cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Madoniella spilota Opitz 2010, new species
Creators: name: Opitz, Weston
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cleridae
Madoniella
Madoniella spilota

description: Madoniella spilota Opitz, new species
Figure 11, 56.
 Holotype. Male. COLOMBIA Norte de Santander ANU Los Estoraques Bosque Piritama 8 o 14' N 73 o 15’S 1815 m Malaise 29.x-18.xi. 2003 J. Vargas & E. Bayona Leg. M. 4603. A second label reads, IavH-E 70315. A third label reads, Instituto Humbolt COLOMBIA (IAVH). (Specimen point mounted, antenna and gender label affixed to paper point; locality label; specimen number label; repository label; IAVH acronymic label; Holotype label.)
 Paratypes. None.
 Diagnosis (Fig. 56): In the key of madoniellan species (Opitz, in press), the Holotype extends to couplet 11(4'), which accommodates Madoniella rubida Opitz. From the latter, M. spilota specimens may be distinguished by the spotted condition of the legs.
 Description. Size: Length 4.8 mm; width 1.6 mm. Integumental Color: Cranium dark reddish-brown; pronotal disc dark brown, more reddish at sides; elytral disc with well-developed insignia, posterolateral extensions of posterior block missing, posterocentral extension of posterior block broadly confluent with yellow macula on elytral apex. Head: Vertex narrower than eyes in head dorsal view; antenna as depicted in figure 11. Thorax: Pronotal side margins very sinuous, anterior margin arcuate plane; elytral form oblong; elytral punctations large; anterior margin of protibia with 5 spines. Abdomen: Aedeagus not available for study.
 Variation. One specimen examined.
 Natural History. The primary type was collected at 1850 m sometime between October 29 th and September 18 th.
 Distribution. Known only from the type locality.
 Etymology. The specific epithet spilota stems from the Greek spilos (= fleck). I refer to the spotty infuscations on the legs.
description: Published as part of Opitz, Weston, 2010, New taxa of Epiphloeinae Kuwert (Cleridae) and Chaetosomatidae Crowson (Coleoptera: Cleroidea), pp. 1-28 in Insecta Mundi 2010 (123) on page 16, DOI: 10.5281/zenodo.5352832
Additional file 2: of Herbal or traditional medicine consumption in a Thai worker population: pattern of use and therapeutic control in chronic diseases
Creators: name: Napatt Kanjanahattakij
name: Pakakrong Kwankhao
name: Prin Vathesatogkit
name: Nisakron Thongmung
name: Yingampa Gleebbua
name: Piyamitr Sritara
name: Chagriya Kitiyakara
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Table S1. The laboratory values and the proportion out of recommended target range of subjects with self-reported conditions. (DOCX 17 kb)
Public Research Yields High Returns... Measured in More Than Dollars
Creators: name: Heisey, Paul W.
name: King, John L.
name: Day-Rubenstein, Kelly A.
name: Heisey, Paul W.
name: King, John L.
name: Day-Rubenstein, Kelly A.
Publisher: name: Unknown
Year: 2011
Subjects: Community/Rural/Urban Development

description: Well-established quantitative approaches find that in the aggregate, public investments in agricultural research yield high returns and spur growth in agricultural productivity. Standard economic approaches may be difficult to apply to evaluations of some research benefits and may not help in gauging important steps necessary to positive research outcomes. In these more difficult cases, economic reasoning can provide qualitative analysis even when quantitative estimates of benefits are intractable.
Bar pattern speeds in CALIFA galaxies: ultrafast bars or too long bars?
Creators: name: Cuomo, Virginia
name: Lee, Y.H.
name: Buttitta, C.
name: Aguerri, J. A. L.
name: Corsini, E.M.
name: Morelli, L.
Publisher: name: Zenodo
Year: 2021

description: More than 10% of the barred galaxies with a direct measurement of bar pattern speed host a bar rotating extremely fast. These bars are generally defined as 'ultrafast'. We selected the ultrafast bars observed in CALIFA and investigated if the bar rotation rates were correctly determined. We tested the measurement of bar pattern speed obtained with the Tremaine-Weinberg method and method proposed by Lee et al. (2020). Most of the galaxies is hosting an inner ring located at the end of the bar and/or strong spiral arms. Our new estimates of bar radius are always shorter with respect to the values used in literature. The corresponding bar rotation rate do not belong to the ultrafast regime, except for one galaxy. The presence of the rings and/or strong spiral arms affected the estimate of the bar radius and of the bar rotation rate. We stressed that a solid estimate of bar radius is missing.
Rural America Benefits From Expanded Use of the Federal Tax Code for Income Support
Creators: name: Farrigan, Tracey L.
name: Durst, Ron L.
name: Farrigan, Tracey L.
name: Durst, Ron L.
Publisher: name: Unknown
Year: 2011
Subjects: Agricultural and Food Policy
Crop Production/Industries

