cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A single population scheme for FR I and FR II radio galaxies
Creators: name: Snellen, Ignas
name: Best, Philip
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The presence of two distant FR I radio galaxies in the Hubble Deep Field plus Flanking Fields indicates that the number density of these objects is about 10-50 times higher at z>1 than in the local universe. This is in strong contrast with the idea that FR Is undergo no cosmological evolution. We advocate that the cosmological evolution of radio sources may be independent of FR class, and instead solely a function of radio power. In this scenario the evolutionary properties of extragalactic radio sources can be fully described within a `single population scheme'.
description: LaTeX, 6 pages, 1 fig: Elsevier science format - NAR. Proceedings of the workshop "Radio galaxies: past, present & future". eds. Matt Jarvis et al. Leiden, Nov, 2002
Additional file 1 of The long way to diagnosis: attention disorder, alcohol addiction or congenital disorder of glycosylation? A case report
Creators: name: Faustmann, Timo Jendrik
name: Hensel, Lukas
name: Bahic, Armin
name: Wada, Yoshinao
name: Grüneberg, Marianne
name: Marquardt, Thorsten
name: Kamp, Daniel
name: Schilbach, Leonhard
Publisher: name: figshare
Year: 2025
Subjects: Medicine
Neuroscience
Pharmacology
Biotechnology
Mental Health
Hematology
Computational Biology

description: Supplementary Material 1
The Effects of Magnetic Resonance Imaging (MRI) On Tensile Strength and Indentation Hardness of Acrylic Resin Denture Base Materials
Creators: name: Taqa, Amer A.
Publisher: name: figshare
Year: 2019
Subjects: subject: 110599 Dentistry not elsewhere classified
subject: FOS: Clinical medicine

description: The Effects of Magnetic Resonance Imaging(MRI) On Tensile Strength and IndentationHardness of Acrylic Resin Denture BaseMaterials
Simulation of Curve Reflector using HFSS
Creators: name: Kar, Girija Nandan
Publisher: name: figshare
Year: 2021
Subjects: subject: 100501 Antennas and Propagation
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: 100505 Microwave and Millimetrewave Theory and Technology

description: Technical report of simulation of a curve reflector antenna at 5GHz in HFSS.
Monitoring RXTE Observations of Markarian 348: the origin of the column density variations
Creators: name: Akylas, A.
name: Georgantopoulos, I.
name: Griffiths, R. G.
name: Papadakis, I. E.
name: Mastichiadis, A.
name: Warwick, R. S.
name: Nandra, K.
name: Smith, D. A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyze 37 RXTE observations of the type 2 Seyfert galaxy Mrk348 obtained during a period of 14 months. We confirm the spectral variability previous reported by Smith et al., in the sense that thecolumn density decreases by a factor of ~3 as the count rate increases. Column density variations could possibly originate either due to the random drift of clouds within the absorption screen, or due to photoionization processes. Our modeling of the observed variations implies that the first scenario is more likely. These clouds should lie in a distance of >2 light years from the source, having a diameter of a few light days and a density of >10^7 cm^(-3), hence probably residing outside the Broad Line Region.
description: 6 pages, 3 figures, to appear in MNRAS
The influence of a new irrigant solution on the apical microleakage of obturated root canals
Creators: name: Taqa, Amer A.
Publisher: name: figshare
Year: 2019
Subjects: subject: 110501 Dental Materials and Equipment
subject: FOS: Clinical medicine

description: The influence of a new irrigant solution on theapical microleakage of obturated root canals
Additional file 1 of Improvement cues of lesion absorption using the adjuvant therapy of traditional Chinese medicine Qinbudan tablet for retreatment pulmonary tuberculosis with standard anti-tuberculosis regimen
Creators: name: Zhang, Shao-Yan
name: Fu, Ji-You
name: Guo, Xiao-Yan
name: Wu, Ding-Zhong
name: Zhang, Tong
name: Li, Cui
name: Qiu, Lei
name: Shao, Chang-Rong
name: Xiao, He-Ping
name: Chu, Nai-Hui
name: Deng, Qun-Yi
name: Zhang, Xia
name: Yan, Xiao-Feng
name: Wang, Zhao-Long
name: Zhang, Zhi-Jie
name: Jiang, Xin
name: Zheng, Yue-Juan
name: Zheng, Pei-Yong
name: Zhang, Hui-Yong
name: Lu, Zhen-Hui
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1.
The Effect Of Addition Of Castor Oil, Grape Seed Oil And Fenugreek Oil On Some Properties Of Cold Cure Acrylic Resin Denture Base Material.
Creators: name: Taqa, Amer A.
Publisher: name: figshare
Year: 2019
Subjects: subject: 110501 Dental Materials and Equipment
subject: FOS: Clinical medicine

description: The Effect Of Addition Of Castor Oil, GrapeSeed Oil And Fenugreek Oil On Some PropertiesOf Cold Cure Acrylic Resin DentureBase Material.
Cabeza baeostigma HANSSON & LASALLE 2003, sp. n.
Creators: name: HANSSON, C.
name: LASALLE, J.
Publisher: name: Zenodo
Year: 2003
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Cabeza
Cabeza baeostigma

