cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
MOESM6 of Quality of maternal and newborn healthcare services in two public hospitals of Bangladesh: identifying gaps and provisions for improvement
Creators: name: Taposh Biswas
name: Hasnat Sujon
name: M. Rahman
name: Perry, Henry
name: Mahbub Chowdhury
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Marine Biology
subject: Science Policy
subject: Hematology

description: Additional file 6. Checklist_Management of Maternal Complications.docx (Maternal complications management checklist).
Hydaticus (Guignotites) histrio Clark 1864
Creators: name: Hájek, Jiří
Publisher: name: Zenodo
Year: 2006
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Curculionidae
Hydaticus
Hydaticus histrio

description: Hydaticus (Guignotites) histrio Clark, 1864
 Published records. GUÉORGUIEV (1967: 474): ‘ Pakistan: 20 km S von Quetta, 1900 m, 14.V.1965 (Kasy & Vartian)’. VAZIRANI (1969a: 258): ‘ Baluchistan: Muski Dist. (E. Vredenburg)’.
 Material studied. IRAN: 13, ‘ SE Iran, Rask, vall r. Sarbáz, 3-4.4.1973’, ‘ Loc. No. 146, Exp. Nat. Mus. Praha’; 3♀♀, ‘ SE Iran, Bahu-Kalat, 3-4.4.1973’, ‘ Loc. No. 147, Exp. Nat. Mus. Praha’; 1♀, ‘ SE Iran, 25 km W Ghasreghand, 9-10.4.1973’, ‘ Loc. No. 153, Exp. Nat. Mus. Praha’; 13, ‘ SE Iran, 9 km S Espakeh, 10.4.1973’, ‘ Loc. No. 155, Exp. Nat. Mus. Praha’; 13, ‘ Iran, 9.IV.2000, Sistan va Baluchestan Prov., Isa Abad env., (26°54′N, 60°10′E), 600 m’, ‘ Iran 2000 Czech Biological Expedition, J. Hájek & M. Mikát leg. ’; 1 3 2 ♀♀, ‘ Iran, 10.-11.IV.2000, Sistan va Baluchestan prov., 25 km S Kahiri, 1050 m, (26°44′N, 61°04′E)’, ‘ Iran 2000 Czech Biological Expedition, J. Hájek & M. Mikát leg.’ (all NMPC).
description: Published as part of Hájek, Jiří, 2006, The westernmost record of Neptosternus circumductus, and a review of Dytiscidae (Coleoptera) of Baluchistan (Iran, Pakistan), pp. 43-56 in Acta Entomologica Musei Nationalis Pragae 46 on page 49, DOI: 10.5281/zenodo.5176688
Reviving Millicharged Dark Matter for 21-cm Cosmology
Creators: name: Liu, Hongwan
name: Outmezguine, Nadav Joseph
name: Redigolo, Diego
name: Volansky, Tomer
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The existence of millicharged dark matter (mDM) can leave a measurable imprint on 21-cm cosmology through mDM-baryon scattering. However, the minimal scenario is severely constrained by existing cosmological bounds on both the fraction of dark matter that can be millicharged and the mass of mDM particles. We point out that introducing a long-range force between a millicharged subcomponent of dark matter and the dominant cold dark matter (CDM) component leads to efficient cooling of baryons in the early universe, while also significantly extending the range of viable mDM masses. Such a scenario can explain the anomalous absorption signal in the sky-averaged 21-cm spectrum observed by EDGES, and leads to a number of testable predictions for the properties of the dark sector. The mDM mass can then lie between 10 MeV and a few hundreds of GeVs, and its scattering cross section with baryons lies within an unconstrained window of parameter space above direct detection limits and below current bounds from colliders. In this allowed region, mDM can make up as little as $10^{-8}$ of the total dark matter energy density. The CDM mass ranges from 10 MeV to a few GeVs, and has an interaction cross section with the Standard Model that is induced by a loop of mDM particles. This cross section is generically within reach of near-future low-threshold direct detection experiments.
description: 11 pages + appendices, 7 figures
MOESM4 of Quality of maternal and newborn healthcare services in two public hospitals of Bangladesh: identifying gaps and provisions for improvement
Creators: name: Taposh Biswas
name: Hasnat Sujon
name: M. Rahman
name: Perry, Henry
name: Mahbub Chowdhury
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology

description: Additional file 4. Checklist_Caesarean Section Delivery.doc (Cesarean delivery checklist).
Multipole expansion of strongly focussed laser beams
Creators: name: Nieminen, T. A.
name: Rubinsztein-Dunlop, H.
name: Heckenberg, N. R.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Multipole expansion of an incident radiation field - that is, representation of the fields as sums of vector spherical wavefunctions - is essential for theoretical light scattering methods such as the T-matrix method and generalised Lorenz-Mie theory (GLMT). In general, it is theoretically straightforward to find a vector spherical wavefunction representation of an arbitrary radiation field. For example, a simple formula results in the useful case of an incident plane wave. Laser beams present some difficulties. These problems are not a result of any deficiency in the basic process of spherical wavefunction expansion, but are due to the fact that laser beams, in their standard representations, are not radiation fields, but only approximations of radiation fields. This results from the standard laser beam representations being solutions to the paraxial scalar wave equation. We present an efficient method for determining the multipole representation of an arbitrary focussed beam.
description: 13 pages, 7 figures
title: LGBTQ+ Affirmative Clinical Supervision: A Scoping Review
Creators: name: Sherman, Isabel
Publisher: name: OSF Registries
Year: 2025
Subjects: subject: Clinical Psychology
subject: Medicine and Health Sciences
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology

description: This scoping review aims to explore the following objectives:

