cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
[Local 5 collective agreements]
Creators: name: Association Of University And College Employees
Publisher: name: The University of British Columbia
Year: 2019

description: File contains Local 5 (College of New Caledonia) collective agreements: October 20, 1977 - October 31, 1978 (signed October 20, 1977); November 1, 1978 - October 31, 1980 (signed February 17, 1979); and November 1, 1980 - October 31, 1982 (signed April 21, 1981). File also contains copy of Local 5 by-laws received by union office on June 26, 1978.
[Local 2 constitution, by-laws, and agreements]
Creators: name: Association Of University And College Employees
Publisher: name: The University of British Columbia
Year: 2019

description: File contains the following booklets produced by AUCE Local 2: - "Articles of Agreement Between SFU and and AUCE Local 2: November 22, 1974 to November 21, 1976", - "Articles of Agreement Between SFU and and AUCE Local 2: November 22, 1976 to March 31, 1978" , - "Articles of Agreement Between SFU and and AUCE Local 2: April 1, 1978 to March 31, 1980", - "AUCE Provincial Constitution & By-Laws of Local #2 (SFU)", and - "AUCE Local Number Two By-Laws: as amended March 1977".
Starburst galaxies and structure in the submillimetre background towards the Hubble Deep Field
Creators: name: Peacock, J. A.
name: Rowan-Robinson, M.
name: Blain, A. W.
name: Dunlop, J. S.
name: Efstathiou, A.
name: Hughes, D. H.
name: Jenness, T.
name: Ivison, R. J.
name: Lawrence, A.
name: Longair, M. S.
name: Mann, R. G.
name: Oliver, S. J.
name: Serjeant, S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use an 850-micron SCUBA map of the HDF to study the dust properties of optically-selected starburst galaxies at high redshift. Although the 850-micron map does not allow detection of the majority of individual sources, we show that the galaxies with the highest UV star-formation rates are detected statistically, with a flux density of about S_{850}=0.2 mJy for an apparent UV star-formation rate of 1 h^{-2} msun yr^{-1}. This level of submillimetre output indicates that the total star-forming activity is on average a factor of approximately 6 times larger than the rate inferred from the UV output of these galaxies. The general population of optical starbursts is then predicted to contribute at least 25 per cent of the 850-micron background. We carry out a power-spectrum analysis of the map, which yields some evidence for angular clustering of the background source population, but at a level lower than that seen in Lyman-break galaxies. Together with other lines of argument, particularly from the NICMOS HDF data, this suggests that the 850-micron background originates over an extremely wide range of redshifts -- perhaps 1 < z < 6.
description: 12 Pages; MNRAS in press. Minor changes to match accepted version
Superconducting transition temperatures of pure vanadium and vanadium-titanium alloys in the presence of dynamical electronic correlations
Creators: name: Jones, D.
name: Östlin, A.
name: Weh, A.
name: Beiuseanu, F.
name: Eckern, U.
name: Vitos, L.
name: Chioncel, L.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Ordinary superconductors are widely assumed insensitive to small concentrations of random nonmagnetic impurities, whereas strong disorder suppresses superconductivity, ultimately leading to a superconductor-insulator transition. In between these limiting cases, a most fascinating regime may emerge where disorder enhances superconductivity. This effect is discussed here for the $β$-phase of vanadium-titanium alloys. Disorder is modeled using the coherent potential approximation while local electronic interactions are treated using dynamical mean-field theory. The McMillan formula is employed to estimate the superconducting transition temperature, showing a maximum at a Ti concentration of around $0.33$ for a local Coulomb interaction $U$ in the range of $2$ to $3$ eV. Our calculations quantitatively agree with the experimentally observed concentration dependent increase of $T_c$, and its maximal value of about $20\%$.
The Evaluation Gap in Astronomy -- Explained through a Rational Choice Framework
Creators: name: Heuritsch, Julia
Publisher: name: arXiv
Year: 2021
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The concept of evaluation gaps captures potential discrepancies between what researchers value about their research, in particular research quality, and what metrics measure. The existence of evaluation gaps can give rise to questions about the relationship between intrinsic and extrinsic motivations to perform research, i.e. how field-specific notions of quality compete with notions captured via evaluation metrics, and consequently how researchers manage the balancing act between intrinsic values and requirements of evaluation procedures. This study analyses the evaluation gap from a rational choice point of view for the case of observational astronomers, based on a literature review and 19 semi-structured interviews with international astronomers. By taking a close look at the role of institutional norms and different forms of capital - such as funding, publication rates and granted telescope time - at play in astronomy, light can be shed on the workings of the balance act and its consequences on research quality in astronomy. We find that astronomers experience an anomie; they want to follow their intrinsic motivation to pursue science in order to push knowledge forward, while at the same time following their extrinsic motivation to comply with institutional norms. The balance act is the art of serving performance indicators in order to stay in academia, while at the same time compromising research quality as little as possible. Gaming strategies shall give the appearance of compliance, while institutionalised means how to achieve a good bibliometric record are used in innovative ways, such as salami slicing or going for easy publications. This leads to an overall decrease in research quality.