description: Cabeza baeostigma sp. n.
(figures 67, 68, 78, 81, 82)
 Diagnosis
Funicular segment 0.3× as long as clava in female (figure 67); female and male scape narrow (figures 67, 68); frons without a blunt transverse edge in front of anterior ocellus (figure 81); scutellum predominantly reticulate, smooth only on sides; fore wing with basal two-thirds of membrane bare; submarginal vein with two setae; stigmal vein very short (figure 78); petiole 0.5× as long as wide.
description: Published as part of HANSSON, C. & LASALLE, J., 2003, Revision of the Neotropical species of the tribe Euderomphalini (Hymenoptera: Eulophidae), pp. 697-778 in Journal of Natural History 37 (6) on page 707, DOI: 10.1080/00222930110096744, http://zenodo.org/record/5274114
Elliptic flow and freezeout from the parton cascade MPC
Creators: name: Molnar, Denes
name: Gyulassy, Miklos
Publisher: name: arXiv
Year: 2001
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Differential elliptic flow out to p_T ~ 5 GeV/c and particle spectra are calculated using the MPC elastic parton cascade model for Au+Au at Ecm ~ 130A GeV. The evolution is computed from parton transport theory, followed by hadronization either via independent fragmentation or by imposing parton-hadron duality. With pQCD elastic cross sections, very large initial gluon densities dN/deta > 7000 are required to reproduce the data measured by the STAR collaboration. In addition, elliptic flow and the p_T spectra are shown to be very sensit ive to particle subdivision.
description: Contribution to Quark Matter 2001, to appear in proceedins. Text + all figures. Corrected label in Fig. 1a
Dual black hole associated with obscured and unobscured AGN: CXO J101527.2+625911
Creators: name: Kim, D. -C.
name: Momjian, E.
name: Yoon, Ilsang
name: Kim, Minjin
name: Evans, A. S.
name: Kim, Ji Hoon
name: Linden, S. T.
name: Barcos-Munoz, L.
name: Privon, G. C.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report the results of an investigation to determine the nature of the offset active galactic nucleus (AGN) found in the source CXO J101527.2+625911. Hubble Space Telescope and Chandra X-ray observatory data had suggested that the offset AGN, which has an angular separation of only 0\farcs26 from the center of the host galaxy, is a recoiled Super Massive Black Hole (rSMBH). We carried out high angular resolution observations with both the VLBA (1.54 GHz) and the VLA (10.0 GHz \& 33.0 GHz) and detected a single compact radio source in the center of the host galaxy, with no radio continuum emission associated with the offset AGN. The detected radio source has a high brightness temperature value of $T_b=7.2\times10^{7}$ K, indicating that the radio emission is associated with an AGN. Furthermore, we present the decomposition of high-resolution KECK spectra of the [O III]5007Åline into two narrow emission line components, which is a characteristic sign of a dual black hole system. These new radio and optical wavelength results suggest that CXO J101527.2+625911 is the host of a dual black hole system rather than a rSMBH.
description: ApJ accepted
Correlations and charge distributions of medium heavy nuclei
Creators: name: Anguiano, Marta
name: Co', Giampaolo
Publisher: name: arXiv
Year: 2001
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The effects of long- and short-range correlations on the charge distributions of some medium and heavy nuclei are investigated. The long-range correlations are treated within the Random Phase Approximation framework and the short-range correlations with a model inspired to the Correlation Basis Function theory. The two type of correlations produce effects of the same order of magnitude. A comparison with the empirical charge distribution difference between 206Pb and 205Tl shows the need of including both correlations to obtain a good description of the data.
description: 20 pages, Latex, accepted for publication in Jour. Phys. G
Quantify entanglement by concurrence hierarchy
Creators: name: Fan, Heng
name: Matsumoto, Keiji
name: Imai, Hiroshi
Publisher: name: arXiv
Year: 2002
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We define the concurrence hierarchy as d-1 independent invariants under local unitary transformations in d-level quantum system. The first one is the original concurrence defined by Wootters et al in 2-level quantum system and generalized to d-level pure quantum states case. We propose to use this concurrence hierarchy as measurement of entanglement. This measurement does not increase under local quantum operations and classical communication.
description: Revtex, 6 pages
Democricetodon gracilis Fahlbusch 1964
Creators: name: Aguilar, Jean-Pierre
name: Michaux, Jacques
name: Bertrand, Aunay
name: Calvet, Marc
name: Lazzari, Vincent
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Democricetodon
Democricetodon gracilis

