cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
M$^3$: A New Muon Missing Momentum Experiment to Probe $(g-2)_μ$ and Dark Matter at Fermilab
Creators: name: Kahn, Yonatan
name: Krnjaic, Gordan
name: Tran, Nhan
name: Whitbeck, Andrew
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Experiment (hep-ex)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: New light, weakly-coupled particles are commonly invoked to address the persistent $\sim 4σ$ anomaly in $(g-2)_μ$ and serve as mediators between dark and visible matter. If such particles couple predominantly to heavier generations and decay invisibly, much of their best-motivated parameter space is inaccessible with existing experimental techniques. In this paper, we present a new fixed-target, missing-momentum search strategy to probe invisibly decaying particles that couple preferentially to muons. In our setup, a relativistic muon beam impinges on a thick active target. The signal consists of events in which a muon loses a large fraction of its incident momentum inside the target without initiating any detectable electromagnetic or hadronic activity in downstream veto systems. We propose a two-phase experiment, M$^3$ (Muon Missing Momentum), based at Fermilab. Phase 1 with $\sim 10^{10}$ muons on target can test the remaining parameter space for which light invisibly-decaying particles can resolve the $(g-2)_μ$ anomaly, while Phase 2 with $\sim 10^{13}$ muons on target can test much of the predictive parameter space over which sub-GeV dark matter achieves freeze-out via muon-philic forces, including gauged $U(1)_{L_μ- L_τ}$.
description: 28 pages, 11 figures, 2 appendices
Boats as housing in Oxford: Trajectories of Informality in a High‐Income Context
Creators: name: Galuszka, Jakub
Publisher: name: Wiley
Year: 2024
Subjects: subject: 600 Technik, Medizin, angewandte Wissenschaften::690 Hausbau, Bauhandwerk::690 Hausbau, Bauhandwerk
subject: informality
subject: formality
subject: everyday approaches
subject: advocacy
subject: gentrification
subject: co-production
subject: precariousness
subject: housing
subject: waterways
subject: houseboats

description: In this article I aim to shed light on boat dwelling as an increasingly popular housing practice in the UK. I investigate the changing nature of this practice in times of housing crisis and of the connection between formal and informal approaches, and discuss how decentralized urban actors influence and safeguard their visions of housing. My investigation concentrates on three intertwined strategies boaters in Oxford use to deal with growing regularization and commodification pressures: (non)compliance, formalization and staying under the radar. My findings challenge several assumptions about housing informality in the global North and document the diverse trajectories that informal processes may take. My analysis reveals that informal and semi‐formal solutions are not simply ‘tolerated’ or ‘overlooked’ by the state, but co‐produced by urban dwellers through a repertoire of everyday actions and ad hoc advocacy approaches. The construction of specific trajectories of informal housing emerges at the interface of complex agendas and attitudes that go beyond the generalized roles attributed to the key urban sectors.
Light Gluinos and the Parton Structure of the Nucleon
Creators: name: Rueckl, R.
name: Vogt, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the effects of light gluinos with mass below about 1 GeV on the nucleon parton densities and the running of alpha_(S). It is shown that from the available high-statistics DIS data no lower bound on the gluino mass can be derived. Also in the new kinematical region accessible at HERA the influence of such light gluinos on structure f unctions is found to be very small and difficult to detect. For use in more direct searches involving final state signatures we present a radiative estimate of the gluino distribution in the nucleon.
description: 23 pages, LateX, 8 figures, MPI-PhT/94-22, LMU-3/94
Solitons, the Korteweg-de Vries equation with step boundary values and pseudo-embedded eigenvalues
Creators: name: Ablowitz, Mark J.
name: Luo, Xu-Dan
name: Cole, Justin T.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences

description: The Korteweg-deVries (KdV) equation with step boundary conditions is considered, with an emphasis on soliton dynamics. When one or more initial solitons are of sufficient size they can propagate through the step; in this case the phase shift is calculated via the inverse scattering transform. On the other hand, when the amplitude is too small they become trapped. In the trapped case the transmission coefficient of the associated associated linear Schrödinger equation can become large at a point exponentially close to the continuous spectrum. This point is referred to as a {\it pseudo-embedded eigenvalue}. Employing the inverse problem it is shown that the continuous spectrum associated with a branch cut in the neighborhood of the pseudo-embedded eigenvalue plays the role of discrete spectra, which in turn leads to a trapped soliton in the KdV equation.
