cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Length Functions and the Dimension of Points in Self-Similar Fractal Trees
Creators: name: Porter, Christopher P.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Logic (math.LO)
subject: Information Theory (cs.IT)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences

description: In this paper, we study the effective dimension of points in infinite fractal trees generated recursively by a finite tree over some alphabet. Using unequal costs coding, we associate a length function with each such fractal tree and show that the channel capacity of the length function is equal to the similarity dimension of the fractal tree (up to a multiplicative constant determined by the size of the alphabet over which our tree is defined). Using this result, we derive formulas for calculating the effective dimension and strong effective dimension of points in fractal trees, establishing analogues of several results due to Lutz and Mayordomo, who studied the effective dimension of points in self-similar fractals in Euclidean space. Lastly, we explore the connections between the channel capacity of a length function derived from a finite tree and the measure of maximum entropy on a related directed multigraph that encodes the structure of our tree, drawing on work by Abram and Lagarias on path sets, where a path set is a generalization of the notion of a sofic shift.
Planetary Nebulae in the Circumnuclear Region of M31: A Spectroscopic Sample
Creators: name: Li, Anqi
name: Li, Zhiyuan
name: Dong, Hui
name: Fang, Xuan
name: Xu, Xiaojie
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Planetary nebulae (PNe) are an important tool for studying the dynamics and chemical evolution of galaxies in the Local Universe, given their characteristic, bright emission line spectra. The Andromeda Galaxy (M31) provides a unique laboratory for studying PNe in the circumnuclear region, thanks to its proximity and almost uniformly low line-of-sight extinction that ensures observations with high resolution and sensitivity. Using the WIYN/Hydra multi-fiber spectrograph, we have obtained optical (4119--6882Å) spectra of 77 PN candidates selected from Hubble Space Telescope narrow-band imaging, which are located within the central $\sim$500pc region of M31. Among these candidates, 49 (64%) are spectroscopically observed for the first time. The spectra of 300 previously known PNe and H II regions, which primarily reside in the disk, are also taken for comparison. All 77 circumnuclear PN candidates exhibit prominent emission lines, including [O III] $λ$5007, [N II] $λ$6583, H$α$ and H$β$, strongly suggesting that they are genuine PNe. We measured the line fluxes, radial velocities and line widths for all objects, and found that the radial velocities of the circumnuclear PNe generally trace rotation of the inner bulge. We also estimated a dynamical mass of $\sim$6.4$\pm$0.5$\times$10$^{9}$$M_{\odot}$ enclosed within an effective galactocentric radius of 340pc, which is compatible with the previously estimated total stellar mass in this region.
description: 30 pages, 11 figures, accepted for publication in RAA
Photon operators for lattice gauge theory
Creators: name: Lewis, Randy
name: Woloshyn, R. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: Photon operators with the proper $J^{PC}$ quantum numbers are constructed, including one made of elementary plaquettes. In compact U(1) lattice gauge theory, these explicit photon operators are shown to permit direct confirmation of the massive and massless states on each side of the phase transition. In the abelian Higgs model, these explicit photon operators avoid some excited state contamination seen with the traditional composite operator, and allow more detailed future studies of the Higgs mechanism.
description: 7 pages, 13 figures. v2: reference added
The higgsino-singlino sector of the NMSSM: Combined constraints from dark matter and the LHC
Creators: name: Ellwanger, Ulrich
name: Hugonie, Cyril
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A light singlino is a promising candidate for dark matter, and a light higgsino is natural in the parameter space of the NMSSM. We study the combined constraints on this scenario resulting from the dark matter relic density, the most recent results from direct detection experiments, LEP and the LHC. In particular limits from a recent search for electroweak production of charginos and neutralinos at $\sqrt{s}=13$ TeV after 35.9 fb$^{-1}$ by CMS and constraints on spin-independent dark matter-nucleon cross sections from XENON1T after one tonne$\times$year exposure are considered. We find that scenarios with higgsino masses below $\sim 250$ GeV as well as singlino masses below $\sim 100$ GeV are strongly constrained depending, however, on assumptions on the bino mass parameter $M_1$. Benchmark points and branching fractions for future searches at the LHC are proposed.
description: 20 pages, 5 figures, references added
Continuous Randomness via Transformations of 2-Random Sequences
Creators: name: Porter, Christopher P.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Logic (math.LO)
subject: FOS: Mathematics