description: Democricetodon gracilis Fahlbusch, 1964 (Fig. 4 A-C; Tableau 2)
MATÉRIEL ET DIMENSIONS. — Dents isolées (BLQ 1 nº 2122 à 2142). Dimensions: voir Tableau 2.
DESCRIPTION
 Molaires inférieures
L’unique m1, de très petite taille (Fig. 3), montre un petit antéroconide dont la partie linguale rejoint le métaconide et un court mésolophide. Sur les m2, le mésolophide est de longueur variable, absent ou à peine marqué (7) court (5), ou moyennement long (3).
 Molaires supérieures
Elles ne sont représentées que par des M2 qui montrent un double protolophule et un métalophule proverse. Le mésolophe est plus développé que sur les molaires inférieures, il est toujours long et atteint le bord de la couronne. Le sinus est bordé par une crête cingulaire plus ou moins forte qui se développe à partir du flanc de l’hypocône.
DISCUSSION
 La présence, au sein du matériel attribué au genre Democricetodon, de quelques molaires singulières par leur petite taille (Figs 3; 5) présentant une morphologie et des dimensions comparables à celles de D. gracilis des gisements de Langenmoosen et de Sandelzhausen (Falbusch 1964; Moser et al. 2009), témoigne de l’existence de cette espèce au sein du gisement.Les molaires de Blanquatère 1 ont toutefois des dimensions inférieures à celles de la population de D. gracilis de Vieux-Collonges (Maridet 2002). Nous noterons que cette espèce est assez rare dans ces deux gisements où le genre Democricetodon est pourtant abondamment représenté.
description: Published as part of Aguilar, Jean-Pierre, Michaux, Jacques, Bertrand, Aunay, Calvet, Marc & Lazzari, Vincent, 2010, Compléments à l'étude des rongeurs (Mammalia, Rodentia, Cricetidae, Eomyidae, Sciuridae) du gisement karstique de Blanquatère 1 (Miocène moyen, sud de la France), pp. 515-533 in Geodiversitas 32 (3) on page 520, DOI: 10.5252/g2010n3a8, http://zenodo.org/record/5381700
Additional file 1 of Online calculator to predict early mortality in patient with surgically treated recurrent lower-grade glioma
Creators: name: Wei, Ruolun
name: Zhao, Chao
name: Li, Jianguo
name: Yang, Fengdong
name: Xue, Yake
name: Wei, Xinting
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 1 Supplementary Table S1. The optimal cutoff values of hematological factors for overall survival by Receiver operating characteristic (ROC) curve analysis.
The effect of recycled polymethylmethacrylate on some physical and chemical properties of acrylic resin denture base
Creators: name: Taqa, Amer A.
Publisher: name: figshare
Year: 2019
Subjects: subject: 110599 Dentistry not elsewhere classified
subject: FOS: Clinical medicine

description: The effect of recycled polymethylmethacrylate on some physical and chemical properties of acrylic resin denture base
Predicting the deposition spot radius and the nanoparticle concentration distribution in an electrostatic precipitator
Creators: name: Preger, Calle
name: Overgaard, Niels C.
name: Messing, Maria E.
name: Magnusson, Martin H.
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biophysics
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer
subject: 60506 Virology

description: Deposition of aerosol nanoparticles using an electrostatic precipitator is widely used in the aerosol community. Despite this, basic knowledge regarding what governs the deposition has been missing. This concerns the prediction of the size of the particle collection zone, but also, perhaps more importantly, prediction of the nanoparticle concentration distribution on the substrate, both of which are necessary to achieve faster and more precise deposition. In this article, we have used COMSOL Multiphysics simulations, experimental depositions, and two analytical models to describe the deposition. Based on that, we propose a simple equation that can be used to predict the size of the deposition spot as well as the particle concentration on the substrate. The equation we derive concludes that the size of the deposition spot only depends on the gas flow rate into the precipitator, and on the constant drift velocity of a particle in an electric field. The equation also displays that the deposited particle concentration is independent of the gas flow rate. Our general mathematical analysis has great applicability, as it can be used to model different geometries and different types of deposition methods than the one described in this article. We can therefore also propose that the drift velocity in this model easily could be replaced by another velocity acting on the particles at other deposition conditions, for instance, the thermophoretic velocity during thermophoretic deposition. This would result in the same dependence as presented in this article. Finally, we demonstrate analytically and through experiment that the particle distribution inside the spot will be homogenous and follows a top hat profile.
Dissecting the Homunculus nebula around Eta Carinae with spatially resolved near-infrared spectroscopy
Creators: name: Smith, Nathan
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Near-infrared emission lines provide unique diagnostics of the geometry, structure, kinematics, and excitation of eta Carinae's circumstellar ejecta, and give clues to the nature of its wind. The infrared spectrum is a strong function of position in eta Car's nebula, with a mix of intrinsic and reflected emission. Molecular hydrogen traces cool gas and dust in the polar lobes, while [Fe II] blankets their inner surfaces. These lines reveal the back wall of the SE polar lobe for the first time, and give the clearest picture yet of the 3-D geometry. Additionally, collisionally-excited [Fe II] reveals the kinematic structure of a recently discovered `Little Homunculus' expanding inside the larger one. Equatorial gas in the `Fan', on the other hand, shows a spectrum indicating recombination and fluorescent pumping. Some equatorial ejecta glow in the He I 10830 line, showing evidence for material ejected in the 1890 outburst of eta Car. Closer to the star, the compact `Weigelt blobs' are marginally resolved, allowing their infrared spectrum to be separated from the star for the first time. In general, infrared spectra reveal a coherent, directional dependence of excitation in the Homunculus: polar ejecta are collisionally excited, whereas equatorial ejecta are dominated by fluorescence and normal photoexcitation. These are important clues to the geometry of the central star's UV radiation field. Reflected near-infrared emission lines also reveal interesting latitudinal dependence in the stellar wind.
description: To appear in Monthly Notices, December 21 2002 (MNRAS, 337, 1252). 18 pages, 20 figures
The Effect of Thyme and Nigella Oil on Some Properties of Acrylic Resin Denture Base
Creators: name: Taqa, Amer A.
Publisher: name: figshare
Year: 2019
Subjects: subject: 110599 Dentistry not elsewhere classified
subject: FOS: Clinical medicine

