cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Active Galactic Nucleus Pairs from the Sloan Digital Sky Survey. III. Chandra X-ray Observations Unveil Obscured Double Nuclei
Creators: name: Hou, Meicun
name: Liu, Xin
name: Guo, Hengxiao
name: Li, Zhiyuan
name: Shen, Yue
name: Green, Paul J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present Chandra ACIS-S X-ray imaging spectroscopy for five dual active galactic nucleus (AGN) candidates. Our targets were drawn from a sample of 1286 [O III]-selected AGN pairs systematically selected from the Sloan Digital Sky Survey Seventh Data Release. Each of the targets contains two nuclei separated by $\sim$3-9 kpc in projection, both of which are optically classified as Type 2 (obscured) AGNs based on diagnostic ratios of the narrow emission lines. Combined with independent, empirical star formation rate estimates based on the host-galaxy stellar continua, the new Chandra X-ray observations allow us to evaluate the dual-AGN hypothesis for each merging system. We confirm two (SDSS J0907+5203 and SDSS J1544+0446) of the five targets as bona-fide dual AGNs. For the other three targets, the existing data are consistent with the dual-AGN scenario, but we cannot rule out the possibility of stellar/shock heating and/or one AGN ionizing both gaseous components in the merger. The average X-ray-to-[O III] luminosity ratio in our targets seems to be systematically smaller than that observed in single AGNs but is higher than that seen in dual AGNs selected from AGNs with double-peaked narrow emission lines. We suggest that the systematically smaller X-ray-to-[O III] luminosity ratio observed in dual AGNs than in single AGNs is due to a high nuclear gas column likely from strong merger-induced inflows. Unlike double-peaked-[O III]-selected dual AGNs, the new sample selected from resolved galaxy pairs are not subject to the orientation bias caused by the double-peak line-of-sight velocity splitting selection, which also contributes to lowering the X-ray-to-[O III] luminosity ratio.
description: 18 pages, 8 figures. Accepted for publication in ApJ. Comments welcome. arXiv admin note: text overlap with arXiv:1209.5418
Directionality of Solar Flare Accelerated Protons and Alpha Particles from Gamma-Ray Line Measurements
Creators: name: Share, G. H.
name: Murphy, R. J.
name: Kiener, J.
name: de Sereville, N.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The energies and widths of gamma-ray lines emitted by ambient nuclei excited by flare-accelerated protons and alpha particles provide information on the ions directionality and spectra, and on the characteristics of the interaction region. We have measured the energies and widths of strong lines from de-excitations of 12C, 16O, and 20Ne in solar flares as a function of heliocentric angle. The line energies from all three nuclei exhibit ~1% redshifts for flares at small heliocentric angles, but are not shifted near the limb. The lines have widths of ~3% FWHM. We compare the 12C line measurements for flares at five different heliocentric angles with calculations for different interacting-particle distributions. A downward isotropic distribution (or one with a small upward component) provides a good fit to the line measurements. An angular distribution derived for particles that undergo significant pitch angle scattering by MHD turbulence in coronal magnetic loops provides comparably good fits.
Additional file 1: of Genome-wide sequencing and metabolic annotation of Pythium irregulare CBS 494.86: understanding Eicosapentaenoic acid production
Creators: name: Fernandes, Bruna
name: Dias, Oscar
name: Costa, Gisela
name: Neto, Antonio Kaupert
name: Resende, Tiago
name: Oliveira, Juliana
name: RiaĂąo-PachĂłn, Diego
name: Zaiat, Marcelo
name: JosĂŠ Pradella
name: Rocha, Isabel
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Inorganic Chemistry

description: Figure S1. Wastewater composition and forecast for 2024 â Vinasse and Glycerol compostion and worldwild forecast production for 2024. (PDF 806 kb)
The shear power spectrum from the COMBO-17 survey
Creators: name: Brown, M. L.
name: Taylor, A. N.
name: Bacon, D. J.
name: Gray, M. E.
name: Dye, S.
name: Meisenheimer, K.
name: Wolf, C.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We perform a cosmic shear analysis of the COMBO-17 survey -- a unique dataset with shear quality R-band imaging and accurate photometric redshift estimates (dz=0.05) for ~90% of galaxies to R=24.0. We undertake a full maximum likelihood analysis to measure the weak lensing power spectra, Cl^kk, Cl^bb & Cl^kb from l=400 to l=10^4. We find a strong measurement of the convergence power over five fields. The b-field has a much lower significance, indicating our data is free of major systematics, while the cross-correlation of k & b is consistent with zero. We have also calculated the shear correlation functions and variance over a range of scales between 0.5 and 20 arcmin. In addition, we have used our results to measure cosmological parameters, constraining the normalisation of the matter power spectrum to be sigma_8=(0.72 \pm 0.09)(Omega_m/0.3)^-0.49, where the errors quoted are 1-sigma due to the intrinsic dispersion in galaxy ellipticities, cosmic and sampling variance. We have significantly reduced the usual additional uncertainty in the median redshift (z_m) of the survey by estimating z_m directly from the data. To demonstrate the power of accurate redshift information, we have also measured parameters from a shear analysis of only those galaxies with accurate redshifts. In this case, we have eliminated the uncertainty in the redshift distribution of sources and we show that the uncertainty in the resulting parameter constraints are reduced by more than a factor of 2 compared to the typical uncertainties found in cosmic shear surveys to date. Finally, we combine our parameter measurements with constraints from the 2dFGRS and from the CMB. With these additional constraints, we measure sigma_8=0.73 +0.05/-0.03 and Omega_m=0.27 +/- 0.02.
description: Matches version to appear in 1st May edition of MNRAS (vol. 341, pp.100-118)
Parajungiella ellisi CR
Creators: name: Omelková, Markéta
name: Ježek, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psychodidae
Parajungiella
Parajungiella ellisi

