cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Stellar dynamics in the central arcsecond of our galaxy
Creators: name: Schoedel, R.
name: Genzel, R.
name: Ott, T.
name: Eckart, A.
name: Mouawad, N.
name: Alexander, T.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present proper motions for $>$40 stars at projected distances $\leq1.2''$ from Sagittarius A* (Sgr A*). We find evidence on a $\geq2σ$ level for radial anisotropy of the cluster of stars within $1''$ of Sgr A*. We find no evidence for a stationary source or variable source at the position of Sgr A*. We confirm/find accelerated motion for 6 stars, with 4 stars having passed the pericenter of their orbits during the observed time span. We calculated/constrained the orbital parameters of these stars. All orbits have moderate to high eccentricities. We discuss the possible bias in detecting preferentially orbits with high eccentricities. We find that the center of acceleration for all the orbits coincides with the radio position of Sgr A*. From the orbit of the star S2, the currently most tightly constrained one, we determine the mass of Sgr A* to be $3.3\pm0.7\times10^{6}$M$_{\odot}$ and its position to $2.0\pm2.4$ mas East and $2.7\pm4.5$ mas South of the nominal radio position. The mass estimate for the central dark mass from the orbit of S2 is fully consistent with the mass estimate of $3.4\pm0.5\times10^{6}$M$_{\odot}$ obtained from stellar proper motions within $1.2''$ of Sgr A* using a Leonard-Merritt mass estimator. We find that radio astronomical observations of the proper motion of Sgr A* in combination with its intrinsic source size place at the moment the tightest constraints on the mass density of Sgr A*, which must exceed $ρ_{\mathrm{Sgr A*}}>3\times10^{19}\mathrm{M}_{\odot}\mathrm{pc}^{-3}$.
description: 51 pages, 16 Figures, reviewed ms submitted to apj
Dynamics and correlations at a quantum phase transition beyond Kibble-Zurek
Creators: name: Roychowdhury, Krishanu
name: Moessner, Roderich
name: Das, Arnab
Publisher: name: arXiv
Year: 2020
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Gases (cond-mat.quant-gas)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Kibble-Zurek theory (KZ) stands out as the most robust theory of defect generation in the dynamics of phase transitions. KZ utilizes the structure of equilibrium states away from the transition point to estimate the excitations due to the transition using adiabatic and impulse approximations. Here we show, the actual nonequilibrium dynamics lead to a qualitatively different scenario from KZ, as far correlations between the defects (rather than their densities) are concerned. For a quantum Ising chain, we show, this gives rise to a Gaussian spatial decay in the domain wall (kinks) correlations, while KZ would predict an exponential fall. We propose a simple but general framework on top of KZ, based on the "quantum coarsening" dynamics of local correlators in the supposed impulse regime. We outline how our picture extends to generic interacting situations.
description: Main draft: 11 pages, 2 figures
From supermembrane to super Yang-Mills theory
Creators: name: Uehara, Shozo
name: Yamada, Satoshi
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We derive p+1-dimensional (p=1,2) maximally supersymmetric U(N) Yang-Mills theory from the wrapped supermembrane on $R^{11-p}\times T^{p}$ in the light-cone gauge by using the matrix regularization. The elements of the matrices in the super Yang-Mills theory are given by the Fourier coefficients in the supermembrane theory. Although our approach never refers to both D-branes and superstring dualities, we obtain the relations which exactly represent T-duality.
description: 18 pages, typos corrected, to appear in Nucl. Phys. B
Large effect of polydispersity on defect concentrations in colloidal crystals
Creators: name: Pronk, Sander
name: Frenkel, Daan
Publisher: name: arXiv
Year: 2004
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We compute the equilibrium concentration of stacking faults and point defects in polydisperse hard-sphere crystals. We find that, while the concentration of stacking faults remains similar to that of monodisperse hard sphere crystals, the concentration of vacancies decreases by about a factor two. Most strikingly, the concentration of interstitials in the maximally polydisperse crystal may be some six orders of magnitude larger than in a monodisperse crystal. We show that this dramatic increase in interstitial concentration is due to the increased probability of finding small particles and that the small-particle tail of the particle size distribution is crucial for the interstitial concentration in a colloidal crystal.
description: 6 pages, 4 figures
Cherenkov Telescope Array potential in the search for Galactic PeVatrons
Creators: name: Angüner, E. O.
name: Cassol, F.
name: Costantini, H.
name: Trichard, C.
name: Verna, G.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: One of the major scientific objectives of the future Cherenkov Telescope Array (CTA) Observatory is the search for PeVatrons. PeVatrons are cosmic-ray factories able to accelerate nuclei at least up to the knee feature seen in the spectrum of cosmic rays measured near the Earth. CTA will perform a survey of the full Galactic plane at TeV energies and beyond with unprecedented sensitivity. The determination of efficient criteria to identify PeVatron candidates during the survey is essential in order to trigger further dedicated observations. Here, we present results from a study based on simulations to determine these criteria. The outcome of the study is a PeVatron figure of merit, defined as a metric that provides relations between spectral parameters and spectral cutoff energy lower limits. In addition, simulations of the PeVatron candidate HESS J1641$-$463 and its parental particle spectrum are presented and discussed. Eventually, our work is applied to simulated population of Galactic PeVatrons, with the aim to determine the sensitivity of CTA.
