cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Fading Radio Emission from SN 1961V: Evidence for a Type II Peculiar Supernova?
Creators: name: Stockdale, Christopher J.
name: Rupen, Michael P.
name: Cowan, John J.
name: Chu, You-Hua
name: Jones, Steven S.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using the Very Large Array (VLA), we have detected radio emission from the site of SN 1961V in the Sc galaxy NGC 1058. With a peak flux density of 0.063 +/- 0.008 mJy/beam at 6 cm and 0.147 +/- 0.026 mJy/beam at 18 cm, the source is non-thermal, with a spectral index of -0.79 +/- 0.23. Within errors, this spectral index is the same value reported for previous VLA observations taken in 1984 and 1986. The radio emission at both wavelengths has decayed since the mid 1980's observations with power-law indices of beta(20cm) = -0.69 +/- 0.23 and beta(6cm) = -1.75 +/- 0.16. We discuss the radio properties of this source and compare them with those of Type II radio supernovae and luminous blue variables.
description: 19 pages, 3 figures; To appear in the Astronomical Journal
Lomaptera exquisita SCHURHOFF 1935
Creators: name: Mitter, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cetoniidae
Lomaptera
Lomaptera exquisita

description: Lomaptera exquisita SCHÜRHOFF 1935
M a t e r i a l: Amboua Lodge bei Tari, Papua Neuguinea, 1990, 22 Ex. leg. H. Franz.
Papua-Neuguinea; äusserst variable Art.
description: Published as part of Mitter, H., 2009, Bemerkenswerte Cetoniidae aus der Sammlung von H. Franz im Naturhistorischen Museum Wien (Coleoptera: Cetoniidae), pp. 743-746 in Linzer biologische Beiträge 41 (1) on page 745, DOI: 10.5281/zenodo.5276267
Southern Québec (CA) dissolved organic carbon, environmental, land use/cover and geomorphic data from 1985 to 2019 and R codes associated to performed complete analysis
Creators: name: Dormoy-Boulanger, Jade
name: Guillemette, François
name: Lapierre, Jean-François
Publisher: name: Zenodo
Year: 2025

description: Using publicly available data spanning the past 35 years for 54 tributaries of the St. Lawrence River (Quebec, Canada), we investigated the occurrence and intensity of increasing (or decreasing) DOC concentrations across catchments with diverse geographic features and land uses. Historical DOC trends and other environmental variables were obtained from the Réseau-Rivières (R-R) monitoring program; we selected 89 stations across 54 rivers  monitored between 1985 to 2018. Catchment contour and surface area, as well as the elevation, slope, and latitude were obtained via a collaboration with the Atlas Hydroclimatique du Québec Méridional. We extracted land use information from Agriculture and Agri-food Canada, leveraging the 2019 Quebec crop inventory for the Quebec territory and we leveraged the 2016 New York and Vermont National Land Cover Database (2016 was the latest year available) using catchments contours from the U.S. Geological Survey. Daily precipitations and air temperature were obtained through the Environment and natural resources Canada’s platform. The file named CJFAS is the R code used for all the analysis.

 

 

 
description: Data is displayed half in French half in English. Here is a list of units and abreviations accross files:

superficie.drainee (km2)

pente.moyenne (degree)

altitude.moyenne (m)

latitude.centroid.bv (degree)

station (refering to the Atlas Hydroclimatique du Québec Méridional)

Urban (%)

Forest (%)

Agriculture (%)

Water (%)

Exposed (%) 

grassland (%)

peatland (%)

wetland (%)

station2 (refering to Réseau-Rivières)

column W and X are to be ignored
Derivation of the Euler equations from many-body quantum mechanics
Creators: name: Nachtergaele, Bruno
name: Yau, Horng-Tzer
Publisher: name: arXiv
Year: 2002
Subjects: subject: Mathematical Physics (math-ph)
subject: Analysis of PDEs (math.AP)
subject: FOS: Physical sciences
subject: FOS: Mathematics
subject: 82C10;82C21;82C40

description: The Heisenberg dynamics of the energy, momentum, and particle densities for fermions with short-range pair interactions is shown to converge to the compressible Euler equations in the hydrodynamic limit. The pressure function is given by the standard formula from quantum statistical mechanics with the two-body potential under consideration. Our derivation is based on a quantum version of the entropy method and a suitable quantum virial theorem. No intermediate description, such as a Boltzmann equation or semi-classical approximation, is used in our proof. We require some technical conditions on the dynamics, which can be considered as interesting open problems in their own right.
Additional file 1 of Acute effect of ambient fine particulate matter on heart rate variability: an updated systematic review and meta-analysis of panel studies
Creators: name: Niu, Zhiping
name: Liu, Feifei
name: Li, Baojing
name: Li, Na
name: Yu, Hongmei
name: Wang, Yongbo
name: Tang, Hong
name: Chen, Xiaolu
name: Lu, Yuanan
name: Cheng, Zilu
name: Liu, Suyang
name: Chen, Gongbo
name: Zhang, Yuxiao
name: Xiang, Hao
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1.
Southern Québec (CA) dissolved organic carbon, environmental, land use/cover and geomorphic data from 1985 to 2019 and R codes associated to performed complete analysis
Creators: name: Dormoy-Boulanger, Jade
name: Guillemette, François
name: Lapierre, Jean-François
Publisher: name: Zenodo
Year: 2024

