analysis and the conclusions of the paper are not affected. (Includes the erratum to appear in Phys. Rev. D.) Source and ps files are also available at ftp://hpteo.roma1.infn.it/pub/preprints/ambr-mele/Rome1-1148/ or at http://feynman.physics.lsa.umich.edu/~ambros/Physics.html#16
Gypsophila fastigiata Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Gypsophila
Gypsophila fastigiata

description: Gypsophila fastigiata, spec. nov.
 5. Gypsophila foliis lanceolato-linearibus obsolete triquetris laevibus obtusis secundis. Gen. nov. 1103.
 Saponaria caule simplici, foliis linearibus ex alis foliorum confertis teretibus. Hort. cliff. 166.
 Saponaria calycibus pentaphyllis, corymbis fastigiatis, foliis linearibus, caule adscendente. It. gotl. 282. Fl. suec. 246. Sauv. monsp. 145.
 Saponaria petalis ovatis, foliis glaucis pulposis linearibus. Hall. jen. 117. t.2. f.1.
 Caryophyllus saxatilis, floribus gramineis, umbellatis corymbis. Bauh. pin. 211.
 Polygonum majus erectum angustifolium, floribus candidis. Mentz. pug. t.2. f.2.
 Habitat in Gotlandiae , Borussiae , Helvetiae rupibus. ♃
 Caulis in hac, non in antecedente, ante florescentiam procumbit, hinc folia secunda.
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 407-408, DOI: 10.5281/zenodo.3931989
Cathedral of St Paul, Wellington
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: While visiting the North Island of New Zealand (Te Ika-a-Māui, Aotearoa) I attended a service in the Cathedral of St Paul, Wellington (Te Whanganui-a-Tara). There were many memorials to distract me. After the service, I took these photos of:The Chancel’s stained-glass windows, that commemorate the armed services, those who flew with the Royal New Zealand Air Force (RNZAF) and Royal Air Force (RAF), the NZ Army, the Royal New Zealand Navy and the Merchant Navy. One inscription reads "In grateful memory of those men and women who lost their lives in the Navies and Merchant Service of the Commonwealth during two World Wars, the above windows were installed by and dedicated presence of former shipmates, 1967."The Cross of Nails, according to the inscriptions are from Coventry Cathedral. When it was destroyed by the bombing nails from its roof were collected, silvered, and made into crucifixes that were sent to organisations committed to peace and reconciliation around the world like this Anglican cathedral.Other inscriptions and displays including "To the glory of God. In memory of all who served in the 14th New Zealand Light Anti-Aircraft Regiment 2NZEF Egypt, North Africa, Italy 1941 1945"; "Given by the Wellington District Group of the Normandy Veterans Association of NZ to honour the memory of our comrades who gave their lives in the Normandy Campaign 6 June to 20 August 1944 which led to the liberation of Western Europe VE Day 8 May 1945"; "To the Glory of God a tribute to Anglican Chaplains to the Forces - past, present and future. Sponsored by the Anglican Church Military Affairs Committee with the support of the New Zealand Defence Force".
Self-consistent interaction of linear gravitational and electromagnetic waves in non-magnetized plasma
Creators: name: Garg, Deepen
name: Dodin, I. Y.
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: This paper explores the hybridization of linear metric perturbations with linear electromagnetic (EM) perturbations in non-magnetized plasma for a general background metric. The local wave properties are derived from first principles for inhomogeneous plasma, without assuming any symmetries of the background metric. First, we derive the effective (``oscillation-center'') Hamiltonian that governs the average dynamics of plasma particles in a prescribed quasimonochromatic wave that involves metric perturbations and EM fields simultaneously. Then, using this Hamiltonian, we derive the backreaction of plasma particles on the wave itself and obtain gauge-invariant equations that describe the resulting self-consistent gravito-electromagnetic (GEM) waves in a plasma. The transverse tensor modes of gravitational waves are found to have no interaction with the plasma and the EM modes in the geometrical-optics limit. However, for ``longitudinal" GEM modes with large values of the refraction index, the interplay between gravitational and EM interactions in plasma can have a strong effect. In particular, the dispersion relation of the Jeans mode is significantly affected by electrostatic interactions. As a spin-off, our calculation also provides an alternative resolution of the so-called Jeans swindle.
description: 15 pages
Additional file 1: Table S1. of B-cell differentiation is pressuromodulated as determined by pressuromodulation mapping: Part I, cell differentiation
Creators: name: Sarin, Hemant
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Plant Biology