description: This is a Preprint written in the context of science studies. The author is a member of the "Reflexive Metrics" junior research group (https://www.sowi.hu-berlin.de/de/lehrbereiche/wissenschaftsforschung/Forschung/reflexivemetrics)
title: 01_0553
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Fermion Masses in Superstring Theory
Creators: name: Antoniadis, I.
name: Taylor, T. R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We give a model-independent discussion of fermion masses in four-dimensional heterotic superstring theories. We discuss the tree level contributions and quantum corrections, including one-loop threshold effects and masses generated as a result of non-perturbative supersymmetry breaking. We also point out that superstring models give rise to a generic $μ$-term in the effective low energy Lagrangian.
description: 13 pages, latex. Based on talks presented at the Spring Workshop on String Theory, ICTP, Trieste, 11-22 April 1994, and at the Joint U.S.-Polish Workshop on Physics from Planck Scale to Electroweak Scale, Warsaw, Poland, 21-24 September 1994
The SMC X-ray transient XTE J0111.2-7317 : a Be/X-ray binary in a SNR?
Creators: name: Coe, M. J.
name: Haigh, N. J.
name: Reig, P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report observations which confirm the identity of the optical/IR counterpart to the Rossi X-ray Timing Explorer transient source XTE J0111.2-7317. The counterpart is suggested to be a B0-B2 star (luminosity class III--V) showing an IR excess and strong Balmer emission lines. The distance derived from reddening and systemic velocity measurements puts the source in the SMC. Unusually, the source exhibits an extended asymetric H alpha structure.
description: 5 pages, 3 figs, accepted by MNRAS
Fluctuation conductivity due to the preformed local pairs
Creators: name: Domanski, T.
name: Baranska, M.
name: Solovjov, A. L.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We investigate the properties of a system where the itinerant electrons coexist and interact with the preformed local pairs. Using the nonperturbative continuous unitary transformation technique we show that Andreev-type scattering between these charge carriers gives rise to the enhanced diamagnetic response and is accompanied by appearance of the Drude peak inside the pseudogap regime ω<2Δ_{pg}. Both thes effects are caused above the transition temperature T_c by the short-range superconducting correlations. In fact, the residual diamagnetism has been detected by the torque magnetometry in the lanthanum and bismuth cuprate superconductors at temperatures up to ~ 1.5T_c. In this work we show how the superconducting correlations can be observed in the a.c. and d.c. conductivity.
description: 7 pages, 6 figures
Renormalization of the next-to-leading-power $γγ\to h $ and $gg\to h$ soft quark functions
Creators: name: Beneke, Martin
name: Ji, Yao
name: Wang, Xing
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We calculate directly in position space the one-loop renormalization kernels of the soft operators $O_γ$ and $O_g$ that appear in the soft-quark contributions to, respectively, the subleading-power $γγ\to h$ and $gg\to h$ form factors mediated by the $b$-quark. We present an IR/rapidity divergence-free definition for $O_g$ and demonstrate that with a correspondent definition of the collinear function, a consistent factorization theorem is recovered. Using conformal symmetry techniques, we establish a relation between the evolution kernels of the leading-twist heavy-light light-ray operator, whose matrix element defines the $B$-meson light-cone distribution amplitude (LCDA), and $O_γ$ to all orders in perturbation theory. Application of this relation allows us to bootstrap the kernel of $O_γ$ to the two-loop level. We construct an ansatz for the kernel of $O_g$ at higher orders. We test this ansatz against the consistency requirement at two-loop and find they differ only by a particular constant.
description: journal version
General correspondence outgoing (3 of 5)
Creators: name: Association Of University And College Employees
Publisher: name: The University of British Columbia
Year: 2019

description: File contains AUCE outgoing correspondence dated April 23, 1981 to June 23, 1981. Topics include parking, AUCE membership and representatives, union dues, membership meetings, leaves of absence, cooperation with other unions, contract negotiations, tax payment, women's rights, grievances with UBC, building inspections, publication orders, arbitration, legal representation, by-law and constitution amendments, job classification, women in the workplace, and financial assistance.
