cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey -- II. Survey status, pulsar census, and first pulsar discoveries
Creators: name: Bhat, N. D. R.
name: Swainston, N. A.
name: McSweeney, S. J.
name: Xue, M.
name: Meyers, B. W.
name: Kudale, S.
name: Dai, S.
name: Tremblay, S. E.
name: van Straten, W.
name: Shannon, R. M.
name: Smith, K. R.
name: Sokolowski, M.
name: Ord, S. M.
name: Sleap, G.
name: Williams, A.
name: Hancock, P. J.
name: Lange, R.
name: Tocknell, J.
name: Johnston-Hollitt, M.
name: Kaplan, D. L.
name: Tingay, S. J.
name: Walker, M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: In Paper I, we presented an overview of the Southern-sky MWA Rapid Two-metre (SMART) survey, including the survey design and search pipeline. While the combination of MWA's large field-of-view and the voltage capture system brings a survey speed of ~450 square degrees per hour, the survey progression relies on the availability of compact configuration of the Phase II array. Over the past few years, by taking advantage of multiple windows of opportunity when the compact configuration was available, we have advanced the survey to 75% completion. To date, about 10% of the data collected thus far have been processed for a first-pass search, where 10 minutes of observation is processed for dispersion measures out to 250 ${\rm pc\,cm^{-3}}$, to realise a shallow survey for long-period pulsars. The ongoing analysis has led to two new pulsar discoveries, as well as an independent discovery and a rediscovery of a previously incorrectly characterised pulsar, all from ~3% of the data for which candidate scrutiny is completed. Here we describe the strategies for further detailed follow-up including improved sky localisation and convergence to timing solution, and illustrate them using example pulsar discoveries. The processing has also led to re-detection of 120 pulsars in the SMART observing band, bringing the total number of pulsars detected to date with the MWA to 180, and these are used to assess the search sensitivity of current processing pipelines. The planned second-pass (deep survey) processing is expected to yield a three-fold increase in sensitivity for long-period pulsars, and a substantial improvement to millisecond pulsars by adopting optimal de-dispersion plans. The SMART survey will complement the highly successful Parkes High Time Resolution Universe survey at 1.2-1.5 GHz, and inform future large survey efforts such as those planned with the low-frequency Square Kilometre Array.
description: 22 pages, 9 figures, 7 tables, Accepted for publication in PASA
Inadequacy of fluvial energetics for describing gravity current autosuspension
Creators: name: Fukuda, Sojiro
name: de Vet, Marijke G. W.
name: Skevington, Edward W. G.
name: Bastianon, Elena
name: Fernandez, Roberto
name: Wu, Xuxu
name: McCaffrey, William D.
name: Naruse, Hajime
name: Parsons, Daniel R.
name: Dorrell, Robert M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: "Consider the [turbidity] current as ... a river" R. A. Bagnold (1962); the foundation of contemporary deep marine sedimentology. Gravity currents, such as sediment-laden turbidity currents, are ubiquitous natural flows that are driven by a density difference. Turbidity currents have provided vital motivation to advance understanding of this class of flows because their enigmatic long run-out and driving mechanisms are not properly understood. Extant models assume that material transport by gravity currents is dynamically similar to fluvial flows. Here, empirical research from different types of particle-driven gravity currents is integrated with our experimental data, to show that material transport is fundamentally different from fluvial systems. Contrary to current theory, buoyancy production is shown to have a non-linear dependence on available flow power, indicating an underestimation of the total kinetic energy lost from the mean flow. A revised energy budget directly implies that the mixing efficiency of gravity currents is enhanced.
description: Combined main text and supplemental notes. Main: 14 pages, 7 figures, 2 tables. Supplemental: 21 pages, 12 figures, 2 tables
"On the Road" - Reflections on the Security of Vehicular Communication Systems
Creators: name: Papadimitratos, P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cryptography and Security (cs.CR)
subject: FOS: Computer and information sciences

description: Vehicular communication (VC) systems have recently drawn the attention of industry, authorities, and academia. A consensus on the need to secure VC systems and protect the privacy of their users led to concerted efforts to design security architectures. Interestingly, the results different project contributed thus far bear extensive similarities in terms of objectives and mechanisms. As a result, this appears to be an auspicious time for setting the corner-stone of trustworthy VC systems. Nonetheless, there is a considerable distance to cover till their deployment. This paper ponders on the road ahead. First, it presents a distillation of the state of the art, covering the perceived threat model, security requirements, and basic secure VC system components. Then, it dissects predominant assumptions and design choices and considers alternatives. Under the prism of what is necessary to render secure VC systems practical, and given possible non-technical influences, the paper attempts to chart the landscape towards the deployment of secure VC systems.
title: On the design of smartphone based plant ID guides
Creators: name: Bewsey, Andrew
Publisher: name: University of Reading
Year: 2022

description: The work presented here is the exploration and discussion of multi-access smartphone-based plant ID guides. The aim of this work was to explore the possibilities of using detailed multi-access keys on smartphones to identify taxa in the field to a professional standard. This involved establishing the most effective method of gathering data, deciding on the best design, evaluating whether users prefer this design over traditional media, and establishing whether or not continuation of this project would be financially sound. As they represented the best source of information, the decision was taken to extract data from extant paper-based ID guides. Two methods were attempted, automatic extraction through pattern matching techniques, and manual extraction. The automatic extraction technique was tested as paper-based ID guides were thought to use a very regular language. It was found, however, that the language used was not regular enough, and manual input of data was required. The design of the app was built from the designs of existing apps, and the principles of ‘simple’ and ‘consistent’, which were found to be the main themes of many design guides. When the design was evaulated, it was well received, only requiring refinements. After several rounds of updates, the app reached about 30% accuracy, similar to traditional paper-based ID guides. The similarity in accuracy to paper-based ID guides is indicative of the difficulty in identification of Equisetum specimens, thus is a positive indication of the quality of the app. The app was preferred by users, who found it easier to use. When the costs of continuation of this project were examined, it was quickly found that, despite a potential market of several thousand, the production costs were simply too high. Continuation was therefore deemed to require financial assistance, via grants or otherwise. This leads to a final suggestion that species x character databases are published with all novel taxonomic works in a standardised format, and that this is a requirement of grant funded work.