description: Using publicly available data spanning the past 35 years for 54 tributaries of the St. Lawrence River (Quebec, Canada), we investigated the occurrence and intensity of increasing (or decreasing) DOC concentrations across catchments with diverse geographic features and land uses. Historical DOC trends and other environmental variables were obtained from the Réseau-Rivières (R-R) monitoring program; we selected 89 stations across 54 rivers (Figure 1A) monitored between 1985 to 2018. Catchment contour and surface area, as well as the elevation, slope, and latitude were obtained via a collaboration with the Atlas Hydroclimatique du Québec Méridional. We extracted land use information from Agriculture and Agri-food Canada, leveraging the 2019 Quebec crop inventory for the Quebec territory and we leveraged the 2016 New York and Vermont National Land Cover Database (2016 was the latest year available) using catchments contours from the U.S. Geological Survey. Daily precipitations and air temperature were obtained through the Environment and natural resources Canada’s platform. 

 

 

 
description: Data is displayed half in French half in English. Here is a list of units and abreviations accross files:

superficie.drainee (km2)

pente.moyenne (degree)

altitude.moyenne (m)

latitude.centroid.bv (degree)

station (refering to the Atlas Hydroclimatique du Québec Méridional)

Urban (%)

Forest (%)

Agriculture (%)

Water (%)

Exposed (%) 

grassland (%)

peatland (%)

wetland (%)

station2 (refering to Réseau-Rivières)

column W and X are to be ignored
Self-consistent solutions for line-driven winds of hot massive stars. The m-CAK procedure
Creators: name: Gormaz-Matamala, Alex C.
name: Curé, Michel
name: Cidale, Lydia S.
name: Venero, Roberto O. J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Massive stars present strong stellar that which are described by the radiation driven wind theory. Accurate mass-loss rates are necessary to properly describe the stellar evolution across the Hertzsprung--Russel Diagram. We present a self-consistent procedure that coupled the hydrodynamics with calculations of the line-force, giving as results the line-force parameters, the velocity field, and the mass-loss rate. Our calculations contemplate the contribution to the line-force multiplier from more than $\sim 900,000$ atomic transitions, an NLTE radiation flux from the photosphere and a quasi-LTE approximation for the occupational numbers. A full set of line-force parameters for $T_\text{eff}\ge 32,000$ K, surface gravities higher than 3.4 dex for two different metallicities are presented, with their corresponding wind parameters (terminal velocities and mass-loss rates). The already known dependence of line-force parameters on effective temperature is enhanced by the dependence on $\log g$. The terminal velocities present a stepper scaling relation with respect to the escape velocity, this might explain the scatter values observed in the hot side of the bistability jump. Moreover, a comparison of self-consistent mass-loss rates with empirical values shows a good agreement. Self-consistent wind solutions are used as input in FASTWIND to calculate synthetic spectra. We show, comparing with the observed spectra for three stars, that varying the clumping factor, the synthetic spectra rapidly converge into the neighbourhood region of the solution. It is important to stress that our self-consistent procedure significantly reduces the number of free parameters needed to obtain a synthetic spectrum.
Arrenurus (Megaluracarus) buccinator
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Arrenuridae
Arrenurus
Arrenurus buccinator

description: Arrenurus (Megaluracarus) buccinator (Müller, 1776)
 Arrenurus caudatus (Geer, 1778): Moniez 1887a: 162; Barrois & Moniez 1887: 24; Barrois 1889d: 6; K. Viets 1913a: 335; Vandel 1919a: 91; Soudan 1920: 5; Mota¸s 1928e: 28, 1928f: 268, 1928g: 13.
 Megaluracarus caudatus (Geer, 1778): Chaudonneret 1947: 5.
 Arrenurus buccinator (Müller, 1776): Hubault 1947: 217; Smit & Van der Hammen 1992: 56.
 Hydrachna elliptica Müller, 1781: De ThØis 1832: 61.
Distribution in France: Aisne, Alpes-Maritimes, Côte-d’Or, Doubs, Haute-Saône, IsŁre, Nord, Pasde-Calais, 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 79, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Simplified Algorithm for Dynamic Demand Response in Smart Homes Under Smart Grid Environment
Creators: name: Singh, Shashank
name: Namboodiri, Aryesh
name: Selvan, M. P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Under Smart Grid environment, the consumers may respond to incentive--based smart energy tariffs for a particular consumption pattern. Demand Response (DR) is a portfolio of signaling schemes from the utility to the consumers for load shifting/shedding with a given deadline. The signaling schemes include Time--of--Use (ToU) pricing, Maximum Demand Limit (MDL) signals etc. This paper proposes a DR algorithm which schedules the operation of home appliances/loads through a minimization problem. The category of loads and their operational timings in a day have been considered as the operational parameters of the system. These operational parameters determine the dynamic priority of a load, which is an intermediate step of this algorithm. The ToU pricing, MDL signals, and the dynamic priority of loads are the constraints in this formulated minimization problem, which yields an optimal schedule of operation for each participating load within the consumer provided duration. The objective is to flatten the daily load curve of a smart home by distributing the operation of its appliances in possible low--price intervals without violating the MDL constraint. This proposed algorithm is simulated in MATLAB environment against various test cases. The obtained results are plotted to depict significant monetary savings and flattened load curves.
description: This paper was accepted and presented in 2019 IEEE PES GTD Grand International Conference and Exposition Asia (GTD Asia). Furthermore, the conference proceedings has been published in IEEE Xplore
Additional file 12 of Intricate genetic variation networks control the adventitious root growth angle in apple
Creators: name: Zheng, Caixia
name: Shen, Fei
name: Wang, Yi
name: Wu, Ting
name: Xu, Xuefeng
name: Zhang, Xinzhong
name: Han, Zhenhai
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 12: Supplementary File 4 Sequence alignment of MdLBD41 cloned from apple rootstocks ‘BC’ and ‘M9’. (A) CDS. (B) Amino acid. (C) Upstream.
Arrenurus (Megaluracarus) conicus Piersig 1894
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Arrenuridae
Arrenurus
Arrenurus conicus