description: Over the past two decades, the Federal tax code increasingly has been used as a tool for achieving social and other policy objectives, primarily through the expanded use of tax credits. A larger share of rural taxpayers benefit from Federal tax policies aimed at lower income taxpayers because they have historically had lower incomes and higher poverty rates than urban households. The earned income and child tax credits have provided a substantial boost in income to low and middle-income rural taxpayers and have reduced the rural poverty rate.
Photonic phase correctors based on phase shifters and grating coupler arrays
Creators: name: Diab, Momen
name: Cheriton, Ross
name: Taylor, Jacob
name: Patel, Dhwanil
name: Rojas, Libertad
name: Barnet, Mark
name: Sivanandam, Suresh
name: Xu, Dan-Xia
name: Schmid, Jens H.
name: Cheben, Pavel
name: Janz, Siegfried
Publisher: name: Proceedings of AO4ELT7 conference 2023 - Editors: Thierry Fusco and Benoit Neichel
Year: 2023
Subjects: ASTROPHOTONICS
ADAPTIVE OPTICS
PHASE CORRECTORS
PHOTONIC SPECTROGRAPH
FREE
SPACE OPTICAL COMMUNICATION

description: We propose an integrated phase corrector that efficiently couples the light distorted by atmospheric turbulence into single-mode fibers for the use of free-space optical communication and photonic spectrographs. The integrated circuit consists of an array of gratings that couple light from the subapertures of the telescope pupil into single-mode waveguides in the photonic integrated circuit (PIC). Resistive elements are used to modulate the refractive index in a coiled segment of the waveguides and shift their phases accordingly. The co-phased beams are combined and delivered to an output single-mode fiber (SMF), where the collected flux is predicted to be greater than that coupled directly without correction into a single-mode fiber at the focus of the telescope.
The thermal conductivity of the spin-1/2 XXZ chain at arbitrary temperature
Creators: name: Kluemper, Andreas
name: Sakai, Kazumitsu
Publisher: name: arXiv
Year: 2001
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Algebra (math.QA)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: Motivated by recent investigations of transport properties of strongly correlated 1d models and thermal conductivity measurements of quasi 1d magnetic systems we present results for the integrable spin-1/2 $XXZ$ chain. The thermal conductivity $κ(ω)$ of this model has $\Reκ(ω)=\tildeκδ(ω)$, i.e. it is infinite for zero frequency $ω$. The weight $\tildeκ$ of the delta peak is calculated exactly by a lattice path integral formulation. Numerical results for wide ranges of temperature and anisotropy are presented. The low and high temperature limits are studied analytically.
description: 12 pages
Additional file 1 of Severe fever with thrombocytopenia syndrome with re-infection in China: a case report
Creators: name: Lv, Shou-Ming
name: Yuan, Chun
name: Zhang, Lan
name: Wang, Yu-Na
name: Dai, Zi-Niu
name: Yang, Tong
name: Dai, Ke
name: Zhang, Xiao-Ai
name: Lu, Qing-Bin
name: Yang, Zhen-Dong
name: Cui, Ning
name: Li, Hao
name: Liu, Wei
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Additional file 1: Table S1. The titers of SFTSV specific IgM and IgG antibodies for two episodes of SFTSV infection from the same patient. Fig. S1. Dynamic ratio of aspartate aminotransferase and alanine aminotransferases for two episodes of SFTSV infection from the same patient.
Facial Makeup Transfer Combining Illumination Transfer
Creators: name: Jin, Xin
name: Han, Rui
name: Ning, Ning
name: Li, Xiaodong
name: Zhang, Xiaokun
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: To meet the women appearance needs, we present a novel virtual experience approach of facial makeup transfer, developed into windows platform application software. The makeup effects could present on the user's input image in real time, with an only single reference image. The input image and reference image are divided into three layers by facial feature points landmarked: facial structure layer, facial color layer, and facial detail layer. Except for the above layers are processed by different algorithms to generate output image, we also add illumination transfer, so that the illumination effect of the reference image is automatically transferred to the input image. Our approach has the following three advantages: (1) Black or dark and white facial makeup could be effectively transferred by introducing illumination transfer; (2) Efficiently transfer facial makeup within seconds compared to those methods based on deep learning frameworks; (3) Reference images with the air-bangs could transfer makeup perfectly.
description: IEEE Access, conference short version: ISAIR2019
AAT/WFI observations of the Extragalactic H I Cloud HIPASS J1712-64
Creators: name: Lewis, Geraint F.
name: Irwin, Michael J.
name: Ibata, Rodrigo A.
name: Gibson, Brad K.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: AAT/WFI optical images of a candidate extragalactic HI cloud, HIPASS J1712-64, are presented. The g and r-band CCD mosaic camera frames were processed using a new data pipeline recently installed at the AAO. The resultant stacked images reach significantly deeper levels than those of previous published optical imaging of this candidate, providing a detection limit M_g -7 at a distance of 3Mpc, the inferred distance to HIPASS J1712-64. However, detailed analysis of the images fails to uncover any stellar population associated with the HI emission. If this system is a member of the Local Group then it is pathologically different to other members. Hence, our observations reinforce earlier suggestions that this HI cloud is most likely Galactic in origin and not a Local Volume dwarf galaxy.
description: 8 pages, accepted for publication in PASA (Figures reduced in resolution, please contact gfl if you wish the higher resolution versions)
Hedychridium elongatum Linsenmaier 1959
Creators: name: Rosa, Paolo
name: Heim, René
name: Bernasconi, Marco Valerio
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Chrysididae
Hedychridium
Hedychridium elongatum

