cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The AGN fueling/feedback cycle in LERGs. A multi-phase study of a sample of nearby radio galaxies
Creators: name: Ruffa, Ilaria
Publisher: name: Zenodo
Year: 2019

description: Feedback associated with active galactic nuclei (AGN) can potentially play a role in shaping galaxies over cosmic time, by changing the physical conditions of the surrounding inter-stellar medium (ISM) or expelling it from the nuclear regions, thus impacting the star formation processes and the subsequent evolution of the host galaxy. The many details of such process, however, still remain poorly understood. Here we present the results obtained so far by analyzing ALMA Cycle 3 CO(2-1) and continuum observations of 9 lowexcitation radio galaxies (LERGs) in the southern sky. LERGs are a class of radio galaxies characterized by low accretion rates (<<0.01MEdd) and their feedback is almost entirely kinetic (i.e. jet-induced). The powering mechanism of these objects is still uncertain. Our work shows that (sub-)kpc rotating molecular discs are very common in LERGs (6 out of 9 sources detected in CO). Although signs of warps or asymmetries (i.e. gas not fully relaxed) are clearly visible in some of the detected discs, the bulk of the gas appears to be in ordered rotation (at least at the resolution of our ALMA observations). It is then likely that most of the cold gas in LERGs is in stable orbits, consistently with a relatively low accretion rate. Whenever possible, we also demonstrated that the CO discs are co-spatial with dust discs/lanes. In a couple of cases the gas shows kinematic misalignment with respect to the stellar component, pointing towards an external origin of the gas. The 3D modeling of the six CO discs indicates the presence of perturbations and/or radial motions in all the cases. In most of them, however, the spatial resolution of the observations does not allow us to draw strong conclusions. In our best resolved case (NGC 3100) the CO structure is disrupted in the direction of the northern jet, likely indicating a jet/ gas interaction. Furthermore, we find indications for non-negligible radial motions in the plane of the CO disc. This is likely consistent with the presence of inflow/outflow streaming motions associated with the spiral pattern that we observe at the centre of the CO disc
The DKP oscillator with a linear interaction in the cosmic string space-time
Creators: name: Hosseinpour, Mansoureh
name: Hassanabadi, Hassan
name: Andrade, Fabiano M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the relativistic quantum dynamics of a DKP oscillator field subject to a linear interaction in cosmic string space-time in order to better understand the effects of gravitational fields produced by topological defects on the scalar field. We obtain the solution of DKP oscillator in the cosmic string background. Also, we solve it with an ansatz in presence of linear interaction. We obtain the eigenfunctions and the energy levels of the relativistic field in that background.
description: 14 pages, no figure, comments are welcome
Pair correlations and the survival of superconductivity in and around a super-conducting impurity
Creators: name: Dubi, Yonatan
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The problem of the survival of superconductivity in a small super-conducting grain placed in a metal substrate is addressed. For this aim the pair correlations and super-conducting gap around and inside a negative-U impurity in one and two dimensions is calculated, in a discrete tight-binding model and a continuous model. Using the Hartree-Fock-Gorkov mean-field decomposition, it is found that pairing inside the gap occurs when the system has a degeneracy between successive number of electron pairs, and is highly sensitive to the chemical potential. For finite pairing in the island, pair correlations in the normal part may either decay exponentially or be long-ranged, depending on the strength of interaction. In addition, it is shown analytically that there is a minimal island size under-which pairing vanishes, and that it scales as a power-law, rather then exponentially as in isolated grains. These results are interpreted in terms of screening of the negative-U impurity by the electron gas.
description: Accepted for publication in Phys.Rev.B
Extracting the Single-Particle Gap in Carbon Nanotubes with Lattice Quantum Monte Carlo
Creators: name: Berkowitz, Evan
name: Koerber, Christopher
name: Krieg, Stefan
name: Labus, Peter
name: Laehde, Timo A.
name: Luu, Thomas
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We show how lattice Quantum Monte Carlo simulations can be used to calculate electronic properties of carbon nanotubes in the presence of strong electron-electron correlations. We employ the path integral formalism and use methods developed within the lattice QCD community for our numerical work and compare our results to empirical data of the Anti-Ferromagnetic Mott Insulating gap in large diameter tubes.
description: 8 pages, 5 figures, Lat2017 proceeding
title: Histoire : qapri bWxsi
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Additional file 3: of Proteomic analysis of Medulloblastoma reveals functional biology with translational potential
Creators: name: Rivero-Hinojosa, Samuel
name: Lau, Ling
name: Stampar, Mojca
name: Staal, Jerome
name: Huizhen Zhang
name: Gordish-Dressman, Heather
name: Northcott, Paul
name: Pfister, Stefan
name: Taylor, Michael
name: Brown, Kristy
name: Rood, Brian
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer

description: Figure S1. Correlation between mRNA and protein abundance by subgroups. a) Frequency distribution plots of mRNA-protein spearman’s correlations for each medulloblastoma subgroup. Positive mRNA-protein correlations were found for 68–80% of mRNA-protein pairs with means between (0.30–0.16) depending on the subgroup. However, just a small proportion of them were significant (10–17%). Group 3 was the subgroup with the highest number of significant positive correlations and the highest mean; in contrast, group 4 had the lowest mean. b) Box-plots depicting the distribution of mRNA-protein Spearman’s correlations by subgroup. p-values for differences between the subgroups were calculated with the Kruskal-Wallis rank-sum test. p-values indicating the differences between group 4 and the others were calculated with a two-sided Wilcoxon rank sum test. (PDF 706 kb)
title: Histoire : xinbada hanghai lixianji
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
The Size, Shape, and Scattering of Sagittarius A* at 86 GHz
Creators: name: Blackburn, Lindy
Publisher: name: Zenodo
Year: 2019

description: High-frequency very-long-baseline Interferometric (VLBI) observations of the Galactic Center supermassive black hole, Sagittarius A* (Sgr A*) have sufficient angular resolution to probe black hole accretion and outflow on event-horizon scales. We present the first unscattered image of Sgr A* taken at 86 GHz (3.5-mm) using the Global Millimeter VLBI Array (GMVA) joined for the first time by ALMA operating as a phased array in April 2017. The network reaches an angular resolution of 87 micro-arcseconds, improving upon previous experiments by a factor of two, and revealing a nearly isotropic intrinsic source. I will discuss the consequences for underlying accretion and emission models of Sgr A*, as well as new constraints on the properties of interstellar scattering using baselines to ALMA.
Additional file 4: of Results of a feasibility cluster randomised controlled trial of a peer-led school-based intervention to increase the physical activity of adolescent girls (PLAN-A)
Creators: name: Sebire, Simon
name: Jago, Russell
name: Banfield, Kathryn
name: Edwards, Mark
name: Campbell, Rona
name: Kipping, Ruth
name: Blair, Peter
name: Bryar Kadir
name: Garfield, Kirsty
name: Matthews, Joe
name: Lyons, Ronan
name: Hollingworth, William
Publisher: name: figshare
Year: 2018
Subjects: subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
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: Computational Biology

description: EQ-5D-Y and QALYs results, by treatment arm. Baseline, Time 1 and Time 2 EQ-5D-Y results and corresponding QALY estimates, by treatment arm (DOCX 14 kb)
Symmetric group representations and Z
Creators: name: Adve, Anshul
name: Yong, Alexander
Publisher: name: arXiv
Year: 2017
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: We discuss implications of the following statement about the representation theory of symmetric groups: every integer appears infinitely often as an irreducible character evaluation, and every nonnegative integer appears infinitely often as a Littlewood-Richardson coefficient and as a Kronecker coefficient.
description: 4 pages
title: Histoire : yiqianlingyiye yinzi
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
A STUDY ON SATISFACTION OF FARMERS TOWARDS MARKETING OF TURMERIC IN ERODE DISTRICT
Creators: name: Dr. M. Sangeetha* & Dr. K. Brindha**
Publisher: name: Zenodo
Year: 2024

description: Turmeric is also known as ancient and scared spice of India. It is otherwise called as golden spice of life. Indian turmeric is considered to be the best in the world. It occupies a distinctive position in Indian spice market and also in international market. Among the major turmeric producing states, Andhra Pradesh occupies 38% of the total area grown and 58.5% of total production in India. In Tamil Nadu, the turmeric growing districts are Erode, Karur, Coimbatore, Namakkal, Salem and Trichy. The present study aims to assess the level of satisfaction of farmers in marketing of turmeric and the various factors involved in determining their satisfaction. For the purpose of the study 755 samples were drawn by using stratified random sampling technique. The data were analysed by using one way ANOVA, descriptive analysis, Regression, Factor analysis and Kruskal Wally test. The study results finds that the turmeric farmers are satisfied with marketing, supports from market intermediaries and availability of rhizomes.
title: Inventaire des titres de propriété et des actes concernant les droits de l'abbaye de Morimond, Manuscrit n° 1, Bibliothèque municipale de Bourbonne-les-Bains, f.241
Creators: name: Rouzeau, Benoît
name: Rouzeau, Benoît
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cistercien