description: Parajungiella ellisi (Withers, 1987) (CR)
 Published records. Citonice (JEŽEK 2003), Horní Břečkov, Devět Mlýnů (JEŽEK et al. 2005).
 Material examined. Citonice, Na hájkách (8), 2 JJ, v., Inv. No. 6061 and 6063.
 Comment. A rare European and West-Siberian species known from Great Britain, Ireland, Austria, Czech Republic and Russia (Siberia). Critically endangered in the Czech Republic.
description: Published as part of Omelková, Markéta & Ježek, Jan, 2012, A new species of the genus Trichomyia (Diptera: Psychodidae) and new faunistic data on non-phlebotomine moth flies from the Podyjí NP and its surroundings (Czech Republic), pp. 505-533 in Acta Entomologica Musei Nationalis Pragae 52 (2) on page 519, DOI: 10.5281/zenodo.5332309
title: The Psychopathological Antecedents of Conspiracy Belief
Creators: name: Thresher-Andrews, Christopher Thomas
Publisher: name: Goldsmiths, University of London
Year: 2020

description: A conspiracy theory can be defined as an alternative explanation for an event that reveals the presence of a hidden group with malevolent intent. Conspiracy theories attract themselves to significant world events with political and social ramifications, and attempt to describe them through the lens of a monological belief system that sees conspiracy as the overwhelming explanation for humanity’s struggles. Although the psychological work exploring the various factors associated with conspiracy belief has grown considerably, the literature has only recently moved to experimental designs that aim to explore causal mechanisms. The current thesis, using a psychopathological framework, attempts to contribute to this. Study 1 found that participants who felt a lack of control showed significantly higher belief in conspiracy theories. Despite this causal link between personal control and conspiracy belief, further analysis in Study 2 raised doubts over the manipulation’s validity. Studies 3-5 attempted to manipulate feelings of paranoia and measure their effect on conspiracy belief; unfortunately, all three studies failed to significantly increase participants’ paranoid feelings. Study 6 attempted a self-esteem manipulation, which again failed to show a significant effect. Correlational work from this chapter found significant relationships between paranoia and conspiracy theories, but not self-esteem or political orientation. Finally, Study 7 successfully demonstrated a relationship between delusional ideation and conspiracy belief. A minority of this non-clinical sample exhibited a jumping-to-conclusions bias when measured using the beads task, but this bias was not related to delusional ideation or conspiracy belief. Study 8 found that belief in conspiracy theories was also related to schizotypy and a range of cognitive biases. To conclude, the thesis discusses the limitations of applying psychopathological models to explain conspiracy theory belief, providing evidence that although conspiracy theories are unlikely to be products of delusion they likely share similar cognitive antecedents.
Resource theory of asymmetric distinguishability for quantum channels
Creators: name: Wang, Xin
name: Wilde, Mark M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: Information Theory (cs.IT)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: This paper develops the resource theory of asymmetric distinguishability for quantum channels, generalizing the related resource theory for states [arXiv:1010.1030; arXiv:1905.11629]. The key constituents of the channel resource theory are quantum channel boxes, consisting of a pair of quantum channels, which can be manipulated for free by means of an arbitrary quantum superchannel (the most general physical transformation of a quantum channel). One main question of the resource theory is the approximate channel box transformation problem, in which the goal is to transform an initial channel box (or boxes) to a final channel box (or boxes), while allowing for an asymmetric error in the transformation. The channel resource theory is richer than its counterpart for states because there is a wider variety of ways in which this question can be framed, either in the one-shot or $n$-shot regimes, with the latter having parallel and sequential variants. As in our prior work [arXiv:1905.11629], we consider two special cases of the general channel box transformation problem, known as distinguishability distillation and dilution. For the one-shot case, we find that the optimal values of the various tasks are equal to the non-smooth or smooth channel min- or max-relative entropies, thus endowing all of these quantities with operational interpretations. In the asymptotic sequential setting, we prove that the exact distinguishability cost is equal to the channel max-relative entropy and the distillable distinguishability is equal to the amortized channel relative entropy of [arXiv:1808.01498]. This latter result can also be understood as a solution to Stein's lemma for quantum channels in the sequential setting. Finally, the theory simplifies significantly for environment-seizable and classical--quantum channel boxes.
description: 39 pages, 6 figures
title: Screaming "Me,me,me": entitled employees and retaliation in the workplace
Creators: name: Westerlaken, Kristie Mae
Publisher: name: Griffith University
Year: 2013
Subjects: subject: Entitlement at work
subject: Organizational justice
subject: Organizational behavior
subject: Retaliation in the workplace

