cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1: of Associations between birth registration and early child growth and development: evidence from 31 low- and middle-income countries
Creators: name: Jeong, Joshua
name: Bhatia, Amiya
name: Fink, Günther
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Country mean values for proportion of children not having a birth certificate, children’s HAZ, WAZ, WHZ, and ECDI z-score values among children aged 0–59 months. (DOCX 96 kb)
Spanning Trees and bootstrap reliability estimation in correlation based networks
Creators: name: Tumminello, M.
name: Coronnello, C.
name: Lillo, F.
name: Micciche', S.
name: Mantegna, R. N.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: We introduce a new technique to associate a spanning tree to the average linkage cluster analysis. We term this tree as the Average Linkage Minimum Spanning Tree. We also introduce a technique to associate a value of reliability to links of correlation based graphs by using bootstrap replicas of data. Both techniques are applied to the portfolio of the 300 most capitalized stocks traded at New York Stock Exchange during the time period 2001-2003. We show that the Average Linkage Minimum Spanning Tree recognizes economic sectors and sub-sectors as communities in the network slightly better than the Minimum Spanning Tree does. We also show that the average reliability of links in the Minimum Spanning Tree is slightly greater than the average reliability of links in the Average Linkage Minimum Spanning Tree.
description: 17 pages, 3 figures
A Comprehensive Renormalisation Group Analysis of the Littlest Seesaw Model
Creators: name: Geib, Tanja
name: King, Stephen F.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present a comprehensive renormalisation group analysis of the Littlest Seesaw model involving two right-handed neutrinos and a very constrained Dirac neutrino Yukawa coupling matrix. We perform the first $χ^2$ analysis of the low energy masses and mixing angles, in the presence of renormalisation group corrections, for various right-handed neutrino masses and mass orderings, both with and without supersymmetry. We find that the atmospheric angle, which is predicted to be near maximal in the absence of renormalisation group corrections, may receive significant corrections for some non-supersymmetric cases, bringing it into close agreement with the current best fit value in the first octant. By contrast, in the presence of supersymmetry, the renormalisation group corrections are relatively small, and the prediction of a near maximal atmospheric mixing angle is maintained, for the studied cases. Forthcoming results from T2K and NOvA will decisively test these models at a precision comparable to the renormalisation group corrections we have calculated.
description: 48 pages, 8 figures
Restoration of the Tully-Fisher Relation by Statistical Rectification
Creators: name: Fu, Hai
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: I employ the Lucy rectification algorithm to recover the inclination-corrected distribution of local disk galaxies in the plane of absolute magnitude ($M_i$) and HI velocity width ($W_{20}$). By considering the inclination angle as a random variable with a known probability distribution, the novel approach eliminates one major source of uncertainty in studies of the Tully-Fisher relation: inclination angle estimation from axial ratio. Leveraging the statistical strength derived from the entire sample of 28,264 HI-selected disk galaxies at $z < 0.06$ from the Arecibo Legacy Fast ALFA (ALFALFA) survey, I show that the restored distribution follows a sharp correlation that is approximately a power law between $-16 > M_i > -22$: $M_i = M_0 - 2.5β\ [\log(W_{\rm 20}/250 {\rm km/s})]$, with $M_0 = -19.77\pm0.04$ and $β= 4.39\pm0.06$. At the brighter end ($M_i < -22$), the slope of the correlation decreases to $β\approx 3.3$, confirming previous results. Because the method accounts for measurement errors, the intrinsic dispersion of the correlation is directly measured: $σ(\log W_{20}) \approx 0.06$ dex between $-17 > M_i > -23$, while $σ(M_i)$ decreases from $\sim$0.8 in slow rotators to $\sim$0.4 in fast rotators. The statistical rectification method holds significant potential, especially in the studies of intermediate-to-high-redshift samples, where limited spatial resolution hinders precise measurements of inclination angles.
description: ApJ Letters accepted. Python notebook and data files are available at https://github.com/fuhaiastro/TFR_Lucy
A study of turbulence and interacting inertial modes in a differentially-rotating spherical shell experiment
Creators: name: Hoff, Michael
name: Harlander, Uwe
name: Triana, Santiago A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: We present a study of inertial modes in a differentially rotating spherical shell (spherical Couette flow) experiment with a radius ratio of $η= 1/3$. Inertial modes are Coriolis-restored linear wave modes which often arise in rapidly rotating fluids. Recent experimental work has shown that inertial modes exist in a spherical Couette flow for $Ω_{i}
Parameter information from nonlinear cosmological fields
Creators: name: Taylor, Andy
name: Watts, Peter
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We develop a general formalism for analysing parameter information from non-Gaussian cosmic fields. The method can be adapted to include the nonlinear effects in galaxy redshift surveys, weak lensing surveys and cosmic velocity field surveys as part of parameter estimation. It can also be used as a test of non-Gaussianity of the Cosmic Microwave Background. Generalising Maximum Likelihood analysis to second-order, we calculate the nonlinear Fisher Information matrix and likelihood surfaces in parameter space. To this order we find that the information content is always increased by including nonlinearity. Our methods are applied to a realistic model of a galaxy redshift survey, including nonlinear evolution, galaxy bias, shot-noise and redshift-space distortions to second-order. We find that including nonlinearities allows all of the degeneracies between parameters to be lifted. Marginalised parameter uncertainties of a few percent will then be obtainable using forthcoming galaxy redshift surveys.
description: 14 pages, 7 figures. Submitted to MNRAS
Profiling Strategies for Accelerating Neural Network Training on HPC GPU Clusters
Creators: name: Cairncross, Oliver
Publisher: name: Zenodo
Year: 2023

