cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Double-Layer Orthogonal-Offset Platforms in fluid and insolation environments
Creators: name: Edgar, Ross
Publisher: name: The Australian National University
Year: 2018
Subjects: Solar energy
Photovoltaic
Solar tracking
DLOOP
PV tracking
Renewable energy
Tracking efficiency

description: The DLOOP is a structure of non-overlapping tiles (typically corner connected) occupying two layers. Interest in the DLOOP arises from Photo-Voltaic (PV) tracking applications. The tiles (PV modules) of contemporary tracking systems are within one contiguous layer, i.e. a side-by-side platform (SSP). Trees collect solar energy using branching structures to support leaves which are, similar to PV modules, planar surfaces of solar energy transformation. The tree's form is naturally excellent for lowering structural stress in limbs and thermal stress in leaves. For analogous reasons, related to the creation of flow paths that would otherwise be blocked, this research hypothesised (and has subsequently shown) that: * the fluid (wind) dynamic force on tiles of high inclination SSP may be reduced (up to 30%) adopting DLOOP arrangements; and * the temperature of heated tiles in SSP may be reduced (up to 5K within nominal and hot terrestrial environments), by passive convective cooling, adopting DLOOP arrangements. Fluid (wind) dynamic force is significant in PV applications because it typically exceeds the force of gravity on the tiles of SSP in 13m/s winds and increases with velocity squared. Hence reducing wind force by 30% should allow 40% more tiles to be fitted to contemporary tracking mechanisms. Temperature is significant in PV applications because the performance of PV tiles typically falls 0.4%/K. Hence a 5K reduction in temperature should improve efficiency 2%. A combination of wind-tunnel tests, Particle Image Velocimetry and Computational Fluid Dynamic (CFD) simulations using Reynolds Averaged Navier Stokes and Large Eddy Simulation turbulence models was used for the fluid dynamic research. A combined Finite Element/CFD simulation of PV panels in platforms was developed to model temperature outcomes of thermal diffusion in solid materials and thermal diffusion, radiation and convection in the fluid (air). If PV-tracking ranges are limited below those of the solar-vector, shading of the DLOOP lower by the upper layer occurs. This DLOOP self-shading raises unique cost-benefits associated with tracking ranges. Consequently, this research develops a means to quantify the insolation received by platforms accounting for technology and tracking range in diverse (Australian) climates. Additionally, multiple tracking platforms may be placed in close proximity and suffer "Parasitic" energy losses when shaded by self-similar neighbours. Therefore, this research study introduces a natural no-shade scale to describe and optimise field layouts according to local insolation and economic conditions.
Antepipona rubicunda GUSENLEITNER 2001
Creators: name: Usenleitner
name: Gusenleitner, J.
name: Madl, M.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eumenidae
Antepipona
Antepipona rubicunda

description: Antepipona rubicunda GUSENLEITNER 2001
 Antepipona rubicunda nov.spec.: GUSENLEITNER 2001: 250 (descr. ♀, South Africa), 255 (fig. 4). D i s t r i b u t i o n:SouthAfrica.
description: Published as part of Usenleitner, Gusenleitner, J. & Madl, M., 2009, A Catalogue of the Eumeninae (Hymenoptera: Vespidae) of the Ethiopian Region excluding Malagasy Subregion. Part I: Introduction, Key to Genera, Genera Aethiopicodynerus GUSENLEITNER 1997 to Cyrtolabulus van der VECHT 1969, pp. 513-638 in Linzer biologische Beiträge 41 (1) on page 574, DOI: 10.5281/zenodo.5276247
Confronting Neutron Star Cooling Theories with New Observations
Creators: name: Tsuruta, S.
name: Teter, M. A.
name: Takatsuka, T.
name: Tatsumi, T.
name: Tamagaki, R.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: With the successful launch of Chandra and XMM/Newton X-ray space missions combined with the lower-energy band observations, we are in the position where careful comparison of neutron star cooling theories with observations will make it possible to distinguish among various competing theories. For instance, the latest theoretical and observational developments already exclude both nucleon and kaon direct URCA cooling. In this way we can now have realistic hope for determining various important properties, such as the composition, degree of superfluidity, the equation of state and steller radius. These developments should help us obtain better insight into the properties of dense matter.
description: 11 pages, 1 figure
Pagurina Lemaitre & Felder & Poupin 2017, n. gen.
Creators: name: Lemaitre, Rafael
name: Felder, Darryl L.
name: Poupin, Joseph
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Paguridae
Pagurina

