cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Luminous carbon stars in the Magellanic Clouds
Creators: name: van Loon, Jacco Th.
name: Zijlstra, Albert A.
name: Groenewegen, M. A. T.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present ground-based 3 micron spectra of obscured Asymptotic Giant Branch (AGB) stars in the Magellanic Clouds (MCs). We identify the carbon stars on the basis of the 3.1 micron absorption by HCN and C2H2 molecules. We show evidence for the existence of carbon stars up to the highest AGB luminosities (Mbol=-7 mag, for a distance modulus to the LMC of 18.7 mag). This proves that Hot Bottom Burning (HBB) cannot, in itself, prevent massive AGB stars from becoming carbon star before leaving the AGB. It also sets an upper limit to the distance modulus of the Large Magellanic Cloud of 18.8 mag. The equivalent width of the absorption band decreases with redder (K-L) colour when the dust continuum emission becomes stronger than the photospheric emission. Carbon stars with similar (K-L) appear to have equally strong 3 micron absorption in the MCs and the Milky Way. We discuss the implications for the carbon and nitrogen enrichment of the stellar photosphere of carbon stars.
description: 6 pages, 4 figures, accepted for publication in Astronomy and Astrophysics Main Journal
Thermal equilibrium of molecular clouds in cooling flow clusters
Creators: name: Puy, D.
name: Grenacher, L.
name: Jetzer, P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In many clusters of galaxies there is evidence for cooling flows in the central regions. The ultimate fate of the gas which cools is still unknown. A possibility is that a fraction of the gas forms cold molecular clouds. We investigate the minimum temperature which can be reached by clouds in cooling flows by computing the cooling function due to H2, HD and CO molecules. As an example, we determine the minimum temperature achievable by clouds in the cooling flows of the Centaurus, Hydra and PKS 0745-191 clusters. Our results suggest that clouds can reach very low temperatures - less than 10 K - which would explain the non-detection of CO in these clusters.
description: 23 pages, 5 figures, Astronomy & Astrophysics in press 1999
Surface wave scattering at nonuniform fluid interfaces
Creators: name: Chou, T.
name: Nelson, David R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Effects of spatially varying interfacial parameters on the propagation of surface waves are studied. These variations can arise from inhomogeneities in coverage of surface active substances such as amphiphillic molecules at the fluid/gas interface. Such variations often occur in phase coexistence regions of Langmuir monolayers. Wave scattering from these surface inhomogeneities are calculated in the limit of small variations in the surface parameters by using the asymptotic form of surface Green's functions in the first order Born approximation. When viscosity and variations in surface elastic moduli become important, modes other than transverse capillary waves can change the characteristics of propagation. Scattering among these modes provides a mechanism for surface wave attenuation in addition to viscous damping on a homogeneous surfactant covered interface. Experimental detection of waves attenuation and scattering is also discussed.
description: 11 pages; 8 figures on request
A Quantitative Measure of the Richness of Galaxy Clusters
Creators: name: Yee, H. K. C.
name: Lopez-Cruz, Omar
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using photometric catalogs from wide-field CCD images, we derive the cluster-galaxy correlation amplitudes, Bgc, for 47 low-redshift Abell clusters. We apply a number of tests to establish the robustness of the Bgc parameter as a quantitative measure of richness of galaxy clusters. These include using different galaxy luminosity functions to normalize the excess galaxy counts, counting galaxies to different absolute magnitude limits, and counting galaxies to different cluster-centric radii. These tests show that with a properly normalized luminosity function, the Bgc parameter is relatively insensitive (at better than 1/2 of an Abell Richness class) to magnitude limit, areal coverage, and photometric errors of up to about 0.25 mag. We compare the Bgc values to both the Abell Richness Class (ARC) and Abell count numbers (N_A). It is found that there is a good correlation between Bgc and N_A for Abell clusters with z~0.1 are much less well correlated with the true cluster richness. We also find evidence that the richness of ARC>=3 clusters has the tendency of being over estimated in the Abell catalog.
description: 28 pages, Latex, 7 postscript figures included. Accepted by the Astronomical Journal, to appear in May 1999
Exchange Enhancement of the Electron-Phonon Pair Interaction
Creators: name: Manske, D.
name: Rieck, C. T.
name: Fay, D.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The critical temperature of high-$T_c$ superconductors is determined, at least in part, by the electron-phonon coupling. We include the effect of an exchange interaction between the electrons and calculate the renormalization of the bare phonon frequencies and the electron-phonon verticies in a random phase approximation and obtain a strongly enhanced attractive phonon-induced electron-electron interaction. Using Fast Fourier Transform techniques, the weak-coupling selfconsistency equation for the order parameter is solved in the 2D first Brillouin zone for the Emery tight-binding band with different band fillings. The enhancement of $T_c$ arises primarily from the softening of the phonon frequencies rather than the vertex renormalization.