1. What methods are being used to explore LGBTQ+ affirmative clinical supervision?
2. Which professions are included in the literature on LGBTQ+ affirmative supervision? (e.g. psychological professions, social work, occupational therapy, nursing)
3. What supervision practices are recommended as affirmative in the literature on LGBTQ+ affirmative clinical supervision?
4. What are suggestions for future research on LGBTQ+ affirmative clinical supervision?

Background Information:

The term ‘LGBTQ+ affirmative’ has been used to describe supervision which embraces and validates all sexual orientations and gender identities and challenges forms of oppression (Ashton, 2016). The literature exploring cultural competence in supervision has expanded in the last 30 years. Within this, the literature exploring sexuality as a cultural factor, and specifically LGBTQ+ affirmative supervision in psychological therapies is varied and limited. Existing literature focuses on different areas of professional psychology such as counselling, psychotherapy and family therapy practice (e.g. Hagler, 2020; Chui, 2018; Biaggio et al., 2003; Halpert et al., 2007; Dollar, 2023; Pfohl, 2004; Satterly & Dyson, 2008; O’Brien & Rigazio-DiGilio, 2016).

This review aims to explore and understand what research to date explores LGBTQ+ affirmative clinical supervision. There has not been a scoping review conducted into this area involving a systematic and transparent process. The findings will be used to make recommendations for future research.
Hydaticus (Guignotites) ponticus Sharp 1882
Creators: name: Hájek, Jiří
Publisher: name: Zenodo
Year: 2006
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Curculionidae
Hydaticus
Hydaticus ponticus

description: Hydaticus (Guignotites) ponticus Sharp, 1882
 Material studied. IRAN: 2 33 3 ♀♀, ‘E Iran, Kuh-e Khvajeh, 3-5.6.1977’, ‘Loc. No. 357, Exp. Nat. Mus. Praha’ (NMPC).
description: Published as part of Hájek, Jiří, 2006, The westernmost record of Neptosternus circumductus, and a review of Dytiscidae (Coleoptera) of Baluchistan (Iran, Pakistan), pp. 43-56 in Acta Entomologica Musei Nationalis Pragae 46 on page 50, DOI: 10.5281/zenodo.5176688
Direct Observation of Gate Tunable Dark Trions in Monolayer WSe2
Creators: name: Li, Zhipeng
name: Wang, Tianmeng
name: Lu, Zhengguang
name: Khatoniar, Mandeep
name: Lian, Zhen
name: Meng, Yuze
name: Blei, Mark
name: Taniguchi, Takashi
name: Watanabe, Kenji
name: McGill, Stephen A.
name: Tongay, Sefaattin
name: Menon, Vinod M.
name: Smirnov, Dmitry
name: Shi, Su-Fei
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Spin-forbidden intravalley dark exciton in tungsten-based transition metal dichalcogenides (TMDCs), owing to its unique spin texture and long lifetime, has attracted intense research interest. Here, we show that we can control the dark exciton electrostatically by dressing it with one free electron or free hole, forming the dark trions. The existence of the dark trions is suggested by the unique magneto-photoluminescence spectroscopy pattern of the boron nitride (BN) encapsulated monolayer WSe2 device at low temperature. The unambiguous evidence of the dark trions is further obtained by directly resolving the radiation pattern of the dark trions through back focal plane imaging. The dark trions possess binding energy of ~ 15 meV, and it inherits the long lifetime and large g-factor from the dark exciton. Interestingly, under the out-of-plane magnetic field, dressing the dark exciton with one free electron or hole results in distinctively different valley polarization of the emitted phonon, a result of the different intervalley scattering mechanism for the electron and hole. Finally, the lifetime of the positive dark trion can be further tuned from ~ 50 to ~ 215 ps by controlling the gate voltage. The gate tunable dark trions ushers in new opportunities for excitonic optoelectronics and valleytronics.
Calculation of the T-matrix: general considerations and application of the point-matching method
Creators: name: Nieminen, T. A.
name: Rubinsztein-Dunlop, H.
name: Heckenberg, N. R.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: The T-matrix method is widely used for the calculation of scattering by particles of sizes on the order of the illuminating wavelength. Although the extended boundary condition method (EBCM) is the most commonly used technique for calculating the T-matrix, a variety of methods can be used. We consider some general principles of calculating T-matrices, and apply the point-matching method to calculate the T-matrix for particles devoid of symmetry. This method avoids the time-consuming surface integrals required by the EBCM.
description: 10 pages. 2 figures, 1 table
Super-Earth ingestion can explain the anomalously high metal abundances of M67 Y2235
Creators: name: Church, Ross P.
name: Mustill, Alexander J.
name: Liu, Fan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We investigate the hypothesis that ingestion of a terrestrial or super-Earth planet could cause the anomalously high metal abundances seen in a turn-off star in the open cluster M67, when compared to other turn-off stars in the same cluster. We show that the mass in convective envelope of the star is likely only $3.45\,\times 10^{-3}\,{\rm M}_\odot$, and hence $5.2\,{\rm M}_\oplus$ of rock is required to obtain the observed 0.128 dex metal enhancement. Rocky planets dissolve entirely in the convective envelope if they enter it with sufficiently tangential orbits: we find that the critical condition for dissolution is that the planet's radial speed must be less than 40% of its total velocity at the stellar surface; or, equivalently, the impact parameter must be greater than about 0.9. We model the delivery of rocky planets to the stellar surface both by planet-planet scattering in a realistic multi-planet system, and by Lidov-Kozai cycles driven by a more massive planetary or stellar companion. In both cases almost all planets that are ingested arrive at the star on grazing orbits and hence will dissolve in the surface convection zone. We conclude that super-Earth ingestion is a good explanation for the metal enhancement in M67 Y2235, and that a high-resolution spectroscopic survey of stellar abundances around the turn-off and main sequence of M67 has the potential to constrain the frequency of late-time dynamical instability in planetary systems.
description: 12 pages, 10 figures, submitted to MNRAS
Prodaticus pictus Sharp 1882
Creators: name: Hájek, Jiří
Publisher: name: Zenodo
Year: 2006
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Dytiscidae
Prodaticus
Prodaticus pictus

