cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Unravelling the complex magnetic structure of multiferroic pyroxene NaFeGe2O6: A combined experimental and theoretical study
Creators: name: Ding, Lei
name: Manuel, Pascal
name: Khalyavin, Dmitry D.
name: Orlandi, Fabio
name: Tsirlin, Alexander A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Magnetic order and the underlying magnetic model of the multiferroic pyroxene NaFeGe2O6 are systematically investigated by neutron powder diffraction, thermodynamic measurements, density-functional bandstructure calculations, and Monte-Carlo simulations. Upon cooling, NaFeGe2O6 first reveals one-dimensional spin-spin correlations in the paramagnetic state below about 50 K, revealed by magnetic diffuse scattering. The sinusoidal spin-density wave with spins along the a-direction sets in at 13 K, followed by the cycloidal configuration with spins lying in the (ac) plane below 11.6 K. Microscopically, the strongest magnetic coupling runs along the structural chains, J1 ' 12 K, which is likely related to the one-dimensional spin-spin correlations. The interchain couplings J2 ' 3:8K and J3 ' 2:1K are energetically well balanced and compete, thus giving rise to the incommensurate order in sharp contrast to other transition-metal pyroxenes, where one type of the interchain couplings prevails. The magnetic model of NaFeGe2O6 is further completed by the weak single-ion anisotropy along the a-direction. Our results resolve the earlier controversies regarding the magnetic order in NaFeGe2O6 and establish relevant symmetries of the magnetic structures. These results, combined with symmetry analysis, enable us to identify the possible mechanisms of the magnetoelectric coupling in this compound. We also elucidate microscopic conditions for the formation of incommensurate magnetic order in pyroxenes.
description: 10 pages 10 figures, PRB(accepted)
Rubia peregrina subsp. longifolia 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
Gentianales
Rubiaceae
Rubia
Rubia peregrina
Rubia peregrina l. subsp. longifolia (poir.)

description: Rubia lucida Linnaeus, Systema Naturae, ed. 12, 2: 732. 1767.
"Habitat in Majorca. D. Richard." RCN: 892.
Lectotype (Natali & Jeanmonod in Jeanmonod, Compl. Prodr. Fl. Corse, Rubiaceae: 167. 2000): Herb. Linn. No. 131.5 (LINN).
Current name: Rubia peregrina L. subsp. longifolia (Poir.) O. Bolòs (Rubiaceae).
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 800, DOI: 10.5281/zenodo.291971
Second class currents and T violation in quasielastic neutrino and antineutrino scattering from nucleons
Creators: name: Fatima, A.
name: Athar, M. Sajjad
name: Singh, S. K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The effect of the second class currents with and without time reversal invariance has been studied in the quasielastic production of nucleons and hyperons induced by neutrinos and antineutrinos from the nucleons. The numerical results are presented for the total scattering cross section~($σ$) as well as for the longitudinal, perpendicular and transverse components of the polarization of the final baryons ($p$, $n$, $Λ$, $Σ^-$, $Σ^0$) and muon produced in the quasielastic (anti)neutrino-nucleon scattering induced by the weak charged current. In the case of the production of $Λ$ hyperon, which is the most suitable candidate for making the polarization measurements, we have also calculated the $Q^2$ dependence of the polarization observables and the differential scattering cross section ($dσ/dQ^2$). The measurement of the polarization observables and their $Q^2$ dependence provides an independent way to determine the nucleon-hyperon transition form factors at high $Q^2$ which can provide tests of the symmetries of the weak hadronic currents like G-invariance, T invariance and SU(3) symmetry.
description: 29 pages, 17 figures, 1 table
Additional file 6: of Linkage analysis and QTL mapping in a tetraploid russet mapping population of potato
Creators: name: Massa, Alicia
name: Manrique-Carpintero, Norma
name: Coombs, Joseph
name: Haynes, Kathleen
name: Bethke, Paul
name: Brandt, Tina
name: Gupta, Sanjay
name: G. Yencho
name: Novy, Richard
name: Douches, David
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Figure S2. Linkage maps of chromosome 5. A: C5 overall map. The blue bar corresponds to the two-LOD support interval for the QTL location. B: C5 overall map; H1 − H4 homologous maps of ‘Rio Grande Russet’; H5 − H8 homologous maps of ‘Premier Russet’. (PDF 93 kb)
Optimally driven quantum systems
Creators: name: Verdeny Vilalta, Albert
Publisher: name: Imperial College London
Year: 2015

