cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Improving the Accuracy of Cosmic Magnification Statistics
Creators: name: Menard, Brice
name: Hamana, Takashi
name: Bartelmann, Matthias
name: Yoshida, Naoki
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The systematic magnification of background sources by the weak gravitational-lensing effects of foreground matter, also called cosmic magnification, is becoming an efficient tool both for measuring cosmological parameters and for exploring the distribution of galaxies relative to the dark matter. We extend here the formalism of magnification statistics by estimating the contribution of second-order terms in the Taylor expansion of the magnification and show that the effect of these terms was previously underestimated. We test our analytical predictions against numerical simulations and demonstrate that including second-order terms allows the accuracy of magnification-related statistics to be substantially improved. We also show, however, that both numerical and analytical estimates can provide only lower bounds to real correlation functions, even in the weak lensing regime. We propose to use count-in-cells estimators rather than correlation functions for measuring cosmic magnification since they can more easily be related to correlations measured in numerical simulations.
description: 12 pages, 8 figures, submitted to Astronomy and Astrophysics
Sennius breveapicalis
Creators: name: Romero, Jesús
name: Johnson, Clarence Dan
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Chrysomelidae
Sennius
Sennius breveapicalis

description: Sennius breveapicalis (Pic)
Distribution: Brazil, Colombia, Mexico, Nicaragua (Granada), Panama, Trinidad, and Tobago. (Udayagiri and Wadhi 1989).
 Host plants: Senna bicapsularis (L.) Roxb., S. fruticosa (Miller) Irwin and Barneby, S. undulata (Bentham) H. Irwin and Barneby. (Udayagiri and Wadhi 1989).
description: Published as part of Romero, Jesús & Johnson, Clarence Dan, 2004, Zabrotes maesi, A New Species from Nicaragua with New Distribution Records for other Bruchids (Coleoptera: Bruchidae: Amblycerinae), pp. 379-387 in The Coleopterists Bulletin 58 (3) on page 386, DOI: 10.1649/632, http://zenodo.org/record/10104502
Enriched Regular Theories
Creators: name: Lack, Stephen
name: Tendas, Giacomo
Publisher: name: arXiv
Year: 2019
Subjects: subject: Category Theory (math.CT)
subject: FOS: Mathematics
subject: 18D20, 18C10, 18C35, 18B15

description: Regular and exact categories were first introduced by Michael Barr in 1971; since then, the theory has developed and found many applications in algebra, geometry, and logic. In particular, a small regular category determines a certain theory, in the sense of logic, whose models are the regular functors into Set. Barr further showed that each small and regular category can be embedded in a particular category of presheaves; then in 1990 Makkai gave a simple explicit characterization of the essential image of the embedding, in the case where the original regular category is moreover exact. More recently Prest and Rajani, in the additive context, and Kuber and Rosický, in the ordinary one, described a duality which connects an exact category with its (definable) category of models. Considering a suitable base for enrichment, we define an enriched notion of regularity and exactness, and prove a corresponding version of the theorems of Barr, of Makkai, and of Prest-Rajani/Kuber-Rosický.
description: Reviewed version: changed statement of Theorem 3.3; changed proof of Lemma 8.2; added minor comments. To appear in the Journal of Pure and Applied Algebra: https://doi.org/10.1016/j.jpaa.2019.106268
Dust and Molecular Emission from the S235 Star Forming Region
Creators: name: Lee, Jeong-Eun
name: Young, Chadwick H.
name: Shirley, Yancy L.
name: Mueller, Kaisa E.
name: Evans, Neal J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of a multi-faceted study of the high-mass star-forming region S235. With the CalTech Submillimeter Observatory (CSO), we have observed and/or mapped over fifty molecular transitions and 350 micron dust emission in an attempt to learn more about the chemistry, kinematics, and mass distribution within this rich region. We have found two dust cores that are not resolved in our molecular line observations and suggest that one of these is a less evolved star-forming core.
description: 2 pages to appear in Hot Star Workshop III: The Earliest Phases of Massive Star Birth, ASP Conference Series, 2002, ed. P.A. Crowther
The effect of Audit & Feedback on prescribing of nimodipine in primary care and engagement with data on OpenPrescribing.net - A Cohort Study
Creators: name: Curtis, Helen
name: Walker, Alex
name: Bacon, Seb
name: Rowland, Matthew
name: Croker, Richard
name: Perera, Rafael
name: Goldacre, Ben
name: MacKenna, Brian
Publisher: name: figshare
Year: 2020
Subjects: subject: 111717 Primary Health Care
subject: FOS: Health sciences

description: Protocol for a cohort study of NHS primary care practices, as part of our programme of work on “audit and feedback” using our OpenPrescribing.net tools.
Zabrotes achiote Romero and Johnson
Creators: name: Romero, Jesús
name: Johnson, Clarence Dan
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Chrysomelidae
Zabrotes
Zabrotes achiote

