cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The MOSDEF survey: a census of AGN-driven ionized outflows at $z = 1.4-3.8$
Creators: name: Leung, Gene C. K.
name: Coil, Alison L.
name: Aird, James
name: Azadi, Mojegan
name: Kriek, Mariska
name: Mobasher, Bahram
name: Reddy, Naveen
name: Shapley, Alice
name: Siana, Brian
name: Fetherolf, Tara
name: Fornasini, Francesca M.
name: Freeman, William R.
name: Price, Sedona H.
name: Sanders, Ryan L.
name: Shivaei, Irene
name: Zick, Tom
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Using data from the MOSFIRE Deep Evolution Field (MOSDEF) survey, we present a census of AGN-driven ionized outflows in a sample of 159 AGNs at $1.4 \le z \le 3.8$. The sample spans AGN bolometric luminosities of $10^{44-47} \mathrm{~erg~s}^{-1}$ and includes both quiescent and star-forming galaxies extending across three orders of magnitude in stellar mass. We identify and characterize outflows from the \hbeta, [OIII], \halpha ~and [NII] emission line spectra. We detect outflows in $17\%$ of the AGNs, seven times more often than in a mass-matched sample of inactive galaxies in MOSDEF. The outflows are fast and galaxy-wide, with velocities of $\sim 400-3500 ~\mathrm{km~s}^{-1}$ and spatial extents of $0.3-11.0$ kpc. The incidence of outflows among AGNs is independent of the stellar mass of the host galaxy, with outflows detected in both star-forming and quiescent galaxies. This suggests that outflows exist across different phases in galaxy evolution. We investigate relations between outflow kinematic, spatial, and energetic properties and both AGN and host galaxy properties. Our results show that AGN-driven outflows are widespread in galaxies along the star-forming main sequence. The mass-loading factors of the outflows are typically $0.1-1$ and increase with AGN luminosity, capable of exceeding unity at $L_\mathrm{AGN} \gtrsim 10^{46.3} \mathrm{~erg~s}^{-1}$. In these more luminous sources the ionized outflow alone is likely sufficient to regulate star formation, and when combined with outflowing neutral and molecular gas may be able to quench star formation in their host galaxies.
description: 24 pages, 12 figures, accepted for publication in the The Astrophysical Journal
title: The History of School Brass Bands in Australia
Creators: name: Boulton, Veronica S
Publisher: name: Griffith University
Year: 2023
Subjects: subject: Australian music education
subject: brass bands
subject: music education history

description: There are currently very few brass bands in schools in Australia, however they were the predominant music ensemble in Australian schools up to the 1970s. The aim of this research is to examine the history and current existence of British-style brass bands in schools in Australia, as well as to consider what the future looks like for Australian brass band musicians. The history of the brass band in Australia and its decline is explored, drawing on historical and scholarly research, and examining various primary sources, such as newspaper articles and photographs, and personal accounts recovered through qualitative interviews. British immigration to Australia played a significant role in shaping the brass band movement, which was distinctly male-dominated and had strong links to the military culture of the first half of the twentieth century. These societal trends followed into the school brass band setting. From the 1970s there were a variety of factors that influenced the gradual change from brass band to concert band in schools in Australia. The current situation for students playing brass band instruments in Australia is examined, with a particular focus on the Salvation Army Just Brass program that has been running brass bands in primary schools for over a decade. The dissertation concludes with an examination of what a career looks like in the 21st century for a musician, with a focus on the availability of higher education courses for players of brass band instruments in Australia, as well as other parts of the world. This research provides a better understanding of the brass band tradition within the context of the school environment in Australia and calls for further research and scholarly inclusion in the literature of music education.
Anisops nasutus Fieber 1851
Creators: name: Zettel, Herbert
name: Lane, David J. W.
name: Pangantihon, Clister V.
name: Freitag, Hendrik
name: Be, Jalan Tungku Link
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Notonectidae
Anisops
Anisops nasutus

description: Anisops nasutus Fieber, 1851
(Fig. 3)
 Anisops nasuta Fieber, 1851: 60; BROOKS (1951: 416).
 Anisops nasutus: NIESER & CHEN (1999: 110); ZETTEL (2003: 126); CHEN et al. (2005: 421); NIESER et al. (2008: 261).
 Material examined. BRUNEI: BRUNEI- MUARA DISTRICT: west of Bandar Seri Begawan, south of Jerudong, large artificial lake, 5 m a.s.l., 04°55′03.0″N 114°49′54.3″E (GPS), 3.xii.2008, leg. H. Zettel & D. J. W. Lane (# 36), 1 J 3 ♀♀ (UBDB, NHMW). PHILIPPINES: BOHOL: northern Bohol, southwest of Talibon, Zamora Dam, 25 m a.s.l., pond, 9.xi.2007, leg. H. Zettel (474b), 5 JJ (NHMW, UPLB, HFDG), leg. C. V. Pangantihon (PC474b), 4 JJ (HZWA).
 Distribution. Anisops nasutus is widely distributed from India to Australia (CHEN et al. 2005). However, listed materials represent the first record from Brunei and the entire island of Borneo. Regarding the Philippines, an unspecific record by NIESER & CHEN (1999) was cited by ZETTEL (2003), but not repeated by CHEN et al. (2005), and was specified ‘Mindanao’ by NIESER et al. (2008). The examined specimens represent the first record from Bohol Island.
description: Published as part of Zettel, Herbert, Lane, David J. W., Pangantihon, Clister V., Freitag, Hendrik & Be, Jalan Tungku Link, 2012, Notes on Notonectidae (Hemiptera: Heteroptera) from southeastern Asia, mostly from Brunei and the Philippines, pp. 29-48 in Acta Entomologica Musei Nationalis Pragae 52 (1) on page 32, DOI: 10.5281/zenodo.5330381
Ultra-High Energy Cosmic Rays and Neutron-Decay Halos from Gamma Ray Bursts
Creators: name: Dermer, C. D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Simple arguments concerning power and acceleration efficiency show that ultra-high energy cosmic rays (UHECRS) with energies >~ 10^{19} eV could originate from GRBs. Neutrons formed through photo-pion production processes in GRB blast waves leave the acceleration site and travel through intergalactic space, where they decay and inject a very energetic proton and electron component into intergalactic space. The neutron-decay protons form a component of the UHECRs, whereas the neutron-decay electrons produce optical/X-ray synchrotron and gamma radiation from Compton-scattered background radiation. A significant fraction of galaxies with GRB activity should be surrounded by neutron-decay halos of characteristic size ~ 100 kpc.
description: 3 pages, in 2nd Rome Workshop on Gamma Ray Bursts in the Afterglow Era (17-20 October 2000)
MOESM2 of Regulatory effect of Garidisan on dysbiosis of the gut microbiota in the mouse model of ulcerative colitis induced by dextran sulfate sodium
Creators: name: Pei, Ling-yan
name: Ke, Yu-shi
name: Zhao, Huan-hu
name: Liu, Wei-zhi
name: Wang, Lin
name: Jia, Chao
name: Shi, Meng-ni
name: Fu, Qian-hui
name: Cui, Jian
name: Li, Shu-chun
Publisher: name: figshare
Year: 2019
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified

description: Additional file 2: Table S2. GC-MC (Phylum level) Metastat analysis.
The Nucleosynthetic Signature of Population III
Creators: name: Heger, A.
name: Woosley, S. E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Growing evidence suggests that the first generation of stars may have been quite massive (~100-300 M_sun). Could these stars have left a distinct nucleosynthetic signature? We explore the nucleosynthesis of helium cores in the mass range M_He=64 to 133 Msun, corresponding to main-sequence star masses of approximately 140 to 260 M_sun. Above M_He=133 M_sun, without rotation and using current reaction rates, a black hole is formed and no nucleosynthesis is ejected. For lighter helium core masses, ~40 to 63 M_sun, violent pulsations occur, induced by the pair instability and accompanied by supernova-like mass ejection, but the star eventually produces a large iron core in hydrostatic equilibrium. It is likely that this core, too, collapses to a black hole, thus cleanly separating the heavy element nucleosynthesis of pair instability supernovae from those of other masses, both above and below. Indeed, black hole formation is a likely outcome for all Population III stars with main sequence masses between about 25 M_sun and 140 M_sun (M_He = 9 to 63 M_sun) as well as those above 260 M_sun. Nucleosynthesis in pair-instability supernovae varies greatly with the mass of the helium core which determines the maximum temperature reached during the bounce. At the upper range of exploding core masses, a maximum of 57 M_sun of Ni56 is produced making these the most energetic and the brightest thermonuclear explosions in the universe. Integrating over a distribution of masses, we find that pair instability supernovae produce a roughly solar distribution of nuclei having even nuclear charge, but are remarkably deficient in producing elements with odd nuclear charge. Also, essentially no elements heavier than zinc are produced due to a lack of s- and r-processes.
description: 20 pages, including 5 figures; accepted by ApJ
The cost-effectiveness of isavuconazole compared to the standard of care in the treatment of patients with invasive fungal infection prior to differential pathogen diagnosis in the United Kingdom
Creators: name: Lefteris Floros
name: Pagliuca, Antonio
name: Taie, Amer Al
name: Weidlich, Diana
name: Capparella, Maria Rita
name: Mihalina Georgallis
name: Sung, Anita Hor-Yun
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Aims: To estimate the cost-effectiveness of isavuconazole compared with the standard of care, voriconazole, for the treatment of patients with invasive fungal infection disease when differential diagnosis of the causative pathogen has not yet been achieved at treatment initiation. Materials and methods: The economic model was developed from the perspective of the UK National Health Service (NHS) and used a decision-tree approach to reflect real-world treatment of patients with invasive fungal infection (IFI) prior to differential pathogen diagnosis. It was assumed that 7.8% of patients with IFI prior to differential pathogen diagnosis at treatment initiation actually had mucormycosis, and confirmation of pathogen identification was achieved for 50% of all patients during treatment. To extrapolate to a lifetime horizon, the model considered expected survival based on the patients’ underlying condition. The model estimated the incremental costs (costs of drugs, laboratory analysis, hospitalization, and management of adverse events) and clinical outcomes (life-years (LYs) and quality-adjusted life-years (QALYs)) of first-line treatment with isavuconazole compared with voriconazole. The robustness of the results was assessed by conducting deterministic and probabilistic sensitivity analyses. Results: Isavuconazole delivered 0.48 more LYs and 0.39 more QALYs per patient at an incremental cost of £3,228, compared with voriconazole in the treatment of patients with IFI prior to differential pathogen diagnosis. This equates to an incremental cost-effectiveness ratio (ICER) of £8,242 per additional QALY gained and £6,759 per LY gained. These results were driven by a lack of efficacy of voriconazole in mucormycosis. Results were most sensitive to the mortality of IA patients and treatment durations. Conclusions: At a willingness to pay (WTP) threshold of £30,000 per additional QALY, the use of isavuconazole for the treatment of patients with IFI prior to differential pathogen diagnosis in the UK can be considered a cost-effective allocation of healthcare resources compared with voriconazole.
title: The Provenance of Sediment in Three Rural Catchments in South East Queensland, Australia
Creators: name: Laceby, John Patrick
Publisher: name: Griffith University
Year: 2012
Subjects: subject: Moreton Bay
subject: Ramsar wetland
subject: Blackfellow Creek catchment
subject: Knapp Creek catchment
subject: Upper Bremer River catchment
subject: Bay ecosystems

