cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A Kähler Compatible Moyal Deformation of the First Heavenly Equation
Creators: name: Maceda, Marco
name: Martínez-Carbajal, Daniel
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences

description: We construct a noncommutative Kähler manifold based on a non-linear perturbations of Moyal integrable deformations of $D=4$ self-dual gravity. The deformed Kähler manifold preserves all the properties of the commutative one, and we obtain the associated noncommutative Kähler potential using the Moyal deformed gravity approach. We apply this construction to the Atiyah-Hitchin metric and its Kähler potential, which is useful in the description of interactions among magnetic monopoles at low energies.
A high-sensitivity OH 5-cm line survey in late-type stars
Creators: name: Desmurs, J. -F.
name: Baudry, A.
name: Sivagnanam, P.
name: Henkel, C.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have undertaken a comprehensive search for 5-cm excited OH maser emission from evolved stars representative of various stages of late stellar evolution. Observed sources were selected from known 18-cm OH sources. This survey was conducted with the 100-m Effelsberg telescope to achieve high signal to noise ratio observations and a sensitivity limit of about 0.05 to 0.1 Jy. A total of 64 stellar sources were searched for both main line and satellite line emission. We confirm the previous detection of 5 cm OH in Vy 2-2, do not confirm emission from NML-Cyg and do not report any other new detection within the above sensitivity limit. Implications of these results on the pumping mechanism of the OH radical in circumstellar envelopes are briefly discussed.
description: 8 pages, 5 figures, A&A in press
Omophlus proteus subsp. megista MUCHE 1964
Creators: name: Yildirim, E.
name: Kiliç, E.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Tenebrionidae
Omophlus
Omophlus proteus
Omophlus proteus megista muche 1964

description: Omophlus proteus megista MUCHE 1964
 Omophlus proteus megista MUCHE 1964 - Ent. Abh. Staatl. Mus. Tierk. Dresden 29 (11): 614, Südanatolien, Gülek Bogasi (=İçel, Tarsus, Gülek Boğazı).
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 966, DOI: 10.5281/zenodo.5429972
Entrevista com Paulo Nunes (Comissão da Verdade e da Preservação da Memória Paraíba)
Creators: name: Hollanda, Cristina Buarque De
Publisher: name: figshare
Year: 2019
Subjects: subject: History
subject: 220104 Human Rights and Justice Issues
subject: FOS: Philosophy, ethics and religion
subject: 210308 Latin American History
subject: FOS: History and archaeology
subject: 180102 Access to Justice
subject: FOS: Law

description: Entrevista com Paulo Nunes, ex-membro oficial da Comissão da Verdade e da Preservação da Memória da Paraíba (2012-2015).
The X-ray Spectra of Black Hole X-ray Novae in Quiescence as Measured by Chandra
Creators: name: Kong, A. K. H.
name: McClintock, J. E.
name: Garcia, M. R.
name: Murray, S. S.
name: Barret, D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present Chandra observations of black hole X-ray novae V404 Cyg, A0620-00, GRO J1655-40 and XTE J1550-564 in quiescence. Their quiescent spectra can be well fitted by a power-law model with slope $α\sim 2$. While a coronal (Raymond-Smith) model is also a statistically acceptable representation of the spectra, the best fit temperatures of these models is $\sim 5$ times higher than that seen in active stellar coronae. These four spectra of quiescent X-ray novae are all consistent with that expected for accretion via an advection-dominated accretion flow (ADAF) and inconsistent with that expected from a stellar corona. This evidence for continued accretion in quiescence further strengthens the case for the existence of event horizons in black holes. Both A0620-00 and GRO J1655-40 were fainter than in previous observations, while V404 Cyg was more luminous and varied by a factor of 2 in a few ksec. A reanalysis of the X-ray data for XTE J1550-564 shows that (like V404 Cyg and A0620-00) its luminosity exceeds the maximum prediction of the coronal model by a large factor. The 0.3-7 keV luminosity of the four sources studied ranges from $\sim 10^{30}-10^{33}$ erg/s.
description: 9 pages, 6 figures, accepted for publication in ApJ
Entrevista com Paulo Nunes (Comissão da Verdade e da Preservação da Memória Paraíba)
Creators: name: Hollanda, Cristina Buarque De
Publisher: name: figshare
Year: 2019
Subjects: subject: History
subject: 220104 Human Rights and Justice Issues
subject: FOS: Philosophy, ethics and religion
subject: 210308 Latin American History
subject: FOS: History and archaeology
subject: 180102 Access to Justice
subject: FOS: Law

