cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Cart. 198-01 (11 H 1055), 185 folios, f. 0048
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/2019
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0048, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0048, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
A Color-Magnitude Diagram for a Globular Cluster In the Giant Elliptical Galaxy NGC 5128
Creators: name: Harris, G. L. H.
name: Poole, G. B.
name: Harris, W. E.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Hubble Space Telescope has been used to obtain WFPC2 (V,I) photometry for a large sample of stars in the outer halo of the giant elliptical NGC 5128 (d = 4 Mpc). The globular cluster N5128-C44, at the center of the Planetary Camera field, is well enough resolved to permit the construction of a color-magnitude diagram (CMD) for it which covers the brightest two magnitudes of the giant branch. The CMD is consistent with that of a normal old, moderately low-metallicity ([Fe/H] = -1.30 globular cluster, distinctly more metal-poor than most of the field halo stars at the same projected location (which average [Fe/H] ~ -0.5). This is the most distant globular cluster in which direct color-magnitude photometry has been achieved to date, and the first one belonging to a giant E galaxy.
description: 12 pages, LaTeX, including 5 postscript figures; submitted to Astronomical Journal
Garcinia humilis C. D. Adams 1970
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Clusiaceae
Garcinia
Garcinia humilis

description: Rheedia lateriflora Linnaeus, Species Plantarum 2: 1193. 1753.
"Habitat in America." RCN: 3816.
Lectotype (Howard, Fl. Lesser Antilles 5: 327. 1989): [icon] " Vanrheedia " in Plumier, Nov. Pl. Amer.: 45, t. 18. 1703.
Generitype of Rheedia Linnaeus.
Current name: Garcinia humilis (Vahl) C.D. Adams (Clusiaceae).
Note: D’Arcy (in Ann. Missouri Bot. Gard. 67: 1014. 1981) treated unseen Plumier material, which he supposed to be in P, as type. Even if it exists, it would not have been seen by Linnaeus and would not have been original material for the name. Howard’s type choice is therefore accepted here.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 792, DOI: 10.5281/zenodo.291971
Development, implementation and application of thermo-hydro-mechanical coupling for soils in finite element analysis
Creators: name: Cui, Wenjie
Publisher: name: Imperial College London
Year: 2015

description: The effect of temperature on the behaviour of soils is a crucial problem in geothermal engineering as soils are subjected to the action of temperature variation in many diverse conditions. It is observed in both laboratory experiments and in situ tests that temperature variations can induce interaction between the thermal, hydraulic and mechanical behaviour of soils, which is known as thermo-hydro-mechanical (THM) coupling. In order to simulate the THM coupling, it is necessary to combine the equations governing heat transfer through the soil mass with the equations governing pore fluid flow through the soil skeleton, and the equations governing the stress-strain behaviour of the soil. Due to the complexities of the governing equations, the finite element (FE) method has been regarded as an appropriate numerical tool to solve THM coupled problems. In this thesis, all of the research has been carried out using the Imperial College Finite Element Program (ICFEP), which has been developed specifically for geotechnical engineering analysis. This thesis develops the governing equations for THM coupled analysis. It then describes the implementation of these equations for fully saturated soils in ICFEP. This theory has been applied to all types of elements in ICFEP, such as solid, beam, bar, joint, membrane and shell elements. Thermal boundary conditions relevant to geotechnical engineering have also been developed and implemented into ICFEP. A series of validation tests on the new facilities has been performed, and the results have been compared to those obtained using analytical and finite difference methods. To avoid numerical oscillations, the time-step constraints in coupled transient FE analyses, as well as an adequate mesh discretisation in highly convective coupled analysis, have been investigated. The findings from the analytical and numerical studies have been applied to a simulation of an open-loop ground source energy system, and the results show an excellent agreement with the available approximate solution.
Cosmological simulations of black hole growth II: how (in)significant are merger events for fuelling nuclear activity?
Creators: name: Steinborn, Lisa K.
name: Hirschmann, Michaela
name: Dolag, Klaus
name: Shankar, Francesco
name: Juneau, Stéphanie
name: Krumpe, Mirko
name: Remus, Rhea-Silvia
name: Teklu, Adelheid F.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Which mechanism(s) are mainly driving nuclear activity in the centres of galaxies is a major unsettled question. In this study, we investigate the statistical relevance of galaxy mergers for fuelling gas onto the central few kpc of a galaxy, potentially resulting in an active galactic nucleus (AGN). To robustly address that, we employ large-scale cosmological hydrodynamic simulations from the Magneticum Pathfinder set, including models for BH accretion and AGN feedback. Our simulations predict that for luminous AGN ($L_{\rm AGN} > 10^{45} {\rm erg/s}$) at $z = 2$, more than 50 per cent of their host galaxies have experienced a merger in the last 0.5~Gyr. These high merger fractions, however, merely reflect the intrinsically high merger fractions of massive galaxies at $z=2$, in which luminous AGN preferentially occur. Apart from that, our simulations suggest that merger events are not the statistically dominant fuelling mechanism for nuclear activity over a redshift range $z=0-2$: irrespective of AGN luminosity, less than 20 per cent of AGN hosts have on average undergone a recent merger, in agreement with a number of observational studies. The central ISM conditions required for inducing AGN activity can be, but are not necessarily caused by a merger. Despite the statistically minor relevance of mergers, at a given AGN luminosity and stellar mass, the merger fractions of AGN hosts can be by up to three times higher than that of inactive galaxies. Such elevated merger fractions still point towards an intrinsic connection between AGN and mergers, consistent with our traditional expectation.
description: 22 pages, 10 figures, accepted for publication in MNRAS, homepage: http://www.magneticum.org
Immunology of the neonatal lung and the long term consequences of neonatal respiratory virus infection for pulmonary innate immunity
Creators: name: Lambert, Laura
Publisher: name: Imperial College London
Year: 2015