description: (2 pages, postscript file, hardcopies available from the authors)
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0702
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0702, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0702, 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
A new approach to Lickorish-Millett type formulae
Creators: name: Zhou, Xin
name: Zhu, Shengmao
Publisher: name: arXiv
Year: 2018
Subjects: subject: Geometric Topology (math.GT)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 57M25, 57M27

description: In this paper, we introduce a new method to prove the Lickorish-Millett type formulae for colored HOMFLY-PT polynomials of links.
description: 18 pages
NPA_ref3104
Creators: name: Santen, Jeffrey A Van
Publisher: name: Zenodo
Year: 2019

description: Citation for NP Atlas reference previously without DOI Citation:  VITALI, R A; INAMIDE, E; JACOB, T A THE ISOLATION OF GAMMA-L-GLUTAMYL PEPTIDES FROM A FERMENTATION BROTH Journal of Biological Chemistry, 1965, 240(None), 2508-2511 PubMed ID: 14304861 Publisher Access: http://www.jbc.org/content/240/6/2508.long
Strong and Weak Equilibria for Time-Inconsistent Stochastic Control in Continuous Time
Creators: name: Huang, Yu-Jui
name: Zhou, Zhou
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optimization and Control (math.OC)
subject: Mathematical Finance (q-fin.MF)
subject: FOS: Mathematics
subject: FOS: Economics and business
subject: 60J27, 91A13, 93E20

description: A new definition of continuous-time equilibrium controls is introduced. As opposed to the standard definition, which involves a derivative-type operation, the new definition parallels how a discrete-time equilibrium is defined, and allows for unambiguous economic interpretation. The terms "strong equilibria" and "weak equilibria" are coined for controls under the new and the standard definitions, respectively. When the state process is a time-homogeneous continuous-time Markov chain, a careful asymptotic analysis gives complete characterizations of weak and strong equilibria. Thanks to Kakutani-Fan's fixed-point theorem, general existence of weak and strong equilibria is also established, under additional compactness assumption. Our theoretic results are applied to a two-state model under non-exponential discounting. In particular, we demonstrate explicitly that there can be incentive to deviate from a weak equilibrium, which justifies the need for strong equilibria. Our analysis also provides new results for the existence and characterization of discrete-time equilibria under infinite horizon.
Phalaena (Tinea) Linnaeus, 1758, subgen. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena

description: Phalaena (Tinea) [subgen. nov.]
* 6 * Tineae.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 534, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The statistical characteristics of static friction
Creators: name: Wang, J.
name: Wang, G. F.
name: Yuan, W. K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Friction is one of the fundamental issues in physics, mechanics and material science with lots of practical applications. However, the understanding of macroscopic friction phenomena from microscopic aspect is still on the way. In this work, molecular dynamic simulations are performed to investigate the static friction between two planar crystal surfaces. The friction force experienced by each atom is tracked and the statistical characteristics of atomic friction force are illuminated. More importantly, the influences of normal load and temperature on the statistical features are generalized. This study provides a new insight on the micro-states of friction.
description: 22 pages, 7 figures
Metallic screening and correlation effects in superconducting fullerenes
Creators: name: Lammert, P. E.
name: Rokhsar, D. S.
name: Chakravarty, S.
name: Kivelson, S.
name: Salkola, M. I.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We consider the frequency dependent Coulomb interaction between electrons in a molecular metal in the limit in which the conduction bandwidth is much less than the plasma frequency, which in turn is much less than intramolecular excitation energies. In particular, we compute the effective interactions at the Fermi energy in alkali-doped C$_{60}$, to second order in the screened interactions. The frequency dependence of the screening substantially reduces the effects of the long-range part of the Coulomb interaction, leading to the possibility of an effective attraction between electrons.
description: 10 pages with four uuencoded PostScript figures appended, RevTeX 3.0
The RR Lyrae Period-Amplitude Relation as a Clue to the Origin of the Oosterhoff Dichotomy
Creators: name: Clement, C.