description: elongatum group
[established by Linsenmaier (1999), based on a single species previously included in the flavipes group]
description: Published as part of Rosa, Paolo, Heim, René & Bernasconi, Marco Valerio, 2022, The Palaearctic types of Chrysididae (Insecta, Hymenoptera) deposited in the Linsenmaier collection. Part 2. Elampini: genus Hedychridium Abeille de Perrin, 1878, pp. 1-94 in Zootaxa 5090 (1) on page 89, DOI: 10.11646/zootaxa.5090.1.1, http://zenodo.org/record/5836207
Adsorption of He atoms in external grooves of single wall carbon nanotube bundles
Creators: name: Siber, Antonio
Publisher: name: arXiv
Year: 2002
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: I calculate the quantum states for He atom in the potential of an external groove of the single wall carbon nanotube bundle. The calculated ground state energy is found to be in fair agreement with the experimental estimate which suggests that the outer groove site is a preferential site for the adsorption of He gas in the samples studied experimentally. I also calculate the specific heat of low-density $^4$He atom gas adsorbed in groove positions. The specific geometry of the groove and its influence on the adsorbate quantum states and specific heat are discussed.
Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud IV: Evidence for Multiple Populations in Hodge 11 and NGC 2210
Creators: name: Gilligan, Christina K.
name: Chaboyer, Brian
name: Cummings, Jeffrey D.
name: Mackey, Dougal
name: Cohen, Roger E.
name: Geisler, Doug
name: Grocholski, Aaron J.
name: Parisi, M. C.
name: Sarajedini, Ata
name: Ventura, Paolo
name: Villanova, Sandro
name: Yang, Soung-Chul
name: Wagner-Kaiser, Rachel
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a multiple population search in two old Large Magellanic Cloud (LMC) Globular Clusters, Hodge 11 and NGC 2210. This work uses data from the Advanced Camera for Surveys and Wide Field Camera 3 on the Hubble Space Telescope from programme GO-14164 in Cycle 23. Both of these clusters exhibit a broadened main sequence with the second population representing ($20 \pm \! \sim \! 5$)% for NGC 2210 and ($30 \pm \! \sim \! 5$)% for Hodge 11. In both clusters, the smaller population is redder than the primary population, suggesting CNO variations. Hodge 11 also displays a bluer second population in the horizontal branch, which is evidence for helium enhancement. However, even though NGC 2210 shows similarities to Hodge 11 in the main sequence, there does not appear to be a second population on NGC 2210's horizontal branch. This is the first photometric evidence that ancient LMC Globular Clusters exhibit multiple stellar populations.
description: 20 pages, 19 figures, submitted to MNRAS, deleted one sentence and fixed Figure 2 which had the same plot twice
Merger shocks in galaxy clusters A665 and A2163 and their relation to radio halos
Creators: name: Markevitch, M.
name: Vikhlinin, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present Chandra gas temperature maps for two hot, intermediate-redshift clusters A665 and A2163. Both show strong temperature variations in their central r=1 Mpc regions, naturally interpreted as product of the subcluster mergers. The A665 map reveals a shock in front of the cool core, while the temperature structure of A2163 is more complicated. On a larger linear scale, our data on A2163 indicate a radial temperature decline in agreement with earlier ASCA results, although the uncertainties are large. Both these clusters exhibit previously known synchrotron radio halos. Comparison of the radio images and the gas temperature maps indicates that radio emission predominantly comes from the hot gas regions, providing a strong argument in favor of the hypothesis that relativistic electrons are accelerated in merger shocks.
description: Updated radio image for A2163, expanded introduction. ApJ in press. 8 pages, uses emulateapj.sty. Color version is at http://hea-www.harvard.edu/~maxim/papers/665.ps.gz (PS) or http://hea-www.harvard.edu/~maxim/papers/665.pdf (PDF)
Additional file 1: of Herbal or traditional medicine consumption in a Thai worker population: pattern of use and therapeutic control in chronic diseases
Creators: name: Napatt Kanjanahattakij
name: Pakakrong Kwankhao
name: Prin Vathesatogkit
name: Nisakron Thongmung
name: Yingampa Gleebbua
name: Piyamitr Sritara
name: Chagriya Kitiyakara
Publisher: name: figshare
Year: 2019
Subjects: subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: EGAT questionnaire (DOCX 21 kb)
On multiplicities of points on Schubert varieties in Graszmannians II
Creators: name: Krattenthaler, Christian
Publisher: name: arXiv
Year: 2001
Subjects: subject: Algebraic Geometry (math.AG)
subject: Commutative Algebra (math.AC)
subject: Combinatorics (math.CO)
subject: Rings and Algebras (math.RA)
subject: FOS: Mathematics
subject: 14M15 (Primary) 05A15 05E15 14H20 (Secondary)