description: Periodically driven quantum systems offer an exceptional platform for quantum simulations due to the possibility to approximate their dynamics in terms of time-independent effective Hamiltonians. This, together with the recent experimental advances, has situated driven systems at center stage of engineered quantum-mechanical devices. The aim of this thesis is to develop theoretical methods in order to design optimal quantum simulations with driven systems. By applying the derived tools to experimentally relevant models, the applicability and significance of the methods are furthermore demonstrated. First, we introduce a method to derive accurate effective Hamiltonians by merging two seemingly unrelated tools: Floquet theory and flow equations. With this, the required analytical identification of the effective Hamiltonian in terms of the system's parameters is achieved. Second, we identify structural properties that determine the accessible effective dynamics of a system of particles on shaken optical lattices, which is arguably one of the most remarkable systems for many-body quantum simulations. In particular, we identify fundamental symmetries of the underlying lattice geometry that determine the emergence of new tunneling processes. Third, we develop an optimal control scheme to design polychromatic driving protocols that optimally simulate specifically targeted dynamics. We apply this scheme to demonstrate an optimal realization of Raman transitions with a Lambda system, a building block in many quantum simulations. Then, we employ it to implement a topological Chern insulator through suitably engineering the geometry-dependent tunneling of particles on a shaken hexagonal lattice. Hereby, a realistic route to experimentally test strongly-correlated topological phases of matter is provided. By determining structural properties of driven systems and suitable driving protocols, the methods described in this thesis open substantial possibilities for the development of optimal quantum simulations and, ultimately, reliable quantum technologies.
Rubia peregrina Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Rubia
Rubia peregrina

description: Rubia peregrina, spec. nov.
 2. Rubia foliis quaternis. Roy. lugdb. 254.
 Rubia quadrifolia asperrima lucida peregrina. Herm. lugdb. 523.
 Habitat - - - - ♃
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 109, DOI: 10.5281/zenodo.3931989
Additional file 3: of Overlapping group screening for detection of gene-gene interactions: application to gene expression profiles with survival trait
Creators: name: Jie-Huei Wang
name: Yi-Hau Chen
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: A reference manual for the â OGSâ package. (PDF 77 kb)
OH(1720 MHz) Masers As Signposts of Molecular Shocks
Creators: name: Frail, Dale A.
name: Mitchell, George F.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present observations of molecular gas made with the 15-m James Clark Maxwell Telescope toward the sites of OH(1720 MHz) masers in three supernova remnants: W28, W44 and 3C391. Maps made in the 12CO J=3-2 line reveal that the OH masers are preferentially located along the edges of thin filaments or clumps of molecular gas. There is a strong correlation between the morphology of the molecular gas and the relativistic gas traced by synchrotron emission at centimeter wavelengths. Broad CO line widths (dV=30-50 km/s) are seen along these gaseous ridges, while narrow lines are seen off the ridges. The ratio of H2CO line strengths is used to determine temperatures in the broad-line gas of 80 K, and the 13CO J=3-2 column density suggests densities of 10^4-10^5 cm{-3}. These observations support the hypothesis that the OH(1720 MHz) masers originate in post-shock gas, heated by the passage of a supernova remnant shock through dense molecular gas. From the observational constraints on the density, velocity and magnetic field we examine the physical properties of the shock and discuss the shock-production of OH. These OH(1720 MHz) masers are useful ``signposts'', which point to the most promising locations to study supernova remnant/molecular cloud interactions.
description: ApJ (in press)
code for DEM simplification (The peer-reviewed publication on IJGIS: An integrated method for DEM simplification with terrain structural features and smooth morphology preserved)
Creators: name: Yu, Wenhao
name: Zhang, Yifan
Publisher: name: figshare
Year: 2020

description: As a key focus of cartography and terrain analysis,
the simplification of a digital elevation model (DEM) is used to preserve the
pattern features of the terrain surface while suppressing its details over multiple
scales. Statistical filtering and structural analysis methods are commonly used
for this process. The structural analysis method performs well in
identifying terrain structural edges, while it tends to discard the smooth morphology
of a terrain surface. In addition, the filter that aims to reduce noise on a
surface may over-smooth the terrain structural edges. Therefore, to preserve
both the terrain structural edges and smooth morphology, we propose to combine
the techniques of statistical filtering and structural analysis. Specifically,
all the critical elevation points and structural edges are first detected from the
DEM surface by using the structural analysis method. Then, the iterative guided
normal filter is used to smooth the generalized DEM with the guidance of the
structure of the original surface. After this process, the terrain structure is
retained in the smooth surface of the DEM. The experimental results with a
real-world dataset show that our method can inherit the merits of both
structural analysis and statistical filter in preserving terrain
features for multi-scale DEM representations.
Low-complexity algorithms for automatic detection of sleep stages and events for use in wearable EEG systems
Creators: name: Imtiaz, Syed Anas
Publisher: name: Imperial College London
Year: 2015