description: 8 pages, 4 figures, Proceedings of ICRC 2019
Formation of Planetary Populations II: Effects of Initial Disk Size & Radial Dust Drift
Creators: name: Alessi, Matthew
name: Pudritz, Ralph E.
name: Cridland, Alex J.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Recent ALMA observations indicate that while a range of disk sizes exist, typical disk radii are small, and that radial dust drift affects the distribution of solids in disks. Here we explore the consequences of these features in planet population synthesis models. A key feature of our model is planet traps - barriers to otherwise rapid type-I migration of forming planets - for which we include the ice line, heat transition, and outer edge of the dead zone. We find that the ice line plays a fundamental role in the formation of warm Jupiters. In particular, the ratio of super Earths to warm Jupiters formed at the ice line depend sensitively on the initial disk radius. Initial gas disk radii of $\sim$50 AU results in the largest super Earth populations, while both larger and smaller disk sizes result in the ice line producing more gas giants near 1 AU. This transition between typical planet class formed at the ice line at various disk radii confirms that planet formation is fundamentally linked to disk properties (in this case, disk size), and is a result that is only seen when dust evolution effects are included in our models. Additionally, we find that including radial dust drift results in the formation of more super Earths between 0.1 - 1 AU, having shorter orbital radii than those produced in models where dust evolution effects are not included.
description: 24 pages, 13 figures. Submitted to MNRAS; revised in response to referee
Podura aquatica Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Entognatha
Collembola
Poduridae
Podura
Podura aquatica

description: Podura aquatica [spec. nov.]
P. nigra aquatica. Fn. svec. 1178.
De Geer act. Ups. 1740. p. 57. t. 3.
Stockh. 1740. p. 279. t. 3, 4.
Habitat in Aquosis Europae.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 609, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Star Formation at z~6: i-dropouts in the ACS GTO fields
Creators: name: Bouwens, R. J.
name: Illingworth, G. D.
name: Rosati, P.
name: Lidman, C.
name: Broadhurst, T.
name: Franx, M.
name: Ford, H. C.
name: Magee, D.
name: Benitez, N.
name: Blakeslee, J. P.
name: Meurer, G. R.
name: Clampin, M.
name: Hartig, G. F.
name: Ardila, D. R.
name: Bartko, F.
name: Brown, R. A.
name: Burrows, C. J.
name: Cheng, E. S.
name: Cross, N. J. G.
name: Feldman, P. D.
name: Golimowski, D. A.
name: Gronwall, C.
name: Infante, L.
name: Kimble, R. A.
name: Krist, J. E.
name: Lesser, M. P.
name: Martel, A. R.
name: Menanteau, F.
name: Miley, G. K.
name: Postman, M.
name: Sirianni, M.
name: Sparks, W. B.
name: Tran, H. D.
name: Tsvetanov, Z. I.
name: White, R. L.
name: Zheng, W.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using an i-z dropout criterion, we determine the space density of z~6 galaxies from two deep ACS GTO fields with deep optical-IR imaging. A total of 23 objects are found over 46 arcmin^2, or ~0.5 objects/arcmin^2 down to z~27.3 (6 sigma; all AB mag) (including one probable z~6 AGN). Combining deep ISAAC data for our RDCS1252-2927 field (J~25.7 and Ks~25.0 (5 sigma)) and NICMOS data for the HDF North (JH~27.3 (5 sigma)), we verify that these dropouts have flat spectral slopes. i-dropouts in our sample range in luminosity from ~1.5 L* (z~25.6) to ~0.3 L* (z~27.3) with the exception of one very bright candidate at z~24.2. The half-light radii vary from 0.09" to 0.29", or 0.5 kpc to 1.7 kpc. We derive the z~6 rest-frame UV luminosity density using three different procedures, each utilizing simulations based on a CDF South V dropout sample. First, we compare our findings with a no-evolution projection of this V-dropout sample. We find 23+/-25% more i-dropouts than we predict. Adopting previous results to z~5, this works out to a 20+/-29% drop in the luminosity density from z~3 to z~6. Second, we use these same V-dropout simulations to derive a selection function for our i-dropout sample and compute the UV-luminosity density (7.2+/-2.5 x 10^25 ergs/s/Hz/Mpc^3 down to z~27). We find a 39+/-21% drop over the same redshift range. This is our preferred value and suggests a star formation rate of 0.0090+/-0.0031 M_sol/yr/Mpc^3 to z~27, or ~0.036+/- 0.012 M_sol/yr/Mpc^3 extrapolating the LF to the faint limit. Third, we follow a very similar procedure, but assume no incompleteness, finding a luminosity density which is ~2-3X lower. This final estimate constitutes a lower limit. All three estimates are within the canonical range of luminosity densities necessary for reionization of the universe at this epoch. (abridged)
description: 36 pages, 13 figures, 2 tables, accepted for publication in ApJ, postscript version with high-resolution figures can be downloaded at http://www.ucolick.org/~bouwens/idropout.ps
Additional file 5 of Tuberomics: a molecular profiling for the adaption of edible fungi (Tuber magnatum Pico) to different natural environments
Creators: name: Vita, Federico
name: Giuntoli, Beatrice
name: Bertolini, Edoardo
name: Taiti, Cosimo
name: Marone, Elettra
name: Dâ€™Ambrosio, Chiara
name: Trovato, Emanuela
name: Sciarrone, Danilo
name: Mariosimone Zoccali
name: Balestrini, Raffaella
name: Scaloni, Andrea
name: Mondello, Luigi
name: Mancuso, Stefano
name: Alessio, Massimo
name: Alpi, Amedeo
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Molecular Biology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Computational Biology

description: Additional file 5: Table S5. RNA-seq statistics from Vita et al. [33].
