cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Exact results for persistent currents of two bosons in a ring lattice
Creators: name: Polo, Juan
name: Naldesi, Piero
name: Minguzzi, Anna
name: Amico, Luigi
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We study the ground state of two interacting bosonic particles confined in a ring-shaped lattice potential and subjected to a synthetic magnetic flux. The system is described by the Bose-Hubbard model and solved exactly through a plane-wave Ansatz of the wave function. We obtain energies and correlation functions of the system both for repulsive and attractive interactions. In contrast with the one-dimensional continuous theory described by the Lieb-Liniger model, in the lattice case we prove that the center of mass of the two particles is coupled with its relative coordinate. Distinctive features clearly emerge in the persistent current of the system. While for repulsive bosons the persistent current displays a periodicity given by the standard flux quantum for any interaction strength, in the attractive case the flux quantum becomes fractionalized in a manner that depends on the interaction. We also study the density after the long time expansion of the system which provides an experimentally accessible route to detect persistent currents in cold atom settings. Our results can be used to benchmark approximate schemes for the many-body problem.
Average search time bound in cue based search strategy
Creators: name: Wasnik, Vaibhav
Publisher: name: arXiv
Year: 2020
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: In this work we consider the problem of searches that utilises past information gathered during searching, to evaluate the probability distribution of finding the source at each step. We start with a sample strategy where the movement at each step is in the immediate neighbourhood direction, with a probability proportional to the normalised difference in probability of finding the source with the present position source finding probability. We evaluate a lower bound for the average search time for this strategy . We next consider the problem of the lowerbound on any strategy that utilities information of the probability distribution evaluated by the searcher at any instant. We derive an expression for the same. Finally we present an analytic expression for this lower bound in the case of homogeneous diffusion of particles by a source. For a general probability distribution with entropy-E, we find that the lower bound goes as exp(E/2).
Resolving the Degeneracy: Experimental tests of the New Self Creation Cosmology and a heterodox prediction for Gravity Probe B
Creators: name: Barber, Garth A
Publisher: name: arXiv
Year: 2003
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The new theory of Self Creation Cosmology has been shown to yield a concordant cosmological solution that does not require inflation, exotic non-baryonic Dark matter or Dark Energy to fit observational constraints. In vacuo there is a conformal equivalence between this theory and canonical General Relativity and as a consequence an experimental degeneracy exists as the two theories predict identical results in the standard tests. However, there are three definitive experiments that are able to resolve this degeneracy and distinguish between the two theories. Here these standard tests and definitive experiments are described. One of the definitive predictions, that of the geodetic precession of a gyroscope, has just been measured on the Gravity Probe B satellite, which is at the present time of writing in the data processing stage. This is the first opportunity to falsify Self Creation Cosmology. The theory predicts a 'frame-dragging' result equal to GR but a geodetic precession of only 2/3 the GR value. When applied to the Gravity Probe B satellite, Self Creation Cosmology predicts an E-W gravitomagnetic/frame-dragging precession, equal to that of GR, of 40.9 milliarcsec/yr but a -S gyroscope (geodetic + Thomas) precession of just 4.4096 arcsec/yr.
description: LaTex, 15 pages. Correction of the prediction of the GP-B geodetic measurement to 4.4096 arcsec/yr
title: Lettre au Professeur Marc Gentilini (Hôpital Pitié - Salpétrière)
Creators: name: Leibowitch, Jacques
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: 3 exemplaires.
description: Source: http://www.calames.abes.fr/pub/ms/Calames-20193111135799614
WR bubbles and HeII emission
Creators: name: Naze, Y.
name: Rauw, G.
name: Manfroid, J.
name: Chu, Y. -H.
name: Vreux, J. -M.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the very first high quality images of the HeII 4686 emission in three high excitation nebulae of the Magellanic Clouds. A fourth high excitation nebula, situated around the WR star BAT99-2, was analysed in a previous letter. Using VLT FORS data, we investigate the morphology of the ring nebulae around the early-type WN stars BAT99-49 & AB7. We derive the total HeII fluxes for each object and compare them with the most recent theoretical WR models. Using Halpha, [OIII] and HeI 5876 images along with long-slit spectroscopy, we investigate the physical properties of these ring nebulae and find only moderate chemical enrichment. We also surveyed seven other LMC WR stars but we failed to detect any HeII emission but note that the nebula around BAT99-11 shows a N/O ratio and an oxygen abundance slightly lower than the LMC values, while the nebula around BAT99-134 presents moderate chemical enrichment similar to the one seen near BAT99-2, 49 and AB7. The third high excitation nebula presented in this paper, N44C, does not harbor stars hotter than mid-O main sequence stars. It was suggested to be a fossil X-ray nebula ionized but our observations of N44C reveal no substantial changes in the excitation compared to previous results reported in the literature.
