cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
TEACHING ENGLISH AT PRIMARY SCHOOLS USING COMMUNICATIVE APPROACH METHOD
Creators: name: Zahro Mirbabayeva
Publisher: name: Academic research in educational sciences
Year: 2021
Subjects: teaching English; communicative approach; primary schools; teaching methods.

description: In Uzbekistan, teacher training and re-training programs started to focus on reforming teaching methods at primary school. However, in English Language Teaching (ELT) methodology, ―Communicative Language Teaching (CLT)‖, which is the most dominant and experienced foreign language teaching method in many current ELT applications, has been widely used in Uzbekistan as well as in other countries in the world. Moreover, it is regarded as the most reliable and efficient way of teaching language not only for English but also for other languages. Morover, until recently, very few studies have been carried out in the field to interpret the CLT applications and their results in teaching English as a foreign language or a second language in the world. Despite the increasing popularity of the communicative approach, very few small-scale classroom studies have been carried out. Although CLT is widely practiced throughout the world via pre-school and school programs, workshops, and university courses, there is little evidence about what teachers understand from CLT and how they apply it in the classroom
High-energy neutrino astronomy and the Baikal-GVD neutrino telescope
Creators: name: Zaborov, Dmitry
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Neutrino astronomy offers a novel view of the non-thermal Universe and is complementary to other astronomical disciplines. The field has seen rapid progress in recent years, including the first detection of astrophysical neutrinos in the TeV-PeV energy range by IceCube and the first identified extragalactic neutrino source (TXS 0506+056). Further discoveries are aimed for with new cubic-kilometer telescopes in the Northern Hemisphere: Baikal-GVD, in Lake Baikal, and KM3NeT-ARCA, in the Mediterranean sea. The construction of Baikal-GVD proceeds as planned; the detector currently includes over 2000 optical modules arranged on 56 strings, providing an effective volume of 0.35 km$^3$. We review the scientific case for Baikal-GVD, the construction plan, and first results from the partially built array.
description: 9 pages, 5 figures, to be published in Proceedings of the 5-th International Conference on Particle Physics and Astrophysics (ICPPA-2020), October 5-9, 2020
ЎЗБЕКИСТОНДА ГРЕКЛАР ДИАСПОРАСИ ТАРИХИ
Creators: name: Жуммагул Номазовна Абдурахманова
Publisher: name: Academic research in educational sciences
Year: 2021
Subjects: Диаспора
кам сонли миллатлар
глобалл масалалар
иккинчи жаҳон уруши
қувғин
инсонпарварлик
ғамҳўрлик
бағрикенглик

description: Мақолада Ўзбекистондаги кам сонли миллатлар тарихи грек миллати мисолида ѐритиб берилган. Грек миллати вакилларининг Иккинчи жаҳон уруши таъсири натижасида ватанидан қувғин қилиниши жараѐни, уларнинг Ўзбекистонга ҳам кўчириб келтирилиши, Ўзбекистонда грек диаспорасининг ҳаѐти, Ўзбекистон халқининг инсонпарварлиги, ғамҳўрлиги, бағрикенглиги ва грекларга ҳам беғараз ѐрдами тадқиқ этилган
The LEGA-C of nature and nurture in stellar populations of galaxies at z~0.6-1.0: D4000 and H-delta reveal different assembly histories for quiescent galaxies in different environments
Creators: name: Sobral, David
name: van der Wel, Arjen
name: Bezanson, Rachel
name: Bell, Eric
name: Muzzin, Adam
name: D'Eugenio, Francesco
name: Darvish, Behnam
name: Gallazzi, Anna
name: Wu, Po-Feng
name: Maseda, Michael
name: Matthee, Jorryt
name: Paulino-Afonso, Ana
name: Straatman, Caroline
name: van Dokkum, Pieter
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Galaxy evolution is driven by a variety of physical processes which are predicted to proceed at different rates for different dark matter haloes and environments across cosmic times. A record of this evolution is preserved in galaxy stellar populations, which we can access using absorption-line spectroscopy. Here we explore the large LEGA-C survey (DR3) to investigate the role of the environment and stellar mass on stellar populations at z~0.6-1.0 in the COSMOS field. Leveraging the statistical power and depth of LEGA-C, we reveal significant gradients in D4000 and H-delta equivalent widths (EWs) distributions over the stellar mass vs environment 2D spaces for the massive galaxy population (M>10^10 M$_{\odot}$) at z~0.6-1.0. D4000 and H-delta EWs primarily depend on stellar mass, but they also depend on environment at fixed stellar mass. By splitting the sample into centrals and satellites, and in terms of star-forming galaxies and quiescent galaxies, we reveal that the significant environmental trends of D4000 and H-delta EW when controlling for stellar mass are driven by quiescent galaxies. Regardless of being centrals or satellites, star-forming galaxies reveal D4000 and H-delta EWs which depend strongly on their stellar mass and are completely independent of the environment at 0.6
description: Accepted for publication in ApJ. 18 pages, 9 figures
БАДИИЙ МАТНЛАРДА УСЛУБИЙ ВОСИТАЛАРНИНГ ИФОДАЛАНИШИ
Creators: name: Сергей Илларионович Абкадиров
Publisher: name: Academic research in educational sciences
Year: 2021
Subjects: бадиий матн
стилистик восита
нутқ
меъѐр

description: Ушбу мақола бадиий матнларда стилистик воситаларнинг қўлланилиш усуллари ва персонаж нутқини ѐритишдаги аҳамиятини назарий билимларга таянган ҳолда мисоллар орқали асослаш масалаларига бағишланган
Assessing the response of microphytobenthic biofilms to multiple stressors
Creators: name: Rimmer, James
Publisher: name: The University of St Andrews
Year: 2023
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: Stressors
subject: Estuary
subject: Biofilm
subject: Interactions
subject: Sediment
subject: Benthic

