cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Reconstructing Positions and Peculiar Velocities of Galaxy Clusters within 20000 km/sec. I: The Cluster 3D Dipole
Creators: name: Branchini, E.
name: Plionis, M.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Starting from the observed distribution of galaxy clusters in redshift space we use a two--step procedure to recover their distances and peculiar velocities. After statistically correcting for the unobserved cluster distribution in the zone of avoidance ($|b|\le 20^{\circ}$) and also for a smooth absorption at higher $|b|$'s, we use a dynamical iterative algorithm to recover the real--space cluster positions by minimizing the redshift space distortions. The whole procedure assumes that clusters trace the mass, that peculiar velocities are caused by gravity and that linear perturbation theory applies. The amplitude of the cluster dipole measured in the 3D space turns out to be $\sim 23\%$ less than that measured in redshift space. In both cases the dipole direction is aligned with the Cosmic Microwave Background dipole within $\sim 10^{\circ}$, taking into account the Virgocentric infall component of the Local Group motion. Observational errors, limitations in the reconstruction procedure and the intrinsic cosmological variance, which is the dominant source of uncertainty, render a stringent determination of the $β$ parameter whose central value turns out to be $β\approx 0.2$ while its total uncertainty is $\pm 0.1$. This implies that for a cluster-mass bias parameter of $\sim 5$, a flat Universe is not excluded, contrary to previous cluster-dipole $z$-space analysis.
description: uuencoded-compressed-tarred PostScript file containing 17 pages + tables + 8 Figures.
Optimistic and pessimistic ambiguous chance constraints with applications
Creators: name: Roitch, Vladimir
Publisher: name: Imperial College London
Year: 2015

description: In this thesis, we consider optimisation problems which involve ambiguous chance constraints, i.e., probabilistic constraints where the probability distribution of the primitive uncertainties is at least partly unknown. In this case, we can define an ambiguity set that contains all distributions consistent with our prior knowledge of the uncertainty and take either a pessimistic (worst-case) or optimistic (best-case) view of the world. The former view can be used to actively optimise a system whilst guaranteeing some predefined level of safety; being robust even if the worst-case scenario materialises. The latter view can be used to actively optimise a system where it is required to reconstruct realisations of a random variable whose distribution is not known precisely. We characterise the ambiguity set through generalised moment bounds and structural properties such as symmetry, unimodality, or independence patterns. Sufficient conditions are presented under which the corresponding chance constraints admit equivalent explicit tractable conic reformulations that can be solved with off-the-shelf solvers. However, in general, ambiguous chance constrained problems are provably difficult and we suggest efficiently computable conservative approximations. To illustrate the effectiveness of our reformulations, we give two detailed and novel examples. First, we consider the pricing problem of a provider of cloud computing services. This provider faces uncertain demand and wishes to maximise profit, whilst maintaining a desired level of quality of service. We show that such a problem naturally fits within the pessimistic ambiguous chance constraint framework. Second, we consider the problem of improving the quality of a photographic image by reconstructing and then removing noise. We show that such a problem can be formulated as an optimistic ambiguous chance constrained program that generalises, and offers new insight to, an existing powerful image denoising approach.
Instability of stationary closed strings winding around flat torus in five-dimensional Schwarzschild spacetimes
Creators: name: Hasegawa, Mitsuharu
name: Ida, Daisuke
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Linear perturbations for a one parameter family of stationary, closed Nambu-Goto strings winding around a flat torus in the five-dimensional Schwarzschild spacetime have been studied. It has been shown that this problem is solvable in the sense that frequency spectra and perturbation modes can be expressed only with arithmetic operations and radicals. It has been proven that the Nambu-Goto strings belonging to this family are always unstable, no matter how they are located at almost flat region distant from the event horizon.
description: 12 pages, no figures
A Dust Lane in the Radio galaxy 3C270
Creators: name: Mahabal, Ashish
name: Kembhavi, Ajit
name: Singh, ; K. P.
name: Bhat, P. N.
name: Prabhu, ; T. P.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present broad band surface photometry of the radio galaxy 3C270 (NGC~4261). We find a distinct dust lane in the $V-R$ image of the galaxy, and determine its orientation and size. We use the major axis profile of the galaxy to estimate the optical depth of the dust lane, and discuss the significance of the lane to the shape of the galaxy.
description: To appear in ApJ. Added a plate and minor elaboration of a procedure. 17 pages in LaTeX. 6 figures and 2 plates not included. These and the paper are available by anonymous ftp at ftp://144.16.31.6/pub/n4261 and at http://iucaa.iucaa.ernet.in/~aam/www/papers/n4261
The differential role of regulatory B cells in cancer and allo-immunity
Creators: name: Sarvaria, Anushruti
Publisher: name: Imperial College London
Year: 2015