description: Arrenurus (Megaluracarus) conicus Piersig, 1894
 Arrenurus conicus Piersig, 1894: Mota¸s 1927b: 3, 1928e: 29, 1928f: 267, 1928g: 15; C. Angelier 1950d: 358, 1951b: 74; C. & E. Angelier 1953a: 73.
Distribution in France: IsŁre, PyrØnØes (PyrØnØes-Orientales, 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 79, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Discovery of a 2 Kpc Binary Quasar
Creators: name: Shields, G. A.
name: Junkkarinen, V.
name: Beaver, E. A.
name: Burbidge, E. M.
name: Cohen, R. D.
name: Hamann, F.
name: Lyons, R. W.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: LBQS 0103$-$2753 is a binary quasar with a separation of only 0.3 arcsec. The projected spacing of 2.3 kpc at the distance of the source (z = 0.848) is much smaller than that of any other known binary QSO. The binary nature is demonstrated by the very different spectra of the two components and the low probability of a chance pairing. LBQS 0103$-$2753 presumably is a galaxy merger with a small physical separation between the two supermassive black holes. Such objects may provide important constraints on the evolution of binary black holes and the fueling of AGN.
description: 6 pages LATEX with 2 EPS figures; uses epsfig, aipproc. Proceedings of the 20th Texas Symposium on Relativistic Astrophysics, ed. J. C. Wheeler and H. Martel, American Institute of Physics, in press (2001)
News Media Coverage of Climate Change in India 1997–2016: Using Automated Content Analysis to Assess Themes and Topics
Creators: name: Keller, Tobias R.
name: Hase, Valerie
name: Jagadish Thaker
name: Mahl, Daniela
name: Schäfer, Mike S.
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Plant Biology

description: News media play an important role for public awareness and perception of climate change – and thus citizens’ behavior. Few studies focus on media coverage in poor and developing countries such as India – the third-largest polluter and an important player in global climate change policies. Further, even these few studies on Indian media coverage span short time periods, focus on specific events, and evaluate pre-defined themes. Applying LDA topic modeling on 18,224 climate change articles published between 1997 and 2016 in two Indian newspapers, we find that climate change coverage in India has increased substantially in the last 20 years. We categorized the coverage into 28 different topics related to four overarching themes: “Climate Change Impacts”, “Climate Science”, “Climate Politics”, and “Climate Change and Society”. Climate change has gained more media attention since 2007 in general with a particular increase in focus on the theme “Climate Change Impacts”. Implications about shifting media discourses and its potential to educate people and change policies are discussed.
Oplostomus fuligineus
Creators: name: Mitter, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cetoniidae
Oplostomus
Oplostomus fuligineus

description: Oplostomus fuligineus (OLIVIER 1789)
M a t e r i a l: Rinosterpoort b. Bronkhorstspruit, Transvaal, 1 Ex. (undatiert), leg. H. Franz.
Kenya, Senegal.
description: Published as part of Mitter, H., 2009, Bemerkenswerte Cetoniidae aus der Sammlung von H. Franz im Naturhistorischen Museum Wien (Coleoptera: Cetoniidae), pp. 743-746 in Linzer biologische Beiträge 41 (1) on page 745, DOI: 10.5281/zenodo.5276267
Sirex juvencus
Creators: name: Schedl, W.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Siricidae
Sirex
Sirex juvencus

description: Sirex juvencus (LINNAEUS 1758)
M a t e r i a l:? Ex. Isla de la Palma (Canarias) siehe CEBALLOS (1963 p. 62). Diese Holzwespen-Art wurde als Nachweis für die Kanarischen Inseln bisher in BÁEZ & ORTEGA (1978) und in ILZQUIERDO et al. (2001) nicht erfasst.
 B i o l o g i e: Larven leben in Symbiose mit dem Pilz Stereum chailletii (PERS.) im Holz von fast allen Koniferen, am häufigsten in Pinus spp., Abies spp., in Ostkanada hauptsächlich in der Balsamtanne, in Australien importiert in Fichte (Picea sp.) (EICHHORN 1982).
V e r b r e i t u n g:Holarktische,mitBau-oderBrennholz importierte Art!
description: Published as part of Schedl, W., 2009, Neunachweise und derzeitiger Faunenbestand von Pflanzenwespen der Kanarischen Inseln II (Insecta: Hymenoptera: Symphyta), pp. 753-757 in Linzer biologische Beiträge 41 (1) on page 754, DOI: 10.5281/zenodo.5276269
Arrenurus (Micruracarus) bifidicodulus Piersig 1897
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Arrenuridae
Arrenurus
Arrenurus bifidicodulus