description: Prodaticus pictus Sharp, 1882
 Material studied. IRAN: 1 3, ‘Iran, Baluchestan, Bampur, 6.-16.6.1997, M. Kafka lgt.’ (NMPC).
description: Published as part of Hájek, Jiří, 2006, The westernmost record of Neptosternus circumductus, and a review of Dytiscidae (Coleoptera) of Baluchistan (Iran, Pakistan), pp. 43-56 in Acta Entomologica Musei Nationalis Pragae 46 on page 50, DOI: 10.5281/zenodo.5176688
MOESM2 of Quality of maternal and newborn healthcare services in two public hospitals of Bangladesh: identifying gaps and provisions for improvement
Creators: name: Taposh Biswas
name: Hasnat Sujon
name: M. Rahman
name: Perry, Henry
name: Mahbub Chowdhury
Publisher: name: figshare
Year: 2019
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Science Policy

description: Additional file 2. Checklist_ANC.docx (ANC Checklist).
Future Patterns of U.S. Grains, Biofuels, and Livestock and Poultry Feeding: Summary
Creators: name: Wisner, Robert
name: Anderson, David P.
name: Plain, Ronald
name: Hofstrand, Don
name: O'Brien, Daniel
name: Wisner, Robert
name: Anderson, David P.
name: Plain, Ronald
name: Hofstrand, Don
name: O'Brien, Daniel
Publisher: name: Unknown
Year: 2012
Subjects: Livestock Production/Industries
Resource /Energy Economics and Policy

description: In this report, we have reviewed recent trends in the U.S. and the global bioenergy, grain, feed, and livestock industries. The report focuses on the impact of development of the U.S. bioenergy industry on grain and feed availability for the livestock sector as well as industry profitability, production, efficiency, demand, and the future of the feed-livestock sector. Bioenergy likely will continue to be a driving force influencing the future direction of the feed and livestock industries. We focused on the feed-livestock industry’s adjustments to the new dynamics of the feed and grain sectors, how the industry has and will be affected, and some key challenges to monitor. Our focal points include: 1) grain and livestock production efficiency; 2) future bioenergy production; 3) rapid foreign economic growth, especially in East Asia, with its implications for dietary change, demand for feedstuffs, and feed availability; and 4) long-term challenges, including global population growth, increased foreign consumption of livestock products, cropland constraints, climate change, and related issues.
description: A project financed by the Institute for Feed Education & Research (IFEEDER) on behalf of the American Feed Industry Association (AFIA) and The Council on Food, Agricultural and Resource Economics (C-FARE)
title: 01_0904
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Sandracottus dejeani
Creators: name: Hájek, Jiří
Publisher: name: Zenodo
Year: 2006
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Dytiscidae
Sandracottus
Sandracottus dejeani