description: Early life is a period of increased vulnerability to infection, particularly of the respiratory tract. The neonatal adaptive immune system is immature, with a bias towards Th2/Th17 responses and against Th1. Very little is understood about the innate response in early life, especially at mucosal surfaces such as the lung. To address this, Toll-like receptor (TLR) ligands were administered intranasally to neonatal and adult mice. In neonates, pulmonary neutrophilic influx was barely detectable, and expression of inflammatory chemokines greatly attenuated. Administration of exogenous CXCL1 elicited a strong neutrophilic response, indicating that diminished chemokine production is a limiting factor for cellular inflammation in early life. An unbiased microarray approach revealed that whilst expression of immune-related genes was mostly suppressed in the naïve neonatal lung, antimicrobial peptides such as cathelicidin were over-expressed. These novel findings challenge the perception that the infant immune system is simply an ‘immature’ version of the adult system, with implications for development of vaccines and adjuvants for this vulnerable population. An important respiratory pathogen of infants is respiratory syncytial virus (RSV), which can cause bronchiolitis, and in clinical studies is linked with lung dysfunction such as asthma and wheezing later in life. However, the mechanisms by which early life RSV infection could cause these delayed sequelae are unknown, and the effect on the innate immune response has not been explored. The long-term consequences of early life RSV infection were investigated using a murine model. Following neonatal RSV infection, allergen challenge resulted in an exaggerated inflammatory response in the adult murine lung, indicating that pulmonary innate immunity was dysregulated. Further, expression of various immune response, apoptosis-related and circadian rhythm genes was found to be altered. These data provide new evidence that infantile RSV has a causative effect on later lung dysfunction and identify gene targets for further investigation.
Additional file 1 of Genome-wide and expression analysis of B-box gene family in pepper
Creators: name: Ma, Jing
name: Dai, Jia-xi
name: Liu, Xiao-wei
name: Lin, Duo
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Table S1. Primer sequences used for real-time qRT-PCR amplification.
Additional file 1: of Risk patterns of lung cancer mortality in northern Thailand
Creators: name: Apinut Rankantha
name: Imjai Chitapanarux
name: Donsuk Pongnikorn
name: Sukon Prasitwattanaseree
name: Walaithip Bunyatisai
name: Patumrat Sripan
name: Patrinee Traisathit
Publisher: name: figshare
Year: 2018
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology

description: Appendix 1. The OpenBugs syntax for the BYM model fitting. (DOCX 13 kb)
COSMOLOGICAL CONSTRAINTS FROM CLUSTER X-RAY MORPHOLOGIES
Creators: name: Mohr, J. J.
name: Evrard, A. E.
name: Fabricant, D. G.
name: Geller, M. J.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use a representative sample of 65 galaxy clusters observed with the Einstein IPC to constrain the range of cluster X-ray morphologies. We develop and apply quantitative and reproducible measures to constrain the intrinsic distributions of emission weighted centroid variation, axial ratio, orientation, and the radial fall--off. We then use the range of cluster X--ray morphologies to constrain three generic cosmological models (Omega=1, Omega_0=0.2, and Omega_0=0.2 & lambda_0=0.8). For each of these models, we evolve eight sets of Gaussian random initial conditions consistent with an effective power spectrum $P(k)\propto k^{-1}$ on cluster scales. Using this sample of 24 numerical cluster simulations, we compare the X--ray morphologies of the observed and simulated clusters. The comparisons indicate that: (i) cluster centroid variations, axial ratios, and radial fall-offs are sensitive to the underlying cosmological model, and (ii) galaxy clusters with the observed range of X--ray morphologies are very unlikely in low Omega_0 cosmologies. The analysis favors the Omega=1 model, though some discrepancies remain. We discuss the effects of changing the initial conditions and including additional physics in the simulations.
description: uuencoded, compressed postscript, (mohr@cfa.harvard.edu)
Additional file 2 of Genome-wide and expression analysis of B-box gene family in pepper
Creators: name: Ma, Jing
name: Dai, Jia-xi
name: Liu, Xiao-wei
name: Lin, Duo
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2: Figure S1. Phylogenetic tree of BBX members from Capsicum annuum, Solanum lycopersicum, Arabidopsis thaliana, Oryza sativa  and Populus trichocarpa (Ca represent Capsicum annuum; Sl represent Solanum lycopersicum; At represent Arabidopsis thaliana; Os represent Oryza sativa; Pt represent Populus trichocarpa). The members marked in circle contain two B-BOX and one CCT domains, and in triangle contain two B-BOX domains (red represent Capsicum annuum; green represent Solanum lycopersicum; black represent Arabidopsis thaliana; purple represent Oryza sativa; blue represent Populus trichocarpa).
Ionization balance for optically thin plasmas: rate coefficients for all atoms and ions of the elements H to Ni
Creators: name: Mazzotta, P.
name: Mazzitelli, G.
name: Colafrancesco, S.
name: Vittorio, N.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present in this paper new and updated calculations of the ionization equilibrium for all the elements from H to Ni. We collected for these elements all the data available in the literature for the ionization and radiative plus dielectronic recombination rates. In particular, the dielectronic rates have been fitted with a single formula and the related coefficients are tabulated. Our results are compared with previous works.
description: 7 pages, 10 figures, 2 tables, accepted for publication in A&AS
Reminiscences of Meier Steinbrink, 1955
Publisher: name: Columbia University
Year: 2021
Subjects: Lawyers
Practice of law

description: Account of the Brooklyn bench and bar; Charles Evans Hughes, Selective Service Board of Appeals; investigation of aircraft industry, 1917; New York, N.Y. politics; notable cases, New York Supreme Court, 1932-1950; associates
Rheum compactum Linnaeus 1762
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rheum
Rheum compactum

description: Rheum compactum Linnaeus, Species Plantarum, ed. 2, 1: 531. 1762.
"Habitat in Tataria, China." RCN: 2929.
Type not designated.
Original material: [icon] in Miller, Fig. Pl. Gard. Dict. 2: 145, t. 218. 1758.
Current name: Rheum compactum L. (Polygonaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 792, DOI: 10.5281/zenodo.291971
Investigating the function of the non-coding RNAs miR-27b and Herna1 in pathologic cardiac hypertrophy
Creators: name: Bischof, Corinne
Publisher: name: Imperial College London
Year: 2016

description: Hypoxia inducible factor 1α (Hif1α) plays a key role in the induction and maintenance of heart disease and many direct Hif1α target genes have been identified. However, a number of genes show a Hif1α-dependent expression pattern although they lack the hypoxia response element (HRE) in their promoter for direct Hif1α binding. This work identified two modes of indirect gene regulation by Hif1α via a microRNA and enhancer RNA (eRNA), respectively, and their function in pathologic cardiac hypertrophy. Hif1α regulates the alpha subunit of ATP synthase, Atp5a1, through the induction of miR-27b. ATP synthase is a component of the respiratory chain and plays a key role in energy homeostasis. ATP synthase inactivation from yeast to man promotes cell growth coincident with ATP depletion. Accumulating mitochondrial ADP is redirected to methylenetetrahydrofolate dehydrogenase 1l (Mthfd1l) to drive DNA biosynthesis, karyokinesis and pathologic growth. In vivo gain- and loss-of-function studies, and correlative analysis of diseased human cohorts, confirm these findings to reveal a novel role for mitochondrial ATP synthase in cell and tissue growth control. Hif1α promotes transcription of Hif1α-activated eRNA 1 (HERNA1) from an active enhancer locus to confer spatio-temporal and signal-dependent control of gene expression in cardiac pathologies. Production of HERNA1 is initiated by direct HIF1α binding to an HRE motif in the promoter of the enhancer and confers hypoxia responsiveness to the nearby genes synaptotagmin XVII, a family member of membrane-trafficking and Ca2+-sensing proteins and SMG1, a phosphatidylinositol 3-kinase-related kinase involved in the control of nonsense-mediated mRNA decay (NMD). HERNA1, SMG1 and SYT17 expression correlate positively with distinct aetiologies of heart disease. Finally, Herna1 promotes the shift to glycolysis, contractile dysfunction and cardiac growth through Smg1 and/or Syt17.
Reminiscences of Melvin L. Krulewitch 1970
Publisher: name: Columbia University
Year: 2019
Subjects: Veterans
World War, 1914-1918
World War, 1939-1945--Naval operations, American
Korean War, 1950-1953