description: Arrenurus (Micruracarus) bifidicodulus Piersig, 1897
 Arrenurus (Micruracarus) bifidicodulus Piersig, 1897: K. Viets 1913a: 335; Soudan 1920: 5; Mota¸s 1928f: 270; Brumpt 1929: 293; C. Angelier 1953: 229.
 Micruracarus bifidicodulus (Piersig, 1897): Chaudonneret 1947: 5 (laps. bifidicadulus).
Distribution in France: Côte-d’Or, IsŁre, Manche, Savoie.
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 81, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Role of the sonic scale in the growth of magnetic field in compressible turbulence
Creators: name: Fouxon, Itzhak
name: Mond, Michael
Publisher: name: arXiv
Year: 2019
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We study the growth of small fluctuations of magnetic field in supersonic turbulence, the small-scale dynamo. The growth is due to the fastest turbulent eddies above the resistive scale. We observe that for supersonic turbulence these eddies are effectively incompressible which creates a robust structure of the growth. The eddies are localised below the sonic scale $l_s$ defined as the scale where the typical velocity of the turbulent eddies equals the speed of sound. Thus the flow below $l_s$ is effectively incompressible and the field growth proceeds as in incompressible flow. At large Mach numbers $l_s$ is much smaller than the integral scale of turbulence so the fastest growing mode of the magnetic field belongs to small-scale turbulence. We derive this mode and the associated growth rate numerically in a white noise in time model of turbulence. The relevance of this model relies on considering evolution time larger than the correlation time of turbulence.
description: 5 pages, 2 figures
Velocity Structure of the ISM as Seen by the Spectral Correlation Function
Creators: name: Ballesteros-Paredes, Javier
name: Vazquez-Semadeni, Enrique
name: Goodman, Alyssa A.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (Abridged) We use the statistical tool known as the ``Spectral Correlation Function" [SCF] to intercompare simulations and observations of the atomic interstellar medium. The simulations considered mimic three distinct sets of physical conditions. One of them (run "ISM") is intended to represent a mixture of cool and warm atomic gas, and includes self-gravity and magnetic fields. For each simulation, H I spectral-line maps are synthesized and intercompared, both with each other, and with observations, using the SCF. We find that, when thermal broadening is large in comparison with fine-scale turbulent velocity structure, it masks sub-thermal velocity sub-structure in the synthesized spectra. The H I observations we use here for comparison are of the North Celestial Pole (NCP) Loop. None of the simulations match the NCP Loop data very well. The most realistic sets of line profiles and SCF statistics comes from artifically rescaling the velocity axis of run ISM. Without rescaling, almost all velocity structure is smeared out by thermal broadening. However, if the velocity axis is expanded by a factor of 6, the SCF distributions of run ISM an the NCP Loop match up fairly well. This means that the ratio of thermal to turbulent pressure in run ISM is much too large as it stands, and that the simulation is deficient in turbulent energy. This is a consequence of run ISM not including the effects of supernovae. We conclude that the SCF is a useful tool for understanding and fine-tuning simulations of interstellar gas, and in particular that realistic simulations of the atomic ISM need to include the effects of energetic stellar winds (e.g. supernovae) in order for the ratio of thermal-to-turbulent pressure to give spectra representative of the observed interstellar medium in our Galaxy.
description: 25 pages, 24 figures. ApJ Accepted (May 20). Also available at: ftp://www.astrosmo.unam.mx/pub/j.ballesteros/Papers/
Corynis sanguinea
Creators: name: Schedl, W.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Cimbicidae
Corynis
Corynis sanguinea

description: Corynis sanguinea (VOLLENHOVEN 1876)
M a t e r i a l: 1♀ Fuerteventura-Nord, östlich von Vallebrón, ca. 250 m, 10.2.2002, von Ruderalflora gestreift, leg., in coll. et det. W. Sch. 2002. Von dort schon von anderen Autoren 62-20 Jahre früher festgestellt; 4♀♀ Gran Canaria, 2 km westlich Tasartico, 27°56‘ N 15°49‘ E, 18.2.2002, leg. Schmidd-Egger (1♀ in coll. Schmid-Egger, 2♀♀ in coll. M. Kraus, 1♀ in coll. W. Schedl), det. M. Kraus.
B i o l o g i e: Larven und Wirtspflanze(n) unbekannt.
V e r b r e i t u n g Von den Kanaren schon seit den Aufsammlungen von Wollaston (1869-85), von Marokko, Algerien und Tunesien bekannt (BENSON 1968; SCHEDL 1979).
description: Published as part of Schedl, W., 2009, Neunachweise und derzeitiger Faunenbestand von Pflanzenwespen der Kanarischen Inseln II (Insecta: Hymenoptera: Symphyta), pp. 753-757 in Linzer biologische Beiträge 41 (1) on page 754, DOI: 10.5281/zenodo.5276269
Comet Hazard to the Earth
Creators: name: Ipatov, S. I.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Migration of trans-Neptunian objects to the Earth is considered. Due to the gravitational influence of large trans-Neptunian objects and mutual collisions, some objects can get such orbits, from which they can be moved inside the Solar System under the gravitational influence of planets. About 10-20% or even more 1-km Earth-crossers could have come from the Edgeworth-Kuiper belt and can move in Jupiter-crossing orbits. The number of former trans-Neptunian objects that cross the Earth's orbit moving in orbits with aphelia inside Jupiter's orbit can be of the same order of magnitude. A total mass of icy planetesimals delivered to the Earth during formation of the giant planets can be about the mass of the Earth's oceans.
description: 12 pages, in press in "Advances in Space Research" (Proc. of COSPAR-2000, Warsaw)
Arrenurus (Micruracarus) bipapillosus Halbert 1911
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Arrenuridae
Arrenurus
Arrenurus bipapillosus

