cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A comparison of three ways to measure time-dependent densities with quantum simulators
Creators: name: Yang, Jun
name: Brown, James
name: Whitfield, James Daniel
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum algorithms are touted as a way around some classically intractable problems such as the simulation of quantum mechanics. At the end of all quantum algorithms is a quantum measurement whereby classical data is extracted and utilized. In fact, many of the modern hybrid-classical approaches are essentially quantum measurements of states with short quantum circuit descriptions. Here, we compare and examine three methods of extracting the time-dependent one-particle probability density from a quantum simulation: direct $Z$-measurement, Bayesian phase estimation and harmonic inversion. We have tested these methods in the context of the potential inversion problem of time-dependent density functional theory. Our test results suggest that direct measurement is the preferable method. We also highlight areas where the other two methods may be useful and report on tests using Rigetti's quantum virtual device. This study provides a starting point for imminent applications of quantum computing.
Philisca robusta Soto & Ramírez 2012, new species
Creators: name: Soto, Eduardo M.
name: Ramírez, Martín J.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Anyphaenidae
Philisca
Philisca robusta

description: Philisca robusta new species
Figs 27, 31a, 33a, b
 Type material: Holotype female from Chile, Región V (Valparaíso), Juan Fernandez Archipelago, Robinson Crusoe Island, Villagra valley, 23–24.IV.1962, B. Malkin (AMNH; temporary preparations EMS-00028–33, EMS-00309).
 Etymology: The specific name is a Latin word referring to the robust appearance of this species, with square carapace and short legs.
 Diagnosis: It resembles other species of the ornata group by the modified male chelicerae and the epigyne with smooth, heart shaped median field close to the epigastric furrow (Fig. 33a, b). It can be easily distinguished by the prosoma almost square, with approximately the same width along the length of the prosoma.
 Description: Female (holotype): Total length 9.44. Prosoma length 3.99, width 3.19. Tibia/metatarsus length: I, 2.26/2.13; II, 2.26/2.13; III, 1.86/2.00; IV, 2.53/3.06. Chelicerae with three teeth (middle tooth larger) on promargin and three on retromargin (basal tooth larger). Sternum length 2.00, width 1.60. Spines: leg I, femur d 1–1–1, p 2ap; tibia v 0–2–p1; metatarsus v 2bas. II, femur d 1–1–1, p and r 1ap; tibia v 0–r1–2 or 0–2–2, p 0–1 or 0; metatarsus v 2bas or 2–p1–0, p 1–0. III, femur d 1–1–1, p and r d1ap; patella r d1; tibia v 0–p1–2 or p1–p1–2, d r1bas, p and r d1– 1; metatarsus v 2–p1–2, d 0–p1–2, p and r d1–1–1. IV, femur d 1–1–1, p and r d1ap; patella r 1; tibia v p1–2–2, d r1– 0–1, p and r 1–1; metatarsus v 2–2–2, d 0–p1–2, p and r d1–1–1. Opisthosoma length 5.05, epigastrium–spiracle 2.39, spiracle–spinnerets 0.80. Color in ethanol (Fig. 27): Prosoma and chelicerae reddish brown. Sternum brown. Legs yellowish brown. Opistosoma light yellowish brown, with dorsal and ventral brown pattern. Epigyne large, very sclerotized and weakly translucent (Fig. 33a). MF heart-shaped. MF smooth, heart-shaped, close to the epigastric furrow. Anterior pouch wide, with short lumen. AB at the sides of the spermathecae. Spermathecae separated by a diameter (Fig. 33b). Females and immatures have thick setae on the base of ALS (Fig. 31a).
 Variability: Spines in females: I, tibia v 0–1–p1. II, femur r 0; tibia v 0–r1–p1. III, tibia d 0; metatarsus v 2– 0–2. IV, tibia v p1–p1–2; metatarsus v 2–p1–2.
 Distribution: Known only from the Juan Fernández Archipelago, Isla Robinson Crusoe, Chile.
 Other material examined:  CHILE: Región V (Valparaíso):  Valparaíso Prov.: Juan Fernández Archipelago, Robinson Crusoe Island, Villagra Valley, 2 females [plus 4 immatures]; 23–24.IV.1962, B. Malkin (AMNH).
description: Published as part of Soto, Eduardo M. & Ramírez, Martín J., 2012, Revision and phylogenetic analysis of the spider genus Philisca Simon (Araneae: Anyphaenidae, Amaurobioidinae) 3443, pp. 1-65 in Zootaxa 3443 (1) on page 46, DOI: 10.11646/zootaxa.3443.1.1, http://zenodo.org/record/5254614
REPRODUCTIVE PROGRAM - THE BASE OF MODERN ORGANISATION OF AGRARIAN - INDUSTRIAL COMPLEX
Creators: name: Markovic, Zivko
name: Markovic, Zivko
Publisher: name: Unknown
Year: 2006
Subjects: subject: Livestock Production/Industries
subject: Production Economics
subject: reproductive agrarian-industrial program
subject: equivalent exchange
subject: cooperative organisation

