cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 9 of Identification of candidate tolerance genes to low-temperature during maize germination by GWAS and RNA-seqapproaches
Creators: name: Zhang, Hong
name: Zhang, Jiayue
name: Xu, Qingyu
name: Wang, Dandan
name: Di, Hong
name: Huang, Jun
name: Yang, Xiuwei
name: Wang, Zhoufei
name: Zhang, Lin
name: Dong, Ling
name: Wang, Zhenhua
name: Zhou, Yu
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 9 Table S7. Germination rates of 222 maize inbred lines at 25 °C.
Atmospheric response to sea-ice variability: role of con6nental snow cover and decadal SST variability
Creators: name: Gastineau, Guillaume
Publisher: name: Zenodo
Year: 2019

description: Workshop on Climate Prediction in the Atlantic-Arctic sector  Jointly organised by the Bjerknes Climate Prediction Unit and the EU Modelling Cluster 5-7th June 2019, Bergen, Norway 
Additional file 3: of Phylogenetic analysis and embryonic expression of panarthropod Dmrt genes
Creators: name: Panara, Virginia
name: Budd, Graham
name: Janssen, Ralf
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: Table S3. Links. (DOCX 45 kb)
Searching for Failed Supernovae With Astrometric Binaries
Creators: name: Gould, Andrew
name: Salim, Samir
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Stars in the mass range 8 Msun
description: Submitted to ApJ, 14 pages including 4 figures
Additional file 1 of Ficolin-A induces macrophage polarization to a novel pro-inflammatory phenotype distinct from classical M1
Creators: name: Zhu, Li-Wen
name: Li, Zihao
name: Dong, Xiaohong
name: Wu, Huadong
name: Cheng, Yifan
name: Xia, Shengnan
name: Bao, Xinyu
name: Xu, Yun
name: Cao, Runjing
Publisher: name: figshare
Year: 2024
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Supplementary Material 1
Are X-ray Clusters Cooled by Heat Conduction to the Surrounding Intergalactic Medium?
Creators: name: Loeb, Abraham
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show that X-ray clusters would have cooled substantially over a Hubble time by transport of heat from their hot interior to the their envelope, if the heat conductivity had not been heavily suppressed relative to the Spitzer value due to magnetic fields. The suppression is required in order for the observed abundance of hot X-ray clusters to be consistent with predictions from popular cosmological models. If a similar or stronger suppression factor applies to cluster cores, then thermal conduction can not be the mechanism that prevents cooling flows there.
description: New Astronomy, accepted for publication
Bose polarons near quantum criticality
Creators: name: Yan, Zoe Z.
name: Ni, Yiqi
name: Robens, Carsten
name: Zwierlein, Martin W.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Atomic Physics (physics.atom-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The emergence of quasiparticles in strongly interacting matter represents one of the cornerstones of modern physics. However, when different phases of matter compete near a quantum critical point, the very existence of quasiparticles comes under question. Here we create Bose polarons near quantum criticality by immersing atomic impurities in a Bose-Einstein condensate (BEC) with near-resonant interactions. Using locally-resolved radiofrequency spectroscopy, we probe the energy, spectral width, and short-range correlations of the impurities as a function of temperature. Far below the superfluid critical temperature, the impurities form well-defined quasiparticles. However, their inverse lifetime, given by their spectral width, is observed to increase linearly with temperature at the Planckian scale $\frac{k_B T}{\hbar}$, a hallmark of quantum critical behavior. Close to the BEC critical temperature, the spectral width exceeds the binding energy of the impurities, signaling a breakdown of the quasiparticle picture.
description: 17 pages, 14 figures
Evidence for a heated gas bubble inside the "cooling flow" region of MKW3s
Creators: name: Mazzotta, P.
name: Kaastra, J. S.
name: Paerels, F. B.
name: Ferrigno, C.
name: Colafrancesco, S.
name: Mewe, R.
name: Forman, W. R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on the deep Chandra observation of central r=200kpc region of the cluster of galaxies MKW3s which was previously identified as a moderate cooling flow cluster. The Chandra image reveals two striking features -- a 100kpc long and 21kpc wide filament, extending from the center to the south-west and a nearly circular, 50kpc diameter depression 90 kpc south of the X-ray peak. The temperature map shows that the filamentary structure is colder while the surface brightness depression is hotter than the average cluster temperature at any radius. The hot and the cold regions indicate that both cooling and heating processes are taking place in the center of MKW3s. We argue that the surface brightness depression is produced by a heated, low-density gas bubble along the line of sight. We suggest that the heated bubble is produced by short-lived nuclear outbursts from the central galaxy.
description: 4 pages, 5 color figures and 1 BW figure, emulateapj5, Accepted for publication in ApJ Letters
title: Optimisation of the biocatalytic component in a ferricyanide mediated approach to rapid biochemical oxygen demand analysis
Creators: name: Morris, Kristy
Publisher: name: Griffith University
Year: 2005
Subjects: subject: Biochemical oxygen demand
subject: ferricyanide ion
subject: biocatalytic component

