cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
NGC 2362: a Template for Early Stellar Evolution
Creators: name: Moitinho, A.
name: Alves, J.
name: Huelamo, N.
name: Lada, C.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present UBVRI photometry for the young open cluster NGC 2362. From analysis of the appropriate color-color and color-magnitude diagrams we derive the fundamental parameters of the NGC 2362 cluster to be: age = 5 (+1-2) Myr, distance = 1480 pc, E(B-V)=0.10 mag. The cluster age was independently determined for both high mass (2.1 - 36Msun) and low mass (0.7 - 1.2Msun) stars with excellent agreement between the ages derived using post-main sequence and pre-main sequence evolutionary tracks for the high and low mass stars respectively. Analysis of this cluster's color-magnitude diagram reveals a well defined pre-main sequence (covering DeltaV ~ 9 magnitudes in V and extending from early A stars to near the hydrogen burning limit) which makes this cluster an ideal laboratory for pre-main sequence evolution studies.
description: 9 pages, 3 figures, to be published in ApJL
The X-Ray Position and Infrared Counterpart of the Eclipsing X-Ray Pulsar OAO 1657-415
Creators: name: Chakrabarty, Deepto
name: Wang, Zhongxiang
name: Juett, Adrienne M.
name: Lee, Julia C.
name: Roche, Paul
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have measured the precise position of the 38-s eclipsing X-ray pulsar OAO 1657-415 with the Chandra X-Ray Observatory: RA = 17h00m48.90s, Dec = -41d39m21.6s, equninox J2000, error radius = 0.5 arcsec. Based on the previously measured pulsar mass function and X-ray eclipse duration, this 10.4-d high-mass X-ray binary is believed to contain a B supergiant companion. Deep optical imaging of the field did not detect any stars at the Chandra source position, setting a limit of V>23. However, near-IR imaging revealed a relatively bright star (J=14.1, H=11.9, K_s=10.7) coincident with the Chandra position, and we identify this star as the IR counterpart of OAO 1657-415. The IR colors and magnitudes and the optical non-detections for this star are all consistent with a highly reddened B supergiant (A_V= 20.4 +/- 1.3) at a distance of 6.4 +/- 1.5 kpc. This implies an X-ray luminosity of 3e36 erg/s (2-10 keV). IR spectroscopy can verify the spectral type of the companion and measure its radial velocity curve, yielding a neutron star mass measurement.
description: 4 pages. ApJ in press (Vol. 573, July 10 issue)
Aulacocypus cavazuttii SMETANA 2003
Creators: name: Smetana, A.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Aulacocypus
Aulacocypus cavazuttii

description: Aulacocypus cavazuttii SMETANA 2003
 Aulacocypus cavazuttii SMETANA 2003: 115.
N e w r e c o r d s: C h i n a: Hubei: Dashenongjia mts. 31.5N 110.3E, 24500- 2900m, 23.6.- 14.7. 2003, leg. J. Turna, 3 (ASC, NMW).
C o m m e n t s: This is the first record of this species from Hubei.
description: Published as part of Smetana, A., 2008, Contributions to the knowledge of the " Staphylinus-complex " (Insecta: Coleoptera, Staphylinidae, Staphylinini) of China. Part 18. Various genera, pp. 943-949 in Linzer biologische Beiträge 40 (1) on page 948, DOI: 10.5281/zenodo.5429958
title: Distance and Immediacy: Investigating narratives of portability
Creators: name: West, Fiona
Publisher: name: Griffith University
Year: 2019
Subjects: subject: South Africa
subject: Puppets
subject: Dolls
subject: Collage