description: Non-chromosome 14 gene location data with tropy pairing and isotropy type. Stem cell marker gene, CD34; transcription factor adapter gene, PRDM1 and B-cell polarization genes, PTPRC and CD40; B-cell cluster of differentiation receptor genes, CD19, MS4A1, CR2, CD27 and CD38; cluster of differentiation receptor B-cell antigen receptor complex-associated proteins, CD79A and CD79B; Third, VDJ recombinase genes, RAG2 and RAG1, and consensus sequence recognition (CSR)/somatic hypermutation enzyme genes, APOBEC3A/APOBEC3B, AICDA, APOBEC3C/APOBEC3D/APOBEC3F/APOBEC3G, and APOBEC3H; and cell proliferation marker genes, PCNA, ENPP1, MKI67 and ESPL1. (PDF 843Â kb)
On norms in some class of exponential type Orlicz spaces of random variables
Creators: name: Zajkowski, Krzysztof
Publisher: name: arXiv
Year: 2017
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 46E30, 60E15

description: A new characterization of the exponential type Orlicz spaces generated by the functions $\exp(|x|^p)-1$ ($p\ge 1$) is given. We define norms for centered random variables belonging to these spaces. We show equivalence of these norms with the Luxemburg norms. On the example of the Hoeffding inequality we present some application of these norms in a probabilistic context.
description: 9 pages
Gypsophila perfoliata Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Gypsophila
Gypsophila perfoliata

description: Gypsophila perfoliata, spec. nov.
6. Gypsophila foliis ovato-lanceolatis semiamplexicaulibus.
 Saponaria foliis lanceolatis, calycibus campanulatis angulatis. Hort. cliff. 165.
 Spergula multiflora, foliis inferioribus saponariae, superioribus behen similibus. Dill. elth. 368. t.276. f.357.
 Habitat in Hispania & Oriente .
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 408, DOI: 10.5281/zenodo.3931989
Quark mass effects in QCD jets
Creators: name: Rodrigo, Germán
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present the calculation of the decay width of the Z-boson into three jets including complete quark mass effects to second order in the strong coupling constant. The study is done for different jet clustering algorithms such as EM, JADE, E and DURHAM. Because three-jet observables are very sensitive to the quark mass we consider the possibility of extracting the bottom quark mass from LEP data.
description: 6 pages, LaTeX. Talk given at High Energy Physics International Euroconference on Quantum Chromodynamics (QCD 96), Montpellier, France, 4-12 Jul 1996. Uses espcrc2.sty
Maximum Brightness and Post-Maximum Decline of Light Curves of SN~Ia: A Comparison of Theory and Observations
Creators: name: Höflich, P.
name: Khokhlov, A.
name: Wheeler, J. C.
name: Hamuy, M.
name: Phillips, M. M.
name: Suntzeff, N. B.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compare the observed correlations between the maximum brightness, postmaximum decline rate and color at maximum light of Type Ia supernovae (SN Ia) with model predictions. The observations are based on a total of 40 SN Ia with 29 SN of the Calan Tololo Supernova Search and 11 local SN which cover a range of 2 mag in the absolute visual brightness. The observed correlations are not tight, one dimensional relations. Supernovae with the same postmaximum decline or the same color have a spread in visual magnitude of about 0.7 mag. The dispersion in the color-magnitude relation may result from uncertainties in the distance determinations or the interstellar reddening within the host galaxy. The dispersion in the decline rate-magnitude relation suggests that an intrinsic spread in the supernova properties exists that cannot be accounted for by any single relation between visual brightness and postmaximum decline. Theoretical correlations are derived from a grid of models which encompasses delayed detonations, pulsating delayed detonations, the merging scenario and helium detonations. We find that the observed correlations can be understood in terms of explosions of Chandrasekhar mass white dwarfs. Our models show an intrinsic spread in the relations of about 0.5 mag in the maximum brightness and about 0.1 mag in the B-V color. Our study provides strong evidence against the mechanism of helium detonation for subluminous, red SN Ia.
description: 7 pages, 3 figures, macros ''aaspp.sty'. LaTeX Style. Astrophysical Journal Letters, submitted Jul. 1995, revised Aug. 1995, resubmitted Sep. 1996
Gypsophila rigida Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Gypsophila
Gypsophila rigida

