cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Coelogyne transversa 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 transversa

description: Coelogyne transversa (Carr) M.W.Chase & Schuit., comb. nov.
 Basionym: Dendrochilum transversum Carr, Gard. Bull. Straits Settlem. 8: 233 (1935).
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
Additional file 1: of Analgesic efficacy of preemptive local wound infiltration plus laparoscopic-assisted transversus abdominis plane block versus wound infiltration in patients undergoing laparoscopic colorectal resection: study protocol for a randomized, multicenter, single-blind, noninferiority trial
Creators: name: Pedrazzani, Corrado
name: Park, Soo
name: Scotton, Giovanni
name: Park, Jun
name: Kim, Hye
name: Polati, Enrico
name: Guglielmi, Alfredo
name: Choi, Gyu
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Immunology
subject: FOS: Clinical medicine
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences

description: Standard Protocol Items: Recommendations for Interventional Trials (SPIRIT) checklist. (DOC 131 kb)
Additional file 1 of Change in mean salt intake over time using 24-h urine versus overnight and spot urine samples: a systematic review and meta-analysis
Creators: name: Santos, Joseph Alvin
name: Li, Ka Chun
name: Huang, Liping
name: Mclean, Rachael
name: Petersen, Kristina
name: Di Tanna, Gian Luca
name: Webster, Jacqui
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Cancer
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy

description: Additional file 1. Full search strategy in Medline. Additional file 1 contains the full search strategy (search terms and syntax) used in the Medline database.
Platamartus Reitter 1892
Creators: name: Hisamatsu, Sadatomo
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Kateretidae
Platamartus

description: Genus Platamartus Reitter, 1892
 Type species. Platamartus jakowlewi Reitter, 1892, by monotypy.
 Diagnosis. Body elongate oval, flattened. Male antennae distinctly longer than those of female. Pronotum transverse, lateral margins distinctly serrate; disc with coarse and large punctures, larger than eye facet; posterior angles prominent; anterior angles not prominent; basal margin nearly straight or with slight curvature. Prosternum (excluding prosternal process) longer than mesoventrite. Male abdominal tergite VIII externally visible. Legs long and slender; tarsal claws simple. Ovipositor with short styli.
 Bionomics. Platamartus jakowlewi was collected from flowers of Carex dispalata Boott (Cyperaceae) (see Bionomics under P. jakowlewi).
 Distribution. Species are known from the Russian Far East and are represented by two species (KIREJTSHUK 1992).
 Note. Siberian species were studied by KIREJTSHUK (1992).
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 560, DOI: 10.5281/zenodo.5329313
Small Intestinal Nematode Infection of Mice Is Associated with Increased Enterobacterial Loads alongside the Intestinal Tract
Creators: name: Rausch, Sebastian
name: Held, Josephin
name: Fischer, André
name: Heimesaat, Markus M.
name: Kühl, Anja A.
name: Bereswill, Stefan
name: Hartmann, Susanne
Publisher: name: Freie Universität Berlin
Year: 2013
Subjects: subject: 600 Technik, Medizin, angewandte Wissenschaften::630 Landwirtschaft::630 Landwirtschaft und verwandte Bereiche