description: Family background, early years, education Columbia University, Columbia Law School; World War I enlisted service, recruit training, service in France, Belleau Wood, occupation duty in Germany; commissioned 1927, Marine Corps Reserve Program in 1930s, World War II, Boston Navy Yard, Marshalls, Saipan-Tinian, Iwo Jima; duty in Korea; personalities and events.
Reminiscences of Melville Henry Cane, 1956
Publisher: name: Columbia University
Year: 2021
Subjects: Poets
Lawyers
Law--United States
Copyright
Publishers and publishing
Poetics
American literature--20th century

description: Columbia University, 1900; legal practice specializing in copyright and publishing matters; recollections of Sinclair Lewis, John Erskine, Thomas Wolfe and Harry Houdini; commentary on writing poetry
Versatile Potential of Photo-Cross-Linkable Silk Fibroin: Roadmap from Chemical Processing Toward Regenerative Medicine and Biofabrication Applications
Creators: name: Jhaleh Amirian
name: Jacek K. Wychowaniec
name: Ehsan Amel Zendehdel
name: Gaurav Sharma
name: Agnese Brangule
name: Dace Bandere
Publisher: name: Zenodo
Year: 2023
Subjects: Biomimetic materials,Biopolymers,Fibers,Organic compounds

description: Over the past two decades, hydrogels have come to the forefront of tissue engineering and regenerative medicine due to their biocompatibility, tunable degradation and low immunogenicity. Due to their porosity and polymeric network built up, it is possible to incorporate inside drugs, bioactive molecules, or other biochemically active monomers. Among biopolymers used for the fabrication of functional hydrogels, silk fibroin (SF) has received considerable research attention owing to its known biocompatibility and tunable range of mechanical properties. However, its relatively simple structure limits the potential usability. One of the emerging strategies is a chemical functionalization of SF, allowing for the introduction of methacrylate groups. This allows the versatile processing capability, including photo-cross-linking, which makes SF a useful polymer as a bioink for 3D printing. The methacrylation reaction has been done using numerous monomers such as methacrylic anhydride (MA), 2-isocyanatoethyl methacrylate (IEM), or glycidyl methacrylate (GMA). In this Review, we summarize the chemical functionalization strategies of SF materials and their resulting physicochemical properties. More specifically, a brief explanation of the different functionalization methods, the cross-linking principles, possibilities, and limitations of methacrylate compound functionalization are provided. In addition, we describe types of functional SF hydrogels and link their design principles to the performance in applications in the broad fields of biofabrication, tissue engineering, and regenerative medicine. We anticipate that the provided guidelines will contribute to the future development of SF hydrogels and their composites by providing the rational design of new mechanisms linked to the successful realization of targeted biomedical application.
Bounds on current fluctuations in periodically driven systems
Creators: name: Barato, Andre C
name: Chetrite, Raphael
name: Faggionato, Alessandra
name: Gabrielli, Davide
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mathematical Physics (math-ph)
subject: Probability (math.PR)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: Small nonequilibrium systems in contact with a heat bath can be analyzed with the framework of stochastic thermodynamics. In such systems, fluctuations, which are not negligible, follow universal relations such as the fluctuation theorem. More recently, it has been found that, for nonequilibrium stationary states, the full spectrum of fluctuations of any thermodynamic current is bounded by the average rate of entropy production and the average current. However, this bound does not apply to periodically driven systems, such as heat engines driven by periodic variation of the temperature and artificial molecular pumps driven by an external protocol. We obtain a universal bound on current fluctuations for periodically driven systems. This bound is a generalization of the known bound for stationary states. In general, the average rate that bounds fluctuations in periodically driven systems is different from the rate of entropy production. We also obtain a local bound on fluctuations that leads to a trade-off relation between speed and precision in periodically driven systems, which constitutes a generalization to periodically driven systems of the so called thermodynamic uncertainty relation. From a technical perspective, our results are obtained with the use of a recently developed theory for 2.5 large deviations for Markov jump processes with time-periodic transition rates.
description: 23 pages, 3 figures
Additional file 3 of Genome-wide and expression analysis of B-box gene family in pepper
Creators: name: Ma, Jing
name: Dai, Jia-xi
name: Liu, Xiao-wei
name: Lin, Duo
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: Figure S2. Amino acid arrangement order of motif of BBX family.
Additional file 1: of Vaginal birth after caesarean birth in Italy: variations among areas of residence and hospitals
Creators: name: Colais, Paola
name: Bontempi, Katia
name: Pinnarelli, Luigi
name: Piscicelli, Carlo
name: Mappa, Ilenia
name: Fusco, Danilo
name: Davoli, Marina
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Marine Biology
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: List of codes used for selection of study population, outcome and comorbidities used for risk adjustment. The document contains the list of ICD-9-CM codes used for selection of study population, outcome and comorbidities used for risk adjustment (DOCX 19 kb)
Scalar product of twisted XXX modified Bethe vectors
Creators: name: Belliard, S.
name: Slavnov, N. A.
name: Vallet, B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider closed XXX spin chains with broken total spin $U(1)$ symmetry within the framework of the modified algebraic Bethe ansatz. We study multiple actions of the modified monodromy matrix entries on the modified Bethe vectors. The obtained formulas of the multiple actions allow us to calculate the scalar products of the modified Bethe vectors. We find an analog of Izergin-Korepin formula for the scalar products. This formula involves modified Izergin determinants and can be expressed as sums over partitions of the Bethe parameters.
description: 26 pages
Rheum palmatum Linnaeus 1759
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rheum
Rheum palmatum

