cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Small Aperture Telescopes for the Simons Observatory
Creators: name: Ali, Aamir M.
name: Adachi, Shunsuke
name: Arnold, Kam
name: Ashton, Peter
name: Bazarko, Andrew
name: Chinone, Yuji
name: Coppi, Gabriele
name: Corbett, Lance
name: Crowley, Kevin D
name: Crowley, Kevin T
name: Devlin, Mark
name: Dicker, Simon
name: Duff, Shannon
name: Ellis, Chris
name: Galitzki, Nicholas
name: Goeckner-Wald, Neil
name: Harrington, Kathleen
name: Healy, Erin
name: Hill, Charles A
name: Ho, Shuay-Pwu Patty
name: Hubmayr, Johannes
name: Keating, Brian
name: Kiuchi, Kenji
name: Kusaka, Akito
name: Lee, Adrian T
name: Ludlam, Michael
name: Mangu, Aashrita
name: Matsuda, Frederick
name: McCarrick, Heather
name: Nati, Federico
name: Niemack, Michael D.
name: Nishino, Haruki
name: Orlowski-Scherer, John
name: Rao, Mayuri Sathyanarayana
name: Raum, Christopher
name: Sakurai, Yuki
name: Salatino, Maria
name: Sasse, Trevor
name: Seibert, Joseph
name: Sierra, Carlos
name: Silva-Feaver, Maximiliano
name: Spisak, Jacob
name: Simon, Sara M
name: Staggs, Suzanne
name: Tajima, Osamu
name: Teply, Grant
name: Tsan, Tran
name: Wollack, Edward
name: Westbrook, Bejamin
name: Xu, Zhilei
name: Zannoni, Mario
name: Zhu, Ningfeng
Publisher: name: arXiv
Year: 2020
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The Simons Observatory (SO) is an upcoming cosmic microwave background (CMB) experiment located on Cerro Toco, Chile, that will map the microwave sky in temperature and polarization in six frequency bands spanning 27 to 285 GHz. SO will consist of one 6-meter Large Aperture Telescope (LAT) fielding $\sim$30,000 detectors and an array of three 0.42-meter Small Aperture Telescopes (SATs) fielding an additional 30,000 detectors. This synergy will allow for the extremely sensitive characterization of the CMB over angular scales ranging from an arcmin to tens of degrees, enabling a wide range of scientific output. Here we focus on the SATs targeting degree angular scales with successive dichroic instruments observing at Mid-Frequency (MF: 93/145 GHz), Ultra-High-Frequency (UHF: 225/285 GHz), and Low-Frequency (LF: 27/39 GHz). The three SATs will be able to map $\sim$10% of the sky to a noise level of 2 $μ$K-arcmin when combining 93 and 145 GHz. The multiple frequency bands will allow the CMB to be separated from galactic foregrounds (primarily synchrotron and dust), with the primary science goal of characterizing the primordial tensor-to-scalar ratio, $r$, at a target level of $σ\left(r\right) \approx 0.003$.
Luidia barbadensis Perrier 1881
Creators: name: Jangoux, Michel
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Paxillosida
Luidiidae
Luidia
Luidia barbadensis

description: convexiuscula Perrier, 1881, Luidia
Luidia convexiuscula Perrier, 1881: 29; 1884: 268, pl. 10, fig. 6.
Luidia barbadensis ‒ Clark & Downey 1992: 11.
CURRENT STATUS. — Luidia barbadensis Perrier, 1881.
TYPE MATERIAL. — Caribbean Sea • 1 syntype; station 45; BLAKE expedition; 1877-1878; 25°33’N, 84°21’W; depth 185 m; MNHN- IE-2014-334.
description: Published as part of Jangoux, Michel, 2022, The type specimens of extant asteroids (Echinodermata) in the Muséum national d'Histoire naturelle of Paris, pp. 259-334 in Zoosystema 44 (11) on page 277, DOI: 10.5252/zoosystema2022v44a11, http://zenodo.org/record/6616817
Invitation to quiver representation and Catalan combinatorics
Creators: name: Rognerud, Baptiste
Publisher: name: Mathematisches Forschungsinstitut Oberwolfach
Year: 2021

description: Representation theory is an area of mathematics that deals with abstract algebraic structures and has numerous applications across disciplines. In this snapshot, we will talk about the representation theory of a class of objects called quivers and relate them to the fantastic combinatorics of the Catalan numbers.
description: Snapshots of modern mathematics from Oberwolfach;2021-04
'Utopian' artisan : David Harding and the town art of Glenrothes
Creators: name: Demetrius, Andrew Jonathan
Publisher: name: The University of St Andrews
Year: 2024
Subjects: Public art
New towns
Environmental art
Scottish art
Community art
Sculpture
Concrete
Social art practice
Planning
Locational identity