description: Zabrotes achiote Romero and Johnson
Distribution: Bonaire, Colombia, Costa Rica, El Salvador, Mexico, Nicaragua (Granada), Venezuela. (Romero and Johnson 2000).
 Host plants: Acacia angustissima (Miller) Kuntze, Bixa orellana L., Rhynchosia phaseoloides (SW.) DC. (Romero and Johnson 2000).
description: Published as part of Romero, Jesús & Johnson, Clarence Dan, 2004, Zabrotes maesi, A New Species from Nicaragua with New Distribution Records for other Bruchids (Coleoptera: Bruchidae: Amblycerinae), pp. 379-387 in The Coleopterists Bulletin 58 (3) on page 386, DOI: 10.1649/632, http://zenodo.org/record/10104502
Laminar Plasma Dynamos
Creators: name: Wang, Zhehui
name: Pariev, Vladimir I.
name: Barnes, Cris W.
name: Barnes, Daniel C.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A new kind of dynamo utilizing flowing laboratory plasmas has been identified. Conversion of plasma kinetic energy to magnetic energy is verified numerically by kinematic dynamo simulations for magnetic Reynolds numbers above 210. As opposed to intrinsically-turbulent liquid-sodium dynamos, the proposed plasma dynamos correspond to laminar flow topology. Modest plasma parameters, 1-20 eV temperatures, 10^{19}-10^{20} m^{-3} densities in 0.3-1.0 m scale-lengths driven by velocities on the order of the Alfven Critical Ionization Velocity (CIV), self-consistently satisfy the conditions needed for the magnetic field amplication. Growth rates for the plasma dynamos are obtained numerically with different geometry and magnetic Reynolds numbers. Magnetic-field-free coaxial plasma guns can be used to sustain the plasma flow and the dynamo.
description: 5 pages, 4 figures, accepted by Physics of Plasmas, RevTeX file
MOESM1 of Five-year real-world outcomes of anti-vascular endothelial growth factor monotherapy versus combination therapy for polypoidal choroidal vasculopathy in a Chinese population: a retrospective study
Creators: name: Yang, Jingyuan
name: Yuan, Mingzhen
name: Wang, Erqian
name: Xia, Song
name: Chen, Youxin
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Computational Biology

description: Additional file 1: Table S1. P-values of comparisons of baseline clinical characteristics in eyes with polypoidal choroidal vasculopathy performed three different regimens, including anti-VEGF monotherapy, initial combination therapy, and deferred combination therapy.
Gravitationally Lensed Quasar SDSS J1442+4055: Redshifts of Lensing Galaxies, Time Delay, Microlensing Variability, and Intervening Metal System at z ~ 2
Creators: name: Shalyapin, Vyacheslav N.
name: Goicoechea, Luis J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present an $r$--band photometric monitoring of the two images A and B of the gravitationally lensed quasar SDSS J1442+4055 using the Liverpool Telescope (LT). From the LT light curves between 2015 December and 2018 August, we derive at once a time delay of 25.0 $\pm$ 1.5 days (1$σ$ confidence interval; A is leading) and microlensing magnification gradients below 10$^{-4}$ mag day$^{-1}$. The delay interval is not expected to be affected by an appreciable microlensing--induced bias, so it can be used to estimate cosmological parameters. This paper also focuses on new Gran Telescopio Canarias (GTC) and LT spectroscopic observations of the lens system. We determine the redshift of two bright galaxies around the doubly imaged quasar using LT spectroscopy, while GTC data lead to low--noise individual spectra of A, B, and the main lensing galaxy G1. The G1 spectral shape is accurately matched to an early--type galaxy template at $z$ = 0.284, and it has potential for further relevant studies. Additionally, the quasar spectra show absorption by metal--rich gas at $z \sim$ 2. This dusty absorber is responsible for an extinction bump at a rest--frame wavelength of 2209 $\pm$ 2 Å, which has strengths of $\sim$ 0.47 and 0.76 mag $μ$m$^{-1}$ for A and B, respectively. In such intervening system, the dust--to--gas ratio, gas--phase metallicity indicator [Zn/H], and dust depletion level [Fe/Zn] are relatively high.
description: 21 pages, 9 figures, 9 tables. The long Tables 1-4 are available at https://grupos.unican.es/glendama/q1442.htm
Metadata record for the article: Development and pilot of an online, personalized risk assessment tool for a breast cancer precision medicine trial
Creators: name: Keane, Holly
name: Huilgol, Yash S.
name: Shieh, Yiwey
name: Tice, Jeffery
name: Belkora, Jeffrey
name: Sepucha, Karen
name: Shibley, W. Patrick
name: Wang, Tianyi
name: Che, Mandy
name: Goodman, Deborah
name: Ozanne, Elissa
name: Fiscalini, Allison
name: Partners, Athena Breast Health Network Investigators and Advocate
name: Esserman, Laura J.
Publisher: name: figshare
Year: 2021
Subjects: subject: 111706 Epidemiology
subject: FOS: Health sciences
subject: 111203 Cancer Genetics
subject: FOS: Clinical medicine
subject: 111202 Cancer Diagnosis