description: Sandracottus dejeani (Aubé, 1838)
 Material studied. IRAN: 1♀, ‘ Iran, Baluchestan, Bampur, 6.-16.6.1997, M. Kafka lgt.’; 1♀, ‘Iran, 11.-12.IV.2000, Sistan va Baluchestan Prov., Pir Sohrab env., 100 m, (25°44′N, 60°50′E)’ (all NMPC).
description: Published as part of Hájek, Jiří, 2006, The westernmost record of Neptosternus circumductus, and a review of Dytiscidae (Coleoptera) of Baluchistan (Iran, Pakistan), pp. 43-56 in Acta Entomologica Musei Nationalis Pragae 46 on page 50, DOI: 10.5281/zenodo.5176688
Discrete--time ratchets, the Fokker--Planck equation and Parrondo's paradox
Creators: name: Amengual, P.
name: Allison, A.
name: Toral, R.
name: Abbott, D.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Parrondo's games manifest the apparent paradox where losing strategies can be combined to win and have generated significant multidisciplinary interest in the literature. Here we review two recent approaches, based on the Fokker-Planck equation, that rigorously establish the connection between Parrondo's games and a physical model known as the flashing Brownian ratchet. This gives rise to a new set of Parrondo's games, of which the original games are a special case. For the first time, we perform a complete analysis of the new games via a discrete-time Markov chain (DTMC) analysis, producing winning rate equations and an exploration of the parameter space where the paradoxical behaviour occurs.
description: 17 pages, 5 figures
MOESM3 of Quality of maternal and newborn healthcare services in two public hospitals of Bangladesh: identifying gaps and provisions for improvement
Creators: name: Taposh Biswas
name: Hasnat Sujon
name: M. Rahman
name: Perry, Henry
name: Mahbub Chowdhury
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Marine Biology
subject: Science Policy
subject: Hematology

description: Additional file 3. Checklist_Blood Transfustion.docx (Blood transfussion checklist).
Herophydrus musicus
Creators: name: Hájek, Jiří
Publisher: name: Zenodo
Year: 2006
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Dytiscidae
Herophydrus
Herophydrus musicus

description: Herophydrus musicus (Klug, 1834)
 Published records. GUÉORGUIEV (1967: 473): ‘ Pakistan: 80 km NW von Quetta, 2100 m, 15.V.1965 (Kasy & Vartian)’. VAZIRANI (1970: 1112): ‘W Pakistan: Quetta, Hanna, 10.xi.1918 (B.S.)’.
 Material studied. IRAN: 1 spec., ‘ E Iran, 2100 m, Taftan, Tamandan, 17-18.4.1973’, ‘ Loc. No. 167, Exp. Nat. Mus. Praha’; 5 spec., ‘ E Iran, Kuh-e Khvajeh, 3-5.6.1977’, ‘ Loc. No. 357, Exp. Nat. Mus. Praha’; 12 spec., ‘ Iran, 9.-10.IV.2000, Sistan va Baluchestan prov., 2 km S Espakeh, (26°48′N, 60°10′E), 690 m’, ‘ Iran 2000 Czech Biological Expedition, J. Hájek & M. Mikát leg. ’; 4 spec., ‘ Iran, 11.-12.IV.2000, Sistan va Baluchestan prov., Pir Sohrab env., 100 m, (25°44′N, 60°50′E)’, ‘ Iran 2000 Czech Biological Expedition, J. Hájek & M. Mikát leg.’ (all NMPC). PAKISTAN: 1 spec., ‘ Pakistan: Baluchistan, 105 km SE Quetta, Sibi, 16.2.1995, leg. Hauck et Čížek’ (HFCB).
description: Published as part of Hájek, Jiří, 2006, The westernmost record of Neptosternus circumductus, and a review of Dytiscidae (Coleoptera) of Baluchistan (Iran, Pakistan), pp. 43-56 in Acta Entomologica Musei Nationalis Pragae 46 on page 50, DOI: 10.5281/zenodo.5176688
Genealogy of Refusal Family Tree
Creators: name: Meyers, Natalie
name: Martinez-Montavon, Anna Michelle
name: Narlock, Mikala
name: Stathers, Kim
Publisher: name: Zenodo
Year: 2021