description: Objective: Diagnosis of sleep disorders is an expensive procedure that requires performing a sleep study, known as polysomnography (PSG), in a controlled environment. This study monitors the neural, eye and muscle activity of a patient using electroencephalogram (EEG), electrooculogram (EOG) and electromyogram (EMG) signals which are then scored in to different sleep stages. Home PSG is often cited as an alternative of clinical PSG to make it more accessible, however it still requires patients to use a cumbersome system with multiple recording channels that need to be precisely placed. This thesis proposes a wearable sleep staging system using a single channel of EEG. For realisation of such a system, this thesis presents novel features for REM sleep detection from EEG (normally detected using EMG/EOG), a low-complexity automatic sleep staging algorithm using a single EEG channel and its complete integrated circuit implementation. Methods: The difference between Spectral Edge Frequencies (SEF) at 95% and 50% in the 8-16 Hz frequency band is shown to have high discriminatory ability for detecting REM sleep stages. This feature, together with other spectral features from single-channel EEG are used with a set of decision trees controlled by a state machine for classification. The hardware for the complete algorithm is designed using low-power techniques and implemented on chip using 0.18μm process node technology. Results: The use of SEF features from one channel of EEG resulted in 83% of REM sleep epochs being correctly detected. The automatic sleep staging algorithm, based on contextually aware decision trees, resulted in an accuracy of up to 79% on a large dataset. Its hardware implementation, which is also the very first complete circuit level implementation of any sleep staging algorithm, resulted in an accuracy of 98.7% with great potential for use in fully wearable sleep systems.
Reminiscences of William H. Simpson, 1972
Publisher: name: Columbia University
Year: 2020
Subjects: Veterans
World War, 1939-1945--Campaigns--Africa, North
World War, 1939-1945--Campaigns--France
Ardennes, Battle of the, 1944-1945

description: With Dwight Eisenhower and others in training; World War II: Africa, 1942, invasion of France, Brest, 1944; Battle of the Bulge; crossing the Rhine; Russian occupation of Berlin
Optimisation of T cell receptors using in vivo recombination and selection
Creators: name: Ghani, Hazim
Publisher: name: Imperial College London
Year: 2016

description: The αβT cell receptor (TCR) orchestrates immunity through the recognition of peptides, derived from degraded proteins, presented on major histocompatibility complex (MHC) molecules. The remarkable ability of the receptor to respond to a vast plethora of antigens is driven by V(D)J recombination, a process which generates a highly diverse TCR repertoire by somatic gene rearrangement of coding DNA. TCR diversity is confined to three short hairpin loops on each TCR chain, called the complementarity determining region (CDR), which form the antigen-binding site. The germline-encoded CDR1 and CDR2 loops predominantly contact MHC, whereas the hypervariable CDR3 are non-germline and primarily bind to the MHC-bound peptide. In this study, we developed a novel in vivo mutagenesis approach which redirects somatic gene rearrangement using V(D)J recombination machinery to diversify and optimise TCR binding. This approach involves embedding a gene recombination cassette into the peptide-binding CDR3β region of established TCRs. A retrogenic system was employed to facilitate the in vivo processes necessary for gene rearrangement and thymic selection. We demonstrate that the recombination cassette can successfully induce gene rearrangement and introduce variation to the targeted CDR3β site. Thymocytes expressing the diversified TCRs can be selected on MHC and develop into functional peripheral T cells. Subsequent exposure to cognate ligands also allowed us to identify optimised and ‘immunodominant’ TCRs. In addition, we produced a novel chimeric TCR chain which comprises Vα and Cβ domains. This TCR chain forms a heterodimer with endogenous TCRα chains to form a unique Vα-Vα antigen-binding surface. Thymocytes expressing this novel form of αβTCR were able to engage efficiently with both MHC classes and develop normally into functional T cells typical of a conventional repertoire. Collectively, these findings suggest that the germline CDR loops are not essential for mediating MHC recognition during MHC-restricted T cell development and function.
Stable and Unstable Accretion Flows with Angular Momentum near a Point Mass
Creators: name: Ryu, Dongsu
name: Brown, Garry L.
name: Ostriker, Jeremiah P.
name: Loeb, Abraham
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The properties of axisymmetric accretion flows of cold adiabatic gas with zero total energy in the vicinity of a Newtonian point mass are characterized by a single dimensionless parameter, the thickness of incoming flow. In the limit of thin accretion flows with vanishing thickness, we show that the governing equations become self-similar, involving no free parameters. We study numerically thin accretion flows with finite thickness as well as those with vanishing thickness. Mass elements of the incoming flow enter the computational regime as thin rings. In the case with finite thickness, after a transient period of initial adjustment, an almost steady-state accretion shock with a small oscillation amplitude forms, confirming the previous work by Molteni, Lanzafame, \& Chakrabarti (1994). The gas in the region of vorticity between the funnel wall and the accretion shock follows closed streamlines, forming a torus. This torus, in turn, behaves as an effective barrier to the incoming flow and supports the accretion shock which reflects the incoming gas away from the equatorial plane. The postshock flow, which is further accelerated by the pressure gradient behind the shock, goes through a second shock which then reflects the flow away from the symmetry axis to form a conical outgoing wind. As the thickness of the inflowing layer decreases (or if the ratio of the half thickness to the distance to the funnel wall along the equatorial plan is smaller than $\sim0.1$), the flow becomes unstable. In the case with vanishing thickness, the accretion shock formed to stop the incoming flow behind the funnel wall oscillates quasi-periodically with an amplitude comparable to the thickness. The structure between the funnel wall and the accretion shock is destroyed as the shock moves inwards toward the central mass and re-generated
description: ApJ accepted, 23 pages, uuencoded, compressed postscript file, 11 figures available upon request from ryu@sirius.chungnam.ac.kr
Reminiscences of William Harvey Allen, 1950
Publisher: name: Columbia University
Year: 2021
Subjects: Social workers
Social problems--20th century.--United States