description: This thesis provides a critical history of the public art of Glenrothes and the role of the town artist, with a focus on David Harding’s tenure, 1968-78, which has been overlooked in academic study and by the art world. It contributes to knowledge of New Town art (town art) and associated practice, particularly in Scotland, with which to connect historical activity to the present, and provides timely consideration of the continued relevance of town art through its enduring yet insecure presence in Glenrothes and in the lived experience of residents. This is pursued through a thematically contextualised cataloguing of town art, a framework that charts Harding’s conceptual development in relation to contemporaneous activity and the shift from “public sculpture” towards site-specific environmental and community art, positioning town art as a significant antecedent to the subsequent evolution of social art practices. The research considers approaches to urbanism and public art whereby town art was made in relation to shortcomings in planning which were addressed by artists who reconceptualised the site, form, and arrangement of art and public space, particularly within housing and infrastructure, its materiality derived from the building site, brick and concrete. The development of Harding’s practice is analysed through the socio-political thinking of the era and the turn toward conceptual and collaborative practices linking community art, participation, and play. This is explored through critical examination of Harding’s collaborative methodology, developed via interactive environmental sculpture, performance and participatory community art projects, and a dialogic art practice with which to engage the audience, leading to the formation of shared identity. Investigation shows how the emplacement of the artist in a corporate hierarchy and in the community, and the embedding of site-specific art in the environment, facilitated the distinction of place. Harding’s town art practice represents a paradigm shift in linking site-specific, collaborative, and community art to provide means of locational identity, and presents a utopian contrast to later concepts of participation and socially engaged art, Creative Placemaking, and non-places.
Kanakaster convexus Mah 2017
Creators: name: Jangoux, Michel
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Valvatida
Goniasteridae
Kanakaster
Kanakaster convexus

description: convexus Mah, 2017, Kanakaster
Kanakaster convexus Mah, 2017: 27, fig. 8A-C.
CURRENT STATUS. — Kanakaster convexus Mah, 2017.
TYPE MATERIAL. — New Caledonia • holotype; Antigona Bank; SMIB 4 expedition; 23°20’S, 168°4’E; MNHN-IE-2013-6835.
description: Published as part of Jangoux, Michel, 2022, The type specimens of extant asteroids (Echinodermata) in the Muséum national d'Histoire naturelle of Paris, pp. 259-334 in Zoosystema 44 (11) on page 277, DOI: 10.5252/zoosystema2022v44a11, http://zenodo.org/record/6616817
title: A Google Earth-Based Framework for Visualization of the Chesapeake Bay Operational Forecast System
Creators: name: Lawson, Gary
Publisher: name: Old Dominion University Libraries
Year: 2011

description: For the persons who live near and travel the waters of the Chesapeake Bay, the data provided by the Chesapeake Bay Operational Forecast System (CBOFS) is invaluable. The information provided includes measurements and forecasts of surface wind velocity, water current velocity, salinity levels, water level, and temperature. Currently, this information is freely available on the CBQ_FS website hosted by the National Oceanographic and Atmospheric Administration (NOAA). It is offered as Nowcast, measured data, and Forecast data and is visualized using 2D images which describe a subset of the data in an easy to read chart. However, if the data were made available in a 3D environment, it would not only provide viewers with the general information currently available on the CBOFS website, but it would also provide users with a means to explore the data in the rich context of the surrounding environment. Viewers would have the ability to look at the data from any viewpoint, zoom in to see individual markers, and receive actual measurements in moments. This would considerably increase the use of the data measured by CBOFS as it would allow those who rely on this information to still receive the same data in a similar format, but it would also provide those interested in the Chesapeake Bay a means to learn more about the bay and how it functions under the water's surface.

This thesis proposes a framework for developing interactive visualizations of CBOFS data in Google Earth by exporting the CBOFS data into KML files which may be loaded into Google Earth from a standalone application or web plugin. Generation of these KML files involves retrieving the data files provided from OPeNDAP servers which host the CBOFS data files in NetCDF format. The pertinent raw data is then extracted from these data files using the Unidata Java library. The raw data is further processed based on the . grids utilized by CBOFS, and different visualization methods are employed to visualize different CBOFS variables. The final visualization results are then converted to KML files for efficient rendering in Google Earth. Finally, the KML files are organized into a carefully designed hierarchical structure and archived on a server for easy retrieval by the website designed to display the CBOFS data using Google Earth. The proposed framework provides several advantages over the current CBOFS visualization at the NOAA website: 1) it produces visualizations that are not available in the current CBOFS visualization; 2) it produces visualizations with resolution and accuracy much higher than that of the current CBOFS visualization; and 3) it provides users interactive capabilities that essentially do not exist in the current CBOFS visualization. Researchers, educators, students, and the general public will benefit greatly from the proposed framework.
The Moyal Bracket in the Coherent States framework
Creators: name: Daoud, M.
name: Kinani, E. H. El
Publisher: name: arXiv
Year: 2003
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The star product and Moyal bracket are introduced using the coherent states corresponding to quantum systems with non-linear spectra. Two kinds of coherent state are considered. The first kind is the set of Gazeau-Klauder coherent states and the second kind are constructed following the Perelomov-Klauder approach. The particular case of the harmonic oscillator is also discussed.
description: 13 pages
Stellaster convexus Jangoux 1981
Creators: name: Jangoux, Michel
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Valvatida
Goniasteridae
Stellaster
Stellaster convexus

