cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0914
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0914, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0914, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: http://www.wikidata.org/entity/Q15945019
description: Provenance: abbaye Saint-Étienne de Dijon
The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck
Creators: name: Valenti, Stefano
name: Sand, David J.
name: Yang, Sheng
name: Cappellaro, Enrico
name: Tartaglia, Leonardo
name: Corsi, Alessandra
name: Jha, Saurabh W.
name: Reichart, Daniel E.
name: Haislip, Joshua
name: Kouprianov, Vladimir
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: During the second observing run of the Laser Interferometer gravitational- wave Observatory (LIGO) and Virgo Interferometer, a gravitational-wave signal consistent with a binary neutron star coalescence was detected on 2017 August 17th (GW170817), quickly followed by a coincident short gamma-ray burst trigger by the Fermi satellite. The Distance Less Than 40 (DLT40) Mpc supernova search performed pointed follow-up observations of a sample of galaxies regularly monitored by the survey which fell within the combined LIGO+Virgo localization region, and the larger Fermi gamma ray burst error box. Here we report the discovery of a new optical transient (DLT17ck, also known as SSS17a; it has also been registered as AT 2017gfo) spatially and temporally coincident with GW170817. The photometric and spectroscopic evolution of DLT17ck are unique, with an absolute peak magnitude of Mr = -15.8 \pm 0.1 and an r-band decline rate of 1.1mag/d. This fast evolution is generically consistent with kilonova models, which have been predicted as the optical counterpart to binary neutron star coalescences. Analysis of archival DLT40 data do not show any sign of transient activity at the location of DLT17ck down to r~19 mag in the time period between 8 months and 21 days prior to GW170817. This discovery represents the beginning of a new era for multi-messenger astronomy opening a new path to study and understand binary neutron star coalescences, short gamma-ray bursts and their optical counterparts.
description: ApJL in press, 4 figures
Osteossíntese em fratura de tíbia de Maritaca Maracanã
Creators: name: OLIVEIRA, ALYSSON DE PAULA
name: DE OLIVEIRA, EMANUELLE SILVA
name: roier, Erica Cristina Rocha
name: do Amaral, Gabriela Vieira
name: Junqueira, Leticia dos SSantos
name: Motta, Lucas Baptista
Publisher: name: Zenodo
Year: 2023

description: Folder informativo elaborado por discentes do Mestrado Profissional em Diagnóstico em Medicina Veterinária e discente de graduação em Medicina Veterinária, com o objetivo de esclarecer médicos veterinários, alunos de graduação e a população em geral sobre doenças, diagnóstico, tratamento e controle de afecções em animais domésticos e silvestres.
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 1088
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 1088, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 1088, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Additional file 2: of A PSTOL-like gene, TaPSTOL, controls a number of agronomically important traits in wheat
Creators: name: Milner, Matthew
name: Howells, Rhian
name: Craze, Melanie
name: Bowden, Sarah
name: Graham, Neil
name: Wallington, Emma
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: 60506 Virology
subject: Computational Biology

description: Figure S1. Location of gene-specific primers and PCR amplification of TaPSTOL genomic regions on DNA extracted from nullisomic (N) / tetrasomic (T) wheat lines. The PCR amplicons correspond to a promoter region (PCR1, 1458Â bp), a promoter and coding region (PCR2, 553Â bp), and a coding region (PCR3, 870Â bp), to demonstrate that TaPSTOL is only present on chromosome 5A. (DOCX 63 kb)
On the relation between RG and ERG
Creators: name: Sonoda, Hidenori
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss how the ordinary renormalization group (RG) equations arise in the context of Wilson's exact renormalization group (ERG) as formulated by Polchinski. We consider the phi4 theory in four dimensional euclidean space as an example, and introduce a particular scheme of parameterizing the solutions of the ERG equations. By analyzing the scalar composite operators of dimension two and four, we show that the parameters obey mass independent RG equations. We conjecture the equivalence of our parameterization scheme with the MS scheme for dimensional regularization.
description: 18 pages, 3 figures, LaTeX2e; small changes made to enhance clarity, especially in sect. 3
Egalitarian aspects of scale-free networks
Creators: name: Fabbri, Renato
name: Pisani, Marilia M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: Scale-free networks are frequently described as the zenith of inequality and sometimes even pin-pointed as a natural cause of concentrations, including accumulation of resources in human society. Although coherent with theory and empirical data, there are at least three aspects of scale-free networks that are egalitarian. Using the social network metaphor (which is easier to grasp): 1) the presence of each agent (vertex or component) in diverse networks, while each agent has the same amount of resources (e.g. time) for engaging (establishing links or edges) with other individual agents, ideas or objects; 2) the constant change in the concentration of resources (in this case, links) of each agent; 3) the uniform distribution of resources with respect to the amount of resources per agent (the more resources per agent, the fewer the agents). We also consider the importance of vertices that are not hubs and overstatements on the importance of the hubs. The conclusions suggest the urge of research to better examine and model the relevance of the vertices that are not hubs (i.e. peripheral and intermediary) and verify the need to better weight the emphasis current literature places in the association of inequality to the scale-free networks (and other phenomena in which power laws are found).
K-PIE: using K-means algorithm for Percentage Infection symptoms Estimation
Creators: name: Bueno-Sancho, Vanessa
name: Corredor-Moreno, Pilar
name: Ngonidzashe Kangara
name: Saunders, Diane G.O.
Publisher: name: Zenodo
Year: 2019
Subjects: Wheat rust
plant pathology
image analysis
K-mean algorithm

