cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Inversion method for content-based networks
Creators: name: Ramasco, Jose J.
name: Mungan, Muhittin
Publisher: name: arXiv
Year: 2007
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: In this paper, we generalize a recently introduced Expectation Maximization (EM) method for graphs and apply it to content-based networks. The EM method provides a classification of the nodes of a graph, and allows to infer relations between the different classes. Content-based networks are ideal models for graphs displaying any kind of community or/and multipartite structure. We show both numerically and analytically that the generalized EM method is able to recover the process that led to the generation of such networks. We also investigate the conditions under which our generalized EM method can recover the underlying contents-based structure in the presence of randomness in the connections. Two entropies, Sq and Sc, are defined to measure the quality of the node classification and to what extent the connectivity of a given network is content-based. Sq and Sc are also useful in determining the number of classes for which the classification is optimal.
description: 12 pages, 10 figs
Telomere-to-telomere Schizosaccharomyces japonicus genome assembly reveals hitherto unknown genome features.
Creators: name: Etherington, Graham J
name: Wu, Pei-Shang
name: Oliferenko, Snezhana
name: Uhlmann, Frank
name: Nieduszynski, Conrad A
Publisher: name: The Francis Crick Institute
Year: 2024
Subjects: classificationCode: Ecology,Evolution & Ethology
subject: Ecology,Evolution & Ethology
classificationCode: Genetics & Genomics
subject: Genetics & Genomics
classificationCode: Computational & Systems Biology
subject: Computational & Systems Biology
classificationCode: Model organisms
subject: Model organisms
classificationCode: Cell Biology
subject: Cell Biology
classificationCode: Cell Cycle & Chromosomes
subject: Cell Cycle & Chromosomes

description: Schizosaccharomyces japonicus belongs to the single-genus class Schizosaccharomycetes, otherwise known as "fission yeasts." As part of a composite model system with its widely studied S. pombe sister species, S. japonicus has provided critical insights into the workings and the evolution of cell biological mechanisms. Furthermore, its divergent biology makes S. japonicus a valuable model organism in its own right. However, the currently available genome assembly contains gaps and has been unable to resolve centromeres and other repeat-rich chromosomal regions. Here we present a telomere-to-telomere long-read genome assembly of the S. japonicus genome. This includes the three megabase-length chromosomes, with centromeres hundreds of kilobases long, rich in 5S ribosomal RNA genes, transfer RNA genes, long terminal repeats, and short repeats. We identify a gene-sparse region on chromosome 2 that resembles a 331 kb centromeric duplication. We revise the genome size of S. japonicus to at least 16.6 Mb and possibly up to 18.12 Mb, at least 30% larger than previous estimates. Our whole genome assembly will support the growing S. japonicus research community and facilitate research in new directions, including centromere and DNA repeat evolution, and yeast comparative genomics.
Results from the Evaluation of Community TOIs
Creators: name: Mireles, Ismael
name: Hesse, Katharine
name: Guerrero, Natalia
name: Kunimoto, Michelle
name: Huang, Chelsea
name: Fong, William
Publisher: name: Zenodo
Year: 2021

description: After three years of observations, the TESS mission has led to over 4300 TESS Objects of Interest (TOIs) being alerted. Of these, 168 TOIs were alerted because they were first identified as Community TOIS (CTOIs). The sample of promoted CTOIs includes full frame image (FFI) targets that are fainter than the Tmag = 10.5 cutoff used by QLP vetting and single transits that were rejected by the periodic signal searches from the QLP and SPOC pipelines. Here we detail the process by which these CTOIs were promoted to TOIs and present examples that highlight how the community has supplemented the standard TESS pipelines. The inclusion of these community targets will help explore longer-period planets as well as fainter targets that would have otherwise not been alerted as TOIs.
Usable Verification: Balancing Thinking and Automating
Creators: name: Wing, Jeannette M.
Publisher: name: Carnegie Mellon University
Year: 2005
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Here are five ideas on how to make verification more usable by and useful for people. They touch on education, techniques, and process. A common theme is the need to balance the need for human to think and the ability for machines to automate.
The Foucault Pendulum Precession and the Additivity of Infinitesimal Rotations
Creators: name: Basano, Lorenzo A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Popular Physics (physics.pop-ph)
subject: FOS: Physical sciences