description: This metadata record provides details of the data supporting the claims of the related article: “Development and pilot of an online, personalized risk assessment tool for a breast cancer precision medicine trial”. The study aimed to develop a new tool that incorporates personalized risk assessments; create a patient-facing web-based software application; and make the risk assessment tool accessible to a low-literacy audience. The pilot study was intended to obtain feedback on the newly developed tool from participants; improve upon the tool before roll-out to a larger study sample; assess the conveyance of personal risk knowledge and motivating preventative actions immediately after consultation with a genetic counselor.
Type of data: personalized risk assessment tool; participant demographic data; survey feedback data; Subject of data: Elevated risk participants in the Women Informed to Screen Depending On Measures of risk (WISDOM) Study Sample size: 20 participantsPopulation characteristics: WISDOM study participants without a breast cancer mutation (namely BRCA1, BCRA2, TP53, PTEN, STK11, CDH1, ATM, PALB2, CHEK2) and classified as elevated risk.Recruitment: A convenience sample of 20 elevated risk WISDOM Study participants who completed their annual breast health questionnaire within a month of tool's completion.Date of data collection: January 2019Geographic location: United States of AmericaTrial registration number: NCT02620852
Data accessThe personalized risk assessment tool is available for non-commercial use only, and can be requested from the corresponding author. Upon request, interested parties will be provided access to the tool in a user testing portal that is separate from the HIPAA-protected, secured patient portal.
The data associated with this study are not publicly available for the following reason: the WISDOM Study portal requires participant authentication and registration. However, the data can be made available upon request to the corresponding author.
Corresponding author for this studyLaura J. Esserman (Laura.Esserman@UCSF.edu)
Study approval University of California, San Francisco Institutional Review Board
title: Innovation in Education in 'Designated Character Schools': a Case Study of the Directors of Discovery 1 and 'Unlimited Paenga Tawhiti'
Creators: name: Doig, Cheryl
Publisher: name: Griffith University
Year: 2005
Subjects: subject: Innovation in education
subject: New Zealand schools
subject: designated character schools
subject: education (New Zealand)

description: This dissertation is a case study into participant perceptions of innovation in education. The participants in this research were four directors from two 'designated character' schools, which were set up to be foundationally different from traditional schools through opportunities to explore radical innovation. That is, both schools were conceptualised as sites for exploring radical rather than incremental change. The central questions asked in this study were - what makes for radical innovation in schools; and how is the use of ICT implicated in innovation in schools? The literature review indicated that while there has been an increase in the information regarding innovation in education there has been little research into how this was being developed in non-traditional settings, or in ways that were radical. The role of ICTs in developing innovation was also reviewed, given that the two 'designated character' schools being studied had strong support for ICTs. The main aims of this study were: to identify the features of radical innovation in schools; to explore the barriers against, and drivers for, innovation in schools; to provide insight into the use of ICTs to influence innovation in schools; to contribute to the literature regarding innovation in schools; and to identify future opportunities to innovate. This study was a qualitative one, with symbolic interactionism as its theoretical underpinning. Data were gathered through the use of concept mapping, interviews and a focus group activity. The findings of the study were that radical innovation in schools occurs when there is a cultural shift in the whole notion of schooling. This is difficult to achieve, even for schools that have been set up to be foundationally different. However, such schools can provide examples of some innovative practices that are 'greenfields'. The use of ICTs, while not required for innovation, helps schools create innovative ideas, especially those ideas based around the needs of individual learners. There is a greater chance that this will lead to innovation being sustained. These findings have implications for policy makers to allow schools that are more innovative to try new ideas and to be supported to do so.
Zabrotes densus
Creators: name: Romero, Jesús
name: Johnson, Clarence Dan
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Chrysomelidae
Zabrotes
Zabrotes densus

description: Zabrotes densus (Horn)
Distribution: Costa Rica, EUA, Guatemala, Honduras, Mexico, Nicaragua (Granada), and Panama. (Romero and Johnson 2000).
Host plants: Unknown.
description: Published as part of Romero, Jesús & Johnson, Clarence Dan, 2004, Zabrotes maesi, A New Species from Nicaragua with New Distribution Records for other Bruchids (Coleoptera: Bruchidae: Amblycerinae), pp. 379-387 in The Coleopterists Bulletin 58 (3) on page 387, DOI: 10.1649/632, http://zenodo.org/record/10104502
Constraints on the Neutron Star Magnetic Field of the two X-ray Transients SAX J1808.4-3658 and Aql X-1
Creators: name: Di Salvo, T.
name: Burderi, L.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The recently discovered coherent X-ray pulsations at a frequency of ~400 Hz in SAX J1808.4-3658, together with a measure of the source luminosity in quiescence, allow us to put an upper limit on the neutron star magnetic field, that is B < 5 10^8 Gauss, using simple considerations on the position of the magnetospheric radius during quiescent periods. Combined with the lower limit inferred from the presence of X-ray pulsations, this constrains the SAX J1808.4-3658 neutron star magnetic field in the quite narrow range (1-5) 10^8 Gauss. Similar considerations applied to the case of Aql X-1 give a neutron star magnetic field lower than ~10^9 Gauss.
description: 6 pages, submitted to A&A
Zabrotes interstitialis
Creators: name: Romero, Jesús
name: Johnson, Clarence Dan
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Chrysomelidae
Zabrotes
Zabrotes interstitialis