Podura aquatica Linnaeus 1758
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Poduromorpha
Poduridae
Podura
Podura aquatica

description: Podura aquatica Linnaeus, 1758 *
Podura aquatica Linnaeus, 1758: 609.
Podura atra aquatica Geoffroy, 1762: 610.
Hypogastrura aquatica Bourlet, 1839: 407.
DISTRIBUTION. — Europe. Latreille 1812.
France. Latreille 1806. — Bourlet 1839, 1841, 1843 (Hypogastrura armata). — Eaux stagnantes (Finot 1890).
Ariège. Forêtde Freychinède, 1350 m (Lek-Ang etal. 2007).
Bouches-du-Rhône. La Tour-du-Valat en Camargue (Cassagnau & Juberthie 1967a).
Calvados. Brébisson 1827.
Corse. Poinsot 1970.
Essonne. Forêtde Sénart (Pichard 1973, 1978; Ponge 1980, 1993). — Maresde Sénart (Pichard etal. 1989).
Finistère. Roscoff (Delamare Deboutteville 1943).
Hautes-Pyrénées. Valléed’Estibère, 2500 m (Cassagnau & Delamare Deboutteville 1951). — Orédon (Cassagnau 1954a). — Massif du Néouvielle (Cassagnau 1961).
Hauts-de-Seine. Forêtde Meudon (Pichard 1973, 1978). — Mares de Clamart (Pichard etal. 1989).
Île-de-France. Environs de Paris (Geoffroy 1762, « la Podura noire aquatique » ou P. a. aquatica; Boisduval & Lacordaire 1835).
Nord. Cambrai (Bourlet 1845, «Pluie de Podurelles»).
Oise. Lalandelle (D’Haese 2002).
Pas-de-Calais. Wimereux (Willem 1925b).
Saone-et-Loire. Uchon en Morvan (Denis 1921).
Seine-Maritime. Montivilliers (Carl 1899).
Vendée. Île-d’Yeu surmare (Denis 1921, 1922a).
PHYSIOLOGIE. — Cassagnau & Juberthie 1967a (complexe endocrine cérébral).
ÉCOLOGIE. — Willem 1925b; Cassagnau 1961; Pichard 1973; Ponge 1980, 1993; Pichard etal. 1989; Lek-Ang etal. 2007.
PRÉDATION. — Pichard 1978 (hémiptère hétéroptère).
DONNÉES MOLÉCULAIRES. — D’Haese 2002 (phylogénie).
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 347, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
Scaling of excitons in carbon nanotubes
Creators: name: Perebeinos, Vasili
name: Tersoff, J.
name: Avouris, Phaedon
Publisher: name: arXiv
Year: 2004
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Light emission from carbon nanotubes is expected to be dominated by excitonic recombination. Here we calculate the properties of excitons in nanotubes embedded in a dielectric, for a wide range of tube radii and dielectric environments. We find that simple scaling relationships give a good description of the binding energy, exciton size, and oscillator strength.
description: 4 pages, 3 figures, accepted for publication in Phys. Rev. Lett
Additional file 1 of Patients with positive malaria tests not given artemisinin-based combination therapies: a research synthesis describing under-prescription of antimalarial medicines in Africa
Creators: name: Shennae O’Boyle
name: Bruxvoort, Katia
name: Ansah, Evelyn
name: Burchett, Helen
name: Chandler, Clare
name: Siân Clarke
name: Goodman, Catherine
name: Mbacham, Wilfred
name: Mbonye, Anthony
name: Obinna Onwujekwe
name: Staedke, Sarah
name: Wiseman, Virginia
name: Whitty, Christopher
name: Hopkins, Heidi
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1: Table S1. Number (%) of mRDT-positive patients i) not prescribed ACT and ii) prescribed other medications. Table S2. Risk factors associated with non-prescription of ACT in mRDT-positive patients not prescribed ACT. Table S3. Risk factors associated with prescription of medications in mRDT-positive patients not prescribed ACT.