description: The purpose of this paper is to give an intuitive explanation of the Foucault pendulum precession (Fpp) by exploiting the easily proved result that infinitesimal spatial rotations about different axes in three dimensions are additive. This allows to explain in a simpler way the Foucault precession by combining physical laws, intuition and a few elementary notions of astronomy. The paper is by no means intended to replace the material given in standard texts of classical mechanics; it is only an interdisciplinary description of the Foucault precession tailored for non specialists.
description: 9 pages, 5 figures
The atmospheric parameters of FGK stars using wavelet analysis of CORALIE spectra
Creators: name: Gill, Samuel
name: Maxted, Pierre. F. L.
name: Smalley, Barry
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Atmospheric properties of F-,G- and K-type stars can be measured by spectral model fitting. These methods require data with good signal-to-noise ratio and reliable continuum normalisation. This is particularly challenging for the spectra we have obtained with the CORALIE échelle spectrograph for FGK stars with transiting M-dwarf companions. The spectra tend to have low signal-to-noise ratios, which makes it difficult to analyse them using existing methods. Our aim is to create a reliable automated spectral analysis routine to determine $T_{\rm eff}$, [Fe/H], $V \sin i$ from the CORALIE spectra of FGK stars. We use wavelet decomposition to distinguish between noise, continuum trends, and stellar spectral features in the CORALIE spectra. A subset of wavelet coefficients from the target spectrum are compared to those from a grid of models in a Bayesian framework to determine the posterior probability distributions of the atmospheric parameters. By testing our method using synthetic spectra we found that our method converges on the best fitting atmospheric parameters. We test the wavelet method on 20 FGK exoplanet host stars for which higher quality data have been independently analysed using equivalent width measurements. We find that we can determine $T_{\rm eff}$ to a precision of $85$K, [Fe/H] to a precision of 0.06 dex and $V \sin i$ to a precision of 1.35 kms$^{-1}$ for stars with $V \sin i$ $\geq$ 5 kms$^{-1}$. We find an offset in metallicity $\approx -$0.18 dex relative to the equivelent width fitting method. We can determine $\log g$ to a precision of $0.13$ dex but measurements are only reliable to confirm dwarf-like surface gravity. The wavelet method can be used to determine $T_{\rm eff}$, [Fe/H] and $V \sin i$ for FGK stars from échelle spectra. We find that our method is self consistent, and robust for spectra with SNR$\gtrapprox 40$.
description: 14 pages, 13 figures, 6 tables. Accepted for publication in A&A
1I/`Oumuamua as a Tidal Disruption Fragment From a Binary Star System
Creators: name: Ćuk, Matija
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: 1I/`Oumuamua is the first known interstellar small body, probably being only about 100~m in size. Against expectations based on comets, `Oumuamua does not show any activity and has a very elongated figure, and also exhibits undamped rotational tumbling. In contrast, `Oumuamua's trajectory indicates that it was moving with the local stars, as expected from a low-velocity ejection from a relatively nearby system. Here I assume that `Oumuamua is typical of 100-m interstellar objects, and speculate on its origins. I find that giant planets are relatively inefficient at ejecting small bodies from inner solar systems of main-sequence stars, and that binary systems offer a much better opportunity for ejections of non-volatile bodies. I also conclude that `Oumuamua is not a member of a collisional population, which could explain its dramatic difference from small asteroids. I observe that 100-m small bodies are expected to carry little mass in realistic collisional populations, and that occasional events when whole planets are disrupted in catastrophic encounters may dominate interstellar population of 100-m fragments. Unlike the Sun or Jupiter, red dwarf stars are very dense and are capable of thoroughly tidally disrupting terrestrial planets. I conclude that the origin of `Oumuamua as a fragment from a planet that was tidally disrupted and then ejected by a dense member of a binary system could explain its peculiarities.
description: Revised for ApJL
Validating TESS Planet Candidates with TRICERATOPS
Creators: name: Giacalone, Steven
name: Dressing, Courtney D
Publisher: name: Zenodo
Year: 2021
Subjects: Exoplanets
Validation of Transiting Planets
Astrostatistics