description: Arrenurus (Micruracarus) bipapillosus Halbert, 1911
 Arrenurus bipapillosus Halbert, 1911: Walter & Mota¸s 1927: 155; Mota¸s 1927b: 3, 1928f: 277, 1928g: 7; LØger & Mota¸s 1928a: 176; C. Angelier 1951b: 77; 1953: 229; C. & E. Angelier 1953a: 74; Smit et al. 2000: 239.
Distribution in France: Corsica, PyrØnØes (PyrØnØes-Orientales), Savoie, Var.
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 81, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
LOCC protocols with bounded width per round optimize convex functions
Creators: name: Leung, Debbie
name: Winter, Andreas
name: Yu, Nengkun
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We start with the task of discriminating finitely many multipartite quantum states using LOCC protocols, with the goal to optimize the probability of correctly identifying the state. We provide two different methods to show that finitely many measurement outcomes in every step are sufficient for approaching the optimal probability of discrimination. In the first method, each measurement of an optimal LOCC protocol, applied to a $d_{\rm loc}$-dim local system, is replaced by one with at most $2d_{\rm loc}^2$ outcomes, without changing the probability of success. In the second method, we decompose any LOCC protocol into a convex combination of a number of "slim protocols" in which each measurement applied to a $d_{\rm loc}$-dim local system has at most $d_{\rm loc}^2$ outcomes. To maximize any convex functions in LOCC (including the probability of state discrimination or fidelity of state transformation), an optimal protocol can be replaced by the best slim protocol in the convex decomposition without using shared randomness. For either method, the bound on the number of outcomes per measurement is independent of the global dimension, the number of parties, the depth of the protocol, how deep the measurement is located, and applies to LOCC protocols with infinite rounds, and the "measurement compression" can be done "top-down" -- independent of later operations in the LOCC protocol. The second method can be generalized to implement LOCC instruments with finitely many outcomes: if the instrument has $n$ coarse-grained final measurement outcomes, global input dimension $D_0$ and global output dimension $D_i$ for $i=1,...,n$ conditioned on the $i$-th outcome, then one can obtain the instrument as a convex combination of no more than $R=\sum_{i=1}^n D_0^2 D_i^2 - D_0^2 + 1$ slim protocols; in other words, $\log_2 R$ bits of shared randomess suffice.
description: see related results by Scott Cohen
Molecular gas in NGC6946
Creators: name: Walsh, W.
name: Beck, R.
name: Thuma, G.
name: Weiss, A.
name: Wielebinski, R.
name: Dumke, M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present imaging of molecular gas emission in the star-forming spiral galaxy NGC6946. Our CO(1-0) and CO(3-2) images, made at 22" resolution with the IRAM 30-m and the Heinrich Hertz 10-m radio telescopes, are the most extensive CO observations of this galaxy and are among the most extensive observations of molecular gas in any spiral galaxy. The molecular component in NGC6946 is unusually massive, with a ratio of molecular to atomic Hydrogen of 0.57. A star formation efficiency image for NGC6946 ranges by over two orders of magnitude with highest values found in the northeastern spiral arm, and anticorrelates with the 6cm polarized emission image, which traces the regular part of the magnetic field. We analyse the ISM in NGC6946's disk by making 1-D and 2-D comparisons of images made in several wavebands. A point-by-point correlation technique finds that the molecular gas is closely associated with the 7micron-emitting dust. The high correlation found between the MIR emission and the radio continuum at 6cm cannot be due to dust heating and gas ionization in star-forming regions because the thermal radio emission is less correlated with the MIR than the nonthermal emission. A coupling of magnetic fields to gas clouds is proposed as a possible scenario.
description: A&A accepted, 23 pages, 11 figures. Version with high resolution figures available at: http://cfa-www.harvard.edu/~wwalsh/sp.html
NGC 1705 and the evolution of blue compact dwarf galaxies
Creators: name: Meurer, Hans-Gerhardt R
Publisher: name: The Australian National University
Year: 1989
Subjects: subject: Dwarf galaxies
subject: Galaxies Evolution