name: Shelton, I.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: An examination of the period-V amplitude relation for RRab stars (fundamental mode pulsators) with `normal' light curves in the Oosterhoff type I clusters M3 and M107 and in the Oosterhoff type II clusters M9 and M68 reveals that the V amplitude for a given period is not a function of metal abundance. Rather, it is a function of the Oosterhoff type. This result is confirmed by published observations of RRab stars in M4, M5 and M92. A method devised by Jurcsik and Kovacs has been used to determine whether the light curve of an RRab star is `normal' or `peculiar'. Although M3 is considered to belong to the Oosterhoff type I group, it has three bright RRab stars that seem to fit the period-amplitude relation for Oosterhoff type II RRab stars. There is evidence that these bright stars are in a more advanced evolutionary state than the other RRab stars in M3, thus leading to the conclusion that the Oosterhoff dichotomy is due to evolution. Our result gives support to the Lee, Demarque & Zinn hypothesis that most RR Lyrae variables in Oosterhoff type I clusters are ZAHB objects while those in the Oosterhoff type II clusters are more evolved. This may have important implications for the derived ages of Oosterhoff type II clusters. If their RR Lyrae variables have all evolved away from the ZAHB, then their ages have been overestimated in studies that assume they are ZAHB objects.
description: Latex file, 2 postscript files
Study of QCD generalized ghost dark energy in FRW universe
Creators: name: Biswas, Mahasweta
name: Debnath, Ujjal
name: Ghosh, Shounak
name: Guha, B. K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: A phenomenological generalized ghost dark energy model has been studied under the framework of FRW universe. In ghost dark energy model the energy density depends linearly on Hubble parameter (H) but in this dark energy model, the energy density contains a the sub-leading term which is depends on $\mathcal{O} (H^2)$, so the energy density takes the form $ρ_D=αH+ βH^2$, where $α$ and $β$ are the constants. The solutions of the Friedman equation of our model leads to a stable universe. We have fitted our model with the present observational data including Stern data set. With the help of best fit results we find the adiabatic sound speed remains positive throughout the cosmic evolution, that claims the stability of the model. The flipping of the signature of deceleration parameter at the value of scale factor $a=0.5$ indicates that the universe is at the stage of acceleration i.e. de Sitter phase of the universe at late time. Our model shows that the acceleration of the universe begin at redshift $z_{ace}\approx 0.617$ and the model is also consistent with the current observational data.
description: 9 pages, 9 figures
Additional file 3 of VCP interaction with HMGB1 promotes hepatocellular carcinoma progression by activating the PI3K/AKT/mTOR pathway
Creators: name: Pu, Zhangya
name: Duda, Dan G.
name: Zhu, Yuanyuan
name: Pei, Siya
name: Wang, Xiaofang
name: Huang, Yan
name: Yi, Panpan
name: Huang, Zebing
name: Peng, Fang
name: Hu, Xingwang
name: Fan, Xuegong
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 3: Table S2. The VCP-interacting proteins that were identified by co-immunoprecipitation combined with the mass spectrometry technology (CoIP/MS).
Convection in porous media with dispersion
Creators: name: Wen, Baole
name: Chang, Kyung Won
name: Hesse, Marc A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We investigate the effect of dispersion on convection in porous media by performing direct numerical simulations (DNS) in a two-dimensional Rayleigh-Darcy domain. Scaling analysis of the governing equations shows that the dynamics of this system are not only controlled by the classical Rayleigh-Darcy number based on molecular diffusion, $Ra_m$, and the domain aspect ratio, but also controlled by two other dimensionless parameters: the dispersive Rayleigh number $Ra_d = H/α_t$ and the dispersivity ratio $r = α_l/α_t$, where $H$ is the domain height, $α_t$ and $α_l$ are the transverse and longitudinal dispersivities, respectively. For $Δ= Ra_d/Ra_m > O(1)$, the influence from the mechanical dispersion is minor; for $Δ\ll 1$, however, the flow pattern is controlled by $Ra_d$ while the convective flux is $F\sim Ra_m$ for large $Ra_m$, but with a prefactor that has a non-monotonic dependence on $Ra_d$. Our DNS results also show that the increase of mechanical dispersion, i.e. decreasing $Ra_d$, will coarsen the convective pattern by increasing the plume spacing. Moreover, the inherent anisotropy of mechanical dispersion breaks the columnar structure of the mega-plumes at large $Ra_m$, if $Ra_d < 5000$. This results in a fan-flow geometry that reduces the convective flux.