description: 8 pages, 2 figures
Additional file 2: of OPTimal IMAging strategy in patients suspected of non-traumatic pulmonary disease at the emergency department: chest X-ray or ultra-low-dose CT (OPTIMACT)â a randomised controlled trial chest X-ray or ultra-low-dose CT at the ED: design and rationale
Creators: name: Berk, Inge Van Den
name: Maadrika Kanglie
name: Engelen, Tjitske Van
name: Shandra Bipat
name: Dijkgraaf, Marcel
name: Bossuyt, Patrick
name: MonyĂŠ, Wouter De
name: Prins, Jan
name: Stoker, Jaap
Publisher: name: figshare
Year: 2018
Subjects: Medicine
Biotechnology
Science Policy

description: Appendix 2. Patient information folder regular version. (PDF 61Â kb)
Deep Learning: A Tool for Computational Nuclear Physics
Creators: name: Negoita, Gianina Alina
name: Luecke, Glenn R.
name: Vary, James P.
name: Maris, Pieter
name: Shirokov, Andrey M.
name: Shin, Ik Jae
name: Kim, Youngman
name: Ng, Esmond G.
name: Yang, Chao
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: In recent years, several successful applications of the Artificial Neural Networks (ANNs) have emerged in nuclear physics and high-energy physics, as well as in biology, chemistry, meteorology, and other fields of science. A major goal of nuclear theory is to predict nuclear structure and nuclear reactions from the underlying theory of the strong interactions, Quantum Chromodynamics (QCD). With access to powerful High Performance Computing (HPC) systems, several ab initio approaches, such as the No-Core Shell Model (NCSM), have been developed to calculate the properties of atomic nuclei. However, to accurately solve for the properties of atomic nuclei, one faces immense theoretical and computational challenges. The present study proposes a feed-forward ANN method for predicting the properties of atomic nuclei like ground state energy and ground state point proton root-mean-square (rms) radius based on NCSM results in computationally accessible basis spaces. The designed ANNs are sufficient to produce results for these two very different observables in 6Li from the ab initio NCSM results in small basis spaces that satisfy the theoretical physics condition: independence of basis space parameters in the limit of extremely large matrices. We also provide comparisons of the results from ANNs with established methods of estimating the results in the infinite matrix limit.
description: 9 pages, 9 figures, published in the Proceedings of the Ninth International Conference on Computational Logics, Algebras, Programming, Tools, and Benchmarking COMPUTATION TOOLS 2018 February 18-22, 2018, Barcelona, Spain by IARIA
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Cart. 192 (11 H 77), 295 folios, f. 0255v
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: Petot, Frédéric
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 général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0255v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0255v, 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
Murex scabriculus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Muricidae
Murex
Murex scabriculus

description: Murex scabriculus [spec. nov.]
M. testa ovata plicata decussatim reticulata: maculis prominulis, columella plicata, cauda truncata.
Gvalt. test. t. 48. f. B, C, D, E.
Habitat ..
Testa nuce coryli major, cancellata & aspera rugis longitudinalibus striisque elevatis acutis transversalibus, colore subferrugineo fasciis suturisque albis. Apertura alba. Columella umbilicata, plicata, labio dentato crenato. Cauda truncata suturis membranaceis & integra a Buccinis differt.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 751, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 1 of Epitranscriptomic analysis reveals clinical and molecular signatures in glioblastoma
Creators: name: de Mendonça Fernandes, Glaucia Maria
name: Wang, Wesley
name: Ahmadian, Saman Seyed
name: Jones, Daniel
name: Peng, Jing
name: Giglio, Pierre
name: Venere, Monica
name: Otero, José Javier
Publisher: name: figshare
Year: 2025
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Supplementary Material 1
Environmental Dependence of the Fundamental Plane of Galaxy Clusters
Creators: name: Miller, Christopher J.
name: Melott, Adrian
name: Gorman, Patrick
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Galaxy clusters approximate a planar (FP) distribution in a three-dimensional parameter space which can be characterized by optical luminosity, half-light radius, and X-ray luminosity. Using a high-quality catalog of cluster redshifts, we find the nearest neighbor cluster for those common to an FP study and the cluster catalog. Examining scatter about the FP, we find 99.2% confidence that it is dependent on nearest neighbor distance. Our study of X-Ray clusters finds that those with high central gas densities are systematically closer to neighbor clusters. If we combine results here with those of Fritsch and Buchert, we find an explanation for some of our previous conclusions: Clusters in close proximity to other clusters are more likely to have massive cooling flows because they are more relaxed and have higher central gas densities.
description: Accepted for publication in Astrophysical Journal Letters. Moderate revisions, including more statistical analysis and discussion. Latex, 7 pages
OGAHIY HAYOTI VA IJODI
Creators: name: Jalolov, Haqberdi
Publisher: name: Zenodo
Year: 2024

description: O'n to'qqizinchi asrning birinchi yarmi o'zbek adabiyoti, xususan Xorazmda vujudga kelgan adabiy harakatning eng ilg'or vakillaridan biri Ogahiydir. Alohida qayd etish lozimki, Ogahiy o'zining yuksak iste'dodi, sermahsul ijodiy merosi bilan adabiyotimiz tarixida zabardast olim, talantli shoir, yetuk tarixchi, mohir tarjimon sifatida alohida o'rin tutadi.