description: When dealing with large datasets, it is important to train machine learning (ML) models quickly and efficiently and profiling is a critical step to achieve this. Running ML code on large HPC clusters is a convenient way to tackle large ML tasks. Nevertheless, we often find that performance is still too slow to be practical. The goal profiling is to identify and resolve bottlenecks in data pipelines, memory utilization, and CPU/GPU usage and optimise performance. our case we focus on training neural networks with large image datasets.

To illustrate the concepts to be discussed, a generic case study will be presented. The study involves training a deep neural network architecture on a large-scale image dataset using a multi-GPU CUDA cluster with a high-performance file system and interconnect. The TensorFlow machine learning framework is employed.

Various tools used for profiling include:
  - system performance tools;
  - machine learning framework profilers;
  - GPU vendor-provided profilers; and
  - specialized profilers supporting multi-GPU frameworks.

Different combinations of these tools are required to address various scenarios. Therefore, how and when they are used is critical to identify, understand, and potentially address performance bottlenecks. Although this presentation focuses on training neural networks, some of concepts (such as data pipelines) can be applied to other tasks.
Potential output purity of completely positive maps
Creators: name: King, Christopher
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The notion of potential output purity of a completely positive map is introduced as a generalization of the regularized output purity. An upper bound is derived for this quantity, and for several classes of maps (including CQ, QC and Hadamard channels) it is shown that potential purity does not exceed the standard output purity. As an application the potential purity is used to bound the logarithmic Sobolev constant of a product of depolarizing channel semigroups.
description: 18 pages
Realization of a classical counterpart of a scalable design for adiabatic quantum computation
Creators: name: Zakosarenko, V.
name: Bondarenko, N.
name: van der Ploeg, S. H. W.
name: Izmalkov, A.
name: Linzen, S.
name: Kunert, J.
name: Grajcar, M.
name: Il'ichev, E.
name: Meyer, H. -G.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We implement a classical counterpart of a scalable design for adiabatic quantum computation. The key element of this design is a coupler providing controllable coupling between two bistable elements (in our case superconducting rings with a single Josephson junction playing the role of a classical counterpart of superconducting flux qubits) The coupler is also a superconducting ring with a single Josephson junction that operates in the non-hysteretic mode. The flux coupling between two bistable rings can be controlled by changing the magnetic flux through the coupler. Thereby, the coupling can be tuned from ferromagnetic trough zero to to anti-ferromagnetic.
description: 3 pages, 3 figures v2: extended discussion experimental results
Gauge fixing and abelianization in simple BRST quantization
Creators: name: Marnelius, Robert
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In a previous paper \cite{Simple} it was shown that the BRST charge $Q$ for any gauge model with a Lie algebra symmetry may be decomposed as $Q=\del+\del^†,\;\;\;\del^2=\del^{†2}=0,\;\;\;[\del, \del^†]_+=0$ provided dynamical Lagrange multipliers are used but without introducing other matter variables in $\del$ than the gauge generators in $Q$. In this paper further decompositions are derived but now by means of gauge fixing operators. As in \cite{Simple} it is shown that $\del=c^{†a}ϕ_a$ where $c^a$ are new ghosts and $ϕ_a$ are nonhermitian variables satisfying the gauge algebra. However, in distinction to \cite{Simple} also solutions of the form $\del=c^{†a}A_a$ where $A_a$ satisfy an abelian algebra is derived (abelianization). By means of a bigrading the BRST condition reduces to $\del|ph\hb=\del^†|ph\hb=0$ on inner product spaces whose general solutions are expressed in terms of the solutions to a proper Dirac quantization. Thus, the procedure provides for inner products for the solutions of a Dirac quantization.
description: 20, G\"{o}teborg ITP 93-17, latexfile
Unveiling a Novel Metal-to-Metal Transition in LuH2: Critically Challenging Superconductivity Claims in Lutetium Hydrides
Creators: name: Wang, Dong
name: Wang, Ningning
name: Zhang, Caoshun
name: Xia, Chunsheng
name: Guo, Weicheng
name: Yin, Xia
name: Bu, Kejun
name: Nakagawa, Takeshi
name: Zhang, Jianbo
name: Gorelli, Federico
name: Dalladay-Simpson, Philip
name: Meier, Thomas
name: Lü, Xujie
name: Sun, Liling
name: Cheng, Jinguang
name: Zeng, Qiaoshi
name: Ding, Yang
name: Mao, Ho-kwang
Publisher: name: arXiv
Year: 2024
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Following the recent report by Dasenbrock-Gammon et al. (2023) of near-ambient superconductivity in nitrogen-doped lutetium trihydride (LuH3-δNε), significant debate has emerged surrounding the composition and interpretation of the observed sharp resistance drop. Here, we meticulously revisit these claims through comprehensive characterization and investigations. We definitively identify the reported material as lutetium dihydride (LuH2), resolving the ambiguity surrounding its composition. Under similar conditions (270-295 K and 1-2 GPa), we replicate the reported sharp decrease in electrical resistance with a 30% success rate, aligning with Dasenbrock-Gammon et al.'s observations. However, our extensive investigations reveal this phenomenon to be a novel, pressure-induced metal-to-metal transition intrinsic to LuH2, distinct from superconductivity. Intriguingly, nitrogen doping exerts minimal impact on this transition. Our work not only elucidates the fundamental properties of LuH2 and LuH3 but also critically challenges the notion of superconductivity in these lutetium hydride systems. These findings pave the way for future research on lutetium hydride systems while emphasizing the crucial importance of rigorous verification in claims of ambient temperature superconductivity.
TeV Gamma-Ray Absorption and the Intergalactic Infrared Background
Creators: name: Stecker, F. W.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper, I will take a synoptic approach to determining the intergalactic infrared radiation field (IIRF). This approach draws on both the multi-TeV gamma-ray observations and the infrared background observations and relates them via the semi-empirical modelling method of Malkan and Stecker. I discuss the evidence for an intergalactic infrared background obtained by an analysis of the HEGRA observations of the high energy gamma-ray spectrum of Mrk 501 and from constraints from Mrk 421 deduced from the Whipple air Cherenkov telescope results. I will show that this evidence is in accord with the predictions made by Malkan and Stecker for the intergalactic infrared spectral energy distribution produced by galaxies. The Malkan-Stecker predictions are also in excellent agreement with mid- and far infrared galaxy counts. However, there may be potential problems relating these predictions with the results of the analysis of COBE-DIRBE far infrared data. The gamma-ray and COBE-DIRBE observations may also need to be reconciled. I will discuss possible ways to resolve this situation including a partial nullification of the $γ$-ray absorption process which can hypothetically occur if Lorentz invariance is broken.
description: 15 latex pages with 5 eps figures and newpasp style file included, Invited Paper for Proc. IAU Symp. 204 "The Extragalactic Background and its Cosmological Implications", M. Harwit and M.G. Hauser, eds., Corrected FIG. 1
The future of digital research infrastructure
Creators: name: Hicks, Rosie
Publisher: name: Zenodo
Year: 2023