description: Zabrotes interstitialis (Chevrolat)
Distribution: Costa Rica, El Salvador, Mexico, Nicaragua (), Panama, and Venezuela. (Romero and Johnson 2000).
 Host plants: Cassia grandis L. f., C. moschata Kunth, Mimosa quadrivalvis L., Senna polyphylla (Jacq.) H. Irwin and Barneby. (Udayagiri and Wadhi 1989).
description: Published as part of Romero, Jesús & Johnson, Clarence Dan, 2004, Zabrotes maesi, A New Species from Nicaragua with New Distribution Records for other Bruchids (Coleoptera: Bruchidae: Amblycerinae), pp. 379-387 in The Coleopterists Bulletin 58 (3) on page 387, DOI: 10.1649/632, http://zenodo.org/record/10104502
Consequences of glacial cycles for magmatism and carbon transport at mid-ocean ridges
Creators: name: Cerpa, Nestor G.
name: Jones, David W. Rees
name: Katz, Richard F.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: Magmatism and volcanism transfer carbon from the solid Earth into the climate system. This transfer may be modulated by the glacial/interglacial cycling of water between oceans and continental ice sheets, which alters the surface loading of the solid Earth. The consequent volcanic-carbon fluctuations have been proposed as a pacing mechanism for Pleistocene glacial cycles. This mechanism is dependant on the amplitude and lag of the mid-ocean ridge response to sea-level changes. Here we develop and analyse a new model for that response, eliminating some questionable assumptions made in previous work. Our model calculates the carbon flux, accounting for the thermodynamic effect of mantle carbon: reduction of the solidus temperature and a deeper onset of melting. We analyse models forced by idealised, periodic sea level and conclude that fluctuations in melting rate are the prime control on magma and carbon flux. We also discuss a model forced by a reconstruction of eustatic sea level over the past 800 kyr. It indicates that peak-to-trough variations of magma and carbon flux are up to about 20% and 10% of the mean flux, respectively. Peaks in mid-ocean ridge emissions lag peaks in sea-level forcing by less than about 20 kyr and the lag could well be shorter. The amplitude and lag are sensitive to the rate of melt segregation. The lag is much shorter than the time it takes for melt to travel vertically across the melting region.
description: 28 pages including supplementary material. 9 figures plus 6 supplementary figures. Accepted for publication in Earth and Planetary Science Letters
The effect of Audit & Feedback on prescribing of nimodipine in primary care and engagement with data on OpenPrescribing.net - A Cohort Study
Creators: name: Curtis, Helen
name: Walker, Alex
name: Bacon, Seb
name: Roland, Matthew
name: Croker, Richard
name: Perera, Rafael
name: Goldacre, Ben
name: MacKenna, Brian
Publisher: name: figshare
Year: 2019
Subjects: subject: 111717 Primary Health Care
subject: FOS: Health sciences

description: Protocol for a cohort study of NHS primary care practices, as part of our programme of work on “audit and feedback” using our OpenPrescribing.net tools.
Towards a Theory of Emergence for the Physical Sciences
Creators: name: De Haro, Sebastian
Publisher: name: arXiv
Year: 2019
Subjects: subject: History and Philosophy of Physics (physics.hist-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: I begin to develop a framework for emergence in the physical sciences. Namely, I propose to explicate ontological emergence in terms of the notion of 'novel reference', and of an account of interpretation as a map from theory to world. I then construe ontological emergence as the "failure of the interpretation to mesh" with an appropriate linkage map between theories. Ontological emergence can obtain between theories that have the same extension but different intensions, and between theories that have both different extensions and intensions. I illustrate the framework in three examples: the emergence of spontaneous magnetisation in a ferromagnet, the emergence of masslessness, and the emergence of space, in specific models of physics. The account explains why ontological emergence is independent of reduction: namely, because emergence is primarily concerned with adequate interpretation, while the sense of reduction that is relevant here is concerned with inter-theoretic relations between uninterpreted theories.
description: 54 pages. Published version, references updated
title: Congolese Men and Women of Good Hope: The Legacies of Refugee Camps for Work Market Readiness in Hyper-Diverse Cities.
Creators: name: Ngendakurio, John Bosco
Publisher: name: Griffith University
Year: 2017
Subjects: subject: Congolese men
subject: Congolese women
subject: Good Hope
subject: Refugee camps
subject: Hyper-diverse cities
subject: Refugee camps and violence