High-efficiency, long-pulse operation of MW-level dual-frequency gyrotron, 84/126GHz, for the TCV Tokamak
Creators: name: Alberti, Stefano
name: Avramidis, Konstantinos A.
name: Bin, William
name: Bertinetti, Andrea
name: Dubray, Jérémie
name: Fasel, Damien
name: Garavaglia, Saul
name: Genoud, Jérémy
name: Goodman, Timothy
name: Hogge, J. P.
name: Isoz, Pierre François
name: Lavanchy, Pierre
name: Legrand, François
name: Marletaz, Blaise
name: Masur, Jonathan
name: Moro, Alessandro
name: Pagonakis, Ioannis Gr.
name: Silva, Miguel
name: Siravo, Ugo
name: Toussaint, Matthieu
Publisher: name: Karlsruhe
Year: 2019

description: The first unit of the dual-frequency gyrotron, 84126GHz/1MW/2s, for the upgrade of the TCV ECH system has been delivered and is presently being commissioned. During a first phase, long-pulse operation (TRF gt 0.5 mathrm{s}) has been achieved and powers in excess of 0.93MW/1.1s and 1MW/1.2s have been measured in the evacuated RF-load at the two frequencies, 84GHz (TE {17,5} mode) and 126GHz (TE {26,7} mode), respectively. Considering the different rf losses in the experimental setup, the power level generated in the gyrotron cavity is in excess of 1.1MW and 1.2MW, with a corresponding electronic efficiency of 35% and 36%. These values are in excellent agreement with the design parameters and would likely lead to a gyrotron total efficiency higher than 50% in case of implementation of a depressed collector. The gyrotron behavior is remarkably reliable and robust with the pulse length extension to 2s presently only limited by external auxiliary systems.
Anne Moody’s Final Resting Place: Family Buries Her Ashes Beside her Mother in Mount Pleasant Missionary Baptist Church Cemetery
Creators: name: Barnes, Roscoe
Publisher: name: figshare
Year: 2018
Subjects: subject: 210304 Biography
subject: FOS: History and archaeology
subject: Gender studies
subject: History
subject: 210399 Historical Studies not elsewhere classified
subject: 210202 Heritage and Cultural Conservation
subject: FOS: Media and communications
subject: Literature
subject: Religious Studies

description: Copyright (c) 2018 by Roscoe Barnes III
#AnneMoody
This blog post presents a news report on the second memorial service held for Anne Moody during which her ashes were buried beside her mother in the Mount Pleasant Missionary Baptist Church Cemetery in Centreville, Miss. The service was held on Saturday, July 7, 2018. Moody, a civil rights pioneer and author of Coming of Age in Mississippi, died on Feb. 5, 2015, at the age of 74. Her first memorial service was held on Saturday, Feb. 14, 2015, in Gloster, Miss. Her family, who organized the July burial, said it was time to bring her home. The Rev. LeReginald Jones officiated the service. He is the assistant pastor of Mount Pleasant.
For more information, visit the Anne Moody page at:
http://roscoereporting.blogspot.com/p/anne-moody.html?m=1
#ComingOfAgeinMississippi
Atmospheric Neutrino Problem in Maximally-Mixed Three Generations of Neutrinos
Creators: name: Giunti, C.
name: Kim, C. W.
name: Kim, J. D.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Motivated by the indication that both the atmospheric and the solar neutrino puzzles may simultaneously be solved by (vacuum as well as matter-induced resonant) oscillations of two generations of neutrinos with large mixing, we have analyzed the data on the atmospheric and solar neutrinos assuming that all {\it three} neutrinos are maximally mixed. It is shown that the values of $ Δm^2 $ obtained from the two-generation analyses are still valid even in the three-generation scheme, i.e. the two puzzles can be solved simultaneously if $ Δm_{31}^2 \simeq 10^{-2} \, \mathrm{eV}^2 $ for the atmospheric neutrinos and $ Δm_{21}^2 \simeq 10^{-10} \, \mathrm{eV}^2 $ for solar neutrinos in the maximally mixed three-generation scheme.
description: Revtex file, 11 pages + 3 figures (included). The postscript file of text and figures is available at ftp://toxd01.to.infn.it/pub/giunti/1994/dftt-54-94/dftt-54-94.ps.Z
Space-time statistics of 2D soliton gas in shallow water studied by stereoscopic surface mapping
Creators: name: Leduque, Thibault
name: Barthélemy, Eric
name: Michallet, Hervé
name: Sommeria, Joël
name: Mordant, Nicolas
Publisher: name: arXiv
Year: 2024
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Pattern Formation and Solitons (nlin.PS)
subject: FOS: Physical sciences

description: We describe laboratory experiments in a 2D wave tank that aim at building up and monitor 2D shallow water soliton gas. The water surface elevation is obtained over a large ($\sim 100\,\text{m}^2$) domain, with centimetre-resolution, by stereoscopic vision using two cameras. Floating particles are seeded to get surface texture and determine the wave field by image correlation. With this set-up, soliton propagation and multiple interactions can be measured with a previously unreachable level of detail. The propagation of an oblique soliton is analysed, the amplitude decay and local incidence are compared to analytical predictions. We further present two cases of 2D soliton gas, emerging from multiple line solitons with random incidence ($|θ|<30^\circ$) and from irregular random waves forced with a {\sc jonswap} spectrum ($|θ|<45^\circ$). To our knowledge, those are the first observations of random 2D soliton gas for gravity waves. In both cases Mach reflections and Mach expansions result in solitons that mainly propagate in directions perpendicular to the wave-makers.