description: We prove a conjecture by Kreiman and Lakshmibai on a combinatorial description of multiplicities of points on Schubert varieties in Graszmannians in terms of certain sets of reflections in the corresponding Weyl group. The proof is accomplished by setting up a bijection between these sets of reflections and the author's previous combinatorial interpretation of these multiplicities in terms of nonintersecting lattice paths (Séminaire Lotharingien Combin. 45 (2001), Article B45c; see http://www.mat.univie.ac.at/~slc/wpapers/s45kratt.html or http://www.arxiv.org/abs/math.AG/0011129).
description: 11 pages, AmS-TeX
The distance to the SNR CTB109 deduced from its environment
Creators: name: Kothes, Roland
name: Uyaniker, Bulent
name: Yar, Aylin
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We conducted a study of the environment around the supernova remnant CTB109. We found that the SNR is part of a large complex of HII regions extending over an area of 400 pc along the Galactic plane at a distance of about 3 kpc at the closer edge of the Perseus spiral arm. At this distance CTB109 has a diameter of about 24 pc. We demonstrated that including spiral shocks in the distance estimation is an ultimate requirement to determine reliable distances to objects located in the Perseus arm. The most likely explanation for the high concentration of HII regions and SNRs is that the star formation in this part of the Perseus arm is triggered by the spiral shock.
description: 6 pages, 6 figures. accepted for publication in the Astrophysical Journal
At the Health Borders
Creators: name: K Moses
Publisher: name: Zenodo
Year: 2021
Subjects: Asthma
SarsCov2
COVID-19
Health_Borders
Teaching
Social_Determinants
HealthDisparities

description: Poster delivered at the Sencer Conference, January 2021 - Notorious Narratives: Crisscrossing a landscape of Health Disparities, I came upon jarring borders.
Semi-classical limit of quantum free energy minimizers for the gravitational Hartree equation
Creators: name: Choi, Woocheol
name: Hong, Younghun
name: Seok, Jinmyoung
Publisher: name: arXiv
Year: 2019
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 81Q20 (81Q10, 35J10, 35Q55, 35Q83)

description: For the gravitational Vlasov-Poisson equation, Guo and Rein constructed a class of classical isotropic states as minimizers of free energies (or energy-Casimir functionals) under mass constraints. For the quantum counterpart, that is, the gravitational Hartree equation, isotropic states are constructed as free energy minimizers by Aki, Dolbeault and Sparber. In this paper, we are concerned with the correspondence between quantum and classical isotropic states. Precisely, we prove that as the Planck constant $\hbar$ goes to zero, free energy minimizers for the Hartree equation converge to those for the Vlasov-Poisson equation in terms of potential functions as well as via the Husimi transform and the Töplitz quantization.
description: Some errors are corrected
Additional file 1: of Improving salt tolerance in potato through overexpression of AtHKT1 gene
Creators: name: Wang, Li
name: Liu, Yuhui
name: Li, Dan
name: Feng, Shoujiang
name: Yang, Jiangwei
name: Zhang, Jingjing
name: Zhang, Junlian
name: Wang, Di
name: Gan, Yantai
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: Table S1. Na+ contents of vermiculite after 30 days NaCl treatment. (DOCX 16 kb)
Relationship between dynamical heterogeneities and stretched exponential relaxation
Creators: name: Simdyankin, S. I.
name: Mousseau, Normand
Publisher: name: arXiv
Year: 2002
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We identify the dynamical heterogeneities as an essential prerequisite for stretched exponential relaxation in dynamically frustrated systems. This heterogeneity takes the form of ordered domains of finite but diverging lifetime for particles in atomic or molecular systems, or spin states in magnetic materials. At the onset of the dynamical heterogeneity, the distribution of time intervals spent in such domains or traps becomes stretched exponential at long time. We rigorously show that once this is the case, the autocorrelation function of the renewal process formed by these time intervals is also stretched exponential at long time.
description: 8 pages, 4 figures, submitted to PRE
Complex eigenvalue splitting for the Dirac operator
Creators: name: Hirota, Koki
name: Wittsten, Jens
Publisher: name: arXiv
Year: 2019
Subjects: subject: Analysis of PDEs (math.AP)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 34L40 (primary), 81Q20 (secondary)