description: The base of modern organisation of agrarian-industrial complex of Serbia should consist of reproductive agrarian-industrial programms. Production capacities should adapt to these agrarian-industrial programms. Agrarian-industrial complex could be successfully constituted only if the appropriate labor sharing is done in accordance with reproductive program. Economic relationships should be established in such a way that each subjekt has economical benefits from the common labor. These economical benefits should correspond to individual contribution of each subjekt to work successfully and well. Reproductive economical connections for realizing agrarian-industrial program requires flexible organisation which is based on cooperative principles. These principles make the free unification of totaly independent economic subjects possible.
Forcipomyia (Forcipomyia) genualis
Creators: name: William L. Grogan, Jr.
name: Hribar, Lawrence J.
name: Murphree, C. Steven
name: Cilek, James E.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ceratopogonidae
Forcipomyia
Forcipomyia genualis

description: Forcipomyia (Forcipomyia) genualis (Loew)
 Ceratopogon genualis Loew, 1866: 128 (Cuba).
 Forcipomyia (Forcipomyia) genualis: Johannsen 1943: 777 (combination); Wirth 1965: 125 (in Nearctic catalog); Wilkening et al. 1985: 516 (Florida records); Borkent and Grogan 2009: 7 (in Nearctic catalog; distribution).
 Discussion. Wilkening et al. (1985) recorded this primarily Neotropical species from nine counties in Florida. We provide the first records from Alachua and Lake counties.
 New records. Alachua Co., Gainesville, Oak Crest, 1-X/ 22-XI-1986, W. W. Wirth, UVLT, 5 females (FSCA). Lake Co., nr. Mt. Dora, 9-VIII-1984, R. E. Woodruff & L. A. Stange, UVLT, 1 female (FSCA).
description: Published as part of William L. Grogan, Jr., Hribar, Lawrence J., Murphree, C. Steven & Cilek, James E., 2010, New records of biting and predaceous midges from Florida, including species new to the fauna of the United States (Diptera: Ceratopogonidae), pp. 1-59 in Insecta Mundi 2010 (147) on page 12, DOI: 10.5281/zenodo.5352908
Variation of mass accretion rate onto the white dwarf in the dwarf nova VW Hyi in quiescence
Creators: name: Nakaniwa, Nozomi
name: Hayashi, Takayuki
name: Takeo, Mai
name: Ishida, Manabu
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We have analysed a series of Suzaku data and one dataset of XMM-Newton of the SU UMa type dwarf nova VW Hyi in optical quiescence. The observed spectra in the 0.2-10 keV band are moderately well represented by multi-temperature thermal plasma emission models with a maximum temperature of 5-9 keV and bolometric luminosity of 2.4-5.2 $\times$ 10$^{30}$ erg s$^{-1}$. The mass accretion rate derived from the hard X-ray spectra does not show any clear trend as a function of time since the last superoutburst, in contradiction to theoretical predictions of the disc behaviour of a SU UMa type dwarf nova. The mass accretion rate, on the other hand, shows a clear declining trend with time since the last outburst (including the superoutburst). The rate of decline is of the same order as that evaluated from the hard X-ray light curves of the other two dwarf novae SS Cyg and SU UMa. The standard disc instability model, on the other hand, predicts that the mass accretion rate should increase throughout the optically-quiescent phase. We need further observation and theoretical consideration to resolve this discrepancy.
description: 11 pages, 7 figures, accepted for publication in Monthly Notices of the Royal Astronomical Society Main Journal
Culama australis Walker 1856
Creators: name: Kallies, Axel
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Cossidae
Culama
Culama australis

description: Culama australis Walker, 1856
(Figs 1, 2, 9–11, 13, 40, 41, 56, 62, 80, 144, 161)
description: Published as part of Kallies, Axel, 2012, Revision of Cossinae and small Zeuzerinae from Australia (Lepidoptera: Cossidae) 3454, pp. 1-62 in Zootaxa 3454 (1) on page 6, DOI: 10.11646/zootaxa.3454.1.1, http://zenodo.org/record/5254709
TRANSITION OF AGRICULTURE IN THE REPUBLIC OF SERBIA - achievements, effects and limitations -
Creators: name: Pejanovic, Radovan
name: Milanovic, Milan R.
name: Cvijanovic, Drago
name: Pejanovic, Radovan
name: Milanovic, Milan R.
name: Cvijanovic, Drago
Publisher: name: Unknown
Year: 2006
Subjects: subject: Agricultural and Food Policy
subject: Risk and Uncertainty
subject: transition
subject: crisis
subject: agriculture
subject: agrarian policy
subject: resistance to changes and limitations