description: Entrevista com Paulo Nunes, ex-membro oficial da Comissão da Verdade e da Preservação da Memória da Paraíba.
title: Bertram, August Wilhelm
title: Catalogus Professorum Halensis
titleType: Subtitle
title: Biografienportal Sachsen-Anhalt
titleType: Other
Creators: name: Catalogus Professorum Halensis
name: Schopferer, Julia
Publisher: name: Historisches Datenzentrum Sachsen-Anhalt,Institut für Landesgeschichte (Sachsen-Anhalt)
Year: 2025
Subjects: subject: History
classificationCode: 4023025-9
subject: Halle (Saale)
valueUri: https://d-nb.info/gnd/4023025-9
classificationCode: 4006804-3
subject: Biografie
valueUri: https://d-nb.info/gnd/4006804-3
classificationCode: 4166546-6
subject: Landesgeschichte
valueUri: https://d-nb.info/gnd/4166546-6
classificationCode: 4051181-9
subject: Sachsen-Anhalt
valueUri: https://d-nb.info/gnd/4051181-9
classificationCode: 1048495779
subject: Universität Halle (Saale) | Halle (Saale)
valueUri: https://d-nb.info/gnd/1048495779
classificationCode: 2024276-1
subject: Martin-Luther-Universität Halle-Wittenberg | Halle (Saale); Wittenberg
valueUri: https://d-nb.info/gnd/2024276-1
classificationCode: 4020517-4
subject: Geschichte
valueUri: https://d-nb.info/gnd/4020517-4
classificationCode: 7504326-9
subject: Universitätsgeschichte
valueUri: https://d-nb.info/gnd/7504326-9
classificationCode: 7504427-4
subject: Wissenschaftsgeschichte
valueUri: https://d-nb.info/gnd/7504427-4
subject: Biografienportal Sachsen-Anhalt
subject: Catalogus Professorum Halensis
classificationCode: 1080911200
subject: Schopferer, Julia | Historikerin
valueUri: https://d-nb.info/gnd/1080911200
classificationCode: 1051477808
subject: Bertram, August Wilhelm | Arzt
valueUri: https://d-nb.info/gnd/1051477808

description: Das Biografienportal Sachsen-Anhalt versammelt in Erst- und Zweitveröffentlichung oder zu Zwecken der Langzeitarchivierung Biografien von Menschen aus und in Sachsen-Anhalt. Integriert wurde der Catalogus Professorum Halensis, der durch Mitarbeitende des Instituts für Geschichte der Martin-Luther-Universität Halle-Wittenberg entstand. Dabei handelt es sich um ein bio-bibliografisches Online-Lexikon zu den Professoren der Universität Halle zwischen 1694 und 1968. Die Texte wurden vor allem von Henrik Eberle und anderen Mitarbeitenden zwischen 2005 und 2010 recherchiert und erstellt. Etliche Artikel zum Zeitraum 1694 bis 1817 verfasste Julia Schopferer. Bei der Überführung in das Biografienportal wurden die Lebensangaben neu recherchiert und Metadaten über Verfahren des Named Entity Recogniton erschlossen. Automatisiert erkannt wurden Personennamen, Ortsbezeichnungen und Körperschaften, die in der hier vorhandenen RTF-Datei indexiert vorliegt. Zudem wurden diese mit GND-Einträgen abgeglichen. Weiterhin erfolgte ein Abgleich mit der „Ontologie der historischen, deutschsprachigen Amts- und Berufsbezeichnungen“. Die Texte liegen im Jahr 2024 in zweifacher Ausgabe im Catalogus Professorum Halensis des Universitätsarchivs und des Biografienportals des Historischen Datenzentrums Sachsen-Anhalts vor. Sie werden hier für die Langzeitarchivierung der ursprünglichen Fassung archiviert.
description: https://www.catalogus-professorum-halensis.de/
description: Biografienportal Sachsen-Anhalt: https://www.histdata.uni-halle.de/
Additional file 1 of Anti-PD-1 antibodies as a salvage therapy for patients with diffuse large B cell lymphoma who progressed/relapsed after CART19/20 therapy
Creators: name: Wang, Chunmeng
name: Shi, Fengxia
name: Liu, Yang
name: Zhang, Yajing
name: Dong, Liang
name: Li, Xiang
name: Tong, Chuan
name: Wang, Yao
name: Su, Liping
name: Nie, Jing
name: Han, Weidong
Publisher: name: figshare
Year: 2021
Subjects: subject: Space Science
subject: Medicine
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Hematology
subject: Virology

description: Additional file 1. Figure S1. PET/CT imaging for UPN1. Figure S2. Immunohistochemistry in tumor samples from all five patients. Figure S3. Biological biomarker detection from blood samples. Table S1. H-scores for PD-1 and PD-L1 in patients before CART19/20 therapy and after failure of CART19/20.
Global polarizability matrix method for efficient modeling of light scattering by dense ensembles of non-spherical particles in stratified media
Creators: name: Bertrand, Maxime
name: Devilez, Alexis
name: Hugonin, Jean-Paul
name: Lalanne, Philippe
name: Vynck, Kevin
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optics (physics.optics)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: We introduce a numerical method that enables efficient modelling of light scattering by large, disordered ensembles of non-spherical particles incorporated in stratified media, including when the particles are in close vicinity to each other, to planar interfaces and/or to localized light sources. The method consists in finding a small set of fictitious polarizable elements -- or numerical dipoles -- that quantitatively reproduces the field scattered by an individual particle for any excitation and at an arbitrary distance from the particle surface. The set of numerical dipoles is described by a global polarizability matrix that is determined numerically by solving an inverse problem relying on fullwave simulations. The latter are classical and may be performed with any Maxwell's equations solver. Spatial non-locality is an important feature of the numerical dipoles set, providing additional degrees of freedom compared to classical coupled dipoles to reconstruct complex scattered fields. Once the polarizability matrix describing scattering by an individual particle is determined, the multiple scattering problem by ensembles of such particles in stratified media can be solved using a Green tensor formalism and only few numerical dipoles, thereby with a low physical memory usage, even for dense systems in close vicinity to interfaces. The performance of the method is studied with the example of large high-aspect-ratio high-index dielectric cylinders. The method is easy to implement and may offer new possibilities for the study of complex nanostructured surfaces, which are becoming widespread in emerging photonic technologies.
Omophlus subcostatus REITTER 1908
Creators: name: Yildirim, E.
name: Kiliç, E.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Tenebrionidae
Omophlus
Omophlus subcostatus