description: This kinship diagram is a lighthearted visualization inspired by the CJAL Special Issue: Refusing Crisis Narratives . We hope it spurs discussion, maybe laughter, and another way of positioning the ways librarians can say and hear "NO" as a complete sentence. We know this genealogy is, by virtue of its motivation, bound to be: arbitrary, incomplete, inaccurate, and always a work in progress, open to argument, revision, and criticism. We are okay with that. This version is static. To view the most recent version, please visit: bit.ly/refusal-kinship-diagram
Influence of the tensor interaction on heavy-ion fusion cross sections
Creators: name: Godbey, K.
name: Guo, Lu
name: Umar, A. S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: [Background] While the tensor interaction has been shown to significantly affect the nuclear structure of exotic nuclei, its influence on nuclear reactions has only recently been investigated. The primary reason for this neglect is the fact that most studies of nuclear dynamics do not include the tensor force at all in their models. Indeed, only a few Skyrme parametrizations consider the tensor interaction in parameter determination. With modern research facilities extending our ability to probe exotic nuclei, a correct description of nuclear dynamics and heavy-ion fusion is vital to both supporting and leading experimental efforts. [Method] Fusion cross sections are calculated using ion-ion potentials generated by the fully microscopic density-constrained time-dependent Hartree-Fock (DC-TDHF) method with the complete Skyrme tensor interaction. [Results] For light nuclei, the tensor force only slightly changes the sub-barrier fusion cross sections at very low energies. Heavier nuclei, however, begin to exhibit a substantial hindrance effect in the sub-barrier region. This effect is strongest in spin-unsaturated systems, though can manifest in other configurations as well. Static, ground state deformation effects of the tensor force can also affect cross sections by shifting the fusion barrier. [Conclusions] The tensor interaction has a measurable effect on the fusion cross sections of nuclei spanning the nuclear chart. The effect comes from both static effects present in the ground state and dynamic processes arising from the time evolution of the system. This motivates the development of a modern Skyrme parameter set that includes all time-odd and tensor terms and that studies moving forward should include the tensor force to ensure a more robust and complete description of nuclei.
description: 8 pages, 6 figures
Future Patterns of U.S. Grains, Biofuels, and Livestock and Poultry Feeding
Creators: name: Wisner, Robert
name: Anderson, David P.
name: Plain, Ronald
name: Hofstrand, Don
name: O'Brien, Daniel
name: Wisner, Robert
name: Anderson, David P.
name: Plain, Ronald
name: Hofstrand, Don
name: O'Brien, Daniel
Publisher: name: Unknown
Year: 2012
Subjects: subject: Crop Production/Industries
subject: Livestock Production/Industries
subject: Resource /Energy Economics and Policy
subject: Biofuels
subject: ethanol
subject: distillers’ grain
subject: pork
subject: beef
subject: broilers
subject: dairy products
subject: livestock product exports

description: Corn and soybeans are key inputs in animal agriculture’s processing of grain into human food. For most of the 1990s and early 2000s, supplies of both crops were ample and low-priced as the markets reacted to policies that were intended to increase use and prevent a build-up of carryover stocks. Extremely rapid growth in the use of corn for biofuels transformed corn from primarily a food and feed crop to a food, feed and fuel crop. Soybeans also became an energy crop through rapid growth in biodiesel production. This report outlines recent and probable future changes in the biofuels and crops sectors of U.S. and global agriculture. Developments in the biofuels and crops sectors are linked to recent changes in patterns of livestock and poultry production, and potential future directions for the animal agriculture and feed industries. Key requirements for future expansion and competitiveness are identified.
description: A project financed by the Institute for Feed Education & Research (IFEEDER) on behalf of the American Feed Industry Association (AFIA) and The Council on Food, Agricultural and Resource Economics (C-FARE)
Is non-market valuation used in environmental policy making?
Creators: name: Rogers, A.
name: Kragt, Marit Ellen
name: Gibson, F.
name: Pannell, David J.
name: Burton, Michael P.
name: Petersen, L.
name: Rogers, A.
name: Kragt, Marit Ellen
name: Gibson, F.
name: Pannell, David J.
name: Burton, Michael P.
name: Petersen, L.
Publisher: name: Unknown
Year: 2013
Subjects: subject: Environmental Economics and Policy
subject: Teaching/Communication/Extension/Profession
subject: Non-market valuation
subject: environmental policy
subject: decision making