description: A novel rapid method for the determination of biochemical oxygen demand (BOD) has been developed. By replacing oxygen, the terminal electron acceptor in the microbial oxidation of organic substrate, with the ferricyanide ion, a significant increase in the rate of the biochemical reaction could be achieved. This arises from the high solubility of the ferricyanide ion (compared to oxygen); therefore allowing for elevated microbial populations without rapid depletion of the electron acceptor. Therefore, the BOD of a sample can be determined within 1-3 hours compared to 5-days with the standard BOD5 assay. A range of microorganisms were shown to be able to use the ferricyanide ion as an alternative electron acceptor for the biodegradation of a range of organic compounds in the ferricyanide mediated BOD (FM-BOD) assay. The most suitable biocatalyst in the FM-BOD method, however, was shown to be a mixture of microorganisms that was capable of degrading large amounts and types of compounds. These mixed consortia of microorganisms included a synthetic mixture prepared in our laboratory and two commercially available consortia, BODseedTM and Bi-ChemTM. When these seed materials were employed in the FM-BOD assay, the method was shown to closely estimate the BOD5 values of real wastewater samples. The linear dynamic working range of the FM-BOD method was also greatly extended compared to the standard BOD5 assay (nearly 50 times greater) and other oxygen based BOD biosensors. The immobilisation of the microbial consortia by both gel entrapment and freeze-drying methods was shown to greatly reduce the preparation and handling time of the mixed consortia for use in the FM-BOD method. Immobilisation of the mixed microbial consortium in LentiKats®, a PVA hydrogel, resulted in a marked increase in the stability of the biocatalyst. Diffusion limitations resulting from the gel matrix, however, reduced the rate and extent of the bioreaction as well as the linear dynamic working range of the method. Freeze-drying techniques were shown to circumvent some of the limitations identified with gel entrapment for the immobilisation of the mixed consortia. The freeze-dried consortia could be used off-the-shelf and demonstrated reduced diffusional restrictions. A marked decrease in the viability of the microorganisms was observed directly following the freeze-drying process and in subsequent storage. Carrageenan, however, was shown to afford a significant degree a protection to the cells during the freeze-drying process.
Heterhelus Jacquelin du Val 1858
Creators: name: Hisamatsu, Sadatomo
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Kateretidae
Heterhelus

description: Key to subgenera and species of Japanese Heterhelus
 1 Labrum shallowly notched. Antenna with distinct 3-segmented club (Fig. 8E). Pronotum strongly convex. Parameres of male genitalia abruptly bent inward at mid-length (Fig. 8A). Head dark brown, always darker than elytra. Subgenus Boreades Parsons, 1943..................................................................................................  H. (B.) solani  (Heer, 1841)
 – Labrum deeply notched. Antenna with indistinct 3-segmented club (Figs. 6O, 7D). Pronotum feebly convex. Parameres of male genitalia regularly arcuate inwards (Figs. 6A, 6D, 7A, 7E). Head always the same color as elytra. Subgenus Heterhelus Jacquelin du Val, 1858......................................................................................................................... 2
 2 Body uniformly black; sides of pronotum regularly arcuate, never angulate; parameres of male genitalia short and wide (LP/WP = 2.1 (n = 1)) (Figs. 7A, 7E); apex of median lobe bluntly rounded in lateral aspect (Figs. 7C, 7F); base of ovipositor pigmented (Fig. 7G)............................................................................................  H. (H.) morio  (Reitter, 1878)
 – Body reddish-yellow to blackish; sides of pronotum regularly arcuate or strongly angulate; parameres of male genitalia long and slender (LP/WP = 3.1 (n = 1)) (Figs. 6A, 6D); apex of median lobe sharply acuminate in lateral aspect (Figs. 6C, 6E); base of ovipositor not pigmented (Fig. 6F).......................................................  H. (H.) scutellaris  (Heer, 1841)
description: Published as part of Hisamatsu, Sadatomo, 2011, A review of the Japanese Kateretidae fauna (Coleoptera: Cucujoidea), pp. 551-585 in Acta Entomologica Musei Nationalis Pragae 51 (2) on page 563, DOI: 10.5281/zenodo.5329313
A Primer on Eulerian Computational Fluid Dynamics for Astrophysics
Creators: name: Trac, Hy
name: Pen, Ue-Li
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a pedagogical review of some of the methods employed in Eulerian computational fluid dynamics (CFD). Fluid mechanics is governed by the Euler equations, which are conservation laws for mass, momentum, and energy. The standard approach to Eulerian CFD is to divide space into finite volumes or cells and store the cell-averaged values of conserved hydro quantities. The integral Euler equations are then solved by computing the flux of the mass, momentum, and energy across cell boundaries. We review both first-order and second-order flux assignment schemes. All linear schemes are either dispersive or diffusive. The nonlinear, second-order accurate total variation diminishing (TVD) approach provides high resolution capturing of shocks and prevents unphysical oscillations. We review the relaxing TVD scheme, a simple and robust method to solve systems of conservation laws like the Euler equations. A 3-D relaxing TVD code is applied to the Sedov-Taylor blast wave test. The propagation of the blast wave is accurately captured and the shock front is sharply resolved. We apply a 3-D self-gravitating hydro code to simulating the formation of blue straggler stars through stellar mergers and present some numerical results. A sample 3-D relaxing TVD code is provided in the appendix.
description: 23 pages, 12 figures; includes sample 3-D hydro code and new section on stellar mergers; accepted by PASP
The milliJansky 12 micron Population: First Followup
Creators: name: Clements, D. L.
name: Desert, F-X.
name: Franceschini, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the first results of our followup programme of optical imaging and spectroscopy of a deep 12 micron survey conducted with the ISO satellite (Clements et al. 1999). We find that the objects are typically of fairly low redshift (z ~ 0.1-0.2), but with a tail that extends to high redshifts. The highest redshift object is a previously unknown quasar at z=1.2. The sample of objects for which spectroscopy has been obtained forms a complete subsample of the original survey with an R band magnitude limit of 19.6. We are thus able to use accessible volume methods to determine the luminosity function. We find that the luminosity function is close to the low redshift 12 micron luminosity function determined by IRAS (Fang et al., 1998; Rush et al., 1993), but with a possible excess at the highest luminosities, which also correspond to the highest redshifts. This excess is compatible with the rapid luminosity evolution of L ~ (1+z)^{4.5} claimed by Xu (2000) and suggested by Elbaz (1999) on the basis of number counts. These conclusions remain tentative because of small number statistics at the highest redshifts. Almost all of the galaxies in this survey are emission line objects. We use the spectra to determine emission line diagnostics for the underlying ionisation source. We find that the majority of objects have HII region-like spectra (roughly 2/3) but there is a significant fraction (about 1/3) that contain an AGN. This confirms suspicions that deep mid-IR surveys will be a powerful way to find obscured AGN. Part of the survey area has been imaged deeply by the INT Wide Field Camera. Nearly all 12 micron sources in this area have good optical identifications. The prospects are thus good for obtaining complete spectroscopy.
description: Accepted for publication in MNRAS
title: Leading from the Middle
Creators: name: Bower, Mary
Publisher: name: Griffith University
Year: 2022
Subjects: subject: middle leader
subject: middle leading
subject: distributed leadership
subject: leadership practices
subject: leading from the middle