description: Inventaire des titres de propriété et des actes concernant les droits de l'abbaye de Morimond, Manuscrit n° 1, Bibliothèque municipale de Bourbonne-les-Bains. Numérisation en mode image
description: Relation: https://cisterciensetressources.lamop.fr/
description: Bibliographic citation: Inventaire des titres de propriété et des actes concernant les droits de l'abbaye de Morimond, Manuscrit n° 1, Bibliothèque municipale de Bourbonne-les-Bains, f.241, in Projet Cisterciens et Ressources [Ressource en ligne], https://cisterciensetressources.lamop.fr
description: Inventaire des titres de propriété et des actes concernant les droits de l'abbaye de Morimond, Manuscrit n° 1, Bibliothèque municipale de Bourbonne-les-Bains, f. 241
title: Histoire : alibaba
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Constructing equivariant vector bundles via the BGG correspondence
Creators: name: Posur, Sebastian
Publisher: name: arXiv
Year: 2017
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 14F05, 16E05, 16E20

description: We describe a strategy for the construction of finitely generated $G$-equivariant $\mathbb{Z}$-graded modules $M$ over the exterior algebra for a finite group $G$. By an equivariant version of the BGG correspondence, $M$ defines an object $\mathcal{F}$ in the bounded derived category of $G$-equivariant coherent sheaves on projective space. We develop a necessary condition for $\mathcal{F}$ being isomorphic to a vector bundle that can be simply read off from the Hilbert series of $M$. Combining this necessary condition with the computation of finite excerpts of the cohomology table of $\mathcal{F}$ makes it possible to enlist a class of equivariant vector bundles on $\mathbb{P}^4$ that we call strongly determined in the case where $G$ is the alternating group on $5$ points.
Navigasi Referensi Berbasis Bibliometrik
Creators: name: Gunawan, Fahmi
Publisher: name: Zenodo
Year: 2021
Subjects: Bibliometrik, Referensi

description: Navigasi referensi merupakan jantung publikasi. Dengan referensi, kita dapat mengetahui informasi terbaru dari tema yang hendak dikaji sehingga kita dapat mengetahui perbedaan riset kita dengan riset sebelumnya. Demikian pula, dengan referensi, kita dapat mendiskusikan riset kita dengan riset sebelumnya. Bahkan, informasi terakhir tentang penggunaan referensi, anda dapat melakukannya dengan menggunakan bibliometrik wa akhawatuha. Anda mau tahu bagaimana cara menavigasinya?
Aspects of Fractional Superstrings
Creators: name: Cleaver, Gerald B.
name: Rosenthal, Philip J.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate some issues relating to recently proposed fractional superstring theories with $D_{\rm critical}<10$. Using the factorization approach of Gepner and Qiu, we systematically rederive the partition functions of the $K=4,\, 8,$ and $16$ theories and examine their spacetime supersymmetry. Generalized GSO projection operators for the $K=4$ model are found. Uniqueness of the twist field, $ϕ^{K/4}_{K/4}$, as source of spacetime fermions is demonstrated. Last, we derive a linear (rather than quadratic) relationship between the required conformal anomaly and the conformal dimension of the supercurrent ghost.
description: 36 pages, CALT-68-1756 Revisions to match form to appear in Comm. Math. Phys. Use standard TeX. Derivation of affine partition functions related to $D=4,6$ models is now shown. References Updated
title: Histoire : fushang he yaomo
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Additional file 2: of Does the prehospital National Early Warning Score predict the short-term mortality of unselected emergency patients?
Creators: name: Hoikka, Marko
name: Silfvast, Tom
name: Ala-Kokko, Tero
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Developmental Biology

