cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Kongsbergia (Kongsbergia) ruttneri Walter 1930
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Aturidae
Kongsbergia
Kongsbergia ruttneri

description: Kongsbergia (Kongsbergia) ruttneri Walter, 1930
 Kongsbergia ruttneri Walter, 1930: Mota¸s 1928e: 31, 1928f: 243 (as nomen nudum); Schwoerbel 1962e: 256, 1965: 477; M.-L. Angelier 1980: 14; E. Angelier et al. 1985: 31.
 New record: Puy-de-Dôme: 1/0/0, La Planchette at Jassat, 45°33.716 N 2°56.339 E, alt. 894 m a.s.l., 20 May 2005, leg. H. Smit.
Distribution in France: Haut-Rhin, IsŁre, Puyde-Dôme, PyrØnØes (Hautes-PyrØnØes), Vosges.
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 71, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Characterising the complex absorber in NGC 4151
Creators: name: Schurch, N. J.
name: Warwick, R. S.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a detailed analysis of the complex absorption apparent in the 2-6 keV X-ray spectrum of the bright nearby Seyfert galaxy NGC 4151. We first utilize the large bandpass and medium spectral resolution afforded by BeppoSAX data to construct a 1-100 keV spectral template, which assumes the absorption arises in both warm (i.e. partially photoionized) and cold gas present in the line of sight to the active nucleus of the source. Application of this spectral model to an ASCA "long-look" observation of NGC 4151 reveals a partial correlation between the underlying continuum flux and the ionization state of the warm absorber. Such a correlation is an intrinsic property of a warm absorber and argues strongly in favour of this interpretation for the complex absorbing column over alternative partial covering models. The inferred relatively low density for the warm gas, implies an equilibration timescale for the dominant ions of the same order or longer than the timescale of the continuum variability. It follows that the warm component will invariably be observed in a non-equilibrium ionization state. We also find that (i) the reported hardening of the spectrum of NGC 4151 as the continuum level falls may be simply due to the presence of an underlying (hard and relatively constant) Compton-reflection component and (ii) the iron Ka line has a relatively narrow Gaussian profile and a line flux that remains constant over both short (days) and long (months to years) timescales - a relativistically broadened iron Ka feature was not required in our modelling.
description: 9 pages, 9 figures (8 colour), 2 tables. Accepted for publication in MNRAS. Updated Zdziarski et al 2002 reference
Hydrogen Emission in Type II White-light Solar Flares
Creators: name: Procházka, Ondřej
name: Reid, Aaron
name: Mathioudakis, Mihalis
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Type II WLFs have weak Balmer line emission and no Balmer jump. We carried out a set of radiative hydrodynamic simulations to understand how the hydrogen radiative losses vary with the electron beam parameters and more specifically with the low energy cutoff. Our results have revealed that for low energy beams, the excess flare Lyman emission diminishes with increasing low energy cutoff as the energy deposited into the top chromosphere is low compared to the energy deposited into the deeper layers. Some Balmer excess emission is always present and is driven primarily by direct heating from the beam with a minor contribution from Lyman continuum backwarming. The absence of Lyman excess emission in electron beam models with high low energy cutoff is a prominent spectral signature of type II WLFs.
description: 7 pages
Interaction-induced charge transfer in a mesoscopic electron spectrometer
Creators: name: Fischer, Stefan G.
name: Park, Jinhong
name: Meir, Yigal
name: Gefen, Yuval
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: A novel mesoscopic electron spectrometer allows for the probing of relaxation processes in quantum Hall edge channels. The device is composed of an emitter quantum dot that injects energy-resolved electrons into the channel closest to the sample edge, to be subsequently probed downstream by a detector quantum dot of the same type. In addition to inelastic processes in the sample that stem from interactions inside the region between the quantum dot energy filters (inner region), anomalous signals are measured when the detector energy exceeds the emitter energy. Considering finite range Coulomb interactions in the sample, we find that energy exchange between electrons in the current inducing source channel and the inner region, similar to Auger recombination processes, is responsible for such anomalous currents. In addition, our perturbative treatment of interactions shows that electrons emitted from the source, which dissipate energy to the inner region before entering the detector, contribute to the current most strongly when emitter-detector energies are comparable. Charge transfer in which the emitted electron is exchanged for a charge carrier from the Fermi sea, on the other hand, preferentially occurs close to the Fermi level.
Cosmic Reionization and Galaxy Formation
Creators: name: Umemura, M.
name: Nakamoto, T.
name: Susa, H.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using 3D radiative transfer calculations on the reionization of an inhomogeneous universe, QSO absorption line systems are simulated and they are compared with observations of Ly$α$ continuum depression at high redshifts. By this comparison, it is found that the metagalactic UV intensity decreases rapidly with $z$ at $z>4$ as $I_{21}=0.5\exp [3(4-z)]$, and the reionization must have taken place between $z=6$ and 10. Based on this time-dependence of UV background intensity, we explore the collapse of pregalactic clouds in the UV background, and find that the self-shielding is prominent above a mass scale as $ M_{BIF}=3.0\times 10^{11} M_\odot [(1+z_c)/5]^{-4.2}(I_{21}/0.5)^{0.6}. $ This mass scale predicts the bifurcation of galactic morphology, and by confrontation with observations it turns out that the bifurcation mass successfully discriminates between elliptical and spiral galaxies.
description: A paper in "The Physics of Galaxy Formation", ASP Conf. Ser. 222, Eds. M. Umemura and H. Susa (ASP: San Francisco), pp.109-114
Pseudoneureclipsis zemarit Malicky 2009, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Polycentropodidae
Pseudoneureclipsis
Pseudoneureclipsis zemarit