description: Middle leaders in schools are important. Alongside holding formal positions of responsibility, they remain active as class teachers, leading the learning of students and staff. Situated as the conduit between classroom teaching and educational leading, some research studies reveal connections between middle leaders and distributed leadership. In addition, commentators suggest that middle leaders have the potential to act as change agents leading school improvement. How middle leaders enact this critical role is the subject of this study. Through examining their leadership practices and patterns of behaviour this research explored how middle leaders approached leading from the middle. Framed by a case study methodological approach, this research employed semi-structured interviews to explore the perspectives of two middle leaders in a secondary school. Examining data describing the actions, interactions, and viewpoints of middle leaders highlighted what enabled and constrained the enactment of their roles. A conceptual framework was proposed to support the examination of the interrelationships of leading from the middle. With a focus on middle leading practice, this framework was further informed by patterns of behaviour described within a discrete dimension of distributed leadership, concertive action. The research findings suggest that quality relationships as well as context specific professional development are key factors in leading from the middle. Further, the findings of this study suggest that the multi-faceted nature of leading from the middle can be conceptualised using the metaphor of what I define as kaleidoscope leading.
title: Affect Regulation of Shame
Creators: name: Krishnamoorthy, Govind
Publisher: name: Griffith University
Year: 2011
Subjects: subject: Adult psychopathology
subject: Shame
subject: Anger

description: Over the past two decades persuasive arguments have been made to expand the role of emotion in clinical psychology. Research within the basic affective sciences suggests a number of ways that current psychological treatments may benefit from interventions explicitly targeting emotions, particularly for resistant forms of adult psychopathology. Research in this area has found that the inability to regulate feelings of shame may be a significant risk factor in the onset and recurrence of major depression and other psychological disorders. Although theoretical and research interest in the nature and consequences of shame have burgeoned in recent decades, little attention has yet been given to research on the regulation of shame. The present research describes two studies designed to redress this situation. Study 1 investigated the effectiveness of cognitive reappraisal relative to rumination in reducing feelings of shame. It was hypothesized that participants who reappraised an autobiographical shame event would report lower levels of shame than those ruminating about the event. Study 1 adapted the experimental methodology used by Ray, Wilhelm, and Gross (2008) in their investigation of the emotion regulation of anger. Participants initially recalled and rated a personal, real-life shame experience and were then asked to think about it in one of two ways: by ruminating about the event or by positively reappraising it. Results revealed lower levels of shame associated with reappraisal, relative to rumination.
Benchmarking Contemporary Deep Learning Hardware and Frameworks:A Survey of Qualitative Metrics
Creators: name: Dai, Wei
name: Berleant, Daniel
Publisher: name: arXiv
Year: 2019
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Machine Learning (cs.LG)
subject: Performance (cs.PF)
subject: FOS: Computer and information sciences