description: A vast literature exists on environmental non-market valuation research. It appears that results from these studies should be useful inputs to decision making about environmental policy or management. Here, we investigate the extent to which this occurs in practice in Australian environmental management bodies. Non-market valuation experts were surveyed about their studies that they believed to have influenced policy. Then, decision makers in environmental bodies were interviewed about the level of influence non-market valuation has had on their decisions. We find that researchers’ perceptions of the influence that non-market valuation has on decision making are overly optimistic. Interviews with decision makers suggest that non-market valuation is little used in decision making. Indeed, the majority of them are unfamiliar with non-market valuation techniques. Nevertheless, once the concept was explained to them, many decision makers believed it could benefit environmental policy. Researchers’ perceptions of the reasons for low usage of non-market valuation are largely inaccurate. We suggest a range of strategies that economists can use to promote the use of non-market valuation in environmental policy and management decisions, including ways to improve communication and engagement with decision makers, and strategies to increase the capacity for decision makers to use non-market valuation results.
description: This paper has been published in a peer-reviewed journal as: Rogers, A., Kragt, M.E., Gibson, F., Pannell, D.J., Burton, M. & Petersen, L. (2015) Non-market valuation: usage and impacts in environmental policy and management in Australia. Australian Journal of Agricultural and Resource Economics, 59(1): 1-15. DOI: 10.1111/1467-8489.12031
Early supernova emission -- logarithmic corrections to the planar phase
Creators: name: Faran, Tamar
name: Sari, Re'em
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: When the shock wave generated in a supernova explosion breaks out of the stellar envelope, the first photons, typically in the X-ray to UV range, escape to the observer. Following this breakout emission, radiation from deeper shells diffuses out of the envelope as the supernova ejecta expands. Previous studies have shown that the radiation throughout the planar phase (i.e., before the expanding envelope has doubled its radius) originates in the same mass coordinate, called the `breakout shell'. We derive a self-similar solution for the radiation inside the envelope, and show that this claim is incorrect, and that the diffusion wave propagates logarithmically into the envelope (in Lagrangian sense) rather than remaining at a fixed mass coordinate. The logarithmic correction implies that the luminosity originates in regions where the density is $\sim 10$ times higher than previously thought, where the photon production rate is increased and helps thermalization. We show that this result has significant implications on the observed temperature. In our model, the radiation emitted from blue supergiant and Wolf-Rayet explosions is still expected to be out of thermal equilibrium during the entire planar phase, but the observed temperature will decrease by two orders of magnitude, contrary to previous estimates. Considering the conditions at the end of the planar phase, we also find how the temperature and luminosity transition into the spherical phase.
description: After first referee report
Low-Voltage Printed, All-Polymer Integrated Circuits Employing a Low-leakage and High-Yield Polymer Dielectric
Creators: name: Stucchi, Elena
name: Dell'Erba, Giorgio
name: Colpani, Paolo
name: Kim, Yun-Hi
name: Caironi, Mario
Publisher: name: arXiv
Year: 2019
Subjects: subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: In the path toward the integration of organic field effect transistors (OFETs) and logic circuits into low-cost and mass produced consumer products, all-organic devices based on printed semiconductors are one of the best options to meet stringent costs requirements. Within this framework, it is still challenging to achieve low voltage operation, as required by the use of thin film batteries and energy harvesters, for which a high capacitance and reliable organic dielectric is required. Here, the development of a parylene-C based dielectric bilayer compatible with top-gate architectures for low-voltage OFETs and logic circuits is presented. The polymer bilayer dielectric allowed the high yield fabrication of all-polymer, bendable, transparent p- and n-type OFETs operating below 2 V, with low leakage, uniform performances and high yield. Such result is a key enabler for the reliable realization of complementary logic circuits that can operate already at a voltage bias of 2 V, such as well-balanced inverters, ring-oscillators and D-Flip-Flops.
Jet formation in BL Lacertae objects with different accretion modes
Creators: name: Cao, Xinwu
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We estimate the masses of massive black holes in BL Lac objects from their host galaxy luminosity. The power of jets and central optical ionizing luminosity for a sample of BL Lac objects are derived from their extended radio emission and the narrow-line emission, respectively. The maximal jet power can be extracted from a standard thin accretion disk/spinning black hole is calculated as a function of dimensionless accretion rate $\dot{m}$ ($\dot{m}=\dot{M}/\dot{M}_{\rm Edd}$). Comparing with the derived jet power, we find that the accretion disks in most BL Lac objects should not be standard accretion disks. For a pure advection dominated accretion flow (ADAF), there is an upper limit on its optical continuum luminosity due to the existence of an upper limit $\dot{m}_{\rm crit}$ on the accretion rate. It is found that a pure ADAF is too faint to produce the optical ionizing luminosity of BL Lac objects derived from their narrow-line luminosity. We propose that an ADAF is present in the inner region of the disk and it becomes a standard thin disk in the outer region in most BL Lac objects, i.e., ADAF+SD(standard disk) scenario. This ADAF+SD scenario can explain both the jet power and optical ionizing continuum emission of these BL Lac objects. The inferred transition radii between the inner ADAF and outer SD are in the range of $40-150 GM_{bh}/c^2$, if the disks are accreting at the rate $\dot{m}=0.01$.
description: accepted by ApJ
Note Illustrative della Carta geologica d'Italia alla scala 1:50.000 F. 171 Cesana Torinese, Servizio Geologico d'Italia - ISPRA
Creators: name: Fioraso, G.
name: Mosca, P.
Publisher: name: INFN Open Access Repository
Year: 2014
Subjects: carta geologica, Cesana Torinese, Piemonte, CARG, stratigrafia, tettonica, sottosuolo, geological map, stratigraphy, tectonics, subsurface

description: Note illustrative redatte per il Foglio geologico n. 171 Cesana Torinese della Carta Geologica d'Italia alla scala 1:50.000. 132 pp.
MOESM1 of Quality of maternal and newborn healthcare services in two public hospitals of Bangladesh: identifying gaps and provisions for improvement
Creators: name: Taposh Biswas
name: Hasnat Sujon
name: M. Rahman
name: Perry, Henry
name: Mahbub Chowdhury
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Science Policy