description: Pseudoneureclipsis zemarit nov.sp. (Tafel 3)
Dunkelbraun, VFL 6,5 mm. KA: 9. Segment in LA als Ganzes birnförmig, dorsal zwar viel schmäler, aber nicht auf eine Spange reduziert. OA in LA annähernd quadratisch, aber mit einer langen, nach innen und oben abstehenden Spitze. Mittellappen rechteckig. Die Mittelplatte besteht aus zwei sehr langen, dünnen, spitzen Stäben, die nach oben und hinten gerichtet sind und OA und Mittellappen weit überragen. 1. Glied der UA in LA schmal und mässig lang, in VA fast rechteckig. Das 2. Glied entspringt aus einer sehr langen Basis, die mehr als die Hälfte des Dorsalrandes des 1. Glieds einnimmt, ist unregelmässig geformt (siehe Zeichnung) und ebenso gross wie das erste. Der PA hat ventral, aus seiner Hälfte entspringend, eine sehr grosse, sklerotisierte, nach hinten weisende Spitze, die fast bis zu seinem Ende reicht. – Ich kenne keine ähnliche Art, denn mit dem besonders geformten 2. Glied der UA und dem riesigen Ventraldorn des PA ist sie einzigartig.
HT 3: Nord-Sumatra, ohne genauen Fundort, leg. Diehl.
description: Published as part of Malicky, H., 2009, Übersicht über die Gattung Pseudoneureclipsis (Trichoptera, Polycentropodidae), mit Beschreibung von neuen Arten, pp. 709-735 in Linzer biologische Beiträge 41 (1) on pages 716-717, DOI: 10.5281/zenodo.5276259
Pan-African structural evolution of Paleoproterozoic basement gneiss and Cu-Co mineralized shear zones in the Domes Region of the Lufilian Belt, Mwombezhi Dome, Zambia
Creators: name: Lupapulo, Hastings
Publisher: name: figshare
Year: 2019
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: A B S T R A C TIn the Domes Region of the Lufillian Belt, world-class stratiform Cu (±Co,±Ni,±U,±Pb,±Zn) deposits areclosely associated with tectonized pre-existing basement unconformities, viz. the pre-Katanga-basementdécollement (KD). In the KD footwall on the Mwombezhi Dome, the Lumwana Mine exploits mineralizationwithin<60m thick, laterally-extensive shear zones beneath kilometer-scale thrust sheets of Paleoproterozoicgneiss and schist. New field data and structural analysis highlight preferential strain localization, kinematics andsequential reactivation of multiple shear zone generations (D1-3) under high- to medium-grade, metamorphicconditions and clockwise P-T-t path during the Lufillian Orogeny (ca. 550-500). Regional, progressive, top-tothe-NNE fore-thrusting is assigned to D1, while D2 represents localized, opposite, top-to-the-SSW kinematicsattributed to under-thrusting by dome-scale fore-thrusted basement slivers. Subsequent D3 shear zones transposedD1-2 structures and represent overall top-to-the-NNE extensional detachment and NNE-SSW-elongationalong a maximum principal extension axis (L3) which defines kilometer-scale shear- or asymmetrical-boudins ofcompetent gneiss in the KD footwall. A pre-existing NNE-SSW prolate dome asymmetry (L1-2) dictates adownlimb-directed sense of shear on the short axes of D3 asymmetrical boudins (WNW-ESE). D3 shear zones arepreferentially localized along relict pre-Katanga anisotropy and D1-2 mylonitic horizons, while Cu–Co bearingore shoots are associated with passive fold hinges in these asymmetrical boudin necks.
Weak symmetries of stochastic differential equations driven by semimartingales with jumps
Creators: name: Albeverio, Sergio
name: De Vecchi, Francesco C.
name: Morando, Paola
name: Ugolini, Stefania
Publisher: name: arXiv
Year: 2019
Subjects: subject: Probability (math.PR)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 60H10, 60G45, 58D19