Energy Production Rates of Multicomponent Granular Gases of Rough Particles. A Unified View of Hard-Disk and Hard-Sphere Systems
Creators: name: Megías, Alberto
name: Santos, Andrés
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Granular gas mixtures modeled as systems of inelastic and rough particles, either hard disks on a plane or hard spheres, are considered. Both classes of systems are embedded in a three-dimensional space ($d=3$) but, while in the hard-sphere case the translational and angular velocities are vectors with the same dimensionality (and thus there are $d_{\text{tr}}=3$ translational and $d_{\text{rot}}=3$ rotational degrees of freedom), in the hard-disk case the translational velocity vectors are planar (i.e., $d_{\text{tr}}=2$ translational degrees of freedom) and the angular velocity vectors are orthogonal to the motion plane (i.e., $d_{\text{rot}}=1$ rotational degree of freedom). This complicates a unified presentation of both classes of systems, in contrast to what happens for smooth, spinless particles, where a treatment of $d$-dimensional spheres is possible. In this paper, a kinetic-theory derivation of the (collisional) energy production rates $ξ_{ij}^{\text{tr}}$ and $ξ_{ij}^{\text{rot}}$ (where the indices $i$ and $j$ label different components) in terms of the numbers of degrees of freedom $d_{\text{tr}}$ and $d_{\text{rot}}$ is presented. Known hard-sphere and hard-disk expressions are recovered by particularizing to $(d_{\text{tr}},d_{\text{rot}})=(3,3)$ and $(d_{\text{tr}},d_{\text{rot}})=(2,1)$, respectively. Moreover, in the case of spinless particles with $d=d_{\text{tr}}$, known energy production rates $ξ_{ij}^{\text{tr}}=ξ_{ij}$ of smooth $d$-dimensional spheres are also recovered.
description: 11 pages, 1 figure; contributed paper at the 31st International Symposium on Rarefied Gas Dynamics (Glasgow, UK, July 23-27, 2018)
Measuring and Modelling the Redshift Evolution of Clustering: the Hubble Deep Field North
Creators: name: Arnouts, Stephane
name: Cristiani, Stefano
name: Moscardini, Lauro
name: Matarrese, Sabino
name: Lucchin, Francesco
name: Fontana, Adriano
name: Giallongo, Emanuele
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (abridged) The evolution of galaxy clustering from z=0 to z=4.5 is analyzed using the angular correlation function and the photometric redshift distribution of galaxies brighter than I_{AB}\le 28.5 in the HDF North. The reliability of the photometric redshift estimates is discussed on the basis of the available spectroscopic redshifts, comparing different codes and investigating the effects of photometric errors. The redshift bins in which the clustering properties are measured are then optimized to take into account the uncertainties of the photometric redshifts. The results show that the comoving correlation length has a small decrease in the range 0
description: 23 pages, Latex using MN style, figures enclosed. Version accepted for publication in MNRAS
NPA_ref3308
Creators: name: Santen, Jeffrey A Van
Publisher: name: Zenodo
Year: 2019

description: Citation for NP Atlas reference previously without DOI Citation:  Huneck, S; Schreiber, K; Snatzke, G; Fehlhaber, H W Miriquidic acid, a new depside from Lecidea lilienstroemii and Lecidea leucophaea Zeitschrift fur Naturforschung B: Journal of Chemical Sciences, 1971, 26(12), 1357-1364 PubMed ID: 4401891 Publisher Access: NONE
Formation of eyes in large-scale cyclonic vortices
Creators: name: Oruba, Ludivine
name: Davidson, Peter
name: Dormy, Emmanuel
Publisher: name: arXiv
Year: 2018
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: FOS: Physical sciences

description: We present numerical simulations of steady, laminar, axisymmetric convection of a Boussinesq fluid in a shallow, rotating, cylindrical domain. The flow is driven by an imposed vertical heat flux and shaped by the background rotation of the domain. The geometry is inspired by that of tropical cyclones and the global flow pattern consists of a shallow, swirling vortex combined with a poloidal flow in the r-z plane which is predominantly inward near the bottom boundary and outward along the upper surface. Our numerical experiments confirm that, as suggested by Oruba et al 2017, an eye forms at the centre of the vortex which is reminiscent of that seen in a tropical cyclone and is characterised by a local reversal in the direction of the poloidal flow. We establish scaling laws for the flow and map out the conditions under which an eye will, or will not, form. We show that, to leading order, the velocity scales with V=(αg β)^{1/2}H, where g is gravity, αthe expansion coefficient, βthe background temperature gradient, and H is the depth of the domain. We also show that the two most important parameters controlling the flow are Re=VH/νand Ro=V/ΩH, where Ωis the background rotation rate and νthe viscosity. The Prandtl number and aspect ratio also play an important, if secondary, role. Finally, and most importantly, we establish the criteria required for eye formation. These consist of a lower bound on Re, upper and lower bounds on Ro, and an upper bound on Ekman number.
description: 18 pages, 14 figures, 1 table
title: Identifying sleep disturbance in children: insights using children's drawings and clinical research portfolio
Creators: name: Clark, Nicola Jane
Publisher: name: University of Glasgow
Year: 2008
Subjects: subject: Clinical psychology, children, sleep disorders, sleep.