description: Flow chart of study cohort. (PDF 35 kb)
Instantons and the Ground State of the Massive Schwinger Model
Creators: name: Paranjape, M. B.
name: Ross, Robin
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the massive Schwinger model, quantum electrodynamics of massive, Dirac fermions, in 1+1 dimensions; with space compactified to a circle. In the limit that transitions to fermion--anti-fermion pairs can be neglected, we study the full ground state. We focus on the effect of instantons which mediate tunnelling transitions in the induced potential for the dynamical degree of freedom in the gauge field.
description: 17 pages, plain tex
Noise driven neuromorphic tuned amplifier
Creators: name: Fanelli, Duccio
name: Ginelli, Francesco
name: Livi, Roberto
name: Zagli, Niccolò
name: Zankoc, Clement
Publisher: name: arXiv
Year: 2017
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Pattern Formation and Solitons (nlin.PS)
subject: Biological Physics (physics.bio-ph)
subject: FOS: Physical sciences

description: Living systems implement and execute an extraordinary plethora of computational tasks. The inherent degree of large scale coordination emerges as a global property, from the intricate sea of microscopic interactions. The brain, with its structural and functional architecture, represents an emblematic example of hierarchic self-organization: elementary units, the neurons, act much like instruments of an orchestra, which combine diverse timbres to create harmonious symphonies. Neurons come indeed in different types, varying in shapes, connections and electrical properties. They all team up to process external stimuli from a number of sources and integrate the information to yield, from neurons to mind, different cognitive faculties. Identifying the coarse grained modules that exert, from bottom to up, pivotal neuronal functions constitutes a goal of paramount importance. On the other hand, the brain and its unraveled secrets could inspire novel biomimetics technologies to adaptively handle complex problems. Here, we investigate the intertwined stochastic dynamics of two populations of excitatory and inhibitory units, arranged in a directed lattice. The endogenous noise seeds a coherent amplification across the chain generating giant oscillations with tunable frequencies, a process that the brain could exploit to enhance, and eventually encode, different signals. The system works as an out-equilibrium thermal device under stationary operating conditions, the associated entropy production rate being analytically quantified. The same scheme could be invoked to design a novel family of manmade detectors capable of reacting to spatially distributed low intensity alerts.
description: Movies of the dynamics (as quoted in the text) are made available upon request. Write to duccio.fanelli@gmail.com
Patient Reported Measures used by Health Professionals for Adults on Home Enteral Nutrition and Contextual Factors surrounding their use: a scoping review protocol
Creators: name: Korai, Andriana
name: Carey, Sharon
name: Chen, Juliana
name: Allman-Farinelli, Margaret
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Dietetics and Clinical Nutrition
subject: Medicine and Health Sciences

description: This scoping review aims to summarise the existing literature on patient-reported outcome and experience measures (PROMs and PREMs) used for adult patients on HEN receiving care from health professionals and to summarise the contextual factors surrounding use of PROMs and PREMs in this population group.
Conversion of entangled states with nitrogen-vacancy centers coupled to microtoroidal resonators
Creators: name: Ji, Y. Q.
name: Shao, X. Q.
name: Yi, X. X.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We propose efficient schemes for converting three-photon, four-photon and five-photon GHZ state to a $W$ state or Dicke state, respectively with the nitrogen-vacancy (N-V) centers via single-photon input-output process and cross-Kerr nonlinearities. The total success probability can be improved by iterating the conversion process for the case of three-photon and five-photon while it does not require iteration for converting four-photon GHZ state to a $W$ state. The analysis of feasibility shows that our scheme is feasible for current experimental technology.
description: 11 pages, 6 figures
Alabama Livestock Research Report 2023
Creators: name: Department Of Animal Sciences
Publisher: name: Auburn University
Year: 2023
Subjects: animal sciences
beef forage
forage management
outreach
meat sciences