description: Ecological systems are exposed to a range of drivers, often referred to as stressors if detrimental or resulting from anthropogenic activities, which affect their functioning. To understand how these systems respond to stressors requires testing their effects on scaled ecosystems or biological components therein, or making predictions based on a mechanistic understanding of their modes of action. However, few stressors occur in isolation, and many – perhaps most – ecological responses are affected by non-additive interactions; net effects which are greater, or less than, the sum of the individual effects of multiple stressors. Cumulative stressor effects on estuarine, intertidal microphytobenthic (MPB) biofilms were examined, as knowledge concerning responses to such effects in soft-sediment habitats is presently limited. The MPB perform key roles in estuaries, such as primary production and biogenic sediment stabilisation. Unexpected, combined stressor effects may propagate to higher trophic levels, and inhibit ecosystem functions provided by the MPB. Mesocosm experiments examined the effects of the herbicide glyphosate and nanoparticles of titanium dioxide, revealing variable stressor responses which appeared to be affected by contextual influences, such as abiotic environmental factors and biofilm condition. A meta-analysis of the experimental data suggested that the nanoparticles mitigated some of the detrimental effects of the herbicide on the biofilms. Experimental findings, with MPB-driver relationship data, were used to predict the probability of detecting stressor effects in natural systems, as well as to estimate statistical power and inform experimental design. Field experiments demonstrated that whilst exposure to glyphosate was likely to detrimentally affect MPB assemblages in accordance with findings from mesocosm experiments, there was little evidence to suggest that antagonistic interactions occurred in a natural system. The ramifications of these results for ecosystem management are considered, and gaps in our understanding of cumulative stressor effects in estuarine systems and more broadly are discussed.
ФИЗИЧЕСКАЯ РЕАБИЛИТАЦИЯ БОРЦОВ С НАРУШЕНИЯМИ В ПОЗВОНОЧНИКЕ У КВАЛИФИЦИРОВАННЫХ БОРЦОВ
Creators: name: Норпулат Ширинович Бобомуродов
Publisher: name: Academic research in educational sciences
Year: 2021
Subjects: физическая реабилитация
восстановление
профессиональные борцы
бщеразвивающие и специальные упражнения

description: В работе использована методика применения средств и методов физической реабилитации профессиональных борцов с нарушениями в отделах позвоночника. Средства физической реабилитации, включали не только дыхательные, общеразвивающие упражнения, но и специальные упражнения, направленные на восстановление нарушений в отделах позвоночника. В конце заключительного периода предложены стретчинговые упражнения, способствующие не только растяжке мышц, но и развивающие связочносуставной аппарат, а также расширяющие диапазона объема движений вокруг суставов позвоночника
Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
Creators: name: Bi, Da
name: Shlosman, Isaac
name: Romano-Diaz, Emilio
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We employ high-resolution zoom-in cosmological simulations to analyze the emerging morphology of galaxies in dark matter halos at redshifts z > 2. We choose DM halos of similar masses of log (Mvir/Mo) ~11.65 +- 0.05 at the target redshifts of z_f = 6, 4 and 2. The rationale for this choice, among others, allows us to analyze how the different growth rate in these halos propagates down to galaxy scales. Halos were embedded in high or low overdensity regions, and two different versions of a galactic wind feedback have been employed. Our main results are: (1) Although our galaxies evolve in different epochs, their global parameters remain within a narrow range. Their morphology, kinematics and stellar populations differ substantially, yet all of them host sub-kpc stellar bars; (2) The SFRs appear higher for larger z_f, in tandem with their energy and momentum feedback; (3) The stellar kinematics allowed separation of bulge from the stellar spheroid. The existence of disk-like bulges has been revealed based on stellar surface density and photometry, but displayed a mixed disk-like and classical bulges based on their kinematics. The bulge-to-total mass ratios appear independent of the last merger time for all z_f. The stellar spheroid-to-total mass ratios of these galaxies lie in the range of ~0.5-0.8; (4) The synthetic redshifted, pixelized and PSF-degraded JWST images allow to detect stellar disks at all z_f. Some bars disappear in degraded images, but others remain visible; (5) Based on the kinematic decomposition, for stellar disks separated from bulges and spheroids. we observe that rotational support in disks depends on the feedback type, but increases with decreasing z_f; (6) Finally, the ALMA images detect disks at all z_f, but their spiral structure is only detectable in z_f=2 galaxies.
description: 18 pages, 22 figures. Submitted
Gewalt brauch Sühne, aber Sühne braucht keine Gewalt: Eine friedenskirchliche Perspektive auf das Kreuz Christi
Creators: name: Hulst, Fulco Van
Publisher: name: Ökumenische Rundschau
Year: 2025

description: Ökumenische Rundschau, Bd. 64 Nr. 2 (2015): Ökumenische Rundschau, Band 64, Heft 2
JSim, an open-source modeling system for data analysis and reproducibility in research
Creators: name: Bassingthwaighte, James
name: Butterworth, Erik
name: Jardine, Bart
name: Raymond, Gary M.
Publisher: name: F1000Research
Year: 2015