description: Rheum palmatum Linnaeus, Systema Naturae, ed. 10, 2: 1010. 1759.
["Habitat in China ad murum. a. Dav. Gortero."] Sp. Pl., ed. 2, 1: 531 (1762). RCN: 2928.
Type not designated.
Original material: Herb. Linn. No. 520.3 (LINN).
Current name: Rheum palmatum L. (Polygonaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 792, DOI: 10.5281/zenodo.291971
Additional file 4 of Genome-wide and expression analysis of B-box gene family in pepper
Creators: name: Ma, Jing
name: Dai, Jia-xi
name: Liu, Xiao-wei
name: Lin, Duo
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 4: Figure S3. Expression profiles of CaBBX genes under different abiotic stresses. The first character C, F, H and N of the abbreviation on the bottom represent control, freezing, heat and NaCl treatment, respectively; the second character L and R represent leaf and root, respectively; the number 0, 0.1 and 0.2 represent 0h treatment; and the number 1, 2, 3, 4, 5 and 6 represent 1h, 1.5h, 3h, 6h, 12h and 24h treatment.
Localization transition for light scattering by cold atoms in an external magnetic field
Creators: name: Skipetrov, S. E.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: We establish a localization phase diagram for light in a random three-dimensional (3D) ensemble of motionless two-level atoms with a three-fold degenerate upper level, in a strong static magnetic field. Localized modes appear in a narrow spectral band when the number density of atoms $ρ$ exceeds a critical value $ρ_c \simeq 0.1 k_0^3$, where $k_0$ is the wave number of light in the free space. A critical exponent of the localization transition taking place upon varying the frequency of light at a constant $ρ> ρ_c$ is estimated to be $ν= 1.57 \pm 0.07$. This classifies the transition as an Anderson localization transition of 3D orthogonal universality class.
description: 5 pages, 3 figures + supplemental material
Dynamic state estimation under stressed conditions in modern power networks
Creators: name: Anagnostou, Georgios
Publisher: name: Imperial College London
Year: 2016