description: Genus Pagurina n. gen.
 TYPE SPECIES. — Pagurina bifida n. gen., n. sp., by monotypy.
 ETYMOLOGY. — The generic name is derived from the genus name Pagurus, and using the Latin feminine suffix - ina, which denotes something diminutive, in reference to the minute size of specimens in the single species of this new genus.
DISTRIBUTION. — Known only from the type species collected in Guadeloupe, Lesser Antilles, Caribbean Sea, at a depth of 10 m.
DIAGNOSIS. — Nine pairs of biserial phyllobranch gills, no pleurobranchs on somite XII (thoracomere 7, above pereopod 4). Rostrum subtriangular. Ischium with weak crista dentata, lacking accessory tooth. Chelipeds subequal. Sternite of somite XI (thoracomere 6, pereopod 3) with anterior lobe rectangular. Pereopod 4 with single row of scales on propodal rasp, dactyl lacking preungual process. Pereopod 5 semi-chelate. Male with paired gonopores, and unpaired left sexual tube on coxa of pereopods 5; with unpaired, left pleopods 3-5. Female conditions unknown. Telson nearly symmetrical, with lateral indentations; terminal margins oblique.
REMARKS
 Although superficially Pagurina n. gen. might give the appearance that it could be placed in the catch-all genus Pagurus Fabricius, 1775, a number of characters clearly indicate that it must be considered a separate genus. The three main characters that place this taxon outside of Pagurus, or any other known genus of Paguridae, are the number of gills (nine in Pagurina n. gen. vs 11 in most Pagurus), the absence of an accessory tooth (present in Pagurus) on the crista dentata, and presence of a short sexual tube (lacking in majority of Pagurus).
description: Published as part of Lemaitre, Rafael, Felder, Darryl L. & Poupin, Joseph, 2017, Discovery of a new micro-pagurid fauna (Crustacea: Decapoda: Paguridae) in the Lesser Antilles, Caribbean Sea, pp. 151-195 in Zoosystema 39 (2) on page 170, DOI: 10.5252/z2017n2a1, http://zenodo.org/record/5391902
Photoelectric effect on dust grains across the L1721 cloud in the rho Ophiuchi molecular complex
Creators: name: Habart, E.
name: Verstraete, L.
name: Boulanger, F.
name: Forets, G. Pineau des
name: Peintre, F. Le
name: Bernard, J. P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present ISO-LWS measurements of the main gas cooling lines, C+ 158 mum and O 63 mum towards a moderate opacity molecular cloud (Av=3), L1721, illuminated by the B2 star nu Sco (X = 5-10). These data are combined with an extinction map and IRAS dust emission images to test our understanding of gas heating and cooling in photo-dissociation regions (PDRs). This nearby PDR is spatially resolved in the IRAS images; variations in the IRAS colors across the cloud indicate an enhanced abundance of small dust grains within the PDR. A spatial correlation between the gas cooling lines and the infrared emission from small dust grains illustrates the dominant role of small dust grains in the gas heating through the photoelectric effect. The photoelectric efficiency, determined from the observations by ratioing the power radiated by gas and small dust grains, is in the range 2 to 3% in close agreement with recent theoretical estimates. The brightness profiles across the PDR in the C+ 158 mum and O 63 mum lines are compared with model calculations where the density profile is constrained by the extinction data and where the gas chemical and thermal balances are solved at each position. We show that abundance variations of small dust grains across the PDR must be considered to account for the LWS observations.
description: 10 pages, 15 figures
A Light Curve Analysis of 32 Recent Galactic Novae --- Distances and White Dwarf Masses
Creators: name: Hachisu, Izumi
name: Kato, Mariko
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We obtained the absolute magnitudes, distances, and white dwarf (WD) masses of 32 recent galactic novae based on the time-stretching method for nova light curves. A large part of the light/color curves of two classical novae often overlap each other if we properly squeeze/stretch their timescales. Then, a target nova brightness is related to the other template nova brightness by $(M_V[t])_{\rm template} = (M_V[t/f_{\rm s}] - 2.5 \log f_{\rm s})_{\rm target}$, where $t$ is the time, $M_V[t]$ is the absolute $V$ magnitude, and $f_{\rm s}$ is their timescaling ratio. Moreover, when these two time-stretched light curves, $(t/f_{\rm s})$-$(M_V-2.5 \log f_{\rm s})$, overlap each other, $(t/f_{\rm s})$-$(B-V)_0$ do too, where $(B-V)_0$ is the intrinsic $B-V$ color. Thus, the two nova tracks overlap each other in the $(B-V)_0$-$(M_V-2.5 \log f_{\rm s})$ diagram. Inversely using these properties, we obtain/confirm the distance and reddening by comparing each nova light/color curves with the well calibrated template novae. We classify the 32 novae into two types, LV Vul and V1500 Cyg types, in the time-stretched $(B-V)_0$-$(M_V-2.5 \log f_{\rm s})$ color-magnitude diagram. The WD mass is obtained by direct comparison of the model $V$ light curves with the observation. Thus, we obtain a uniform set of 32 galactic classical novae that provides the distances and WD masses from a single method. Many novae broadly follow the universal decline law and the present method can be applied to them, while some novae largely deviate from the universal decline law and so the method cannot be directly applied to them. We discuss such examples.
description: 175 pages including 126 figures, to appear in ApJS
Design of Quantum Repeaters
Creators: name: Li, Yi
Publisher: name: The Australian National University
Year: 2017
Subjects: quantum communication
quantum information
quantum repeater
quantum key distribution
quantum amplification
channel equalisation