description: Reimann and Slaman initiated the study of sequences that are Martin-Löf random with respect to a continuous measure, establishing fundamental facts about NCR, the collection of sequences that are not Martin-Löf random with respect to any continuous measure. In the case of sequences that are random with respect to a computable, continuous measure, the picture is fairly well-understood: such sequences are truth-table equivalent to a Martin-Löf random sequence. However, given a sequence that is random with respect to a continuous measure but not with respect to any computable measure, we can ask: how close to effective is the measure with respect to which it is continuously random?
 In this study, we take up this question by examining various transformations of 2-random sequences (sequences that are Martin-Löf random relative to the halting set $\emptyset'$) to establish several results on sequences that are continuously random with respect to a measure that is computable in $\emptyset'$. In particular, we show that (i) every noncomputable sequence that is computable from a 2-random sequence is Martin-Löf random with respect to a continuous, $\emptyset'$-computable measure and (ii) the Turing jump of every 2-random sequence is Martin-Löf random with respect to a continuous, $\emptyset'$-computable measure. From these results, we obtain examples of sequences that are not proper, i.e., not random with respect to any computable measure, but are random with respect to a continuous, $\emptyset'$-computable measure. Lastly, we consider the behavior of 2-randomness under a wider class of effective operators (c.e. operators, pseudojump operators, and operators defined in terms of pseudojump inversion), showing that these too yield sequences that are Martin-Löf random with respect to a continuous, $\emptyset'$-computable measure.
Additional file 1 of RGD-p21Ras-scFv expressed prokaryotically on a pilot scale inhibits ras-driven colorectal cancer growth by blocking p21Ras-GTP
Creators: name: Lin, Peng
name: Qian, Jing
name: Huang, Cheng-Cheng
name: Xu, Wen-Mang
name: Wang, Yuan-Yuan
name: Gao, Zi-Ran
name: Zheng, Shi-Qi
name: Wang, Peng
name: Jia, Da-Qi
name: Feng, Qiang
name: Yang, Ju-Lun
Publisher: name: figshare
Year: 2024
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: Pharmacology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Supplementary Material 1
A brown dwarf candidate in the Praesepe Open Cluster
Creators: name: Magazzu, A.
name: Rebolo, R.
name: Osorio, M. R. Zapatero
name: Martin, E. L.
name: Hodgkin, S. T.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present optical and infrared observations of RPr1, a faint (I = 21.01) and very red object (I - K = 4.57) discovered in a deep CCD survey, covering an area of 800 square arcmin of the Praesepe open cluster. A low resolution spectrum shows that RPr1 is a very late object, the latest object in Praesepe for which a spectrum has been taken to date. Our estimates give a mass between 0.063 and 0.084 solar masses, and indicate that RPr1 may turn out to be the first brown dwarf in this cluster.
description: 7 pages, 3 Postscript figures, to be published in The Astrophysical Journal Letters
Oral history interview with Millie Hanson, 2002
Publisher: name: Columbia University
Year: 2019
Subjects: Obstetricians
Gynecologists
Abortion--United States
Abortion
Abortion--Law and legislation--United States
Abortion--History--20th century.--United States
Abortion services--United States
Physicians--Attitudes.--United States
Reproductive rights--United States