description: Moreton Bay, in South East Queensland, Australia, is a Ramsar wetland of international significance. A decline of the bay’s ecosystem health has been primarily attributed to sediments and nutrients from catchment sources. The Healthy Country (HC) project, a Queensland Government funded ‘proof of concept’ initiative, is dedicated to reducing rural diffuse sediments and nutrients entering waterways and ultimately Moreton Bay. Three focal catchments, Blackfellow Creek, Knapp Creek and the Upper Bremer River, were selected to trial rehabilitation techniques for the region. Sediment budgets for these focal catchments, developed using catchment scale modelling (SedNet), indicated gully erosion dominates the supply of sediment in Knapp Creek (90%) and the Upper Bremer River (80%) whereas erosion from cultivated soils is the primary sediment source in Blackfellow Creek (40%). These sediment budgets, that include predictions of both the spatial sources of sediment and the primary erosion processes, form a series of hypotheses in each focal catchment that are tested in this thesis. Fallout-radionuclide activity concentrations (137Cs and 210Pbex) of in-stream sediment sampled in each focal catchment were used in conjunction with regional source data to test hypotheses pertaining to dominant erosion processes, specifically the relative sediment contributions from surface and subsoil (gully and channel bank) sources. Distribution modelling results indicated subsoil erosion processes dominate the supply of sediment in both Knapp Creek (100%) and the Upper Bremer River (100%). In Blackfellow Creek, the similarity of cultivated (surface) and subsoil source fallout-radionuclide activity concentrations resulted in no discrimination between these sources that were modelled in combination to contribute >90% of sediments. Importantly there was no discrimination between gully and channel bank erosion sources in Knapp Creek and the Upper Bremer River.
Extremely hard GRB spectra prune down the forest of emission models
Creators: name: Ghirlanda, Giancarlo
name: Celotti, Annalisa
name: Ghisellini, Gabriele
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We consider the evidence for very hard low energy spectra during the prompt phase of Gamma-Ray Bursts (GRB). In particular we examine the spectral evolution of GRB 980306 together with the detailed analysis of some other bursts already presented in the literature (GRB 911118, GRB 910807, GRB 910927 and GRB 970111), and check for the significance of their hardness (i.e. extremely steep spectral slopes below the $EF_{E}$ peak) by applying different tests. These bursts, detected by the Burst And Transient Source Experiment (BATSE) in the $\sim 30$ keV -- 2 MeV energy range, are sufficiently bright to allow time resolved spectral studies on time intervals of the order of tenths of a second. We discuss the hard spectra of these bursts and their evolution in the context of several non--thermal emission models, which all appear inadequate to account for these cases. The extremely hard spectra, which are detected in the early part of the BATSE light curve, are also compared with a black body spectral model: the resulting fits are remarkably good, except for an excess at high energies (in several cases) which could be simply accounted for by the presence of a supra--thermal component. The findings on the possible thermal character of the evolving spectrum and the implications on the GRB physical scenario are considered in the frameworks of photospheric models for a fireball which is becoming optically thin, and of Compton drag models, in which the fireball boosts "ambient" seed photons by its own bulk motion. Both models, according to simple estimates, appear to be qualitatively and quantitatively consistent with the found spectral characteristics, although their possible caveats are discussed.
description: 14 pages, 10 figures, 2 tables - Accepted for publication in Astronomy & Astrophysics
Anisops nigrolineatus Lundblad 1933
Creators: name: Zettel, Herbert
name: Lane, David J. W.
name: Pangantihon, Clister V.
name: Freitag, Hendrik
name: Be, Jalan Tungku Link
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Notonectidae
Anisops
Anisops nigrolineatus

description: Anisops nigrolineatus Lundblad, 1933
 Anisops nigrolineata Lundblad, 1933: 160; BROOKS (1951: 409).
 Anisops nigrolineatus: NIESER & CHEN (1999: 120); ZETTEL (2003: 126); CHEN et al. (2005: 421); NIESER et al. (2008: 262).
 Material examined. BRUNEI: BELAIT DISTRICT: Sungai Ingei, Site C, pool on East bank opposite Base Camp, 04º09’26.66”N 114º43’06.51”E, 14.vi.2010, leg.D. J. W.Lane (#16), 1J (UBDB).Sungai Ingei, Site A, pool on East bank opposite Base Camp, 04º09’25.81”N 114º43’08.10”E, 14.vi.2010, leg. D. J. W. Lane (#17), 1 J (UBDB).
 Distribution. Anisops nigrolineatus is widely distributed from India to the Philippines and Java (NIESER & CHEN 1999, CHEN et al. 2005) and very common in southeastern Asia, especially Thailand (NIESER et al. 2008). However, listed materials represent the first record from Brunei and the entire island of Borneo.
description: Published as part of Zettel, Herbert, Lane, David J. W., Pangantihon, Clister V., Freitag, Hendrik & Be, Jalan Tungku Link, 2012, Notes on Notonectidae (Hemiptera: Heteroptera) from southeastern Asia, mostly from Brunei and the Philippines, pp. 29-48 in Acta Entomologica Musei Nationalis Pragae 52 (1) on page 32, DOI: 10.5281/zenodo.5330381
Theoretical Limitations of Self-Attention in Neural Sequence Models
Creators: name: Hahn, Michael
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computation and Language (cs.CL)
subject: Formal Languages and Automata Theory (cs.FL)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Transformers are emerging as the new workhorse of NLP, showing great success across tasks. Unlike LSTMs, transformers process input sequences entirely through self-attention. Previous work has suggested that the computational capabilities of self-attention to process hierarchical structures are limited. In this work, we mathematically investigate the computational power of self-attention to model formal languages. Across both soft and hard attention, we show strong theoretical limitations of the computational abilities of self-attention, finding that it cannot model periodic finite-state languages, nor hierarchical structure, unless the number of layers or heads increases with input length. These limitations seem surprising given the practical success of self-attention and the prominent role assigned to hierarchical structure in linguistics, suggesting that natural language can be approximated well with models that are too weak for the formal languages typically assumed in theoretical linguistics.
description: Accepted by: Transactions of the Association for Computational Linguistics
Oxybelus pilosus ARNOLD 1927
Creators: name: Dollfuss, H.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Crabronidae
Oxybelus
Oxybelus pilosus

