cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 6: of Genetic variation and structure of maize populations from Saoura and Gourara oasis in Algerian Sahara
Creators: name: Miyassa Aci
name: Lupini, Antonio
name: Mauceri, Antonio
name: Abdelkader Morsli
name: Khelifi, Lakhdar
name: Sunseri, Francesco
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Plant Biology
subject: 60506 Virology

description: Table S8. Analysis of Molecular Variance. (DOCX 12 kb)
Anomalous scaling of the optimal cost in the one-dimensional random assignment problem
Creators: name: Caracciolo, Sergio
name: D'Achille, Matteo
name: Sicuro, Gabriele
Publisher: name: arXiv
Year: 2018
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We consider the random Euclidean assignment problem on the line between two sets of $N$ random points, independently generated with the same probability density function $\varrho$. The cost of the matching is supposed to be dependent on a power $p>1$ of the Euclidean distance of the matched pairs. We discuss an integral expression for the average optimal cost for $N\gg 1$ that generalizes a previous result obtained for $p=2$. We also study the possible divergence of the given expression due to the vanishing of the probability density function. The provided regularization recipe allows us to recover the proper scaling law for the cost in the divergent cases, and possibly some of the involved coefficients. The possibility that the support of $\varrho$ is a disconnected interval is also analysed. We exemplify the proposed procedure and we compare our predictions with the results of numerical simulations.
description: 18 pages, 12 figures
Acceptor-induced bulk dielectric loss in superconducting circuits on silicon
Creators: name: Zhang, Zi-Huai
name: Godeneli, Kadircan
name: He, Justin
name: Odeh, Mutasem
name: Zhou, Haoxin
name: Meesala, Srujan
name: Sipahigil, Alp
Publisher: name: arXiv
Year: 2024
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The performance of superconducting quantum circuits is primarily limited by dielectric loss due to interactions with two-level systems (TLS). State-of-the-art circuits with engineered material interfaces are approaching a limit where dielectric loss from bulk substrates plays an important role. However, a microscopic understanding of dielectric loss in crystalline substrates is still lacking. In this work, we show that boron acceptors in silicon constitute a strongly coupled TLS bath for superconducting circuits. We discuss how the electronic structure of boron acceptors leads to an effective TLS response in silicon. We sweep the boron concentration in silicon and demonstrate the bulk dielectric loss limit from boron acceptors. We show that boron-induced dielectric loss can be reduced in a magnetic field due to the spin-orbit structure of boron. This work provides the first detailed microscopic description of a TLS bath for superconducting circuits, and demonstrates the need for ultrahigh purity substrates for next-generation superconducting quantum processors.
Storage and Repair Bandwidth Tradeoff for Distributed Storage Systems with Clusters and Separate Nodes
Creators: name: Wang, Jingzhao
name: Wang, Tinghan
name: Luo, Yuan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: The optimal tradeoff between node storage and repair bandwidth is an important issue for distributed storage systems (DSSs). As for realistic DSSs with clusters, when repairing a failed node, it is more efficient to download more data from intra-cluster nodes than from cross-cluster nodes. Therefore, it is meaningful to differentiate the repair bandwidth from intra-cluster and cross-cluster. For cluster DSSs the tradeoff has been considered with special repair assumptions where all the alive nodes are utilized to repair a failed node. In this paper, we investigate the optimal tradeoff for cluster DSSs under more general storage/repair parameters. Furthermore, a regenerating code construction strategy achieving the points in the optimal tradeoff curve is proposed for cluster DSSs with specific parameters as a numerical example. Moreover, the influence of separate nodes for the tradeoff is also considered for DSSs with clusters and separated nodes.
Additional file 7: of Genetic variation and structure of maize populations from Saoura and Gourara oasis in Algerian Sahara
Creators: name: Miyassa Aci
name: Lupini, Antonio
name: Mauceri, Antonio
name: Abdelkader Morsli
name: Khelifi, Lakhdar
name: Sunseri, Francesco
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology

description: Table S9. Partition of the gene diversity among clusters. (DOCX 12 kb)
Active Perception and Modeling of Deformable Surfaces using Gaussian Processes and Position-based Dynamics
Creators: name: Caccamo, Sergio
name: Güler, Püren
name: Kjellström, Hedvig
name: Kragic, Danica
Publisher: name: arXiv
Year: 2018
Subjects: subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: Exploring and modeling heterogeneous elastic surfaces requires multiple interactions with the environment and a complex selection of physical material parameters. The most common approaches model deformable properties from sets of offline observations using computationally expensive force-based simulators. In this work we present an online probabilistic framework for autonomous estimation of a deformability distribution map of heterogeneous elastic surfaces from few physical interactions. The method takes advantage of Gaussian Processes for constructing a model of the environment geometry surrounding a robot. A fast Position-based Dynamics simulator uses focused environmental observations in order to model the elastic behavior of portions of the environment. Gaussian Process Regression maps the local deformability on the whole environment in order to generate a deformability distribution map. We show experimental results using a PrimeSense camera, a Kinova Jaco2 robotic arm and an Optoforce sensor on different deformable surfaces.
description: 8 pages, video of an experiment available at https://youtu.be/mDNSDZz7Qzs
Variability of GRB Afterglows Due to Interstellar Turbulence
Creators: name: Wang, Xiaohu
name: Loeb, Abraham
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Gamma-Ray Burst (GRB) afterglows are commonly interpreted as synchrotron emission from a relativistic blast wave produced by a point explosion in an ambient medium, plausibly the interstellar medium of galaxies. We calculate the amplitude of flux fluctuations in the lightcurve of afterglows due to inhomogeneities in the surrounding medium. Such inhomogeneities are an inevitable consequence of interstellar turbulence, but could also be generated by variability and anisotropy in a precursor wind from the GRB progenitor. Detection of their properties could provide important clues about the environments of GRB sources. We apply our calculations to GRB990510, where an rms scatter of 2% was observed for the optical flux fluctuations on the 0.1--2 hour timescale during the first day of the afterglow, consistent with it being entirely due to photometric noise (Stanek et al. 1999). The resulting upper limits on the density fluctuations on scales of 20-200 AU around the source of GRB990510, are lower than the inferred fluctuation amplitude on similar scales in the Galactic interstellar medium. Hourly monitoring of future optical afterglows might therefore reveal fractional flux fluctuations at the level of a few percent.
description: 18 pages, submitted to ApJ
Characterization of Banach spaces $Y$ satisfying that the pair $ (\ell_\infty^4,Y )$ has the Bishop-Phelps-Bollobás property for operators
Creators: name: Acosta, María D.
name: Dávila, José L.
name: Soleimani-Mourchehkhorti, Maryam
Publisher: name: arXiv
Year: 2018
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 46B20, 47B99

description: We study the Bishop-Phelps-Bollobás property for operators from $\ell_\infty ^4 $ to a Banach space. For this reason we introduce an appropiate geometric property, namely the AHSp-$\ell_\infty ^4$. We prove that spaces $Y$satisfying AHSp-$\ell_\infty ^4$ are precisely those spaces $Y$ such that $(\ell_\infty^4,Y)$ has the Bishop-Phelps-Bollobás property. We also provide classes of Banach spaces satisfying this condition. For instance, finite-dimensional spaces, uniformly convex spaces, $C_0(L)$ and $L_1 (μ)$ satisfy AHSp-$\ell_\infty ^4 $.
description: 28 pages
Stranger in the Light: The Strange Vector Form Factors of the Nucleon
Creators: name: Forkel, Hilmar
name: Nielsen, Marina
name: Jin, Xuemin
name: Cohen, Thomas D.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A model combining vector meson dominance, $ω- ϕ$ mixing and a kaon cloud contribution is used to estimate the strangeness vector form factors of the nucleon in the momentum range of the planned measurements at MIT-Bates and CEBAF. We compare our results with some other theoretical estimates and discuss the nucleon strangeness radius in models based on dynamically dressed, extended constituent quarks. For a quantitative estimate in the latter framework we use the Nambu-Jona-Lasinio model.
description: 36 pages, UMPP \#94--097 (six figures available by e-mail or FAX)
Study of Three-Dimensional Magnetic Structure and the Successive Eruptive Nature of Active Region 12371
Creators: name: Vemareddy, P.
name: Demóulin, P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We study the magnetic structure of successively erupting sigmoid in active region 12371 by modeling the quasi-static coronal field evolution with non-linear force-free field (NLFFF) equilibria. HMI/SDO vector magnetograms are used as input to the NLFFF model. In all eruption events, the modeled structure resembles the observed pre-eruptive coronal sigmoid and the NLFFF core-field is a combination of double inverse J-shaped and inverse-S field-lines with dips touching the photosphere. Such field-lines are formed by flux-cancellation reconnection of opposite-J field-lines at bald-patch locations. It implies the formation of a weakly twisted flux-rope from large scale sheared arcade field lines. Later on, this flux-rope undergo coronal tether-cutting reconnection until a CME is triggered. The modeled structure captured these major features of sigmoid-to-arcade-to-sigmoid transformation, that is being recurrent under continuous photospheric flux motions. Calculations of the field-line twist reveal a fractional increase followed by a decrease of the number of pixels having a range of twist. This traces the buildup process of a twisted core-field by slow photospheric motions and the relaxation after eruption, respectively. Our study infers that the large eruptivity of this AR is due to a steep decrease of the background coronal field meeting the torus instability criteria at low height ($\approx 40$ Mm) in contrast to non-eruptive ARs.
description: 16 pages, 11 Figures; Accepted in ApJ
Three-micron imaging of the Hubble Deep Field
Creators: name: Hogg, David W.
name: Neugebauer, Gerry
name: Cohen, Judith G.
name: Dickinson, Mark
name: Djorgovski, S. G.
name: Matthews, Keith
name: Soifer, B. T.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Images of the Hubble Deep Field at 3.2 um, taken with the 10-m Keck Telescope, are presented. The images cover a total area of ~2.5 arcmin^2. To a 5-sigma limit of [3.2](total)=17.5 mag (Vega-relative), 11 sources are detected, 9 of which are extragalactic. The integrated galaxy number counts are therefore ~1.3x10^4 deg^{-2} to this depth. The galaxies detected at 3.2 um have a median redshift of z=0.56. All 3.2 um sources have 1.6 um, 1.1 um and visual counterparts, all of fairly regular morphologies; several also have 6.7 um, 15 um, 850 um, 8.5 GHz, or 1.4 GHz counterparts. No sources are found which are either anomalously red or anomalously blue in their H-[3.2] color, and there are significant detections of most of the known near-infrared HDF sources for which detection in these 3.2 um data seemed likely.
description: Accepted for publication in the Astronomical Journal. Better-quality figures and reduced data available at http://www.sns.ias.edu/~hogg/deep/
Towards Consistency Analysis Between Formal and Informal Software Architecture Artefacts
Creators: name: Keim, Jan
name: Schneider, Yves
name: Koziolek, Anne
Publisher: name: Institute of Electrical and Electronics Engineers (IEEE)
Year: 2019
Subjects: Natural language processing
Software architecture
Software engineering
Software architecture documentation
Consistency
Natural language understanding