description: Additional file 1. Checklist _Normal Vaginal Delivery.doc (Nomal delivery checklist).
WISE J072003.20-084651.2B Is A Massive T Dwarf
Creators: name: Dupuy, Trent J.
name: Liu, Michael C.
name: Best, William M. J.
name: Mann, Andrew W.
name: Tucker, Michael A.
name: Zhang, Zhoujian
name: Baraffe, Isabelle
name: Chabrier, Gilles
name: Forveille, Thierry
name: Metchev, Stanimir A.
name: Tremblin, Pascal
name: Do, Aaron
name: Payne, Anna V.
name: Shappee, B. J.
name: Bond, Charlotte Z.
name: Cetre, Sylvain
name: Chun, Mark
name: Delorme, Jacques-Robert
name: Jovanovic, Nemanja
name: Lilley, Scott
name: Mawet, Dimitri
name: Ragland, Sam
name: Wetherell, Ed
name: Wizinowich, Peter
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present individual dynamical masses for the nearby M9.5+T5.5 binary WISE J072003.20$-$084651.2AB, a.k.a. Scholz's star. Combining high-precision CFHT/WIRCam photocenter astrometry and Keck adaptive optics resolved imaging, we measure the first high-quality parallactic distance ($6.80_{-0.06}^{+0.05}$ pc) and orbit ($8.06_{-0.25}^{+0.24}$ yr period) for this system composed of a low-mass star and brown dwarf. We find a moderately eccentric orbit ($e = 0.240_{-0.010}^{+0.009}$), incompatible with previous work based on less data, and dynamical masses of $99\pm6$ $M_{\rm Jup}$ and $66\pm4$ $M_{\rm Jup}$ for the two components. The primary mass is marginally inconsistent (2.1$σ$) with the empirical mass$-$magnitude$-$metallicity relation and models of main-sequence stars. The relatively high mass of the cold ($T_{\rm eff} = 1250\pm40$ K) brown dwarf companion indicates an age older than a few Gyr, in accord with age estimates for the primary star, and is consistent with our recent estimate of $\approx$70 $M_{\rm Jup}$ for the stellar/substellar boundary among the field population. Our improved parallax and proper motion, as well as an orbit-corrected system velocity, improve the accuracy of the system's close encounter with the solar system by an order of magnitude. WISE J0720$-$0846AB passed within $68.7\pm2.0$ kAU of the Sun $80.5\pm0.7$ kyr ago, passing through the outer Oort cloud where comets can have stable orbits.
description: accepted to AJ
Hydroglyphus flammulatus
Creators: name: Hájek, Jiří
Publisher: name: Zenodo
Year: 2006
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Dytiscidae
Hydroglyphus
Hydroglyphus flammulatus

description: Hydroglyphus flammulatus (Sharp, 1882)
 Material studied. IRAN: 3 spec., ‘ SE Iran, 13 km SSE Niksahr (riv.), 8-9.4.1973’, ‘ Loc. No. 152, Exp. Nat. Mus. Praha’; 9 spec., ‘ Iran, 9.-10.IV.2000, Sistan va Baluchestan prov., 2 km S Espakeh, (26°48′N, 60°10′E), 690 m’, ‘ Iran 2000 Czech Biological Expedition, J. Hájek & M. Mikát leg.’ (all NMPC).
description: Published as part of Hájek, Jiří, 2006, The westernmost record of Neptosternus circumductus, and a review of Dytiscidae (Coleoptera) of Baluchistan (Iran, Pakistan), pp. 43-56 in Acta Entomologica Musei Nationalis Pragae 46 on page 51, DOI: 10.5281/zenodo.5176688
Miniaturized fiber dosimeter of medical radiations on a narrow optical fiber
Creators: name: Suarez, Miguel Angel
name: Lim, Tony
name: Robillot, Louise
name: Maillot, Valentin
name: Lihoreau, Thomas
name: Bontemps, Patrick
name: Pazart, Lionel
name: Grosjean, Thierry
Publisher: name: arXiv
Year: 2019
Subjects: subject: Medical Physics (physics.med-ph)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Fiber dosimeters have recently drawn much interest for measuring in vivo and in real time the dose of medical radiations. This paper presents the first miniaturized fiber dosimeter integrated at the end of a narrow 125-micron outer diameter optical fiber. Miniaturization is rendered possible by exploiting the concept of a leaky wave optical antenna for interfacing the scintillators and the fiber, and by taking advantage of the low propagation loss of narrow silica fibers and high detection yield of single-pixel photon counters. Upon irradiation at 6 MV, our fiber probe led to a linear detection response with a signal-to-noise ratio as high as 190 in air. Although implemented with inorganic scintillators and fiber, our fiber probe induces an intensity contrast in the impinging radiation lower than 0.9% over an area of 0.153 mm2. Our nano-optically driven approach opens the route for ultra-compact fiber dosimeters of negligible footprint in the radiotherapeutic processes, even with non-water equivalent fibers and scintillators. A large panel of therapies relying on ionizing radiations (photons or charged particles) may take benefit of this nano-optically-driven technology.
Probing the regoliths of the classical Uranian satellites: Are their surfaces mantled by a layer of tiny H2O ice grains?
Creators: name: Cartwright, Richard J.
name: Emery, Joshua P.
name: Grundy, William M.
name: Cruikshank, Dale P.
name: Beddingfield, Chloe B.
name: Pinilla-Alonso, Noemi
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We investigate whether the surfaces of the classical moons of Uranus are compositionally stratified, with a thin veneer of mostly tiny H2O ice grains (<= 2 micron diameters) mantling a lower layer composed of larger grains of H2O ice, dark material, and CO2 ice (~10 - 50 micron diameters). Near-infrared observations (~1 - 2.5 microns) have determined that the H2O ice-rich surfaces of these moons are overprinted by concentrated deposits of CO2 ice, found almost exclusively on their trailing hemispheres. However, best fit spectral models of longer wavelength datasets (~3 - 5 microns) indicate that the spectral signature of CO2 ice is largely absent, and instead, the exposed surfaces of these moons are composed primarily of tiny H2O ice grains. To investigate possible compositional layering of these moons, we have collected new data using the Infrared Array Camera (IRAC) onboard the Spitzer Space Telescope (~3 - 5 microns). Spectral modeling of these new data is consistent with prior analyses, suggesting that the exposed surfaces of the Uranian moons are primarily composed of tiny H2O ice grains. Furthermore, analysis of these new data reveal that the trailing hemispheres of these moons are brighter than their leading hemispheres over the 3 to 5 micron wavelength range, except for Miranda, which displays no hemispherical asymmetries in its IRAC albedos. Our analyses also revealed that the surface of Ariel displays five distinct, regional-scale albedo zones, possibly consistent with the spatial distribution of CO2 ice on this moon. We discuss possible processes that could be enhancing the observed leading/trailing albedo asymmetries exhibited by these moons, as well as processes that could be driving the apparent compositional stratification of their near surfaces.
description: To be published in Icarus [2019, accepted]. 10 tables and 7 figures
Tailored joint fabrication process derived ultra-low resistance MgB2 superconducting joint
Creators: name: Patel, Dipak
name: Matsumotoa, Akiyoshi
name: Kumakura, Hiroaki
name: Nishijima, Gen
name: Maeda, Minoru
name: Kim, Su-Hun
name: Choi, Seyong
name: Kim, Jung Ho
Publisher: name: arXiv
Year: 2019
Subjects: subject: Applied Physics (physics.app-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report an ultra-low resistance superconducting joint using unreacted multifilament MgB2 wires produced by tailoring the powder compaction pressure within the joint with heat treatment conditions. The joint demonstrated an ultra-low resistance of 5.48 x 10^-15 ohms and critical current (Ic) of 91.3 A at 20 K in self-field. The microstructural and composition studies of the joint revealed cracks and a high amount of MgO, respectively. These two features reduced the Ic of the joint to some extent; nevertheless, the joint resistance was not affected by it. Our tailored joining process will play a pivotal role in superconducting joint development.
MOESM3 of Unraveling candidate genes underlying biomass digestibility in elephant grass (Cenchrus purpureus)
Creators: name: Rocha, João
name: Marçal, Tiago
name: Salvador, Felipe
name: Adriel Silva
name: Carneiro, Pedro
name: Resende, Marcos
name: Jailton Carneiro
name: Azevedo, Ana
name: Pereira, Jorge
name: Juarez Machado
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Marine Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Computational Biology