Additional file 2 of Intranasal HD-Ad vaccine protects the upper and lower respiratory tracts of hACE2 mice against SARS-CoV-2
Creators: name: Cao, Huibi
name: Mai, Juntao
name: Zhou, Zhichang
name: Li, Zhijie
name: Duan, Rongqi
name: Watt, Jacqueline
name: Chen, Ziyan
name: Bandara, Ranmal Avinash
name: Li, Ming
name: Ahn, Sang Kyun
name: Poon, Betty
name: Christie-Holmes, Natasha
name: Gray-Owen, Scott D.
name: Banerjee, Arinjay
name: Mossman, Karen
name: Kozak, Rob
name: Mubareka, Samira
name: Rini, James M.
name: Hu, Jim
name: Liu, Jun
Publisher: name: figshare
Year: 2021
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 2: Table S1. Codon optimized RBD (residues 328 to 528) of the SARS-CoV-2 Spike Protein. Table S2. Primers used in qRT-PCR analysis of cytokine and chemokine mRNAs.
Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres
Creators: name: Hook, Anson
name: Kahn, Yonatan
name: Safdi, Benjamin R.
name: Sun, Zhiquan
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We show that axion dark matter (DM) may be detectable through narrow radio lines emitted from neutron stars. The neutron star magnetosphere hosts a strong magnetic field and a plasma frequency that increases towards the neutron star surface. As the axions pass through the magnetosphere, they can resonantly convert into radio photons in a narrow region around the radius at which the plasma frequency equals the axion mass. The bandwidth of the signal is set by the small DM velocity dispersion far away from the neutron star. We solve the axion-photon mixing equations, including a full treatment of the magnetized plasma and associated anisotropic dielectric tensor, to obtain the conversion probability. We discuss possible neutron-star targets and how they may probe the QCD axion parameter space in the mass range of ~0.2-40 $μ$eV.
description: 7+8 pages, 1+4 figures
Additional file 2: of Mutations in dock1 disrupt early Schwann cell development
Creators: name: Cunningham, Rebecca
name: Herbert, Amy
name: Harty, Breanne
name: Ackerman, Sarah
name: Monk, Kelly
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Hematology

description: Figure S2. A) The stl365 allele was generated by a TALEN that resulted in one base pair insertion causing an early stop. B) Genotyping assay for the stl365 lesion. The PCR amplified product is digested with EcoRV and run on a 3% agarose gel. C) The stl366 allele was generated by a TALEN that resulted in a 13 base-pair deletion causing an early stop. D) Genotyping assay for the stl366 lesion. The PCR amplified product is digested with HpyCH4III and run on a 3% agarose gel. E) RT-PCR for dock1 on adult PLLn cDNA shows dock1 is expressed in the PLLn. F) Control reaction performed with Milli-q water as a substrate. (PDF 362 kb)
Well it works! Reflections on the Audiamus model for corpus building and where it could go from here
Creators: name: Thieberger, Nick
Publisher: name: Zenodo
Year: 2006
Subjects: transcription, citable media, language documentation

description: Audiamus (1998-2010) is a tool that was created using HyperCard for interacting with field recordings via their transcripts. It allows the user to build a citable corpus of media via linked transcripts assuming persistent identification of primary data (as given by an archive) to provide citability of data at the most granular level. This takes advantage of transcription tools to give the analyst instant access to primary data and so increases the accountability of linguistic analysis. Ease of use is paramount! Audiamus takes the output of Transcriber or Elan as input. It was first written in HyperCard, then built in proprietary software, Runtime Revolution (rapid prototyping), with Win/Mac (&Linux) standalone versions.
description: Video demo of Audiamus on this page: https://nthieberger.net/audiamus.htm
description: {"references": ["Thieberger, Nicholas. 2004. Documentation in practice: Developing a linked media corpus of South Efate. Peter Austin (ed). Language documentation and description, Volume 2. London: Hans Rausing Endangered Languages Project, SOAS. 169-178."]}
Additional file 1 of Severity and factors of menopausal symptoms in middle-aged women in Gansu Province of China: a cross-sectional study
Creators: name: Wang, LiRong
name: Zhang, Rui
name: Yang, Ye
name: Sun, XiaoYan
name: Zhang, BaoLi
name: Zhu, HaiYing
name: Luo, XiaoRong
name: Ma, XiaoLing
name: Zhang, XueHong
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Table S1. Measurements of variables.