description: Almost $450 million worth of cattle and calves were sold in Alabama last year, generating a $2.5 billion impact. Hay and haylage production resulted in a value of $235 million to producers supporting the cattle and horse industries. Over $8 million worth of pork was marketed and $7 million of dairy products was generated in the state. With 47,000 meat goats, the state ranks 8th in goat production. Animal agriculture is alive and well in Alabama. At a time when the world population continues to grow, there is a greater demand for high‐quality animal protein. However, with population growth resulting in more urban sprawl, fewer land resources are available to meet the food and animal production needs. This increases the need for basic and targeted food animal research programs to provide technology that increases the efficiency of food animal production systems. The Department of Animal Science faculty and staff are answering this call by working synergistically in the development of research and extension programming across the state. Multidisciplinary programs are being developed, implemented, and delivered to meet the needs of stakeholders (both food animal producers and food animal consumers) across the state, region, nation, and world. Thus, it is with great pleasure that we present to you the second edition of the Alabama Livestock Research Report. Building upon the success of our first publication, this edition continues to serve as a comprehensive overview of the research and outreach initiatives developed in the Department of Animal Sciences at Auburn University. This publication combines reports from faculty, staff, and graduate students on campus and Experiment Stations. We provide in-depth information on our research programs, which incorporate growth biology, reproductive physiology, nutrition, genetics, meat science, animal health, management, and production practices into a comprehensive program. Additionally, we showcase our outreach activities and partnerships with industry stakeholders. We are proud to say that this report and research are made possible thanks to the financial support of funding agencies, organizations, and stakeholders who believe in the value of our work. Thank you to the faculty, students, and staff that contributed to this publication. Together, we can continue our mission of improving the lives of livestock producers and enhancing the sustainability of the livestock industry in Alabama and beyond. We invite you to explore our findings, learn about our progress, and engage with us as we work together to build a brighter future for our state’s agriculture. Should you have any questions about the research reported in this publication, do not hesitate to contact us or any of the authors of the individual reports. Sincerely, L. Wayne Greene Professor and Head Department of Animal Sciences 210 Upchurch Hall, Auburn Univ, AL 36849 greenlw@auburn.edu
title: Histoire : fushang he yaomo1
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
MILITARY PATRIOTIC EDUCATION - A COMPONENT PART OF SPIRITUAL EDUCATION
Creators: name: Vakhobov, Anvar
Publisher: name: Zenodo
Year: 2024

description: The article presents formation of our young people with intellectual potential, loyal to their country, the President, brave, brave and of course, healthy generation, forming in them the skills and competences of organizing defense in emergency situations and high moral and ethical qualities, the current in accordance with the principle of the interdependence and inseparability of education and upbringing of modern pedagogy, military-patriotic education is closely related to military pedagogical education.
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Cart. 185 (11 H 70), f. 0030v
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
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0030v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0030v, 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
Additional file 1: of Does the prehospital National Early Warning Score predict the short-term mortality of unselected emergency patients?
Creators: name: Hoikka, Marko
name: Silfvast, Tom
name: Ala-Kokko, Tero
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology

description: NEWS usage; calculation of NEW-score and definition of the clinical risk. (DOCX 137 kb)
Quiescent carbon in the CGM of high redshift radio galaxies
Creators: name: De Breuck, Carlos
Publisher: name: Zenodo
Year: 2019

description: The circum-galactic medium (CGM) is the location where galaxies directly interact with their environment through accretion and feedback events. These reservoirs can cover scales of several 100s of kpc, and are mostly studied in the optical through bright emission lines such as Lyman-alpha tracing their ionized gas. However, these optical/near-IR observations are likely missing an important part of the picture. I will present ALMA observations of the atomic carbon line [CI] in a sample of nine radio galaxies at redshifts 2 to 4.5. While some of these show broad [CI] lines up to 1000 km/s likely powered by the central AGN, we also find several examples of intriguingly narrow 50-120 km/s [CI] lines in the haloes of these massive galaxies. We compare these with our VLT/MUSE observations of the same galaxies, showing that the narrow [CI] gas detected by ALMA is tracing at least as much gas the ionized gas. Our [CI] detections reach beyond the regions where the radio jets have stirred up the gas kinematics, and therefore seem to trace the elusive CGM gas reservoirs from which these massive galaxies are forming. Future ALMA observations of other redshifted fine structure lines (e.g. [CII]158um, [NII]122/205, [OI]63/145um, [OIII]52/88um) should open up a new diagnostics of the physical conditions (density, ionization, metallicity) in the CGM at their epoch of formation.
Comment on ``Universal Spin-Flip Transition in Itinerant Antiferromagnets"
Creators: name: Dupuis, N.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: In a recent paper [Phys. Rev. Lett. 91, 117201 (2003)], it is argued that an itinerant antiferromagnet in an external magnetic field undergoes a spin-flip transition, in marked contrast with the behavior of a localized antiferromagnet: for a weak magnetic field, the magnetization is parallel to the field, and flips to the perpendicular configuration at a critical value of the field. In this Comment we show that these conclusions are incorrect. The canted state (not considered in the Letter) is the antiferromagnetic ground state of the system up to a critical value of the field where the normal state is restored, in qualitative agreement with the behavior of the magnetization in a localized antiferromagnet.
description: 1 page, 2 figures
Two extremely young objects in Barnard 1-b probed with the ALMA
Creators: name: Hirano, Naomi
Publisher: name: Zenodo
Year: 2019