description: Stochastic symmetries and related invariance properties of finite dimensional SDEs driven by general cadlag semimartingales taking values in Lie groups are defined and investigated. The considered set of SDEs, first introduced by S. Cohen, includes affine and Marcus type SDEs as well as smooth SDEs driven by Levy processes and iterated random maps. A natural extension to this general setting of reduction and reconstruction theory for symmetric SDEs is provided. Our theorems imply as special cases non trivial invariance results concerning a class of affine iterated random maps as well as symmetries for numerical schemes (of Euler and Milstein type) for Brownian motion driven SDEs.
description: arXiv admin note: substantial text overlap with arXiv:1708.01764
Equivalent forms of the Bessis-Moussa-Villani conjecture
Creators: name: Lieb, Elliott H.
name: Seiringer, Robert
Publisher: name: arXiv
Year: 2002
Subjects: subject: Mathematical Physics (math-ph)
subject: General Mathematics (math.GM)
subject: Rings and Algebras (math.RA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: The BMV conjecture for traces, which states that $Tr exp(A -λB)$ is the Laplace transform of a positive measure, is shown to be equivalent to two other statements: (i) The polynomial $λ\mapsto Tr(A+λB)^p$ has only non-negative coefficients for all $A, B \geq 0$, $p\in N$ and (ii) $λ\mapsto \Tr (A+λB)^{-p}$ is the Laplace transform of a positive measure for $A, B \geq 0$, $p>0$.
description: LaTeX2e, 6 pages; additional explanations and dedication added; add. reference added
Pseudoneureclipsis sobak MALICKY & CHANTARAMONGKOL 2009, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Polycentropodidae
Pseudoneureclipsis
Pseudoneureclipsis sobak

description: Pseudoneureclipsis sobak MALICKY & CHANTARAMONGKOL nov.sp. (Tafel 5)
VFL 4–5 mm. KA: 9. Segment in LA ventral breiter, dann stark verschmälert, mit einem nach hinten vorstehenden Winkel und dann auf eine schmale Spange reduziert. OA in LA rundlich, Mittellappen stumpf dreieckig. Mittelplatte als zwei stumpfe Finger ausgebildet. UA lang und schlank, in LA kahnförmig, in VA schlank und fast parallelrandig, mit einer kleinen, aber deutlichen subdistalen Ausnehmung der Innenkante. 2. Glied mit einer besonders langen Basis, die 2/3 der Dorsalkante des 1. Glieds einnimmt, und einer nur sehr kurzen Kralle; basal von dieser ist eine grosse, bauchige Struktur vorhanden. PA mit vielen feinen Dörnchen im Endteil. – Mit der angeschwollenen Form des 2. Glieds der UA ist die Art gut charakterisiert.
HT 3 und viele 3 PT: Thailand, Prov. Kanchanaburi, Erawan NP, 200m, 14°22‘N, 99°08‘E, 22.- 24.4.200 1.
description: Published as part of Malicky, H., 2009, Übersicht über die Gattung Pseudoneureclipsis (Trichoptera, Polycentropodidae), mit Beschreibung von neuen Arten, pp. 709-735 in Linzer biologische Beiträge 41 (1) on pages 717-718, DOI: 10.5281/zenodo.5276259
Enantioselective synthesis of spiro[4H-pyran-3,3′-oxindole] derivatives catalyzed by cinchona alkaloid thioureas: Significant water effects on the enantioselectivity
Creators: name: Konda, Swapna
name: Jakkampudi, Satish
name: Arman, Hadi D.
name: Zhao, John C.-G.
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: An efficient stereoselective three-component reaction for the synthesis of functionalized spiro[4H-pyran-3,3′-oxindole] derivatives was realized through an organocatalyzed domino Knoevenagel/Michael/cyclization reaction using a cinchonidine-derived thiourea as the catalyst. Using water as the additive was found to improve the product ee values significantly. Under the optimized conditions, the reactions between isatins, malononitrile, and 1,3-dicarbonyl compounds yield the desired spirooxindole products in good yields (71–92%) and moderate to high ee values (up to 87% ee).
Ljania macilenta Koenike 1908
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Aturidae
Ljania
Ljania macilenta