description: Background: Child-centred approaches have been gaining favour in recent years in almost every domain of health care. However, few methods are available which are developmentally sensitive enough to elicit children's voices, whilst also accommodating for cognitive and verbal ability. Drawing is a natural and spontaneous childhood activity which has recently been gaining support. Despite increasing popularity, the use of children's drawings as a reliable and valid clinical tool, continues to be debated. Aims: This paper aims to systematically review studies exploring children's drawings as a means of facilitating psychological evaluation in health care research. Methods: Fifteen articles, that satisfied the criteria of this review, were identified using a systematic search strategy including searching electronic databases and hand searching of relevant articles. The methodological quality of articles fulfilling inclusion criteria were rated using an idiosyncratic quality criteria. Results: Overall, there is little available high-quality evidence to support the use of children's drawings as the sole means of psychological evaluation, as currently too few studies meet the gold standard criteria. More encouragingly, it appears that drawing is an effective tool for establishing relationships and rapport building. Conclusions: Research employing children's drawings as a clinical tool has generally been of poor quality and has prevented any firm conclusions being drawn with regards to the usefulness of children's drawings as a means of facilitating psychological evaluation in health care research.
Growth Kinetics in the $Φ^6$ N-Component Model. Conserved Order Parameter
Creators: name: Corberi, F.
name: Marconi, U. Marini. Bettolo
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We extend the discussion of the growth kinetics of the large-N time-dependent Ginzburg-Landau model with an order parameter described by a $Φ^6$ free energy functional, to the conserved case. Quenches from a high temperature initial state to a zero temperature state are studied for different selections of parameters entering the effective potential. In all cases we obtain the asymptotic form of the structure factor. As expected in analogy with the well studied $Φ^4$ model, we find multiscaling behavior whenever stable equilibrium is reached in the ordering region. On the other hand the present model also displays a novel feature, namely the occurrence of metastable relaxation.
description: 20 pages,Plain Latex
NPA_ref3462
Creators: name: Santen, Jeffrey A Van
Publisher: name: Zenodo
Year: 2019

description: Citation for NP Atlas reference previously without DOI Citation:  Machlowitz, R a; Fisher, W p; Mckay, B s; Tytell, A a; Charney, J Xanthothricin, a new antibiotic Antibiotics and Chemotherapy, 1954, 4(3), 259-261 PubMed ID: 24542943 Publisher Access: NONE
Advance Your Geospatial Technology--Empowered by Your Curriculum Standards
Creators: name: Baker, Thomas R
name: Duke, Barbaree
name: Jo, Injeong
Publisher: name: figshare
Year: 2021
Subjects: subject: 130306 Educational Technology and Computing
subject: FOS: Educational sciences
subject: 160808 Sociology and Social Studies of Science and Technology
subject: FOS: Sociology
subject: 130313 Teacher Education and Professional Development of Educators
subject: 130105 Primary Education (excl. Maori)
subject: 130106 Secondary Education

description: This study sampled over 250 state curriculum standards frameworks, guidelines, and documents to assess the presence of select spatial and geospatial keywords in those documents. The curriculum standards included the five core areas of Math, English language arts, social studies, science, and career and technical education (CTE). Although several important macro-factors discussed in the poster exist when comparing state standards, the authors chose to report simple counts of occurrences.
Of all states, Minnesota state social studies standards had the greatest amount of spatial language, when a dozen states had none at all - across the five core subjects. Social studies standards more often contained spatial language than other disciplines, although CTE and science included some use of spatial terms. The authors also show a positive, statistically significant relationship between spatial language in standards and the use of spatial software, like ArcGIS Online.
http://bit.ly/geospatialwords
Persistence of Non-Markovian Gaussian Stationary Processes in Discrete Time
Creators: name: Nyberg, Markus
name: Lizana, Ludvig
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The persistence of a stochastic variable is the probability that it does not cross a given level during a fixed time interval. Although persistence is a simple concept to understand, it is in general hard to calculate. Here we consider zero mean Gaussian stationary processes in discrete time $n$. Few results are known for the persistence $P_0(n)$ in discrete time, except the large time behavior which is characterized by the nontrivial constant $θ$ through $P_0(n)\sim θ^n$. Using a modified version of the Independent Interval Approximation (IIA) that we developed before, we are able to calculate $P_0(n)$ analytically in $z$-transform space in terms of the autocorrelation function $A(n)$. If $A(n)\to0$ as $n\to\infty$, we extract $θ$ numerically, while if $A(n)=0$, for finite $n>N$, we find $θ$ exactly (within the IIA). We apply our results to three special cases: the nearest neighbor-correlated "first order moving average process" where $A(n)=0$ for $ n>1$, the double exponential-correlated "second order autoregressive process" where $A(n)=c_1λ_1^n+c_2λ_2^n$, and power law-correlated variables where $A(n)\sim n^{-μ}$. Apart from the power-law case when $μ<5$, we find excellent agreement with simulations.