description: Two extremely young protostars, B1-bN and B1-bS, have been observed with the Atacama Large Millimeter/submillimeter Array at an angular resolution of ~0.2". The high resolution data successfully revealed spatially compact C17O emission localized to B1-bN and B1-bS. The radii of the C17O emitting regions around B1-bN and B1-bS are ~0.25" (75 au) and ~0.5" (150 au), respectively. B1-bN shows a velocity gradient of ~7--8 m s-1 au-1 along the north-south direction, which is perpendicular to the outflow traced by the CH3OH. This velocity gradient in B1-bN is explained by the rotation around the central protostar with a mass of 0.03--0.04 M_sun. The outflow from B1-bN consists of the highly collimated blueshifted lobe extending to the west and spatially compact and misaligned redshifted lobe in the east. The radial velocity of the blueshifted lobe increases linearly as a function of distance from the central star, suggesting that the lobe was formed by the single explosive event that happened at ~1000 years ago. The outflow from B1-bS consists of three pairs of collimated lobes, each of which has similar velocity structure as that of the blueshifted lobe in B1-bN. The terminal velocities of the B1-bN and B1- bS outflow reaches ~9 km/s and ~8 km/s (without inclination correction), respectively, both of which are higher than that of the outflow from the first hydrostatic core. This indicates that both B1-bN and B1-bS have already experienced the second collapse.
Infrared L Band Observations of the Trapezium Cluster: A Census of Circumstellar Disks and Candidate Protostars
Creators: name: Lada, Charles J.
name: Muench, August A.
name: Haisch, Karl E.
name: Lada, Elizabeth A.
name: Alves, Joao F.
name: Tollestrup, Eric V.
name: Willner, S. P.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the results of a sensitive near-infrared JHKL imaging survey of the Trapezium cluster in Orion. We use the JHKL colors to obtain a census of infrared excess stars in the cluster. Of (391) stars brighter than 12th magnitude in the K and L bands, 80 +/- 7% are found to exhibit detectable infrared excess on the J-H, K-L color-color diagram. Examination of a subsample of 285 of these stars with published spectral types yields a slightly higher infrared excess fraction of 85%. We find that 97% of the optical proplyds in the cluster exhibit excess in the JHKL color-color diagram indicating that the most likely origin of the observed infrared excesses is from circumstellar disks. We interpret these results to indicate that the fraction of stars in the cluster with circumstellar disks is between 80-85%. Moreover, we find that the probability of finding an infrared excess/protoplanetary disk around a star is independent of stellar mass over essentially the entire range of the stellar mass function down to the hydrogen burning limit. We identify 78 stars in our sample characterized by K-L colors suggestive of deeply embedded protostellar objects. If even a modest fraction fraction (i.e., ~ 50%) of these objects are protostars, then star formation could be continuing in the molecular ridge at a rate comparable to that which produced the foreground Trapezium cluster.
description: 33 pages plus 3 separate color figures. For higher resolution color figures and a single file containing the entire paper, figures and tables see http://cfa-www.harvard.edu/~gmuench/thesis/clusters/TRAP/traplband.html Used AASTEX macros v 5.0. Paper will appear in December AJ
Charm quark effects on the strong coupling extracted from the static force
Creators: name: Cali, Salvatore
name: Knechtli, Francesco
name: Korzec, Tomasz
name: Panagopoulos, Haralambos
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We compute the fermionic contribution to the strong coupling $α_{qq}$ extracted from the static force in Lattice QCD up to order $g^4$ in perturbation theory. This allows us to subtract the leading fermionic lattice artifacts from recent determinations of $α_{qq}$ produced in simulations of two dynamical charm quarks. Moreover, by using a suitable parametrization of the $β_{qq}$-function, we can evaluate the charm loop effects on $α_{qq}$ in the continuum limit.
description: 8 pages, 2 figures; Proceedings of the 35th International Symposium on Lattice Field Theory, Granada, Spain
title: Histoire : tAzrAj
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
On the one-loop calculations with Reggeized quarks
Creators: name: Nefedov, Maxim
name: Saleev, Vladimir
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The technique of one-loop calculations for the processes involving Reggeized quarks is described in the framework of gauge invariant effective field theory for the Multi-Regge limit of QCD, which has been introduced by Lipatov and Vyazovsky. The rapidity divergences, associated with the terms enhanced by $\log (s)$, appear in the loop corrections in this formalism. The covariant procedure of regularization of rapidity divergences, preserving the gauge invariance of effective action is described. As an example application, the one-loop correction to the propagator of Reggeized quark and $γQ q$-scattering vertex are computed. Obtained results are used to construct the Regge limit of one-loop $γγ\to q\bar q$ amplitude. The cancellation of rapidity divergences and consistency of the effective field theory prediction with the full QCD result is demonstrated. The rapidity renormalization group within the effective field theory is discussed.
description: 11 pages, 2 figures
Direct Evidence for a Geometry-Dependent Dust Temperature in High-Redshift Galaxies
Creators: name: Burnham, Anne
Publisher: name: Zenodo
Year: 2019