description: Validation has played an important role in the discovery of planets detected by TESS. This process of scrutinizing a planet candidate typically involves an analysis of TESS photometry and a combination of different follow-up observations that rule out sources of astrophysical false positives. Despite its usefulness, validation of TESS planet candidates often lacks a robust statistical framework with which to argue for the existence of a planet. We present TRICERATOPS, an easy-to-use tool that resolves this shortcoming using a Bayesian probability calculation. By combining data from TESS and ground-based facilities, our tool quantifies the chance of a transit-like signal originating from both known and unresolved stars located near the potential planet-hosting star on the sky. We display that these quantities reliably predict which candidates are bona fide planets and which candidates are astrophysical false positives, such as nearby eclipsing binaries. We also discuss contexts in which validation with TRICERATOPS is particularly valuable, such as the discovery of planets around stars that make difficult targets for precise radial velocity observations.
description: {"references": ["Demangeon, Olivier D. S. et al. (2018). doi:10.1051/0004-6361/201731735", "Giacalone, Steven et al. (2021). doi:10.3847/1538-3881/abc6af", "Hedges, Christina et al. (2021). doi:10.3847/1538-3881/ac06cd", "Hillenbrand, Lynne et al. (2015). arXiv:1408.3475", "Kempton, Eliza M. -R. et al. (2018). doi:10.1088/1538-3873/aadf6f"]}
Challenges of the Dynamic Detection of Functionally Similar Code Fragments
Creators: name: Deissenboeck, Florian
name: Heinemann, Lars
name: Hummel, Benjamin
name: Wagner, Stefan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: Classic clone detection approaches are hardly capable of finding redundant code that has been developed independently, i.e., is not the result of copy&paste. To automatically detect such functionally similar code of independent origin, we experimented with a dynamic detection approach that applies random testing to selected chunks of code similar to Jiang&Su's approach. We found that such an approach faces several limitations in its application to diverse Java systems. This paper details on our insights regarding these challenges of dynamic detection of functionally similar code fragments. Our findings support a substantiated discussion on detection approaches and serve as a starting point for future research.
description: 11 pages, 3 figures
Determination of the superconducting gap in near optimally doped Bi_2Sr_{2-x}La_xCuO_{6+δ} (x ~ 0.4) from low-temperature specific heat
Creators: name: Wang, Yue
name: Liu, Zhi-Yong
name: Lin, C. T.
name: Wen, Hai-Hu
Publisher: name: arXiv
Year: 2011
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Low-temperature specific heat of the monolayer high-Tc superconductor Bi_2Sr_{2-x}La_xCuO_{6+δ} has been measured close to the optimal doping point (x ~ 0.4) in different magnetic fields. The identification of both a T^2 term in zero field and a \sqrt{H} dependence of the specific heat in fields is shown to follow the theoretical prediction for d-wave pairing, which enables us to extract the slope of the superconducting gap in the vicinity of the nodes (v_Δ, which is proportional to the superconducting gap Δ_0 at the antinodes according to the standard d_{x^2-y^2} gap function). The v_Δ or Δ_0 (~ 12 meV) determined from this bulk measurement shows close agreement with that obtained from spectroscopy or tunneling measurements, which confirms the simple d-wave form of the superconducting gap.
description: 5 pages, 4 figures, 1 table
[PhD output] Youth participatory mural guidebook
Creators: name: Puspita, Vina
Publisher: name: University of Lincoln
Year: 2024
Subjects: W900 - Others in creative arts & design

description: This Youth Participatory Mural Guidebook serves as the body of work submitted as part of a practice-based PhD research degree. It is accompanied by a portolio and written thesis that provide further context and analysis.Vina Puspita's practice-based research explores participatory art with young people in urban neighbourhoods in Jakarta to promote meaningful participation in peacebuilding. Focusing on the use of murals with children at risk of violence to express social and environmental issues, her study proposes a model of community-based participatory mural art that places children at the centre, working alongside local leaders. The study explores the potential of public art to promote power-sharing and intergenerational collaboration while challenging the idea of children's participation in public space in Jakarta, which has been contested. The research project involves young people aged 12-18, primarily but not limited to those who are members of the Children's Forums at the urban village level in East Jakarta. In total, 49 children participated in the study, although the number varied between each mural project.Through a series of mural projects, they work with different levels of government agencies and occupy different types of spaces. The study highlights the importance of child-friendly approaches, such as collaborative mural painting, in facilitating children's participation in society and encouraging critical reflection on their conditions. It reveals the complex issues facing young people in urban Jakarta and demonstrates how art can be used as a tool for advocacy and for bringing local leaders and young people into dialogue.Following a series of mural projects that took place from July to December 2022, together with young people and youth facilitators, a guidebook was co-created. The contents of the guidebook were formulated from the process and experiences of creating murals in four locations in the Jatinegara Sub-district. The guidebook includes a detailed technical step-by-step guide to making a mural that focuses on youth topics.This study is in connection with Mobile Arts for Peace (MAP): Informing the National Curriculum and Youth Policy for Peacebuilding in Kyrgyzstan, Rwanda, Indonesia, and Nepal (2020-2024).
Upgrading distributed applications with the version manager
Creators: name: Agrawal, Mukesh
name: Nath, Suman
name: Srinivasan  Seshan
Publisher: name: Carnegie Mellon University
Year: 2001
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Abstract: "Developers and managers of distributed systems today face a difficult choice. To provide for the evolution of their systems, they can either require that the software running on all nodes is inter-operable, or they can shut down the entire system when an upgrade is required. The former complicates the life of system developers, while the latter annoys users. We propose Version Manager, a middle ground between these approaches: an upgrade framework that limits the the [sic] extent of support required for interoperability, while also providing availability during upgrades. We evaluate the feasibility of our approach by applying it to two existing distributed systems: the Cooperative File System [11], and IrisLog [3]. Our proposal enables the upgrade of these systems while maintaining system availability, and without requiring code modifications."
Characterization of graphene through anisotropy of constant-energy maps in angle-resolved photoemission
Creators: name: Mucha-Kruczynski, M.
name: Tsyplyatyev, O.
name: Grishin, A.
name: McCann, E.
name: Fal'ko, Vladimir I.
name: Bostwick, A.
name: Rotenberg, E.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We show theoretically how constant-energy maps of the angle-resolved photoemission intensity can be used to test wave function symmetry in graphene. For monolayer graphene, we demonstrate that the observed anisotropy of ARPES spectra is a manifestation of what has been recently branded as electronic chirality. For bilayer graphene, we show that the anisotropy of the constant-energy maps may be used to extract information about the magnitude and sign of interlayer coupling parameters and about symmetry breaking inflicted on a bilayer by the underlying substrate.
description: 11 pages, 9 figures; improvements made to Fig. 7 and the text
Additional file 1 of Characterizing street-connected children and youths’ social and health inequities in Kenya: a qualitative study
Creators: name: L. Embleton
name: P. Shah
name: A. Gayapersad
name: R. Kiptui
name: D. Ayuku
name: P. Braitstein
Publisher: name: figshare
Year: 2020
Subjects: subject: Sociology
subject: FOS: Sociology