description: Childhood: Turtle lake and Clayton, Northern Wisconsin; education: River Falls State College, River Falls, Wisconsin; medical school, University of Minnesota; farm life in rural Wisconsin; early experience of abortion-related deaths within family; the state of abortion legislation in the Midwest pre-Roe v. Wade; discussion of abortion complications; internship at Minneapolis General Hospital; medical school's treatment of the abortion issue; discussion of physical dangers to abortion doctors; hospital administration and legal risks in regards to abortions; traumatic experience with female student via telephone; establishment of personal practice; explanation of bureaucratic gymnastics involved for legal abortions; fears regarding the future of pro-choice legislation
Radial-angular coupling in self phase modulation with structured light
Creators: name: de Oliveira, M. Gil
name: Pereira, L. J.
name: Santos, A. S.
name: Dechoum, K.
name: Bramati, A.
name: Khoury, A. Z.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: In this work we study the evolution of an optical vortex undergoing self phase modulation inside a nonlinear Kerr medium. The intensity dependent phase evolution couples the angular and radial degrees of freedom of the input vortex, giving rise to a rich dynamics where new radial modes are created. In the short propagation range, this dynamics is well described by a perturbative approach, predicting the generation of modes with radial numbers between zero and the absolute value of the vortex topological charge. This prediction is confirmed by numerical simulations of the nonlinear propagation equation.
Additional file 1: of Identity and validity of conserved B cell epitopes of filovirus glycoprotein: towards rapid diagnostic testing for Ebola and possibly Marburg virus disease
Creators: name: Peace Babirye
name: Musubika, Carol
name: Kirimunda, Samuel
name: Downing, Robert
name: Lutwama, Julian
name: Mbidde, Edward
name: Weyer, Jacqueline
name: Paweska, Janusz
name: Joloba, Moses
name: Wayengera, Misaki
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: S1 Cloning, Expression and Purification of EBOV GP1, 2 in HEK293-6E mammalian cell-lines. This file details the cloning, expression and purification of EBOV GP1, 2 in HEK293-6E mammalian cell-lines. (PDF 1555 kb)
Exotic Hadrons at LHCb
Creators: name: Johnson, Daniel
name: Polyakov, Ivan
name: Skwarnicki, Tomasz
name: Wang, Mengzhen
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It has been five years since the data sample from the LHCb detector, the first experiment optimized for heavy-flavor physics studies at a hadronic collider, was completed. These data led to many major discoveries in exotic hadron spectroscopy, which we review in this article. We supplement the experimental results with a selection of phenomenological interpretations. As the upgraded LHCb detector is expected to collect a larger data sample starting in 2024, the near- and further-future potential of the LHCb program in exotic hadron physics is also discussed.
The Monadic Electron Universe: A Single Braided Worldline Approach to Spin-½, Multi-Fermion States, and Pauli Exclusion
Creators: name: ELBIZRI, SAMER
Publisher: name: Zenodo
Year: 2025
Subjects: subject: Physics
subject: Physics
subject: Mathematical physics
subject: Particle physics

description: We revisit the classic Wheeler–Feynman “one-electron universe” speculation—where all electrons and positrons are manifestations of a single zigzagging worldline in 4D spacetime—and develop it into a rigorous framework using worldline methods and Grassmann variables to account for spin-½. We show how:

Dirac spinors and the standard QED fermion propagator naturally emerge from a single, braided worldline with local supersymmetry (the “spinning particle” formalism).

The Pauli exclusion principle arises from topological and Grassmann constraints, eliminating the need to impose antisymmetrization by hand.

Multi-electron processes (e.g., scattering, multi-point correlators) appear as segments of the same cosmic thread, reproducing the usual results of second-quantized QED.

The Schwinger correction to the electron’s magnetic moment (g−2) arises from loop-like self-interactions of the worldline, demonstrating the calculational power of the framework.

Gauge interactions are generalized to non-Abelian symmetry via color-carrying Grassmann variables, allowing confinement and asymptotic freedom to emerge geometrically.

Knot invariants and topological quantum numbers (e.g., Gauss linking number, Jones polynomial) provide a new layer of observable structure, predicting testable deviations in spectroscopy, scattering, and quantum interference.