description: A sense of entitlement is defined as an expectation of special or preferential treatment and is considered a trait for some individuals (Campbell, Bonacci, Shelton, Exline, & Bushman, 2004). The construct of entitlement is currently garnering attention amongst researchers in disciplines such as psychology, marketing, academia, and management. Arguably, the reasons for the increasing attention on this construct are widespread perceptions, albeit largely anecdotal, that a sense of entitlement is escalating in individuals across Western society. Prior research has also found numerous negative characteristics and outcomes to be positively associated with entitlement, including aggression, hostility anti-sociality, and conflict. To date, there is very limited research on entitlement in the workplace (Fisk, 2010; Harvey & Harris, 2010; Harvey & Martinko, 2009; Hochwarter, Summers, Thompson, Perrewé, & Ferris, 2010). Despite some discipline-based definitions in law, marketing, and academia, entitlement has yet to be clearly and consistently conceptualised in management literature, which may provide some explanation for the lack of existing research. Understanding entitlement at work is important given the links to counterproductive attitudes and behaviours. Counterproductive work attitudes and behaviours are phenomena that cost organisations much in both human capital and financial losses.
Review of Simon Jeffes: Music from the Penguin Cafe, Roger Dean’s Lysis: Lysis Live, David Rosenboom & J.B. Floyd: Suitable for Framing, The Sounds of Sound Sculpture, and David Rosenboom: Brainwave Music
Creators: name: Roberts, David
Publisher: name: Contact: A Journal for Contemporary Music (1971-1988)
Year: 2019

description: -
description: Contact: A Journal for Contemporary Music (1971-1988), No 16 (1977): Contact: A Journal for Contemporary Music
title: Nursing Care Practices and Workplace Relations in a Thai Surgical Ward: An Exploration of Clinical Decision-Making
Creators: name: Maneewat, Khomapak
Publisher: name: Griffith University
Year: 2010
Subjects: subject: Thai surgical ward
subject: nursing care practices
subject: workplace relations
subject: Thai surgical nurse
subject: Thai surgical nursing

description: This thesis offers a study of how a local ward culture underpins nursing actions of Thai surgical nurses in order to account for issues such as lack of sustainability, and failure to use research, including evidence-based nursing practice and the new multimodal model of care which has been officially adopted in the Thai hospital context. The study was conducted at a Thai surgical ward to illuminate and describe the culture of the Thai surgical nurse, including the ways in which the organizational culture influences or guides their thinking, decision-making, and actions in a patterned way. The knowledge about how the Thai surgical nurses allocate care, and make clinical decisions in the surgical ward in the context of social relations and staff culture is constructed through an ethnographic approach based on fieldwork at the non-private general surgical wards of one university hospital in Southern Thailand. A better understanding of the diversity of Thai surgical nursing practice is then enacted from a typical day in the life of the Thai surgical nurses, which consists of the realities, ritualised practices, relations, and integration both with within their group and with others. The study results represent the way that nursing organizational culture informs the practices, decision-making, and the predictions of the nurses’ possible response to change. The pre- and post-operative cares allocated by the nurses of the TSW are routinised, almost ritualised, and reflect fixed assumptions about the way cares ought to be delivered, including those reflecting the lack of commitment to implementing new multimodal models of care as well as research utilization and evidence-based practice. The study raises significant concerns about the status of professional nursing in Thailand in terms of professional autonomy and the status of the nurses within the Thai hospital context. Empowering professional nursing is therefore recommended as a first priority to change Thai nursing culture. The ritualised practices, task-oriented working system, and the dominance of the medical model in the Thai nursing culture further reflect the need to establish an evidence-based nursing culture to create professional identity and improve the quality of care.
Solar System Objects in the ISOPHOT 170 micron Serendipity Survey
Creators: name: Mueller, T. G.
name: Hotzel, S.
name: Stickel, M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The ISOPHOT Serendipity Survey (ISOSS) covered approximately 15 % of the sky at a wavelength of 170 micron while the ISO satellite was slewing from one target to the next. By chance ISOSS slews went over many solar system objects (SSOs). We identified the comets, asteroids and planets in the slews through a fast and effective search procedure based on N-body ephemeris and flux estimates. The detections were analysed from a calibration and scientific point of view. Through the measurements of the well-known asteroids Ceres, Pallas, Juno and Vesta and the planets Uranus and Neptune it was possible to improve the photometric calibration of ISOSS and to extend it to higher flux regimes. We were also able to establish calibration schemes for the important slew end data. For the other asteroids we derived radiometric diameters and albedos through a recent thermophysical model. The scientific results are discussed in the context of our current knowledge of size, shape and albedos, derived from IRAS observations, occultation measurements and lightcurve inversion techniques. In all cases where IRAS observations were available we confirm the derived diameters and albedos. For the five asteroids without IRAS detections only one was clearly detected and the radiometric results agreed with sizes given by occultation and HST observations. Four different comets have clearly been detected at 170 micron and two have marginal detections. The observational results are presented to be used by thermal comet models in the future. The nine ISOSS slews over Hale-Bopp revealed extended and asymmetric structures related to the dust tail. We attribute the enhanced emission in post-perihelion observations to large particles around the nucleus. The signal patterns are indicative of a concentration of the particles in trail direction.
description: 15 pages, 6 figures, 6 tables; Accepted for publication in Astronomy and Astrophysics
Identification of volatile components and analysis of aroma characteristics of Jiangxi Congou black tea
Creators: name: Yue, Cuinan
name: Yang, Puxiang
name: Qin, Dandan
name: Cai, Hailan
name: Wang, Zhihui
name: Li, Chen
name: Wu, Hualing
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Space Science
subject: Molecular Biology
subject: Neuroscience
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Plant Biology