Baryon - Antibaryon Production by Disordered Chiral Condensates
Creators: name: Kapusta, Joseph I.
name: Srivastava, Ajit M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We investigate the production of baryons and antibaryons in the central rapidity region of high energy nuclear collisions within the framework of the Skyrme model taking into account the effects of explicit chiral symmetry breaking. We argue that the formation of disordered chiral condensates may lead to enhanced baryon-antibaryon production at low transverse momentum.
description: 13 pages (LATEX), 2 figures in postscript (uuencoded, compressed tar file included at the end of the paper), NSF-ITP-94-40, NUC-MINN-94/4-T
The dual role of starburst and active galactic nuclei in driving extreme molecular outflows
Creators: name: Gowardhan, Avani
name: Spoon, Henrik
name: Riechers, Dominik A.
name: González-Alfonso, Eduardo
name: Farrah, Duncan
name: Fischer, Jacqueline
name: Darling, Jeremy
name: Fergulio, Chiara
name: Afonso, Jose
name: Bizzocchi, Luca
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report molecular gas observations of IRAS 20100-4156 and IRAS 03158+4227, two local ultraluminous infrared galaxies (ULIRGs) hosting some of the fastest and most massive molecular outflows known. Using ALMA and PdBI observations, we spatially resolve the CO(1-0) emission from the outflowing molecular gas in both and find maximum outflow velocities of $ v_{\rm max} \sim 1600$ and $\sim 1700$ km/s for IRAS 20100-4156 and IRAS 03158+4227, respectively. We find total gas mass outflow rates of $\dot M_{\rm OF} \sim 670$ and $\sim 350$ Msun/yr, respectively, corresponding to molecular gas depletion timescales $τ^{\rm dep}_{\rm OF} \sim 11$ and $\sim 16$ Myr. This is nearly 3 times shorter than the depletion timescales implied by star formation, $τ^{\rm dep}_{\rm SFR} \sim 33$ and $\sim 46$ Myr, respectively. To determine the outflow driving mechanism, we compare the starburst ($L_{*}$) and AGN ($L_{\rm AGN}$) luminosities to the outflowing energy and momentum fluxes, using mid-infrared spectral decomposition to discern $L_{\rm AGN}$. Comparison to other molecular outflows in ULIRGs reveals that outflow properties correlate similarly with $L_{*}$ and $L_{\rm IR}$ as with $L_{\rm AGN}$, indicating that AGN luminosity alone may not be a good tracer of feedback strength and that a combination of AGN and starburst activity may be driving the most powerful molecular outflows. We also detect the OH 1.667 GHz maser line from both sources and demonstrate its utility in detecting molecular outflows.
description: 29 pages, 17 figures, 6 tables, accepted to ApJ
Murex senticosus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Muricidae
Murex
Murex senticosus

description: Murex senticosus [spec. nov.]
M. testa subturrita longitudinaliter costata transversim cancellata, apertura striata.
Bonan. recr. 3. t. 35.
Gvalt. test. t. 51. f. G.
Argenv. conch. t. 12. f. O.
Habitat ..
*? * Bullacei: testa diaphana.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on pages 751-752, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Effects of a Neonicotinoid Insecticide and Population Density on Behaviour and Development of Wood Frogs (Lithobates sylvaticus)
Creators: name: Bouffard, Jeremie
Publisher: name: Université d'Ottawa / University of Ottawa
Year: 2021
Subjects: Amphibians
Imidacloprid
Personality
Development
Metamorphosis
Behaviours
Density
Ecotoxicology
Predation cues
Neonicotinoids

description: Amphibians have been facing global declines over the last decades due to direct and indirect effects of anthropogenic activities. One of the leading causes is environmental contamination, particularly that of waterbodies which are used by many amphibian species for reproduction, development, and adult life. An important source of contamination comes from agricultural runoffs of pesticides such as neonicotinoids, which are known to alter anuran survival, behaviour, predation stress response, and development. However, few studies have investigated the possible interactions between neonicotinoids and natural environmental stressors which could alter the strength and direction of observed neonicotinoid effects. This study investigated how a concentration of imidacloprid (a neonicotinoid) measured in surface waters interacted with high population density, an important environmental stressor, to influence behaviour and development across metamorphosis in wood frogs (Lithobates sylvaticus) known to breed in agricultural landscapes. I reared tadpoles in a fully crossed design experiment, between two densities (0.33 and 1 tadpole/L) and clean vs contaminated water (10 µg/L imidacloprid). Behaviours were measured in the absence and presence of predation cues using open-field tests at three distinct developmental stages, up to the metamorph stage. I found that imidacloprid did not interact with population density or independently affect behaviours in the absence of predation cues. However, individuals raised at high density compared with low density were more active at an early developmental stage but less active at metamorphic climax. Furthermore, both density and imidacloprid independently decreased the natural behavioural response (i.e., “freezing”) of tadpoles to predation cues. Both treatments also slightly accelerated metamorphosis while only density altered final mass at metamorphosis. Finally, I found that distance travelled was weakly repeatable between aquatic stages but not repeatable across metamorphosis, a pattern that was not affected by treatments. This study provides novel insights on the ecotoxicology of imidacloprid in the presence of a natural stressor, highlighting the importance of including behavioural assays and stressors in studies of amphibian ecotoxicology.