description: This thesis presents the way dynamic state estimation can be conducted in the context of power networks under stressed operating conditions, in order to enhance grid monitoring. Resilience is fundamental for modern power systems, which are experiencing significant changes; renewable energy based technologies diversify power generation, dramatically affecting system response to contingencies, whereas increased energy consumption, in combination with lack of investments and aged equipment, lead to system operation close to its limits. This stressed system operation is associated with the activation of limiting devices, such as overexcitation limiters, whose impact on the power system stability margin has been proven and quantified in this thesis. This is based on a dynamic security assessment (DSA) methodology developed in this context, and two stability limit metrics have been used, the critical clearing time (CCT) and the power limits (PLs). Having proven that the system stability margin is likely to decrease under stressed operating conditions, a stressed system conditions indicator has been proposed, considering the overexcitation limiter activation as an event denoting system stress. The proposed stress identification technique is based on Unscented Kalman filtering (UKF) dynamic state estimation, where phasor measurement units (PMUs) play a significant role in data transmission. In order to enhance the accuracy of power system monitoring, even in cases when limiting devices with unknown dynamics have been activated during stressed system operation, a novel UKF based dynamic state estimation algorithm has been developed in this thesis, considering unknown inputs in the power system models used. These studies have been carried out using two model power systems: A small 9-bus 3-machine system, and a large 68-bus 16-machine system.
COBE CONSTRAINTS ON KALUZA-KLEIN COSMOLOGIES
Creators: name: Faraoni, V.
name: Cooperstock, F. I.
name: Overduin, J. M.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A class of Kaluza-Klein cosmologies recently proposed is compared with observations of the cosmic microwave background. Some models are ruled out, while others turn out to be viable, with the number of extra dimensions being constrained by the COBE and Tenerife experiments.
description: 12 pages, LaTex, no figures
The X-ray Spectral Variability of the Seyfert Galaxy NGC 3227
Creators: name: George, I. M.
name: Mushotzky, R. F.
name: Turner, T. J.
name: Yaqoob, T.
name: Ptak, A.
name: Nandra, K.
name: Netzer, H.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (Abridged) We present the results from {\it ASCA} observations of NGC 3227 along with those from a {\it ROSAT} observation. The 0.6--10 keV continuum is consistent with a powerlaw with $Γ\sim 1.6$, flatter than that typically observed in Seyfert galaxies. Fe $K$-shell emission is observed with an EW and profile typical of Seyfert 1 galaxies. The {\it ASCA} observations in 1993 reveal absorption by a screen $N_{H,z}^{ion} \simeq 3\times10^{21} cm^{-2}}$ of ionized material with $U_X \simeq 0.01$. Joint analysis of the {\it ASCA} and {\it ROSAT} data show an additional screen of neutral material instrinsic to NGC 3227 with $N_{H,z}^{neu} \sim $few$\times10^{20} cm^{-2}}$. NGC 3227 exhibits spectral variability both within and between the observations, due to short-term variability in the continuum emission and longer-term variability in the absorption. Time-resolved spectroscopy show the continuum steepened by $ΔΓ\simeq 0.1$ during a flare of duration $\sim 10^4$s. The column increased by a factor of $\sim10$ by the 1995 epoch, while the continuum is consistent with that observed in 1993. The 1995 data also show evidence that the warm absorber allows $\sim$10% of the nuclear emission to escape without attenuation.
description: Accepted for publn in ApJ. LaTeX, 38 pages (inc 7 figs) & a PS file w/ 4 tables. For full abstract and other download options, see href="http://lheawww.gsfc.nasa.gov/~george/papers/3227/abstract.html
Cosmological parameters and the redshift distribution of gravitational lenses
Creators: name: Helbig, Phillip
name: Kayser, Rainer
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: For known gravitational lens systems the redshift distribution of the lenses is compared with theoretical expectations for $10^{4}$~Friedmann-Lema\^ıtre~cosmological models, which more than cover the range of possible cases. The comparison is used for assigning a relative probability to each of the models. The entire procedure is repeated for different values of the inhomogeneity parameter~$η$ and the limiting spectroscopic magnitude~$m_{\rm lim}$, which is important for selection effects. The dependence on these two parameters is examined in more detail for the special cases~$λ_{0}=0$ and $k=0$. Previous results that this method is a better probe for~$λ_{0}$ than $Ω_{0}$ are confirmed, but it appears that the low probability of models with large~$λ_{0}$~values found using similar methods is due to a selection effect. The power of this method to discriminate between cosmological models can of course be improved if more gravitational lens systems are found. However, our numerical simulations indicate that a reasonable number of observed systems cannot deliver interesting constraints on the cosmological parameters.