description: JSim is a simulation system for developing models, designing experiments, and evaluating hypotheses on physiological and pharmacological systems through the testing of model solutions against data. It is designed for interactive, iterative manipulation of the model code, different data sets, parameter sets, and for making comparisons among different models running simultaneously or separately. Interactive use is supported by a large collection of graphical user interfaces handling model writing and compilation diagnostics, defining input functions, model runs, selection of algorithms solving ordinary and partial differential equations, run-time multidimensional graphics, parameter optimization (8 methods), sensitivity analysis, and Monte Carlo simulation for defining confidence ranges. JSim uses Mathematical Modeling Language (MML) a declarative syntax specifying ODEs and PDEs. The model coding and displaying of results is basically simply defining the parameters, variables, and writing the equations in MML in usual form (except for using x:t for dx/dt) making it good for teaching modeling as well as for model analysis for research. JSim can be run as a batch job. JSim can automatically translate models from the repositories for Systems Biology Markup Language (SBML) and CellML models. Stochastic modeling is supported. JSim encourages assigning physical units to variables and parameters and automates the first steps of verification testing by checking for dimensional balance with automatic unit scaling included in the computation. The JSim Project File sets a standard for reproducible modeling analysis by including in one ascii file everything for a complete analysis of experiments: the data, the quantitative hypotheses defined by the models, and the data analysis. JSim is open source; it and about 400 human readable open source models are available at http://www.physiome.org/jsim/.

The issue is reproducibility of a scientific process. The processes include experiment design, data acquisition, developing successive models, testing them  for verification of numerical accuracy and for validation versus the data, determining parameters and their confidence ranges, quantifying uncertainty of predictions, and evaluating utility for diagnosis and prognosis. All of these can be captured, along with the provenance of the successive models and with the multiple sets of data, in a single human readable JSim project file for ease of retention and dissemination in open source form. JSim computes fast compared to Matlab (average about 300 times faster), and coding the models is easy using declarative expressions in standard equation form, so the project file is an ideal Reproducible Exchange Package, REP, for archiving and disseminating a scientific project.
A Bayesian model selection analysis of WMAP3
Creators: name: Parkinson, David
name: Mukherjee, Pia
name: Liddle, Andrew R
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a Bayesian model selection analysis of WMAP3 data using our code CosmoNest. We focus on the density perturbation spectral index $n_S$ and the tensor-to-scalar ratio $r$, which define the plane of slow-roll inflationary models. We find that while the Bayesian evidence supports the conclusion that $n_S \neq 1$, the data are not yet powerful enough to do so at a strong or decisive level. If tensors are assumed absent, the current odds are approximately 8 to 1 in favour of $n_S \neq 1$ under our assumptions, when WMAP3 data is used together with external data sets. WMAP3 data on its own is unable to distinguish between the two models. Further, inclusion of $r$ as a parameter weakens the conclusion against the Harrison-Zel'dovich case (n_S = 1, r=0), albeit in a prior-dependent way. In appendices we describe the CosmoNest code in detail, noting its ability to supply posterior samples as well as to accurately compute the Bayesian evidence. We make a first public release of CosmoNest, now available at http://www.cosmonest.org.
description: 7 pages RevTex with 4 figures included. Updated to match PRD accepted version. Main results unchanged. CosmoNest code now version 1.0 and includes calculation of the Information. Code available at http://www.cosmonest.org
Differentiable Refraction-Tracing for Mesh Reconstruction of Transparent Objects
Creators: name: Lyu, Jiahui
name: Wu, Bojian
name: Lischinski, Dani
name: Cohen-Or, Daniel
name: Huang, Hui
Publisher: name: arXiv
Year: 2020
Subjects: subject: Graphics (cs.GR)
subject: FOS: Computer and information sciences

description: Capturing the 3D geometry of transparent objects is a challenging task, ill-suited for general-purpose scanning and reconstruction techniques, since these cannot handle specular light transport phenomena. Existing state-of-the-art methods, designed specifically for this task, either involve a complex setup to reconstruct complete refractive ray paths, or leverage a data-driven approach based on synthetic training data. In either case, the reconstructed 3D models suffer from over-smoothing and loss of fine detail. This paper introduces a novel, high precision, 3D acquisition and reconstruction method for solid transparent objects. Using a static background with a coded pattern, we establish a mapping between the camera view rays and locations on the background. Differentiable tracing of refractive ray paths is then used to directly optimize a 3D mesh approximation of the object, while simultaneously ensuring silhouette consistency and smoothness. Extensive experiments and comparisons demonstrate the superior accuracy of our method.
description: 13 pages, 21 figures
Compensatory growth of three herbaceous perennial species : the effects of clipping and nutient availability
Creators: name: Hicks, Samantha Louise
Publisher: name: University of British Columbia
Year: 2009

