cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Macrophthalmus (Macrophthalmus) telescopicus Owen 1839
Creators: name: Castro, Peter
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Macrophthalmidae
Macrophthalmus
Macrophthalmus telescopicus

description: Macrophthalmus (Macrophthalmus) telescopicus Owen, 1839
 Gelasimus telescopicus Owen, 1839: 78, pl. 24, figs. 1, 1 a–f [type locality: O‘ahu; type material destroyed (see Crane 1975: 324)].
 Additional Hawaiian Is. records:
 Macrophthalmus compressipes Randall, 1840: 123 [type locality: “ Sandwich Islands; ” syntypes: ANSP CA3074].
 Macrophthalmus podophthalmus Eydoux & Souleyet, 1842: 241. pl. 3, figs. 6 [color], 7 [type locality: îles “Sandwich;” holotype: MNHN-B12634].
 Macrophthalmus telescopicus Owen, 1839 — Dana 1852b: 314, 1577 [“Sandwich Is.”]. — Cano 1889b: 229 [O‘ahu]. — Rathbun 1906: 834 [O‘ahu, H.I.]. — Edmondson 1946: 311, fig. 185 a [O‘ahu]; 1962b: 20, fig. 8b [O‘ahu, Maui]. — Tinker 1965: 122, pl. 49 [H.I.]. — Banner 1968: 25 [O‘ahu]. — Titcomb et al. 1979: 367 [H.I.]. — Coles et al. 1997: C–74 [O‘ahu]. — Coles, DeFelice & Eldredge 1999: 156 [O‘ahu].
 Macrophthalmus (Macrophthalmus) telescopicus Owen, 1839 — Serène 1973a: 109, figs. 2c–e, pl. 3, figs. A, B, Pl. 4, fig. D [H.I.].
 Remarks. Macrophthalmus verreauxi H. Milne Edwards, 1848 (a junior synonym of M. telescopicus Owen, 1839) was listed as occurring in the Hawaiian Is. by Sakai (1976), Davie (2002), and McLaughlin et al. (20005) although no previous records of M. (Macrophthalmus) telescopicus under this name are known from the archipelago.
 Taxonomy. Serène (1973a), Nagai et al. (2006), McLay et al. (2010)
 Geographical distribution. Across Indo-West Pacific region.
 Habitat. Soft sediments in shallow subtidal.
description: Published as part of Castro, Peter, 2011, Catalog of the anomuran and brachyuran crabs (Crustacea: Decapoda: Anomura, Brachyura) of the Hawaiian Islands 2947, pp. 1-154 in Zootaxa 2947 (1) on pages 122-123, DOI: 10.11646/zootaxa.2947.1.1, http://zenodo.org/record/5283044
Scalar leptoquark effects on $B \to μ\barν$ decay
Creators: name: Hou, Wei-Shu
name: Modak, Tanmoy
name: Wong, Gwo-Guang
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: Purely leptonic $B$ meson decays provide unique probes for physics Beyond the Standard Model. We study the impact of a scalar leptoquark, $S_1$, on $B \to μ\barν$ decay. We find that, for $m_{S_1}\sim 1$ TeV, the $S_1$ leptoquark can modify the $B \to μ\barν$ rate significantly. Such a leptoquark can in prinicple also alter the $B \to τ\barν$ rate. However, current searches from LHC and low energy physics provide some constraints on the parameter space.
description: matches the published version
Localisation of massive fermions on the brane
Creators: name: Ringeval, C.
name: Peter, P.
name: Uzan, J. -P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We construct an explicit model to describe fermions confined on a four dimensional brane embedded in a five dimensional anti-de Sitter spacetime. We extend previous works to accommodate massive bound states on the brane and exhibit the transverse structure of the fermionic fields. We estimate analytically and calculate numerically the fermion mass spectrum on the brane, which we show to be discrete. The confinement life-time of the bound states is evaluated, and it is shown that existing constraints can be made compatible with the existence of massive fermions trapped on the brane for durations much longer than the age of the Universe.
description: 20 pages, LaTeX-RevTex, 15 figures, submitted to PRD
Additional file 1 of Phytotoxin sorption to clay minerals
Creators: name: Schönsee, Carina D.
name: Wettstein, Felix E.
name: Bucheli, Thomas D.
Publisher: name: figshare
Year: 2021
Subjects: subject: Space Science
subject: Medicine
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: Cancer
subject: 60506 Virology