description: With reference to the global emigration of South Africans (South African diaspora), this thesis explores themes of displacement, identity and cultural belonging. The hybrid figurine of a modified hula doll, adapted specifically from tourist memorabilia is used as a key motif in my investigation of narratives of portability and the portability of identity in particular. My research relies on a mix of puppet and collage typology, and the manipulation of miniatures and scale that emphasize spatial experiences. Hula dolls and a plastic Kewpie Doll, directly referencing Ray Lawler’s Summer of the Seventeenth Doll, are recurring motifs. These figurines act as metaphors for implied journeys, displacement and transformation. I work with a wide range of materials and mixed mediums to construct imagined worlds, in which I choreograph light, handcrafted stencils and kinetic objects. I aim to reconcile my use of these contrived or synthetic constructions and assembled collages through the amplification of their artifice within my videos and photographs. Working within the established range of methodologies associated with practice-based research, I draw particularly on phenomenology as lived experience, and utilize the phenomenological perspective of Merleau-Ponty. The aim of the studio investigation is to add to an understanding of the experience of South Africans living in Australia and perhaps the broader narrative and other mechanisms of displacement and construction of identity.
Convergence issues in derivatives of Monte Carlo null-collision integral formulations: a solution
Creators: name: Tregan, J-M
name: Blanco, S.
name: Dauchet, J.
name: Hafi, M
name: Fournier, R.
name: Ibarrart, L
name: Lapeyre, P
name: Villefranque, N
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: When a Monte Carlo algorithm is used to evaluate a physical observable A, it is possible to slightly modify the algorithm so that it evaluates simultaneously A and the derivatives $\partial$ $ς$ A of A with respect to each problem-parameter $ς$. The principle is the following: Monte Carlo considers A as the expectation of a random variable, this expectation is an integral, this integral can be derivated as function of the problem-parameter to give a new integral, and this new integral can in turn be evaluated using Monte Carlo. The two Monte Carlo computations (of A and $\partial$ $ς$ A) are simultaneous when they make use of the same random samples, i.e. when the two integrals have the exact same structure. It was proven theoretically that this was always possible, but nothing insures that the two estimators have the same convergence properties: even when a large enough sample-size is used so that A is evaluated very accurately, the evaluation of $\partial$ $ς$ A using the same sample can remain inaccurate. We discuss here such a pathological example: null-collision algorithms are very successful when dealing with radiative transfer in heterogeneous media, but they are sources of convergence difficulties as soon as sensitivity-evaluations are considered. We analyse theoretically these convergence difficulties and propose an alternative solution.
Phase mixing of a three dimensional magnetohydrodynamic pulse
Creators: name: Tsiklauri, D.
name: Nakariakov, V. M.
name: Rowlands, G.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Phase mixing of a three dimensional magnetohydrodynamic (MHD) pulse is studied in the compressive, three-dimensional (without an ignorable coordinate) regime. It is shown that the efficiency of decay of an Alfvenic part of a compressible MHD pulse is related linearly to the degree of non-planeness of the pulse in the homogeneous transverse direction. In the developed stage of phase mixing (for large times), coupling to its compressive part does not alter the power-law decay of an Alfvenic part of a compressible MHD pulse. The same applies to the dependence upon the resistivity of the Alfvenic part of the pulse. All this implies that the dynamics of Alfven waves can still be qualitatively understood in terms of the previous 2.5D models. Thus, the phase mixing remains a relevant paradigm for the coronal heating applications in the realistic 3D geometry and compressive plasma.
description: final accepted version Astron. Astrophys
Veri Yönetim Planları, FAIR Prensipleri
Creators: name: Alper, Pınar
Publisher: name: Zenodo
Year: 2021
Subjects: veri yönetim planı
FAIR prensipleri
Araştırma Verilerinin Yönetimi
UAVS2021

description: 25-26 Mayıs 2021 Ulusal Araştırma Verileri Sempozyumu Araştırma Verilerinin Yönetimi Veri Yönetim Planı Hangi Başlıklardan Oluşur? FAIR Prensipleri nedir? FAIR olmaya giden yollar nelerdir?
Additional file 17 of A systems genetics approach reveals PbrNSC as a regulator of lignin and cellulose biosynthesis in stone cells of pear fruit
Creators: name: Wang, Runze
name: Xue, Yongsong
name: Fan, Jing
name: Yao, Jia-Long
name: Qin, Mengfan
name: Lin, Tao
name: Lian, Qun
name: Zhang, Mingyue
name: Li, Xiaolong
name: Li, Jiaming
name: Sun, Manyi
name: Song, Bobo
name: Zhang, Jiaying
name: Zhao, Kejiao
name: Chen, Xu
name: Hu, Hongju
name: Fei, Zhangjun
name: Xue, Cheng
name: Wu, Jun
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 17. Review history.
Globular Clusters and the Mira Period-Luminosity Relation
Creators: name: Feast, Michael
name: Whitelock, Patricia
name: Menzies, John
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A globular cluster distance scale based on Hipparcos parallaxes of subdwarfs has been used to derive estimates of M_K for cluster Miras, including one in the SMC globular cluster NGC121. These lead to a zero-point of the Mira infrared period-luminosity relation, PL(K), in good agreement with that derived from Hipparcos parallaxes of nearby field Miras. The mean of these two estimates together with data on LMC Miras yields an LMC distance modulus of 18.60 +/- 0.10 in evident agreement with a metallicity corrected Cepheid modulus (18.59 +/- 0.10). The use of luminous AGB stars as extragalactic population indicators is also discussed.
description: 6 pages, 3 figures, to be published in MNRAS (pink pages)
Chaos in networks of coupled oscillators with multimodal natural frequency distributions
Creators: name: Smith, Lachlan D.
name: Gottwald, Georg A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Dynamical Systems (math.DS)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We explore chaos in the Kuramoto model with multimodal distributions of the natural frequencies of oscillators and provide a comprehensive description under what conditions chaos occurs. For a natural frequency distribution with $M$ peaks it is typical that there is a range of coupling strengths such that oscillators belonging to each peak form a synchronized cluster, but the clusters do not globally synchronize. We use collective coordinates to describe the inter- and intra-cluster dynamics, which reduces the Kuramoto model to $2M-1$ degrees of freedom. We show that under some assumptions, there is a time-scale splitting between the slow intracluster dynamics and fast intercluster dynamics, which reduces the collective coordinate model to an $M-1$ degree of freedom rescaled Kuramoto model. Therefore, four or more clusters are required to yield the three degrees of freedom necessary for chaos. However, the time-scale splitting breaks down if a cluster intermittently desynchronizes. We show that this intermittent desynchronization provides a mechanism for chaos for trimodal natural frequency distributions. In addition, we use collective coordinates to show analytically that chaos cannot occur for bimodal frequency distributions, even if they are asymmetric and if intermittent desynchronization occurs.
Luminous Matter Distribution, Bulk Flows and Baryon Contents in Cosmological Models with a Local Void
Creators: name: Tomita, Kenji
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: First, we consider galaxy formation from the viewpoint of hierarchical clustering theory and discuss the possibility that inhomogeneous models with a local void may be compatible with the observed homogeneity of galactic distributions found by recent redshift surveys, because their inhomogeneity can be weakened by the difference in the feedback system of galaxy formation between the inner and outer regions. Next, it is shown with the results of numerical simulations that the observed inhomogeneity of two-point correlations of galaxies can be accounted for by these models. Also, the natural appearance of bulk flows for an off-central observer is shown. Finally the inhomogeneity of baryon contents is discussed from the viewpoint of our inhomogeneous models.
description: 15 pages, 5 figures
title: Private Sector Participation in Municipal Solid Waste Management in Indian Cities and its Implications
Creators: name: Sandhu, Kirandeep
Publisher: name: Griffith University
Year: 2017
Subjects: subject: Municipal solid waste, India
subject: Municipal solid waste disposal, Privatisation
subject: Sustainability assessment framework, Amritsar, India

