cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 3: of Factors influencing national implementation of innovations within community pharmacy: a systematic review applying the Consolidated Framework for Implementation Research
Creators: name: Weir, Natalie
name: Newham, Rosemary
name: Dunlop, Emma
name: Bennie, Marion
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Characteristics of included studies. (DOCX 69 kb)
Leopoldius valvatus Krober 1914
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Conopidae
Leopoldius
Leopoldius valvatus

description: Leopoldius valvatus Kröber, 1914. (Stuke & van Eck 2009).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Observations of the interstellar medium in the Magellanic Bridge
Creators: name: Lehner, N.
name: Sembach, K. R.
name: Dufton, P. L.
name: Rolleston, W. R. J.
name: Keenan, F. P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present ultraviolet and optical spectra of DI 1388, a young star in the Magellanic Bridge, a region of gas between the Small and Large Magellanic Clouds. The data have signal-to-noise ratios of 20 to 45 and a spectral resolution of 6.5 km/s. Interstellar absorption by the Magellanic Bridge at v_LSR = 200 km/s is visible in the lines of C I, C II,C II*, C IV, N I, O I, Al II, Si II, Si III, Si IV, S II, Ca II, Fe II, and Ni II. The relative gas-phase abundances of C II, N I, O I, Al II, Si II, Fe II, and Ni II with respect to S II are similar to those found in Galactic halo clouds, despite a significantly lower metallicity in the Magellanic Bridge. The higher ionization species in the cloud have a column density ratio N(C IV)/N(Si IV) about 1.9, similar to that inferred for collisionally ionized Galactic cloud interfaces at temperatures 10^5 K.We identify sub-structure in the stronger interstellar lines, with a broad component (FWHM = 20 km/s) at 179 km/s and a sharp component (FWHM = 11 km/s) at 198 km/s. The abundance analysis for these clouds indicates that the feature at 198 km/s consists of a low electron density, mainly neutral gas that may be associated with an interface responsible for the highly ionized gas. The 179 km/s cloud consists of warmer, lower density gas that is partially ionized.
description: Accepted for publication in ApJ (April 10, 2001). Minor corrections in Figures 1 and 3, and in references
Review: Marie Kawthar Daouda, L’Anti-Salomé: Représentations de la féminité bienveillante au temps de la Décadence (1850-1910) (Oxford: Peter Lang, 2020)
Creators: name: Burin, Alexandre
Publisher: name: Volupté
Year: 2021

description: Volupté, Vol 4 No 1 (2021): Ends of Worlds
Investigation of long-period variables in the Catalina Southern catalog: new carbon stars and false objects
Creators: name: Mauron, Nicolas
name: Gigoyan, Kamo S.
name: Gigoyan, Karen K.
name: Maurin, Luc P. A.
name: Kendall, Tim R.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: As part of our ongoing study of the evolved giants in the galactic halo, we consider the sample of 1286 long-period variables (LPVs) in the southern hemisphere provided by the Catalina Sky Survey experiment. These LPVs have periods P larger than 80 days and amplitudes over 0.2 mag. First, by using the Hamburg-ESO spectral survey, we aim to determine the spectral type as either M-type or C-type for objects located in the imprint of this survey, $|b| > 30$ degrees. Of 135 LPVs obeying this selection, we classified 93, and found only 2 new carbon stars. Secondly, we consider faint LPVs. We discovered that many lie at about 1 arcmin from a bright Mira catalogued in the General Catalog of Variable Stars, with identical period. We study these suspicious cases in detail, and conclude that, for as many as 56 faint Catalina LPVs, their variability is due to contamination by light from the bright, neighbouring GCVS Mira: an instrumental artefact. We conclude that when dealing with distant, faint Miras in the Catalina catalog, researchers should pay attention to the polluting effects of neighbouring bright and variable objects.
description: 8 pages, 4 figures, accepted to Astrophysics
Additional file 1: of Factors influencing national implementation of innovations within community pharmacy: a systematic review applying the Consolidated Framework for Implementation Research
Creators: name: Weir, Natalie
name: Newham, Rosemary
name: Dunlop, Emma
name: Bennie, Marion
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Medline search strategy. (DOCX 27 kb)
Myopa hirsuta Stuke & Clements 2008
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Conopidae
Myopa
Myopa hirsuta

description: Myopa hirsuta Stuke & Clements, 2008. (Stuke & Clements 2008).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
On the unimodality of convolutions of sequences of binomial coefficients
Creators: name: Brown, Tricia Muldoon
Publisher: name: arXiv
Year: 2018
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: We provide necessary and sufficient conditions on the unimodality of a convolution of two sequences of binomial coefficients preceded by a finite number of ones. These convolution sequences arise as as rank sequences of posets of vertex-induced subtrees for a particular class of trees. The number of such trees whose poset of vertex-induced subgraphs containing the root is not rank unimodal is determined for a fixed number of vertices $i$.