description: Oxybelus pilosus ARNOLD 1927 (5, 8)
M a l a w i:3, 6, 85 km SE Lilongwe Dedza, 5.-12.I.2002, leg. J. Halada.
Z a m b i a: 1, 60 km W Solwezi, 4.-6.I.2003, leg. J. Halada; 1, 2, 45 km SE Kitwe, 12.- 15.I.2003, leg. J. Halada.
description: Published as part of Dollfuss, H., 2008, The Crabronid Wasps of the Genera Oxybelus LATREILLE 1796 and Brimocelus ARNOLD 1927 of " Biologiezentrum Linz " Collection in Linz, Austria (Hymenoptera, Apoidea, Crabronidae), pp. 463-505 in Linzer biologische Beiträge 40 (1) on page 487, DOI: 10.5281/zenodo.5428013
Direct observation of bimolecular reactions of ultracold KRb molecules
Creators: name: Hu, Ming-Guang
name: Liu, Yu
name: Grimes, David D.
name: Lin, Yen-Wei
name: Gheorghe, Andrei H.
name: Vexiau, Romain
name: Bouloufa-Maafa, Nadia
name: Dulieu, Olivier
name: Rosenband, Till
name: Ni, Kang-Kuen
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Quantum Gases (cond-mat.quant-gas)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Femtochemistry techniques have been instrumental in accessing the short time scales necessary to probe transient intermediates in chemical reactions. Here we take the contrasting approach of prolonging the lifetime of an intermediate by preparing reactant molecules in their lowest ro-vibronic quantum state at ultralow temperatures, thereby drastically reducing the number of exit channels accessible upon their mutual collision. Using ionization spectroscopy and velocity-map imaging of a trapped gas of potassium-rubidium molecules at a temperature of 500~nK, we directly observe reactants, intermediates, and products of the reaction $^{40}$K$^{87}$Rb + $^{40}$K$^{87}$Rb $\rightarrow$ K$_2$Rb$^*_2$ $\rightarrow$ K$_2$ + Rb$_2$. Beyond observation of a long-lived energy-rich intermediate complex, this technique opens the door to further studies of quantum-state resolved reaction dynamics in the ultracold regime.
description: 4 figures in main, 4 figures in SM, 2 table in SM
NGC 4314. IV. Photometry of Star Clusters with Hubble Space Telescope - History of Star Formation in the Vicinity of a Nuclear Ring
Creators: name: Benedict, G. Fritz
name: Howell, D. Andrew
name: Jorgensen, Inger
name: Kenney, Jeffrey D. P.
name: Smith, Beverly J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using HST WFPC2 images, we have obtained U, B, V, I, and H-alpha photometry for 76 star clusters in the nuclear star-forming ring of the barred spiral galaxy NGC 4314. These clusters are likely associated with an inner Inner Lindblad Resonance, or IILR. The blue colors and H-alpha emission for most of these clusters imply very young ages of 1-15 Myr. Age estimates based on several reddening-free parameters indicate that the present epoch of star formation has lasted at least 30 Myr. By estimating the masses of stars in the clusters and comparing with the H-alpha luminosity, we conclude that a significant fraction of ongoing star formation in the nuclear ring of NGC 4314 occurs in clusters. The cluster masses identify these as young open clusters, not young globular clusters. Further out in the galaxy, just exterior to the ring of young stars, previous ground-based observations revealed two symmetric stellar spiral arms which may be associated with an outer Inner Lindblad Resonance, or OILR. With our HST data, we have revealed part of this structure and its colors in more detail. The spiral arm colors are consistent with stellar ages between 40 and 200 Myr. The age difference between the inner ring of young stars (IILR) and the larger oval-like feature containing the blue arms (OILR) supports an interpretation of the morphology of the nuclear region of NGC 4314 that requires a reservoir of gas that becomes more compact over time. We speculate that as the gas distribution becomes more centrally concentrated, it interacts with these two resonances. Each resonance triggers star formation, resulting in two distinct epochs of star formation.
description: To appear in The Astronomical Journal, March 2002. For a version with higher quality figures, see http://clyde.as.utexas.edu/pub/galaxy/N4314NEW/AJPAPER/BenedictR7.ps.gz
The radio colour-colour diagram of Van der Laan bubbles - an application to SS433
Creators: name: Paragi, Zsolt
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A radio "colour-colour" diagram is defined in order to determine the evolutionary state of synchrotron-emitting plasma bubbles that are ejected during outbursts in microquasars. We establish the colour-colour diagram for the plasmons of SS433 observed on 18 April 1998 using VLBI observations. We show that the radio plasmons are not consistent with a simple expanding sphere of plasmon. This may indicate that in-situ particle acceleration is taking place away from the central engine.
description: Latex 2e, 6 pages, 3 figures. Submitted to proc. 2nd Workshop of Young Scientists in Astronomy and Astrophysics, ELTE Univ., Budapest, 2002
Conserved currents and $\text{T}\bar{\text{T}}_s$ irrelevant deformations of 2D integrable field theories
Creators: name: Conti, Riccardo
name: Negro, Stefano
name: Tateo, Roberto
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: It has been recently discovered that the $\text{T}\bar{\text{T}}$ deformation is closely-related to Jackiw-Teitelboim gravity. At classical level, the introduction of this perturbation induces an interaction between the stress-energy tensor and space-time and the deformed EoMs can be mapped, through a field-dependent change of coordinates, onto the corresponding undeformed ones. The effect of this perturbation on the quantum spectrum is non-perturbatively described by an inhomogeneous Burgers equation. In this paper, we point out that there exist infinite families of models where the geometry couples instead to generic combinations of local conserved currents labelled by the Lorentz spin. In spirit, these generalisations are similar to the $\text{J}\bar{\text{T}}$ model as the resulting theories and the corresponding scattering phase factors are not Lorentz invariant. The link with the $\text{J}\bar{\text{T}}$ model is discussed in detail. While the classical setup described here is very general, we shall use the sine-Gordon model and its CFT limit as explanatory quantum examples. Most of the final equations and considerations are, however, of broader validity or easily generalisable to more complicated systems.
description: 39 pages, 3 figures. v2: typos corrected, extended version with more results on the link between the classical and the quantum analysis
SNO and Supernovae
Creators: name: Virtue, C. J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Sudbury Neutrino Observatory (SNO) has unique capabilities as a supernova detector. In the event of a galactic supernova there are opportunities, with the data that SNO would collect, to constrain certain intrinsic neutrino properties significantly, to test details of the various models of supernova dynamics, and to provide prompt notification to the astronomical community through the Supernova Early Warning System (SNEWS). This paper consists of a discussion of these opportunities illustrated by some preliminary Monte Carlo results.
description: 7 pages, latex, 3 eps figures, Invited paper at Neutrino Oscillations Workshop (NOW 2000), Otranto, Italy, September 9-16, 2000, to be published in the Proceedings
Additional file 1 of Changes of cerebral cortical structure and cognitive dysfunction in “healthy hemisphere” after stroke: a study about cortical complexity and sulcus patterns in bilateral ischemic adult moyamoya disease
Creators: name: Liu, Ziqi
name: He, Shihao
name: Wei, Yanchang
name: Duan, Ran
name: Zhang, Cai
name: Li, Tian
name: Ma, Ning
name: Lou, Xin
name: Wang, Rong
name: Liu, Xiaoyuan
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Mental Health