description: Ljania macilenta Koenike, 1908
 Ljania macilenta Koenike, 1908: Mota¸s 1927b: 3, 1928e: 17, 1928f: 225, 1928g: 30.
 New records. ArdŁche: 0/1/0, La Drobie RiviŁre, upstream of SabliŁres, 44°32.256 N 4°03.364 S, leg. H. Smit. Cantal: 0/1/0, Jordanne RiviŁre at Mandailles-Saint Julien, 45°04.225 N 2°39.510 E, alt. 927 m a.s.l., 927 m a.s.l., leg. H. Smit. Gard: 0/1/0, l’HØrault 3 km upstream of Valleraugue, 44°05.190 N 3°36.475 E, alt. 405 m a.s.l., 15 May 2005, leg. H. Smit.
Distribution in France: ArdŁche, Cantal, Gard, IsŁre, Puy-de-Dôme.
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 72, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Coexistence of metallic and nonmetallic properties in the pyrochlore Lu$_2$Rh$_2$O$_7$
Creators: name: Hallas, Alannah M.
name: Sharma, Arzoo Z.
name: Mauws, Cole
name: Chen, Qiang
name: Zhou, Haidong D.
name: Ding, Cui
name: Gong, Zizhou
name: Tachibana, Makoto
name: Sarte, Paul M.
name: Attfield, J. Paul
name: Luke, Graeme M.
name: Wiebe, Christopher R.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Transition metal oxides of the $4d$ and $5d$ block have recently become the targets of materials discovery, largely due to their strong spin-orbit coupling that can generate exotic magnetic and electronic states. Here we report the high pressure synthesis of Lu$_2$Rh$_2$O$_7$, a new cubic pyrochlore oxide based on $4d^5$ Rh$^{4+}$ and characterizations via thermodynamic, electrical transport, and muon spin relaxation measurements. Magnetic susceptibility measurements reveal a large temperature-independent Pauli paramagnetic contribution, while heat capacity shows an enhanced Sommerfeld coefficient, $γ$ = 21.8(1) mJ/mol-Rh K$^2$. Muon spin relaxation measurements confirm that Lu$_2$Rh$_2$O$_7$ remains paramagnetic down to 2 K. Taken in combination, these three measurements suggest that Lu$_2$Rh$_2$O$_7$ is a correlated paramagnetic metal with a Wilson ratio of $R_W = 2.5$. However, electric transport measurements present a striking contradiction as the resistivity of Lu$_2$Rh$_2$O$_7$ is observed to monotonically increase with decreasing temperature, indicative of a nonmetallic state. Furthermore, although the magnitude of the resistivity is that of a semiconductor, the temperature dependence does not obey any conventional form. Thus, we propose that Lu$_2$Rh$_2$O$_7$ may belong to the same novel class of non-Fermi liquids as the nonmetallic metal FeCrAs.
description: 11 pages, 5 figures
Mapping the submillimeter spiral wave in NGC 6946
Creators: name: Alton, P. B.
name: Bianchi, S.
name: Richer, J.
name: Pierce-Price, D.
name: Combes, F.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have analysed SCUBA 850\mum images of the (near) face-on spiral galaxy NGC 6946, and found a tight correlation between dust thermal emission and molecular gas. The map of visual optical depth relates well to the distribution of neutral gas (HI+H2) and implies a global gas-to-dust ratio of 90. There is no significant radial variation of this ratio: this can be understood, since the gas content is dominated by far by the molecular gas. The latter is estimated through the CO emission tracer, which is itself dependent on metallicity, similarly to dust emission. By comparing the radial profile of our visual optical depth map with that of the SCUBA image, we infer an emissivity (dust absorption coefficient) at 850\mum that is 3 times lower than the value measured by COBE in the Milky Way, and 9 times lower than in NGC 891. A decomposition of the spiral structure half way out along the disk of NGC 6946 suggests an interarm optical depth of between 1 and 2. These surprisingly high values represent 40-80% of the visual opacity that we measure for the arm region (abridged).
description: 12 pages, 9 figures, accepted in A&A
Additional file 4 of Associations between the morphological parameters of proximal tibiofibular joint (PTFJ) and changes in tibiofemoral joint structures in patients with knee osteoarthritis
Creators: name: Chang, Jun
name: Chen, Tianyu
name: Yan, Yizhu
name: Zhu, Zhaohua
name: Han, Weiyu
name: Zhao, Yi
name: Antony, Benny
name: Wluka, Anita
name: Winzenberg, Tania
name: Cicuttini, Flavia
name: Ding, Changhai
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 4: Table S4. Longitudinal associations between the morphological parameters of PTFJ and increases in tibiofemoral BMLs.
The politics of patronage : Israel and Egypt between the superpowers 1962-1973
Creators: name: Indyk, Martin
Publisher: name: The Australian National University
Year: 1977

description: This thesis is a study of the interaction between two weak states and their superpower patrons through the application of a theoretical analysis of the 'power of the weak' to the study of the political and military conduct of relations between Israel, Egypt, the United States and the Soviet Union in the period from 1962 to 1973. The thesis establishes some of the conditions under which lesser powers, engaged in a protracted conflict and dependent upon the military, economic and political support of the superpowers, could nevertheless resist and thereby influence the policies of their patrons. ii In the Arab-Israeli context, the thesis examines the effect that the politics of patronage have had on the conduct and settlement of the conflict and analyses the successes and failures of Israeli and Egyptian diplomacy in securing the support of their superpower patrons while resisting the imposition of an order inimical to their own interests.
Semantics of HTS AC loss modelling: Theories, models and experiments
Creators: name: Lahtinen, Valtteri
name: Stenvall, Antti
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: Computer-assisted modelling is an essential approach to design new devices. It speeds up the process from the initial idea to an actual device and saves resources by reducing the number of built prototypes. This is also a significant practical motivator behind scientific research in contemporary high-temperature superconductor (HTS) AC loss modelling. However, in the scientific literature in this field, consistent practices about modelling terminology have not been established. Then, it is up to the reader to decide, what is the true intent and meaning of the authors. Consequently, the interpretation of such literature might be very much reader-dependent. Moreover, an inseparable part of the whole modelling process is the development of modelling approaches and numerical methods and comparing the predictions obtained via modelling to experimentally achieved results: It is commonplace to discuss the accuracy of modelling results or the validation of a model. In this paper, we discuss the terminology related to theories, models and experiments in the context of HTS AC loss modelling. We discuss the recursive nature of theories and models in this context, discuss the compatibility of discrete formulations of physics utilized in our field with the corresponding continuum descriptions, as well as with intuition, and interpret the perceived meaning of validation of a self-consistent model, shedding light on the relationships between theories, models and measurements. We present our view on understanding these relations in the familiar context of AC losses in HTS. As a result, we end this paper with four conjectures describing our views.
description: Presented at the Sixth International Workshop on Numerical Modelling of HTS held in Caparica, Portugal, 26-29 June 2018
Momonia falcipalpis Halbert 1911
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Momoniidae
Momonia
Momonia falcipalpis