description: Jiangxi Congou black tea is one of the earliest Congou black tea in China. In order to explore its sensory characteristics and molecular sensory basis, quantitative description analysis (QDA) and gas chromatography-mass spectrometry (GC-MS) were used to analyze the sensory characteristics and volatile components of 11 Congou black tea samples from Jiangxi Province in China. The results showed that the aroma characteristics of Jiangxi Congou black were composed of 11 aroma descriptors, namely, sweet-smell, floral, fruity, roasted, spicy, fresh, green, oil, off-odor, woody and smoky. There was also interaction effect between sensory attributes of aroma, which were significant negative correlation between floral, and fruity, and green. The presence of roasted incense could significantly enhance the olfactory perception of off-odor and smoky, and off-odor was an important attribute that affects the aroma quality of Jiangxi Congou black tea. Volatile components (i.e. 74 kinds) were identified, among which the highest content and species were alcohols, followed by esters, and the lowest were heterocycles and terpenes. The results of partial least square variable import project (PLS-VIP) showed that there were 29 volatile compounds that had an important contribution to the aroma characteristics of Congou black tea, and the volatile compounds that had an important influence on six aroma attributes were obtained.
Phase tunable second-order topological superconductor
Creators: name: Franca, S.
name: Efremov, D. V.
name: Fulga, I. C.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Two-dimensional second-order topological superconductors (SOTSCs) have gapped bulk and edge states, with zero-energy Majorana bound states localized at corners. Motivated by recent advances in Majorana nanowire experiments, we propose to realize a tunable SOTSC as a two-dimensional nanowire array. We show that the coupling between the Majorana modes of adjacent wires can be controlled by phase-biasing the device, allowing to access a variety of topological phases. We characterize the system using scattering theory, which provides access to its transport properties and its topological invariants. The setup is robust against disorder, both in the nanowires themselves and in the Josephson junctions formed between adjacent wires. Further, we identify a parameter regime in which an initially trivial system is rendered topological upon adding disorder, providing an example of a second-order topological Anderson phase.
description: 8 + 7 pages, 7 + 2 figures; the published version
title: Considering Cruelty: Animals in Contemporary Art
Creators: name: Hughes, Angela
Publisher: name: Griffith University
Year: 2015
Subjects: subject: Animals in art
subject: Animal exploitation
subject: Art criticism
subject: Art and society

description: Animals have been represented in art from earliest times, emphasising the integral roles they have played within human civilisation as labourers, food, entertainment, spiritual influences and companions. In contemporary society, this representation has come to include the use of physical animals in art, often causing their harm or death. This research investigates the exploitation of animals in the making of contemporary art. It asks how art is complicit in furthering the exploitation of animals within society more broadly, and describes the artwork made in order to evoke a discussion of these cruelties and educate viewers about how society treats animals. Key themes surrounding the different types of exploitation that animals endure within art and society are identified. These themes include: use of the animal as metaphor; violence towards animals in art; how these types of shocking exploitation have the ability to normalise cruelty to animals within society; hypocrisy and the placing of blame as effective ways of looking at the artist–viewer relationship; speciesism and anthropomorphism as at the base of these exploitative practices, with particular emphasis on art that causes harm to ‘lesser’ animals, such as insects and rodents; the animal as an artistic medium; and the concept of education as a solution to this enduring problem. Each theme is approached from the perspective of art criticism while discussing the impact on and by society.
Implications of Variability Patterns observed in TeV Blazars on the Structure of the Inner Jet
Creators: name: Tanihata, Chiharu
name: Takahashi, Tadayuki
name: Kataoka, Jun
name: Madejski, Greg M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The recent long look X-ray observations of TeV blazars have revealed many important new features concerning their time variability. In this paper, we suggest a physical interpretation for those features based on the framework of the internal and external shock scenarios. We present a simplified model applicable to TeV blazars, and investigate through simulations how each of the model parameters would affect to the observed light curve or spectrum. In particular, we show that the internal shock scenario naturally leads to all the observed variability properties including the structure function, but for it to be applicable, the fractional fluctuation of the initial bulk Lorentz factors must be small, with sigma_gamma / gamma_average < 0.01. This implies very low dynamical efficiency of the internal shock scenario. We also suggest that several observational quantities -- such as the characteristic time scale, the relative amplitude of flares as compared to the steady (``offset'') component, and the slope of the structure function -- can be used to probe the inner jet. The results are applied to the TeV blazar Mrk421, and this, within the context of the model, leads to the determination of several physical parameters: the ejection of a shell with average thickness of ~1E13 cm occurs on average every 10 minutes, and the shells collide ~1E17 cm away from the central source.
description: 12 pages, 13 figures, to appear in ApJ
Cantharocnemis spondyloides SERVILLE 1832
Creators: name: Adlbauer, K.
name: Ayalew, Amare
name: Beck, R.
name: Drumont, A.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cerambycidae
Cantharocnemis
Cantharocnemis spondyloides