description: 13 pages, 8 figures (7 in jpg), accepted by A&A, also available from http://vela.astro.ulg.ac.be/Preprints/P81/index.html
Eigenmodes of Dodecahedral space
Creators: name: Marc, Lachieze-Rey
Publisher: name: arXiv
Year: 2004
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Cosmological models where spatial sections are the Poincaré dodecahedral space D have been recently invoked to give an account of the lower modes of the angular anisotropies of the cosmic microwave background. Further explorations of this possibility require the knowledge of the eigenmodes of the Laplacian of D. Only the first modes have been calculated numerically. Here we give an explicit form for these modes up to arbitrary order, in term of eigenvectors of a small rank matrix, very easy to calculate numerically. As an illustration we give the first modes, up to the eigenvalue $-k (k+2)$ for $k=62$. These results are obtained by application of a more general method (presented in a previous work) which allows to express the properties of any eigenfunction of the Laplacian of the three sphere under an arbitrary rotation of SO(4).
description: 11 pages, no figure
Additional file 2 of The risk factors of local recurrence and distant metastasis on pT1/T2N0 mid-low rectal cancer after total mesorectal excision
Creators: name: I-Li Lai
name: Jeng-Fu You
name: Yih-Jong Chern
name: Wen-Sy Tsai
name: Jy-Ming Chiang
name: Pao-Shiu Hsieh
name: Hsin-Yuan Hung
name: Hsu, Yu-Jen
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Additional file 2: Supplementary table 2 Patient characteristics for non-RT vs. RT
Vortex shedding in high-Reynolds-number axisymmetric bluff-body wakes: local linear instability and global bleed control
Creators: name: Sevilla, Alejandro
name: Martínez-Bazán, Carlos
Publisher: name: arXiv
Year: 2019
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We study the large-scale helical vortex shedding regime in the wake of an axisymmetric body with a blunt trailing edge at high Reynolds numbers, both experimentally and by means of local, linear, spatiotemporal stability analysis. In the instability analysis we take into account the detailed downstream evolution of the basic flow behind the body base. The study confirms the existence of a finite region of absolute instability for the first azimuthal number in the near field of the wake. Such instability is believed to trigger the large scale helical vortex shedding downstream of the recirculating zone. Inhibition of vortex shedding is examined by blowing a given flow rate of fluid through the base of the slender body. The extent of the locally absolute region of the flow is calculated as a function of the bleed coefficient, $C_b=q_b/(πR^2u_\infty)$, where $q_b$ is the bleed flow rate, $R$ is the radius of the base and $u_\infty$ is the incident free-stream velocity. It is shown that the basic flow becomes convectively unstable everywhere for a critical value of the bleed coefficient of $C_b^*\sim 0.13$, such that no self-excited regime is expected for $C_b>C_b^*$. In addition, we report experimental results of flow visualizations and hot-wire measurements for increasing values of the bleed coefficient. When a sufficient amount of base bleed is applied, flow visualizations indicate that vortex shedding is suppressed and that the mean flow becomes axisymmetric. The critical bleed coefficient predicted by linear instability analysis is shown to fall within the experimental values in the range of Reynolds numbers analyzed here.
description: 14 pages, 13 figures
The pentaquark in K-plus-d total cross section data
Creators: name: Gibbs, W. R.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: An analysis of $K^+$-d total cross section data is undertaken to explore possible effects of the recently observed resonance in the S=+1 hadronic system with mass around 1.55 GeV. It is found that a structure corresponding to the resonance is visible in the data. The width consistent with the observed deviation from background is found to be $0.9\pm 0.3$ MeV and the mass is $1.559\pm 0.003$ GeV/c$^2$ for spin-parity $\h^+$ and $1.547\pm0.002$\ GeV/c$^2$ for $\h^-$. The errors are one standard deviation and statistical only. \
description: 10 pages, 5 figures Replaced to correct references, add and correct text. No change in content. More discussion of errors, increased error on width, corrected one figure
MOESM1 of Improving the performance of spray operators through monitoring and evaluation of insecticide concentrations of pirimiphos-methyl during indoor residual spraying for malaria control on Bioko Island
Creators: name: Fuseini, Godwin
name: Hanafy Ismail
name: Fricken, Michael
name: Weppelmann, Thomas
name: Smith, Jordan
name: Logan, Rhiannon Ellis
name: Folasade Oladepo
name: Walker, Kyle
name: Wonder Phiri
name: Paine, Mark
name: García, Guillermo
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Space Science
subject: Molecular Biology
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: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Cancer

description: Additional file 1: Table 1. Comparison of primiphos-methyl recovery by Bostik adhesive glue dots from rough tile surface treated with various concentrations (0.25–3 g/m2) of Actellic 300CS® formulation.