description: The most visible outcome of the increasing pace of urbanisation, along with the rise in the spate of consumerism in the liberalised economic setup, has been the sharp increase in municipal solid waste generation across the urban centres in the developing countries. As the challenge of providing this service becomes more and more pressing, municipalities are turning to the private sector to fill the gap and become the prime service providers. Privatisation of solid waste management services has thus emerged as „the‟ alternative and, as such, several municipalities have taken hasty steps to introduce private sector participation in solid waste management services, treating it as a panacea for the municipal solid waste management woes of the cities. The logic of private sector participation in municipal solid waste management services hinges on the assertion of it performing more efficiently on all fronts. While there is a flurry of rhetoric and excitement around private participation in municipal solid waste management services across Indian cities, there is an acute lack of empirical evidence and research (MoUD, 2010, Anderson, 2011) assessing the impacts of private sector participation in municipal solid waste management. Moreover, none of these studies, to the best knowledge of the researcher, have been conducted explicitly and in detail in conjunction with the principles of sustainability of municipal solid waste management systems.
Foreign ownership and global city characteristics: unpacking the connectivity of micro-locations
Creators: name: Asmussen, Christian Geisler
name: Nielsen, Bo Bernhard
name: Weatherall, Cecilie Dohlmann
name: Lyngemark, Ditte Håkonsson
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology

description: This paper develops the idea that global city characteristics in distinct micro-locations attract foreign and domestic firms differentially. The hypotheses are tested on a large data set of workplaces during the period 2007–16 and a complex relationship is found between global connectivity and foreign-owned location choice. Specifically, global infrastructure is strongly associated with foreign ownership in the upstream value chain (manufacturing or wholesale), whereas cosmopolitanism exhibits a stronger association with foreign ownership in downstream value-chain activities, such as retail. The agglomeration of producer services in a given location and the likelihood of foreign ownership in that location is higher in highly knowledge-intensive industries.
Thermal conductivity of the quantum spin liquid candidate EtMe3Sb[Pd(dmit)2]2: No evidence of mobile gapless excitations
Creators: name: Bourgeois-Hope, P.
name: Laliberté, F.
name: Lefrançois, E.
name: Grissonnanche, G.
name: de Cotret, S. René
name: Gordon, R.
name: Kitou, S.
name: Sawa, H.
name: Cui, H.
name: Kato, R.
name: Taillefer, L.
name: Doiron-Leyraud, N.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The thermal conductivity $κ$ of the quasi-2D organic spin-liquid candidate EtMe$_3$Sb[Pd(dmit)$_2$]$_2$ (dmit-131) was measured at low temperatures, down to 0.07 K. We observe a vanishingly small residual linear term $κ_0/T$, in $κ/T$ vs $T$ as $T \to 0$. This shows that the low-energy excitations responsible for the sizeable residual linear term $γ$ in the specific heat $C$, seen in $C/T$ vs $T$ as $T \to 0,$ are localized. We conclude that there are no mobile gapless excitations in this spin liquid candidate, in contrast with a prior study of dmit-131 that reported a large $κ_0/T$ value [Yamashita et al., Science 328, 1246 (2010)]. Our study shows that dmit-131 is in fact similar to $κ$-(BEDT-TTF)$_2$Cu$_2$(CN)$_3$, another quasi-2D organic spin-liquid candidate where a vanishingly small $κ_0/T$ and a sizeable $γ$ are seen. We attribute heat conduction in these organic insulators without magnetic order to phonons undergoing strong spin-phonon scattering, as observed in several other spin-liquid materials.
description: This revision includes a response to Yamashita's paper [M. Yamashita, Journal of the Physical Society of Japan 88, 083702 (2019)], data on a new sample, two new figures (Figs. 5 and 8), and a Supplementary Material (available upon request)
Veri Yönetim Planı Hazırlama: TÜBİTAK Veri Yönetim Planı
Creators: name: YAVUZ, BEGUM
Publisher: name: Zenodo
Year: 2021
Subjects: veri yönetim planı hazırlama
TÜBİTAK Veri Yönetim Planı
Araştırma Verilerinin Yönetimi
UAVS2021

description: 25-26 Mayıs 2021 Ulusal Araştırma Verileri Sempozyumu Veri yönetim planı nasıl yazılır? TÜBİTAK Veri Yönetim Planı Örneği Araştırma Verileri Yönetimi
Talauma inflata P. Parm.
Creators: name: Turner, I. M.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Magnoliales
Magnoliaceae
Talauma
Talauma inflata