description: The authors consider the current issues of the transition of agriculture in the Republic of Serbia, its achievements, effects and limitations. According to their opinion, the transitional reforms, so far, have not had the anticipated positive effects. The causes lie in the system. It is manifested in different ways: the developing instability of agriculture; unfavourable agrarian structure and decrease in productivity; decline of competitiveness; inefficiency of agrarian policy; the decrease in population and deterioration of villages; growing resistance to changes. The authors propose the measures and activities for overcoming the existing status, as to make the transition more efficient and bearable.
The Oldest Stars of the Extremely Metal-Poor Local Group Dwarf Irregular Galaxy Leo A
Creators: name: Schulte-Ladbeck, Regina E.
name: Hopp, Ulrich
name: Drozdovsky, Igor O.
name: Greggio, Laura
name: Crone, Mary M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present deep Hubble Space Telescope single-star photometry of Leo A in B, V, and I. Our new field of view is offset from the centrally located field observed by Tolstoy et al. (1998) in order to expose the halo population of this galaxy. We report the detection of metal-poor red horizontal branch stars, which demonstrate that Leo A is not a young galaxy. In fact, Leo A is as least as old as metal-poor Galactic Globular Clusters which exhibit red horizontal branches, and are considered to have a minimum age of about 9 Gyr. We discuss the distance to Leo A, and perform an extensive comparison of the data with stellar isochrones. For a distance modulus of 24.5, the data are better than 50% complete down to absolute magnitudes of 2 or more. We can easily identify stars with metallicities between 0.0001 and 0.0004, and ages between about 5 and 10 Gyr, in their post-main-sequence phases, but lack the detection of main-sequence turnoffs which would provide unambiguous proof of ancient (>10 Gyr) stellar generations. Blue horizontal branch stars are above the detection limits, but difficult to distinguish from young stars with similar colors and magnitudes. Synthetic color-magnitude diagrams show it is possible to populate the blue horizontal branch in the halo of Leo A. The models also suggest ~50% of the total astrated mass in our pointing to be attributed to an ancient (>10 Gyr) stellar population. We conclude that Leo A started to form stars at least about 9 Gyr ago. Leo A exhibits an extremely low oxygen abundance, of only 3% of Solar, in its ionized interstellar medium. The existence of old stars in this very oxygen-deficient galaxy illustrates that a low oxygen abundance does not preclude a history of early star formation.
description: 44 pages, 18 figures, accepted for publication in the August 2002 issue of AJ. High resolution figures is available at http://www.astro.spbu.ru/staff/dio/preprints.html
Additional file 4 of A Bayesian non-inferiority approach using expertsâ margin elicitation â application to the monitoring of safety events
Creators: name: Aupiais, Camille
name: Alberti, Corinne
name: Schmitz, Thomas
name: Baud, Olivier
name: Ursino, Moreno
name: Zohar, Sarah
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Plots of posterior class a and class b misclassifications according to the stopping thresholds for each of the 13 pairs of priors. The plots analogous to Fig.Â 3 for the 3 other events: (a) Death, (b) Necrotizing enterocolitis, (c) Retinopathy. (PDF 2969 kb)
Forcipomyia (Forcipomyia) pictoni Macfie 1938
Creators: name: William L. Grogan, Jr.
name: Hribar, Lawrence J.
name: Murphree, C. Steven
name: Cilek, James E.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ceratopogonidae
Forcipomyia
Forcipomyia pictoni

description: Forcipomyia (Forcipomyia) pictoni Macfie
 Forcipomyia pictoni Macfie, 1938: 161 (Trinidad).
 Forcipomyia (Forcipomyia) pictoni: Wirth 1974: 6 (in New World catalog south of USA; distribution); Wilkening et al. 1985: 516 (Florida records); Borkent and Grogan 2009: 7 (in Nearctic catalog; distribution).
 Discussion. Wilkening et al. (1985) recorded this widely distributed New World species from 14 Florida counties. We provide the first records from Dade Co.
 New records. Dade Co., Homestead, 17-X-1984, R. Woodruff & L. Stange, UVLT, 3 males (FSCA).
description: Published as part of William L. Grogan, Jr., Hribar, Lawrence J., Murphree, C. Steven & Cilek, James E., 2010, New records of biting and predaceous midges from Florida, including species new to the fauna of the United States (Diptera: Ceratopogonidae), pp. 1-59 in Insecta Mundi 2010 (147) on page 12, DOI: 10.5281/zenodo.5352908
Multichannel remote polarization control enabled by nanostructured Liquid Crystalline Networks
Creators: name: Zanotto, Simone
name: Sgrignuoli, Fabrizio
name: Nocentini, Sara
name: Martella, Daniele
name: Parmigiani, Camilla
name: Wiersma, Diederik S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optics (physics.optics)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: In this article we demonstrate that a grating fabricated through nanoscale volumetric crosslinking of a liquid crystalline polymer enables remote polarization control over the diffracted channels. This functionality is a consequence of the responsivity of liquid crystal networks upon light stimuli. Tuning the photonic response of the device is obtained thanks to both a refractive index and a shape change of the grating elements induced by a molecular rearrangement under irradiation. In particular, the material anisotropy allows for nontrivial polarization state management over multiple beams. Absence of any liquid component and a time response down to 0.2 milliseconds make our device appealing in the fields of polarimetry and optical communications.
description: 16 pages,8 figures, featured article in ALP
Culama anthracica Kallies 2012, sp. nov.
Creators: name: Kallies, Axel
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Cossidae
Culama
Culama anthracica

description: Culama anthracica sp. nov.
(Figs 3, 4, 12, 42, 57, 63, 145, 146, 162)
 Literature. Zborovski & Edwards 2007: p. 92 (as C. australis); Yakovlev 2010: p. 102, Figs 1, 2 (as C. australis); Yakovlev 2011: p. 9, color plate 1, Fig. 5 (as C. australis).
description: Published as part of Kallies, Axel, 2012, Revision of Cossinae and small Zeuzerinae from Australia (Lepidoptera: Cossidae) 3454, pp. 1-62 in Zootaxa 3454 (1) on page 9, DOI: 10.11646/zootaxa.3454.1.1, http://zenodo.org/record/5254709
Galaxy evolution and environment: the cluster view at z < 1
Creators: name: Poggianti, Bianca Maria
Publisher: name: Zenodo
Year: 2021