description: convexus Jangoux, 1981, Stellaster
Stellaster convexus Jangoux, 1981: 472, pl. 5, figs 4-6. — Clark 1993: 285.
CURRENT STATUS. — Stellaster convexus Jangoux, 1981.
TYPE MATERIAL. — Philippines • holotype; station 53; MUSORSTOM expedition; 1976; 13°49’N, 120°04’E; depth 40-50 m; MNHN- IE-2014-41 • 6 paratypes; same as holotype; MNHN-IE-2014-35.
description: Published as part of Jangoux, Michel, 2022, The type specimens of extant asteroids (Echinodermata) in the Muséum national d'Histoire naturelle of Paris, pp. 259-334 in Zoosystema 44 (11) on page 278, DOI: 10.5252/zoosystema2022v44a11, http://zenodo.org/record/6616817
Lean Production Applied in Civil Construction: Application of the Last Planner System Methodology
Creators: name: De Castro Lopes, Samuel Jônatas
name: Dias, Samuel
name: De Almeida Silva, Humberto Denys
name: De Moura Sousa, Linardy
name: Nascimento, Laécio Guedes Do
name: Menezes, Mariana Sousa
name: Evanielle Barbosa Ferreira
name: Da Silva Filho, Paulo Henrique Nogueira
Publisher: name: figshare
Year: 2021
Subjects: subject: 99999 Engineering not elsewhere classified
subject: FOS: Other engineering and technologies
subject: 91099 Manufacturing Engineering not elsewhere classified
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: 90599 Civil Engineering not elsewhere classified
subject: FOS: Civil engineering

description: Abstrato:
O objetivo desta pesquisa é elaborar uma proposta de aplicação do Sistema Last Planner. (LPS) no planejamento de uma obra civil de médio porte, com produção repetidaescala, apresentando projeto, planilhas e modelo de acompanhamento semanal. Esta metodologia foi aplicada como um modelo de planejamento da construção de casas populares de 45m² seguindo o mesmo padrão. Um LPS de três níveis sequência foi usada, ou seja, planejamento inicial, planejamento antecipado e planejamento de compromisso. O primeiro nível era uma forma de planejamento mestre, onde as informações iniciais da obra são coletadas. Este nível é usado para facilitar a identificação dos objetivos principais do trabalho e para definir os ritmos do principal processo de produção. No segundo nível, é feito um ajuste ao plano inicial e seu detalhamento é melhorado, serve também como forma de proteção à produção, restrição que impede a liberação deatividades que não atendam aos critérios de qualidade, controlando a liberação das atividades do meio para o curto prazo somente após analisar e remover todos os impedimentos possíveis em cada estágio. O terceiro nível acontece de acordo com planos de trabalho semanais, nos quais a execução da obra é orientada diretamente, através da empenho de pacotes de serviços às equipas, respeitando o seu empenho em realizá-los. A proposta elaborada melhorou a gestão do processo, reduziu o desperdício de materiais e serviu como um padrão para a construção de outros edificios.
Probing the close environment of young stellar objects with interferometry
Creators: name: Malbet, Fabien
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The study of Young Stellar Objects (YSOs) is one of the most exciting topics that can be undertaken by long baseline optical interferometry. The magnitudes of these objects are at the edge of capabilities of current optical interferometers, limiting the studies to a few dozen, but are well within the capability of coming large aperture interferometers like the VLT Interferometer, the Keck Interferometer, the Large Binocular Telescope or 'OHANA. The milli-arcsecond spatial resolution reached by interferometry probes the very close environment of young stars, down to a tenth of an astronomical unit. In this paper, I review the different aspects of star formation that can be tackled by interferometry: circumstellar disks, multiplicity, jets. I present recent observations performed with operational infrared interferometers, IOTA, PTI and ISI, and I show why in the next future one will extend these studies with large aperture interferometers.
description: Review to be published in JENAM'2002 proceedings "The Very Large Telescope Interferometer Challenges for the future"
Vanishing of the conformal anomaly for strings in a gravitational wave
Creators: name: Duval, C.
name: Horvath, Z.
name: Horvathy, P. A.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Using the non-symmetric-connection approach proposed by Osborn, we demonstrate that, for a bosonic string in a specially chosen plane-fronted gravitational wave and an axion background, the conformal anomaly vanishes at the two-loop level. Under some conditions, the anomaly vanishes at all orders.
description: Previously not available in hep-th. Published as Physics Letters B 313, 10 (1993). Plain TeX 6 pages. No figures
title: Carte de vœux ICCARRE envoyée à Pierre Bergé
Creators: name: Leibowitch, Jacques
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Source: http://www.calames.abes.fr/pub/ms/Calames-20193111132541127
The survival of star clusters with black hole subsystems
Creators: name: Wang, Long
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Recent observations have detected top-heavy IMFs in dense star forming regions like the Arches cluster. Whether such IMFs also exist in old dense stellar systems like globular clusters is difficult to constrain, because massive stars already became black holes (BHs) and neutron stars (NSs). However, studies of stellar dynamics find that BHs/NSs influence the long-term evolution of star clusters. Following Breen & Heggie (2013) and by carrying out two-component $N$-body simulations, we demonstrate how this dynamical impact connects with the shape of IMFs. By investigating the energy balance between the BH subsystem and the global, we find that to properly describe the evolution of clusters, a corrected two-body relaxation time, $T_{rh,p} = T_{rh}/ψ$, is necessary. Because $ψ$ depends on the total mass fraction of BHs, $M_2 / M$, and the mass ratio, $m_2 / m_1$, the cluster dissolution time is sensitive to the property of BHs or IMFs. Especially, the escape rate of BHs via ejections from few-body encounters is linked to mass segregation. In strong tidal fields, top-heavy IMFs easily lead to the fast dissolution of star clusters and the formation of BH-dominant dark clusters, which suggests that the observed massive GCs with dense cores are unlikely to have extreme top-heavy IMFs. With the future observations of gravitational waves providing unique information of BHs/NSs, it is possible to combine the multi-message observations to have better constrains on the IMFs of old star clusters.
description: 12 pages, 13 figures, accepted for MNRAS
Thoracaster cylindratus Sladen 1883
Creators: name: Jangoux, Michel
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Paxillosida
Porcellanasteridae
Thoracaster
Thoracaster cylindratus

