cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Lung protection in cardio-pulmonary bypass
Creators: name: Salameh, A.
name: Greimann, W.
name: Vollroth, M.
name: Dhein, S.
name: Bahramsoltani, Mahtab
name: Dahnert, I.
Publisher: name: Freie Universität Berlin
Year: 2017
Subjects: subject: minocycline
subject: cardio-pulmonary bypass
subject: lung injury
subject: apoptosis
subject: adenosine triphosphate
subject: tumor necrosis factor-alpha
subject: poly-ADP-ribose
subject: bronchial epithelium
subject: 600 Technik, Medizin, angewandte Wissenschaften::610 Medizin und Gesundheit

description: Since the invention of the heart-lung machine paediatric cardiac surgery developed rapidly. For correction of complex cardiac malformations the application of a cardio-pulmonary bypass (CPB) has become indispensable but possible negative effects of this technique should not be neglected. Especially, both bypassed organs i.e. heart and lung are not perfused during the procedure and therefore are threatened by ischemia and reperfusion injury. Additionally, CPB was developed with a non-pulsatile flow but there are clinical observations that pulsatile flow might be superior with improved patient outcomes. Thus, the aim of our study was to evaluate the effect of CPB on lung structure and to assess whether different flow modalities (pulsatile vs. non-pulsatile flow) or application of the antibiotic minocycline might be advantageous. Thirty five piglets of four weeks age were examined and divided into five experimental groups: control (no CPB) without or with minocycline, CPB (non-pulsatile flow) without or with minocycline and CPB with pulsatile flow. CPB was performed for 90 min followed by a 120 min reperfusion and recovery phase. Thereafter, adenosine triphosphate-content of lung biopsies and histology was carried out. We found that CPB was associated with a significant thickening of alveolar wall accompanied by an infiltration of neutrophil leucocytes. Moreover, markers for hypoxia, apoptosis, nitrosative stress, inflammation and DNA damage were significantly elevated after CPB. These cellular damages could be partially inhibited by minocycline or pulsatile flow. Both, minocycline and pulsatile flow attenuate lung damage after CPB.
First attempt at measuring the CMB cross-polarization
Creators: name: de Oliveira-Costa, Angelica
name: Tegmark, Max
name: Zaldarriaga, Matias
name: Barkats, Denis
name: Gundersen, Josh O.
name: Hedman, Matt M.
name: Staggs, Suzanne T.
name: Winstein, Bruce
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compute upper limits on CMB cross-polarization by cross-correlating the PIQUE and Saskatoon experiments. We also discuss theoretical and practical issues relevant to measuring cross-polarization and illustrate them with simulations of the upcoming BOOMERanG 2002 experiment. We present a method that separates all six polarization power spectra (TT, EE, BB, TE, TB, EB) without any other "leakage" than the familiar EE-BB mixing caused by incomplete sky coverage. Since E and B get mixed, one might expect leakage between TE and TB, between EE and EB and between BB and EB - our method eliminates this by preserving the parity symmetry under which TB and EB are odd and the other four power spectra are even.
description: Polarization movies can be found at http://www.hep.upenn.edu/~angelica/polarization.html
Connecting galaxy structure and star formation: the role of environment in formation of S0 galaxies
Creators: name: Mishra, Preetish K.
name: Wadadekar, Yogesh
name: Barway, Sudhanshu
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In this work, we investigate the reason behind the increased occurrence of S0 galaxies in high density environments. Our sample comprises of $\sim$ 2500 spiral and $\sim$ 2000 S0 galaxies spanning a wide range of environments. Dividing the galaxies into categories of classical and pseudobulge hosting spiral and S0 galaxies, we have studied their properties as a function of the environment. We find that the fraction of pseudobulge hosting disc galaxies decreases with increase in density. The classical bulge hosting spirals and S0 galaxies follow a similar trend in less dense environments but towards higher densities, we observe an increase in the fraction of classical bulge host S0 galaxies at the expense of spirals. Comparing the structural and the star formation properties of galaxies on the size-mass and $NUV-r$ colour-mass planes respectively, we infer that classical bulge hosting spirals are likely to get transformed into S0 morphology. We notice a trend of galaxy structure with environment such that the fraction of classical bulge hosting spiral galaxies is found to increase with environment density. We also find that among classical bulge hosting spirals, the fraction of quenched galaxies increases in denser environments. We surmise that the existence of more classical bulge hosting spirals galaxies and more efficient quenching leads to the observed increased occurrence of S0 galaxies in high density environments. The relation between galaxy structure and environment also exists for the disc galaxies irrespective of their visual morphology, which is driven mainly by halo mass.
description: 14 pages, 8 figures, accepted for publication in Monthly Notices of the Royal Astronomical Society
Comments on the Deformed W_N Algebra
Creators: name: Odake, Satoru
Publisher: name: arXiv
Year: 2001
Subjects: subject: Quantum Algebra (math.QA)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: We obtain an explicit expression for the defining relation of the deformed W_N algebra, DWA(^sl_N)_{q,t}. Using this expression we can show that, in the q-->1 limit, DWA(^sl_N)_{q,t} with t=e^{-2πi/N}q^{(k+N)/N} reduces to the sl_N-version of the Lepowsky-Wilson's Z-algebra of level k, ZA(^sl_N)_k. In other words DWA(^sl_N)_{q,t} with t=e^{-2πi/N}q^{(k+N)/N} can be considered as a q-deformation of ZA(^sl_N)_k. In the appendix given by H.Awata, S.Odake and J.Shiraishi, we present an interesting relation between DWA(^sl_N)_{q,t} and ζ-function regularization.
description: 10 pages, LaTeX2e with ws-ijmpb.cls, Talk at the APCTP-Nankai Joint Symposium on ``Lattice Statistics and Mathematical Physics'', 8-10 October 2001, Tianjin China
Applying Polynomial Decoupling Methods to the Polynomial NARX Model
Creators: name: Karami, Kiana
name: Westwick, David
name: Schoukens, Johan
Publisher: name: arXiv
Year: 2022
Subjects: subject: Systems and Control (eess.SY)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: System identification uses measurements of a dynamic system's input and output to reconstruct a mathematical model for that system. These can be mechanical, electrical, physiological, among others. Since most of the systems around us exhibit some form of nonlinear behavior, nonlinear system identification techniques are the tools that will help us gain a better understanding of our surroundings and potentially let us improve their performance. One model that is often used to represent nonlinear systems is the polynomial NARX model, an equation error model where the output is a polynomial function of the past inputs and outputs. That said, a major disadvantage with the polynomial NARX model is that the number of parameters increases rapidly with increasing polynomial order. Furthermore, the polynomial NARX model is a black-box model, and is therefore difficult to interpret. This paper discusses a decoupling algorithm for the polynomial NARX model that substitutes the multivariate polynomial with a transformation matrix followed by a bank of univariate polynomials. This decreases the number of model parameters significantly and also imposes structure on the black-box NARX model. Since a non-convex optimization is required for this identification technique, initialization is an important factor to consider. In this paper the decoupling algorithm is developed in conjunction with several different initialization techniques. The resulting algorithms are applied to two nonlinear benchmark problems: measurement data from the Silver-Box and simulation data from the Bouc-Wen friction model, and the performance is evaluated for different validation signals in both simulation and prediction.
description: 28 pages, 16 figures
Universal Results for Correlations of Characteristic Polynomials: Riemann-Hilbert Approach
Creators: name: Strahov, Eugene
name: Fyodorov, Yan V.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Mathematical Physics (math-ph)
subject: Condensed Matter (cond-mat)
subject: High Energy Physics - Theory (hep-th)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences

description: We prove that general correlation functions of both ratios and products of characteristic polynomials of Hermitian random matrices are governed by integrable kernels of three different types: a) those constructed from orthogonal polynomials; b) constructed from Cauchy transforms of the same orthogonal polynomials and finally c) those constructed from both orthogonal polynomials and their Cauchy transforms. These kernels are related with the Riemann-Hilbert problem for orthogonal polynomials. For the correlation functions we obtain exact expressions in the form of determinants of these kernels. Derived representations enable us to study asymptotics of correlation functions of characteristic polynomials via Deift-Zhou steepest-descent/stationary phase method for Riemann-Hilbert problems, and in particular to find negative moments of characteristic polynomials. This reveals the universal parts of the correlation functions and moments of characteristic polynomials for arbitrary invariant ensemble of $β=2$ symmetry class.
description: 34pages
Additional file 8: of Genes, pathways and transcription factors involved in seedling stage chilling stress tolerance in indica rice through RNA-Seq analysis
Creators: name: Sharat Pradhan
name: Elssa Pandit
name: Nayak, Deepak
name: Lambodar Behera
name: Trilochan Mohapatra
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: Plant Biology
subject: Computational Biology

description: Table S2. Differentially expressed genes (DEGs) of CSV and CTV genotype at each time interval. (DOCX 13 kb)
Necremnus rugulosus Delucchi
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Necremnus
Necremnus rugulosus

description: Necremnus rugulosus Delucchi (Eulophidae)
 Necremnus rugulosus Delucchi, 1962c: 56. Holotype m, Morocco: Rif, 15 km SE Chauen [ChechaoueÁn], Jebala, Haouta el Kasdir (VD [examined]).
 Material. HOLOTYPE m (mp) labelled`Talasoltane [sic] RifÐ 1850 m 4±11.7.61; HOLOTYPE [red]; NECREMNUS rugulosus n. V. Delucchi det.’.
PARATYPES, VD: 14 mm (mp). Two slides (sc) with antennae and wings (1962c: 57, ®gures 6, 7) of paratypes.
 Remarks. Two female paratypes mentioned by Delucchi could not be located. I could not trace the localities given by Delucchi on his labels and in the original publication (1962c: 58). From the date and altitude, however, it seems likely that Talasoltane is the same as or at least very near Haouta el Kasdir.
 Status. Necremnus rugulosus Delucchi.
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on page 97, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
Additional file 9: of Genes, pathways and transcription factors involved in seedling stage chilling stress tolerance in indica rice through RNA-Seq analysis
Creators: name: Sharat Pradhan
name: Elssa Pandit
name: Nayak, Deepak
name: Lambodar Behera
name: Trilochan Mohapatra
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: Plant Biology
subject: Computational Biology