Myopa pellucida
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Conopidae
Myopa
Myopa pellucida

description: Myopa pellucida (Robineau-Desvoidy, 1830). (Stuke & Clements 2008).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Topological band structure of surface acoustic waves on a periodically corrugated surface
Creators: name: Inoue, Tomohiro
name: Murakami, Shuichi
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Surface acoustic waves (SAWs) are elastic waves localized on a surface of an elastic body. We theoretically study topological edge modes of SAWs for a corrugated surface. We introduce a corrugation forming a triangular lattice on the surface of an elastic body. We treat the corrugation as a perturbation, and construct eigenmodes on a corrugated surface by superposing those for the flat surface at wavevectors which are mutually different by reciprocal lattice vectors. We thereby show emergence of Dirac cones at the $K$ and $K'$ points analytically. Moreover, by breaking the time-reversal symmetry, we show that the Dirac cones open a gap, and that the Chern number for the lowest band has a nonzero value. It means existence of topological chiral edge modes of SAWs in the gap.
description: 14 pages, 7 figures
Vanishing of phase coherence in underdoped Bi_2Sr_2CaCu_2O_8+d
Creators: name: Corson, J.
name: Mallozzi, R.
name: Orenstein, J.
name: Eckstein, J. N.
name: Bozovic, I.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Coherent time-domain spectroscopy is used to measure the screening and dissipation of high-frequency electromagnetic fields in a set of underdoped Bi_2Sr_2CaCu_2O_8+d thin films. The measurements provide direct evidence for a phase-fluctuation driven transition from the superconductor to normal state, with dynamics described well by the Berezinskii-Kosterlitz-Thouless theory of vortex-pair unbinding.
description: Nature, Vol. 398, 18 March 1999, pg. 221 4 pages with 4 included figures
Sicus abdominalis Krober 1915
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Conopidae
Sicus
Sicus abdominalis

description: Sicus abdominalis Kröber, 1915. (Monnerat 2009).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Magnetically Accreting Isolated Old Neutron Stars
Creators: name: Rutledge, Robert E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Previous work on the emission from isolated old neutron stars (IONS) accreting the inter-stellar medium (ISM) focussed on gravitational capture - Bondi accretion. We propose a new class of sources which accrete via magnetic interaction with the ISM. While for the Bondi mechanism, the accretion rate decreases with increasing NS velocity, in magnetic accretors (MAGACs="magics") the accretion rate increases with increasing NS velocity. MAGACs will be produced among high velocity (~> 100 km s-1) high magnetic field (B> 1e14 G) radio pulsars - the ``magnetars'' - after they have evolved first through magnetic dipole spin-down, followed by a ``propeller'' phase (when the object sheds angular momentum on a timescale ~< 1e10 yr). The properties of MAGACS may be summarized thus: dipole magnetic fields of B~>1e14 G; minimum velocities relative to the ISM of >25-100 km s-1, depending on B, well below the median in the observed radio-pulsar population; spin-periods of >days to years; accretion luminosities of 1e28- 1e31 ergs s-1 ; and effective temperatures kT=0.3 - 2.5 keV if they accrete onto the magnetic polar cap. We find no examples of MAGACs among previously observed source classes (anomalous X-ray pulsars, soft-gamma-ray repeaters or known IONS). However, MAGACs may be more prevelant in flux-limited X-ray catalogs than their gravitationally accreting counterparts.
description: ApJ, accepted
Applying Deep Learning To Airbnb Search
Creators: name: Haldar, Malay
name: Abdool, Mustafa
name: Ramanathan, Prashant
name: Xu, Tao
name: Yang, Shulin
name: Duan, Huizhong
name: Zhang, Qing
name: Barrow-Williams, Nick
name: Turnbull, Bradley C.
name: Collins, Brendan M.
name: Legrand, Thomas
Publisher: name: arXiv
Year: 2018
Subjects: subject: Machine Learning (cs.LG)
subject: Artificial Intelligence (cs.AI)
subject: Information Retrieval (cs.IR)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: The application to search ranking is one of the biggest machine learning success stories at Airbnb. Much of the initial gains were driven by a gradient boosted decision tree model. The gains, however, plateaued over time. This paper discusses the work done in applying neural networks in an attempt to break out of that plateau. We present our perspective not with the intention of pushing the frontier of new modeling techniques. Instead, ours is a story of the elements we found useful in applying neural networks to a real life product. Deep learning was steep learning for us. To other teams embarking on similar journeys, we hope an account of our struggles and triumphs will provide some useful pointers. Bon voyage!
