cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
INTERNATIONAL CONFERENCE ON FOOD AND AGRICULTURAL ECONOMICS
Creators: name: May, Daniel
name: May, Daniel
Publisher: name: Unknown
Year: 2017
Subjects: subject: Agricultural and Food Policy
subject: Innovation
subject: Business Environments
subject: Policy Change
subject: Sugar Beet Reform
subject: Sugar Beet farmers

description: Current research has found that farmers’ incentives to innovate are influenced by non-economic and social-psychological factors. This research, however, has not explored whether these drivers remain robust through different business environments (i.e. stable vs. turbulent business environments). In addition, related works that have study innovation in turbulent environments have only considered turbulence caused by technological changes but not by changes in policies that affect the agricultural sector. The objective of this article is to fill this gap by analysing farmers’ incentives to innovate before and after a policy shock referred to as the Sugar Regime reform. Before the reform sugar beet farmers in Shropshire faced a stable business environment because they knew ex-ante the price that they would receive for their sugar beet production. However, after the reform the environment became very unstable because the sugar beet factory where the farmers used to sell their production was closed. In order to explore the effect of this change of business environment on farmers’ incentives to innovate, a probit econometric model was adopted and run with data obtained from a questionnaire supplied to ex-sugar beet farmers in Shropshire, UK. The results revealed that drivers of innovation may change under different business environments. Based on this result it is proposed in this article that farmers reach a steady state in stable environments where they have few incentives to innovate in order to favour long run goals. In contrast, in turbulent business environments this steady state is broken and short run drives of innovation are triggered.
Very High Energy Gamma-Ray Astronomy
Creators: name: Catanese, Michael
name: Weekes, Trevor C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a review of the current status of very high energy gamma-ray astronomy. The development of the atmospheric Cherenkov imaging technique for ground-based gamma-ray astronomy has led to a rapid growth in the number of observatories. The detection of TeV gamma rays from Active Galactic Nuclei was unexpected and is providing new insights into the emission mechanisms in the jets. Next generation telescopes are under construction and will increase dramatically the knowledge available at this extreme end of the cosmic electromagnetic spectrum.
description: Invited review to appear in PASP, 30 pages, 25 figures
Amplitude Zeros in $W^\pm Z$ Production
Creators: name: Baur, U.
name: Han, T.
name: Ohnemus, J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We demonstrate that the Standard Model amplitude for $f_1 \bar f_2 \rightarrow W^\pm Z $ at the Born-level exhibits an approximate zero located at $\cosθ= (g^{f_1}_{-} + g^{f_2}_{-}) / (g^{f_1}_{-} - g^{f_2}_{-})$ at high energies, where the $g^{f_i}_{-}$ ($i=1,2$) are the left-handed couplings of the $Z$-boson to fermions and $θ$ is the center of mass scattering angle of the $W$-boson. The approximate zero is the combined result of an exact zero in the dominant helicity amplitudes ${\cal M}(\pm,\mp)$ and strong gauge cancelations in the remaining amplitudes. For non-standard $WWZ$ couplings these cancelations no longer occur and the approximate amplitude zero is eliminated.
description: 11 pages, 4 figures submitted separately as uuencoded tar-ed postscript files, FSU-HEP-940307, UCD-94-5
OGLE-2017-BLG-1434Lb: Eighth q < 1 * 10^-4 Mass-Ratio Microlens Planet Confirms Turnover in Planet Mass-Ratio Function
Creators: name: Udalski, A.
name: Ryu, Y. -H.
name: Sajadian, S.
name: Gould, A.
name: Mróz, P.
name: Poleski, R.
name: Szymański, M. K.
name: Skowron, J.
name: Soszyński, I.
name: Kozłowski, S.
name: Pietrukowicz, P.
name: Ulaczyk, K.
name: Pawlak, M.
name: Rybicki, K.
name: Iwanek, P.
name: Albrow, M. D.
name: Chung, S. -J.
name: Han, C.
name: Hwang, K. -H.
name: Jung, Y. K.
name: Shin, I. -G.
name: Shvartzvald, Y.
name: Yee, J. C.
name: Zang, W.
name: Zhu, W.
name: Cha, S. -M.
name: Kim, D. -J.
name: Kim, H. -W.
name: Kim, S. -L.
name: Lee, C. -U.
name: Lee, D. -J.
name: Lee, Y.
name: Park, B. -G.
name: Pogge, R. W.
name: Bozza, V.
name: Dominik, M.
name: Helling, C.
name: Hundertmark, M.
name: Jørgensen, U. G.
name: Longa-Peña, P.
name: Lowry, S.
name: Burgdorf, M.
name: Campbell-White, J.
name: Ciceri, S.
name: Evans, D.
name: Jaimes, R. Figuera
name: Fujii, Y. I.
name: Haikala, L. K.
name: Henning, T.
name: Hinse, T. C.
name: Mancini, L.
name: Peixinho, N.
name: Rahvar, S.
name: Rabus, M.
name: Skottfelt, J.
name: Snodgrass, C.
name: Southworth, J.