description: Over the last decade, eResearch has changed from being at the frontier to an underpinning capability required for all research. As digital research infrastructure matures and evolves, we must optimise the delivery of digital services to researchers, reduce duplication of effort across institutions and research domains, and build enduring capability for the research community.

The ARDC has responded to this challenge by creating Thematic Research Data Commons. Our vision is for world leading knowledge infrastructure that enables Australian researchers to transform our lives. We are committed to delivering enduring digital research infrastructure that will support researchers to tackle the grand challenges facing our society.

Over the past 12 months, we've undertaken extensive nation-wide consultations to gain a deep understanding of the research community's needs. This presentation will describe the data challenges identified and set out the initial program of work for our first three Research Data Commons: People RDC for health and medical research, Planet RDC for earth and environmental sciences, and HASS and Indigenous RDC for humanities, arts, social sciences and Indigenous research.

To deliver on this transformative strategy, the ARDC has also undergone an organisational restructure to  ensure our world-class team is best positioned to work across boundaries to deliver a seamless experience for researchers. The presentation will include an introduction to the new Team ARDC who are committed to enhancing our national digital research infrastructure for the betterment of research and innovation.
Excitations with fractional spin less than 1/2 in frustrated magnetoelastic chains
Creators: name: Gazza, C. J.
name: Dobry, A. O.
name: Cabra, D. C.
name: Vekua, T.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We study the magnetic excitations on top of the plateaux states recently discovered in spin-Peierls systems in a magnetic field. We show by means of extensive density matrix renormalization group (DMRG) computations and an analytic approach that one single spin-flip on top of $M=1-\frac2N$ ($N=3,4,...$) plateau decays into $N$ elementary excitations each carrying a fraction $\frac1N$ of the spin. This fractionalization goes beyond the well-known decay of one magnon into two spinons taking place on top of the M=0 plateau. Concentrating on the $\frac13$ plateau (N=3) we unravel the microscopic structure of the domain walls which carry fractional spin-$\frac13$, both from theory and numerics. These excitations are shown to be noninteracting and should be observable in x-ray and nuclear magnetic resonance experiments.
description: 6 pages, 5 figures. Accepted to be published in Phys. Rev. B
Effects of Nongauge Potentials on the Spin-1/2 Aharonov-Bohm Problem
Creators: name: Hagen, C. R.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Some recent work has attempted to show that the singular solutions which are known to occur in the Dirac description of spin-1/2 Aharonov-Bohm scattering can be eliminated by the inclusion of strongly repulsive potentials inside the flux tube. It is shown here that these calculations are generally unreliable since they necessarily require potentials which lead to the occurrence of Klein's paradox. To avoid that difficulty the problem is solved within the framework of the Galilean spin-1/2 wave equation which is free of that particular complication. It is then found that the singular solutions can be eliminated provided that the nongauge potential is made energy dependent. The effect of the inclusion of a Coulomb potential is also considered with the result being that the range of flux parameter for which singular solutions are allowed is only half as great as in the pure Aharonov-Bohm limit. Expressions are also obtained for the binding energies which can occur in the combined Aharonov-Bohm-Coulomb system.
description: (Minor corrections plus additions described in last sentence of abstract), 13 pages, UR-1317, ER-767-40685
AccessLens: Auto-detecting Inaccessibility of Everyday Objects
Creators: name: Kwon, Nahyun
name: Lu, Qian
name: Qazi, Muhammad Hasham
name: Liu, Joanne
name: Oh, Changhoon
name: Kong, Shu
name: Kim, Jeeeun
Publisher: name: arXiv
Year: 2024
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: In our increasingly diverse society, everyday physical interfaces often present barriers, impacting individuals across various contexts. This oversight, from small cabinet knobs to identical wall switches that can pose different contextual challenges, highlights an imperative need for solutions. Leveraging low-cost 3D-printed augmentations such as knob magnifiers and tactile labels seems promising, yet the process of discovering unrecognized barriers remains challenging because disability is context-dependent. We introduce AccessLens, an end-to-end system designed to identify inaccessible interfaces in daily objects, and recommend 3D-printable augmentations for accessibility enhancement. Our approach involves training a detector using the novel AccessDB dataset designed to automatically recognize 21 distinct Inaccessibility Classes (e.g., bar-small and round-rotate) within 6 common object categories (e.g., handle and knob). AccessMeta serves as a robust way to build a comprehensive dictionary linking these accessibility classes to open-source 3D augmentation designs. Experiments demonstrate our detector's performance in detecting inaccessible objects.