description: 34. Talauma inflata P.Parm.
Bulletin scientifique de la France et de la Belgique 27: 208, 273, 274, 327, pl. VIII, fig. 10 (1896).
— Type: Sumatra, Mt Singalan, VI-VII.1878, O. Beccari P.S. 76 (holo-, P [P00734840]; iso-, BM, BO, FI-B, L).
Magnolia liliifera (L.) Baill.: Histoire des Plantes 1: 141 (1868) (Frodin & Govaerts 1996; Govaerts et al. 2012).
description: Published as part of Turner, I. M., 2012, The taxa described by Paul Évariste Parmentier in Histoire des Magnoliacées, pp. 237-249 in Adansonia (3) (3) 34 (2) on page 243, DOI: 10.5252/a2012n2a3, http://zenodo.org/record/5205948
Halectinosoma gothiceps
Creators: name: Clément, Michel
name: Moore, Colin G.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Hexanauplia
Harpacticoida
Ectinosomatidae
Halectinosoma
Halectinosoma gothiceps

description: HALECTINOSOMA GOTHICEPS (GIESBRECHT, 1881)
 Ectinosoma gothiceps Giesbrecht, 1881: 255
 Ektinosoma gothiceps Giesbrecht, 1882: 106, pl. I figs 3, 12, pl. IV fig. 17, 35, pl. V fig. 3, pl. VII fig. 8, pl. VIII figs 10–11, pl. IX fig. 17, pl. X figs 10, 21, pl. XI fig. 13, pl. XII fig. 6, 10
 Halectinosoma gothiceps Mielke, 1975: 23, fig. 9
 ? Ectinosoma (Halectinosoma) gothiceps Lang, 1948: 216–217, figs 112.10, 117.2
 ? Halectinosoma gothiceps Lang, 1965: 38
 Not Ectinosoma gothiceps Sars, 1904: 37, pl. XX fig. 2
 Material examined: Alaska: 2♀ from Island Flats, Port Valdez, collected by H. M. Feder, 6.ii.1973 (in R. Hamond’s personal collection). Scotland: S17 (4♀ dissected on six slides NHM1990.378–381, 1♂ dissected on two slides NHM1990.383, 9♀ in tubes NHM1990.1169 – 1177); S18 (20♀, 2♂ in tubes NHM1990.1180–1189 and NHM1990.1190 – 1191);
description: Published as part of Clément, Michel & Moore, Colin G., 2007, Towards a revision of the genus Halectinosoma (Copepoda, Harpacticoida, Ectinosomatidae): new species from the North Atlantic and Arctic regions, pp. 453-475 in Zoological Journal of the Linnean Society 149 (3) on page 462, DOI: 10.1111/j.1096-3642.2007.00267.x, http://zenodo.org/record/10114588
The Deep Lens Survey
Creators: name: Wittman, D.
name: Tyson, J. A.
name: Dell'Antonio, I. P.
name: Becker, A. C.
name: Margoniner, V. E.
name: Cohen, J.
name: Norman, D.
name: Loomba, D.
name: Squires, G.
name: Wilson, G.
name: Stubbs, C.
name: Hennawi, J.
name: Spergel, D.
name: Boeshaar, P.
name: Clocchiatti, A.
name: Hamuy, M.
name: Bernstein, G.
name: Gonzalez, A.
name: Guhathakurta, P.
name: Hu, W.
name: Seljak, U.
name: Zaritsky, D.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Deep Lens Survey (DLS) is a deep BVRz' imaging survey of seven 2x2 degree fields, with all data to be made public. The primary scientific driver is weak gravitational lensing, but the survey is also designed to enable a wide array of other astrophysical investigations. A unique feature of this survey is the search for transient phenomena. We subtract multiple exposures of a field, detect differences, classify, and release transients on the Web within about an hour of observation. Here we summarize the scientific goals of the DLS, field and filter selection, observing techniques and current status, data reduction, data products and release, and transient detections. Finally, we discuss some lessons which might apply to future large surveys such as LSST.
description: to appear in Proc. SPIE Vol. 4836. v2 contains very minor changes
title: Konzeption und Entwicklung eines Systems zur Verwaltung und Erstellung von Modulhandbüchern
Creators: name: Wylega, Tobias
Publisher: name: Hochschule Hannover
Year: 2025
Subjects: subject: 004 Informatik

description: Diese Bachelorarbeit befasst sich mit der Konzeption und Entwicklung eines webbasierten Systems zur Verwaltung und Erstellung von Modulhandbüchern. Ziel der Arbeit ist es, den bisherigen – durch manuelle Prozesse und redundante Datenpflege gekennzeichneten – Workflow an der Hochschule Hannover zu optimieren, um eine effiziente und benutzerfreundliche Alternative zu schaffen.

Ausgehend von einer fundierten Anforderungsanalyse – die unter anderem eine Aufstellung der Use Cases sowie eine kritische Betrachtung des bestehenden Systems umfasst – wird ein ganzheitlicher Lösungsansatz verfolgt. Die Implementierung beinhaltet die Weiterentwicklung eines Backends auf Basis von NestJS und Prisma sowie die Neuentwicklung eines Frontends mit Angular. Besondere Aufmerksamkeit gilt dabei der Codequalität, der Benutzerfreundlichkeit und der Mehrsprachigkeit, um ein langfristig wartbares, erweiterbares und benutzbares System zu gewährleisten.