description: Additional file 1: Table S1. Analyzed phytotoxins and their experimental and predicted properties; Table S2. Molecular structures of all investigated phytotoxins; Table S3. Measurement wavelength, recovery and pKa values of all analyzed phytotoxins; Figure S1. Flow rate effects on retention factor (k) observed for the phytotoxins CAFfeine, CYTisine, GALanthamine, LYcOrine and STRophanthidin on a 1% montmorillonite column; Figure S2. Retention time (tR) comparison of the non-retained tracers nitrate and thiourea (THI) on a 1% montmorillonite column; Table S4. Maximum sorbed concentrations and the percentage of occupied cation exchange sites on both montmorillonite and kaolinite; Figure S3. Amaryllidaceae alkaloid (GALanthamine, LYcOrine) sorption isotherms on kaolinite and montmorillonite; Figure S4. Amine (HORdenine) sorption isotherms on kaolinite and montmorillonite; Figure S5. Cardenolide and bufadienolide (CINobufagin, OLEandrin) sorption isotherms on kaolinite and montmorillonite; Figure S6. Imidazole alkaloid (PILocarpine) sorption isotherms on kaolinite and montmorillonite; Figure S7. Indole alkaloid (BRUcine, GELsemine, GRAmine, STrYchnine, VINcamine, YOHimbine) sorption isotherms on kaolinite and montmorillonite; Figure S8. Isoquinoline alkaloid (BICuculline, ISoCorydine, NUCiferine, PROtopine) sorption isotherms on kaolinite and montmorillonite; Figure S9. Pyrrolizidine alkaloid (ECHimidine, ERUcifoline, JACobine, LASiocarpine, MONocrotaline, RETrorsine, SEnKirkine, SENecionine) sorption isotherms on kaolinite and montmorillonite; Figure S10. Pyridine alkaloid (NICotine) sorption isotherms on kaolinite and montmorillonite; Figure S11. Quinoline alkaloid (QUInine) sorption isotherms on kaolinite and montmorillonite; Figure S12. Quinolizidine alkaloid (CYTisine, MATrine, SOPhocarpine) sorption isotherms on kaolinite and montmorillonite; Figure S13. Steroid alkaloid (CEVadine) sorption isotherms on kaolinite and montmorillonite; Figure S14. Tropolone alkaloid (COLchicine) sorption isotherms on montmorillonite.
Radio-selected Galaxies in Very Rich Clusters at z < 0.25: II. Radio Properties and Analysis
Creators: name: Morrison, Glenn E.
name: Owen, Frazer N.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (Abridged) We report on the properties of radio-selected galaxies within 30 very-rich Abell clusters with z < 0.25. These radio data sample the ultra-faint (L(1.4) > 2E22 W/Hz) radio galaxy population with M_R < -21 using the well-known FIR/radio correlation to link the radio with ongoing star formation within individual cluster galaxies. These radio-selected galaxies reveal the `active' galaxy population (starburst and active galactic nuclei) within these rich cluster environments that can be identified regardless of their level of dust obscuration. For all clusters in our sample, we are sensitive to star formation rates (M > 5 M_sun) > 5 M_sun/yr. We have found that the excess number of low-luminosity `starburst' radio-selected galaxies (SBRG) found by Owen et. al. 1999 in Abell 2125 is not indicative of other rich clusters in our sample. The average fraction of SBRG is = 0.022+/-0.003. The A2125 fraction is f(SBRG) = 0.09+/-10.03 which is significantly different from the sample average at a >99.99% confidence level. The bimodal structure of both the x-ray brightness distribution and optical adaptively smoothed images of A1278 and A2125 suggests that ongoing cluster-cluster mergers may be enhancing this SBRG population. There is a significant spatial distribution difference between the low and high-luminosity (HLRG) radio-selected populations. The HLRGs seem to be a subclass of the cluster's massive red elliptical population, while the SBRGs have a projected radial distribution more like the blue spiral population. Our results indicate that most of the SBRGs are probably gas-rich disk galaxies undergoing > 5 M_sun/yr of star-formation.
description: 18 pages, 6 figures, accepted by AJ
Productive Impacts of Cash Transfer and Conditional Cash Transfer Programs in Bangladesh: Propensity Score Matching Analysisi
Creators: name: Begum, Ismat
name: Alam, Mohammad
name: Haque, M.
name: Begum, Ismat
name: Alam, Mohammad
name: Haque, M.
Publisher: name: Unknown
Year: 2015
Subjects: subject: Consumer/Household Economics
subject: Public Economics
subject: Cash transfer
subject: conditional cash transfer
subject: safety net
subject: impact
subject: PSM
subject: Bangladesh