Scientific discourse on YouTube: Motivations for citing research in comments
Creators: name: Striewski, Sören
name: Zagovora, Olga
name: Peters, Isabella
Publisher: name: arXiv
Year: 2024
Subjects: subject: Computers and Society (cs.CY)
subject: Digital Libraries (cs.DL)
subject: FOS: Computer and information sciences

description: YouTube is a valuable source of user-generated content on a wide range of topics, and it encourages user participation through the use of a comment system. Video content is increasingly addressing scientific topics, and there is evidence that both academics and consumers use video descriptions and video comments to refer to academic research and scientific publications. Because commenting is a discursive behavior, this study will provide insights on why individuals post links to research publications in comments. For this, a qualitative content analysis and iterative coding approach were applied. Furthermore, the reasons for mentioning academic publications in comments were contrasted with the reasons for citing in scholarly works and with reasons for commenting on YouTube. We discovered that the primary motives for sharing research links were (1) providing more insights into the topic and (2) challenging information offered by other commentators.
description: Accepted at the Association for Information Science and Technology
The dependence of convective core overshooting on stellar mass: Additional binary systems and improved calibration
Creators: name: Claret, Antonio
name: Torres, Guillermo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Many current stellar evolution models assume some dependence of the strength of convective core overshooting on mass for stars more massive than 1.1-1.2 solar masses, but the adopted shapes for that relation have remained somewhat arbitrary for lack of strong observational constraints. In previous work we compared stellar evolution models to well-measured eclipsing binaries to show that, when overshooting is implemented as a diffusive process, the fitted free parameter f(ov) rises sharply up to about 2 solar masses, and remains largely constant thereafter. Here we analyze a new sample of eight binaries selected to be in the critical mass range below 2 solar masses where f(ov) is changing the most, nearly doubling the number of individual stars in this regime. This interval is important because the precise way in which f(ov) changes determines the shape of isochrones in the turnoff region of 1-5 Gyr clusters, and can thus affect their inferred ages. It also has a significant influence on estimates of stellar properties for exoplanet hosts, on stellar population synthesis, and on the detailed modeling of interior stellar structures, including the calculation of oscillation frequencies that are observable with asteroseismic techniques. We find that the derived f(ov) values for our new sample are consistent with the trend defined by our earlier determinations, and strengthen the relation. This provides an opportunity for future series of models to test the new prescription, grounded on observations, against independent observations that may constrain overshooting in a different way.
description: 8 pages in emulateapj format, including figures and tables. Accepted for publication in The Astrophysical Journal
Multiple Scattering in Clumpy Media. II. Galactic Environments
Creators: name: Witt, Adolf N.
name: Gordon, Karl D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present and discuss the results of new multiple-scattering radiative transfer calculations for three representative types of galactic environments, filled with either homogeneous or two-phase clumpy dust distributions. Extinction and scattering properties for two types of interstellar dust, similar to those found in the average diffuse medium of the Milky Way Galaxy (MW) and the Bar of the Small Magellanic Cloud (SMC), are considered. The wavelength coverage extends from 1000 A to 30,000 A, with particular emphasis on the rest-frame UV. This makes these models especially applicable to starburst galaxies and Lyman-break galaxy samples. The examination of the models concentrates on the study of UV/visual/near-IR reddening effects, the wavelength dependence of attenuation, and on the changes that arise from the transition from homogeneous to clumpy dust distributions in different star/dust geometries. Embedded dust, especially when clumpy, leads to saturation at fairly low reddening values with correspondingly gray attenuation functions. This makes the assessment of the attenuation of the far-UV flux from starburst galaxies difficult, if only UV/visual/near-IR data are available. Existing data for UV-selected starburst galaxies indicate a range of UV attenuation factors of 0-150. Our models reproduce the "Calzetti Attenuation Law", provided one adopts SMC-type dust and a clumpy shell-type dust distribution surrounding the starbursts. The average far-UV attenuation factor for the Calzetti sample is found to be 7.4. The only relatively reliable measure for the UV attenuation factor for single galaxies was found in the ratio of the integrated far-IR flux to the far-UV flux, measured near 1600 A, requiring the measurement of the entire spectral energy distribution of galaxies.