description: This study focuses on the active responses of plants to herbivore damage, specifically on the ability of plants to regrow following an episode of herbivory. The Continuum of Responses model (CRM) and the Growth Rate model (GRM) make some conflicting predictions about the effects of soil nutrient availability on compensatory growth by grazed (clipped) plants. A factorial field experiment was conducted to examine the effects of longterm fertilization, short-term fertilization and clipping on the rate of (re)growth and the amount of (re)growth of three herbaceous perennial species, Achillea millefolium, Festuca altaica and Mertensia paniculata. Plants were collected from areas with different soil nutrient levels (low soil fertility and high soil fertility), planted in a common garden in the field and subjected to one of three simulated herbivory events (0%, 50% and 100% leaf loss) and one of two fertilizing treatments (no fertilizer and fertilizer addition). Concordant with both models, clipping was detrimental to plant growth which decreased as clipping intensity increased. From the plant's perspective, the impact of herbivory on the proportional leaf area of clipped plants relative to undipped controls, was independent of short-term fertilization. When biomass was measured, short-term fertilization reduced the compensatory ability of A. millefolium and M. paniculata, but improved it for F. altaica. From the animal's perspective, the impact of herbivory on the absolute size of clipped plants relative to controls was reduced by short-term fertilization, regardless of species and the measure of growth considered. Under natural soil nutrient conditions, M paniculata is more likely to compensate for leaf loss than A millefolium and F. altaica. These results indicate that short-term nutrient availability may affect the compensatory growth of clipped plants, but compensatory responses of the three species studied were only partly consistent with the predictions of the two models.
An EAGLE view of the missing baryons
Creators: name: Tuominen, Toni
name: Nevalainen, Jukka
name: Tempel, Elmo
name: Kuutma, Teet
name: Wijers, Nastasha
name: Schaye, Joop
name: Heinämäki, Pekka
name: Bonamente, Massimiliano
name: Veena, Punyakoti Ganeshaiah
Publisher: name: arXiv
Year: 2020
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Context. A significant fraction of the predicted baryons remains undetected in the local universe. We adopted the common assumption that a large fraction of the missing baryons corresponds to the hot (log T(K) = 5.5-7) phase of the Warm Hot Intergalactic Medium (WHIM). We base our missing baryons search on the scenario whereby the WHIM has been heated up via accretion shocks and galactic outflows, and is concentrated towards the filaments of the Cosmic Web. Aims. Our aim is to improve the observational search of the poorly detected hot WHIM. Methods. We detect the filamentary structure within the EAGLE simulation by applying the Bisous formalism to the galaxy distribution. In addition, we use the MMF/NEXUS+ classification of the large scale environment of the dark matter component in EAGLE. We then study the spatio-thermal distribution of the hot baryons within the extracted filaments. Results. While the filaments occupy only 5% of the full simulation volume, the diffuse hot intergalactic medium in filaments amounts to 23% $-$ 25% of the total baryon budget, or 79% $-$ 87% of all the hot WHIM. The most optimal filament sample, with a missing baryon mass fraction of 82%, is obtained by selecting Bisous filaments with a high galaxy luminosity density. For these filaments we derived analytic formulae for the radial gas density and temperature profiles, consistent with recent Planck SZ and CMB lensing observations within the central $r$~ 1 Mpc. Conclusions. Results from EAGLE suggest that the missing baryons are strongly concentrated towards the filament axes. Since the filament finding methods used here are applicable to galaxy surveys, a large fraction of the missing baryons can be localised by focusing the observational efforts on the central 1 Mpc regions of the filaments. Moreover, focusing on high galaxy luminosity density regions will optimise the observational signal.
description: 22 pages, 16 figures, accepted for publication in Astronomy and Astrophysics (A&A)
A Third Epoch Proper Motion Study of The Forward Shock in Kepler's Supernova Remnant
Creators: name: Coffin, Sadie C.
name: Williams, Brian J.
name: Katsuda, Satoru
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present measurements of the expansion of Kepler's Supernova Remnant (SNR) over three epochs of Chandra X-ray observations from 2000, 2006, and 2014. As the remnant of a historical supernova (observed in 1604 CE), Kepler's SNR presents the rare opportunity to study the dynamical evolution of such an object in real time. Measurements of the asymmetry in forward shock velocity can also provide insight into the nature of the explosion and density of the circumstellar material. Combining data from 2014 with previous epochs in 2000 and 2006, we can observe the proper motion of filaments along the outer rim of the SNR. Prior studies of Kepler's SNR have shown proper motion differences up to a factor of 3 between northern and southern regions around the remnant. With the longer time baseline we use here, we find results that are consistent with previous studies, but with smaller uncertainties. Additionally, by adding a third epoch of observations, we search for any systemic change in the velocity in the form of a deceleration of the blast wave, as was recently reported in Tycho's SNR. We find little to no conclusive evidence of such deceleration, and conclude that Kepler's SNR is encountering circumstellar material that is roughly constant in density, though substantially varied around the periphery.
description: Accepted for publication in ApJ
Reply to comment ``On the test of the modified BCS at finite temperature''
Creators: name: Ponomarev, V. Yu.
name: Vdovin, A. I.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: This is our formal Reply to revised version (v2) of arXiv: nucl-th/0510004v2.
description: accepted in Physical Review C
Isospin Diffusion Observables in heavy ion reactions
Creators: name: Liu, T. X.
name: Lynch, W. G.
name: Tsang, M. B.
name: Liu, X. D.
name: Shomin, R.
name: Tan, W. P.
name: Verde, G.
name: Wagner, A.
name: Xi, H. F.
name: Xu, H. S.
name: Davin, B.
name: Larochelle, Y.
name: de Souza, R. T.
name: Charity, R. J.
name: Sobotka, L. G.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Collisions of 112Sn and 124Sn nuclei, which differ in their isospin asymmetry, provide information about the rate of isospin diffusion and equilibration. While several different probes can provide accurate diffusion measurements, the ratios of the mirror nuclei may be the simplest and most promising one. Ratios of the mass seven mirror nuclei yields are analyzed to show the rapidity, transverse momentum and impact parameter dependence of isospin diffusion.
description: 22 pages, 7 figures
Supplementary Figures from Laser-stimulated fluorescence reveals unseen details in fossils from the Upper Jurassic Solnhofen Limestones
Creators: name: Barlow, Luke A.
name: Pittman, Michael
name: Butcher, Anthony
name: Martill, David M.
name: Kaye, Thomas G.
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: 40308 Palaeontology (incl. Palynology)
subject: FOS: Earth and related environmental sciences