Hidden shock powering the peak of SN 2020faa
Creators: name: Salmaso, I.
name: Cappellaro, E.
name: Tartaglia, L.
name: Benetti, S.
name: Botticella, M. T.
name: Elias-Rosa, N.
name: Pastorello, A.
name: Patat, F.
name: Reguitti, A.
name: Tomasella, L.
name: Valerin, G.
name: Yang, S.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The link between the fate of the most massive stars and the resulting supernova (SN) explosion is still a matter of debate, in major part because of the ambiguity among light-curve powering mechanisms. When stars explode as SNe, the light-curve luminosity is typically sustained by a central engine (radioactive decay, magnetar spin-down, or fallback accretion). However, since massive stars eject considerable amounts of material during their evolution, there may be a significant contribution coming from interactions with the previously ejected circumstellar medium (CSM). Reconstructing the progenitor configuration at the time of explosion requires a detailed analysis of the long-term photometric and spectroscopic evolution of the related transient. In this paper, we present the results of our follow-up campaign of SN 2020faa. Given the high luminosity and peculiar slow light curve, it is purported to have a massive progenitor. We present the spectro-photometric dataset and investigate different options to explain the unusual observed properties that support this assumption. We computed the bolometric luminosity of the supernova and the evolution of its temperature, radius, and expansion velocity. We also fit the observed light curve with a multi-component model to infer information on the progenitor and the explosion mechanism. Reasonable parameters are inferred for SN 2020faa with a magnetar of energy Ep=1.5(+0.5,-0.2)x10^50 erg and spin-down time t(spin)=15+/-1 d, a shell mass M(shell)=2.4(+0.5,-0.4) Msun and kinetic energy Ekin(shell)=0.9(+0.5,-0.3)x 10^51 erg, and a core with M(core)=21.5(+1.4,-0.7) Msun and Ekin(core)=3.9(+0.1,-0.4)x10^51 erg. In addition, we need an extra source to power the luminosity of the second peak. We find that hidden interaction with either a CSM disc or delayed, choked jets is a viable mechanism for supplying the required energy to achieve this effect.
description: 14 pages, 14 figures. Accepted to Astronomy & Astrophysics
title: ÐÐºÑÐ¸Ð²Ð¸Ð·Ð°ÑÐ¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ñ ÑÐµÐ»ÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¥Ð½ÑÐºÐ¸Ð½Ð°, ÐÐ»Ð¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð°ÐºÑÐ¸Ð²Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°
ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ
ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¸ Ð¾ÑÐµÐ½ÐºÐ°
Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ñ Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÐµÑÐ° Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð Ð¾ÑÑÐ¸Ð¸. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¾ÑÐ¼ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸ÑÑ Ð¿ÑÑÐµÐ¼ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÑÐºÐ¾-Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð° Ð¸ ÑÐ¾ÑÐ¼ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¸ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð². ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ»Ð¾Ð¶Ð¸Ð²ÑÐµÐ¹ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸ÐµÐ¹ Ð½Ð° ÑÑÐ½ÐºÐµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ ÑÑÐ»ÑÐ³ Ð² ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐµ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð·Ð½Ð°ÑÐ¸Ð¼ÑÐµ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° Ð¸ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸ ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÑÐºÐ¾-Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¾ÑÐ¼ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¸ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ ÑÑÐ°ÑÐ¸ÑÑÑ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ°ÑÐµÑÑÐ²Ð° Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð² ÑÑÐµÑÐµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐ¹ Ð½Ð° Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÐ°ÑÐ¸ÑÑÑ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° Ð°ÐºÑÐ¸Ð²Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÑÐºÐ¾-Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð° Ð¿ÑÑÐµÐ¼ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð¸ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð½Ð¾Ð²ÑÐ¹ Ð²Ð¸Ð´ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÑÑÐ°ÑÐ¸ÑÑÑ, ÑÑÐ¾ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÐ¾Ð²Ð½Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°.
A simple method for the evaluation of the information content and complexity in atoms. A proposal for scalability
Creators: name: Panos, C. P.
name: Nikolaidis, N. S.
name: Chatzisavvas, K. Ch.
name: Tsouros, C. C.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present a very simple method for the calculation of Shannon, Fisher, Onicescu and Tsallis entropies in atoms, as well as SDL and LMC complexity measures, as functions of the atomic number Z. Fractional occupation probabilities of electrons in atomic orbitals are employed, instead of the more complicated continuous electron probability densities in position and momentum spaces, used so far in the literature. Our main conclusions are compatible with the results of more sophisticated approaches and correlate fairly with experimental data. We obtain for the Tsallis entropic index the value q=1.031, which shows that atoms are very close to extensivity. A practical way towards scalability of the quantification of complexity for systems with more components than the atom is indicated. We also discuss the issue if the complexity of the electronic structure of atoms increases with Z. A Pair of Order-Disorder Indices (PODI), which can be introduced for any quantum many-body system, is evaluated in atoms. We conclude that "atoms are ordered systems, which do not grow in complexity as Z increases".