name: von Essen, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We report the discovery of a cold Super-Earth planet (m_p=4.4 +/- 0.5 M_Earth) orbiting a low-mass (M=0.23 +/- 0.03 M_Sun) M dwarf at projected separation a_perp = 1.18 +/- 0.10 AU, i.e., about 1.9 times the snow line. The system is quite nearby for a microlensing planet, D_Lens = 0.86 +/- 0.09 kpc. Indeed, it was the large lens-source relative parallax pi_rel=1.0 mas (combined with the low mass M) that gave rise to the large, and thus well-measured, "microlens parallax" that enabled these precise measurements. OGLE-2017-BLG-1434Lb is the eighth microlensing planet with planet-host mass ratio q < 1 * 10^-4. We apply a new planet-detection sensitivity method, which is a variant of "V/V_max", to seven of these eight planets to derive the mass-ratio function in this regime. We find dN/d(ln q) ~ q^p, with p = 1.05 (+0.78,-0.68), which confirms the "turnover" in the mass function found by Suzuki et al. relative to the power law of opposite sign n = -0.93 +/- 0.13 at higher mass ratios q >~ 2 * 10^-4. We combine our result with that of Suzuki et al. to obtain p = 0.73 (+0.42,-0.34).
description: 53 pages, 16 figures
Ostrea varia Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Ostreoida
Ostreidae
Ostrea
Ostrea varia

description: Ostrea varia [spec. nov.]
O. testa radiis 30 scabris compressis uniaurita.
Habitat in O. australiore.
Simillima priori, sed numero radiorum differens. Color maxime variat.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 698, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Ostrea glabra Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Ostreoida
Ostreidae
Ostrea
Ostrea glabra

description: Ostrea glabra [spec. nov.]
O. testa radiis 10 laevibus planiusculis, internis striis elevatis duplicatis. M. L. U.
Gualt. test. t. 73. f. H.
Kratzenst. Regenf. t. 1. f. 10.
& t. 2. f. 16.
Habitat in M. Mediterraneo.
Testa aequivalvis subrotunda glabra, absque striis extus, obsolete plicata, incarnata extus. Auriculae aequales.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 698, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Supplementary document for Simultaneous bond-selective deuterium-based isotopic labeling sensing with disposable ultra-miniature CARS fiber probe - 6705087.pdf
Creators: name: Wang, Tong
name: Jiang, Junfeng
name: Liu, Kun
name: Shuang, Wang
name: Xu, Tianhua
name: Niu, Panpan
name: Ma, Jinying
name: Yin, Jinde
name: Liu, T.
Publisher: name: Optica Publishing Group
Year: 2023
Subjects: Uncategorized

description: Stokes wide-frequency-interval dual-pulse generation and adjustment
Young stars and non-stellar emission in the aligned radio galaxy 3C 256
Creators: name: Simpson, Chris
name: Eisenhardt, Peter
name: Armus, Lee
name: Chokshi, Arati
name: Dickinson, Mark
name: Djorgovski, S. G.
name: Elston, Richard
name: Jannuzi, Buell T.
name: McCarthy, Patrick J.
name: Pahre, Michael A.
name: Soifer, B. T.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present ground-based images of the z=1.824 radio galaxy 3C 256 in the standard BVRIJHK filters and an interference filter centered at 8800A, a Hubble Space Telescope image in a filter dominated by Ly-alpha emission (F336W), and spectra covering rest-frame wavelengths from Ly-alpha to [O III] 5007. Together with published polarimetry observations, we use these to decompose the overall spectral energy distribution into nebular continuum emission, scattered quasar light, and stellar emission. The nebular continuum and scattered light together comprise half (one third) of the V-band (K-band) light within a 4-arcsec aperture, and are responsible for the strong alignment between the optical/near-infrared light and the radio emission. The stellar emission is dominated by a population estimated to be 100-200 Myr old (assuming a Salpeter IMF), and formed in a short burst with a peak star formation rate of 1-4x10^3 Msun/yr. The total stellar mass is estimated to be no more than 2x10^{11} Msun, which is far less than other luminous radio galaxies at similar redshifts, and suggests that 3C 256 will undergo further star formation or mergers.
description: 35 pages including 10 figures; to appear in Nov 10 ApJ
Physical, spectral, and dynamical properties of asteroid (107) Camilla and its satellites
Creators: name: Pajuelo, M.
name: Carry, B.
name: Vachier, F.
name: Marsset, M.
name: Berthier, J.
name: Descamps, P.
name: Merline, W. J.
name: Tamblyn, P. M.
name: Grice, J.
name: Conrad, A.
name: Storrs, A.
name: Timerson, B.
name: Dunham, D.
name: Preston, S.
name: Vigan, A.
name: Yang, B.
name: Vernazza, P.
name: Fauvaud, S.
name: Bernasconi, L.
name: Romeuf, D.
name: Behrend, R.
name: Dumas, C.
name: Drummond, J. D.
name: Margot, J. -L.
name: Kervella, P.
name: Marchis, F.