This single-entity picture remains fully consistent with known quantum field theory yet offers a fresh geometric/topological interpretation of fermionic statistics, gauge invariance, and the role of spin—all within 3+1-dimensional spacetime, echoing Penrose’s insistence on retaining geometric intuition and building on our earlier work reinterpreting the “one-electron universe” hypothesis [Bizri, 2025],. We also propose a shift in this framework—from reinterpretation to prediction—and outline how this model could unify aspects of the Standard Model in a purely topological and spacetime-realistic manner.
title: ADCO, Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Cart. 177 (11 H 289), 197 folios, f. 0052
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2015
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 177 (11 H 289), 197 folios, f. 0052, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 177 (11 H 289), 197 folios, f. 0052, 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
Black Hole Thermodynamics from Calculations in Strongly-Coupled Gauge Theory
Creators: name: Kabat, Daniel
name: Lifschytz, Gilad
name: Lowe, David A.
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We develop an approximation scheme for the quantum mechanics of N D0-branes at finite temperature in the 't Hooft large-N limit. The entropy of the quantum mechanics calculated using this approximation agrees well with the Bekenstein-Hawking entropy of a ten-dimensional non-extremal black hole with 0-brane charge. This result is in accord with the duality conjectured by Itzhaki, Maldacena, Sonnenschein and Yankielowicz. Our approximation scheme provides a model for the density matrix which describes a black hole in the strongly-coupled quantum mechanics.
description: 16 pages, 5 figures, latex, (v2 minor corrections)
Fast Coherent Differential Imaging on Ground-Based Telescopes using the Self-Coherent Camera
Creators: name: Gerard, Benjamin L.
name: Marois, Christian
name: Galicher, Raphaël
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Direct imaging and spectral characterization of exoplanets using extreme adaptive optics (ExAO) is a key science goal of future extremely large telescopes and space observatories. However, quasi-static wavefront errors will limit the sensitivity of this endeavor. Additional limitations for ground-based telescopes arise from residual AO-corrected atmospheric wavefront errors, generating millisecond-lifetime speckles that average into a halo over a long exposure. A solution to both of these problems is to use the science camera of an ExAO system as a wavefront sensor to perform a fast measurement and correction method to minimize these aberrations as soon as they are detected. We develop the framework for one such method based on the self-coherent camera (SCC) to be applied to ground-based telescopes, called Fast Atmospheric SCC Technique (FAST). We show that with the use of a specially designed coronagraph and coherent differential imaging algorithm, recording images every few milliseconds allows for a subtraction of atmospheric and static speckles while maintaining a close to unity algorithmic exoplanet throughput. Detailed simulations reach a contrast close to the photon noise limit after 30 seconds for a 1 % bandpass in H band on both 0$^\text{th}$ and 5$^\text{th}$ magnitude stars. For the 5th magnitude case, this is about 110 times better in raw contrast than what is currently achieved from ExAO instruments if we extrapolate for an hour of observing time, illustrating that sensitivity improvement from this method could play an essential role in the future detection and characterization of lower mass exoplanets.
Constraining the multiplicity statistics of the coolest brown dwarfs: binary fraction continues to decrease with spectral type
Creators: name: Fontanive, Clémence
name: Biller, Beth
name: Bonavita, Mariangela
name: Allers, Katelyn
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Binary statistics of the latest-type T and Y brown dwarfs are sparse and it is unclear whether the trends seen in the multiplicity properties of their more massive counterparts hold for the very coolest brown dwarfs. We present results from a search for substellar and planetary-mass companions to a sample of 12 ultracool T8$-$Y0 field brown dwarfs with the Hubble Space Telescope/Wide Field Camera 3. We find no evidence for resolved binary companions among our sample down to separations of 0.7$-$2.5 AU. Combining our survey with prior searches, we place some of the first statistically robust constraints to date on the multiplicity properties of the coolest, lowest-mass brown dwarfs in the field. Accounting for observational biases and incompleteness, we derive a binary frequency of $f = 5.5^{+5.2}_{-3.3}$% for T5$-$Y0 brown dwarfs at separations of 1.5$-$1000 AU, for an overall binary fraction of $f_\mathrm{tot} = 8\pm6$%. Modelling the projected separation as a lognormal distribution, we find a peak in separation at $ρ_0 = 2.9^{+0.8}_{-1.4}$ AU with a logarithmic width of $σ= 0.21^{+0.14}_{-0.08}$. We infer a mass ratio distribution peaking strongly towards unity, with a power law index of $γ= 6.1^{+4.0}_{-2.7}$, reinforcing the significance of the detection of a tighter and higher mass ratio companion population around lower-mass primaries. These results are consistent with prior studies and support the idea of a decreasing binary frequency with spectral type in the Galactic field.
description: 26 pages, 22 figures, accepted for publication in MNRAS
title: 03_0211
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/
Additional file 1: of Efficient generation of stable, heritable gene edits in wheat using CRISPR/Cas9
Creators: name: Howells, Rhian
name: Craze, Melanie
name: Bowden, Sarah
name: Wallington, Emma
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Figure S1. Sequence alignment of TaPDS from wheat variety Fielder and HvPDS from barley variety Golden Promise with guide sites indicated. (DOCX 149Â kb)
Oral history interview with Milton S. Eisenhower, 1967
Publisher: name: Columbia University
Year: 2020
Subjects: Educators
Government executives--United States
Presidents--Election--1960.--United States