description: Table S3. Comparison of DEGs of CSV and CTV genotypes at each time interval. (DOCX 14 kb)
Revisiting fission-probability data using $\mathcal{R}$-matrix Monte-Carlo simulations : application to Pu fissile isotopes over the 4 to 8 MeV excitation energy range
Creators: name: Bouland, O.
name: Jurado, B.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Theory (nucl-th)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: This article describes an original approach to analyze simultaneously cross sections and surrogate data measurements using efficient Monte Carlo extended $\mathcal{R}$-matrix theory algorithm based on unique set of nuclear structure parameters. The alternative analytical path based on the manifold Hauser-Feshbach equation was intensively used in this work to gauge the errors carried by the surrogate-reaction method commonly taken to predict neutron-induced cross sections from observed partial decay probabilities. Present paper emphasizes in particular a dedicated way to treat direct reaction entrance and prior decay excited nucleus outgoing channels widths correlations. Present smart theoretical foundation brought the opportunity to apply successfully our method to both fission-probability data and directly measured neutron cross sections according to Pu fissile isotopes; namely the $^{237, 238, 240, 242~and~244}$Pu$^*$ nuclei. This new capability opens genuine perspectives in matter of 'evaluation process' from foreseen fission- and $γ$-decay probabilities simultaneously measured as derived data will become available.
description: 33 pages ; 50 Figures Prior submission to PRC
Bandakia concreta Thor 1913
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Anisitsiellidae
Bandakia
Bandakia concreta

description: Bandakia concreta Thor, 1913
 Bandakia concreta Thor, 1913: Mota¸s 1928f: 146, 1928g: 30; K. Viets 1939a: 2; Schwoerbel 1959a: 19, 1965: 477; Vinçon 1987: 240; Gerecke 1994: 268.
Distribution in France: Corsica, Haut-Rhin, IsŁre, PyrØnØes (PyrØnØes-Atlantiques), 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 37, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Prospects for Detection of Intracluster Gas Bulk Velocities Through the Sunyaev-Zel'dovich Effect
Creators: name: Dupke, Renato A.
name: Bregman, Joel N.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Intracluster gas velocity gradients have been recently detected by the authors in the Centaurus cluster (Abell 3526) using the Doppler shift of X-ray spectral lines with ASCA Solid-state Imaging Spectrometers. The velocity gradient was found to be maximum along a line roughly perpendicular to the direction of the incoming subgroup Cen 45 and has a correspondent velocity difference of ~ (3.4+-1.1) x 1000 km/s within a ~10'-diameter region centered on the cD galaxy NGC 4696. Such bulk velocities should Comptonize the Cosmic Microwave Background Radiation producing variations of intensity and temperature that can be detectable in the near future with bolometers such as BOLOCAM . In this paper we realistically estimate the expected CMBR Comptonization for the central region of Abell 3526, using ASCA and ROSAT data to constrain the S-Z parameter expectations.
description: 10 pages, 3 eps figures, Accepted for publication in the Astrophysical Journal
Basis Generator for M-Scheme SU(3) Shell Model Calculations
Creators: name: Gueorguiev, Vesselin G.
name: Draayer, Jerry P.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Nuclear Theory (nucl-th)
subject: Group Theory (math.GR)
subject: Representation Theory (math.RT)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: A FORTRAN code for generating the leading SU(3) irreducible representation (irrep) of N identical spin 1/2 fermions in a harmonic oscillator mean field is introduced. The basis states are labeled by N--the total number of particles, the SU(3) irrep labels ($λ,μ$), and S -- the total spin of the system. The orthonormalized basis states have two additional good quantum numbers: $ε$ -- the eigenvalue of the quadruple operator, $Q_{0}$; and $M_{J}$ -- the eigenvalues of the projection of the total angular momentum operator, $J_{0}=L_{0}+S_{0}$. The approach that is developed can be used for a description of nuclei in a proton-neutron representation and is part of a larger program aimed at integrating SU(3) symmetry into the best of the currently available exact shell-model technologies.
description: 10 pages, 6 figures, talk presented at the XXI Symposium on Nuclear Physics, Oaxtepec, Morelos, Mexico, 1998
First in-flight synchrotron X-ray absorption and photoemission study of carbon soot nanoparticles
Creators: name: Ouf, F. -X.
name: Parent, P.
name: Laffon, C.
name: Marhaba, I.
name: Ferry, D.
name: Marcillaud, B.
name: Antonsson, Egill
name: Benkoula, S.
name: Liu, X. -J.
name: Nicolas, Robert
name: Patanen, M.
name: Barreda, F. -A.
name: Sublemontier, O.
name: Coppalle, A.
name: Yon, J.
name: Miserque, F.
name: Mostefaoui, T.
name: Regier, T. Z.
name: Mitchell, J. -B. A.
name: Miron, C.
Publisher: name: Freie Universität Berlin
Year: 2016
Subjects: subject: Characterization and analytical techniques
subject: 500 Naturwissenschaften und Mathematik::570 Biowissenschaften; Biologie