description: The key question this thesis asks is the following: “What are the key determinants of market readiness for Congolese refugees in today’s hyper-diverse cities with particular focus on their Australian settlement?” This question is sparked by the lack of a wide ranging existing literature to develop a full understanding of Congolese refugees’ post-migration conditions and factors that influence their settlement and integration in their new home country including language, education, employment and social cohesion. But even less attention has been paid to these refugees’ pre-resettlement conditions and how they impact on Congolese refugees’ work market readiness in Australia, particularly in hyper-diverse cities. This study aims to highlight critical barriers to accessing meaningful employment within the Congolese communities in Australia and raise awareness about special needs of Congolese-Australians who have experienced long stays in the refugee camps. The research draws on original qualitative research that involves face-to-face interviews with ten female and ten male Congolese refugees resettled from various refugee camps in Africa. The thesis interrogates ongoing legacies of refugee camps for work readiness, community trust and social cohesion. These refugees’ stories, history and experiences are discussed in this research and they will become helpful to both migrant and non-migrant Australian communities to understand Congolese refugees’ performances in different sectors. Outlining the underlying factors of work market readiness in Australia will also enable the Congolese community and their settlement services providers to understand refugees’ need and the level of their readiness for the work market in Australia, to re-shape their business model to improve services delivery, promote social cohesion and help African refugees to access appropriate services. These factors, as discussed in greater detail in chapter four, include verbatim accounts of their health and wellbeing, their histories of torture and trauma, their prospects for education and training, the resettlement process, social network, social cohesion, self- confidence and self-image plus government policies and the cultural significance of work.
Predicting GPS-based PWV Measurements Using Exponential Smoothing
Creators: name: Manandhar, Shilpa
name: Dev, Soumyabrata
name: Lee, Yee Hui
name: Winkler, Stefan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: FOS: Physical sciences

description: Global Positioning System (GPS) derived precipitable water vapor (PWV) is extensively being used in atmospheric remote sensing for applications like rainfall prediction. Many applications require PWV values with good resolution and without any missing values. In this paper, we implement an exponential smoothing method to accurately predict the missing PWV values. The method shows good performance in terms of capturing the seasonal variability of PWV values. We report a root mean square error of 0.1~mm for a lead time of 15 minutes, using past data of 30 hours measured at 5-minute intervals.
Confrontation of Intracluster and Interstellar Gas in Cluster-Centered Elliptical Galaxies: M87 in Virgo and NGC 4874 in Coma
Creators: name: Brighenti, Fabrizio
name: Mathews, William G.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: X-ray observations of M87 in the Virgo cluster and NGC 4874 in Coma reveal that the gas temperature beyond about 50 kpc from these cD galaxies is comparable to the virial temperature of the cluster, 3 or 9 keV respectively, but within the optical galaxy the temperature drops to the galactic virial temperature, about 1 keV. We show that these steep thermal (and density) gradients follow naturally from the usual cooling inflow assumptions without recourse to thermal conductivity. To avoid unobserved central mass concentrations, most of the gas must radiatively cool (``dropout'') before it flows to the galactic core, i.e. the gas must be multiphase. Recent XMM spectra of M87 indicate single phase flow at every radius with no apparent radiative cooling to low temperatures. However, the X-ray spectral evidence for multiphase cooling beginning at lower temperatures near 1 keV (within about 10 kpc) may be less apparent and may have escaped detection. Finally, we show that the standard decomposition method used by X-ray observers to determine the mass flow dM/dt(r) may fail rather badly due to small deviations from perfectly steady state flow. When applied to our slightly non-steady computed flows, this decomposition (incorrectly) gives the usual result, dM/dt proportional to r, and overestimates the mass dropout dM/dt(r) at large radii.
description: 12 pages (emulateapj5) with 10 figures; accepted by The Astrophysical Journal
Muscini PROPOSED IN THE
Creators: name: Nihei, Silvio Shigueo
name: Carvalho, Claudio José Barros De
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae

description: GENERA OF MUSCINI PROPOSED IN THE NEW CLASSIFICATION   Biopyrellia Townsend, 1932
 Curranosia Paterson, 1957
 spekei group gemma group (genus-ranked taxon, to be described) Dasyphora Robineau-Desvoidy, 1830
 Subgenus Dasyphora s.s.
 Subgenus Eudasyphora Townsend, 1911 syn. nov., stat. nov.
 Subgenus Rypellia Malloch, 1931 syn. nov., stat. nov.
 Deltotus Séguy, 1935
 Hennigmyia Peris, 1967
 Mesembrina Meigen, 1826
 Mitroplatia Enderlein, 1935
 Morellia Robineau-Desvoidy, 1830
 Subgenus Morellia s.s.
 Subgenus Parapyrellia Townsend, 1915 syn. nov., stat. nov.
 Subgenus Trichomorellia Stein, 1918 syn. nov., stat. nov.
 Subgenus Xenomorellia Malloch, 1923 syn. nov., stat. nov.
 nigricosta group (genus-ranked taxon, to be described)
 Musca Linnaeus, 1758
 Myiophaea Enderlein, 1935
 Neomyia Walker, 1859
 Neorypellia Pont, 1972
 Polietes Rondani, 1866
 Polietina Schnabl & Dziedzicki, 1911 Pyrellia Robineau-Desvoidy, 1830
 Pyrellina Malloch, 1923
 Sarcopromusca Townsend, 1927
 Ziminellia Nihei & de Carvalho, nom. nov.
description: Published as part of Nihei, Silvio Shigueo & Carvalho, Claudio José Barros De, 2007, Phylogeny and classification of Muscini (Diptera, Muscidae), pp. 493-532 in Zoological Journal of the Linnean Society 149 (4) on page 530, DOI: 10.1111/j.1096-3642.2007.00252.x, http://zenodo.org/record/5429076
title: What is the role of a safety professional? The identity, practice and future of the profession
Creators: name: Provan, David John
Publisher: name: Griffith University
Year: 2018
Subjects: subject: Safety
subject: Safety practice
subject: Organisational challenges
subject: Safety specific processes
subject: Future design