description: The K-means algorithm is one of the most effective clustering methods that has been widely used in plant disease detection. Herein, we developed a script termed K-PIE (K-means algorithm for Percentage Infection symptoms Estimation) that utilises the k-means algorithm to analyse images of both yellow and stem rust infected wheat leaves to estimate the percentage of disease symptoms based on colour analysis.
Insights into Allosteric Inhibition of AcrB Efflux Pump: Role of Distinct Binding Pockets, Protomer Preferences, and Crosstalk Disruption
Creators: name: Roy, Rakesh Kumar
name: Abhishek, Bera
name: Patra, Niladri
Publisher: name: Zenodo
Year: 2024

description: Supplementary Information for the manuscript "Insights into Allosteric Inhibition of AcrB Efflux Pump: Role of Distinct Binding Pockets, Protomer Preferences, and Crosstalk Disruption" by Rakesh Kumar Roy, Abhishek Bera and Niladri Patra, Department of Chemistry and Chemical Biology, Indian Institute of Technology (ISM) Dhanbad, Dhanbad - 826004, India
A comparison between SALT/SAAO observations and kilonova models for AT 2017gfo: the first electromagnetic counterpart of a gravitational wave transient - GW170817
Creators: name: Buckley, David A. H.
name: Andreoni, Igor
name: Barway, Sudhanshu
name: Cooke, Jeff
name: Crawford, Steven M.
name: Gorbovskoy, Evgeny
name: Gromadzki, Mariusz
name: Lipunov, Vladimir
name: Mao, Jirong
name: Potter, Stephen B.
name: Pretorius, Magaretha L.
name: Pritchard, Tyler A.
name: Romero-Colmenero, Encarni
name: Shara, Michael M.
name: Vaisanen, Petri
name: Williams, Ted B.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report on SALT low resolution optical spectroscopy and optical/IR photometry undertaken with other SAAO telescopes (MASTER-SAAO and IRSF) of the kilonova AT 2017gfo (aka SSS17a) in the galaxy NGC4993 during the first 10 days of discovery. This event has been identified as the first ever electromagnetic counterpart of a gravitational wave event, namely GW170817, which was detected by the LIGO and Virgo gravitational wave observatories. The event is likely due to a merger of two neutron stars, resulting in a kilonova explosion. SALT was the third telescope to obtain spectroscopy of AT 2017gfo and the first spectrum, 1.2 d after the merger, is quite blue and shows some broad features, but no identifiable spectral lines and becomes redder over time. We compare the spectral and photometric evolution with recent kilonova simulations and conclude that they are in qualitative agreement for post-merger wind models with proton: nucleon ratios of $Y_e$ = 0.25$-$0.30. The blue colour of the first spectrum is consistent with the lower opacity of the Lathanide-free r-process elements in the ejecta. Differences between the models and observations are likely due to the choice of system parameters combined with the absence of atomic data for more elements in the ejecta models.
description: 5 pages, 4 figures, 1 table
Additional file 1 of Tensorial blind source separation for improved analysis of multi-omic data
Creators: name: Teschendorff, Andrew
name: Jing, Han
name: Paul, Dirk
name: Virta, Joni
name: Nordhausen, Klaus
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
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