description: Additional file 1. Neuropsychological assessments.
Anisops rhomboides Nieser & Chen 1999
Creators: name: Zettel, Herbert
name: Lane, David J. W.
name: Pangantihon, Clister V.
name: Freitag, Hendrik
name: Be, Jalan Tungku Link
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Notonectidae
Anisops
Anisops rhomboides

description: Anisops rhomboides Nieser & Chen, 1999
 Anisops tahitiensis (nec A. tahitiensis Lundblad, 1933, misidentifications): LANSBURY (1967: 97); NIESER & ZETTEL (1999: 123).
 Anisops rhomboides Nieser & Chen, 1999: 111; ZETTEL (2003: 126); CHEN et al. (2005: 422).
 Material examined. BRUNEI: BELAIT DISTRICT: Peat-swampy area draining to Sungai Ingei, 6.vi.2010, leg. D. J. W. Lane (15), 1 J (UBDB). PHILIPPINES: LEYTE: Leyte Province, Mahaplag, Hilusig River, 6.iii.2001, leg. F. E. Bendanillo, 1 J (USCP).
 Distribution. Anisops rhomboides is a West Malesian species so far recorded from Borneo, Sulawesi, and the Philippines (NIESER & CHEN 1999, CHEN et al. 2005). This species is the only notonectid species previously recorded from Brunei (from km 29.5 on Labi road [in Belait District], NIESER & CHEN 1999). Philippine records are only from the south: Mindanao (South Cotabato) (NIESER & CHEN 1999), Tawi Tawi (LANSBURY 1967, as A. tahitiensis), and Palawan (ZETTEL 2003). This first record from Leyte (Leyte Province) represents the species’ northernmost occurrence.
description: Published as part of Zettel, Herbert, Lane, David J. W., Pangantihon, Clister V., Freitag, Hendrik & Be, Jalan Tungku Link, 2012, Notes on Notonectidae (Hemiptera: Heteroptera) from southeastern Asia, mostly from Brunei and the Philippines, pp. 29-48 in Acta Entomologica Musei Nationalis Pragae 52 (1) on page 35, DOI: 10.5281/zenodo.5330381
title: In the Field of Information Systems: Factors Influencing the Adoption and Usage of e-Commerce in Saudi Arabia
Creators: name: Alghaith, Waleed Abdulrahman
Publisher: name: Griffith University
Year: 2011
Subjects: subject: e-Commerce Saudi Arabia
subject: Information systems

description: The internet, one of the most successful innovations in the world, initially regarded as a great catalyst of information exchange, is slowly evolving and being used as an important medium for trade and adverstising within the sphere of eCommerce. This has notably impacted on customer services as well as on industries such as retailing, financial services, publishing, communication, advertisements and travel. Saudi Arabia's accession to the World Trade Organization WTO in December 2005 has raised competition among local and global firms. This has created great opportunities for foreign companies to sell online to Saudis, it also created threats to local companies in various business and services sectors. As such businesses, either willingly or reluctantly, are increasingly embracing the Internet as a distribution channel in order to remain competitive or gain market share.
Oxybelus rubrocaudatus ARNOLD 1927
Creators: name: Dollfuss, H.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Crabronidae
Oxybelus
Oxybelus rubrocaudatus