description: 8 pages
Time reversal symmetry breaking superconductivity
Creators: name: Ghosh, Haranath
Publisher: name: arXiv
Year: 1998
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We study time reversal symmetry breaking superconductivity with $Δ_k = Δ_{x^2-y^2} (k) +e^{iθ} Δ_α$ ($α= s$ or $d_{xy}$) symmetries. It is shown that the behavior of such superconductors could be {\em qualitatively} different depending on the minor components ($α$) and its phase at lower temperatures. It is argued that such {\em qualitatively different} behaviors in thermal as well as in angular dependencies could be a {\em source} of consequences in transport and Josephson physics. Orthorhombicity is found to be a strong mechanism for mixed phase (in case of $α= s$). We show that due to electron correlation the order parameter is more like a pure $d_{x^2-y^2}$ symmetry near optimum doping.
description: 5 pages, 5 figures (attached), to be published in Physical Review B
Variance Suppression: Balanced Training Process in Deep Learning
Creators: name: Yi, Tao
name: Wang, Xingxuan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: Stochastic gradient descent updates parameters with summation gradient computed from a random data batch. This summation will lead to unbalanced training process if the data we obtained is unbalanced. To address this issue, this paper takes the error variance and error mean both into consideration. The adaptively adjusting approach of two terms trading off is also given in our algorithm. Due to this algorithm can suppress error variance, we named it Variance Suppression Gradient Descent (VSSGD). Experimental results have demonstrated that VSSGD can accelerate the training process, effectively prevent overfitting, improve the networks learning capacity from small samples.
description: More experiments are needed to prove this theory, but I'm not quite sure yet
Additional file 5: of Genomic analysis of Leptospira interrogans serovar Paidjan and Dadas isolates from carrier dogs and comparative genomic analysis to detect genes under positive selection
Creators: name: Alongkorn Kurilung
name: Chantisa Keeratipusana
name: Prapat Suriyaphol
name: Hampson, David
name: Nuvee Prapasarakul
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Figure S1. Circular genome map of L. interrogans serovar Lai strain 56601 and the other 13 representative strains studied, with the location of 74 predicted genes under positive selection and recombination marked. (DOCX 1410 kb)
Multifractal Behaviour of n-Simplex Lattice
Creators: name: Kumar, Sanjay
name: Giri, D.
name: Krishna, Sujata
Publisher: name: arXiv
Year: 2000
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study the asymptotic behaviour of resistance scaling and fluctuation of resistance that give rise to flicker noise in an {\em n}-simplex lattice. We propose a simple method to calculate the resistance scaling and give a closed-form formula to calculate the exponent, $β_L$, associated with resistance scaling, for any n. Using current cumulant method we calculate the exact noise exponent for n-simplex lattices.
description: Latex, 9 pages including one figure
Energetics of magnetic transients in a solar active region plage
Creators: name: Chitta, L. P.
name: Sukarmadji, A. R. C.
name: van der Voort, L. Rouppe
name: Peter, H.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Densely packed coronal loops are rooted in plages in the vicinity of active regions on the Sun. The photospheric magnetic features underlying these plages are patches of mostly unidirectional magnetic field extending several arcsec on the solar surface. We aim to explore the transient nature of the magnetic field, its mixed-polarity characteristics, and the associated energetics in plages using high resolution observations and simulations. We used photospheric Fe I 6173 Å spectropolarimetric observations of a decaying active region obtained from the SST. These data were inverted to retrieve the photospheric magnetic field underlying the plage as identified in the EUV emission maps obtained from the SDO/AIA. To obtain better insight into the evolution of plages, we performed 3D radiation magnetohydrodynamic simulations of magnetoconvection using the MURaM code. The observations show transient magnetic flux emergence and cancellation events within the plage on timescales of a few 100 s and on spatial scales comparable to granules. These transient events occur at the footpoints of active region plage loops. In one case the coronal response at the footpoints of these loops is clearly associated with the underlying transient. The simulations also reveal similar magnetic flux emergence and cancellation events that extend to even smaller spatial and temporal scales. Individual simulated transient events transfer an energy flux in excess of 1 MW m$^{-2}$ through the photosphere. We suggest that the magnetic transients could play an important role in the energetics of active region plage. Both in observations and simulations, the opposite-polarity magnetic field brought up by transient flux emergence cancels with the surrounding plage field. Magnetic reconnection associated with such transient events likely conduits magnetic energy to power the overlying chromosphere and coronal loops.
description: Published in A&A (abridged abstract)
Thecophora bimaculata
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Conopidae
Thecophora
Thecophora bimaculata

description: Thecophora bimaculata (Preyssler, 1791)
. Stuke (2006) zeigte auf, dass sich unter der Art Th. pusilla (Meigen, 1824) zwei Arten verbergen. Eine Nachkontrolle von J.-H. Stuke im Jahr 2008 der früher als Th. pusilla bezettelten Tiere ergab, dass viele Tiere aus zahlreichen Kantonen als Th. bimaculata bestimmt werden müssen.