description: Accepted for publication in Experiments in Fluids
Gamma-Ray Burst Arrival-Time Localizations: Simultaneous Observations by Ulysses, Pioneer Venus Orbiter, SIGMA, WATCH, and PHEBUS
Creators: name: Hurley, K.
name: Laros, J.
name: Brandt, S.
name: Fenimore, E.
name: Klebesadel, R.
name: Terrell, J.
name: Cline, T.
name: Barat, C.
name: Boer, M.
name: Dezalay, J. -P.
name: Lund, N.
name: Claret, A.
name: Paul, J.
name: Castro-Tirado, A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Between the launch of the Ulysses spacecraft in 1990 October and the entry of Pioneer Venus Orbiter (PVO) into the atmosphere of Venus in 1992 October, concurrent coverage by Ulysses, PVO, the WATCH experiments aboard the Granat and EURECA spacecraft, and the SIGMA and PHEBUS experiments aboard the Granat spacecraft was obtained for numerous gamma-ray bursts. 15 of them were detected by 3 or more instruments on spacecraft separated by distances of several AU, and could therefore be accurately localized by triangulation. In some cases independent, accurate locations were obtained by SIGMA and/or WATCH. We present these localizations, which range in area from 0.9 to 530 arcminutes$^2$.
description: Accepted for publication in the Astrophysical Journal Supplements, May 2000
New Corrections of Order $α^6$ to $s$-Levels of Two-Body Systems
Creators: name: Eides, Michael I.
name: Grotch, Howard
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: New corrections to the energy of $S$-levels of positronium of order $mα^6$ which are as large as several hundred kilohertz are obtained. A new recoil correction of order $α(Zα)^5(m/M)m$ to the Lamb shift in hydrogen is calculated. This correction turns out to be too small from the phenomenological point of view.
description: 9 pages, LaTeX, 2 figures; Subtraction procedure is improved in the new version, two of the numerical results have changed
A Bio-inspired Redundant Sensing Architecture
Creators: name: Nguyen, Anh Tuan
name: Xu, Jian
name: Yang, Zhi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Neural and Evolutionary Computing (cs.NE)
subject: Information Theory (cs.IT)
subject: Signal Processing (eess.SP)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Sensing is the process of deriving signals from the environment that allows artificial systems to interact with the physical world. The Shannon theorem specifies the maximum rate at which information can be acquired. However, this upper bound is hard to achieve in many man-made systems. The biological visual systems, on the other hand, have highly efficient signal representation and processing mechanisms that allow precise sensing. In this work, we argue that redundancy is one of the critical characteristics for such superior performance. We show architectural advantages by utilizing redundant sensing, including correction of mismatch error and significant precision enhancement. For a proof-of-concept demonstration, we have designed a heuristic-based analog-to-digital converter - a zero-dimensional quantizer. Through Monte Carlo simulation with the error probabilistic distribution as a priori, the performance approaching the Shannon limit is feasible. In actual measurements without knowing the error distribution, we observe at least 2-bit extra precision. The results may also help explain biological processes including the dominance of binocular vision, the functional roles of the fixational eye movements, and the structural mechanisms allowing hyperacuity.
Holographic Mutual and Tripartite Information in a Symmetry Breaking Quench
Creators: name: Asadi, M.
name: Ali-Akbari, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the time evolution of holographic mutual and tripartite information for a zero temperature $CFT$, derives to a non-relativistic thermal Lifshitz field theory by a quantum quench. We observe that the symmetry breaking does not play any role in the phase space, phase of parameters of sub-systems, and the length of disentangling transition. Nevertheless, mutual and tripartite information indeed depend on the rate of symmetry breaking. We also find that for large enough values of $δt$ the quantity $t_{eq}δt^{-1}$, where $δt$ and $t_{eq}$ are injection time and equilibration time respectively, behaves universally, $i.e.$ its value is independent of length of separation between sub-systems. We also show that tripartite information is always non-positive during the process indicates that mutual information is monogamous.
description: 15 pages, 6 figures
Additional file 1 of Evaluation of cell-cell interaction methods by integrating single-cell RNA sequencing data with spatial information
Creators: name: Liu, Zhaoyang
name: Sun, Dongqing
name: Wang, Chenfei
Publisher: name: figshare
Year: 2022
Subjects: Biophysics
Biochemistry
Cell Biology
Molecular Biology
Environmental Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Information Systems not elsewhere classified
Mathematical Sciences not elsewhere classified
Cancer
Hematology

description: Additional file 1: Figure S1-S9. It includes all the supplementary figures and legends.