description: Youth and education; Universities of Chicago and Pennsylvania; Association for Improving the Condition of the Poor, 1903-07; Bureau of Municipal Research, 1907-14; Rockefeller Foundation and Carnegie Foundation; Training School for Public Service, 1911-14; University of Wisconsin Survey; Dr. Charles Van Hise; Institute for Public Service; New York City Municipal Civil Service Commission, 1934-37; New York state and city politics; impressions of Fiorello La Guardia, James Walker, and Thomas E. Dewey
Reminiscences of William Hammatt Davis, 1958
Publisher: name: Columbia University
Year: 2021
Subjects: New Deal, 1933-1939
Labor unions
World War, 1939-1945--Manpower

description: Work as Deputy Administrator and Compliance Director of National Recovery Administration; New York State Mediation Board; work as Chairman of National Defense Mediation Board and War Labor Board; impressions of James Byrnes, John L. Lewis, Herbert Lehman, George Meany, Robert Wagner and Robert Taft
Hydrogen Electron Capture in Accreting Neutron Stars and the Resulting g-Mode Oscillation Spectrum
Creators: name: Bildsten, Lars
name: Cumming, Andrew
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate hydrogen electron capture in the oceans of neutron stars accreting at rates appropriate for most Low-Mass X-Ray Binaries. These stars burn the accreted hydrogen and helium unstably in the upper atmosphere and accumulate material which usually contains some small amount of hydrogen (mass fractions are typically 10%) mixed in with the heavier iron group ashes. The subsequent evolution of this matter is determined by compression towards higher densities until electron capture on the hydrogen occurs. We construct steady-state models of the electron captures and the subsequent neutron recombinations onto the heavy nuclei. The density discontinuity from these captures gives rise to a new g-mode (much like a surface wave), which has a lowest order (l=1) frequency of 35 Hz when X=0.1 on a slowly rotating star. We also discuss, for the first time, a new set of non-radial g-modes unique to these neutron stars. These modes have most of their nodes in the finite thickness layer where the electron captures are occurring. The lowest order mode frequencies are in the 1-10 Hz range for a few radial nodes on a slowly rotating star. We conclude by discussing how the dispersion relations for these modes are modified for a rapidly rotating neutron star. Whether any of these modes are observable depends on their excitation and damping mechanisms and the ability to excite them, issues we will address in a future paper.
description: 46 pages, LaTex, 20 figures, to Appear in The Astrophysical Journal, October 20, 1998
title: ADCO, Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Cart. 29 (G 134), 996 folios, f. 0196
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0196, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0196, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Wave-optical treatment of the shadow cast by a large gravitating sphere
Creators: name: Turyshev, Slava G.
name: Toth, Viktor T.
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study the shadow cast by a large gravitating sphere, similar to our Sun. For this, we consider the gravitational field produced by a static mass monopole within the first post-Newtonian approximation of the general theory of relativity. We study the propagation of a monochromatic electromagnetic wave in the vicinity of a large, opaque, gravitating sphere. To treat the opaque nature of the body and its physical size, we implement fully absorbing boundary conditions and develop a wave-optical treatment of the shadow formed by this object. Based on this approach, we demonstrate that the structure of the shadow is determined by the Schwarzschild radius of the body and its physical size. The shadow's boundary has the shape of a concave rotational hyperboloid bent inward due to the refractive properties of the curved spacetime. We show that there is no light in the shadow. However, even in the presence of gravity and related gravitational bending of photon trajectories there is the bright spot of Arago that is formed behind a perfectly spherical obscuration.
description: 16 pages, 3 figures
Rubia peregrina 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
Gentianales
Rubiaceae
Rubia
Rubia peregrina

