cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Green and efficient three-component synthesis of novel isoniazid pyrazoles, molecular docking, antioxidant and antitubercular evaluation
Creators: name: Koli, Bharti P.
name: Gore, Rambhau P.
name: Malasane, Pravin R.
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: A series of novel isoniazid pyrazole derivatives were synthesized by an efficient, multicomponent reaction of various substituted aromatic aldehydes, isoniazid, and malononitrile in aqueous ethanol. The catalyst-free, green, three-component reaction took place well with good to excellent yields of the desired derivatives. The synthesized novel derivatives were screened for antimicrobial, antioxidant, and anti-TB properties along with the molecular docking study. Some of the synthesized compounds exhibit moderate antibacterial and comparable antifungal properties, while all of them display strong antioxidant activity. The compound 4l demonstrates the most significant activity against M. tuberculosis with MIC = 0.125 µg/mL. The various analytical techniques including FT-IR, 1H NMR, 13C NMR, and HRMS were utilized to confirm the structures of the newly synthesized compounds.
Atmospheric Neutrino Oscillations in IceCube DeepCore
Creators: name: Leonard, Kayla
Publisher: name: Zenodo
Year: 2020

description: The DeepCore sub-array within the IceCube Neutrino Observatory is a densely instrumented region of Antarctic ice designed to observe atmospheric neutrino interactions above 5 GeV, via Cherenkov radiation. At these energies, Earth-crossing muon neutrinos have a high chance of oscillating away to tau neutrinos. These oscillations have been previously observed in DeepCore through both muon neutrino disappearance and tau neutrino appearance channels. This poster will present the status of the IceCube Collaboration's newest analysis of the atmospheric neutrino oscillation parameters using 8 years of data. In addition to several more years of data, this analysis benefits from recent significant efforts in improving background rejection, reconstruction techniques, modeling of systematic uncertainties, particle identification, and much more.
Spin and parity measurement of the Λ(1405) baryon
Creators: name: Moriya, Kei
name: Schumacher, Reinhard A.
name: M.  Bellis
name: B.  Dey
name: McCracken, Michael E.
name: Meyer, Curtis
name: CLAS Collaboration
Publisher: name: Figshare
Year: 2018
Subjects: subject: 20399 Classical Physics not elsewhere classified
subject: FOS: Physical sciences

description: A determination of the spin and parity of the Λ(1405) is presented using photoproduction data from the CLAS detector at Jefferson Lab. The reaction γ+p→K++Λ(1405) is analyzed in the decay channel Λ(1405)→Σ++π−, where the decay distribution to Σ+π− and the variation of the Σ+ polarization with respect to the Λ(1405) polarization direction determines the parity. The Λ(1405) is produced, in the energy range 2.55
Multiresolution Division Multiplex (MRDM): A New Wavelet-based Multiplex System
Creators: name: de Oliveira, H. M.
name: Bouton, E. A.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: An original multiplex scheme is introduced, which is based on Mallat's multiresolution formulation of wavelet systems. This system is adaptable and its implementation is well matched to digital signal processors and computers. The approach termed multiresolution division multiplex (MRDM) is intensive in signal processing (SP) tools, extremely flexible and can combine a variety of tributaries at different bit rates. A broad variety of orthogonal wavelet systems can endow with MRDM and the channel waveforms, and consequently the spectral shape and system performance depend upon the selected wavelets. Demultiplex can be done efficiently, since the number of floating multiplications and additions increase only linearly with the length of signals. A Haar-based MRDM scheme is presented to illustrate the versatility of this new multiplex approach.
description: 5 pages, 8 figures, ITS International Telecomm. Symposium, Brazil, 2006
Step Formation on Hydrogen-etched 6H-SiC{0001} Surfaces
Creators: name: Nie, Shu
name: C. D. Lee
name: Feenstra, Randall
name: Y.  Ke
name: R. P. Devaty
name: W. J. Choyke
name: C. K. Inoki
name: T. S. Kuan
name: Gu, Gong
Publisher: name: Figshare
Year: 2018
Subjects: subject: 20399 Classical Physics not elsewhere classified
subject: FOS: Physical sciences

description: The formation of step bunches and/or facets on hydrogen-etched SiC (0001) and (000-1) surfaces has been studied, using both nominally on-axis and intentionally miscut (i.e. vicinal) substrates. It is found that small miscuts on the (0001) surface produce full unit-cell high steps, while half unit-cell high steps are observed on the (000-1) surface. The observed step normal direction is found to be <1-100> for both surfaces. Hence, for intentionally miscut material, a miscut oriented towards this direction produces much better order in the step array compared to a miscut oriented towards a <11-20> direction. For (0001) vicinal surfaces that are miscut towards the <1-100> direction, the formation of surface ripples is observed for 3° miscut and the development of small facets (nanofacets) is found for higher miscut angles. Much less faceting is observed on miscut (000-1) surfaces. Additionally, the (0001) surface is found to have a much larger spatial anisotropy in step energies than the (000-1) surface.
The Accelerator Neutrino Neutron Interaction Experiment (ANNIE)
Creators: name: Mayly Sanchez
name: Pickard, Leon
Publisher: name: Zenodo
Year: 2020