description: Bangladesh has a comprehensive portfolio of social protection programs, fruits are yet to be reaped more effectively. However, the extent of their productive impacts is not yet analysed in great detail. The objective of this study is to estimate the productive impacts of cash transfer (old age allowance, allowances for the widowed, destitute and deserted women) and conditional cash transfer programs (stipend for primary students, secondary students and a combination of CFW, FFW, VGD, and 100 days employment scheme) in Bangladesh. The study used the HIES 2010 data. The study used PSM method. The outcome variables were i) labor allocation changes, ii) income generating activities, iii) investments in land, tools, animals, family enterprises, durable goods and housing, iv) investments in human capital, and v) coping mechanisms. Results show that different programs are producing different outcomes. So, policy makers should implement a number of interventions simultaneously to serve the needy.
Correlation-function spectroscopy of inelastic lifetime in heavily doped GaAs heterostructures
Creators: name: Könemann, J.
name: König, P.
name: Schmidt, T.
name: McCann, E.
name: Fal'ko, V. I.
name: Haug, R. J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Measurements of resonant tunneling through a localized impurity state are used to probe fluctuations in the local density of states of heavily doped GaAs. The measured differential conductance is analyzed in terms of correlation functions with respect to voltage. A qualitative picture based on the scaling theory of Thouless is developed to relate the observed fluctuations to the statistics of single particle wavefunctions. In a quantitative theory correlation functions are calculated. By comparing the experimental and theoretical correlation functions the effective dimensionality of the emitter is analyzed and the dependence of the inelastic lifetime on energy is extracted.
description: 41 pages, 14 figures
食品中750种污染物免疫定量快速检测技术和产品
Creators: name: 胥 传来
Publisher: name: figshare
Year: 2021
Subjects: subject: 90804 Food Packaging, Preservation and Safety
subject: FOS: Other engineering and technologies

description: 江苏省奖附加材料清单
Superconducting Properties of Heavy Fermion UTe$_2$ Revealed by $^{125}$Te-Nuclear Magnetic Resonance
Creators: name: Nakamine, Genki
name: Kitagawa, Shunsaku
name: Ishida, Kenji
name: Tokunaga, Yo
name: Sakai, Hironori
name: Kambe, Shinsaku
name: Nakamura, Ai
name: Shimizu, Yusei
name: Homma, Yoshiya
name: Li, Dexin
name: Honda, Fuminori
name: Aoki, Dai
Publisher: name: arXiv
Year: 2019
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We have performed the $^{125}$Te-nuclear magnetic resonance (NMR) measurement in the field along the $b$ axis on the newly discovered superconductor UTe$_2$, which is a candidate of a spin-triplet superconductor. The nuclear spin-lattice relaxation rate divided by temperature $1/T_1T$ abruptly decreases below a superconducting (SC) transition temperature $T_c$ without showing a coherence peak, indicative of UTe$_2$ being an unconventional superconductor. It was found that the temperature dependence of $1/T_1T$ in the SC state cannot be understood by a single SC gap behavior but can be explained by a two SC gap model. The Knight shift, proportional to the spin susceptibility, decreases below $T_c$, but the magnitude of the decrease is much smaller than the decrease expected in the spin-singlet pairing. Rather, the small Knight-shift decrease as well as the absence of the Pauli-depairing effect can be interpreted by the spin triplet scenario.
description: 10 pages, 8 figures, including supplemental materials, chosen as Editors' choice, open access
Chiral dynamics with strange quarks: Mysteries and opportunities
Creators: name: Meißner, Ulf-G.
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Recent developments and open issues in chiral dynamics with strange quarks are reviewed. Topics include: Order parameters of chiral symmetry breaking, the flavor dependence of these order parameters, speculations about the phase structure of QCD with varying number of flavors, OZI violation and its natural emergence in case of a small strange quark condensate, heavy kaon chiral perturbation theory, an update on pion-pion, pion-kaon and pion-nucleon sigma terms, the dynamics and nature of scalar mesons, the role of the scalar pion and kaon form factors, attempts to describe some strange baryons employing coupled channel dynamics tied to unitarity and chiral perturbation theory, and the role of final state interactions in Goldstone boson pair production in proton-proton collisions.
description: 26 pp, LaTeX2e, 14 figs (uses epsf,epsfig), contribution to the ``Eta Physics Handbook'', Workshop on Eta Physics, Uppsala, Sweden, Oct. 2001, 2 figs replaced, references added
Computational Study of Magnetic Behaviour in Ni-Adsorbed Nb2C-OF MXene using Density Functional Theory
Creators: name: Khan, Zarah
name: Khan, Saleem Ayaz
name: Zaheer, Ayesha
name: Rizwan, Syed
Publisher: name: arXiv
Year: 2025
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Magnetic 2D materials have achieved significantly consideration owing to their encouraging applications. A variation of these 2D materials by occurrence of defects, by the transition-metal doping or adsorption or by the surface functionalization can initiate both the spin-polarization and magnetic properties in these materials. Density functional theory (DFT) is used to determine the electric, magnetic properties along with the electronic structures and stability of synthesized two-dimensional materials. This work describes the magnetic properties of Ni-ad-Nb2C-OF MXene. The study focuses on the computational approach based first principal calculation providing insight onto the magnetic properties of adsorbed compound and comparing it with pristine Nb2C-OF MXene. The pristine Nb2C-OF and Ni-ad-Nb2C-OF structures are simulated and optimized using Wien2k software. Using exchange-correlational functionals; spin-GGA and spin-GGA+U (for Nickel U= 6eV), Ni-ad-Nb2C-OF electronic band structure is found to be metallic having magnetic moment calculated +1.01516μ_\b{eta} showing its non-superconducting and ferromagnetic behaviour. Owing to this magnetic nature, this 2D compound can be used for new upcoming applications such as spintronics and nano magnetic data storage devices.
description: 9 figures
Additional file 1 of Extended similarity indices: the benefits of comparing more than two objects simultaneously. Part 1: Theory and characteristics†
Creators: name: Miranda-Quintana, Ramón Alain
name: Bajusz, Dávid
name: Rácz, Anita
name: Héberger, Károly
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer

description: Additional file 1. Tables S1–S5 and figures S1–S21 with binary similarity formulas, rankings and ANOVA results.
Eupelmus (Episolindelia) Girault
Creators: name: Gibson, Gary A. P.
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eupelmidae
Eupelmus

description: Eupelmus (Episolindelia) Girault
 Episolindelia Girault, 1914.
 Eupelmus (Episolindelia); Gibson, 1995.
 Remarks. Females of E. (Episolindelia) are differentiated from females of E. (Eupelmus) by the features given in Gibson (1995) and in the key to subgenera above. Females are always macropterous, have hyaline forewings, and the ovipositor sheaths are obliquely strigose basally. The strigose region constitutes the basal dark region in those females with a bicolored sheath, and usually has noticeably longer setae dorsally and often is slightly thinner than the rest of the sheath. The latter feature is most conspicuous for females of E. varicauda in which the sheaths appear somewhat clavate.
 Unlike males of E. (Eupelmus) and most males of E. (Macroneura), it is likely that males of at least regional species of E. (Episolindelia) do not have a differentiated long seta below the malar sulcus or a row of distally curved setae along the ventral margin of the pedicel. This conclusion is based on the males of E. australiensis and the proposed sex association for E. rubicola. It is further likely that regional males E. (Episolindelia) have a filiform or clavate flagellum depending on whether conspecific females have a similar antennal structure (cf. Figs 1, 6 and 3, 7).
description: Published as part of Gibson, Gary A. P., 2011, 2951, pp. 1-97 in Zootaxa 2951 on page 9
The complex scaling behavior of non--conserved self--organized critical systems
Creators: name: Drossel, Barbara
Publisher: name: arXiv
Year: 2002
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The Olami--Feder--Christensen earthquake model is often considered the prototype dissipative self--organized critical model. It is shown that the size distribution of events in this model results from a complex interplay of several different phenomena, including limited floating--point precision. Parallels between the dynamics of synchronized regions and those of a system with periodic boundary conditions are pointed out, and the asymptotic avalanche size distribution is conjectured to be dominated by avalanches of size one, with the weight of larger avalanches converging towards zero as the system size increases.
description: 4 pages revtex4, 5 figures
Additional file 1 of How effective are electronic cigarettes for reducing respiratory and cardiovascular risk in smokers? A systematic review
Creators: name: Goniewicz, Maciej L.
name: Miller, Connor R.
name: Sutanto, Edward
name: Li, Dongmei
Publisher: name: figshare
Year: 2020
Subjects: Medicine
Biotechnology
Biological Sciences not elsewhere classified
Science Policy

description: Additional file 1: Table S1. Summary of Search Results. Table S2. Details of the PubMed run (conducted September 17th, 2020). Table S3. Details of the Embase run (conducted September 17th, 2020). Figure S1. Screenshot depicting the Embase run (conducted September 17th, 2020). Appendix 1. Calculation of Odds Ratios (ORs) for Composite Smoking and Vaping Variables. Appendix 2. Calculation of Odds Ratios (ORs) for Separate Smoking and Vaping Variable. Appendix 3. Reference list of 51 studies excluded after full text screening.
Agricultural Trade, Biodiversity Effects and Food Price Volatility
Creators: name: Bellora, Cecilia
name: Bourgeon, Jean-Marc
name: Bellora, Cecilia
name: Bourgeon, Jean-Marc
Publisher: name: Unknown
Year: 2015
Subjects: subject: Agribusiness
subject: Agricultural and Food Policy
subject: Agricultural Finance
subject: Food Consumption/Nutrition/Food Safety
subject: agricultural trade
subject: food prices
subject: agrobiodiversity
subject: pesticides