description: Oxybelus rubrocaudatus ARNOLD 1927 (13, 39)
M a l a w i: 7, 50 km SW Blantrye Chickwawa, 22.XII.2001, leg. J. Halada.
M o z a m b i q u e:1, Inhambaene pr., 15 km SE Seve, 17.XII.2003, leg. J. Halada; 1, Manicala pr., 30 km NW Calandica, 17.-18.XII.2003, leg. J. Halada; 2, Ihambane pr., 25 km N Massinga, 5.+ 29.XII.2003, leg. J. Halada.
R. S. A.:8, 24, Eastern Cape, 10 km SE Alexandria Nat. Res., 28.-31.I.2000, leg. J. Halada; 1, W. Cape Nuwerus, 31.X.1999, leg. M. Halada; 1, Kwazulu Natal Utrecht, 28.XI.2002, leg. Snizek; 1, Maputoland SW Emanguzi, 29.I.2003, leg. Snizek.
T a n z a n i a:1, Mombo or., 9.-11.I.1996, leg. Snizek.
Z i m b a b w e: 1, 40 km Schipinge Mt. Selinda, 13.XII.1998, leg. M. Halada; 1, Mushandike N.P., Masvingo, 10.XII.1998, leg. J. Halada; 2, St. Benedict, 1300m, 30 km NE Macheke, 27.IV.1985, leg. J. Gusenleitner; 1, St. Benedict, 1300m, 30 km NE Macheke, 8.IV.1985, leg. J. Gusenleitner.
description: Published as part of Dollfuss, H., 2008, The Crabronid Wasps of the Genera Oxybelus LATREILLE 1796 and Brimocelus ARNOLD 1927 of " Biologiezentrum Linz " Collection in Linz, Austria (Hymenoptera, Apoidea, Crabronidae), pp. 463-505 in Linzer biologische Beiträge 40 (1) on page 492, DOI: 10.5281/zenodo.5428013
Commissioning Progress of the FAST
Creators: name: Jiang, Peng
name: Yue, Youling
name: Gan, Hengqian
name: Yao, Rui
name: Li, Hui
name: Pan, Gaofeng
name: Sun, Jinghai
name: Yu, Dongjun
name: Liu, Hongfei
name: Tang, Ningyu
name: Qian, Lei
name: Lu, Jiguang
name: Yan, Jun
name: Peng, Bo
name: Zhang, Shuxin
name: Wang, Qiming
name: Li, Qi
name: Li, Di
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The Five-hundred-meter Aperture Spherical radio Telescope (FAST) was completed with its main structure installed on September 25, 2016, after which it entered the commissioning phase. This paper aims to introduce the commissioning progress of the FAST over the past two years. To improve its operational reliability and ensure effective observation time, FAST has been equipped with a real-time information system for the active reflector system and hierarchical commissioning scheme for the feed support system, which ultimately achieves safe operation of the two systems. For meeting the high-performance indices, a high-precision measurement system was set up based on the effective control methods that were implemented for the active reflector system and feed support system. Since the commissioning of the FAST, a low-frequency ultra-wideband receiver and 19-beam 1.05-1.45 GHz receiver have been mainly used. Telescope efficiency, pointing accuracy, and system noise temperature were completely tested and ultimately achieved the acceptance indices of the telescope. The FAST has been in the process of national acceptance preparations and has begun to search for pulsars. In the future, it will still strive to improve its capabilities and expand its application prospects.
description: Sci. China-Phys. Mech. Astron. 62, 959502 (2019)
Modified log-Sobolev inequality for a compact PJMP with degenerate jumps
Creators: name: Papageorgiou, Ioannis
Publisher: name: arXiv
Year: 2019
Subjects: subject: Probability (math.PR)
subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 60K35, 26D10, 60G99

description: We study the modified log-Sobolev inequality for a class of pure jump Markov processes that describe the interactions between brain neurons. In particular, we focus on a finite and compact process with degenerate jumps inspired by the model introduced by Galves and Löcherbach. As a result, we obtain concentration properties for empirical approximations of the process.
Oxybelus ruficaudis CAMERON 1905
Creators: name: Dollfuss, H.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Crabronidae
Oxybelus
Oxybelus ruficaudis