description: Quantum communication holds the promise of achieving long-distance secure message transmission by exploiting quantum entanglement between remote locations. Quantum repeaters are indispensable to the realization of quantum networks for long-distance quantum communication. Similar to its classical analogue, a good quantum repeater should be able to compensate channel attenuation with a quantum ampliﬁer, and to combat channel distortion through a quantum equaliser. This quantum repeater should also operate by an eﬃcient and robust protocol. The ﬁrst part of this project researches the continuous mode operation of a noiseless linear ampliﬁer (NLA). We develop a dynamical model to describe the operation of the nondeterministic NLA in the regime of continuous-mode inputs. Both the quantum scissor based NLA and the photon addition-subtraction based NLA are analysed. Simulation results are also presented to conﬁrm theoretical analysis. The second part proposes two quantum protocols. An atomic ensemble based quantum protocol is developed to generate distributed W-states. These generated distributed W-states could be considered as an entanglement resource between more than two distant nodes and would be useful in quantum communication and distributed quantum computation in the future. We also propose a protocol by which quantum key distribution can be achieved deterministically between multiple nodes.This deterministic quantum key distribution scheme may be used to guarantee secure communication for wireless sensor networks and Internet of Things. The last project analyses distortion of quantum channels and develops physically realisable modules to combat it. The minimum phase channel and non-minimum phase all pass channel are discussed separately.
The X-ray jet and halo of PKS 0521-365
Creators: name: Birkinshaw, M.
name: Worrall, D. M.
name: Hardcastle, M. J.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Chandra ACIS observations of PKS 0521-365 find that the X-ray emission of this BL Lac object consists of emission from an unresolved core, a diffuse halo, and a 2 arcsec jet feature coincident with the inner radio/optical jet. A comparison with a new ATCA 8.6-GHz map also finds X-ray emission from the bright hotspot south-east of the nucleus. The jet spectrum, from radio to X-ray, is probably synchrotron emission from an electron population with a broken power-law energy distribution, and resembles the spectra seen from the jets of low-power (FR I) radio galaxies. The hotspot X-ray flux is consistent with the expectations of synchrotron self-Compton emission from a plasma close to equipartition, as seen in studies of high-power (FR II) radio galaxies. While the angular structure of the halo is similar to that found by an analysis of the ROSAT HRI image, its brightness is seen to be lower with Chandra, and the halo is best interpreted as thermal emission from an atmosphere of similar luminosity to the halos around FR I radio galaxies. The X-ray properties of PKS 0521-365 are consistent with it being a foreshortened, beamed, radio galaxy.
description: 9 pages, 12 figures, accepted for publication in MNRAS
Resonance Category
Creators: name: Kozlov, Dmitry N.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Category Theory (math.CT)
subject: Combinatorics (math.CO)
subject: General Topology (math.GN)
subject: FOS: Mathematics
subject: 32S20; 18B30 32S60 58K15

description: The main purpose of this paper is to introduce a new category, which we call a resonance category, whose combinatorics reflect that of canonical stratifications of $n$-fold symmetric smash products. The study of the stratifications can then be abstracted to the study of functors satisfying certain sets of axioms, which we name resonance functors. One frequently studied stratification is that of the set of all polynomials of degree $n$, defined by fixing the allowed multiplicities of roots. We apply our abstract combinatorial framework, in particular, the notion of direct product of relative resonances, to study the Arnold problem of computing the algebro-topological invariants of these strata.
description: 22 pages, 1 figure. This is the final journal version. The paper appears in Commentarii Mathematici Helvetici
Antepipona scutellaris subsp. scutellaris GIORDANI SOIKA 1985
Creators: name: Usenleitner
name: Gusenleitner, J.
name: Madl, M.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eumenidae
Antepipona
Antepipona scutellaris
Antepipona scutellaris scutellaris giordani soika 1985

description: Antepipona scutellaris scutellaris GIORDANI SOIKA 1985
 Antepipona scutellaris GIORDANI SOIKA: GESS 1981: 16 (biol., South Africa).
 Antepipona scutellaris n.sp.: GIORDANI SOIKA 1985: 34 (key), 53 (descr. Ƌ ♀, South Africa).
 Antepipona scutellaris GIORDANI SOIKA: GESS & GESS 1991: 249 (biol., South Africa), 250 (fig. 2), 251 (fig. 3), 252 (fig. 4).
 Antepipona scutellaris GIORDANI SOIKA: BORSATO & ROSSI 1999: 94 (cat.).
 Antepipona scutellaris GIORDANI SOIKA: GESS & GESS 2003: 76 (biol., South Africa), 487 (biol., South Africa), 511 (biol., South Africa).
D i s t r i b u t i o n:SouthAfrica.
description: Published as part of Usenleitner, Gusenleitner, J. & Madl, M., 2009, A Catalogue of the Eumeninae (Hymenoptera: Vespidae) of the Ethiopian Region excluding Malagasy Subregion. Part I: Introduction, Key to Genera, Genera Aethiopicodynerus GUSENLEITNER 1997 to Cyrtolabulus van der VECHT 1969, pp. 513-638 in Linzer biologische Beiträge 41 (1) on page 574, DOI: 10.5281/zenodo.5276247
Additional file 1 of Autism symptoms in anorexia nervosa: a comparative study with females with autism spectrum disorder
Creators: name: Kerr-Gaffney, Jess
name: Hayward, Hannah
name: Jones, Emily J. H.
name: Halls, Daniel
name: Murphy, Declan
name: Tchanturia, Kate
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Science Policy
Mental Health