description: cordifer Perrier, 1885, Pseudaster
Pseudaster cordifer Perrier, 1885: 68; 1894: 235, pl. 16, fig. 3a-e.
Thoracaster cylindratus ‒ Clark & Downey 1992: 105.
CURRENT STATUS. — Thoracaster cylindratus Sladen, 1883.
TYPE MATERIAL. — Atlantic Ocean • holotype. Station 134; Talisman expedition; 1883; 42°19’N, 23°36’W; depth 4060 m; MNHN- IE-2014-209.
description: Published as part of Jangoux, Michel, 2022, The type specimens of extant asteroids (Echinodermata) in the Muséum national d'Histoire naturelle of Paris, pp. 259-334 in Zoosystema 44 (11) on page 278, DOI: 10.5252/zoosystema2022v44a11, http://zenodo.org/record/6616817
Electron-molecule scattering calculations in a 3D finite element R-matrix approach
Creators: name: Tonzani, Stefano
name: Greene, Chris H.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We have implemented a three-dimensional finite element approach, based on tricubic polynomials in spherical coordinates, which solves the Schrodinger equation for scattering of a low energy electron from a molecule, approximating the electron exchange as a local potential. The potential is treated as a sum of three terms: electrostatic, exchange and polarization. The electrostatic term can be extracted directly from ab initio codes (GAUSSIAN 98 in the work described here), while the exchange term is approximated using different local density functionals. A local polarization potential approximately describes the long range attraction to the molecular target induced by the scattering electron.
description: 17 pages, 8 figures, TeX (RevTex4), double spaced
Maternal and Neonatal Factors Associated with Indomethacin-induced Ductal Closure in Extremely-Low-Birth-Weight Infants
Creators: name: Pham, Jennifer
name: Kellyn Moran
name: Saurabh Patel
name: Nishant Srinivasan
Publisher: name: University of Illinois at Chicago
Year: 2021
Subjects: Uncategorized