description: Additional file 1. Interview Guide for Community Members Key Informant Interviews & Focus Group Discussions.
Accurate stellar parameters for stars in Tight Triple Systems
Creators: name: Moharana, Ayush
name: Hełminiak, K.G.
name: Marcadon, F.
name: Pawar, T.
name: Konacki, M.
Publisher: name: Zenodo
Year: 2021
Subjects: Stellar Astrophysics
Triple stars
Eclipsing Binaries
Accurate stellar parameters

description: Tight Triple Systems (TTS) have stars in a hierarchical configuration with a third star orbiting the inner binary with a period of fewer than 1000 days. Such systems are a hub of various dynamical interactions and are important for understanding the formation and evolution of stars in multiple systems. Having a detached eclipsing binary (DEB) as one of its components allows us to obtain precise stellar and orbital parameters of these systems. Various recent discoveries have been due to space-based photometry from Kepler and TESS. We present the accurate stellar and orbital parameters of a TTS, TIC 284595199, using TESS photometry coupled with radial velocities extracted from the triple-lined (SB3) spectra from HIDES spectrograph. Using these accurate parameters we determine the evolutionary states of the stars and the dynamic interactions possible in this system.
description: {"references": ["Hajdu et al., 2017, MNRAS, 471, 1230 (https://doi.org/10.1093/mnras/stx1523)", "Izumiura et al., 1999, in Proc. EAMA, 77", "Conroy et al., 2020, ApJS, 250, 34 (https://doi.org/10.3847/1538-4365/abb4e2)", "Mazeh & Zucker, 1994, Ap&SS, 212, 349 (https://doi,org/10.1007/BF00984538 )", "Konacki et al., 2009, ApJ, 704, 513 (https://doi.org/10.1088/0004-637X/704/1/513)", "Choi et al., 2016, ApJ, 823,102 (https://doi.org/10.3847/0004-637X/823/2/102)", "Toonen et al., 2020, A&A, 640, A16 (https://doi.org/10.1051/0004-6361/201936835)"]}
Rb-NMR study of the quasi-one dimensional competing spin-chain compound Rb2Cu2Mo3O12
Creators: name: Matsui, Kazuki
name: Yagi, Ayato
name: Hoshino, Yukihiro
name: Atarashi, Sochiro
name: Hase, Masashi
name: Sasaki, Takahiko
name: Goto, Takayuki
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Rb-NMR study has been performed on the quasi-one dimensional competing spin chain Rb2Cu2Mo3O12 with ferromagnetic and antiferromagnetic exchange interactions on nearest neighboring and next nearest neighboring spins, respectively. The system changes from a gapped ground state at zero field to the gapless state at H_C \simeq 2 T, where the existence of magnetic order below 1 K was demonstrated by a broadening of NMR spectrum, associated with a critical divergence of 1/T_1. In higher temperature region, 1/T_1 showed a power-law type temperature dependence, from which the field dependence of Luttinger parameter K was obtained and compared with theoretical calculations based on the spin nematic Tomonaga Luttinger Liquid (TLL) state.
Microbubble formation and pinch-off scaling exponent in flow-focusing devices
Creators: name: van Hoeve, Wim
name: Dollet, Benjamin
name: Versluis, Michel
name: Lohse, Detlef
Publisher: name: arXiv
Year: 2011
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We investigate the gas jet breakup and the resulting microbubble formation in a microfluidic flow-focusing device using ultra high-speed imaging at 1 million frames/s. In recent experiments [Dollet et al., Phys. Rev. Lett. 100, 034504 (2008)] it was found that in the final stage of the collapse the radius of the neck scales with time with a 1/3 power-law exponent, which suggested that gas inertia and the Bernoulli suction effect become important. Here, ultra high-speed imaging was used to capture the complete bubble contour and quantify the gas flow through the neck. It revealed that the resulting decrease in pressure, due to Bernoulli suction, is too low to account for an accelerated pinch-off. The high temporal resolution images enable us to approach the final moment of pinch-off to within 1 μs. We observe that the final moment of bubble pinch-off is characterized by a scaling exponent of 0.41 +/- 0.01. This exponent is approximately 2/5, which can be derived, based on the observation that during the collapse the neck becomes less slender, due to the exclusive driving through liquid inertia.
title: ADCO, Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Cart. 198-01 (11 H 1055), 185 folios, f. 0337
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0337, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0337, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Random walks in a random environment on a strip: a renormalization group approach
Creators: name: Juhász, Róbert
Publisher: name: arXiv
Year: 2007
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We present a real space renormalization group scheme for the problem of random walks in a random environment on a strip, which includes one-dimensional random walk in random environment with bounded non-nearest-neighbor jumps. We show that the model renormalizes to an effective one-dimensional random walk problem with nearest-neighbor jumps and conclude that Sinai scaling is valid in the recurrent case, while in the sub-linear transient phase, the displacement grows as a power of the time.
description: 9 pages
"What is the structural chemistry of the living organism at its temperature and pressure?"
Creators: name: Helliwell, John R
Publisher: name: Zenodo
Year: 2019
Subjects: UK XFEL
Macromolecular crystallography
Room temperature
Cryo temperature
X-rays
Neutrons