description: We analyze the eigenvalue problem for the semiclassical Dirac (or Zakharov-Shabat) operator on the real line with general analytic potential. We provide Bohr-Sommerfeld quantization conditions near energy levels where the potential exhibits the characteristics of a single or double bump function. From these conditions we infer that near energy levels where the potential (or rather its square) looks like a single bump function, all eigenvalues are purely imaginary. For even or odd potentials we infer that near energy levels where the square of the potential looks like a double bump function, eigenvalues split in pairs exponentially close to reference points on the imaginary axis. For even potentials this splitting is vertical and for odd potentials it is horizontal, meaning that all such eigenvalues are purely imaginary when the potential is even, and no such eigenvalue is purely imaginary when the potential is odd.
description: 31 pages, 8 figures
Collisional excitation of hydrogen and the determination of the primordial helium abundance from H II regions
Creators: name: Stasinska, G.
name: Izotov, Y. I.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This paper investigates the effect of collisional enhancement of the hydrogen lines on the derivation of the helium abundances in low metallicity H II regions. For this, we have constructed a grid of photoionization models relevant for the analysis of giant \hii regions in blue compact galaxies. We show that the effect of collisional excitation on the Halpha/Hbeta ratio can be quite important (up to 8% or more). The impact of this effect on the determination of the helium mass fraction has been tracked on four low-metallicity blue compact galaxies for which Keck spectra are available and which are among the best objects for the quest of the pregalactic helium abundance. We find that taking into account the effects of collisional excitation of hydrogen results in an upward correction of the helium mass fraction Y by up to 5%. However, combining with other systematic effects usually not considered in the determination of the helium abundance in low-metallicity galaxies, the resulting uncertainty should be much less.
description: 10 pages, 6 Postscript figures, accepted for publication in the Astronomy and Astrophysics
Human and Social Capital Characteristics Near the Frontier of Production Technology
Creators: name: Martin, Michael J.
name: Taylor, Timothy G.
name: Martin, Michael J.
name: Taylor, Timothy G.
Publisher: name: Unknown
Year: 1997
Subjects: subject: Institutional and Behavioral Economics
subject: Research and Development/Tech Change/Emerging Technologies
subject: Human Capital
subject: Social Capital
subject: Stochastic Frontier
subject: Technical Efficiency
subject: Central America
subject: Honduras

description: This paper presents insights into how human and social capital factors improve production efficiency in impoverished rural areas. A stochastic frontier production function is estimated for over 400 Honduran maize producers. Deubreu-Farrell technical and allocative measures are calculated relative to the observed "best practice" production frontier. Group means compare efficiencies by various socioeconomic characteristics that are intuitively related to production, but have not yet been examined. Efficiency is positively related to proportion of output marketed, education, health and experience. Personal extension assistance also improves efficiency, and farmers with no extension assistan,ce are noticeably inefficient. Religion shows mixed effects on efficiency.
A measurement method for responsivity of microwave kinetic inductance detector by changing power of readout microwaves
Creators: name: Kutsuma, Hiroki
name: Hattori, Makoto
name: Koyano, Ryo
name: Mima, Satoru
name: Oguri, Shugo
name: Otani, Chiko
name: Taino, Tohru
name: Tajima, Osamu
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Superconducting detectors are a modern technology applied in various fields. The microwave kinetic inductance detector (MKID) is one of cutting-edge superconducting detector. It is based on the principle of a superconducting resonator circuit. A radiation entering the MKID breaks the Cooper pairs in the superconducting resonator, and the intensity of the radiation is detected as a variation of the resonant condition. Therefore, calibration of the detector responsivity, i.e., the variation of the resonant phase with respect to the number of Cooper-pair breaks (quasiparticles), is important. We propose a method for responsivity calibration. Microwaves used for the detector readout locally raise the temperature in each resonator, which increases the number of quasiparticles. Since the magnitude of the temperature rise depends on the power of readout microwaves, the number of quasiparticles also depends on the power of microwaves. By changing the power of the readout microwaves, we simultaneously measure the phase difference and lifetime of quasiparticles. We calculate the number of quasiparticles from the measured lifetime and by using a theoretical formula. This measurement yields a relation between the phase response as a function of the number of quasiparticles. We demonstrate this responsivity calibration using the MKID maintained at 285mK. We also confirm consistency between the results obtained using this method and conventional calibration methods in terms of the accuracy.
description: 4 pages, 4 figures
Pyticeroides parvoporis Opitz 2010, new species
Creators: name: Opitz, Weston
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cleridae
Pyticeroides
Pyticeroides parvoporis

description: Pyticeroides parvoporis Opitz, new species
Figure 18, 44, 61.
 Holotype. Male. ECUADOR: Orellana: 1 km S Onkone Gare Camp, 00 o 39’S 76 o 26’W, 2-VII- 1995, 220 m, T.L. Erwin; a second label reads-Fogging leaves in terre firme forest (USNM). (Specimen point mounted, antenna and gender symbol affixed to paper point; support card; locality label; Natural History label; USNM acronymic label; Holotype label).
 Paratypes. None.
 Diagnosis (Fig. 61): The very small elytral disc punctations conveniently distinguish the members of this species from superficially similar specimens of P. latisentis. Also, the pronotal disc is much more concave paralaterally in specimens of P. parvoporis.
 Description. Size: Length 6.0 mm; width 2.1 mm. Integument: Cranium bicolorous, upper frons infuscated, gena infuscated, vertex flavotestaceous, postocular streaks well expressed; pronotum yellow at upper sides, infuscated at lower sides, piceous discal vitta broad, thoracic venter and abdomen brown; elytra castaneous, except with yellow middiscal fascia that connects to yellow humeral angle by broad yellow epipleural streak; legs predominantly castaneous, femora flavotestaceous in basal half, dark brown in remainder. Head: As wide as pronotum (63:63); ratio of eye width to width of vertex (28:15); antennal funicular antennomeres particularly explanate (Fig.18). Thorax: Pronotum transverse-quadrate (61:51); side margins slightly convex; elytral punctations arranged into 11 rows, 11 th row indistinct near sutural margin, punctations small and spheroid, those near sutural margin may be misaligned, subseriate, interstitial spaces arenose; elytra about 5.6 x longer than length of pronotum; elytral length to width ratio 6:2; anterior margin of protibia with 9 spines, 9 th very small. Abdomen: Male pygidium not emarginate; aedeagus (Fig.44) short lanceolate; phallic struts slightly broadened at extremities.
 Variation. No information available.
 Natural History. The Holotype was collected by fogging tree branches during July, at 220 m.
 Distribution. Specimens are known only from the type locality.
 Etymology. The specific epithet parvoporis is a Latin compound name that stems from the adjective parvus (= little) and the noun porus (= hole). I refer to the diminutive punctations on the elytral disc.
 Taxonomic Notes. The most closely related known species of P. parvoporis, P. latisentis, is also made available in this contribution, therefore no modified key is presented in this section.
description: Published as part of Opitz, Weston, 2010, New taxa of Epiphloeinae Kuwert (Cleridae) and Chaetosomatidae Crowson (Coleoptera: Cleroidea), pp. 1-28 in Insecta Mundi 2010 (123) on pages 21-22, DOI: 10.5281/zenodo.5352832
Additional file 2: of Improving salt tolerance in potato through overexpression of AtHKT1 gene
Creators: name: Wang, Li
name: Liu, Yuhui
name: Li, Dan
name: Feng, Shoujiang
name: Yang, Jiangwei
name: Zhang, Jingjing
name: Zhang, Junlian
name: Wang, Di
name: Gan, Yantai
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Science Policy
subject: Plant Biology