description: Parasitic nematodes are potent modulators of immune reactivity in mice and men. Intestinal nematodes live in close contact with commensal gut bacteria, provoke biased Th2 immune responses upon infection, and subsequently lead to changes in gut physiology. We hypothesized that murine nematode infection is associated with distinct changes of the intestinal bacterial microbiota composition. We here studied intestinal inflammatory and immune responses in mice following infection with the hookworm Heligmosomoidespolygyrusbakeri and applied cultural and molecular techniques to quantitatively assess intestinal microbiota changes in the ileum, cecum and colon. At day 14 post nematode infection, mice harbored significantly higher numbers of γ-Proteobacteria/Enterobacteriaceae and members of the Bacteroides/Prevotella group in their cecum as compared to uninfected controls. Abundance of Gram- positive species such as Lactobacilli, Clostridia as well as the total bacterial load was not affected by worm infection. The altered microbiota composition was independent of the IL-4/-13 - STAT6 signaling axis, as infected IL-4Rα(-/-) mice showed a similar increase in enterobacterial loads. In conclusion, infection with an enteric nematode is accompanied by distinct intestinal microbiota changes towards higher abundance of gram-negative commensal species at the small intestinal site of infection (and inflammation), but also in the parasite-free large intestinal tract. Further studies should unravel the impact of nematode-induced microbiota changes in inflammatory bowel disease to allow for a better understanding of how theses parasites interfere with intestinal inflammation and bacterial communities in men.
Clockwork Neutrinos
Creators: name: Hong, Sungwoo
name: Kurup, Gowri
name: Perelstein, Maxim
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Clockwork (CW) mechanism can explain the smallness of neutrino masses without introducing unnaturally small input parameters. In this paper we study the simplest CW neutrino model, the "uniform" clockwork, as well as a broader class of "generalized" clockwork models. We derive constraints on such models from lepton-flavor violating processes, as well as precision electroweak fits. These constraints allow excited CW neutrino states with masses of order 100 GeV -- 1 TeV, within reach of the LHC and proposed lepton colliders, as long as the input neutrino Yukawa coupling is of order $10^{-1}-10^{-2}$. We study collider phenomenology of these models. At the LHC, models with light ($\sim 100$~GeV) CW neutrinos can be discovered using the $3\ell+$ MET signature. Lepton colliders will be able to discover the CW neutrinos as long as they are within their kinematic range.
description: 33 pages, 23 figures
Radio Properties of Pinwheel Nebulae
Creators: name: Monnier, J. D.
name: Greenhill, L. J.
name: Tuthill, P. G.
name: Danchi, W. C.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A small number of dusty Wolf-Rayet stars have been resolved into pinwheel nebulae, defined by their ``rotating'' spiral dust shells observed in the infrared. This morphology is naturally explained by dust formation associated with colliding winds in a binary system. In order to confirm and further explore this hypothesis, we have observed the known pinwheel nebulae (WR 104 and WR 98a) as well as the suspected binary WR 112 at multiple radio wavelengths with the Very Large Array to search for non-thermal radio emission from colliding winds. The spectrum of each target is nearly flat between 5 and 22 GHz, consistent with the presence of non-thermal emission that is reduced at low frequencies by free-free absorption. This emission must lie outside the radio ``photosphere,'' leading us to estimate a lower limit to the physical size of the non-thermal emitting region that is larger than expected from current theory. Based on a radio and infrared comparison to WR 104 and 98a, we conclude that WR 112 is a likely candidate pinwheel nebula, but its temporal variability indicates an eccentric binary orbit or a pinwheel viewed nearly edge-on. A sensitive radio survey of IR-bright WRs would stringently test the hypothesis that colliding winds lie at the heart of_all_ dusty WR systems. We also discuss the effects of dust obscuration in the ultra-violet and how radio-determined mass-loss rates of pinwheel nebulae (and dusty WR stars in general) may be underestimated due to shadowing effects.
description: 21 pages, 5 figures. Accepted for publication in Astrophysical Journal (2002 Feb 10)
Why Every Bipolar Planetary Nebula is `Unique'
Creators: name: Soker, Noam
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the many evolutionary routes that progenitors of bipolar planetary nebulae (BPNe) can take. Overall, there are about a hundred qualitatively different evolutionary routes, hence about a hundred qualitatively different types of BPNe. Within each type there are quantitative differences as well. Adding the dependence of the appearance on inclination, we find that the number of different apparent structures of BPN is about equal to, or even larger than the number of known BPNe and proto-BPNe. Accordingly we argue that every BPN is a `unique' object in its appearance, but all can be explained within the binary model paradigm. Therefore, we request a stop to the attaching of adjectives such as `unique', `peculiar', and `unusual' to BPNe and proto-BPNe, thereby removing the need to invoke a new model for almost every `unusual' BPN. As a case study we try to build a binary model for the proto-BPN OH231.8+4.2. In our preferred model the AGB Mira-type star has a main sequence companion of mass 1 Mo, orbital period of five years, and eccentricity of 0.1.
description: 11 pages, 1 Table; Submitted to MNRAS
Additional file 3 of Change in mean salt intake over time using 24-h urine versus overnight and spot urine samples: a systematic review and meta-analysis
Creators: name: Santos, Joseph Alvin
name: Li, Ka Chun
name: Huang, Liping
name: Mclean, Rachael
name: Petersen, Kristina
name: Di Tanna, Gian Luca
name: Webster, Jacqui
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Cancer
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy

description: Additional file 3. Random effects model based on the DerSimonian-Laird method. Additional file 3 contains the pooled effect estimates using the method of DerSimonian and Laird.
Risky Action Recognition in Lane Change Video Clips using Deep Spatiotemporal Networks with Segmentation Mask Transfer
Creators: name: Yurtsever, Ekim
name: Liu, Yongkang
name: Lambert, Jacob
name: Miyajima, Chiyomi
name: Takeuchi, Eijiro
name: Takeda, Kazuya
name: Hansen, John H. L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Artificial Intelligence (cs.AI)
subject: Machine Learning (cs.LG)
subject: Image and Video Processing (eess.IV)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Advanced driver assistance and automated driving systems rely on risk estimation modules to predict and avoid dangerous situations. Current methods use expensive sensor setups and complex processing pipeline, limiting their availability and robustness. To address these issues, we introduce a novel deep learning based action recognition framework for classifying dangerous lane change behavior in short video clips captured by a monocular camera. We designed a deep spatiotemporal classification network that uses pre-trained state-of-the-art instance segmentation network Mask R-CNN as its spatial feature extractor for this task. The Long-Short Term Memory (LSTM) and shallower final classification layers of the proposed method were trained on a semi-naturalistic lane change dataset with annotated risk labels. A comprehensive comparison of state-of-the-art feature extractors was carried out to find the best network layout and training strategy. The best result, with a 0.937 AUC score, was obtained with the proposed network. Our code and trained models are available open-source.
description: 8 pages, 3 figures, 1 table. The code is open-source
title: The Electronic Spectroscopy of Neutral and Ionic Clusters
Creators: name: Bieske, Evan John
Publisher: name: Griffith University
Year: 1989
Subjects: subject: Electronic spectroscopy
subject: Neutral clusters
subject: Ionic clusters
subject: van der Waals frequencies
subject: Hamiltonians

description: This thesis is concerned with weakly bound neutral and ionic clusters. Spectra of the region near the S1fS0 electronic origin of four neutral van der Waals molecules - aniline-argon, phenol-argon, chlorobenzene-argon and fluorobenzene-argon - were obtained using resonance enhanced multiphoton ionization (REMPI). These spectra indicate that Fermi resonances between van der Waals stretching and bending motions are important in these molecules. Effective Hamiltonians are constructed that describe well the low frequency vibrations. In order to better discuss the low frequency van der Waals motions of aromatics bound to one and two rare gas atoms a simple model for the vibrations is developed. The model enables expression of van der Waals frequencies in terms of fundamental molecular properties and enables facile comparison of effective force constants in a variety of van der Waals molecules. The model is successfully employed to explain van der Waals vibrational structure associated with the origin region of aniline-(argon)2 using van der Waals potential parameters derived from the aniline-(argon)1 spectrum. REMPI and emission spectra of larger clusters of aniline and argon are also reported and discussed. Using atom-atom potentials, equilibrium structures for aniline-(argon)n (n=l, 2, 3) are calculated. The calculations prove useful in the analysis of the spectra.The BfX transitions of the cation complexes fluorobenzene+-argon and chlorobenzene+-argon have been investigated. The cations were prepared by resonance enhanced multiphoton ionization of the neutral van der Waals molecules. A time delayed tunable dye laser was then used to dissociate the cations, loss of an argon atom being the dominant process. When the second laser was tuned to a cation resonance the dissociation cross section increased markedly, allowing characterization of BfX transition. The resulting spectra are presented and discussed.
Beam Models for Gamma-Ray Bursts Sources: Outflow Structure, Kinematics and Emission Mechanisms
Creators: name: Ramirez-Ruiz, Enrico
name: Lloyd-Ronning, Nicole M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The variety of gamma-ray burst phenomenology could be largely attributable to differences in the opening angle of an isotropic outflow or to a standard type of event viewed from different orientations. Motivated by this currently popular idea, we study the effects of varying the energy per unit solid angle in the unsteady expelled outflow by an increase either in the bulk Lorentz factor or in the baryon loading. We apply these models to interpret the observed correlations between variability, luminosity and spectral peak energy and find that while the latter scenario fails to provide a good description, bursts produced by collisions between similar mass shells but with increasingly large Lorentz factors are both more variable and have larger peak spectral energies. We present detailed internal shock calculations confirming this interpretation and discuss the roles various timescales, radii and the optical thickness of the wind play in determining this wide range of behaviors. Finally, we discuss the variety of scenarios in which large variations of the source expansion velocity are naturally expected.
description: 17 pages, 5 figures, with final revisions
Coelogyne tricallosa 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 tricallosa