description: Latin American relations; Eisenhower brothers; President Eisenhower and his administration; White House staff and organization; General Eisenhower's decisions to run in 1952 and 1956; 1960 campaign; Republican Critical Issues Council; impressions of Harry S. Truman, Richard Nixon, Joseph R. McCarthy, Lyndon B. Johnson, John Foster Dulles, Fidel Castro
Massless preheating with full Einstein gravity
Creators: name: Szmigiel, Mariusz
Publisher: name: Imperial College London
Year: 2013

description: Cosmic microwave background (CMB) radiation fills the universe almost uniformly and it has imprints of the primordial curvature perturbations. Observations of the CMB showed that to a large extent they are Gaussian [1]. However, there are hints of some non-Gaussianity in the CMB that is within the reach of experiments such as the Planck satellite. Different models of inflation predict different levels of non-Gaussianity. Comparison with the experiments could be used to falsify some models and single out the one describing the physics of inflation most correctly [2]. It has been found that preheating can produce substantial levels of non- Gaussianity in the massless model in the FRW backgroud [28]. In my thesis I present a detailed description of a refined calculation, which does not assume an FRW Universe but allows for the subhorizon inhomogeneous metric perturbations to interact with the scalar fields in a fully non linear fashion. Including the subhorizon metric perturbations in the dynamics is a physically much more accurate calculation. It allows for increasing the lattice size at will and therefore allows for including in the dynamics even those modes whose wavelengths are equal to or greater than the size of the horizon. I combined the lattice simulations with the separate universe approximation [5, 40]. The latter states that points in space separated by more than one Hubble distance cannot interact with each other and therefore evolve independently. The numerical integration of the Einstein Equations uses the BSSN scheme [7], a technique used to solve initial value problems in the 3+1 formulation of numerical relativity. I found that it is indeed possible to compute the superhorizon curvature perturbations at a constant density hypersurface including full metric perturbations. However, I also identified that accuracy improvements are needed to compare my results to the literature. I identified and successfully implemented a number of the improvements and presented some suggestions for the future research.
title: ADCO, Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.1 (début XIIIe siècle), Cart. 166 (11 H 64), 136 folios, f. 0029r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.1 (début XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 166 (11 H 64), 136 folios, f. 0029r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'abbaye de Cîteaux dit Cartulare Antiquum t.1 (début XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 166 (11 H 64), 136 folios, f. 0029r, 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
Astrometric Observation of MACHO Gravitational Microlensing
Creators: name: Boden, A. F.
name: Shao, M.
name: Van Buren, D.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Following previous suggestions of other researchers, this paper discusses the prospects for astrometric observation of MACHO gravitational microlensing events. We derive the expected astrometric observables for a simple microlensing event with either a dark or self-luminous lens, and demonstrate that accurate astrometry can determine the lens mass, distance, and proper motion in a very general fashion. In particular we argue that in limited circumstances ground-based, narrow-angle differential astrometric techniques are sufficient to measure the lens mass directly, and other lens properties (distance, transverse motion) by applying an independent model for the source distance and motion. We investigate the sensitivity of differential astrometry in determining lens parameters by Monte Carlo methods, and derive a quasi-empirical relationship between astrometric accuracy and mass uncertainty.
description: 28 p, 12 fig, To appear in the ApJ
Libellula americana Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Odonata
Libellulidae
Libellula
Libellula americana