description: Additional file 1. Participant recruitment information.
All Optical Neural Network with Nonlinear Activation Functions
Creators: name: Zuo, Ying
name: Li, Bohan
name: Zhao, Yujun
name: Jiang, Yue
name: Chen, You-Chiuan
name: Chen, Peng
name: Jo, Gyu-Boong
name: Liu, Junwei
name: Du, Shengwang
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optics (physics.optics)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: Artificial neural networks (ANNs) have now been widely used for industry applications and also played more important roles in fundamental researches. Although most ANN hardware systems are electronically based, optical implementation is particularly attractive because of its intrinsic parallelism and low energy consumption. Here, we propose and demonstrate fully-functioned all optical neural networks (AONNs), in which linear operations are programmed by spatial light modulators and Fourier lenses, and optical nonlinear activation functions are realized with electromagnetically induced transparency in laser-cooled atoms. Moreover, all the errors from different optical neurons here are independent, thus the AONN could scale up to a larger system size with final error still maintaining in a similar level of a single neuron. We confirm its capability and feasibility in machine learning by successfully classifying the order and disorder phases of a typical statistic Ising model. The demonstrated AONN scheme can be used to construct various ANNs of different architectures with the intrinsic parallel computation at the speed of light.
description: 6 pages, 4 figures
Additional file 2: of Estimated dengue force of infection and burden of primary infections among Indian children
Creators: name: Bhavsar, Amit
name: Tam, Clarence
name: Suneela Garg
name: Guru Jammy
name: Anne-Frieda Taurel
name: Sher-Ney Chong
name: Nealon, Joshua
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: 60506 Virology
subject: Computational Biology

description: Table S2. Estimates of the number of children experiencing primary dengue infections in 2011, in India overall. (DOCX 18 kb)
A spectrophotometric atlas of Narrow-Line Seyfert 1 galaxies
Creators: name: Veron-Cetty, M. -P.
name: Veron, P.
name: Goncalves, A. C.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have compiled a list of 83 objects classified as Narrow-Line Seyfert 1 galaxies (NLS1s) or known to have a broad Balmer component narrower than 2000 km/s. Out of these, 19 turned out to have been spectroscopically misidentified in previous studies; only 64 of the selected objects are genuine NLS1s. We have spectroscopically observed 59 of them and tried to characterize their Narrow and Broad-Line Regions (NLR and BLR) by fitting the emission-lines with Gaussian and/or Lorentzian profiles. In most cases, the broad Balmer components are well fitted by a single Lorentzian profile. This has consequences concerning their FWHMs and line ratios: when the broad Balmer components are fitted with a Lorentzian, most narrow line regions have line ratios typical of Seyfert 2s while, when a Gaussian profile isused for fitting the broad Balmer components, the line ratios are widely scattered in the usual diagnostic diagrams (Veilleux & Osterbrock 1987). We find that, in general, the [O III] lines have a relatively narrow Gaussian profile (~ 200-500 km/s FWHM) with often, in addition, a second broad (~ 500-1800 km/s FWHM), blueshifted Gaussian component. We do not confirm that the [O III] lines are weak in NLS1s. As previously suggested, there is a continuous transition of all properties between NLS1s and classical Broad-Line Seyfert 1 Galaxies (BLS1s) and the limit of 2000 km/s used to separate the two species is arbitrary; R_4570, the ratio of the Fe II to the H_beta fluxes, could be a physically more meaningful parameter to distinguish them. (abridged abstract)
description: LaTeX file, 24 pages, 15 figures, uses the new A&A macro (enclosed: aa5.cls). Figs. 1-5 and 7 are bitmapped; non-bitmapped, high quality figures are included in the .ps and .pdf versions of the paper, available at http://www.obs-hp.fr/www/preprints.html. Accepted for publication in Astronomy & Astrophysics
A cultural political economy of South Korea's development model in variegated capitalism
Creators: name: Park, Jihoon
Publisher: name: Lancaster University
Year: 2018