Experimental Cosmic Statistics I: Variance
Creators: name: Colombi, Stéphane
name: Szapudi, István
name: Jenkins, Adrian
name: Colberg, Jörg
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Counts-in-cells are measured in the $τ$CDM Virgo Hubble Volume simulation. This large N-body experiment has 10^9 particles in a cubic box of size 2000 h^{-1} Mpc. The unprecedented combination of size and resolution allows for the first time a realistic numerical analysis of the cosmic errors and cosmic correlations of statistics related to counts-in-cells measurements, such as the probability distribution function P_N itself, its factorial moments F_k and the related cumulants $\xiav$ and S_N's. These statistics are extracted from the whole simulation cube, as well as from 4096 sub-cubes of size 125 h^{-1}Mpc, each representing a virtual random realization of the local universe. The measurements and their scatter over the sub-volumes are compared to the theoretical predictions of Colombi, Bouchet & Schaeffer (1995) for P_0, and of Szapudi & Colombi (1996, SC) and Szapudi, Colombi & Bernardeau (1999a, SCB) for the factorial moments and the cumulants. The general behavior of experimental variance and cross-correlations as functions of scale and order is well described by theoretical predictions, with a few percent accuracy in the weakly non-linear regime for the cosmic error on factorial moments. (... more in paper >...)
description: latex, 16 pages, 11 postscript figures. Accepted for publication in MNRAS
Additional file 2: of CsINV5, a tea vacuolar invertase gene enhances cold tolerance in transgenic Arabidopsis
Creators: name: Qian, Wenjun
name: Xiao, Bin
name: Wang, Lu
name: Hao, Xinyuan
name: Yue, Chuan
name: Cao, Hongli
name: Wang, Yuchun
name: Li, Nana
name: Yu, Youben
name: Zeng, Jianming
name: Yang, Yajun
name: Wang, Xinchao
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Neuroscience
subject: Evolutionary Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: Mental Health
subject: Plant Biology
subject: Virology

description: S1. The genome DNA sequence of CsINV5. 1154Â bp promoter sequence and 7 exons have been highlighted: (i) stress signaling (ARE, fully outlined in red; HSE, double outlined in red; TC-rich repeats, dot outlined in red; LTR, viridity highlighted; MYC, viridescence highlighted); (ii) light signaling (MRE, navy highlighted; I BOX, violet highlighted; L BOX, pink highlighted; SP1, underlined); (iii) Hormones signaling (ERE, blue highlighted; TCA-element, green highlighted); (iv) sugar repression (SRE, highlighted in deep yellow) and activation (WBOXHVISO1, highlighted in gray). The CAAT-box and TATA-box are yellow highlighted. PCR primer sequences highlighted in bold and italic. The exons were showed by red font. (DOCX 32 kb)
title: ADCO, Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402) (11 H 1160), f. 00307
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2017
name: Petot, Frédéric
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: comptes
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160), f. 00307, 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
Semileptonic Decays of Heavy Tetraquarks
Creators: name: Chow, Chi-Keung
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: There exist heavy tetraquark states $QQ \bar q \bar q$ in the heavy quark limit. These states are stable with respect to strong interactions and hence must decay weakly. It is shown that the semileptonic decay depends on a single Isgur--Wise form factor, which can be expressed in term of the Isgur--Wise form factors which govern the semileptonic decays of the $Qqq$ and $QQq$ baryons.
description: 7 pages in REVTeX, no figures
Data-driven modeling of the regular and chaotic dynamics of an inverted flag from experiments
Creators: name: Xu, Zhenwei
name: Kaszás, Bálint
name: Cenedese, Mattia
name: Berti, Giovanni
name: Coletti, Filippo
name: Haller, George
Publisher: name: arXiv
Year: 2024
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We use video footage of a water tunnel experiment to construct a two-dimensional reduced-order model of the flapping dynamics of an inverted flag in uniform flow. The model is obtained as the reduced dynamics on an attracting spectral submanifold (SSM) that emanates from the two slowest modes of the unstable fixed point of the flag. Beyond an unstable fixed point and a limit cycle expected from observations, our SSM-reduced model also confirms the existence of two unstable fixed points for the flag, which were found by previous studies. Importantly, the model correctly reconstructs the dynamics from a small number of general trajectories and no further information on the system. In the chaotic flapping regime, we construct a 4D SSM-reduced model that captures the system's chaotic attractor.