description: Prepared for the UK XFEL Science Case 2019 consultation coordinated by Professor Jon Marangos of Imperial College, London.
description: I was not able to present on the Workshop day due to a family travel commitment and so I make my presentation available here on Zenodo.
description: {"references": ["45.\tJR Helliwell New developments in crystallography: exploring its methods, technology and scope in the molecular biosciences Bioscience Reports (2017) 37 BSR20170204 DOI: 10.1042/BSR20170204"]}
Determining Uncertainty in TESS Light Curves Using Eclipsing Binaries
Creators: name: Swanson, Jaide
name: Bell, Keaton
name: Davenport, J.R.A.
Publisher: name: Zenodo
Year: 2021
Subjects: Eclipsing Binaries

description: Large TESS pixels typically capture light from multiple stars, and the data processing pipeline subtracts the estimated contributions of contaminant stars from the light curves it produces. If these crowdedness factors (recorded as the header keyword CROWDSAP) are not exact, they will cause systematic errors on measurements of transit depths and variability amplitudes. We are performing an independent determination of estimated CROWDSAP factors by comparing the depths of binary eclipses between TESS light curves and ground-based data from ASAS-SN with a Markov Chain Monte Carlo analysis. This allows us to accurately appraise the precision of pipeline CROWDSAP factors, the uncertainty on which should be incorporated into TESS analyses as an extrinsic error.
description: {"references": ["Stumpe et al. 2012, PASP, 124, 985. doi:10.1086/667698", "Dalba,et al. 2017, AJ, 153, 59. doi:10.1088/1361-6528/aa5278", "Kochanek et al. 2017, PASP, 129, 104502. doi:10.1088/1538-3873/aa80d9", "Foreman-Mackey et al. 2013, Astrophysics Source Code Library. ascl:1303.002", "Maxted, P.~F.~L. 2016, AAP, 591, A111. doi:10.1051/0004-6361/201628579", "Morton, T.~D. 2015, Astrophysics Source Code Library. ascl:1503.010"]}
Study of gravitational radiation from cosmic domain walls
Creators: name: Kawasaki, Masahiro
name: Saikawa, Ken'ichi
Publisher: name: arXiv
Year: 2011
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this paper, following the previous study, we evaluate the spectrum of gravitational wave background generated by domain walls which are produced if some discrete symmetry is spontaneously broken in the early universe. We apply two different methods to calculate the gravitational wave spectrum: One is to calculate the gravitational wave spectrum directly from numerical simulations, and another is to calculate it indirectly by estimating the unequal time anisotropic stress power spectrum of the scalar field. Both analysises indicate that the slope of the spectrum changes at two characteristic frequencies corresponding to the Hubble radius at the decay of domain walls and the width of domain walls, and that the spectrum between these two characteristic frequencies becomes flat or slightly red tilted. The second method enables us to evaluate the GW spectrum semi-analytically for the frequencies which can not be resolved in the finite box lattice simulations, but relies on the assumptions for the unequal time correlations of the source.
description: 17 pages, 9 figures; revised version of the manuscript, accepted for publication in JCAP
Colour Rearrangement for Dipole Showers
Creators: name: Bellm, Johannes
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present an algorithm to rearrange the colour chains of dipole showers in the shower process according to the colour amplitudes of a simple matrix element. We implement the procedure in the dipole shower of Herwig and show comparisons to data.
description: 4 pages, 6 figures, HERWIG-2018-01, LU-TP-18-01, MCnet-18-01
Impacts of regional sea ice loss – a global response
Creators: name: Eade, Rosemary
name: Smith, Doug
name: Hermanson, Leon
name: Dunstone, Nick
Publisher: name: Zenodo
Year: 2019