description: accepted by the ApJ (10 Dec 1999), 17 pages, color figures included, paper and data tables also at http://mips.as.arizona.edu/~kgordon/papers/clumpy_dust_II.html
Cryogenic Trapped-Ion System for Large Scale Quantum Simulation
Creators: name: Pagano, G.
name: Hess, P. W.
name: Kaplan, H. B.
name: Tan, W. L.
name: Richerme, P.
name: Becker, P.
name: Kyprianidis, A.
name: Zhang, J.
name: Birckelbaw, E.
name: Hernandez, M. R.
name: Wu, Y.
name: Monroe, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We present a cryogenic ion trapping system designed for large scale quantum simulation of spin models. Our apparatus is based on a segmented-blade ion trap enclosed in a 4 K cryostat, which enables us to routinely trap over 100 $^{171}$Yb$^+$ ions in a linear configuration for hours due to a low background gas pressure from differential cryo-pumping. We characterize the cryogenic vacuum by using trapped ion crystals as a pressure gauge, measuring both inelastic and elastic collision rates with the molecular background gas. We demonstrate nearly equidistant ion spacing for chains of up to 44 ions using anharmonic axial potentials. This reliable production and lifetime enhancement of large linear ion chains will enable quantum simulation of spin models that are intractable with classical computer modelling.
description: 16 pages, 11 figures
Supplementary information from Milling as a route to porous graphitic carbons from biomass
Creators: name: Hunter, R. D.
name: Davies, J.
name: Hérou, S. J. A.
name: Kulak, A.
name: Schnepp, Z.
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: 30203 Inorganic Green Chemistry
subject: FOS: Chemical sciences
subject: 30399 Macromolecular and Materials Chemistry not elsewhere classified
subject: 30504 Organic Green Chemistry

description: Document containing supplementary figures including Raman spectroscopy and adsorption data
Predicting Software Defects through SVM: An Empirical Approach
Creators: name: Reshi, Junaid Ali
name: Singh, Satwinder
Publisher: name: arXiv
Year: 2018
Subjects: subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: Software defect prediction is an important aspect of preventive maintenance of a software. Many techniques have been employed to improve software quality through defect prediction. This paper introduces an approach of defect prediction through a machine learning algorithm, support vector machines (SVM), by using the code smells as the factor. Smell prediction model based on support vector machines was used to predict defects in the subsequent releases of the eclipse software. The results signify the role of smells in predicting the defects of a software. The results can further be used as a baseline to investigate further the role of smells in predicting defects.
Direct evidence of AGN-feedback: a post starburst galaxy stripped of its gas by AGN-driven winds
Creators: name: Baron, Dalya
name: Netzer, Hagai
name: Prochaska, J. Xavier
name: Cai, Zheng
name: Cantalupo, Sebastiano
name: Martin, D. Christopher
name: Matuszewski, Mateusz
name: Moore, Anna M.
name: Morrissey, Patrick
name: Neill, James D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Post starburst E+A galaxies show indications of a powerful starburst that was quenched abruptly. Their disturbed, bulge-dominated morphologies suggest that they are merger remnants. The more massive E+A galaxies are suggested to be quenched by AGN feedback, yet little is known about AGN-driven winds in this short-lived phase. We present spatially-resolved IFU spectroscopy by the Keck Cosmic Web Imager of SDSS J003443.68+251020.9, at z=0.118. The system consists of two galaxies, the larger of which is a post starburst E+A galaxy hosting an AGN. Our modelling suggests a 400 Myrs starburst, with a peak star formation rate of 120 Msun/yr. The observations reveal stationary and outflowing gas, photoionized by the central AGN. We detect gas outflows to a distance of 17 kpc from the central galaxy, far beyond the region of the stars (about 3 kpc), inside a conic structure with an opening angle of 70 degrees. We construct self-consistent photoionization and dynamical models for the different gas components and show that the gas outside the galaxy forms a continuous flow, with a mass outflow rate of about 24 Msun/yr. The gas mass in the flow, roughly $10^9$ Msun, is larger than the total gas mass within the galaxy, some of which is outflowing too. The continuity of the flow puts a lower limit of 60 Myrs on the duration of the AGN feedback. Such AGN are capable of removing, in a single episode, most of the gas from their host galaxies and expelling enriched material into the surrounding CGM.
description: submitted to MNRAS; comments are welcome!