description: This paper surveys benchmarking principles, machine learning devices including GPUs, FPGAs, and ASICs, and deep learning software frameworks. It also reviews these technologies with respect to benchmarking from the perspectives of a 6-metric approach to frameworks and an 11-metric approach to hardware platforms. Because MLPerf is a benchmark organization working with industry and academia, and offering deep learning benchmarks that evaluate training and inference on deep learning hardware devices, the survey also mentions MLPerf benchmark results, benchmark metrics, datasets, deep learning frameworks and algorithms. We summarize seven benchmarking principles, differential characteristics of mainstream AI devices, and qualitative comparison of deep learning hardware and frameworks.
description: 8 pages, 4 figures, 2 tables
Chandra Detection of a TypeII Quasar at z=3.288
Creators: name: Stern, Daniel
name: Moran, Edward C.
name: Coil, Alison L.
name: Connolly, Andrew
name: Davis, Marc
name: Dawson, Steve
name: Dey, Arjun
name: Eisenhardt, Peter
name: Elston, Richard
name: Graham, James R.
name: Harrison, Fiona
name: Helfand, David J.
name: Holden, Brad
name: Mao, Peter
name: Rosati, Piero
name: Spinrad, Hyron
name: Stanford, S. A.
name: Tozzi, Paolo
name: Wu, K. L.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on observations of a TypeII quasar at redshift z=3.288, identified as a hard X-ray source in a 185 ks observation with the Chandra X-ray Observatory and as a high-redshift photometric candidate from deep, multiband optical imaging. CXOJ084837.9+445352 (hereinafter CXO52) shows an unusually hard X-ray spectrum from which we infer an absorbing column density N(H) = (4.8+/-2.1)e23 / cm2 (90% confidence) and an implied unabsorbed 2-10 keV rest-frame luminosity of L(2-10) = 3.3e44 ergs/s, well within the quasar regime. Hubble Space Telescope imaging shows CXO52 to be elongated with slight morphological differences between the WFPC2 F814W and NICMOS F160W bands. Optical and near-infrared spectroscopy of CXO52 show high-ionization emission lines with velocity widths ~1000 km/s and flux ratios similar to a Seyfert2 galaxy or radio galaxy. The latter are the only class of high-redshift TypeII luminous AGN which have been extensively studied to date. Unlike radio galaxies, however, CXO52 is radio quiet, remaining undetected at radio wavelengths to fairly deep limits, f(4.8GHz) < 40 microJy. High-redshift TypeII quasars, expected from unification models of active galaxies and long-thought necessary to explain the X-ray background, are poorly constrained observationally with few such systems known. We discuss recent observations of similar TypeII quasars and detail search techniques for such systems: namely (1) X-ray selection, (2) radio selection, (3) multi-color imaging selection, and (4) narrow-band imaging selection. Such studies are likely to begin identifying luminous, high-redshift TypeII systems in large numbers. We discuss the prospects for these studies and their implications to our understanding of the X-ray background.
description: 28 pages, 5 figures; to appear in The Astrophysical Journal
Sibirhelus Kirejtshuk 1989
Creators: name: Hisamatsu, Sadatomo
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Kateretidae
Sibirhelus

description: Genus Sibirhelus Kirejtshuk, 1989
 Type species. Heterhelus corpulentus Reitter, 1900, by original designation.
 Diagnosis. Body elongate oval, strongly convex. Antennae moniliform. Pronotum with lateral margins uniformly rounded; punctures on disc larger than eye facet; posterior angles obtusely angulate; basal margin nearly straight or with slight curvature. Male abdominal tergite VIII externally visible. Tarsal claws more or less expanded at the base. Ovipositor with short styli.
 Bionomics. Sibirhelus corpulentus was collected from flowers of Carex dispalata Boott (Cyperaceae) (see Bionomics of S. corpulentus below).
 Distribution. Siberia and Japan (JELÍNEK & AUDISIO 2007).
 Note. Sibirhelus is a monotypic genus with only one species, S. corpulentus, occurring from Siberia to Japan.
description: Published as part of Hisamatsu, Sadatomo, 2011, A review of the Japanese Kateretidae fauna (Coleoptera: Cucujoidea), pp. 551-585 in Acta Entomologica Musei Nationalis Pragae 51 (2) on page 572, DOI: 10.5281/zenodo.5329313
Mass-Loss Rate Determination for the Massive Binary V444 Cyg using 3-D Monte-Carlo Simulations of Line and Polarization Variability
Creators: name: Kurosawa, R.
name: Hillier, D. J.
name: Pittard, J. M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A newly developed 3-D Monte Carlo model is used, in conjunction with a multi-line non-LTE radiative transfer model, to determine the mass-loss rate of the Wolf-Rayet (W-R) star in the massive binary \object{V444 Cyg} (WN5+O6). This independent estimate of mass-loss rate is attained by fitting the observed \HeI (5876) Åand \HeII (5412) Åline profiles, and the continuum light curves of three Stokes parameters ((I, Q, U)) in the (V) band simultaneously. The high accuracy of our determination arises from the use of many observational constraints, and the sensitivity of the continuum polarization to the mass-loss rate. Our best fit model suggests that the mass-loss rate of the system is (\dot{M}_{\WR}=0.6(\pm 0.2) \times 10^{-5} M_{\sun} \mathrm{yr}^{-1} ), and is independent of the assumed distance to \object{V444 Cyg}. The fits did not allow a unique value for the radius of the W-R star to be derived. The range of the volume filling factor for the W-R star atmosphere is estimated to be in the range of 0.050 (for $R_{\WR}=5.0 R_{\sun}$) to 0.075 (for $R_{\WR}=2.5 R_{\sun}$). We also found that the blue-side of \HeI (5876 ) Åand \HeII (5412) Ålines at phase 0.8 is relatively unaffected by the emission from the wind-wind interaction zone and the absorption by the O-star atmosphere; hence, the profiles at this phase are suitable for spectral line fittings using a spherical radiative transfer model.
description: 18 pages, 17 figures: Accepeted for publication in A&A
Coelogyne trusmadiensis M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne trusmadiensis