description: Documenting the architecture of a software system is important, especially to capture reasoning and design decisions. A lot of tacit knowledge can easily get lost when the documentation is incomplete, resulting in threats for the software system’s success and increased costs. However, software architecture documentation is often missing or outdated. One explanation for this phenomenon is the tedious and costly process of creating documentation in comparison to (perceived) low beneﬁts. In this paper, we ﬁrst present our long-term vision, where we plan to persist information from any sources, e.g. from whiteboard discussions, to avoid losing crucial information about a system. A core problem in this vision is the possible inconsistency of information from different sources. A major
challenge of ensuring consistency is the consistency between formal artefacts, i.e. models, and informal documentation. We plan to address consistency analyses between models and textual natural language artefacts using natural language understanding and plan to include knowledge bases to improve these analyses.
After extracting information out of the natural language documents, we plan to create traceability links and check whether statements within the textual documentation are consistent with the software architecture models. In this paper, we also outline our requirements for evaluating our approach with the help of a community-wide infrastructure and how our approach can be used to maintain community-wide case studies.
MOESM1 of Systemic Administration of a Cyclic Signal Transducer and Activator of Transcription 3 (STAT3) Decoy Oligonucleotide Inhibits Tumor Growth without Inducing Toxicological Effects
Creators: name: Sen, Malabika
name: Paul, Kathleen
name: Freilino, Maria
name: Li, Hua
name: Li, Changyou
name: Johnson, Daniel
name: Wang, Lin
name: Eiseman, Julie
name: Grandis, Jennifer
Publisher: name: figshare
Year: 2013
Subjects: Biochemistry
Molecular Biology
Pharmacology
Biotechnology
Cancer

description: Supplementary material, approximately 1.19 MB.
Survival amplitude, instantaneous energy and decay rate of an unstable system: Analytical results
Creators: name: Raczynska, K.
name: Urbanowski, K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider a model of a unstable state defined by the truncated Breit-Wigner energy density distribution function. An analytical form of the survival amplitude $a(t)$ of the state considered is found. Our attention is focused on the late time properties of $a(t)$ and on effects generated by the non--exponential behavior of this amplitude in the late time region: In 1957 Khalfin proved that this amplitude tends to zero as $t$ goes to the infinity more slowly than any exponential function of $t$. This effect can be described using a time-dependent decay rate $γ(t)$ and then the Khalfin result means that this $γ(t)$ is not a constant but at late times it tends to zero as $t$ goes to the infinity. It appears that the energy $E(t)$ of the unstable state behaves similarly: It tends to the minimal energy $E_{min}$ of the system as $t \to \infty$. Within the model considered we find two first leading time dependent elements of late time asymptotic expansions of $E(t)$ and $γ(t)$. We discuss also possible implications of such a late time asymptotic properties of $E(t)$ and $γ(t)$ and cases where these properties may manifest themselves.
description: 24 pages, 4 figures, typos corrected, commnts added
Optimal Operation of Cascade Reservoir Systems under Climate Change: Case Study of Tekeze Hydropower Reservoir in the Tributary of the Blue Nile River
Creators: name: F. Abera, Fikru
name: Shumete, Asalf
Publisher: name: Abyssinia Journal of Engineering and Computing
Year: 2021