description: A new wave of research recognizes a distinct subset of B regulatory cells (Breg) that maintain immune tolerance. Breg cells have been shown to exert immunoregulatory functions through the production of interleukin (IL)-10 and appear to play important roles in autoimmunity and in cancer. Despite the extensive body of evidence reinforcing the notion of B cells as potential regulatory cells, some controversy over the paucity of markers that can unequivocally identify Bregs still exists. To study the role of Breg in immune surveillance, I designed a comprehensive multi‐parameter panel of surface antibodies to define B-cell subsets in peripheral blood (PB) and cord blood (CB). The intracellular detection of IL-10 combined with flow cytometric phenotyping presented in my thesis demonstrate the presence of IL-10– producing Bregs with Treg-independent immunosuppressive functions in both the IgM memory (CD19+IgM+CD27+) and transitional (CD19+CD24hiCD38hi) PB B-cell subsets in healthy donors. The regulatory function PB Bregs against CD4+T cells and CD56+NK cells required both cell-cell contact and IL-10 production. Moreover, I demonstrate that Breg populations are expanded in the PB of AML patients and exert potent suppression of NK function mediated through 2B4-CD48 signaling. I further demonstrated the presence of IL-10- producing B cells with Treg-independent immunosuppressive properties in CB with the ability to suppress allogeneic-CD4+T cells through IL-10, as well as cell-cell contact mediated mechanisms involving CTLA-4 and CD80/CD86. I found an early and robust recovery of IL-10+B cells post-CBT. High Breg frequencies in CB may attenuate T-cell responses and contribute to the lower rates of cGVHD. My findings have important clinical implications and suggest that Bregs may be exploited to treat immune-mediated diseases. Whereas, strategies to deplete Bregs for optimal anti-cancer immunotherapy may benefit antitumor activity in AML and other cancers, adoptive transfer of donor-derived Bregs post transplant may offer a potentially effective immunomodulatory therapy for the treatment of GVHD.
Additional file 7 of Whole-genome resequencing of three Coilia nasus population reveals genetic variations in genes related to immune, vision, migration, and osmoregulation
Creators: name: Gao, Jun
name: Xu, Gangchun
name: Xu, Pao
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 7.
Formation of Plumes in Head-on Collisions of Galaxies
Creators: name: Tsuchiya, Toshio
name: Korchagin, Vladimir
name: Wada, Keiichi
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using N-body and SPH modeling we perform 3D numerical simulations of head-on collisions between gas rich disk galaxies, including collisions between counter-rotating disks and off-center collisions. Pure stellar intruders do not produce gaseous plumes similar to those seen in the Cartwheel and VII Zw466 complexes of interacting galaxies; the presence of gas in an intruder galaxy and radiative cooling are important for the formation of a gaseous plume extending from the disk of a target galaxy. A noticeable plume structure can be formed if the mass of an intruder is a few percent of the mass of the primary. The halo of the intruder is stripped in the collision, and dispersed particles form a broad stellar bridge connecting the two galaxies. The fraction of the intruder's halo dispersed in the collision depends on the total mass of the intruder, and low-mass intruders lose most of their mass.
description: 15 pages, 14 figures in GIF. To appear ApJ. Vol. 505 #2
Numerical study of wings with wavy leading and trailing edges
Creators: name: Serson, Douglas
Publisher: name: Imperial College London
Year: 2016