description: Additional figures and references that did not make it into the final manuscript but still show valuable results.
Theory of the Strain Engineering of Graphene Nanoconstrictions
Creators: name: Hayashi, Masahiko
name: Yoshioka, Hideo
name: Tomori, Hikari
name: Kanda, Akinobu
Publisher: name: arXiv
Year: 2020
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Strain engineering is one of the key technologies for using graphene as an electronic device: the strain-induced pseudo-gauge field reflects Dirac electrons, thus opening the so-called conduction gap. Since strain accumulates in constrictions, graphene nanoconstrictions can be a good platform for this technology. On the other hand, in the graphene nanoconstrictions, Fabry-Perot type quantum interference dominates the electrical conduction at low bias voltages. We argue that these two effects have different strain dependence; the pseudo-gauge field contribution is symmetric with respect to positive (tensile) and negative (compressive) strain, whereas the quantum interference is antisymmetric. As a result, a peculiar strain dependence of the conductance appears even at room temperatures.
description: 4 pages, 3 figures
The HI Structure of the Local Volume Dwarf Galaxy Pisces A
Creators: name: Beale, Luca
name: Meyer, Jennifer Donovan
name: Tollerud, Erik J.
name: Putman, Mary E.
name: Peek, J. E. G.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Dedicated HI surveys have recently led to a growing category of low-mass galaxies found in the Local Volume. We present synthesis imaging of one such galaxy, Pisces A, a low-mass dwarf originally confirmed via optical imaging and spectroscopy of neutral hydrogen (HI) sources in the Galactic Arecibo L-band Feed Array HI (GALFA-HI) survey. Using HI observations taken with the Karl G. Jansky Very Large Array (JVLA), we characterize the kinematic structure of the gas and connect it to the galaxy's environment and evolutionary history. While the galaxy shows overall ordered rotation, a number of kinematic features indicate a disturbed gas morphology. These features are suggestive of a tumultuous recent history, and represent $\sim 3.5$% of the total baryonic mass. We find a total baryon fraction $f_{\rm bary} = 0.13$ if we include these features. We also quantify the cosmic environment of Pisces A, finding an apparent alignment of the disturbed gas with nearby, large scale filamentary structure at the edge of the Local Void. We consider several scenarios for the origin of the disturbed gas, including gas stripping via ram pressure or galaxy-galaxy interactions, as well as accretion and ram pressure compression. Though we cannot rule out a past interaction with a companion, our observations best support the suggestion that the neutral gas morphology and recent star formation in Pisces A is a direct result of its interactions with the IGM.
description: 16 pages, 12 figures, accepted to ApJ
ИҚТИСОДИЁТНИ МОДЕРНИЗАЦИЯЛАШ ШАРОИТИДА АНДИЖОН ВИЛОЯТИДА ТУРИЗМНИ ДИВЕРСИФИКАЦИЯ ҚИЛИШ МАСАЛАЛАРИ
Creators: name: Муҳаммадисмоил Мухитдинович Маҳмудов
Publisher: name: Academic research in educational sciences
Year: 2021
Subjects: Диверсификация
инфратузилма
туризм
саноат
аҳоли
урбанизация
Shopping
агротуризм

description: Ушбу мақолада Андижон вилоятида туризмни диверсификация қилиш масалаларига алоҳида эътибор қаратилган. Туризмнинг айнан алоҳида бир турини ривожлантириш қийин бўлган Андижон вилоятида аралаш туристик маршрутларни тузиш, шу орқали минтақага сайѐҳлар қизиқишини оширишга қаратилган чора-тадбирларни ишлаб чиқиш масалаларига тўхталиб ўтилган. Туризмни ривожлантиришга таъсир кўрсатувчи аҳоли, хизмат кўрсатиш, тиббиѐт, инфратузилма, саноат, қишлоқ хўжалиги, тадбиркорлик, ҳунармандчилик каби қатор соҳалардан туризм саноатини ривожлантиришда кенг фойдаланиш ҳусусида фикр-мулоҳазалар билдирилган
Evolutionary genetics of male sex comb variation and the sex-combs reduced gene in Drosophila
Creators: name: Mittleman, Briana
name: Noor, Mohamed A.F.
Publisher: name: F1000Research
Year: 2015

description: Part of this work published in Mittleman, B. E., A. B. Abrams, and M. A. F. Noor. 2014. Lack of evidence for directional selection on Sex combs reducedgene in Drosophila species differing in sex comb morphology. Drosophila Information Service, 97: 42-44.
Hetzjagden der Gegenwart und die Frage nach dem Kreuz
Creators: name: Niewiadomski, Józef
Publisher: name: Ökumenische Rundschau
Year: 2025

description: Ökumenische Rundschau, Bd. 64 Nr. 2 (2015): Ökumenische Rundschau, Band 64, Heft 2
Equivalence of real Milnor's fibrations for quasi homogeneous singularities
Creators: name: Santos, R. Araujo dos
Publisher: name: arXiv
Year: 2008
Subjects: subject: Geometric Topology (math.GT)
subject: Algebraic Topology (math.AT)
subject: FOS: Mathematics
subject: 32S55, 57Q45

description: We are going to use the Euler's vector fields in order to show that for real quasi-homogeneous singularities with isolated critical value, the Milnor's fibration in a "thin" hollowed tube involving the zero level and the fibration in the complement of "link" in sphere are equivalents, since they exist. Moreover, in order to do that, we explicitly characterize the critical points of projection $\frac{f}{\|f\|}:S_ε^{m}\setminus K_ε\to S^{1}$, where $K_ε$ is the link of singularity.
NOGIRONLIGI BOR SHAXSLARNI KASB HUNAR EGALLASHI VA ULARNI ISH BILAN BAND QILISH MUAMMOLARI VA YECHIMLARI
Creators: name: Yaxshiyev, Dilshod
Publisher: name: Zenodo
Year: 2024