description: Rubia peregrina Linnaeus, Species Plantarum 1: 109. 1753.
"Habitat - - - –” RCN: 891.
Lectotype (Natali & Jeanmonod in Jeanmonod, Compl. Prodr. Fl. Corse, Rubiaceae: 162. 2000): Herb. A. van Royen No. 908.221-523 (L).
Current name: Rubia peregrina L. (Rubiaceae).
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 800, DOI: 10.5281/zenodo.291971
Reminiscences of William Howard Schuman, 1977
Publisher: name: Columbia University
Year: 2021
Subjects: Conductors (Music)
Composers
Music--Instruction and study
Conservatories of music--United States
Composition (Music)
Music--Performance

description: Childhood, education, career; conception, revision, perfomances of each of his major works; choral conducting, composition for film, for dance; innovations and conflicts as administrator of Juilliard School of Music, President, 1945-1962, emeritus, 1962- , and Lincoln Center, President, 1962-1969, emeritus, 1969- ; opinions and anecdotes of many figures in the performing arts, including Serge Koussevitzky, Roy Harris, Leopold Stokowski, Peter Mennin
A Study of the Large--Scale Distribution of Galaxies in the South Galactic Pole Region: I. The Data
Creators: name: Ettori, S.
name: Guzzo, L.
name: Tarenghi, M.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the data from an extensive, moderately deep (b_J = 19.5) spectroscopic survey of $\sim 600$ galaxies within four regions of sky located near the South Galactic Pole. About 75% of the measured galaxies are in a 3deg x 1.5deg region dominated by the rich cluster Klemola 44 (Abell 4038). The other three smaller areas cover about 1 square degree each. Here we discuss in detail the observing and data reduction strategies, the completeness and errors on the measured redshifts. The data collected are being used for: (1) a study of the large--scale redshift distribution of the galaxies in each field, and (2) a thorough dynamical investigation of Klemola 44. Results from these analyses will be presented in forthcoming papers.
description: 7 MN-style text pages + 5 reduced-size tables, all in uu-compressed- tarred PS format. 16 figures available in hardcopy from the authors. MNRAS, in press
MOESM4 of Physiciansâ utilization of microbiologic reports and determinants of their preference to order culture in Tikur Anbessa Specialized Hospital, Addis Ababa, Ethiopia
Creators: name: Getachew Alemkere
name: Getu Gilagil
name: Teklu Gebrehiwot
name: Zelalem Tilahun
name: Hylemariam Mengist
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: Hematology

description: Additional file 4. Microbiologic reports available and/or used for therapy adjustment in hospitalized patients in the internal medicine ward of TASH in 2014, Addis Ababa, Ethiopia.
A 1.4 GHz radio continuum and polarization survey at medium Galactic latitudes: I. Observation and reduction technique
Creators: name: Uyaniker, B.
name: Fuerst, E.
name: Reich, W.
name: Reich, P.
name: Wielebinski, R.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A radio continuum survey at medium Galactic latitudes with the Effelsberg 100-m telescope is being carried out at a centre frequency of 1.4 GHz in total power and linear polarization. Areas up to +/- 20 degree of Galactic latitude are now being observed at a sensitivity of 15 mK TB total intensity and 8 mK TB in linear polarization with an angular resolution of 9'35. This paper describes the observing and reduction technique applied which results in absolutely calibrated maps. The methods are illustrated by examples of images from the survey.
description: 12 pages, 9 figures, Accepted for publication in Astronomy and Astrophysics Supp. Ser
Initial Shock Waves for Explosive Nucleosynthesis in Type II Supernova
Creators: name: Nagataki, S.
name: Hashimoto, M.
name: Yamada, S.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have performed 1-dimensional calculations for explosive nucleosynthesis in collapse-driven supernova and investigated its sensitivity to the initial form of the shock wave. We have found the tendency that the peak temperature becomes higher around the mass cut if the input energy is injected more in the form of kinetic energy rather than internal energy. Then, the mass cut becomes larger, and, as a result, neutron-rich matter is less included in the ejecta; this is favorable for producing the observational data compared with a previous model. Our results imply that the standard method to treat various processes for stellar evolution, such as convection and electron capture during the silicon burning stage, are still compatible with the calculation of explosive nucleosynthesis.
description: 20 pages, 6 figures, LaTex
EVOLUTION OF IR-SELECTED GALAXIES IN Z~0.4 CLUSTERS
Creators: name: Stanford, S. A.
name: Eisenhardt, P. R. M.
name: Dickinson, Mark
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Wide-field optical and near--IR ($JHK$) imaging is presented for two rich galaxy clusters: Abell~370 at $z=0.374$ and Abell~851 (Cl0939+47) at $z=0.407$. Galaxy catalogs selected from the near--IR images are 90\% complete to approximately 1.5 mag below $K^\ast$ resulting in samples with $\sim$100 probable member galaxies per cluster in the central $\sim$2 Mpc. Comparison with $HST$ WFPC images yields subsamples of $\sim$70 galaxies in each cluster with morphological types. Analysis of the complete samples and the $HST$ subsamples shows that the $z\sim 0.4$ E/S0s are bluer than those in the Bower et al.\ (1992) Coma sample in the optical$-K$ color by $0.13$~mag for Abell~370 and by $0.18$~mag for Abell~851. If real, the bluing of the E/S0 populations at moderate redshift is consistent with that calculated from the Bruzual and Charlot (1993) models of passive elliptical galaxy evolution. In both clusters the intrinsic scatter of the known E/S0s about their optical$-K$ color--mag relation is small ($\sim 0.06$ mag) and not significantly different from that of Coma E/S0s as given by Bower et al.\ (1992), indicating that the galaxies within each cluster formed at the same time at an early epoch.
description: uuencoded gzipped tar file containing latex files of manuscript (42 pages) plus tables (9 pages); figures available by anonymous ftp at ftp://ipac.caltech.edu//pub/pickup/sed ; accepted for publication in the ApJ
Supplementary document for Monolithic integration of multicolor InGaN LEDs with uniform luminescence emission - 5438701.pdf
Creators: name: Liu, Xianhe
name: Sun, Yi
name: Malhotra, Yakshita
name: wu, yuanpeng
name: Mi, Zetian
Publisher: name: Optica Publishing Group
Year: 2021
Subjects: Uncategorized