description: The underlying distribution of galaxies' evolving dust SEDs (i.e. spectrum re-radiated by dust from rest-frame ~3 um - 3 mm) still remains relatively unconstrained due to a dearth of FIR/ (sub)mm data for large samples. It has been claimed in the literature that a galaxy's dust temperature — observed as the wavelength where the dust SED peaks (lambda_peak) — is traced most closely by its specific star-formation rate or parameterized 'distance' to the SFR-M_star relation (the galaxy 'main-sequence'). We present 0.12" resolved 870 um ALMA dust continuum observations of 7 dusty star-forming galaxies (DSFGs) chosen to have a large range of well- constrained luminosity-weighted dust temperatures (lambda_peak). They span redshifts z=1.4-4.6 and are drawn from the central deep portion of SCUBA-2 coverage in COSMOS with photometry drawn from Spitzer, Herschel, SCUBA-2, and ALMA. We also draw on similar resolution dust continuum maps of DSFGs from ALESS (Hodge et al. 2016) to expand the analysis sample. We constrain dust continuum morphology and the physical scales over which the dust radiates and compare those measurements to characteristics of the integrated SED. The effective radii (R_e) of these galaxies range from 1.6-7.7 kpc, and their morphology is well fit to a Gaussian profile (Sersic index n = 0.62). We confirm significant correlations of lambda_peak (or T_d ) with both L_IR (or SFR) and L_IR / R_e^2 (SFR surface density). Using a galaxy-scale Stefan-Boltzmann-type argument for the relationship between incident radiation heating dust in the ISM, we investigate the correlation between lambda_peak and L_IR / R_e^2. We find a value of the slope of this relation, eta = -0.22, which deviates from the theoretical value of -0.25 by 2.6 sigma. The correlations of lambda_peak with sSFR and distance from the main sequence are less significant; therefore, we conclude that the more fundamental tracer of galaxies' integrated dust temperatures are indeed their star-formation surface densities.
Recent Results from the SOFIA Airborne Observatory
Creators: name: Chambers, Edward
Publisher: name: Zenodo
Year: 2019