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Schwinger-Keldysh Approach to Disordered and Interacting Electron Systems: Derivation of Finkelstein's Renormalization Group Equations
Creators: name: Chamon, Claudio
name: Ludwig, Andreas W. W.
name: Nayak, Chetan
Publisher: name: arXiv
Year: 1998
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We develop a dynamical approach based on the Schwinger-Keldysh formalism to derive a field-theoretic description of disordered and interacting electron systems. We calculate within this formalism the perturbative RG equations for interacting electrons expanded around a diffusive Fermi liquid fixed point, as obtained originally by Finkelstein using replicas. The major simplifying feature of this approach, as compared to Finkelstein's is that instead of $N \to 0$ replicas, we only need to consider N=2 species. We compare the dynamical Schwinger-Keldysh approach and the replica methods, and we present a simple and pedagogical RG procedure to obtain Finkelstein's RG equations.
description: 22 pages, 14 figures
Dominant $s$-wave superconducting gap in PdTe$_2$ observed by tunneling spectroscopy on side-junctions
Creators: name: Voerman, J. A.
name: de Boer, J. C.
name: Hashimoto, T.
name: Huang, Yingkai
name: Li, Chuan
name: Brinkman, A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We have fabricated superconductor-normal metal side-junctions with different barrier transparencies out of PdTe$_2$ crystalline flakes and measured the differential conductance spectra. Modeling our measurements using a modified Blonder Tinkham Klapwijk (BTK) formalism confirms that the superconductivity is mostly comprised of the conventional $s$-wave symmetry. We have found that for junctions with very low barrier transparencies, the junctions can enter a thermal regime, where the critical current becomes important. Adding this to the BTK-model allows us to accurately fit the experimental data, from which we conclude that the superconductivity in the $a$-$b$ plane of PdTe$_2$ is dominated by conventional $s$-wave pairing.
description: 6 pages, 3 figures, supplementary info
Stripes in Doped Antiferromagnets: Single-Particle Spectral Weight
Creators: name: Zacher, Marc G.
name: Eder, Robert
name: Arrigoni, Enrico
name: Hanke, Werner
Publisher: name: arXiv
Year: 2000
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Recent photoemission (ARPES) experiments on cuprate superconductors provide important guidelines for a theory of electronic excitations in the stripe phase. Using a cluster perturbation theory, where short-distance effects are accounted for by exact cluster diagonalization and long-distance effects by perturbation (in the hopping), we calculate the single-particle Green's function for a striped t-J model. The data obtained quantitatively reproduce salient (ARPES-) features and may serve to rule out "bond-centered" in favor of "site-centered" stripes.
description: final version as appeared in PRL; (c) 2000 The American Physical Society; 4 pages, 4 figures
Additional file 1: of Health providersâ experiences, perceptions and readiness to provide HIV services to men who have sex with men and female sex workers in Uganda â a qualitative study
Creators: name: Matovu, Joseph
name: Geofrey Musinguzi
name: Kiguli, Juliet
name: Nuwaha, Fred
name: Mujisha, Geoffrey
name: Musinguzi, Joshua
name: Arinaitwe, Jim
name: Wanyenze, Rhoda
Publisher: name: figshare
Year: 2019
Subjects: subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Key Informant Interview Guide. This KII guide includes questions that were administered to health providers as part of a large mixed-methods study aimed at exploring the barriers and opportunities for improving access to HIV services among MSM and FSWs in Uganda. Only questions that explored health providersâ experiences, perceptions and readiness to provide HIV services to MSM and FSWs were analyzed for this paper. (PDF 193 kb)
The Problem of Aggregation in Spatial Causality Analysis
Creators: name: Blank, Steven C.
name: Schmiesing, Brian H.
name: Blank, Steven C.
name: Schmiesing, Brian H.
Publisher: name: Unknown
Year: 1986
Subjects: Research Methods/ Statistical Methods

description: Aggregation across time has major implications for interpretation of causality tests. Empirical tests for three corn markets reveal one-way causality to be "fragile" with respect to changes in the level of time aggregation in data. Dynamic multipliers are discussed as one method of checking model specification.