description: This thesis investigates the Park Chung Hee model (PCHM). This term refers to a South Korean variant of the East Asian model of capitalism—particularly, the historical model that guided the rapid and sustained growth of the economy since the mid-1960s. This historical investigation is theoretically informed by a cultural political economy of variegated capitalism (VarCap-CPE) that enables a differential and integral exploration of both historical and contemporary capitalism. In this context, my contribution is twofold. The first is theoretical. While a theoretically informed historical investigation into East Asian capitalism requires an approach to (post-)colonialism, imperialism and hegemony as a prerequisite, VarCap-CPE has still not fully integrated such an approach into its analytical framework. So, my first aim is to improve this paradigm by drawing on Marx’s insights into colonialism, the world market, and international hegemony and propose how they might be put in their place, provisionally, in a VarCap-CPE analysis. My second goal is empirical. Based on the enhanced version of the VarCap-CPE, I aim to give a better account of the PCHM than previous literature in political economy. Specifically, I show how the model was informed by two contradictory state strategies: (1) the fascist and autarkic state strategies of Imperial Japan; and (2) the liberal and free trade-oriented developmentalism, based on W.W. Rostow’s modernization theory. I thereby demonstrate that the PCHM was self-contradictory and, in this context, present it as a “chimerical” model that combines in a contradictory manner the DNA of two rival species. On this basis, I provide an integral account of its seemingly miraculous performance as well as the dilemmas, contradictions and crisis-proneness that beset it. In addition, unlike much of the extant literature on the Park model, my analysis permits theoretically consistent further research into its crisis and subsequent neoliberalisation.
Chandra observation of Abell 1689: New determination of mass distribution and comparison to lensing measurements
Creators: name: Xue, Sui-Jian
name: Wu, Xiang-Ping
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a new estimate of the projected X-ray mass of Abell 1689 observed with Chandra, in an attempt to clarify the issue of whether or not there exists a discrepancy between X-ray and gravitational lensing mass estimates claimed in previous investigations based on {\it Einstein}, {\it ROSAT} and {\it ASCA} observations. A particular attention is paid to examining if there is an offset between X-ray centroid and central dominant cD galaxy, which may be an indicator of the presence of local dynamical activities of intracluster gas in the central core and therefore, explain the discrepancy between X-ray and lensing mass estimates, if any. The unprecedentedly high spatial resolution achieved by Chandra allows us to precisely localize the X-ray centroid of Abell 1689, which appears to coincide perfectly with the central cD galaxy. This fact, along with the symmetry and regularity of the X-ray surface brightness and temperature distributions, suggests that Abell 1689 is a fully-relaxed cluster. We thus employ hydrostatic equilibrium hypothesis to determine the projected mass profile of Abell 1689, and compare it with the results obtained by different lensing techniques available in the literature. Our analysis confirms the existance of the discrepancy of a factor of $\sim2$ between X-ray and lensing mass estimates in the central region of $r\approx0.2$ Mpc, although the two methods yield essentially consistent result on large radii. If the perfect coincidence between the X-ray center and the cD galaxy of Abell 1689 detected by Chandra observation is not a projection effect, the central mass discrepancy between X-ray and lensing measurements may pose a challenge to our conventional understanding of dynamical evolution of the intracluster gas in the central regions of clusters.
description: 26 pages, 7 figures, Accepted for publication in the Astrophysical Journal
Antepipona solstitialis subsp. frogna GIORDANI SOIKA 1985
Creators: name: Usenleitner
name: Gusenleitner, J.
name: Madl, M.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eumenidae
Antepipona
Antepipona solstitialis
Antepipona solstitialis frogna giordani soika 1985

description: Antepipona solstitialis frogna GIORDANI SOIKA 1985
 Antepipona solstitialis frogna n.ssp.: GIORDANI SOIKA 1985: 43 (key), 124 (descr. Ƌ ♀, Lesotho, South Africa).
 Antepipona solstitialis frogna GIORDANI SOIKA: BORSATO & RATTI 1999: 95 (cat.).
D i s t r i b u t i o n: Lesotho, South Africa.
description: Published as part of Usenleitner, Gusenleitner, J. & Madl, M., 2009, A Catalogue of the Eumeninae (Hymenoptera: Vespidae) of the Ethiopian Region excluding Malagasy Subregion. Part I: Introduction, Key to Genera, Genera Aethiopicodynerus GUSENLEITNER 1997 to Cyrtolabulus van der VECHT 1969, pp. 513-638 in Linzer biologische Beiträge 41 (1) on page 576, DOI: 10.5281/zenodo.5276247
Paguruncio Lemaitre & Felder & Poupin 2017, n. gen.
Creators: name: Lemaitre, Rafael
name: Felder, Darryl L.
name: Poupin, Joseph
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Paguridae
Paguruncio

description: Genus Paguruncio n. gen.
 TYPE SPECIES. — Paguruncio parvulus n. gen., n. sp., by present designation. Gender: masculine.
 ETYMOLOGY. — The generic name is derived from the genus name Pagurus, and using the masculine Latin suffix - uncio which denotes something diminutive, in reference to the minute size of specimens in the single species of this new genus.
DIAGNOSIS. — Eight pairs of biserial phyllobranch gills, no gill on third maxilliped and cheliped, no pleurobranchs on somites X, XI (thoracomeres 5, 6, above pereopods 2 and 3). Rostrum broadly triangular. Ocular acicles terminating in simple spine. Ischium with accessory tooth.Chelipeds subequal in length, right not much stronger than left. Sternite of somite XI (thoracomere 6, pereopod 3) with subrectangular anterior lobe. Pereopod 4 with single row of scales on propodal rasp, dactyl lacking preungual process. Pereopod 5 semi-chelate. Male with paired, subequal, slender, membranous sexual tubes directed posteriorly, on coxae of pereopods 5; pleopod condition unknown. Female with paired gonopores; plepood condition incompletely known except for presence of unpaired left pleopod 5. Telson nearly symmetrical, with lateral indentations; terminal margins oblique, armed with spines.
DISTRIBUTION. — Known based on the type species found in Curaçao, at a depth of 224 m
REMARKS
 There is no clear morphological relationship or similarity between the single species of Paguruncio n. gen. and the other species described in this report that also have male sexual tubes. Paguruncio, n. gen. and Paguriscus n. gen. both have paired, subequal sexual tubes, although the tubes are morphologically different (Figs 16G; 18E). Both new genera have eight pairs of biserial gills; however, the gill formula is quite different in the two (see respective Diagnoses).
description: Published as part of Lemaitre, Rafael, Felder, Darryl L. & Poupin, Joseph, 2017, Discovery of a new micro-pagurid fauna (Crustacea: Decapoda: Paguridae) in the Lesser Antilles, Caribbean Sea, pp. 151-195 in Zoosystema 39 (2) on pages 178-179, DOI: 10.5252/z2017n2a1, http://zenodo.org/record/5391902
Additional file 1: of Impact of the warm summer 2015 on emergency hospital admissions in Switzerland
Creators: name: Ragettli, Martina
name: Vicedo-Cabrera, Ana
name: Flückiger, Benjamin
name: Röösli, Martin
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases

description: Additional tables and figures. Figure S1. Map of Switzerland showing the seven study regions and corresponding measurement station of temperature of the Swiss Monitoring Network. Figure S2. Daily number of emergency hospital admissions (EHA) (7 day moving average) in Switzerland by age group (0–14 years, 15–64 years, 65–74 years, ≥75 years) during the warm season between 2005 and 2015. External causes of morbidity are excluded except effects of heat and light (ICD10-code T67). Figure S3. Daily number of emergency hospital admissions (EHA) (7 day moving average) for selected diagnoses in Switzerland from 2005 to 2015. The reference years (2012–2015) for the 2015 excess morbidity are shown as bold grey lines. Vertical bars represent the heatwaves in 2015. (DOCX 5663 kb)
A Brown Dwarf Companion for the Accreting Millisecond Pulsar SAX J1808.4-3658
Creators: name: Bildsten, Lars
name: Chakrabarty, Deepto
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: BeppoSAX has revealed a population of faint neutron star X-ray transients in the Galactic bulge. King conjectured that these neutron stars are accreting from brown dwarfs (BD) with a time-averaged mass transfer rate \approx 10^{-11} M_sun/year. We show that the orbital parameters of the 401 Hz accreting millisecond pulsar SAX J1808.4-3658 support this hypothesis. A main-sequence mass donor requires a nearly face-on inclination and a higher than observed. However, the range of allowed inclinations is substantially relaxed and the predicted mass transfer rate is consistent with that observed if a hot 0.05 M_sun BD is the donor. We then explain the BD radius required (0.13 R_\sun) to fill the Roche lobe. All transiently accreting neutron stars have a minimum luminosity in quiescence set by the time-averaged mass transfer rate onto the neutron star. We show that the constant heating of the BD by this emission can maintain the higher entropy implied by a 0.13 R_\sun radius. Our work bolsters the case that SAX J1808.4-3658 is a progenitor to compact ms radio pulsar binaries (e.g. like those found in 47 Tuc). The very low 's implies that the progenitors to these radio pulsars are long-lived (Gyrs) transient systems, rather than short-lived (Myrs) Eddington-limited accretors. Hence, the accreting progenitor population to millisecond radio pulsars in 47 Tuc could still be present and found in quiescence with Chandra.(abridged)
description: To appear in Astrophysical Journal
Hot Outflowing Gas from the X-ray Binary Hercules X-1
Creators: name: Boroson, Bram
name: Kallman, Tim
name: Vrtilek, Saeqa Dil
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a unified picture of outflowing gas from the X-ray binary system Hercules X-1/HZ Herculis. We suggest that the outflowing gas (a wind) causes UV emission seen in mid-eclipse, narrow UV absorption lines, and broad UV P Cygni lines. Observations with the FOS and STIS spectrographs on the Hubble Space Telescope (HST) show UV emission lines in the middle of X-ray eclipse, when the X-ray heated atmosphere of the normal star and accretion disk should be entirely hidden from view. Narrow absorption lines (FWHM~50 km/s) blueshifted by 500 km/s during observations in 1998 and by 400 km/s during observations in 1999 were seen from phi=0.0-0.3. The line velocity was constant to within 20 km/s. The P Cygni profiles from Hercules~X-1 have optical depths tau<1 with a maximum expansion velocity of 600 km/s, and are seen in the resonance lines N V 1238.8,1242.8, Si IV 1393.7,1402.8, and C IV 1548.2, 1550.8. We discuss whether this wind originates in the accretion disk or on the companion star, and how the relevant ions can survive X-ray ionization by the neutron star.
description: Accepted for publication in The Astrophysical Journal, v562, December 2001
Antepipona splendida GUSENLEITNER 2005
Creators: name: Usenleitner
name: Gusenleitner, J.
name: Madl, M.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eumenidae
Antepipona
Antepipona splendida

description: Antepipona splendida GUSENLEITNER 2005
 Antepipona splendida nova spec.: GUSENLEITNER 2005b: 1189 (descr. ♀, Tanzania), 1197 (figs 12, 13).
D i s t r i b u t i o n: Tanzania.
description: Published as part of Usenleitner, Gusenleitner, J. & Madl, M., 2009, A Catalogue of the Eumeninae (Hymenoptera: Vespidae) of the Ethiopian Region excluding Malagasy Subregion. Part I: Introduction, Key to Genera, Genera Aethiopicodynerus GUSENLEITNER 1997 to Cyrtolabulus van der VECHT 1969, pp. 513-638 in Linzer biologische Beiträge 41 (1) on page 576, DOI: 10.5281/zenodo.5276247
Pusillopagurus Lemaitre & Felder & Poupin 2017, n. gen.
Creators: name: Lemaitre, Rafael
name: Felder, Darryl L.
name: Poupin, Joseph
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Paguridae
Pusillopagurus