description: Omophlus subcostatus REITTER 1908
 Omophlus subcostatus REITTER 1908 - Wien Ent. Ztg. 27: 56, Tokat.
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 966, DOI: 10.5281/zenodo.5429972
title: Communication and peer interactions of three autistic students in an inclusive synchronous online EAL classroom in Indonesia
Creators: name: Muharikah, Afifah
Publisher: name: Griffith University
Year: 2023
Subjects: subject: Autism Spectrum Disorder (ASD)
subject: autistic communication
subject: conversation analysis
subject: English as an additional language (EAL)

description: The increasing number of autistic learners of English as an additional language (EAL) at the college level has turned many mainstream EAL classrooms into inclusive classrooms. The increase, however, does not align with the available studies related to autistic EAL learners, especially at the college level. Moreover, research on the communication of autistic individuals in English as an Additional Language (EAL) contexts remains limited (Muharikah et al., 2022). Consequently, EAL practitioners have insufficient guidance on creating inclusive classrooms for autistic learners, specifically at the college level. This study seeks to address the existing gap by providing insights into this underexplored area. [...]
'We Just Want to Help', Community Disaster Resilience - Profit in Nonprofits
Creators: name: FIONA JANE BRAKE ROBERTS
Publisher: name: Monash University
Year: 2019
Subjects: subject: 111799 Public Health and Health Services not elsewhere classified
subject: FOS: Health sciences

description: ‘We just want to help’ exemplifies how Lions Clubs, Rotary Clubs and Neighbourhood Houses can offer assistance before, during and after disasters. This thesis provides a first-time analysis of the actions and strengths that nonprofit organisations can deliver in times of crises; as well as identifying barriers and suggesting enablers to action. The embeddedness of nonprofit organisations’ local knowledge and connections offers enormous capacity to strengthen and build community resilience to disasters. Importantly, with increasing evidence of climate change intensifying disaster events around the world, this research emphasises how nonprofit organisations can help in the disaster space.
The dust disk of HR4049
Creators: name: Dominik, C.
name: Dullemond, C. P.
name: Cami, J.
name: van Winckel, H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the Spectral Energy Distribution of HR 4049 based on literature data and new continuum measurements at 850 micron. The SED shows variable absorption in the UV, and a large IR excess, both caused by circumstellar dust. The shape of the IR excess from 1 micron all the way down to 850 micron can be nearly perfectly fitted with a single blackbody function at T ~ 1150 K or alternatively with a sum of blackbodies in a narrow temperature range. The energy emitted in this IR continuum radiation is about one-third of the stellar luminosity. We show that this blackbody radiation must be due to the presence of a circumbinary disk with a large height. This disk must also be gas-rich, in agreement with the observations of molecular bands in the ISO-SWS spectrum. We present two possible scenario's for explaining the shape and the intensity of the IR excess. The first scenario involves large grains (a >1 mm) that each radiate like a blackbody. The second scenario argues that the blackbody radiation is due to a very optically thick circumbinary disk. We investigate if such a disk would indeed produce blackbody radiation by presenting results from radiative transfer calculations. We further quantify the properties of such a disk and its stability in the framework of (hydro)dynamics, grain settling, radiation pressure and grain drift. The virtues and shortcomings of both models for the origin of the IR blackbody are discussed by contrasting them with other observations and assessing them in the framework of (binary) (post-)AGB evolution.
description: 16 pages, 12 figures, accepted for publication in A&A
Dust traps in the protoplanetary disc MWC 758: two vortices produced by two giant planets?
Creators: name: Baruteau, Clément
name: Barraza, Marcelo
name: Pérez, Sebastián
name: Casassus, Simon
name: Dong, Ruobing
name: Lyra, Wladimir
name: Marino, Sebastián
name: Christiaens, Valentin
name: Zhu, Zhaohuan
name: Carmona, Andrés
name: Debras, Florian
name: Alarcon, Felipe
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Resolved ALMA and VLA observations indicate the existence of two dust traps in the protoplanetary disc MWC 758. By means of 2D gas+dust hydrodynamical simulations post-processed with 3D dust radiative transfer calculations, we show that the spirals in scattered light, the eccentric, asymmetric ring and the crescent-shaped structure in the (sub)millimetre can all be caused by two giant planets: a 1.5-Jupiter mass planet at 35 au (inside the spirals) and a 5-Jupiter mass planet at 140 au (outside the spirals). The outer planet forms a dust-trapping vortex at the inner edge of its gap (at ~85 au), and the continuum emission of this dust trap reproduces the ALMA and VLA observations well. The outer planet triggers several spiral arms which are similar to those observed in polarised scattered light. The inner planet also forms a vortex at the outer edge of its gap (at ~50 au), but it decays faster than the vortex induced by the outer planet, as a result of the disc's turbulent viscosity. The vortex decay can explain the eccentric inner ring seen with ALMA as well as the low signal and larger azimuthal spread of this dust trap in VLA observations. Finding the thermal and kinematic signatures of both giant planets could verify the proposed scenario.
description: 18 pages, 8 figures, accepted for publication in MNRAS
Standard model Higgs field and hidden sector cosmology
Creators: name: Tenkanen, Tommi
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider scenarios where the inflaton field decays dominantly to a hidden dark matter (DM) sector. By studying the typical behavior of the Standard Model (SM) Higgs field during inflation, we derive a relation between the primordial tensor-to-scalar ratio $r$ and amplitude of the residual DM isocurvature perturbations $β$ which is typically generated if the DM is thermally decoupled from the SM sector. We consider different expansion histories and find that if the Universe was radiation- or matter-dominated after inflation, a future discovery of primordial DM isocurvature will rule out all simple scenarios of this type because generating observable $β$ from the Higgs is not possible without violating the bounds on $r$. Seen another way, the Higgs field is generically not a threat to models where both the inflaton and DM reside in a decoupled sector. However, this is not necessarily the case for an early kination-dominated epoch, as then the Higgs can source sizeable $β$. We also discuss why the Higgs cannot source the observed curvature perturbation at large scales in any of the above cases but how the field can still be the dominant source of curvature perturbations at small scales.
description: 10 pages, 1 figure. v2: Minor corrections, a slight change in title, matches the version accepted for publication in Phys. Rev. D
Entrevista com Norton Nohama (Comissão da Verdade do Paraná Teresa Urban)
Creators: name: Hollanda, Cristina Buarque De
Publisher: name: figshare
Year: 2019
Subjects: subject: 180102 Access to Justice
subject: FOS: Law
subject: History
subject: 220104 Human Rights and Justice Issues
subject: FOS: Philosophy, ethics and religion