The Arches cluster revisited: II. A massive eclipsing spectroscopic binary in the Arches cluster
Creators: name: Lohr, M. E.
name: Clark, J. S.
name: Najarro, F.
name: Patrick, L. R.
name: Crowther, P. A.
name: Evans, C. J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have carried out a spectroscopic variability survey of some of the most massive stars in the Arches cluster, using K-band observations obtained with SINFONI on the VLT. One target, F2, exhibits substantial changes in radial velocity; in combination with new KMOS and archival SINFONI spectra, its primary component is found to undergo radial velocity variation with a period of 10.483+/-0.002 d and an amplitude of ~350 km/s. A secondary radial velocity curve is also marginally detectable. We reanalyse archival NAOS-CONICA photometric survey data in combination with our radial velocity results to confirm this object as an eclipsing SB2 system, and the first binary identified in the Arches. We model it as consisting of an 82+/-12 M_sun WN8-9h primary and a 60+/-8 M_sun O5-6 Ia+ secondary, and as having a slightly eccentric orbit, implying an evolutionary stage prior to strong binary interaction. As one of four X-ray bright Arches sources previously proposed as colliding-wind massive binaries, it may be only the first of several binaries to be discovered in this cluster, presenting potential challenges to recent models for the Arches' age and composition. It also appears to be one of the most massive binaries detected to date; the primary's calculated initial mass of >~120 M_sun would arguably make this the most massive binary known in the Galaxy.
description: 15 pages, 18 figures, accepted for publication in Astronomy & Astrophysics. Paper II in a series; for Paper I see arXiv:1803.09567
Signature of the atmospheric asymmetries of hot and ultra-hot Jupiters in lightcurves
Creators: name: Falco, Aurélien
name: Leconte, Jérémy
name: Mechineau, Alexandre
name: Pluriel, William
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: With the new generation of space telescopes such as the James Webb Space Telescope (JWST), it is possible to better characterize the atmospheres of exoplanets. The atmospheres of Hot and Ultra Hot Jupiters are highly heterogeneous and asymmetrical. The difference between the temperatures on the day-side and the night-side is especially extreme in the case of Ultra Hot Jupiters. We introduce a new tool to compute synthetic lightcurves from 3D GCM simulations, developed in the Pytmosph3R framework. We show how rotation induces a variation of the flux during the transit that is a source of information on the chemical and thermal distribution of the atmosphere. We find that the day-night gradient linked to Ultra Hot Jupiters has an effect close to the stellar limb-darkening, but opposite to tidal deformation. We confirm the impact of the atmospheric and chemical distribution on variations of the central transit time, though the variations found are smaller than that of available observational data, which could indicate that the east-west asymmetries are underestimated, due to the chemistry or clouds.
description: Accepted for publication in A&A (16th Feb.) 17 pages, 18 figures + 7 in appendices
A Transformer-Based Approach for Smart Invocation of Automatic Code Completion
Creators: name: de Moor, Aral
name: van Deursen, Arie
name: Izadi, Maliheh
Publisher: name: arXiv
Year: 2024
Subjects: subject: Software Engineering (cs.SE)
subject: Artificial Intelligence (cs.AI)
subject: Human-Computer Interaction (cs.HC)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Transformer-based language models are highly effective for code completion, with much research dedicated to enhancing the content of these completions. Despite their effectiveness, these models come with high operational costs and can be intrusive, especially when they suggest too often and interrupt developers who are concentrating on their work. Current research largely overlooks how these models interact with developers in practice and neglects to address when a developer should receive completion suggestions. To tackle this issue, we developed a machine learning model that can accurately predict when to invoke a code completion tool given the code context and available telemetry data.
 To do so, we collect a dataset of 200k developer interactions with our cross-IDE code completion plugin and train several invocation filtering models. Our results indicate that our small-scale transformer model significantly outperforms the baseline while maintaining low enough latency. We further explore the search space for integrating additional telemetry data into a pre-trained transformer directly and obtain promising results. To further demonstrate our approach's practical potential, we deployed the model in an online environment with 34 developers and provided real-world insights based on 74k actual invocations.
description: 10 pages, 3 figures; Accepted at FSE AIWARE'24
Dynamical dark energy in light of cosmic distance measurements II: a study using current observations
Creators: name: Wang, Xiaoma
name: Gu, Gan
name: Mu, Xiaoyong
name: Yuan, Shuo
name: Zhao, Gong-Bo
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We extract key information of dark energy from current observations of BAO, OHD and $H_0$, and find hints of dynamical behaviour of dark energy. In particular, a dynamical dark energy model whose equation of state crosses $-1$ is favoured by observations. We also find that the Universe has started accelerating at a lower redshift than expected.
description: 10 pages, 4 figures; version accepted to RAA
Subelliptic sharp Gårding inequality on compact Lie groups
Creators: name: Cardona, Duván
name: Federico, Serena
name: Ruzhansky, Michael
Publisher: name: arXiv
Year: 2021
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: In this work we establish a subelliptic sharp Gårding inequality on compact Lie groups for pseudo-differential operators with symbols belonging to global subelliptic Hörmander classes. In order for the inequality to hold we require the global matrix-valued symbol to satisfy the suitable classical nonnegativity condition in our setting. Our result extends to $\mathscr{S}^m_{ρ,δ}(G)$-classes, $0\leq δ<ρ$, the one in [26] about the validity of the sharp Gårding inequality for the class $\mathscr{S}^m_{1,0}(G)$. We remark that the result we prove here is already new and sharp in the case of the torus.