description: 7 pages, 4 figures
The AGN/Normal Galaxy Connection : Summary
Creators: name: Lawrence, Andy
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The connection between normal and active galaxies is reviewed, by summarizing our progress on answering nine key questions. (1) Do all galaxies contain massive dark objects (MDOs)? (2) Are these MDOs actually supermassive black holes? (3) Why are the dark objects so dark? (4) Do all galaxies contain an Active Galactic Nucleus (AGN)? (5) Are the "dwarf AGN" really AGN? (6) Does AGN activity correlate with host galaxy properties? (7) How are AGN fuelled? (8) Is AGN activity related to starburst activity? (9) How do quasars relate to galaxy formation?
description: 10 pages, LateX file. To appear in proceedings of workshop at 32nd COSPAR Symposium, "The AGN/Normal Galaxy Connection", eds Schmidt, Kinney and Ho
The gamma construction and asymptotic invariants of line bundles over arbitrary fields
Creators: name: Murayama, Takumi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Algebraic Geometry (math.AG)
subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics
subject: 14C20 (Primary) 13A35, 14F17, 14B05 (Secondary)

description: We extend results on asymptotic invariants of line bundles on complex projective varieties to projective varieties over arbitrary fields. To do so over imperfect fields, we prove a scheme-theoretic version of the gamma construction of Hochster and Huneke to reduce to the setting where the ground field is $F$-finite. Our main result uses the gamma construction to extend the ampleness criterion of de Fernex, Küronya, and Lazarsfeld using asymptotic cohomological functions to projective varieties over arbitrary fields, which was previously known only for complex projective varieties. We also extend Nakayama's description of the restricted base locus to klt or strongly $F$-regular varieties over arbitrary fields.
description: 27 pages; comments welcome. v2: Added Appendix B, other small changes. v3: Added Remark 4.4 and Proposition 4.6, updated references, other small changes
Additional file 2 of VCP interaction with HMGB1 promotes hepatocellular carcinoma progression by activating the PI3K/AKT/mTOR pathway
Creators: name: Pu, Zhangya
name: Duda, Dan G.
name: Zhu, Yuanyuan
name: Pei, Siya
name: Wang, Xiaofang
name: Huang, Yan
name: Yi, Panpan
name: Huang, Zebing
name: Peng, Fang
name: Hu, Xingwang
name: Fan, Xuegong
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2: Table S1. The correlation of VCP expression and clinicopathologic features in HCC patients in GSE14520 dataset from GEO database.
Oblique Confinement and Phase Transitions in Chern-Simons Gauge Theories
Creators: name: Diamantini, M. C.
name: Sodano, P.
name: Trugenberger, C. A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate non-perturbative features of a planar Chern-Simons gauge theory modeling the long distance physics of quantum Hall systems, including a finite gap M for excitations. By formulating the model on a lattice, we identify the relevant topological configurations and their interactions. For M bigger than a critical value, the model exhibits an oblique confinement phase, which we identify with Lauglin's incompressible quantum fluid. For M smaller than the critical value, we obtain a phase transition to a Coulomb phase or a confinement phase, depending on the value of the electromagnetic coupling.
description: 8 pages, harvmac, DFUPG 91/94 and MPI-PhT/94-92
Phalaena sociella Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena sociella

description: Phalaena sociella [spec. nov.]
P. Tinea alis oblongis cinereis: antice albidis: postice striga pallida.
Fn. svec. 905.
Habitat in Europa.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 534, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Unusual Burst Emission from the New Soft Gamma Repeater SGR1627-41
Creators: name: Mazets, E. P.
name: Aptekar, R. L.
name: Butterworth, P. S.
name: Cline, T. L.
name: Frederiks, D. D.
name: Golenetskii, S. V.
name: Hurley, K.