description: Additional file 3: Table S3. Molecular data for the 90 elephant grass genotypes. “Code” indicates de code of the genotypes (see Additional file 1: Table S1).
Dielectric photonic crystal as medium with negative electric permittivity and magnetic permeability
Creators: name: Efros, A. L.
name: Pokrovsky, A. L.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We show that a two-dimensional photonic crystal (PC) made from a non-magnetic dielectric is a left-handed material in the sense defined by Veselago. Namely, it has negative values of both the electric permittivity $ε$ and the magnetic permeability $μ$ in some frequency range. This follows from a recently proven general theorem. The negative values of $ε$ and $μ$ are found by a numerical simulation. Using these values we demonstrate the Veselago lens, a unique optical device predicted by Veselago. An approximate analytical theory is proposed to calculate the values of $ε$ and $μ$ from the PC band structure. It gives the results that are close to those obtained by the numerical simulation. The theory explains how a non-zero magnetization arises in a non-magnetic PC.
description: 11 pages 4 figures
On Recovering the Nonlinear Bias Function from Counts in Cells Measurements
Creators: name: Szapudi, Istvan
name: Pan, Jun
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a simple and accurate method to constrain galaxy bias based on the distribution of counts in cells. The most unique feature of our technique is that it is applicable to non-linear scales, where both dark matter statistics and the nature of galaxy bias are fairly complex. First, we estimate the underlying continuous distribution function from precise counts-in-cells measurements assuming local Poisson sampling. Then a robust, non-parametric inversion of the bias function is recovered from the comparison of the cumulative distributions in simulated dark matter and galaxy catalogs. Obtaining continuous statistics from the discrete counts is the most delicate novel part of our recipe. It corresponds to a deconvolution of a (Poisson) kernel. For this we present two alternatives: a model independent algorithm based on Richardson-Lucy iteration, and a solution using a parametric skewed lognormal model. We find that the latter is an excellent approximation for the dark matter distribution, but the model independent iterative procedure is more suitable for galaxies. Tests based on high resolution dark matter simulations and corresponding mock galaxy catalogs show that we can reconstruct the non-linear bias function down to highly non-linear scales with high precision in the range of $-1 \le δ\le 5$. As far as the stochasticity of the bias, we have found a remarkably simple and accurate formula based on Poisson noise, which provides an excellent approximation for the scatter around the mean non-linear bias function. In addition we have found that redshift distortions have a negligible effect on our bias reconstruction, therefore our recipe can be safely applied to redshift surveys.
description: 32 pages, 18 figures; submitted to ApJ