description: Oxybelus ruficaudis CAMERON 1905 (9, 42)
K e n y a:1, Voi (Tsavo) env. 22.XI.-2.XII.1996, leg. Mi. Halada; 1, 1, Voi, 10.XII.1999, leg. Snizek; 9, Taita Hills Wundanyi, 18.-22. III.1997, leg. Ma. Halada; 2, (Tsavo) Tai Hills Wundanyi, 19.-21.XI.1996, leg. Mi. Halada.
M a l a w i: 1, 80 km E Liongwe Selima env., 3.-4.I.2002, leg. J. Halada; 3, 85 km SE Liongwe Dedza, 5.-12.I.2002, leg. J. Halada; 1, 160 km SE Liongwe Balaka, 20.XII.2001, leg. J. Halada.
N a m i b i a:1, 22. km SE Keetmanshoop, Road B1, Huns river, 29.III.-1.IV.2000, leg. Zabransky.
R. S. A.:6, 10, 10 km SE Alexandria Nat. Res., 28.-31.I.2000, leg. J. Halada; 3, N. Cape, 50 km SW Springbok wadi Buffels, 18.X.1999, leg. M. Halada; 1, Northern Cape, SW Springbok Buffels wadi, 4 XI.1999, leg. M. Halada; 2, W. Cape, 40 km S Lamberts Bay, 30.X.1999, leg. Ma. Halada; 1, W. Cape, 40 km S Lamberts Bay coast, 29.X.1999, leg. M. Halada; 1, N. Cape, 40 km SW Garies wadi, Groen, 16.X.1999, leg. M. Halada; 2, Eastern Cape, 30 km W Grahamstown Olifantskop pass, 25.I.2000, leg. J. Halada; 2, N. Cape, 25 km E Hondeklipbay wadi, 17.X.1999, leg. Ma. Halada; 1, N. Cape, SW Loriesfontein, 13.X.1999, leg. Ma. Halada; 1, Eastern Cape pro., Nat. Res. 10 km SE Alexandria, 28.-31.I.2000, leg. Becvar.
Z i m b a b w e: 1, Troutbeck, 1900m, Inyanga Mts., 23.IV.1985, leg. J. Gusenleitner; 2, St. Benedict, 1300m, 30 km NE Macheke, 21.IV.1985, leg. J. Gusenleitner; 1, St. Benedict, 1300m, 30 km NE Macheke, 20.IV.1985, leg. J. Gusenleitner; 1, St. Benedict, 1300m, 30 km NE Macheke, 27.IV.1985, leg. J. Gusenleitner; 1, 15 km NW Chinhoyi (= Sinola), 1250m, 11.IV.1985, leg. J. Gusenleitner; 1, Chimanimani (= Melsetter), 1050m, 25.IV.1985, leg. J. Gusenleitner.
description: Published as part of Dollfuss, H., 2008, The Crabronid Wasps of the Genera Oxybelus LATREILLE 1796 and Brimocelus ARNOLD 1927 of " Biologiezentrum Linz " Collection in Linz, Austria (Hymenoptera, Apoidea, Crabronidae), pp. 463-505 in Linzer biologische Beiträge 40 (1) on page 493, DOI: 10.5281/zenodo.5428013
Orbital Evolution of Scattered Planets
Creators: name: Yeh, Li-Chin
name: Jiang, Ing-Guey
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A simple dynamical model is employed to study the possible orbital evolution of scattered planets and phase plane analysis is used to classify the parameter space and solutions. Our results reconfirm that there is always an increase in eccentricity when the planet was scattered to migrate outward when the initial eccentricity is zero. Applying our study on the Solar System and considering the existence of the Kuiper Belt, this conclusion implies that Neptune was dynamically coupled with the Kuiper Belt in the early phase of the Solar System, which is consistent with the simulational model in Thommes, Duncan & Levison (1999).
description: AAS Latex file, 21 pages, accepted by ApJ
title: Can a Self-Reflexive Auteur Film Exploring the Mental Health Lived Experiences of Young People Generate Therapeutic Outcomes?
Creators: name: Menzies-Brown, Marie June
Publisher: name: Griffith University
Year: 2017
Subjects: subject: Films in health education
subject: Mental health documentaries
subject: Creative arts in therapy
subject: Films in therapy

description: The Merriam-Webster Dictionary defines ‘ontology’ as ‘the state of being’. It is generally understood as the way a person is seen in their present state. For this thesis, the term refers more to the inner thinking and deeper state of an individual than their external appearance. This research explores the lived experience of the ‘states of being’ of four young people through their narratives; their voices are represented in visual form. This research project employs the medium of film using visual ‘experiments’ that explore creative and alternate ways of presenting an artwork. Featuring unusual angles, disruption to the timeline, impromptu backstage director’s instructions, and voice overs, the filmic outcome of this research, Ontology: An Intimate Look into Lived Experiences, is an auteur-driven, selfreflective essay film. Ontology synergistically collated acting, theatre and stage direction, photography, text, music, fashion and interviews into an auteur self-reflective project delivered through film. It is hypothesised that this alternative technique of presentation, also referred to as ‘experiments’ (by the auteur), will be effective in reaching its intended audience: adolescents and young people. It is hoped that Ontology may be a starting point in prompting community discussions about, as well as promoting awareness on, mental illness. The methodology used combined various approaches, but specifically utilised the response of the auteur to a social issue around the topic of mental health concerns affecting young people. The auteur also used self-reflection as a response to the grief of the loss of a loved one, and reflected on her experience with this process as a method to answer the research question. Ontology explores the use of creative expressive therapies as a medium for healing and proving therapeutic benefits to participants through the process of art making.
The SXS Collaboration catalog of binary black hole simulations
Creators: name: Boyle, Michael
name: Hemberger, Daniel
name: Iozzo, Dante A. B.
name: Lovelace, Geoffrey
name: Ossokine, Serguei
name: Pfeiffer, Harald P.
name: Scheel, Mark A.
name: Stein, Leo C.
name: Woodford, Charles J.
name: Zimmerman, Aaron B.
name: Afshari, Nousha
name: Barkett, Kevin
name: Blackman, Jonathan
name: Chatziioannou, Katerina
name: Chu, Tony
name: Demos, Nicholas
name: Deppe, Nils
name: Field, Scott E.
name: Fischer, Nils L.
name: Foley, Evan
name: Fong, Heather
name: Garcia, Alyssa
name: Giesler, Matthew
name: Hebert, Francois
name: Hinder, Ian
name: Katebi, Reza
name: Khan, Haroon
name: Kidder, Lawrence E.
name: Kumar, Prayush
name: Kuper, Kevin
name: Lim, Halston
name: Okounkova, Maria
name: Ramirez, Teresita
name: Rodriguez, Samuel
name: Rüter, Hannes R.
name: Schmidt, Patricia
name: Szilagyi, Bela
name: Teukolsky, Saul A.
name: Varma, Vijay
name: Walker, Marissa
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Accurate models of gravitational waves from merging black holes are necessary for detectors to observe as many events as possible while extracting the maximum science. Near the time of merger, the gravitational waves from merging black holes can be computed only using numerical relativity. In this paper, we present a major update of the Simulating eXtreme Spacetimes (SXS) Collaboration catalog of numerical simulations for merging black holes. The catalog contains 2018 distinct configurations (a factor of 11 increase compared to the 2013 SXS catalog), including 1426 spin-precessing configurations, with mass ratios between 1 and 10, and spin magnitudes up to 0.998. The median length of a waveform in the catalog is 39 cycles of the dominant $\ell=m=2$ gravitational-wave mode, with the shortest waveform containing 7.0 cycles and the longest 351.3 cycles. We discuss improvements such as correcting for moving centers of mass and extended coverage of the parameter space. We also present a thorough analysis of numerical errors, finding typical truncation errors corresponding to a waveform mismatch of $\sim 10^{-4}$. The simulations provide remnant masses and spins with uncertainties of 0.03% and 0.1% ($90^{\text{th}}$ percentile), about an order of magnitude better than analytical models for remnant properties. The full catalog is publicly available at https://www.black-holes.org/waveforms .
description: 33+18 pages, 13 figures, 4 tables, 2,018 binaries. Catalog metadata in ancillary JSON file. v2: Matches version accepted by CQG. Catalog available at https://www.black-holes.org/waveforms
The USNO-B Catalog
Creators: name: Monet, D.
name: Levine, S.
name: Canzian, B.
name: Ables, H.
name: Bird, A.
name: Dahn, C.
name: Guetter, H.
name: Harris, H.
name: Henden, A.
name: Leggett, S.
name: Levison, H.
name: Luginbuhl, C.
name: Martini, J.
name: Monet, A.
name: Munn, J.
name: Pier, J.
name: Rhodes, A.
name: Riepe, B.
name: Sell, S.
name: Stone, R.
name: Vrba, F.
name: Walker, R.
name: Westerhout, G.
name: Brucato, R.
name: Reid, N.
name: Schoening, W.
name: Hartley, M.
name: Read, M.
name: Tritton, S.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: USNO-B is an all-sky catalog that presents positions, proper motions, magnitudes in various optical passbands, and star/galaxy estimators for 1,042,618,261 objects derived from 3,643,201,733 separate observations. The data were obtained from scans of 7,435 Schmidt plates taken for the various sky surveys during the last 50 years. USNO-B1.0 is believed to provide all-sky coverage, completeness down to V = 21, 0.2 arcsecond astrometric accuracy at J2000, 0.3 magnitude photometric accuracy in up to five colors, and 85% accuracy for distinguishing stars from non-stellar objects. A brief discussion of various issues is given here, but the actual data are available from http://www.nofs.navy.mil and other sites.
description: Accepted by Astronomical Journal
Some Existence Results for Algebraically Sub-Holomorphic Manifolds
Creators: name: Graham, Miranda
name: Robertson, Peter
name: Smith Moore
Publisher: name: figshare
Year: 2019
Subjects: subject: 10504 Mathematical Aspects of General Relativity
subject: FOS: Mathematics
subject: 19999 Mathematical Sciences not elsewhere classified