name: Girard, J. H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The population of large asteroids is thought to be primordial and they are the most direct witnesses of the early history of our Solar System. Those satellites allow study of the mass, and hence density and internal structure. We study here the properties of the triple asteroid (107) Camilla from lightcurves, stellar occultations, optical spectroscopy, and high-contrast and high-angular-resolution images and spectro-images. Using 80 positions over 15 years, we determine the orbit of its larger satellite to be circular, equatorial, and prograde, with RMS residuals of 7.8 mas. From 11 positions in three epochs only, in 2015 and 2016, we determine a preliminary orbit for the second satellite. We find the orbit to be somewhat eccentric and slightly inclined to the primary's equatorial plane, reminiscent of the inner satellites of other asteroid triple systems. Comparison of the near-infrared spectrum of the larger satellite reveals no significant difference with Camilla. Hence, these properties argue for a formation of the satellites by excavation from impact and re-accumulation of ejecta. We determine the spin and 3-D shape of Camilla. The model fits well each data set. We determine Camilla to be larger than reported from modeling of mid-infrared photometry, with a spherical-volume-equivalent diameter of 254 $\pm$ 36 km (3 $σ$ uncertainty), in agreement with recent results from shape modeling (Hanus2017+). Combining the mass of (1.12 $\pm$ 0.01) $\times$ 10$^{19}$ kg determined from the dynamics of the satellites and the volume from the 3-D shape model, we determine a density of 1,280 $\pm$ 130 SI. From this density, and considering Camilla's spectral similarities with (24) Themis and (65) Cybele (for which water ice coating on surface grains was reported), we infer a silicate-to-ice mass ratio of 1-6, with a 10-30% macroporosity.
description: 40 pages, 16 figures, accepted for publication
Higher Order $1/m$ Corrections at Zero Recoil
Creators: name: Mannel, Thomas
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The general structure of the $1/m$ corrections at zero recoil is studied. The relevant matrix elements are forward matrix elements of local higher dimensional operators and their time ordered products with higher order terms from the Lagrangian. These matrix elements may be classified in a simple way and the analysis at the non recoil point for the form factor of heavy quark currents simplifies drastically. The second order recoil corrections to the form factor $h_{A1}$ of the axial vector current, relevant for the $|V_{cb}|$ determination from $B \to D^*$ decays, are estimated to be $-5\% < h_{A1} - 1 < 0$.
description: LaTeX, 25 pages, one figure, appended after \end{document} as uu-encoded and compressed eps file, uses epsf, CERN-TH.7162/94
Reseña Final Química Inorgánica Metales en la Medicina.docx
Creators: name: V. Irizarry
Publisher: name: figshare
Year: 2018
Subjects: subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Cancer

description: Reseña Final Química Inorgánica Metales en la Medicina
Application of HS-SPME-GC-MS combined with electronic nose technology in the odor recognition of pseudostellariae radix
Creators: name: Huang, Tehui
name: Sun, Yan
name: Guo, Yuanyuan
name: Wang, Wei
name: He, Ting
name: Cao, Junling
Publisher: name: Taylor & Francis
Year: 2022
Subjects: Space Science
Environmental Sciences not elsewhere classified
Chemical Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Science Policy

description: Correct identification of the substance basis of Pseudostellariae Radix (PR) odor is important not only for the quality control of the products, but also for the safety of the consumers. PR is often described with a special smell, such as strange, moldy or earthy. Electronic nose-based technology coupled with headspace solid phase microextraction gas chromatography-mass spectrometry (HS-SPME-GC-MS) was used to investigate the volatile components in PR from 47 germplasms cultivated in traditional fields. A total of 48 common compounds were identified based on HS- SPME-GC-MS technology, and 25 of them with aroma characteristics were found based on Alpha soft 13.4. The 1-Octen-3-ol, geosim, (E)-2-nonenal and 1- methylnaphthalene as contributing marker compounds of the ‘specific smell’ of PR were identified. The odor recognition mode, with demonstrated excellent accuracy in recognition abilities, enabled the correct identification of commercial samples including complex mixtures.
title: ADCO, Grènetier de Cîteaux : comptes (1497-1504) (11 H 1172), f. 00217
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172), f. 00217, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
The dragonfly nearby galaxies survey. Iv. A giant stellar disk in ngc 2841
Creators: name: Zhang, Jielai
name: Abraham, Roberto
name: van Dokkum, Pieter
name: Merritt, Allison
name: Janssens, Steven
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Neutral gas is commonly believed to dominate over stars in the outskirts of galaxies, and investigations of the disk-halo interface are generally considered to be in the domain of radio astronomy. This may simply be a consequence of the fact that deep HI observations typically probe to a lower mass surface density than visible wavelength data. This paper presents low surface brightness optimized visible wavelength observations of the extreme outskirts of the nearby spiral galaxy NGC 2841. We report the discovery of an enormous low-surface brightness stellar disk in this object. When azimuthally averaged, the stellar disk can be traced out to a radius of $\sim$70 kpc (5 $R_{25}$ or 23 inner disk scale lengths). The structure in the stellar disk traces the morphology of HI emission and extended UV emission. Contrary to expectations, the stellar mass surface density does not fall below that of the gas mass surface density at any radius. In fact, at all radii greater than $\sim$20 kpc, the ratio of the stellar to gas mass surface density is a constant 3:1. Beyond $\sim$30 kpc, the low surface brightness stellar disk begins to warp, which may be an indication of a physical connection between the outskirts of the galaxy and infall from the circumgalactic medium. A combination of stellar migration, accretion and in-situ star formation might be responsible for building up the outer stellar disk, but whatever mechanisms formed the outer disk must also explain the constant ratio between stellar and gas mass in the outskirts of this galaxy.