description: Planning and optimal operation of reservoirs under the paradigm of climate change is one of the most momentous problems in the planning and management of water resources due to the rapid growth of economy and population. In this study, Soil and Water Assessment Tool (SWAT) and reservoir operation optimization (HEC-ResPRM) models have been employed in the three cascade hydropower reservoirs in Tekeze basin, Ethiopia to investigate the impact of planned cascade reservoirs’ operation on the existing reservoir on the face of climate change. Results showed that an increase in rainfall and temperature in the future will be critical to future inflow in cascade hydropower reservoirs, with rainfall variability having a greater impact than temperature variability. HEC-ResPRM was prepared to reproduce optimum hydropower reservoir storage and water levels on the joint cascade operation of Tekeze reservoirs in each mode under climate change effect. Joint optimum operation of cascade reservoirs in different operation modes under climate change in both RCP4.5 and RCP8.5 climate scenarios affects existing reservoir operation in the future. Therefore, it is better to improve existing reservoir operation before investing into new planned cascade reservoirs and incorporate climate change scenarios in the planning, design, and operation of new reservoirs in Tekeze Basin. The results of this study can help the water resources planners and managers to plan and manage the future water resources of Ethiopian Rivers.
description: Abyssinia Journal of Engineering and Computing, Vol. 1 No. 2 (2021)
The Frequency of Barred Spiral Galaxies in the Near-IR
Creators: name: Eskridge, Paul B.
name: Frogel, Jay A.
name: Pogge, Richard W.
name: Quillen, Alice C.
name: Davies, Roger L.
name: DePoy, D. L.
name: Houdashelt, Mark L.
name: Kuchinski, Leslie E.
name: Ramirez, Solange V.
name: Sellgren, K.
name: Terndrup, Donald M.
name: Tiede, Glenn P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have determined the fraction of barred galaxies in the H-band for a statistically well-defined sample of 186 spirals drawn from the Ohio State University Bright Spiral Galaxy survey. We find 56% of our sample to be strongly barred at H, while another 16% is weakly barred. Only 27% of our sample is unbarred in the near-infrared. The RC3 and the Carnegie Atlas of Galaxies both classify only about 30% of our sample as strongly barred. Thus strong bars are nearly twice as prevalent in the near-infrared as in the optical. The frequency of genuine optically hidden bars is significant, but lower than many claims in the literature: 40% of the galaxies in our sample that are classified as unbarred in the RC3 show evidence for a bar in the H-band, while for the Carnegie Atlas this fraction is 66%. Our data reveal no significant trend in bar fraction as a function of morphology in either the optical or H-band. Optical surveys of high redshift galaxies may be strongly biased against finding bars, as bars are increasingly difficult to detect at bluer rest wavelengths.
description: LaTeX with AASTeX style file, 23 pages with 6 figures. Accepted for publication in The Astronomical Journal (Feb. 2000)
Additional file 5: of Genetic variation and structure of maize populations from Saoura and Gourara oasis in Algerian Sahara
Creators: name: Miyassa Aci
name: Lupini, Antonio
name: Mauceri, Antonio
name: Abdelkader Morsli
name: Khelifi, Lakhdar
name: Sunseri, Francesco
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Plant Biology

description: Table S7. Landraces summary statistics based on SSR analysis. (DOCX 14 kb)
All-electrical manipulation of silicon spin qubits with tunable spin-valley mixing
Creators: name: Bourdet, Léo
name: Niquet, Yann-Michel
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We show that the mixing between spin and valley degrees of freedom in a silicon quantum bit (qubit) can be controlled by a static electric field acting on the valley splitting $Δ$. Thanks to spin-orbit coupling, the qubit can be continuously switched between a spin mode (where the quantum information is encoded into the spin) and a valley mode (where the the quantum information is encoded into the valley). In the spin mode, the qubit is more robust with respect to inelastic relaxation and decoherence, but is hardly addressable electrically. It can however be brought into the valley mode then back to the spin mode for electrical manipulation. This opens new perspectives for the development of robust and scalable, electrically addressable spin qubits on silicon. We illustrate this with tight-binding simulations on a so-called "corner dot" in a silicon-on-insulator device where the confinement and valley splitting can be independently tailored by a front and a back gate.
Effects of Anaerobic Co-digestion of Cow Dung using Biodegradable Municipal Wastes for Biogas Production
Creators: name: Lissanu, Teklie
name: Assefa, Animut
name: Ayalew, Assamen
name: Gemeda, Samuel
Publisher: name: Abyssinia Journal of Engineering and Computing
Year: 2021