description: Momonia falcipalpis Halbert, 1911
 Momonia falcipalpis Halbert, 1911: LØger & Mota¸s 1928a: 176; Mota¸s 1927f: 321, 1928f: 211, 1928g: 7; Smit et al. 2000: 203.
Distribution in France: PyrØnØes-Atlantiques, Var.
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 73, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Pseudoneureclipsis bonaventura Malicky 2009, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Polycentropodidae
Pseudoneureclipsis
Pseudoneureclipsis bonaventura

description: Pseudoneureclipsis bonaventura nov.sp. (Tafel 5)
Braun, VFL 4 mm. KA: 9. Segment in LA ventral breit, dann rasch verschmälert; die dorsale schmale Spange entspringt in einem rechten Winkel. OA in LA fast kreisrund, am Hinterrand mit groben Dornen besetzt. Mittellappen kurz, dreilappig. Mittelplatte aus zwei kurzen Fingern bestehend, die distal starke Dornen tragen. UA lang und schlank, in LA leicht s-förmig, in VA parallelrandig mit ziemlich spitzem Ende. Dorsalkralle (2. Glied) aus sehr langer Basis nur kurz nach unten gebogen, bis ungefähr zur Mitte des 1. Glieds reichend. PA im Endteil mit einem Paar Stäbe; daneben verläuft beiderseits eine schmale, stumpfe Leiste. Um die Mitte des PA herum verläuft ein häutiges Band, das mit feinen Dörnchen besetzt ist. Unter den vielen Arten mit so langen, schlanken UA fällt diese vor allem durch das dörnchenbesetzte Band um den PA auf.
HT 3 und 1 3 PT: Indien (C.), Bandarkhal, 9.5.196 0, leg. F. Schmid, coll. CNC.
description: Published as part of Malicky, H., 2009, Übersicht über die Gattung Pseudoneureclipsis (Trichoptera, Polycentropodidae), mit Beschreibung von neuen Arten, pp. 709-735 in Linzer biologische Beiträge 41 (1) on page 718, DOI: 10.5281/zenodo.5276259
SI Appendix and Raw Data for Manuscript: Staphylococcus aureus exhibits heterogeneous siderophore production within the vertebrate host
Creators: name: Perry, William
name: Spraggins, Jeffrey
name: Sheldon, Jessica R.
name: Grunenwald, Caroline M.
name: Heinrichs, David E.
name: Cassat, James E.
name: Skaar, Eric P.
name: Caprioli, Richard M.
Publisher: name: figshare
Year: 2019
Subjects: subject: 60101 Analytical Biochemistry
subject: FOS: Biological sciences
subject: Microbiology
subject: Molecular Biology

description: Siderophores, iron scavenging small molecules, are fundamental to bacterial nutrient metal acquisition and enable pathogens to overcome challenges imposed by nutritional immunity. Multimodal imaging mass spectrometry allows visualization of host-pathogen iron competition by mapping siderophores within infected tissue. We have observed heterogeneous distributions of Staphylococcus aureus siderophores across infectious foci, challenging the paradigm that the vertebrate host is a uniformly iron deplete environment to invading microbes. The attached file includes methodological information in the acquisition of data as well as supplemental data.
Signatures of resonance and phase mixing in the Galactic disc
Creators: name: Hunt, Jason A. S.
name: Bub, Mathew W.
name: Bovy, Jo
name: Mackereth, J. Ted
name: Trick, Wilma H.
name: Kawata, Daisuke
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Gaia DR2 has provided an unprecedented wealth of information about the kinematics of stars in the Solar neighbourhood, and has highlighted the degree of features in the Galactic disc. We confront the data with a range of bar and spiral models in both action-angle space, and the $R_{\mathrm{G}}-v_ϕ$ plane. We find that the phase mixing induced by transient spiral structure creates ridges and arches in the local kinematics which are consistent with the Gaia data. We are able to produce a qualitatively good match to the data when combined with a bar with a variety of pattern speeds, and show that it is non trivial to decouple the effects of the bar and the spiral structure.
description: 18 pages, 15 figures, submitted to MNRAS
Towards a model of educational outcomes : investigations with Australian and Filipino students
Creators: name: Watkins, David Arthur
Publisher: name: The Australian National University
Year: 1983

description: The research described in the papers summarised above is multifaceted necessarily so, since its “object”, learning processes and outcome, is complexly governed by a large number of variables. Serious research in this area involves the initial determination of the relevant factors, the resolution of problems relating to the measurement of these variables, the formulation of a theoretical model to guide empirical work on the relationships and/or interactions between the selected variables and the actual empirical testing of hypotheses generated by the model. In the present case, the research results led to refinements of the model, rendering the investigation even more complex. A further complicating dimension was added to the present research by its investigation of the cross-cultural applicability of concepts and variables derived from western theory and research. Such cross-cultural work is deemed essential to the development of a general model of human learning in the educational context.
Neoacarus hibernicus Halbert 1944
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Neoacaridae
Neoacarus
Neoacarus hibernicus