description: This thesis presents a multi-waveband study of the amorphous galaxy NGC 1705. It is shown to be a nearby (D « 5 Mpc for Hq = 75 kms-1 Mpc-1) nucleated blue compact dwarf (BCD) galaxy. Its emission line spectrum is like that seen in typical emission line galaxies, with an oxygen abundance like that of the LMC. NGC 1705 contains two stellar populations: a central high surface brightness (HSB) population, a kpc in diameter, which is actively forming stars, and a lower surface brightness (LSB) population with an exponential distribution of light, which is also a star forming population around 3 Gyr old. The HSB population of NGC 1705 defines its BCD morphology. It is a region of relatively continuous star formation at least 50 Myr old; about a Gyr old if the star formation rate has remained constant. Embedded objects within the boundaries of the HSB population are manifestations of its recent star formation. These objects include star clusters, some of which are ionizing sources, and perhaps individual supergiant stars. The brightest object is the unresolved off-centre nucleus which is probably a young (13 Myr old) globular cluster with a mass of of ~ 1.5 x 106 Mq. In the light of Ha, NGC 1705 has a bipolar morphology, with the axis of the flow roughly along the continuum minor axis. The expulsive nature of this flow is confirmed by the emission line kinematics, which show velocity splits of around 100 kms-1 over much of the face of the galaxy. A comparison of the integrated Ha and HI velocity profiles indicates that the neutral material is probably entrained in this flow. A simple expansion model is constructed and found to yield an expansion time-scale on the order of the age of the nucleus for any likely set of its free parameters. A comparison of the estimated mechanical energy release of the nucleus, HSB and LSB populations, and that required for the flow confirms that the nucleus provides the largest fraction of the energy required for the flow. It is shown that velocities greater than the escape velocity have already been achieved in the flow, and thus NGC 1705 is losing mass in a galactic wind. This result holds for all mass to light ratios expected for BCD’s, and is not sensitive to details of the flow geometry. The possible evolutionary outcomes from this mass loss includes complete destruction of the galaxy, if the total mass to light ratio is low (MT / LB
Elinora canariensis SCHEDL 1979
Creators: name: Schedl, W.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Tenthredinidae
Elinora
Elinora canariensis

description: Elinora canariensis SCHEDL 1979
M a t e r i a l: 2♀♀ Fuerteventura Nord, östlich Vallebrón, ca 250 m, 10.2.2002, von Ruderalflora gestreift, leg., in coll. et det. W. Sch. 2002.
 B i o l o g i e: Das Typenmaterial wurde von Marcos Báez auf Lanzerotte, Los Valles, 20.- 23.2.1979 von der Cruciferae Sisymbrium sp. gestreift. Ob sich die Larven auch an dieser Pflanze entwickelt, ist unbekannt.
V e r b r e i t u n g endemische Art der Kanaren von Lanzerotte und Fuertoventura (SCHEDL 1979; ORTEGA & BÁEZ 1996).
description: Published as part of Schedl, W., 2009, Neunachweise und derzeitiger Faunenbestand von Pflanzenwespen der Kanarischen Inseln II (Insecta: Hymenoptera: Symphyta), pp. 753-757 in Linzer biologische Beiträge 41 (1) on pages 754-755, DOI: 10.5281/zenodo.5276269
Asymptotic behavior for a Schrödinger equation with nonlinear subcritical dissipation
Creators: name: Cazenave, Thierry
name: Han, Zheng
Publisher: name: arXiv
Year: 2019
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35Q55, 35B40

description: We study the time-asymptotic behavior of solutions of the Schrödinger equation with nonlinear dissipation \begin{equation*} \partial _t u = i Δu + λ|u|^αu \end{equation*} in ${\mathbb R}^N $, $N\geq1$, where $λ\in {\mathbb C}$, $\Re λ<0$ and $0
Ecologías de aprendizaje en estudiantes con discapacidades
Creators: name: Tabuenca, Bernardo
name: Rodrigo, Covadonga
Publisher: name: figshare
Year: 2019
Subjects: subject: 130306 Educational Technology and Computing
subject: FOS: Educational sciences

description: Se pueden distinguir cinco ecologías de aprendizaje en estudiantes con discapacidad basadas en las diferencias sensoriales y limitaciones que presenta cada discapacidad. Al presentar cada ecología, se resumen las dificultades inherentes a cada diversidad funcional. Además se presentan herramientas de apoyo o soluciones tecnológicas que ayudan a afrontar dichas barreras.
Arrenurus (Micruracarus) forpicatus Neuman 1880
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Arrenuridae
Arrenurus
Arrenurus forpicatus

description: Arrenurus (Micruracarus) forpicatus Neuman, 1880
 Arrenurus (Micruracarus) forpicatus Neuman, 1880: Vandel 1919a: 91 (laps. forcipatus); Mota¸s 1928f: 278; C. Angelier 1953: 227; C. & E. Angelier 1953a: 74.
Distribution in France: Doubs, Jura, PyrØnØes (PyrØnØes-Orientales), Savoie.
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 81, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Calameuta pygmaea
Creators: name: Schedl, W.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Tenthredinidae
Calameuta
Calameuta pygmaea

