cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
'Loving Vincent' and 'I'm OK': two approaches to documenting the life of an artist
Creators: name: Christophini, Myria
Publisher: name: https://animateddocs.wordpress.com/
Year: 2020
Subjects: Lizzy Hobbs, I' m OK, Loving Vincent, Animated documentary, lives of artists

description: A short review and comparison of two animated films on lives of artists: Loving Vincent (directed by D. Kobiela and H. Welchman) and I'm OK (directed by Lizzy Hobbs).
Exploring the dimming event of RW Aur A through multi-epoch VLT/X-Shooter spectroscopy
Creators: name: Koutoulaki, M.
name: Facchini, S.
name: Manara, C. F.
name: Natta, A.
name: Lopez, R. Garcia
name: Fedriani, R.
name: Garatti, A. Caratti o
name: Coffey, D.
name: Ray, T. P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: RW Aur A is a CTTS that has suddenly undergone three major dimming events since 2010. We aim to understand the dimming properties, examine accretion variability, and derive the physical properties of the inner disc traced by the CO ro-vibrational emission at NIR wavelengths (2.3 mic). We compared two epochs of X-Shooter observations, during and after the dimming. We modelled the rarely detected CO bandhead emission in both epochs to examine whether the inner disc properties had changed. The SED was used to derive the extinction properties of the dimmed spectrum and compare the infrared excess between the two epochs. Lines tracing accretion were used to derive the mass accretion rate in both states. The CO originates from a region with physical properties of T=3000 K, N$_{CO}$=1x10$^{21}$ cm$^{-2}$ and vsini=113 km/s. The extinction properties of the dimming layer were derived with the effective optical depth ranging from teff 2.5-1.5 from the UV to the NIR. The inferred mass accretion rate Macc is $1.5x 10^{-8}$ Msun/yr and $\sim 2x 10^{-8}$ Msun/yr after and during the dimming respectively. By fitting the SED, additional emission is observed in the IR during the dimming event from dust grains with temperatures of 500-700K. The physical conditions traced by the CO are similar for both epochs, indicating that the inner gaseous disc properties do not change during the dimming events. The extinction curve is flatter than that of the ISM, and large grains of a few hundred microns are thus required. When we correct for the observed extinction, Macc is constant in the two epochs, suggesting that the accretion is stable and therefore does not cause the dimming. The additional hot emission in the NIR is located at about 0.5 au from the star. The dimming events could be due to a dust-laden wind, a severe puffing-up of the inner rim, or a perturbation caused by the recent star-disc encounter.
description: Accepted by Astronomy & Astrophysics
Shape Reconstruction and Weak Lensing Measurement with Interferometers: A Shapelet Approach
Creators: name: Chang, Tzu-Ching
name: Refregier, Alexandre
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a new approach for image reconstruction and weak lensing measurements with interferometers. Based on the shapelet formalism presented in Refregier (2001), object images are decomposed into orthonormal Hermite basis functions. The shapelet coefficients of a collection of sources are simultaneously fit on the uv plane, the Fourier transform of the sky brightness distribution observed by interferometers. The resulting chi-square fit is linear in its parameters and can thus be performed efficiently by simple matrix multiplications. We show how the complex effects of bandwidth smearing, time averaging and non-coplanarity of the array can be easily and fully corrected for in our method. Optimal image reconstruction, co-addition, astrometry, and photometry can all be achieved using weighted sums of the derived coefficients. As an example we consider the observing conditions of the FIRST radio survey (Becker et al. 1995; White et al. 1997). We find that our method accurately recovers the shapes of simulated images even for the sparse uv sampling of this snapshot survey. Using one of the FIRST pointings, we find our method compares well with CLEAN, the commonly used method for interferometric imaging. Our method has the advantage of being linear in the fit parameters, of fitting all sources simultaneously, and of providing the full covariance matrix of the coefficients, which allows us to quantify the errors and cross-talk in image shapes. It is therefore well-suited for quantitative shape measurements which require high-precision. In particular, we show how our method can be combined with the results of Refregier & Bacon (2001) to provide an accurate measurement of weak lensing from interferometric data.
description: 9 pages, 5 figures. To appear in ApJ; minor changes to match accepted version
Superpotential method for chiral cosmological models connected with modified gravity
Creators: name: Chervon, S. V.
name: Fomin, I. V.
name: Pozdeeva, E. O.
name: Sami, M.
name: Vernov, S. Yu.
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We consider the Chiral Cosmological Models (CCMs) and modified gravity theories associated with them. Generalization of the superpotential method for a general CCM with several scalar fields is performed, and the method of construction CCMs admitting exact solutions is developed. New classes of exact solutions in the two-component CCM connected with an $f(R)$ gravity model with an additional scalar field have been constructed. We construct new cosmological solutions for a diagonal metric of the target space, including modified power-law solutions. In particular, we propose the reconstruction procedure based on the superpotential method and present examples of kinetic part reconstruction for periodic and hyperbolic Hubble parameters. We also focus on a cyclic type of Universe dubbed the Quasi-Steady State (QSS) model, with the aim of constructing single- and double-field potentials for one and the same behaviour of the Hubble parameter using the developed superpotential method for the CCM. The realization of this task includes a new set of solutions for a CCM with a scale factor characterized by the QSS theory. We also propose a method for reducing the two-field CCM to the single scalar field model.
description: 27 pages, minor clarifications added, typos corrected, revised version to appear in Phys. Rev. D
Why the Bradley aberration cannot be used to measure absolute speeds. A comment
Creators: name: Kassner, Klaus
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In a recent article in this journal [G. Sardin, Measure of the absolute speed through the Bradley aberration of light beams on a three-axis frame, Europhys. Lett. 53 (2001) 310], Sardin proposed to use the Bradley aberration of light for the construction of a speedometer capable of measuring absolute speeds. The purpose of this comment is to show that the device would not work.
description: 2 pages, LaTeX, accepted for Europhysics Letters
title: Governing Forests and Carbon: Reducing Emissions from Deforestation and Forest Degradation (REDD+) in Indonesia
Creators: name: Boer, Henry
Publisher: name: Griffith University
Year: 2015
Subjects: subject: Reducing Emissions from Deforestation and Forest Degradation (REDD+)
subject: United Nations Framework Convention on Climate Change (UNFCCC)
subject: REDD+ strategies, Indonesia
subject: Carbon emissions
subject: Greenhouse warming