Dwarf Nova Oscillations and Quasi-Periodic Oscillations in Cataclysmic Variables: III. A New Kind of Dwarf Nova Oscillation, and Further Examples of the Similarities to X-Ray Binaries
Creators: name: Warner, Brian
name: Woudt, Patrick A.
name: Pretorius, Magaretha L.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present measurements of the periods of Dwarf Nova Oscillations (DNOs) and Quasi-Periodic Oscillations (QPOs) in Cataclysmic Variable stars (CVs), many culled from published literature, but also others newly observed (in VZ Pyx, CR Boo, OY Car, Z Cha, AQ Eri, TU Men, HX Peg, CN Ori, V893 Sco, WX Hyi and EC2117-54). These provide data for 26 systems. We show that in general P_QPO ~ 15 P_DNO and that the correlation for CVs extends by three orders of magnitude lower in frequency the similar relationship found for X-Ray binaries. In addition, we have found that there is a second type of DNO, previously overlooked, which have periods ~ 4 times those of the regular DNOs (As well as those mined from publications, we have observed them in VW Hyi, OY Car, AQ Eri, V803 Cen, CR Boo, VZ Pyx, HX Peg and EC2117-54). Often both types of DNO coexist. Unlike the standard DNOs, the periods of the new type, which we refer to as longer period DNOs (lpDNOs), are relatively insensitive to accretion luminosity and can even appear in quiescence of dwarf novae. We interpret them as magnetically channelled accretion onto the differentially rotating main body of the white dwarf primary, rather than onto a rapidly slipping equatorial belt as in the case of the standard DNOs. This is supported by published measurements of v sin(i) for some of the primaries. Some similarities of the DNOs, lpDNOs and QPOs in CVs to the three types of QPO in X-Ray binaries (burst pulsation, high and low frequency QPOs) are noted.
description: 19 pages, 30 figures. To appear in MNRAS
Rotation in string cosmology
Creators: name: Obukhov, Yuri N.
name: Chrobok, Thoralf
name: Scherfner, Mike
Publisher: name: arXiv
Year: 2003
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We describe exact cosmological solutions with rotation and expansion in the low-energy effective string theory. These models are spatially homogeneous (closed Bianchi type IX) and they belong to the family of shear-free metrics which are causal (no closed timelike curves are allowed), admit no parallax effects and do not disturb the isotropy of the background radiation. The dilaton and the axion fields are nontrivial, in general, and we consider both cases with and without the central charge (effective cosmological constant).
description: 15 pages, 1 figure, Revtex, to appear in Class. Quantum Grav
Holographic spontaneous anisotropy
Creators: name: Hoyos, Carlos
name: Jokela, Niko
name: Penín, José Manuel
name: Ramallo, Alfonso V.
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We construct a family of holographic duals to anisotropic states in a strongly coupled gauge theory. On the field theory side the anisotropy is generated by giving a vacuum expectation value to a dimension three operator. We obtain our gravity duals by considering the geometry corresponding to the intersection of D3- and D5- branes along 2+1 dimensions. Our backgrounds are supersymmetric and solve the fully backreacted equations of motion of ten-dimensional supergravity with smeared D5-brane sources. In all cases the geometry flows to $AdS_{5}\times {\mathbb S}^5$ in the UV, signaling an isotropic UV fixed point of the dual field theory. In the IR, depending on the parameters of the solution, we find two possible behaviors: an isotropic fixed point or a geometry with anisotropic Lifshitz-like scaling symmetry. We study several properties of the solutions, including the entanglement entropy of strips. We show that any natural extension of existing $c$-functions will display non-monotonic behavior, conforming with the presence of new degrees of freedom only at intermediate energy scales.
description: 23 pages+3 appendices, 9 figures
Dislocation Formation and Work-Hardening in Two-Phase Alloys
Creators: name: Minami, Akihiko
name: Onuki, Akira
Publisher: name: arXiv
Year: 2004
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: A phase field model is presented to investigate dislocation formation (coherency loss) and workhardening in two-phase binary alloys. In our model the elastic energy density is a periodic function of the shear and tetragonal strains, which allows multiple formation of slips (dislocation dipoles). By numerically integrating the dynamic equations in two dimensions, we find that dislocations appear in pairs in the interface region and grow into slips. One end of each slip glides preferentially into the softer region, while the other end remains trapped at the interface. Under uniaxial stretching at deep quenching, slips appear in the softer regions and do not penetrate into the harder domains, giving rise to an increase of the stress with increasing applied strain in plastic flow.
description: 14 figures (Higher resolution figures can be obtained at http://stat.scphys.kyoto-u.ac.jp/~minami_a/pict/cond-mat0405177/)
Additional file 1 of Identification of circulating CD31+CD45+ cell populations with the potential to differentiate into erythroid cells
Creators: name: Monaco, Maria Chiara G.
