cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Exploring Commercial and Management Issues Arising in Tourist Based Strata-Title Accommodation Complexes
Creators: name: Cassidy, Kelly
Publisher: name: Griffith University
Year: 2008
Subjects: subject: Strata title tourism accommodation
subject: strata title management
subject: unit owner satisfaction

description: This thesis investigates management issues arising in Australian strata title tourism accommodation (STTA) properties. It is believed to represent the first comprehensive academic analysis addressing STTA management issues. A sequential mixed methods approach has been adopted comprising exploratory and in-depth interviews and a questionnaire survey. The research draws on stakeholder theory to identify key STTA stakeholders and describe the nature of their involvement in the industry. The study also examines the owner/manager relationship in STTA properties and determines factors affecting unit owner satisfaction. In addition, management challenges are identified and discussed and a typology of STTA properties is developed. Based on the qualitative data collected, nine generic STTA best governance management recommendations are presented. Agency theory has been drawn upon in determining that it appears that tension between agent (manager) and principal (unit owner) is greatest in owner/operator complexes and those managed by a corporate entity. It has also been concluded that the most sustainable form of STTA management delivery is in branded hotel operations. The quantitative data collected provides statistically significant evidence that STTA unit owners are more satisfied in independent management complexes relative to STTA complexes where the management rights are owned by a corporation.
Correlated Insulating States in Twisted Double Bilayer Graphene
Creators: name: Burg, G. William
name: Zhu, Jihang
name: Taniguchi, Takashi
name: Watanabe, Kenji
name: MacDonald, Allan H.
name: Tutuc, Emanuel
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We present a combined experimental and theoretical study of twisted double bilayer graphene with twist angles between 1° and 1.35°. Consistent with moiré band structure calculations, we observe insulators at integer moiré band fillings one and three, but not two. An applied transverse electric field separates the first moiré conduction band from neighbouring bands, and favors the appearance of correlated insulators at 1/4, 1/2, and 3/4 band filling. Insulating states at 1/4 and 3/4 band filling emerge only in a parallel magnetic field (B_{||}), whereas the resistance at half band filling is weakly dependent on B_{||}. These findings suggest that correlated insulators are favored when a moiré flat band is spectrally isolated, with spin polarization at 1/4 and 3/4 band filling and valley polarization at 1/2 band filling.
description: 5 pages, 4 figures, includes supplementary material
Antepipona defecta GIORDANI SOIKA 1963
Creators: name: Gusenleitner, J.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eumenidae
Antepipona
Antepipona defecta

description: Antepipona defecta GIORDANI SOIKA 1963
N i g e r i a: 26 km SSE Abuja, 9°06’N 7°45’E, 400m, 14.5.201 1, 1, leg. J. Halada, coll. OLM.
Bisher waren von dieser Art nur Funde in Gambia und Senegal bekannt (CARPENTER et al. 2009).
description: Published as part of Gusenleitner, J., 2012, Über bemerkenswerte Faltenwespen aus der äthiopischen Region Teil 9 (Hymenoptera: Vespidae: Eumeninae), pp. 1159-1176 in Linzer biologische Beiträge 44 (2) on page 1167, DOI: 10.5281/zenodo.5329007
title: Interpreting the Modern: Flatland in Brisbane 1920-1941 Living in Multiple-Occupancy Dwellings in Interwar Brisbane
Creators: name: Bennett, Helen Margaret
Publisher: name: Griffith University
Year: 2011
Subjects: subject: Apartment dwelling in Brisbane
subject: Housing Brisbane
subject: Blocks of flats
subject: Twentieth century modern lifestyle

description: This thesis investigates the fundamental social, cultural, demographic, economic and political changes that precipitated and encouraged the first significant wave of multiple-occupancy dwelling in Brisbane: the residential flats of the interwar period of the twentieth century. Brisbane’s earliest ‘flats’ had emerged by the 1910s, the product of converting large, obsolete nineteenth-century residences into multiple dwellings. Often not fully self-contained, they differed only marginally from the traditional rooming-house, and were widely considered as a short-term expedient in the face of a severe housing shortage. In the 1920s Brisbane residents were introduced to the purpose-designed, modern urban flat. Acceptance was gradual, but by the second half of the 1930s, new flat construction in Brisbane was booming. The emergence of the purpose-built flat represented, physically and culturally, the city’s introduction to a distinctively twentieth century, modern lifestyle. The shift to flat-living created: vigorous community debate over the fear of slum creation; formal responses to these concerns in the form of local ordinances controlling the construction and licensing of flat buildings; and substantial change to the character of inner-suburban Brisbane. Defining, accounting for, deriving meaning from, and exploring the significance of, the fashion for flat-dwelling in interwar Brisbane – in particular the popularity of the purpose-designed, purpose-built blocks of flats – are the objectives of this research. The fashion for living in flats in Brisbane is considered within three broad frameworks: the continuity of the urban experience across time and place; the democratisation of modernity and notions of what it meant to be ‘modern’ in Brisbane in the 1920s and 1930s; and the cultural legacy. In pursuing these objectives the study considers contemporary debates about the nature of urban living and the need for town planning initiatives in Queensland; the inter-relationship between the compact flat and the lifestyle it generated; generic profiles of those who occupied and invested in purpose-built flat developments; interwar controls (overt and covert) on new flat construction; and the resultant environmental impact in terms of location, form, scale, materials and neighbourhood character. In conclusion, the cultural value of Brisbane’s interwar flats as a distinctive built form is addressed.
Materiais Educativos sobre TEV: Prevenção e Capacitação para Diversos Encontros/Eventos
Creators: name: Alves do Nascimento, Letícia
name: GONÇALVES ROCHA, RONILSON
name: Oliveira de Araújo, Williana
Publisher: name: Zenodo
Year: 2025

description: O projeto de  Extensão Universitária ¨Prevenção de riscos de tromboembolismo venoso: ações e estratégias para redução da morbimortalidade e aumento da segurança do paciente em ambientes de atenção à saúde¨, criou diversos materiais para prevenção e capacitação para diversos encontros em eventos. Dentre os materias criados para os eventos, estão os seguintes: 

Folder educativo sobre TEV com informações detalhadas sobre a doença e seus fatores de risco;

Banner de divulgação do Projeto TEV para eventos;

Apostila de treinamento sobre TEV;

Fichas clínica pré-teste e pós-teste sobre o conhecimento de profissionais de saúde sobre riscos de TEV, formas de prevenção e aplicativos usados na estratificação de riscos.
Perturbative approach to the astrometric microlensing due to an extrasolar planet
Creators: name: Asada, Hideki
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have developed a perturbative approach to microlensing due to an extrasolar planetary lens. In particular, we have found analytic formulae for triple images. We have used the formulae to investigate the astrometric microlensing due to the extrasolar planetary lens, in expectation of dramatic improvements in the precision of the future astrometric measurements. For a weak lensing case, we have shown how the maximum angular size and the typical time scale of the anomalous shift of the lightcentroid are dependent on the mass ratio and angular separation between the star and the planet.
description: 11 pages (LaTeX); accepted for publication in Astrophys. J
Addendum: "The Dynamics of M15: Observations of the Velocity Dispersion Profile and Fokker-Planck Models" (ApJ, 481, 267 [1997])
Creators: name: Dull, J. D.
name: Cohn, H. N.
name: Lugger, P. M.
name: Murphy, B. W.
name: Seitzer, P. O.
name: Callanan, P. J.
name: Rutten, R. G. M.
name: Charles, P. A.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: It has recently come to our attention that there are axis scale errors in three of the figures of Dull et al. (1997, hereafter D97). D97 presented Fokker-Planck models for the collapsed-core globular cluster M15 that include a dense, centrally concentrated population of neutron stars and massive white dwarfs, but do not include a central black hole. In this Addendum, we present corrected versions of Figures 9, 10, and 12, and an expanded version of Figure 6. This latter figure, which shows the full run of the velocity dispersion profile, indicates that the D97 model predictions are in good agreement with the moderately rising HST-STIS velocity dispersion profile for M15 reported by Gerssen et al. (2002, astro-ph/0209315). Thus, a central black hole is not required to fit the new STIS velocity measurements, provided that there is a sufficient population of neutron stars and massive white dwarfs. This conclusion is consistent with the findings of Gerssen et al. (2002, astro-ph/0210158), based on a reapplication of their Jeans equation analysis using the corrected mass-to-light profile (Figure 12) for the D97 models.
description: 4 pages, 4 figures, submitted to ApJ
NMR relaxation in the spin-1 Heisenberg chain
Creators: name: Capponi, Sylvain
name: Dupont, Maxime
name: Sandvik, Anders W.
name: Sengupta, Pinaki
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We consider the isotropic $S=1$ Heisenberg chain with a finite Haldane gap $Δ$ and use state-of-the-art numerical techniques to investigate its dynamical properties at finite temperature, focusing on the nuclear spin-lattice relaxation rate $1/T_1$ measured in nuclear magnetic resonance (NMR) experiments for instance. In particular, we analyze the contributions from modes with momenta close to $q\approx 0$ and $q\approx π$ as a function of temperature. At high-temperature, we observe spin diffusion with a non-trivial exponent. At low-temperature, we argue that a simple activated behavior $1/T_1 \propto\exp(-Δ/T)$ can only be observed at temperatures much smaller than the gap $Δ$.
description: published version
Atomic Physics with the Goddard High Resolution Spectrograph on the Hubble Space Telescope. V. Oscillator Strengths for Neutral Carbon Lines below 1200 Angstrom
Creators: name: Federman, S. R.
name: Zsargo, J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyzed high resolution spectra of interstellar neutral carbon absorption toward $λ$ Ori, 1 Sco, and $δ$ Sco that were obtained with the Goddard High Resolution Spectrograph on the Hubble Space Telescope. Several multiplets were detected within the wavelength interval 1150 to 1200 A, where most neutral carbon lines have ill-defined oscillator strength; multiplets at longer wavelengths with well-defined atomic parameters were also seen. We extracted accurate column densities and Doppler parameters from lines with precise laboratory-based f-values. These column densities and b-values were used to obtain a self-consistent set of f-values for all the observed neutral carbon lines. For many of the lines with wavelength below 1200 A, the derived f-values differ appreciably from the values quoted in the compilation by Morton (1991). The present set of f-values extends and in some cases supersedes those given in Zsargo et al. (1997), which were based on lower resolution data.
description: 8 pages, 2 figures, 6 tables, accepted for publication in ApJ
Coelogyne pyrranthela M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne pyrranthela

description: Coelogyne pyrranthela (Gagnep.) M.W.Chase & Schuit., comb. nov.
 Basionym: Pholidota pyrranthela Gagnep., Bull. Mus. Natl. Hist. Nat., sér. 2, 22: 507 (1950).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 124, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
Ultraviolet Broad Absorption Features and the Spectral Energy Distribution of the QSO PG 1351+64
Creators: name: Zheng, W.
name: Kriss, G. A.
name: Wang, J. X.
name: Brotherton, M.
name: Oegerle, W. R.
name: Blair, W. P.
name: Davidsen, A. F.
name: Green, R. F.
name: Hutchings, J. B.
name: Kaiser, M. E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a moderate-resolution (~20 km/s) spectrum of the mini broad-absorption-line QSO PG1351+64 between 915-1180 A, obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE). Additional spectra at longer wavelengths were also obtained with the HST and ground-based telescopes. Broad absorption is present on the blue wings of CIII 977, Ly-beta, OVI 1032,1038, Ly-alpha, NV 1238,1242, SiIV 1393,1402, and CIV 1548,1450. The absorption profile can be fitted with five components at velocities of ~ -780, -1049, -1629, -1833, and -3054 km/s with respect to the emission-line redshift of z = 0.088. All the absorption components cover a large fraction of the continuum source as well as the broad-line region. The OVI emission feature is very weak, and the OVI/Lyalpha flux ratio is 0.08, one of the lowest among low-redshift active galaxies and QSOs. The UV continuum shows a significant change in slope near 1050 A in the restframe. The steeper continuum shortward of the Lyman limit extrapolates well to the observed weak X-ray flux level. The absorbers' properties are similar to those of high-redshift broad absorption-line QSOs. The derived total column density of the UV absorbers is on the order of 10^21 cm^-2, unlikely to produce significant opacity above 1 keV in the X-ray. Unless there is a separate, high-ionization X-ray absorber, the QSO's weak X-ray flux may be intrinsic. The ionization level of the absorbing components is comparable to that anticipated in the broad-line region, therefore the absorbers may be related to broad-line clouds along the line of sight.
description: 23 pages, Latex, 5 figures
Antepipona mucronata
Creators: name: Gusenleitner, J.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eumenidae
Antepipona
Antepipona mucronata

description: Antepipona mucronata (DE SAUSSURE 1862)
C e n t r a l A f r i c a n R e p u b l i k: 60 km SE Bouar, 660m, 5°45’E 15°13’N, 23.3.201 0, 2; 860m, 30.3.201 0, 1, leg. J. Halada, coll. OLM.
Aus diesem Staat wurde diese Art bisher nicht gemeldet (CARPENTER et al. 2009).
U g a n d a: 1 km südl. Budibugyo, am Kyemahizi, 0°40’12’’N 30°02’06’’E, 920m, 19.3.201 2, 1, 2, leg. et coll.Oehlke.
description: Published as part of Gusenleitner, J., 2012, Über bemerkenswerte Faltenwespen aus der äthiopischen Region Teil 9 (Hymenoptera: Vespidae: Eumeninae), pp. 1159-1176 in Linzer biologische Beiträge 44 (2) on page 1167, DOI: 10.5281/zenodo.5329007
Matrix Gla protein regulates adipogenesis and is serum marker of visceral adiposity
Creators: name: Li, Chaomin
name: Li, Jing
name: He, Fang
name: Li, Kun
name: Li, Xu
name: Zhang, Yan
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Computational Biology

description: Objective Matrix Gla protein (MGP) is a potent calcification inhibitor. Mgp-/- mice display increased proportion of brown adipose tissue. However, whether MGP is involved in fat metabolism remains unclear. This study aims to investigate the involvement. Methods Expression of adipocyte differentiation markers was examined by RT-qPCR. Adipocyte formation was assessed by Oil Red staining. Serum triglyceride, cholesterol, and desphosphorylated-uncarboxylated MGP (dp-ucMGP) were quantified by ELISA. Visceral fat was detected by bioelectrical impedance analysis. Results MGP is highly expressed in visceral fat. MGP expression is induced during preadipocyte differentiation. Knockout of MGP leads to retardation of 3T3-L1 differentiation. Intracellular triglyceride amount is impaired while glycerol release is increased in MGP-depleted cells. Serum dp-ucMGP level is significantly increased in individual with higher visceral fat index (VFI) and waist height ratio (WHtR), but not body mass index (BMI). Additionally, dp-ucMGP positively correlates to low-density lipoprotein cholesterol (LDL-C) level. Conclusions MGP is involved in fat metabolism and serum inactive MGP level is associated with visceral fat. Our study uncovers for the first time the link between MGP and fat metabolism, and sheds light on the potential of dp-ucMGP as a novel serum marker.
A Search for Water Maser Emission in Southern AGN and Star Forming Galaxies -- Discovery of a Maser in the Edge-on Galaxy IRASF01063-8034
Creators: name: Greenhill, L. J.
name: Ellingsen, S. P.
name: Norris, R. P.
name: McGregor, P. J.
name: Gough, R. G.
name: Sinclair, M. W.
name: Rayner, D. P.
name: Phillips, C. J.
name: Herrnstein, J. R.
name: Moran, J. M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the cumulative results of five surveys for water maser emission at 1.35 cm wavelength in 131 active galactic nuclei (AGNs) and star-forming galaxies, conducted at the Parkes Observatory between 1993 and 1998. We detected one new maser, in the edge-on galaxy IRASF01063-8034, which exhibits a single, about 0.1 Jy spectral feature at 4282+/-6 km/s (heliocentric) with an unusually large 54+/-16 km/s half-power full width. The centroid velocity of the emission increased to 4319.6+/-0.6 km/s (38+/-2 km/s width) over the 13 days between discovery and confirmation of the detection. A similarly broad linewidth and large change in velocity has been noted for the maser in NGC1052, wherein jet activity excites the emission. Neither optical spectroscopy, radio-infrared correlations, nor infrared colors provide compelling evidence of unusual activity in the nucleus of IRASF01063-8034. Since the galaxy appears to be outwardly normal at optical and infrared wavelengths, detection of a water maser therein is unique. The maser emission is evidence that the galaxy harbors an AGN that is probably obscured by the edge-on galactic disk. The detection highlights the possibility that undetected AGNs could be hidden in other relatively nearby galaxies. No other maser emission features have been identified at velocities between 3084 km/s and 6181 km/s.
description: To appear in The Astrophysical Journal, 2002 Jan. 20. 29 pages, 6 figures, 3 tables
title: The influence of contextual factors on short-term post-exercise muscle glycogen replenishment: a focus on sleep
Creators: name: Craven, Jonathan D
Publisher: name: Griffith University
Year: 2023
Subjects: subject: muscle glycogen
subject: short-term recovery
subject: post-exercise
subject: sleep

description: AIM: The aim of this thesis was to gain a deeper understanding of the influence contextual factors have on short-term post-exercise muscle glycogen replenishment, with a specific focus on the influence of sleep and its subsequent impact on next day exercise performance. The thesis comprises two studies that are systematic and meta-analytical reviews and one experimental, empirical study. Study 1 was a systematic and meta-analytical review aimed to explore the effect of consuming carbohydrate (CHO) with and without protein (PRO) on the rate of muscle glycogen re-synthesis during short-term post-exercise recovery (less than or equal to 8h), while considering contextual factors (e.g., CHO- dose, timing). [...] Study 2 was a systematic and meta-analytical review aimed to explore the magnitude of influence acute sleep loss has on next day exercise performance, while considering key contextual factors (e.g., sleep loss protocol used, exercise type (e.g., strength, endurance) and the time of day exercise is performed). [...]
Retention in clinical trials after prison release: results from a clinical trial with incarcerated men with HIV and opioid dependence in Malaysia
Creators: name: Chandra, Divya K.
name: Bazazi, Alexander R.
name: Muzammil A. Nahaboo Solim
name: Adeeba Kamarulzaman
name: Altice, Frederick L.
name: Culbert, Gabriel J.
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences
subject: Computational Biology

description: Background: Study retention is a major challenge in HIV clinical trials conducted with persons recruited from correctional facilities. Objective: To examine study retention in a trial of within-prison methadone initiation and a behavioral intervention among incarcerated men with HIV and opioid dependence in Malaysia. Methods: In this 2x2 factorial trial, 296 incarcerated men with HIV and opioid dependence were allocated to (1) an HIV risk reduction intervention, the Holistic Health Recovery Program for Malaysia (HHRP-M), (2) pre-release methadone initiation, (3) both interventions, or (4) standard care (NCT02396979). Here we estimate effects of these interventions on linkage to the study after prison release and completion of post-release study visits. Results: Most participants (68.9%) completed at least one post-release study visit but few (18.6%) completed all 12. HHRP-M was associated with a 13.5% (95% confidence interval (CI): 3.8%, 23.2%) increased probability of completing at least one post-release study visit. Although not associated with initial linkage, methadone treatment was associated with an 11% (95% CI: 2.0%, 20.6%) increased probability of completing all twelve post-release study visits. Being subject to forced relocation outside Kuala Lumpur after prison release decreased retention by 43.3% (95% CI: −51.9%, −34.8%). Conclusion: Retaining study participants in HIV clinical trials following prison release is challenging and potentially related to the broader challenges that participants experience during community reentry. Researchers conducting clinical trials with this population may want to consider methadone and HHRP as means to improve post-release retention, even in clinical trials where these interventions are not being directly evaluated.
title: All Fade Away: Death, Grief and Loss: An Exploration on How Sculptural Installation can Trigger an Empathic Engagement.
Creators: name: Sanstrom, Brian
Publisher: name: Griffith University
Year: 2016
Subjects: subject: Symbolic imagery
subject: Sculptural installation
subject: Loss (Emotion)

description: This exegetical study considers how the experience of death, grief, and, in particular, loss can be considered through symbolic imagery and sculptural installation. I surveyed academic writing on these emotions and experiences as well as artists’ visual responses to them. My research has at its starting point the death of my marriage, and the surrounding feelings of grief and loss. My built structures or sculptural installation reference the body in situ, absent, and in its corporeal decline leading to death. All three states become dominant metaphors that symbolise trauma, grief, loss, separation, and fear. I discovered that loss triggers emotions that dismantle the way in which one perceives the link between past, present, and future relationships. In other words, loss has the ability to destroy a sense of order, logic, and continuity in one’s life and to deconstruct existing belief structures. As an individual, major loss is generally associated with the death of a family member or close friend. The intensity of grief experienced by the individual is related to the intensity of the personal involvement. This study questions how my art practice can effectively communicate notions of death, grief, and loss, and, in so doing, seeks to show how human experience can be re-contextualised into a physical form.
Does the Slim-Disk Model Correctly Consider Photon-Trapping Effects?
Creators: name: Ohsuga, Ken
name: Mineshige, Shin
name: Mori, Masao
name: Umemura, Masayuki
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the photon-trapping effects in the super-critical black hole accretion flows by solving radiation transfer as well as the energy equations of radiation and gas. It is found that the slim-disk model generally overestimates the luminosity of the disk at around the Eddington luminosity (L_E) and is not accurate in describing the effective temperature profile, since it neglects time delay between energy generation at deeper inside the disk and energy release at the surface. Especially, the photon-trapping effects are appreciable even below L ~ L_E, while they appear above ~ 3L_E according to the slim disk. Through the photon-trapping effects, the luminosity is reduced and the effective temperature profile becomes flatter than r^{-3/4} as in the standard disk. In the case that the viscous heating is effective only around the equatorial plane, the luminosity is kept around the Eddington luminosity even at very large mass accretion rate, Mdot>>L_E/c^2. The effective temperature profile is almost flat, and the maximum temperature decreases in accordance with rise in the mass accretion rate. Thus, the most luminous radius shifts to the outer region when Mdot/(L_E/c^2) >> 10^2. In the case that the energy is dissipated equally at any heights, the resultant luminosity is somewhat larger than in the former case, but the energy-conversion efficiency still decreases with increase of the mass accretion rate, as well. The most luminous radius stays around the inner edge of the disk in the latter case. Hence, the effective temperature profile is sensitive to the vertical distribution of energy production rates, so is the spectral shape. Future observations of high L/L_E objects will be able to test our model.
description: 10 pages, 7 figures, accepted for publication in ApJ
title: Material Determinism and Beyond
title: Spatial Categories in the Study of Violent Conflict
titleType: Subtitle
Creators: name: Chojnacki, Sven
name: Engels, Bettina
Publisher: name: Freie Universität Berlin
Year: 2013
Subjects: subject: 300 Sozialwissenschaften::360 Soziale Probleme, Sozialdienste::363 Andere soziale Probleme und Sozialdienste

description: This paper reviews recent debates in peace and conflict studies on the theoretical and empirical integration of spatial categories. We examine three notable strands of research. The first consists of studies that analyze the influence of topography, borders, and resource availability on the occurrence of international and intra-state war. The second strand comprises recent studies in civil war research focusing on territory and territorial control. The third strand is the debate on so-called environmental conflicts. We argue that most studies in all three fields are limited to the analysis of allegedly external material influences on violent conflict, failing to take into account the social and political meaning of physical materiality. We examine how recent research methodologically deals with interrelated scales (local, national, global). We argue that an analysis of the relationship between space and conflict should encompass both the materiality of space and its social meaning, and that these two aspects find themselves in a mutually constitutive relationship. Spatial theory therefore provides a useful approach.
description: Dieser Beitrag untersucht, wie Raumkategorien theoretisch und empirisch in der Friedens- und Konfliktforschung verwandt werden. Im Mittelpunkt stehen dabei drei Forschungsstränge: erstens Arbeiten zum Einfluss topographischer Faktoren, von Grenzen sowie Ressourcenvorkommen auf das Auftreten internationaler und innerstaatlicher Kriege; zweitens Studien aus dem Bereich der Bürgerkriegsforschung zu Territorium und territorialer Kontrolle; und drittens die so genannte Umweltkonfliktforschung. Festzustellen ist, dass die meisten Arbeiten sich auf die Analyse vermeintlich externer materieller Einflüsse auf Gewaltkonflikte beschränken und dabei die soziale und politische Bedeutung der physischen Materialität außer Acht lassen. Wir argumentieren, dass demgegenüber die Analyse des Verhältnisses von Raum und Konflikt zugleich die Materialität von Raum und ihre soziale Besetzung umfassen sollte, und dass beide sich wechselseitig konstitutiv aufeinander beziehen. Für eine solche Analyse stellt die sozialwissenschaftliche Raumtheorie hilfreiche Kategorien bereit.
title: Enhancing musical practice and performance in a variety of contexts: An autoethnographic investigation
Creators: name: Shipard, Rachael Catherine Lee
Publisher: name: Griffith University
Year: 2019
Subjects: subject: Musical practice
subject: Performance
subject: Autoethnographic investigation
subject: Mental and physical preparation
subject: Pre-performance routines

description: This research project involved an autoethnographic investigation of strategies that can improve practice and pre-performance routines. Although much research has already been conducted in the area of optimal performance (Wrigley & Emmerson, 2011; Freedman, 2015; Groth, 2016; Csikszentmihalyi, 1990), this study is conducted from my own personal viewpoint as a young classical pianist, to improve the reliability and consistency of my performances, and enhance my satisfaction with them.
A Primordial Origin of the Laplace Relation Among the Galilean Satellites
Creators: name: Peale, S. J.
name: Lee, Man Hoi
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Understanding the origin of the orbital resonances of the Galilean satellites of Jupiter will constrain the longevity of the extensive volcanism on Io, may explain a liquid ocean on Europa, and may guide studies of the dissipative properties of stars and Jupiter-like planets. The differential migration of the newly formed Galilean satellites due to interactions with a circumjovian disk can lead to the primordial formation of the Laplace relation n_1 - 3 n_2 + 2 n_3 = 0, where the n_i are the mean orbital angular velocities of Io, Europa, and Ganymede, respectively. This contrasts with the formation of the resonances by differential expansion of the orbits from tidal torques from Jupiter.
description: 13 pages, including 4 figures; uses scicite.sty
title: Parental Concerns about Children’s Independent Mobility in Australian Cities
Creators: name: Moghtaderi Esfahani, Farinaz
Publisher: name: Griffith University
Year: 2016
Subjects: subject: iMATCH (independent Mobility, Active Travel and Children’s Health) Project
subject: Children's mobility
subject: Independent mobility, Children
subject: Children's physical health
subject: Children's exercise

description: In countries such as Australia, children's active and independent mobility has declined in the past 40 years, with less children walking to school. As physical activity is a key component of child health and well-being this decrease in children’s independent mobility (CIM) and active travel (AT) has placed children at greater risk of physical and mental health problems. To confront this problem, travel behaviour change interventions to promote active and independent school travel are currently deployed in Australia by local and state governments. To date there have been few comprehensive studies of these interventions and in particular, whether and how they relate to contemporary parental attitudes and perceptions about CIM. There remain significant research gaps about the relative importance of travel behaviour change programs in parental decision-making processes. As part of the larger iMATCH (independent Mobility, Active Travel and Children’s Health) Project this research sought to identify the range of current interventions being used in Australia, the attitudes and perceptions of parents and guardians in a range of urban environments across the country, and to explore how interventions may better respond to these concerns to increase their effectiveness. A theoretical framework based on Azjen’s (1988) Theory of Planned Behaviour (TPB) and the Trans- theoretical model of behaviour change (TTM) was developed to guide the research. The suggested theoretical model was examined by adopting the structural equation modelling (SEM). The valid and reliable model was introduced regarding evaluating, designing, and running travel behaviour change interventions. This model was employed as a fundamental structure for guiling the research process. Interventions used in Australia were examined firstly using published project evaluations, websites and other reports, with attention given to their treatment of CIM and their efficacy. The broader iMATCH study used child and parent surveys and travel diaries, amongst other methods, collected from schools in nine neighbourhoods in Perth, Melbourne, Brisbane and Rockhampton. Responses provided in 309 parent surveys were examined in detail. A total of nine parents from two schools in Brisbane and one in Ipswich that were part of the broader study were then recruited for either a focus group discussion or a face-to-face interview, eliciting further detail on their attitudes.
Power Spectra for Galaxy Shape Correlations
Creators: name: Mackey, Jonathan
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: It has recently been argued that the observed ellipticities of galaxies may be determined at least in part by the primordial tidal gravitational field in which the galaxy formed. Long-range correlations in the tidal field could thus lead to an ellipticity-ellipticity correlation for widely separated galaxies. I present results of a calculation of the angular power spectrum of intrinsic galaxy shape correlations using a new model relating ellipticity to angular momentum. I show that for low redshift galaxy surveys, the model predicts that intrinsic correlations will dominate correlations induced by weak lensing, in good agreement with previous theoretical work and observations. The model also produces `E-mode' correlations enhanced by a factor of 3.5 over `B-modes' on small scales, making it harder to disentangle intrinsic correlations from weak lensing.
description: 4 pages, 1 figure. in ``The Shapes of Galaxies and Their Dark Halos,'' Yale Cosmology Workshop, Ed. P. Natarajan (New Haven CT, May 2001). Revised web version corrects lensing curve normalisation in fig.1; text as published
Mode of action for a new potential fungicide candidate, 3-(4-Methyl-1,2,3-thiadiazolyl)-6-trichloromethyl-[1,2,4]-triazolo-[3,4-b][1,3,4]-thiadiazole by iTRAQ
Creators: name: Zhao, Bin
name: Wang, Haixia
name: Fan, Zhijin
name: Wu, Qifan
name: Guo, Xiaofeng
name: Zhang, Nailou
name: Yang, Dongyan
name: Yu, Bin
name: Zhou, Shuang
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified

description: The mode of action is the basis for the rational design of the novel agrochemicals. 3-(4-Methyl-1,2,3-thiadiazolyl)-6-trichloromethyl [1,2,4]triazolo [3,4-b][1,3,4]thiadiazole (YZK-C22) is a novel fungicide candidate. The aim of this study was identification of the mechanism of YZK-C22 against fungi. The results indicated that YZK-C22 inhibited the mycelial growth and spore germination of Botrytis cinerea. Total 56 differentially expressed proteins (DEPs) including 27 up regulated and 29 down regulated proteins were identified by isobaric tags for relative and absolute quantification (iTRAQ). The DEPs mainly concentrated on metabolic pathways, and the results were consistent across the studies of RNA and protein platforms. The pyruvate kinase (PK) activity in the glycolytic pathway was inhibited over 50% by 20 μg/mL of YZK-C22. Molecular docking analysis also validated that YZK-C22 could dock into the active centre of the PK instead of phosphoenolpyruvate. In summary, iTRAQ was an effective way for target identification of YZK-C22.
The Evolution of Stellar Populations
Creators: name: Diaz, Angeles
name: Hardy, Eduardo
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We summarize the discussion section on ``Evolution of Stellar Populations'' we led on May 27, 2000 in Granada, Spain, as part of the Euroconference on The Evolution of Galaxies. I- Observational Clues. We also provide a partial comparison between the present knowledge of these topics and that which existed at the time of the Crete Conference of 1995.
description: 10 pages, no figures, To appear in Proceedings of First Euroconference "The Evolution of Galaxies. I-Observational Clues" (Astrophys. & Sp. Sc., Vilchez, Stasinska, and Perez, eds. Kluwer)
Antepipona pakasae
Creators: name: Gusenleitner, J.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eumenidae
Antepipona
Antepipona pakasae

description: Antepipona pakasae (MEADE- WALDO 1915)
K e n i a: E of Mwingi, 14.5.200 7, 1, leg. M. Halada, coll. OLM.
Aus Kenia war diese Art bisher nicht bekannt (CARPENTER et al. 2009).
description: Published as part of Gusenleitner, J., 2012, Über bemerkenswerte Faltenwespen aus der äthiopischen Region Teil 9 (Hymenoptera: Vespidae: Eumeninae), pp. 1159-1176 in Linzer biologische Beiträge 44 (2) on page 1167, DOI: 10.5281/zenodo.5329007
title: Assimilative and Accommodative Resources in Young Adults
Creators: name: Haratsis, Jessica Megan
Publisher: name: Griffith University
Year: 2015
Subjects: subject: Assimilative resources
subject: Accommodative resources
subject: Career goal attainability
subject: LIfe satisfaction

description: The aims of the research program were: (a) to develop and validate new measures to assess assimilative and accommodative resources (cf. Brandtstädter & Rothermund, 2002) in young adults (Study 1), (b) to test the cross-sectional associations among assimilation and accommodation, career goal appraisals and attitudes, career goal engagement and disengagement, and life satisfaction (Study 2), and (c) to investigate the cross-lagged relationships between assimilation and accommodation, career goal attainability and optimism, and well-being over time (Study 3). The studies were informed by the dual-process framework (Brandtstädter & Rothermund, 2002) and are reported as three journal articles that have been accepted for publication in international, peer reviewed journals. In Study 1, new scales were developed and validated to measure assimilative and accommodative resources in young adults. Existing scales demonstrated poor validity and were developed for use with middle aged to older adults. Experts reviewed the content validity of the two existing measures (Tenacious Goal Pursuit and Flexible Goal Adjustment Scales; Brandtstädter & Renner, 1990) to identify items that could be modelled for the new scales. New items were generated, then refined by an expert panel and focus groups of young adults.
Coelogyne quadricarinata M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne quadricarinata

description: Coelogyne quadricarinata (Shih C.Hsu, Gravend. & de Vogel) M.W.Chase & Schuit., comb. nov.
 Basionym: Geesinkorchis quadricarinata Shih C.Hsu, Gravend. & de Vogel, Blumea 50: 513 (2005).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 124, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
HD 209458: Physical Parameters of the Parent Star and the Transiting Planet
Creators: name: Cody, A.
name: Sasselov, Dimitar D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Sun-like star HD209458 harbors a close-in giant planet which transits across the star's disk, and thus allows an unprecedented access to the basic parameters of the planet, given a certain knowledge of the basic parameters of the star, namely its mass and radius. We present theoretical stellar evolution model calculations for HD 209458 and discuss the uncertainties involved in deriving the stellar mass and radius. We derive the mass, M=1.06 Msun, radius, R=1.18 Rsun,and age, t=5.2 Gyr of the star with uncertainties of 10% or more. The dominant sources of uncertainty remain to be the helium abundance estimate and the treatment of convection, even after an optimistic estimate for the effective temperature of the star. However, we find that in deriving the radius of the planet, R_p, the relevant stellar model input is the M/R relation, which runs orthogonal to a degeneracy in the transit light curve solution and greatly improves the estimate of R_p. Theoretically the M/R relation has a lower uncertainty than the M and R separately. We estimate the planet radius and mass to be R_p =1.42 +0.10/-0.13 R_J and M_p =0.69 +/- 0.02 M_J.
description: 24 pages, 5 figures, accepted by the Astrophysical Journal; added correct version of figure 5 and fixed references
Traveling band formation in feedback-driven colloids
Creators: name: Tarama, Sonja
name: Egelhaaf, Stefan U.
name: Löwen, Hartmut
Publisher: name: arXiv
Year: 2019
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: FOS: Physical sciences

description: Using simulation and theory we study the dynamics of a colloidal suspension in two dimensions subject to a time-delayed repulsive feedback that depends on the positions of the colloidal particles. The colloidal particles experience an additional potential that is a superposition of repulsive potential energies centered around the positions of all the particles a delay time ago. Here we show that such a feedback leads to self-organization of the particles into traveling bands. The width of the bands and their propagation speed can be tuned by the delay time and the range of the imposed repulsive potential. The emerging traveling band behavior is observed in Brownian dynamics computer simulations as well as microscopic dynamic density functional theory (DDFT). Traveling band formation also persists in systems of finite size leading, in the case of circularly confined systems, to rotating traveling waves.
description: 15 pages, 13 figures; Results unchanged, Section IV has been modified to connect the theory to previous one-particle studies. The final version of the article can be found at: https://journals.aps.org/pre/abstract/10.1103/PhysRevE.100.022609 \copyright 2019 American Physical Society
A Globular Cluster Metallicity Scale Based on the Abundance of Fe II
Creators: name: Kraft, Robert P.
name: Ivans, Inese I.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Assuming that in the atmospheres of low-mass, metal-poor red giant stars, 1-D models based on LTE accurately predict the abundance of iron from Fe II, we derive a globular cluster metallicity scale based on the equivalent widths of Fe II lines measured from high resolution spectra of giants in 16 key clusters lying in the abundance range -2.4 < [Fe/H]II < -0.7. We base the scale largely on the analysis of spectra of 149 giant stars in 11 clusters by the Lick-Texas group supplemented by high-resolution studies of giants in five other clusters. We also derive ab initio the true distance moduli for M5, M3, M13, M92, and M15 as a means of setting stellar surface gravities. We find that [Fe/H]II is correlated linearly with , the reduced strength of the near infra-red Ca II triplet defined by Rutledge et al, although the actual correlation coefficients depend on the atmospheric model employed. We also discuss how to estimate [X/Fe]-ratios. We suggest that C, N, and O, as well as elements appearing in the spectrum in the singly ionized state, e.g., Ti, Sc, Ba, La and Eu, should be normalized to the abundance of Fe II. Other elements, which appear mostly in the neutral state, but for which the dominant species is nevertheless the ionized state, are probably best normalized to Fe I, but uncertainties remain.
description: 23 pages + appendix + 4 figures + 17 tables = 61 pages; accepted by PASP
title: Integration of the Peripheral and Central Nervous System During Development of the Murine Olfactory Nerve
Creators: name: Amaya, Daniel Alejandro
Publisher: name: Griffith University
Year: 2016
Subjects: subject: Murine olfactory nerve
subject: Neurodegenerative diseases
subject: Spinal cord injuries
subject: Olfactory ensheathing cells
subject: Radial glia

description: The need to develop therapies for neurodegenerative diseases and spinal cord injuries has led researchers to study the primary olfactory system, as it continuously renews itself throughout life, and completely regenerates after injury. A pool of cells that line the basal surface of the olfactory epithelium gives rise to new olfactory neurons both during normal olfactory nervous system turnover and to a greater extent following injury. The unique, growth promoting olfactory system environment is crucial for this neurogenesis and regeneration. Significantly glial scarring (as is typically seen in neurodegeneration and neural damage elsewhere in the nervous system) is largely absent following injury to the olfactory tract. Thus replicating the favourable condition in the olfactory nervous system would be invaluable for developing these successful therapies. If we can mimic the cellular and molecular mechanisms responsible for maintenance andregeneration of the olfactory neurons, we can promote regeneration and facilitate the reestablishment of connectivity in damaged neural tracts. To model neural regeneratio n strategies in the olfactory nervous system we need to understand the normal olfactory system biology.