description: Many studies have been conducted on the environmental impacts of combustion generated aerosols. Due to their complex composition and morphology, their chemical reactivity is not well understood and new developments of analysis methods are needed. We report the first demonstration of in-flight X-ray based characterizations of freshly emitted soot particles, which is of paramount importance for understanding the role of one of the main anthropogenic particulate contributors to global climate change. Soot particles, produced by a burner for several air-to-fuel ratios, were injected through an aerodynamic lens, focusing them to a region where they interacted with synchrotron radiation. X-ray photoelectron spectroscopy and carbon K-edge near-edge X-ray absorption spectroscopy were performed and compared to those obtained for supported samples. A good agreement is found between these samples, although slight oxidation is observed for supported samples. Our experiments demonstrate that NEXAFS characterization of supported samples provides relevant information on soot composition, with limited effects of contamination or ageing under ambient storage conditions. The highly surface sensitive XPS experiments of airborne soot indicate that the oxidation is different at the surface as compared to the bulk probed by NEXAFS. We also report changes in soot’s work function obtained at different combustion conditions.
Shallow Ultraviolet Transits of WD 1145+017
Creators: name: Xu, Siyi
name: Hallakoun, Na'ama
name: Gary, Bruce
name: Dalba, Paul A.
name: Debes, John
name: Dufour, Patrick
name: Fortin-Archambault, Maude
name: Fukui, Akihiko
name: Jura, Michael A.
name: Klein, Beth
name: Kusakabe, Nobuhiko
name: Muirhead, Philip S.
name: Narita, Norio
name: Steele, Amy
name: Su, Kate Y. L.
name: Vanderburg, Andrew
name: Watanabe, Noriharu
name: Zhan, Zhuchang
name: Zuckerman, Ben
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: WD 1145+017 is a unique white dwarf system that has a heavily polluted atmosphere, an infrared excess from a dust disk, numerous broad absorption lines from circumstellar gas, and changing transit features, likely from fragments of an actively disintegrating asteroid. Here, we present results from a large photometric and spectroscopic campaign with Hubble, Keck , VLT, Spitzer, and many other smaller telescopes from 2015 to 2018. Somewhat surprisingly, but consistent with previous observations in the u' band, the UV transit depths are always shallower than those in the optical. We develop a model that can quantitatively explain the observed "bluing" and the main findings are: I. the transiting objects, circumstellar gas, and white dwarf are all aligned along our line of sight; II. the transiting object is blocking a larger fraction of the circumstellar gas than of the white dwarf itself. Because most circumstellar lines are concentrated in the UV, the UV flux appears to be less blocked compared to the optical during a transit, leading to a shallower UV transit. This scenario is further supported by the strong anti-correlation between optical transit depth and circumstellar line strength. We have yet to detect any wavelength-dependent transits caused by the transiting material around WD 1145+017.
description: 16 pages, 11 figures, 6 tables, ApJ, in press
Oomara locustae Delucchi
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Oomara
Oomara locustae

description: Oomara locustae Delucchi (Pteromalidae)
 Oomara locustae Delucchi, 1964a: 29. Holotype m, Madagascar: Province Betioky, Simearano (MHNG [examined]).
 Material. HOLOTYPE m (cp) labelled` HOLOTYPUS; Oomara locustae m. V. Delucchi det.; ds oeufs Locusta SIMEARANO 9.IX.1962 D. WINTREBERT rec.; Betioky Madagascar Descamps C.I.L.B.; Ex.: Locusta migratoria capito Acrididae C.I.L.B.’.
PARATYPES, MHNG: 4 mm, allotype l(cp), two slides (scx) with female and male antenna and a left fore wing (1964a: 29, ®gure 5) of paratypes. VD: 7 mm, 3 ll(cp).
 Remarks. Seven female paratypes mentioned by Delucchi could not be located. Delucchi (1964a: 31) cited`Amborompotsy, 20 aouÃt 1962’ as origin for the holotype. However, the latter is labelled with`SIMEARANO 9.IX.1962 ’.
 Status. Oomara locustae Delucchi.
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on page 98, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
Dark Matter Search in the EDELWEISS experiment
Creators: name: Juillard, A.
name: Benoit, A.
name: Berge, L.
name: Bonnevaux, A.
name: Bouvier, R.
name: Broniatowski, A.
name: Chambon, B.
name: Chapellier, M.
name: Chardin, G.
name: Charvin, P.
name: Cluzel, P.
name: De Jesus, M.
name: Di Stefano, P.
name: Drain, D.
name: Dumoulin, L.
name: Gascon, J.
name: Gerbier, G.
name: Goldbach, C.
name: Goyot, M.
name: Gros, M.
name: Hadjout, J. P.
name: De Lesquen, A.
name: Loidl, M.
name: Loiseau, D.
name: Mallet, J.
name: Marnieros, S.
name: Martineau, O.
name: Mirabolfathi, N.
name: Mosca, L.
name: Navick, X-F.
name: Nollez, G.
name: Pari, P.
name: Pastor, C.
name: Simon, E.
name: Stern, M.
name: Vagneron, L.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The EDELWEISS Dark Matter Search uses low-temperature Ge detectors with heat and ionisation read-out to identify nuclear recoils induced by elastic collisions with WIMPs from the galactic halo. Preliminary results obtained with 320g bolometers are described. After a few weeks of data taking, data accumulated with one of these detectors already allow to reach the upper part of the DAMA region. Prospects for the present run and the second stage of the experiment, EDELWEISS-II, using an innovative reversed cryostat allowing data taking with 100 detectors, are briefly described.
description: 4 pages, LaTeX, 3 figures, contribution to " Very High Energy Phenomena in the Universe ", Les Arcs, France (January 20-27, 2001)
Additional file 7: of Genes, pathways and transcription factors involved in seedling stage chilling stress tolerance in indica rice through RNA-Seq analysis
Creators: name: Sharat Pradhan
name: Elssa Pandit
name: Nayak, Deepak
name: Lambodar Behera
name: Trilochan Mohapatra
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: Plant Biology
subject: Computational Biology