name: Maric, Dragan
name: Salvucci, Ombretta
name: Passeri, Cristina Antonetti Lamorgese
name: Accorsi, Patrizia
name: Major, Eugene O.
name: Berardi, Anna Concetta
Publisher: name: figshare
Year: 2021
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Computational Biology

description: Additional file 1: Figure 1. Flow cytometric characterization of circulating CD31-CD45+ Control cells in human peripheral blood. (A) Flow cytometric analysis of fresh adult human Lin- CD31-CD45+ cell population, used as a control, from enriched hematopoietic Lin- cells peripheral blood. Representative flow cytometric analysis. (B) Representative plots showing the distribution of CD31-CD45+ CTRL cell population and immunophenotypic after three days of cytokine stimulation. (F) Cumulative data are shown as means ± SD of 3 independent experiments in the bar graph.
Anoplopomatidae
Creators: name: Arai, Hisao P.
name: Smith, John W.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Actinopterygii
Scorpaeniformes
Anoplopomatidae

description: Family Anoplopomatidae
Anoplopoma fimbria (Pallas) Sablefish Anisakis sp.
Nematoda gen. sp.
Pseudoterranova decipiens
Pseudoterranova sp.
description: Published as part of Arai, Hisao P. & Smith, John W., 2016, Guide to the Parasites of Fishes of Canada Part V: Nematoda, pp. 1-274 in Zootaxa 4185 (1) on page 207, DOI: 10.11646/zootaxa.4185.1.1, http://zenodo.org/record/165530
Sub-chronic toxicological studies of transition metal complexes of naproxen on sprague-dawley rats
Creators: name: Md. Sharif Hasan
name: Narhari Das
name: Begum, Farida
name: S M Abdur Rahman
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biochemistry
subject: Physiology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified

description: The purpose of this research was to investigate sub-chronic toxicity in animal model. A detailed study was done on the physical, hematological, biochemical and hormonal parameters of both male and female Sprague-Dawley rats after 28 days administration of naproxen and its metal complexes. There were no significant changes found in physical parameters on observation for both male and female rats without some minor differences. However, Naproxen metal complexes showed comparatively lower side effects than naproxen. Hematological report suggested that naproxen was in process of initiating inflammation which was justified by decreasing the mean value hemoglobin and hematocrit level and increasing the white blood cells level. There were no significant changes in biochemical parameters, however, the mean value of blood glucose level and cholesterol seemed to be higher and triglyceride was lower. Thyroid hormone levels were found lower, that was another indication inflammatory process. However, this might have the ability to lower the insulin secretion resulting in increasing blood glucose level. In the present investigation, there were no significant alterations in histopathological studies and physical parameters though some signs of abnormalities had been found but hematological and hormonal data did not suggest any inflammatory or toxicological activity. However, we observed that naproxen showed more side effects than metal complexes which indicated that carboxylic group (–COOH) of naproxen may be responsible for showing those most of the side effects.
Maximum Entropy Method Approach to $θ$ Term
Creators: name: Imachi, Masahiro
name: Shinno, Yasuhiko
name: Yoneyama, Hiroshi
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: In Monte Carlo simulations of lattice field theory with a $θ$ term, one confronts the complex weight problem, or the sign problem. This is circumvented by performing the Fourier transform of the topological charge distribution $P(Q)$. This procedure, however, causes flattening phenomenon of the free energy $f(θ)$, which makes study of the phase structure unfeasible. In order to treat this problem, we apply the maximum entropy method (MEM) to a Gaussian form of $P(Q)$, which serves as a good example to test whether the MEM can be applied effectively to the $θ$ term. We study the case with flattening as well as that without flattening. In the latter case, the results of the MEM agree with those obtained from the direct application of the Fourier transform. For the former, the MEM gives a smoother $f(θ)$ than that of the Fourier transform. Among various default models investigated, the images which yield the least error do not show flattening, although some others cannot be excluded given the uncertainty related to statistical error.
description: PTPTEX , 25 pages with 11 figures
Emergent Relativity
Creators: name: Laughlin, R. B.
Publisher: name: arXiv
Year: 2003
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: A possible resolution of the incompatibility of quantum mechanics and general relativity is that the relativity principle is emergent. I show that the central paradox of black holes also occurs at a liquid-vapor critical surface of a bose condensate but is resolved there by the phenomenon of quantum criticality. I propose that real black holes are actually phase boundaries of the vacuum analogous to this, and that the Einstein field equations simply fail at the event horizon the way quantum hydrodynamics fails at a critical surface. This can occur without violating classical general relativity anywhere experimentally accessible to external observers. Since the low-energy effects that occur at critical points are universal, it is possible to make concrete experimental predictions about such surfaces without knowing much, if anything about the true underlying equations. Many of these predictions are different from accepted views about black holes - in particular the absence of Hawking radiation and the possible transparency of cosmological black hole surfaces. [To appear in the C. N Yang Festschrift (World Sci., Singapore, 2003).]