Additional file 2: of Genomic analysis of Leptospira interrogans serovar Paidjan and Dadas isolates from carrier dogs and comparative genomic analysis to detect genes under positive selection
Creators: name: Alongkorn Kurilung
name: Chantisa Keeratipusana
name: Prapat Suriyaphol
name: Hampson, David
name: Nuvee Prapasarakul
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Figure S1. The structure of the rfb locus of L. interrogans serovar Paidjan strain CUDO5 and serovar Dadas strain CUDO8. (DOCX 4487 kb)
Coulomb Blockade Fluctuations in Strongly Coupled Quantum Dots
Creators: name: Maurer, S. M.
name: Patel, S. R.
name: Marcus, C. M.
name: Duruoz, C. I.
name: Harris,, J. S.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Quantum fluctuations of Coulomb blockade are investigated as a function of the coupling to reservoirs in semiconductor quantum dots. We use fluctuations in the distance between peaks $ΔN$ apart to characterize both the amplitude and correlation of peak motion. For strong coupling, peak motion is greatly enhanced at low temperature, but does not show an increase in peak-to-peak correlation. These effects can lead to anomalous temperature dependence in the Coulomb valleys, similar to behavior ascribed to Kondo physics.
description: figures made smaller so download works. Revised, including new data. Related papers at http://www.stanford.edu/group/MarcusLab/grouppubs.html
Chamaepsila confusa Shatalkin & Merz 2010
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psilidae
Chamaepsila
Chamaepsila confusa

description: Chamaepsila confusa Shatalkin & Merz, 2010. (Shatalkin & Merz 2010).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Chacaltaya: towards a solution of the knee ....?
Creators: name: Saavedra, O.
name: Jones, L.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Cosmic rays physics is currently being studied with rather sophisticated detectors running in a variety of experimental conditions and atmospheric depths around the world. In this paper we describe the reasons why cosmic ray physics experiments at high altitudes like Chacaltaya are so important for resolving some of the open problems in cosmic physics. A discussion on the future prospects of the high altitude mountain laboratories such as Chacaltaya for cosmic ray physics is presented.
description: 8 pages, 4 figures, to appear in Proceedings of the "Chacaltaya Meeting on Cosmic Ray Physics", Il Nuovo Cimento
946-nm Nd:YAG digital-locked laser at $1.1\times10^{-16}$ in 1 s and transfer-locked to a cryogenic silicon cavity
Creators: name: Didier, A.
name: Ignatovich, S.
name: Benkler, E.
name: Okhapkin, M.
name: Mehlstäubler, T. E.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We present a Nd:YAG ultra-stable laser system operating at 946 nm and demonstrate a fractional frequency instability of $1.1\times10^{-16}$ at 1 s by pre-stabilizing it to a 30 cm-long ULE cavity at room temperature. All key analog components have been replaced by FPGA-based digital electronics. To reach an instability below the $10^{-16}$ level, we transfer the stability of a 1542 nm laser stabilized to a cryogenic silicon cavity exhibiting a fractional frequency instability of $4\times10^{-17}$ at 1 s to the laser at 946 nm.
description: 5 pages, 5 figures
Identifying the 3FHL catalog: CTIO results
Creators: name: Desai, Abhishek
name: Marchesi, Stefano
name: Rajagopal, Meenakshi
name: Ajello, Marco
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Active galactic Nuclei (AGNs) with their relativistic jets pointed towards the observer, form a subclass of luminous gamma-ray sources commonly known as blazars. The study of blazars is essential to improve our understanding on the AGNs emission mechanisms and evolution, as well as to map the extragalactic background light. To do so, however, one needs to correctly classify and measure a redshift for a large sample of these sources. The Third {\it Fermi}--LAT Catalog of High-Energy Sources (3FHL) contains $\approx1160$ blazars reported at energies greater than $10$\,GeV. However $\sim$25\% of these sources are unclassified and $\sim$50\% lack of redshift information. To increase the spectral completeness of the 3FHL catalog, we are working on an optical spectroscopic follow up campaign using 4--m and 8--m telescopes. In this paper, we present the results of the second part of this campaign, where we observed 23 blazars using the 4\,$m$ telescope at CTIO in Chile. We report all the 23 sources to be classified as BL Lacs, a confirmed redshift measurement for 3 sources, a redshift lower limit for 2 sources and a tentative redshift measurement for 3 sources.