description: The Effect of Thyme and Nigella Oil on Some Properties of Acrylic Resin Denture Base
Fabrication and characterization of aluminum SQUID transmission lines
Creators: name: Planat, Luca
name: Al-Tavil, Ekaterina
name: Martinez, Javier Puertas
name: Dassonneville, Remy
name: Foroughi, Farshad
name: Leger, Sebastien
name: Bharadwaj, Karthik
name: Delaforce, Jovian
name: Milchakov, Vladimir
name: Naud, Cecile
name: Buisson, Olivier
name: Hasch-Guichard, Wiebke
name: Roch, Nicolas
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We report on the fabrication and characterization of 50 Ohms, flux-tunable, low-loss, SQUID-based transmission lines. The fabrication process relies on the deposition of a thin dielectric layer (few tens of nanometers) via Atomic Layer Deposition (ALD) on top of a SQUID array, the whole structure is then covered by a non-superconducting metallic top ground plane. We present experimental results from five different samples. We systematically characterize their microscopic parameters by measuring the propagating phase in these structures. We also investigate losses and discriminate conductor from dielectric losses. This fabrication method offers several advantages. First, the SQUID array fabrication does not rely on a Niobium tri-layer process but on a simpler double angle evaporation technique. Second, ALD provides high quality dielectric leading to low-loss devices. Further, the SQUID array fabrication is based on a standard, all-aluminum process, allowing direct integration with superconducting qubits. Moreover, our devices are in-situ flux tunable, allowing mitigation of incertitude inherent to any fabrication process. Finally, the unit cell being a single SQUID (no extra ground capacitance is needed), it is straightforward to modulate the size of the unit cell periodically, allowing band-engineering. This fabrication process can be directly applied to traveling wave parametric amplifiers.
description: 9 pages, 9 figures, Appendixes
Supplementary figures S1 to S5 from Articulation and growth of skeletal elements in balanid barnacles (Balanidae, Balanomorpha, Cirripedia)
Creators: name: Checa, Antonio G.
name: Salas, Carmen
name: Rodríguez-Navarro, Alejandro B.
name: Grenier, Christian
name: Lagos, Nelson A.
Publisher: name: The Royal Society
Year: 2019
Subjects: subject: Biophysics
subject: 90301 Biomaterials
subject: FOS: Medical engineering

description: Supplementary figure S1. Growth plasticity in A. psittacus. Supplementary figure S2. Micro-CT analysis of A. psittacus. Supplementary figure S3. Dorsoventral thin section through the carina and rostrum of the shell of a methacrylate-embedded specimen of A. psittacus, showing the main morphological elements. Supplementary figure S4. TEM of membranes of A. psittacus extracted from different areas of the plates and plate margins. Supplementary figure S5. Formation of elongated viscous fingers using the lifting procedure.
The size of a quasar's mid-IR emission region inferred from microlensed images of Q2237+0305
Creators: name: Wyithe, J. S. B.
name: Agol, E.
name: Fluke, C. J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use published mid-IR and V-band flux ratios for images A and B of Q2237+0305 to demonstrate that the size of the mid-IR emission region has a scale comparable to or larger than the microlens Einstein Radius (ER, ~10^17 cm for solar mass stars). Q2237+0305 has been monitored extensively in the R and V-bands for ~15 years. The variability record shows significant microlensing variability of the optical emission region, and has been used by several studies to demonstrate that the optical emission region is much smaller than the ER for solar-mass objects. For the majority of the monitoring history, the optical flux ratios have differed significantly from those predicted by macro-models. In contrast, recent observations in mid-IR show flux ratios similar to those measured in the radio, and to predictions of some lens models, implying that the mid-IR flux is emitted from a region that is at least 2 orders of magnitude larger than the optical emission region. We have calculated the likeli-hood of the observed mid-IR flux ratio as a function of mid-IR source size given the observed V-band flux ratio. The expected flux ratio for a source having dimensions of ~1 ER is a sensitive function of the macro model adopted. However we find that the probability of source size given the observed flux ratios is primarily sensitive to the ratio of the macro-model magnifications. The majority of published macro models for Q2237+0305 yield a flux ratio for images B and A of 0.8 - 1.1. By combining probabilities from the ratios A/B and C/D we infer that the diameter of a circular IR emission region is >1ER with >95% confidence. For microlensing by low-mass stars, this source size limit rules out non-thermal processes such as synchrotron as mechanisms for mid-IR emission.
description: 13 pages, 8 figures. To be published in MNRAS
Void Analysis of Hadronic Density Fluctuations at Phase Transition
Creators: name: Hwa, Rudolph C.
name: Zhang, Qing-hui
Publisher: name: arXiv
Year: 2001
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The event-to-event fluctuations of hadron multiplicities are studied for a quark system undergoing second-order phase transition to hadrons. Emphasis is placed on the search for an observable signature that is realistic for heavy-ion collisions. It is suggested that in the 2-dimensional y-phi space the produced particles selected in a very narrow p_T window may exhibit clustering patterns even when integrated over the entire emission time. Using the Ising model to simulate the critical phenomenon and taking into account a p_T distribution that depends on the emission time, we study in the framework of the void analysis proposed earlier and find scaling behavior. The scaling exponents turn out to be larger than the ones found before for pure configurations without mixing. The signature is robust in that it is insensitive to the precise scheme of simulating time evolution. Thus it should reveal whether or not the dense matter created in heavy-ion collisions is a quark-gluon plasma before hadronization.
description: 11 pages in LaTeX + 6 figures in ps
Neutron electric form factor at large momentum transfer
Creators: name: Tomasi-Gustafsson, Egle
name: Rekalo, Michail P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Based on the recent, high precision data for elastic electron scattering from protons and deuterons, at relatively large momentum transfer $Q^2$, we determine the neutron electric form factor up to $Q^2=3.5$ GeV$^2$. The values obtained from the data (in the framework of the nonrelativistic impulse approximation) are larger than commonly assumed and are in good agreement with the Gari-Krümpelmann parametrization of the nucleon electromagnetic form factors.
description: 11 pages 2 figures
Development and evaluation of a catalytic stripper for the measurement of solid ultrafine particle emissions from internal combustion engines
Creators: name: A. D. Melas
name: V. Koidi
name: D. Deloglou
name: E. Daskalos
name: D. Zarvalis
name: E. Papaioannou
name: A. G. Konstandopoulos
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Biotechnology
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: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Solid particle number vehicle exhaust measurements necessitate an aerosol conditioning system that removes efficiently volatile particles, does not create artifacts, and minimizes solid nucleation particle losses. Here, we present the development and evaluation of a catalytic stripper (CS) based on a unique dual-function monolithic reactor that oxidizes hydrocarbons and stores sulfur material. The CS was tested for its tetracontane particle removal efficiency, sulfur adsorption capacity with sulfur dioxide, and particle penetration with solid CAST-generated particles. The optimal operation conditions were examined including different aerosol flows and configurations, i.e., as a stand-alone device and as part of a volatile removal system with a hot and a cold dilution stage upstream and downstream of the CS, respectively. The CS managed to comply with current legislation requirements for solid particle number measurements down to 23 nm as a stand-alone device and showed great potential as part of a volatile particle removal (VPR) system for measurements at least down to 10 nm. Finally, we compared the performance of two VPR systems that use the developed CS (VPR-CS) and an evaporation tube (VPR-ET), respectively. Our results suggest that the VPR-CS exhibits higher volatile removal efficiency without creating artifacts while the particle losses are lower with the VPR-ET. Nevertheless, when measuring solid nucleation particles generated by a diesel engine with the VPR-CS, the measurement uncertainty was very low due to its high particle penetration fractions.
Cabeza laticeps HANSSON & LASALLE 2003, sp. n.
Creators: name: HANSSON, C.
name: LASALLE, J.
Publisher: name: Zenodo
Year: 2003
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Cabeza
Cabeza laticeps