description: Table S2. Principle component analysis (PCA) total variance explained. (DOCX 17 kb)
The Fundamental Plane of Spiral Galaxies: Theoretical Expectations
Creators: name: Shen, Shiyin
name: Mo, H. J.
name: Shu, Chenggang
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Current theory of disk galaxy formation is used to study fundamental-plane (FP) type of relations for disk galaxies. We examine how the changes in model parameters affect these relations and explore the possibility of using such relations to constrain theoretical models. The distribution of galaxy disks in the space of their fundamental properties are predicted to be concentrated in a plane, with the Tully-Fisher (TF) relation (a relation between luminosity $L$ and maximum rotation velocity $V_m$) being an almost edge-on view. Using rotation velocities at larger radii generally leads to larger TF scatter. In searching for a third parameter, we find that both the disk scale-length $R_d$ (or surface brightness) and the rotation-curve shape are correlated with the TF scatter. The FP relation in the $(\Log L, \Log V_m, \Log R_d)$-space obtained from the theory is $L\propto R_d^{α'} V_m^{β'}$, with ${α'}\sim 0.50$ and ${β'}\sim 2.60$, consistent with the preliminary result we obtain from observational data. Among the model parameters we probe, variation in any of them can generate significant scatter in the TF relation, but the effects of the spin parameter and halo concentration can be reduced significantly by introducing $R_d$ while the scatter caused by varying $m_d$ (the ratio between disk mass and halo mass) is most effectively reduced by introducing the parameters which describes the rotation-curve shape. The TF and FP relations combined should therefore provide useful constraints on models of galaxy formation.
description: 25 pages, 11 figures, 4 tables; submitted to MNRAS
Hedychrum margaritaceum
Creators: name: Rosa, Paolo
name: Heim, René
name: Bernasconi, Marco Valerio
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Chrysididae
Hedychrum
Hedychrum margaritaceum