description: Ba'zi odamlar bor, ular boshqa odamlar kabi ishlay olishlari uchun maxsus yordamga muhtoj. Ular o'z qobiliyatları namoyon qilishlari uchun juda ko'p e'tibor talab qiladi. Ularning jamiyatda o'z o'rnini topishi, ya'ni barcha bilan birga yashashi uchun, jamiyatdagi boshqa odamlar ve qoidalar juda muhim. Biz bu masalani maqolamizda batafsil muhokama qildik.
СОВРЕМЕННЫЕ ПОДХОДЫ И “МЕХАНИЗМЫ” В ОБУЧЕНИИ ИНОСТРАННОГО ЯЗЫКА В КАЧЕСТВЕ ИНОСТРАННОГО НА ПРИМЕРЕ МЕТОДОЛОГИЧЕСКИХ ТЕХНИК И СИСТЕМ РАЗВИТИЯ НАВЫКОВ ГОВОРЕНИЯ И ЧТЕНИЯ В АНГЛИЙСКОМ ЯЗЫКЕ
Creators: name: Амир Камилевич Абушаев
Publisher: name: Academic research in educational sciences
Year: 2021
Subjects: клише
стереотипность
популярность
обучение
интенсивная методика
процессы обучения

description: В научной статье рассматриваются современные подходы и процессы, которые используются в обучении иностранному языку. Например, интенсивная техника приобрела особую популярность среди тех, кто стремится научиться говорить по-английски в кратчайшие сроки. Достичь этой, казалось бы, нереальной цели позволяет высокий уровень стереотипного языка английский на 25% является клише. Благодаря изучению большого количества устойчивых выражений, их запоминанию и отработке, человек может за относительно короткое время научиться объяснять на иностранном языке и понимать собеседника
Model selection forecasts for the spectral index from the Planck satellite
Creators: name: Pahud, Cédric
name: Liddle, Andrew R
name: Mukherjee, Pia
name: Parkinson, David
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The recent WMAP3 results have placed measurements of the spectral index n_S in an interesting position. While parameter estimation techniques indicate that the Harrison-Zel'dovich spectrum n_S=1 is strongly excluded (in the absence of tensor perturbations), Bayesian model selection techniques reveal that the case against n_S=1 is not yet conclusive. In this paper, we forecast the ability of the Planck satellite mission to use Bayesian model selection to convincingly exclude (or favour) the Harrison-Zel'dovich model.
description: 4 pages RevTeX with one figure included. Updated to match PRD accepted version. Improved likelihood function implementation; no qualitative change to results but some tiny numerical shifts
viR-SCAN – a tool for detection of viroid- and virus-derived small RNAs using plant next generation sequencing datasets.
Creators: name: Dimitrov, Dilyan
name: Gozmanova, Mariyana
name: Daskalova, Evelina
name: Ivanova, Desislava
name: Minkov, Ivan
name: Yahubyan, Galina
name: Baev, Vesselin
Publisher: name: F1000Research
Year: 2015

description: Small RNAs (sRNA), including microRNAs (miRNA) and small interfering RNAs (siRNA) are produced abundantly in plants and animals. They are critical players in defense against virus and viroid infections and in gene expression regulation. On the other side the accumulation in plant tissues of virus- and viroid-derived small RNAs (v-sRNAs) is usually associated with ongoing pathogen infection. Analysis of plant sRNA libraries and their profiles can indicate if plant sustains viral-induced silencing process, even more – it may allow strain differentiation, and de novo assembly of virus/viroid genomes.

We have developed a stand-alone tool called viR-SCAN, based on an algorithm for search of v-sRNAs in plant sRNA libraries. The tool allows characterization of identified v-sRNAs (size, sequence, strand polarity etc.) and mapping of (+) or/and (-) v-sRNAs on the reference genome with visualization of their hotspots and distribution profiles. The present version of the viR-SCAN allows users to identify 45 viroids and 1724 plant viruses. It also includes a module for endogenous plants miRNA detection in samples and miRNAs differential expression upon viral infection.
Photon echo polarimetry of excitons and biexcitons in a CH$_3$NH$_3$PbI$_3$ perovskite single crystal
Creators: name: Trifonov, A. V.
name: Grisard, S.
name: Kosarev, A. N.
name: Akimov, I. A.
name: Yakovlev, D. R.
name: Höcker, J.
name: Dyakonov, V.
name: Bayer, M.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Lead halide perovskites show remarkable performance when used in photovoltaic and optoelectronic devices. However, the peculiarities of light-matter interactions in these materials in general are far from being fully explored experimentally and theoretically. Here we specifically address the energy level order of optical transitions and demonstrate photon echos in a methylammonium lead triiodide single crystal, thereby determining the optical coherence times $T_2$ for excitons and biexcitons at cryogenic temperature to be 0.79 ps and 0.67 ps, respectively. Most importantly, we have developed an experimental photon-echo polarimetry method that not only identifies the contributions from exciton and biexciton complexes, but also allows accurate determination of the biexciton binding energy of 2.4 meV, even though the period of quantum beats between excitons and biexcitons is much longer than the coherence times of the resonances. Our experimental and theoretical analysis methods contribute to the understanding of the complex mechanism of quasiparticle interactions at moderate pump density and show that even in high-quality perovskite crystals and at very low temperatures, inhomogeneous broadening of excitonic transitions due to local crystal potential fluctuations is a source of optical dephasing.
ПРИНЦИПЫ СОВРЕМЕННОЙ ПЕДАГОГИЧЕСКОЙ ПОДГОТОВКИ
Creators: name: Тураев Махмуд Мухамедович
name: Курбанов Джурабек Исматович
name: Хамраев Искандар Турсунович
Publisher: name: Academic research in educational sciences
Year: 2021
Subjects: современная профессиональная подготовка
профессиональная подготовка учителя
цели современной подготовки учителя
принципы современной подготовки учителя