Im Rahmen der Implementierung wird zudem ein automatisierter Prozess zur Generierung von PDF-Dokumenten integriert, der den administrativen Aufwand reduziert und die Konsistenz der Modulhandbücher sicherstellt. Die Evaluation des Prototyps zeigt, dass das entwickelte System die identifizierten Schwachstellen des bisherigen Prozesses adressiert und als solide Grundlage für zukünftige Arbeiten dient.
TÜBİTAK Veri Yönetimi Çalışmaları ve APERTA
Creators: name: Satoğlu, M. Mirat
Publisher: name: Zenodo
Year: 2021
Subjects: TÜBİTAK Veri Çalışmaları
Aperta
Harman
TÜBİTAK Veri Yönetim Planı
UAVS2021

description: 25-26 Mayıs 2021 Ulusal Araştırma Verileri Sempozyumu TÜBİTAK Veri Çalışmaları Aperta TÜBİTAK Veri Yönetim Planı Araştırma Verilerinin Yönetimi
High-resolution single-pulse studies of the Vela Pulsar
Creators: name: Kramer, M.
name: Johnston, S.
name: van Straten, W.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present high-resolution multi-frequency single-pulse observations of the Vela pulsar, PSR B0833-45, aimed at studying micro-structure, phase-resolved intensity fluctuations and energy distributions at 1.41 and 2.30 GHz. We show that the micro-pulse width in pulsars has a period dependence. Like individual pulses, Vela's micro-pulses are highly elliptically polarized. There is a strong correlation between Stokes parameters V and I in the micro-structure. We show that the V/I distribution is Gaussian with a narrow width and that this width appears to be constant as a function of pulse phase. The phase-resolved intensity distributions of I are best fitted with log-normal statistics. Extra emission components, i.e.``bump'' and ``giant micro-pulses'', discovered by Johnston et al.(2001) are also present at 2.3 GHz. The bump component seems to be an extra component superposed on the main pulse profile but does not appear periodically. The giant micro-pulses are time-resolved and have significant jitter in their arrival times. Their flux density distribution is best fitted by a power-law, indicating a link between these features and ``classical'' giant pulses as observed for the Crab pulsar, (PSR B0531+21), PSR B1937+21 and PSR B1821-24. We find that Vela contains a mixture of emission properties representing both ``classical'' properties of radio pulsars (e.g. micro-structure, high degree of polarization, S-like position angle swing, orthogonal modes) and features which are most likely related to high-energy emission (e.g. extra profile components, giant micro-pulses). It hence represents an ideal test case to study the relationship between radio and high-energy emission in significant detail.
description: accepted for publication in MNRAS (11 pages, 10 figures)
title: Integrated model for seabed instability around a breakwater
Creators: name: Li, Zhengxu
Publisher: name: Griffith University
Year: 2023
Subjects: subject: OpenFOAM
subject: breakwater
subject: wave-structure-seabed interaction

description: Coastal regions are experiencing a growing demand for various activities, including commerce, transportation, leisure, and industries, leading to the development of coastal areas and highlighting the need to manage and protect shorelines. Breakwaters, commonly used as coastal defence structures, play a crucial role in mitigating the destructive effects of ocean waves, such as beach erosion. However, breakwaters are exposed to harsh marine conditions and may experience soil liquefaction near their foundations, leading to structural failures. The interaction between fluids, structures, and seabed in the marine environment is complex and can contribute to the failure of breakwaters. To accurately assess breakwater stability and predict liquefaction potential, an integrated numerical model is developed in OpenFOAM that considers dynamic permeability effects and investigates the stability of breakwater foundations in both two-dimension (2D) and three-dimension (3D) engineering conditions. [...]
Omophlus anatolicus REITTER 1906
Creators: name: Yildirim, E.
name: Kiliç, E.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Tenebrionidae
Omophlus
Omophlus anatolicus

description: Omophlus anatolicus REITTER 1906
 Omophlus anatolicus REITTER 1906 - Verh. Nat. Ver. Brünn XLV: 155, Karakeny.
D i s t r i b u t i o n: Turkey.
description: Published as part of Yildirim, E. & Kiliç, E., 2008, Distributional checklist of the species of genus Omophlus (Insecta: Coleoptera; Alleculidae; Omophlinae) of Turkey, pp. 961-967 in Linzer biologische Beiträge 40 (1) on page 961, DOI: 10.5281/zenodo.5429972
Disentangling magnification in combined shear-clustering analyses
Creators: name: Thiele, Leander
name: Duncan, Christopher A. J.
name: Alonso, David
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate the sensitivity to the effects of lensing magnification on large-scale structure analyses combining photometric cosmic shear and galaxy clustering data (i.e. the now commonly called "3$\times$2-point" analysis). Using a Fisher matrix bias formalism, we disentangle the contribution to the bias on cosmological parameters caused by ignoring the effects of magnification in a theory fit from individual elements in the data vector, for Stage-III and Stage-IV surveys, assuming well-known redshift distributions, sample selection based on magnitude, and magnification strengths inferred from CFHTLenS and DES Y1 data. We show that the removal of elements of the data vectors that are dominated by magnification does not guarantee a reduction in the cosmological bias due to the magnification signal, but can instead increase the sensitivity to magnification. We find that the most sensitive elements of the data vector come from the shear-clustering cross-correlations, particularly between the highest-redshift shear bin and any lower-redshift lens sample, and that the parameters $Ω_{M}$, $S_8=σ_8\sqrt{Ω_M/0.3}$ and $w_0$ show the most significant biases for both survey models. Our forecasts predict that current analyses are not significantly biased by magnification, but this bias will become highly significant with the continued increase of statistical power in the near future. We therefore conclude that future surveys should measure and model the magnification as part of their flagship "3$\times$2-point" analysis.
description: 13 pages, 7 figures; matches MNRAS published version
title: Place Matters: Women's lived and Imagined Experience of Legal Practice in Regional, Rural and Remote Communities in Queensland
Creators: name: Mundy, Patricia Karen
Publisher: name: Griffith University
Year: 2013
Subjects: subject: Women lawyer's career choices
subject: Legal practice in remote and regional Queensland
subject: Female lawyers, Regional Queensland
subject: Legal practice ,Queensland