description: Contains all supplementary figures and supplementary tables. (DOCX 14322 kb)
Meeting the Challenges of Modeling Astrophysical Thermonuclear Explosions: Castro, Maestro, and the AMReX Astrophysics Suite
Creators: name: Zingale, M.
name: Almgren, A. S.
name: Sazo, M. G. Barrios
name: Beckner, V. E.
name: Bell, J. B.
name: Friesen, B.
name: Jacobs, A. M.
name: Katz, M. P.
name: Malone, C. M.
name: Nonaka, A. J.
name: Willcox, D. E.
name: Zhang, W.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We describe the AMReX suite of astrophysics codes and their application to modeling problems in stellar astrophysics. Maestro is tuned to efficiently model subsonic convective flows while Castro models the highly compressible flows associated with stellar explosions. Both are built on the block-structured adaptive mesh refinement library AMReX. Together, these codes enable a thorough investigation of stellar phenomena, including Type Ia supernovae and X-ray bursts. We describe these science applications and the approach we are taking to make these codes performant on current and future many-core and GPU-based architectures.
description: submitted to Proceedings of AstroNum 2017 / Journal of Physics Conference Series; 10 pages, 6 figures; all code freely available on github (see text for repo links)
Evaluation of phenomenological one-phase criteria for the melting and freezing of softly repulsive particles
Creators: name: Saija, Franz
name: Prestipino, Santi
name: Giaquinta, Paolo V.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We test the validity of some widely used phenomenological criteria for the localization of the fluid-solid transition thresholds against the phase diagrams of particles interacting through the exp-6, inverse-power-law, and Gaussian potentials. We find that one-phase rules give, on the whole, reliable estimates of freezing/melting points. The agreement is ordinarily better for a face-centered-cubic solid than for a body-centered-cubic crystal, even more so in the presence of a pressure-driven re-entrant transition of the solid into a denser fluid phase, as found in the Gaussian-core model.
description: 16 pages, 3 figures, to appear in J. Chem. Phys
title: Stellungnahme zum Umweltbundesamt (UBA), Dessau-Roßlau
Creators: name: German Science And Humanities Council
Publisher: name: German Science and Humanities Council
Year: 2024
Subjects: Ressortforschung
Evaluation

description: Der Wissenschaftsrat bescheinigt dem Umweltbundesamt (UBA) eine ausgesprochen positive Entwicklung seit der letzten Evaluation im Jahr 2015. Über alle Themenfelder hinweg gelingt es ihm erfolgreich, sehr gute Forschungsleistungen mit effektiver Politikberatung und Kompetenzen in der Regulierung zu verknüpfen. Das UBA mit Sitz in Dessau-Roßlau ist als selbstständige Bundesoberbehörde für Forschung, Politikberatung, Vollzug und Dialog mit der Öffentlichkeit in Fragen des Umwelt-, Gesundheits- und Klimaschutzes sowie der Nachhaltigkeit im Geschäftsbereich des Bundesministeriums für Umwelt, Naturschutz, nukleare Sicherheit und Verbraucherschutz (BMUV) angesiedelt. Es erledigt in eigener Zuständigkeit Verwaltungsaufgaben auf dem Gebiet der Umwelt, der gesundheitlichen Belange des Umweltschutzes sowie des Verbraucherschutzes und der Verbraucherrechtsdurchsetzung, die ihm durch das Errichtungsgesetz oder andere Bundesgesetze zugewiesen werden.
The Distance to NGC 4993: The Host Galaxy of the Gravitational-wave Event GW170817
Creators: name: Hjorth, Jens
name: Levan, Andrew J.
name: Tanvir, Nial R.
name: Lyman, Joe D.
name: Wojtak, Radosław
name: Schrøder, Sophie L.
name: Mandel, Ilya
name: Gall, Christa
name: Bruun, Sofie H.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The historic detection of gravitational waves from a binary neutron star merger (GW170817) and its electromagnetic counterpart led to the first accurate (sub-arcsecond) localization of a gravitational-wave event. The transient was found to be $\sim$10" from the nucleus of the S0 galaxy NGC 4993. We report here the luminosity distance to this galaxy using two independent methods. (1) Based on our MUSE/VLT measurement of the heliocentric redshift ($z_{\rm helio}=0.009783\pm0.000023$) we infer the systemic recession velocity of the NGC 4993 group of galaxies in the cosmic microwave background (CMB) frame to be $v_{\rm CMB}=3231 \pm 53$ km s$^{-1}$. Using constrained cosmological simulations we estimate the line-of-sight peculiar velocity to be $v_{\rm pec}=307 \pm 230$ km s$^{-1}$, resulting in a cosmic velocity of $v_{\rm cosmic}=2924 \pm 236$ km s$^{-1}$ ($z_{\rm cosmic}=0.00980\pm 0.00079$) and a distance of $D_z=40.4\pm 3.4$ Mpc assuming a local Hubble constant of $H_0=73.24\pm 1.74$ km s$^{-1}$ Mpc$^{-1}$. (2) Using Hubble Space Telescope measurements of the effective radius (15.5" $\pm$ 1.5") and contained intensity and MUSE/VLT measurements of the velocity dispersion, we place NGC 4993 on the Fundamental Plane (FP) of E and S0 galaxies. Comparing to a frame of 10 clusters containing 226 galaxies, this yields a distance estimate of $D_{\rm FP}=44.0\pm 7.5$ Mpc. The combined redshift and FP distance is $D_{\rm NGC 4993}= 41.0\pm 3.1$ Mpc. This 'electromagnetic' distance estimate is consistent with the independent measurement of the distance to GW170817 as obtained from the gravitational-wave signal ($D_{\rm GW}= 43.8^{+2.9}_{-6.9}$ Mpc) and confirms that GW170817 occurred in NGC 4993.
description: 9 pages, 5 figures
title: Buzzards Bay Aquarium New Bedford, Massachusetts
Creators: name: (:Unkn) Unknown
Publisher: name: University of Massachusetts Amherst
Year: 1994
Subjects: subject: Whaling
subject: Manufacturing
subject: Textile
subject: Fishing
subject: Tourism
subject: FOS: Economics and business
subject: Economics
subject: Growth and Development
subject: Urban, Community and Regional Planning
subject: Urban Studies and Planning