description: margaritaceum group
[established by Linsenmaier (1968) based on a single species later moved in the flavipes group (1997). This species (group) is anyway well distinct from all other species and placed separately in Linsenmaier’s collection. We consider valid the interpretation given by Linsenmaier (1968)]
Hedychridium (Hedychridium) margaritaceum * (Semenov-Tian-Shanskij, 1954) (= Irenula margaritacea Semenov-Tian-Shanskij, 1954).
description: Published as part of Rosa, Paolo, Heim, René & Bernasconi, Marco Valerio, 2022, The Palaearctic types of Chrysididae (Insecta, Hymenoptera) deposited in the Linsenmaier collection. Part 2. Elampini: genus Hedychridium Abeille de Perrin, 1878, pp. 1-94 in Zootaxa 5090 (1) on page 89, DOI: 10.11646/zootaxa.5090.1.1, http://zenodo.org/record/5836207
Additional file 1: of Gas exchange, biomass and non-structural carbohydrates dynamics in vines under combined drought and biotic stress
Creators: name: Savi, Tadeja
name: González, Almudena García
name: Herrera, Jose
name: Forneck, Astrid
Publisher: name: figshare
Year: 2019
Subjects: subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: FigureS1. Microclimatic data recorded in the greenhouse during the experimental period: average midday water pressure deficit (grey area, right axis), minimum (closed circles) and maximum (open circles) daily temperatures (left axis). The two arrows indicate the inoculation and the final sampling days, respectively. Figure S2. Stomatal conductance to water vapor (gs) measured in 5C (a) and Riesling grafted on 5C (b) during treatments application (n = 4–7). W = well-watered plants; D = drought-stressed; C = control, non-phylloxerated; P = root phylloxerated. Letters and asterisk indicate statistically significant difference within Irrigation (Factor I; W and D) and Infestation (Factor II; C and P), respectively. No statistically significant interaction between factors was observed. Figure S3. Leaf temperature (Tleaf) measured in 5C (a) and Riesling grafted on 5C (b) during treatments application (n = 4–7). W = well-watered plants; D = drought-stressed; C = control, non-phylloxerated; P = root phylloxerated. Letters denote statistically significant differences within Irrigation (Factor I; W and D). No statistically significant differences within factor Infestation or interaction between factors were observed. Figure S4. Sub-stomatal CO2 (Ci) measured in 5C (a) and Riesling grafted on 5C (b) during treatments application (n = 4–7). W = well-watered plants; D = drought-stressed; C = control, non-phylloxerated; P = root phylloxerated. Letters denote statistically significant differences within Irrigation (Factor I; W and D). No statistically significant differences within factor Infestation or interaction between factors were observed.
An Efficient and Layout-Independent Automatic License Plate Recognition System Based on the YOLO detector
Creators: name: Laroca, Rayson
name: Zanlorensi, Luiz A.
name: Gonçalves, Gabriel R.
name: Todt, Eduardo
name: Schwartz, William Robson
name: Menotti, David
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: This paper presents an efficient and layout-independent Automatic License Plate Recognition (ALPR) system based on the state-of-the-art YOLO object detector that contains a unified approach for license plate (LP) detection and layout classification to improve the recognition results using post-processing rules. The system is conceived by evaluating and optimizing different models, aiming at achieving the best speed/accuracy trade-off at each stage. The networks are trained using images from several datasets, with the addition of various data augmentation techniques, so that they are robust under different conditions. The proposed system achieved an average end-to-end recognition rate of 96.9% across eight public datasets (from five different regions) used in the experiments, outperforming both previous works and commercial systems in the ChineseLP, OpenALPR-EU, SSIG-SegPlate and UFPR-ALPR datasets. In the other datasets, the proposed approach achieved competitive results to those attained by the baselines. Our system also achieved impressive frames per second (FPS) rates on a high-end GPU, being able to perform in real time even when there are four vehicles in the scene. An additional contribution is that we manually labeled 38,351 bounding boxes on 6,239 images from public datasets and made the annotations publicly available to the research community.
The Processing Sector of the Sugar Industries of Cuba and Florida
Creators: name: Castellanos, Lazaro Peno
name: Alvarez, Jose
name: Castellanos, Lazaro Peno
name: Alvarez, Jose
Publisher: name: Unknown
Year: 1997
Subjects: subject: Crop Production/Industries
subject: Production Economics
subject: Cuba
subject: efficiency
subject: energy
subject: Florida
subject: sugar
subject: UBPC

description: The main characteristics of the industrial (processing) sector of the sugar industries in Cuba and Florida are analyzed. In addition to the discussion on industrial parameters and industry efficiency in both places, the section on Cuba includes a description of the current process of economic reforms taking place in its sugar agro-industry.
Maximizing the Impact of New Physics in $b\rightarrow c τν$ Anomalies
Creators: name: Asadi, Pouya
name: Shih, David
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We develop a rigorous, semi-analytical method for maximizing any $b\to cτν$ observable in the full 20-real-dimensional parameter space of the dimension 6 effective Hamiltonian, given some fixed values of $R_{D^{(*)}}$. We apply our method to find the maximum allowed values of $F^L_{D^*}$ and $R_{J/ψ}$, two observables which have both come out higher than their SM predictions in recent measurements by the Belle and LHCb collaborations. While the measurements still have large error bars, they add to the existing $R_{D^{(*)}}$ anomaly, and it is worthwhile to consider NP explanations. It has been shown that none of the existing, minimal models in the literature can explain the observed values of $F^L_{D^*}$ and $R_{J/ψ}$. Using our method, we will generalize beyond the minimal models and show that there is no combination of dimension 6 Wilson operators that can come within $1σ$ of the observed $R_{J/ψ}$ value. By contrast, we will show that the observed value of $F^L_{D^*}$ can be achieved, but only with sizable contributions from tensor and mixed-chirality vector Wilson coefficients.
description: 18 pages, 3 figures
Stability of Satellites Around Close-in Extrasolar Giant Planets
Creators: name: Barnes, Jason W.
name: O'Brien, D. P.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the long-term dynamical stability of hypothetical moons orbiting extrasolar giant planets. Stellar tides brake a planet's rotation and, together with tidal migration, act to remove satellites; this process limits the lifetimes of larger moons in extrasolar planetary systems. Because more massive satellites are removed more quickly than less massive ones, we are able to derive an upper mass limit for those satellites that might have survived to the present day. For example, we estimate that no primordial satellites with masses greater than 7 x 10^{-7} M_Earth$ (~ \70km radius for rho=3 g cm^{-3}) could have survived around the transiting planet HD209458b for the age of the system. No meaningful mass limits can be placed on moons orbiting Jovian planets more than ~0.6 AU from their parent stars. Earth-like moons of Jovian planets could exist for 5 Gyr in systems where the stellar mass is greater than 0.15 M_Sun. Transits show the most promise for the discovery of extrasolar moons -- we discuss prospects for satellite detection via transits using space-based photometric surveys and the limits on the planetary tidal dissipation factor Q that a discovery would imply.
description: 8 pages, 3 figures, to be published in Aug 20 ApJ
Deep spectroscopy of the low-metallicity blue compact dwarf galaxy SBS 0335-052
Creators: name: Izotov, Y. I.
name: Chaffee, F. H.
name: Schaerer, D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The results of deep long-slit spectroscopy of the extremely low-metallicity blue compact dwarf (BCD) galaxy SBS 0335-052 are presented. Down to intensity levels of 10^{-3 ... -4} of Hbeta, unprecedented for spectroscopy of extra-galactic giant H II regions, we detect numerous weak permitted and forbidden nebular lines in the brightest part of the galaxy. With varying degrees of confidence, the detections include lines of high-ionization ions like Fe^{4+} -Fe^{6+}, implying very hard ionizing radiation. Two broad emission features, possibly from Wolf-Rayet stars, and stellar He II 4200 absorption are seen in the same region. The large spatial extent of He II 4686 emission (implying the presence of sufficient ionizing photons with energies above 54 eV) and the spatial distribution of the electron temperature suggest that at least some part of the hard radiation is associated with shocks. Extended Halpha emission is detected over ~ 6 - 8 kpc, a much larger area than in previous studies, suggesting that hot ionized gas is spread out far away from the central ionizing clusters. This shows that nebular line and continuous emission can significantly modify the colours of these extended regions and must be taken into account in studies of the underlying stellar population.
description: 5 pages, 3 Postscript figures, accepted for publication in the Astronomy and Astrophysics
Low inclination jets driving equatorial outflows in quasar host galaxies
Creators: name: Girdhar, Aishwarya
name: Harrison, C.
name: Mainieri, V.
Publisher: name: Zenodo
Year: 2021