description: Cantharocnemis (s.str.) spondyloides SERVILLE 1832
M a t e r i a l:5 Umg. Konso, Omo Reg., Gamo Gofa, IV.-V.1992 und VI.2004, C. Di Gennaro leg., in Coll. A. Drumont. – 5 8 Prov. Gamo Gofa, 6°37´N / 37°8´E, IV.1994, R.C. Owen leg., in Coll. A. Drumont. – 2 4 Arba Minch, IV.1994, K. Werner leg., in Coll. A. Drumont. – 2 1 Arba Minch, 1300-1500 m, 24.V.-4.VI.1999, R. Beck leg. und 16.IV.- 3.V.2001, R. Beck und G. Riedel leg. – 4 Sof Omar, Bale, IV.2005, C. Di Gennaro leg., in Coll. A. Drumont. – 2 15 km und 50 km SE Jabelo, Sidano, 15.IV.und 18.IV.2007, K. Werner leg., in Coll. A. Drumont.
V: Mauretanien, Senegal, Mali, Burkina Faso, Niger, Ägypten, Saudi Arabien, Yemen, Sudan, Äthiopien, Eritrea, Djibouti, Somalia, Kenya, Uganda, Tanzania, Botswana, Namibia (ADLBAUER 1999a). Erst kürzlich wurde die Art auch von Oman und RSA bekannt (DRUMONT 2004).
description: Published as part of Adlbauer, K., Ayalew, Amare, Beck, R. & Drumont, A., 2008, Cerambyciden aus Äthiopien (Coleoptera, Cerambycidae), pp. 1153-1191 in Linzer biologische Beiträge 40 (2) on page 1156, DOI: 10.5281/zenodo.5430603
Parajungiella pseudolongicornis CR
Creators: name: Omelková, Markéta
name: Ježek, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psychodidae
Parajungiella
Parajungiella pseudolongicornis

description: Parajungiella pseudolongicornis (Wagner, 1975) (CR)
 Published records. Citonice, Čížov, Horní Břečkov, Fládnická chata hut, Lesná (JEŽEK 2003), Hnanice, Horní Břečkov, Čížovský rybník pond, Faltýskův Mlýn, Devět Mlýnů (JEŽEK et al. 2005).
 Material examined. Citonice, Na hájkách (8), 2 JJ, v., Inv. No. 6057 and 6062; Čížov, rills (15), J, v., Inv. No. 6039; Hnanice, Devět Mlýnů (16), J, vi., Inv. No. 8349; Vranov nad Dyjí, Lesná (31), 2 JJ, v., Inv. No. 6023 and 6025.
 Comment. A rare species, recorded only from Great Britain, Ireland, Austria, Czech Republic, Slovakia, Bosnia and Herzegovina, and Serbia. It occurs in habitats with decaying organic matter (ponds, brooks, meanders of rivers, rills and swamps). Critically endangered in the Czech Republic.
description: Published as part of Omelková, Markéta & Ježek, Jan, 2012, A new species of the genus Trichomyia (Diptera: Psychodidae) and new faunistic data on non-phlebotomine moth flies from the Podyjí NP and its surroundings (Czech Republic), pp. 505-533 in Acta Entomologica Musei Nationalis Pragae 52 (2) on page 520, DOI: 10.5281/zenodo.5332309
title: Factors in the Adoption of solar Domestic Hot water Systems in Brisbane (SEQ)
Creators: name: Thetadig, Rita Ah Wa
Publisher: name: Griffith University
Year: 2009
Subjects: subject: Solar hot water systems
subject: Solar domestic hot water technology

description: The economical, technological and environmental viability of Solar Domestic Hot Water (SDHW) technology is well established. Its potential role as a major contributor to meeting residential hot water needs is the view promoted in this research and the major reason why it is taken up by users. There is also a need to explore the barriers preventing a household’s adoption of Solar Domestic Hot Water (SDHW), particularly in Queensland, the “Sunshine State” of Australia. This research is based on eight hypotheses, suggesting factors that may be related to the household decision to adopt solar. A household survey collected data to test the hypotheses in an effort to explain underlying factors that influence the pattern of household take-up as evident in Brisbane, South East Queensland. The research identified the following factors as important to the adoption of solar domestic hot water: 1. Newspapers/magazines and personal recommendations by friends and relatives are key sources of information that households access when making a decision on SDHW; 2. There are five other factors which help explain both organizational subsystems and behavioral subsystems as having a relationship with household adoption of SDHW. These are: factors related to energy suppliers, operating factors, government initiatives (specifically SDHW Rebate), environmental issues; namely attractiveness of the system because solar energy is renewable and socio-economic factor such as the presence of ‘Other’ household residents in occupational groups, in particular, managers and administrators; 3. The findings offer evidence to enhance issues already identified in previous work and pursued in the current research on SDHW in Queensland (Berrill 1991), which identifies socio-political and environmental issues, as two of the three issues relating to “Quality of life”. The third economic issue is also looked at in this research. 4. New findings are evident in support of interrelationships’ between socio-political, energy supply systems and technological awareness factors, namely Government Rebate, Energy Supplier and Operating Factors and the household decision to adopt SDHW; 5. The findings offer an explanation as to why technological factors pertaining to SDHW and factors involved in assessing satisfaction with the system have been misunderstood. The results clearly indicate an overwhelming satisfaction with the SDHW system; 6. This research contributes to the body of research in this area, especially as it puts forward evidence of why socio-economic characteristics of household’s are a fundamental aspect in understanding the adoption of SDHW. It provides households’ perspectives to the identified issues that directly affect them. These perspectives can then be incorporated into the identification, development and implementation of public and private energy policy.
Additional file 2: of The experience of parents of children with rare diseases when communicating with healthcare professionals: towards an integrative theory of trust
Creators: name: Gómez-Zúñiga, Beni
name: Moyano, Rafael Pulido
name: Fernández, Modesta Pousada
name: Oliva, Alicia García
name: Ruiz, Manuel Armayones
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Blocks and categories built through the analysis. (DOCX 7 kb)
Idactus usambaricus HINTZ 1900
Creators: name: Adlbauer, K.
name: Ayalew, Amare
name: Beck, R.
name: Drumont, A.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cerambycidae
Idactus
Idactus usambaricus