description: The Center for Economic Development at the University of Massachusetts, in Amherst, is part of the Landscape Architecture and Regional Planning Department, and is funded by the Economic Development Administration of the U.S. Department of Commerce, and the University of Massachusetts.
description: This report was done in six parts: a history and background analysis of New Bedford, Massachusetts, and market research was carried out to understand local tourism efforts and visitors profiles. Then a study of existing aquariums throughout the country was taken to establish type, size, location and demographics, and analysis of the three possible aquarium sites in New Bedford in terms of size, location, access, parking and complementary facilities. Fifth, to enable New Bedford to remain in keeping with the existing marine industrial zoning on its waterfront the team investigated research and development possibilities for the aquarium and determine how an aquarium could be linked to local educational institutions. Finally, the report looks at the financial feasibility of the Buzzard Bay Aquarium.
Comment on Mie Scattering from a Sonoluminescing Bubble with High Spatial and Temporal Resolution [Physical Review E 61, 5253 (2000)]
Creators: name: Weninger, K. R.
name: Evans, P. G.
name: Putterman, S. J.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: A key parameter underlying the existence of sonoluminescence (SL)is the time relative to SL at which acoustic energy is radiated from the collapsed bubble. Light scattering is one route to this quantity. We disagree with the statement of Gompf and Pecha that -highly compressed water causes the minimum in scattered light to occur 700ps before SL- and that this effect leads to an overestimate of the bubble wall velocity. We discuss potential artifacts in their experimental arrangement and correct their description of previous experiments on Mie scattering.
description: 10 pages, 2 figures
Coordinated Reactive Power-Voltage Controller for Steam Power Plant Nikola Tesla B
Creators: name: Dragosavac, Jasna
name: Janda, Zarko
name: Gajic, Tomislav
name: Dobricic, Sava
name: Josifovic, Slobodan
Publisher: name: Zenodo
Year: 2024

description: U cilju prevazilaţenja nedostataka ručnog upravljanja naponima i reaktivnim snagama, razvijeni su sistemi za automatsko upravljanje naponima u EES sa namerom da se unaprede sigurnost, smanje gubici i olakša proces upravljanja sistemom. Automatizacijom upravljanja naponima i reaktivnim snagama na nivou sistema predviĎeno je da dispečer prenosne mreţe postavi vrednosti napona u odreĎenim čvorovima sistema i da se reaktivne snage generatora koji utiču na napone posmatranih čvorova postave automatski na potrebne vrednosti. Na ovaj način se eliminiše kašnjenje zbog učešća operatera u izvršenju komandi dispečera prenosne mreţe. Ukoliko se i raspodela reaktivnog opterćenja meĎu generatorima vrši koordinisano prema ţeljenoj optimizacionoj funkciji, postiţe se koordinisana naponsko-reaktivna regulacija.
Placentite em Equinos
Creators: name: Erica Cristina Rocha Roier
name: Mylena Magalhães Cotrim Rodrigues
name: Larissa de Almeida Placido
Publisher: name: Zenodo
Year: 2023