description: Preprint, 25 pages, 15 figures, 1 Table
Nuclei, Primes and the Random Matrix Connection
Creators: name: Firk, Frank W. K.
name: Miller, Steven J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Number Theory (math.NT)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 11M26, 15A52, 82D99

description: In this article, we discuss the remarkable connection between two very different fields, number theory and nuclear physics. We describe the essential aspects of these fields, the quantities studied, and how insights in one have been fruitfully applied in the other. The exciting branch of modern mathematics, random matrix theory, provides the connection between the two fields. We assume no detailed knowledge of number theory, nuclear physics, or random matrix theory; all that is required is some familiarity with linear algebra and probability theory, as well as some results from complex analysis. Our goal is to provide the inquisitive reader with a sound overview of the subjects, placing them in their historical context in a way that is not traditionally given in the popular and technical surveys.
description: 54 pages, 11 images
Dependence on dilution of critical and compensation temperatures of a two dimensional mixed spin-1/2 and spin-1 system
Creators: name: Aydiner, E.
name: Yuksel, Y.
name: Kis-Cam, E.
name: Polat, H.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: In this study, dependence on site dilution of critical and compensation temperatures of a two dimensional mixed spin-1/2 and spin-1 system has been investigated with Monte Carlo simulation. The dependence of the thermal and magnetic behaviors on dilution of mixed spin system have been discussed. We have shown that the critical and compensation temperatures of diluted mixed spin system linearly decrease with increasing number of diluted sites.
description: 5 pages, 8 figures
JWST Observations of the Enigmatic Y Dwarf WISE 1828+2650: I. Limits to a Binary Companion
Creators: name: De Furio, Matthew
name: Lew, Ben W.
name: Beichman, Charles A.
name: Roellig, Thomas
name: Bryden, Geoffrey
name: Ciardi, David R.
name: Meyer, Michael R.
name: Rieke, Marcia J.
name: Greenbaum, Alexandra Z.
name: Leisenring, Jarron
name: Llop-Sayson, Jorge
name: Ygouf, Marie
name: Albert, Loïc
name: Boyer, Martha L.
name: Eisenstein, Daniel J.
name: Hodapp, Klaus W.
name: Horner, Scott
name: Johnstone, Doug
name: Kelly, Douglas M.
name: Misselt, Karl A.
name: Rieke, George H.
name: Stansberry, John A.
name: Young, Erick T.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The Y-dwarf WISE 1828+2650 is one of the coldest known Brown Dwarfs with an effective temperature of $\sim$300 K. Located at a distance of just 10 pc, previous model-based estimates suggest WISE1828+2650 has a mass of $\sim$5-10 Mj, making it a valuable laboratory for understanding the formation, evolution and physical characteristics of gas giant planets. However, previous photometry and spectroscopy have presented a puzzle with the near-impossibility of simultaneously fitting both the short (0.9-2.0 microns) and long wavelength (3-5 microns) data. A potential solution to this problem has been the suggestion that WISE 1828+2650 is a binary system whose composite spectrum might provide a better match to the data. Alternatively, new models being developed to fit JWST/NIRSpec and MIRI spectroscopy might provide new insights. This article describes JWST/NIRCam observations of WISE 1828+2650 in 6 filters to address the binarity question and to provide new photometry to be used in model fitting. We also report Adaptive Optics imaging with the Keck 10 m telescope. We find no evidence for multiplicity for a companion beyond 0.5 AU with either JWST or Keck. Companion articles will present low and high resolution spectra of WISE 1828+2650 obtained with both NIRSpec and MIRI.
description: 15 pages, 9 figures, Accepted by ApJ on Feb. 21 2023
title: Phylogenetics and characterisation of Lamiaceae tribe Ocimeae, subtribe Ociminae
Creators: name: Althobaiti, Ashwaq T.
Publisher: name: University of Reading
Year: 2024

description: Phylogenetic analyses of the subtribe Ociminae (Lamiaceae) based on four plastid DNA regions (trnL–trnF intergenic spacer, trnH-psbA intergenic spacer, matK and rps16 intron) and two nuclear DNA regions (ITS and ETS) are presented. Bayesian inference was utilized for the reconstruction of phylogenies and for the assessment of statistical support for clades. The phylogeny was used for the investigation of the clade in terms of the distribution of morphology and geography. The subtribe Ociminae is monophyletic and can be simply diagnosed by morphological synapomorphies and is of African origin. The results clarify the relationships among Orthosiphon and its related genera Fuerstia and Hoslundia. Orthosiphon is monophyletic with exclusion Or. fruticosus, and it is a sister to Fuerstia and Hoslundia. Because Fuerstia and Hoslundia formed a monophyletic group with high morphological similarity between them, these genera will be merged under the earliest name Hoslundia. Ocimum is monophyletic with the inclusion of subgenus Nautochilus. Ocimum subgenus Nautochilus is a sister to the rest of Ocimum (subgenus Ocimum and subgenus Gymnocimum). Surprisingly, Orthosiphon fruticosus is a member of subgenus Nautochilus and highly supported, therefore, nomenclatural changes are required if the groups are to remain monophyletic. Analysis displayed strong congruence between the combinable component consensus trees and the traditional classification for most of genera and the results supported by morphological and geographic distribution. However, more taxon sampling to cover some regions of geography missed in this study is required. Moreover, the efficiency of ITS, matK, trnH-psbA and in combination for species identification of Orthosiphon was assessed. For DNA barcode analysis, the determination of intraspecific and interspecific divergence, assessment of barcoding gap, reconstruction of phylogenetic trees and evaluation of barcode regions for species identification (based on best match and best close match) were carried out. The results revealed that ITS is a significant barcode region for identifying Orthosiphon species as a single marker and, for the combination, ITS+matK+trnH-psbA.