description: Since 2005, negotiations under the United Nations Framework Convention on Climate Change (UNFCCC) have focused on deforestation in developing countries. These negotiations led to the global initiative Reducing Emissions from Deforestation and Forest Degradation (REDD+), an incentive based program to provide finance and technical support to developing countries for mitigation initiatives in the Agriculture, Forestry and Other Land Use sector. REDD+ has rapidly evolved into a complex array of policy reforms, initiatives and demonstration projects in approximately 60 countries across Asia, Latin America and Africa, funded primarily from multilateral climate funds and bilateral development assistance. Under UNFCCC rules and funding agreements, participating countries are required to develop national REDD+ strategies and actions, design funding and benefit distribution mechanisms, and develop robust measurement, monitoring, reporting, and verification (MRV) systems. In addition, governments should implement social and environmental safeguards, such as engaging with local communities and resolving tenure issues, improving governance in the forest sector, and protecting biodiversity. However, the international REDD+ framework is incomplete and it remains at the discretion of participating countries to initiate policies and activities that address local drivers of deforestation, and meet domestic priorities.
MOESM1 of Arf6-driven endocytic recycling of CD147 determines HCC malignant phenotypes
Creators: name: Qi, Shanshan
name: Su, Linjia
name: Li, Jing
name: Zhang, Chuanshan
name: Ma, Zhe
name: Liu, Guiqiu
name: Zhang, Qing
name: Jia, Guhe
name: Piao, Yongjun
name: Zhang, Sihe
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Additional file 1: Figure S1. CD147 expression and stable knock-down in liver cancer cells. Figure S2. Flow cytometry analysis of CD147 level on liver cancer cell surface. Figure S3. Arf6-mediated CD147 recycling promotes Huh7 and HepG2 cell adhesion to ECM. Figure S4. Arf6-KD impaired the cell-cell aggregation of Huh7 and HepG2 cells. Arf6-perturbed cells were reseeded on agar for static culture, and cell aggregation clusters were evaluated. Figure S5. Morphometric analyses of Arf6-perturbed liver cancer cells. Figure S6. ARF6-specific GEFs and GAPs expressed in liver cancer patients. Box plots depict the expression level difference between liver cancer (T) and normal tissues (N). Figure S7. Co-expression network analysis of the Arf6-CD147 gene pair. Figure S8. Pair-wise correlation analysis for the expression (IHC staining) levels of CD147, Arf6, Rac1 and ARNO in primary HCC tissues. Table S1. Clinicopathological features of HCC patients and association with co-expression of CD147, Arf6, ARNO, and Rac1.
Exephanes hungaricus KISS 1915
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Exephanes
Exephanes hungaricus