description: Gypsophila rigida, spec. nov.
 7. Gypsophila foliis lineari-lanceolatis planis, caule dichotomo, pedunculis bifloris, petalis emarginatis. Gen. nov. 1103.
 Saponaria caule dichotomo, foliis subulatis planis. Hort. cliff. 445. Roy. lugdb. 445.
 Saponaria caule brachiato, capillaceo folio, calyce campanulato, floribus sparsis. Sauv. monsp. 145.
 Tunica minima. Dalech. hist. 1191.
 Habitat Monspelii et forte in Belgio . ♃
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 408, DOI: 10.5281/zenodo.3931989
Deep Network Approximation: Beyond ReLU to Diverse Activation Functions
Creators: name: Zhang, Shijun
name: Lu, Jianfeng
name: Zhao, Hongkai
Publisher: name: arXiv
Year: 2023
Subjects: subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: This paper explores the expressive power of deep neural networks for a diverse range of activation functions. An activation function set $\mathscr{A}$ is defined to encompass the majority of commonly used activation functions, such as $\mathtt{ReLU}$, $\mathtt{LeakyReLU}$, $\mathtt{ReLU}^2$, $\mathtt{ELU}$, $\mathtt{CELU}$, $\mathtt{SELU}$, $\mathtt{Softplus}$, $\mathtt{GELU}$, $\mathtt{SiLU}$, $\mathtt{Swish}$, $\mathtt{Mish}$, $\mathtt{Sigmoid}$, $\mathtt{Tanh}$, $\mathtt{Arctan}$, $\mathtt{Softsign}$, $\mathtt{dSiLU}$, and $\mathtt{SRS}$. We demonstrate that for any activation function $\varrho\in \mathscr{A}$, a $\mathtt{ReLU}$ network of width $N$ and depth $L$ can be approximated to arbitrary precision by a $\varrho$-activated network of width $3N$ and depth $2L$ on any bounded set. This finding enables the extension of most approximation results achieved with $\mathtt{ReLU}$ networks to a wide variety of other activation functions, albeit with slightly increased constants. Significantly, we establish that the (width,$\,$depth) scaling factors can be further reduced from $(3,2)$ to $(1,1)$ if $\varrho$ falls within a specific subset of $\mathscr{A}$. This subset includes activation functions such as $\mathtt{ELU}$, $\mathtt{CELU}$, $\mathtt{SELU}$, $\mathtt{Softplus}$, $\mathtt{GELU}$, $\mathtt{SiLU}$, $\mathtt{Swish}$, and $\mathtt{Mish}$.
The Population of Damped Lyman-alpha and Lyman Limit Systems in the Cold Dark Matter Model
Creators: name: Gardner, Jeffrey P.
name: Katz, Neal
name: Hernquist, Lars
name: Weinberg, David H.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Lyman limit and damped Lyman-alpha absorption systems probe the distribution of collapsed, cold gas at high redshift. Numerical simulations that incorporate gravity and gas dynamics can predict the abundance of such absorbers in cosmological models. We develop a semi-analytical method to correct the numerical predictions for the contribution of unresolved low mass halos, and we apply this method to the Katz et al. (1996) simulation of the standard cold dark matter model ($Ω=1$, $h=0.5$, $Ω_b=0.05$, $σ_8=0.7$). Using this simulation and higher resolution simulations of individual low mass systems, we determine the relation between a halo's circular velocity $v_c$ and its cross section for producing Lyman limit or damped absorption. We combine this relation with the Press-Schechter formula for the abundance of halos to compute the number of absorbers per unit redshift. The resolution correction increases the predicted abundances by about a factor of two at z=2, 3, and 4, bringing the predicted number of damped absorbers into quite good agreement with observations. Roughly half of the systems reside in halos with circular velocities $v_c>100\kms$ and half in halos with $35\kms150\kms$ typically harbor two or more systems capable of producing damped absorption. Even with the resolution correction, the predicted abundance of Lyman limit systems is a factor of three below observational estimates, signifying either a failure of standard CDM or a failure of these simulations to resolve the systems responsible for most Lyman limit absorption. By comparing simulations with and without star formation, we find that depletion of the gas supply by star formation affects absorption line statistics at $z>=2$ only for column densities exceeding $N_{HI}=10^{22} cm^{-2}$.
description: AASlatex, 17 pages w/ 3 embedded ps figures. Submitted to ApJ
Gypsophila muralis Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Gypsophila
Gypsophila muralis