description: Let $G$ be a complex, non-positive vector. In \cite{cite:0}, the main result was the classification of unconditionally irreducible matrices.
Enithares intha Paiva 1918
Creators: name: Zettel, Herbert
name: Lane, David J. W.
name: Pangantihon, Clister V.
name: Freitag, Hendrik
name: Be, Jalan Tungku Link
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Notonectidae
Enithares
Enithares intha

description: Enithares intha Paiva, 1918
(Figs. 10, 16, 18)
 Enithares intha Paiva, 1918: 27; LANSBURY (1968: 438); LANSBURY (1973: 228); NIESER et al. (2008: 274, 279); THIRUMALAI (2007: 43).
 Material examined. MYANMAR: SHAN STATE: 2.5 km north of Mintaingbin Forest Camp, 1250 m a.s.l., 20°55.722′N 96°32.913′E, 12.+ 16.vi.2004, leg. H. Shaverdo & Myint Hlaing (149), 3 ♀♀ (NHMW).
 Distribution and notes. Until recently, Enithares intha was only known from the type series, two males, from Inle Lake, also in Shan State, Myanmar. While the identity of this species was unknown to Ivor Lansbury when preparing his revision of Enithares (LANSBURY 1968), he redescribed the types later (LANSBURY 1973). THIRUMALAI (2007) recorded E. intha from Meghalaya, northeastern India, based on a personal note by J.T. Polhemus. NIESER et al. (2008) included E. intha in a key to species from Thailand and adjacent areas, referring to LANSBURY’ s (1973) redescription, without having seen further specimens. Material in NHMW consists only of females. The shape of the metaxiphus agrees well with the illustration provided by LANSBURY (1973) for males and allows identification. The females strongly resemble E. sinica (comp. Fig. 12) except for slightly smaller body size, for a distinct spur on the mesotrochanter (Fig. 16), which is absent in E. sinica females (Fig. 17) and for the shape of the metaxiphus (Fig. 18), which is not expanded and has less highly elevated margins than in E. sinica (Fig. 19). The small spur on the mesotrochanter distinguishes females from all species in the region.
 Description of female. Body length 8.38–8.95 mm, head width 2.38–2.58 mm, median head length (in exact dorsal aspect of specimen) 1.24–1.30 mm, anterior width of vertex 1.05–1.09 mm, synthlipsis 0.48–0.51 mm, pronotum width 2.95–3.19 mm, median pronotum length 1.03–1.19 mm. Colour see Fig. 10, extension of dark colour on mesoscutellum and hemelytra slightly varying. Head large. Vertex anteriorly convex, clearly surpassing anterior eye margin. Medial margin of pronotal foveae directed slightly laterally. Metaxiphus (Fig. 18), relatively narrow, with distinctly, but not very strongly elevated sides and short apex. Mesotrochanter (Fig. 16) with distinct spur similar to that of male. Metafemur without tooth.
description: Published as part of Zettel, Herbert, Lane, David J. W., Pangantihon, Clister V., Freitag, Hendrik & Be, Jalan Tungku Link, 2012, Notes on Notonectidae (Hemiptera: Heteroptera) from southeastern Asia, mostly from Brunei and the Philippines, pp. 29-48 in Acta Entomologica Musei Nationalis Pragae 52 (1) on pages 37-38, DOI: 10.5281/zenodo.5330381