description: The Accelerator Neutrino Neutron Interaction Experiment (ANNIE) aims at measuring the neutron abundance in the final state of neutrino-nucleus interactions. This measurement will have a direct impact on our understanding of neutrino interactions and will lead to a better reduction of systematic errors and an improvement of signal-background discrimination in future large neutrino detectors. The ANNIE detector uses 30 tons of gadolinium-loaded water to enhance the neutron-caputre cross section. It is instrumented with a combination of conventional photomultipliers and novel Lare Area Picosecond Photodetectors (LAPPDs). After a background characterization phase, the detectors has been installed in the Booster Neutrino beam at Fermilab and has begun taking data. This presentation will show early data from the ANNIE experiment.
Event Selection for the NOvA Sterile Neutrino Search
Creators: name: Norrick, Anne
name: Lister, Adam
Publisher: name: Zenodo
Year: 2020

description: The NOvA experiment consists of two functionally identical liquid scintillator detectors in Fermilab's NuMI neutrino beam: a 300 ton near detector at a 1km baseline, and a 14,000 ton far detector 810km away in Ash River, MN. The primary physics goal of NOvA is to characterise neutrino oscillations, with focus on the three-neutrino flavor paradigm. This poster presents an extension to this goal by using the detectors to search for oscillations involving sterile neutrinos. The search is performed by leveraging neutrino disappearance in neutral current interactions between the near and far detectors as well as by performing a joint fit of electron neutrino appearance and muon neutrino disappearance at the Near Detector. Techniques for event selection and our systematics will be presented and discussed.
The holomorphic couch theorem
Creators: name: Bourque, Maxime Fortier
Publisher: name: arXiv
Year: 2015
Subjects: subject: Complex Variables (math.CV)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 30F60, 30C75, 32H02

description: We prove that if two conformal embeddings between Riemann surfaces with finite topology are homotopic, then they are isotopic through conformal embeddings. Furthermore, we show that the space of all conformal embeddings in a given homotopy class deformation retracts into a point, a circle, a torus, or the unit tangent bundle of the codomain, depending on the induced homomorphism on fundamental groups. Quadratic differentials play a central role in the proof.
description: 70 pages, 13 figures. Sections 4 and 8 modified following referee's report
Information-Theoretic Caching: Sequential Coding for Computing
Creators: name: Wang, Chien-Yi
name: Lim, Sung Hoon
name: Gastpar, Michael
Publisher: name: arXiv
Year: 2015
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: Under the paradigm of caching, partial data is delivered before the actual requests of users are known. In this paper, this problem is modeled as a canonical distributed source coding problem with side information, where the side information represents the users' requests. For the single-user case, a single-letter characterization of the optimal rate region is established, and for several important special cases, closed-form solutions are given, including the scenario of uniformly distributed user requests. In this case, it is shown that the optimal caching strategy is closely related to total correlation and Wyner's common information. Using the insight gained from the single-user case, three two-user scenarios admitting single-letter characterization are considered, which draw connections to existing source coding problems in the literature: the Gray--Wyner system and distributed successive refinement. Finally, the model studied by Maddah-Ali and Niesen is rephrased to make a comparison with the considered information-theoretic model. Although the two caching models have a similar behavior for the single-user case, it is shown through a two-user example that the two caching models behave differently in general.
description: submitted to IEEE Trans. Inf. Theory and presented in part at ISIT 2015
Templates for the Sunyaev-Zel'dovich Angular Power Spectrum
Creators: name: Trac, Hy
name: Bode, Paul
name: Ostriker, Jeremiah P.
Publisher: name: Figshare
Year: 2018
Subjects: subject: 20399 Classical Physics not elsewhere classified
subject: FOS: Physical sciences

description: We present templates for the Sunyaev-Zel'dovich (SZ) angular power spectrum based on four models for the nonlinear gas distribution. The frequency-dependent SZ temperature fluctuations, with thermal (TSZ) and kinetic (KSZ) contributions, are calculated by tracing through a dark matter simulation, processed to include gas in dark matter halos and in the filamentary intergalactic medium. Different halo gas models are compared to study how star formation, energetic feedback, and nonthermal pressure support influence the angular power spectrum. The standard model has been calibrated to reproduce the stellar and gas fractions and X-ray scaling relations measured from low-redshift clusters and groups. The other models illustrate the current theoretical and empirical uncertainties relating to properties of the intracluster medium. Relative to the standard model, their angular power spectra differ by approximately ±50% (TSZ), ±20% (KSZ), and ±40% (SZ at 148 GHz) for l = 3000, σ8 = 0.8, and homogeneous reionization at z = 10. The angular power spectrum decreases in amplitude as gas mass and binding energy are removed through star formation, and as gas is pushed out to larger radii by energetic feedback. With nonthermal pressure support, less pressure is required to maintain hydrostatic equilibrium, thus reducing the thermal contribution to the SZ power. We also calculate the SZ templates as a function of σ8 and quantify this dependence. Assuming Cl ∝ (σ8/0.8)α, the effective scaling index ranges from 7  αTSZ  9, 4.5  αKSZ  5.5, and 6.5  αSZ (148 GHz)  8 at l = 3000 for 0.6 < σ8 < 1. The template spectra are publicly available and can be used when fitting for the SZ contribution to the cosmic microwave background on arcminute scales.
Generalized fermion algebra
Creators: name: Chung, Won Sang
name: Daoud, Mohammed
Publisher: name: arXiv
Year: 2014
Subjects: subject: Mathematical Physics (math-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: A one-parameter generalized fermion algebra ${\cal B}_κ(1)$ is introduced. The Fock representation is studied. The associated coherent states are constructed and the polynomial representation, in the Bargmann sense, is derived. A special attention is devoted to the limiting case $κ\rightarrow 0$ where the fermionic coherent states, labeled by Grassmann variables, are obtained. The physical relevance of the algebra is illustrated throughout Calogero-Sutherland system.
description: 11 pages, typos in eqs. 2 and 3 are corrected
Psithyrus sylvestris
Creators: name: Wagner, Rainer
Publisher: name: Zenodo
Year: 1971
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Apidae
Psithyrus
Psithyrus sylvestris