description: Exephanes hungaricus KISS 1915
 Exephanes hungaricus KISS 1915: 24 – Holotypus (): "Ferenczfalva Hungaria" (= Valiug/ Rumänien) und Determinationsetiketten, Budapest.
 G ü l t i g e r N a m e Triptognathus unifasciatus (SPINOLA 1843) (YU & HORSTMANN 1997: 657). KISS (1929: 90) und HEINRICH (1929: 322 f.) stellen das Taxon zu T. unidentatus (BERTHOUMIEU), einem jüngeren Synonym von T. unifasciatus.
description: Published as part of Horstmann, K., 2008, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae. II. Ichneumoninae (Hymenoptera, Ichneumonidae), pp. 771-784 in Linzer biologische Beiträge 40 (1) on page 774, DOI: 10.5281/zenodo.5429664
ISOCAM observations of the rho Ophiuchi cloud: Luminosity and mass functions of the pre-main sequence embedded cluster
Creators: name: Bontemps, S.
name: Andre, P.
name: Kaas, A. A.
name: Nordh, L.
name: Olofsson, G.
name: Huldtgren, M.
name: Abergel, A.
name: Blommaert, J.
name: Boulanger, F.
name: Burgdorf, M.
name: Cesarsky, C. J.
name: Cesarsky, D.
name: Copet, E.
name: Davies, J.
name: Falgarone, E.
name: Lagache, G.
name: Montmerle, T.
name: Perault, M.
name: Persi, P.
name: Prusti, T.
name: Puget, J. L.
name: Sibille, F.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of the first extensive mid-infrared (IR) imaging survey of the rho Ophiuchi embedded cluster, performed with the ISOCAM camera on board the ISO satellite. The main molecular cloud L1688, as well as L1689N and L1689S, have been completely surveyed for point sources at 6.7 and 14.3 micron. A total of 425 sources are detected including 16 Class I, 123 Class II, and 77 Class III young stellar objects (YSOs). Essentially all of the mid-IR sources coincide with near-IR sources, but a large proportion of them are recognized for the first time as YSOs. Our dual-wavelength survey allows us to identify essentially all the YSOs with IR excess in the embedded cluster down to Fnu ~ 10 - 15 mJy. It more than doubles the known population of Class II YSOs and represents the most complete census to date of newly formed stars in the rho Ophiuchi central region. The stellar luminosity function of the complete sample of Class II YSOs is derived with a good accuracy down to L= 0.03 Lsun. A modeling of this lumino- sity function, using available pre-main sequence tracks and plausible star for- mation histories, allows us to derive the mass distribution of the Class II YSOs which arguably reflects the IMF of the embedded cluster. We estimate that the IMF in rho Ophiuchi is well described by a two-component power law with a low- mass index of -0.35+/-0.25, a high-mass index of -1.7 (to be compared with the Salpeter value of -1.35), and a break occurring at M = 0.55+/-0.25 Msun. This IMF is flat with no evidence for a low-mass cutoff down to at least 0.06 Msun.
description: A&A Document Class -- version 5.01, 27 pages, 10 figures v2: typos added including few changes in source numbering
Cold QCD at finite isospin density: confronting effective models with recent lattice data
Creators: name: Avancini, Sidney S.
name: Bandyopadhyay, Aritra
name: Duarte, Dyana C.
name: Farias, Ricardo L. S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We compute the QCD equation of state for zero temperature and finite isospin density within the Nambu-Jona-Lasinio model in the mean field approximation, motivated by the recently obtained Lattice QCD results for a new class of compact stars: pion stars. We have considered both the commonly used Traditional cutoff Regularization Scheme and the Medium Separation Scheme, where in the latter purely vacuum contributions are separated in such a way that one is left with ultraviolet divergent momentum integrals depending only on vacuum quantities. We have also compared our results with the recent results from Lattice QCD and Chiral Perturbation Theory.
description: 10 pages, 6 figures, replaced with updated version matching the published one
Acanthaceae
Creators: name: Masharabu, Tatien
name: Bigendako, Marie Josée
name: Nzigidahera, Benoît
name: Mpawenayo, Balthazar
name: Lejoly, Jean
name: Bangirinama, Frédéric
name: Bogaert, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Lamiales
Acanthaceae

description: Acanthaceae.
Hypoestes verticillaris (L.f.) Sol. ex Roem. & Schult., Thunbergia alata Bojer ex Sims.
description: Published as part of Masharabu, Tatien, Bigendako, Marie Josée, Nzigidahera, Benoît, Mpawenayo, Balthazar, Lejoly, Jean, Bangirinama, Frédéric & Bogaert, Jan, 2012, Vascular flora inventory and plant diversity of the Ruvubu National Park, Burundi, pp. 155-162 in Adansonia (3) (3) 34 (1) on page 159, DOI: 10.5252/a2012n1a17, http://zenodo.org/record/4599304
The Effects of a Stellar Encounter on a Planetesimal Disk
Creators: name: Kobayashi, Hiroshi
name: Ida, Shigeru
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the effects of a passing stellar encounter on a planetesimal disk through analytical calculations and numerical simulations, and derive the boundary radius ($a_{\rm planet}$) outside which planet formation is inhibited by disruptive collisions with high relative velocities.
description: 25 pages, 11 figures, included in 15 tex-files, 7 ps-files and 4 eps-files
Additional file 6: of Are interventions focused on gender-norms effective in preventing domestic violence against women in low and lower-middle income countries? A systematic review and meta-analysis
Creators: name: Agumasie Semahegn
name: Kwasi Torpey
name: Abubakar Manu
name: Nega Assefa
name: Gezahegn Tesfaye
name: Ankomah, Augustine
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: GRADE for the summary of evidence for different outcomes. (DOCX 18 kb)
Hemichneumon hungaricus KISS 1924
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Hemichneumon
Hemichneumon hungaricus

description: Hemichneumon hungaricus KISS 1924
 Hemichneumon hungaricus KISS 1924: 47 – Holotypus (!) von SAWONIEWICZ (1988: 485) revidiert. Kiss hat den Typus irrtümlich als beschrieben. Der Typenfundort Borosjenö heisst jetzt Ineu in Rumänien.
 G ü l t i g e r N a m e Pleolophus brachypterus (GRAVENHORST 1815) (SAWONIEWICZ, l.c.).
description: Published as part of Horstmann, K., 2008, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae. II. Ichneumoninae (Hymenoptera, Ichneumonidae), pp. 771-784 in Linzer biologische Beiträge 40 (1) on page 774, DOI: 10.5281/zenodo.5429664
Eysarcoris ventralis
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Eysarcoris
Eysarcoris ventralis