description: Figure 2 is made up of 23 individual plot figures and while Figure 3 is made up of 8 individual plot figures. APJ accepted 01/24/2019
Chamaepsila sardoa
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psilidae
Chamaepsila
Chamaepsila sardoa

description: Chamaepsila sardoa (Rondani, 1876). (Shatalkin & Merz 2010).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 126, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
The local and distant Universe: stellar ages and $H_0$
Creators: name: Jimenez, Raul
name: Cimatti, Andrea
name: Verde, Licia
name: Moresco, Michele
name: Wandelt, Benjamin
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The ages of the oldest stellar objects in our galaxy provide an independent test of the current cosmological model as they give a lower limit to the age of the Universe. Recent accurate parallaxes by the Gaia space mission, accurate measurements of the metallicity of stars, via individual elemental abundances, and advances in the modelling of stellar evolution, provide new, higher-precision age estimates of the oldest stellar populations in the galaxy: globular clusters and very-low-metallicity stars. The constraints on the age of the Universe, $t_U$, so obtained are determined from the local Universe and at late time. It is well known that local and early-Universe determinations of another cosmological parameter closely related to the age of the Universe, the Hubble constant $H_0$, show a $\gtrsim 3 σ$ tension. In the standard cosmological model, $Λ$CDM, $t_U$ and $H_0$ are related by the matter density parameter $Ω_{m,0}$. We propose to combine local $t_U$ constraints with late-time $Ω_{m,0}$ estimates in a $Λ$CDM framework, to obtain a low-redshift $H_0$ determination that does not rely on early Universe physics. A proof-of-principle of this approach with current data gives $H_0=71\pm2.8$ ($H_0= 69.3 \pm 2.7$) km s$^{-1}$ Mpc$^{-1}$ from globular clusters (very-low-metallicity stars) with excellent prospects for improved constraints in the near future.
description: Matches published version in JCAP; references added, no other changes
Impact of Future Submillimeter and Millimeter Large Facilities on the Studies of Galaxy Formation and Evolution
Creators: name: Takeuchi, Tsutomu T.
name: Kawabe, Ryohei
name: Kohno, Kotaro
name: Nakanishi, Koichiro
name: Ishii, Takako T.
name: Hirashita, Hiroyuki
name: Yoshikawa, Kohji
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate what we can learn about galaxy formation and evolution from the data which will be obtained by the forthcoming large submillimeter/millimeter facilities, mainly by the Atacama Submillimeter Telescope Experiment (ASTE) and the Atacama Large Millimeter Array/Large Millimeter and Submillimeter Array (ALMA/LMSA). We first calculate the source counts from 350 um to 3 mm using the empirical infrared galaxy number count model of Takeuchi et al. (2001). Based on the number counts, we evaluate the source confusion and determine the confusion limit at various wavebands as a function of the characteristic beam size. At submillimeter wavelengths, source confusion with the 10-15-m class facilities becomes severe at 0.1 to 1 mJy level, and astrometry and flux measurements will be difficult. However, we show that very a large-area survey of submillimeter sources brighter than 10-50 mJy can provide a unique constraint on infrared galaxy evolution at z = 1-2. We also find that the 5σ-confusion limit of the LMSA is fainter than 1 μJy. The source counts at such faint flux levels give important information of the epoch of galaxy formation. We then show that multiband photometry from the infrared (by ASTRO-F) to the millimeter can be utilized as a redshift estimator. In addition, we compare the observed 1.4, 5, and 8-GHz source counts with our model counts to examine the contribution of star forming galaxies to the faint radio galaxies.
description: 17 pages LaTeX, PASP accepted. Abstract abridged
Statistical Properties of Contact Maps
Creators: name: Vendruscolo, M.
name: Subramanian, B.
name: Kanter, I.
name: Domany, E.
name: Lebowitz, J.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Soft Condensed Matter (cond-mat.soft)
subject: Quantitative Biology (q-bio)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: A contact map is a simple representation of the structure of proteins and other chain-like macromolecules. This representation is quite amenable to numerical studies of folding. We show that the number of contact maps corresponding to the possible configurations of a polypeptide chain of N amino acids, represented by (N-1)-step self avoiding walks on a lattice, grows exponentially with N for all dimensions D>1. We carry out exact enumerations in D=2 on the square and triangular lattices for walks of up to 20 steps and investigate various statistical properties of contact maps corresponding to such walks. We also study the exact statistics of contact maps generated by walks on a ladder.
description: Latex file, 15 pages, 12 eps figures. To appear on Phys. Rev. E
Chamaepsila unilineata
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psilidae
Chamaepsila
Chamaepsila unilineata

description: Chamaepsila unilineata (Zetterstedt, 1847). (Shatalkin & Merz 2010).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 127, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Additional file 3: of Isocytosine deaminase Vcz as a novel tool for the prodrug cancer therapy
Creators: name: Arunas Kazlauskas
name: Adas Darinskas
name: Meškys, Rolandas
name: Tamašauskas, Arimantas
name: Urbonavičius, Jaunius
Publisher: name: figshare
Year: 2019
Subjects: Space Science
Medicine
Cell Biology
Pharmacology
Developmental Biology

description: MSC transduction with the letivirus encoding Vcz and EGFP. a Fluorescence image and (b) the bright field view of MSC cells transduced with letivirus. The scale bar of 100 μm is shown. (PDF 145 kb)
The AGB phase-transition outside the Local Group: K-band observations of young star clusters in NGC 7252
Creators: name: Maraston, C.