description: One self-unpacking uuencoded compressed PostScript file (created with uufiles) containing the complete text with all figures included (here 140kb gzipped, unpacked 975kb). 10 pages. Should be printable without loss on US-size paper. Paper version available on request. Changes--nothing removed, typos corrected, the following additions: one figure, one table and some text explaining the structure in the plots in more detail; more detailed explanation of the statistics used. Accepted by Astronomy and Astrophysics
X-ray Signatures of an Ionized Reprocessor in the Seyfert galaxy Ton S 180
Creators: name: Turner, T. J.
name: George, I. M.
name: Nandra, K.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss the hard X-ray properties of the Seyfert galaxy Ton S 180, based upon the analysis of ASCA data. We find the X-ray flux varied by a factor ~2 on a time scale of a few thousand seconds. The source showed significantly higher amplitude of variability in the 0.5-2 keV band than in the 2-10 keV band. The continuum is adequately parameterized as a Gamma ~ 2.5 power-law across the 0.6--10 keV band . We confirm the recent discovery of an emission line of high equivalent width, due to Fe K-shell emission from highly-ionized material. These ASCA data show the Fe line profile to be broad and asymmetric and tentatively suggest it is stronger during the X-ray flares, consistent with an origin from the inner parts of an accretion disk. The X-ray spectrum is complex below 2 keV, possibly due to emission from a blend of soft X-ray lines, which would support the existence of an ionized reprocessor, most likely due to a relatively high accretion rate in this source.
description: 24 pages, 8 figures. LaTeX with encapsulated postscript. To appear in the Astrophysical Journal
Domain walls in topological phases and the Brauer-Picard ring for $\operatorname{Vec}(\mathbb{Z}/p\mathbb{Z})$
Creators: name: Barter, Daniel
name: Bridgeman, Jacob C.
name: Jones, Corey
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Algebra (math.QA)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mathematical Physics (math-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: We show how to calculate the relative tensor product of bimodule categories (not necessarily invertible) using ladder string diagrams. As an illustrative example, we compute the Brauer-Picard ring for the fusion category $\operatorname{Vec}(\mathbb{Z}/p\mathbb{Z})$. Moreover, we provide a physical interpretation of all indecomposable bimodule categories in terms of domain walls in the associated topological phase. We show how this interpretation can be used to compute the Brauer-Picard ring from a physical perspective.
description: 16 pages, 1 figure, 3 tables, comments welcome
Ring structure and warp of NGC5907 -- Interaction with dwarf galaxies
Creators: name: Shang, Zhaohui
name: Zheng, Zhongyuan
name: Brinks, Elias
name: Chen, Jiansheng
name: Burstein, David
name: Su, Hongjun
name: Byun, Yong-IK
name: Deng, Licai
name: Deng, Zugan
name: Fan, Xiaohui
name: Jiang, Zhaoji
name: Li, Yong
name: Lin, Weipeng
name: Ma, Feng
name: Sun, Wei-hsin
name: Wills, Beverley
name: Windhorst, Rogier A.
name: Wu, Hong
name: Xia, Xiaoyang
name: Xu, Wen
name: Xue, Suijian
name: Yan, Haojing
name: Zhou, Xu
name: Zhu, Jin
name: Zou, Zhenlong
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The edge-on, nearby spiral galaxy NGC5907 has long been used as the prototype of a ``non-interacting'' warped galaxy. We report here the discovery of two interactions with companion dwarf galaxies that substantially change this picture. First, a faint ring structure is discovered around this galaxy that is likely due to the tidal disruption of a companion dwarf spheroidal galaxy. The ring is elliptical in shape with the center of NGC5907 close to one of the ring's foci. This suggests the ring material is in orbit around NGC5907. No gaseous component to the ring has been detected either with deep H$α$ images or in Very Large Array (VLA) HI 21-cm line maps. The visible material in the ring has an integrated luminosity <= 10^8 L_sun and its brightest part has a color R-I ~ 0.9. All of these properties are consistent with the ring being a tidally-disrupted dwarf spheroidal galaxy. Second, we find that NGC5907 has a dwarf companion galaxy, PGC54419, projected to be only 36.9 kpc from the center of NGC5907, close in radial velocity (ΔV = 45 km s^{-1}) to the giant spiral galaxy. This dwarf is seen at the tip of the HI warp and in the direction of the warp. Hence, NGC5907 can no longer be considered ``non-interacting,'' but is obviously interacting with its dwarf companions much as the Milky Way interacts with its dwarf galaxies. These results, coupled with the finding by others that dwarf galaxies tend to be found around giant galaxies, suggest that tidal interaction with companions, even if containing a mere 1% of the mass of the parent galaxy, might be sufficient to excite the warps found in the disks of many large spiral galaxies.
description: Accepted for publication in ApJL, 8 pages, AASTeX, 3 figures
Additional file 5 of Genome-wide and expression analysis of B-box gene family in pepper
Creators: name: Ma, Jing
name: Dai, Jia-xi
name: Liu, Xiao-wei
name: Lin, Duo
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 5: Figure S4. The classification of BBX genes investigated in 13 higher plants (A-E representative five different subclasses in the BBXs Groups I ~ V, respectively).
Reminiscences of Merwin H. Silverthorn 1969
Publisher: name: Columbia University
Year: 2019
Subjects: Veterans
World War, 1914-1918
World War, 1939-1945--Naval operations, American
Korean War, 1950-1953