description: Inspired by the pectoral flippers of the humpback whale, the use of spanwise waviness in wings has been considered in the literature as a possible way of delaying the stall, and possibly also reducing the drag coefficient, allowing for improved aerodynamic characteristics. In order to provide a better understanding of this flow control mechanism, the present work investigates numerically the effect of the waviness on the flow around infinite wings with a NACA0012 profile. The study consists of direct numerical simulations employing the spectral/hp method, which is available through the nektar++ library. Considering the high computational cost of the simulations performed, several improvements were introduced to the method, making it more efficient and allowing higher Reynolds numbers to be analysed. These improvements to the method include a coordinate transformation technique to treat the waviness, changes to the parallelism strategy, and an adaptive polynomial order refinement procedure. Initially, simulations were performed for a very low value of the Reynolds number Re=1,000, allowing the three-dimensional flow structures to be observed in detail. In this case, the results show that the waviness leads to a decrease in the lift-to-drag ratio, accompanied by a strong reduction in the fluctuations of the lift force. The reduction in the lift-to-drag ratio is the combined effect of lower drag and lift forces, and is associated with a regime where the flow remains attached behind the peaks of the leading edge while there are distinct regions of flow separation behind the troughs. Then, simulations with Re=10,000 were considered. For high angles of attack, the results for this case are similar to the lower Re, with the waviness leading to separation behind the troughs and reducing both the lift and the drag. However, for a lower angle of attack the waviness leads to a large increase in the lift coefficient. This was observed to be related to the fact that flow around the straight wing is laminar in this case, with the waviness inducing transition to a turbulent state. Finally, the case Re=50,000 was considered, with the results showing a good agreement with experiments presented in the literature.
Shell formation and star formation in superbubble DEM 192
Creators: name: Oey, M. S.
name: Smedley, S. A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Was star formation in the OB associations, LH 51 and LH 54, triggered by the growth of the superbubble DEM 192? To examine this possibility, we investigate the stellar contents and star formation history, and model the evolution of the shell. H-R diagrams constructed from UBV photometry and spectral classifications indicate highly coeval star formation, with the entire massive star population having an age of ~< 2-3 Myr. However, LH 54 is constrained to an age of ~3 Myr by the presence of a WR star, and the IMF for LH 51 suggests a lower-mass limit implying an age of 1-2 Myr. There is no evidence of an earlier stellar population to create the superbubble, but the modeled shell kinematics are consistent with an origin due to the strongest stellar winds of LH 54. It might therefore be possible that LH 54 created the superbubble, which in turn may have triggered the creation of LH 51. Within the errors, the spatial distribution of stellar masses and IMF appear uniform within the associations. We reinvestigate the estimates for stellar wind power L_w(t), during the H-burning phase, and note that revised mass-loss rates yield a significantly different form for L_w(t), and may affect stellar evolution timescales. We also model superbubble expansion into an ambient medium with a sudden, discontinuous drop in density, and find that this can easily reproduce the anomalously high shell expansion velocities seen in many superbubbles.
description: 18 pages, 12 figures, AASTeX; Figure 1 bitmapped. Accepted to AJ. Table of Contents and preprint, including hi-resolution version of Figure 1, available at: http://www.ast.cam.ac.uk/~oey/oeypubs.html
Crystal fields and Kondo effect: Magnetic susceptibility of Cerium ions in axial crystal fields
Creators: name: Desgranges, Hans-Ulrich
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The thermodynamic Bethe ansatz equations of the Coqblin-Schrieffer model have been solved numerically. The full N=6 (J=5/2) degeneracy of the Hund's rule ionic ground state of Ce is taken into account. Results for the temperature dependent magnetic susceptibility parallel and perpendicular to the crystal axis are presented. The deviations, due to the Kondo effect, to the non-interacting ion results are pointed out.
description: 4 pages, 2 figures, accepted for publication in Journal of Magnetism and Magnetic Materials
Mechanical performance of transparent laminated materials for aircraft
Creators: name: Wang, Yi
Publisher: name: Imperial College London
Year: 2016