Optical Resonators in Current and Future Experiments of the ALPS Collaboration
Creators: name: Meier, T.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Optics (physics.optics)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The ALPS collaboration runs a "light shining through a wall" (LSW) experiment to search for weakly interacting sub-eV particles (WISPs). Its sensitivity is significantly enhanced by the incorporation of a large-scale production resonator and a small-scale high-power resonant second harmonic generator. Here we report on important experimental details and limitations of these resonators and derive recommendations for further experiments. A very promising improvement for a future ALPS experiment is the incorporation of an additional large-scale regeneration resonator. We present a rough sketch of how to combine a regeneration resonator with a single-photon counter (SPC) as detector for regenerated photons.
description: 7 pages; Proceedings paper of the Axions 2010 workshop, Gainesville, FL, USA
Tuning non-linear charge transport between integer and fractional quantum Hall states
Creators: name: Roddaro, Stefano
name: Paradiso, Nicola
name: Pellegrini, Vittorio
name: Biasiol, Giorgio
name: Sorba, Lucia
name: Beltram, Fabio
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Controllable point junctions between different quantum Hall phases are a necessary building block for the development of mesoscopic circuits based on fractionally-charged quasiparticles. We demonstrate how particle-hole duality can be exploited to realize such point-contact junctions. We show an implementation for the case filling factors $ν=1$ and $ν^*\le1$ in which both the fractional filling $ν^*$ and the coupling strength can be finely and independently tuned. A peculiar crossover from insulating to conducting behavior as $ν^*$ goes from 1/3 to 1 is observed. These results highlight the key role played on inter-edge tunneling by local charge depletion at the point contact.
description: 4 pages, 3 figures, suppl.mat
title: The role of Staphylococcus aureus FadB in resistance to bile
Creators: name: Alsultan, Amjed
Publisher: name: University of Reading
Year: 2022

description: Resistance to the bactericidal effects of bile is crucial for the survival of Staphylococcus aureus in the human gut. This study was conducted to identify and characterize components of the bacteria, which allow it to resist bile acids. A comparative study was used to investigate the natural protein diversity within the Staphylococcus in relation to bile resistance. Imaging of one-dimension gel electrophoresis showed a unique protein band in samples prepared from bile-treated S. aureus. Mass spectrometry and database analysis showed the protein to be FadB. which has a role in lipid metabolism in Escherichia coli. It is hypothesized that fadB was responsible for the observed bile salt resistance phenotype; to test this, a ΔfadB strain was created in S. aureus SH1000. The mutant phenotype showed a significant decrease in viability upon exposure to bile acids in comparison with the parental wild type. Furthermore, survival of S. aureus ΔfadB was attenuated in an in vitro human colonic model, implicating fadB in S. aureus colonization of the human intestine. Moreover, upregulated expression of fadB was detected upon exposure to bile salts. To further confirm the role of FadB in bile salt resistance, the gene was cloned under the control of an inducible promoter, which enabled arabinose-dose dependent expression of fadB in E. coli JW113 as a heterologous host, confirming a bile resistant phenotype. Recombinant FadB was purified and shown to have affinity for cholic acid and might possess an ability to modify bile salts.
Towards quantifying Taiji Qigong: development of a feedback system
Creators: name: Baldinger, Melanie
name: Lippmann, Kevin
name: Lisca, Gheorghe
name: Senner, Veit
Publisher: name: Loughborough University
Year: 2024

description: Engineering of Sport 15 - Proceedings from the 15th International Conference on the Engineering of Sport (ISEA 2024)
The rapid digitalization in various domains has yet to leave sports untouched, where technology has been employed for automated event recognition and assessment. However, in the consumer realm, trainees rely on human observation and coaching, whereby incorrect exercise execution poses injury risks and diminishes exercise effectiveness. This research explores the capturable parameters of the developed Taiji Qigong (Qi) motioncapturing (MoCap) system (cf. “Development of a motion capture system to quantify Taji Qigong exercises”) with respect to possible feedback (FB) parameters. Thereby machine learning's potential for classifying movements and viable sensor options are investigated, along with the needs of Qi beginners (B) and masters (M) using qualitative interviews. A series of studies (S1-5) provide valuable insights into assessing Qi and offering personalized FB to B and evaluating M.