description: Biogas is a renewable energy resource produced by anaerobic digestion (AD). Biogas production trough anaerobic digestion was found to be unstable when the cattle manure is used as mono substrate due to the low carbon to nitrogen ratio. The aim of this research is to extract biogas by anaerobic-digestion technique using cow dung (CD) and municipal solid waste (MSW) at different proportions. It was carried out by 15, 0.5 L digesters at 38 °C using oven atmesophilic condition. Samples were analysed for its total solids (TS), volatile solids (VS), fixed solids, organic carbon, moisture content, and potential of hydrogen (pH) according to standard method for the examination of water and wastewater. Biogas yield was recorded by using volume displacement method. Maximum cumulative biogas production by the substrate mixes of 0% MSW+100% CD (2818.3 ml) and a maximum daily biogas production for 75% CD+25% MSW (620 ml) with minimum of 0 ml for all substrate mix at end of day 22. Cumulative biogas yield of 100% CD digestion was found to be better yielding. It is also observed that, co-digestion of MSW with cow dung does not increase the amount of biogas production over only with 100 % CD. However, cow dung added with MSW has enhanced the amount of biogas yield and reduction in percentage of VS and TS as compared to 100 % MSW.
description: Abyssinia Journal of Engineering and Computing, Vol. 1 No. 2 (2021)
Concurrent Changes to Hadley Circulation and the Meridional Distribution of Tropical Cyclones
Creators: name: Studholme, Joshua H. P.
name: Gulev, Sergey K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: Poleward trends in seasonal-mean latitudes of tropical cyclones (TCs) have been identified in direct observations from 1980 to present. Paleoclimate reconstructions also indicate poleward-equatorward migrations over centennial to millennial timescales. Hadley circulation (HC) is often both implicitly and explicitly invoked to provide dynamical linkages to these shifts, although no direct analysis of concurrent changes in the recent period has been presented. Here the observational TC record (1981-2016) and the ERA-Interim, JRA55 and MERRA2 reanalyses are studied to examine potential relationships between the two. A zonally-asymmetric HC is defined by employing Helmholtz theory for vector decomposition and this permits the derivation of novel HC diagnostics local to TC basins. Coherent variations in both long-term linear trends and detrended interannual variability are found. TC genesis and lifetime maximum intensity latitudes share trend sign and magnitude with shifts in local HC extent, with rates being ~0.25 plus/minus 0.1 degrees latitude decade-1. Both these lifecycle stages in hemispheric means and all Pacific TC basins, as well as poleward-extreme North Atlantic lysis latitudes, shared ~35% of their interannual variability with HC extent. Local HC intensity is linked only to eastern North Pacific TC latitudes, where strong local overturning corresponds to equatorward TC shifts. Examination of potential dynamical linkages implicates La Niña-like sea surface temperature gradients to poleward HC termini. This corresponds to increased tropical and reduced subtropical vertical wind shear everywhere except in the North Atlantic and western North Pacific, where the opposite is true. These results quantify a long-hypothesized link between TCs and the large-scale oceanic-atmospheric state.
description: In press in Journal of Climate (2018)
Additional file 3: of Genetic variation and structure of maize populations from Saoura and Gourara oasis in Algerian Sahara
Creators: name: Miyassa Aci
name: Lupini, Antonio
name: Mauceri, Antonio
name: Abdelkader Morsli
name: Khelifi, Lakhdar
name: Sunseri, Francesco
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Evolutionary Biology
subject: Ecology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Plant Biology

description: Table S6. Eigenvalues, variances and coefficients associated with first three principal components. (DOCX 15 kb)
Impact of Land Use Land Cover Dynamics on Stream Flow: A case of Borkena Watershed, Awash Basin, Ethiopia
Creators: name: Asmare Abebe, Metafet
name: Enku, Temesgen
name: Desale Meselaw, Tewodrose
name: Endris Ahmed, Seid
Publisher: name: Abyssinia Journal of Engineering and Computing
Year: 2021

description: Land use and land cover in recent decades have changed ecosystems more rapidly and extensively than in any comparable period. Land used land cover (LULC) change is one of the major factors that affect the watershed response. The LULC change analysis was performed by using supervised classification method in ENVI software. The study results showed that the watershed experienced significant LULC change from 1986 to 2016. During the study period, most parts of the grass land, cultivation land, and shrub land were changed to build-up area and bare Land. The LULC map shows an increase of buildup area and bare Land by 3.6% and 5.9% respectively over the last 31 years. The SWAT model was used to assess the impact of LULC change on stream flow for the period 1996 to 2016. The result showed that there was a good agreement between observed and simulated stream flow with a coefficient of determination (R) and NashSutcliff efficiency (Nef) values of 0.81 and 0.79 for calibration, and 0.75 and 0.74 for validation periods, respectively. The evaluation of the SWAT hydrologic response unit (HRU) due to LULC change between the years 1996 and 2016 showed that monthly stream flow was increased by 5.4 m3 /s in wet season and decreased by 0.5 m3/s in dry season from 1996 to 2016. Understanding the effect of LULC change on stream flow is crucial for knowledge-based decision making in the development of water resources projects.
description: Abyssinia Journal of Engineering and Computing, Vol. 1 No. 2 (2021)
Additional file 9: of Global identification and characterization of lncRNAs that control inflammation in malignant cholangiocytes
Creators: name: Han, Bo-Wei
name: Ye, Hua
name: Wei, Pan-Pan
name: He, Bo
name: Han, Cai
name: Chen, Zhen-Hua
name: Chen, Yue-Qin
name: Wang, Wen-Tao
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified

description: Table S6. Genome-wide correlation between lncRNA and mRNA levels (Pearson correlation coefficientâ >â 0.95). (DOCX 221 kb)
Imaging of objects through a thin scattering layer using a spectrally and spatially separated reference
Creators: name: Xu, Xiaoqing
name: Xie, Xiangsheng
name: Thendiyamma, Abhilash
name: Zhuang, Huichang
name: Xie, Junpeng
name: Liu, Yikun
name: Zhou, Jianying
name: Mosk, Allard P
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Incoherently illuminated or luminescent objects give rise to a low-contrast speckle-like pattern when observed through a thin diffusive medium, as such a medium effectively convolves their shape with a speckle-like point spread function (PSF). This point spread function can be extracted in the presence of a reference object of known shape. Here it is shown that reference objects that are both spatially and spectrally separated from the object of interest can be used to obtain an approximation of the point spread function. The crucial observation, corroborated by analytical calculations, is that the spectrally shifted point spread function is strongly correlated to a spatially scaled one. With the approximate point spread function thus obtained, the speckle-like pattern is deconvolved to produce a clear and sharp image of the object on a speckle-like background of low intensity.
Redshifts of the Gravitational Lenses MG1131+0456 and B1938+666
Creators: name: Tonry, John L.
name: Kochanek, Christopher S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The redshifts of the gravitational lens galaxies in MG1131+0456 and B1938+666 are 0.844 and 0.881 respectively. Both are early-type galaxies lying at the redshifts predicted by assuming that they are early-type galaxies with old stellar populations lying on the fundamental plane. We also find evidence for a foreground group of galaxies at z=0.343 near MG1131+0456. The source redshifts are predicted to be >1.8 in both systems, but they are so red that infrared spectra will be required to determine their redshifts.
description: 10 pages, AASTeX Latex, including 1 JPEG and 2 postscript figures, submitted to Astronomical Journal Minor typos fixed
Gas, Dust, Stars, Star Formation and their Evolution in M33 at Giant Molecular Cloud Scales
Creators: name: Komugi, Shinya
name: Miura, Rie E.
name: Kuno, Nario
name: Tosaki, Tomoka
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: We report on a multi parameter analysis of giant molecular clouds (GMCs) in the nearby spiral galaxy M33. A catalog of GMCs identifed in 12CO(J=3-2) was used to compile associated 12CO(J=1-0), dust, stellar mass and star formation rate. Each of the 58 GMCs are categorized by their evolutionary stage. Applying the principal component analysis on these parameters, we construct two principal components PC1 and PC2 which retain 75% of the information in the original dataset. PC1 is interpreted as expressing the total interstellar matter content, and PC2 as the total activity of star formation. Young (<10Myr) GMCs occupy a distinct region in the PC1-PC2 plane, with lower ISM content and star formation activity compared to intermediate age and older clouds. Comparison of average cloud properties in different evolutionary stages imply that GMCs may be heated or grow denser and more massive via aggregation of diffuse material in their first ~10 Myr. The PCA also objectively identified a set of tight relations between ISM and star formation. The ratio of the two CO lines is nearly constant, but weakly modulated by massive star formation. Dust is more strongly correlated with the star formation rate than the CO lines, supporting recent findings that dust may trace molecular gas better than CO. Stellar mass contributes weakly to the star formation rate, reminiscent of an extended form of the Schmidt Kennicutt relation with the molecular gas term substituted by dust.
description: 9 pages, 3 figures, accepted for publication in PASJ
Stellar Populations of the Sagittarius Dwarf Irregular Galaxy
Creators: name: Lee, Myung Gyoon
name: Kim, Sang Chul
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present deep BVRI CCD photometry of the stars in the dwarf irregular galaxy SagDIG. The color-magnitude diagrams of the measured stars in SagDIG show a blue plume which consists mostly of young stellar populations, and a well-defined red giant branch (RGB). The foreground reddening of SagDIG is estimated to be E(B-V)=0.06. The tip of the RGB is found to be at I_(TRGB)=21.55 +/- 0.10 mag. From this the distance to this galaxy is estimated to be d = 1.18 +/- 0.10 Mpc. This result, combined with its velocity information, shows that it is a member of the Local Group. The mean metallicity of the red giant branch is estimated to be [Fe/H] < -2.2 dex. This shows that SagDIG is one of the most metal-poor galaxies. Total magnitudes of SagDIG (< r_H (= 107 arcsec)) are derived to be B^T=13.99 mag, V^T=13.58 mag, R^T=13.19 mag, and I^T=12.88 mag, and the corresponding absolute magnitudes are M_B=-11.62 mag, M_V=-11.97 mag, M_R=-12.33 mag, and M_I=-12.60 mag. Surface brightness profiles of the central part of SagDIG are approximately fit by a King model with a core concentration parameter c = log (r_t / r_c) ~ 0.6, and those of the outer part follow an exponential law with a scale length of 37 arcsec. The central surface brightness is measured to be mu_B (0) = 24.21 mag arcsec^(-2) and mu_V (0) =23.91 mag arcsec^(-2). The magnitudes and colors of the brightest blue and red stars in SagDIG (BSG and RSG) are measured to be, respectively, _BSG = 19.89 +/- 0.13 mag, _BSG = 0.08 +/- 0.07 mag, _RSG = 20.39 +/- 0.10 mag, and _RSG = 1.29 +/- 0.12 mag. The corresponding absolute magnitudes are derived to be _BSG = -5.66 mag and _RSG = -5.16 mag, which are about one magnitude fainter than those expected from conventional correlations with galaxy luminosity.
description: 16 pages(AASLaTeX), 10 Postscript figures, Accepted for publication in Astronomical Journal, 2000
A Precise Determination of $α_s$ from Lattice QCD
Creators: name: Davies, C. T. H.
name: Hornbostel, K.
name: Lepage, G. P.
name: Lidsey, A.
name: Shigemitsu, J.
name: Sloan, J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We present a new determination of the QCD strong coupling constant based on precise lattice calculations of the $Υ$ spectrum. The largest systematic uncertainty in previous such determinations resulted from the absence of vacuum polarization from light quarks. We substantially reduce this error by including two flavors of dynamical light quarks and extrapolating to three. We find $\alphathree_\V(8.2~\GeV) = 0.196(3)$ for three light flavors, corresponding to $\alphafive_\msbar(M_Z) = 0.115(2)$. This is significantly more accurate than previous determinations using this or any other technique.
description: 11 pages (LaTeX), OHSTPY-HEP-T-94-013, FSU-SCRI-94-79 (includes minor corrections in tables, additional references)
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0385
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2012
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: LaMOP