description: 5. Ps. sylvestris (Lepeletier, 1833) Flugzeit: altes ♀ 21. 5. 1961. — In Deutschland weit verbreitet, aber nicht häufig; nach Alfken (1913) sehr selten, besonders die Weibchen, von denen er innerhalb von 5 Jahren nur 3 Exemplare fing. Weder von ihm noch von A. C. W. Wagner (1914 u. 1937) werden Fundorte von Cuxhaven oder seiner Umgebung erwähnt. Am 21. 5. 1961 konnte 1 Weibchen dieser Art in Fanggebiet I erbeutet werden. — Wirte: B. pratorum und B. jonellus. Der Wirt von Ps. sylvestris im Raum Cuxhaven könnte B. jonellus gewesen sein.
description: Published as part of Wagner, Rainer, 1971, Die Veränderung der Hummelfauna Cuxhavens in diesem Jahrhundert. Der Versuch einer Deutung.), pp. 207-232 in Ent. Mitt. Zool. Mus. Hamburg 4 (75) on page 218, DOI: 10.5281/zenodo.7289873
description: {"references": ["Alfken, J. D., 1913: Die Bienenfauna von Bremen. - Abh. naturw. Ver. Bre- men 22, 1 - 220.", "Wagner A. C. W., 1914: Die Bienenfauna der Niederelbe. - Abh. Ver. naturw. Unterh. 15, 3 - 56, Hamburg."]}
The GREAT3 Challenge
Creators: name: Hironao  Miyatake
name: Mandelbaum, Rachel
name: Rowe, Barnaby
name: GREAT3 Collaboration
Publisher: name: Figshare
Year: 2018
Subjects: subject: 20399 Classical Physics not elsewhere classified
subject: FOS: Physical sciences

description: The GRavitational lEnsing Accuracy Testing 3 (GREAT3) challenge is an image analysis competition that aims to test algorithms to measure weak gravitational lensing from astronomical images. The challenge started in October 2013 and ends 30 April 2014. The challenge focuses on testing the impact on weak lensing measurements of realistically complex galaxy morphologies, realistic point spread function, and combination of multiple different exposures. It includes simulated ground- and space-based data. The details of the challenge are described in [1], and the challenge website and its leader board can be found at http://great3challenge.info andhttp://great3.projects.phys.ucl.ac.uk/leaderboard/, respectively.
Additional file 16 of Genome-scale analysis of Arabidopsis splicing-related protein kinase families reveals roles in abiotic stress adaptation
Creators: name: Rodriguez Gallo, M. C.
name: Li, Q.
name: Mehta, D.
name: Uhrig, R. G.
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 16.
Gaze Stabilization for Humanoid Robots: a Comprehensive Framework
Creators: name: Roncone, Alessandro
name: Pattacini, Ugo
name: Metta, Giorgio
name: Natale, Lorenzo
Publisher: name: arXiv
Year: 2014
Subjects: subject: Robotics (cs.RO)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Gaze stabilization is an important requisite for humanoid robots. Previous work on this topic has focused on the integration of inertial and visual information. Little attention has been given to a third component, which is the knowledge that the robot has about its own movement. In this work we propose a comprehensive framework for gaze stabilization in a humanoid robot. We focus on the problem of compensating for disturbances induced in the cameras due to self-generated movements of the robot. In this work we employ two separate signals for stabilization: (1) an anticipatory term obtained from the velocity commands sent to the joints while the robot moves autonomously; (2) a feedback term from the on board gyroscope, which compensates unpredicted external disturbances. We first provide the mathematical formulation to derive the forward and the differential kinematics of the fixation point of the stereo system. We finally test our method on the iCub robot. We show that the stabilization consistently reduces the residual optical flow during the movement of the robot and in presence of external disturbances. We also demonstrate that proper integration of the neck DoF is crucial to achieve correct stabilization.
description: 6 pages, appears in 2014 IEEE-RAS International Conference on Humanoid Robots
2022-On-Just-Terms-Submission.pdf
Creators: name: Poelina, Anne
Publisher: name: figshare
Year: 2022
Subjects: subject: 180101 Aboriginal and Torres Strait Islander Law
subject: FOS: Law
subject: 160501 Aboriginal and Torres Strait Islander Policy
subject: FOS: Political science
subject: 130301 Aboriginal and Torres Strait Islander Education
subject: FOS: Educational sciences
subject: 111701 Aboriginal and Torres Strait Islander Health
subject: FOS: Health sciences
subject: 200201 Aboriginal and Torres Strait Islander Cultural Studies
subject: FOS: Other humanities
subject: 210301 Aboriginal and Torres Strait Islander History
subject: FOS: History and archaeology
subject: 80701 Aboriginal and Torres Strait Islander Knowledge Management
subject: FOS: Media and communications
subject: 200319 Aboriginal and Torres Strait Islander Languages
subject: FOS: Languages and literature
subject: 169902 Studies of Aboriginal and Torres Strait Islander Society
subject: FOS: Sociology
subject: 190401 Aboriginal and Torres Strait Islander Performing Arts
subject: FOS: Arts (arts, history of arts, performing arts, music)
subject: 50201 Aboriginal and Torres Strait Islander Environmental Knowledge
subject: FOS: Earth and related environmental sciences
subject: 200501 Aboriginal and Torres Strait Islander Literature
subject: 80601 Aboriginal and Torres Strait Islander Information and Knowledge Systems
subject: FOS: Computer and information sciences