description: CHI2024
Role of Planetary Radius on Atmospheric Escape of Rocky Exoplanets
Creators: name: Chin, Laura
name: Dong, Chuanfei
name: Lingam, Manasvi
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Large-scale characterization of exoplanetary atmospheres is on the horizon, thereby making it possible in the future to extract their statistical properties. In this context, by using a well validated model in the solar system, we carry out three-dimensional magnetohydrodynamic simulations to compute nonthermal atmospheric ion escape rates of unmagnetized rocky exoplanets as a function of their radius based on fixed stellar radiation and wind conditions. We find that the atmospheric escape rate is, unexpectedly and strikingly, a nonmonotonic function of the planetary radius $R$ and that it evinces a maximum at $R \sim 0.7\,R_\oplus$. This novel nonmonotonic behavior may arise from an intricate tradeoff between the cross-sectional area of a planet (which increases with size, boosting escape rates) and its associated escape velocity (which also increases with size, but diminishes escape rates). Our results could guide forthcoming observations because worlds with certain values of $R$ (such as $R \sim 0.7\,R_\oplus$) might exhibit comparatively higher escape rates when all other factors are constant.
description: 8 pages, 2 figures, 2 tables; to appear in The Astrophysical Journal Letters
Electronic theory for itinerant in-plane magnetic fluctuations in Na$_x$CoO$_2$
Creators: name: Korshunov, M. M.
name: Eremin, I.
name: Shorikov, A.
name: Anisimov, V. I.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Starting from {\it ab-initio} band structure for Na$_x$CoO$_2$, we derive the single-electron energies and the effective tight-binding description for the $t_{2g}$ bands using a projection procedure. We find that due to the presence of the next-nearest-neighbor hoppings a local minimum in the electronic dispersion close to the $Γ$ point of the first Brillouin zone forms. Therefore, in addition to a large Fermi surface an electron pocket close to the $Γ$ point emerges at high doping concentrations. The latter yields the new scattering channel resulting in a peak structure of the itinerant magnetic susceptibility at small momenta. This indicates itinerant in-plane ferromagnetic state above certain critical concentration $x_m$, in agreement with neutron scattering data. Below $x_m$ the magnetic susceptibility shows a tendency towards the antiferromagnetic fluctuations. We estimate the value of $0.58 < x_m < 0.7$ within the rigid band model and within the Hubbard model with infinite on-site Coulomb repulsion consistent with the experimental phase diagram.
description: 4 pages, 4 figures; LDA calculations were done with Na in the symmetric 2d position contrary to the 6h position in a previous version of this paper
Neutron Stars in X-ray Binaries and their Environments
Creators: name: Paul, Biswajit
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Neutron stars in X-ray binary systems are fascinating objects that display a wide range of timing and spectral phenomena in the X-rays. Not only parameters of the neutron stars, like magnetic field strength and spin period evolve in their active binary phase, the neutron stars also affect the binary systems and their immediate surroundings in many ways. Here we discuss some aspects of the interactions of the neutron stars with their environments that are revelaed from their X-ray emission. We discuss some recent developments involving the process of accretion onto high magnetic field neutron stars: accretion stream structure and formation, shape of pulse profile and its changes with accretion torque. Various recent studies of reprocessing of X-rays in the accretion disk surface, vertical structures of the accretion disk and wind of companion star are also discussed here. The X-ray pulsars among the binary neutron stars provide excellent handle to make accurate measurement of the orbital parameters and thus also evolution of the binray orbits that take place over time scale of a fraction of a million years to tens of millions of years. The orbital period evolution of X-ray binaries have shown them to be rather complex systems. Orbital evolution of X-ray binaries can also be carried out from timing of the X-ray eclipses and there have been some surprising results in that direction, including orbital period glitches in two X-ray binaries and possible detection of the most massive circum-binary planet around a Low Mass X-ray Binary.
description: Has appeared in Journal of Astrophysics and Astronomy special issue on 'Physics of Neutron Stars and Related Objects', celebrating the 75th birth-year of G. Srinivasan
title: CiteBench: A Benchmark for Scientific Citation Text Generation
Creators: name: Funkquist, Martin
name: Kuznetsov, Ilia
name: Hou, Yufang
name: Gurevych, Iryna
Publisher: name: ACL
Year: 2024