description: Female solicitors are not choosing to practise in regional, rural and remote (RRR) areas at the same rate as male solicitors and are more concentrated in city and suburban practice. Very little is understood about why this might be so. This thesis explores lived and ‘imagined’ experience and meaning-making as a way of understanding the attraction and retention of female solicitors in RRR communities. This study comprises two distinct but interrelated parts: the first involves a phenomenological study of the lived experience of female solicitors practising in RRR communities in Queensland. It asks 23 solicitors (male and female) about their experience of life and legal practice in their community. The second part of the research involves a narrative analysis of in-depth interviews with 12 final year law students in order to explore their future practice intentions and attitudes to, and perceptions of, RRR practice. Each part of the research is designed to reflect different aspects of the attraction and retention equation. Interviewing already practising solicitors aims to gauge actual lived experience while the interviews with final year law students seeks to understand imagined experience. Together, these provide a picture of, or narrative about, the nature and dynamics of women’s career choices in the context of RRR practice.
Preparation of a Novel Restricted Access Material Combined to Core-Shell Magnetic Molecularly Imprinted Polymers for Determination of Dimethyl phthalate in Soils
Creators: name: Haigen Zuo
name: Yusuo Lin
name: Xinxin Ma
name: Yanhong Feng
name: Qiuhong Luo
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biochemistry
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer

description: A novel superparamagnetic Fe3O4 surface molecularly imprinted polymers (MIPs) coated with restricted access materials (RAMs) were prepared for the analysis of dimethyl phthalate (DMP) residues in soils. RAM-MIP with core-shell structure was prepared by coated MIP layer on superparamagnetic Fe3O4 nanoparticle, and 3-glycidoxypropyl trimethoxysilane (KH 560) was grafted on the surface to form hydroxyl group so as to block macromolecules accession. RAM-MIPs were characterized by transmission electron microscope (TEM), scan electron microscope (SEM), vibrating sample magnetometer (VSM), thermal analyzer (TA), and others. RAM-MIPs can be magnetically separated from the matrix easily and exhibited efficient adsorption performance for DMP. The residue of DMP in soil was extracted by acetone:n-hexane (1:1, V/V), cleaned up by RAM-MIPs, and determined by gas chromatography-mass spectrometry (GC-MS). The limits of quantification (LOQ, S/N > 10) for DMP in soil samples were confined to 0.04 mg kg−1. The recoveries and relative standard deviations (RSDs) of DMP spiked at 0.04–0.2 mg.kg−1 were 70.27–80.83% and 2.1–5.7%, respectively. Thus, RAM-MIPs can be successfully applied to the determination of DMP in soil samples.
Gross Anatomy And Morphology Of Egyptian Water Buffalo’s Liver (Bubalus Bubalis) With Reference To Some Histochemical And Immunohistochemical Evaluation.
Creators: name: Rashad, Eman
Publisher: name: figshare
Year: 2021
Subjects: subject: 79999 Agricultural and Veterinary Sciences not elsewhere classified
subject: FOS: Other agricultural sciences
subject: 70207 Humane Animal Treatment
subject: FOS: Animal and dairy science
subject: 70706 Veterinary Medicine
subject: FOS: Veterinary sciences
subject: 70705 Veterinary Immunology
subject: 70702 Veterinary Anatomy and Physiology
subject: 70703 Veterinary Diagnosis and Diagnostics