description: To fully understand mechanical and structural performance of laminated glass, seven laminated cases were designed to assess the influence of glass types, polymer interlayer thickness, polymer interlayer types and multi-layered interlayer. An innovative apparatus combining 3D-Digital-Image-Correlation and ring on ring tests have been tested successfully, major strain and out of plane displacement at the supporting side were monitored. Novel sabot design helped the rubber projectile to eject without deformation in gas gun tests. The third innovative design was the gas gun system which allowed a stereo system of two high speed cameras for 3D-Digital-Image-Correlation and one camera monitoring impact performance, strain gauge system, and detecting velocity to be synchronised at the same time. Regarding major research findings, for monolithic glasses, an approximate 0.8% major failure strain was identified regardless of its thickness which was used as a failure criterion for laminated glass. For laminated glasses, an increase of thermoplastic-polyurethane thickness will allow laminate to absorb more energy at quasi static and low velocity ranges, but lower the supporting face strain at high velocity. Chemically strengthened glass used as frontal glass layer has better performance in terms of energy consumption in quasi static and low velocity ranges comparing to thermally strengthened glass. Different types of interlayer have different functionalities. Sentry-glass-plus is more rigid comparing thermoplastic-polyurethane and polyvinyl-butyral which can transfer more shear between layers and lower the strain at the back. However, it has poor adhesion on glass proven by large peeling off of the glass fragments after gas gun experiments. Comparing with polyvinyl-butyral, thermoplastic-polyurethane has good adhesive properties with Sentry-glass-plus and glass. A multi-layered interlayer system using structural Sentry-glass-plus and adhesive thermoplastic-polyurethane as interlayers can significantly reduce the strain during impact and prevent glass fragments from flying off at high velocity which is favourable in real scenarios (e.g. bird-strike).
Additional file 8 of QTL and candidate gene identification of the node of the first fruiting branch (NFFB) by QTL-seq in upland cotton (Gossypium hirsutum L.)
Creators: name: Zhang, Jingjing
name: Jia, Xiaoyun
name: Guo, Xiaohao
name: Wei, Hengling
name: Zhang, Meng
name: Wu, Aimin
name: Cheng, Shuaishuai
name: Cheng, Xiaoqian
name: Yu, Shuxun
name: Wang, Hantao
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 8: Figure S4. SNP and Indel mutations in the promoter regions of GhAPL and GhHDA5 genes. The red boxes represent the specific location of mutation sites.
The Mass Distribution of the Lens Galaxy in MG1131+0456
Creators: name: Chen, G. H.
name: Kochanek, C. S.
name: Hewitt, J. N.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of modeling 5, 8 and 15 GHz maps of the gravitational lens MG1131+0456 using the LensClean algorithm. Two models for the mass distribution in the lens were fit: a de Vaucouleurs model and a model with the two-dimensional potential phi = b^{2-alpha}(r^2+s^2)^{alpha/2}/2alpha, both in an external shear field. The best fit de Vaucouleurs model has an effective radius of R_e = 0.83+-0.13 arcseconds, larger than that measured at optical wavelengths. The best fit ``alpha model'' has alpha=0.6+-0.2 and a core radius of s = 0.19 +- 0.07 arcseconds. An isothermal model (alpha=1) is inconsistent with the data. The best alpha model fits the 8 GHz map significantly better than the best de Vaucouleurs model. Although it is difficult to distinguish visually the original image and the reconstructions, none of the models is statistically consistent with the data. We believe the primary problem is that an external shear is an inadequate model for the angular structure of the lens galaxy. The finite core radius in the models is required by the structure of the extended ring, so we confirm that the central component in the 8 GHz map is a central, lensed image of the source rather than the lens galaxy. The model lens positions, the position angle of the shear, and the mass interior to the ring are determined very precisely by the lens models. The time delay between the compact components is predicted with an uncertainty we estimate to be at most +- 9%; the formal uncertainty is +- 4%.
description: 47 pages. There are 2 Postscript files in the package.
Time Dilation in the Peak-to-Peak Time Scale of GRBs
Creators: name: Deng, Ming
name: Schaefer, Bradley E.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present strong evidence of time stretching in the peak-to-peak time scales in the light curves of BATSE Gamma Ray Bursts (GRBs). Extensive tests are performed on artificially dilated bursts to verify that the procedure for extracting the peak-to-peak time scales correctly recovers the stretching of bursts. The resulting robust algorithm is then applied to the 4B GRB database. We derive a stretching factor of $1.92 \pm 0.13$ between the brightest burst group ($P > 7.7 photon \cdot cm^{-2} \cdot s^{-1}$) and the dimmest burst group ($P = 1.0 \sim 1.4 photon \cdot cm^{-2} \cdot s^{-1}$) with several independent peak-to-peak time scale definitions and they agree within uncertainties. Such an agreement strongly supports the interpretation of the observed time stretching as time dilation caused by the cosmological expansion, rather than physical selection effects. We fit the result to cosmological models with $Λ= 0$, $Ω_{0}$ from 0.2 to 1.0, and contrained the standard candle luminosity to be $L_{0}= 7.0 \pm 2.0 \pm 2.7 \times 10^{56} photons \cdot s^{-1}$. Our luminosity value is fully consistent with the value from the combined PVO and BATSE LogN-LogP curve with the BATSE bright bursts at low redshifts of $z_{bright} = 0.11 \pm 0.02 \pm 0.025$. This luminosity fit is definitely inconsistent with the the larger distance scale implied from associating burst density with star formation rates.
description: 17 pages, 3 figures, Submitted to ApJL
Targeting Schlemm’s canal endothelium to modulate aqueous humour outflow facility as a potential treatment for glaucoma
Creators: name: Reina Torres, Ester
Publisher: name: Imperial College London
Year: 2016