description: Climate model studies have shown a wide range of responses in the northern hemisphere to reduced sea ice loss in the Arctic. The most robust is the thermodynamic response with local warming in the region of the sea ice loss. Many studies also find a shift in the tropospheric jet towards the equator and a tendency towards the negative phase of the North Atlantic Oscillation. However, these mid-latitude dynamic responses seem somewhat dependent on the extent and location of sea ice loss as well as model differences. We use new atmosphere-only experiments from the Polar-Amplification-MIP of CMIP6 to further explain how the dynamic responses in the atmosphere relate to the pattern of sea ice loss in the Arctic on multi-decadal time-scales. We find exciting new results that suggest that Arctic sea ice loss can also impact the southern hemisphere, while Antarctic sea ice loss can impact the northern hemisphere, and we propose possible atmospheric mechanisms to explain this linkage. We also highlight the importance of large ensembles to differentiate between robust responses and atmospheric noise.
Long-Term Stability of Planets in the $α$ Centauri System, II: Forced Eccentricities
Creators: name: Quarles, Billy
name: Lissauer, Jack J.
name: Kaib, Nathan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We extend our study of the extent of the regions within the $α$ Centauri AB star system where small planets are able to orbit for billion-year timescales (Quarles & Lissauer 2016, AJ 151, 111) to investigate the effects of minimizing the forced eccentricity of initial trajectories. We find that initially prograde, circumstellar orbits require a piecewise quadratic function to accurately approximate forced eccentricity as a function of semimajor axis, but retrograde orbits can be modeled using a linear function. Circumbinary orbits in the $α$ Centauri AB system are less affected by the forced eccentricity. {Planets on circumstellar orbits that begin with eccentricity vectors near their forced values are generally stable, up to $\sim$$10^9$ yr, out to a larger semimajor axis than are planets beginning on circular orbits. The amount by which the region of stability expands is much larger for retrograde orbits than it is for prograde orbits. The location of the stability boundary for two planet systems on prograde, circular orbits is much more sensitive to the initial eccentricity state than it is for analogous single planet systems.
description: 11 pages, 10 figures, 3 tables; Accepted in Astronomical Journal
Additional file 1 of Comparison of a home-based (multi) systemic intervention to promoting Medication AdheRence and Self-management among kidney transplant recipients with care-as-usual: the MARS randomized controlled trial protocol
Creators: name: Beck, Denise Karin
name: Tielen, Mirjam
name: Rechards, Marloes
name: Timman, Reinier
name: Boonstra, Charlotte
name: Versteegh, Josette
name: Wetering, Jacqueline Van De
name: Zietse, Robert
name: Gelder, Teun Van
name: Weimar, Willem
name: Saase, Jan Van
name: Busschbach, Jan Van
name: Massey, Emma Kay
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Supplementary file 1. Self-developed social support items. Two self-developed items in addition to the existing social support scales to assess social support.
Multiferroic vertically aligned nanocomposite with CoFe2O4 nanocones embedded in layered Bi2WO6 matrix
Creators: name: Wang, Han
name: Li, Leigang
name: Huang, Jijie
name: Gao, Xingyao
name: Sun, Xing
name: Wang, Haiyan
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Evolutionary Biology
subject: Chemical Sciences not elsewhere classified
subject: Astronomical and Space Sciences not elsewhere classified
subject: Cancer
subject: Virology