description: Cabeza laticeps sp. n.
(figures 71, 80, 86)
 Diagnosis
Male scape strongly flattened and wide (figure 71); head very transverse, 2.2× as wide as high (figure 86); frons with a blunt transverse edge in front of anterior ocellus (figure 86); submarginal vein with one seta (figure 80); basal two-thirds of wing membrane bare, setae in apical one-third sparsely situated; dorsellum visible as a wide and short stripe; petiole 0.5× as long as wide, dorsal surface smooth and shiny.
 Male (length of body= 1.1 mm)
 Colour. Scape and pedicel dark brown; flagellar segment 1 yellowish brown, 2–4 pale yellowish brown. Frons metallic bluish-purple. Vertex dark brown with metallic tinges. Mesoscutum metallic purple. Scutellum golden with purple tinges. Propodeum golden-green, laterally with purple tinges. Coxae and femora dark brown; fore tibia pale with infuscate base, mid tibia infuscate with apical one-half paler, hind tibia dark; tarsi pale. Fore wing hyaline with surface just below base of marginal vein strongly infuscate. Petiole dark brown. Gaster shiny, metallic purplish blue.
 Head. Antenna as in figure 71. HE/MS/MO: 1.2/1.0/1.1. Frons with weak small meshed reticulation laterad to antennal scrobes, meshes ± isodiametric, surface between scrobes smooth and shiny. Vertex smooth and shiny in front of vertexal suture, behind suture with strong small meshed reticulation and ± wrinkled. POL/OOL/POO: 1.4/1.0/not measurable. Occipital margin as a sharp edge. WH/WT=1.4.
 Mesosoma. Mesoscutum with weak and engraved reticulation. Scutellum 0.7× as long as wide, with weak and engraved reticulation. Dorsellum visible as a wide and short shiny stripe. TPS distinctly curved. Fore wing with two admarginal setae; submarginal vein with one seta; basal two-thirds of wing membrane bare, apical one-third with sparse setation; LW/LM/HW: 1.7/1.0/1.0; PM/ST =0.8. Propodeum smooth and shiny.
 Metasoma. Petiole 0.5× as long as wide; dorsal surface smooth and shiny. MM/LG=1.2.
 Material examined
 H: W, Brazil: Santa Catarina, Nova Teutonia, 10 December 1949, F. Plaumann (BMNH).
description: Published as part of HANSSON, C. & LASALLE, J., 2003, Revision of the Neotropical species of the tribe Euderomphalini (Hymenoptera: Eulophidae), pp. 697-778 in Journal of Natural History 37 (6) on page 709, DOI: 10.1080/00222930110096744, http://zenodo.org/record/5274114
Superhumps in Cataclysmic Binaries. XXIII. V442 Ophiuchi and RX J1643.7+3402
Creators: name: Patterson, Joseph
name: Fenton, William
name: Thorstensen, John
name: Harvey, David
name: Skillman, David
name: Fried, Robert
name: Monard, Berto
name: O'Donoghue, Darragh
name: Beshore, Edward
name: Martin, Brian
name: Niarchos, Panos
name: Vanmunster, Tonny
name: Foote, Jerry
name: Bolt, Greg
name: Rea, Robert
name: Cook, Lewis
name: Butterworth, Neil
name: Wood, Matt
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the results of long observing campaigns on two novalike variables: V442 Ophiuchi and RX J1643.7+3402. These stars have high-excitation spectra, complex line profiles signifying mass loss at particular orbital phases, and similar orbital periods (respectively 0.12433 and 0.12056 d). They are well-credentialed members of the SW Sex class of cataclysmic variables. Their light curves are also quite complex. V442 Oph shows periodic signals with periods of 0.12090(8) and 4.37(15) days, and RX J1643.7+3402 shows similar signals at 0.11696(8) d and 4.05(12) d. We interpret these short and long periods respectively as a "negative superhump" and the wobble period of the accretion disk. The superhump could then possibly arise from the heating of the secondary (and structures fixed in the orbital frame) by inner-disk radiation, which reaches the secondary relatively unimpeded since the disk is not coplanar. At higher frequencies, both stars show another type of variability: quasi-periodic oscillations (QPOs) with a period near 1000 seconds. Underlying these strong signals of low stability may be weak signals of higher stability. Similar QPOs, and negative superhumps, are quite common features in SW Sex stars. Both can in principle be explained by ascribing strong magnetism to the white dwarf member of the binary; and we suggest that SW Sex stars are borderline AM Herculis binaries, usually drowned by a high accretion rate. This would provide an ancestor channel for AM Hers, whose origin is still mysterious.
description: PDF, 41 pages, 4 tables, 16 figures; accepted, in press, to appear December 2002, PASP; more info at http://cba.phys.columbia.edu/
Democricetodon gaillardi
Creators: name: Aguilar, Jean-Pierre
name: Michaux, Jacques
name: Bertrand, Aunay
name: Calvet, Marc
name: Lazzari, Vincent
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Democricetodon
Democricetodon gaillardi