title: ÐÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ½Ð°Ñ ÑÐ¿ÐµÐºÑÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ñ ÑÐ³Ð»ÐµÑÐ¾Ð´Ð½ÑÑ Ð½Ð°Ð½Ð¾ÑÐ¾ÑÐµÐº
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ±Ð°ÑÐ¾Ð², ÐÐ°ÑÐº
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ñ
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description: ÐÐ·ÑÑÐµÐ½Ð° Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ñ ÑÐ³Ð»ÐµÑÐ¾Ð´Ð½ÑÑ Ð½Ð°Ð½Ð¾ÑÐ¾ÑÐµÐº, Ð¿Ð¾Ð»ÑÑÐµÐ½ÑÑ Ð¿ÑÑÑÐ¼ Ð¿Ð¸ÑÐ¾Ð»Ð¸Ð·Ð° Ð°Ð¼Ð¸Ð½Ð¾Ð¿ÑÐ¾Ð¿Ð¸Ð»ÑÑÐ¸ÑÑÐ¾ÐºÑÐ¸ÑÐ¸Ð»Ð°Ð½Ð° (APTES) Ð² Ð½Ð°Ð½Ð¾Ð¿Ð¾ÑÐ°Ñ Ð¼Ð°ÑÑÐ¸ÑÑ Ð¼ÐµÐ·Ð°Ð¿Ð¾ÑÐ¸ÑÑÐ¾Ð³Ð¾ ÐºÑÐµÐ¼Ð½ÐµÐ·ÑÐ¼Ð° (SiO2). ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ ÑÑÐ´Ð° Ð²Ð½ÐµÑÐ½Ð¸Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð½Ð° ÑÐ¿ÐµÐºÑÑÑ Ð¸Ð·Ð»ÑÑÐµÐ½Ð¸Ñ Ð½Ð°Ð½Ð¾ÑÐ¾ÑÐµÐº, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÑÐµÐºÑ ÑÐ¾ÑÐ¾Ð¸Ð½Ð´ÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ð¸. ÐÐ»Ð¸ÑÐ½Ð¸Ðµ Ð¸Ð½ÑÐµÐ½ÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð½Ð°ÐºÐ°ÑÐºÐ¸ Ð½Ð° Ð¸Ð½ÑÐµÐ½ÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐ»ÑÐ¾ÑÐµÑÑÐµÐ½ÑÐ¸Ð¸ Ð½Ð°Ð½Ð¾ÑÐ¾ÑÐµÐº Ð¾Ð±ÑÑÑÐ½ÐµÐ½Ð¾ Ð² ÑÐ°Ð¼ÐºÐ°Ñ ÑÑÑÑÑÑÐ¾Ð²Ð½ÐµÐ²Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸, ÑÑÐ¸ÑÑÐ²Ð°ÑÑÐµÐ¹ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° Ð¸Ð½ÑÐµÐ½ÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐ»ÑÐ¾ÑÐµÑÑÐµÐ½ÑÐ¸Ð¸ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÑÐ»ÑÐ¾ÑÐµÑÑÐµÐ½ÑÐ½Ð¾Ð³Ð¾ (ÑÐ¸Ð½Ð³Ð»ÐµÑÐ½Ð¾Ð³Ð¾) ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¸ Ð½Ð¸Ð¶ÐµÐ»ÐµÐ¶Ð°ÑÐµÐ³Ð¾ ÑÑÐ¸Ð¿Ð»ÐµÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ.
Paradigmatic examples for testing models of optical light polarization by spheroidal dust
Creators: name: Peest, C.
name: Siebenmorgen, R.
name: Heymann, F.
name: Vannieuwenhuyse, T.
name: Baes, M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a general framework on how the polarization of radiation due to scattering, dichroic extinction, and birefringence of aligned spheroidal dust grains can be implemented and tested in 3D Monte Carlo radiative transfer (MCRT) codes. We derive a methodology for solving the radiative transfer equation governing the changes of the Stokes parameters in dust-enshrouded objects. We utilize the Müller matrix, and the extinction, scattering, linear, and circular polarization cross sections of spheroidal grains as well as electrons. An established MCRT code is used and its capabilities are extended to include the Stokes formalism. We compute changes in the polarization state of the light by scattering, dichroic extinction, and birefringence on spheroidal grains. The dependency of the optical depth and the albedo on the polarization is treated. The implementation of scattering by spheroidal grains both for random walk steps as well as for directed scattering (peel-off) are described. The observable polarization of radiation of the objects is determined through an angle binning method for photon packages leaving the model space as well as through an inverse ray-tracing routine for the generation of images. We present paradigmatic examples for which we derive analytical solutions of the optical light polarization by spheroidal dust particles. These tests are suited for benchmark verification of MCpol and other such codes, and allow to quantify the numerical precision reached. We demonstrate that MCpol is in excellent agreement to within 0.1% of the Stokes parameters when compared to the analytical solutions.
description: A&A accepted by Editor
title: Investigating Saudi English language teachers' use and perceptions of the interactive whiteboard for teaching vocabulary in English as a foreign language in Saudi primary schools
Creators: name: Alshaikhi, Mohammed A.
Publisher: name: University of Reading
Year: 2021

description: Teaching vocabulary is a fundamental factor in English language teaching, as breadth of vocabulary is closely related to success in other areas of language learning such as reading, writing, speaking and listening. ICT has a potentially important role in teaching vocabulary within English as a foreign language, including through such media as the Interactive WhiteBoard (IWB), offering as it does a range of presentation formats that may facilitate the deeper and more effective processing of language. Despite this, relatively little is known about how teachers actually use the IWB, or indeed how they perceive it as a teaching tool. Understanding these issues is important in terms of informing the future development of the training offered to teachers in the use of the IWB. The current study includes the use of mixed methods, including a survey (319 responses). Six teachers participated in the qualitative part of the research, with four classroom observations of six teachers at three private and three state primary schools, followed by interviews with these same teachers. For the quantitative research, frequencies and descriptive statistics were computed to give an overview of teachers' reported use of the IWB and their attitudes towards it. Spearman Rank Order correlations and Mann-Whitney U-tests were employed in order to explore the relationships between key variables and whether different groups of respondents reported different perceptions and uses of the IWB. Teachers' perceptions and uses of the IWB were then further explored through a qualitative analysis of the interviews and classroom observations. Three complementary theoretical frameworks underpinned the study design and data analysis: Borg's (2003) work exploring language teachers' cognition and mental lives; the "Levels of Processing Hypothesis" (Craik & Lockhart, 1972) that outlines principles for vocabulary acquisition and retention; and Social-Cultural theory (Vygotsky, 1978), which guided the exploration of the classroom environment and how teachers scaffold learning from a low level to a high level through the IWB. The findings of this present study suggest a positive relationship between teachers' levels of skill/training in ICT and the frequency with which they make use of the IWB and the range of strategies for teaching vocabulary. The observations revealed that teachers who were trained in III ICT tended to use more varied teaching methods than those with less developed ICT skills. The interview analysis suggests that the majority of teachers believed that the use of the IWB in lessons assisted them in improving their students' new vocabulary retention. These findings make an important contribution to the field of educational technology for language learning by emphasising the link between training in ICT and the development of language teaching pedagogy.