description: Coelogyne trusmadiensis (J.J.Wood) M.W.Chase & Schuit., comb. nov.
 Basionym: Dendrochilum trusmadiense J.J.Wood, Lindleyana 5: 93 (1990).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 130, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
Lagrangian Covector Fluid with Free Surface
Creators: name: Li, Zhiqi
name: Börcsök, Barnabás
name: Chen, Duowen
name: Sun, Yutong
name: Zhu, Bo
name: Turk, Greg
Publisher: name: arXiv
Year: 2024
Subjects: subject: Graphics (cs.GR)
subject: FOS: Computer and information sciences

description: This paper introduces a novel Lagrangian fluid solver based on covector flow maps. We aim to address the challenges of establishing a robust flow-map solver for incompressible fluids under complex boundary conditions. Our key idea is to use particle trajectories to establish precise flow maps and tailor path integrals of physical quantities along these trajectories to reformulate the Poisson problem during the projection step. We devise a decoupling mechanism based on path-integral identities from flow-map theory. This mechanism integrates long-range flow maps for the main fluid body into a short-range projection framework, ensuring a robust treatment of free boundaries. We show that our method can effectively transform a long-range projection problem with integral boundaries into a Poisson problem with standard boundary conditions -- specifically, zero Dirichlet on the free surface and zero Neumann on solid boundaries. This transformation significantly enhances robustness and accuracy, extending the applicability of flow-map methods to complex free-surface problems.
description: 10 pages, 17 figures, SIGGRAPH Conference Papers '24
Brachypterus Kugelann 1794
Creators: name: Hisamatsu, Sadatomo
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Kateretidae
Brachypterus