description: 11 pages, 5 figures, accepted for publication in ApJ
Energy is Entanglement
Creators: name: Leichenauer, Stefan
name: Levine, Adam
name: Shahbazi-Moghaddam, Arvin
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We compute the local second variation of the von Neumann entropy of a region in theories with a gravity dual. For null variations our formula says that the diagonal part of the Quantum Null Energy Condition is saturated in every state, thus providing an equivalence between energy and entropy. We prove that the formula holds at leading order in 1/N, and further argue that it will not be affected at higher orders. We conjecture that the QNEC is saturated in all interacting theories. We also discuss the special case of free theories, and the implications of our formula for the Averaged Null Energy Condition, Quantum Focusing Conjecture, and gravitational equations of motion. We show that the leading-order gravitational equations of motion, Einstein's equations, are equivalent to leading-order saturation of the QFC for Planck-width deformations.
description: 37 pages, 2 figures
Allotriozoon heterandromorphum Grandi 1916
Creators: name: Rasplus, Jean-Yves
name: Harry, Myriam
name: Perrin, Hélène
name: Chassagnard, Marie-Thérèse
name: Lachaise, Daniel
Publisher: name: Zenodo
Year: 2003
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Agaonidae
Allotriozoon
Allotriozoon heterandromorphum

description: Allotriozoon heterandromorphum Grandi
MATÉRIEL EXAMINÉ. — 35 ♀, mont Nimba, Guinée, x-1951, collectées au Berlèse (Lamotte & Roy) (Joseph 1959).
DISTRIBUTION. — Sénégal, Guinée, Côte d’Ivoire, Ghana, Nigeria, République Démocratique du Congo, Kenya, Tanzanie, Iles Comores, Iles Seychelles, Madagascar.
 ÉCOLOGIE. — Pollinisateur nocturne de Ficus lutea.
description: Published as part of Rasplus, Jean-Yves, Harry, Myriam, Perrin, Hélène, Chassagnard, Marie-Thérèse & Lachaise, Daniel, 2003, Les Ficus (Moraceae) et l'entomofaune des figues (Hym. Agaonidae, Pteromalidae, Torymidae, Eurytomidae; Dipt. Drosophilidae; Col. Curculionidae) du mont Nimba en Guinée, pp. 107-182 in Mémoires du Muséum national d'Histoire naturelle 190 on page 132, DOI: 10.5281/zenodo.10683835
Linear Polarization and Proper Motion in The Afterglow of Beamed GRBs
Creators: name: Sari, Re'em
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the polarization and proper motion expected in a beamed Gamma-Ray Burst's ejecta. We find that even if the magnetic field has well defined orientation relative to the direction of motion of the shock, the polarization is not likely to exceed 20%. Taking into account the dynamics of beamed ejecta we find that the polarization rises and decays with peak around the jet break time (when the Lorentz factor of the flow is comparable to the initial opening angle of the jet). Interestingly, we find that when the offset of the observer from the center of the beam is large enough, the polarization as function of time has three peaks, and the polarization direction of the middle peak is rotated by 90 degrees relative to the two other peaks. We also show that some proper motion is expected, peaking around the jet break time. Detection of both proper motion and the direction of polarization can determine which component of the magnetic field is the dominant.
description: 12 pages including 4 figures
Two-loop next-to-leading $\mt$ corrections to the $ρ$ parameter
Creators: name: Degrassi, G.
name: Fanchiotti, S.
name: Gambino, P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The $O(G^2_μm_t^4)$ correction to the $ρ$ parameter is computed within the Standard Model using the current algebra formulation of radiative corrections. This approach is proved to be equivalent to the effective Lagrangian method proposed by Barbieri {\em et al.} Using the same framework, the $O(G^2_μm_t^2 m_z^2)$ correction to the ratio of neutral-to-charged current amplitudes is analysed in an $SU(2)$ model. The $O(G^2_μm_t^2 m_z^2)$ contribution is shown to be numerically comparable to the leading $O(G^2_μm_t^4)$ term for realistic values of the top mass. The resummation of higher-order effects is discussed.