description: Science progresses by building upon the prior body of knowledge documented in scientific publications. The acceleration of research makes it hard to stay up-to-date with the recent developments and to summarize the ever-growing body of prior work. To address this, the task of citation text generation aims to produce accurate textual summaries given a set of papers-to-cite and the citing paper context. Due to otherwise rare explicit anchoring of cited documents in the citing paper, citation text generation provides an excellent opportunity to study how humans aggregate and synthesize textual knowledge from sources. Yet, existing studies are based upon widely diverging task definitions, which makes it hard to study this task systematically. To address this challenge, we propose CiteBench: a benchmark for citation text generation that unifies multiple diverse datasets and enables standardized evaluation of citation text generation models across task designs and domains. Using the new benchmark, we investigate the performance of multiple strong baselines, test their transferability between the datasets, and deliver new insights into the task definition and evaluation to guide future research in citation text generation. We make the code for CiteBench publicly available at https://github.com/UKPLab/citebench.
Dissecting users' needs for search result explanations
Creators: name: Juneja, Prerna
name: Zhang, Wenjuan
name: Smith-Renner, Alison Marie
name: Lamba, Hemank
name: Tetreault, Joel
name: Jaimes, Alex
Publisher: name: arXiv
Year: 2024
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: Information Retrieval (cs.IR)
subject: FOS: Computer and information sciences

description: There is a growing demand for transparency in search engines to understand how search results are curated and to enhance users' trust. Prior research has introduced search result explanations with a focus on how to explain, assuming explanations are beneficial. Our study takes a step back to examine if search explanations are needed and when they are likely to provide benefits. Additionally, we summarize key characteristics of helpful explanations and share users' perspectives on explanation features provided by Google and Bing. Interviews with non-technical individuals reveal that users do not always seek or understand search explanations and mostly desire them for complex and critical tasks. They find Google's search explanations too obvious but appreciate the ability to contest search results. Based on our findings, we offer design recommendations for search engines and explanations to help users better evaluate search results and enhance their search experience.
A Trust and Identity Policy Toolkit for collaborative research environments
Creators: name: Mora, Kerry
Publisher: name: Zenodo
Year: 2023
Subjects: authorised access
trusted identity

description: Modern research is multidisciplinary, requiring access to many infrastructures outside of a researcher's home institution. In this complex environment, the question of trust (between users, resource providers, and infrastructures) is crucial.

The Australian Access Federation (AAF) is working with NCRIS facilities to develop a standard set of policies that can build and facilitate trust. These policies outline the operational measures undertaken to securely and effectively provide research infrastructure and services.

The Policy Toolkit includes policies that:
•define the roles and the responsibilities of all participants
•define expected behaviour of all the participants
•define the security response procedure and responsibilities of individuals during a cyber incident
•manage the risk of capturing, storing and using personal information about users and their data.