description: The key edited submission 'On Just terms' submitted in good faith on a no prejudice basis for review, to the Land and Public Works Legislation Amendments board by Professor Anne Poelina, Nulungu Research Institute, Notre Dame University.
Strong bimodality in the host halo mass of central galaxies from galaxy-galaxy lensing
Creators: name: Mandelbaum, Rachel
name: Wenting  Wang
name: Zu, Ying
name: White, Simon
name: Henriques, Bruno
name: Surhud  More
Publisher: name: Figshare
Year: 2018
Subjects: subject: 20399 Classical Physics not elsewhere classified
subject: FOS: Physical sciences

description: We use galaxy-galaxy lensing to study the dark matter halos surrounding a sample of Locally Brightest Galaxies (LBGs) selected from the Sloan Digital Sky Survey. We measure mean halo mass as a function of the stellar mass and colour of the central galaxy. Mock catalogues constructed from semi-analytic galaxy formation simulations demonstrate that most LBGs are the central objects of their halos, greatly reducing interpretation uncertainties due to satellite contributions to the lensing signal. Over the full stellar mass range, 10.310.7. Tests using the mock catalogues and on the data themselves clarify the effects of LBG selection and show that it cannot artificially induce a systematic dependence of halo mass on LBG colour. The bimodality in halo mass at fixed stellar mass is reproduced by the astrophysical model underlying our mock catalogue, but the sign of the effect is inconsistent with recent, nearly parameter-free age-matching models. The sign and magnitude of the effect can, however, be reproduced by halo occupation distribution models with a simple (few-parameter) prescription for type-dependence.
Additional file 17 of Genome-scale analysis of Arabidopsis splicing-related protein kinase families reveals roles in abiotic stress adaptation
Creators: name: Rodriguez Gallo, M. C.
name: Li, Q.
name: Mehta, D.
name: Uhrig, R. G.
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 17.
Hub Location under Uncertainty: a Minimax Regret Model for the Capacitated Problem with Multiple Allocations
Creators: name: Kazemian, Iman
name: Aref, Samin
Publisher: name: arXiv
Year: 2015
Subjects: subject: Data Structures and Algorithms (cs.DS)
subject: Optimization and Control (math.OC)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics
subject: 90B80 90C05 65K05 90-08 90C47

description: In this paper the capacitated hub location problem is formulated by a minimax regret model, which takes into account uncertain setup cost and demand. We focus on hub location with multiple allocations as a strategic problem requiring one definite solution. Investigating how deterministic models may lead to sub-optimal solutions, we provide an efficient formulation method for the problem. A computational analysis is performed to investigate the impact of uncertainty on the location of hubs. The suggested model is also compared with an alternative method, seasonal optimization, in terms of efficiency and practicability. The results indicate the importance of incorporating stochasticity and variability of parameters in solving practical hub location problems. Applying our method to a case study derived from an industrial food production company, we solve a logistical problem involving seasonal demand and uncertainty. The solution yields a definite hub network configuration to be implemented throughout the planning horizon.
description: 11 pages, 10 tables, 3 figures, accepted pre-print (author copy) with supplementary data
The Atacama Cosmology Telescope: cosmological parameters from three seasons of data
Creators: name: Sievers, Jonathan L.
name: Hlozek, Renee A.
name: Nolta, Michael R.
name: Battaglia, Nicholas
name: Trac, Hy
name: ACT Collaboration
Publisher: name: Figshare
Year: 2018
Subjects: subject: 20399 Classical Physics not elsewhere classified
subject: FOS: Physical sciences

description: We present constraints on cosmological and astrophysical parameters from high-resolution microwave background maps at 148 GHz and 218 GHz made by the Atacama Cosmology Telescope (ACT) in three seasons of observations from 2008 to 2010. A model of primary cosmological and secondary foreground parameters is fit to the map power spectra and lensing deflection power spectrum, including contributions from both the thermal Sunyaev-Zeldovich (tSZ) effect and the kinematic Sunyaev-Zeldovich (kSZ) effect, Poisson and correlated anisotropy from unresolved infrared sources, radio sources, and the correlation between the tSZ effect and infrared sources. The power ℓ2Cℓ/2π of the thermal SZ power spectrum at 148 GHz is measured to be3.4±1.4  μK2 at ℓ = 3000, while the corresponding amplitude of the kinematic SZ power spectrum has a 95% confidence level upper limit of 8.6  μK2. Combining ACT power spectra with the WMAP 7-year temperature and polarization power spectra, we find excellent consistency with the LCDM model. We constrain the number of effective relativistic degrees of freedom in the early universe to be Neff = 2.79±0.56, in agreement with the canonical value of Neff = 3.046 for three massless neutrinos. We constrain the sum of the neutrino masses to be Σmν < 0.39 eV at 95% confidence when combining ACT and WMAP 7-year data with BAO and Hubble constant measurements. We constrain the amount of primordial helium to be Yp = 0.225±0.034, and measure no variation in the fine structure constant α since recombination, withα/α0 = 1.004±0.005. We also find no evidence for any running of the scalar spectral index, dns/dln k = −0.004±0.012.
Additional file 18 of Genome-scale analysis of Arabidopsis splicing-related protein kinase families reveals roles in abiotic stress adaptation
Creators: name: Rodriguez Gallo, M. C.
name: Li, Q.
name: Mehta, D.
name: Uhrig, R. G.
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 18.
Long-lived heavy neutrino searches at the colliders
Creators: name: Arindam Das
Publisher: name: Zenodo
Year: 2020