Nonequilibrium Quantum Dynamics Of Disoriented Chiral Condensates
Creators: name: Cooper, Fred
name: Kluger, Yuval
name: Mottola, Emil
name: Paz, Juan Pablo
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The nonequilibrium dynamics of the chiral phase transition expected during the expansion of the quark-qluon plasma produced in a high energy hadron or heavy ion collision is studied in the O(4) linear sigma model to leading order in a large $N$ expansion. Starting from an approximate equilibrium configuration at an initial proper time $τ$ in the disordered phase we study the transition to the ordered broken symmetry phase as the system expands and cools. We give results for the proper time evolution of the effective pion mass, the order parameter $$ as well as for the pion two point correlation function expressed in terms of a time dependent phase space number density and pair correlation density. We determine the phase space of initial conditions that lead to instabilities (exponentially growing long wave length modes) as the system evolves in time. These instabilities are what eventually lead to disoriented chiral condensates. In our simulations,we found that instabilities that are formed during the initial phases of the expansion exist for proper times that are at most $3 fm/c$ and lead to condensate regions that do not contain large numbers of particles. The damping of instabilities is a consequence of strong coupling.
description: 49 pages, figures available by request
Deep HST/UVIS imaging of the candidate dark galaxy CDG-1
Creators: name: van Dokkum, Pieter
name: Li, Dayi David
name: Abraham, Roberto
name: Danieli, Shany
name: Eadie, Gwendolyn M.
name: Harris, William E.
name: Romanowsky, Aaron J.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: CDG-1 is a tight grouping of four likely globular clusters in the Perseus cluster, and a candidate dark galaxy with little or no diffuse light. Here we provide new constraints on the luminosity of any underlying stellar emission, using HST/UVIS F200LP imaging. No diffuse emission is detected, with a 2$σ$ upper limit of F200LP>28.1 mag/arcsec$^2$ on the 5'' scale of CDG-1. This surface brightness limit corresponds to a 2$σ$ lower limit of >0.5 for the fraction of the total luminosity that is in the form of globular clusters. The most likely alternative, although improbable, is that CDG-1 is a chance grouping of four globular clusters in the halo of the Perseus galaxy IC312.
description: To appear in Research Notes of the American Astronomical Society
Murex ficus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Muricidae
Murex
Murex ficus

description: Murex ficus [spec. nov.]
M. testa obovato-clavata reticulato-striata subdiaphana, cauda patula exserta, spira oblitterata.
List. conch. 4. s. 10. c. 8. t. 2. f. 3.
Bonan. recr. 3. t. 15.
Rumph. mus. t. 27. f. K.
Petiv. amboin. t. 6. f. 9.
Gvalt. test. t. 26. f. I, M.
Argenv. conch. t. 20. f. O.
Klein. ostr. t. 5. f. 93.
Habitat ..
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 752, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Doubly-charged scalar in rare decays of $B_c$ meson
Creators: name: Wang, Tianhong
name: Jiang, Yue
name: Wang, Zhi-Hui
name: Wang, Guo-Li
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this paper, we study the lepton number violation processes of $B_c$ meson induced by possible doubly-charged scalars. Both the three-body decay channels and the four-body decay channels are considered. For the former, $Br\times\left(\frac{s_Δh_{ij}}{M_Δ^2}\right)^{-2}$ is of the order of $10^{-7}\sim 10^{-9}$, and for the later channels, $Br\times\left(\frac{s_Δh_{ij}}{M_Δ^2}\right)^{-2}$ is of the order of $10^{-12}\sim 10^{-20}$, where $s_Δ$, $h_{ij}$, $M_Δ$ are the constants related to the doubly-charged boson.
description: 15 pages, 2 figures
Additional file 6 of Epitranscriptomic analysis reveals clinical and molecular signatures in glioblastoma
Creators: name: de Mendonça Fernandes, Glaucia Maria
name: Wang, Wesley
name: Ahmadian, Saman Seyed
name: Jones, Daniel
name: Peng, Jing
name: Giglio, Pierre
name: Venere, Monica
name: Otero, José Javier
Publisher: name: figshare
Year: 2025
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Supplementary Material 6
Coulomb branches with complex singularities
Creators: name: Argyres, Philip C.
name: Martone, Mario
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We construct 4d superconformal field theories (SCFTs) whose Coulomb branches have singular complex structures. This implies, in particular, that their Coulomb branch coordinate rings are not freely generated. Our construction also gives examples of distinct SCFTs which have identical moduli space (Coulomb, Higgs, and mixed branch) geometries. These SCFTs thus provide an interesting arena in which to test the relationship between moduli space geometries and conformal field theory data. We construct these SCFTs by gauging certain discrete global symmetries of $\mathcal N=4$ superYang-Mills (sYM) theories. In the simplest cases, these discrete symmetries are outer automorphisms of the sYM gauge group, and so these theories have lagrangian descriptions as $\mathcal N=4$ sYM theories with disconnected gauge groups.
description: 43 pages
Constraints on Type Ia Supernova Models from X-ray Spectra of Galaxy Clusters
Creators: name: Dupke, Renato A.