description: Libellula americana [spec. nov.]
L. alis purpurascentibus: fascia alba, primoribus apice albis; posticis linea baseos alba.
Edw. av. 174. t. 174.
Habitat in America.
Corpus viride. Alae fusco-purpurascentes.
* * Oculi distantes remotique.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 545, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Conductivity and Resistivity of Dirac Electrons in Single-Component Molecular Conductor [Pd(dddt)_2]
Creators: name: Suzumura, Yoshikazu
name: Cui, HenBo
name: Kato, Reizo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Dirac electrons, which have been found in the single-component molecular conductor [Pd(dddt)_2] under pressure, are examined by calculating the conductivity and resistivity in terms of a tight-binding model for several pressures of P GPa, which give a nodal line semimetal or insulator. The temperature (T) dependence of the conductivity shows that the conductivity increases linearly under pressure at low T due to the Dirac cone but stays almost constant at high T. Further, at lower pressures, the conductivity is suppressed due to an unconventional gap, which is examined by calculating the resistivity. The resistivity exhibits a pseudogap-like behavior even in the case described by the Dirac cone. Such behavior originates from a novel role of the nodal line semimetal followed by a pseudogap that is different from a band gap. The present result reasonably explains the resistivity observed in the experiment.
description: 16 pages, 7 figures
MOESM1 of Translocated duplication of a targeted chromosomal segment enhances gene expression at the duplicated site and results in phenotypic changes in Aspergillus oryzae
Creators: name: Takahashi, Tadashi
name: Ogawa, Masahiro
name: Sato, Atsushi
name: Koyama, Yasuji
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1. Supplementary figures and tables.
Flowing from a noncommmutative (OM) five brane via its supergravity dual
Creators: name: Berman, D. S.
name: Sundell, P.
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The dual supergravity description of the flow between (2,0) five-brane theory and the noncommutative five-brane (OM) theory is examined at critical five-brane field strength. The self-duality of the field strength is shown to arise as a consequence of the supergravity solution. Open membrane solutions are examined in the background of the five-brane giving rise to an M analogue of the noncommutative open string (NCOS) solution.
description: 13 pages, 1 figure, revtex, typos corrected and an additional condition on how to take the decoupling limit is incorporated, references added
A radio survey of supersoft, persistent and transient X-ray sources in the Magellanic Clouds
Creators: name: Fender, R. P.
name: Southwell, K.
name: Tzioumis, A. K.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a radio survey of X-ray sources in the Large and Small Magellanic clouds with the Australia Telescope Compact Array at 6.3 and 3.5 cm. Specifically, we have observed the fields of five LMC and two SMC supersoft X-ray sources, the X-ray binaries LMC X-1, X-2, X-3 & X-4, the X-ray transient Nova SMC 1992, and the soft gamma-ray repeater SGR 0525-66. None of the targets are detected as point sources at their catalogued positions. In particular, the proposed supersoft jet source RXJ 0513-69 is not detected, placing constraints on its radio luminosity compared to Galactic jet sources. Limits on emission from the black hole candidate systems LMC X-1 and X-3 are consistent with the radio behaviour of persistent Galactic black hole X-ray binaries, and a previous possible radio detection of LMC X-1 is found to almost certainly be due to nearby field sources. The SNR N49 in the field of SGR 0525-66 is mapped at higher resolution than previously, but there is still no evidence for any enhanced emission or disruption of the SNR at the location of the X-ray source.
description: 5 pages, LaTeX. Accepted for publication in MNRAS
The effect of L-cysteine on appetite in humans
Creators: name: Amin, Anjali
Publisher: name: Imperial College London
Year: 2013

description: High protein diets suppress appetite and facilitate weight loss. However, they are difficult to adhere to. Understanding the mechanisms by which protein suppresses appetite may establish targets for more acceptable interventions to treat or prevent obesity. Receptor systems that respond to amino acids, the products of protein digestion, have been identified. However, the specific mechanisms regulating protein-induced satiety are unknown. Previous work within our laboratory has investigated the effect of specific amino acids which act as ligands for the following G-protein coupled receptors: CaR, T1R1/T1R3 and GPRC6A on food intake in rodents. L-cysteine activates the CaR, the T1R1/T1R3 and the GPRC6A. A diet that includes high levels of whey protein, which contains high levels of L-cysteine, has been reported to be more satiating and to suppress circulating levels of the orexigenic hormone ghrelin to a greater extent than other types of protein in humans. Pilot studies suggested that ligands for the GPRC6A receptor can reduce food intake in rodents, and that this effect is at least partly mediated by a reduction in circulating ghrelin levels. The putative role of L-cysteine in food intake in humans was investigated. The effect of a high protein meal on circulating levels of cysteine was determined. Subsequently, the time course of changes in the circulating levels of L-cysteine following oral consumption of L-cysteine was established. Finally, the effects of different doses of cysteine on subjective assessment of appetite and acute food intake were investigated. These studies suggested that oral administration of L-cysteine at 0.04 or 0.07g/kg resulted in supraphysiological levels of L-cysteine in circulation. Oral administration of L-cysteine significantly influenced subjective markers of appetite compared to vehicle or glycine controls, but did not affect food intake. These data suggest that L-cysteine may be suitable for manipulating appetite in humans.
Entropy Methods for the Confidence Assessment of Probabilistic Classification Models
Creators: name: Tornetta, Gabriele Nunzio
Publisher: name: Statistica
Year: 2022