description: Biotic elements such as pests create biodiversity effects that increase production risks and impede land productivity when agriculture becomes more specialized. We show in a Ricardian two-country trade setup that production specialization is incomplete under free trade because of the decrease in land productivity. Pesticides allow farmers to reduce these effects, but they are damaging for the environment and for human health. When regulating farming practices under free trade, governments face a trade-off: they are induced to restrict pesticides use compared to autarky because national food consumption depends less on them, but they also want to preserve the competitiveness of their agricultural sector on international markets. We show that at the symmetric equilibrium under free trade, restrictions on pesticides are generally more stringent than under autarky. As a result, trade increases the price volatility of crops produced by both countries, and of some or all of the crops that are country-specific depending of the intensity of the biodiversity effects.
On Holomorphic Factorization in Asymptotically AdS 3D Gravity
Creators: name: Krasnov, Kirill
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: This paper studies aspects of ``holography'' for Euclidean signature pure gravity on asymptotically AdS 3-manifolds. This theory can be described as SL(2,C) CS theory. However, not all configurations of CS theory correspond to asymptotically AdS 3-manifolds. We show that configurations that do have the metric interpretation are parameterized by the so-called projective structures on the boundary. The corresponding asymptotic phase space is shown to be the cotangent bundle over the Schottky space of the boundary. This singles out a ``gravitational'' sector of the SL(2,C) CS theory. It is over this sector that the path integral has to be taken to obtain the gravity partition function. We sketch an argument for holomorphic factorization of this partition function.
description: 32+1 pages, no figures; (v2) one reference added, a statement regarding priorities modified; (v3) presentational changes, an important sign mistake corrected
Food Crop Marketing and Agricultural Productivity in a High Price Environment: Evidence and Implications for Mozambique
Creators: name: Benfica, Rui
name: Boughton, Duncan
name: Uaiene, Rafael
name: Benfica, Rui
name: Boughton, Duncan
name: Uaiene, Rafael
Publisher: name: Unknown
Year: 2015
Subjects: subject: Agribusiness
subject: Food Consumption/Nutrition/Food Safety
subject: Marketing
subject: FOS: Economics and business
subject: Agricultural productivity
subject: endogeneity
subject: intensification
subject: and marketing performance

description: The recent high food price environment is an opportunity for Africa’s smallholder farmers. This paper assesses the relationship between agricultural productivity and market participation/performance in smallholder response to a high food price environment in Mozambique. We use panel data before and after the change in price regime to identify the relative importance of market access/participation versus household and farm-level factors in explaining productivity differences. Conversely, we look at the relative importance of productivity investments and outcomes versus marketing investments in explaining household market performance. Results suggest that creating an enabling environment for greater access to markets can have important effects on productivity of cereals and groundnuts/beans, but direct investments that lead to increased adoption of productivity enhancing technologies are also important to maximize market access benefits. Finally, we highlight investment priorities to strengthening agricultural market participation and performance and improve productivity.
The Effects of Smallholder Agricultural Involvement on Household Food Consumption and Dietary Diversity: Evidence from Malawi
Creators: name: Benfica, Rui
name: Kilic, Talip
name: Benfica, Rui
name: Kilic, Talip
Publisher: name: Unknown
Year: 2015
Subjects: subject: Agribusiness
subject: Agricultural Finance
subject: Consumer/Household Economics
subject: Agricultural involvement
subject: consumption
subject: dietary diversity
subject: and endogeneity

description: We investigate how household agricultural involvement affects food consumption and dietary diversity in Malawi. Ceteris paribus, a 10% increase in onfarm income share increases food consumption/capita by 2.9%, calorie intake/person/day by 1.7%, and leads to small improvements in dietary diversity. There are significant differences in the relationship between on-farm income shares and caloric shares: a positive and significant relationship with the shares from energy dense/low protein cereals/grains, but not significant with shares from nuts/pulses and sugars. Negative relationships are found with shares from roots/tubers, vegetables/fruits, oils/fats, and meat/fish/milk. While food consumption and dietary diversity increase with agricultural involvement, the quality of diets is an issue. As purchased calories are associated with richer/high quality diets, particularly protein rich, households with lower dependency on agriculture meet those diets more easily, highlighting the importance of crop and income diversification to dietary diversity. Nutrition education and crop diversification programs can improve food security and nutritional outcomes.
Time-dependent AMS-02 electron-positron fluxes in an extended force-field model
Creators: name: Kuhlen, Marco
name: Mertsch, Philipp
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: The magnetised solar wind modulates the Galactic cosmic ray flux in the heliosphere up to rigidities as high as 40 GeV. In this work, we present a new and straightforward extension of the popular, but limited force-field model, thus providing a fast and robust method for phenomenological studies of Galactic cosmic rays. Our semi-analytical approach takes into account charge-sign dependent modulation due to drifts in the heliospheric magnetic field and has been validated via comparison to a fully numerical code. Our model nicely reproduces the time-dependent AMS-02 measurements and we find the strength of diffusion and drifts to be strongly correlated with the heliospheric tilt angle and magnitude of the magnetic field. We are able to predict the electron and positron fluxes beyond the range for which measurements by AMS-02 have been presented. We have made an example script for the semi-analytical model publicly available and we urge the community to adopt this approach for phenomenological studies.
description: 5+5 pages, 2+2 figures; example script available at https://git.rwth-aachen.de/kuhlenmarco/effmod-code; Accepted for publication in PRL
Additional file 1: of Identification and characterization of histone modification gene family reveal their critical responses to flower induction in apple
Creators: name: Fan, Sheng
name: Wang, Jue
name: Lei, Chao
name: Gao, Cai
name: Yang, Yang
name: Li, Youmei
name: An, Na
name: Zhang, Dong
name: Han, Mingyu
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology

description: Table S1. List of Pfam accession number of each HMs gene family (DOCX 13Â kb)
Standar Penulisan Artikel Ilmiah
Creators: name: Mochammad Tanzil Multazam
Publisher: name: Zenodo
Year: 2021
Subjects: author publication ethics
etika publikasi ilmiah untuk penulis
authorship
Relawan Jurnal Indonesia
Universitas Muhammadiyah Sidoarjo