description: A $𝑈(1)_𝑋$ extension of the Standard Model is a simple and consistent framework to naturally incorporate three Right-Handed Neutrinos for generating the observed light neutrino masses and mixing by the seesaw mechanism.We examine the collider testability of the $𝑈(1)_𝑋$ model,both in its minimal form with the conventional charges,as well as with an alternative charge assignment,via the resonant production of the 𝑍'-boson and its subsequent decay into a pair of RHNs.We first derive an updated upper limit on the new gauge coupling $𝑔_𝑋$ as a function of the $M_{𝑍^′}$ from the latest LHC dilepton searches.Then we identify the maximum possible cross section for the RHN pair-production under these constraints.We investigate the possibility of having one of the RHNs long-lived,even for a TeV-scale mass.Employing the general parametrization for the light neutrino mass matrix to reproduce the observed neutrino data,we perform a parameter scan to find the allowed region for the long-lived RHNs.
Psithyrus norvegicus Sparre- Schneider 1918
Creators: name: Wagner, Rainer
Publisher: name: Zenodo
Year: 1971
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Apidae
Psithyrus
Psithyrus norvegicus

description: 6. Ps. norvegicus Sparre- Schneider, 1918 Flugzeit: ♂ 10. 5. 1969. — Diese erst 1918 beschriebene Art ist an­ scheinend in Deutschland weit verbreitet, dürfte aber überall eine Selten­ heit sein. Aus Deutschland wurden bisher nur wenige Fundorte bekannt (Stoeckhert 1933 u. 1954). Von A. C. W. Wagner (1937) und Alfken (1938) wurde kein Exemplar genannt. Ein Männchen konnte in Fanggebiet II. in dem. hypnorum 1969 erstmals ausserhalb menschlicher Siedlungen auf­ trat, am 10. 5. 1969 gefangen werden.
description: Published as part of Wagner, Rainer, 1971, Die Veränderung der Hummelfauna Cuxhavens in diesem Jahrhundert. Der Versuch einer Deutung.), pp. 207-232 in Ent. Mitt. Zool. Mus. Hamburg 4 (75) on page 218, DOI: 10.5281/zenodo.7289873
description: {"references": ["Stoeckhert, F. K., 1933: Die Bienen Frankens (Hym. Apid.). Eine okologisch- tiergeographische Untersuchung. - Dtsch. Ent. Zeitschr., Beiheft. Berlin."]}
Additional file 19 of Genome-scale analysis of Arabidopsis splicing-related protein kinase families reveals roles in abiotic stress adaptation
Creators: name: Rodriguez Gallo, M. C.
name: Li, Q.
name: Mehta, D.
name: Uhrig, R. G.
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 19.
The impact of cosmic variance on simulating weak lensing surveys
Creators: name: Kannawadi, Arun
name: Mandelbaum, Rachel
name: Lackner, Claire
Publisher: name: Figshare
Year: 2018
Subjects: subject: 20399 Classical Physics not elsewhere classified
subject: FOS: Physical sciences

description: Upcoming weak lensing surveys will survey large cosmological volumes to measure the growth of cosmological structure with time and thereby constrain dark energy. One major systematic uncertainty in this process is the calibration of the weak lensing shape distortions, or shears. Most upcoming surveys plan to test several aspects of their shear estimation algorithms using sophisticated image simulations that include realistic galaxy populations based on high-resolution data from the Hubble Space Telescope (HST). However, existing data sets from the HST cover very small cosmological volumes, so cosmic variance could cause the galaxy populations in them to be atypical. A narrow redshift slice from such surveys could be dominated by a single large overdensity or underdensity. In that case, the morphology–density relation could alter the local galaxy populations and yield an incorrect calibration of shear estimates as a function of redshift. We directly test this scenario using the COSMOS survey, the largest-area HST survey to date, and show how the statistical distributions of galaxy shapes and morphological parameters (e.g. Sérsicn) are influenced by redshift-dependent cosmic variance. The typical variation in rms ellipticity due to environmental effects is 5 per cent (absolute, not relative) for redshift bins of width Δz = 0.05, which could result in uncertain shear calibration at the 1 per cent level. We conclude that the cosmic variance effects are large enough to exceed the systematic error budget of future surveys, but can be mitigated with careful choice of training data set and sufficiently large redshift binning.
title: Algorithm for driver intention detection with Fuzzy Logic and Edit Distance
Creators: name: Heine, Jens
name: Sylla, Michael
name: Schramm, Thomas
name: Langer, Ingmar
name: Abendroth, Bettina
name: Bruder, Ralph
Publisher: name: IEEE
Year: 2023