description: The role of a safety professional is central to the way organisations understand and manage safety since it is these expert roles that provide their organisations with their safety narrative. Yet despite the importance of this role, we understand very little about safety professional identity and safety professional practice – who are they and what do they do? This thesis asks the fundamental question for the existence of the safety profession – What is the role of a safety professional? The primary research design involved a 6-month longitudinal ethnographic case-study of professional identity and safety professional practice within a large Australian energy company. 12 mid-level and senior-level safety professionals were interviewed monthly regarding their work, and this data was supplemented by continuous work observations by an embedded researcher throughout the study period. Through the research design, the results of this study provide a deeper and broader perspective of safety professional practice, than the existing descriptive research into the role of safety professionals. Safety Professional identify is rife with tensions and contradictions that reveal the complex social and organisational challenges associated with the role. Safety Professionals are both friend and enemy of line management and the frontline workforce. Safety professionals through the practice of their role: align themselves and their work with management objectives, develop safety specific processes and practices, satisfy organisational needs at the expense of worker safety risk reduction, and lack a working connection between safety science knowledge and their safety professional work, decisions and advice. Contemporary safety theory describes new ways for achieving safety in organisations that are largely at odds with current organisational safety approaches and existing safety professional practice. This thesis provides the first practical description of the role of a safety professional thorough a resilience engineering, safety-II, and safety differently theoretical lens. The conclusion from this research, is that organisations expect safety professionals to perform their existing role, and that the contemporary safety science literature demands them to work vastly differently. This thesis makes a significant scientific contribution to the understanding of safety professional identity, safety professional practice, and the future design of the role of a safety professional which will narrow the gap between safety professional work and the safety of work.
Screened fifth forces in parity-breaking correlation functions
Creators: name: Kodwani, Darsh
name: Desmond, Harry
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Cross-correlating two different types of galaxy gives rise to parity breaking in the correlation function that derives from differences in the galaxies' properties and environments. This is typically associated with a difference in galaxy bias, describing the relation between galaxy number density and dark matter density, although observational effects such as magnification bias also play a role. In this paper we show that the presence of a screened fifth force adds additional degrees of freedom to the correlation function, describing the effective coupling of the force to the two galaxy populations. These are also properties of the galaxies' environments, but with different dependence in general to galaxy bias. We derive the parity-breaking correlation function analytically as a function of fifth-force strength and the two populations' fifth-force charges, and explore the result numerically using Hu-Sawicki $f(R)$ as a toy model of chameleon screening. We find that screening gives rise to an octopole, which, in the absence of magnification bias, is not present in any gravity theory without screening and thus is a qualitatively distinct signature. The modification to the dipole and octopole can be $\mathcal{O}(10\%)$ and $\mathcal{O}(100\%)$ respectively at redshift $z \gtrsim 0.5$ due to screening, but decreases towards lower redshift. The change in the background power spectrum in $f(R)$ theories induces a change in the dipole of roughly the same size, but dominant to the effect of screening at low $z$. While current data is insufficient to measure the parity-breaking dipole or octopole to the precision required to test these models, future surveys such as DESI, Euclid and SKA have the potential to probe screened fifth forces through the dipole.
description: Matches published version
An alternative formulation of vibrational heat-bath configuration interaction
Creators: name: Bhatty, Abuzar U.
name: Brorsen, Kurt R.
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Computational Biology

description: Recently, a selected vibrational configuration interaction method was introduced where the selection of the vibrational basis was performed using the heat-bath algorithm (VHCI). This method was adapted from the heat-bath configuration interaction (HCI) method used to solve the electronic Schrödinger equation. The selection algorithm in electronic HCI exploits the fact that most nonzero Hamiltonian matrix elements correspond to a double electronic excitation from one determinant to another and have values equal to the two-electron molecular orbital integrals such that they can be computed once, sorted, stored, and easily accessed later using a dictionary data structure. However, the Hamiltonian matrix elements in VHCI are more complicated than their electronic HCI counterparts, which lead to the possibility of different VHCI implementations. We explore one such implementation. The most significant differences compared to the original VHCI implementation is that we (i) explicitly compute all one- and two-quanta excitations, (ii) include all occupation-number contributions to the Hamiltonian matrix elements, and (iii) add individual Hartree product basis functions to the variational space rather than multiple basis functions as determined by operator products. We apply the new VHCI algorithm to ethylene oxide and naphthalene and achieve good accuracy relative to previous results at a modest computational cost.
Additional file 1 of Inclusion of purified dietary fiber during gestation improved the reproductive performance of sows
Creators: name: Zhuo, Yong
name: Feng, Bo
name: Xuan, Yuedong
name: Che, Lianqiang
name: Fang, Zhengfeng
name: Lin, Yan
name: Xu, Shengyu
name: Li, Jian
name: Feng, Bing
name: Wu, De
Publisher: name: figshare
Year: 2020
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Mental Health