In this presentation, we will highlight the policies that make up the Toolkit and how important they are to enable research collaboration nationally and internationally. We will cover how it is being developed and how other research environments can adopt it with their existing policy structures.
Additional file 1: of PanDrugs: a novel method to prioritize anticancer drug treatments according to individual genomic data
Creators: name: Piñeiro-Yáñez, Elena
name: Reboiro-Jato, Miguel
name: Gómez-López, Gonzalo
name: Perales-Patón, Javier
name: Troulé, Kevin
name: Rodríguez, José
name: Tejero, Héctor
name: Shimamura, Takeshi
name: López-Casas, Pedro
name: Carretero, Julián
name: Valencia, Alfonso
name: Hidalgo, Manuel
name: Glez-Peña, Daniel
name: Al-Shahrour, Fátima
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Supplementary materials and methods, Figures S1–S11 and Tables S1–S8. (PDF 14845 kb)
Two-Dimensional Black Hole and Nonperturbative String Theory
Creators: name: Dhar, Avinash
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss the interpertation of the $c=1$ matrix model as two-dimensional string theory in a dilaton-black hole background. The nonperturbative formulation of $c=1$ matrix model in terms of an integrable model of nonrelativistic fermions enables us to study the quantum fate of the classical black hole singularity. We find that the classical singularity is wiped out by quantum corrections when summed to all orders.
description: 28p, TIFR-TH-93/34
Search for Neutrinoless $β^{+}\hspace{-0.2em}EC$ Decay of $^{120}$Te with CUORE-0
Creators: name: CUORE Collaboration
name: Alduino, C.
name: Alfonso, K.
name: Artusa, D. R.
name: Avignone, F. T.
name: Azzolini, O.
name: Bari, G.
name: Bellini, F.
name: Benato, G.
name: Bersani, A.
name: Biassoni, M.
name: Branca, A.
name: Brofferio, C.
name: Bucci, C.
name: Camacho, A.
name: Caminata, A.
name: Canonica, L.
name: Cao, X. G.
name: Capelli, S.
name: Cappelli, L.
name: Cardani, L.
name: Carniti, P.
name: Casali, N.
name: Cassina, L.
name: Chiesa, D.
name: Chott, N.
name: Clemenza, M.
name: Copello, S.
name: Cosmelli, C.
name: Cremonesi, O.
name: Creswick, R. J.
name: Cushman, J. S.
name: D'Addabbo, A.
name: D'Aguanno, D.
name: Dafinei, I.
name: Davis, C. J.
name: Dell'Oro, S.
name: Deninno, M. M.
name: Di Domizio, S.
name: Di Vacri, M. L.
name: Drobizhev, A.
name: Fang, D. Q.
name: Faverzani, M.
name: Ferri, E.
name: Ferroni, F.
name: Fiorini, E.
name: Franceschi, M. A.
name: Freedman, S. J.
name: Fujikawa, B. K.
name: Giachero, A.
name: Gironi, L.
name: Giuliani, A.
name: Gladstone, L.
name: Gorla, P.
name: Gotti, C.
name: Gutierrez, T. D.
name: Han, K.
name: Heeger, K. M.
name: Hennings-Yeomans, R.
name: Huang, H. Z.
name: Keppel, G.
name: Kolomensky, Yu. G.
name: Leder, A.
name: Ligi, C.
name: Lim, K. E.
name: Ma, Y. G.
name: Marini, L.
name: Martinez, M.
name: Maruyama, R. H.
name: Mei, Y.
name: Moggi, N.
name: Morganti, S.
name: Mosteiro, P. J.
name: Nagorny, S. S.
name: Napolitano, T.
name: Nastasi, M.
name: Nones, C.
name: Norman, E. B.
name: Novati, V.
name: Nucciotti, A.
name: O'Donnell, T.
name: Ouellet, J. L.
name: Pagliarone, C. E.
name: Pallavicini, M.
name: Palmieri, V.
name: Pattavina, L.
name: Pavan, M.
name: Pessina, G.
name: Pira, C.
name: Pirro, S.
name: Pozzi, S.
name: Previtali, E.
name: Rosenfeld, C.
name: Rusconi, C.
name: Sakai, M.
name: Sangiorgio, S.
name: Santone, D.
name: Schmidt, B.
name: Schmidt, J.
name: Scielzo, N. D.
name: Singh, V.
name: Sisti, M.
name: Taffarello, L.
name: Terranova, F.
name: Tomei, C.
name: Vignati, M.
name: Wagaarachchi, S. L.
name: Wang, B. S.
name: Wang, H. W.
name: Welliver, B.
name: Wilson, J.
name: Winslow, L. A.
name: Wise, T.
name: Woodcraft, A.
name: Zanotti, L.
name: Zhang, G. Q.
name: Zimmermann, S.
name: Zucchelli, S.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We have performed a search for neutrinoless $β^{+}\hspace{-0.2em}EC$ decay of $^{120}$Te using the final CUORE-0 data release. We describe a new analysis method for the simultaneous fit of signatures with different event topology, and of data subsets with different signal efficiency, obtaining a limit on the half-life of the decay of $T_{1/2}>1.6\cdot10^{21}$ yr at $90\%$ CI. Combining this with results from Cuoricino, a predecessor experiment, we obtain the strongest limit to date, corresponding to $T_{1/2}>2.7\cdot10^{21}$ yr at $90\%$ CI.
description: 10 pages, 6 figures, 3 tables
Successful Joint Ventures Among Farmer Cooperatives
Creators: name: Frederick, Donald A.
name: Frederick, Donald A.
Publisher: name: Unknown
Year: 1987
Subjects: subject: Livestock Production/Industries
subject: Marketing
subject: FOS: Economics and business
subject: Cooperatives
subject: efficiency
subject: joint venture
subject: structure