description: As part of our Quasar Feedback Survey of z<0.2 quasars we are using ESO/VIMOS and ESO/MUSE to spatially-resolve ionised-gas and stellar kinematics in quasar host galaxies. Combined with multi-wavelength information we are assessing: (1) the properties of galactic multiphase outflows driven by jets and/or winds; (2) what impact these have on the star formation (SF) properties of the host galaxies. I will give an overview of our survey, highlighting the crucial role of ESO's spectroscopic instruments. As a showcase, I will present detailed observations of a target. We have used MUSE, to measure gas and the stellar kinematics, and isolated non-gravitational motion caused by the small-scale radio jet that is ploughing into the galaxy disk. We have further analysed the prevalence of the molecular phase of the outflow by using the data from ALMA. By combining the study of the ionised and molecular gas, to the stellar kinematics, we can infer the feedback effects on SF in the host galaxy.
Ordering of the Heisenberg Spin Glass in High Dimensions
Creators: name: Imagawa, Daisuke
name: Kawamura, Hikaru
Publisher: name: arXiv
Year: 2002
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Ordering of the Heisenberg spin glass with the nearest-neighbor Gaussian coupling is investigated by equilibrium Monte Carlo simulations in four and five dimensions. Ordering of the mean-field Heisenberg spin-glass is also studied for comparison. Particular attention is paid to the nature of the spin-glass and the chiral-glass orderings. Our numerical data suggest that, in five dimensions, the model exhibits a single spin-glass transition at a finite temperature, where the spin-glass order accompanying the simultaneous chiral-glass order sets in. In four dimensions, by contrast, the model exhibits a chiral-glass transition at a finite temperature, not accompanying the standard spin-glass order. The critical region associated with the chiral-glass transition, however, is very narrow, suggesting that dimension four is close to the marginal dimensionality.
description: 18 pages, 12 figures
The Radio-to-Submillimeter Flux Density Ratio of Galaxies as a Measure of Redshift
Creators: name: Rengarajan, T. N.
name: Takeuchi, Tsutomu T.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We re-examine the technique of determining the redshifts of galaxies from the ratio of the submillimeter-to-radio continuum flux densities based on a recently published catalog of 850~$μ$m sources. We derived the expected variation of this ratio as a function of redshift incorporating the expected average luminosity and the spectral energy distribution (SED) of dust emission and the radio continuum. We find that the existing data for most of the high redshift ($z \gtsim 1$) sources correspond to our new calculation. Amongst the well-identified sources, there is none with an index significantly higher than predicted. Sources which have an index lower than predicted are either within the error zone or much lower, the latter presumably having AGN-dominated radio-continuum emission. We find the median redshift to be $\sim 2$, which is consistent with that deduced by previous work ($\sim 3$) within the error. We also discuss the various systematic effects that can affect the accuracy of the redshift estimate. We examine other methods of redshift estimation, like photometric ratio in the submillimeter and locating the peak of the SED in the rest system of the objects. We conclude that while the various methods are helpful in identifying high-redshift objects and making a crude estimate of the redshift, they are not, at present, accurate enough for a detailed study of redshift distribution of the submillimeter galaxies.
description: 6 pages LaTeX, PASJ in press