description: Genus Pusillopagurus n. gen.
 TYPE SPECIES. — Pusillopagurus polulus n. gen., n. sp., by present designation. Gender: masculine.
 ETYMOLOGY. — The generic name is a combination of the genus name Pagurus with the Latin pusillus, which refers to something very small, and used in reference to the minuscule size of specimens in the single species of this new genus.
DISTRIBUTION. — Known based on the type species found in Curaçao, at a depth of 15.2-115.8 m.
DIAGNOSIS. — Eight pairs of biserial phyllobranch gills, only 1 pleurobranch on somite XII (thoracomere 7, above pereopod 4). Rostrum triangular. Ischium edge of crista dentata projected medially, lacking accessory tooth. Chelipeds subequal in length, somewhat slender. Sternite of somite XI (thoracomere 6, pereopod 3) with anterior lobe subrectangular, bilobed. Pereopod 4 with single row of scales on propodal rasp, dactyl lacking preungual process. Pereopod 5 semi-chelate. Male with coxae of pereopods 5 symmetrical, with paired, unequal sexual tubes, right tube much longer than left, distally coiled and filamentous, left tube not coiled or filamentous; with unpaired, left pleopods 3-5. Female with paired gonopores, and unpaired, left pleopods 2-5. Telson nearly symmetrical, longer than broad, with lateral indentations dividing anterior and posterior lobes; terminal margins of posterior lobes weakly oblique, armed with distinct spines.
REMARKS
 There are no clear morphological similarities between this new genus and other known pagurid genera in which the male has sexual tubes, despite some having similar sexual tubes. As in Pusillopagurus n. gen. and at least 18 other pagurid genera in which the male has paired sexual tubes, the right is longer than the left. In general morphology, the tubes of Pusillopagurus n. gen. are most similar to those of Trichopagurus de Saint Laurent, 1968 (described in more detail in de Saint Laurent [1970b]), and to a lesser extent those of Alainopaguroides McLaughlin, 1997 and Icelopagurus McLaughlin, 1997. However, in most other important morphological features, such as the cephalic shield and appendages, third maxilliped crista dentata, chelipeds, ambulatory legs, and telson, Pusillopagurus n. gen. differs markedly from these three genera. Furthermore, the number of gills in this new genus is eight, whereas it is 11 in those other three.
description: Published as part of Lemaitre, Rafael, Felder, Darryl L. & Poupin, Joseph, 2017, Discovery of a new micro-pagurid fauna (Crustacea: Decapoda: Paguridae) in the Lesser Antilles, Caribbean Sea, pp. 151-195 in Zoosystema 39 (2) on page 187, DOI: 10.5252/z2017n2a1, http://zenodo.org/record/5391902
Formation of the binary pulsars J1141-6545 and B2023+46
Creators: name: Davies, Melvyn B.
name: Ritter, Hans
name: King, Andrew
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The binaries PSR J1141-6545 and PSR B2303+46 each appear to contain a white dwarf which formed before the neutron star. We describe an evolutionary pathway to produce these two systems. In this scenario, the primary transfers its envelope onto the secondary which is then the more massive of the two stars, and indeed sufficiently massive later to produce a neutron star via a supernova. The core of the primary produces a massive white dwarf which enters into a common envelope with the core of the secondary when the latter evolves off the main sequence. During the common envelope phase, the white dwarf and the core of the secondary spiral together as the envelope is ejected. The evolutionary history of PSR J1141-6545 and PSR B2303+46 differ after this phase. In the case of PSR J1141--6545, the secondary (now a helium star) evolves into contact transferring its envelope onto the white dwarf. We propose that the vast majority of this material is in fact ejected from the system. The remains of the secondary then explode as a supernova producing a neutron star. Generally the white dwarf and neutron star will remain bound in tight, often eccentric, systems resembling PSR J1141-6545. These systems will spiral in and merge on a relatively short timescale and may make a significant contribution to the population of gamma ray burst progenitors. In PSR B2303+46, the helium-star secondary and white dwarf never come into contact. Rather the helium star loses its envelope via a wind, which increases the binary separation slightly. Only a small fraction of such systems will remain bound when the neutron star is formed (as the systems are wider). Those systems which are broken up will produce a population of high-velocity white dwarfs and neutron stars.
description: 9 pages, 10 figures; MNRAS in press
Martu Paint Country. The archaeology of colour and aesthetics in Western Desert rock art and contemporary acrylic art
Creators: name: Higgs, Samantha Lee
Publisher: name: The Australian National University
Year: 2016
Subjects: Martu
Western Desert
colour
color
archaeology
rock art
acrylic
archeology
anthropology
aesthetics