Capability of Cherenkov Telescopes to Observe Ultra-fast Optical Flares
Creators: name: Deil, C.
name: Domainko, W.
name: Hermann, G.
name: Clapson, A. -C.
name: Förster, A.
name: van Eldik, C.
name: Hofmann, W.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The large optical reflector (~ 100 m^2) of a H.E.S.S. Cherenkov telescope was used to search for very fast optical transients of astrophysical origin. 43 hours of observations targeting stellar-mass black holes and neutron stars were obtained using a dedicated photometer with microsecond time resolution. The photometer consists of seven photomultiplier tube pixels: a central one to monitor the target and a surrounding ring of six pixels to veto background events. The light curves of all pixels were recorded continuously and were searched offline with a matched-filtering technique for flares with a duration of 2 us to 100 ms. As expected, many unresolved (<3 us) and many long (>500 us) background events originating in the earth's atmosphere were detected. In the time range 3 to 500 us the measurement is essentially background-free, with only eight events detected in 43 h; five from lightning and three presumably from a piece of space debris. The detection of flashes of brightness ~ 0.1 Jy and only 20 us duration from the space debris shows the potential of this setup to find rare optical flares on timescales of tens of microseconds. This timescale corresponds to the light crossing time of stellar-mass black holes and neutron stars.
description: Accepted for publication in Astroparticle Physics, 8 pages, 9 figures, 1 table
title: ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð¾Ð¶Ð¸Ð´Ð°ÐµÐ¼Ð¾Ð³Ð¾ ÑÑÐµÑÐ±Ð° Ð¿ÑÐ¸ ÑÐ°Ð·ÑÑÑÐµÐ½Ð¸Ð¸ Ð¿Ð»Ð¾ÑÐ¸Ð½ Ð³Ð¸Ð´ÑÐ¾ÑÐ·Ð»Ð¾Ð² Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¡Ð°ÑÐ½Ð¾-Ð¨ÑÑÐµÐ½ÑÐºÐ¾Ð¹ ÐÐ­Ð¡
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸ÑÐ°Ð¹Ð»Ð¾Ð²Ð°, ÐÐ°ÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð³Ð¸Ð´ÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸
Ð¡Ð°ÑÐ½Ð¾-Ð¨ÑÑÐµÐ½ÑÐºÐ°Ñ ÐÐ­Ð¡
ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÐµ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸
Ð³Ð¸Ð´ÑÐ¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ
Ð²Ð¾Ð»Ð½Ð° Ð¿ÑÐ¾ÑÑÐ²Ð°
HPS
emergencies
hydraulic structures
break wave

description: ÐÐ¾Ð»Ð½Ð° Ð¿ÑÐ¾ÑÑÐ²Ð° - Ð¾Ð´Ð½Ð° Ð¸Ð· Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð¾Ð¿Ð°ÑÐ½ÑÑ Ð¿ÑÐ¸ÑÐ¾Ð´Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½Ð¾ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐµÐ¹. ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ Ð½Ð° Ð¾ÑÐ¾Ð±Ð¾ Ð¾Ð¿Ð°ÑÐ½Ð¾Ð¼ Ð¾Ð±ÑÐµÐºÑÐµ - Ð¡Ð°ÑÐ½Ð¾-Ð¨ÑÑÐµÐ½ÑÐºÐ¾Ð¹ ÐÐ­Ð¡. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð¾ÑÐµÐ½Ð¸ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð² Ð½Ð¸Ð¶Ð½ÐµÐ¼ Ð±ÑÐµÑÐµ Ð¡Ð°ÑÐ½Ð¾-Ð¨ÑÑÐµÐ½ÑÐºÐ¾Ð¹ ÐÐ­Ð¡. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¸ÑÑ Ð´Ð°Ð½Ð½ÑÐµ Ð¾ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ°Ñ Ð¿Ð»Ð¾ÑÐ¸Ð½ Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð Ð¤.
description: Break wave - is one of the most dangerous natural processes; its forecasting is an extremely urgent task. An object of the research is the industrial security on a particularly dangerous object - the Sayano-Shushenskaya HPP. The aim of the work is to evaluate the possibility of increasing the safety of objects in the downstream of the power plant. In the work were used data of the characteristics of the dams on the territory of the Russian Federation.
Negative R$\acute{\text{e}}$nyi entropy and Brane intersection
Creators: name: Tian, Jia
name: Xu, Xiaoge
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this work, we revisit the calculation of R$\acute{\text{e}}$nyi entropy in AdS$_3$/(B)CFT$_2$. We find that gravity solutions brane intersection will lead to negative R$\acute{\text{e}}$nyi entropy.