description: Supplemental Document
High Ratio of 44Ti/56Ni in Cas A and Axisymmetric Collapse-Driven Supernova Explosion
Creators: name: Nagataki, S.
name: Hashimoto, M.
name: Sato, K.
name: Yamada, S.
name: Mochizuki, Y. S.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The large abundance ratio of $^{44}Ti/^{56}Ni$ in Cas A is puzzling. In fact, the ratio seems to be larger than the theoretical constraint derived by Woosley & Hoffman (1991). However, this constraint is obtained on the assumption that the explosion is spherically symmetric, whereas Cas A is famous for the asymmetric form of the remnant. Recently, Nagataki et al. (1997) calculated the explosive nucleosynthesis of axisymmetrically deformed collapse-driven supernova. They reported that the ratio of $^{44}Ti/^{56}Ni$ was enhanced by the stronger alpha-rich freezeout in the polar region. In this paper, we apply these results to Cas A and examine whether this effect can explain the large amount of $^{44}Ti$ and the large ratio of $^{44}Ti/^{56}Ni$. We demonstrate that the conventional spherically symmetric explosion model can not explain the $^{44}$Ti mass produced in Cas A if its lifetime is shorter than $\sim$ 80 years and the intervening space is transparent to the gamma-ray line from the decay of $^{44}$Ti. On the other hand, we show the axisymmetric explosion models can solve the problem. We expect the same effect from a three dimensionally asymmetric explosion, since the stronger alpha-rich freezeout will also occur in that case in the region where the larger energy is deposited.
description: 10 pages, LaTeX text and 3 postscript figures
Characterisation of enteric viruses in dogs
Creators: name: Caddy, Sarah
Publisher: name: Imperial College London
Year: 2015