description: This talk focuses on what we have learned about galaxy evolution from large spectroscopic surveys of galaxy clusters at z<1. Multi-object spectroscopy and integral-field spectroscopy have been at the core of our progress in understanding the physical processes that govern galaxy evolution before and after galaxies become part of a cluster, in their journey through different environments. In addition, the most massive haloes in the universe are the best sites to study those environmental effects (ram pressure stripping, strangulation, harassment) that are most -- but not uniquely -- efficient in clusters. Milestones of cluster spectroscopic surveys include studies of the mass assembly, star formation histories and structure (morphologies and sizes) of galaxies. I will focus on some of the observational highlights, and the outstanding questions.
Forcipomyia (Forcipomyia) quatei : Wirth 1965
Creators: name: William L. Grogan, Jr.
name: Hribar, Lawrence J.
name: Murphree, C. Steven
name: Cilek, James E.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ceratopogonidae
Forcipomyia
Forcipomyia quatei

description: Forcipomyia (Forcipomyia) quatei Wirth
 Forcipomyia quatei Wirth, 1952a: 142 (California).
 Forcipomyia (Forcipomyia) quatei: Wirth 1965: 126 (in Nearctic catalog); Wilkening et al. 1985: 516 (Florida records); Borkent and Grogan 2009: 7 (in Nearctic catalog; distribution).
 Discussion. Wilkening et al. (1985) recorded this wide ranging New World species from 12 counties in Florida. We discovered a large series of this species in the FSCA from Indian River, Highlands and St. Lucie counties, which are the first records from these counties.
 New records. Highlands Co., Archbold Biol. Sta., 13-19-April-1989, W. W. Wirth, light trap, 2 females, 1 male; same data except Lake Placid, 1-IV-1990, at UV light, 2 females, 1 male (FSCA). Indian River Co., Fellesmere, 17-III-1956, LT, 1 male; Vero Beach, Ent. Res. Cntr., May 1958 - Dec. 1960, light trap, 16 females, 36 males (FSCA). St. Lucie Co. (no locality given), 11-VI-1986, R. L. Escher, C. F. PETA, 1 female; same data except 18 March-27 May 1987, 3 females (FSCA).
description: Published as part of William L. Grogan, Jr., Hribar, Lawrence J., Murphree, C. Steven & Cilek, James E., 2010, New records of biting and predaceous midges from Florida, including species new to the fauna of the United States (Diptera: Ceratopogonidae), pp. 1-59 in Insecta Mundi 2010 (147) on pages 12-13, DOI: 10.5281/zenodo.5352908
MACROECONOMIC EFFICIENCY MEASUREMENT OF THE INVESTED FUNDS INTO A RURAL AREA OR SECTOR WITH A METHOD OF A CAPITAL COEFFICIENT
Creators: name: Popovic, Goran
name: Popovic, Goran
Publisher: name: Unknown
Year: 2006
Subjects: subject: Agricultural Finance
subject: Community/Rural/Urban Development
subject: International Relations/Trade
subject: capital coefficients
subject: investments
subject: efficiency
subject: rural development
subject: sustainable development
subject: country price

description: Macroeconomic efficiency analysis of the investment is one of the definite economic area. The efficiency in creation and development implementation does not imply only sufficient investment sum, but also the efficiently of their use. The relation of the investment and a realized GDP or for example a capital relation, fixed funds respectively, according to a realized inputs, we call them the capital coefficients. They express the macroeconomic efficiency of the invested funds into a certain area or sector. The capital coefficients can appear also as the constituents of the more composite developed models. Their use is important for the efficiency valuation of the adopted decision by the central, regional and local institucions, that conduct the policy and the measures of the sustainable and integral rural development. The capital coefficients of the rural area we can calculate as the territorial and sector ones, the approximate and marginal ones, the usual and tehnological ones, and the coefficients to gross or not base. Their circulation in a rural complex understand the certain specifications, the analysis of the important subbefects in the investment process and the accumulation of the fixed funds respectively. This is particulary related to the changes of the country prices in the circulation, as a result of the long-standing investments into the sustainable development and the rural areas.
Ab-Initio Solution of the Many-Electron Schrödinger Equation with Deep Neural Networks
Creators: name: Pfau, David
name: Spencer, James S.
name: Matthews, Alexander G. de G.
name: Foulkes, W. M. C.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Machine Learning (cs.LG)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: Given access to accurate solutions of the many-electron Schrödinger equation, nearly all chemistry could be derived from first principles. Exact wavefunctions of interesting chemical systems are out of reach because they are NP-hard to compute in general, but approximations can be found using polynomially-scaling algorithms. The key challenge for many of these algorithms is the choice of wavefunction approximation, or Ansatz, which must trade off between efficiency and accuracy. Neural networks have shown impressive power as accurate practical function approximators and promise as a compact wavefunction Ansatz for spin systems, but problems in electronic structure require wavefunctions that obey Fermi-Dirac statistics. Here we introduce a novel deep learning architecture, the Fermionic Neural Network, as a powerful wavefunction Ansatz for many-electron systems. The Fermionic Neural Network is able to achieve accuracy beyond other variational quantum Monte Carlo Ansätze on a variety of atoms and small molecules. Using no data other than atomic positions and charges, we predict the dissociation curves of the nitrogen molecule and hydrogen chain, two challenging strongly-correlated systems, to significantly higher accuracy than the coupled cluster method, widely considered the most accurate scalable method for quantum chemistry at equilibrium geometry. This demonstrates that deep neural networks can improve the accuracy of variational quantum Monte Carlo to the point where it outperforms other ab-initio quantum chemistry methods, opening the possibility of accurate direct optimization of wavefunctions for previously intractable many-electron systems.
description: Final proof for Physical Review Research
STRENGTHENING THE ROLE OF THE MARKET AND FURTHER DEVELOPMENT OF ACTIVE MACROECONOMIC POLICY
Creators: name: Cocovic-Krstic, Mirjana
name: Cocovic-Krstic, Mirjana
Publisher: name: Unknown
Year: 2006
Subjects: subject: Financial Economics
subject: International Relations/Trade
subject: Public Economics
subject: market
subject: law of value
subject: economic policy
subject: monetary-credit policy
subject: fiscal policy
subject: economic growth
subject: employment
subject: inflation
subject: development strategy
subject: complementarity
subject: coordination
subject: synchronization
subject: restructuring
subject: privatization
subject: competiition
subject: economic solvency
subject: macroeconomic stability
subject: European union