description: Many classification models produce a probability distribution as the outcome of a prediction. This information is generally compressed down to the single class with the highest associated probability. In this paper we argue that part of the information that is discarded in this process can be in fact used to further evaluate the goodness of models, and in particular the confidence with which each prediction is made. As an application of the ideas presented in this paper, we provide a theoretical explanation of a confidence degradation phenomenon observed in the complement approach to the (Bernoulli) Naïve Bayes generative model.
description: Statistica, Vol. 81 No. 4 (2021)
Additional file 1 of Characteristics of acute kidney injury and its impact on outcome in patients with acute-on-chronic liver failure
Creators: name: Huang, Yue
name: Cai, Junjun
name: Ha, Fushuang
name: Guo, Beichen
name: Xin, Shaojie
name: Duan, Zhongping
name: Han, Tao
Publisher: name: figshare
Year: 2022
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Developmental Biology
subject: Science Policy

description: Additional file 1: Comparison of clinical characteristics between training cohort and validation cohort.
The action of a casual set
Creators: name: Benincasa, Dionigi Maria Teofilo
Publisher: name: Imperial College London
Year: 2013

description: A causal set is a model for a discrete spacetime in which the “atoms of spacetime” carry a relation of ancestry. This order relation is mathematically given by a partial order, and is is taken to underly the macroscopic causal notions of before and after. The work presented in this thesis proposes a definition for the action of a causal set analogous to the continuum Einstein-Hilbert action. The path taken towards the definition of this action is somewhat indirect. We first construct a retarded wave operator on causal sets well-approximated by 4-dimensional spacetimes and prove, under certain assumptions, that this operator gives the usual continuum d’Alembertian and the scalar curvature of the approximating spacetime in the continuum limit. We use this result to define both the scalar curvature and the action of a causal set. This definition can be shown to work in any dimension, so that an explicit form of the action exists in all dimensions. We conjecture that, under certain conditions, the continuum limit of the action is given by the Einstein-Hilbert action up to boundary terms, whose explicit form we also conjecture. We provide evidence for this conjecture through analytic and numerical calculations of the expected action of various spacetime regions. The 2-dimensional action is shown to possess topological properties by calculating its expectation value for various regions of 2-dimensional spacetimes with different topologies. We find that the topological character of the 2d action breaks down for causally convex regions of the trousers spacetime that contain the singularity, and for non-causally convex rectangles. Finally, we propose a microscopic account of the entropy of causal horizons based on the action. It is a form of “spacetime mutual information” arising from the partition of spacetime by the horizon. Evidence for the proposal is provided by analytic results and numerical simulations in 2- dimensional examples. Further evidence is provided by numerical results for the Rindler and cosmic deSitter horizons in both 3 and 4-dimensions, and for a non-equilibrium horizon in a collapsing shell spacetime in 4-dimensions.
Molecular gas in the northern nucleus of Mrk273: Physical and chemical properties of the disk and its outflow
Creators: name: Aladro, R.
name: König, S.
name: Aalto, S.
name: González-Alfonso, E.
name: Falstad, N.
name: Martín, S.
name: Muller, S.
name: García-Burillo, S.
name: Henkel, C.
name: van der Werf, P.
name: Mills, E.
name: Fischer, J.
name: Costagliola, F.
name: Krips, M.
name: .
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Aiming to characterise the properties of the molecular gas in the ultraluminous infrared galaxy Mrk273 and its outflow, we used the NOEMA interferometer to image the dense gas molecular tracers HCN, HCO+, HNC, HOC+ and HC3N at 86GHz and 256GHz with angular resolutions of 4.9x4.5 arcsec (3.7x3.4 kpc) and 0.61x0.55 arcsec (460x420 pc). We also modelled the flux of several H2O lines observed with Herschel using a radiative transfer code that includes excitation by collisions as well as by far-infrared photons. The disk of the Mrk273 north nucleus has two components with decoupled kinematics. The gas in the outer parts (1.5 kpc) rotates with a south-east to north-west direction, while in the inner disk (300 pc) follows a north-east to south-west rotation. The central 300 pc, which hosts a compact starburst region, is filled with dense and warm gas, contains a dynamical mass of (4-5)x10^9M_sun, a luminosity of L'_HCN=(3-4)x10^8 K km/s pc^2, and a dust temperature of 55 K. At the very centre, a compact core with R~50 pc has a luminosity of L_IR=4x10^11L_sun (30% of the total infrared luminosity), and a dust temperature of 95 K. The core is expanding at low velocities ~50-100 km/s, probably affected by the outflowing gas. We detect the blue-shifted component of the outflow, while the red-shifted counterpart remains undetected in our data. Its cold and dense phase reaches fast velocities up to ~1000 km/s, while the warm outflowing gas has more moderate maximum velocities of ~600 km/s. The outflow is detected as far as 460 pc from the centre in the northern direction, and has a mass of dense gas <8x10^8M_sun. The difference between the position angles of the inner disk (~70 degree) and the outflow (~10 degree) indicates that the outflow is likely powered by the AGN, and not by the starburst. Regarding the chemistry, we measure an extremely low HCO+/HOC+ ratio of 10+-5 in the inner disk of Mrk273.
description: Accepted for publication in A&A. 21 pages, 17 figures, 7 tables, and a lot of interesting text
Optical MEMS Design for Telecommunications Applications
Creators: name: Aksyuk, Vladimir A.
name: Simon, Maria E.
name: Pardo, Flavio
name: Arney, Susanne
name: Lopez, Daniel
name: Villanueva, Anita
Publisher: name: arXiv
Year: 2024
Subjects: subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: As optical telecommunication networks become more complex, there is an emerging need for systems capable of very complex switching and manipulation of large numbers of optical signals. MEMS enable these systems by combining excellent capabilities and optical properties of macroscopic optomechanics with dense integration of multiple actuators on a single chip. Such optical MEMS present common design and process challenges, such as multiple electrical and optical IO, optical surface quality, optical integration density (fill factor) and actuator performance and reliability. We have used general design approaches such as pure-flexure design, electrostatic actuation and residual stress engineering in addressing these challenges. On several examples in this paper we illustrate these approaches along with underlying design tradeoffs and process requirements. We also describe specific numerical techniques useful for electrostatic actuator optimization and for analyzing the effects of residual stress.
description: https://www.transducer-research-foundation.org/technical_digests/past_digests.html
Effects of percutaneous balloon mitral valvuloplasty in patients with mitral stenosis and atrial fibrillation: a systematic review and meta-analysis
Creators: name: Liu, Bojiang
name: Wang, Yunyun
name: Liu, Yingwu
name: Wu, Peng
name: Li, Tong
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Science Policy