description: Genus Brachypterus Kugelann, 1794
 Type species. Dermestes urticae Fabricius, 1792, subsequent designation by THOMSON (1859).
 Diagnosis. Body oval, strongly convex. Pronotum transverse, lateral margins uniformly rounded; disc with punctures larger than eye facet; posterior angles obtusely angulate; basal margin slightly sinuate before posterior angles. Antennae with distinct three-segmented club. Male abdominal tergite VIII externally visible. Tarsal claws strongly dentate at the base. Ovipositor without styli.
 Bionomics. Larval stages have been found on flowers of Gesnouinia and Urtica (Urticaceae) (JELÍNEK & CLINE 2010).
 Distribution. Twenty-three species have been recorded. The species have wide distributional ranges in the Palaearctic, Oriental, Nearctic, and Afrotropical Regions (JELÍNEK & CLINE 2010).
description: Published as part of Hisamatsu, Sadatomo, 2011, A review of the Japanese Kateretidae fauna (Coleoptera: Cucujoidea), pp. 551-585 in Acta Entomologica Musei Nationalis Pragae 51 (2) on page 574, DOI: 10.5281/zenodo.5329313
Leptogenesis in $Δ(27)$ with a Universal Texture Zero
Creators: name: Björkeroth, Fredrik
name: Varzielas, Ivo de Medeiros
name: López-Ibáñez, M. L.
name: Melis, Aurora
name: Vives, Óscar
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate the possibility of viable leptogenesis in an appealing $Δ(27)$ model with a universal texture zero in the (1,1) entry. The model accommodates the mass spectrum, mixing and CP phases for both quarks and leptons and allows for grand unification. Flavoured Boltzmann equations for the lepton asymmetries are solved numerically, taking into account both $N_1$ and $N_2$ right-handed neutrino decays. The $N_1$-dominated scenario is successful and the most natural option for the model, with $M_1 \in [10^9, 10^{12}]$ GeV, and $M_1/M_2 \in [0.002, 0.1]$, which constrains the parameter space of the underlying model and yields lower bounds on the respective Yukawa couplings. Viable leptogenesis is also possible in the $N_2$-dominated scenario, with the asymmetry in the electron flavour protected from $N_1$ washout by the texture zero. However, this occurs in a region of parameter space which has a stronger mass hierarchy $M_1/M_2 < 0.002 $, and $M_2$ relatively close to $M_3$, which is not a natural expectation of the $Δ(27)$ model.
description: v2: 20 pages, 2 figures. Version accepted in JHEP
The Centaurus A Northern Middle Lobe as a Buoyant Bubble
Creators: name: Saxton, Curtis J.
name: Sutherland, Ralph S.
name: Bicknell, Geoffrey V.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We model the northern middle radio lobe of Centaurus A (NGC 5128) as a buoyant bubble of plasma deposited by an intermittently active jet. The extent of the rise of the bubble and its morphology imply that the ratio of its density to that of the surrounding ISM is less than 10^{-2}, consistent with our knowledge of extragalactic jets and minimal entrainment into the precursor radio lobe. Using the morphology of the lobe to date the beginning of its rise through the atmosphere of Centaurus A, we conclude that the bubble has been rising for approximately 140Myr. This time scale is consistent with that proposed by Quillen et al. (1993) for the settling of post-merger gas into the presently observed large scale disk in NGC 5128, suggesting a strong connection between the delayed re-establishment of radio emission and the merger of NGC 5128 with a small gas-rich galaxy. This suggests a connection, for radio galaxies in general, between mergers and the delayed onset of radio emission. In our model, the elongated X-ray emission region discovered by Feigelson et al. (1981), part of which coincides with the northern middle lobe, is thermal gas that originates from the ISM below the bubble and that has been uplifted and compressed. The "large-scale jet" appearing in the radio images of Morganti et al. (1999) may be the result of the same pressure gradients that cause the uplift of the thermal gas, acting on much lighter plasma, or may represent a jet that did not turn off completely when the northern middle lobe started to buoyantly rise. We propose that the adjacent emission line knots (the "outer filaments") and star-forming regions result from the disturbance, in particular the thermal trunk, caused by the bubble moving through the extended atmosphere of NGC 5128.
description: 38 pages, 13 figures, submitted to ApJ; a version with higher resolution figures is available at http://www.mso.anu.edu.au/~saxton/papers/cena.pdf
The Spectral Energy Distribution of the Seyfert galaxy Ton S180
Creators: name: Turner, T. J.
name: Romano, P.
name: Kraemer, S. B.
name: George, I. M.
name: Yaqoob, T.
name: Crenshaw, D. M.
name: Storm, J.
name: Alloin, D.
name: Lazzaro, D
name: Da Silva, L.
name: Pritchard, J. D.
name: Kriss, G.
name: Zheng, W.
name: Mathur, S.
name: Wang, J.
name: Dobbie, P.
name: Collins, N. R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present spectral results from a multi-satellite, broad-band campaign on the Narrow-line Seyfert 1 galaxy Ton S180 performed at the end of 1999. We discuss the spectral-energy distribution of the source, combining simultaneous Chandra, ASCA and EUVE data with contemporaneous FUSE, HST, and ground-based optical and infra-red data. The resulting SED shows that most of the energy is emitted in the 10 -- 100 eV regime, which must be dominated by the primary energy source. No spectral turnover is evident in the UV regime. This, the strong soft X-ray emission, and the overall shape of the SED indicate that emission from the accretion disk peaks between 15 and 100 eV. High resolution FUSE spectra showing UV absorption due to O VI and the lack of detectable X-ray absorption in the Chandra spectrum demonstrate the presence of a low column density of highly ionized gas along our line-of-sight. The highly-ionized state of the circumnuclear gas is most likely linked to the high luminosity and steep spectrum of the active nucleus. Given the strong ionizing flux in Ton S180, it is possible that the clouds within a few tens of light days of the central source are too highly ionized to produce much line emission. Thus the narrow width of the emission lines in Ton S180 is due to the emission arising from large radii.
description: 38 pages, 8 figures, some color figures. Accepted for publication in the Astrophysical Journal
title: The Double Thread of Fiction: Voice and Vision in the Novels of Henry Green
Creators: name: Poacher, Jeffrey James
Publisher: name: Griffith University
Year: 2009
Subjects: subject: Voice and vision
subject: Henry,Green, 1905-1974