description: Human noroviruses (HuNoV) are a significant cause of viral gastroenteritis in man worldwide. Noroviruses are also associated with intestinal disease in multiple species, including dogs. Canine norovirus (CNV) was initially discovered in 2007 and the first aim of this thesis was to determine the prevalence of CNV in the UK dog population. qPCR screening of canine stool samples did not identify CNV RNA, but canine astroviruses (CaAstV) were serendipitously identified and subsequently characterized according to the second aim of this work. For serological screening, CNV virus-like particles (VLPs) to three CNV strains were produced. CNV circulation in the UK was confirmed by identification of CNV-specific antibodies in 60% of canine serum samples collected in 2012-2013. The third aim of this thesis was investigate to CNV interactions with host cells by identifying the cellular attachment factor for CNV. Synthetic carbohydrates and canine tissue samples were used to assess the binding specificity of CNV VLPs, and it was shown that antigens of the HBGA family were recognized. Phenotyping studies then demonstrated expression of HBGAs in dogs. As HuNoV also uses HBGAs to attach to cells, this raised concerns that dogs may be susceptible to HuNoV. Evaluating the zoonotic risk of enteric viruses in dogs was the final aim of this thesis. The susceptibility of dogs to HuNoV and hepatitis E virus (HEV) was determined by screening canine samples for the presence of HuNoV or HEV RNA and HuNoV or HEV-specific antibodies. Antibodies to both HuNoV and HEV were identified in dogs, and results confirmed HuNoV VLPs can bind to canine gastrointestinal samples. This data indicates that dogs are susceptible to HuNoV and HEV infections. In conclusion, this thesis has provided epidemiological and molecular characterization of CNV and CaAstV, in addition to highlighting the zoonotic potential for CNV, HuNoV and HEV in dogs.
Dispersion of Inferred SNe Ia/SNe II Ratios for Current Models of Supernova Nucleosynthesis
Creators: name: Nagataki, S.
name: Hashimoto, M.
name: Sato, K.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have estimated the dispersion of the inferred relative frequencies of Type-Ia and Type- II supernovae ($N_{Ia}/ N_{II}$) in our Galaxy by fitting the numerical results of supernova nucleosynthesis to the solar-system abundances. The ratio $N_{Ia}/ N_{II}$ is estimated to be 0.056--0.14, which is consistent with the observation, if the model of Woosley and Weaver (1995, WW95) is adopted for Type-II supernovae (SNe II). On the other hand, the upper limit of $N_{Ia}/ N_{II}$ becomes too large for the model of Hashimoto (1995, Ha95). However, Ha95 can fit the solar values better than WW95 as far as the abundant nuclei are concerned. These results mean that Ha95 can reproduce the main nuclei of the solar-system well and that WW95 can reproduce the solar values over a wide mass-number range. We also note that $N_{Ia}/ N_{II}$ tends to become smaller if the delayed detonation model is adopted for Type-Ia supernovae (SNe Ia). The dispersion of $N_{Ia}/ N_{II}$ obtained in the present investigation is larger than that concluded by Tsujimoto et al. (1995), which will have an influence on the estimate of the average life time of SNe Ia's progenitors and/or the star-formation rate history in our galaxy.
description: 15 pages, including LaTeX text and 3 postscript figures
Natural Inflation with a periodic non-minimal coupling
Creators: name: Ferreira, Ricardo Z.
name: Notari, Alessio
name: Simeon, Guillem
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Natural inflation is an attractive model for primordial inflation, since the potential for the inflaton is of the pseudo Nambu-Goldstone form, $V(ϕ)=Λ^4 [1+\cos (ϕ/f)]$, and so is protected against radiative corrections. Successful inflation can be achieved if $f \gtrsim {\rm few}\, M_{P}$ and $Λ\sim m_{GUT}$ where $Λ$ can be seen as the strong coupling scale of a given non-abelian gauge group. However, the latest observational constraints put natural inflation in some tension with data. We show here that a non-minimal coupling to gravity $γ^2(ϕ) R$, that respects the symmetry $ϕ\rightarrow ϕ+2 πf$ and has a simple form, proportional to the potential, can improve the agreement with cosmological data. Moreover, in certain cases, satisfactory agreement with the Planck 2018 TT, TE, EE and low P data can be achieved even for a periodicity scale of approximately $M_p$.
description: Version to match the published version
The Distribution of Mass and Gas in the Center of Clusters of Galaxies Implied by X-Ray and Lensing Observations
Creators: name: Waxman, Eli
name: Miralda-Escudé, Jordi
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Observations of gravitational lensing indicate that the mass distribution in clusters of galaxies (where most of the mass is dark matter) is highly peaked towards the center, while X-ray observations imply that the gas is more extended. The additional fact that the gas is cooling in the center has often led one to expect that the gas temperature should be lower near the center, and therefore the gas should be more concentrated than the dark matter. We show that such expectation is not correct, and that the gas temperature must remain approximately constant within the cooling region in order to have consistency with the observed X-ray profiles and lenses. A multiphase cooling flow naturally produces an approximately constant temperature profile, and a more extended distribution for the gas compared to the mass. Cool phases are deposited at relatively large radius, while hot phases are adiabatically heated as they flow inwards and can keep the average temperature constant. Thus, cooling flows result in an {\it increase} of the central temperature, relative to a case where there is no cooling and the gas follows the mass distribution. The increased central temperatures caused by cooling flows give a characteristic core radius to the gas profiles, which is of order the cooling radius. This provides a natural explanation for the typical cores observed in X-ray clusters. It also brings into better agreement with observations the rate of cluster evolution expected in self-similar hierarchical models. We propose that clusters having core radii much larger than their cooling radii are in the process of merging and are not in dynamical equilibrium.
description: 30 pages, PostScript
1- and 3-photon dynamical Casimir effects using nonstationary cyclic qutrit
Creators: name: Dessano, H
name: Dodonov, A V
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We consider the nonstationary circuit QED setup in which a 3-level artificial atom in the $Δ$-configuration interacts with a single-mode cavity field of natural frequency $ω$. It is demonstrated that when some atomic energy level(s) undergoes a weak harmonic modulation, photons can be generated from vacuum via effective 1- and 3-photon transitions, while the atom remains approximately in the ground state. These phenomena occur in the dispersive regime when the modulation frequency is accurately tuned near $ω$ and $3ω$, respectively, and the generated field states exhibit strikingly different statistics from the squeezed vacuum state attained in standard cavity dynamical Casimir effect.
description: 7 pages, 3 figures
Reminiscences of William J. Wallace 1967
Publisher: name: Columbia University
Year: 2019
Subjects: Veterans
Air pilots
Aeronautics, Military
Aviation
World War, 1939-1945--Aerial operations, American
Amphibious warfare