description: Glaucoma is an ocular neurodegenerative disease generally associated to sustained elevated intraocular pressure (IOP). Lowering IOP is the only suitable therapeutic strategy for glaucoma but current treatments do not target the root cause of elevated IOP: increased aqueous humour outflow resistance. The mechanisms involved in outflow resistance generation are not fully understood. It is thought that resistance is generated at the vicinity of the juxtacanalicular connective tissue, the inner wall of Schlemm’s canal (SC) and its basement membrane. We hypothesise that the continuity of SC endothelium, and especially its pores, are key regulators of outflow resistance. To test this hypothesis, we assessed the role of physiological processes known to be relevant for pore formation by measuring changes in outflow facility (C) using the newly developed iPerfusion system. First, we showed that vascular endothelial growth factor (VEGF) is involved in C regulation and that steroid-treated mice have altered VEGF signaling, potentially contributing to outflow dysfunction and ocular hypertension. Second, we demonstrated that down regulation of plasmalemmal vesicle-associated protein results in reduced C, probably because of impaired ability to form intracellular pores. Third, we proved that the inhibition of tight junction related proteins results in increased C and lower IOP. Additionally, we also examined the effects of anesthetics on IOP and we propose a new protocol to measure IOP by rebound tonometry. Altogether, these studies support the idea that the inner wall of SC plays a crucial regulatory role in aqueous humour outflow resistance. Therefore, targeting SC endothelium and more precisely the mechanisms of pore formation may provide a new therapeutic approach for ocular hypertension.
In vitro and in vivo molecular analysis of cyclooxygenase-2 (COX-2)-dependent and COX-2 independent cytoprotective pathways in the vascular endothelium
Creators: name: Alrashed, Fahad Abdulaziz M
Publisher: name: Imperial College London
Year: 2016

description: Purpose: Non-steroidal anti-inﬂammatory drugs (NSAIDs) are important for limiting pain and inﬂammation, although many increase the risk of cardiovascular events including myocardial infarction, stroke and heart failure. However, celecoxib (a selective COX-2 inhibitor), has been associated with a more positive cardiovascular proﬁle. We explored the hypothesis that celecoxib induces anti-oxidant and anti-inﬂammatory genes in the vascular endothelium via AMP kinase (AMPK), thereby limiting inﬂammation-mediated injury. Methods/Results: In vitro cultured human umbilical vein endothelial cells were studied. Our results indicate that celecoxib induces cytoprotective genes; including heme oxygenase-1 (HO-1) and manganese superoxide dismutase (MnSOD). Importantly, these observations were reproduced in human aortic endothelial cells. In contrast, the traditional NSAIDs (ibuprofen and naproxen) failed to reproduce the cytoprotective actions of celecoxib. Subsequently, we found celecoxib increased expression of additional cytoprotective genes (Bcl-2, FHC, DAF and TXNRD1) in vitro, and importantly, celecoxib treatment of C57BL/6 mice led to increased HO-1 and ferritin heavy chain (FHC) expression in the aortic endothelium in vivo. The actions of celecoxib were shown to be independent of COX-2 by using dimethyl-celecoxib, which lacks COX-2 inhibitory properties and reproduced celecoxib’s cytoprotective effects. Mechanistically, celecoxib led to the generation of mitochondrial reactive oxygen species, which activated AMPK leading to HO-1 and MnSOD induction. Celecoxib treatment led to AMPKα (Thr172) and CREB (Ser133) phosphorylation via a linear pathway, and the nuclear translocation of NRF-2. The effects of celecoxib were inhibited by siRNA-mediated depletion of AMPKα1, CREB-1 and NRF2. Further functional analyses revealed celecoxib to inhibit, via activation of AMPK, TNFα-mediated phosphorylation of NF-κB p65, p65 nuclear translocation, TNFα-induced VCAM-1 expression and IL-1β-induced IL-6 mRNA expression. Conclusion: Our data demonstrate that celecoxib regulates cytoprotective gene expression in ECs via a novel mtROS-AMPK-CREB-Nrf2-dependent pathway. A deeper understanding of the mechanisms of action of NSAIDs will inform clinical practice and ultimately assist the development of safer therapeutics.
Additional file 1: of Grouping of nanomaterials to read-across hazard endpoints: from data collection to assessment of the grouping hypothesis by application of chemoinformatic techniques
Creators: name: L. Lamon
name: D. Asturiol
name: A. Richarz
name: E. Joossens
name: R. Graepel
name: K. Aschberger
name: A. Worth
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Science Policy
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Grouping of nanomaterials to read-across hazard endpoints: from data collection to assessment of the grouping hypothesis by application of chemoinformatic techniques. (DOCX 1335 kb)
Rheum undulatum 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 undulatum

description: Rheum undulatum Linnaeus, Species Plantarum, ed. 2, 1: 531. 1762.
"Habitat in China, Sibiria." RCN: 2927.
Type not designated.
Original material: [icon] in Linnaeus, Amoen. Acad. 3: 212, t. 4. 1751; [icon] in Amman, Stirp. Rar. Ruth.: 9. 1739.
Current name: Rheum undulatum 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
Reminiscences of Milton S. Eisenhower 1969
Publisher: name: Columbia University
Year: 2020
Subjects: Educators
Government executives--United States
Presidents--Election--1952.--United States