description: Disampaikan pada acara webinar yang dselenggarakan oleh duniadosen.com. Pada tanggal 21 Mei 2021 pukul 09.00 WIB.
Atiyah-Manton Approach to Skyrmion Matter
Creators: name: Park, B. -Y.
name: Min, D. -P.
name: Rho, M.
name: Vento, V.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We propose how to approach, and report on the first results in our effort for, describing nuclear matter starting from the solitonic picture of baryons which is supposed to represent QCD for large number of colors. For this purpose, the instanton-skyrmion connection of Atiyah and Manton is exploited to describe skyrmion matter. We first modify 't Hooft's multi-instanton solution so as to suitably incorporate proper dynamical variables into the skyrmion matter and then by taking these variables as variational parameters, we show that they cover a configuration space sufficient to adequately describe the ground state properties of nuclear matter starting from the skyrmion picture. Our results turn out to be comparable to those so far found in different numerical calculations, with our solution reaching stability at high density for a crystal structure and obtaining a comparable value for the energy per baryon at the minimum, thus setting the stage for the next step.
Additional file 2 of Roquin1 inhibits the proliferation of breast cancer cells by inducing G1/S cell cycle arrest via selectively destabilizing the mRNAs of cell cycle–promoting genes
Creators: name: Lu, Wenbao
name: Zhou, Meicen
name: Wang, Bing
name: Liu, Xueting
name: Li, Bingwei
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Additional file 2.
Market internalized value of bio-friendly agriculture: An evaluation of impact of stork-friendly rice production on a local economy
Creators: name: Hayashi, Takashi
name: Takahashi, Yoshifumi
name: Hayashi, Takashi
name: Takahashi, Yoshifumi
Publisher: name: Unknown
Year: 2015
Subjects: subject: Agricultural and Food Policy
subject: Environmental Economics and Policy
subject: Bio-friendly agriculture
subject: Biodiversity
subject: Ecosystem service
subject: Internalized value
subject: Input-output analysis

description: Although there are many studies on evaluating ecosystem services in recent years, most of the studies focus on the externality of ecosystem services. Fundamentally, it is important to understand market internalized value of ecosystem services, but studies on this point of view are rare as far as the author knows. This study evaluates the impacts on the local economy, as an internalized value of ecosystem services, caused by shifting from conventional to bio-friendly rice farming, using a case study of stork-friendly rice farming (to help conserve white storks) in Toyooka, Japan. After applying an input-output analysis, we consider whether stork-friendly rice farming created a net positive economic impact on the local economy. The results shows that changing from conventional to stork-friendly rice faming had a high induced effect and that shifting to stork-friendly rice faming creates a net positive economic impact on the local economy.
The Open Universe VOU-Blazars tool
Creators: name: Chang, Yu-Ling
name: Brandt, Carlos
name: Giommi, Paolo
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Blazars are a remarkable type of Active Galactic Nuclei (AGN) that are playing an important and rapidly growing role in today's multi-frequency and multi-messenger astrophysics. In the past several years, blazars have been discovered in relatively large numbers in radio, microwave, X-ray and gamma-ray surveys, and more recently have been associated to high-energy astrophysical neutrinos and possibly to ultra-high energy cosmic rays. Blazars are expected to dominate the high-energy extragalactic sky that will soon be surveyed by the new generation of very-high-energy gamma-ray observatories such as CTA. In parallel to the discovery of many blazars at all frequencies, the technological evolution, together with the increasing adoption of open data policies is causing and exponential growth of astronomical data that is freely available through the network of Virtual Observatories (VO) and the web in general, providing an unprecedented potential for multi-wavelength and multi-messenger data analysis. We present VOU-Blazars, a tool developed within the OU, initiative that has been designed to facilitate the discovery of blazars and build their spectral energy distributions (SED) using multi-wavelength photometric and spectral data that are available from public archives, or that have been generated as part of the OU, initiative and are accessible through VO services. VOU-Blazars implements a heuristic approach based on the well known SED that differentiate blazars from other astronomical sources. The VOU-Blazars outputs are flux tables, bibliographic references, sky plots and SEDs. VOU-Blazars has been extensively tested during the selection of new high-energy peaked (HSP) blazars recently published in the 3HSP catalog, and has been used to search for blazar counterparts of Fermi 3FHL, Fermi 4FGL, AGILE sources, and of IceCube astrophysical neutrinos.
Large-Scale, Low-Energy Excitations in the Two-Dimensional Ising Spin Glass
Creators: name: Hartmann, A. K.
name: Young, A. P.
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: We study large-scale, low-energy excitations in the Ising spin glass with Gaussian interactions in two-dimensions at zero temperature, using an optimization algorithm to determine exact ground states. Periodic boundary conditions are applied. Our results for the fractal dimension of the surface, d_s, and stiffness exponent, theta', for "droplet" excitations, are in reasonable agreement with estimates from "domain wall" calculations, and so support the predictions of the "droplet theory". Restricting our analysis to small lattices, we do not find an effective value of theta' close to -0.47 as has been recently proposed. The effects of averaging over droplets of different sizes are studied and are also found to be too small to give theta' approx -0.47 for smaller sizes. Larger corrections to finite-size scaling would be needed in three and four dimensions in order for the numerical data used to support the "TNT" scenario to be compatible with the droplet theory prediction that the stiffness exponent is the same for droplets and domain walls.
description: 10 pages, 11 figures. Replaced with published version
Ferulic acid enhances the radiation sensitivity of lung and liver carcinoma cells by collapsing redox homeostasis: mechanistic involvement of Akt/p38 MAPK signalling pathway
Creators: name: Das, Ujjal
name: Krishnendu Manna
name: Arghya Adhikary
name: Snehasis Mishra
name: Saha, Krishna Das
name: Sharma, Rakhi Dey
name: Biswanath Majumder
name: Sanjit Dey
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer

description: The major drawback of anticancer therapy is the development of resistance against drugs and radiation at the later phase of treatment which may lead to recurrences of the disease. Therefore, strategy was taken to enhance radiation sensitivity of lung (A549) and liver (HepG2) carcinoma cells by treatment with ferulic acid (FA) prior to irradiation. FA pre-treatment initially decreased reactive oxygen species (ROS) level in carcinoma cells which induced reductive stress and cytostasis. To overcome this stress, cellular mechanism increased the Keap1 level to down-regulate nuclear localisation of Nrf2 and its dependent antioxidant system. The antioxidant system reached the lowest level after 3 and 6 h of FA treatment in A549 and HepG2 cells respectively. As endogenous ROS were still being generated at same rate, ROS level was clearly higher than control which changed the reductive stress to oxidative stress. Exposure to γ-radiation in this condition further increased ROS level and caused radio-sensitisation of carcinoma cells. Combination of irradiation (IR) and FA activated mitochondrial apoptotic pathway and concomitantly inhibited the cell cycle progression and survival pathway over the IR group. Moreover, the combination treatment showed significant tumour regression, caspase 3 activation and nuclear fragmentation in tumour tissue compared to radiation alone. In contrast, FA pre-treatment protected peripheral blood mononuclear cells (PBMC) and normal lung fibroblast WI38 cells from radiation damage. Together, combination treatment offers effective strategy of killing cancer cells and demonstrates its potential for increasing the efficacy of radio-therapy.
Polarized Dirac fermions in de Sitter spacetime
Creators: name: Cotaescu, Ion I.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The tetrad gauge invariant theory of the free Dirac field in two special moving charts of the de Sitter spacetime is investigated pointing out the operators that commute with the Dirac one. These are the generators of the symmetry transformations corresponding to isometries that give rise to conserved quantities according to the Noether theorem. With their help the plane wave spinor solutions of the Dirac equation with given momentum and helicity are derived and the final form of the quantum Dirac field is established. It is shown that the canonical quantization leads to a correct physical interpretation of the massive or massless fermion quantum fields.
description: 19 pages, LaTeX w AMS symb
Hybrid Numerical Simulations of Pulsar Magnetospheres
Creators: name: Contopoulos, Ioannis
name: Petri, Jerome
name: Stefanou, Petros
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We continue our investigation of particle acceleration in the pulsar equatorial current sheet (ECS) that began with Contopoulos (2019) and Contopoulos & Stefanou (2019). Our basic premise has been that the charge carriers in the current sheet originate in the polar caps as electron-positron pairs, and are carried along field lines that enter the equatorial current sheet beyond the magnetospheric Y-point. In this work we investigate further the charge replenishment of the ECS. We discovered that the flow of pairs from the rims of the polar caps cannot supply both the electric charge and the electric current of the ECS. The ECS must contain an extra amount of positronic (or electronic depending on orientation) electric current that originates in the stellar surface and flows outwards along the separatrices. We develop an iterative hybrid approach that self-consistently combines ideal force-free electrodynamics in the bulk of the magnetosphere with particle acceleration along the ECS. We derive analytic approximations for the orbits of the particles, and obtain the structure of the pulsar magnetosphere for various values of the pair-formation multiplicity parameter kappa. For realistic values kappa >> 1, the magnetosphere is practically indistinguishable from the ideal force-free one, and therefore, the calculation of the spectrum of high-energy radiation must be based on analytic approximations for the distribution of the accelerating electric field in the ECS.
description: 7 pages, 5 figures, Monthly Notices in press
Non-randomised probability integral transform and additional figures from Model building and assessment of the impact of covariates for disease prevalence mapping in low-resource settings: to explain and to predict
Creators: name: Giorgi, Emanuele
name: Fronterrè, Claudio
name: Macharia, Peter M.
name: Alegana, Victor A.
name: Snow, Robert W.
name: Diggle, Peter J.
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: 111602 Human Biophysics
subject: FOS: Basic medicine
subject: 80109 Pattern Recognition and Data Mining
subject: FOS: Computer and information sciences