description: CERN-TH.7180/94, DFPD 94/TH/12 and NYU-Th-94/02/01, 26 pages (LaTeX + PS figures, needs psfig (optional to include figures), doublespace, equations, and cite styles)
INTERNATIONAL CONFERENCE ON FOOD AND AGRICULTURAL ECONOMICS
Creators: name: Oren, Mehmet
name: Gurer, Betul
name: Abay, Canan
name: Turkekul, Berna
name: Ozalp, Burhan
name: Oren, Mehmet
name: Gurer, Betul
name: Abay, Canan
name: Turkekul, Berna
name: Ozalp, Burhan
Publisher: name: Unknown
Year: 2017
Subjects: subject: Agricultural and Food Policy
subject: Agricultural Policies
subject: Policy analysis matrix
subject: competitiveness
subject: social profits
subject: corn

description: With this study, it is aimed to determine the competitiveness of corn production in terms of profitability and to measure the effects of agricultural policies in Turkey on regional basis. Aegean, Mediterranean and Southeastern Anatolia Regions are selected as a field of research area because the agricultural enterprises in these regions have experienced due to intensive corn production. Firstly, agricultural policies applied for corn production in Turkey is examined. Policy transfers, resource utilization, costs, private and social profits resulting from these applications are also presented with Policy Analysis Matrix (PAM). This method is widely used in the world in the analysis of the impact of policies on production economics and it is a very effective method. PAM is mainly based on benefit-cost analysis. PAM also may be used to generate scenarios for comparison of alternative policies. Besides the secondary data analysis of the effects of policy, the data obtained through face to face interviews with 256 producers selected through stratified sampling method in Aegean, Mediterranean and Southeastern Anatolia Regions. The results show that corn production in Turkey has a comparatively disadvantage stemming mainly from input costs and output prices higher than in the world. The corn productivity is high but high prices of inputs negatively affect Turkish corn producers. Under the existing policy circumstances, the producers earn profit. Farmers would start earning much higher revenues if the tax on fuel will be lowered which in turn decrease production costs. As a result sector’s competitiveness and comparative advantage is also significantly improved.
Apocrypta guineensis Grandi 1916
Creators: name: Rasplus, Jean-Yves
name: Harry, Myriam
name: Perrin, Hélène
name: Chassagnard, Marie-Thérèse
name: Lachaise, Daniel
Publisher: name: Zenodo
Year: 2003
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Agaonidae
Apocrypta
Apocrypta guineensis

description: Apocrypta guineensis Grandi
Fig. 27
 MATÉRIEL EXAMINÉ. — ♁ ♀, mont Nimba nord-nord-ouest, Guinée, la source du Gouan, alt. 1220 m., iv-1993, ex figues de F. sur (Rasplus).
DISTRIBUTION. — Guinée, Côte d’Ivoire, Nigeria, Cameroun, Zambie, Tanzanie, Afrique du Sud.
 ÉCOLOGIE. — Considérées probablement à tort comme des parasitoïdes des Ceratosolen, les espèces du genre Apocrypta semblent en fait séminivores consommant les graines des figuiers du sous-genre Sycomorus (Kerdelhué et al. 2000).
description: Published as part of Rasplus, Jean-Yves, Harry, Myriam, Perrin, Hélène, Chassagnard, Marie-Thérèse & Lachaise, Daniel, 2003, Les Ficus (Moraceae) et l'entomofaune des figues (Hym. Agaonidae, Pteromalidae, Torymidae, Eurytomidae; Dipt. Drosophilidae; Col. Curculionidae) du mont Nimba en Guinée, pp. 107-182 in Mémoires du Muséum national d'Histoire naturelle 190 on page 138, DOI: 10.5281/zenodo.10683835
Anomalous Evolution of Nonsinglet Nucleon Structure Functions
Creators: name: Ball, R. D.
name: Barone, V.
name: Forte, S.
name: Genovese, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We calculate the scale dependence of nonsinglet nucleon structure functions. Due to anomalous axial symmetry breaking a large flavour asymmetry of the quark--antiquark sea is generated nonperturbatively. This produces a strong scale dependence of the nonsinglet structure function in an intermediate range of $Q^2$. Evolving nonperturbatively a pure valence distribution from an infrared scale we can thus compute $F_2^p-F_2^n$ as measured by the NMC, and give detailed predictions for its $Q^2$ dependence at fixed $x$. We also compare our results with Drell--Yan data.
description: 13, harvmac 6 figures, CERN-TH.7189/94 and DFTT 02/94
Ostrea opercularis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Ostreoida
Ostreidae
Ostrea
Ostrea opercularis

description: Ostrea opercularis [spec. nov.]
O. testa radiis 20 subrotundis, decussata striato-sca- bra, operculo convexiore. M. L. U.
Habitat in O. meridionali.
Testa opercularis, magis quam altera convexa.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 698, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Small oscillations of non-dissipative Lagrangian systems
Creators: name: Massa, Enrico
name: Vignolo, Stefano
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mathematical Physics (math-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The small oscillations of an arbitrary scleronomous system subject to time-independent non dissipative forces are discussed. The linearized equations of motion are solved by quadratures. As in the conservative case, the general integral is shown to consist of a superposition of harmonic oscillations. A complexification of the resolving algorithm is presented.
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0875
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0875, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0875, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Morphological and photometric evolution of ultra-luminous infrared galaxies: Nature of faint SCUBA sources
Creators: name: Bekki, Kenji
name: Shioya, Yasuhiro
name: Tanaka, Ichi
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate when and how a dusty starburst galaxy merger can be heavily obscured by dust and consequently becomes an ultra-luminous infrared galaxy (ULIRG), based on numerical simulations of chemodynamical and photometric evolution of dusty gas-rich major galaxy mergers. We found that a major galaxy merger is more likely to become an ULIRG preferentially in the merger late phase, when the two disks become very close and the very high-density dusty gas can obscure heavily the central secondary massive starburst. We furthermore show how the optical and near-infrared morphology of a simulated ULIRG at intermediate (z=0.4) and high redshift (z=1 - 2) can be observed by the Hubble Space Telescope (HST) in order to present a plausible explanation for the origin of some host galaxies of the faint SCUBA sources recently observed by Smail et al. (1998). The results of our numerical simulations imply that some SCUBA sources with apparently faint and compact HST morphology can be higher redshift dust-enshrouded starburst mergers with their outer low surface brightness tidal features hardly detectable in the present optics of the HST.