description: Entrevista com Norton Nohama, ex-membro titular da Comisão da Verdade do Paraná Teresa Urban.(2012-2014)
Large Scale Structure at z=1.2 Outlined by MgII Absorbers
Creators: name: Williger, G. M.
name: Campusano, L. E.
name: Clowes, R. G.
name: Graham, M. J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The largest known structure in the high redshift universe is mapped by at least 18 quasars and spans ~5 deg x 2.5 deg on the sky, with a quasar spatial overdensity of 6-10 times above the mean. This large quasar group provides an extraordinary laboratory ~100 x 200 x 200 h^-3 comoving Mpc^3 in size (q0=0.5, Lambda=0, H0=100h km/s/Mpc) covering 1.20
description: 56 pages with 8 encapulated Postscript files, 6 JPEG files, with clarified graphics and statistics, aastex Latex, accepted by ApJ
title: The Impact of Macroeconomic Conditions, Economic Development and Government Industrial Policy on Capital Structure of Firms: Evidence from Taiwan
Creators: name: Yeh, Hsien-Hung
Publisher: name: Griffith University
Year: 2009
Subjects: subject: capital structure
subject: macroeconomic conditions
subject: economic development
subject: government industrial policy
subject: knowledge gap
subject: Partial Adjustment Model
subject: PAM
subject: growth opportunities
subject: industrial policy

description: The thesis examines the impact of macroeconomic conditions, economic development and government industrial policy on capital structure. These three macro-level factors have been neglected by most of the voluminous studies on capital structure that have emerged since Modigliani and Miller’s irrelevance propositions in 1958. Very few studies have examined the impact of macroeconomic conditions and economic development on capital structure. In the case of macroeconomic conditions, a few studies on capital structure have analysed this variable in the context of default risk or investor protections while, in regards to economic development, a handful of studies have found that the impact of economic development on capital structure varies amongst countries. No study on capital structure decisions has examined the impact of government industrial policy. Thus, the effect of these three important variables on capital structure is not yet clearly established in the literature. The thesis therefore addresses this knowledge gap. The investigation of these three factors is conducted based on the Partial Adjustment Model, i.e. PAM, of Capital Structure that the thesis reformulates. The thesis considers two important situations that have not been addressed by previous studies based on PAM – when firms are under financial constraint of either over-leverage or under-leverage relative to their target capital structure. Unlike previous studies, the thesis investigates macroeconomic conditions, economic development and government industrial policy guided by the agency theory of capital structure and with consideration given to growth opportunities. The thesis research is undertaken in the context of Taiwan – a country that has recently joined the ranks of developed countries after successfully transforming itself from being a Third World country, and with industries that are widely recognised worldwide. The period of study is from 1983 to 1995. This period has been chosen due to the limited availability of data for the electronics industry before 1980 and to control for the potential impact of intervening factors such as the Asian Financial Crisis in 1997, Taiwan’s implementation of a new tax policy in 1998 and both the bubble economy and the dot-com problem in the early 2000s. The sample used in the thesis includes the listed firms in the textile, plastics and electronics industries that were financially supported by the Taiwanese government’s industrial policy during the periods of the 1960s, the 1970s to the mid-1980s and the mid-1980s to the mid-1990s...
MOESM1 of Effect of nitric oxide on postoperative acute kidney injury in patients who underwent cardiopulmonary bypass: a systematic review and meta-analysis with trial sequential analysis
Creators: name: Hu, Jie
name: Spina, Stefano
name: Zadek, Francesco
name: Kamenshchikov, Nikolay
name: Bittner, Edward
name: Pedemonte, Juan
name: Berra, Lorenzo
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Science Policy