description: Table S1. Summary of RNA-Seq reads and their mapping on the rice genome. (DOCX 22 kb)
Evolution of Hard X-Ray Radiation from Clusters of Galaxies: Bremsstrahlung or Inverse Compton Scattering?
Creators: name: Takizawa, Motokazu
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have calculated evolution of a non-thermal electron population from super-thermal but weakly relativistic to highly relativistic energy range in clusters of galaxies. We investigate evolution of hard X-ray radiation due to both bremsstrahlung and inverse Compton scattering of the cosmic microwave background photons. The bremsstrahlung component is more significant than the inverse Compton scattering one when the momentum spectra of electron sources are steeper than $\sim P_e^{-3.0}$ and vice versa in the case of Coma, where $P_e$ is an electron momentum. The resultant hard X-ray spectra are flatter when the bremsstrahlung component is dominant. When the spectral indices of the source term are in the intermediate range ($ -2.5 \sim -3.5$), too much extreme ultraviolet emission is produced. Inverse Compton dominant models can reproduce Coma cluster results with reasonable injection rates, which are possible in cluster mergers and/or ambient gas accretion.
description: 11 pages with 6 figures, Accepted for publication in PASJ
The Rhipicephalus appendiculatus tick vector of Theileria parva is absent from cape buffalo (Syncerus caffer) populations and associated ecosystems in northern Uganda
Creators: name: Obara, Isaiah
name: Githaka, N.
name: Nijhof, Ard
name: Krücken, Jürgen
name: Nanteza, A.
name: Odongo, D.
name: Lubembe, D.
name: Atimnedi, Patrick
name: Ahmed, Jabbar S.
name: Clausen, Peter-Henning
Publisher: name: Freie Universität Berlin
Year: 2020
Subjects: subject: T. parva
subject: East Coast fever
subject: R. appendiculatus
subject: Uganda
subject: Cape buffalo
subject: 600 Technik, Medizin, angewandte Wissenschaften::630 Landwirtschaft::630 Landwirtschaft und verwandte Bereiche

description: Rhipicephalus appendiculatus is the major tick vector of Theileria parva, an apicomplexan protozoan parasite that causes the most economically important and lethal disease of cattle in East and central Africa. The African cape buffalo (Syncerus caffer) is the major wildlife host of T. parva from southern Uganda and Kenya to southern Africa. We show herein that R. appendiculatus appears to be absent from the two largest national parks in northern Uganda. Syncerus caffer is common in both of these national parks, specifically Murchison falls (MFNP) and Kidepo Valley (KVNP). We re-confirmed the previously reported absence of T. parva in buffalo sampled in the two northern parks based on RLB data using a nested PCR based on the T. parva p104 gene. By contrast, T. parva-infected R. appendiculatus ticks and parasite-infected buffalo were present in Lake Mburo (LMNP) in South central Uganda. This suggests that the distribution of R. appendiculatus, which is predicted to include the higher rainfall regions of northern Uganda, may be limited by additional, as yet unknown factors.
Lebertia (Lebertia) glabra Thor 1897
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Lebertiidae
Lebertia
Lebertia glabra