description: В статье обобщены и охарактеризованы такие принципы, как учет требований компетентносного подхода; фундаментализация; опережающий характер педагогического образования; непрерывность; преемственность; интегративность; вариативность; гибкость и открытость педагогического образования; практикоориентированность (технологичность) подготовки учителя.
Anisotropic phonon-mediated electronic transport in chiral Weyl semimetals
Creators: name: Garcia, Christina A. C.
name: Nenno, Dennis M.
name: Varnavides, Georgios
name: Narang, Prineha
Publisher: name: arXiv
Year: 2020
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Discovery and observations of exotic, quantized optical and electrical responses have sparked renewed interest in nonmagnetic chiral crystals. Within this class of materials, six group V transition metal ditetrelides, that is, XY$_2$ (X = V, Nb, Ta and Y = Si, Ge), host composite Weyl nodes on high-symmetry lines, with Kramers-Weyl fermions at time-reversal invariant momenta. In addition, at least two of these materials, NbGe$_2$ and NbSi$_2$, exhibit superconducting transitions at low temperatures. The interplay of strong electron-phonon interaction and complex Fermi surface topology present an opportunity to study both superconductivity and hydrodynamic electron transport in these systems. Towards this broader question, we present an ab initio theoretical study of the electronic transport and electron-phonon scattering in this family of materials, with a particular focus on NbGe$_2$ vs. NbSi$_2$, and the other group V ditetrelides. We shed light on the microscopic origin of NbGe$_2$'s large and anisotropic room temperature resistivity and contextualize its strong electron-phonon scattering with a presentation of other relevant scattering lifetimes, both momentum-relaxing and momentum-conserving. Our work explores the intriguing possibility of observing hydrodynamic electron transport in these chiral Weyl semimetals.
description: 13 pages, 9 figures including Supplementary Information
IBN MISKAVAYHNING ARAB TILIDA YOZILGAN ASARLARI TAVSIFI
Creators: name: Sulaymonova, Shahnoza Nodirovna
Publisher: name: Academic research in educational sciences
Year: 2021
Subjects: faylasuf
tilshunos olim
“Uchinchi muallim”
arab tili
“Al-favz al-asg„ar”
“Tajoribul-umam”
“Tahzibul-axloq”
“Kitab at-Tahora”
“TathirulA‟roq”

description: Maqola Musulmon Sharqi ijtimoiy-falsafiy tafakkuri tarixida yorqin iz qoldirgan buyuk mutafakkirlardan biri Abu Ali Ibn Miskavayhning arab tilida yozilgan asarlari tavsifiga bag‟ishlanadi. Miskavayh asarlarining butun musulmon olamiga tarqalishida arab tilining tutgan o„rni tahlil qilinadi
Charge and spin Hall conductivity in metallic graphene
Creators: name: Sinitsyn, N. A.
name: Hill, J. E.
name: Min, Hongki
name: Sinova, Jairo
name: MacDonald, A. H.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Graphene has an unusual low-energy band structure with four chiral bands and half-quantized and quantized Hall effects that have recently attracted theoretical and experimental attention. We study the Fermi energy and disorder dependence of its spin Hall conductivity. In the metallic regime we find that vertex corrections enhance the intrinsic spin Hall conductivity and that skew scattering can lead to its values that exceed the quantized ones expected when the chemical potential is inside the spin-orbit induced energy gap. We predict that large spin Hall conductivities will be observable in graphene even when the spin-orbit gap does not survive disorder.
description: 4 pages, 2 figures
Rank one HCIZ at high temperature: interpolating between classical and free convolutions
Creators: name: Mergny, Pierre
name: Potters, Marc
Publisher: name: arXiv
Year: 2021
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mathematical Physics (math-ph)
subject: Probability (math.PR)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We study the rank one Harish-Chandra-Itzykson-Zuber integral in the limit where $\frac{N β}{2} \to c $, called the high temperature regime and show that it can be used to construct a promising one-parameter interpolation, with parameter $c$ between the classical and the free convolution. This $c$-convolution has a simple interpretation in terms of another associated family of distribution indexed by $c$, called the Markov-Krein transform: the $c$-convolution of two distributions corresponds to the classical convolution of their Markov-Krein transforms. We derive first cumulants-moments relations, a central limit theorem, a Poisson limit theorem and shows several numerical examples of $c$-convoluted distributions.
description: 37 pages, 5 figures
ВЛИЯНИЕ ТЕПЛО И ЭНЕРГОПОТРЕБЛЕНИЯ МНОГОЭТАЖНЫХ ЗДАНИЙ НА ОСОБЕННОСТИ ПРОЦЕССА ГЛОБАЛЬНОГО ПОТЕПЛЕНИЯ И В УЗБЕКИСТАНЕ
Creators: name: Моҳинур Асрорбек Қизи Мўминова
name: Азамат Аскарович Таубалдиев
name: Бахрам Рузиевич Таджибаев
Publisher: name: Academic research in educational sciences
Year: 2021
Subjects: Климат
глобальное потепление
многоэтажные постройки
энергетические подсистемы
тепловая энергия