description: Idactus usambaricus HINTZ 1900
M a t e r i a l:1 3 Arba Minch, 1300-1500 m, 10.-20.IX.2000, 16.IV.-3.V.2001, V.2004 und 1110 m, V.2001, R. Beck leg.
 A: Der aus Arba Minch beschriebene Idactus konso QUENTIN & VILLIERS 1981, mit dem unsere Exemplare ebenfalls gut übereinstimmen, ist mit hoher Wahrscheinlichkeit ein Synonym von I. usambaricus, der seinerseits eine Subspezies von I. ellioti GAHAN 1890 sein soll (J. Sudre, in litteris).
V: Äthiopien, Uganda, Kenya, Tanzania, Zimbabwe (ADLBAUER 2000a).
description: Published as part of Adlbauer, K., Ayalew, Amare, Beck, R. & Drumont, A., 2008, Cerambyciden aus Äthiopien (Coleoptera, Cerambycidae), pp. 1153-1191 in Linzer biologische Beiträge 40 (2) on page 1174, DOI: 10.5281/zenodo.5430603
AYRIM XORIJIY DAVLATLARDA EKOLOGIYA SOHASIDAGI JINOIY JAVOBGARLIK MASALALARI
Creators: name: Akramova, Marjona
Publisher: name: Zenodo
Year: 2024

description: Hozirgi kunda dunyoning barcha mintaqalarida ekologik vaziyat dolzarbligicha qolayotgan bir sharoitda ekologik jinoyatlar uchun jinoiy javobgarlikni kuchaytirish, ayrim ekologik huquqbuzarliklarga jinoiy tus berish ekologik barqarorlikning kafolatlaridan biri ekanligini inobatga olgan holda, ushbu tezisda xorijiy davlatlarning ekologik qonunchiligi tahlil qilingan. Shuningdek, rivojlangan mamlakatlarning jinoyat huquqida ekologik jinoyatlarning tavsifi va ular uchun belgilangan jinoiy jazoning xususiyatlari muhokama qilingan.
A Limit on the Metallicity of Compact High Velocity Clouds
Creators: name: Sembach, Kenneth R.
name: Gibson, Brad K.
name: Fenner, Yeshe
name: Putman, Mary E.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: There is a fortuitous coincidence in the positions of the quasar TonS210 and the compact H I high velocity cloud CHVC224.0-83.4-197 on the sky. Using Far Ultraviolet Spectroscopic Explorer observations of the metal-line absorption in this cloud and sensitive H I 21cm emission observations obtained with the multibeam system at Parkes Observatory, we determine a metallicity of (O/H) <0.46 solar at a confidence of 3 sigma. The metallicity of the high velocity gas is consistent with either an extragalactic or Magellanic Cloud origin, but is not consistent with a location inside the Milky Way unless the chemical history of the gas is considerably different from that of the interstellar medium in the Galactic disk and halo. Combined with measurements of highly ionized species (C III and O VI) at high velocities, this metallicity limit indicates that the cloud has a substantial halo of ionized gas; there is as much ionized gas as neutral gas directly along the Ton S210 sight line. We suggest several observational tests that would improve the metallicity determination substantially and help to distinguish between possible origins for the high velocity gas. Additional observations of this sight line would be valuable since the number of compact HVCs positioned in front of background sources bright enough for high resolution absorption-line studies is extremely limited.
description: 15 pages, 3 postscript figures + 1 JPEG figure (reduced from postscript for size considerations), accepted for publication in ApJ (June 2002)
Idactus exiguus
Creators: name: Adlbauer, K.
name: Ayalew, Amare
name: Beck, R.
name: Drumont, A.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cerambycidae
Idactus
Idactus exiguus