description: Dwight D. Eisenhower as president; decision to run, 1952 convention; Nixon as Vice-presidential candidate, selection of cabinet; Senator Joseph McCarthy, public sentiment; military-industrial complex
TURBULENCE IN MOLECULAR CLOUDS
Creators: name: Dubinski, John
name: Narayan, Ramesh
name: Phillips, T. G.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We generate random Gaussian turbulent velocity fields with a Kolmogorov spectrum and use these to obtain synthetic line-of-sight velocity profiles. The profiles are found to be similar to line profiles observed in molecular clouds. We suggest methods for analysing measured line profiles to test whether they might arise from Gaussian Kolmogorov turbulence.
description: accepted in ApJ, compressed postscript, figures not included. Complete preprint available at http://ucowww.ucsc.edu/~dubinski/home.html or by request to dubinski@lick.ucsc.edu
Drag-based CME modeling with heliospheric images incorporating frontal deformation: ELEvoHI 2.0 - supplementary material
Creators: name: Hinterreiter, Jürgen
name: Amerstorfer, Tanja
name: Temmer, Manuela
name: Reiss, Martin
name: Weiss, Andreas
name: Moestl, Christian
name: Barnard, Luke
name: Pomoell, Jens
name: Bauer, Maike
name: Amerstorfer, Ute
Publisher: name: figshare
Year: 2021
Subjects: subject: Solar System, Solar Physics, Planets and Exoplanets
subject: 20109 Space and Solar Physics
subject: FOS: Physical sciences

description: These supplementary material belongs to the Study "Drag-based CME modeling with heliospheric images incorporating frontal deformation: ELEvoHI 2.0" by Hinterreiter et al.
The files contain movies and results plots of ELEvoHI ensemble simulations for a coronal mass ejections on 3 February 2010. Additionally, the solutions of the three ambient solar wind models (HUX, HUXt, EUHFORIA) are provided.
Reminiscences of Milton Meltzer, 1978
Publisher: name: Columbia University
Year: 2021
Subjects: Authors
Student movements
Depressions--1929--New York (State)
New Deal, 1933-1939

description: Early life, education, Worcester, Mass.; New York, N.Y. during the Depression; college experiences and radical political movements at New College, Columbia, 1932-36; beginnings as a writer; work for the Works Progress Administration Federal Theater Project, 1936-39; VIOLINS AND SHOVELS
Additional file 11 of Whole-genome resequencing of three Coilia nasus population reveals genetic variations in genes related to immune, vision, migration, and osmoregulation
Creators: name: Gao, Jun
name: Xu, Gangchun
name: Xu, Pao
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 11.
title: ADCO, Grènetier de Cîteaux : comptes (1499-1503) (11 H 1173), f. 00726
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: Petot, Frédéric
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173), f. 00726, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Formation of undermassive single white dwarfs and the influence of planets on late stellar evolution
Creators: name: Nelemans, G.
name: Tauris, T. M.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We propose a scenario to form low-mass, single, slow rotating white dwarfs from a solar-like star accompanied by a massive planet, or a brown dwarf, in a relatively close orbit (e.g. HD 89707). Such white dwarfs were recently found by Maxted & Marsh (1998). When the solar-like star ascends the giant branch it captures the planet and the subsequent spiral-in phase expels the envelope of the giant leaving a low-mass helium white dwarf remnant. In case the planet evaporizes, or fills its own Roche-lobe, the outcome is a single undermassive white dwarf. The observed distribution of planetary systems supports the applicability of this scenario.
description: 4 pages, accepted for publication in A&A letters
Additional file 3 of Machine Learning for detection of viral sequences in human metagenomic datasets
Creators: name: Bzhalava, Zurab
name: Tampuu, Ardi
name: BaĹA, Piotr
name: Vicente, Raul
name: Dillner, Joakim
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 60506 Virology

description: Methods description in detail. (DOCX 19 kb)
THERMAL RADIATION FROM MAGNETIZED NEUTRON STARS: A look at the Surface of a Neutron Star.
Creators: name: Page, Dany
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Surface thermal emission has been detected by ROSAT from four nearby young neutron stars. Assuming black body emission, the significant pulsations of the observed light curves can be interpreted as due to large surface temperature differences produced by the effect of the crustal magnetic field on the flow of heat from the hot interior toward the cooler surface. However, the energy dependence of the modulation observed in Geminga is incompatible with blackbody emission: this effect will give us a strong constraint on models of the neutron star surface.
description: 10 pages. tar-compressed and uuencoded postcript file. talk given at the `Jubilee Gamow Seminar', St. Petersburg, Sept. 1994.
Attributes of Gravitational Lensing Parallax
Creators: name: Nemiroff, Robert J.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The density of stars and MACHOs in the universe could theoretically be determined or limited by simultaneous measurements of compact sources by well separated observers. A gravitational lens effect would be expected to create a slight differential amplification between the observers detectable with sufficiently sensitive relative photometry: "lensing parallax." When applied to expanding fireballs such as those from GRBs and supernovae, the mass of the lens can be indicated by the end of lensing parallax, when the angular size of the source becomes much greater than the angular size of the Einstein ring of the lens.
description: 7 pages, to be published in Astrophysics and Space Science
Acisanthera quadrata Pers.
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
Myrtales
Melastomataceae
Acisanthera
Acisanthera quadrata