description: 12 pages of RevTeX, 9 eps figures, corrected typos
Nonlinear optical response spatial self-hase modulation in MoTe2: correlations between \c{hi}(3) and mobility or effective mass
Creators: name: Hu, Lili
name: Sun, Fei
name: Zhao, Hui
name: Zhao, Jimin
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optics (physics.optics)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: We report an unambiguous observation of third-order nonlinear optical effect, spatial self-phase modulation (SSPM), in a MoTe2 dispersion. The values of the third order nonlinear optical coefficients effectively for one layer MoTe2, \c{hi}(3)one-layer, are obtained through the SSPM method at excitation wavelengths 473, 532, 750 and 801 nm, respectively. The wind-chime model is used to explain the ring formation time. The wavelength dependence of \c{hi}(3)one-layer compares well with the photo-absorption spectra. Significantly, we find a correlation between \c{hi}(3) and the carrier mobility μ or effective mass m*, which again further supports the laser-induced ac electron coherence in 2D materials.
High Angular Resolution, Sensitive CS J=2-1 and J=3-2 Imaging of the Protostar L1551 NE: Evidence for Outflow-Triggered Star Formation ?
Creators: name: Yokogawa, S.
name: Kitamura, Y.
name: Momose, M.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: High angular resolution and sensitive aperture synthesis observations of CS ($J=2-1$) and CS ($J=3-2$) emissions toward L1551 NE, the second brightest protostar in the Taurus Molecular Cloud, made with the Nobeyama Millimeter Array are presented. L1551 NE is categorized as a class 0 object deeply embedded in the red-shifted outflow lobe of L1551 IRS 5. Previous studies of the L1551 NE region in CS emission revealed the presence of shell-like components open toward L1551 IRS 5, which seem to trace low-velocity shocks in the swept-up shell driven by the outflow from L1551 IRS 5. In this study, significant CS emission around L1551 NE was detected at the eastern tip of the swept-up shell from $V_{\rm{lsr}}$ = 5.3 km s$^{-1}$ to 10.1 km s$^{-1}$, and the total mass of the dense gas is estimated to be 0.18 $\pm$ 0.02 $M_\odot$. Additionally, the following new structures were successfully revealed: a compact disklike component with a size of $\approx$ 1000 AU just at L1551 NE, an arc-shaped structure around L1551 NE, open toward L1551 NE, with a size of $\sim 5000$ AU, i.e., a bow shock, and a distinct velocity gradient of the dense gas, i.e., deceleration along the outflow axis of L1551 IRS 5. These features suggest that the CS emission traces the post-shocked region where the dense gas associated with L1551 NE and the swept-up shell of the outflow from L1551 IRS 5 interact. Since the age of L1551 NE is comparable to the timescale of the interaction, it is plausible that the formation of L1551 NE was induced by the outflow impact. The compact structure of L1551 NE with a tiny envelope was also revealed, suggesting that the outer envelope of L1551 NE has been blown off by the outflow from L1551 IRS 5.
description: 29 pages, 12 figures, Accepted for Publication in the Astrophysical Journal
title: Text/Conference Paper
Creators: name: Chircu, Alina
name: Sultanow, Eldar
name: Baum, David
name: Koch, Christian
name: Seßler, Matthias
Publisher: name: Gesellschaft für Informatik e.V.
Year: 2019
Subjects: subject: Data Center
subject: Forecasting
subject: Machine Learning
subject: Monitoring
subject: Response Time
subject: Time Series
subject: Utilization
subject: Visualization

description: In this paper, we present a novel tool for data center management that incorporates data visualization and machine learning capabilities. We developed the tool in the context of an action design research project conducted at a large government agency in Germany, which hosts three highly available data centers containing more than 10,000 servers. We derived the requirements for the tool from qualitative interviews with agency employees who are familiar with monitoring the data center infrastructure as well as from a review of existing data center and other large infrastructure monitoring solutions. We implemented a web-based 3D prototype for the tool as an Angular 6 application running on Node.js, and evaluated it with the same employees. Most participants preferred the new tool, which provided a significantly better option and enabled visualization of historical data for all server instances at the same time, as well as real-time charts. Planned improvements will take advantage of the full potential of machine learning for time series forecasting.
title: Text/Conference Paper
Creators: name: Auth, Gunnar
name: Czarnecki, Christian
name: Bensberg, Frank
Publisher: name: Gesellschaft für Informatik e.V.