description: This thesis documents an archaeological study of the use of colour in the Australian Western Desert, which set out to test the thesis that there is a discernible, uniquely Martu aesthetic in relation to colour. It did this by looking at colour preferences in two Martu art types; the rock art which was created prior to European contact and the acrylic art which has come about by a degree of fusion with Australian European culture. Acrylic colour has been described as only colour; distinct from traditional mediums (such as ochres) which encode context from their source within their material. So when this embedded contextual meaning is stripped away what do the Martu do with pure colour? Or does this description ignore the role that colour plays in art, and in life? Colour is a ubiquitous part of life and material culture; all humans use the same physical mechanisms to see colour but we do not necessarily all perceive it in the same way. Colour is both a static aspect of material culture and a part of an individual’s cultural perceptual landscape; in this sense colour operates as part of our cultural aesthetic not wholly anchored to the immediate material context. Western Desert acrylic art has been considered by many as a product of the Western European art world rather than a new expression of traditional culture. This research in contrast has found that in the Martu acrylic art colour is used to express Country and to obfuscate information in the same way as dotting. In this way the acrylic palette shares meaning with the more traditional palettes and is being used in new ways to deal with a new way of life. My research has shown that colour works as a mnemonic in the same way an icon or a painting (as a complete object) does by recalling natural features through their visual coloured expression. The results show that colour is an important element of the art that contributes to the meaning and function of the art in the same way that form does. Colour has a representative and contextual cultural value in both the rock art and acrylic art and is more than ‘just colour’ regardless of its source: ochre mined direct from Country or acrylic purchased from a shop. While art practice has developed and changed through practice with the new medium this practice is rooted within traditional Martu cultural context and aesthetic.
A panorama on zeta functions
Creators: name: Deitmar, Anton
Publisher: name: arXiv
Year: 2002
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics

description: In this essay I will give a strictly subjective selection of different types of zeta functions. Instead of providing a complete list, I will rather try to give the central concepts and ideas underlying the theory. This article is going to appear in the collected works of Erich Kähler.
description: LaTex, 15 pages
Infinitesimal Operations on Complexes of Graphs
Creators: name: Conant, Jim
name: Vogtmann, Karen
Publisher: name: arXiv
Year: 2001
Subjects: subject: Quantum Algebra (math.QA)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 17B62, 17B63, 17B70, 20F28, 57M07, 57M15, 57M27

description: In two seminal papers Kontsevich used a construction called_graph homology_ as a bridge between certain infinite dimensional Lie algebras and various topological objects, including moduli spaces of curves, the group of outer automorphisms of a free group, and invariants of odd dimensional manifolds. In this paper, we show that Kontsevich's graph complexes, which include graph complexes studied earlier by Culler and Vogtmann and by Penner, have a rich algebraic structure. We define a Lie bracket and cobracket on graph complexes, and in fact show that they are Batalin-Vilkovisky algebras, and therefore Gerstenhaber algebras. We also find natural subcomplexes on which the bracket and cobracket are compatible as a Lie bialgebra. Kontsevich's graph complex construction was generalized to the context of operads by Ginzburg and Kapranov, with later generalizations by Getzler-Kapranov and Markl. In [CoV], we show that Kontsevich's results in fact extend to general cyclic operads. For some operads, including the examples associated to moduli space and outer automorphism groups of free groups, the subcomplex on which we have a Lie bi-algebra structure is quasi-isomorphic to the entire connected graph complex. In the present paper we show that all of the new algebraic operations canonically vanish when the homology functor is applied, and we expect that the resulting constraints will be useful in studying the homology of the mapping class group, finite type manifold invariants and the homology of Out(F_n).
description: In this final revision, we settle one of the conjectures from the original paper. We also eliminate the discussion of "symmetric Jacobi algebras," dealing only with Lie algebras instead. To appear in Math. Annalen
Attraction centers and PT-symmetric delta-functional dipoles in critical and supercritical self-focusing media
Creators: name: Wang, Li
name: Malomed, Boris A.
name: Yan, Zhenya
Publisher: name: arXiv
Year: 2019
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: Quantum Gases (cond-mat.quant-gas)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We introduce a model based on the one-dimensional nonlinear Schroedinger equation (NLSE) with the critical (quintic) or supercritical self-focusing nonlinearity. We demonstrate that a family of solitons, which are unstable in this setting against collapse, is stabilized by pinning to an attractive defect, that may also include a parity-time (PT)-symmetric gain-loss component. The model can be realized as a planar waveguide in optics, and in a super-Tonks-Girardeau bosonic gas. For the attractive defect with the delta-functional profile, a full family of the pinned solitons is found in an exact form. In the absence of the gain-loss term, the solitons' stability is investigated analytically too, by means of the Vakhitov-Kolokolov criterion; in the presence of the PT-balanced gain and loss, the stability is explored by means of numerical methods. In particular, the entire family of pinned solitons is stable in the quintic medium if the gain-loss term is absent. A stability region for the pinned solitons persists in the model with an arbitrarily high power of the self-focusing nonlinearity. A weak gain-loss component gives rise to alternations of stability and instability in the system's parameter plane. Those solitons which are unstable under the action of the supercritical self-attraction are destroyed by the collapse. If the self-attraction-driven instability is weak and the gain-loss term is present, unstable solitons spontaneously transform into localized breathers. The same outcome may be caused by a combination of the critical nonlinearity with the gain and loss. Instability of the solitons is also possible when the PT-symmetric gain-loss term is added to the subcritical nonlinearity. The system with self-repulsive nonlinearity is briefly considered too, producing completely stable families of pinned localized states.
description: To be published in Phys. Rev. E
Additional file 1: of Estimated dengue force of infection and burden of primary infections among Indian children
Creators: name: Bhavsar, Amit
name: Tam, Clarence
name: Suneela Garg
name: Guru Jammy
name: Anne-Frieda Taurel
name: Sher-Ney Chong
name: Nealon, Joshua
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Table S1. Number of subjects with IgG data available from DNG10 study according to age (% seropositive). (DOCX 20 kb)