Excursion decompositions for $\SLE$ and Watts' crossing formula
Creators: name: Dubedat, Julien
Publisher: name: arXiv
Year: 2004
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 60K35; 82B43; 60G18; 60G51

description: It is known that Schramm-Loewner Evolutions (SLEs) have a.s. frontier points if $κ>4$ and a.s. cutpoints if $44$, an appropriate version of $\SLE(κ)$ has a renewal property: it starts afresh after visiting its frontier. Thus one can give an excursion decomposition for this particular $\SLE(κ)$ ``away from its frontier''. For $4
description: 36 pages
Recognizing black holes in gravitational-wave observations: Challenges in telling apart impostors in mass-gap binaries
Creators: name: Datta, Sayak
name: Phukon, Khun Sang
name: Bose, Sukanta
Publisher: name: arXiv
Year: 2020
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We study how by careful monitoring of the presence or absence of tidal deformability (TD) and tidal-heating (TH) in the inspiral signal of compact object binaries in ground-based gravitational wave (GW) detectors, one can test if its components are black holes or not. The former property (TD) is finite for neutron stars but vanishes for black holes (in general relativity), whereas the latter is finite for black holes and negligible for neutron stars, and affects the GW phase evolution of binaries in a distinctly different way. We introduce waveform parameters that characterize the strength of tidal-heating, and are zero when there is no horizon. We develop Bayesian methods that use TD and TH for distinguishing the presence or absence of horizons in a binary. This is timely owing to several claims that these stellar-mass objects, especially, with masses heavier than those of neutron stars, may not have a horizon but may be black hole mimickers or exotic compact objects (ECOs). It is also astrophysically important to have the tools to test the presence or absence of horizons in mass-gap binaries and, thereby, help detect the heaviest neutron star or the lightest black hole. A proper accounting of tidal-heating in binary waveform models will also be critical for an unbiased measurement of characteristics of the equation of state of neutron stars in GW observations of binaries containing them -- or even to probe the existence of ECOs. We show that purely based on GW waveforms it will not be possible to discern binary horizons in the mass gap in Advanced LIGO, Virgo and KAGRA detectors unless the binary is within a few tens of Mpc. However, third generation ground-based detectors will be able to do so for binaries a few hundred Mpc away.
Blending of nanoscale and microscale in uniform large-area sculptured thin-film architectures
Creators: name: Horn, Mark W.
name: Pickett, Matthew D.
name: Messier, Russell
name: Lakhtakia, Akhlesh
Publisher: name: arXiv
Year: 2003
Subjects: subject: Optics (physics.optics)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The combination of large thickness ($>3$ $μ$m), large--area uniformity (75 mm diameter), high growth rate (up to 0.4 $μ$m/min) in assemblies of complex--shaped nanowires on lithographically defined patterns has been achieved for the first time. The nanoscale and the microscale have thus been blended together in sculptured thin films with transverse architectures. SiO$_x$ ($x\approx 2$) nanowires were grown by electron--beam evaporation onto silicon substrates both with and without photoresist lines (1--D arrays) and checkerboard (2--D arrays) patterns. Atomic self--shadowing due to oblique--angle deposition enables the nanowires to grow continuously, to change direction abruptly, and to maintain constant cross--sectional diameter. The selective growth of nanowire assemblies on the top surfaces of both 1--D and 2--D arrays can be understood and predicted using simple geometrical shadowing equations.
description: 17 pages, 9 figures
Blockchain Enabled Smart Contract Based Applications: Deficiencies with the Software Development Life Cycle Models
Creators: name: Miraz, Mahdi H.
name: Ali, Maaruf
Publisher: name: arXiv
Year: 2020
Subjects: subject: Computers and Society (cs.CY)
subject: Networking and Internet Architecture (cs.NI)
subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: With the recent popularity of Blockchain and other Distributed Ledger Technologies (DLT), blockchain enabled smart contract applications has attracted increased research focus. However, the immutability of the blocks, where the smart contracts are stored, causes conflicts with the traditional Software Development Life Cycle (SDLC) models usually followed by software engineers. This clearly shows the unsuitability of the application of SDLC in designing blockchain enabled smart contract based applications. This research article addresses this current problem by first exploring the six traditional SDLC models, clearly identifying the conflicts in a table with the application of smart contracts and advocates that there is an urgent need to develop new standard model(s) to address the arising issues. The concept of both block immutability and contract is introduced. This is further set in a historical context from legacy smart contracts and blockchain enabled smart contracts extending to the difference between "shallow smart contracts" and "deep smart contracts". To conclude, the traditional SDLC models are unsuitable for blockchain enabled smart contract-based applications.
The Hubble Constant from the Gravitational Lens B1608+656
Creators: name: Koopmans, L. V. E.
name: Treu, T.
name: Fassnacht, C. D.
name: Blandford, R. D.
name: Surpi, G.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a refined gravitational lens model of the four-image lens system B1608+656 based on new and improved observational constraints: (i) the three independent time-delays and flux-ratios from VLA observations, (ii) the radio-image positions from VLBA observations, (iii) the shape of the deconvolved Einstein Ring from optical and infrared HST images, (iv) the extinction-corrected lens-galaxy centroids and structural parameters, and (v) a stellar velocity dispersion, sigma_ap=247+-35 km/s, of the primary lens galaxy (G1), obtained from an echelle spectrum taken with the Keck--II telescope. The lens mass model consists of two elliptical mass distributions with power-law density profiles and an external shear, totaling 22 free parameters, including the density slopes which are the key parameters to determine the value of H_0 from lens time delays. This has required the development of a new lens code that is highly optimized for speed. The minimum-chi^2 model reproduces all observations very well, including the stellar velocity dispersion and the shape of the Einstein Ring. A combined gravitational-lens and stellar dynamical analysis leads to a value of the Hubble Constant of H_0=75(+7/-6) km/s/Mpc (68 percent CL; Omega_m=0.3, Omega_Lambda=0.7. The non-linear error analysis includes correlations between all free parameters, in particular the density slopes of G1 and G2, yielding an accurate determination of the random error on H_0. The lens galaxy G1 is ~5 times more massive than the secondary lens galaxy (G2), and has a mass density slope of gamma_G1=2.03(+0.14/-0.14) +- 0.03 (68 percent CL) for rho~r^-gamma', very close to isothermal (gamma'=2). (Abridged)
description: 17 pages, 6 figures, 5 tables; revised version with correct fig.6 and clarified text based on referee report; conclusions unchanged
Willowsia guangdongensis Zhang & Chen 2007, sp. nov.