description: Additional file 1. Search strategy.
ShinySurfer: A tool for visualization and statistical analysis of cortical parameters
Creators: name: Klawitter, Sandra
name: Yixiao Cai
name: Baichao Ye
name: Klawonn, Frank
name: Sörös, Peter
Publisher: name: F1000 Research Limited
Year: 2021

description: Structural magnetic resonance imaging (MRI) of the brain can be analyzed quantitatively by surface-based morphometry, e.g. with the software package FreeSurfer. FreeSurfer is able to determine the thickness, area, and volume of the cortex, i.e. the superficial layer of the brain containing billions of neurons.

 ShinySurfer is a software tool for 3D visualization and statistical analysis of cortical data obtained by FreeSurfer.

 ShinySurfer has been developed in R using the shiny package. ShinySurfer reads tables generated by FreeSurfer's aparcstats2table command, in which each line is an individual participant and each column represents a cortical area.

 For visualization of cortical parcellations, the R packages ggseg, ggseg3d, and ggsegExtra are used (Mowinckel & Vidal-Piñeiro 2020). Cortical areas are displayed on a semi-inflated surface that allows the inspection of cortical sulci. For the inspection of the medial surfaces, the left or right hemisphere can be displayed alone. The brain model may be freely rotated.

 For convenient visual quality control and identification of potential outliers, the values for every cortical area can be displayed as a raincloud plot (Allen et al. 2021). The raincloud plot combines a dot plot of raw data, a plot of probability density, and a box plot, showing the median and the quartiles.

 For statistical analysis, ShinySurfer is able to perform univariate linear regression analysis. In addition, ShinySurfer may also perform bootstrapped lasso (least absolute shrinkage and selection operator) regression analysis (Tibshirani 1996).

 ShinySurfer is being developed by Sandra Klawitter, Frank Klawonn, and Peter Sörös at the Helmholtz Centre for Infection Research (Braunschweig, Germany), the Ostfalia University of Applied Sciences (Wolfenbüttel, Germany), and the University of Oldenburg (Oldenburg, Germany).

 ShinySurfer Homepage
 ShinySurfer on GitHub
Bledius furcatus
Creators: name: Anlaş, S.
name: A. F
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Bledius
Bledius furcatus

description: Bledius furcatus (OLIVIER 1811)
M a t e r i a l e x a m i n e d: Mazandaran: Central province, 2 exs., 09.V.2008, leg. E. Sürmen.
C o m m e n t s: The species is here reported from Iran for the first time.
description: Published as part of Anlaş, S. & A. F, 2010, Distributional checklist of the Staphylinidae (Coleoptera) of Iran, with new and additional records, pp. 335-388 in Linzer biologische Beiträge 42 (1) on page 339, DOI: 10.5281/zenodo.5331927
Omophlus wittmeri MUCHE 1979
Creators: name: Yildirim, E.
name: Kiliç, E.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Tenebrionidae
Omophlus
Omophlus wittmeri

description: Omophlus wittmeri MUCHE 1979
 Omophlus wittmeri MUCHE 1979 - Reichenbauchia Staat. Mus. Fur. Tierk. in Dresden 17 (20): 171, Turkey (no locality).
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 966, DOI: 10.5281/zenodo.5429972
Entrevista com Norton Nohama (Comissão da Verdade do Paraná Teresa Urban)
Creators: name: Hollanda, Cristina Buarque De
Publisher: name: figshare
Year: 2019
Subjects: subject: 180102 Access to Justice
subject: FOS: Law
subject: History
subject: 220104 Human Rights and Justice Issues
subject: FOS: Philosophy, ethics and religion

description: Entrevista com Norton Nohama, ex-membro titular da Comisão da Verdade do Paraná Teresa Urban.
PCOS and Cardiometabolic Health over the Reproductive Years
Creators: name: NADIRA SULTANA KAKOLY
Publisher: name: Monash University
Year: 2019
Subjects: subject: 111706 Epidemiology
subject: FOS: Health sciences

description: This thesis explores the poorly understood area of long-term cardiometabolic health among women with and without polycystic ovary syndrome (PCOS) over their reproductive years. It aims to analyze and present evidence of when, how and if PCOS per se influences cardiometabolic health outcomes. It is the first body of work to longitudinally assess the link between PCOS and cardiometabolic health in a nationally representative population-based cohort of women aged 18-42 years over their reproductive years using a series of different epidemiological methodologies to address challenges in the data. It fills critical gaps in our understanding of the natural history of PCOS over the reproductive years and advances the field by providing a greater understanding into when and how PCOS influences cardiometabolic health across a woman’s reproductive years.
Bradynobaenidae Saussure 1892
Creators: name: Yildirim, E.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Bradynobaenidae