description: Driver intention detection is helpful to parameterize advanced driver assistance systems to reduce the warning dilemma and so to raise the driver’s acceptance to such systems. An algorithm to predict driver’s intention with Fuzzy Logic and Edit Distance is presented. The main features and the functionality is explained. The necessary steps for training the algorithm and the validation are presented. The performance of the first configuration is discussed and the future steps for improving the performance are shown.
Test Particle Motion in the Born-Infeld Black Hole
Creators: name: Linares, Román
name: Maceda, Marco
name: Martínez-Carbajal, Daniel
Publisher: name: arXiv
Year: 2014
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this work we review the classification of geodesics of massive test particles in the gravitational background of the black hole solutions of Einstein-Born-Infeld spacetime. Even though some features are quite similar to those of Reissner-Nordström spacetime there are also important differences, particularly those related to the effective potential governing the geodesic motion. Explicit solutions involving Weierstrass functions are given for a pair of specific scenarios.
description: 10 pages, 8 figures
Neutrino Oscillations in Dark Matter
Creators: name: Choi, Ki-Young
name: Chun, Eung Jin
name: Jongkuk Kim
Publisher: name: Zenodo
Year: 2020

description: We study neutrino oscillations in a medium of dark matter which generalizes the standard matter effect. A general formula is derived to describe the effect of various mediums and their mediators to neutrinos. Neutrinos and anti-neutrinos receive opposite contributions from asymmetric distribution of (dark) matter and anti-matter, and thus it could appear in precision measurements of neutrino or anti-neutrino oscillations. Furthermore, it leads to an amusing possibility that neutrino oscillations can occur from the dark-matter-induced flavorful potential even for massless neutrinos.
title: Disentangling Capabilities for Industry 4.0 : An Information Systems Capability Perspective
Creators: name: Huber, Rocco
name: Oberländer, Anna Maria
name: Faisst, Ulrich
name: Röglinger, Maximilian
Publisher: name: University of Bayreuth
Year: 2022
Subjects: subject: Industry 4.0
subject: Fourth industrial revolution
subject: Information Systems capabilities
subject: Capability framework
subject: 004
subject: 330

description: Digital technologies revolutionise the manufacturing industry by connecting the physical and digital worlds. The resulting paradigm shift, referred to as Industry 4.0, impacts manufacturing processes and business mod-els. While the ‘why’ and ‘what’ of Industry 4.0 have been extensively researched, the ‘how’ remains poorly understood. Manufacturers struggle with exploiting Industry 4.0’s full potential as a holistic understanding of required Information Systems (IS) capabilities is missing. To foster such understanding, we present a holistic IS capability framework for Industry 4.0, including primary and support capabilities. After developing the framework based on a structured literature review, we refined and evaluated it with ten Industry 4.0 experts from research and practice. We demonstrated its use with a German machinery manufacturer. In sum, we con-tribute to understanding and analysing IS capabilities for Industry 4.0. Our work serves as a foundation for further theorising on Industry 4.0 and for deriving theory-led design recommendations for manufacturers.
The MassiveBlack-II simulation: the evolution of haloes and galaxies to z ∼ 0
Creators: name: Nishikanta  Khandai
name: Matteo, Tiziana Di
name: Croft, Rupert
name: Wilkins, Stephen
name: Feng, Yu
name: Tucker, Evan
name: DeGraf, Colin
name: Liu, Mao-Sheng
Publisher: name: Figshare
Year: 2018
Subjects: subject: 20399 Classical Physics not elsewhere classified
subject: FOS: Physical sciences

description: We investigate the properties of haloes, galaxies and black holes to z = 0 in the high-resolution hydrodynamical simulation MassiveBlack-II (MBII) which evolves a Λ cold dark matter cosmology in a comoving volumeVbox = (100 Mpc h−1)3. MBII is the highest resolution simulation of this size which includes a self-consistent model for star formation, black hole accretion and associated feedback. We provide a simulation browser web application which enables interactive search and tagging of the MBII data set and publicly release our galaxy catalogues. We find that baryons affect strongly the halo mass function (MF), with 20–33 per cent change in the halo abundance below the knee of the MF (Mhalo < 1013.2 M⊙ h−1 at z = 0) when compared to dark-matter-only simulations. We provide a fitting function for the halo MF out to redshift z = 11 and discuss its limitations. We study the halo occupation distribution and clustering of galaxies, in particular the evolution and scale dependence of stochasticity and bias finding reasonable agreement with observational data. The shape of the cosmic spectral energy distribution of galaxies in MBII is consistent with observations, but lower in amplitude. The Galaxy stellar mass function (GSMF) function is broadly consistent with observations at z ≥ 2. At z < 2, the population of passive low-mass (M* < 109 M⊙) galaxies in MBII makes the GSMF too steep compared to observations whereas at the high-mass end (M* > 1011 M⊙) galaxies hosting bright AGNs make significant contributions to the GSMF. The quasar bolometric luminosity function is also largely consistent with observations. We note however that more efficient AGN feedback is necessary for the largest, rarest objects/clusters at low redshifts.
Additional file 1 of Genome-scale analysis of Arabidopsis splicing-related protein kinase families reveals roles in abiotic stress adaptation
Creators: name: Rodriguez Gallo, M. C.
name: Li, Q.
name: Mehta, D.
name: Uhrig, R. G.
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 1.
Quasiparticle interfacial level alignment of highly hybridized frontier levels: H$_2$O on TiO$_2$(110)
Creators: name: Migani, Annapaola
name: Mowbray, Duncan J.
name: Zhao, Jin
name: Petek, Hrvoje
Publisher: name: arXiv
Year: 2015
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Knowledge of the frontier levels' alignment prior to photo-irradiation is necessary to achieve a complete quantitative description of H$_2$O photocatalysis on TiO$_2$(110). Although H$_2$O on rutile TiO$_2$(110) has been thoroughly studied both experimentally and theoretically, a quantitative value for the energy of the highest H$_2$O occupied levels is still lacking. For experiment, this is due to the H$_2$O levels being obscured by hybridization with TiO$_2$(110) levels in the difference spectra obtained via ultraviolet photoemission spectroscopy (UPS). For theory, this is due to inherent difficulties in properly describing many-body effects at the H$_2$O-TiO$_2$(110) interface. Using the projected density of states (DOS) from state-of-the-art quasiparticle (QP) $G_0W_0$, we disentangle the adsorbate and surface contributions to the complex UPS spectra of H$_2$O on TiO$_2$(110). We perform this separation as a function of H$_2$O coverage and dissociation on stoichiometric and reduced surfaces. Due to hybridization with the TiO$_2$(110) surface, the H$_2$O 3a$_1$ and 1b$_1$ levels are broadened into several peaks between 5 and 1 eV below the TiO$_2$(110) valence band maximum (VBM). These peaks have both intermolecular and interfacial bonding and antibonding character. We find the highest occupied levels of H$_2$O adsorbed intact and dissociated on stoichiometric TiO$_2$(110) are 1.1 and 0.9 eV below the VBM. We also find a similar energy of 1.1 eV for the highest occupied levels of H$_2$O when adsorbed dissociatively on a bridging O vacancy of the reduced surface. In both cases, these energies are significantly higher (by 0.6 to 2.6 eV) than those estimated from UPS difference spectra, which are inconclusive in this energy region. Finally, we apply self-consistent QP$GW$ (scQP$GW$1) to obtain the ionization potential of the H$_2$O-TiO$_2$(110) interface.
description: 12 pages, 12 figures, 1 table
The Role of the Positively Charged Amino Acids in Bacteriorhodopsin
Creators: name: Tristram, Stephanie Ann
Publisher: name: Figshare
Year: 2018
Subjects: subject: 20399 Classical Physics not elsewhere classified
subject: FOS: Physical sciences