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0385, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0385, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
The Dramatic Size and Kinematic Evolution of Massive Early-Type Galaxies
Creators: name: Lapi, A.
name: Pantoni, L.
name: Zanisi, L.
name: Shi, J.
name: Mancuso, C.
name: Massardi, M.
name: Shankar, F.
name: Bressan, A.
name: Danese, L.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: [ABRIDGED] We aim to provide a holistic view on the typical size and kinematic evolution of massive early-type galaxies (ETGs), that encompasses their high-$z$ star-forming progenitors, their high-$z$ quiescent counterparts, and their configurations in the local Universe. Our investigation covers the main processes playing a relevant role in the cosmic evolution of ETGs. Specifically, their early fast evolution comprises: biased collapse of the low angular momentum gaseous baryons located in the inner regions of the host dark matter halo; cooling, fragmentation, and infall of the gas down to the radius set by the centrifugal barrier; further rapid compaction via clump/gas migration toward the galaxy center, where strong heavily dust-enshrouded star-formation takes place and most of the stellar mass is accumulated; ejection of substantial gas amount from the inner regions by feedback processes, which causes a dramatic puffing up of the stellar component. In the late slow evolution, passive aging of stellar populations and mass additions by dry merger events occur. We describe these processes relying on prescriptions inspired by basic physical arguments and by numerical simulations, to derive new analytical estimates of the relevant sizes, timescales, and kinematic properties for individual galaxies along their evolution. Then we obtain quantitative results as a function of galaxy mass and redshift, and compare them to recent observational constraints on half-light size $R_e$, on the ratio $v/σ$ between rotation velocity and velocity dispersion (for gas and stars) and on the specific angular momentum $j_\star$ of the stellar component; we find good consistency with the available multi-band data in average values and dispersion, both for local ETGs and for their $z\sim 1-2$ star-forming and quiescent progenitors.
description: 28 pages, 10 figures. Accepted by ApJ
Correlated Dynamics in Aqueous Proton Diffusion
Creators: name: Fischer, Sean A.
name: Dunlap, Brett I.
name: Gunlycke, Daniel
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: The aqueous proton displays an anomalously large diffusion coefficient that is up to 7 times that of similarly sized cations. There is general consensus that the proton achieves its high diffusion through the Grotthuss mechanism, whereby protons hop from one molecule to the next. A main assumption concerning the extraction of the timescale of the Grotthuss mechanism from experimental results has been that, on average, there is an equal probability for the proton to hop to any of its neighboring water molecules. Herein, we present ab initio simulations that show this assumption is not generally valid. Specifically, we observe that there is an increased probability for the proton to revert back to its previous location. These correlations indicate that the interpretation of the experimental results need to be re-examined and suggest that the timescale of the Grotthuss mechanism is significantly shorter than was previously thought.
Additional file 1: of Genetic variation and structure of maize populations from Saoura and Gourara oasis in Algerian Sahara
Creators: name: Miyassa Aci
name: Lupini, Antonio
name: Mauceri, Antonio
name: Abdelkader Morsli
name: Khelifi, Lakhdar
name: Sunseri, Francesco
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology

description: Table S4. Augmented ANOVA (mean squares) for 24 agro-morphological traits in 47 Algerian maize landraces and 7 checks. (DOCX 17 kb)
Foulkes et al_Supplement.docx
Creators: name: Foulkes, Stephen
name: D Wagner, Peter
name: Wang, Jing
name: LaGerche, Andre
name: Haykowsky, Mark J
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 420702
subject: Exercise physiology

description: Supplementary Figure S1. Flow of trials through the search and screening process.
Hard X-ray detection of the high redshift quasar 4C 71.07
Creators: name: Malizia, A.
name: Bassani, L.
name: Dean, A. J.
name: McCollough, M.
name: Stephen, J. B.
name: Zhang, S. N.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: BATSE/OSSE observations of the high redshift quasar 4C 71.07 indicate that this is the brightest and furthest AGN so far detected above 20 keV. BATSE Earth occultation data have been used to search for emission from 4C 71.07 from nearly 3 years of observation. The mean source flux over the whole period in the BATSE energy range 20-100 keV is (13.2 +/- 1.06) x 10^(-11) erg cm^(-2) s^(-1) corresponding to a luminosity of 2 x 10^(48) erg s^(-1). The BATSE light curve over the 3 years of observations shows several flare-like events, one of which (in January 1996) is associated with an optical flare (R=16.1) but with a delay of 55 days. The OSSE/BATSE spectral analysis indicates that the source is characterized by a flat power spectrum (Gamma about 1.1 - 1.3) when in a low state; this spectral form is consistent within errors with the ASCA and ROSAT spectra. This means that the power law observed from 0.1 to 10 keV extends up to at least 1 MeV but steepens soon after to meet EGRET high energy data. BATSE data taken around the January 1996 flare suggests that the spectrum could be steeper when the source is in a bright state. The nuF-nu representation of the source is typical of a low frequency peaked/gamma-ray dominated blazar, with the synchrotron peak in the mm-FIR band and the Compton peak in the MeV band. The BATSE and OSSE spectral data seem to favour a model in which the high energy flux is due to the sum of the synchrotron self-Compton and the external Compton contributions; this is also supported by the variability behaviour of the source.
description: 19 pages, LaTeX, plus 4 .ps figures. accepted by Astrophysical Journal
Use of Crop Water Stress Index to Improve Irrigation Scheduling for Wheat Crop in Koga Irrigation Scheme, Ethiopia
Creators: name: Desale, Tewodrose
name: Atanaw, Fasikaw
name: Schmitter, Petra
name: Tilahun, Seifu
Publisher: name: Abyssinia Journal of Engineering and Computing
Year: 2021

description: Water status detection by thermal imaging is a non-invasive and rapid assessment method; it provides great potential to improve irrigation planning. This research evaluates the use of crop water stress index to improve irrigation scheduling for the wheat crop. Besides, the effects of different irrigation scheduling on the yield, canopy temperature, crop water stress index (CWSI), and irrigation water productivity of wheat crop were investigated. An infrared thermometry handheld thermal camera was used to detect the temperature of wheat canopies under three different irrigation treatments: wetting front detector (WFD), Chameleon, and current practices by farmers as control. The result indicated that there were no significant differences (p>0.05) in the effect of irrigation treatment on the CWSI during the different crop phonological stages. This shows that irrespective of the irrigation scheduling method, the CWSI could be determined. The maximum Irrigation Water Productivity (IWP) of the two blocks was from the WFD field which was 0.72kg/m3, 0.64 kg/m3 for Adibera and Chihona block respectively which was significant (p<0.05) at both blocks within control farmer however there was no significant difference between the two technology (WFD and Chameleon).From the result both irrigation treatment irrigates when the CWSI reaches with rang of 0.4 to 0.6, this suggests that the wheat in Koga irrigation scheme should be irrigated when the CWSI reaches a value of 0.4 up to 0.6.
description: Abyssinia Journal of Engineering and Computing, Vol. 1 No. 2 (2021)