description: The study aimed to systematically review the existing literature and assess the effects of percutaneous balloon mitral valvuloplasty (PBMV) in patients with mitral stenosis and atrial fibrillation (AF) as opposed to sinus rhythm (SR). Eligible studies were identified from six electronic databases before June 2021. The primary outcome was mitral valve area (MVA), and secondary outcomes were hemodynamic measurements, in-hospital complications, and long-term outcomes. Relative risks (RRs) or weighted mean differences (WMDs) with 95% confidence intervals (CIs) were used as effect sizes. Fifteen studies were included involving 6351 patients. For the primary outcome, the AF group obtained less favourable changes in MVA (WMD: −0.10, 95%CI: −0.14, −0.06) and a significantly smaller postoperative and long-term MVA (WMD: −0.13, 95%CI: −0.18, −0.08 and WMD: −0.10, 95%CI: −0.17, −0.03, respectively) compared to the SR group. For secondary outcome, the AF group was associated with suboptimal outcomes as following (WMD/RR, [95%CI]): higher LAP (1.37, [0.86, 1.87]), more embolism (2.85, [1.44, 5.63]), lower event-free survival (0.89, [0.80, 1.00]), higher incidences of mitral valve replacement (2.20, [1.40, 3.46]), re-PBMV (2.28, [1.63, 3.19]), and mortality (3.28, [2.42, 4.44]). No significant differences were found in other outcomes. The currently available evidence suggests that PBMV may be less effective in patients with AF than in those with SR. However, early treatment and appropriate management of AF patients undergoing PBMV may benefit the immediate and long-term outcomes.