description: Eysarcoris ventralis (Westwood, 1837)
 Material examined. Many specimens: KHUZESTAN: Abadan, 10.–11.vi.2005; near Ahvaz, 29.iv.–1.v.2007; Ahvaz – Ghazevieh, 7.–8.vi.2005;Ahvaz – Jangieh, 11.–12.vi.2006; near Ahvaz, Karun river, 10.–11.vi.2006; near Andimeshk, 5.–6.v.2007; Andimeshk – Tangvan, 9.–10.vi.2006; Bandar-e-Mahshar, 12.–13.vi.2006; Behbahan, 27.–28.iv.2007; Dezful, 6.–7.vi.2005; Estahban, 1710 m a.s.l., 10.–11.vi.1996; Lali, 6.–7.vi.2008; near Ramhormoz, 7.–9.vi.2008; Sadde-e-Daz, 6.–7.vi.2005; Shadegan, 9.–10.vi.2008. BUSHEHR: Ab Pakhs, 25.–26.iv.2007. FARS: Estahban, 1710 m a.s.l., 10.–11.vi.1996; Firuzabad, 15.–16.vi.2008; Maharlu, 1. and 18.vi.2002, 14.–15.vi.2003; Mokhah near Ghotb Abad, 13.vi.2003; 15 km E Sa’adatshahr, 1650 m a.s.l., 6.–7.vi.1996; Zarqan Bamon National Park, 1650 m a.s.l., 13.–14.vi.1996. WEST AZERBAIJAN: Marangalu near Urmiyeh, 15.–17.vii.2007.
 Comments. In fields, gardens and fresh meadows. Holomediterranean, extending to the Ethiopian and Oriental Regions.
description: Published as part of Linnavuori, Rauno E., 2012, Studies on Pyrrhocoroidea, Coreoidea and Pentatomoidea of Khuzestan and the adjacent provinces in Iran (Hemiptera: Heteroptera), pp. 67-88 in Acta Entomologica Musei Nationalis Pragae 52 (1) on page 78, DOI: 10.5281/zenodo.5330439
Influence of Rotation on Pulsar Radiation Characteristics
Creators: name: Ahmadi, Peyman
name: Gangadhara, R. T.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a relativistic model for pulsar radio emission by including the effect of rotation on coherent curvature radiation by bunches. We find that rotation broadens the width of leading component compared to the width of trailing component. We estimate the component widths in the average pulse profiles of about 24 pulsars, and find that 19 of them have a broader leading component. We explain this difference in the component widths by using the nested cone emission geometry. We estimate the effect of pulsar spin on the Stokes parameters, and find that the inclination between the rotation and magnetic axes can introduce an asymmetry in the circular polarization of the conal components. We analyze the single pulse polarization data of PSR B0329+54 at 606 MHz, and find that in its conal components, one sense of circular polarization dominates in the leading component while the other sense dominates in the trailing component. Our simulation shows that changing the sign of the impact parameter changes the sense of circular polarization as well as the swing of polarization angle.
description: 20 pages, 4 Postscript figures, uses aastex.cls. Accepted for Publication in ApJ 2001
Additional file 2: of DNA methylation links prenatal smoking exposure to later life health outcomes in offspring
Creators: name: Wiklund, Petri
name: Karhunen, Ville
name: Richmond, Rebecca
name: Parmar, Priyanka
name: Rodriguez, Alina
name: Maneka Silva
name: Wielscher, Matthias
name: Rezwan, Faisal
name: Richardson, Tom
name: Veijola, Juha
name: Karl-Heinz Herzig
name: Holloway, John
name: Relton, Caroline
name: Sebert, Sylvain
name: Marjo-Riitta JĂ¤Rvelin
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Molecular Biology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Characteristics of the participants based on exposure to maternal smoking during pregnancy in the ALSPAC studies. (DOCX 13 kb)
"Hidden" Seyfert 2 Galaxies and the X-ray Background
Creators: name: Moran, E. C.
name: Filippenko, A. V.
name: Chornock, R.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Obscured active galactic nuclei, which are classified optically as type 2 (narrow-line) Seyfert galaxies in the local universe, are by far the most promising candidates for the origin of the hard (2-10 keV) X-ray background radiation. However, optical follow-up observations of faint X-ray sources in deep Chandra images have revealed surprising numbers of apparently normal galaxies at modest redshift. Such objects represent ~40-60% of the sources classified in deep Chandra surveys, raising the possibility that the X-ray galaxy population has evolved with cosmic time. Alternatively, most of the faint X-ray galaxies in question are so distant that their angular diameters are comparable to the slit widths used in ground-based spectroscopic observations; thus, their nuclear spectral features may be overwhelmed (``hidden'') by host-galaxy light. To test this hypothesis, we have obtained integrated spectra of a sample of nearby, well-studied Seyfert 2 galaxies. The data, which accurately simulate observations of distant Chandra sources, demonstrate convincingly that the defining spectral signatures of Seyfert 2s can be hidden by light from their host galaxies. In fact, 60% of the observed objects would not be classified as Seyfert 2s on the basis of their integrated spectra, similar to the fraction of faint X-ray sources identified with ``normal'' galaxies. Thus, the numbers of narrow-line active galaxies in deep Chandra surveys (and perhaps all ground-based spectroscopic surveys of distant galaxies) are likely to have been underestimated.
description: 9 pages, including 1 figure. To appear in ApJ Letters
title: Branded Content and Australian Hybrid Film Financing
Creators: name: Chircop, Dean
Publisher: name: Griffith University
Year: 2017
Subjects: subject: Feature film financing, Australia
subject: Fictional narrative screenplay
subject: Commercial brand partners
subject: Creative integrity