Magnetic Field Limits on SGRs
Creators: name: Rothschild, R. E.
name: Marsden, D.
name: Lingenfelter, R. E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We measure the period and spin-down rate for SGR 1900+14 during the quiescient period two years before the recent interval of renewed burst activity. We find that the spin-down rate doubled during the burst activity which is inconsistent with both mangetic dipole driven spin down and a magnetic field energy source for the bursts. We also show that SGRs 1900+14 and 1806-20 have braking indices of $\sim$1 which indicate that the spin-down is due to wind torques and not magnetic dipole radiation. We further show that a combination of dipole radiation, and wind luminosity, coupled with estimated ages and present spin parameters, imply that the magnetic fields of SGRs 1900+14 and 1806-20 are less than the critical field of 4$\times10^{13}$ G and that the efficiency for conversion of wind luminosity to x-ray luminosity is <2%.
description: 5 pages, 2 figures submitted to 5th Huntsville GRB Symposium proceedings
Spherical curves whose curvature depends on distance to a great circle
Creators: name: Castro, Ildefonso
name: Castro-Infantes, Ildefonso
name: Castro-Infantes, Jesús
Publisher: name: arXiv
Year: 2021
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 53A04 (Primary) 74H05 (Secondary)

description: Motivated by a problem posed by David A. Singer in 1999 and by the elastic spherical curves, we study the spherical curves whose curvature is expressed in terms of the distance to a great circle (or from a point). By introducing the notion of spherical angular momentum, we provide new characterizations of some well known curves, like the mentioned elastic curves, spherical catenaries, loxodromic-type spherical curves, the Viviani's curve, and the spherical Archimedean spirals curves. Furthermore, we show that they may be obtained as critical points of some energy curvature functionals. We also find out several new families of spherical curves whose intrinsic equations are expressed in terms of elementary functions or Jacobi elliptic functions, and we are able to get arc length parametrizations of them.
description: 22 pages, 11 figures
Experimental Cosmic Statistics II: Distribution
Creators: name: Szapudi, István
name: Colombi, Stéphane
name: Jenkins, Adrian
name: Colberg, Jörg
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Colombi et al. 1999 (paper I) investigated the counts-in-cells statistics and their respective errors in the $τ$CDM Virgo Hubble Volume simulation. This extremely large $N$-body experiment also allows a numerical investigation of the {\em cosmic distribution function}, $Υ(\tA)$ itself for the first time. For a statistic $A$, $Υ(\tA)$ is the probability density of measuring the value $\tA$ in a finite galaxy catalog. $Υ$ was evaluated for the distribution of counts-in-cells, $P_N$, the factorial moments, $F_k$, and the cumulants, $\xiav$ and $S_N$'s, using the same subsamples as paper I. While paper I concentrated on the first two moments of $Υ$, i.e. the mean, the cosmic error and the cross-correlations, here the function $Υ$ is studied in its full generality, including a preliminary analysis of joint distributions $Υ(\tA,\tB)$. The most significant, and reassuring result for the analyses of future galaxy data is that the cosmic distribution function is nearly Gaussian provided its variance is small. A good practical criterion for the relative cosmic error is that $ΔA/A \la 0.2$. This means that for accurate measurements, the theory of the cosmic errors, presented by Szapudi & Colombi (1996) and Szapudi, Colombi & Bernardeau (1999), and confirmed empirically by paper I, is sufficient for a full statistical description and thus for a maximum likelihood rating of models. As the cosmic error increases, the cosmic distribution function $Υ$ becomes increasingly skewed and is well described by a generalization of the lognormal distribution. The cosmic skewness is introduced as an additional free parameter. (...more in paper...)
description: Latex, 11 pages, 8 postscript figures. Accepted for pulication in MNRAS
AUCE Provincial Constitution, policies, procedures and rules of order governing Convention as amended June 1981 (1 of 2)
Creators: name: Association Of University And College Employees
Publisher: name: The University of British Columbia
Year: 2019

description: File contains a copy of the AUCE Provincial constitution (amended June 1981), a copy of the "Rules of Order Governing AUCE Convention", and a copy of the Provincial's "Policies and Procedures" (amended June 1981).