description: In the process of transition and globalization, the creation of an efficient system of economic activities has to be based on the market- oriented economy and adequate measures of economic policy. The strengthening and enlargement of the role of the market and economic laws becomes a need all the more as the market is the best factor of valuation of all values. However, economy cannot show optimal economic results if it rests only on the market. It requires certain measures of macroeconomic policy in the field of economic activities, employment, price stability, that is, inflation and problems regarding foreign economy. The starting point for economic policy should be the market and the market effects, in the sense that it corrects or removes its randomness, adjusts the development and contributes to efficiency and rationality. Therefore, the existence of certain lavel of complementarity between the market and economic policy is very important for accomplishing development strategy, that is for rational and successful economic activities Of the same importance is the coordination and intergration of monetarycredit and fiscal policy(.public revenue and tax policy). The instruments of economic policy, monetary and fiscal policy, are two economic disciplines, only two parts, two sub-systems of the inique financial policy. Joint activity of monetary and fiscal policy becomes a necessity – the law of modern finances. What is needed is that both policies are complementary and at the same time used with other partial policies in order to accomplish stability in the broadest sense of the word. The strategy for successful economic reforms in our economy has to be aimed at strengthening the competittion in tne market, at making more decisive steps towards market reforms, privatization administration and judicial reform, and all this in accordance with legal and administrative standards of the European Union. In other words, our economy needs new investments, a clearly-stated development strategy, more rapid growth of industrial development, new technologies and repositioning in the market in order to achieve a better position compared to our competition and more dynamuc marketing in the foreign market. The aim of all these activities is macroeconomic stability and joining the European Union.
Point-nonpoint emissions trading for Minnesota River phosphorus
Creators: name: Johansson, Robert Charles
name: Johansson, Robert Charles
Publisher: name: Unknown
Year: 2000
Subjects: Agricultural and Food Policy
Environmental Economics and Policy
Land Economics/Use

description: A thesis submitted to the faculty of the Graduate School of the University of Minnesota in partial fulfillment of the requirements for the degree of Doctor of Philosophy. Advisor: Jay Coggins
Where we stand on structure dependence of ISGMR in the Zr-Mo region: Implications on K_\infty
Creators: name: Howard, K. B.
name: Garg, U.
name: Gupta, Y. K.
name: Harakeh, M. N.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Isoscalar giant resonances, being the archetypal forms of collective nuclear behavior, have been studied extensively for decades with the goal of constraining bulk nuclear properties of the equation of state, as well as for modeling dynamical behaviors within stellar environments. An important such mode is the isoscalar electric giant monopole resonance (ISGMR) that can be understood as a radially symmetric density vibration within the saturated nuclear volume. The field has a few key open questions, which have been proposed and remain unresolved. One of the more provocative questions is the extra high-energy strength in the $A\approx 90$ region, which manifested in large percentages of the $E0$ sum rule in $^{92}$Zr and $^{92}$Mo above the main ISGMR peak. The purpose of this article is to introduce these questions within the context of experimental investigations into the phenomena in the zirconium and molybdenum isotopic chains, and to address, via a discussion of previously published and preliminary results, the implications of recent experimental efforts on extraction of the nuclear incompressibility from this data.
description: 9 pages, 7 figures, invited to be submitted to a special issue of EPJA honoring Prof. P. F. Bortignon
Additional file 1 of Sorafenib and triptolide loaded cancer cell-platelet hybrid membrane-camouflaged liquid crystalline lipid nanoparticles for the treatment of hepatocellular carcinoma
Creators: name: Li, Zhe
name: Yang, Gang
name: Han, Lu
name: Wang, Rong
name: Gong, Chunai
name: Yuan, Yongfang
Publisher: name: figshare
Year: 2021
Subjects: Biophysics
Space Science
Physical Sciences not elsewhere classified
Medicine
Cell Biology
Pharmacology
Biotechnology
Biological Sciences not elsewhere classified
Cancer