description: Background: Ductal response to indomethacin in extremely-low-birth-weight (ELBW) infants is not well studied. Objective: The purpose of this study was to identify predictors of ductal closure in ELBW infants treated with indomethacin.
Methods: A single-center, retrospective cohort of ELBW infants treated with indomethacin for patent ductus arteriosus (PDA) were included. Predictors of PDA closure were identified using multivariable adjusted logistic regression.
Results: One hundred and five infants with a PDA were treated with indomethacin. Primary PDA closure with one course of indomethacin occurred in 61.9%. The rate of primary PDA closure was lower in infants with gestational age (GA) < 28 weeks compared to infants ≥ 28 weeks (58.1% vs 91.7%, p =0.03). Multivariable logistic regression model identified PDA size (OR 0.29, 95% CI 0.11-0.74, p =0.009) and exposure to antenatal indomethacin (OR 0.28, 95% CI 0.08–0.99, p =0.048) and magnesium (OR 0.31, 95% CI 0.12–0.82, p =0.019) as significant predictors for failure of ductal closure in infants treated with indomethacin. Infants with failed PDA closure were more likely to have moderate/severe bronchopulmonary dysplasia, severe intraventricular hemorrhage, and longer duration of hospitalization (p <0.05).
Conclusions: Large PDA and antenatal indomethacin and magnesium were predictors for failure of ductal closure with indomethacin. The negative association between antenatal indomethacin and magnesium on ductal closure with postnatal indomethacin warrants further investigation regarding routine use in mothers at risk for preterm delivery. Future studies focusing on developing predictive models to identify ideal candidates for indomethacin within the ELBW population could reduce the burden of the disease and improve overall outcomes.
Qualitative Theory for Lensed QSOs
Creators: name: Saha, Prasenjit
name: Williams, Liliya L. R.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show that some characteristics of multiply-imaged QSO systems are very model-independent and can be deduced accurately by simply scrutinizing the relative positions of images and galaxy-lens center. These include the time-ordering of the images, the orientation of the lens potential, and the rough morphology of any ring. Other features can differ considerably between specific models; H_0 is an example. Surprisingly, properties inherited from a circularly symmetric lens system are model-dependent, whereas features that arise from the breaking of circular symmetry are model-independent. We first develop these results from some abstract geometrical ideas, then illustrate them for some well-known systems (the quads Q2237+030, H1413+117, HST14113+5211, PG1115+080, MG0414+0534, B1608+656, B1422+231, and RXJ0911+0551, and the ten-image system B1933+507), and finally remark on two systems (B1359+154 and PMN J0134-0931) where the lens properties are more complex. We also introduce a Java applet which produces simple lens systems, and helps further illustrate the concepts.
description: 26 pages, incl. 15 figs; accepted to AJ; java applet available at http://ankh-morpork.maths.qmw.ac.uk/~saha/astron/lens/
Communication Behaviour: A Struggle Against Illiteracy in Eastern Indonesia
Creators: name: Ramallah, Zaqia
name: Dadang Rahmat Hidayat
name: Anter Venus
name: Agus Rahmat
Publisher: name: figshare
Year: 2020
Subjects: subject: 200199 Communication and Media Studies not elsewhere classified
subject: FOS: Media and communications
subject: 130201 Creative Arts, Media and Communication Curriculum and Pedagogy
subject: FOS: Educational sciences
subject: 200101 Communication Studies
subject: 200105 Organisational, Interpersonal and Intercultural Communication
subject: 200103 International and Development Communication

description: The illiteracy phenomenon is a trial that requires effort in order to defeat it. The children of Kadi Wone village, East Wewewa District, Southwest Sumba, East Nusa Tenggara, Indonesia attempt to defeat this phenomenon by engaging in their education and studying. However as this is deemed insufficient, children may choose to join a reading centre (Taman Bacaan Masyarakat) called Dyatame. The social circle of Dyatame reading centre provides an opportunity to enhance interest in reading and learning. The purpose of this study was to reveal the meaning of reading in terms of it being a resource to fight illiteracy and further, to study the communication behaviour created through interactions in the social circle of Dyatame reading centre. The results of this study reveal that children can be empowered with learning spirit in the fight against illiteracy. This motivation can also build their capacity through an understanding of the meaning of reading, as a source of insight and an information tool. This study also envisages that this learning process can shape communication behaviour, verbally and non-verbally in both positive and negative ways.
title: Early sole editorship of natural philosophical and scientific periodicals in the Holy Roman Empire and Britain, 1770s-1830s
Creators: name: Gielas, Anna Maria
Publisher: name: University of St Andrews
Year: 2019

description: Today, editors of science journals exercise a significant power over academic careers and the production of scientific knowledge—their editorial influence is rooted in the period 1770-1830 and the advent of sole editorship (in contrast to group-based editorship at scientific societies and academies). This dissertation focuses on six sole editors from Britain and the Holy Roman Empire to investigate why individuals founded natural philosophical periodicals, how their editorship played out on a day-to-day basis, and what it meant for their professional and personal lives. The contrasting experiences of Johann Ernst Immanuel Walch, Lorenz Crell, Lorenz Oken and William Nicholson, Alexander Tilloch, William Thomas Brande demonstrate the importance of personal motivations and local contexts. In the German lands, monarchs and their administrative elites indirectly incentivised academics to assume natural philosophical editorship. On the British side, there were no such incentives and editorship challenged established natural philosophical infrastructures. This thesis discusses both national contexts and their influence on the editorship of the six editors. This thesis also reveals a crucial transnational parallel for the first generation of sole editors between 1770 and 1810: editorship of natural philosophical journals could be used by those on the philosophical periphery to design a philosophical identity for themselves, at a time before the development of formalised mechanisms for becoming a man-of-science. The experiences of editors after 1810 show that, even once sole editorship had become a familiar concept among men-of-science, it was not necessarily easier to be a successful editor than it had been for its pioneers: sole editorship could, in fact, be outright detrimental to scientific self-fashioning. This thesis also investigates what contributed to the ‘success’ of sole editorship. It turns out that neither a supportive publisher, nor a steady stream of contributions, was as important as one might expect. While acknowledging that economic concerns did matter, this thesis demonstrates that sole editorship was a highly adaptable socio-cultural instrument. And that the editorial activities of sole editors were not as far distant from learned society publishing as has often been assumed.
Edgeworth expansions for network moments
Creators: name: Zhang, Yuan
name: Xia, Dong
Publisher: name: arXiv
Year: 2020
Subjects: subject: Statistics Theory (math.ST)
subject: Social and Information Networks (cs.SI)
subject: Methodology (stat.ME)
subject: Machine Learning (stat.ML)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: 62E17, 91D30, 60F05