description: Bi2WO6:CoFe2O4 (BWO:CFO) vertically aligned nanocomposite (VAN) in epitaxial thin film form has been demonstrated on single-crystal LaAlO3 (LAO) (001) substrates via pulsed laser deposition (PLD). CFO nanopillars exhibit a unique nanocone shape embedded in the epitaxial BWO matrix with an Aurivillius layered oxide structure. The growth direction of the CFO nanopillars is (004), different from that of its epitaxial single-phase counterpart (220), which is attributed to the interfacial strain effect. Magnetic measurements show robust and anisotropic magnetic properties from the CFO nanocone structures, and obvious ferroelectric responses are demonstrated in the BWO matrix, both at room temperature. The BWO:CFO VAN thin film combining a ferroelectric layered oxide matrix and magnetic vertical nanocone present a new hybrid material platform for room temperature multiferroics design towards nanoscale sensors and actuators.
Decelerating microdynamics can accelerate macrodynamics in the voter model
Creators: name: Stark, Hans-Ulrich
name: Tessone, Claudio J.
name: Schweitzer, Frank
Publisher: name: arXiv
Year: 2007
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: For the voter model, we study the effect of a memory-dependent transition rate. We assume that the transition of a spin into the opposite state decreases with the time it has been in its current state. Counter-intuitively, we find that the time to reach a macroscopically ordered state can be accelerated by slowing-down the microscopic dynamics in this way. This holds for different network topologies, including fully-connected ones. We find that the ordering dynamics is governed by two competing processes which either stabilize the majority or the minority state. If the first one dominates, it accelerates the ordering of the system. The conclusions of this Letter are not restricted to the voter model, but remain valid to many other spin systems as well.
description: See http://www.sg.ethz.ch for related publications
Unsupervised Induction of Natural Language Morphology Inflection Classes
Creators: name: Monson, Christian
name: Lavie, Alon
name: Carbonell, Jaime G.
name: Levin, Lorraine
Publisher: name: Carnegie Mellon University
Year: 2009
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: We propose a novel language-independent framework for inducing a collection of morphological inflection classes from a monolingual corpus of full form words. Our approach involves two main stages. In the first stage, we generate a large data structure of candidate inflection classes and their interrelationships. In the second stage, search and filtering techniques are applied to this data structure, to identify a select collection of "true" inflection classes of the language. We describe the basic methodology involved in both stages of our approach and present an evaluation of our baseline techniques applied to induction of major inflection classes of Spanish. The preliminary results on an initial training corpus already surpass an F1 of 0.5 against ideal Spanish inflectional morphology classes.
Origins of Hot Jupiters
Creators: name: Dawson, Rebekah I.
name: Johnson, John Asher
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Hot Jupiters were the first exoplanets to be discovered around main sequence stars and astonished us with their close-in orbits. They are a prime example of how exoplanets have challenged our textbook, solar-system inspired story of how planetary systems form and evolve. More than twenty years after the discovery of the first hot Jupiter, there is no consensus on their predominant origin channel. Three classes of hot Jupiter creation hypotheses have been proposed: in situ formation, disk migration, and high eccentricity tidal migration. Although no origin channel alone satisfactorily explains all the evidence, two major origins channels together plausibly account for properties of hot Jupiters themselves and their connections to other exoplanet populations.
description: Submitted to ARAA. Comments/suggestions welcome
title: ADCO, Cartulaire des Dominicains de Dijon (1286), Cart. 221 (H 53), 170 folios, f. 0303
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios, f. 0303, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: Dijon
description: Provenance: http://www.wikidata.org/entity/Q7003
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb15250518p
description: Provenance: http://www.idref.fr/02643413X/id
description: Provenance: https://www.geonames.org/6453767
Landweber exact formal group laws and smooth cohomology theories
Creators: name: Bunke, Ulrich
name: Schick, Thomas
name: Schroeder, Ingo
name: Wiethaup, Moritz
Publisher: name: arXiv
Year: 2007
Subjects: subject: K-Theory and Homology (math.KT)
subject: Algebraic Topology (math.AT)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics

description: The main aim of this paper is the construction of a smooth (sometimes called differential) extension \hat{MU} of the cohomology theory complex cobordism MU, using cycles for \hat{MU}(M) which are essentially proper maps W\to M with a fixed U(n)-structure and U(n)-connection on the (stable) normal bundle of W\to M. Crucial is that this model allows the construction of a product structure and of pushdown maps for this smooth extension of MU, which have all the expected properties. Moreover, we show, using the Landweber exact functor principle, that \hat{R}(M):=\hat{MU}(M)\otimes_{MU^*}R defines a multiplicative smooth extension of R(M):=MU(M)\otimes_{MU^*}R whenever R is a Landweber exact MU*-module. An example for this construction is a new way to define a multiplicative smooth K-theory.
description: 40 pages v2: serious mistake in definition of MU(M) corrected, v3: small mistakes corrected, minor additions, fontsize changed v4: final version, to appear in Algebraic and Geometric Topology, typos corrected, changed to journal house style; v5: typos corrected, one references updated, v6: DOI-glitch and page numbers corrected
Dirac State in a Centrosymmetric Superconductor alpha-PdBi2
Creators: name: Dimitri, Klauss
name: Hosen, M. Mofazzel
name: Dhakal, Gyanendra
name: Choi, Hongchul
name: Kabir, Firoza
name: Kaczorowski, Dariusz
name: Durakiewicz, Tomasz
name: Zhu, Jian-Xin
name: Neupane, Madhab
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Topological superconductor (TSC) hosting Majorana fermions has been established as a milestone that may shift our scientific trajectory from research to applications in topological quantum computing. Recently, superconducting Pd-Bi binaries have attracted great attention as a possible medium for the TSC phase as a result of their large spin-orbit coupling strength. Here, we report a systematic high-resolution angle-resolved photoemission spectroscopy (ARPES) study on the normal state electronic structure of superconducting alpha-PdBi2 (Tc = 1.7 K). Our results show the presence of Dirac states at higher-binding energy with the location of the Dirac point at 1.26 eV below the chemical potential at the zone center. Furthermore, the ARPES data indicate multiple band crossings at the chemical potential, consistent with the metallic behavior of alpha-PdBi2. Our detailed experimental studies are complemented by first-principles calculations, which reveal the presence of surface Rashba states residing in the vicinity of the chemical potential. The obtained results provide an opportunity to investigate the relationship between superconductivity and topology, as well as explore pathways to possible future platforms for topological quantum computing.
description: 6 pages, 4 figures
The Occurrence-weighted Median Planets Discovered by Transit Surveys Orbiting Solar-type Stars and Their Implications for Planet Formation and Evolution
Creators: name: Schlaufman, Kevin C
name: Halpern, Noah D
Publisher: name: Zenodo
Year: 2021
Subjects: Exoplanets
Data Analysis Techniques