description: Half of the radiant energy in the Universe emerges in the mid- to far-infrared portion of the electromagnetic spectrum (wavelengths of ~10 to 300 microns). Yet, due to absorption by the Earth's lower atmosphere, mid- and far-infrared astronomy is nearly impossible from even the best ground-based sites. At its operating altitude of 12 km, SOFIA flies a 2.7 m diameter telescope above 99.9% of the atmosphere's absorbing water in a highly modified Boeing 747. SOFIA can therefore observe broad swaths of the infrared spectrum available to no other observatory. With its state-of-the-art suite of instruments, SOFIA performs broadband imaging, high-resolution spectroscopy, and polarimetry in the mid- and far-infrared to address fundamental astrophysical problems concerning the formation of stars and planets, the synthesis of biomolecules, and extreme environments in the Galactic Center and nearby galaxies. In this talk I will describe some of SOFIA's recent scientific achievements, including measurements of magnetic field directions in star-forming gas filaments, a luminous episode of enhanced mass accretion toward a young high-mass protostar, expansion of a gas "bubble" in Orion being driven by the wind from a high-mass star, and the detection of helium hydride (HeH+), the first molecule ever formed in the Universe. I will describe how SOFIA's new instrument HIRMES, to be deployed in 2021, will make fundamental measurements of water vapor and water ice in protoplanetary disks to advance our knowledge of how planets form. Finally, I will discuss the many synergies ALMA has with SOFIA.
title: Histoire : yufu yu mogui
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
title: ADCO, Cartulaire de Cîteaux pour les possessions d'Aloxe (XVe siècle), Cart. 182 (11 H 233), 105 folios, f. 0191
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2017
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
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: cartulaire
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de Cîteaux pour les possessions d'Aloxe (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 182 (11 H 233), 105 folios, f. 0191, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions d'Aloxe (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 182 (11 H 233), 105 folios, f. 0191, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
High-Pressure Synthesized Materials: a Chest of Treasure and Hints
Creators: name: Brazhkin, V. V.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The present review covers the production of new materials under high pressures. A primary limitation on the use of pressures higher than 1 GPa is a small volume and mass of a produced material. Therefore, despite an extremely wide range of new high-pressure synthesized substances with unique properties, synthesis on an commercial scale is applied up to now only to obtain superhard materials, this real treasure of today's industry. At the same time, high-pressure experiments often give material scientists a hint at what new intriguing substances can exist in principle. This is true for new superhard, semiconducting, magnetic, superconducting and optical materials already synthesized under pressure, and as well as for a large number of hypothetic new polymers from low-Z elements. Many of new materials, including the above polymers, may exist in the metastable form at normal pressure at sufficiently high temperatures.
description: 32 pages
Kleinian Geometry and the N=2 Superstring
Creators: name: Barrett, J.
name: Gibbons, G. W.
name: Perry, M. J.
name: Pope, C. N.
name: Ruback, P. J.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: This paper is devoted to the exploration of some of the geometrical issues raised by the $N=2$ superstring. We begin by reviewing the reasons that $β$-functions for the $N=2$ superstring require it to live in a four-dimensional self-dual spacetime of signature $(--++)$, together with some of the arguments as to why the only degree of freedom in the theory is that described by the gravitational field. We then move on to describe at length the geometry of flat space, and how a real version of twistor theory is relevant to it. We then describe some of the more complicated spacetimes that satisfy the $β$-function equations. Finally we speculate on the deeper significance of some of these spacetimes.
description: 30 pages, AMS-TeX
Cosmological-Model-Parameter Determination from Satellite-Acquired Type Ia and IIP Supernova Data
Creators: name: Podariu, Silviu
name: Nugent, Peter
name: Ratra, Bharat
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the constraints that satellite-acquired Type Ia and IIP supernova apparent magnitude versus redshift data will place on cosmological model parameters in models with and without a constant or time-variable cosmological constant $Λ$. High-quality data which could be acquired in the near future will result in tight constraints on these parameters. For example, if all other parameters of a spatially-flat model with a constant $Λ$ are known, the supernova data should constrain the non-relativistic matter density parameter $Ω_0$ to better than 1% (2%, 0.5%) at 1$σ$ with neutral (worst case, best case) assumptions about data quality.
description: 16 pages, 6 figures
The role of accretion and extended SiO emission in forming high mass protocluster NGC 6334-V
Creators: name: Aghababaei, Atefeh
Publisher: name: Zenodo
Year: 2019

description: Most stars form within the massive clumps which are embedded in the filamentary molecular clouds. Characterizing how the material is accreted from the filaments to the clusters, and from the clusters onto the cluster members is a long standing problem. We study observationally the formation of the massive protocluster NGC 6334-V embedded in filamentary cloud NGC6334 to investigate the manner of accretion using different molecular tracers. We used ALMA observations at 3 mm in continuum and different dense gas tracers like HCN and HCO+ isotopologues and reveal protocluster NGC 6334-V on small scale. Comparing the intermediate scale ALMA data with the large scale APEX data shows a clear correlation between both scales. In order to reliably identify the filaments, we applied DisPerse to the APEX and ALMA data. All identified filaments are converging to the center of the protocluster where a density cavity is located. The extended SiO is appeared on where the filaments converge in the central hubs. The SiO molecular emission reveals widespread and a shell-like morphology. The narrow lines on SiO spectrum tracing slow shocks are likely with the accretion process into the cores. These observations suggest that the filaments on small scale ALMA observations follow the same pattern as seen in large scale APEX observations and indicate how the gas falls from large scale NGC 6334 cloud into the small scale protocluster through distinctive converging flows. Moreover, the spectacular extended morphology of SiO with narrow Gaussian line profile explains the presence of low-velocity shock from colliding flows and outflow process together. However, based on our data the cloud-cloud collision is more dominant.