description: This exegesis proposes an alternative strategy for financing feature films in Australia, one centred on working to create a fictional narrative screenplay in conjunction with commercial brand partners. The studio project at the heart of this reflective practice research is the writing and development of King of Speed, a feature film script set in the realm of competitive automobile racing. I argue that the alignment of this milieu and industry with my narrative interests has provided a unique opportunity to partner with key corporations and brands without ceding creative control. I suggest that a major challenge confronted in the design of the project is the aesthetic contextualisation of commercial content. A key aim of the script development is to provide opportunities for sponsorship and the showcasing of ‘products’ that appear to be contextually naturalised and hence not to violate the integrity of the artwork. This research contributes to the field of screen producing and filmmakers who are seeking ways to finance feature films that are outside entrenched and established models. The exegesis investigates the process of script development; the financial advantages and disadvantages that can be gained from associating films with brands; the ethical and aesthetic limits of product placement; the complex issues surrounding artists’ rights; and the commercial challenges to influences on creative integrity.
MOESM1 of Case report: two novel VPS13B mutations in a Chinese family with Cohen syndrome and hyperlinear palms
Creators: name: Zhao, Sha
name: Luo, Zhenqing
name: Xiao, Zhenghui
name: Li, Liping
name: Zhao, Rui
name: Yang, Yongjia
name: Zhong, Yan
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Computational Biology

description: Additional file 1: Table S1. Primers and PCR conditions in this study.
Stagonomus (Dalleria) devius Seidenstucker 1965
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Stagonomus
Stagonomus devius

description: Stagonomus (Dalleria) devius Seidenstücker, 1965
 Material examined. FARS: 15 km E Sa’adatshahr, 1680 m a.s.l., 1 specimen, 6.–7.vi.1996.
 Comments. In hilly steppes. Syrio-Anatolian, recorded from Armenia, Turkey, Iran, Iraq, Israel, Syria, and Turkmenistan.
description: Published as part of Linnavuori, Rauno E., 2012, Studies on Pyrrhocoroidea, Coreoidea and Pentatomoidea of Khuzestan and the adjacent provinces in Iran (Hemiptera: Heteroptera), pp. 67-88 in Acta Entomologica Musei Nationalis Pragae 52 (1) on page 79, DOI: 10.5281/zenodo.5330439
title: Economic Modelling Methods for the Estimation of Resource Use, Cost-Effectiveness and Allocative Efficiency of Health Care Provision in a Capacity Constrained Health Care System
Creators: name: Standfield, Lachlan Barry
Publisher: name: Griffith University
Year: 2017
Subjects: subject: Health care provision
subject: Health care, Cost effectiveness
subject: Health care capacity
subject: Health care, Economic modelling

description: Cost-effectiveness models for health care interventions generally make the assumption that all resources are available, as required, without capacity constraints. This assumption may be a reasonable approximation of the truth for a range of questions faced by decision makers in health care. However, in some health care settings, capacity constraints predominate leading to queue development. In these situations the use of a modelling technique that can accommodate these constraints would appear advisable to allow the efficiency of competing healthcare interventions to be determined. Nevertheless, there have been no empirical comparisons of economic modelling techniques that capture capacity constraints and those that do not. Further, there are only a few cost-effectiveness analyses (CEA) of health care that capture the effect of capacity constraints at all. This research seeks to explore these gaps in the literature in an applied manner.
Additional file 7: of Are interventions focused on gender-norms effective in preventing domestic violence against women in low and lower-middle income countries? A systematic review and meta-analysis
Creators: name: Agumasie Semahegn
name: Kwasi Torpey
name: Abubakar Manu
name: Nega Assefa
name: Gezahegn Tesfaye
name: Ankomah, Augustine
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Confirmation letter for funding. (PDF 1930 kb)
Brown Dwarf Atmospheres as the Potentially Most Detectable and Abundant Sites for Life
Creators: name: Lingam, Manasvi
name: Loeb, Abraham
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: We show that the total habitable volume in the atmospheres of cool brown dwarfs with effective temperatures of $\sim 250$-$350$ K is possibly larger by two orders of magnitude than that of Earth-like planets. We also study the role of aerosols, nutrients and photosynthesis in facilitating life in brown dwarf atmospheres. Our predictions might be testable through searches for spectral edges in the near-infrared and chemical disequilibrium in the atmospheres of nearby brown dwarfs that are either free-floating or within several AU of stars. For the latter category, we find that the James Webb Space Telescope (JWST) may be able to achieve a signal-to-noise ratio of $\sim 5$ after a few hours of integration time per source for the detection of biogenic spectral features in $\sim 10^3$ cool brown dwarfs.
description: Published in The Astrophysical Journal; 19 pages; 3 figures
Herpestomus banaticus KISS 1924
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Herpestomus
Herpestomus banaticus