description: This report describes development, purposes, operations, and challenges of four successful joint ventures among dairy cooperatives. Provides guidelines applicable to any cooperative for deciding whether to enter into a joint venture with one or more cooperatives, and how to structure such a venture to maximize the chances of achieving its objectives.
Mean number of visits to sites in Levy flights
Creators: name: Ferraro, M.
name: Zaninetti, L.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: Formulas are derived to compute the mean number of times a site has been visited during symmetric Levy flights. Unrestricted Levy flights are considered first, for lattices of any dimension: conditions for the existence of finite asymptotic maps of the visits over the lattice are analysed and a connection is made with the transience of the flight. In particular it is shown that flights on lattices of dimension greater than one are always transient. For an interval with absorbing boundaries the mean number of visits reaches stationary values, which are computed by means of numerical and analytical methods; comparisons with Monte Carlo simulations are also presented.
description: 9 pages 3 figures. Accepted for publication on Physical Review E
MOESM4 of A porcine model for pathomorphological age assessment of surgically excised skin wounds
Creators: name: Barington, Kristiane
name: Dich-Jørgensen, Kristine
name: Jensen, Henrik
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Physiology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Hematology
subject: 110309 Infectious Diseases

description: Additional file 4. Infiltration of neutrophils and macrophages was scored as: (0) absent; (1) 200 using a 40× objective and 10× ocular with FN 22 mm in one high power field (HPF) of 0.237 mm2. The scoring was carried out in the HPF with the highest number of neutrophils and macrophages within areas 1–4 in the wounds (Fig. 2a, b). From each wound, only the highest score was registered, i.e. one neutrophil score and one macrophage score per wound. Location of the wound (1–4), wound age, neutrophil score and macrophage score are presented.
Cosmic expansion beyond $Λ$CDM: Investigating power-law and logarithmic corrections
Creators: name: Koussour, M.
name: Kavya, N. S.
name: Venkatesha, V.
name: Myrzakulov, N.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The cosmic acceleration observed in the expansion of the Universe has sparked extensive research into the nature of dark energy, which is known to constitute approximately 70\% of the Universe's energy content. In this study, we explore two parametrizations of the Hubble parameter, namely power-law and logarithmic corrections, as alternatives to the standard $Λ$CDM model. Using observational data from Cosmic Chronometers (CC), Pantheon+, and the Baryonic Acoustic Oscillations (BAO) datasets, we investigate the dynamics of essential cosmological parameters, including the deceleration parameter, energy density, pressure, and equation of state (EoS) parameter. The $Om(z)$ diagnostic test is employed to classify different dark energy models. Our cosmological models, with the power-law and logarithmic corrections, are found to provide a good fit to the recent observational data and efficiently describe the cosmic expansion scenario.
description: The European Physical Journal Plus accepted version
MOJAVE: XV. VLBA 15 GHz Total Intensity and Polarization Maps of 437 Parsec-Scale AGN Jets From 1996-2017
Creators: name: Lister, M. L.
name: Aller, M. F.
name: Aller, H. D.
name: Hodge, M. A.
name: Homan, D. C.
name: Kovalev, Y. Y.
name: Pushkarev, A. B.
name: Savolainen, T.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present 5321 milliarcsecond-resolution total intensity and linear polarization maps of 437 active galactic nuclei (AGNs) obtained with the VLBA at 15 GHz as part of the MOJAVE survey, and also from the NRAO data archive. The former is a long-term program to study the structure and evolution of powerful parsec-scale outflows associated with AGNs. The targeted AGNs are drawn from several flux-limited radio and gamma-ray samples, and all have correlated VLBA flux densities greater than about 50 mJy at 15 GHz. Approximately 80% of these AGNs are associated with gamma-ray sources detected by the Fermi LAT instrument. The vast majority were observed with the VLBA on 5 to 15 occasions between 1996 January 19 and 2016 December 26, at intervals ranging from a month to several years, with the most typical sampling interval being six months. A detailed analysis of the linear and circular polarization evolution of these AGN jets are presented in other papers in this series.
description: 6 pages, 5 figures, 2 tables; accepted by ApJS; full electronic version of table 2 is available from the preprint source; the images are available from http://www.physics.purdue.edu/MOJAVE/MOJAVE_XV/natwgtmaps.tar
Active sieving across driven nanopores for tunable selectivity
Creators: name: Marbach, Sophie
name: Bocquet, Lydéric
Publisher: name: arXiv
Year: 2017