description: Democricetodon aff. gaillardi (Schaub, 1925) (Fig. 4 P-R; Tableau 4)
MATÉRIEL ET DIMENSIONS. — Dents isolées (BLQ 1 nº 2143 à 2159). Dimensions: voir Tableau 4.
DESCRIPTION
 Molaires inférieures
Elles sont caractérisées par un mésolophide très développé, atteignant le bord lingual et pouvant développer un petit mésostylide. Le sinuside est fermé par une crête labiale issue de la partie postéro-basale du protoconide tandis que le mésosinuside est obturé par une crête linguale issue de la partie postéro-basale du métaconide sur laquelle est éventuellement présent le mésostylide.
 Molaires supérieures
Les M1 montrent un mésolophe bien développé qui n’atteint le bord lingual que sur deux dents. Il y a un double protolophule sur trois dents, le métacône est isolé sur une molaire, tandis que sur les autres le métalophule est rétroverse et délimite avec le postérolophe un petit postérosinus. Sur la M2 le mésolophe atteint le bord lingual, le protolophule est double et le métalophule rétroverse.
DISCUSSION
 Ces molaires se distinguent des autres molaires de Democricetodon, présentes dans le gisement par un mésolophe(ide) plus développé en hauteur et longueur et des dimensions légèrement supérieures (Figs 3; 5). En effet, chez D. aff. mutilus le mésolophide est rarement long et ne développe pas de mésostylide alors que ce caractère se retrouve chez D. gaillardi. En revanche, ces molaires se différencient de l’espèce D. gaillardi par une morphologie beaucoup plus simple: antérocone(ide) non dédoublé, mésostyle(ide) peu développé et absence d’ectomésolophe(ide), caractères généralement présents chez l’espèce de Sansan.Toutefois dans la population de D. gaillardi de Sansan, présente dans les collections de l’Université Montpellier 2, il existe quelques dents avec des morphotypes plus simples comparables à celles de Blanquatère 1. Comme les dimensions entrent dans le domaine de variation de celui des molaires de Sansan (Baudelot 1972; Maridet 2002) et que la morphologie simplifiée pourrait s’expliquer par l’âge plus ancien de Blanquatère 1, nous attribuons ces quelques molaires à Democricetodon aff. gaillardi.
description: Published as part of Aguilar, Jean-Pierre, Michaux, Jacques, Bertrand, Aunay, Calvet, Marc & Lazzari, Vincent, 2010, Compléments à l'étude des rongeurs (Mammalia, Rodentia, Cricetidae, Eomyidae, Sciuridae) du gisement karstique de Blanquatère 1 (Miocène moyen, sud de la France), pp. 515-533 in Geodiversitas 32 (3) on pages 522-523, DOI: 10.5252/g2010n3a8, http://zenodo.org/record/5381700
Interweaving Pathways of Innovation: Visualizing the R&D Dynamics of Companies Provided by Patent Data
Creators: name: Smuc, Michael
name: Windhager, Florian
name: Federico, Paolo
name: Amor-Amoros, Albert
Publisher: name: Zenodo
Year: 2015
Subjects: patent data, visual analytics, visualization, information visualization, space-time cube, time-oriented data, innovation