description: This study has used chemical modification techniques to
investigate the role of the only two types of positively charged
amino acids, lysines and arginines, in the membrane-bound protein,
bacteriorhodopsin (bR). The results of these chemical modifications
have significance both for the structure of bR and for the molecular
mechanism of light-activated photocycling and proton pumping.
The implications for the secondary structure of bR are:
LYS 40 is totally exposed to the aqueous phase, while the other
five reactive lysines are partially buried in the hydrophobic domain;
LYS 30, LYS 129 and LYS 159 are buried by only one or two residues
within the hydrophobic domain; all but two arginines are totally
exposed to the aqueous phase; and at least three ionic bridges form
between arginines and carboxyl groups. These results were used to
construct a new model of the secondary structure of bR. The implication
for the tertiary structure of bR is that Model A (126) is
the preferred model of fitting the bR sequence into the helices seen
by electron diffraction. The implication for the quaternary structure
is that one structural role of retinal is to increase the intermolecular
distances between bR molecules in a trimer. This focuses
attention on the bR trimer as the primary structural unit.

Regarding the molecular mechanism of photocycling and proton
pumping, two specific arginines were responsible for the slowdown of
the photocycle. This result was obtained by a quantitative analysis
of the inhibition of M decay as a function of fraction of arginines
modified by 2,3-butanedione. Possible roles of the two important
arginines, including controlling the conformational changes of the
protein by ionic linkages to carboxyl groups and participating directly
in proton pathways, are discussed. Bifunctional imidoester modification
of lysines revealed that a conformational change of the bR protein is
needed for photocycling, since cross-linking lysines slowed the photocycle.
2,3-Butanedione modification of arginines supported this
result, since this modification caused a marked slowdown of the photocycle
and also protein conformational changes as evidenced by
tryptophan fluorescence and circular dichroism spectroscopy.
A visual and neural evaluation of the affective impression on embodied conversational agents
Creators: name: Li, Fengxiang
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Psychology
subject: FOS: Psychology
subject: Operations Research, Systems Engineering and Industrial Engineering
subject: Engineering
subject: Social and Behavioral Sciences

description: This project is designed to explore the human visual and neural evaluation of the young people when they freely view embodied conversational agents. Several independennt variables are taken into account that affect human visual and neural evaluation.
Towards a space-based beyond 5G converged communications infrastructure
Creators: name: Gavras, Anastasius
Publisher: name: Zenodo
Year: 2022

description: This presentation introduces a study, funded by ESA, on how a 5G and beyond 5G space-based infrastructure can provide services for consumers and various industries meeting 5G key performance indicators in terms of performance, reliability, resilience, and security. The scope of the study encompasses the challenging task to propose a non-terrestrial network (NTN) infrastructure and its deployment scenarios to deliver advanced communication services in a timely and cost-efficient manner - converging towards a future Satcom technology roadmap in line with the emerging 6G concepts.
Force-induced rupture of a DNA duplex
Creators: name: Mosayebi, Majid
name: Louis, Ard A.
name: Doye, Jonathan P. K.
name: Ouldridge, Thomas E.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Biological Physics (physics.bio-ph)
subject: FOS: Physical sciences