description: Lebertia (Lebertia) glabra Thor, 1897
 Lebertia glabra Thor, 1897: E. Angelier et al. 1985: 30.
 Lebertia lineata Thor, 1906: Mota¸s 1927b: 2, 1928e: 4, 1928f: 157; K. Viets 1952c: 245; E. Angelier 1953b: 68; Vaillant 1956: 156; Schwoerbel 1959a: 16; M.-L. Angelier 1980: 13; Smit & Van der Hammen 1992: 55.
 Pseudolebertia glabra (Thor, 1897): Hubault 1927: 98.
 New record. Gard: 0/2/0, Monts du Cantal, rheocrene Buron des Gardes, 45°04’084” N, 2°45’355” E, alt. 1494 m a.s.l., 17.05.2005, leg. H.Smit.
Distribution in France: Gard, Haut-Rhin, IsŁre, Meurthe-et-Moselle, Pas-de-Calais, PyrØnØes (Hautes-PyrØnØes).
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 38, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
On the accretion flow geometry in A0535+26
Creators: name: Ikhsanov, N. R.
name: Larionov, V. M.
name: Beskrovnaya, N. G.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The geometry of accretion flow in the Be/X-ray transient A0535+26 is explored. It is shown that neither moderate nor giant X-ray flaring events observed in the system can be interpreted within the spherically symmetrical accretion model and hence the formation of an accretion disk around the neutron star magnetosphere during the both types of flares is required. The accretion disk can be formed at the periastron if (i) the expansion velocity of the Be star envelope in the equatorial plane is V_wr < 150 km/s and (ii) the parameter accounting for the accretion flow inhomogeneities, xi, satisfies the following condition: xi > 0.16 (Mdot_17)^-1/7, where (Mdot_17)^-1/7 is the rate of mass capture by the neutron star expressed in units of 1017 g/s. We suggest that the `missing' outburst phenomenon can be associated with the spherically symmetrical accretion onto the interchange-stable magnetosphere of the neutron star. The average spin up rate of the neutron star during moderate flares < 3.5 x 10^-12 Hz/s is predicted.
description: 6 pages, published in A&A 372, 227 (2001)
Second Outburst of the Yellow Symbiotic Star LT Delphini
Creators: name: Ikonnikova, N. P.
name: Komissarova, G. V.
name: Arkhipova, V. P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the results of our photoelectric $UBV$ observations of the yellow symbiotic star LT Del over 2010-2018. The binary system LT Del, which consists of a bright K giant and a compact hot star with a temperature of $\sim$100 000 K, has an orbital period of 476 days. In 2017 the variable experienced a second low-amplitude ($ΔV\sim 0.^{m}7$) outburst in the history of its studies whose maximum occurred at an orbital phase of 0.15$\pm$0.05. The outburst duration was $\sim$60 days. The $B-V$ and $U-B$ colors in the outburst became noticeably bluer. A difference in the photometric behavior of the star in the 1994 and 2017 outburst has been detected. In the orbital cycle preceding the 2017 outburst a secondary minimum with a depth of $0.^{m}15$ and $0.^{m}20$ appeared in the $B$ and $V$ light curves, respectively, whose cause is discussed. The phase light and color curves are presented and explained; the position of the star on the color-color diagram is interpreted. We have estimated the parameters of the cool and hot components of the system based on the distance determination from Gaia DR2.
description: 14 pages, 5 figures, 2 tables, accepted for publication in Astronomy Letters
Lebertia intronata Gerecke 2009
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Lebertiidae
Lebertia
Lebertia intronata

description: Lebertia intronata Gerecke, 2009: 72.
Distribution in France: Corsica.
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 38, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Crystallographic orientation dependence of work function: Carbon adsorption on Au surfaces
Creators: name: Jooya, H. Z.
name: Fan, X.
name: McKay, K. S.
name: Pappas, D. P.
name: Hite, D. A.
name: Sadeghpour, H. R.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We investigate the work function (WF) variation of different Au crystallographic surface orientations with carbon atom adsorption. Ab-initio calculations within density-functional theory are performed on carbon deposited (100), (110), and (111) gold surfaces. The WF behavior with carbon coverage for the different surface orientations is explained by the resultant electron charge density distributions. The dynamics of carbon adsorption at sub-to-one-monolayer (ML) coverage depends on the landscape of the potential energy surfaces. At higher ML coverage, because of adsorption saturation, the WF will have weak surface orientation dependence. This systematic study has consequential bearing on studies of electric-field noise emanating from polycrystalline gold ion-trap electrodes that have been largely employed in microfabricated electrodes.
description: 4 pages, 3 figures. arXiv admin note: text overlap with arXiv:1805.06931
Tracing the Mass during Low-Mass Star Formation. III. Models of the Submillimeter Dust Continuum Emission from Class 0 Protostars
Creators: name: Shirley, Yancy L.
name: Evans, Neal J.
name: Rawlings, Jonathan M. C.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Seven Class 0 sources mapped with SCUBA at 850 and 450 micron are modeled using a one dimensional radiative transfer code. The modeling takes into account heating from an internal protostar, heating from the ISRF, realistic beam effects, and chopping to model the normalized intensity profile and spectral energy distribution. Power law density models, n(r) ~ r^{-p}, fit all of the sources; best fit values are mostly p = 1.8 +/- 0.1, but two sources with aspherical emission contours have lower values (p ~ 1.1). Including all sources, = 1.63 +/- 0.33. Based on studies of the sensitivity of the best-fit p to variations in other input parameters, uncertainties in p for an envelope model are Δp = +/- 0.2. If an unresolved source (e.g., a disk) contributes 70% of the flux at the peak, p is lowered in this extreme case and Δp = ^{+0.2}_{-0.6}. The models allow a determination of the internal luminosity ( = 4.0 \lsun) of the central protostar as well as a characteristic dust temperature for mass determination ( = 13.8 +/- 2.4 K). We find that heating from the ISRF strongly affects the shape of the dust temperature profile and the normalized intensity profile, but does not contribute strongly to the overall bolometric luminosity of Class 0 sources. There is little evidence for variation in the dust opacity as a function of distance from the central source. The data are well-fitted by dust opacities for coagulated dust grains with ice mantles (Ossenkopf & Henning 1994). The density profile from an inside-out collapse model (Shu 1977) does not fit the data well, unless the infall radius is set so small as to make the density nearly a power-law.
description: Accepted to ApJ. 28 pages, 13 figures, uses emulateapj5.sty
Preserving π-conjugation in covalently functionalized carbon nanotubes for ptoelectronic applications
Creators: name: Setaro, Antonio
name: Adeli, Mohsen
name: Glaeske, Mareen
name: Przyrembel, Daniel
name: Bisswanger, Timo
name: Gordeev, Georgy
name: Maschietto, Federica
name: Faghani, Abbas
name: Paulus, Beate
name: Weinelt, Martin
name: Arenal, Raúl
name: Haag, Rainer
name: Reich, Stephanie
Publisher: name: Freie Universität Berlin
Year: 2017
Subjects: subject: Carbon nanotubes and fullerenes
subject: Chemical physics
subject: Electronic properties and materials
subject: Synthesis and processing
subject: 500 Naturwissenschaften und Mathematik::530 Physik
subject: 500 Naturwissenschaften und Mathematik::540 Chemie