description: The global competition between research and development agencies (universities, organizations or individual inventors)
 is regulated by public patent databases, which are a rich source of data, offering insights into the dynamics of technological
 innovation The EXPAND research project is dedicated to the visual exploration of patent dynamics, with a focus on how to
 visualize R&D trends and dynamics of corporate actors over time We show various options to explore selected data of
 companies, countries or technology areas in a three dimensional space, which unfolds between the knowledge maps of patent
 classifications and the temporal dimension Within this space, individual pathways of innovation are weaving into collaborative
 innovation networks and bundles, which again are feeding into collective flows, aiming for strategically relevant R&D areas
The Effect of recycled polymethylmethacrylate Additive on the physical properties of Dental Modelling Wax
Creators: name: Taqa, Amer A.
Publisher: name: figshare
Year: 2019
Subjects: subject: 110502 Dental Therapeutics, Pharmacology and Toxicology
subject: FOS: Clinical medicine

description: TThe Effect of recycled polymethylmethacrylate Additive on the physical properties of Dental Modelling Wax
Multiple scattering and $p_t$-broadening at RHIC energies
Creators: name: Papp, G.
name: Barnafoldi, G. G.
name: Fai, G.
name: Levai, P.
name: Zhang, Y.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: In ultrarelativistic heavy-ion collisions, in the 2 GeV$
description: 4 pages, talk presented at the 15th International Conference on Ultra-Relativistic Nucleus-Nucleus Collisions (QM 2001), Long Island, New York, January 15 - 20, 2001
Constraints on the mass-profile of the lens galaxy G2237+0305
Creators: name: Wyithe, J. S. B.
name: Agol, E.
name: Turner, E. L.
name: Schmidt, R. W.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Published parametric models of the Einstein Cross gravitational lens demonstrate that the image geometry can be reproduced by families of models. In particular, the slope of the mass-profile for the lens galaxy is unconstrained. However, recent models predict a dependence of image flux ratios on the slope of the mass profile. We use this dependence to constrain the mass profile by calculating the likelihood of the slope using published mid-IR flux ratios (including microlensing variability). We find that the galaxy is likely to be flatter than isothermal, and therefore that the mass-to-light ratio is decreasing in the inner kpc.
description: 9 pages 7 figures. To be published in MNRAS
Three-dimensional charge transport mapping by two-photon absorption edge transient-current technique in synthetic single-crystalline diamond
Creators: name: Dorfer, C.
name: Hits, D.
name: Kasmi, L.
name: Kramberger, G.
name: Lucchini, M.
name: Mikuz, M.
name: Wallny, R.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: We demonstrate the application of two-photon absorption transient current technique to wide bandgap semiconductors. We utilize it to probe charge transport properties of single-crystal Chemical Vapor Deposition (scCVD) diamond. The charge carriers, inside the scCVD diamond sample, are excited by a femtosecond laser through simultaneous absorption of two photons. Due to the nature of two-photon absorption, the generation of charge carriers is confined in space (3-D) around the focal point of the laser. Such localized charge injection allows to probe the charge transport properties of the semiconductor bulk with a fine-grained 3-D resolution. Exploiting spatial confinement of the generated charge, the electrical field of the diamond bulk was mapped at different depths and compared to an X-ray diffraction topograph of the sample. Measurements utilizing this method provide a unique way of exploring spatial variations of charge transport properties in transparent wide-bandgap semiconductors.
description: This article may be downloaded for personal use only. Any other use requires prior permission of the author and AIP Publishing. The following article appeared in Applied Physics Letters and may be found at https://doi.org/10.1063/1.5090850
The effect of oil piper Cubeba on the cariogenic bacteria( Streptococcus mutans and staphylococcus
Creators: name: Taqa, Amer A.
Publisher: name: figshare
Year: 2019
Subjects: Biochemistry