description: Rhexia acisanthera Linnaeus, Systema Naturae, ed. 10, 2: 998. 1759.
["Habitat in Jamaica."] Sp. Pl., ed. 2, 1: 491 (1762). RCN: 2651.
Lectotype (designated here by Cellinese): Browne, Herb. Linn. No. 483.2 (LINN).
Current name: Acisanthera quadrata Pers. (Melastomataceae).
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
Enhancing the efficiency of density functionals with a novel iso-orbital indicator
Creators: name: Furness, James W
name: Sun, Jianwei
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Due to its efficiency and reasonable accuracy, density functional theory is one of the most widely used electronic structure theories in condensed matter physics, materials physics, and quantum chemistry. The accuracy and efficiency of a density functional is dependent on the basic ingredients it uses, and how the ingredients are built into the functional as a whole. An iso-orbital indicator based on the electron density, its gradients, and the kinetic energy density, has proven an essential dimensionless variable that allows density functionals to recognise and correctly treat various types of chemical bonding, both strong and weak. Density functionals constructed around the iso-orbital indicator usually require dense real-space grids for numerical implementation that deteriorate computational efficiency, with poor grid convergence compromising the improved accuracy. Here, a novel iso-orbital indicator is proposed based on the same ingredients that retains the capability to identify the same chemical bonds while significantly relieving the requirement of dense grids, and giving an improved recognition for tail regions of electron densities. The novel iso-orbital indicator is therefore expected to be the prime choice for further density functional development.
Additional file 10 of Whole-genome resequencing of three Coilia nasus population reveals genetic variations in genes related to immune, vision, migration, and osmoregulation
Creators: name: Gao, Jun
name: Xu, Gangchun
name: Xu, Pao
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 10.
Rhexia mariana Linnaeus 1753
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
Myrtales
Melastomataceae
Rhexia
Rhexia mariana

description: Rhexia mariana Linnaeus, Species Plantarum 1: 346. 1753.
"Habitat in Marilandia." RCN: 2650.
Lectotype (James in Brittonia 8: 224. 1956): [icon] " Lysimachia non papposa Terrae Marianae, leptoneurophyllos, flore tetrapetalo rubello, folio & caule hirsutie ferruginea hispidis " in Plukenet, Amalth. Bot.: t. 428, f. 1. 1705; Almag. Mant.: 123. 1700. - Typotype: Herb. Sloane 92: 90 (BM-SL).
Current name: Rhexia mariana L. (Melastomataceae).
Note: A detailed discussion is provided by Reveal & al. (in Huntia 7: 227. 1987).
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
COBE Constraints on Baryon Isocurvature Models
Creators: name: Hu, Wayne
name: Bunn, Emory F.
name: Sugiyama, Naoshi
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We consider Bayesian constraints on standard isocurvature baryon models from the slope and normalization of the anisotropy power spectrum detected by the COBE DMR experiment in their two year maps. In conjunction with either the amplitude of matter fluctuations $σ_8$ {\it or} its slope, all open models are ruled out at greater than 95\% confidence, whereas cosmological constant $Λ$ dominated models are constrained to be highly ionized. By including the COBE FIRAS 95\% confidence upper limit on spectral distortion, we further reduce the available parameter space for $Λ$ models by excluding these highly ionized models. These constraints define a single class of barely viable standard models which makes definite and testable predictions for degree scale anisotropies and large scale structure.
description: 9 pgs, uuencoded-tarred postscript
Finanzialisiertes Wohnen - Zuhause bei börsennotierten Wohnungsunternehmen am Beispiel Vonovia in Leipzig Connewitz
Creators: name: Postert, Luise
Publisher: name: Zenodo
Year: 2022
Subjects: Vonovia
Finanzialisierung
Börsennotierte Wohnungsunternehmen
Wohnentfremdung
ontologische Sicherheit

description: Forschungsarbeit zum Wohnen bei börsennotierten Wohnungsunternehmen am Beispiel Vonovia in Leipzig-Connewitz. Dabei werden die Auswirkungen dieser Wohnerfahrungen auf den Zustand ontologischer Sicherheit der Bewohnerschaft untersucht.
Reminiscences of Mimi Perr, Susan Andrews, and Barbara Bernstein 1990
Publisher: name: Columbia University
Year: 2020
Subjects: Campaign management
Presidents--Election--1972.--United States
Judaism