description: Coelogyne tricallosa (Rolfe) M.W.Chase & Schuit., comb. nov.
 Basionym: Panisea tricallosa Rolfe, Bull. Misc. Inform. Kew 1901: 148 (1901).
 Homotypic synonym: Sigmatogyne tricallosa (Rolfe) Pfitzer in H.G.A.Engler (ed.), Pflanzenr., IV, 50(32): 133 (1907).
 Heterotypic synonyms: Sigmatogyne pantlingii Pfitzer in H.G.A.Engler (ed.), Pflanzenr., IV, 50(32): 134 (1907). Panisea pantlingii (Pfitzer) Schltr., Orchideen Beschreib. Kult. Zücht.: 155 (1914). Sigmatogyne bia Kerr, J. Siam Soc., Nat. Hist. Suppl. 9: 236 (1933). Panisea bia (Kerr) Tang & F.T.Wang, Acta Phytotax. Sin. 1: 79 (1951). Panisea unifolia S.C.Chen, Acta Bot. Yunnan. 2: 304 (1980).
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
Additional file 5 of Change in mean salt intake over time using 24-h urine versus overnight and spot urine samples: a systematic review and meta-analysis
Creators: name: Santos, Joseph Alvin
name: Li, Ka Chun
name: Huang, Liping
name: Mclean, Rachael
name: Petersen, Kristina
name: Di Tanna, Gian Luca
name: Webster, Jacqui
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Cancer
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy

description: Additional file 5. Sensitivity analyses forest plots. Additional file 5 contains the forest plots of the three sensitivity analyses conducted: (a) using the Intersalt equation for studies that used spot-based equation; (b) using alternative follow-up data point (second-to-last), and; (c) excluding studies of poor quality.
title: Translating Song Writing to a Recorded Work: Comparing Two Modes of Music Production from the Perspective of the Songwriter
Creators: name: James, Caleb Paul
Publisher: name: Griffith University
Year: 2016
Subjects: subject: Song writing
subject: Music production
subject: Songwriter
subject: Performance
subject: Creative objectivity

description: The collaboration of music producer and artist has long been an effective and successful one, with the former providing oversight, technical knowledge and some portion of creative objectivity, and the latter focused on the delivery of a performance. Even after the emergence of song-writing artists such as The Beatles, producers were still regarded as specialists in their own right because they were highly trained studio technicians operating equipment far beyond the budgets of average musicians. With the increased availability of affordable technology, one person can now fill all roles, acting as creator, performer and producer. This has seen a reduction in the traditional separation of artist/creator and production roles, and led to environments where one person can be all entities. Although this can provide an efficient and convenient solution for many artists, is it always ideal? Does it provide a more effective translation of the original vision, or does the lack of objective oversight and collaborative input prevent discovery of more potent outcomes? This thesis explores the nature of decision-making processes, both creative and practical, undertaken by an artist/creator acting as the music producer of recordings of their own songs, and compares this with input from an external co-producer. A case study will be used as the primary vehicle for analysis along with direct comparison of original demos and final rendered recordings resulting from the production process.
Chandra observations of NGC 253. II: On the origin of diffuse X-ray emission in the halos of starburst galaxies
Creators: name: Strickland, D. K.
name: Heckman, T. M.
name: Weaver, K. A.
name: Hoopes, C. G.
name: Dahlem, M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a detailed case study of the diffuse X-ray and H-alpha emission in the halo of NGC 253, a nearby edge-on starburst galaxy driving a galactic superwind. The arcsecond spatial resolution of the Chandra ACIS instrument allows us to study the spatial and spectral properties of the diffuse X-ray emitting plasma with greatly superior spatial and spectral resolution compared to previous X-ray instruments. We find statistically significant structure within the X-ray diffuse emission on angular scales down to ~10 arcsec (~130 pc). There is no statistically significant evidence for any spatial variation in the spectral properties of the diffuse emission, over scales from ~400 pc to \~3 kpc. We show that the X-shaped soft X-ray morphology of the superwind, previously revealed by ROSAT, is matched by very similar X-shaped H-alpha emission, extending at least 8 kpc above the plane of the galaxy. In the northern halo the X-ray emission appears to lie slightly interior to the boundary marked by the H-alpha emission. The total 0.3-2.0 keV energy band X-ray luminosity of the northern halo, L_X ~ 5e38 erg/s, is very similar to the halo H-alpha luminosity of L_Ha ~ 4e38 erg/s, both of which are a small fraction of the estimated wind energy injection rate of ~1e42 erg/s from supernovae in the starburst. We show that there are a variety of models that can simultaneously explain spatially-correlated X-ray and H-alpha emission in the halos of starburst galaxies. These findings indicate that the physical origin of the X-ray-emitting million-degree plasma in superwinds is closely linked to the presence of much cooler and denser T ~ 1e4 K gas, not only within the central kpc regions of starbursts, but also on ~10 kpc-scales within the halos of these galaxies. (Abridged)
description: Accepted for publication in the ApJ. LOW RESOLUTION version with 42 pages and 11 figures. For a postscript with decent-quality figures please access http://proteus.pha.jhu.edu/~dks/dks_published.html
Additional file 1: of â Thinking outside the boxâ : advanced geriatric nursing in primary health care in Scandinavia
Creators: name: Boman, Erika
name: Ann-Louise Glasberg
name: Levy-Malmberg, Rika
name: FagerstrĂśm, Lisbeth
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Marine Biology
subject: Cancer
subject: Science Policy