description: Education, Washington College; commissioned 1918; early assignments, flight training; China; carrier training in 1930s; World War II, Pearl Harbor, Guadalcanal, Okinawa; Fleet Marine Force ir Commands, Atlantic and Pacific; Director of Aviation, Headquarters Marine Corps, 1948-1950.
Rubia tinctorum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Rubia
Rubia tinctorum

description: Rubia tinctorum, spec. nov.
 1. Rubia foliis senis. Hort. cliff. 35. Hort. ups. 28. Mat. med. 44. Roy. lugdb. 254.
 Rubia perennis, foliis saepius quinis. Sauv. monsp. 161.
 Rubia sylvestris aspera. Bauh. pin. 33.
 β. Rubia tinctorum sativa. Bauh. pin. 33.
 Habitat Monspelii & ad Danubium . ♃
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 109, DOI: 10.5281/zenodo.3931989
Consistency of a gauged two-Higgs-doublet model: Scalar sector
Creators: name: Arhrib, Abdesslam
name: Huang, Wei-Chih
name: Ramos, Raymundo
name: Tsai, Yue-Lin Sming
name: Yuan, Tzu-Chiang
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the theoretical and phenomenological constraints imposed on the scalar sector of the gauged two Higgs doublet model proposed recently as a variant of the popular inert Higgs doublet model of dark matter. The requirements of tree-level vacuum stability and perturbative unitarity in the scalar sector are analyzed in detail. Furthermore, taking into account the constraints from the 125 GeV Higgs boson measurements at the Large Hadron Collider, we map out the allowed ranges for the fundamental parameters of the scalar potential in the model.
description: 41 pages, 31 figures. V2: Content added to section III.A, references added, content matches version published in PRD
Rubia tinctorum 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
Gentianales
Rubiaceae
Rubia
Rubia tinctorum

description: Rubia tinctorum Linnaeus, Species Plantarum 1: 109. 1753.
"Habitat Monspelii & ad Danubium." RCN: 890.
Lectotype (Natali in Jarvis & al., Regnum Veg. 127: 83. 1993): Herb. Clifford: 35, Rubia 1 β (BM-000557792).
Generitype of Rubia Linnaeus (vide Hitchcock, Prop. Brit. Bot.: 124. 1929).
Current name: Rubia tinctorum L. (Rubiaceae).
Note: Nazimuddin & Qaiser (in Nasir & Ali, Fl. Pakistan 190: 46. 1989) indicated unspecified material in LINN as type. They did not distinguish between sheets 131.1 and 131.2 (LINN) but, as they are not part of the same gathering, Art. 9.15 does not apply.
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 800, DOI: 10.5281/zenodo.291971
Reminiscences of William L. Lee, 1972
Publisher: name: Columbia University
Year: 2020
Subjects: Air pilots
Aeronautics, Military
Aviation
Military education

description: United States Army service; pre-World War II duty in the Philippines with Dwight D. Eisenhower; training pilots in Texas; duty in Italy; return to Philippines after World War II; impressions of General Eisenhower; reminiscences of Air Force career
Alpha Cygnids - a possible July minor meteor shower
Creators: name: Olech, Arkadiusz
name: Gajos, Marcin
name: Jurek, Michal
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a comprehensive study of a possible $α$-Cygnid meteor shower. Based on visual and telescopic observations made by Polish observers we estimate basic parameters of the stream. Activity of $α$-Cygnids lasts from around June 30 to July 31 with clear maximum near July 18 (solar longitude $λ_\odot=116.5^\circ$). Maximal Zenithal Hourly Rates (ZHRs) are equal to $3.6\pm1.2$. The structure of the radiant analyzed by {\sc radiant} software is most compact for geocentric velocity of the events equal to 41 km/s, and for the drift of the radiant (in units $^\circ$/day) equal to $Δα=+0.6$ $Δδ=+0.2$. Center of the radiant for the moment of maximum is $α=302.5^\circ$ $δ=+46.3^\circ$.We derive population index $r$ equal to $2.55\pm0.14$ from magnitude distribution of 738 possible members of the stream. Comparing the velocity distributions of 754 possible $α$-Cygnids and 4339 sporadic events by $χ^2$ and Kolmogorov-Smirnov tests we conclude that both distributions are different with probability very close to 1.0. Telescopic observations strictly confirm the results obtained from visual observations. The smallest values of $χ^2$ parameter we obtained for the geocentric velocity equal to 40 km/s and for the drift of the radiant (in units $^\circ$/day) equal to $Δα=+0.6$ $Δδ=+0.2$. The center of the radiant for moment of maximum is $α=304.9^\circ$ $δ=+46.2^\circ$. In spite of making many photographic exposures we still have no photographic or video confirmation of the existence of this stream.
description: accepted for publication in Astronomy and Astrophysics, Supplement Series, 8 pages with 4 figures