description: Additional file 1: Fig. S1. Stability of (SFN+TPL)@LCNPs and (SFN+TPL)@CPLCNPs in plasma (n=3). As shown in Fig. S1, the particle size of (SFN+TPL)@LCNPs and (SFN+TPL)@CPLCNPs did not change significantly after 72 h in plasma, and still remained stable, indicating that the preparation had good stability and no precipitation or aggregation occurred. Table S1. The concentrations of SFN and TPL at a 50% inhibition rate against Huh-7 cells for different combinations and the corresponding CI (n=3)
New physics effects on quantum coherence in neutrino oscillations
Creators: name: Dixit, Khushboo
name: Alok, Ashutosh Kumar
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Several measures of quantum correlations such as Leggett-Garg and Bell-type inequalities have been extensively studied in the context of neutrino oscillations. However these analyses are performed under the assumption of standard model (SM) interactions of neutrinos. In this work we study new physics effects on $l_1$-norm based measure of quantum coherence which quantifies the quantumness embedded in the system and is also intrinsically related to various measures of quantum correlations. Moreover, it is considered to be a resource theoretical tool which can be utilized in quantum algorithms and quantum channel discrimination. The new physics effects are incorporated in a model independent way by using the effective Lagrangian for the neutral current non-standard neutrino interactions (NSI). Bounds on the NSI parameters are extracted from a recent global analysis of oscillation experiments including COHERENT (coherent neutrino-nucleus scattering experiment) data. In the context of upcoming DUNE experimental setup, we find that the most favourable combination of LMA-Light sector of $θ_{12}$ (i.e., $θ_{12}< 45^o$) with normal mass ordering decreases the coherence in the system in comparison to the SM prediction for all values of neutrino energy E and CP violating phase $δ$ (except in the narrow region around E ~ 2 GeV). On the other hand, a large enhancement in the value of coherence parameter in the entire $(E-δ)$ plane is possible for the dark octant of $θ_{12}$ ($θ_{12}> 45^o$) with inverted ordering. For almost all values of CP violating phase, the enhancement is more protuberant in the region around E ~ 4 GeV where maximum neutrino flux is expected in the DUNE experiment. Therefore for the normal mass ordering, the SM interaction provides favourable conditions for quantum information tasks while the NSI favours inverted ordering scenario for such tasks.
description: 8 pages, 2 figures; Matches published version
The weak imprint of environment on the stellar populations of galaxies
Creators: name: Trussler, James
Publisher: name: Zenodo
Year: 2021

description: Leveraging on the statistical power of the SDSS, and by separating starforming, green valley and passive galaxies, I will show that the imprint of environment on the stellar populations of galaxies is much weaker than previously thought. Satellite galaxies are in fact only marginally more metal-rich (<0.03 dex) and older (<0.5 Gyr) than central galaxies of the same stellar mass, with stellar metallicities that show only a weak dependence (<0.05 dex) on the density of the environment within which satellites reside. Thus, while the environment plays a crucial role in the quenching of star formation in galaxies, it only plays a minor role in shaping the properties of star-forming and passive galaxies. Furthermore, by comparing the levels of chemical enrichment in star-forming and passive galaxies, I will show that it is in fact starvation (rather than gas stripping) that becomes progressively more important in quenching star formation in satellites in progressively denser environments.
Accountability and sustainability of Estonian local governments: An analysis of legal acts
Creators: name: Roostalu, Lea
name: Roostalu, Lea
Publisher: name: Unknown
Year: 2012
Subjects: subject: Political Economy
subject: Public Economics
subject: CSR (corporate social responsibility)
subject: local government
subject: public sector management
subject: social capital
subject: sustainability reporting
subject: value creation

description: This case study examines the challenges of the legal area of Estonia in supporting the corporate social responsibility and sustainability of local government by analyzing the main legal acts regulating the activities of this level of government. Both qualitative and quantitative content analyses were used. As a result of the study an original model describing sustainability orientation within the bodies of legal acts was designed. Taken together, the findings of the study suggest an actual and ever-growing role for public sector management in fostering social capital and promoting sustainability reporting within private, public and third sector organizations.
The impact of real exchange rate volatility on economic growth: Kenyan evidence
Creators: name: Musyoki, Danson
name: Pokhariyal, Ganesh P.
name: Pundo, Moses
name: Musyoki, Danson
name: Pokhariyal, Ganesh P.
name: Pundo, Moses
Publisher: name: Unknown
Year: 2012
Subjects: subject: Financial Economics
subject: Public Economics
subject: Real exchange rate
subject: nominal exchange rate
subject: real effective exchange rate
subject: nominal effective exchange rate
subject: volatility
subject: GARCH

description: This paper examines the impact of real exchange rate volatility on economic growth in Kenyan. The study employed the Generalized Autoregressive Condition of Heteroscedasticity (GARCH) and computation of the unconditional standard deviation of the changes to measure volatility and Generalized Method Moments (GMM) to assess the impact of the real exchange rate volatility on economic growth for the period January 1993 to December 2009. Data for the study was collected from Kenya National Bureau of Statistics, Central Bank of Kenya and International Monetary Fund Data Base by taking monthly frequency. The study found that RER was very volatility for the entire study period. Kenya’s RER generally exhibited a appreciating and volatility trend, implying that in general, the country’s international competitiveness deteriorated over the study period. The RER Volatility reflected a negative impact on economic growth of Kenya.
A burst from the direction of UZ Fornacis with XMM-Newton
Creators: name: Still, Martin
name: Mukai, Koji
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The XMM-Newton pointing towards the magnetic cataclysmic variable UZ For finds the source to be a factor > 10^3 fainter than previous EXOSAT and ROSAT observations. The source was not detected for the majority of a 22 ksec exposure with the EPIC cameras, suggesting that the accretion rate either decreased, or stopped altogether. However a 1.1 ksec burst was detected from UZ For during the observation. Spectral fits favour optically thin, kT = 4.4 keV thermal emission. Detection of the burst by the on-board Optical Monitor indicates that this was most probably an accretion event. The 0.1-10 keV luminosity of 2.1 x 10^30 erg/s is typical for accretion shock emission from high state polars and would result from the potential energy release of ~ 10^16 g of gas. There is no significant soft excess due to reprocessing in the white dwarf atmosphere.
description: 7 pages, 2 postscript figures, ApJL, in press
Culama dasythrix Turner 1945
Creators: name: Kallies, Axel
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Cossidae
Culama
Culama dasythrix