description: Gypsophila muralis, spec. nov.
 8. Gypsophila foliis linearibus planis, caule dichotomo, petalis crenatis. Gen. nov. 1103.
 Saponaria calycibus pentaphyllis, corollis crenato-emarginatis, foliis subulatis planis. Fl. suec. 347. Sauv. monsp. 144.
 Saponaria foliis linearibus. Fl. lapp. 171.
 Caryophyllus minimus muralis. Bauh. pin. 211.
 Lychnis parva palustris, foliis acutis lanceolatis, flosculis purpureis. Mentz. pug. t.7. f.4.
 Habitat in Suecia , Germania , Helvetia ad vias. ☉
 Similis Diantho saxifrago, at caret squamis calycinis.
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 408, DOI: 10.5281/zenodo.3931989
NuSTAR and XMM-Newton observations of the 2015 outburst decay of GX 339-4
Creators: name: Stiele, H.
name: Kong, A. K. H.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The extent of the accretion disk in the low/hard state of stellar mass black hole X-ray binaries remains an open question. There are some evidence suggesting that the inner accretion disk is truncated and replaced by a hot flow, while the detection of relativistic broadened iron emission lines seems to require an accretion disk extending fully to the innermost stable circular orbit. We present comprehensive spectral and timing analyses of six Nuclear Spectroscopic Telescope Array (NuSTAR) and XMM-Newton observations of GX 339-4 taken during outburst decay during the autumn of 2015. Using a spectral model consisting of a thermal accretion disk, Comptonized emission, and a relativistic reflection component we obtain a decreasing photon index, consistent with an X-ray binary during outburst decay. Although, we observe a discrepancy in the inner radius of the accretion disk and that of the reflector, which can be addressed to the different underlying assumptions in each model, both model components indicate a truncated accretion disk that resiles with decreasing luminosity. The evolution of the characteristic frequency in Fourier power spectra and their missing energy dependence support the interpretation of a truncated and evolving disk in the hard state. The XMM-Newton dataset allowed us to study, for the first time, the evolution of the covariance spectra and ratio during outburst decay. The covariance ratio increases and steeps during outburst decay, consistent with increased disk instabilities.
description: 18 pages, 8 figures, accepted by ApJ
WikiJournal of Science 2018
Creators: name: Shafee, Thomas
Publisher: name: La Trobe
Year: 2018
Subjects: subject: 100504 Data Communications
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: Uncategorized

description: This is a promotional poster explaining the aims and scope of the WikiJournal of Science.
Saponaria officinalis Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Saponaria
Saponaria officinalis

description: Saponaria officinalis, spec. nov.
 1. Saponaria calycibus cylindricis, foliis ovato-lanceolatis. Hort. cliff. 165. Hort. ups. 106. Mat. med. 214. Roy. lugdb. 444. Gron. virg. 160. Gort. gelr. 245.
 Saponaria major laevis. Bauh. pin. 206.
 Saponaria vulgaris. Cam. epit. 152.
 Habitat in Europa media. ♃
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 408-409, DOI: 10.5281/zenodo.3931989
Saponaria officinalis var. hybrida Linnaeus, 1753, var. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Caryophyllaceae
Saponaria
Saponaria officinalis
Saponaria officinalis var. hybrida

description: Saponaria officinalis var. hybrida, var. nov.
 β. Saponaria concava anglica. Bauh. pin. 206. Moris. hist. 2. p.548. s.5. t.22. f.52.
 Gentiana folio convoluto. Bauh. hist. 3. p. 521.
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 408-409, DOI: 10.5281/zenodo.3931989
Discovery of Striking Difference of Molecular-Emission-Line Richness in the Potential Proto-Binary System NGC 2264 CMM3
Creators: name: Watanabe, Yoshimasa
name: Sakai, Nami
name: Lopez-Sepulcre, Ana
name: Sakai, Takeshi
name: Hirota, Tomoya
name: Liu, Sheng-Yuan
name: Su, Yu-Nung
name: Yamamoto, Satoshi
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have conducted an interferometric line survey in the 0.8 mm band toward the young high-mass protostar candidate NGC 2264 CMM3 with ALMA. CMM3 is resolved into the two continuum peaks, CMM3A and CMM3B, at an angular separation of 0.9". Thus, CMM3 is found to be a binary system candidate. We have detected molecular outflows associated with CMM3A and CMM3B each, indicating active star formation. In addition to the two peaks, six faint continuum peaks are detected around CMM3A and CMM3B, most of which are thought to be evolved low-mass protostars. CMM3A is found to be rich in molecular line emission including complex organic molecules such as HCOOCH3 and CH3OCH3. The emission of complex organic molecules is distributed within a compact region around the continuum peak of CMM3A. Hence, CMM3A apparently harbors a hot core. On the other hand, CMM3B is deficient in molecular line emission, although its continuum flux is almost comparable to that of CMM3A. Possible origins of the striking difference between CMM3A and CMM3B are discussed.
description: Accepted for publication in ApJ, 7 figures, 2 tables
Theoretical Uncertainties in the QCD Evolution of Structure Functions and their Impact on $α_s(M_Z^2)$
Creators: name: Blümlein, J.
name: Riemersma, S.
name: van Neerven, W. L.
name: Vogt, A.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The differences are discussed between various next-to-leading order prescriptions for the QCD evolution of parton densities and structure functions. Their quantitative impact is understood to an accuracy of 0.02\%. The uncertainties due to the freedom to choose the renormalization and factorization scales are studied. The quantitative consequences of the different uncertainties on the extraction of the strong coupling constant $α_s$ from scaling violations in deep--inelastic scattering are estimated for the kinematic regime accessible at HERA.
description: 10 pages Latex, including 3 eps-figures, and a style file. To appear in: Proc. of the International Workshop: QCD and QED in Higher Orders, Rheinsberg, April, 1996, Nucl. Phys. {\bf B} (Proc. Suppl); The lay-out of the paper has been changed, one figure sent separately before has been bound in