description: Neoacarus hibernicus Halbert, 1944
 Neoacarus hibernicus Halbert, 1944: E. Angelier et al. 1963: 462; Schwoerbel 1962e: 256, 1965: 477.
 New record. Var: 1/0/0, unnamed creek, Massif des Maures, 43°15.312 N 6°23.954 E, 5 May 2003, leg. H. Smit.
Distribution in France: Haut-Rhin, Tarn, Var.
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 74, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Anomalous X-ray Pulsars and Soft Gamma-Ray Repeaters in supernova remnants
Creators: name: Gaensler, B. M.
name: Slane, P. O.
name: Gotthelf, E. V.
name: Vasisht, G.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Important constraints on the properties of the Anomalous X-ray Pulsars (AXPs) and Soft Gamma-Ray Repeaters (SGRs) can be provided by their associations with supernova remnants (SNRs). We have made a radio search for SNRs towards the AXPs RX J170849-400910 and 4U 0142+61 - we find that the former lies near a possible new SNR with which it is unlikely to be physically associated, but see no SNR in the vicinity of the latter. We review all claimed pairings between AXPs and SNRs; the three convincing associations imply that AXPs are young (< 10 000 yr) neutron stars with low projected space velocities (< 500 km/s). Contrary to previous claims, we find no evidence that the density of the ambient medium around AXPs is higher than that in the vicinity of radio pulsars. Furthermore, the non-detection of radio emission from AXPs does not imply that these sources are radio-silent. We also review claimed associations between SGRs and SNRs. We find none of these associations to be convincing, consistent with a scenario in which SGRs and AXPs are both populations of high-field neutron stars ("magnetars") but in which the SGRs are an older or longer-lived group of objects than are the AXPs. If the SGR/SNR associations are shown to be valid, then SGRs must be high-velocity objects and most likely represent a different class of source to the AXPs.
description: 13 pages, 3 embedded EPS figures. Minor alterations following referee's report; no significant changes. Accepted to ApJ
Resolving gravitational microlensing events with long-baseline optical interferometry. Prospects for the ESO Very Large Telescope Interferometer
Creators: name: Delplancke, F.
name: Gorski, K. M.
name: Richichi, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Until now, the detailed interpretation of the observed microlensing events has suffered from the fact that the physical parameters of the phenomenon cannot be uniquely determined from the available astronomical measurements, i.e. the photometric lightcurves. The situation will change in the near-future with the availability of long-baseline, sensitive optical interferometers, which should be able to resolve the images of the lensed objects into their components. For this, it will be necessary to achieve a milliarcsecond resolution on sources with typical magnitudes K $\ga 12$. Indeed, brighter events have never been observed up to now by micro-lensing surveys. We discuss the possibilities opened by the use of long baseline interferometry in general, and in particular for one such facility, the ESO VLT Interferometer, which will attain the required performance. We discuss the expected accuracy and limiting magnitude of such measurements. On the basis of the database of the events detected by the OGLE experiment, we estimate the number of microlenses that could be available for measurements by the VLTI. We find that at least several tens of events could be observed each year. In conjunction with the photometric data, our ability to measure the angular separation between the microlensed images will enable a direct and unambiguous determination of both their masses and locations.
description: Accepted for publication in Astronomy & Astrophysics
The development of the story of Tuladhara in the Mahabharata with reference to the ideal of non-violence
Creators: name: Proudfoot, Ian MacLeod
Publisher: name: The Australian National University
Year: 1977