description: Planet occurrence and primordial atmospheric retention probability increase with period. The heavily irradiated short-period planets discovered by duration-limited transit surveys like that being executed by the Transiting Exoplanet Survey Satellite (TESS) may be very different from the lightly irradiated longer-period planets that are now known to be a much more common outcome of the planet formation process. We show that an occurrence-weighted mass--radius relation for the low-mass planets discovered so far by transit surveys orbiting solar-type stars requires both occurrence-weighted median Earth-mass and Neptune-mass planets to have a few percent of their masses in hydrogen/helium (H/He) atmospheres. It also implies core masses Mc in the range 2 MEarth < Mc < 8 MEarth that can retain their primordial atmospheres. In contrast to Uranus and Neptune that have at least 10% of their masses in H/He atmospheres, these occurrence-weighted median Neptune-mass planets are H/He poor. The implication is that they experienced collisions or formed in much shorter-lived and/or hotter parts of their parent protoplanetary disks than Uranus and Neptune's formation location in the protosolar nebula.
Additional file 1 of Urine neutrophil gelatinase-associated lipocalin and urine output as predictors of the successful discontinuation of continuous renal replacement therapy in critically ill patients with acute kidney injury
Creators: name: Thomsen, Josefine
name: Sprogøe, Ulrik
name: Toft, Palle
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Marine Biology
subject: Science Policy
subject: Hematology
subject: 60506 Virology

description: Additional file 1. Appendix
Flavor Asymmetry of the Nucleon Sea and the Five-Quark Components of the Nucleons
Creators: name: Chang, Wen-Chen
name: Peng, Jen-Chieh
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The existence of the five-quark Fock states for the intrinsic charm quark in the nucleons was suggested some time ago, but conclusive evidence is still lacking. We generalize the previous theoretical approach to the light-quark sector and study possible experimental signatures for such five-quark states. In particular, we compare the $\bar d - \bar u$ and $\bar u + \bar d - s -\bar s$ data with the calculations based on the five-quark Fock states. The qualitative agreement between the data and the calculations is interpreted as evidence for the existence of the intrinsic light-quark sea in the nucleons. The probabilities for the $|uudu\bar{u}>$ and $|uudd\bar{d}>$ Fock states are also extracted.
description: 4 pages, 3 figures
Community Access to CHEOPS
Creators: name: Isaak, Kate
Publisher: name: Zenodo
Year: 2021
Subjects: Exoplanets
CHEOPS
ESA Guest Observers Programme

description: CHEOPS (CHaracterising ExOPlanet Satellite) is the first mission dedicated to the follow-up and study of known exoplanets orbiting bright stars using ultra-high precision, transit photometry. The mission is a partnership between ESA’s Science Programme and Switzerland, through a Consortium of 11 ESA member states led by University of Bern (CH). In this poster we outline how the Community can access CHEOPS.
The rank of a quiver representation
Creators: name: Kinser, Ryan
Publisher: name: arXiv
Year: 2007
Subjects: subject: Representation Theory (math.RT)
subject: Rings and Algebras (math.RA)
subject: FOS: Mathematics
subject: 16G20; 19A22; 15A03; 15A69; 18D10

description: We define a functor which gives the "global rank of a quiver representation" and prove that it has nice properties which make it a generalization of the rank of a linear map. We demonstrate how to construct other "rank functors" for a quiver Q, which induce ring homomorphisms (called "rank functions") from the representation ring of Q to Z. These rank functions give discrete numerical invariants of quiver representations, useful for computing tensor product multiplicities of representations and determining some structure of the representation ring. We also show that in characteristic 0, rank functors commute with the Schur operations on quiver representations, and the homomorphisms induced by rank functors are lambda-ring homomorphisms.
description: 17 pages, hyper-linked. Various typos and formatting corrected, final version