description: Quite recently, considerable attention has been paid to water buffalo species (Bubalus bubalis) and its economic importance. Liver is complex organ and susceptible to many diseases. So, this paper concentrated on the buffalo liver in terms of their anatomy, histology, histochemistry and immunohistochemical characteristics of its cells, with regard to the functional importance. 20 samples of fresh buffalo liver selected, 5 injected by latex for anatomical studies, 5 injected by urographine for radiograph pictures and the last 10 directly fixed in neutral buffered formalin 10% and processed for histological, histochemical and immunohistochemical examination. The result revealed that Portal vein divided into three main branches right, left and caudal omental ones. The hepatic vein branches classified as right, middle and left branch. The common bile duct formed by union of right hepatic duct, left hepatic duct and cystic duct. The liver of buffalo showed a well fibrous capsule of Glisson's with high amount of collagen fibers by Masson's Trichrome stain. Reticular fibers found to have dispersed characteristic shape with Gomori's method. PAS and Best's carmine stains gave positive results. Perl's Prussian demonstrated the presence of hemosiderin and ferric salts in von kupffer cells. These cells stained positive to CD68. Anti-insulin and anti-glucagon showed positive reaction. CK7 and CD10 were immune positive to biliary epithelium.CD34 gave positive to portal endothelial cells. Alfa smooth muscle actin showed unique normal positivity along the hepatic tissue. The results obtained, not only contribute to the knowledge of buffalo species; but also define a normal structure reference for the diagnosis and treatment of liver diseases.
Big Bang Nucleosynthesis, Population III, and Stellar Genetics in the Galactic Halo
Creators: name: Ryan, Sean G.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The diverse isotopic and elemental signatures produced in different nucleosynthetic sites are passed on to successive generations of stars. By tracing these chemical signatures back through the stellar populations of the Galaxy, it is possible to unravel its nucleosynthetic history and even to study stars which are now extinct. This review considers recent applications of "stellar genetics" to examine the earliest episodes of nucleosynthesis in the Universe, in Population III stars and the Big Bang.
description: 14 pages, 4 figures Refereed conference paper, accepted for publication in Publications of the Astronomical Society of Australia
Wolf-Rayets in IC10: Probing the Nearest Starburst
Creators: name: Massey, Philip
name: Holmes, Shadrian
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: IC10 is the nearest starburst galaxy, as revealed both by its Halpha surface brightness and the large number of Wolf-Rayet stars (WRs) per unit area. The relative number of known WC- to WN-type WRs has been thought to be unusually high (~2), unexpected for IC10's metallicity. In this Letter we report the first results of a new and deeper survey for WRs in IC10. We sucessfully detected all of the spectroscopically known WRs, and based upon comparisons with a neighboring control field, estimate that the total number of WRs in IC10 is about 100. We present spectroscopic confirmation of two of our WR candidates, both of which are of WN type. Our photometric survey predicts that the actual WC/WN ratio is ~0.3. This makes the WC/WN ratio of IC 10 consistent with that expected for its metallicity, but greatly increases the already unusually high number of WRs, resulting in a surface density that is about 20 times higher than in the LMC. If the majority of these candidates are spectroscopically confirmed, IC10 must have an exceptional population of high mass stars.
description: Accepted by ApJL; only minor correction in this version
Gelae cognatum, new combination
Creators: name: Miller, Kelly B.
name: Wheeler, Quentin D.
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Leiodidae
Gelae
Gelae cognatum

description: Gelae cognatum (Matthews), new combination
(Figs. 19–20, 31)
description: Published as part of Miller, Kelly B. & Wheeler, Quentin D., 2004, Two New Genera of Agathidiini from the Nearctic and Neotropical Regions (Coleoptera: Leiodidae), pp. 466-487 in The Coleopterists Bulletin 58 (4) on page 481, DOI: 10.1649/633, http://zenodo.org/record/10104530
title: Neuromotor Characteristics of Lateral Epicondylalgia
Creators: name: Manickaraj, Nagarajan
Publisher: name: Griffith University
Year: 2017
Subjects: subject: Lateral epicondylalgia
subject: Neuromotor dysfunction
subject: Gripping
subject: Forearm muscles
subject: Extensor carpi radialis brevis
subject: Extensor digitorum communicis

description: Neuromotor dysfunction such as delayed upper extremity reaction time and altered wrist posture during gripping, are considered part of the pathophysiology in lateral epicondylalgia (LE). This might manifest as changes in the forearm muscle activity patterns in LE. In addition to a systematic review (Study 1) of the current literatures of forearm muscle activity in LE, this thesis presents three case-control studies that provide new insights into: the timing of forearm muscle activity during wrist extension reaction time (RT) (Study 2), the magnitude of forearm muscle activity during isometric gripping with different wrist postures (Study 3), and forearm muscle synergies during ramp and steady-state phases of isometric gripping (Study 4) in individuals with LE. This thesis also presents the association of forearm muscle activity with the clinical, sensory and tendon structural changes associated with LE. The systematic review identified consistent evidence of increased electromechanical delay and altered cortical excitability associated with the forearm extensor muscles in LE. These findings suggest both peripheral and central contribution to altered motor control in LE. The second study, which used intramuscular electromyography (EMG), provided evidence that delayed RT in LE is due to prolonged extensor carpi radialis brevis (ECRB) and extensor digitorum communicis (EDC) motor time, with no between-group differences in premotor time. Wrist extension RT was associated only with ECRB and EDC premotor time but not with extensor carpi ulnaris (ECU) premotor in LE. Increased duration of LE symptoms was associated with shorter RT, as well as shorter ECRB and anconeus premotor time.
Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals
Creators: name: Schmidt, Patricia
name: Hinderer, Tanja
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The recent detection of gravitational waves (GWs) from the neutron star binary inspiral GW170817 has opened a unique avenue to probe matter and fundamental interactions in previously unexplored regimes. Extracting information on neutron star matter from the observed GWs requires robust and computationally efficient theoretical waveform models. We develop an approximate frequency-domain GW phase model of a main GW signature of matter: dynamic tides associated with the neutron stars' fundamental oscillation modes ($f$-modes). We focus on nonspinning objects on circular orbits and demonstrate that, despite its mathematical simplicity, the new "$f$-mode tidal" (fmtidal) model is in good agreement with the effective-one-body dynamical tides model up to GW frequencies of $\gtrsim 1$ kHz and gives physical meaning to part of the phenomenology captured in tidal models tuned to numerical-relativity. The advantages of the fmtidal model are that it makes explicit the dependence of the GW phasing on the characteristic equation-of-state parameters, i.e., tidal deformabilities and $f$-mode frequencies; it is computationally efficient; and it can readily be added to any frequency-domain baseline waveform. The fmtidal model is easily amenable to future improvements and provides the means for a first step towards independently measuring additional fundamental properties of neutron star matter beyond the tidal deformability as well as performing novel tests of general relativity from GW observations.
description: 7 pages, 3 figures; matches published version
Teorik Parçacık Fizikçisi Gözüyle Açık Veri
Creators: name: Ozpineci, Altug
Publisher: name: Zenodo
Year: 2021
Subjects: Fizikçi Gözüyle Açık Veri
Fizik Verileri
Açık Veri
Araştırma Verilerinin Yönetimi
Fizik Alanında Veriler
UAVS2021