description: Recollections of Allard K. Lowenstein: personality, political philosophy, ambitions, relations with friends, family, discussion of personal conflicts with Judaism, congressional campaigns, California, New York, 1966-1976: impact of anti-Communism, problems with district choices, opponents, anecdotes about various campaigns; support of Edward M. Kennedy's presidential campaign, 1976
Additional File 9:
Creators: name: Thobani Ntshiqa
name: Musekiwa, Alfred
name: Mandla Mlotshwa
name: Mangold, Kerry
name: Reddy, Carl
name: Williams, Seymour
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Table S3. Access to media and exposure to HIV Communication Programmes among young women aged 16â 24Â years, National HIV Communication Survey, South Africa, 2012, Frequency distribution table showing Access to media and exposure to HIV Communication Programmes among Sexually Active Young Women in South Africa with percentages and Chi-square Inferences, Access to media and exposure to HIV Communication Programmes (DOCX 16 kb)
title: ADCO, Grènetier de Cîteaux : comptes (1499-1503) (11 H 1173), f. 00158
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
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes

description: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173), f. 00158, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Reminiscences of Miriam Massey Johnson 1988
Publisher: name: Columbia University
Year: 2020
Subjects: Women teachers
Educators
Antisemitism

description: Recollections of Allard Lowenstein: early friendship at the University of North Carolina, Chapel Hill; participation in Encampment, 1947; developing relationship; Lowenstein's family life; influence of Dr. Frank Graham; effect of anti-semitism and other subtle biases on his political aspirations; Lowenstein's influence on her courtship with Guy Benton Johnson
Additional File 8:
Creators: name: Thobani Ntshiqa
name: Musekiwa, Alfred
name: Mandla Mlotshwa
name: Mangold, Kerry
name: Reddy, Carl
name: Williams, Seymour
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Figure S6. Media sources accessed by young women aged 16â 24Â years, National HIV Communication Survey, South Africa, 2012, Graphical presentation of media sources accessed by young women using percentages, Media sources. (DOCX 28 kb)
Additional file 1 of Whole-genome resequencing of three Coilia nasus population reveals genetic variations in genes related to immune, vision, migration, and osmoregulation
Creators: name: Gao, Jun
name: Xu, Gangchun
name: Xu, Pao
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1.
The Influence of Parameters on the Flow Structure in Semidetached Binary Systems: 3D Numerical Simulation
Creators: name: Bisikalo, D. V.
name: Boyarchuk, A. A.
name: Kuznetsov, O. A.
name: Chechetkin, V. M.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The basic parameters determining the flow pattern for a nonviscous, non-heat-conducting gas in a semidetached binary system without a magnetic field are identified. Three-dimensional gas-dynamical modeling of the mass transfer enables investigation of the influence of these parameters on the structure of gas flows. The parameter on which the flow pattern depends most strongly is the adiabatic index $γ$. The effect of other parameters is small, and only leads to unimportant quantitative changes in the solutions obtained. The main properties of flows typical of semidetached binaries without magnetic fields are summarized.
description: 16 pages, LaTeX, 8 EPS figures, using AAS2PP4 style, accepted by Astron. Reports
Think then act or act then think?
Creators: name: Jędrzejewski, Arkadiusz
name: Marcjasz, Grzegorz
name: Nail, Paul R.
name: Sznajd-Weron, Katarzyna
Publisher: name: arXiv
Year: 2018
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: We introduce a new agent-based model of opinion dynamics in which binary opinions (yes/no) of each agent can be measured and described regarding both pre- and post-influence at both of two levels, public and private, vis-à-vis the influence source. The model combines ideas introduced within the $q$-voter model with noise, proposed by physicists, with the descriptive, four-dimensional model of social response, formulated by social psychologists. We investigate two versions of the same model that differ only by the updating order: an opinion on the public level is updated before an opinion on the private level or vice versa. We show how the results on the macroscopic scale depend on this order. The main finding of this paper is that both models produce the same outcome if one looks only at such a macroscopic variable as the total number of the individuals with positive opinions. However, if also the level of internal harmony (viz., dissonance) is measured, then significant, qualitative differences are seen between these two versions of the model. All results were obtained simultaneously within Monte Carlo simulations and analytical calculations. We discuss the importance of our studies and findings from three points of view: the theory of phase transitions, agent-based modeling of social systems, and social psychology.
description: 24 pages, 5 figures, corrected typos and the algorithm description, extended Methods and results section, replaced Fig. 1., added supporting materials with derivations, layout issues solved