description: 15 pages 3 figures, ApJL in press
Gauge covariant fermion propagator in quenched, chirally-symmetric quantum electrodynamics
Creators: name: Dong, Zhihua
name: Munczek, Herman J.
name: Roberts, Craig D.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We discuss the chirally symmetric solution of the massless, quenched, Dyson-Schwinger equation for the fermion propagator in three and four dimensions. The solutions are manifestly gauge covariant. We consider a gauge covariance constraint on the fermion--gauge-boson vertex, which motivates a vertex Ansatz that both satisfies the Ward identity when the fermion self-mass is zero and ensures gauge covariance of the fermion propagator.
description: 11 pages. REVTEX 3.0. ANL-PHY-7711-TH-94
Some Observational Consequences of GRB Shock Models
Creators: name: Kumar, Pawan
name: Piran, Tsvi
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In the internal shock scenario for GRBs we expect some fraction of the energy of the burst to be carried by slow moving shells that were ejected at late times. These slow shells collide with faster moving outer shells when the outer shells have slowed down as a result of sweeping up material from the ISM. This gives rise to a forward shock that moves into the outer shell producing a bump in the afterglow light curve of amplitude roughly proportional to the ratio of the energy in the inner and the outer shells. In addition, a reverse shock propagates in the inner shell and produces emission at a characteristic frequency that is typically much smaller than the peak of the emission from the outer shell by a factor of $\sim 7 γ_{0c}^2 (E_2/E_1)^{1.1}$, and the observed flux at this frequency from the reverse shock is larger compared to the flux from the outer shell by a factor of $\sim 8 (γ_{0c} E_2/E_1)^{5/3} $; where $γ_{0c}$ is the bulk Lorentz factor of the outer shell at the time of collision, and $E_1 & E_2$ are the total energy in the outer and the inner shells respectively. The Lorentz factor is related to the observer time as $\sim 5 (t/day)^{3/8}$. The shell collision could produce initial temporal variability in the early afterglow signal. The lack of significant deviation from a power-law decline of the optical afterglow from half a dozen bursts suggests that $E_2/E_1$ is small. Future multi-wavelength observations should be able to either detect bumps in the light curve corresponding to both the forward and the reverse shocks or further constrain the late time release of energy in ejecta with small Lorentz factor, which is expected generically in the internal shock models for the gamma-ray bursts.
description: 17 pages and 5 figs; ApJ March 20, 2000
Upsilon \bar BB$ Couplings, Slope of the Isgur-Wise Function and Improved Estimate of \boldmath{$V_{cb}$}}
Creators: name: Narison, S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We estimate the sum of the $Υ\bar BB $ couplings using QCD Spectral Sum Rules (QSSR). Our result implies the phenomenological bound $ξ'(vv'=1) \geq -1.04$ for the slope of the Isgur-Wise function. An analytic estimate of the (physical) slope to two loops within QSSR leads to the accurate value $ξ'(vv'=1) \simeq -(1.00 \pm 0.02)$ due to the (almost) complete cancellations between the perturbative and non-perturbative corrections at the stability points. Then, we deduce, from the present data, the improved estimate $\vert V_{cb} \vert \simeq \ga 1.48 \mbox{ps}/τ_B \dr ^{1/2}(37.3 \pm 1.2 \pm 1.4)\times 10^{-3}$ where the first error comes from the data analysis and the second one from the different model parametrizations of the Isgur-Wise function.
description: {{\bf $\bf 10 pages, Latex, (1 Figure on request), CERN-TH-7103/93 (Phys. Lett. B in press)
Forging "Methodological inductivism" in the interests  of better science: Encouraging Methodological  inductivism as a harbinger of meaningful change in  different kinds of scientific endeavour
Creators: name: Rao Mandavilli, Sujay
Publisher: name: Zenodo
Year: 2024

description: We begin this paper by defining various pertinent and relevant terms such as the term inductivism in science, hypothetico-deductivism, and subsequently also provide the definitions of various other terms such as a methodology which naturally also include and encompass terms such as research and scientific methodology, scientific methods, scientific techniques, scientific processes and scientific procedures; we then proceed to lay down the bare essentials of what we would like to call “Methodological inductivism”, and also provide a justification and a raison d’etre for the same. We also discuss other allied, related and contingent approaches in the market such as method triangulation, methodological holism, methodological individualism, methodological pluralism, etc in a fair level of detail. We also present, list and lay down bare and in great detail, the various steps involved in the aforesaid technique of “Methodological inductivism”, and also analyse and discuss the various advantages of the this approach. We also discuss why this could be a defining characteristic of contemporary science, and could help distinguish modern science from we would like to call legacy science, and discuss how this could propel science to an altogether new trajectory and take it to new heights besides forging a healthier collaboration among scientists and researchers across disciplines and geographies. It could also reduce gaps in a multi-speed civilization and lead to scientific progress at the speed of light.