description: Folder informativo elaborado por discentes do Mestrado Profissional em Diagnóstico em Medicina Veterinária e discente de graduação em Medicina Veterinária, com o objetivo de esclarecer médicos veterinários, alunos de graduação e a população em geral sobre doenças, diagnóstico, tratamento e controle de afecções em animais domésticos e silvestres.
Additional file 3: of Effect of psychosocial interventions on the quality of life of patients with colorectal cancer: a systematic review and meta-analysis
Creators: name: Heesook Son
name: Youn-Jung Son
name: Hyerang Kim
name: Yoonju Lee
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Overall effect size when one study was removed. (DOCX 25Â kb)
title: Préface_Choix du matériel et installation du laboratoire
Creators: name: AmateurS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Préface
description: ID_PARA_00761
On sigma model RG flow, "central charge" action and Perelman's entropy
Creators: name: Tseytlin, A. A.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Differential Geometry (math.DG)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: Zamolodchikov's c-theorem type argument (and also string theory effective action constructions) imply that the RG flow in 2d sigma model should be gradient one to all loop orders. However, the monotonicity of the flow of the target-space metric is not obvious since the metric on the space of metric-dilaton couplings is indefinite. To leading (one-loop) order when the RG flow is simply the Ricci flow the monotonicity was proved by Perelman (math.dg/0211159) by constructing an ``entropy'' functional which is essentially the metric-dilaton action extremised with respect to the dilaton with a condition that the target-space volume is fixed. We discuss how to generalize the Perelman's construction to all loop orders (i.e. all orders in α'). The resulting ``entropy'' is equal to minus the central charge at the fixed points, in agreement with the general claim of the c-theorem.
description: 14 pages. v2: minor comments added, misprints corrected
A High-Resolution Combined Scanning Laser- and Widefield Polarizing Microscope for Imaging at Temperatures from 4 K to 300 K
Creators: name: Lange, Matthias
name: Guénon, Stefan
name: Lever, Felix
name: Kleiner, Reinhold
name: Koelle, Dieter
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Other Condensed Matter (cond-mat.other)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: Polarized light microscopy, as a contrast-enhancing technique for optically anisotropic materials, is a method well suited for the investigation of a wide variety of effects in solid-state physics, as for example birefringence in crystals or the magneto-optical Kerr effect (MOKE). We present a microscopy setup that combines a widefield microscope and a confocal scanning laser microscope with polarization-sensitive detectors. By using a high numerical aperture objective, a spatial resolution of about 240 nm at a wavelength of 405 nm is achieved. The sample is mounted on a $^4$He continuous flow cryostat providing a temperature range between 4 K and 300 K, and electromagnets are used to apply magnetic fields of up to 800 mT with variable in-plane orientation and 20 mT with out-of-plane orientation. Typical applications of the polarizing microscope are the imaging of the in-plane and out-of-plane magnetization via the longitudinal and polar MOKE, imaging of magnetic flux structures in superconductors covered with a magneto-optical indicator film via Faraday effect or imaging of structural features, such as twin-walls in tetragonal SrTiO$_3$. The scanning laser microscope furthermore offers the possibility to gain local information on electric transport properties of a sample by detecting the beam-induced voltage change across a current-biased sample. This combination of magnetic, structural and electric imaging capabilities makes the microscope a viable tool for research in the fields of oxide electronics, spintronics, magnetism and superconductivity.
description: 14 pages, 11 figures. The following article has been accepted by Review of Scientific Instruments. After it is published, it will be found at http://aip.scitation.org/journal/rsi
Chenopodium album Linn (Bathua): Review of Health Benefits
Creators: name: 1 Pallavi Tomar And 2 Verma Anisha
Publisher: name: The Science world a Monthly e magazine
Year: 2024

description: The plant bathua, or Chenopodium album, is a rich source of a wide range of nutrients, including minerals, vitamins, bioactive carbohydrates, flavonoids and phenolics, and anticancer, antidiabetic, anti-inflammatory, and antioxidant activities. The plant’s anthelmintic properties are partly attributed to ascaridole, a significant phytoconstituent found in the aerial sections of the plant. Despite widespread historical usage and substantial health advantages, its reputation has not grown, and consumption has sharply declined in recent years. The plant is now referred to as Non-conventional Edible plant (NCEP) gradually. Beyond its obvious nutritional advantages, C. album is a vegetable with significant functional potential that is underutilized. Traditionally, the plant has been utilized as an anthelmintic against round and hookworms, as well as bloodpurifier, diuretic, sedative, hepatoprotective and antiscorbutic laxative.
Berberine plays a positive metabolic role in polycystic ovary syndrome - insulin resistance by regulating gut microbiotas
Creators: name: Shen, Hao-Ran
Publisher: name: Zenodo
Year: 2019
Subjects: Polycystic ovary syndrome; insulin resistance; gut microbiota; berberine; treatment/amelioration