description: Bradynobaenidae  A total of two species from genus belonging to subfamily
Bradynobaenidae were recorded in Turkey up to now (YILDIRIM 2006, PAGLIANO 2002).
description: Published as part of Yildirim, E., 2008, The present situation of some families of Hymenoptera in Turkey, pp. 973-978 in Linzer biologische Beiträge 40 (1) on page 975, DOI: 10.5281/zenodo.5429976
Astenus thoracicus
Creators: name: Anlaş, S.
name: A. F
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Astenus
Astenus thoracicus

description: Astenus thoracicus (BAUDI DI SELVE 1857)
M a t e r i a l e x a m i n e d: Mazandaran: Chaloos, 3 exs., 09.V.2008, leg. E. Sürmen.
C o m m e n t s: The species is here reported from Iran for the first time.
description: Published as part of Anlaş, S. & A. F, 2010, Distributional checklist of the Staphylinidae (Coleoptera) of Iran, with new and additional records, pp. 335-388 in Linzer biologische Beiträge 42 (1) on page 339, DOI: 10.5281/zenodo.5331927
Heavy Element Abundances and Dust Depletions in the Host Galaxies of Three Gamma-Ray Bursts
Creators: name: Savaglio, S.
name: Fall, S. M.
name: Fiore, F.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have derived the column densities of heavy elements in three gamma-ray burst (GRB) optical transients, associated with the circumburst or interstellar medium (ISM) of the host galaxy. In comparison with the same elements observed in damped Lyman-alpha (DLA) systems along QSO sight lines, we find evidence for much higher column densities of ZnII. The gap between the QSO-DLA and GRB-DLA distributions is smoothly bridged by observations of the interstellar absorption in the Milky Way and the Magellanic Clouds. Very small [Fe/Zn], [Si/Zn], and [Cr/Zn] values in GRB-DLAs indicate large dust depletions. Once the dust-to-metals ratios are determined, we find an optical extinction A_V ~ 1 mags, to be compared with typical A_V < 0.1 in most QSO-DLAs. Our inference of high dust content appears to be in contradiction with the typical low reddening previously found in GRBs. One possible way to reconcile is a dust grain-size distribution biased towards big grains, which would give a grey extinction. Possibly the small dust grains have been destroyed by the GRBs themselves. Our findings support the idea that primarily optically selected QSOs probe mainly low gas/dust regions of high redshift galaxies, while the more powerful GRBs can be detected through denser regions of their ISM (molecular clouds and star forming regions). Therefore GRB-DLAs and QSO-DLAs together provide a more complete picture of the global properties of the interstellar medium in high redshift galaxies.
description: Final version, ApJ in press (Vol. 585, March 10, 2003)
Spiral-wave wind for the blue kilonova
Creators: name: Nedora, Vsevolod
name: Bernuzzi, Sebastiano
name: Radice, David
name: Perego, Albino
name: Endrizzi, Andrea
name: Ortiz, Néstor
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The AT2017gfo kilonova counterpart of the binary neutron star merger event GW170817 was characterized by an early-time bright peak in optical and UV bands. Such blue kilonova is commonly interpreted as a signature of weak $r$-process nucleosynthesis in a fast expanding wind whose origin is currently debated. Numerical-relativity simulations with microphysical equations of state, approximate neutrino transport, and turbulent viscosity reveal a new mechanism that can power the blue kilonova. Spiral density waves in the remnant generate a characteristic wind of mass ${\sim}10^{-2}~M_{\odot}$ and velocity ${\sim}0.2$c. The ejected material has electron fraction mostly distributed above $0.25$ being partially reprocessed by hydrodynamic shocks in the expanding arms. The combination of dynamical ejecta and spiral-wave wind can account for solar system abundances of $r$-process elements and early-time observed light curves.
description: 5 pages, 4 figures
Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Tail contributions and post-adiabatic corrections
Creators: name: Boetzel, Yannick
name: Mishra, Chandra Kant
name: Faye, Guillaume
name: Gopakumar, Achamveedu
name: Iyer, Bala R.
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We compute the tail contributions to the gravitational-wave mode amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order of general relativity. We combine them with the already available instantaneous pieces and include the post-adiabatic corrections required to fully account for the effects of radiation-reaction forces on the motion. We compare the resulting waveform in the small eccentricity limit to the circular one, finding perfect agreement.
description: 17 pages
Supplementary File from Multiple sex chromosomes in teleost fishes from a cytogenetic perspective: state of the art and future challenges
Creators: name: Sember, Alexandr
name: Nguyen, Petr
name: Perez, Manolo F.
name: Altmanová, Marie
name: Ráb, Petr
name: Cioffi, Marcelo de Bello
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 60408 Genomics