description: 25-26 Mayıs 2021 Ulusal Araştırma Verileri Sempozyumu Fizikçi Gözüyle Açık Veri Teorik Fizikçileri Verisi Araştırma Verileri Yönetimi
Line formation in convective stellar atmospheres. I. Granulation corrections for solar photospheric abundances
Creators: name: Steffen, M.
name: Holweger, H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In an effort to estimate the largely unknown effects of photospheric temperature fluctuations on spectroscopic abundance determinations, we have studied the problem of LTE line formation in the inhomogeneous solar photosphere based on detailed 2-dimensional radiation hydrodynamics simulations of the convective surface layers of the Sun. By means of a strictly differential 1D/2D comparison of the emergent equivalent widths, we have derived "granulation abundance corrections" for individual lines, which have to be applied to standard abundance determinations based on homogeneous 1D model atmospheres in order to correct for the influence of the photospheric temperature fluctuations. In general, we find a line strengthening in the presence of temperature inhomogeneities as a consequence of the non-linear temperature dependence of the line opacity. For many lines of practical relevance, the magnitude of the abundance correction may be estimated from interpolation in the tables and graphs provided with this paper. The application of abundance corrections may often be an acceptable alternative to a detailed fitting of individual line profiles based on hydrodynamical simulations. The present study should be helpful in providing upper bounds for possible errors of spectroscopic abundance analyses, and for identifying spectral lines which are least sensitive to the influence of photospheric temperature inhomogeneities.
description: Accepted by A&A
İyi Veri İyi Yapay Zeka Araştırması
Creators: name: Pakdemirli, Ahu
Publisher: name: Zenodo
Year: 2021
Subjects: Sağlıkta Yapay Zeka
Sağlık Alanında Araştırma Verisi
Araştırma Verilerinin Yönetimi
UAVS2021

description: 25-26 Mayıs 2021 Ulusal Araştırma Verileri Sempozyumu Araştırma Verilerinin Yönetimi Sağlık Alanında Araştırma Verileri Sağlıkta Yapay Zeka
Letter from Alice R. Appenzeller to William Elliot Griffis, February 16, 1913
Creators: name: Appenzeller, Alice R.
Publisher: name: No Publisher Supplied
Year: 1913

description: Writes prior to Griffis' travels to Milwaukee. Discusses the Japanese bazaar they will have at church, a visit from Miss Merrill, the Berlin Fever, and Mrs. Dodge's sister's marriage to James Lee Kaufman (teaches law in the Imperial University, Tokyo).
Morphogenesis Software based on Epigenetic Code Concept
Creators: name: Bessonov, N.
name: Butuzova, O.
name: Minarsky, A.
name: Penner, R.
name: Soule, C.
name: Tosenberger, A.
name: Morozova, N.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Other Quantitative Biology (q-bio.OT)
subject: FOS: Biological sciences

description: The process of morphogenesis is an evolution of the shape of an organism together with the differentiation of its parts. This process encompasses numerous biological processes ranging from embryogenesis to regeneration following crisis such as amputation or transplantation. A fundamental theoretical question is where exactly do these instructions for (re-)construction reside and how are they implemented? We have recently proposed a set of concepts, aiming to respond to these questions and to provide an appropriate mathematical formalization of the geometry of morphogenesis [1]. First, we consider the possibility that evolution of shape is determined by epigenetic information, responsible for realization of different types of cell events. Second, we suggest a set of rules for converting this epigenetic information into instructive signals for cell events for each cell, as well as for transforming it after each cell event. Next we give notions of cell state, determined by its epigenetic array, and cell event, which is a change of cell state, and formalize development as a graph (tree) of cell states connected by 5 types of cell events, corresponding to the processes of cell division, cell growth, cell death, cell movement and cell differentiation. Here we present a Morphogenesis Software capable of simulating the evolution of a 3D embryo starting from zygote, following a set of rules based on our theoretical assumptions, and thus to provide a proof-of-concept for the hypothesis of epigenetic code regulation. The software creates a developing embryo and a corresponding graph of cell events according to the zygotic epigenetic spectrum and chosen parameters of the developmental rules. Variation of rules influencing the resulting shape of an embryo may help elucidating the principal laws underlying pattern formation.