description: Технический прогресс приводит к появлению большого многообразия разнообразных конструкций, что отрицательно влияет на окружающую среду, главным образом на повышения средней температуры климатической системы Земли. В статье рассматривается и анализируется влияние многоэтажных домов на климатические изменения, а также даѐтся оценка данных воздействий
Spectroscopy of the helium-rich binary ES Ceti reveals accretion via a disc and evidence for eclipse
Creators: name: Bakowska, K.
name: Marsh, T. R.
name: Steeghs, D.
name: Nelemans, G.
name: Groot, P. J.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Amongst the hydrogen-deficient accreting binaries known as the "AM~CVn stars" are three systems with the shortest known orbital periods: HM Cnc (321 s), V407 Vul (569 s) and ES Cet (620 s). These compact binaries are predicted to be strong sources of persistent gravitational wave radiation. HM Cnc and V407 Vul are undergoing direct impact accretion in which matter transferred from their donor hits the accreting white dwarfs directly. ES Cet, is the longest period of the three and is amongst the most luminous AM CVn stars, but it is not known whether it accretes via a disk or direct impact. ES Cet displays strong HeII 4686 line emission, which is sometimes a sign of magnetically-controlled accretion. Peculiarly, although around one third of hydrogen accreting white dwarfs show evidence for magnetism, none have been found amongst helium accretors. We present the results of Magellan and VLT spectroscopic and spectropolarimetric observing campaigns dedicated to ES Cet with the aim of understanding its accretion structure. We find strong variability in our spectra on the 620 s period. The lines show evidence for double-peaked emission, characteristic for an accretion disc, with an additional component associated with the outermost disc, rather than a direct impact, that is broadly consistent with "S"-wave emission from the gas stream/disc impact region. This confirms beyond any doubt that 620\,s is the orbital period of ES Cet. We find no significant circular polarisation (below 0.1 %). The trailed spectra show that ES Cet's outer disc is eclipsed by the mass donor, revealing at the same time that the photometric minimum coincides with the hitherto unrecognised eclipse. ES Cet shows spectroscopic behaviour consistent with accretion via a disc, and is the shortest orbital period eclipsing AM CVn star known.
description: 8 pages, 8 figures, 2 tables, accepted for publication in Astronomy and Astrophysics
The Finite Size Error in Many-body Simulations with long-Ranged Interactions
Creators: name: Chiesa, Simone
name: Ceperley, David M.
name: Martin, Richard M.
name: Holzmann, Markus
Publisher: name: arXiv
Year: 2006
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We discuss the origin of the finite size error of the energy in many-body simulation of systems of charged particles and we propose a correction based on the random phase approximation at long wave lengths. The correction comes from contributions mainly determined by the organized collective oscillations of the interacting system. Finite size corrections, both on kinetic and potential energy, can be calculated within a single simulation. Results are presented for the electron gas and silicon.
description: 4 pages, 4 figures, submitted to PRL; corrected typos
title: Keep it Jugo, do it Švabo
Creators: name: Camacho-Trefil, Petra
Year: 2023

description: Die vorliegende Arbeit behandelt die Repräsentation der Jugoslawiener*innen im Tschuschen-Rap. Dafür wird zunächst ein Einblick in die für die Forschung wesentlichen theoretischen Grundlagen gegeben, wobei Aspekte zur Migrationsgesellschaft sowie die Hintergründe und Motive des Jugoslawiener*innen-Raps vorgestellt werden. Im Verlauf wird deutlich, dass sich die Nachkommen der ex-jugoslawischen Gastarbeiter*innen in Wien tagtäglich mit einem Gefühl der Ambivalenz auseinandersetzen müssen, welches sie davon abhält, sich vollends in die österreichische Gesellschaft zu integrieren. Sie verharren daher in einer Art Zwischenwelt, die aber durchaus Potenzial hat, um persönliche Eindrücke und Empfindungen mit der Außenwelt zu teilen. Anhand der Analyse ausgewählter Lyrics namhafter Vertreter der sog. Tschuschen-Rap-Szene wird gezeigt, dass sich Herkunft, südslawische Kultur, ausgewählte Orte und die Mischung von mehreren Sprachen außerordentlich auf Inhalte, Darstellung und Rezeption auswirken. Durch die Kombination aus diesen Faktoren entsteht eine wirklich interessante Musik, die prinzipiell als eine eigene Kunstform betrachtet werden kann. Der Tschuschen-Rap äußert sich dabei vor allem auch im Lebensstil, wobei er mitunter ebenfalls als Kommunikationsmittel dient, in dem durch unterschiedliche Formen der verbalen und körperlichen Sprache bestimmte Lebensweisen und mögliche Identitätskrisen verarbeitet werden. Sowohl die konkreten Lyrics der dargestellten Lieder als auch die dahinter liegenden Motive machen deutlich, dass die Absichten und Ziele für alle Tschuschen-Rapper*innen ähnlich sind: Sie möchten konkrete Botschaften an ihre Außenwelt vermitteln und somit ein Gefühl der Zugehörigkt schüren. Ihre Musik ist dabei das perfekte Medium, um sich selbst darzustellen und den Wunsch nach Anerkennung zum Ausdruck zu bringen. Durch die intensive Auseinandersetzung mit der Thematik, den ausgewählten Rappern und ihren Songs kann schlussendlich zusammengefasst werden, dass die Ursachen und Intentionen, die zur vermeintlichen Ausgrenzung führen, oftmals eher der Integration dienlich sind. Vielfalt sorgt in diesem Kontext also für eine Erweiterung des persönlichen Horizonts – und kann im Tschuschen-Rap öffentlich ausgelebt und gefeiert werden.