Year: 2019
Subjects: subject: Robotic Process Automation
subject: Enterprise Architecture
subject: Software Robots

description: The initial idea of Robotic Process Automation (RPA) is the automation of business processes through the presentation layer of existing application systems. For this simple emulation of user input and output by software robots, no changes of the systems and architecture is required. However, considering strategic aspects of aligning business and technology on an enterprise level as well as the growing capabilities of RPA driven by artificial intelligence, interrelations between RPA and Enterprise Architecture (EA) become visible and pose new questions. In this paper we discuss the relationship between RPA and EA in terms of perspectives and implications. As workin- progress we focus on identifying new questions and research opportunities related to RPA and EA.
Additional file 2 of Identification of circulating CD31+CD45+ cell populations with the potential to differentiate into erythroid cells
Creators: name: Monaco, Maria Chiara G.
name: Maric, Dragan
name: Salvucci, Ombretta
name: Passeri, Cristina Antonetti Lamorgese
name: Accorsi, Patrizia
name: Major, Eugene O.
name: Berardi, Anna Concetta
Publisher: name: figshare
Year: 2021
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Computational Biology

description: Additional file 2.
title: Text/Conference Paper
Creators: name: Röller, Klaus
name: Brockmann, Carsten
name: Klingmann, Philipp
Publisher: name: Gesellschaft für Informatik e.V.
Year: 2019
Subjects: subject: Replacement of hardware
subject: upgrade operating system
subject: plan and manage roll-out

description: The rollout of a new version of an operating system can be performed through the upgrade of the operating system on existing devices as well as the replacement of hardware. In this contribution, we propose core process steps and activities to perform both kinds of migrations.
Ecnomina trifurcata Kimmins 1953
Creators: name: Cartwright, David I.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Ecnomidae
Ecnomina
Ecnomina trifurcata

description: Ecnomina trifurcata Kimmins, 1953
Figs 144–146
 Ecnomina trifurcata Kimmins in Mosely and Kimmins, 1953: 382, fig. 263. – Neboiss 1986: 158.
 Diagnosis. Ecnomina trifurcata is a distinctive species which is distinguished by the relatively slender superior appendages and the deep V-shaped split in the inferior appendages meso-distally.
 Description. Head, body and wings brownish; wings (fig. 263a, Mosely and Kimmins 1953) similar to E. legula (Fig. 3). Forewing length about 3.2 times width: male 3.5 mm. Forewing fork 2 relatively long, sessile, length about 1.2 times length of fork 3; fork 3 relatively long, with short footstalk, fork greater than 7 times length footstalk, footstalk length about 0.8 times length cross-vein m, r-m and m nearly contiguous at footstalk fork 3, r-m and m separated by about 0.2 times length of cross-vein m; fork 4 shorter than fork 3; fork 5 long, length about 1.7 times length of fork 4. Hindwing length about 3.5 times width, fork 2 sessile, length about 1.4 times length of fork 3.
Male. (Revised after Kimmins in Mosely and Kimmins 1953). Tergum X membranous, with one pair of relatively slender dorsal processes, fused basally, and with a slightly more elongate ventral pair (Fig. 146). Superior appendages slender; in lateral view, narrowed slightly in distal third, length about 6.5 times width (Fig. 144); in dorsal view, length about 6 times width, dilated slightly distally (Fig. 146). Phallus simple, tubelike, slender, flanged and curved about mid length (Fig. 144). Inferior appendages shorter than superior appendages; in ventral view, fused basally, length about 1.4 times width, rounded laterally, with deep Vshaped split meso-distally (Fig. 145); in lateral view, robust, length about three times width (Fig. 144).
Female. Unknown.
 Type material (not seen): Holotype male, New South Wales, Wentworth Park, Wentworth Falls, 24 Nov 1916, R. J. Tillyard. (BMNH).
 Remarks. No new material of this species has been seen or collected since the holotype in 1916. Ecnomina trifurcata appears to be restricted in distribution and probably is rare as only one male has been collected from the type locality (latitude 33°43'S). Kimmins’ (in Mosely and Kimmins 1953) figures have been redrawn to allow direct comparisons and to accompany the description that is revised in light of new interpretations of Ecnomina genitalic and wing structures.
description: Published as part of Cartwright, David I., 2008, A review of the Australian species of Ecnomina Kimmins and Daternomina Neboiss (Trichoptera: Ecnomidae), pp. 1-76 in Zootaxa 1774 (1) on pages 63-64, DOI: 10.11646/zootaxa.1774.1.1, http://zenodo.org/record/5124133
title: Text/Conference Paper
Creators: name: Kress, Viktor
name: Jung, Janis
name: Zernetsch, Stefan
name: Doll, Konrad
name: Sick, Bernhard
Publisher: name: Gesellschaft für Informatik e.V.