description: The history of a conception like ahimsa presents problems of interpretation which can best be overcome by analysing a self-consciously developed tradition which embodies changing or differing views. The Mahabharata comprises such material, but it cannot be validly employed unless segmented on grounds extrinsic to the issue under examination. Taking the story of Tuladhara (Hbh.xii.252-257) as a paradigm, a segmentation of the material on internal formal evidence proves feasible, from the analysis of that material conclusions are drawn concerning the character and history of the Moksadharma text tradition from a consideration of the material segmented into its historically separate components, light is cast upon some aspects of the evolution of the ideal of ahimsa, The analysis discusses the implications of the trader hero as an embodiment of disinterested non-involvement, and the association of the ideal of ahimsa with altruistic reciprocity, with bralumanic disputes over the proper form of the sacrifice, and with the virtue of cow-protection.
Bose-Einstein Condensation of Dilute Gases in Traps
Creators: name: Lieb, Elliott H.
name: Seiringer, Robert
Publisher: name: arXiv
Year: 2002
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The ground state of a gas of Bosons confined in an external trap potential and interacting via repulsive two-body forces has recently been shown to exhibit complete Bose-Einstein condensation in the dilute limit, yielding for the first time a rigorous proof of this phenomenon in a physically realistic setting. We give here an account of this work about the Gross-Pitaevskii limit where the particle number $N$ goes to infinity with $Na$ fixed, where $a$ is the scattering length of the interparticle interaction, measured in units of the trap size.
description: To appear in the proceedings of the UAB2002 conference at Birmingham, Alabama
Further advantages of data augmentation on convolutional neural networks
Creators: name: Hernández-García, Alex
name: König, Peter
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Data augmentation is a popular technique largely used to enhance the training of convolutional neural networks. Although many of its benefits are well known by deep learning researchers and practitioners, its implicit regularization effects, as compared to popular explicit regularization techniques, such as weight decay and dropout, remain largely unstudied. As a matter of fact, convolutional neural networks for image object classification are typically trained with both data augmentation and explicit regularization, assuming the benefits of all techniques are complementary. In this paper, we systematically analyze these techniques through ablation studies of different network architectures trained with different amounts of training data. Our results unveil a largely ignored advantage of data augmentation: networks trained with just data augmentation more easily adapt to different architectures and amount of training data, as opposed to weight decay and dropout, which require specific fine-tuning of their hyperparameters.
description: Preprint of the manuscript accepted for presentation at the International Conference on Artificial Neural Networks (ICANN) 2018. Best Paper Award
Additional file 1 of A novel DNA methylation-related gene signature for the prediction of overall survival and immune characteristics of ovarian cancer patients
Creators: name: Wang, Sixue
name: Fu, Jie
name: Fang, Xiaoling
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1:  Fig. S1. The relationship between the expression levels of the 36 DNA methylation-related genes and DNA methylation levels in OC patients. Fig. S2. Differential expression status and survival analyses of the 12 DNA methylation-related genes. Fig. S3. Validation of the differential expression status of these 12 genes in OC tumor tissues and adjacent normal tissues of our center. Fig. S4. Immune analysis between the high- and low-risk groups.Table S1. Clinicopathological features of the TCGA-OC patients. Table S2. Univariate and multivariate Cox analyses of the 36 DNA methylation-related genes. Table S3. List of the 12 prognostic genes and their corresponding risk coefficients. Table S4. The primer sequences used in this study. Table S5. Univariate and multivariate Cox analyses of the risk score and clinicopathological features. Table S6. Pearson correlation between drug IC50 and gene expression.
Fundamental Properties and Distances of LMC Eclipsing Binaries: III. EROS 1044
Creators: name: Ribas, Ignasi
name: Fitzpatrick, Edward L.
name: Maloney, Frank P.
name: Guinan, Edward F.
name: Udalski, Andrzej
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results from a detailed analysis of a third eclipsing binary (EB) system in the Large Magellanic Cloud, EROS 1044 (~B2 IV-V + ~B2 III-IV). Our study combines the "classical" EB study of light and radial velocity curves with detailed modeling of the observed spectral energy distribution, and yields an essentially complete picture of the stellar properties of the system and a determination of its distance. The observational data exploited include optical photometry, space-based UV spectroscopy, and UV/optical spectrophotometry. The advantages of our technique include numerous consistency checks and, in the case of the distance determinations, the absence of zero point uncertainties and adjustable parameters. We find the EROS 1044 system to consist of a pair of normal, mildly-evolved ~21000 K stars, whose derived properties are consistent with stellar evolution calculations. The distance to the system is 47.5+/-1.8 kpc. We discuss the implications of our results for three EB systems (HV 2274, HV 982, and EROS 1044) on the general distance to the Large Magellanic Cloud.
description: 18 pages, 8 figures, accepted for publication in ApJ
Hungarohydracarus subterraneus Szalay 1943
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Hungarohydracaridae
Hungarohydracarus
Hungarohydracarus subterraneus

description: Hungarohydracarus subterraneus Szalay, 1943
 Hungarohydracarus subterraneus Szalay, 1943: E. Angelier 1953b: 58, 1959: 16, 1959a: 73; Santucci 1970: 193, 1971: 83; Smit et al. 2000: 212.
 Hungarohydracarus subterraneus multiporus E. Angelier, 1949a: 90, 1949b: 252.
Distribution in France: Corsica, IsŁre, PyrØnØes (PyrØnØes-Orientales).
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 74, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
SI Appendix for Manuscript: Staphylococcus aureus exhibits heterogeneous siderophore production within the vertebrate host
Creators: name: Perry, William
name: Spraggins, Jeffrey
name: Sheldon, Jessica R.
name: Grunenwald, Caroline M.
name: Heinrichs, David E.
name: Cassat, James E.
name: Skaar, Eric P.
name: Caprioli, Richard M.
Publisher: name: figshare
Year: 2019
Subjects: subject: 60101 Analytical Biochemistry
subject: FOS: Biological sciences
subject: Microbiology
subject: Molecular Biology

description: Siderophores, iron scavenging small molecules, are fundamental to bacterial nutrient metal acquisition and enable pathogens to overcome challenges imposed by nutritional immunity. Multimodal imaging mass spectrometry allows visualization of host-pathogen iron competition by mapping siderophores within infected tissue. We have observed heterogeneous distributions of Staphylococcus aureus siderophores across infectious foci, challenging the paradigm that the vertebrate host is a uniformly iron deplete environment to invading microbes. The attached file includes methodological information in the acquisition of data as well as supplemental data.
Pseudoneureclipsis thiras MALICKY & CHANTARAMONGKOL 2009, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Polycentropodidae
Pseudoneureclipsis
Pseudoneureclipsis thiras