description: Culama dasythrix Turner, 1945
(Figs 6, 44, 166)
description: Published as part of Kallies, Axel, 2012, Revision of Cossinae and small Zeuzerinae from Australia (Lepidoptera: Cossidae) 3454, pp. 1-62 in Zootaxa 3454 (1) on page 11, DOI: 10.11646/zootaxa.3454.1.1, http://zenodo.org/record/5254709
Forcipomyia (Forcipomyia) swezeyana Tokunaga and Murachi
Creators: name: William L. Grogan, Jr.
name: Hribar, Lawrence J.
name: Murphree, C. Steven
name: Cilek, James E.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ceratopogonidae
Forcipomyia
Forcipomyia swezeyana

description: Forcipomyia (Forcipomyia) swezeyana Tokunaga and Murachi
 Forcipomyia (Forcipomyia) swezeyana Tokunaga and Murachi, 1959: 145 (Guam, Tinian, Palau); Debenham 1987: 303 (Australia); Wirth and Spinelli 1992c: 599 (Florida records).
 Discussion. As noted by Wirth and Spinelli (1992c), F. swezeyana belongs to an Old World complex that Debenham (1987) termed the “ swezeyana Group”, several members of which have been reared from tropical plants (bananas, cassava, etc.). Wirth and Spinelli (1992c) suggested that this was probably how this species was introduced into Florida, and listed specimens from Dade, Orange and Palm Beach counties, all but one of which were reared from portions of decaying banana and Philodendron.
description: Published as part of William L. Grogan, Jr., Hribar, Lawrence J., Murphree, C. Steven & Cilek, James E., 2010, New records of biting and predaceous midges from Florida, including species new to the fauna of the United States (Diptera: Ceratopogonidae), pp. 1-59 in Insecta Mundi 2010 (147) on page 13, DOI: 10.5281/zenodo.5352908
AGN activity and star formation of optically-selected Type II AGN in VIMOS spectroscopic surveys
Creators: name: Vietri, Giustina
name: Garilli, B.
name: Polletta, M.
name: Bisogni, S.
name: Cassarà, L.
name: Franzetti, P.
name: Fumana, M.
name: Gargiulo, A.
name: Mancini, C.
name: Scodeggio, M.
Publisher: name: Zenodo
Year: 2021

description: Using a large (812) sample of optically-selected Type II AGN at redshift range 0.510ˆ10 Msun) exhibit low level of SF activity. For both populations we find a positive correlation between the AGN power, probed by the [OIII] luminosity, and SF MS offset, which could reflect the co-evolutionary path between the AGN and SF, with a common gas supply which both triggers SF and fuels the AGN activity. Moreover, I will discuss the possible effect of AGN feedback on the SF content of luminous and massive host galaxies, as suggested by the presence of outflowing gas traced by the [OIII] emission line.
The Ingot Wavefront Sensor: Updates from the Laboratory Test Bench
Creators: name: Gomes Machado, Tania Sofia
name: Di Filippo, Simone
name: Bergomi, Maria
name: Radhakrishnan, Kalyan
name: Greggio, Davide
name: Portaluri, Elisa
name: Arcidiacono, Carmelo
name: Viotto, Valentina
name: Ragazzoni, Roberto
name: Dima, Marco
name: Marafatto, Luca
name: Farinato, Jacopo
name: Magrin, Demetrio
Publisher: name: Proceedings of AO4ELT7 conference 2023 - Editors: Thierry Fusco and Benoit Neichel
Year: 2023
Subjects: EXTENDED SOURCES
SODIUM LASER GUIDE STAR
LGS
ADAPTIVE OPTICS
WAVEFRONT SENSING
INGOT WFS
ELT
WAVEFRONT SENSOR

description: Sodium LGS let Adaptive Optics (AO) systems dramatically increase the sky coverage, but at the same time, they suffer from some limitations imposed by their natural geometry, which differently from natural guide stars, are not point-like sources but more elongated objects in the sky. The Ingot WFS is a possible solution to overcome these limitations increasing the performance of the AO system. In this work, we report the status of the laboratory activities performed at the INAF Osservatorio Astronomico di Padova, in which we have developed a test bench working in an open loop scenario, which aims to investigate the behavior of the Ingot WFS both in terms of the LGS variation in the sky, and on the sensitivity. In this framework, we show the results obtained with a robust and automatic Python-code alignment procedure of the Ingot WFS with respect to the movements and density profile variations of the simulated LGS source.
Culama suffusca Kallies 2012, sp. nov.
Creators: name: Kallies, Axel
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Cossidae
Culama
Culama suffusca