description: 24 pages, 6 figures
title: ÐÑÐ»Ð¸Ð²ÐºÐ¸ Ð¸Ð· Ð¼ÐµÐ´Ð¸ Ð¸ Ð¼ÐµÐ´Ð½ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð². Ð§. 1
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¯ÑÐ¾Ð¿Ð¾Ð»Ð¾Ð², ÐÐ²Ð°Ð½
name: ÐÐµÑÐ²ÐµÑÐ°ÐµÐ², ÐÐ½Ð°ÑÐ¾Ð»Ð¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐÐ£
Year: 2004
Subjects: ÐÑÐ»Ð¸Ð²ÐºÐ¸ Ð¼ÐµÐ´Ð½ÑÐµ
ÐÐµÐ´Ð½ÑÐµ ÑÐ¿Ð»Ð°Ð²Ñ

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐ°ÐµÑÑÑ Ð´Ð»Ñ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð², Ð¼Ð°ÑÑÐµÑÐ¾Ð² Ð¸ Ð²ÑÑÐ¾ÐºÐ¾ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ°Ð±Ð¾ÑÐ¸Ñ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ². Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ Ð² ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸Ð¸ 000 Â«ÐÐ¸ÑÐµÐ¹Ð½Ð°Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ "ÐÐÐ¢ÐÐÐ ÐÐ ÐÐÐÐÐ¢"Â» (ÐÐ¸ÑÐµÐ½Ð·Ð¸Ñ â 567 Ð¾Ñ 31.08.2001 Ð³. ÐÐ¾Ð¼Ð¸ÑÐµÑÐ° Ð¿Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ) Ð¿Ð¾ Ð°Ð´ÑÐµÑÑ: 198097, Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³, ÑÐ». Ð¢ÑÐµÑÐ¾Ð»ÐµÐ²Ð°, Ð´. 2. Ð¢ÐµÐ»./ÑÐ°ÐºÑ 252-10-32.
Dual central point theorems and their generalizations
Creators: name: Karasev, R. N.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 52A35, 52C35, 55M35

description: We prove some analogues of the central point theorem and Tverberg's theorem, where instead of points, we consider hyperplanes or affine flats of given dimension.
description: This is a revised version, compared to the journal publication. Some errors were corrected, and references were added
title: ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð¾Ð´Ð½Ð¾-ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÐÐ­Ð¡ Sihwa
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¶Ð°ÑÐ°ÑÐºÑÐ»Ð¸ÐµÐ²Ð°, ÐÐµÑÐ¾Ð½Ð¸ÐºÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÐÐ¸Ð´ÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸ Ð¿ÑÐ¸Ð»Ð¸Ð²Ð½ÑÐµ
Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÐÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð²Ð¾Ð´Ð½Ð¾-ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ
ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐ°Ð±Ð¾ÑÑ
water and energy calculations
modes of operation

description: Ð ÑÐ°Ð¼ÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð²Ð¾Ð´Ð½Ð¾-ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÑÐµÑÐ¾Ð² Ð¿Ð¾ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¶Ð¸Ð¼Ð° ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¸Ð»Ð¸Ð²Ð½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸ Ð¸ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÐµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð² ÑÑÐµÐ´Ðµ Excel. ÐÐ¾Ð´ÐµÐ»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð´Ð»Ñ Ð¾Ð´Ð½Ð¾ÑÑÐ¾ÑÐ¾Ð½Ð½ÐµÐ³Ð¾ Ð¸ Ð´Ð²ÑÑÑÑÐ¾ÑÐ¾Ð½Ð½ÐµÐ³Ð¾ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ°Ð±Ð¾ÑÑ. Ð ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð¼Ð¾Ð´ÐµÐ»ÑÐ¼Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ ÑÐ°ÑÑÐµÑÐ° ÑÐµÐ¶Ð¸Ð¼Ð° ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¸Ð»Ð¸Ð²Ð½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸ Ñ ÐµÐ³Ð¾ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸ÐµÐ¹. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ Ð²Ð¾Ð´Ð½Ð¾-ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¡Ð¸ÑÐ²Ð¸Ð½ÑÐºÐ¾Ð¹ Ð¿ÑÐ¸Ð»Ð¸Ð²Ð½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸ Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸ÐµÐ¹ ÑÐµÐ¶Ð¸Ð¼Ð° ÑÐ°Ð±Ð¾ÑÑ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ Ð¾Ð´Ð½Ð¾ÑÑÐ¾ÑÐ¾Ð½Ð½ÐµÐ³Ð¾ Ð¸ Ð´Ð²ÑÑÑÑÐ¾ÑÐ¾Ð½Ð½ÐµÐ³Ð¾ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ°Ð±Ð¾ÑÑ. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° ÑÑÐµÐ¿ÐµÐ½Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÑÐµÐ¶Ð¸Ð¼Ð° ÑÐ°Ð±Ð¾ÑÑ Ð½Ð° Ð²ÑÑÐ°Ð±Ð¾ÑÐºÑ, Ð¾Ð±ÑÐµÐ¼ ÑÑÐ¾ÐºÐ° Ð² ÑÑÑÐ±Ð¸Ð½Ð½Ð¾Ð¼ ÑÐµÐ¶Ð¸Ð¼Ðµ Ð¸ ÑÑÐµÐ´Ð½ÐµÐ²Ð·Ð²ÐµÑÐµÐ½Ð½ÑÐ¹ Ð½Ð°Ð¿Ð¾Ñ. ÐÐ°Ð¹Ð´ÐµÐ½Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐµ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ Ð½Ð°Ð¿Ð¾ÑÐ¾Ð² Ð¿ÑÑÐºÐ° Ð¸ Ð¾ÑÑÐ°Ð½Ð¾Ð²Ð°.
description: As part of this project the method of water-energy calculations for justification of tidal power station's mode was developed. Based on this method the computer models for one-side and double-side modes were designed using Excel. According to these models the algorithm of tidal power station's operating mode was proposed. Water-energy calculations were performed for Sihwa tidal power station with optimization of parameters afterwards. In additions, the comparison of working mode on production, flow amount in turbine mode and average pressure was estimated. Then optimal values of start and stop pressures were calculated.