description: Network method of moments arXiv:1202.5101 is an important tool for nonparametric network inference. However, there has been little investigation on accurate descriptions of the sampling distributions of network moment statistics. In this paper, we present the first higher-order accurate approximation to the sampling CDF of a studentized network moment by Edgeworth expansion. In sharp contrast to classical literature on noiseless U-statistics, we show that the Edgeworth expansion of a network moment statistic as a noisy U-statistic can achieve higher-order accuracy without non-lattice or smoothness assumptions but just requiring weak regularity conditions. Behind this result is our surprising discovery that the two typically-hated factors in network analysis, namely, sparsity and edge-wise observational errors, jointly play a blessing role, contributing a crucial self-smoothing effect in the network moment statistic and making it analytically tractable. Our assumptions match the minimum requirements in related literature. For sparse networks, our theory shows a simple normal approximation achieves a gradually depreciating Berry-Esseen bound as the network becomes sparser. This result also refines the best previous theoretical result. For practitioners, our empirical Edgeworth expansion is highly accurate, fast and easy to implement. We demonstrate the clear advantage of our method by comprehensive simulation studies. We showcase three applications of our results in network inference. We prove, to our knowledge, the first theoretical guarantee of higher-order accuracy for some network bootstrap schemes, and moreover, the first theoretical guidance for selecting the sub-sample size for network sub-sampling. We also derive one-sample test and Cornish-Fisher confidence interval for a given moment with higher-order accurate controls of confidence level and type I error, respectively.
description: 32 pages, 4 figures
title: 02_1563
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/
Constraints on neutrino oscillation parameters from the SNO salt phase data
Creators: name: Bandyopadhyay, Abhijit
name: Choubey, Sandhya
name: Goswami, Srubabati
name: Petcov, S. T.
name: Roy, D. P.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The physics implications of the just published salt phase data from the SNO experiment are examined. The effect of these data on the allowed ranges of the solar neutrino oscillation parameters, $Δ_m^2_{21}$ and $\sin^2θ_{12}$, are studied in the cases of two- and three- neutrino mixing. In the latter case we derive an upper limit on the angle $θ_{13}$. Constraints on the solar $ν_e$ transitions into a mixture of active and sterile neutrinos are also presented. Finally, we give predictions for the day-night asymmetry in the SNO experiment, for the event rate in the BOREXINO and LowNu experiments, and discuss briefly the constraints on the solar neutrino oscillation parameters which can be obtained with prospective KamLAND data.
description: Version to appear in PLB
Social [un]Distancing : The exploration of social connection in quarantine
Creators: name: Chan, Maverick
Publisher: name: The University of British Columbia
Year: 2024

description: The COVID-19 pandemic forced the world to retreat behind closed doors and live life at a distance. Quarantine, lockdowns, and social distancing defined a new reality marked by the sudden and drastic reconfiguration of our social interactions and relationships. The unprecedented drop in human contact across the globe was critical for saving lives and preserving an already over-burdened healthcare system. However, these life-saving measures also amplified an already existing epidemic of social isolation and loneliness, particularly amongst older adults. As human populations continue to grow and changes in the world’s climate continue to disrupt natural ecosystems, how might we re-imagine quarantine to address the social health of seniors in an inevitable future pandemic? Social [un]distancing explores the fictional stories of four older adults living in this world. From proposals designed at the scale of the human body to interventions at the urban infrastructural scale, this project proposes different ways for seniors to stay connected during a pandemic.
Microscopic determination of the nuclear incompressibility within the non-relativistic framework
Creators: name: Colo`, G.
name: Van Giai, N.
name: Meyer, J.
name: Bennaceur, K.
name: Bonche, P.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The nuclear incompressibility $K_\infty$ is deduced from measurements of the Isoscalar Giant Monopole Resonance (ISGMR) in medium-heavy nuclei, and the resulting value turns out to be model dependent. Since the considered nuclei have neutron excess, it has been suggested that the model dependence is due to the different behaviour of the symmetry energy in different models. To clarify this issue, we make a systematic and careful analysis based on new Skyrme forces which span a wide range of values for $K_\infty$, for the value of the symmetry energy at saturation and for its density dependence. By calculating, in a fully self-consistent fashion, the ISGMR centroid energy in $^{208}$Pb we reach, for the first time within the non-relativistic framework, three important conclusions: (i) the monopole energy, and consequently the deduced value of $K_\infty$, depend on a well defined parameter related to the shape of the symmetry energy curve and called $K_{sym}$; (ii) Skyrme forces of the type of SLy4 predict $K_\infty$ around 230 MeV, in agreement with the Gogny force (previous estimates using Skyrme interactions having been plagued by lack of full self-consistency); (iii) it is possible to build forces which predict $K_\infty$ around 250 MeV, although part of this increase is due to our poor knowledge of the density dependence and effective mass.
description: 19 pages, 8 figures. Submitted to PRC
Culcita coriacea Muller & Troschel 1842
Creators: name: Jangoux, Michel
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Valvatida
Oreasteridae
Culcita
Culcita coriacea