description: Calameuta pygmaea (PODA 1761)
M a t e r i a l: 1♀ 13 Fuerteventura Nord, Vallebrón, 15.2. 2002, 300 m; 1♀ oberhalb Vallebrón, 400 m, von Ruderalfläche mit Getreidehalmen (z. B. Hafer); 1♀ 13 unterhalb Vallebrón, 200 m, von Ruderalwiese mit Grashalmen gestreift, alle leg., in coll. et det. W.Sch. 2003; 1♀ 233 Fuerteventura Mitte West, Vega del Rio Palma, 300 m, 12.2.2002, von Ruderalflora und Gräsern im Bachbett gestreift (1♀ fliegend entkommen), leg., in coll. et det. W. Sch. 2003.
B i o l o g i e: Larven in Stengeln von Gramineen (BENSON 1955).
V e r b r e i t u n g SW-Europa, N-Afrika, Israel, (BENSON 1968; MUCHE 1981), Balearen, Kanaren (SCHEDL 1987).
description: Published as part of Schedl, W., 2009, Neunachweise und derzeitiger Faunenbestand von Pflanzenwespen der Kanarischen Inseln II (Insecta: Hymenoptera: Symphyta), pp. 753-757 in Linzer biologische Beiträge 41 (1) on page 755, DOI: 10.5281/zenodo.5276269
The truncation of stellar discs: the magnetic hypothesis
Creators: name: Battaner, E.
name: Florido, E.
name: Jimenez-Vicente, J.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We propose a hypothesis of the truncation of stellar discs based on the magnetic model of the rotation curve of spiral galaxies. Once the disc had formed and acquired its present structure, approximately, three balanced forces were acting on the initial gas: gravity and magnetic forces, inwards, and centrifugal force. When stars are formed from this gas, the magnetic force is suddenly suppressed. Gravitation alone cannot retain the newly-formed stars and at birth places beyond a certain galactocentric radius they escape to intergalactic space. This radius is the so-called ``truncation radius'', which is predicted to be at about 4-5 disc radial scale lengths, in promising agreement with observations.
description: 6 pages, accepted for publication in Astronomy and Astrophysics Replaced using new A&A style
Ornstein-Zernike Theory for the finite range Ising models above T_c
Creators: name: Campanino, M.
name: Ioffe, D.
name: Velenik, Y.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Probability (math.PR)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 60F15, 60K15, 60K35, 82B20, 37C30

description: We derive precise Ornstein-Zernike asymptotic formula for the decay of the two-point function in the general context of finite range Ising type models on Z^d. The proof relies in an essential way on the a-priori knowledge of the strict exponential decay of the two-point function and, by the sharp characterization of phase transition due to Aizenman, Barsky and Fernandez, goes through in the whole of the high temperature region T > T_c. As a byproduct we obtain that for every T > T_c, the inverse correlation length is an analytic and strictly convex function of direction.
description: 36 pages, 5 figures
String theory on $\boldsymbol{\text{AdS}_{\mathbf{3}}}$ and the symmetric orbifold of Liouville theory
Creators: name: Eberhardt, Lorenz
name: Gaberdiel, Matthias R.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: For string theory on AdS$_3$ with pure NS-NS flux a complete set of DDF operators is constructed, from which one can read off the symmetry algebra of the spacetime CFT. Together with an analysis of the spacetime spectrum, this allows us to show that the CFT dual of superstring theory on ${\rm AdS}_3 \times {\rm S}^3 \times \mathbb{T}^4$ for generic NS-NS flux is the symmetric orbifold of $({\cal N}=4$ Liouville theory$)\times \mathbb{T}^4$. For the case of minimal flux ($k=1$), the Liouville factor disappears, and we just obtain the symmetric orbifold of $\mathbb{T}^4$, thereby giving further support to a previous claim. We also show that a similar analysis can be done for bosonic string theory on ${\rm AdS}_3 \times X$.
description: 33+10 pages
Phytotoxic metabolites produced by Verticillium dahliae Kleb. in olive wilting: a chemical and spectroscopic approach for their molecular characterisation
Creators: name: D’Orazio, Valeria
name: Stallone, Domenico
name: Sermani Samer
name: Loffredo, Elisabetta
name: Cirulli, Matteo
name: Bruno, Giovanni Luigi
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biochemistry
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Inorganic Chemistry
subject: Plant Biology

description: Most of the symptoms associated with Verticillium wilt disease in olive cultivation are due to complexes excreted by Verticillium dahliae. In this study chemical and physico-chemical techniques were combined to investigate how the molecular structure of phytotoxins isolated from two pathotypes of Verticillium dahliae, defoliating, D, and non-defoliating, ND, grown on two different media, Verticillium-dahliae-Medium (VdM) and Simulated Xylem-fluid-Medium (SXM), can affect their aggressiveness. Data obtained highlight important structural differences, both in term of elemental composition and in functional groups distribution. Such peculiarities strongly affect their solubility, resulted higher for the phytotoxins from D pathotype. This property likely induces serious modifications of the conformational state of the proteinaceous component, making tyrosine residues accessible to the phosphate ion. A phosphorylation mechanism would thus be promoted, that is going to interfere with the function of the involved proteins in intracellular signalling networks, likely by altering its role in modulating the plant’s response.
Design, synthesis and biological evaluation of N-substituted α-hydroxyimides and 1,2,3-oxathiazolidine-4-one-2,2-dioxides with anticonvulsant activity
Creators: name: Sabatier, Laureano L.
name: Palestro, Pablo H.
name: Enrique, Andrea V.
name: Pastore, Valentina
name: Sbaraglini, María L.
name: Martín, Pedro
name: Gavernet, Luciana
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified

description: In this investigation, we studied a family of compounds with an oxathiazolidine-4-one-2,2-dioxide skeleton and their amide synthetic precursors as new anticonvulsant drugs. The cyclic structures were synthesized using a three-step protocol that include solvent-free reactions and microwave-assisted heating. The compounds were tested in vivo through maximal electroshock seizure test in mice. All the structures showed activity at the lower doses tested (30 mg/Kg) and no signs of neurotoxicity were detected. Compound encoded as 1g displayed strong anticonvulsant effects in comparison with known anticonvulsants (ED50 = 29 mg/Kg). First approximations about the mechanisms of action of the cyclic structures were proposed by docking simulations and in vitro assays against sodium channels (patch clamp methods).
Arrenurus (Micruracarus) integrator
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Arrenuridae
Arrenurus
Arrenurus integrator

description: Arrenurus (Micruracarus) integrator (Müller, 1776)
 Arrenurus (Micruracarus) integrator (Müller, 1776): Barrois & Moniez 1887: 25 (?, possibly A. bifidicodulus, see K. Viets 1956); Mota¸s 1928f: 270; C. Angelier 1953: 229.
 Micruracarus integrator (Müller, 1776): Chaudonneret 1947: 5.
Distribution in France: Côte-d’Or, Nord, Savoie.
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 81, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Disk Diffusion Propagation Model for the Outburst of XTE J1118+480
Creators: name: Wood, Kent S.
name: Titarchuk, Lev
name: Ray, Paul S.
name: Wolff, Michael T.
name: Lovellette, Michael N.
name: Bandyopadhyay, Reba M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a linear diffusion model for the evolution of the double-peaked outburst in the transient source XTEJ1118+480. The model treats the two outbursts as episodic mass deposition at the outer radius of the disk followed by evolution of disk structure according to a diffusion process. We demonstrate that light curves with fast-rise, exponential decay profile are a general consequence of the diffusion process. Deconvolution of the light curve proves to be feasible and gives an input function specifying mass deposition at the outer disk edge as well as the total mass of the disk, both as functions of time. The derived evolution of total disk mass can be correlated with the observed evolution of the ~0.1 Hz QPO in the source reported in Wood et al. (2000).
description: 26 pages, 6 figures, accepted for publication in ApJ
Campsiura scutellaris
Creators: name: Mitter, H.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cetoniidae
Campsiura
Campsiura scutellaris

description: Campsiura scutellaris (GORY & PERCHERON 1833)
M a t e r i a l: Hann b. Dakar, Senegal, 1963, 1 Ex. leg. H. Franz.
Äthiopien, Senegal, Sierra Leone.
description: Published as part of Mitter, H., 2009, Bemerkenswerte Cetoniidae aus der Sammlung von H. Franz im Naturhistorischen Museum Wien (Coleoptera: Cetoniidae), pp. 743-746 in Linzer biologische Beiträge 41 (1) on page 745, DOI: 10.5281/zenodo.5276267
Pre-distortion and Pre-equalization for Non-Linearities and Low-Pass Effect Mitigation in OFDM-VLC Systems
Creators: name: Mathias, Luis Carlos
name: Filho, Jose Carlos Marinello
name: Abrao, Taufik
Publisher: name: arXiv
Year: 2019
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: The orthogonal frequency division multiplexing (OFDM) transmission has shown promise in applications of visible light communication (VLC). However, the variation of the nonlinearity of the optical power emitted by the high power light emitting diode (HPLED) as a function of current and temperature implies in drastic OFDM-VLC performance degradation. The first part of this work, experimentally confirms and models this degradation due to temperature in a high power white HPLED. The higher attenuation at high frequencies, which is inherent to the HPLED and which is accentuated by the effect of the intrinsic capacitance of the photodiode, is another factor of degradation due to the reduction of the signal-to-noise ratio (SNR) at the receiver for such frequencies. For the mitigation of these effects, we propose a pre-distortion and digital pre-equalization scheme using a luminous feedback signal in the transmitter module. The system is modeled so that the operating points are mathematically deduced and evaluated by simulations and by an experimental setup. By allowing the linearization of the transmitted light signal and the maintenance of an average SNR in all OFDM subcarriers, the performance improvement is confirmed in comparison with other schemes, such as with non-predistortion, pre-distortion with fixed parameters, and simple post-equalization.
description: 25 pages, 14 figures, 2 tables
Arrenurus (Micruracarus) octagonus Halbert 1906
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Arrenuridae
Arrenurus
Arrenurus octagonus

description: Arrenurus (Micruracarus) octagonus Halbert, 1906
 New record. Indre: 0/1/0, Étang Nuret, La Brenne, 46°47’30.57" N 1°12’35.98" E, 9 July 2000, leg. H. van der Hammen.
Distribution in France: Indre. New for the fauna of France.
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 pages 81-82, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293