description: Covalent functionalization tailors carbon nanotubes for a wide range of applications in varying environments. Its strength and stability of attachment come at the price of degrading the carbon nanotubes sp2 network and destroying the tubes electronic and optoelectronic features. Here we present a non- destructive, covalent, gram-scale functionalization of single-walled carbon nanotubes by a new [2+1] cycloaddition. The reaction rebuilds the extended π-network, thereby retaining the outstanding quantum optoelectronic properties of carbon nanotubes, including bright light emission at high degree of functionalization (1 group per 25 carbon atoms). The conjugation method described here opens the way for advanced tailoring nanotubes as demonstrated for light-triggered reversible doping through photochromic molecular switches and nanoplasmonic gold-nanotube hybrids with enhanced infrared light emission.
Pachycrepoideus elongata Delucchi 1955
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Pachycrepoideus
Pachycrepoideus elongata

description: Pachycrepoideus elongata Delucchi (Pteromalidae)
 Pachycrepoideus elongata Delucchi, 1955b: 141. Holotype m, Morocco: Rabat (MHNG [examined]).
 Material. HOLOTYPE m (cp, left antenna, right wings, and right protarsus partly lacking) labelled` Morocco. Rabat 30.X.1928. J. Mimeur. No. 4. [?, illegible]; Ex pupa of Ceratitis capitata.; Pupe Ceratitis capitata W. Figu. [?, illegible] 30.10.28. Rabat.; Coll. FerrieÁre; Pachycrepoideus elongatus [sic] n. sp. V. Delucchi det.; TYPE [red]’. One slide (sc) labelled`40; Pachycrepoideus elongatus [sic] m. elongata antenna m Rabat.; Perixysma [sic] elongata n. antenna m Rabat [pasted over by former label]’ with left antenna (1955b: 140, ®gure 3d) and one slide (sc) labelled`41; (Perixysma) [sic] elongata Del. ala m (Typus) Pachycrepoideus’ with right fore wing of holotype.
 Status. Junior synonym of Pachycrepoideus vindemmiae (Rondani) (Graham, 1969: 847).
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on pages 98-99, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
Decrypting live SSH traffic in virtual environments
Creators: name: McLaren, Peter
name: Russell, Gordon
name: Buchanan, William J.
name: Tan, Zhiyuan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cryptography and Security (cs.CR)
subject: FOS: Computer and information sciences

description: Decrypting and inspecting encrypted malicious communications may assist crime detection and prevention. Access to client or server memory enables the discovery of artefacts required for decrypting secure communications. This paper develops the MemDecrypt framework to investigate the discovery of encrypted artefacts in memory and applies the methodology to decrypting the secure communications of virtual machines. For Secure Shell, used for secure remote server management, file transfer, and tunnelling inter alia, MemDecrypt experiments rapidly yield AES-encrypted details for a live secure file transfer including remote user credentials, transmitted file name and file contents. Thus, MemDecrypt discovers cryptographic artefacts and quickly decrypts live SSH malicious communications including the detection and interception of data exfiltration of confidential data.
Lebertia (Pilolebertia) insignis Neuman 1880
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Lebertiidae
Lebertia
Lebertia insignis