description: Between 1926 and 1952, the English writer Henry Green published nine novels. From the outset, his work showed a particular fascination with the relationship between voice and vision. Green’s early novels, in particular, were characterised by various forms of visual failure – blindness, hallucinations, impenetrable fogs, wartime blackouts – yet at the same time his work contained many striking passages of visual description. There are also contradictions in the way voice is represented throughout his writing. Conversations in Green’s novels are often confused affairs, in which characters lie or dissemble, or simply garble their words; this complete unreliability of the spoken word is a major part of his fiction’s comedy. On the other hand, there are also moments in his novels when voices seem to possess an almost rapturous power, enchanting their listeners with the beauty of song. This dissertation shows that Green’s writing possessed a double character. It is not simply the case that his novels preferred orality over visuality (though they sometimes did do that). Rather, his work demonstrated the paradoxes of both voice and vision – their powers and their limitations, their clashes and their complementarities. Green’s success as a novelist came from this sense of duality; his finest work was concerned with the nuances of both sight and sound. Only in his last two novels did he abandon the richness of visually-oriented description in favour of a narrative style that consisted almost wholly of reported speech. Though this final phase of his career might be considered in some respects a failure, Green deserves to be regarded as one of the most important English-language novelists of the twentieth century. His work, however, has received much less critical attention than that of his contemporaries. This dissertation undertakes a close reading of his major novels, concentrating on their language and formal elements in order to suggest a new approach to his work that recognises its fundamental duality.
Infrared Observations During the Secondary Eclipse of HD 209458b: I. 3.6-Micron Occultation Spectroscopy Using the VLT
Creators: name: Richardson, L. Jeremy
name: Deming, Drake
name: Wiedemann, Guenter
name: Goukenleuque, Cedric
name: Steyert, David
name: Harrington, Joseph
name: Esposito, Larry W.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We search for an infrared signature of the transiting extrasolar planet HD 209458b during secondary eclipse. Our method, which we call `occultation spectroscopy,' searches for the disappearance and reappearance of weak spectral features due to the exoplanet as it passes behind the star and later reappears. We argue that at the longest infrared wavelengths, this technique becomes preferable to conventional `transit spectroscopy'. We observed the system in the wing of the strong nu-3 band of methane near 3.6 microns during two secondary eclipses, using the VLT/ISAAC spectrometer at a spectral resolution of 3300. Our analysis, which utilizes a model template spectrum, achieves sufficient precision to expect detection of the spectral structure predicted by an irradiated, low-opacity (cloudless), low-albedo, thermochemical equilibrium model for the exoplanet atmosphere. However, our observations show no evidence for the presence of this spectrum from the exoplanet, with the statistical significance of the non-detection depending on the timing of the secondary eclipse, which depends on the assumed value for the orbital eccentricity. Our results reject certain specific models of the atmosphere of HD 209458b as inconsistent with our observations at the 3-sigma level, given assumptions about the stellar and planetary parameters.
description: 26 pages, 8 figures Accepted to Astrophysical Journal
Additively manufactured ultra-high vacuum chamber below $10^{-10}$ mbar
Creators: name: Cooper, N.
name: Coles, L. A.
name: Everton, S.
name: Campion, R. P.
name: Madkhaly, S.
name: Morley, C.
name: Evans, W.
name: Saint, R.
name: Krüger, P.
name: Oručević, F.
name: Tuck, C.
name: Wildman, R. D.
name: Fromhold, T. M.
name: Hackermueller, L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: Metal-based additive manufacturing (AM) represents a paradigm change in engineering and production methods across multiple industries and sectors. AM methods enable mass reduction and performance optimisation well beyond that achievable via conventional manufacturing, thereby impacting significantly on aerospace and space technologies. Technologies relying on high and ultra-high vacuum (UHV), such as x-ray photo-electron spectroscopy, photo-sensors, cameras and cryostats, could also benefit greatly from AM. Despite recent advances in AM processing of metals, additively manufactured UHV chambers have so far not been achieved. Reducing the mass of UHV equipment is particularly critical for the development of portable cold atom systems, which are expected to underpin the next generation of sensing and timekeeping technologies and to allow novel space-based sensors for fundamental research. We demonstrate here an additively manufactured UHV chamber reaching a pressure below $10^{-10}$ mbar, enabling a cloud of cold $^{85}$Rb atoms to be trapped - the starting point for many precision timekeeping and sensing devices. The chamber is manufactured from aluminium alloy AlSi10Mg by laser powder bed fusion and has a mass of less than a third of a commercially-available equivalent. Outgassing analysis based on mass spectrometry was performed and it was demonstrated that even without active pumping the system remains in the $10^{-9}$ mbar regime for up to 48 hours.
Coelogyne tuberculata M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne tuberculata

description: Coelogyne tuberculata (J.J.Wood & J.B.Comber) M.W.Chase & Schuit., comb. nov.
 Basionym: Dendrochilum tuberculatum J.J.Wood & J.B.Comber, Lindleyana 10: 67 (1995).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 130, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
A window into NV center kinetics via repeated annealing and spatial tracking of thousands of individual NV centers
Creators: name: Chakravarthi, Srivatsa
name: Moore, Chris
name: Opsvig, April
name: Pederson, Christian
name: Hunt, Emma
name: Ivanov, Andrew
name: Christen, Ian
name: Dunham, Scott
name: Fu, Kai-Mei C
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Knowledge of the nitrogen-vacancy center formation kinetics in diamond is critical to engineering sensors and quantum information devices based on this defect. Here we utilize the longitudinal tracking of single NV centers to elucidate NV defect kinetics during high-temperature annealing from 800-1100 $^\circ$C in high-purity chemical-vapor-deposition diamond. We observe three phenomena which can coexist: NV formation, NV quenching, and NV orientation changes. Of relevance to NV-based applications, a 6 to 24-fold enhancement in the NV density, in the absence of sample irradiation, is observed by annealing at 980 $^\circ$C, and NV orientation changes are observed at 1050 $^\circ$C. With respect to the fundamental understanding of defect kinetics in ultra-pure diamond, our results indicate a significant vacancy source can be activated for NV creation between 950-980 $^\circ$C and suggests that native hydrogen from NVH$_y$ complexes plays a dominant role in NV quenching, in agreement with recent {\it ab initio} calculations. Finally, the direct observation of orientation changes allows us to estimate an NV diffusion barrier of 5.1~eV.
Unbounded Algebraic Derivators
Creators: name: Alonso, Leovigildo
name: Álvarez, Beatriz
name: Jeremías, Ana
Publisher: name: arXiv
Year: 2021
Subjects: subject: Category Theory (math.CT)
subject: Algebraic Geometry (math.AG)
subject: Representation Theory (math.RT)
subject: FOS: Mathematics
subject: 18G80 (primary), 18G35, 13D45, 20J06 (secondary)