description: Herpestomus banaticus KISS 1924
 Herpestomus banaticus KISS 1924: 47 f. – Holotypus () von DILLER (1983: 56) revidiert. Der Typenfundort Ferenczfalva heisst jetzt Valiug in Rumänien.
 G ü l t i g e r N a m e Dicaelotus rufiventris (BERTHOUMIEUL 1899) (DILLER, l.c.).
description: Published as part of Horstmann, K., 2008, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae. II. Ichneumoninae (Hymenoptera, Ichneumonidae), pp. 771-784 in Linzer biologische Beiträge 40 (1) on page 774, DOI: 10.5281/zenodo.5429664
Stagonomus (Stagonomus) amoenus
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Stagonomus
Stagonomus amoenus

description: Stagonomus (Stagonomus) amoenus (Brullé, 1832)
 Material examined. FARS: 15 km E Sa’adatshahr, 1680 m a.s.l., 1 specimen, 6.–7.vi.1996.
 Comments. In a mountain steppe. Euromediterranean-Turanian.
description: Published as part of Linnavuori, Rauno E., 2012, Studies on Pyrrhocoroidea, Coreoidea and Pentatomoidea of Khuzestan and the adjacent provinces in Iran (Hemiptera: Heteroptera), pp. 67-88 in Acta Entomologica Musei Nationalis Pragae 52 (1) on page 79, DOI: 10.5281/zenodo.5330439
Smoothed Particle Hydrodynamics with particle splitting, applied to self-gravitating collapse
Creators: name: Kitsionas, S.
name: Whitworth, A. P.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe and demonstrate a method for increasing the resolution locally in a Smoothed Particle Hydrodynamic (SPH) simulation, by splitting particles. We show that in simulations of self-gravitating collapse (of the sort which are presumed to occur in star formation) the method is stable, and affords great savings in computer time and memory. When applied to the standard Boss & Bodenheimer test -- which has been shown to depend critically on fulfilment of the Jeans Condition -- the results are comparable both with those obtained using Adaptive Mesh Refinement, and with those obtained using a standard high-resolution SPH simulation, but they are achieved with considerably less computational resource. Further development and testing is required before the method can safely be applied to more general flows.
description: 8 pages, 6 figures
MPEC 2024-C165 : 2024 CP4
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 CP4

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
SHALOS: Statistical Herschel-ATLAS Lensed Objects Selection
Creators: name: González-Nuevo, J.
name: Gómez, S. L. Suárez
name: Bonavera, L.
name: Sánchez-Lasheras, F.
name: Argüeso, F.
name: Toffolatti, L.
name: Herranz, D.
name: González-Gutiérrez, C.
name: Riesgo, F. García
name: Juez, F. J. de Cos
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The statistical analysis of large sample of strong lensing events can be a powerful tool to extract astrophysical and/or cosmological valuable information. However, the number of such events is still relatively low, mostly because of the lengthily observational validation process on individual events. In this work we propose a new methodology with a statistical selection approach in order to increase by a factor of $\sim 5$ the number of such events. Although the methodology can be applied to address several selection problems, it has particular benefits in the case of the identification of strongly lensed galaxies: objectivity, minimal initial constrains in the main parameter space, preservation of the statistical properties. The proposed methodology is based on the Bhattacharyya distance as a measure of the similarity between probability distributions of properties of two different cross-matched galaxies. The particular implementation for the aim of this work is called SHALOS and it combines the information of four different properties of the pair of galaxies: angular separation, luminosity percentile, redshift and optical/sub-mm flux density ratio. The SHALOS method provided a ranked list of strongly lensed galaxies. The number of candidates for the final associated probability, $P_{tot}>0.7$, is 447 with an estimated mean amplification factor of 3.12 for an halo with a typical cluster mass. Additional statistical properties of the SHALOS candidates, as the correlation function or the source number counts, are in agreement with previous results indicating the statistical lensing nature of the selected sample.
description: 9 pages, 6 figures, submitted to Astronomy & Astrophysics
MOESM1 of Adverse drug reactions experienced by out-patients taking chlorpromazine or haloperidol at Zomba Mental Hospital, Malawi
Creators: name: Chikowe, Ibrahim
name: McDonald Domingo
name: Mwakaswaya, Vasco
name: Shagufta Parveen
name: Chitsanzo Mafuta
name: Kampira, Elizabeth
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1: Table S1. Demographic and health information about respondents.
Wiedemann-Franz Law For Hot QCD Matter in a Color String Percolation Scenario
Creators: name: Sahoo, Pragati
name: Sahoo, Raghunath
name: Tiwari, Swatantra Kumar
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Transport coefficients serve as important probes in characterizing the QCD matter created in high-energy heavy-ion collisions. Thermal and electrical conductivities as transport coefficients have got special significance in studying the time evolution of the created matter. We have adopted color string percolation approach for the estimation of thermal conductivity ($κ$), electrical conductivity ($σ_{el}$) and their ratio, which is popularly known as Wiedemann-Franz law in condensed matter physics. The ratio $κ/σ_{el}T$, which is also known as Lorenz number ($\mathbb{L}$) is studied as a function of temperature and is compared with various theoretical calculations. We observe that the thermal conductivity for hot QCD medium is almost temperature independent in the present formalism and matches with the results obtained in ideal equation of state (EOS) for quark-gluon plasma with fixed coupling constant ($α_s$). The obtained Lorenz number is compared with the Stefan-Boltzmann limit for an ideal gas. We observe that a hot QCD medium with color degrees of freedom behaves like a free electron gas.
description: No change in the MS. arXiv admin note: text overlap with arXiv:1804.07980
A Catalog of OB Associations in the spiral galaxy NGC 300
Creators: name: Pietrzynski, G.
name: Gieren, W.
name: Fouque, P.
name: Pont, F.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results of a search for OB associations in NGC 300. Using an automatic and objective method (PLC technique) 117 objects were found. Statistical tests indicate that our sample is contaminated by less than 10 % of spurious detections due to random concentrations of blue stars. Spatial distributions of detected associations and H II regions are strongly correlated. The size distribution reveals a significant peak at about 60 $μ$rad which corresponds to 125 parsecs if a distance modulus of 26.66 mag is assumed. Besides the objects with sizes corresponding to typical associations we also found several much larger objects. A second level application of our detection method revealed that most of these are composed of smaller subgroups, with sizes of about 100 pc.
description: 9 pages, Latex, 5 Figures, Appendix (two pages, maps of 6 typical associations in NGC 300 and map of one potential stellar complex in NGC 300). Accepted for publication in Astronomy & Astrophysics
Amaranthaceae
Creators: name: Masharabu, Tatien
name: Bigendako, Marie Josée
name: Nzigidahera, Benoît
name: Mpawenayo, Balthazar
name: Lejoly, Jean
name: Bangirinama, Frédéric
name: Bogaert, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Amaranthaceae

description: Amaranthaceae.
Alternanthera pungens Kunth.
description: Published as part of Masharabu, Tatien, Bigendako, Marie Josée, Nzigidahera, Benoît, Mpawenayo, Balthazar, Lejoly, Jean, Bangirinama, Frédéric & Bogaert, Jan, 2012, Vascular flora inventory and plant diversity of the Ruvubu National Park, Burundi, pp. 155-162 in Adansonia (3) (3) 34 (1) on page 159, DOI: 10.5252/a2012n1a17, http://zenodo.org/record/4599304
Supplementary document for Deep Learning-Based Autofocus Method Enhances Image Quality in Light-Sheet Fluorescence Microscopy - 5292160.pdf
Creators: name: Li, Chen
name: MOATTI, ADELE
name: Zhang, Xuying
name: Ghashghaei, H
name: Greenbaum, Alon
Publisher: name: Optica Publishing Group
Year: 2021
Subjects: Uncategorized
Nonlinear Optics and Spectroscopy

description: Supplementary materials
Mecidea lindbergi Wagner 1954
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Mecidea
Mecidea lindbergi

description: Mecidea lindbergi Wagner, 1954
 Material examined. KHUZESTAN: Andimeshk – Tangvan, 1 specimen, 9.–10.vi.2006; near Lali, 1 specimen, 6.–8.v.2007; near Ramhormoz, 1 specimen, 7.–9.vi.2008; Sadde-e-Dez, 2 specimens, 6.–7.vi.2003. BUSHEHR: near Bandar-e-Genaveh, 2 specimens, 23.–24.iv.2007. FARS: Maharlu, 1 specimen, 16.–17.vi.2008; 15 km E Sarvestan, 1 specimen, 15.–16.vi.2003. LORESTAN: near Khoram Abad, 1 specimen, 5.–6.vi.2005.
 Comments. On grasses in dry localities. Eremian, extending from the Cape Verde and Canary Islands to Afghanistan and Turkmenistan.
description: Published as part of Linnavuori, Rauno E., 2012, Studies on Pyrrhocoroidea, Coreoidea and Pentatomoidea of Khuzestan and the adjacent provinces in Iran (Hemiptera: Heteroptera), pp. 67-88 in Acta Entomologica Musei Nationalis Pragae 52 (1) on page 79, DOI: 10.5281/zenodo.5330439
Developing a coding scheme for analysing classroom dialogue across d educational contexts.
Creators: name: Hofmann, RJ
name: Hennessy, Sara
name: Rojas-Drummond, S
name: Barrera, MJ
name: García Carrión, R
name: Howe, C
name: Kershner,
name: Littleton, K
name: Marquez, AM
name: Mercer, Neil
Publisher: name: Apollo - University of Cambridge Repository
Year: 2016
Subjects: dialogue
coding scheme
communicative act
classroom interaction
sociocultural theory

description: The research reported sought to develop a framework for systematically analysing classroom dialogue for application across a range of educational settings. The paper outlines the development and refinement of a coding scheme that attempts to represent and operationalise commonalities amongst some key theorists in the field concerning productive forms of educational dialogue. The team has tested it using video recordings from classroom settings in the UK and Mexico, across age phases, subject areas, and different interactional contexts including whole class, group and paired work. Our Scheme for Educational Dialogue Analysis (SEDA) is situated within a sociocultural paradigm, and draws on Hymes' Ethnography of Communication to highlight the importance of context. We examined how such a tool could be used in practice. We found that concentrating on the ‘communicative act’ to explore dialogue between participants was an appropriate level of granularity, while clustering the 33 resulting codes according to function of the acts helped to highlight dialogic sequences within lessons. We report on the application of the scheme in two different learning contexts and reflect on its fitness for purpose, including perceived limitations. Development of specialised sub-schemes and a version for teachers is underway.
Cosmology with galaxy-galaxy lensing on non-perturbative scales: Emulation method and application to BOSS LOWZ
Creators: name: Wibking, Benjamin D.
name: Weinberg, David H.
name: Salcedo, Andrés N.
name: Wu, Hao-Yi
name: Singh, Sukhdeep
name: Rodríguez-Torres, Sergio
name: Garrison, Lehman H.
name: Eisenstein, Daniel J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We describe our nonlinear emulation (i.e., interpolation) framework that combines the halo occupation distribution (HOD) galaxy bias model with $N$-body simulations of nonlinear structure formation, designed to accurately predict the projected clustering and galaxy-galaxy lensing signals from luminous red galaxies (LRGs) in the redshift range $0.16 < z < 0.36$ on comoving scales $0.6 < r_p < 30$ \hMpc. The interpolation accuracy is $\lesssim 1-2$ per cent across the entire physically plausible range of parameters for all scales considered. We correctly recover the true value of the cosmological parameter $S_8 = ({σ_8}/{0.8228}) ({Ω_{\text{m}}}/{0.3107})^{0.6}$ from mock measurements produced via subhalo abundance matching (SHAM)-based lightcones designed to approximately match the properties of the SDSS LOWZ galaxy sample. Applying our model to Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 14 (DR14) LOWZ galaxy clustering and galaxy-shear cross-correlation measurements made with Sloan Digital Sky Survey (SDSS) Data Release 8 (DR8) imaging, we perform a prototype cosmological analysis marginalizing over $w$CDM cosmological parameters and galaxy HOD parameters. We obtain a 4.4 per cent measurement of $S_8 = 0.847 \pm 0.037$, in $3.5σ$ tension with the Planck cosmological results of $1.00 \pm 0.02$. We discuss the possibility of underestimated systematic uncertainties or astrophysical effects that could explain this discrepancy.
description: Updated to match accepted version
X-Ray Microlensing of Bright Quasars
Creators: name: Takahashi, Rohta
name: Yonehara, Atsunori
name: Mineshige, Shin
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We calculated the expected microlens light curves for several accretion-flow models and compared the results to find what aspects of distinct flow structures can be extracted from the microlens light curves. As for the flow models, we considered the standard disk, optically thin advection-dominated flow, and the disk-corona model by Kawaguchi et al., which can nicely reproduce the observed quasar spectra. The calculated microlens light curves of the disk-corona model exhibit rapid soft X-ray and slow hard X-ray variations. This is because the former is generated by Compton up-scattering of soft (optical -- UV) photons from the innermost part of the disk body, while the latter is emitted via bremsstrahlung within the corona at relatively large radii. Furthermore, an inhomogeneous emissivity distribution over the disk produces humps in the microlens light curves because of enhanced microlens amplification of the bright areas. It is hoped that black-hole accretion theory coupled with future multi-wavelength microlens observations will be able to reveal such spatial and temporal behaviors of flows in the vicinity of black holes.
description: 12 pages, 4 Postscript figures
Supplementary document for Optical force induced by strong exciton-plasmon coupling - 5539673.pdf
Creators: name: Li, Wanjun
name: Yu, Yang
name: Yan, Haochen
name: Zeng, Qing-Guang
name: Xiao, Tinghui
Publisher: name: Optica Publishing Group
Year: 2021
Subjects: Uncategorized

description: Dependence of the optical forces on the coupling strength
Herpestomus brunneus KISS 1924
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Herpestomus
Herpestomus brunneus

description: Herpestomus brunneus KISS 1924
 Herpestomus brunneus KISS 1924: 48 f. – Holotypus () von DILLER (1983: 56) und HORSTMANN (1992: 236) revidiert. Der Typus war zeitweilig verschollen (HORSTMANN 1973: 71), wurde aber von mir bei einem Besuch in Budapest aufgefunden. Der Typenfundort Oroszmezö heisst jetzt Rus in Rumänien.
 G ü l t i g e r N a m e Dichrogaster modesta (GRAVENHORST 1829) (TOWNES 1983: 120).
description: Published as part of Horstmann, K., 2008, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae. II. Ichneumoninae (Hymenoptera, Ichneumonidae), pp. 771-784 in Linzer biologische Beiträge 40 (1) on page 774, DOI: 10.5281/zenodo.5429664