name: Kissler-Patig, M.
name: Brodie, J. P.
name: Barmby, P.
name: Huchra, J. P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have extended the study of the young star clusters observed in the merger remnant galaxy NGC 7252 by obtaining K band photometry for these clusters. Our K band data significantly complement the optical photometry and spectroscopy in the literature: K band data are fundamental to study the Asymptotic Giant Branch (AGB) population of these clusters, since the AGB phase transition (occuring between the age of 200 Myr and 1 Gyr) causes abrupt changes in the near-infrared luminosity of the clusters while producing only small changes in the optical. Therefore, the e.g. V-K colour is ideal to study this evolutionary phase of stellar populations. For the present analysis we present models for Simple Stellar Populations which include the contribution of the AGB stellar phase, calibrated with the young and intermediate age star clusters of the Magellanic Clouds. The comparison with the colour distribution of the NGC 7252 star clusters shows that they are indeed intermediate age clusters undergoing the AGB phase transition. The AGB phase transition is observed for the first time outside the Local Group. Most of the studied clusters span the very narrow age range 300-500 Myr, and likely have metallicities 0.5-1 Z_{\odot}. A very important exception is the cluster W32, which has already completed its AGB epoch, its colours being consistent with an age of 1-2 Gyr. This impacts on the duration of the merger-induced starburst. The strengths of the magnesium and iron lines in the spectrum of the best observed cluster W3, and in the spectrum of the diffuse central light of NGC 7252, do not show an overabundance in alpha-elements, in contrast to the bulk stellar population of elliptical galaxies.
description: Accepted for publication in Astronomy & Astrophysics, 17 pages, 12 figures
Critical level statistics at the Anderson transition in four-dimensional disordered systems
Creators: name: Zharekeshev, I. Kh.
name: Kramer, B.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The level spacing distribution is numerically calculated at the disorder-induced metal--insulator transition for dimensionality d=4 by applying the Lanczos diagonalisation. The critical level statistics are shown to deviate stronger from the result of the random matrix theory compared to those of d=3 and to become closer to the Poisson limit of uncorrelated spectra. Using the finite size scaling analysis for the probability distribution Q_n(E) of having n levels in a given energy interval E we find the critical disorder W_c = 34.5 \pm 0.5, the correlation length exponent ν= 1.1 \pm 0.2 and the critical spectral compressibility k_c \approx 0.5.
description: 10 pages, LaTeX2e, 7 fig, invited talk at PILS (Percolation, Interaction, Localization: Simulations of Transport in Disordered Systems) Berlin, Germany 1998, to appear in Annalen der Physik
Charge-Density-Wave induced modifications to the quasiparticle self-energy in 2H TaSe2
Creators: name: Valla, T.
name: Fedorov, A. V.
name: Johnson, P. D.
name: Xue, J.
name: Smith, K. E.
name: Di Salvo, F. J.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The self-energy of the photo-hole in 2H-TaSe2 is measured by angle-resolved photoemission spectroscopy (ARPES) as a function of binding energy and temperature. In the charge-density wave (CDW) state, a structure in the self- energy is detected at ~ 65 meV that can not be explained by electron-phonon scattering. A reduction in the scattering rates below this energy indicates the collapse of a major scattering channel with the formation of the CDW state, accompanying the appearance of a bosonic "mode" in the excitation spectrum of the system.
description: 4 pages, 4 eps figures, minor changes, references added
Tunable magnetoplasmonics in lattices of Ni/SiO$_2$/Au dimers
Creators: name: Pourjamal, Sara
name: Kataja, Mikko
name: Maccaferri, Nicolò
name: Vavassori, Paolo
name: van Dijken, Sebastiaan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We present a systematic study on the optical and magneto-optical properties of Ni/SiO$_2$/Au dimer lattices. By considering the excitation of orthogonal dipoles in the Ni and Au nanodisks, we analytically demonstrate that the magnetoplasmonic response of dimer lattices is governed by a complex interplay of near- and far-field interactions. Near-field coupling between dipoles in Ni and low-loss Au enhances the polarizabilty of single dimers compared to that of isolated Ni nanodisks. Far-field diffractive coupling in periodic lattices of these two particle types enlarges the difference in effective polarizability further. This effect is explained by an inverse relationship between the damping of collective surface lattice resonances and the imaginary polarizability of individual scatterers. Optical reflectance measurements, magneto-optical Kerr effect spectra, and finite-difference time-domain simulations confirm the analytical results. Hybrid dimer arrays supporting intense plasmon excitations are a promising candidate for active magnetoplasmonic devices.