description: We show that the unbounded derived category of a Grothendieck category with enough projective objects is the base category of a derivator whose category of diagrams is the full 2-category of small categories. With this structure, we give a description of the localization functor associated to a specialization closed subset of the spectrum of a commutative noetherian ring. In addition, using the derivator of modules, we prove some basic theorems of group cohomology for complexes of representations over an arbitrary base ring.
description: V3, final version, V2 Corrected proof of Proposition 2.10 and several other improvements. 32 pages
A simple framework for contrastive learning phases of matter
Creators: name: Han, Xiao-Qi
name: Xu, Sheng-Song
name: Feng, Zhen
name: He, Rong-Qiang
name: Lu, Zhong-Yi
Publisher: name: arXiv
Year: 2022
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Machine Learning (cs.LG)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: A main task in condensed-matter physics is to recognize, classify, and characterize phases of matter and the corresponding phase transitions, for which machine learning provides a new class of research tools due to the remarkable development in computing power and algorithms. Despite much exploration in this new field, usually different methods and techniques are needed for different scenarios. Here, we present SimCLP: a simple framework for contrastive learning phases of matter, which is inspired by the recent development in contrastive learning of visual representations. We demonstrate the success of this framework on several representative systems, including classical and quantum, single-particle and many-body, conventional and topological. SimCLP is flexible and free of usual burdens such as manual feature engineering and prior knowledge. The only prerequisite is to prepare enough state configurations. Furthermore, it can generate representation vectors and labels and hence help tackle other problems. SimCLP therefore paves an alternative way to the development of a generic tool for identifying unexplored phase transitions.
description: 7 pages, 6 figures
UBVRI photometric comparison sequences for symbiotic stars. II
Creators: name: Henden, Arne
name: Munari, Ulisse
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present accurate and deep UBVRI photometric sequences for an additional 20 symbiotic stars. As for the 20 targets of Paper I, the sequences extend over wide brightness and color ranges, and are suited to cover both quiescence and outburst phases. The sequences are intended to assist both present time photometry as well as measurement of photographic plates from historical archives.
description: A&A, in press
Multivalent glycoconjugates as vaccines and potential drug candidates
Creators: name: Bhatia, Sumati
name: Dimde, Mathias
name: Haag, Rainer
Publisher: name: Freie Universität Berlin
Year: 2014
Subjects: subject: 500 Naturwissenschaften und Mathematik::540 Chemie

description: Pathogens adhere to the host cells during the first steps of infection through multivalent interactions which involve protein–glycan recognition. Multivalent interactions are also involved at different stages of immune response. Insights into these multivalent interactions generate a way to use suitable carbohydrate ligands that are attached to a basic scaffold consisting of e.g., dendrimer, polymer, nanoparticle, etc., with a suitable linker. Thus a multivalent architecture can be obtained with controllable spatial and topology parameters which can interfere with pathogen adhesion. Multivalent glycoconjugates bearing natural or unnatural carbohydrate antigen epitopes have also been used as carbohydrate based vaccines to stimulate an innate and adaptive immune response. Designing and synthesizing an efficient multivalent architecture with optimal ligand density and a suitable linker is a challenging task. This review presents a concise report on the endeavors to potentially use multi- and polyvalent glycoconjugates as vaccines as well as anti-infectious and anti-inflammatory drug candidates.
Brachypterolus Grouvelle 1913
Creators: name: Hisamatsu, Sadatomo
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Kateretidae
Brachypterolus

description: Genus Brachypterolus Grouvelle, 1913
 Type species: Catheretes gravidus Illiger, 1798 (= Brachypterolus pulicarius (Linnaeus, 1758)), subsequent designation by JELÍNEK & STEELE (1966).
 Diagnosis. Body oval, strongly convex, dorsal and ventral disc densely covered with long whitish setae. Antennae with distinct 3-segmented club. Pronotum transverse, lateral margins rounded; disc with punctures larger than eye facet; posterior angles distinctly angulate, more or less projecting posteriorly; basal margin strongly sinuate before posterior angles. Male abdominal tergite VIII externally visible. Tarsal claws strongly dentate at base. Ovipositor without styli.
 Bionomics. Larval stages occur on flowers of Antirrinum and Linaria (Scrophulariaceae) (JELÍNEK & CLINE 2010).
 Distribution. Eleven species are included in the genus, all of them from the Palaearctic region, and one Holarctic (PARSONS 1943, JELÍNEK & CLINE 2010).
description: Published as part of Hisamatsu, Sadatomo, 2011, A review of the Japanese Kateretidae fauna (Coleoptera: Cucujoidea), pp. 551-585 in Acta Entomologica Musei Nationalis Pragae 51 (2) on page 577, DOI: 10.5281/zenodo.5329313