description: coriacea Müller & Troschel, 1842, Culcita
(Fig. 10)
Culcita coriacea Müller & Troschel, 1842: 38, pl. 12, figs 1-5. — Clark 1993: 298.
CURRENT STATUS. — Culcita coriacea Müller & Troschel, 1842.
TYPE MATERIAL. — Red Sea • 1 syntype; MNHN-IE-2014-461.
description: Published as part of Jangoux, Michel, 2022, The type specimens of extant asteroids (Echinodermata) in the Muséum national d'Histoire naturelle of Paris, pp. 259-334 in Zoosystema 44 (11) on page 278, DOI: 10.5252/zoosystema2022v44a11, http://zenodo.org/record/6616817
Transition-metal phthalocyanine monolayers as new Chern insulators
Creators: name: Li, Jie
name: Gu, Lei
name: Wu, Ruqian
Publisher: name: arXiv
Year: 2020
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: To explore new materials for the realization of the quantum anomalous Hall effect (QAHE), we studied electronic, magnetic and topological properties of transition-metal phthalocyanine (TMPc) monolayers in a square lattice. Many of them have large topologically nontrivial band gaps and integer Chern numbers. In particular, the Fermi level of MoPc lies right in the band gap (Eg=8.1 meV) and has large magnetic anisotropy energy (MAE=2.0 meV per Mo atom) and a Curie temperature of 16 K, showing its usefulness for applications. The presence of topologically protected edge state in a MoPc nanoribbon further confirms it as a new two-dimensional topological insulator. This much widens the search of QAHE materials for the design of quantum devices.
description: 14 pages, 4 figures
Cloud Properties and Correlations with Star Formation in Numerical Simulations of the Three-Phase ISM
Creators: name: Mao, S. Alwin
name: Ostriker, Eve C.
name: Kim, Chang-Goo
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We apply gravity-based and density-based methods to identify clouds in numerical simulations of the star-forming, three-phase interstellar medium (ISM), and compare their properties and their global correlation with the star formation rate over time. The gravity-based method identifies bound objects, which have masses M ~ 10^3 - 10^4 M_solar at densities n_H ~ 100 cm^-3, and traditional virial parameters alpha_v ~ 0.5 - 5. For clouds defined by a density threshold n_H,min , the average virial parameter decreases, and the fraction of material that is genuinely bound increases, at higher n_H,min. Surprisingly, these clouds can be unbound even when alpha_v < 2, and high mass clouds (10^4 - 10^6 M_solar) are generally unbound. This suggests that the traditional alpha_v is at best an approximate measure of boundedness in the ISM. All clouds have internal turbulent motions increasing with size as sigma ~ 1 km/s(R/ pc)^1/2, similar to observed relations. Bound structures comprise a small fraction of the total simulation mass, with star formation efficiency per free-fall time epsilon_ff ~ 0.4. For n_H,min = 10 - 100 cm^-3, epsilon_ff ~ 0.03 - 0.3, increasing with density. Temporal correlation analysis between SFR(t) and aggregate mass M(n_H,min;t) at varying n_H,min shows that time delays to star formation are t_delay ~ t_ff(n_H,min). Correlation between SFR(t) and M(nH,min;t) systematically tightens at higher n_H,min. Considering moderate-density gas, selecting against high virial parameter clouds improves correlation with SFR, consistent with previous work. Even at high n_H,min, the temporal dispersion in (SFR-epsilon_ff M/t_ff )/ is ~ 50%, due to the large-amplitude variations and inherent stochasticity of the system.
description: 31 pages, 17 figures, submitted to ApJ
Observing the Sunyaev-Zel'dovich Effect Closer to Home
Creators: name: Taylor, James E.
name: Moodley, Kavilan
name: Diego, J. M.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Hot gas trapped in a dark matter halo will produce a decrement in the surface brightness of the microwave background, the Sunyaev-Zel'dovich (SZ) effect. While massive clusters produce the strongest central SZ decrements, we point out that a local galaxy halo, specifically the halo of M31, may be one of the brightest integrated SZ sources in the sky. For various realistic gas distributions consistent with current X-ray limits, we show that the integrated SZ decrement from M31 will be comparable to decrements already detected in more distant sources, provided its halo contains an appreciable quantity of hot gas. A measurement of this decrement would provide direct information on the mass, spatial distribution and thermodynamic state of hot gas in a low-mass halo, and could place important constraints on current models of galaxy formation. Detecting such an extended (~ 10 degree), low-amplitude signal will be challenging, but should be possible with all-sky SZ maps from satellite missions such as the Wilkinson Microwave Anisotropy Probe or the Planck Surveyor.
description: 5 pages, 3 figures; submitted to MNRAS
Age-related differences in motives for contacting out-of-hours primary care: a cross-sectional questionnaire study in Denmark
Creators: name: Moth, Grete
name: Christensen, Morten B.
name: Christensen, Helle Collatz
name: Carlsen, Anders H.
name: Riddervold, Ingunn S.
name: Huibers, Linda
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Demands for out-of-hours primary care (OOH-PC) services are increasing. Many citizens call because of non-urgent health problems. Nevertheless, the patients’ motives for requesting medical help outside office hours remains an understudied area. This study aimed to examine motives for calling OOH-PC services in various age groups. Cross-sectional paper based questionnaire study conducted during two weeks in 2015. The OOH-PC services in two Danish regions. Randomly selected patients calling the two healthcare services and accepting to participate in the study received a questionnaire on patient characteristics, health problems, and 26 pre-defined motives based on the Andersen Behavioural Model. Multivariate regression analyses were conducted for various age groups to calculate the probability of each motive to be a significant factor for the decision to call. A total of 1,871 patients were included in the study; half were parents of children aged 0-12 years. Young adults (18 to 39 years) differed significantly from other age groups as they more often stated perceived barriers and benefits such as “Own GP no time available soon enough” and “Need for quick help because of work”. Young adults more often perceive barriers and benefits, which may suggest af difference in expectations regarding the purpose of out-of-hours services and accessibility. Further research is needed to address this issue and further explore the potential gap between the citizens’ expectations to the OOH-PC services and the prevailing health policies.Key pointsThe out-of-hours primary healthcare services are increasingly contacted for non-urgent problems, but little is known about the citizens’ motives for calling.Age is associated with differences in the perceived importance of various motives for calling out-of-hours care.Young adults are more often than other age groups motivated to call due to logistical issues, such as their job. The out-of-hours primary healthcare services are increasingly contacted for non-urgent problems, but little is known about the citizens’ motives for calling. Age is associated with differences in the perceived importance of various motives for calling out-of-hours care. Young adults are more often than other age groups motivated to call due to logistical issues, such as their job.
Cheiraster (Christopheraster) mirabilis Perrier 1881
Creators: name: Jangoux, Michel
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Asteroidea
Notomyotida
Benthopectinidae
Cheiraster
Cheiraster mirabilis

description: coronatus Perrier, 1883, Archaster
Archaster coronatus Perrier, 1884: 262.
Cheiraster (Christopheraster) mirabilis ‒ Clark & Downey 1992: 132.
CURRENT STATUS. — Cheiraster (Christopheraster) mirabilis Perrier, 1881.
TYPE MATERIAL. — Caribbean Sea • 1 syntype; BLAKE expedition; 1877-1878; MNHN-IE-2014-358.
REMARK
Of the two specimens dredged by the BLAKE, one came from off Moro Ligth (Porto Rico), the other from 23°03’N, 83°10’W. The second specimen should be housed in the MCZ.
description: Published as part of Jangoux, Michel, 2022, The type specimens of extant asteroids (Echinodermata) in the Muséum national d'Histoire naturelle of Paris, pp. 259-334 in Zoosystema 44 (11) on page 278, DOI: 10.5252/zoosystema2022v44a11, http://zenodo.org/record/6616817
Methods used to meta-analyse results from interrupted time series studies: A methodological systematic review protocol - Completed PRISMA-P checklist
Creators: name: Korevaar, Elizabeth
name: Karahalios, Emily
name: Forbes, Andrew
name: Turner, Simon
name: McDonald, Steve
name: Taljaard, Monica
name: Grimshaw, Jeremy
name: Cheng, Allen
name: Bero, Lisa
name: McKenzie, Joanne
Publisher: name: Monash University
Year: 2020
Subjects: Uncategorized

description: This document includes the completed PRISMA-P checklist for the paper 'Methods used to meta-analyse results from interrupted time series studies: A methodological systematic review protocol'
Tumor ablation due to inhomogeneous -- anisotropic diffusion in generic 3-dimensional topologies
Creators: name: Kara, Erdi
name: Rahman, Aminur
name: Aulisa, Eugenio
name: Ghosh, Souparno
Publisher: name: arXiv
Year: 2019
Subjects: subject: Medical Physics (physics.med-ph)
subject: Tissues and Organs (q-bio.TO)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: We derive a full 3-dimensional (3-D) model of inhomogeneous -- anisotropic diffusion in a tumor region coupled to a binary population model. The diffusion tensors are acquired using Diffusion Tensor Magnetic Resonance Imaging (DTI) from a patient diagnosed with glioblastoma multiform (GBM). Then we numerically simulate the full model with Finite Element Method (FEM) and produce drug concentration heat maps, apoptosis regions, and dose-response curves. Finally, predictions are made about optimal injection locations and volumes, which are presented in a form that can be employed by doctors and oncologists.
description: 23 pages