description: 13 pages, 7 figures
Psila helvetica Shatalkin & Merz 2010
Creators: name: Bächli, Gerhard
name: Merz, Bernhard
name: Haenni, Jean-Paul
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psilidae
Psila
Psila helvetica

description: Psila helvetica Shatalkin & Merz, 2010. (Shatalkin & Merz 2010).
description: Published as part of Bächli, Gerhard, Merz, Bernhard & Haenni, Jean-Paul, 2014, Dritter Nachtrag zur Checkliste der Diptera der Schweiz, pp. 119-140 in Entomo Helvetica 7 on page 127, DOI: 10.5169/seals-985967, http://zenodo.org/record/8096745
Laser slicing: a thin film lift-off method for GaN-on-GaN technology
Creators: name: Voronenkov, Vladislav
name: Bochkareva, Natalia
name: Gorbunov, Ruslan
name: Zubrilov, Andrey
name: Kogotkov, Viktor
name: Latyshev, Philipp
name: Lelikov, Yuri
name: Leonidov, Andrey
name: Shreter, Yuri
Publisher: name: arXiv
Year: 2019
Subjects: subject: Applied Physics (physics.app-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: A femtosecond laser focused inside bulk GaN was used to slice a thin GaN film with an epitaxial device structure from a bulk GaN substrate. The demonstrated laser slicing lift-off process did not require any special release layers in the epitaxial structure. GaN film with a thickness of 5 $μ$m and an InGaN LED epitaxial device structure was lifted off a GaN substrate and transferred onto a copper substrate. The electroluminescence of the LED chip after the laser slicing lift-off was demonstrated.
Improvement of the Spatial Resolution of the ACIS Using Split Pixel Events
Creators: name: Tsunemi, Hiroshi
name: Mori, Koji
name: Miyata, Emi
name: Baluta, Christopher
name: Burrows, David N.
name: Garmire, Gordon P.
name: Chartas, George
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The position accuracy of X-ray photons on a CCD detector is generally believed to be limited by the CCD pixel size. While this is true in general, the position accuracy for X-ray events which deposit charge in more than one pixel can be better than that of the CCD pixel size. Since the position uncertainty for corner events is much better than the pixel size, we can improve the Chandra ACIS spatial resolution by selecting only these events. We have analyzed X-ray images obtained with the Chandra ACIS for six point-like sources observed near the optical axis. The image quality near the optical axis is characterized by a half power diameter (HPD) of $0.^{\!\!\prime \prime}66$ that is a convolution of the PSF of the HRMA and the CCD pixel shape ($24\,μ$m square). By considering only corner events the image quality is improved to $0.^{\!\!\prime \prime}56$ (HPD), which is very close to the image quality of the HRMA alone. We estimated the degradation of the image quality obtained by using all events, compared to that obtained using only corner events, to be $0.^{\!\!\prime \prime}33$, which coincides with that expected from the pixel size. Since the fraction of the corner events is relatively small, this technique requires correspondingly longer exposure time to achieve good statistics.
description: 12 pages, 5 figures. Accepted for publication of ApJ. High resolution and color figures are available at http://wwwxray.ess.sci.osaka-u.ac.jp/~miyata/paper/acis_subpixel.pdf
The Sklyanin Bracket and Cluster Adjacency at All Multiplicity
Creators: name: Golden, John
name: McLeod, Andrew J.
name: Spradlin, Marcus
name: Volovich, Anastasia
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We argue that the Sklyanin Poisson bracket on Gr(4,n) can be used to efficiently test whether an amplitude in planar ${\cal{N}}=4$ supersymmetric Yang-Mills theory satisfies cluster adjacency. We use this test to show that cluster adjacency is satisfied by all one- and two-loop MHV amplitudes in this theory, once suitably regulated. Using this technique we also demonstrate that cluster adjacency implies the extended Steinmann relations at all particle multiplicities.
description: 25 pages; v2: added reference
MOESM1 of AntAngioCOOL: computational detection of anti-angiogenic peptides
Creators: name: Zahiri, Javad
name: Khorsand, Babak
name: Yousefi, Ali
name: Mohammadjavad Kargar
name: Zade, Ramin Shirali Hossein
name: Ghasem Mahdevar
Publisher: name: figshare
Year: 2019
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Additional file 1. Supplementary Materials and Methods. Train and test datasets; 227 different classifiers.