name: White, Raymond E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present constraints on theoretical models of Type Ia supernovae using spatially resolved ASCA X-ray spectroscopy of three galaxy clusters: Abell 496, Abell 2199 and Abell 3571. All three clusters have central iron abundance enhancements; an ensemble of abundance ratios are used to show that most of the iron in the central regions of the clusters comes from SN Ia. These observations are consistent with the suppressed galactic wind scenario proposed by Dupke and White (1999). At the center of each cluster, simultaneous analysis of spectra from all ASCA instruments shows that the nickel to iron abundance ratio (normalized by the solar ratio) is Ni/Fe ~ 4. We use the nickel to iron ratio as a discriminator between SN Ia explosion models: the Ni/Fe ratio of ejecta from the "Convective Deflagration" model W7 is consistent with the observations, while those of "delayed detonation" models are not consistent at the 90% confidence level.
description: 20 pages, 2 figures, accepted by The Astrophysical Journal
Additional file 1: of OPTimal IMAging strategy in patients suspected of non-traumatic pulmonary disease at the emergency department: chest X-ray or ultra-low-dose CT (OPTIMACT)â a randomised controlled trial chest X-ray or ultra-low-dose CT at the ED: design and rationale
Creators: name: Berk, Inge Van Den
name: Maadrika Kanglie
name: Engelen, Tjitske Van
name: Shandra Bipat
name: Dijkgraaf, Marcel
name: Bossuyt, Patrick
name: MonyĂŠ, Wouter De
name: Prins, Jan
name: Stoker, Jaap
Publisher: name: figshare
Year: 2018
Subjects: Medicine
Cell Biology
Cancer
Science Policy

description: Appendix 1. SPIRIT OPTIMACT checklist. (PDF 56Â kb)
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Cart. 192 (11 H 77), 295 folios, f. 0015v
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0015v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0015v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Gravitational instability of a dust layer composed of porous silicate dust aggregates in a protoplanetary disk
Creators: name: Tatsuuma, Misako
name: Michikoshi, Shugo
name: Kokubo, Eiichiro
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Planetesimal formation is one of the most important unsolved problems in planet formation theory. In particular, rocky planetesimal formation is difficult because silicate dust grains are easily broken when they collide. Recently, it has been proposed that they can grow as porous aggregates when their monomer radius is smaller than $\sim$ 10 nm, which can also avoid the radial drift toward the central star. However, the stability of a layer composed of such porous silicate dust aggregates has not been investigated. Therefore, we investigate the gravitational instability of this dust layer. To evaluate the disk stability, we calculate Toomre's stability parameter $Q$, for which we need to evaluate the equilibrium random velocity of dust aggregates. We calculate the equilibrium random velocity considering gravitational scattering and collisions between dust aggregates, drag by mean flow of gas, stirring by gas turbulence, and gravitational scattering by gas density fluctuation due to turbulence. We derive the condition of the gravitational instability using the disk mass, dust-to-gas ratio, turbulent strength, orbital radius, and dust monomer radius. We find that, for the minimum mass solar nebula model at 1 au, the dust layer becomes gravitationally unstable when the turbulent strength $α\lesssim10^{-5}$. If the dust-to-gas ratio is increased twice, the gravitational instability occurs for $α\lesssim10^{-4}$. We also find that the dust layer is more unstable in disks with larger mass, higher dust-to-gas ratio, and weaker turbulent strength, at larger orbital radius, and with a larger monomer radius.
description: 17 pages, 11 figures, accepted for publication in ApJ
A Comprehensive K2 and Ground-Based Study of CRTS J035905.9+175034, an Eclipsing SU UMa System with a Large Mass Ratio
Creators: name: Littlefield, Colin
name: Garnavich, Peter
name: Kennedy, Mark
name: Szkody, Paula
name: Dai, Zhibin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: CRTS J035905.9+175034 is the first eclipsing SU UMa system for which a superoutburst has been observed by Kepler in the short-cadence mode. The light curve contains one superoutburst, eight normal outbursts (including a precursor to the superoutburst), and several minioutbursts that are present before -- but not after -- the superoutburst. The superoutburst began with a precursor normal outburst, and shortly after the peak of the precursor, the system developed large-amplitude superhumps that achieved their maximum amplitude after just three superhump cycles. The period excess of the initial superhump period relative to the orbital period implies a mass ratio of 0.281 +/- 0.015, placing it marginally above most theoretical predictions of the highest-possible mass ratio for superhump formation. In addition, our analysis of the variations in eclipse width and depth, as well as the hot spot amplitudes, generally provides substantiation of the thermal-tidal instability model. The K2 data, in conjunction with our ground-based time-resolved spectroscopy and photometry from 2014-2016, allows us to determine many of the fundamental parameters of this system.
description: accepted for publication, AJ