description: This paper provides statistical guidance on the development and application of model-based geostatistical methods for disease prevalence mapping. We illustrate the different stages of the analysis, from exploratory analysis to spatial prediction of prevalence, through a case study on malaria mapping in Tanzania. Throughout the paper, we distinguish between predictive modelling, whose main focus is on maximizing the predictive accuracy of the model, and explanatory modelling, where greater emphasis is placed on understanding the relationships between the health outcome and risk factors. We demonstrate that these two paradigms can result in different modelling choices. We also propose a simple approach for detecting over-fitting based on inspection of the correlation matrix of the estimators of the regression coefficients. To enhance the interpretability of geostatistical models, we introduce the concept of domain effects in order to assist variable selection and model validation. The statistical ideas and principles illustrated here in the specific context of disease prevalence mapping are more widely applicable to any regression model for the analysis of epidemiological outcomes but are particularly relevant to geostatistical models, for which the separation between fixed and random effects can be ambiguous.
CLASH-VLT: Enhancement of (O/H) in z=0.35 RXJ 2248-4431 cluster galaxies
Creators: name: Ciocan, B. I.
name: Maier, C.
name: Ziegler, B. L.
name: Verdugo, M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: (Abridged) We explore the Frontier Fields cluster RXJ2248-443 at z~0.35 with VIMOS/VLT spectroscopy from CLASH-VLT, which covers a central region corresponding to almost 2 virial radii. The fluxes of [OII], Hbeta, [OIII], Halpha and [NII] emission lines were measured allowing the derivation of (O/H) gas metallicities, star formation rates based on extinction-corrected Halpha fluxes and active galactic nuclei (AGN) contamination. We compare our sample of cluster galaxies to a population of field galaxies at similar redshifts. We use the location of galaxies in projected phase-space to distinguish between cluster and field galaxies. Both populations follow the star-forming-sequence in the diagnostic diagrams, which allow disentangling between the ionising sources in a galaxy, with only few galaxies classified as Seyfert II. Both field and cluster galaxies follow the "Main-Sequence" of star forming galaxies, with no substantial difference observed between the two populations. In the Mass - Metallicity (MZ) plane, both high mass field and cluster galaxies show comparable (O/H)s to the local SDSS MZ relation, with an offset of low mass galaxies towards higher metallicities. While both the metallicities of "accreted" (R < R500) and "infalling" (R > R500) cluster members are comparable at all masses, the cluster galaxies from the intermediate, mass complete bin show more enhanced metallicities than their field counterparts. The intermediate mass field galaxies are in accordance with the expected (O/H)s from the Fundamental Metallicity relation, while the cluster members deviate strongly from the model predictions. The results of this work are in accordance with studies of other clusters at z < 0.5 and favour the scenario in which the hot halo gas of log(M/Msun)<10.2 cluster galaxies is removed due to mild ram pressure stripping, leading to an increase in their gas-phase metallicity.
description: Accepted for publication in A&A on 22 November 2019
X-ray Spectral Properties of Low-Mass X-ray Binaries in Nearby Galaxies
Creators: name: Irwin, Jimmy A.
name: Athey, Alex E.
name: Bregman, Joel N.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigated the X-ray spectral properties of a collection of low-mass X-ray binaries (LMXBs) within a sample of 15 nearby early-type galaxies observed with Chandra. We find that the spectrum of the sum of the sources in a given galaxy is remarkably similar from galaxy to galaxy when only sources with X-ray luminosities less than 10^39 ergs/s (0.3-10 keV) are considered. Fitting these lower luminosity sources in all galaxies simultaneously yielded a best-fit power law exponent of Gamma = 1.56 +/- 0.02 (or kT_brem = 7.3 +/- 0.3 keV). This is the tightest constraint to date on the spectral properties of LMXBs in external galaxies. There is no apparent difference in the spectral properties of LMXBs that reside inside and outside globular clusters. We demonstrate how the uniformity of the spectral properties of LMXBs can lead to more accurate determinations of the temperature and metallicity of the hot gas in galaxies. Although few in number in any given galaxy, sources with luminosities of 1-2 x 10^39 ergs/s are present in 10 of the galaxies. The spectra of these luminous sources are softer than the spectra of the rest of the sources, and are consistent with the spectra of Galactic black hole X-ray binary candidates when they are in their very high state. The spectra of these sources are very different than those of ultraluminous X-ray sources (ULXs) found within spiral galaxies, suggesting that the two populations of X-ray luminous objects have different formation mechanisms. The number of sources with apparent luminosities above 2 x 10^39 ergs/s is equal to the number of expected background AGN and thus appear to not be associated with the galaxy, indicating that very luminous sources are absent or very rare in early-type galaxies. (Abridged)
description: 11 pages in emulateapj5 style with 4 embedded Postscript figures; to be accepted by ApJ