description: Objective: To investigate the treatment/amelioration effects of berberine on insulin resistance (IR) associated with polycystic ovary syndrome (PCOS). Methods: 16S amplicon and metabolomics analyses were performed on different groups of rat models treated with berberine. We used 16S amplicon analysis to demonstrate the microbiota with the quasi-likelihood (QL) F-test of the edgeR package. We performed different metabolite analysis using principal component analysis (PCA), partial least squares discrimination analysis (PLS-DA), and orthogonal partial least squares discrimination analysis (OPLS-DA). We then constructed a correlation network of different microbiotas and metabolites through relevance, and analyzed correlations between/among different microbiotas and metabolites. Results: We obtained a total of 43 different microbiota bacterial communities, including 20 bacteria that were up-regulated and 23 that were down-regulated at the genus level. Regarding co-occurrence, Alistipes and the Family_XIII_AD3011_group that rejected each other were found in Ruminiclostridium_6 and Tyzzerella. Metabolomics analysis produced a total of three different metabolites that included one up-regulated (glutamine) and two down-regulated (unsaturated acids, UFA [CH=CH] and glucose) metabolites, as well as 22 pathways (including type 2 diabetes mellitus, 2-component system, and streptomycin biosynthesis). We subsequently screened those with a significance level of less than 0.05. Integrational analysis results showed that Lachnospiraceae_NC2004_group, Flavonifractor, Parasutterella, glucose, and glutamine were directly regulated. A literature search revealed that the Lacchinospiraceae_NC2004_group, glucose, and glutamine were affected by berberine and exerted a treatment/amelioration effect on IR associated with PCOS. Akkermansia, Bacteroides, and glucose were also associated with IR. Conclusion: Our results suggest that berberine plays a positive role in the treatment/amelioration of PCOS by affecting gut microbiota, and can therefore modulate metabolism.
MOE11 Emittance Growth from the Thermalization of Space-Charge Nonuniformities
Creators: name: Lund, Steven M.
name: Barnard, John J.
name: Lee, Edward P.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: Beams injected into a linear focusing channel typically have some degree of space-charge nonuniformity. In general, injected particle distributions with systematic charge nonuniformities are not equilibria of the focusing channel and launch a broad spectrum of collective modes. These modes can phase-mix and have nonlinear wave-wave interactions which, at high space-charge intensities, results in a relaxation to a more thermal-like distribution characterized by a uniform density profile. This thermalization can transfer self-field energy from the initial space-charge nonuniformity to the local particle temperature, thereby increasing beam phase space area (emittance growth). In this paper, we employ a simple kinetic model of a continuous focusing channel and build on previous work that applied system energy and charge conservation quantify emittance growth associated with the collective thermalization of an initial azimuthally symmetric, rms matched beam with a radial density profile that is hollowed or peaked. This emittance growth is shown to be surprisingly modest even for high beam intensities with significant radial structure in the initial density profile.
description: Paper MOE11, XX International Linac Conference, Monterey, CA 21-25 August 2000 3 pages, 3 figures
title: ADCO, Comptes du Petit-Cîteaux (1477-1491) (11 H 1179), f. 00120
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/2019
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: cartulaire
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179), f. 00120, 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
Testing the Hypothesis of the Morphological Transformation from Field Spiral to Cluster S0
Creators: name: Kodama, Tadayuki
name: Smail, Ian
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Hubble Space Telescope observations of distant clusters have suggested a steep increase in the proportion of S0 galaxies between clusters at high redshifts and similar systems the present-day. It has been proposed that this increase results from the transformation of the morphologies of accreted field galaxies from spirals to S0s. We have simulated the evolution of the morphological mix in clusters based on a simple phenomenological model where the clusters accrete a mix of galaxies from the surrounding field, the spiral galaxies are transformed to S0s (through an unspecified process) and are added to the existing cluster population. We find that in order to reproduce the apparently rapid increase in the ratio of S0 galaxies to ellipticals in the clusters, our model requires that: (1) galaxy accretion rate has to be high (typically, more than half of the present-day cluster population must have been accreted since z~0.5), and (2) most of the accreted spirals, with morphological types as late as Scdm, must have transformed to S0's. Although the latter requirement may be difficult to meet, it is possible that such bulge-weak spirals have already been `pre-processed' into the bulge-strong galaxies prior to entering the cluster core and are eventually transformed into S0's in the cluster environment. On the basis of the evolution of the general morphological mix in clusters our model suggests that the process responsible for the morphological transformation takes a relatively long time (1-3Gyr) after the galaxy has entered the cluster environment.
description: 7 pages, 2 figures, Accepted for publication in MNRAS
Response functions and superfluid density in a weakly interacting Bose gas with non-quadratic dispersion
Creators: name: Keeling, Jonathan
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Motivated by the experimental search for Bose condensation of quasiparticles in semiconductors, the response functions of a weakly interacting Bose gas, with isotropic but non-quadratic dispersion, are considered. Non-quadratic dispersion modifies the definition of particle current, and leads to modified sum rules for the current-current response function. The effect of these modifications on the Berezhinski-Kosterlitz-Thouless transition is discussed.
description: 4 pages, 2 figures
title: ADCO, Ordre cistercien : comptes (1403-1423) (11 H 1161), f. 00227
Creators: name: de la Côte-d'Or, Archives départementales
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
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: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Ordre cistercien : comptes (1403-1423), Archives départementales de la Côte-d'Or, (11 H 1161). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien : comptes (1403-1423), Archives départementales de la Côte-d'Or, (11 H 1161), f. 00227, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
A two wire waveguide and interferometer for cold atoms
Creators: name: Hinds, E. A.
name: Vale, C. J.
name: Boshier, M. G.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: A versatile miniature de Broglie waveguide is formed by two parallel current-carrying wires in the presence of a uniform bias field. We derive a variety of analytical expressions to describe the guide and present a quantum theory to show that it offers a remarkable range of possibilities for atom manipulation on the sub-micron scale. These include controlled and coherent splitting of the wavefunction as well as cooling, trapping and guiding. In particular we discuss a novel microscopic atom interferometer with the potential to be exceedingly sensitive.
description: 17 pages, 5 figures, PDF
A Deep ROSAT HRI Observation of NGC 1313
Creators: name: Schlegel, Eric M.
name: Petre, Robert
name: Colbert, E. J. M.
name: Miller, Scott
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe a series of observations of NGC 1313 using the ROSAT HRI with a combined exposure time of 183.5 ksec. The observations span an interval between 1992 and 1998; the purpose of observations since 1994 was to monitor the X-ray flux of SN1978K, one of several luminous sources in the galaxy. No diffuse emission is detected in the galaxy to a level of ~1-2x10^37 ergs/s/arcmin^-2. A total of eight sources are detected in the summed image within the D_25 diameter of the galaxy. The luminosities of five of the eight range from \~6x10^37 to ~6x10^38 erg/s; these sources are most likely accreting X-ray binaries, similar to sources obseved in M31 and M33. The remaining three sources all emit above 10^39 erg/s. We present light curves of the five brightest sources. Variability is detected at the 99.9% level from four of these. We identify one of the sources as an NGC 1313 counterpart of a Galactic X-ray source. The light curve, though crudely sampled, most closely resembles that of a Galactic black hole candidate such as GX339-4, but with considerably higher peak X-ray luminosity. An additional seven sources lie outside of the D_25 diameter and are either foreground stars or background AGN.
description: 18 pages, 9 figures; accepted AJ, scheduled for November 2000
Additional file 1: of A PSTOL-like gene, TaPSTOL, controls a number of agronomically important traits in wheat
Creators: name: Milner, Matthew
name: Howells, Rhian
name: Craze, Melanie
name: Bowden, Sarah
name: Graham, Neil
name: Wallington, Emma
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: Table S1. Primers used in this study. (DOCX 33 kb)
D9.1. First report on TA provision
Creators: name: Puertas, Jerónimo
name: Ciambra, Andrea
name: Naves, Juan
name: Anta, Jose
Publisher: name: Zenodo
Year: 2023
Subjects: Co-UDlabs
Research Infrastructures
Transnational Access