Creators: name: Zhang, Feng
name: Chen, Guo-Liang Xu Jian-Xiu
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Entognatha
Collembola
Entomobryidae
Willowsia
Willowsia guangdongensis

description: Willowsia guangdongensis sp. nov.
Figs 1–20, Tab.1
Type material. HOLOTYPE: male, China, Guangdong Province, Heshan, Heshan Hilly Land Interdisciplinary Experimental Station, Chinese Academy of Sciences, 15.ix.2006, collection number C9522, coll. Jian-xiu Chen, Feng Zhang, and Jigang Jiang. PARATYPES: two females and two males, same data as holotype.
Description. Body length: up to 1.86 mm.
Color pattern. Ground color pale yellow in alcohol. Eye patches dark blue. Antennae and each segment gradually darker towards apex, Ant. III and IV dark blue. Transverse dark blue band present just behind antennal bases. Body dorsum with scattered blue pigment present on area anterior to eye patches, along lateral margins from thorax to anterior parts of Abd. III, along posterior margins of Abd. IV and V, and on whole Abd. VI. Abd. III and IV respectively with one pair of pale blue patches on dorso-lateral sides. Each leg with two dark blue bands respectively on apex of femur and mid of tibiotarsus (Fig. 1).
Head. Antenna 1.9-2.3 times as long as cephalic diagonal. Antennal segments ratio as I: II: III: IV = 1: 1.56–1.78: 1.33-1.56: 2.00–2.22. Antennal apical bulb distinct and unilobed (Fig. 2). Sensory organ of Ant. III as two small rods (Fig. 3).
 Eyes 8+8, eyes A and B largest and subequal, G and H smallest and subequal. Labral papillae absent. Prelabral and labral setae 4/ 5, 5, 4, all smooth. Outer differentiated seta of labial palp slightly curved, as thick as normal setae, with tip nearly reaching apex of labial papilla (Fig. 4). Subapical seta of maxillary outer lobe large, subequal in length to and slightly thicker than apical one; 3 smooth hairs on sublobal plate (Fig. 5). Labial triangular setae (after Chen & Christiansen 1993) as M 1, r, E, L 1, L 2; all finely ciliate, r 0.5 length of M 1 (Fig. 6). Cephalic dorsal chaetotaxy with four antennal (An), three median (M) and four sutural (S) macrochaetae. Interocular setae (after Mari-Mutt 1986) as pqrst (Fig. 7).
Thorax and legs. Dorsal macrochaetae (after Szeptycki 1979) shown in Fig. 8. Th. II with three posterior macrochaetae (p1–3) on each side. Th. III with totally 9 macrosetae, four of them (p5, p6, m6 and m6e) on posterior lateral margin.
description: Published as part of Zhang, Feng & Chen, Guo-Liang Xu Jian-Xiu, 2007, A new species of Willowsia (Collembola: Entomobryidae) from South China, pp. 63-68 in Zootaxa 1645 (1) on pages 64-65, DOI: 10.11646/zootaxa.1645.1.6, http://zenodo.org/record/5103773
An Effective Automatic Image Annotation Model Via Attention Model and Data Equilibrium
Creators: name: Vatani, Amir
name: Ahvanooey, Milad Taleby
name: Rahimi, Mostafa
Publisher: name: arXiv
Year: 2020
Subjects: subject: Multimedia (cs.MM)
subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences

description: Nowadays, a huge number of images are available. However, retrieving a required image for an ordinary user is a challenging task in computer vision systems. During the past two decades, many types of research have been introduced to improve the performance of the automatic annotation of images, which are traditionally focused on content-based image retrieval. Although, recent research demonstrates that there is a semantic gap between content-based image retrieval and image semantics understandable by humans. As a result, existing research in this area has caused to bridge the semantic gap between low-level image features and high-level semantics. The conventional method of bridging the semantic gap is through the automatic image annotation (AIA) that extracts semantic features using machine learning techniques. In this paper, we propose a novel AIA model based on the deep learning feature extraction method. The proposed model has three phases, including a feature extractor, a tag generator, and an image annotator. First, the proposed model extracts automatically the high and low-level features based on dual-tree continues wavelet transform (DT-CWT), singular value decomposition, distribution of color ton, and the deep neural network. Moreover, the tag generator balances the dictionary of the annotated keywords by a new log-entropy auto-encoder (LEAE) and then describes these keywords by word embedding. Finally, the annotator works based on the long-short-term memory (LSTM) network in order to obtain the importance degree of specific features of the image. The experiments conducted on two benchmark datasets confirm that the superiority of the proposed model compared to the previous models in terms of performance criteria.
description: 9 pages, 3 figures
Agrenia bidenticulata
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Entomobryomorpha
Isotomidae
Agrenia
Agrenia bidenticulata

description: Agrenia bidenticulata (Tullberg, 1876) *
Isotoma bidenticulata Tullberg, 1876: 35.
Agrenia bidenticulata – Axelson 1907: 131.
DISTRIBUTION. — Hautes-Alpes. Rif-Blanc du Lautaret Massif du Pelvoux (Vaillant 1956).
Loire-Atlantique. Le Croisic (Moniez 1890a).
Vosges. Chaume du Rouge-Gazon (Denis 1925a).