description: Culama suffusca sp. nov.
(Figs 7, 8, 14, 45, 59, 65, 81, 147, 163)
description: Published as part of Kallies, Axel, 2012, Revision of Cossinae and small Zeuzerinae from Australia (Lepidoptera: Cossidae) 3454, pp. 1-62 in Zootaxa 3454 (1) on page 12, DOI: 10.11646/zootaxa.3454.1.1, http://zenodo.org/record/5254709
The impact of working capital on the value of the company in light of differing size, growth, and debt
Creators: name: Sabri, Tamer Bahjat
name: Sabri, Tamer Bahjat
Publisher: name: Unknown
Year: 2012
Subjects: subject: Financial Economics
subject: Industrial Organization
subject: Tobin's Q
subject: working capital
subject: company size
subject: company growth
subject: leverage

description: This study investigates the potential effect of the working capital management on the value of the industrial companies in Jordan, by studying determinants (company size, company growth, leverage) that affect company value measured by Tobin's Q (TQ). Also it uses an improved methodology to produce three indexes (benchmarks) that can present the suitable information for mangers and investors. To achieve the objectives of the study, a sample constituted by forty-one (41) industrial companies was studied. The study covered the period from 2000 to 2007. Regression analysis and Mann-Whitney-U Test were used to test the hypotheses of the study. The results shows that R2 for small size companies is higher than big size companies. And it is noted that the average TQ for companies with big size is higher than the average for small-sized companies.
An excursion set model of hierarchical clustering: Ellipsoidal collapse and the moving barrier
Creators: name: Sheth, Ravi K.
name: Tormen, Giuseppe
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The excursion set approach allows one to estimate the abundance and spatial distribution of virialized dark matter haloes efficiently and accurately. The predictions of this approach depend on how the nonlinear processes of collapse and virialization are modelled. We present simple analytic approximations which allow us to compare the excursion set predictions associated with spherical and ellipsoidal collapse. In particular, we present formulae for the universal unconditional mass function of bound objects and the conditional mass function which describes the mass function of the progenitors of haloes in a given mass range today. We show that the ellipsoidal collapse based moving barrier model provides a better description of what we measure in the numerical simulations than the spherical collapse based constant barrier model, although the agreement between model and simulations is better at large lookback times. Our results for the conditional mass function can be used to compute accurate approximations to the local-density mass function which quantifies the tendency for massive haloes to populate denser regions than less massive haloes. This happens because low density regions can be thought of as being collapsed haloes viewed at large lookback times, whereas high density regions are collapsed haloes viewed at small lookback times. Although we have only applied our analytic formulae to two simple barrier shapes, we show that they are, in fact, accurate for a wide variety of moving barriers. We suggest how they can be used to study the case in which the initial dark matter distribution is not completely cold.
description: 18 pages, submitted to MNRAS
The Stochastic Feynman-Hellmann Method
Creators: name: Gambhir, Arjun Singh
name: Berkowitz, Evan
name: Brantley, David
name: Chang, Chia Cheng
name: Clark, M. A.
name: Kurth, Thorsten
name: Monahan, Chris
name: Nicholson, Amy
name: Vranas, Pavlos
name: Walker-Loud, André
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: The Feynman-Hellmann method, as implemented by Bouchard et al. [1612.06963], was recently employed successfully to determine the nucleon axial charge. A limitation of the method was the restriction to a single operator and a single momentum during the computation of each "Feynman- Hellmann" propagator. By using stochastic techniques to estimate the all-to-all propagator, we relax this constraint and demonstrate the successful implementation of this new method. We show reproduction of the axial charge on a test ensemble and non-zero momentum transfer points of the axial and vector form factors.
description: 7 pages, 5 figures, Proceedings for The 36th International Symposium on Lattice Field Theory
Physics of Cosmic Microwave Background anisotropies and primordial fluctuations
Creators: name: Durrer, Ruth
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The physics of the origin and evolution of CMB anisotropies is described. I explain the idea and status of cosmic parameter estimation and follow it up with critical comments on its dependence on model assumptions and initial conditions.
description: 13 pages, 6 figs. Talk given at "Matter in the Universe", ISSI Bern
Additional file 2 of A Bayesian non-inferiority approach using experts’ margin elicitation – application to the monitoring of safety events
Creators: name: Aupiais, Camille
name: Alberti, Corinne
name: Schmitz, Thomas
name: Baud, Olivier
name: Ursino, Moreno
name: Zohar, Sarah
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Histogram of the acceptable differences in events, and mixtures of beta distributions fitted from experts’ elicitation, through 3 different methods, with their criteria for goodness of fit. The plots analogous to Fig. 2 for the 3 other events: (a) Death, (b) Necrotizing enterocolitis, (c) Retinopathy. (PDF 992 kb)
On mode trapping in pulsating DA white dwarf stars
Creators: name: Benvenuto, O. G.
name: Corsico, A. H.
name: Althaus, L. G.
name: Serenelli, A. M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The present work is designed to explore the effects of the time-dependent element diffusion on the mode trapping properties of DA white dwarf models with various thickness of the hydrogen envelope. Our predictions are compared with the standard assumption of diffusive equilibrium in the trace element approximation. We find that element diffusion markedly weakens the presence of mode trapping originated in the outer layers of the models, even for the case of thin hydrogen envelopes.
description: 5 pages, 6 figures, to be published in MNRAS