description: This document is Deliverable D9.1 of the Co-UDlabs project, funded under the European Union's Horizon 2020 research and innovation programme under Grant Agreement No. 101008626. The Deliverable is included in Work Package 9, "Transnational Access Provision". The lead beneficiary of the Work Package is the University of A Coruña (Universidade da Coruña, UDC). UDC is the main author of this Deliverable.
The aim of this document is to provide a report of the TA Projects developed during the first call of Co-UDlabs' Transnational Access programme, carried out from March 2022, when 13 proposals out of the 15 submissions received were eventually selected, until July 2023, the official closing date of the first call.
Using Strong Gravitational Lensing to Identify Fossil Group Progenitors
Creators: name: Johnson, Lucas E.
name: Irwin, Jimmy A.
name: White, Raymond E.
name: Wong, Ka-Wah
name: Maksym, W. Peter
name: Dupke, Renato A.
name: Miller, Eric D.
name: Carrasco, Eleazar R.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Fossil galaxy systems are classically thought to be the end result of galaxy group/cluster evolution, as galaxies experiencing dynamical friction sink to the center of the group potential and merge into a single, giant elliptical that dominates the rest of the members in both mass and luminosity. Most fossil systems discovered lie within $z < 0.2$, which leads to the question: what were these systems' progenitors? Such progenitors are expected to have imminent or ongoing major merging near the brightest group galaxy (BGG) that, when concluded, will meet the fossil criteria within the look back time. Since strong gravitational lensing preferentially selects groups merging along the line of sight, or systems with a high mass concentration like fossil systems, we searched the CASSOWARY survey of strong lensing events with the goal of determining if lensing systems have any predisposition to being fossil systems or progenitors. We find that $\sim$13% of lensing groups are identified as traditional fossils while only $\sim$3% of non-lensing control groups are. We also find that $\sim$23% of lensing systems are traditional fossil progenitors compared to $\sim$17% for the control sample. Our findings show that strong lensing systems are more likely to be fossil/pre-fossil systems than comparable non-lensing systems. Cumulative galaxy luminosity functions of the lensing and non-lensing groups also indicate a possible, fundamental difference between strong lensing and non-lensing systems' galaxy populations with lensing systems housing a greater number of bright galaxies even in the outskirts of groups.
description: 14 pages, 6 figures, 2 tables, submitted to ApJ
Brahmanic Cyclic-Continuum Theory (BCCT): A Hypothesis Integrating Quantum Mechanics and Vedic Cosmology
Creators: name: Sahil, Tarapada
Publisher: name: Zenodo
Year: 2024
Subjects: subject: Physical cosmology
subject: Quantum physics
subject: Energy conversion