description: Additional file 1: Table S1. Bacterial phyla correlated by Pearson’s correlation to gestation stage and DF level. Table S2. Bacterial genera correlated by Pearson’s correlation to gestation stage and DF level.
Gelae parile, new combination
Creators: name: Miller, Kelly B.
name: Wheeler, Quentin D.
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Leiodidae
Gelae
Gelae parile

description: Gelae parile (Fall), new combination
(Figs. 7–9, 26)
description: Published as part of Miller, Kelly B. & Wheeler, Quentin D., 2004, Two New Genera of Agathidiini from the Nearctic and Neotropical Regions (Coleoptera: Leiodidae), pp. 466-487 in The Coleopterists Bulletin 58 (4) on page 476, DOI: 10.1649/633, http://zenodo.org/record/10104530
title: Design and Development of Asymmetric Organocatalysts
Creators: name: James, Samantha N
Publisher: name: Griffith University
Year: 2014
Subjects: subject: Hydrogen bonding organocatalysts
subject: Amide coupling
subject: Borane reduction
subject: N-acylsulfonamides
subject: TAD DOL class of compounds
subject: Asymmetric organocatalysts

description: This thesis describes the design and synthesis of a new class of hydrogen bonding organocatalysts. After various synthetic strategies were investigated, a convenient two-step process, involving an amide coupling followed by borane reduction of the resulting N-acylsulfonamide, resulted in the formation of the targeted racemic 1,5-bis-sulfonamides. This synthesis also provided access to a second series of potential organocatalysts, the N-acylsulfonamides. The catalytic ability of both libraries of racemic compounds was tested in Friedel-Crafts type reactions of N-methylindole with ethyl glyoxylate and p-nitrostyrene. Following on from this work, a small number of N-acylsulfonamides were synthesised in enantiomerically enriched form, after resolution of the starting material trans-1,3-cyclohexanedicarboxylic acid using strychnine. Testing of the enantiopure N-acylsulfonamides showed that they were able to promote the Friedel-Crafts type reaction between N-methylindole and P-nitrostyrene, in good yields but poor enantioselectivities. A second group of catalysts were synthesised based on the TAD DOL class of compounds. Attempts to form his-sulfonamide TADDOL derivatives were unsuccessful, with only mono-sulfonamides being isolated, possibly due to a stabilising intramolecular hydrogen bond present in the mono-sulfonamides. A p-tolyl N-acylsulfonamide TADDOL derivative was also synthesised. The mono sulfonamide and N-acylsulfonamide TADDOL derivatives did not effectively catalyse the Friedel-Crafts type reaction between N-methylindole and P­ nitrostyrene. The TADDOL derivatives catalysed the model reaction between N­ methylindole and ethyl glyoxylate with low to moderate efficiency.
The Luminosity & Mass Function of the Trapezium Cluster: From B stars to the Deuterium Burning Limit
Creators: name: Muench, A.
name: Lada, E.
name: Lada, C.
name: Alves, J.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use the results of a new, multi-epoch, multi-wavelength, near-infrared census of the Trapezium Cluster in Orion to construct and to analyze the structure of its infrared (K band) luminosity function. Specifically, we employ an improved set of model luminosity functions to derive this cluster's underlying Initial Mass Function (IMF) across the entire range of mass from OB stars to sub-stellar objects down to near the deuterium burning limit. We derive an IMF for the Trapezium Cluster that rises with decreasing mass, having a Salpeter-like IMF slope until near ~0.6 M_sun where the IMF flattens and forms a broad peak extending to the hydrogen burning limit, below which the IMF declines into the sub-stellar regime. Independent of the details, we find that sub-stellar objects account for no more than ~22% of the total number of likely cluster members. Further, the sub-stellar Trapezium IMF breaks from a steady power-law decline and forms a significant secondary peak at the lowest masses (10-20 times the mass of Jupiter). This secondary peak may contain as many as \~30% of the sub-stellar objects in the cluster. Below this sub-stellar IMF peak, our KLF modeling requires a subsequent sharp decline toward the planetary mass regime. Lastly, we investigate the robustness of pre-main sequence luminosity evolution as predicted by current evolutionary models, and we discuss possible origins for the IMF of brown dwarfs.
description: 74 pages, 30 figures, AASTeX5.0. To be published in the 01 July 2002 ApJ. For color version of figure 1 and online data table see http://www.astro.ufl.edu/~muench/PUB/publications.html
Open quantum systems are harder to track than open classical systems
Creators: name: Warszawski, Prahlad
name: Wiseman, Howard M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: For a Markovian open quantum system it is possible, by continuously monitoring the environment, to know the stochastically evolving pure state of the system without altering the master equation. In general, even for a system with a finite Hilbert space dimension $D$, the pure state trajectory will explore an infinite number of points in Hilbert space, meaning that the dimension $K$ of the classical memory required for the tracking is infinite. However, Karasik and Wiseman [Phys. Rev. Lett., 106(2):020406, 2011] showed that tracking of a qubit ($D=2$) is always possible with a bit ($K=2$), and gave a heuristic argument implying that a finite $K$ should be sufficient for any $D$, although beyond $D=2$ it would be necessary to have $K>D$. Our paper is concerned with rigorously investigating the relationship between $D$ and $K_{\rm min}$, the smallest feasible $K$. We confirm the long-standing conjecture of Karasik and Wiseman that, for generic systems with $D>2$, $K_{\rm min}>D$, by a computational proof (via Hilbert Nullstellensatz certificates of infeasibility). That is, beyond $D=2$, $D$-dimensional open quantum systems are provably harder to track than $D$-dimensional open classical systems. Moreover, we develop, and better justify, a new heuristic to guide our expectation of $K_{\rm min}$ as a function of $D$, taking into account the number $L$ of Lindblad operators as well as symmetries in the problem. The use of invariant subspace and Wigner symmetries makes it tractable to conduct a numerical search, using the method of polynomial homotopy continuation, to find finite physically realizable ensembles (as they are known) in $D=3$. The results of this search support our heuristic. We thus have confidence in the most interesting feature of our heuristic: in the absence of symmetries, $K_{\rm min} \sim D^2$, implying a quadratic gap between the classical and quantum tracking problems.
description: 35 pages, 3 figures, Accepted in Quantum Journal, minor changes
Nimble evolution for pretzel Khovanov polynomials
Creators: name: Anokhina, Aleksandra
name: Morozov, Alexei
name: Popolitov, Aleksandr
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: Geometric Topology (math.GT)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We conjecture explicit evolution formulas for Khovanov polynomials for pretzel knots in some regions in the windings space. Our description is exhaustive for genera 1 and 2. As previously observed, evolution at T != -1 is not fully smooth: it switches abruptly at the boundaries between different regions. We reveal that this happens also at the boundary between thin and thick knots, moreover, the thick-knot domain is further stratified. For thin knots evolution is governed by the standard T-deformation lambda of the eigenvalues of the R-matrix. Emerging in the thick knots regions are additional Lyapunov exponents, which are multiples of the naive ones. Such frequency doubling is typical for non-linear dynamics, and our observation can signal about a hidden non-linearity of superpolynomial evolution. Since evolution with eigenvalues lambda^2, ..., lambda^g is "faster" than the one with lambda in the thin-knot region, we name it "nimble.
description: 16 pages
Black Hole Binary Dynamics
Creators: name: Aarseth, Sverre J
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss a new N-body simulation method for studying black hole binary dynamics. This method avoids previous numerical problems due to large mass ratios and trapped orbits with short periods. A treatment of relativistic effects is included when the associated time-scale becomes small. Preliminary results with up to N = 240 000 particles are obtained showing systematic eccentricity growth until the relativistic regime is reached, with subsequent coalescence in some cases.
description: 5 pages, 2 figures, To appear in Fred Hoyle's Universe, eds. G. Burbidge, J.V. Narlikar and N.C. Wickramasinghe
The forensic comparison of trace amounts of soil on a pyjama top with hypersulphidic subaqueous soil from a river as evidence in a homicide cold case
Creators: name: Fitzpatrick, Robert W.
name: Raven, Mark D.
Publisher: name: Geological Society of London
Year: 2019
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: S1: SEM images and spectra of samples
Sphaerobulbus ornatus SMETANA 2006
Creators: name: Smetana, A.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Sphaerobulbus
Sphaerobulbus ornatus