description: Family background and education; World War I duty in France; Haiti, 1923-26; General Smedley Butler; Guam, 1930-32; Naval War College; Staff, Admiral Ernest King, Pacific Fleet, 1941-43; preparations for invasion of Japan, occupations of Japan and North China; demobilization; reorganization of Marine units in Pacific; mobilization of reserves for Korea; Assistant Commandant, United States Marine Corps, 1949-50; Chief of Staff, Headquarters Marine Corps, 1950-52, the Clifton Cates Commandancy.
Antibacterial effects of oak bark (Quercus robur) and heather herb (Calluna vulgaris L.) extracts against the causative bacteria of bovine mastitis
Creators: name: Renāte Šukele
name: Ingus Skadiņš
name: Rudīte Koka
name: Dace Bandere
Publisher: name: Zenodo
Year: 2022
Subjects: antibacterial, bovine mastitis, Escherichia coli, heather herb, in vitro, oak bark, Staphylococcus aureus, Streptococcus.

description: Bovine mastitis has a negative impact on animals, and improper antibiotic use has caused an increase in bacterial resistance. Therefore, medicinal plants could serve as an alternative treatment for this condition. Polyphenols have potential as antibiotic agents. Oak bark has long been used as a medicine and has shown antibacterial effects. Moreover, research on heather plant demonstrated that it has antibacterial properties. This study aimed to assess the antibacterial effects of oak (Quercus robur) bark and heather (Calluna vulgaris L.) herb extracts against common bovine mastitis pathogens.
Rheum rhabarbarum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rheum
Rheum rhabarbarum

description: Rheum rhabarbarum, spec. nov.
 2. Rheum foliis subvillosis, petiolis aequalibus. Diss. Rhabarb. 1. t.1. *
 Rheum foliis subvillosis. Hort. ups. 98. Mat. med. 197.
 Rhabarbarum sinense, folio crispo, flagellis rarioribus & minoribus. Amm. herb. 206.
 Rhabarbarum folio longiori hirsuto crispo, florum thyrso longiori & tenuiori. Amm. ruth.9.
 Acetosa montana, folio cubitali oblongiore crispo, floribus in subviridi luteolis. Messerschmidii. Amm. ruth. 226.
 Habitat in China ad murum & in Sibiria . ♃
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 372, DOI: 10.5281/zenodo.3931989
Additional file 1: of The cost-effectiveness and cost-utility of at-home infrared temperature monitoring in reducing the incidence of foot ulcer recurrence in patients with diabetes (DIATEMP): study protocol for a randomized controlled trial
Creators: name: Stegge, Wouter Aan De
name: Mejaiti, Nora
name: Netten, Jaap Van
name: Dijkgraaf, Marcel
name: Baal, Jeff Van
name: Busch-Westbroek, Tessa
name: Bus, Sicco
Publisher: name: figshare
Year: 2018
Subjects: Medicine
Marine Biology
Science Policy

description: Standard Protocol Items: Recommendations for Interventional Trial (SPIRIT) 2013 Checklist: recommended items to address in a clinical trial protocol and related documents. (PDF 57 kb)
LIMITS ON ANISOTROPY AND INHOMOGENEITY FROM THE COSMIC BACKGROUND RADIATION,
Creators: name: Maartens, Roy
name: Ellis, George F. R.
name: Stoeger, William R.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We consider directly the equations by which matter imposes anisotropies on freely propagating background radiation, leading to a new way of using anisotropy measurements to limit the deviations of the Universe from a Friedmann-Robertson-Walker (FRW) geometry. This approach is complementary to the usual Sachs-Wolfe approach: the limits obtained are not as detailed, but they are more model-independent. We also give new results about combined matter-radiation perturbations in an almost-FRW universe, and a new exact solution of the linearised equations.
description: 18 pages Latex.
Gaia and the Galactic Center Origin of Hypervelocity Stars
Creators: name: Brown, Warren R.
name: Lattanzi, Mario G.
name: Kenyon, Scott J.
name: Geller, Margaret J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We use new Gaia measurements to explore the origin of the highest velocity stars in the Hypervelocity Star Survey. The measurements reveal a clear pattern in the B-type stars. Halo stars dominate the sample at speeds about 100 km/s below Galactic escape velocity. Disk runaway stars have speeds up to 100 km/s above Galactic escape velocity, but most disk runaways are bound. Stars with speeds about 100 km/s above Galactic escape velocity originate from the Galactic center. Two bound stars may also originate from the Galactic center. Future Gaia measurements will enable a large, clean sample of Galactic center ejections for measuring the massive black hole ejection rate of hypervelocity stars, and for constraining the mass distribution of the Milky Way dark matter halo.
description: 10 pages, revised and accepted to ApJ
Coupled Topological Surface Modes in Gyrotropic Structures: Green's Function Analysis
Creators: name: Gangaraj, S. Ali Hassani
name: Monticone, F.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: At a transition in a wave-guiding structure, part of the incident energy is transmitted and part of the energy is reflected. When the waveguide has non-trivial topological properties, however, the transition may occur with no backscattering, and with unusual modal coupling/transformations. Within this context, we discuss the response of a nonreciprocal topological structure composed of two nearby interfaces between oppositely-biased gyrotropic media and an isotropic medium, which support unidirectional surface modes (topological modes). We provide an exact Green's function analysis of this structure, and we discuss how the topological surface modes are modified when the two interfaces are brought closer and eventually merged. We show that the resulting mode conversion is independent of the transition geometry.
Reminiscences of Michael Horowitz 1989
Publisher: name: Columbia University
Year: 2020
Subjects: Government executives--United States
Civil rights--United States
Student movements

description: Relationship with Allard Lowenstein; City College of New York student body president, 1958; involvement with National Student Association; Central Intelligence Agency; Mississippi Freedom Democratic Party formation, 1963; University of Mississippi, civil rights courses, 1967-68; disillusionment with Democratic party; general counsel in Office of Management and Budget, administration of Ronald Reagan