description: Pseudoneureclipsis thiras MALICKY & CHANTARAMONGKOL nov.sp. (Tafel 7)
Braun, VFL 5–5,5 mm. KA: 9. Segment in LA im unteren Teil breit rundlich, im mittleren Drittel sehr schmal und im dorsalen Drittel, das rechtwinkelig abgeknickt ist, auf eine schmale Spange reduziert. Die OA haben eine schmal dreieckige Aussenplatte, von deren Basis innen ein viel längerer, spitzer Finger entspringt, der nach hinten gerichtet und länger als die UA ist. Der Mittellappen ist kurz und mit vielen langen borstentragenden Sockeln besetzt. Die Mittelplatte besteht aus einem Paar langer, dünner, distal zweispitziger Stäbe, die ebenfalls nach hinten gerichtet sind. UA kurz, 1. Glied in LA abgerundet dreieckig, in VA abgerundet rechteckig. 2. Glied (Dorsalkralle) aus kurzer Basis bis in ca. zwei Drittel des 1. Glieds reichend. PA im Endteil mit vielen feinen Börstchen. – Der Dorsalkomplex dieser Art ist so charakteristisch, dass keine ähnliche Art auszumachen war.
HT 3 und 13 PT: Thailand, Prov. Mae Hong Son, Paembok Wasserfall, 650m, 19°19‘N, 98°24‘E, 24.4.200 0. – 433 PT: Thailand, Prov. Mae Hong Son, Muang Pai Resort, 800m, 19°23‘N, 98°24‘E, 16.5.200 5. – 1133 PT: do., aber 10.- 27.4.2000.
description: Published as part of Malicky, H., 2009, Übersicht über die Gattung Pseudoneureclipsis (Trichoptera, Polycentropodidae), mit Beschreibung von neuen Arten, pp. 709-735 in Linzer biologische Beiträge 41 (1) on page 720, DOI: 10.5281/zenodo.5276259
Life at the Mughal court as revealed in contemporary paintings
Creators: name: Schonbaum, Anthony Pawlas
Publisher: name: The Australian National University
Year: 1977

description: Mughal history is a branch of Indian history which compels the full attention. In consequence of the Mughals' achievements, political, military, and artistic, their fabulous fame and wealth, 'Mughal' is not a mere name, but has grown into a concept, often and gladly quoted. Their history is never dull - from whatever angle it is examined and not just the military part of it - the empire-founding, the battles, the expansion and consolidation - but also its peacetime activities draw our full interest - its economic development - how it was built into a solid, mighty structure and especially its achievements in the field of fine arts and literature - reaching dizzying heights, from architecture and painting through to jewellery. But also of interest are the very personal activities of some of its rulers like Jahangir, the accounts of whose hunting parties vie with the best written adventure stories ever written. The accounts of Mughal court life with its magnificence, the dazzling colourfulness of its darbars, its receptions of famous visitors, and foreign ambassadors - even when it is most routine - are never boring; but there is the feeling that one has witnessed an unforgettable spectacular event.
Additional file 1 of Expanding hepatitis C virus test uptake using self-testing among men who have sex with men in China: two parallel randomized controlled trials
Creators: name: Wang, Cheng
name: Zhao, Peizhen
name: Weideman, Ann Marie
name: Xu, Wenqian
name: Ong, Jason J.
name: Jamil, Muhammad S.
name: Yang, Bin
name: Tucker, Joseph D.
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Chemical Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Mental Health

description: Additional file 1. Study protocol.
Dark energy and cosmic microwave background bispectrum
Creators: name: Verde, Licia
name: Spergel, David N.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compute the cosmic microwave background bispectrum arising from the cross-correlation of primordial, lensing and Rees-Sciama signals. The amplitude of the bispectrum signal is sensitive to the matter density parameter, Omega_0, and the equation of state of the dark energy, which we parameterize by w_Q. We conclude that the dataset of the Atacama Cosmology Telescope, combined with MAP 2-year data or the Planck data set alone will allow us to break the degeneracy between Omega_0 and w_Q that arises from the analysis of CMB power spectrum. In particular a joint measurement of Omega_0 and w_Q with 10% and 30% error on the two parameters respectively, at the 90% confidence level can realistically be achieved.
description: To appear in PRD, 6 pages, 3 figures, minor changes to match the accepted version
Distributional Borel Summability for Vacuum Polarization by an External Electric Field
Creators: name: Caliceti, Emanuela
Publisher: name: arXiv
Year: 2002
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: It is proved that the divergent perturbation expansion for the vacuum polarization by an external constant electric field in the pair production sector is Borel summable in the distributional sense.
description: 14 pages
A 168-s X-Ray Pulsar in the SMC Observed with ASCA
Creators: name: Yokogawa, Jun
name: Torii, Ken'ichi
name: Kohmura, Takayoshi
name: Koyama, Katsuji
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This paper has been withdrawn because the class file must not be uploaded.
description: 4 pages, 3 figures, to be published in PASJ. Also available at http://www-cr.scphys.kyoto-u.ac.jp/member/jun/job/