INTERNATIONAL CONFERENCE ON FOOD AND AGRICULTURAL ECONOMICS: AGRO-TOURISM APPLICATIONS IN THE CONTEXT OF RURAL DEVELOPMENT: EVIDENCE FROM EMERGING AND DEVELOPED COUNTRIES
Creators: name: Sahin, Levent
name: Sahin, Dilek
name: Sahin, Levent
name: Sahin, Dilek
Publisher: name: Unknown
Year: 2017
Subjects: Community/Rural/Urban Development
International Development

description: Economic development is the elimination of social poverty, economic inequality, education and health deficiencies. Rural development has an important role in removing socio-economic differences between rural and urban areas. Rural development aims to make better the economic and socio-cultural conditions in rural areas. In 1960, rural development has been began to become a topic of researchs. Since 1970, it has been understood that Rural development has a different and significant influence on the economic development of countries. Rural development has been recognized as a new strategy in the field of development by organizations that have influenced the development policies of countries such as the World Bank and the United Nations for the last decade. Rural development focuses on poverty and inequalities between urban and rural areas. Agrotourism is one of the most important tools used in the realization of rural development. Today, the importance of agrotourism is increasing in both developed and developing countries. Agrotourism is mostly applied in the United States of America, France, Spain, Italy and England. In the United States of America, farms are open to the public in the context of agrotourism almost every period of the year. Agricultural tourism is the involvement of agricultural activities in rural areas in touristic activities. With agrotourism, people, living in cities, are offered the opportunity to take part in farm activities. In the agrotourism area, tourists can pick vegetables and fruits, feed farm animals, buy fresh agricultural products from local markets, horse ride etc., can do similiar activities. In addition, with agrotourism, agricultural entrepreneurship activities of the people in the region are supported. People are employed in rural areas. Also, as people are employed in the villages, migrations from rural to urban areas are decreasing. Concepts of development and rural development are primarily included in the study. Agrotourism is an effective element in rural development. In this context, the concept of agrotourism is explained. Agrotourism practices in both developed and developing countries are examined. In addition, the development of agrotourism in Turkey are emphasized. With the development of agrotourism, development and employment in rural areas will increase. Suggestions are made to policy makers for the development of agro-tourism in Turkey in the light of the samples country examined. Key words: Development, Rural Development, Agrotourism
Panchromatic SED modelling of spatially-resolved galaxies
Creators: name: Smith, Daniel J. B.
name: Hayward, Christopher C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We test the efficacy of the energy-balance spectral energy distribution (SED) fitting code Magphys for recovering the spatially-resolved properties of a simulated isolated disc galaxy, for which it was not designed. We perform 226,950 Magphys SED fits to regions between 0.2kpc and 25kpc in size across the galaxy's disc, viewed from three different sight-lines, to probe how well Magphys can recover key galaxy properties based on 21 bands of UV--far-infrared model photometry. Magphys yields statistically acceptable fits to $> 99$ per cent of the pixels within the $r$-band effective radius and between 59 and 77 per cent of pixels within 20kpc of the nucleus. Magphys is able to recover the distribution of stellar mass, star formation rate (SFR), specific SFR, dust luminosity, dust mass, and $V$-band attenuation reasonably well, especially when the pixel size is $> \sim1$ kpc, whereas non-standard outputs (stellar metallicity and mass-weighted age) are recovered less well. Accurate recovery is more challenging in the smallest sub-regions of the disc (pixel scale $< \sim 1$ kpc), where the energy balance criterion becomes increasingly incorrect. Estimating integrated galaxy properties by summing the recovered pixel values, the true integrated values of all parameters considered except metallicity and age are well recovered at all spatial resolutions, ranging from 0.2kpc to integrating across the disc, albeit with some evidence for resolution-dependent biases. These results must be considered when attempting to analyse the structure of real galaxies with actual observational data, for which the `ground truth' is unknown.
description: 21 pages, 15 figures, Accepted for publication in MNRAS
Far Infrared Observations of the Galactic Star Forming Regions associated with IRAS 00338+6312 & RAFGL 5111
Creators: name: Mookerjea, B.
name: Ghosh, S. K.
name: Karnik, A. D.
name: Rengarajan, T. N.
name: Tandon, S. N.
name: Verma, R. P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Two Galactic star forming regions, one in a very early phase of evolution and another evolved one, associated with the IRAS sources 00338+6312 and 03595+5110 (RAFGL 5111) respectively have been studied in detail. These sources have been mapped simultaneously in two far infrared bands at 143 & 185 \micron), with about 1.5 arcmin angular resolution, using the TIFR 100 cm balloon borne telescope. The HIRES processed IRAS maps at 12, 25, 60 & 100 \micron, have been used for comparison. Whereas IRAS 00338+6312 is resolved only in the TIFR bands, RAFGL 5111 is very well resolved in both the TIFR bands, as well as in at least 3 IRAS bands. The neighbouring fainter source IRAS 04004+5114 has also been resolved in the TIFR bands. Taking advantage of the identical beams in the two TIFR bands at 143 & 185 \micron, dust colour temperature, $T(143/185)$, and optical depth, $τ_{150}$, maps have been generated for RAFGL 5111. These maps show interesting structural details. Radiative transfer modelling in spherical geometry has been carried out for individual sources. The best fit models are in good agreement with the observed spectral energy distribution (SED), radio continuum data etc. Another scheme of radiative transfer through the interstellar dust-gas cloud including the heavier elements has been used to predict ionic nebular line emission, which are in reasonable agreement with the measurements for RAFGL 5111. An important conclusion from the present study is that, for all the three sources (IRAS 00338+6312; 03595+5110; and 04004+5114, a faint source in the neighbourhood of RAFGL 5111), the best fit to the observed SED is obtained for a uniform density ($n(r) \sim r^0$) cloud.