ÉCOLOGIE. — Vaillant 1956 (faune hygropétrique).
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 347, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
The decay time scale for highly excited nuclei as seen from asymmetrical emission of particles
Creators: name: Jandel, M.
name: Botvina, A. S.
name: Yennello, S. J.
name: Souliotis, G. A.
name: Shetty, D. V.
name: Bell, E.
name: Keksis, A.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: A novel method was developed for the extraction of short emission times of light particles from the projectile-like fragments in peripheral deep-inelastic collisions in the Fermi energy domain. We have taken an advantage of the fact that in the external Coulomb field particles are evaporated asymmetrically. It was possible to determine the emission times in the interval 50-500 fm/c using the backward emission anisotropy of alpha-particles relative to the largest residue, in the reaction 28Si + 112Sn at 50 MeV/nucleon. The extracted times are consistent with predictions based on the evaporation decay widths calculated with the statistical evaporation model generalized for the case of the Coulomb interaction with the target.
description: 13 pages, 5 figures, submitted to Phys. Lett. B
X-ray spectral and timing properties of the 2001 superburst of 4U 1636-536
Creators: name: Kuulkers, Erik
name: Zand, Jean in 't
name: Homan, Jeroen
name: van Straaten, Steve
name: Altamirano, Diego
name: van der Klis, Michiel
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Preliminary results are reported on the spectral and timing properties of the spectacular 2001 superburst of 4U 1636-536 as seen by the RXTE/PCA. The (broad-band) power-spectral and hardness properties during the superburst are compared to those just before and after the superburst. Not all of the superburst emission can be fitted by pure black-body radiation. We also gathered BeppoSAX/WFC and RXTE/ASM data, as well as other RXTE/PCA data, obtained days to months before and after the superburst to investigate the normal X-ray burst behavior around the time of the superburst. The first normal X-ray burst after the 2001 superburst was detected 23 days later. During inspection of all the RXTE/ASM data we found a third superburst. This superburst took place on June 26, 1999, which is ~2.9 yrs after the 1996 superburst and ~1.75 yrs before the 2001 superburst. The above findings are the strongest constraints observed so far on the duration of the cessation of normal X-ray bursts after a superburst and the superburst recurrence times.
description: 4 pages, 4 figures,to appear in the proceedings of "X-Ray Timing 2003: Rossi and Beyond", eds. P. Kaaret, F.K. Lamb, & J.H. Swank (Melville, NY: AIP)
title: An efficient out-of-core multifrontal solver for large-scale unsymmetric element problems
Creators: name: Reid, JK
name: Scott, JA
Publisher: name: STFC
Year: 2007
Subjects: Fortran 95
large sparse unsymmetric linear systems
partial pivoting
element problems
multifrontal
out-of-core solver
rook pivoting

description: In many applications where the efficient solution of large sparse linear systems of equations is required, a direct method is frequently the methos of choice. Unfortunately, direct methods have a potentially severe limitation: as the problem size grows, the memory needed generally increases rapidly. However the in-core memory requirements can be limited by storing the matrix and its factors externally, allowing the solver to be used for very large problems. The code, which is called HSL_MA78, implements a multifrontal algorithm and achieves efficiency through the use of specially designed code for handling the input/output operations and efficient dense linear algebra kernals. These kernals, which are available as a separate package called HSL_MA74, use high level BLAS to perform the partial factorization of the frontal matrices and offer both threshold partial and rook pivoting. In this paper, we describe the algorithms used by HSL_MA74 and illustrate the performance of our new codes using problems from a range of practical applications.
Carnegie Supernova Project-II: Near-infrared Spectroscopic Diversity of Type II Supernovae
Creators: name: Davis, S.
name: Hsiao, E. Y.
name: Ashall, C.
name: Hoeflich, P.
name: Phillips, M. M.
name: Marion, G. H.
name: Kirshner, R. P.
name: Morrell, N.
name: Sand, D. J.
name: Burns, C.
name: Contreras, C.
name: Stritzinger, M.
name: Anderson, J. P.
name: Baron, E.
name: Diamond, T.
name: Gutierrez, C. P.
name: Hamuy, M.
name: Holmbo, S.
name: Kasliwal, M. M.
name: Krisciunas, K.
name: Kumar, S.
name: Lu, J.
name: Pessi, P. J.
name: Piro, A. L.
name: Prieto, J. L.
name: Shahbandeh, M.
name: Suntzeff, N. B.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present $81$ near-infrared (NIR) spectra of $30$ Type II supernovae (SNe II) from the Carnegie Supernova Project-II (CSP-II), the largest such dataset published to date. We identify a number of NIR features and characterize their evolution over time. The NIR spectroscopic properties of SNe II fall into two distinct groups. This classification is first based on the strength of the He I $\lambda1.083\,μ$m absorption during the plateau phase; SNe II are either significantly above (spectroscopically strong) or below $50$ angstroms (spectroscopically weak) in pseudo equivalent width. However between the two groups, other properties, such as the timing of CO formation and the presence of Sr II, are also observed. Most surprisingly, the distinct weak and strong NIR spectroscopic classes correspond to SNe II with slow and fast declining light curves, respectively. These two photometric groups match the modern nomenclature of SNe IIP and IIL. Including NIR spectra previously published, 18 out of 19 SNe II follow this slow declining-spectroscopically weak and fast declining-spectroscopically strong correspondence. This is in apparent contradiction to the recent findings in the optical that slow and fast decliners show a continuous distribution of properties. The weak SNe II show a high-velocity component of helium that may be caused by a thermal excitation from a reverse-shock created by the outer ejecta interacting with the red supergiant wind, but the origin of the observed dichotomy is not understood. Further studies are crucial in determining whether the apparent differences in the NIR are due to distinct physical processes or a gap in the current data set.