description: This hypothesis presents the Brahmanic Cyclic-Continuum Theory (BCCT), a speculative model that suggests the universe operates within a dual-state continuum of matter and consciousness. Based on principles from both quantum mechanics and Vedic cosmology, BCCT posits that consciousness is a fundamental force interacting with matter and energy, influencing cosmic cycles of expansion, preservation, and dissolution. The theory explores the potential for a self-aware, interconnected universe and offers a framework for explaining phenomena like the quantum measurement problem and dark energy. By merging scientific and spiritual insights, BCCT aims to provide a holistic view of cosmic evolution.
Surface Roughness Data.xlsx
Creators: name: Muflikhun, Muhammad
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 401799
subject: Mechanical engineering not elsewhere classified
classificationCode: 401401
subject: Additive manufacturing
classificationCode: 401406
subject: Machining
classificationCode: 401412
subject: Precision engineering

description: The data contained measurement of surface roughness data related to the hybrid manufacturing consist of additive manufacturing process and substractive process
High-temperature ferromagnetism of $sp$ electrons in narrow impurity bands: Application to CaB$_6$
Creators: name: Edwards, D. M.
name: Katsnelson, M. I.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Ferromagnetism with high Curie temperature $T_c$, well above room temperature, and very small saturation moment has been reported in various carbon and boron systems. It is argued that the magnetization must be very inhomogeneous with only a small fraction of the sample ferromagnetically ordered. It is shown that a possible source of high $T_c$ within the ferromagnetic regions is itinerant electrons occupying a narrow impurity band. Correlation effects do not reduce the effective interaction which enters the Stoner criterion in the same way as in a bulk band. It is also shown how, in the impurity band case, spin wave excitations may not be effective in lowering $T_c$ below its value given by Stoner theory. These ideas are applied to CaB$_6$ and a thorough review of the experimental situation in this material is given. It is suggested that the intrinsic magnetism of the B$_2$ and O$_2$ dimers might be exploited in suitable structures containing these elements.
description: 26 pages, 2 figures
Beyond the Illusion of Self: A Comparative Exploration of Jiddu Krishnamurti and Acharya Prashant's Pathways to Liberation
Creators: name: Bhushan Deore
Publisher: name: Bhushan Deore
Year: 2024
Subjects: J,Krishnamurti
Acharya Prashant
Advait Vedanta
Non-Dualism
spirituality
philosophy
Osho

description: This paper delves into the profound similarities between Jiddu Krishnamurti's and Acharya Prashant's philosophies, emphasizing their shared focus on the illusory nature of the self, the transformative power of awareness, and the rejection of belief systems as foundational to their teachings. Despite differences in their communication styles and backgrounds, a comparative analysis reveals how both teachers guide individuals towards a profound truth: liberation from the ego-driven mind opens a pathway towards an unbounded reality of pure awareness. Drawing from their talks, writings, and online resources, this paper provides a nuanced exploration of how these two influential spiritual figures encourage a radical shift in perception.