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Molecular separation traditionnally relies on sieving processes across passive nanoporous membranes. Here we explore theoretically the concept of non-equilibrium active sieving. We investigate a simple model for an active noisy nanopore, where gating - in terms of size or charge - is externally driven at a tunable frequency. Our analytical and numerical results unveil a rich sieving diagram in terms of the forced gating frequency. Unexpectedly, the separation ability is strongly increased as compared to its passive (zero frequency) counterpart. It points also to the possibility of tuning dynamically the osmotic pressure. Active separation outperforms passive sieving and represents a promising avenue for advanced filtration.
description: 11 pages, 9 figures
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Cart. 190 (11 H 75), 316 folios, f. 0085v
Creators: name: de la Côte d'Or, Archives départementales
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 général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0085v, 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 VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0085v, 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
Detections of SiO and H$_2$O Masers in the Bipolar Nebula IRAS 19312+1950
Creators: name: Nakashima, Jun-ichi
name: Deguchi, Shuji
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on the detection of SiO and water masers toward a newly found bipolar nebula, IRAS 19312+1950. This object exhibits extreme red IRAS color log (F25/F12)=0.5 and log (F60/F25)=0.7 and a nebulosity having a size of about 30" extended to the South-West in the 2MASS near-infrared image. Toward this object, we have detected emission from the H2O 6(1,6)-5(2,3) transition, the SiO J=1-0, v=1 and 2, and J=2-1, v=1 transitions, and the SO 2(2)--1(1) and H13CN J=1-0 transitions. The thermal lines of SO and H13CN are shifted by about 12 km/s in radial velocity with respect to the maser lines, indicating that thermal emission comes from the background molecular cloud. However, the SiO J=2-1, v=2 spectrum shows another component of SiO emission separated by 26 km/s from the main component, that might be formed in a rotating or expanding shell.
description: 5 peges including 1 table, and 2 jpeg figures. Accepted for PASJ (Publication of the Astronomical Society of Japan)
Displacement Operators and Constraints on Boundary Central Charges
Creators: name: Herzog, Christopher
name: Huang, Kuo-Wei
name: Jensen, Kristan
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Boundary conformal field theories have several additional terms in the trace anomaly of the stress tensor associated purely with the boundary. We constrain the corresponding boundary central charges in three- and four-dimensional conformal field theories in terms of two- and three-point correlation functions of the displacement operator. We provide a general derivation by comparing the trace anomaly with scale dependent contact terms in the correlation functions. We conjecture a relation between the a-type boundary charge in three dimensions and the stress tensor two-point function near the boundary. We check our results for several free theories.
description: 5 pages
Luminosities and mass-loss rates of Local Group AGB stars and Red Supergiants
Creators: name: Groenewegen, Martin A. T.
name: Sloan, Greg C.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We aim to investigate mass loss and luminosity in a large sample of evolved stars in several Local Group galaxies with a variety of metalliticies and star-formation histories: the Small and Large Magellanic Cloud, and the Fornax, Carina, and Sculptor dwarf spheroidal galaxies. Dust radiative transfer models are presented for 225 carbon stars and 171 oxygen-rich evolved stars for which spectra from the Infrared Spectrograph on Spitzer are available. The spectra are complemented with available optical and infrared photometry to construct spectral energy distributions. A minimization procedure was used to determine luminosity and mass-loss rate (MLR). Pulsation periods were derived for a large fraction of the sample based on a re-analysis of existing data. New deep K-band photometry from the VMC survey and multi-epoch data from IRAC and AllWISE/NEOWISE have allowed us to derive pulsation periods longer than 1000 days for some of the most heavily obscured and reddened objects. We derive (dust) MLRs and luminosities for the entire sample. The estimated MLRs can differ significantly from estimates for the same objects in the literature due to differences in adopted optical constants (up to factors of several) and details in the radiative transfer modelling. Updated parameters for the super-AGB candidate MSX SMC 055 (IRAS 00483-7347) are presented. Its current mass is estimated to be 8.5 +- 1.6 \msol, suggesting an initial mass well above 8~\msol. Using synthetic photometry, we present and discuss colour-colour and colour-magnitude diagrams which can be expected from the James Webb Space Telescope.
description: A&A accepted. The full version (100 pages, 12 MB) with complete tables and all figures of the appendices is available at http://homepage.oma.be/marting/articlesgroen.html