description: 32 pages, 17 figures, accepted to ApJ
Additional file 3 of Tuberomics: a molecular profiling for the adaption of edible fungi (Tuber magnatum Pico) to different natural environments
Creators: name: Vita, Federico
name: Giuntoli, Beatrice
name: Bertolini, Edoardo
name: Taiti, Cosimo
name: Marone, Elettra
name: Dâ€™Ambrosio, Chiara
name: Trovato, Emanuela
name: Sciarrone, Danilo
name: Mariosimone Zoccali
name: Balestrini, Raffaella
name: Scaloni, Andrea
name: Mondello, Luigi
name: Mancuso, Stefano
name: Alessio, Massimo
name: Alpi, Amedeo
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Computational Biology

description: Additional file 3: Table S3. Additional information related to the uncharacterized and predicted proteins identified through mass spectrometry.
Anurophorus laricis Nicolet 1842
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Entomobryomorpha
Isotomidae
Anurophorus
Anurophorus laricis

description: Anurophorus laricis Nicolet, 1842 *
Anurophorus laricis Nicolet, 1842: 53.
Adicranus corticinus Bourlet, 1841: 127.
Lipura corticinia Lubbock, 1862a: 600.
DISTRIBUTION. — France. Bourlet 1841, 1843, 1845 (A. corticinus). — Finot 1890 (Lipura corticinia).
Aisne. Jouz (Lécaillon 1901).
Ardèche. Serre des Fourches près de Lagorce (Stomp et al. 1982).
Ariège. Saint-Jean-de-Verges et Col de Latour-Lafont (Cassagnau 1954d).
Bouches-du-Rhône. Forêtde Cadarache (Rougon & Rougon 1970). — Cadarache (Poinsot-Balaguer 1976d).
Corse. Poinsot-Balaguer 1978.
Côte-d’Or. Fontaines-les-Dijon (Denis 1924d).
Finistère. Embouchure du Guillec et à Kérestat près de Roscoff (Delamare Deboutteville 1943).
Haute-Garonne. Toulouse, Fenouillet etbois dela Laramette (Cassagnau 1954d). — Toulouse (Cassagnau 1962a, b).
Haute-Marne ou Suisse? Chaumont (Nicolet 1842).
Hautes-Pyrénées. Massif du Néouvielle (Cassagnau & Lauga-Reyrel 1985, A. clavipilus). — Montagned’Arize (Deharveng 1996).
Hérault. Montpellier (Denis 1924d).
Marne. Environsde Reims (Lemoine 1883).
Savoie. Forêtde Mâcot-la-Plagne, 950- 2150 m (Loranger etal. 2001). Sud-Ouestde la France et Pyrénées. Cassagnau 1961 (A. clavipilus). Tarn, Aude. Montagne Noire (Cassagnau 1965).
Tarn. Sidobre (Izarra 1969). — Bonnet etal. 1970, 1972, 1975.
CHÉTOTAXIE, MORPHO- ANATOMIE. — Cassagnau & Lauga-Reyrel 1985 (architecture cuticulaire, A. clavipilus).
DÉVELOPPEMENT. — Lemoine 1883 (développement embryonnaire).
ÉCOLOGIE. — Cassagnau 1962a, b (biocénose), 1965 (écologie, sol); Bonnet etal. 1970, 1972, 1975 (écologie, muscicoles); Rougon &
Rougon 1970; Poinsot-Balaguer 1976d (irradiation); Deharveng 1996 (déboisement, reboisement); Loranger etal. 2001 (sol acide).
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on pages 347-348, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
Additional file 4 of Tuberomics: a molecular profiling for the adaption of edible fungi (Tuber magnatum Pico) to different natural environments
Creators: name: Vita, Federico
name: Giuntoli, Beatrice
name: Bertolini, Edoardo
name: Taiti, Cosimo
name: Marone, Elettra
name: Dâ€™Ambrosio, Chiara
name: Trovato, Emanuela
name: Sciarrone, Danilo
name: Mariosimone Zoccali
name: Balestrini, Raffaella
name: Scaloni, Andrea
name: Mondello, Luigi
name: Mancuso, Stefano
name: Alessio, Massimo
name: Alpi, Amedeo
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Computational Biology

description: Additional file 4: Table S4. Summary of sulfur-related proteins identified by nanoLC-ESI-LIT-MS/MS analysis.