description: Despite decades of cytogenetic and genomic research of dynamic sex chromosome evolution in teleost fishes, multiple sex chromosomes have been largely neglected. In this review, we compiled available data on teleost multiple sex chromosomes, identified major trends in their evolution and suggest further trajectories in their investigation. In a compiled dataset of 440 verified records of fish sex chromosomes, we counted 75 multiple sex chromosome systems with 60 estimated independent origins. We showed that male-heterogametic systems created by Y-autosome fusion predominate and that multiple sex chromosomes are overrepresented in the order Perciformes. We documented a striking difference in patterns of differentiation of sex chromosomes between male and female heterogamety and hypothesize that faster W sex chromosome differentiation may constrain sex chromosome turnover in female-heterogametic systems. We also found no significant association between the mechanism of multiple sex chromosome formation and percentage of uni-armed chromosomes in teleost karyotype. Last but not least, we hypothesized that interaction between fish populations, which differ in their sex chromosomes, can drive the evolution of multiple sex chromosomes in fishes. This underlines the importance of broader inter-population sampling in studies of fish sex chromosomes.This article is part of the theme issue ‘Challenging the paradigm in sex chromosome evolution: empirical and theoretical insights with a focus on vertebrates (Part II)’.
On the space of ultradistributions vanishing at infinity
Creators: name: Debrouwere, Andreas
name: Neyt, Lenny
name: Vindas, Jasson
Publisher: name: arXiv
Year: 2019
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 46F05 (Primary), 42B10, 46F12, 81S30 (Secondary)

description: We study the structural and linear topological properties of the space $\dot{\mathcal{B}}^{\prime \ast}_ω$ of ultradistributions vanishing at infinity (with respect to a weight function $ω$). Particularly, we show the first structure theorem for $\dot{\mathcal{B}}^{\prime \ast}_ω$ under weaker hypotheses than were known so far. As an application, we determine the structure of the S-asymptotic behavior of ultradistributions.
description: 18 pages
A VLT/FORS2 spectroscopic survey in the HDF-S
Creators: name: Vanzella, E.
name: Cristiani, S.
name: Arnouts, S.
name: Dennefeld, M.
name: Fontana, A.
name: Grazian, A.
name: Nonino, M.
name: Petitjean, P.
name: Saracco, P.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on low-resolution multi-object spectroscopy of 65 objects from I(AB) ~= 20 to I(AB) ~= 25 in the HDF-S obtained with the VLT Focal Reducer/low dispersion Spectrograph (FORS2). 18 objects belong to the HDF-S proper, i.e. the WFPC2 deep area. 15 high-redshift galaxies with 2.0 < z < 3.5 (10 in the HDF-S proper) have been identified. The spectroscopic redshifts are in good agreement with the photometric ones derived from a chi^{2} minimization technique comparing the observed spectral energy distribution with synthetic libraries and with a new neural network (NN) approach. The dispersion with the former method is sigma_z=0.16 whereas the latter provides sigma_z=0.13. No "catastrophic" difference is encountered. The inferred star formation rates of the individual objects range from tens to a few hundreds of M_{\odot} yr^{-1} and the global star formation rate of the Universe at =~2.4 is estimated to be 0.15 M_{\odot} yr^{-1} Mpc^{-3} with a statistical error of 0.04. Evidence for large scale structure is found with two groups' redshifts observed at z ~= 2.1 and z ~= 2.7 and a pronounced low redshift peak around z ~= 0.58. An elliptical galaxy lensing a background object turns out to be at a redshift z=0.577.
description: 11 pages, 9 figures, Accepted for publication in A&A
title: Composing and performing original works for the trombone
Creators: name: Hounsome-Vail, Dale W
Publisher: name: Griffith University
Year: 2020
Subjects: subject: trombone
subject: soloist instrument

description: This dissertation explores composing and performing new works for the trombone, and their presentation in a recital designed to demonstrate the potential of the trombone as a soloist instrument. The study builds on the author’s experiences as an orchestral trombonist, as well as his exploration of other styles of trombone playing, including those of brass band and jazz. The author discusses the current repertoire available to trombonists performing recitals, and explores the various qualities of the trombone they demonstrate well. However it goes further to consider what could be done to showcase further its many qualities as a solo instrument. In addition to this artistic research exegesis, the research submission includes the scores of five new compositions by the author featuring a solo trombone, and discusses the process of composing, rehearsing, and performing these works. Their effectiveness in showing off the potential of the trombone as a solo instrument is demonstrated through recordings of live performances of the new works by the author together with colleagues from the Australian National Academy of Music. The research questions posed by the author are addressed through the design and execution of a recital programme that utilises a range of different styles and genres in which the trombone excels. It is proposed that such a programme can potentially showcase more the instrument’s abilities as a solo instrument than is frequently done in traditional trombone recitals.
Estudio físico-químico del río Manzanares, Cumaná, Venezuela
Creators: name: Senior, William
name: Godoy, Gonzalo
Publisher: name: figshare
Year: 2019
Subjects: Environmental Chemistry