description: The rupture of double-stranded DNA under stress is a key process in biophysics and nanotechnology. In this article we consider the shear-induced rupture of short DNA duplexes, a system that has been given new importance by recently designed force sensors and nanotechnological devices. We argue that rupture must be understood as an activated process, where the duplex state is metastable and the strands will separate in a finite time that depends on the duplex length and the force applied. Thus, the critical shearing force required to rupture a duplex within a given experiment depends strongly on the time scale of observation. We use simple models of DNA to demonstrate that this approach naturally captures the experimentally observed dependence of the critical force on duplex length for a given observation time. In particular, the critical force is zero for the shortest duplexes, before rising sharply and then plateauing in the long length limit. The prevailing approach, based on identifying when the presence of each additional base pair within the duplex is thermodynamically unfavorable rather than allowing for metastability, does not predict a time-scale-dependent critical force and does not naturally incorporate a critical force of zero for the shortest duplexes. Additionally, motivated by a recently proposed force sensor, we investigate application of stress to a duplex in a mixed mode that interpolates between shearing and unzipping. As with pure shearing, the critical force depends on the time scale of observation; at a fixed time scale and duplex length, the critical force exhibits a sigmoidal dependence on the fraction of the duplex that is subject to shearing.
description: 10 pages, 6 figures
Epistemic gratitude - Experiment 4
Creators: name: Karabegovich, Mia
name: Mercier, Hugo
name: Boyer, Pascal
name: Guley, Olha
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Psychology
subject: FOS: Psychology
subject: Social and Behavioral Sciences

description: In this experiment, we investigate whether one can attribute gratitude retroactively, when a piece of information that was initially rejected (due to lack of epistemic authority from the source) turns out to be correct and beneficial.
Filling of closed Surfaces
Creators: name: Sanki, Bidyut
Publisher: name: arXiv
Year: 2015
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics

description: Let $F_g$ denote a closed oriented surface of genus $g$. A set of simple closed curves is called a filling of $F_g$ if its complement is a disjoint union of discs. The mapping class group $\text{Mod}(F_g)$ of genus $g$ acts on the set of fillings of $F_g$. The union of the curves in a filling forms a graph on the surface which is a so-called decorated fat graph. It is a fact that two fillings of $F_g$ are in the same $\text{Mod}(F_g)$-orbit if and only if the corresponding fat graphs are isomorphic. We prove that any filling of $F_2$ whose complement is a single disc (i.e., a so-called minimal filling) has either three or four closed curves and in each of these two cases, there is a unique such filling up to the action of $\text{Mod}(F_2)$. We provide a constructive proof to show that the minimum number of discs in the complement of a filling pair of $F_2$ is two. Finally, given positive integers $g$ and $k$ with $(g, k)\neq (2, 1)$, we construct a filling pair of $F_g$ such that the complement is a union of $k$ topological discs.
description: 15 Pages, 11 Figures, To appear in J. Topol. Anal
Evolution of Mass-Mixing Parameters in Matter with Neutrino NSIs
Creators: name: Das, Sudipta
name: Mehedi Masud
name: Sanjib Kumar  Agarwalla
name: Pragyanprasu Swain
Publisher: name: Zenodo
Year: 2020

description: We explore the role of matter effect in the evolution of neutrino oscillation parameters in the presence of all possible lepton-flavour-conserving and lepton-flavour-violating non-standard interactions (NSIs) of the neutrino. We derive simple approximate analytical expressions for the mass-mixing parameters in matter in presence of NSIs. We observe that only the NSIs in 2-3 block($\varepsilon_{\mu\mu}, \varepsilon_{\tau\tau}$,and $\varepsilon_{\mu\tau}$) affect the running of $\theta_{23}$. Though all the NSIs influence the evolution of $\theta_{13}$, but, $\varepsilon_{e\mu}$ and $\varepsilon_{e\tau}$ have prominent impact at the energies relevant for DUNE. We demonstrate the utility of our approach in addressing several important features related to neutrino oscillation such as: a) estimating the resonance energy in presence of NSIs when $\theta_{13}$ in matter becomes maximal, b) figuring out the required baseline length and neutrino energies to have maximal matter effect in $\nu_{\mu}$ to $\nu_{e}$ transition, and c) unraveling interesting degeneracies between $\theta_{23}$ and NSI parameters.
Turbulent energy dissipation and intermittency in ambipolar diffusion magnetohydrodynamics
Creators: name: Momferratos, Georgios
name: Lesaffre, Pierre
name: Falgarone, Edith
name: Forêts, Guillaume Pineau des
Publisher: name: arXiv
Year: 2015
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: The dissipation of kinetic and magnetic energy in the interstellar medium (ISM) can proceed through viscous, Ohmic or ambipolar diffusion (AD). It occurs at very small scales compared to the scales at which energy is presumed to be injected. This localized heating may impact the ISM evolution but also its chemistry, thus providing observable features. Here, we perform 3D spectral simulations of decaying magnetohydrodynamic turbulence including the effects of AD. We find that the AD heating power spectrum peaks at scales in the inertial range, due to a strong alignment of the magnetic and current vectors in the dissipative range. AD affects much greater scales than the AD scale predicted by dimensional analysis. We find that energy dissipation is highly concentrated on thin sheets. Its probability density function follows a lognormal law with a power-law tail which hints at intermittency, a property which we quantify by use of structure function exponents. Finally, we extract structures of high dissipation, defined as connected sets of points where the total dissipation is most intense and we measure the scaling exponents of their geometric and dynamical characteristics: the inclusion of AD favours small sizes in the dissipative range.