name: Il'inskii, V. N.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In June-July,1998 the Konus-Wind burst spectrometer observed a series of bursts from the new soft gamma repeater SGR1627-41. Time histories and energy spectra of the bursts have been studied, revealing fluences and peak fluxes in the ranges of 3x10^{-7} - 7.5x10^{-6} erg cm^{-2} and 10^{-5} - 10^{-4}erg cm^{-2}/s respectively. One event, 18 June 6153.5sUT stands out dramatically from this series. Its fluence is ~7x10^{-4} erg cm^{-2} and peak flux ~2x10^{-2} erg cm^{-2}/s. These values from a source at a distance of 5.8 kpc yield an energy output of ~3x10^{42}erg and maximum luminosity of ~8x10^{43} erg/s, similar to the values for the famous March 5, 1979 and August27,1998 events. In terms of energy, this event is another giant outburst seen in a third SGR! However, this very energetic burst differs significantly from the other giant outbursts. It exhibits no separate initial pulse with a fast rise time, no extended tail, and no pulsations. It is rather similar to ordinary repeated bursts but is a few hundred times stronger in intensity. According to the magnetar model by Thompson and Duncan (1995) such a burst may be initiated by a strong starquake when a crust fracture propagates over the whole surface of a neutron star.
description: 7 pages, 5 figures. To be appeared in ApJL
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Cart. 190 (11 H 75), 316 folios, f. 0075v
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Archives Départementales De La Côte-D'Or
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0075v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0075v, 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
On the contrasting spin dynamics of $La_{2-x}Sr_xCuO_4$, $Nd_{2-x}Ce_xCuO_4$ and $YBa_2Cu_3O_{6+x}$ near half filling
Creators: name: Chubukov, Andrey V.
name: Musaelian, Karen A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We present simple calculations which show that incommensurability upon doping and the width of the magnetically ordered phase in Mott-Hubbard insulators depend strongly on the location of the hole/electron pockets in the Brillouin zone. For $LaSrCuO$ systems, we found the pockets at $(\pm π/2,\pm π/2)$, in which case the corrections to the antiferromagnetic spin stiffness grow with doping and destroy the commensurate antiferromagnetic ordering already at a very small doping. On the other hand, in $NdCeCuO$, the hole pockets are located at $(π,0)$ and the symmetry related points, in which case the corrections to the stiffness scale linearly with the density of carriers and do not destroy commensurate spin ordering. For $YBCuO$, systems the situation is less certain, but our results favor hole pockets at $(π/2,π/2)$. We also discuss briefly the tendency towards phase separation.
description: 18 pages, LaTex
Codimension and Projective Dimension up to Symmetry
Creators: name: Van Le, Dinh
name: Nagel, Uwe
name: Nguyen, Hop D.
name: Roemer, Tim
Publisher: name: arXiv
Year: 2018
Subjects: subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics
subject: 13A50, 13C15, 13D02, 13F20, 16P70, 16W22

description: Symmetric ideals in increasingly larger polynomial rings that form an ascending chain are investigated. We focus on the asymptotic behavior of codimensions and projective dimensions of ideals in such a chain. If the ideals are graded it is known that the codimensions grow eventually linearly. Here this result is extended to chains of arbitrary symmetric ideals. Moreover, the slope of the linear function is explicitly determined. We conjecture that the projective dimensions also grow eventually linearly. As part of the evidence we establish two non-trivial lower linear bounds of the projective dimensions for chains of monomial ideals. As an application, this yields Cohen-Macaulayness obstructions.
description: 19 pages; revised version, to appear in Math. Nachr
Additional file 1 of Construction of an immune-related lncRNA signature pair for predicting oncologic outcomes and the sensitivity of immunosuppressor in treatment of lung adenocarcinoma
Creators: name: Zhuang, Jinman
name: Chen, Zhongwu
name: Chen, Zishan
name: Chen, Jin
name: Liu, Maolin
name: Xu, Xinying
name: Liu, Yuhang
name: Yang, Shuyan
name: Hu, Zhijian
name: He, Fei
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 1. Methods in selection of 8 IRLPs.
NPA_ref3671
Creators: name: Santen, Jeffrey A Van
Publisher: name: Zenodo
Year: 2019

description: Citation for NP Atlas reference previously without DOI Citation:  Daeschel, M a; Klaenhammer, T r Association of a 13.6-Megadalton Plasmid in Pediococcus pentosaceus with Bacteriocin Activity Applied and Environmental Microbiology, 1985, 50(6), 1538-1541 PubMed ID: 16346954 Publisher Access: https://aem.asm.org/content/50/6/1538.long
Performance analysis of the prototype THz-driven electron gun for the AXSIS project
Creators: name: Vashchenko, G.
name: Assmann, R.
name: Dorda, U.
name: Fakhari, M.
name: Fallahi, A.
name: Galaydych, K.
name: Kaertner, F.
name: Marchetti, B.
name: Matlis, N.
name: Vinatier, T.
name: Qiao, W.