description: Sphaerobulbus ornatus SMETANA 2006
 Sphaerobulbus ornatus SMETANA 2006a: 45.
N e w r e c o r d s: C h i n a: Shaanxi: Qinling Shan Mts., Taibai Shan, Houzhenzi, 1500-2000m, 33°52'N 107°44'E, IV.-V.2000, leg. A. Plutenko, 1, 2 (ASC, MSC).
C o m m e n t s: Additional specimens from the type locality.
description: Published as part of Smetana, A., 2008, Contributions to the knowledge of the " Staphylinus-complex " (Insecta: Coleoptera, Staphylinidae, Staphylinini) of China. Part 18. Various genera, pp. 943-949 in Linzer biologische Beiträge 40 (1) on page 948, DOI: 10.5281/zenodo.5429958
Regular scalar field around reflecting stars and black holes, and reflecting star polarization
Creators: name: Sadjadi, H. Mohseni
name: Khodaei, M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The existence of a regular non-trivial scalar field in the background of an asymptotically flat static reflecting star is discussed. The scalar field is assumed to be conformally coupled to the outside matter. The induced scalar charge is determined and the required conditions to have regular field are obtained. The results are compared with the case of a black hole. Conditions to have regular non-trivial scalar field out of the black hole horizon are investigated. We show that in the presence of a scalar source, in contrast to the black holes, the reflecting star becomes polarized.
description: 14 pages, references updated
Additional file 6 of Comparative analyses of the Hymenoscyphus fraxineus and Hymenoscyphus albidus genomes reveals potentially adaptive differences in secondary metabolite and transposable element repertoires
Creators: name: Elfstrand, Malin
name: Chen, Jun
name: Cleary, Michelle
name: Halecker, Sandra
name: Ihrmark, Katarina
name: Karlsson, Magnus
name: Davydenko, Kateryna
name: Stenlid, Jan
name: Stadler, Marc
name: Durling, Mikael Brandström
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 6: