cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Self-Regulation and Wisdom in Relationship Satisfaction
Creators: name: Charker, Jillian H
Publisher: name: Griffith University
Year: 2003
Subjects: subject: relationships
subject: relationship self-regulation
subject: relationship effort
subject: relationship satisfaction
subject: couples
subject: couple relationships

description: This thesis describes a program of research which aimed to explore the role of relationship self-regulation (or relationship "effort") and wisdom in relationship satisfaction. Three separate studies were conducted to examine the association between self-regulation and satisfaction, and the mechanisms for this association. Study 1 examined self-regulation, wisdom and satisfaction, using a sample of 61 couples in long-term relationships, and found that while wisdom shared little association with satisfaction, self-regulation was a significant correlate of satisfaction for men and women. Study 2 examined whether the association between self-regulation and satisfaction was mediated by communication skills in a sample of 101 couples in the early stages of their relationship. Results replicated the self-regulation/satisfaction association found in Study 1, but provided no evidence for mediation by communication. Study 3 tested for mediation of the self-regulation/satisfaction association by attributions in a sample of 73 newly-wed couples. The association between self-regulation and satisfaction was partially mediated by attributions, but self-regulation also had a direct relationship with satisfaction. It was concluded that self-regulation is an important correlate of satisfaction in relationships, and that this association cannot be fully explained by communication or attributions. Several directions for future research were provided, including the need to examine self-regulation and its predictors longitudinally, ways in which a behavioural measure of self-regulation could be developed, and the implications of self-regulation for couple therapy.
Additional file 1 of A 5′-tRNA halve, tiRNA-Gly promotes cell proliferation and migration via binding to RBM17 and inducing alternative splicing in papillary thyroid cancer
Creators: name: Han, Litao
name: Lai, Hejing
name: Yang, Yichen
name: Hu, Jiaqian
name: Li, Zhe
name: Ma, Ben
name: Xu, Weibo
name: Liu, Wanlin
name: Wei, Wenjun
name: Li, Duanshu
name: Wang, Yu
name: Zhai, Qiwei
name: Ji, Qinghai
name: Liao, Tian
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1.
Synagris rubescens
Creators: name: Dvo, L.
name: M, J.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eumenidae
Synagris
Synagris rubescens

description: Synagris rubescens (GIORDANI SOIKA 1989)
M a t e r i a l: Sukhnah, NE Al Mansuriah, N=14°50’, E=43°31’, 774 m, 8.4.2007, 1.
GIORDANI SOIKA (1989) reported 1 and 1 from Yemen, 1 from Saudi Arabia, and WAHIS (2000) 1 from Yemen. This is the fifth known specimen.
description: Published as part of Dvo, L. & M, J., 2010, New records of vespid wasps from Yemen with synonymy in Belonogaster (Hymenoptera: Vespidae: Polistinae and Eumeninae), pp. 561-563 in Linzer biologische Beiträge 42 (1) on page 562, DOI: 10.5281/zenodo.5332555
A New Algorithm for Radiative Feedback and its Application to the Formation of Massive Stars
Creators: name: Edgar, R. G.
name: Clarke, C. J.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have developed a simplified method of treating the radiative acceleration of dusty flows. This method retains the sharp impulse at the dust destruction radius that is a feature of frequency dependent radiative transfer, whilst placing minimal demands on computing resources. As such, it is suitable for inclusion in hydrodynamic codes. We have applied this method to the formation of massive stars in spherical geometry, and find that the fraction of a cloud which can accrete on to the central star is a strong function of the Jeans' Number and density profile of the cloud. Massive star formation is favoured by cold homogeneous conditions, as might result in regions where gas is swept up by some external triggering agent. We find (in contrast to previous authors) that massive star formation does not require a depleted dust mixture, although the use of dust at typical interstellar abundances does reduce the final stellar mass compared to cores formed from a depleted mixture.
description: 12 pages, 12 figures Accepted by MNRAS
Observations of r- and s-process elements in Population II stars
Creators: name: Ryan, Sean G.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The framework for the interpretation of neutron-capture elements observed in Population II stars, established 20-25 years ago, is that these stars primarily exhibit r-process signatures, due to the inefficiency of the s-process at low metallicity. A view developed later that the r-process might be universal, which is to say that the same r-process element ratios would exist at high and low metallicity. However, observations of s-process abundances in low-metallicity environments, and departures from a universal r-process ratio for the lightest neutron-capture elements have required revisions to the framework. Observations indicating the need for and nature of these changes will be presented.
description: 8 pages, 2 figures Conference paper: Nuclei in the Cosmos VII, Fuji-Yoshida, 8-12 July 2002
Spin-$S$ designer hamiltonians and the square lattice $S=1$ Haldane nematic
Creators: name: Desai, Nisheeta
name: Kaul, Ribhu K.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We introduce a strategy to write down lattice models of spin rotational symmetric Hamiltonians with arbitrary spin-$S$ that are Marshall positive and can be simulated efficiently using world line Monte Carlo methods. As an application of our approach we consider a square lattice $S=1$ model for which we design a $3\times 3$ - spin plaquette interaction. By numerical simulations we establish that our model realizes a novel "Haldane nematic" phase that breaks lattice rotational symmetry by the spontaneous formation of Haldane chains, while preserving spin rotations, time reversal and lattice translations. By supplementing our model with a two-spin Heisenberg interaction, we present a study of the transition between Néel and Haldane nematic phase, which we find to be of first order.
Additional file 1 of Chemotherapy in the treatment of different histological types of appendiceal cancers: a SEER based study
Creators: name: Wang, Gang
name: Li, Qiken
name: Chen, Weiping
Publisher: name: figshare
Year: 2021
Subjects: subject: Cell Biology
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer

description: Additional file 1: Table S1. Risk factors associated with cancer-specific and overall survival for all appendiceal patients diagnosed during 1998–2011. Table S2. Risk factors correlated with overall survival in patients with NECs or NETs appendiceal cancer. Fig. S1. Effect of chemotherapy on cancer specific and overall survival curves in all patients with appendiceal cancer during different period. (A) Cancer specific survival (1998–2011). (B) Overall survival (1998–2011). (c) Cancer specific survival (2012–2016). (B) Overall survival (2012–2016).
Anomalous Topological Active Matter
Creators: name: Sone, Kazuki
name: Ashida, Yuto
Publisher: name: arXiv
Year: 2019
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Active systems exhibit spontaneous flows induced by self-propulsion of microscopic constituents and can reach a nonequilibrium steady state without an external drive. Constructing the analogy between the quantum anomalous Hall insulators and active matter with spontaneous flows, we show that topologically protected sound modes can arise in a steady-state active system in continuum space. We point out that the net vorticity of the steady-state flow, which acts as a counterpart of the gauge field in condensed-matter settings, must vanish under realistic conditions for active systems. The quantum anomalous Hall effect thus provides design principles for realizing topological metamaterials. We propose and analyze the concrete minimal model and numerically calculate its band structure and eigenvectors, demonstrating the emergence of nonzero bulk topological invariants with the corresponding edge sound modes. This new type of topological active systems can potentially expand possibilities for their experimental realizations and may have broad applications to practical active metamaterials. Possible realization of non-Hermitian topological phenomena in active systems is also discussed.
description: 6+5 pages, 4+4 figures, to appear in PRL, see also supplementary movie published with the manuscript
title: Doubting Conventional Reality: Visual Art and Quantum Mechanics
Creators: name: Stone, Lynden
Publisher: name: Griffith University
Year: 2014
Subjects: subject: Conventional reality
subject: Quantum mechanics
subject: Visual arts
subject: Metaphase Typewriter Revival Project
subject: Mind Lamp Project
subject: Mind dispenser

description: Quantum mechanics give significant cause to doubt conventional reality. This exegesis answers the question of how visual art, in engaging with quantum concepts, can enable a viewer to doubt conventional reality. I argue that visual art can do this by an artwork’s capacity to provoke unconventional thinking in the viewer and by the artist’s prudent considerations of materials and metaphor. I discuss my own artworks and those of others to assess the capacity of such works to cause ruptures of expected reality and so enable a viewer to doubt conventional reality. In particular, I argue that my three ‘mind works’ projects (the Metaphase Typewriter revival project, the Mind Lamp project and the Mind dispenser) are successful (even just on a metaphoric level) in enabling a viewer to doubt conventional reality. Specifically, this is because they provide the viewer opportunities to interact with events of quantum superposition, using only consciousness, to arguably affect or even create material reality.
DEVELOPMENT OF CLINICAL ALGORITHMS FOR THE TREATMENT OF SECONDARY CATARACTS AND PUPILLARY MEMBRANES IN CHILDREN
Creators: name: Kariyev, Abdufarrux
name: Zokirkhuzhaev, Rustam
Publisher: name: Zenodo
Year: 2025

description: This study presents the development and clinical validation of diagnostic and treatment algorithms for secondary cataracts and pupillary membranes in pediatric patients. A total of 160 children (320 eyes), aged 6 months to 15 years (mean age 5.2 ± 3.1 years), were examined post-cataract surgery. Based on cataract etiology, age, and intraocular lens status, personalized laser intervention protocols were created. The proposed algorithm improved visual outcomes and reduced complications. Postoperative optical axis clarity was achieved in 92.5% (296 eyes), and visual acuity increased by two or more lines in 88.4% (283 eyes). The algorithm provides structured decision-making for pediatric ophthalmologists.
Richardsoniscus VANDEL 1963
Creators: name: Schmidt, Christian
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Scleropactidae
Richardsoniscus

description: RICHARDSONISCUS VANDEL, 1963
 Type species: Sphaeroniscus portoricensis Richardson, 1901 (by monotypy).
 Diagnosis
By endoantennal conglobation ability and simple coxal plates. Eyes represented by dark pigment, but no lenses are visible. In dorsal view, the visible portion of the uropod sympodite is nearly twice as wide as long. Pleotelson with median shallow tubercle.
description: Published as part of Schmidt, Christian, 2007, Revision of the Neotropical Scleropactidae (Crustacea: Oniscidea), pp. 1-339 in Zoological Journal of the Linnean Society 151 on page 27, DOI: 10.1111/j.1096-3642.2007.00286.x, http://zenodo.org/record/5430080
H2O Masers and Supersonic Turbulence
Creators: name: Strelnitski, V.
name: Alexander, J.
name: Gezari, S.
name: Holder, B. P.
name: Moran, J. M.
name: Reid, M. J.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use unpublished and published VLBI results to investigate the geometry and the statistical properties of the velocity field traced by H2O masers in five galactic regions of star formation -- Sgr B2(M), W49N, W51(MAIN), W51N, and W3(OH). In all sources the angular distribution of the H2O hot spots demonstrates approximate self-similarity (fractality) over almost four orders of magnitude in scale, with the calculated fractal dimension d between (approximately) 0.2 and 1.0. In all sources, the lower order structure functions for the line-of-sight component of the velocity field are satisfactorily approximated by power laws, with the exponents near their classic Kolmogorov values for the high-Reynolds-number incompressible turbulence. These two facts, as well as the observed significant excess of large deviations of the two-point velocity increments from their mean values, strongly suggest that the H2O masers in regions of star formation trace turbulence. We propose a new conceptual model of these masers in which maser hot spots originate at the sites of ultimate dissipation of highly supersonic turbulence produced in the ambient gas by the intensive gas outflow from a newly-born star. Due to the high brightness and small angular sizes of masing hot spots and the possibility of measuring their positions and velocities with high precision, they become a unique probe of supersonic turbulence.
description: 40 pages with 14 total figures (figures 9 and 10 are multi-part) Accepted for publication ApJ, December 20, 2002, Vol. 581, n2
title: Effects of a Multi-modal Exercise Program on Cognitive and Physical Functions and Brain-Derived Neurotrophic Factor in Older Women
Creators: name: Vaughan, Susan Maria
Publisher: name: Griffith University
Year: 2014
Subjects: subject: Age-related cognitive decline (ARCD)
subject: Cognitive processes
subject: Life-long neuronal capacity

description: Age-related cognitive decline (ARCD) is a pattern of deterioration in cognitive functions that gradually impairs the ability to think, reason, concentrate and remember. It has been identified as a major health threat for older adults because of the potential deleterious effects on independence, social engagement and quality of life. The trend in the experimental literature suggests that cardiovascular exercise training may have the capacity to counter ARCD. However, the efficacy of single modality interventions is inconclusive and there is currently a move towards investigating the effects of combination exercise interventions. The assumption is that optimisation of the intervention stimulus, in this way, might induce more pronounced cognitive outcomes than the modest levels of enhancement elicited by cardiovascular training alone. There are theoretical indications that these effects may be more likely to be achieved by the inclusion of motor skills training; as this modality involves complexity and novelty that requires sustained mental effort or cognitive load. The suggestion is that sustained mental effort is likely to both induce (positive) brain changes and stimulate higher-order cognitive processes (executive functions). In theory, the inclusion of these design elements may benefit executive function (higher order cognitive processes most susceptible to ARCD) and induce positive neuroplasticity (the life-long neuronal capacity of the brain to preserve or optimise function, in response to experiential stimuli).
Additional file 1 of Ruyiping formula inhibits metastasis via the microRNA-134-SLUG axis in breast cancer
Creators: name: Jiang, Ziwei
name: Pei, Lixia
name: Xie, Ying
name: Ye, Qun
name: Liang, Xiaoqiang
name: Ye, Yiyi
name: Liu, Sheng
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 1.
title: Consumer Decision-Making: An Empirical Exploration of Multi-Phased Decision Processes
Creators: name: Shao, Wei
Publisher: name: Griffith University
Year: 2007
Subjects: subject: Consumer
subject: decision-making
subject: phases
subject: strategies
subject: heterogeneity

description: Over the past 50 years, a great deal of research has conceptualised and modelled consumer decision-making as a single-or two-stage decision process. Today, the decision complexity has increased and consumers need to filter out a large amount of information prior to the final choice decision. This poses a challenge for marketing modellers to develop decision models that are more representative of real-world decision-making. An important rationale for the present study is to improve our understanding of consumer decision-making by providing empirical evidence that consumer decision-making may go beyond a single-or two-stage structure. This thesis aims to provide an insightful view of consumer decision-making, which may help marketers to develop and reinforce marketing programs to address consumer needs and hence increase profits, with knowledge of the types of decisions made and how decisions are made at different stages of the decision process. The literature review identified single-and two-stage decision models. Data analysis did not fully support this conceptualisation. An empirical exploration of consumer decision-making for a durable product revealed that the existing literature is limited in scope and predictability as they failed to capture multi-phase decision processes, which accounted for approximately one-half of consumer decisions. Empirical evidence was found suggesting that consumers seldom use a single strategy throughout the decision process. Consumer heterogeneity was also evident in this research as different consumers approached the same decision task with different processes and outcomes. Finally, this research identified those aspects of decision processes that have not been captured by the literature-based decision strategies. This research suggests that consumer decisions are more contingent than previously conceived in a single-and two-stage model. This research recommends that marketers should reconsider their understanding of consumer decision-making and bear in mind that one marketing strategy does not fit all customers. Marketers need to develop marketing strategies to address the entire decision process instead of focusing only on the decision outcome. By identifying different decision paths that are used by consumers, marketers can effectively segment the market; marketers can also benchmark consumers' perceptions of their performance on the important attributes against competitors to ensure that their product/brand is not eliminated prior to the selection from within the choice set. Future research requires us to understand how consumer differences interact with the decision environment to influence decision processes and outcomes. To do so, researchers must adopt a multi-phase perspective.
Cerium: the lithium substitute in post-AGB stars
Creators: name: Reyniers, Maarten
name: Van Winckel, Hans
name: Biemont, Emile
name: Quinet, Pascal
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this letter we present an alternative identification for the line detected in the spectra of s-process enriched low-mass post-AGB stars around 6708A and which was interpreted in the literature as due to Li. Newly released line lists of lanthanide species reveal, however, the likely identification of the line to be due to a CeII transition. We argue that this identification is consistent with the Ce abundance of all the objects discussed in the literature and conclude that in none of the low-mass s-process enriched post-AGB stars there is indication for Li-production.
description: 5 pages, 2 figures, accepted for publication as A&A Letter
Supplemental Material from Bigger isn't necessarily better: empirical tests show that dispersal proxies misrepresent actual dispersal ability
Creators: name: Lancaster, Jill
name: Downes, Barbara
name: Kayll, Zachary
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 310399
subject: Ecology not elsewhere classified

description: WMD Supp Material PRS final.pdf
Additional file 2: of Non-controlled, open-label clinical trial to assess the effectiveness of a dietetic food on pruritus and dermatologic scoring in atopic dogs
Creators: name: Witzel-Rollins, Angela
name: Murphy, Maryanne
name: Becvarova, Iveta
name: Werre, Stephen
name: Marie-Christine Cadiergues
name: Meyer, Hein
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: Figure S2. Dog owner assessment form. Dog owners were asked to complete the assessment form to rate their dogâ s quality of life, skin and coat quality, and acceptance of the dermatologic diet at weeks 0, 4, 8. (DOCX 13 kb)
Additional file 1: of Non-controlled, open-label clinical trial to assess the effectiveness of a dietetic food on pruritus and dermatologic scoring in atopic dogs
Creators: name: Witzel-Rollins, Angela
name: Murphy, Maryanne
name: Becvarova, Iveta
name: Werre, Stephen
name: Marie-Christine Cadiergues
name: Meyer, Hein
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Computational Biology

description: Figure S1. Dermatological evaluation chart provided to veterinarians. Veterinarians were asked to fill in the table above to describe skin lesions and body regions affected at weeks 0, 4, and 8. (DOCX 73 kb)
A multiwavelength approach to the SFR estimation in galaxies at intermediate redshifts
Creators: name: Cardiel, N.
name: Elbaz, D.
name: Schiavon, R. P.
name: Willmer, C. N. A.
name: Koo, D. C.
name: Phillips, A. C.
name: Gallego, J.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use a sample of 7 starburst galaxies at intermediate redshifts (z ~ 0.4 and z ~ 0.8) with observations ranging from the observed ultraviolet to 1.4 GHz, to compare the star formation rate (SFR) estimators which are used in the different wavelength regimes. We find that extinction corrected Halpha underestimates the SFR, and the degree of this underestimation increases with the infrared luminosity of the galaxies. Galaxies with very different levels of dust extinction as measured with SFR(IR)/SFR(Halpha, uncorrected for extinction) present a similar attenuation A[Halpha], as if the Balmer lines probed a different region of the galaxy than the one responsible for the bulk of the IR luminosity for large SFRs. In addition, SFR estimates derived from [OII]3727 match very well those inferred from Halpha after applying the metallicity correction derived from local galaxies. SFRs estimated from the UV luminosities show a dichotomic behavior, similar to that previously reported by other authors in galaxies at z
description: Accepted for publication in The Astrophysical Journal
Evidence for a warm ISM in the Fornax dEs FCC046 and FCC207
Creators: name: De Rijcke, S.
name: Zeilinger, W. W.
name: Dejonghe, H.
name: Hau, G. K. T.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present Halpha+[NII] narrow-band imaging of FCC046 and FCC207, two dES in the Fornax Cluster. B-R and B-I color-maps clearly show signs of dust-absorption in FCC207. FCC046 has a very bright blue nucleus, offset by about 1.1'' with respect to the outer isophotes. Moreover, FCC046 shows a pronounced lopsided shape. The emitting regions differ considerably between the two galaxies. Whereas FCC207 has only one central emission region, FCC046 also contains fainter emission regions. Based on broad-band colours, its disturbed shape and its very bright nucleus, FCC046 is akin to the class of amorphous dwarfs. The central emission regions of both galaxies are resolved and we estimate their diameters at about 60 pc. Their Halpha luminosities can be explained as photo-ionisation by post-AGB stars in an old population. Some of the emission regions in FCC046 are resolved and have diameters of the order of 50-150 pc and H$α$ luminosities of the order of 10^30 W, comparable to supernova remnants or nebulae around Wolf-Rayet stars. Hence, FCC046 is clearly undergoing star-formation while for FCC207 the case is not as clearcut. We estimate the mass of the HII gas in FCC046 at M(HII) = 40-150 Mo. The ionised-gas content of FCC207 is somewhat higher : M(HII) = 60-190 Mo.
description: 11 pages, 14 figures, accepted for publication in MNRAS
Scleropactes
Creators: name: Schmidt, Christian
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Scleropactidae
Scleropactes

description: SCLEROPACTES BUDDE- LUND, 1885
 Type species: Scleropactes concinnus Budde-Lund, 1885 [designated by Mulaik (1960)].
 Diagnosis
 Cephalothorax with frontal shield, behind frontal line with transverse furrow that laterally is recurved and ending medially to the eyes. Mandible with right one/left two penicils on the hairy lobe, and one penicil between the lobe and the pars molaris, which is represented by a tuft of hairy setae. First maxilla with two laterally flattened penicils on the median endite, lateral endite with four plus six teeth, an additional tooth, and a cuticular stalk with a hirsute apex on the rostral surface (cf. Ferrara et al. 1995). Second maxilla with fine setation on the mesal and lateral lobe, both lobes subequal in length. Mesal lobe with a field of sensilla. Maxilliped with a large or vestigial penicil on the frontal face of the endite. Maxilliped palp with one large and one somewhat smaller seta on the basal joint, and the distal tuft of setae on the medial article on a socket. Second and distal article weakly delimited. Carpus of first pereiopod with a welldeveloped antenna-grooming brush in both sexes. Males with brush-like fields of scales, at least the merus and carpus of pereiopods 1 and 2. Exopodites of first two pairs of pleopods have a respiratory area, delimited mesally by a sulcus (no respiratory field visible in Scleropactes pululahua). Male endopodite 2 slender and straight. Protopodites of uropods filling the gap between pleotelson and epimera of pleonites. Endopodite inserted on the inner edge of protopodite, which is dorsoventrally flattened [based on the definition given by Leistikow (1997)].
 Remark
 Vandel (1972) enumerated several characters that Scleropactes has in common with the Scyphacidae (first antenna with aesthetascs in several rows, second antenna with three-jointed flagellum, maxilliped endite with penicil, ‘well-developed’ dactylar seta, pleopod exopodites with haemolymph sinus). All these are plesiomorphies, and after Vandel they prove that Scleropactes is the most primitive genus of the Scleropactidae. Schultz (1995) erroneously mentioned that the flagellum of the second antenna of Scleropactes has two joints.
 The mention of Scleropactes concinnus as ‘genotipo’ of Scleropactes by Mulaik (1960) is regarded as the designation of the type species, according to ICZN Art. 69 a iii.
 At present, the genus Scleropactes is probably still paraphyletic. The present analysis revealed only very weak characters as putative apomorphies.
description: Published as part of Schmidt, Christian, 2007, Revision of the Neotropical Scleropactidae (Crustacea: Oniscidea), pp. 1-339 in Zoological Journal of the Linnean Society 151 on pages 40-41, DOI: 10.1111/j.1096-3642.2007.00286.x, http://zenodo.org/record/5430080
BC-SIM-IAPSUPA-TR-001 HRIC NECP report
Creators: name: DELLA CORTE, VINCENZO
name: ZUSI, MICHELE
name: PALUMBO, PASQUALE
Publisher: name: IAPS Roma
Year: 2019

description: The present document has been issued with the aim of describing the NECP (Near Earth Commissioning Phase) Tests results of HRIC channel part of the SIMBIO-SYS instrument suite on board the BepiColombo ESA mission.
title: Interprofessional Practice (IPP): from Text to Context
Creators: name: Frey, Nicolette
Publisher: name: Griffith University
Year: 2016
Subjects: subject: Interprofessional practice (IPP)
subject: Healthcare system
subject: Mental healtcare
subject: Severe mental illness

description: There is a significant gap between the theorising of interprofessional practice (IPP) and the existence of IPP in community healthcare teams who provide services to people with severe mental illness (SMI). This study aims to clarify the concept of IPP both in the literature and in self-identified teams focused on improving the physical health of people with SMI in Queensland. It is widely acknowledged that the physical health of people with SMI is poor and their healthcare needs remain unmet. The reasons for their poor health outcomes are multiple and complex, and as the complexities of their healthcare needs increase, so too does their reliance on the healthcare system. However, the healthcare system is also complex with multiple problems, including a lack of continuity, fragmentation of services, and shortages in workforce and skills. In response to this complex situation, scholars and policymakers repeatedly call for the integration of care through multidisciplinary healthcare teams that practise in interprofessional ways. The challenges to the implementation of IPP are many, and include professional educational differences, a paucity of opportunities to learn together, and competition for limited resources. The community mental healthcare team is one place where an interprofessional approach is thought to be critical, especially to deliver services to those with multiple complex needs created by SMI and comorbidities. People with complex needs rely on multiple healthcare providers who are required to operate with continuity across disciplinary and organisational boundaries.
Observational constraints of a new unified dark fluid and the $H_0$ tension
Creators: name: Yang, Weiqiang
name: Pan, Supriya
name: Paliathanasis, Andronikos
name: Ghosh, Subir
name: Wu, Yabo
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Unified cosmological models have received a lot of attention in astrophysics community for explaining both the dark matter and dark energy evolution. The Chaplygin cosmologies, a well known name in this group have been investigated matched with observations from different sources. Obviously, Chaplygin cosmologies have to obey restrictions in order to be consistent with the observational data. As a consequence, alternative unified models, differing from Chaplygin model, are of special interest. In the present work we consider a specific example of such a unified cosmological model, that is quantified by only a single parameter $μ$, that can be considered as a minimal extension of the $Λ$-cold dark matter cosmology. We investigate its observational boundaries together with an analysis of the universe at large scale. Our study shows that at early time the model behaves like a dust, and as time evolves, it mimics a dark energy fluid depicting a clear transition from the early decelerating phase to the late cosmic accelerating phase. Finally, the model approaches the cosmological constant boundary in an asymptotic manner. We remark that for the present unified model, the estimations of $H_0$ are slightly higher than its local estimation and thus alleviating the $H_0$ tension.
description: 18 pages, 15 captioned figures, 6 tables; Accepted for publication by Monthly Notices of the Royal Astronomical Society
A Search for Core-Collapse Supernova Progenitors In Hubble Space Telescope Images
Creators: name: Van Dyk, Schuyler D.
name: Li, Weidong
name: Filippenko, Alexei V.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Identifying the massive progenitor stars that give rise to core-collapse supernovae (SNe) is one of the main pursuits of supernova and stellar evolution studies. Using ground-based images of recent, nearby SNe obtained primarily with KAIT, astrometry from 2MASS, and archival images from HST, we have attempted the direct identification of the progenitors of 16 SNe II and SNe Ib/c. We may have identified the progenitors of the SNe II 1999br, 1999ev, and 2001du as supergiant stars with M^0_V ~ -6 mag in all three cases. We may have also identified the progenitors of the SNe Ib 2001B and 2001is as very luminous supergiants with M^0_V ~ -8 to -9 mag, and possibly the progenitor of the SN Ic 1999bu as a supergiant with M^0_V ~ -7.5 mag. Additionally, we have recovered at late times SNe 1999dn, 2000C, and 2000ew, although none of these had detectable progenitors on pre-SN images. In fact, for the remaining SNe only limits can be placed on the absolute magnitude and color (when available) of the progenitor. The detected SN II progenitors and limits are consistent with red supergiants as progenitor stars, although possibly not as red as we had expected. Our results for the SNe Ib/c do not strongly constrain either Wolf-Rayet stars or massive interacting binary systems as progenitors.
description: 19 pages, 23 figures, to appear in PASP (2003 Jan)
BC-SIM-TR-012 HRIC ICO1 REPORT
Creators: name: DELLA CORTE, VINCENZO
name: ZUSI, MICHELE
name: SIMIONI, EMANUELE
name: CAPACCIONI, FABRIZIO
name: CAPRIA, MARIA TERESA
name: Doressundiram, Alain
name: Langevin, Yves
name: PALUMBO, PASQUALE
name: Vincedon, Mathieu
name: CREMONESE, Gabriele
Publisher: name: IAPS Roma
Year: 2021

description: The present document has been issued to describe the Instrument Check Out Phase (ICO#1) Tests of HRIC channel of the Spectrometers and Imagers for MPO BepiColombo Integrated Observatory SYStem (SIMBIO-SYS).
A Flaring L5 Dwarf: The Nature of HαEmission in Very Low Mass (Sub)Stellar Objects
Creators: name: Liebert, James
name: Kirkpatrick, J. Davy
name: Cruz, K. L.
name: Reid, I. Neill
name: Burgasser, Adam
name: Tinney, C. G.
name: Gizis, John E.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Time series spectrophotometry of the L5 dwarf 2MASS 01443536-0716142 showed strong Hαemission which declined by nearly 75% in four consecutive exposures. The line was not detected in emission on a spectrum obtained eleven months later. This behavior constrasts with that of 2MASSI J1315309-264951, an L5 dwarf which has shown even stronger Hαemission on four separate occasions. The observational database suggests that L dwarfs can be found in such strong flares only occasionally, with a duty cycle of order 1%. In contrast, the few, continuously-strong Hαemitters, including PC 0025+0447 and 2MASSI J1237392+652615, must either be (1) objects no older than 10-100 Myrs with continuously-active accretion and/or chromospheres, but which apparently formed in isolation from known young stellar clusters and associations, or (2) objects empowered by a different and unknown mechanism for the Hαenergy.
description: 11 pages, 2 figures, Astronomical Journal in press -- Jan 2003 issue
HI Imaging of LGS 3 and an Apparently Interacting High-Velocity Cloud
Creators: name: Robishaw, Timothy
name: Simon, Joshua D.
name: Blitz, Leo
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a 93' by 93' map of the area near the Local Group dwarf galaxy LGS 3, centered on an HI cloud 30' away from the galaxy. Previous authors associated this cloud with LGS 3 but relied on observations made with a 36' beam. Our high-resolution (3.4'), wide-field Arecibo observations of the region reveal that the HI cloud is distinct from the galaxy and suggest an interaction between the two. We point out faint emission features in the map that may be gas that has been tidally removed from the HI cloud by LGS 3. We also derive the rotation curve of the cloud and find that it is in solid-body rotation out to a radius of 10', beyond which the rotation velocity begins to decline. Assuming a spherical geometry for the cloud, the implied mass is 2.8 x 10^7 (d/Mpc) M_{Sun}, where d is the distance in Mpc. The observed HI mass is 5.5 x 10^6 (d/Mpc)^2 M_{Sun}, implying that the cloud is dark-matter dominated unless its distance is at least 1.9 Mpc. We propose that the cloud is a high-velocity cloud that is undergoing a tidal interaction with LGS 3 and therefore is located roughly 700 kpc away from the Milky Way. The cloud then contains a total mass of ~2.0 x 10^7 M_{Sun}, 82% of which consists of dark matter.
description: 5 pages, 2 color figures. Accepted for publication in ApJ Letters
Generalization of Lieb-Wu wave function inspired by one-dimensional ionic Hubbard model
Creators: name: Hosseinzadeh, Abolfath
name: Jafari, S. A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Gases (cond-mat.quant-gas)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: With the ionic Hubbard model (IHM) in mind, we construct a non-trivial generalization of the Bethe ansatz (BA) wave function which naturally generalizes the Lieb-Wu wave function with an ionic parameter $Δ$, and reduces to Lieb-Wu solution in the limit $Δ\to 0$. The resulting two-particle scattering matrix satisfies the Yang-Baxter equation. To the extent that the unit cells with more than two electrons (Choy-Haldane issue) are avoided on average, our wave function represents an effective soluiton for the one-dimensional IHM. The Choy-Haldane issue restricts the validity of our solution to low-filling and large $U\gtrsim 4$. This regime is attainable in cold atom realizations of the IHM. For this regime, we numerically solve the generalized Bethe equations and compute the ground state energy in the thermodynamic limit.
The Infrared Counterpart of the Microquasar GRS 1758-258
Creators: name: Rothstein, D. M.
name: Eikenberry, S. S.
name: Chatterjee, S.
name: Egami, E.
name: Djorgovski, S. G.
name: Heindl, W. A.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present revised infrared (2.2 micron) astrometry of the field containing the Galactic microquasar GRS 1758-258, using observations at the Keck I 10-m telescope. We find three candidates for the microquasar within a 3 sigma error circle, but none within 2 sigma. We show that if the 18.4 day X-ray period of GRS 1758-258 is due to a binary orbit, then only one of the three candidates, an early K-type giant, is large enough to power the microquasar via Roche lobe overflow. We therefore identify this star as the infrared counterpart of GRS 1758-258, which we classify as a low mass X-ray binary. Long term infrared monitoring of this source should provide further information about the microquasar system, including a confirmation of the X-ray period and an estimate of the compact object's mass.
description: 4 pages, 2 figures; accepted for publication in ApJ Letters
Polarizability assessments of ion-based optical clocks
Creators: name: Barrett, M. D.
name: Arnold, K. J.
name: Safronova, M. S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: It is shown that the dynamic differential scalar polarisability of the $S_{1/2}-D_{5/2}$ transition in $^{138}$Ba$^+$ can be determined to an inaccuracy below $0.5\%$ across a wide wavelength range ($λ>700\,\mathrm{nm}$). This can be achieved using measurements for which accurate determination of laser intensity is not required, and most of the required measurements are already in the literature. Measurement of a laser-induced ac-stark shift of the clock transition would then provide an \emph{in situ} measurement of the laser's intensity to the same $0.5\%$ level of inaccuracy, which is not easily achieved by other means. This would allow accurate polarisability measurements for clock transitions in other ions, through comparison with $^{138}$Ba$^+$. The approach would be equally applicable to Sr$^+$ and Ca$^+$, with the latter being immediately applicable to Al$^+$/Ca$^+$ quantum logic clocks.
description: 5 pages and two figures
Additional file 7 of Plant super-barcode: a case study on genome-based identification for closely related species of Fritillaria
Creators: name: Wu, Lan
name: Wu, Mingli
name: Cui, Ning
name: Xiang, Li
name: Li, Ying
name: Li, Xiwen
name: Chen, Shilin
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 7: Verification of discrimination ability of 57 highly variable loci selected by published works.
Additional file 1: of Epidemiological assessment of the factors associated with antimicrobial use in French free-range broilers
Creators: name: Adam, Cécile
name: Fortané, Nicolas
name: Coviglio, Alexandra
name: Delesalle, Léa
name: Ducrot, Christian
name: Paul, Mathilde
Publisher: name: figshare
Year: 2019
Subjects: subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer
subject: 60506 Virology

description: Questionnaire used in the case-control study of risk factors for the use of antimicrobials in French free-range broilers (n = 260 flocks) in 2016. (PDF 935 kb)
2MASS 1315-2649: A High Proper Motion L Dwarf with Strong H-alpha Emission
Creators: name: Hall, Patrick B.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In Hall (2002) I reported that 2MASSI J1315309-264951 is an L dwarf with strong H-alpha emission. Two spectroscopic epochs appeared to show that the H-alpha was variable, decreasing from 121 Angstroms to 25 Angstroms EW, which I interpreted as a flare during the first observation. Gizis (2002) independently discovered this object, and his intermediate spectroscopic epoch shows H-alpha with 97 Angstroms EW. A new fourth epoch of spectroscopy again shows a very large H-alpha EW (124 Angstroms), confirming this object to be a persistent, strong H-alpha emitter. Whether the H-alpha is steady (like 2MASS 1237+6526) or from continuous strong flaring (like PC0025+0447) remains unclear. Imaging confirms that 2MASS 1315-2649 has a high proper motion (0.71"/year), corresponding to a transverse velocity of ~76 km/s at its distance of ~23 pc. Thus 2MASS 1315-2649 is consistent with being >~2 Gyr old and therefore relatively massive. If that is so, the correlation of H-alph activity with mass found by Gizis et al. (2000) would seem to support the continuous strong flaring scenario, though it does not rule out a brown dwarf binary accretion scenario.
description: 2 pages, ApJL accepted
On the Incidence of Strong Gravitational Lensing by Clusters in the Las Campanas Distant Cluster Survey
Creators: name: Zaritsky, Dennis
name: Gonzalez, Anthony H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The observed incidence of strongly lensing clusters exceeds the predictions of a Lambda-CDM model by about a factor of 10. We revisit the observational side of this discrepancy by measuring the incidence of strong lensing in a subsample of clusters drawn from the Las Campanas Distant Cluster Survey (LCDCS). Among clusters with 0.5<= z <= 0.7, the redshift range in which we focus our search, we find two strongly lensed systems within an effective search area of 69 sq. deg. There is at least one other strongly lensed system in the LCDCS outside of this redshift range, where we are less complete. Over all redshifts, the Lambda-CDM model produces one large arc every 146 sq. degrees. Assuming Poisson statistics, the probability of finding 3 or more strongly lensing clusters in 69 sq. degrees is 0.012. The lensing incidence within the LCDCS is in agreement with that derived from an X-ray selected sample and what has been preliminarily presented from an independent optical cluster survey. The origin of the disagreement between theory and observations, which remains at least at the order of magnitude scale for the Lambda-CDM model, lies either in the concordance cosmological model, in the characteristics of the resulting cluster potentials, or in the adopted source population.
description: 31 pages, accepted for publication in ApJ
Amazoniscus LEMOS DE CASTRO 1967
Creators: name: Schmidt, Christian
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Scleropactidae
Amazoniscus

description: AMAZONISCUS LEMOS DE CASTRO, 1967
 Type species: Amazoniscus arlei Lemos de Castro, 1967.
 Diagnosis (after Lemos de Castro 1969):
 Exoantennal conglobation. Linea frontalis distant from vertex to form a frontal shield, linea supraantennalis present. Coxal plates all simple, coxal plate 1 sinuous near the hind corner (as in Circoniscus, but without schisma). Second antenna with two-jointed flagellum. Male pereiopod 7 ischium with ventrocaudal tubercle on the distal margin. Pleotelson triangular, with concave sides. Uropod protopodites rectangular, distinctly projecting beyond the pleotelson. Exopodites not exceeding endopodites.
description: Published as part of Schmidt, Christian, 2007, Revision of the Neotropical Scleropactidae (Crustacea: Oniscidea), pp. 1-339 in Zoological Journal of the Linnean Society 151 on page 64, DOI: 10.1111/j.1096-3642.2007.00286.x, http://zenodo.org/record/5430080