Probability distribution of substituted Titanium in RT12 (R = Nd, Sm, T = Fe, Co) structures
Creators: name: Skelland, Connor
name: Ostler, Thomas
name: Westland, Samuel
name: Evans, Richard
name: Chantrell, Roy
name: Yano, Masao
name: Shoji, Tetsuya
name: Manabe, Akira
name: Kato, Akira
name: Winklhofer, Michael
name: Zimanyi, Gergely
name: Fischbacher, Johannes
name: Schrefl, Thomas
name: Hrkac, Gino
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We investigated the atomic fill site probability distributions across supercell structures of RT12-xTi (R=Nd, Sm, T=Fe, Co). We use a combined molecular dynamics and Boltzmann distribution approach to extrapolate the probability distributions for Ti substitution from lower to higher temperatures with an equilibrium condition to assess how temperature affects the predictability of the structures fill path. It was found that the Nd and Sm based Fe systems have the highest filling probability path at lower temperatures but the cohesive energy change due to Ti substitution in Sm and Nd based crystals indicates that a more stable system could be achieved with a combination Co and Fe in the transition metal site.
description: 5 pages, 4 figures, 2 tables
Measuring angular diameters of extended sources
Creators: name: van Hoof, P. A. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: When measuring diameters of partially resolved sources often a technique called gaussian deconvolution is used. This technique yields a gaussian diameter which subsequently has to be multiplied with a conversion factor to obtain the true angular diameter of the source. This conversion factor is a function of the FWHM of the beam or point spread function and also depends on the intrinsic surface brightness distribution of the source. In this paper conversion factors are presented for a number of simple geometries: a circular constant surface brightness disk and a spherical constant emissivity shell, using a range of values for the inner radius. Also more realistic geometries are studied, based on a spherically symmetric photo-ionization model of a planetary nebula. This enables a study of optical depth effects, a comparison between images in various emission lines and the use of power law density distributions. It is found that the conversion factor depends quite critically on the intrinsic surface brightness distribution, which is usually unknown. The uncertainty is particularly large if extended regions of low surface brightness are present in the nebula. In such cases the use of gaussian or second moment deconvolution is not recommended. As an alternative, a new algorithm is presented which allows the determination of the intrinsic FWHM of the source using only the observed surface brightness distribution and the FWHM of the beam. Tests show that this implicit deconvolution method works well in realistic conditions, even when the signal-to-noise is low, provided that the beam size is less than roughly 2/3 of the observed FWHM and the beam profile can be approximated by a gaussian.
description: 11 pages, 7 figures, accepted for publication in MNRAS
Chang Palais-Smale condition and global inversion
Creators: name: Gutú, Olivia
Publisher: name: arXiv
Year: 2018
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 46T20

description: Let f be local diffeomorphism between real Banach spaces. We prove that if the locally Lipschitz functional F(x)=1/2|f(x)-y|^2 satisfies the Chang Palais-Smale condition for all y in the target space of f, then f is a norm-coercive global diffeomorphism. We also give a version of this fact for a weighted Chang Palais-Smale condition. Finally, we study the relationship of this criterion to some classical global inversion conditions.
description: 10 pages
THE USE OF SPECIFIC PROMPTS TO ENHANCE EFL WRITING SKILLS
Creators: name: Akhrorova, Munisakhon
Publisher: name: Zenodo
Year: 2025

description: This study examines the role of specific prompts in enhancing EFL learners’ writing skills. Writing is often considered one of the most challenging aspects of language acquisition, especially for learners who lack motivation or struggle with idea generation. Specific prompts provide structured guidance, helping students organize their thoughts and develop coherent, well-structured texts. The study explores various types of prompts, such as narrative, argumentative, and descriptive, and their impact on fluency, accuracy, and creativity in writing. By analyzing students’ written outputs and conducting qualitative interviews, the research identifies effective prompt-based techniques that foster critical thinking and linguistic competence in EFL learners.
Ultra-High Energy Cosmic Rays from Young Neutron Star Winds
Creators: name: Blasi, P.
name: Epstein, R. I.
name: Olinto, A. V.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The long-held notion that the highest-energy cosmic rays are of distant extragalactic origin is challenged by observations that events above $\sim 10^{20}$ eV do not exhibit the expected high-energy cutoff from photopion production off the cosmic microwave background. We suggest that these unexpected ultra-high-energy events are due to iron nuclei accelerated from young strongly magnetized neutron stars through relativistic MHD winds. We find that neutron stars whose initial spin periods are shorter than $\sim 4 (B_S/10^{13}{\rm G})^{1/2}$ ms, where $B_S$ is the surface magnetic field, can accelerate iron cosmic rays to greater than $\sim 10^{20}$ eV. These ions can pass through the remnant of the supernova explosion that produced the neutron star without suffering significant spallation reactions. For plausible models of the Galactic magnetic field, the trajectories of the iron ions curve sufficiently to be consistent with the observed arrival directions of the highest energy events.
description: 11 pages, 1 figure, replaced with revised version, some references added