description: 34 Pages AAMS style manuscript + 9 ps figures -- to appear in ApJ, September 1, 1999 issue
Ficus sur Forskall 1775
Creators: name: Rasplus, Jean-Yves
name: Harry, Myriam
name: Perrin, Hélène
name: Chassagnard, Marie-Thérèse
name: Lachaise, Daniel
Publisher: name: Zenodo
Year: 2003
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Moraceae
Ficus
Ficus sur

description: Ficus sur Forskåll, 1775
Fig. 3
Nimba 1350 m; ravin de la source du Gouan, 1220 m; Nimba 1200 m, 1060 m; savane niveau Cité-2 Base Technique 850 m; savane Zougué 800 m, 790 m, 780 m, 750 m; Nimba 750 m, 740 m; savane de Mifergui 725 m; Nimba 710 m; forêt colline Gban 645 m, 600 m, 580 m, 570 m; chantier Gbakoré 595 m; Ziéla 525 m; Foromota 525 m; Gbakoré 500 m; zone bambou 500 m; Zouguépo 500 m; Forêt-galerie du Cavally 500 m; savane à buttes 550 m, 500 m.
description: Published as part of Rasplus, Jean-Yves, Harry, Myriam, Perrin, Hélène, Chassagnard, Marie-Thérèse & Lachaise, Daniel, 2003, Les Ficus (Moraceae) et l'entomofaune des figues (Hym. Agaonidae, Pteromalidae, Torymidae, Eurytomidae; Dipt. Drosophilidae; Col. Curculionidae) du mont Nimba en Guinée, pp. 107-182 in Mémoires du Muséum national d'Histoire naturelle 190 on page 114, DOI: 10.5281/zenodo.10683835
A Proposal of Interactive Growing Hierarchical SOM
Creators: name: Ichimura, Takumi
name: Yamaguchi, Takashi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Neural and Evolutionary Computing (cs.NE)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Self Organizing Map is trained using unsupervised learning to produce a two-dimensional discretized representation of input space of the training cases. Growing Hierarchical SOM is an architecture which grows both in a hierarchical way representing the structure of data distribution and in a horizontal way representation the size of each individual maps. The control method of the growing degree of GHSOM by pruning off the redundant branch of hierarchy in SOM is proposed in this paper. Moreover, the interface tool for the proposed method called interactive GHSOM is developed. We discuss the computation results of Iris data by using the developed tool.
description: 6 pages, 11 figures, Proc. of 2011 IEEE International Conference on Systems, Man, and Cybernetics (IEEE SMC 2011). arXiv admin note: text overlap with arXiv:cs/0405030 by other authors
Hoyle-Lyttleton Accretion onto Accretion Disks
Creators: name: Fukue, Jun
name: Ioroi, Masayuki
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate Hoyle-Lyttleton accretion for the case where the central source is a luminous accretion disk. %In classical Hoyle-Lyttleton accretion onto a ``spherical'' source, accretion takes place in an axially symmetric manner around a so-called accretion axis. The accretion rate of the classical Hoyle-Lyttleton accretion onto a non-luminous object and $Γ$ the luminosity of the central object normalized by the Eddington luminosity. %If the central object is a compact star with a luminous accretion disk, the radiation field becomes ``non-spherical''. %Although the gravitional field remains spherical. In such a case the axial symmetry around the accretion axis breaks down; the accretion radius $R_{acc}$ generally depends on an inclination angle $i$ between the accretion axis and the symmetry axis of the disk and the azimuthal angle $ϕ$ around the accretion axis. %That is, the cross section of accretion changes its shape. Hence, the accretion rate $\dot{M}$, which is obtained by integrating $R_{acc}$ around $ϕ$, depends on $i$. % as well as $M$, $Γ$, and $v_\infty$. %In the case of an edge-on accretion ($i=90^{\circ}$), The accretion rate is larger than that of the spherical case and approximately expressed as $\dot{M} \sim \dot{M}_{HL} (1-Γ)$ for $Γ\leq 0.65$ and $\dot{M} \sim \dot{M}_{HL} (2-Γ)^2/5$ for $Γ\geq 0.65$. %Once the accretion disk forms and the anisotropic radiation fields are produced around the central object,the accretion plane will be maintained automatically (the direction of jets associated with the disk is also maintained). %Thus, the anisotropic radiation field of accretion disks drastically changes the accretion nature, that gives a clue to the formation of accretion disks around an isolated black hole.
description: 5 figures