description: Se realizaron muestreos mensuales de las aguas del río Manzanares entre noviembre de 1988 y julio de 1989 y evaluamos la distribución y evolución del oxígeno disuelto, y del pH lo cual puso en evidencia la presencia de una fuerte cantidad de materia orgánica en la zona estuarina, la cual tiene como origen la descarga de diferentes aportes externos al ecosistema. Los nitratos en las aguas del río se encontraron en concentraciones relativamente elevadas, mientras que la distribución del amonio y de los ortofosfatos señalaron para todo el período de estudio la existencia de un aporte puntual en la parte alta del ecosistema.Los silicatos presentan altas concentraciones a nivel del agua dulce y su distribución fue conservativa, con la excepción del mes de mayo cuando se apreció una disminución de las concentraciones a lo largo del estuario. La elevada turbidez y el corto tiempo de residencia de las aguas son dos factores que limitan la producción fitoplanctónica y por consecuencia, y por consecuencia el consumo de elementos nutritivos en las zonas altas e intermedias del ecosistema.
A dajkanyelv akusztikájának és a csecsemők temperamentumának vizsgálata
Creators: name: Kohári, Anna
name: Reichel, Uwe D.
name: Mády, Katalin
name: Lakatos, Krisztina
name: Balázs, Andrea
Publisher: name: Pannon Egyetem
Year: 2024

description: Alkalmazott nyelvtudomány, vol. 24. issue 2. ISSN 1587-1061, eISSN 2498-4442
Phyllodrepa melis Hansen 1940
Creators: name: Zanetti, A.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Phyllodrepa
Phyllodrepa melis

description: Phyllodrepa melis HANSEN 1940
 Phyllodrepa melis HANSEN 1940
 Phyllodrepa linderi SCHEERPELTZ 1966 nov.syn. Lectotype (male) (here designated) labelled / Freiburg 1934 / ex coll. Scheerpeltz (blue) / Typus Phyllodrepa Linderi O. Scheerpeltz (red) / vidit A. Zanetti 1985 / Lectotype Phyllodrepa linderi Scheerp. des. A. Zanetti 2008 / Phyllodrepa melis Hansen det. Zanetti 2008; paralectotype with the same data (NHMW).
 C o m m e n t s: Phyllodrepa linderi was described as closely related to P. melis, a North and Central European species inhabiting the burrows of badger (Meles meles). In a previous work (ZANETTI 1987) I considered the synonymy of these taxa most likely. I have re-examined the type series and designated the lectotype, whose aedeagus is deformed by the dryness, as often happens in the Omaliinae (Fig. 12), but has the general shape that corresponds to that of P. melis (Fig. 11). Also the external characters fall in the variability range of P. melis.
description: Published as part of Zanetti, A., 2008, Synonymies in the European Omaliinae, with notes on distribution (Coleoptera: Staphylinidae), pp. 979-992 in Linzer biologische Beiträge 40 (1) on page 982, DOI: 10.5281/zenodo.5429978
Adapterops Frieser 2010
Creators: name: Trýzna, Miloš
name: Baňař, Petr
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Anthribidae
Adapterops

description: Adapterops Frieser, 2010
 Type species. Adapterops nasalis Frieser, 2010: 18, by original designation.
 Diagnosis. Head small, eyes large, situated laterally, conspicuously convex, separated from each other, not emarginate. Dorsal pronotal transverse carina basal, sinuate laterally, most lateral part curved posteriorly. Postero-lateral edges of pronotum somewhat protruding posteriorly in lateral view, more or less acutangulate, lateral carina absent, therefore sides of pronotum rounded.
 The genus Adapterops is similar to the genus Pilitrogus Frieser, 1980 (both classified in the tribe Araecerini) which is hitherto known from three species from Réunion Island (FRIESER 1980). From the latter, Adapterops can be distinguished by antennal scrobe large, carinate on dorsal margin, conspicuously reaching towards middle of rostrum; rostrum with lateral margins strongly sinuate at antennal scrobes, strongly narrowed between antennal scrobes, minimum distance between scrobes about half of the eye width (Figs. 8–12).
description: Published as part of Trýzna, Miloš & Baňař, Petr, 2012, New species of Adapterops (Coleoptera: Anthribidae) from east Madagascar with a key to species and notes on sexual dimorphism and biodiversity of the family, pp. 475-485 in Acta Entomologica Musei Nationalis Pragae 52 (2) on page 476, DOI: 10.5281/zenodo.5332048
title: Methodology for Determining the Integrity of Process Engineering Design
Creators: name: Stapelberg, Rudolph Frederick
Publisher: name: Griffith University
Year: 2004
Subjects: subject: Process engineering design
subject: Engineering integrity
subject: Knowledge-based expert systems

description: In the past decade, Australian industry, and particularly the mining industry, has witnessed the development of several large “super-projects”, most in excess of a billion dollars. These large super-projects include the exploitation of Australia’s mineral wealth in alumina, copper, iron, nickel, uranium, and zinc, through the construction of huge complex industrial process plant ranging in cost from one to two billion dollars. Although these super-projects create many thousands of jobs resulting in significant decreases in unemployment especially during construction, as well as projected increases in the wealth and growth of the Australian economy, they bear a high risk in achieving their forecast profitability through maintaining budgeted costs. Most of the super-projects have either exceeded their budgeted establishment costs, or have experienced operational costs far in excess of what was originally estimated in their feasibility prospectus scope. Some of the more significant contributors to the cost “blow-outs” experienced by these super-projects can be attributed to the complexity of their engineering design, both in technology and in the complex integration of systems, as well as a lack of meticulous project management.