description: Idactus exiguus (QUEDENFELDT 1891)
M a t e r i a l:1 Arba Minch, 1440 m, 21.-23.X.2003, R. Beck leg.
V: Mali, Côte d´Ivoire, Kamerun, Rep. Centrafricaine, Tanzania, Mocambique, Zimbabwe, RSA (TÉOCCHI 1997, ADLBAUER 2000b).
Erste Meldung aus Äthiopien.
description: Published as part of Adlbauer, K., Ayalew, Amare, Beck, R. & Drumont, A., 2008, Cerambyciden aus Äthiopien (Coleoptera, Cerambycidae), pp. 1153-1191 in Linzer biologische Beiträge 40 (2) on page 1174, DOI: 10.5281/zenodo.5430603
Quantized thermal Hall conductance from edge current calculations in lattice models
Creators: name: Tang, Wei
name: Xie, X. C.
name: Wang, Lei
name: Tu, Hong-Hao
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The quantized thermal Hall effect is an important probe for detecting chiral topological order and revealing the nature of chiral gapless edge states. The standard Kubo formula approach for the thermal Hall conductance $κ_{xy}$ based on the linear-response theory faces difficulties in practical application due to the lack of a reliable numerical method for calculating dynamical quantities in microscopic models at finite temperature. In this work, we propose an approach for calculating $κ_{xy}$ in two-dimensional lattice models displaying chiral topological order. Our approach targets at the edge current localized at the boundary which involves only thermal averages of local operators in equilibrium, thus drastically lowering the barrier for the calculation of $κ_{xy}$. We use the chiral $p$-wave superconductor (with and without disorder) and the Hofstadter model as benchmark examples to illustrate several sources of finite-size effects, and we suggest the infinite (or sufficiently long) strip as the best geometry for carrying out numerical simulations.
description: 12 pages, 9 figures, published version
The Galaxy Luminosity Function and Luminosity Density at Redshift z=0.1
Creators: name: Blanton, Michael R.
name: Hogg, David W.
name: Brinkmann, J.
name: Connolly, Andrew J.
name: Csabai, Istvan
name: Bahcall, Neta A.
name: Fukugita, Masataka
name: Loveday, Jon
name: Meiksin, Avery
name: Munn, Jeffrey A.
name: Nichol, R. C.
name: Okamura, Sadanori
name: Quinn, Thomas
name: Schneider, Donald P.
name: Shimasaku, Kazuhiro
name: Strauss, Michael A.
name: Tegmark, Max
name: Vogeley, Michael S.
name: Weinberg, David H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using a catalog of 147,986 galaxy redshifts and fluxes from the Sloan Digital Sky Survey (SDSS) we measure the galaxy luminosity density at z=0.1 in five optical bandpasses corresponding to the SDSS bandpasses shifted to match their restframe shape at z=0.1. We denote the bands {0.1}{u}, {0.1}{g}, {0.1}{r}, {0.1}{i}, {0.1}{z}, with λ_{eff} = [3216, 4240, 5595, 6792, 8111] Angstroms respectively. We use a maximum likelihood method which allows for a general form for the shape of the luminosity function, simple luminosity and number evolution, incorporates flux uncertainties, and accounts for the flux limits of the survey. We find luminosity densities at z=0.1 in absolute AB magnitudes in a Mpc^3 of [-14.10 \pm 0.15, -15.18 \pm 0.03, -15.90 \pm 0.03, -16.24 \pm 0.03, -16.56 \pm 0.02] in [{0.1}{u}, {0.1}{g}, {0.1}{r}, {0.1}{i}, {0.1}{z}], respectively, using Ω_0 =0.3, Ω_Λ=0.7, and h=1, and using Petrosian magnitudes. Similar results are obtained using Sersic model magnitudes, suggesting that flux from outside the Petrosian apertures is not a major correction. In the {0.1}{r} band, the best fit Schechter function to our results has ϕ_\ast = (1.49 \pm 0.04) \times 10^{-2} h^3 Mpc^{-3}, M_\ast - 5\log_{10} h = -20.44 \pm 0.01, and α= -1.05\pm 0.01. In solar luminosities, the luminosity density in {0.1}{r} is (1.84 \pm 0.04) h 10^8 L_{{0.1}{r},\odot} Mpc^{-3}. Our results are consistent with other estimates of the luminosity density, from the Two-degree Field Galaxy Redshift Survey and the Millenium Galaxy Catalog. They represent a substantial change (\sim 0.5 mag) from earlier SDSS luminosity density results based on commissioning data, almost entirely because of the inclusion of evolution in the luminosity function model.
description: submitted to ApJ
Additional file 1: of The experience of parents of children with rare diseases when communicating with healthcare professionals: towards an integrative theory of trust
Creators: name: Gómez-Zúñiga, Beni
name: Moyano, Rafael Pulido
name: Fernández, Modesta Pousada
name: Oliva, Alicia García
name: Ruiz, Manuel Armayones
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: Plant Biology

description: Interviews guidelines for data collection. (DOCX 19 kb)
Paramormia (Paramormia) polyascoidea
Creators: name: Omelková, Markéta
name: Ježek, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psychodidae
Paramormia
Paramormia polyascoidea