Year: 2019
Subjects: subject: Detection
subject: Cyclist
subject: LSTM Network

description: In this article, we present an approach for start intention detection of cyclists based on their head trajectories. Therefore, we are using a network architecture based on Long Short-Term Memory (LSTM) cells, which is able to handle input sequences of different lengths. This is important because, for example, due to occlusions, cyclists often only become visible to approaching vehicles shortly before dangerous situations occur. Hence, the dependency of the results on the input sequence length is investigated. We use a dataset with 206 situations where cyclists were transitioning from waiting to moving that was recorded from a moving vehicle in inner-city traffic.With an input sequence length of 1.0 s we achieve an F1-score of 96.2% on average 0.680 s after the first movement of the bicycle. We obtain similar results for sequence lengths down to 0.2 s. For shorter sequences, the results regarding the F1-score and the mean detection time deteriorate considerably.
title: 01_0327
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
An X-ray review of MS1054-0321: hot or not?
Creators: name: Gioia, I. M.
name: Braito, V.
name: Branchesi, M.
name: Della Ceca, R.
name: Maccacaro, T.
name: Tran, K. -V.
name: .
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: XMM-Newton observations are presented for the z=0.83 cluster of galaxies MS1054-0321, the highest redshift cluster in the Einstein Extended Medium Sensitivity Survey (EMSS). The temperature inferred by the XMM-Newton data, T=7.2 (+0.7, -0.6) keV, is much lower than the temperature previously reported from ASCA data, T=12.3 (+3.1, -2.2) keV (Donahue et al. 1998), and a little lower than the Chandra temperature, T=10.4(+1.7, -1.5) keV, determined by Jeltema et al. 2001. The discrepancy between the newly derived temperature and the previously derived temperatures is discussed in detail. If one allows the column density to be a free parameter, then the best fit temperature becomes T=8.6 (+1.2, -1.1) keV, and the best fit column density becomes N_(H)=1.33 (+0.15 -0.14) x 10^20 atoms/cm^2. The iron line is well detected in the XMM-Newton spectrum with a value for the abundance of Z=0.33 (+0.19 -0.18) Zsol, in very good agreement with previous determinations. The derived XMM X-ray luminosity for the overall cluster in the 2-10 keV energy band is L_X=(3.81 +/- 0.19) x 10^44 h^-2 erg s^-1 while the bolometric luminosity is L_BOL=(8.05+/-0.40) x 10^44 h^-2 erg s^-1. The XMM-Newton data confirm the substructure in the cluster X-ray morphology already seen by ROSAT and in much more detail by Chandra. The central weak lensing clump is coincident with the main cluster component and has a temperature T=8.1 (+1.3, -1.2) keV. The western weak lensing clump coincides with the western X-ray component which is much cooler with a temperature T=5.6 (+0.8, -0.6)$ keV. Given the newly determined temperature, MS1054-0321 is no longer amongst the hottest clusters known.
description: To appear in the A&A main Journal, 13 pages including 3 postscript figures and 4 tables. Figs. 1, 4, 5 and 7 are too large and are not given here. The whole paper as pdf file is posted at http://www.ira.cnr.it/~gioia/PUB/publications.html
MOESM4 of Protocol for a cluster randomised controlled trial to determine the effectiveness and cost-effectiveness of independent pharmacist prescribing in care homes: the CHIPPS study
Creators: name: Bond, Christine
name: Holland, Richard
name: Alldred, David
name: Arthur, Antony
name: Barton, Garry
name: Blyth, Annie
name: Desborough, James
name: Ford, Joanna
name: Handford, Christine
name: Hill, Helen
name: Hughes, Carmel
name: Maskrey, Vivienne
name: Massey, Kate
name: Phyo Myint
name: Norris, Nigel
name: Poland, Fiona
name: Shepstone, Lee
name: Turner, David
name: Zermansky, Arnold
name: Wright, David
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Additional file 4. SPIRIT 2013 Checklist: Recommended items to address in a clinical trial protocol and related documents.
Additional file 1 of Comparison of 15 dinoflagellate genomes reveals extensive sequence and structural divergence in family Symbiodiniaceae and genus Symbiodinium
Creators: name: González-Pech, Raúl A.
name: Stephens, Timothy G.
name: Yibi Chen
name: Mohamed, Amin R.
name: Yuanyuan Cheng
name: Shah, Sarah
name: Dougan, Katherine E.
name: Fortuin, Michael D. A.
name: Lagorce, Rémi
name: Burt, David W.
name: Debashish Bhattacharya
name: Ragan, Mark A.
name: Chan, Cheong Xin
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: Ecology

description: Additional file 1. Supplementary Note.
MOESM6 of Associations between complex multimorbidity, activities of daily living and mortality among older Norwegians. A prospective cohort study: the HUNT Study, Norway
Creators: name: Storeng, Siri
name: Vinjerui, Kristin
name: Sund, Erik
name: Krokstad, Steinar
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 6 Association between complex multimorbidity (HUNT2) and IADL (HUNT3), mortality and non-participation (HUNT3), multinomial logistic regression.* n = 8340.