Candesartan Attenuates Ischemic Brain Edema and Protects the Blood–Brain Barrier Integrity from Ischemia/Reperfusion Injury in Rats
Creators: name: Hamdollah Panahpour
name: Nekooeian, Ali Akbar
name: Dehghani, Gholam Abbas
Publisher: name: the Pasteur Institute of Iran
Year: 1996
Subjects: subject: Basic Sciences

description: Iranian Biomedical Journal (IBJ); ISSN 1028-852X
Charmonium production in a thermalizing heat bath
Creators: name: Song, Taesoo
name: Aichelin, Joerg
name: Bratkovskaya, Elena
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Using the Remler formalism for the creation of composed particles, we study charmonium production both in thermalized and thermalizing boxes, which contain charm and anticharm quarks. The thermalizing box studies include the lowering of the box temperature, the spatial diffusion of charm and anticharm quarks, which are initially confined in the central region, as well as the combination of both, what imitates heavy-ion collisions. Comparing numerical and analytical results we demonstrate that the rate of the original Remler formalism has to be supplemented by two rates to obtain, for $t\to \infty$, results, which are consistent with the statistical model predictions: i) a rate, which takes into account the temperature dependence of the Wigner density of the quarkonium during the expansion and, in the case that a heavy quark potential is not implemented in the Monte Carlo approach, ii) a rate which comes from the change of the relative distance between the heavy quark and antiquark. These results provide the basis for future applications of the Remler formalism to heavy-ion collisions.
description: 9 pages, 5 figures
title: Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼ÐµÑ Ð°Ð½Ð¸ÐºÐ°. Ð£Ð¿ÑÑÐ³Ð¸Ðµ Ð¸ ÑÐµÐ¿Ð»Ð¾Ð²ÑÐµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¸Ð´ÐµÐ°Ð»ÑÐ½ÑÑ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÑÐ¸Ð½ÑÐºÐ¸Ð¹, ÐÐ³Ð¾ÑÑ
name: ÐÐ²Ð°Ñ, ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹
name: ÐÑÐ¸Ð²ÑÐ¾Ð², ÐÐ½ÑÐ¾Ð½
name: ÐÑÐ¸Ð²ÑÐ¾Ð², ÐÐ½ÑÐ¾Ð½
name: ÐÑÐ·ÑÐºÐ¸Ð½, ÐÐ¸ÑÐ°Ð»Ð¸Ð¹
name: ÐÑÐ¸Ð²ÑÐ¾Ð², ÐÐ½ÑÐ¾Ð½
name: ÐÐµ-ÐÐ°ÑÐ°ÑÐ¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ¾Ð±Ð¾Ð´Ð°, ÐÐ»ÑÐ³Ð°
name: ÐÐµÐ¹Ð³ÐµÐ±Ð°ÑÑÑ, Ð.
name: ÐÐ¾Ð´Ð¾Ð»ÑÑÐºÐ°Ñ, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2009
Subjects: ÐÑÐ¸ÑÑÐ°Ð»Ð»Ñ
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The Lyman $α$ Reference Sample XIV: Lyman $α$ imaging of 45 low redshift star-forming galaxies and inferences on global emission
Creators: name: Melinder, Jens
name: Östlin, Göran
name: Hayes, Matthew
name: Rasekh, Armin
name: Mas-Hesse, J. Miguel
name: Cannon, John M.
name: Kunth, Daniel
name: Laursen, Peter
name: Runnholm, Axel
name: Herenz, E. Christian
name: Messa, Matteo
name: Schaerer, Daniel
name: Verhamme, Anne
name: Rivera-Thorsen, T. Emil
name: Guaita, Lucia
name: Marquart, Thomas
name: Puschnig, Johannes
name: Reste, Alexandra Le
name: Sandberg, Andreas
name: Freeland, Emily
name: Bridge, Joanna
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present Ly $α$ imaging of 45 low redshift star-forming galaxies observed with the Hubble Space Telescope. The galaxies have been selected to have moderate to high star formation rates using far-ultraviolet (FUV) luminosity and \ha equivalent width criteria, but no constraints on Ly $α$ luminosity. We employ a pixel stellar continuum fitting code to obtain accurate continuum subtracted Ly $α$, H $α$ and H $β$ maps. We find that Ly $α$ is less concentrated than FUV and optical line emission in almost all galaxies with significant Ly $α$ emission. We present global measurements of Ly $α$ and other quantities measured in apertures designed to capture all of the Ly $α$ emission. We then show how the escape fraction of Ly $α$ relates to a number of other measured quantities (mass, metallicity, star formation, ionisation parameter, and extinction). We find that the escape fraction is strongly anti-correlated with nebular and stellar extinction, weakly anti-correlated with stellar mass, but no conclusive evidence for correlations with other quantities. We show that Ly $α$ escape fractions are inconsistent with common dust extinction laws, and discuss how a combination of radiative transfer effects and clumpy dust models can help resolve the discrepancies. We present a star formation rate calibration based on Ly $α$ luminosity, where the equivalent width of Ly $α$ is used to correct for non-unity escape fraction, and show that this relation provides a reasonably accurate SFR estimate. We also show stacked growth curves of Ly $α$ for the galaxies that can be used to find aperture loss fractions at a given physical radius.
description: 48 pages, 21 figures, accepted for publication in The Astrophysical Journal Supplement Series. Multipanel figures for all 45 galaxies will be available in the online version of the published paper (and here: https://stockholmuniversity.box.com/s/ghvnvjyhxts64hpbqh90uwcj5dlczlhm ). Data products will be available as a MAST HLSP soon (placeholder DOI: 10.17909/pbe1-m743)