description: The effect of oil piper Cubeba on the cariogenic bacteria( Streptococcus mutans and staphylococcus
Additional file 4: of Menstrual hygiene management in rural schools of Zambia: a descriptive study of knowledge, experiences and challenges faced by schoolgirls
Creators: name: Chinyama, Joyce
name: Chipungu, Jenala
name: Rudd, Cheryl
name: Mwale, Mercy
name: Verstraete, Lavuun
name: Sikamo, Charity
name: Mutale, Wilbroad
name: Chilengi, Roma
name: Sharma, Anjali
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: KII guide for teachers. (DOCX 29 kb)
Thermal Tides in Rotating Hot Jupiters
Creators: name: Lee, Umin
name: Murakami, Daiki
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We calculate tidal torque due to semi-diurnal thermal tides in rotating hot Jupiters, taking account of the effects of radiative cooling in the envelope and of the planets rotation on the tidal responses. We use a simple Jovian model composed of a nearly isentropic convective core and a thin radiative envelope. To represent the tidal responses of rotating planets, we employ series expansions in terms of spherical harmonic functions $Y_l^m$ with different $l$s for a given $m$. For low forcing frequency, there occurs frequency resonance between the forcing and the $g$- and $r$-modes in the envelope and inertial modes in the core. We find that the resonance enhances the tidal torque, and that the resonance with the $g$- and $r$-modes produces broad peaks and that with the inertial modes very sharp peaks, depending on the magnitude of the non-adiabatic effects associated with the oscillation modes. We also find that the behavior of the tidal torque as a function of the forcing frequency (or period) is different between prograde and retrograde forcing, particularly for long forcing periods because the $r$-modes, which have long periods, exist only on the retrograde side.
description: 18 pages, 13 figures
On the D-wave state component of the deuteron in the Nambu-Jona-Lasinio model of light nuclei
Creators: name: Ivanov, A. N.
name: Ivanova, V. A.
name: Oberhummer, H.
name: Troitskaya, N. I.
name: Faber, M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The D-wave state component of the neutron-proton bound state in the deuteron is calculated in the Nambu-Jona-Lasinio model of light nuclei - the relativistically covariant quantum field theoretic approach to the description of low-energy nuclear forces. The theoretical value of the fraction of the D-wave state relative to the S-wave state is equal to eta_d = 0.0238. This agrees well with the phenomenological value eta_d = 0.0256(4) quoted by Kamionkowski and Bahcall (ApJ. 420, 884 (1994)).
description: 7 pages, latex, no figures
Development and evaluation of a catalytic stripper for the measurement of solid ultrafine particle emissions from internal combustion engines
Creators: name: A.D. Melas
name: V. Koidi
name: D. Deloglou
name: E. Daskalos
name: D. Zarvalis
name: E. Papaioannou
name: A.G. Konstandopoulos
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Biotechnology
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: Ecology
subject: FOS: Biological sciences
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Solid particle number vehicle exhaust measurements necessitate an aerosol conditioning system that removes efficiently volatile particles, does not create artifacts and minimizes solid nucleation particle losses. Here, we present the development and evaluation of a catalytic stripper based on a unique dual-function monolithic reactor that oxidizes hydrocarbons and stores sulphur material. The catalytic stripper was tested for its tetracontane particle removal efficiency, sulphur adsorption capacity with sulphur dioxide, and particle penetration with solid CAST-generated particles. The optimal operation conditions were examined including different aerosol flows and configurations, i.e. as a stand-alone device and as part of a volatile removal system with a hot and a cold dilution stage upstream and downstream of the catalytic stripper, respectively. The catalytic stripper managed to comply with current legislation requirements for solid particle number measurements down to 23 nm as a stand-alone device and showed great potential as part of a volatile particle removal (VPR) system for measurements at least down to 10 nm. Finally, we compared the performance of two VPR systems that use the developed catalytic stripper (VPR-CS) and an evaporation tube (VPR-ET), respectively. Our results suggest that the VPR-CS exhibits higher volatile removal efficiency without creating artifacts while the particle losses are lower with the VPR-ET. Nevertheless, when measuring solid nucleation particles generated by a diesel engine with the VPR-CS, the measurement uncertainty was very low due to its high particle penetration fractions.
Radiative and mechanical feedback into the molecular gas in the Large Magellanic Cloud. II. 30 Doradus
Creators: name: Lee, Min-Young
name: Madden, Suzanne
name: Petit, Franck Le
name: Gusdorf, Antoine
name: Lesaffre, Pierre
name: Wu, Ronin
name: Lebouteiller, Vianney
name: Galliano, Frederic
name: Chevance, Melanie
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: With an aim of probing the physical conditions and excitation mechanisms of warm molecular gas in individual star-forming regions, we performed Herschel SPIRE FTS observations of 30 Doradus in the LMC. In our FTS observations, important FIR cooling lines in the ISM, including CO J=4-3 to 13-12, [CI] 370 micron, and [NII] 205 micron, were clearly detected. In combination with ground-based CO data, we then constructed CO spectral line energy distributions (SLEDs) on 10 pc scales over a 60 pc x 60 pc area and found that the shape of the observed CO SLEDs considerably changes across 30 Doradus, e.g., the peak transition varies from J=6-5 to 10-9, while the slope characterized by the high-to-intermediate J ratio ranges from 0.4 to 1.8. To examine the source(s) of these variations in CO transitions, we analyzed the CO observations, along with [CII] 158 micron, [CI] 370 micron, [OI] 145 micron, H2 0-0 S(3), and FIR luminosity data, using state-of-the-art models of PDRs and shocks. Our detailed modeling showed that the observed CO emission likely originates from highly-compressed (thermal pressure ~ 1e7-1e9 K cm-3) clumps on 0.7-2 pc scales, which could be produced by either UV photons (UV radiation field ~ 1e3-1e5 Mathis fields) or low-velocity C-type shocks (pre-shock medium density ~ 1e4-1e6 cm-3 and shock velocity ~ 5-10 km s-1). Considering the stellar content in 30 Doradus, however, we tentatively excluded the stellar origin of CO excitation and concluded that low-velocity shocks driven by kpc scale processes (e.g., interaction between the Milky Way and the Magellanic Clouds) are likely the dominant source of heating for CO. The shocked CO-bright medium was then found to be warm (temperature ~ 100-500 K) and surrounded by a UV-regulated low pressure component (a few (1e4-1e5) K cm-3) that is bright in [CII] 158 micron, [CI] 370 micron, [OI] 145 micron, and FIR dust continuum emission.
description: Accepted for publication in A&A