name: Zhou, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: The AXSIS project (Attosecond X-ray Science: Imaging and Spectroscopy) aims to develop a THz-driven compact X-ray source for applications e.g. in chemistry and biology by using ultrafast coherent diffraction imaging and spectroscopy. The key components of AXSIS are the THz-driven electron gun and THz-driven dielectric loaded linear accelerator as well as an inverse Compton scattering scheme for the X-rays production. This paper is focused on the prototype of the THz-driven electron gun which is capable of accelerating electrons up to tens of keV. Such a gun was manufactured and tested at the test-stand at DESY. Due to variations in gun fabrication and generation of THz-fields the gun is not exactly operated at design parameters. Extended simulations have been performed to understand the experimentally observed performance of the gun. A detailed comparison between simulations and experimental measurements is presented in this paper.
description: EAAC proceeding at NIM-A
A Morphological Classification Scheme for ULIRGs: Evidence for Multiple Mergers
Creators: name: Borne, K. D.
name: Bushouse, H.
name: Colina, L.
name: Lucas, R. A.
name: Baker, A.
name: Clements, D.
name: Lawrence, A.
name: Rowan-Robinson, M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have used the Hubble Space Telescope (HST) to study a large sample of ultraluminous IR galaxies (ULIRGs). With a rich legacy database of 150 high-resolution images, we are studying the fine-scale structure of this unique collection of violently starbursting systems. We review here some of the latest results from our survey. We present a simple morphological classification scheme, consisting of 4 ULIRG classes, showing that there is very little luminosity variation (in the mean) between the classes, and that there is equal likelihood of a ULIRG being a recent merger (single) as an on-going collision (multiple). It now appears that the fraction of ULIRGs that show evidence for interaction or merging is very close to 100%. A star-like nucleus is seen in about 15% of the ULIRGs, for which the dominant power source may be a dust-enshrouded AGN/QSO. Many of the results on ULIRGs are pointing to a complicated dynamical history for this sample of galaxies. One possible explanation for this dynamical diversity is the multiple-merger model proposed by Taniguchi & Shioya (1998, ApJ, 501, L167). We present strong observational evidence for multiple mergers among a large fraction of our ULIRG sample. If this is a valid model, then ULIRGs could be the merger remnants of an earlier generation of compact groups of galaxies.
description: 6 pages, 2 Postscript figures, uses crckapb.sty and psfig.sty. Refereed paper, to be published in "Astrophysics and Space Science", for the proceedings of the Ringberg (Germany, Sept.98) conference: "Ultraluminous Galaxies: Monsters or Babies"
Cross-sectional physician survey on the use of minimal residual disease testing in the management of pediatric and adult patients with acute lymphoblastic leukemia
Creators: name: Kim, Christopher
name: Delaney, Kara
name: McNamara, Michelle
name: Chia, Victoria
name: Romanov, Vadim
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: Pharmacology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Plant Biology
subject: FOS: Biological sciences

description: Objectives: Minimal residual disease (MRD) is a strong prognostic factor in acute lymphoblastic leukemia (ALL), which progresses quickly and is fatal within months if untreated. This study explored use of MRD testing in adult and pediatric B-cell ALL patients, and academic versus community settings. Methods: A survey was administered to US-based hematologists/oncologists currently managing ≥5 B-cell ALL patients and using MRD tests. Descriptive analyses (frequencies and percentages) and Pearson’s chi square testing assessed any differences in various characteristics. Results: 150 adult treaters (treating physicians: 100 community, 50 academic) and 30 pediatric treaters participated. Use of MRD testing was higher among pediatric treaters (93% of patients) than adult treaters (73% of patients) (p p Discussion: MRD testing is an important tool in the prediction of relapse in ALL. Resolving barriers could improve detection of molecular relapse in patients with ALL, particularly among adults and in community settings. Conclusion: MRD testing is fairly common in treatment of ALL, but some barriers still exist in access.
Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
Creators: name: Park, Chan-Gyung
name: Ratra, Bharat
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: Cosmic microwave background (CMB) anisotropy (spatial inhomogeneity) data provide the tightest constraints on the Hubble constant, matter density, spatial curvature, and dark energy dynamics. Other data, sensitive to the evolution of only the spatially homogeneous part of the cosmological model, such as Type Ia supernova apparent magnitude, baryon acoustic oscillation distance, and Hubble parameter measurements, can be used in conjunction with the CMB data to more tightly constrain parameters. Recent joint analyses of CMB and such non-CMB data indicate that slightly closed spatial hypersurfaces are favored in nonflat untilted inflation models and that dark energy dynamics cannot be ruled out, and favor a smaller Hubble constant. We show that the constraints that follow from these non-CMB data alone are consistent with those that follow from the CMB data alone and so also consistent with, but weaker than, those that follow from the joint analyses of the CMB and non-CMB data.
description: 8 pages, 4 figures, 3 tables. Accepted for publication in Astrophysics and Space Science