description: Lebertia (Pilolebertia) insignis Neuman, 1880
 Pachygaster tauinsignitus insignis Neuman, 1880: Barrois & Moniez 1887: 21.
 Lebertia insignis Neuman, 1880: Le Roux 1907: 271; Soudan 1920: 4 (?); C. Angelier 1931: 23; E. Angelier et al. 1985: 30; Vinçon 1987: 240.
Distribution in France: Gers, IsŁre, Nord, PyrØnØes (Hautes-PyrØnØes, PyrØnØes-Atlantiques), Haute-Savoie, Val-de-Marne.
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 40, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Are the hotspots of radio galaxies the sites of in-situ acceleration of relativistic particles?
Creators: name: Gopal-Krishna
name: Subramanian, Prasad
name: Wiita, Paul J.
name: Becker, Peter A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using a large set of optically detected hotspots in powerful extragalactic double radio sources, we examine the basic question of whether the detection of optical synchrotron radiation requires in-situ acceleration of relativistic electrons within the hotspots/lobes. For this, we take into account the jet's bulk relativistic motion, as well as its likely misalignment from the plane of the sky. Together, both these factors can drastically reduce the apparent range of the ultra-relativistic electrons ejected from the nucleus in the form of a jet. The conventionally adopted parameter space for the fundamental variables, namely, the hotspot magnetic field, radio source orientation angle relative to the line-of-sight and the bulk speed of the jet plasma, is considered. We find that the observed optical/near-IR synchrotron emission of the hotspots can be explained even if the radiating relativistic electrons were accelerated exclusively within the nuclear region, provided the energy losses incurred by the electrons during their transport down the jet are dominated by inverse Compton upscatterings of the cosmic microwave background photons. Under this circumstance, in-situ acceleration of relativistic electrons inside the hotspots or lobes is not found to be mandated by their reported optical/near-infrared detections.
description: 9 pages, 1 figure, accepted by A&A, minor additions
Additional file 1 of Healthcare workers’ behaviors on infection prevention and control and their determinants during the COVID-19 pandemic: a cross-sectional study based on the theoretical domains framework in Wuhan, China
Creators: name: Yang, Qiuxia
name: Wang, Xuemei
name: Zhou, Qian
name: Tan, Li
name: Zhang, Xinping
name: Lai, Xiaoquan
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1:. Survey of infection prevention and control behaviors among healthcare workers.
Learning big Gaussian Bayesian networks: partition, estimation, and fusion
Creators: name: Gu, Jiaying
name: Zhou, Qing
Publisher: name: arXiv
Year: 2019
Subjects: subject: Machine Learning (stat.ML)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Structure learning of Bayesian networks has always been a challenging problem. Nowadays, massive-size networks with thousands or more of nodes but fewer samples frequently appear in many areas. We develop a divide-and-conquer framework, called partition-estimation-fusion (PEF), for structure learning of such big networks. The proposed method first partitions nodes into clusters, then learns a subgraph on each cluster of nodes, and finally fuses all learned subgraphs into one Bayesian network. The PEF method is designed in a flexible way so that any structure learning method may be used in the second step to learn a subgraph structure as either a DAG or a CPDAG. In the clustering step, we adapt the hierarchical clustering method to automatically choose a proper number of clusters. In the fusion step, we propose a novel hybrid method that sequentially add edges between subgraphs. Extensive numerical experiments demonstrate the competitive performance of our PEF method, in terms of both speed and accuracy compared to existing methods. Our method can improve the accuracy of structure learning by 20% or more, while reducing running time up to two orders-of-magnitude.
description: 26 pages, 2 figures, and 5 tables
Fabrication of thermoresponsive nanogels by thermo-nanoprecipitation and in situ encapsulation of bioactives
Creators: name: Giulbudagian, Michael
name: Asadian-Birjand, Mazdak
name: Steinhilber, Dirk
name: Achazi, Katharina
name: Molina, Maria
name: Calderón, Marcelo
Publisher: name: Freie Universität Berlin
Year: 2015
Subjects: subject: 500 Naturwissenschaften und Mathematik::540 Chemie

description: A synthetic method for thermoresponsive, glycerol based nanogels has been developed. The nanogels were synthesized by nanoprecipitation of the orthogonally functionalized macromonomers and their gelation in water. The crosslinking points were generated by strain promoted azide–alkyne cycloaddition which enabled the in situ encapsulation of Doxorubicin HCl. The mild and surfactant free reaction conditions make these nanogels ideal candidates for biomedical applications.
Evolution of Lithium-Beryllium-Boron and Oxygen in the early Galaxy
Creators: name: Vangioni-Flam, Elisabeth
name: Casse, Michel
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Oxygen is a much better evolutionary index than iron to describe the history of Lithium-Beryllium-Boron (LiBeB) since it is the main producer of these light elements at least in the early Galaxy. The O-Fe relation is crucial to the determination of the exact physical process responsible for the LiBeB production. At low metallicity, if [O/Fe] vs [Fe/H] is flat, then the production mode is independent of the interstellar metallicity, BeB is proportional to oxygen, i.e. is of primary nature. If not, the production mode is function of the progressive enrichment in O of the interstellar medium, BeB varies rather as the square of O, i.e. is of secondary nature. In the first case, fast nuclei enriched into He, C and O injected by supernovae and accelerated in surrounding superbubbles would explain the primary trend. In the second case, the main spallative agent would be the standard galactic cosmic rays. Calculated nucleosynthetic yields of massive stars, estimates of the energy cost of production of beryllium nuclei, and above all recent observations reported in this meeting seem to favor the primary mechanism, at least in the early Galaxy.
description: invited review, IAU Symposium, JD8, Manchester, August 2000, New Astronomy Review, in press 6 pages 1 figure