On the Measurement of Solar Neutrino Oscillation Parameters with KamLAND
Creators: name: Bandyopadhyay, Abhijit
name: Choubey, Sandhya
name: Goswami, Srubabati
name: Petcov, S. T.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: A new reactor power plant Shika-2, with a power of approximately 4 GW and at a distance of about 88 km from the KamLAND detector is scheduled to start operating in March 2006. We study the impact of the $\barν_e$ flux from this reactor on the sensitivity of the KamLAND experiment to the solar neutrino oscillation parameters. We present results on prospective determination of $Δm^2_\odot$ and $\sin^2θ_\odot$ using the combined data from KamLAND and the solar neutrino experiments, including the effect of the Shika-2 contribution to the KamLAND signal and the latest data from the salt enriched phase of the SNO experiment. We find that contrary to the expectations, the addition of the Shika-2 reactor flux does not improve the $\sin^2θ_\odot$ sensitivity of KamLAND, while the ambiguity in $Δm^2_\odot$ measurement may even increase, as a result of the averaging effect between Kashiwazaki and the Shika-2 reactor contributions to the KamLAND signal.
description: Version to appear in Phys. Lett. B
BRCA1 and TP53 mutations in ovarian cancer: Molecular genetic insights and updated situations in Thailand
Creators: name: Sumana Dakeng, Sureerut Porntadavity
Publisher: name: Genetics Society of Thailand
Year: 2018
Subjects: ovarian cancer
BRCA1
TP53
mutations
Thailand

description: Genomics and Genetics, 11, 3, 26-34
In vitro histomechanical effects of enzymatic degradation in carotid arteries during inflation tests with pulsatile loading
Creators: name: Trabelsi, Olfa
name: Dumas, Virginie
name: Breysse, Edouard
name: Laroche, Norbert
name: Avril, StéPhane
Publisher: name: arXiv
Year: 2019
Subjects: subject: Medical Physics (physics.med-ph)
subject: Tissues and Organs (q-bio.TO)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: In this paper, the objective is to assess the histomechanical effects of collagen proteolysis in arteries under loading conditions reproducing in vivo environment. Thirteen segments of common porcine carotid arteries (8 proximal and 5 distal) were immersed in a bath of bacterial collagenase and tested with a pulsatile tension/inflation machine. Diameter, pressure and axial load were monitored throughout the tests and used to derive the stress-stretch curves and to determine the secant circumferential stiffness. Results were analyzed separately for proximal and distal segments, before and after 1, 2 and 3 hours of enzymatic degradation. A histological analysis was performed to relate the arterial microstructure to its mechanical behavior under collagen proteolysis. Control (before enzymatic degradation) and treated populations (after 1, 2 or 3 hours of enzymatic degradation) were found statistically incomparable, and histology confirmed the alteration of the fibrous structure of collagen bundles induced by the collagenase treatment. A decrease of the secant circumferential stiffness of the arterial wall was noticed mostly at the beginning of the treatment, and was less pronounced after 1 hour. These results constitute an important set of enzymatically damaged arteries that can be used to validate biomechanical computational models correlating structure and properties of blood vessels.
Reconstructing Three-dimensional Structure of Underlying Triaxial Dark Halos From Xray and Sunyaev-Zel'dovich Effect Observations of Galaxy Clusters
Creators: name: Lee, Jounghun
name: Suto, Yasushi
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: While the use of galaxy clusters as {\it tools} to probe cosmology is established, their conventional description still relies on the spherical and/or isothermal models that were proposed more than 20 years ago. We present, instead, a deprojection method to extract their intrinsic properties from X-ray and Sunyaev--Zel'dovich effect observations in order to improve our understanding of cluster physics. First we develop a theoretical model for the intra-cluster gas in hydrostatic equilibrium in a triaxial dark matter halo with a constant axis ratio. In this theoretical model, the gas density profiles are expressed in terms of the intrinsic properties of the dark matter halos. Then, we incorporate the projection effect into the gas profiles, and show that the gas surface brightness profiles are expressed in terms of the eccentricities and the orientation angles of the dark halos. For the practical purpose of our theoretical model, we provide several empirical fitting formulae for the gas density and temperature profiles, and also for the surface brightness profiles relevant to X-ray and Sunyaev--Zel'dovich effect observations. Finally, we construct a numerical algorithm to determine the halo eccentricities and orientation angles using our model, and demonstrate that it is possible in principle to reconstruct the 3D structures of the dark halos from the X-ray and/or Sunyaev-Zel'dovich effect cluster data alone without requiring priors such as weak lensing informations and without relying on such restrictive assumptions as the halo axial symmetry about the line-of-sight.
description: Accepted version, new discussions added, typos and minor mistakes corrected, ApJ in press (2004, Feb. 1 scheduled, Vol. 601, No. 2 issue),26 pages, 7 postscript figures
Anurophorus massoudi Poinsot 1970
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Entomobryomorpha
Isotomidae
Anurophorus
Anurophorus massoudi

description: Anurophorus massoudi Poinsot, 1970
Anurophorus massoudi Poinsot, 1970: 23.
DISTRIBUTION. — Var. Mont des Oiseaux près de Carqueiranne et au Col de Babaou dans les Maures (Poinsot 1970). — Poinsot- Balaguer & Kabakibi 1987.
ÉCOLOGIE. — Poinsot-Balaguer & Kabakibi 1987.
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 348, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
Additional file 1 of Application of artificial intelligence in a real-world research for predicting the risk of liver metastasis in T1 colorectal cancer
Creators: name: Han, Tenghui
name: Zhu, Jun
name: Chen, Xiaoping
name: Chen, Rujie
name: Jiang, Yu
name: Wang, Shuai
name: Xu, Dong
name: Shen, Gang
name: Zheng, Jianyong
name: Xu, Chunsheng
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Hematology

description: Additional file 1: Table S1. Normalization standards of clinical data in outer validation set.