Mapping metallicity variations across nearby galaxy disks
Creators: name: Kreckel, K.
name: Ho, I. -T.
name: Blanc, G. A.
name: Groves, B.
name: Santoro, F.
name: Schinnerer, E.
name: Bigiel, F.
name: Chevance, M.
name: Congiu, E.
name: Emsellem, E.
name: Faesi, C.
name: Glover, S. C. O.
name: Grasha, K.
name: Kruijssen, J. M. D.
name: Lang, P.
name: Leroy, A. K.
name: Meidt, S. E.
name: McElroy, R.
name: Pety, J.
name: Rosolowsky, E.
name: Saito, T.
name: Sandstrom, K.
name: Sanchez-Blazquez, P.
name: Schruba, A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The distribution of metals within a galaxy traces the baryon cycle and the buildup of galactic disks, but the detailed gas phase metallicity distribution remains poorly sampled. We have determined the gas phase oxygen abundances for 7,138 HII regions across the disks of eight nearby galaxies using VLT/MUSE optical integral field spectroscopy as part of the PHANGS-MUSE survey. After removing the first order radial gradients present in each galaxy, we look at the statistics of the metallicity offset (Delta O/H) and explore azimuthal variations. Across each galaxy, we find low (sigma=0.03-0.05 dex) scatter at any given radius, indicative of efficient mixing. We compare physical parameters for those HII regions that are 1 sigma outliers towards both enhanced and reduced abundances. Regions with enhanced abundances have high ionization parameter, higher Halpha luminosity, lower Halpha velocity dispersion, younger star clusters and associated molecular gas clouds show higher molecular gas densities. This indicates recent star formation has locally enriched the material. Regions with reduced abundances show increased Halpha velocity dispersions, suggestive of mixing introducing more pristine material. We observe subtle azimuthal variations in half of the sample, but can not always cleanly associate this with the spiral pattern. Regions with enhanced and reduced abundances are found distributed throughout the disk, and in half of our galaxies we can identify subsections of spiral arms with clearly associated metallicity gradients. This suggests spiral arms play a role in organizing and mixing the ISM.
description: 14 pages, 9 figures, 4 Appendices including image atlases, ApJ accepted
Influence of rotational motion of molecules on the thermal conductivity of solid SF6, CHCl3, C6H6, and CCl4
Creators: name: Konstantinov, V. A.
name: Purskii, O. I.
name: Zholonko, N. N.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The thermal conductivity of solid SF6, CHCI3, C6H6, and CCl4 was investigated by the linear-flow method under saturated vapor pressures in the temperature range from 80 K to the corresponding melting temperatures and then recalculated for a constant density of the samples.The contributions of the phonon -phonon and phonon -rotation interactions to the total thermal resis tance were separated using the modified method of reduced coordinates.It is shown that the phonon- rotation contribution to the thermal resistance of the crystals decreases as the rotational motion of the molecules attains more freedom.
description: PDF file,6pages with 8 figures,1 table
Interacting galaxies in the IllustrisTNG simulations -- II: Star formation in the post-merger stage
Creators: name: Hani, Maan H.
name: Gosain, Hayman
name: Ellison, Sara L.
name: Patton, David R.
name: Torrey, Paul
Publisher: name: arXiv
Year: 2020
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Galaxy mergers are a major evolutionary transformation whose effects are borne out by a plethora of observations and numerical simulations. However, most previous simulations have used idealised, isolated, binary mergers and there has not been significant progress on studying statistical samples of galaxy mergers in large cosmological simulations. We present a sample of 27,691 post-merger (PM) galaxies ($0\le z \le 1$) identified from IllustrisTNG: a cosmological, large box, magneto-hydrodynamical simulation suite. The PM sample spans a wide range of merger and galaxy properties ($M_\star$, $μ$, $f_\mathrm{gas}$). We demonstrate that star forming (SF) PMs exhibit enhanced star formation rates (SFRs) on average by a factor of $\sim 2$, while the passive PMs show no statistical enhancement. We find that the SFR enhancements: (1) show no dependence on redshift, (2) anti-correlate with the PM's stellar mass, and (3) correlate with the gas fraction of the PM's progenitors. However, SF PMs show stronger enhancements which may indicate other processes being at play (e.g., gas phase, feedback efficiency). Although the SFR enhancement correlates mildly with the merger mass ratio, the more abundant minor mergers ($0.1 \le μ< 0.3 $) still contribute $\sim 50\%$ of the total SFR enhancement. By tracing the PM sample forward in time, we find that galaxy mergers can drive significant SFR enhancements which decay over $\sim 0.5$ Gyr independent of the merger mass ratio, although the decay timescale is dependent on the simulation resolution. The strongest merger-driven starburst galaxies evolve to be passive/quenched on faster timescales than their controls.
description: accepted for publication in MNRAS