description: Paramormia (Paramormia) polyascoidea (Krek, 1971)
 Published records. Horní Břečkov (JEŽEK et al. 2005).
 Material examined. Horní Břečkov, pond (26), J, v., Inv. No. 5345.
 Comment. A European and western Siberian species known from Germany, Great Britain, Czech Republic, Poland, Austria, Bosnia and Herzegovina, Abkhazia (Caucasus) and Russia (Novosibirsk region). It has been collected in swampy meadows and pastures, spring areas, alongside brooks, near ponds, and in bottomlands of meandering flows from lowland to mountains.
description: Published as part of Omelková, Markéta & Ježek, Jan, 2012, A new species of the genus Trichomyia (Diptera: Psychodidae) and new faunistic data on non-phlebotomine moth flies from the Podyjí NP and its surroundings (Czech Republic), pp. 505-533 in Acta Entomologica Musei Nationalis Pragae 52 (2) on page 520, DOI: 10.5281/zenodo.5332309
title: Natural Product and Fragment-Based Drug Discovery Against Malaria Protein Targets by Native Mass Spectrometry
Creators: name: Pedro, Liliana Antunes
Publisher: name: Griffith University
Year: 2017
Subjects: subject: Malaria control
subject: Plasmodium falciparum (P. falciparum)
subject: Plasmodium vivax (P. vivax)
subject: Fragment-based drug discovery (FBDD)
subject: Native mass spectrometry

description: Malaria control interventions have been effective in reducing malaria incidence and mortality rates globally over the last decade. However, increasing resistance of Plasmodium falciparum (P. falciparum) and Plasmodium vivax (P. vivax), the two most prevalent parasite species, to the most used antimalarial drugs, threatens to halt the progress. Given the current limited arsenal of antimalarial drugs has been inspired by natural product scaffolds, these have the potential to be the source of new and structurally different antimalarial drugs, acting through novel mechanisms of action, that are urgently needed. Translating the structural and biologically relevant diversity of natural products into an efficient and effective drug development process is, nonetheless, not trivial. Fragment-based drug discovery (FBDD) is a relatively recent and promising approach for drug discovery. It involves the identification of small molecular weight compounds, called fragments, that weakly bind to a biological target and their elaboration through chemical synthesis to produce high affinity and selective drugs. For a rational and effective elaboration process, structural and thermodynamic information are essential.
ПРИМЕНЕНИЯ РЕСУРСОВ СЕТИ ИНТЕРНЕТ В ОБРАЗОВАТЕЛЬНОМ ПРОЦЕССЕ
Creators: name: Нуридинова, Зарнигор
name: Нуридинов, Зухриддин
Publisher: name: Zenodo
Year: 2024

description: Статья оценивает значимость адаптации учебного материала в контексте преподавания русского языка как иностранного. Авторы исследуют процесс адаптации с учетом различных аспектов, включая уровень языковой подготовки студентов, культурные особенности, их потребности и предпочтения.
Paramormia (Duckhousiella) ustulata
Creators: name: Omelková, Markéta
name: Ježek, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Psychodidae
Paramormia
Paramormia ustulata

description: Paramormia (Duckhousiella) ustulata (Walker, 1856)
 Material examined. Hnanice, Šobes vineyard and Nad papírnou hills (45), ♀, viii., Inv. No. 8356; Štítary, village vicinity (51), J, viii., Inv. No. 6789; Vrbovec, Vrbovecký potok brook (60), J, vi., Inv. No. 7586.
 Comment. Known from most of Europe, very common locally mainly on extreme localities (salt works, thermal springs, calcareous water, mineral-rich springs). Recorded as well in Algeria, Morocco, Israel, Afghanistan, Iran, and USA.
description: Published as part of Omelková, Markéta & Ježek, Jan, 2012, A new species of the genus Trichomyia (Diptera: Psychodidae) and new faunistic data on non-phlebotomine moth flies from the Podyjí NP and its surroundings (Czech Republic), pp. 505-533 in Acta Entomologica Musei Nationalis Pragae 52 (2) on page 520, DOI: 10.5281/zenodo.5332309
The EXPLORE Project I: A Deep Search for Transiting Extrasolar Planets
Creators: name: Mallen-Ornelas, G.
name: Seager, S.
name: Yee, H. K. C.
name: Minniti, D.
name: Gladders, M. D.
name: Mallen-Fullerton, G.
name: Brown, T. M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (Abridged) We discuss the design considerations of the EXPLORE (EXtra-solar PLanet Occultation REsearch) project, a series of transiting planet searches using 4-m-class telescopes to continuously monitor a single field of stars in the Galactic Plane in each ~2 week observing campaign. We discuss the general factors which determine the efficiency and the number of planets found by a transit search, including time sampling strategy and field selection. The primary goal is to select the most promising planet candidates for radial velocity follow-up observations. We show that with very high photometric precision light curves that have frequent time sampling and at least two detected transits, it is possible to uniquely solve for the main parameters of the eclipsing system (including planet radius) based on several important assumptions about the central star. Together with a measured spectral type for the star, this unique solution for orbital parameters provides a powerful method for ruling out most contaminants to transiting planet candidates. For the EXPLORE project, radial velocity follow-up observations for companion mass determination of the best candidates are done on 8-m-class telescopes within two or three months of the photometric campaigns. This same-season follow-up is made possible by the use of efficient pipelines to produce high quality light curves within weeks of the observations. We conclude by presenting early results from our first search, EXPLORE I, in which we reached <1% rms photometric precision (measured over a full night) on ~37,000 stars to I <= 18.2.
description: accepted by ApJ. Main points unchanged but more thorough discussion of some issues. 36 pages, including 14 figures