description: Interview guide. (DOCX 16 kb)
Chandra X-Ray Spectroscopy and Imaging of the Galaxy Cluster PKS 0745-191
Creators: name: Hicks, Amalia K.
name: Wise, Michael W.
name: Houck, John C.
name: Canizares, Claude R.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a detailed spectral and spatial analysis of the galaxy cluster PKS 0745-191, using recent observations from the Chandra X-ray Observatory. The data provide information on the temperature and metallicity of the intracluster medium, the distribution of emission throughout the cluster, morphology of the cluster core, and an independent mass estimate which can be compared to that from gravitational lensing. X-ray spectra extracted from the central 300 kpc (~2 arcmin) are well described by a two-temperature plasma and the mean cluster temperature is consistent with previously determined values. The distribution of both temperature and metallicity within the inner 360 kpc (2.3 arcmin) of PKS 0745-191 is probed on scales of 8 arcsec (~20 kpc), yielding a relatively constant abundance throughout the region and a strong temperature gradient (down to ~4-5 keV) within the central 215 kpc. Beta-model fits to the surface brightness profile of PKS 0745-191 indicate that a second beta-model component is required to fit the inner ~10 kpc. Imaging analysis of the cluster core reveals an irregular morphology within the inner 50 kpc, and confirms that the X-ray emission peak lies within 0.5 arcsec (the spatial resolution of Chandra) of both the optical and radio central cD positions. The cluster mass, based on both two temperature and multiphase fits to the X-ray spectrum, is in close agreement with lensing mass estimates of PKS-0745-191.
description: 30 pages, 4 tables, 10 figures
title: Strontianit
title: von der Entdeckung des Strontiums im Strontianit durch Klaproth und Hope 1793 über den Bergbau im Münsterland 1880 zu modernen Anwendungen von Strontium und seinen Verbindungen in Technik und Medizin
titleType: Subtitle
Creators: name: Börnchen, Martin
Publisher: name: Freie Universität Berlin
Year: 2005
Subjects: subject: 500 Naturwissenschaften und Mathematik::550 Geowissenschaften, Geologie::550 Geowissenschaften

description: Führer durch eine Ausstellung von Dr. Martin Börnchen in Zusammenarbeit mit dem Galilei Gymnasium Hamm/Westf. in der Universitätsbibliothek der Freien Universität Berlin vom 7. November bis 31. Dezember 2005
Variability in the extreme helium star LSS 5121
Creators: name: Woolf, V. M.
name: Cuadrado, R. Aznar
name: Pandey, G.
name: Jeffery, C. Simon
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report a photometric and spectroscopic study of the hot extreme helium star LSS 5121. We found photometric variability, but no period was evident in its periodogram. This is consistent with the previous proposal, based on spectral line variations, that LSS 5121 is a non-radial pulsator similar to other hot extreme helium stars.
description: 5 pages, 6 figures
Physical Constraints From Broadband Afterglow Fits:GRB000926 as an Example
Creators: name: Yost, Sarah A.
name: Sari, Re'em
name: Harrison, Fiona A.
name: Berger, Edo
name: Diercks, Alan
name: Galama, Titus
name: Reichart, Dan
name: Frail, Dale
name: Price, Paul A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We develop a model to fit the broadband afterglows of GRBs from the intrinsic parameters of the fireball's synchrotron emission, and apply it to a few well-studied events, with the goal of constraining the intrinsic variability of GRB parameters. We give an example here of fitting to the recent bright event GRB000926.
description: to appear in the proceedings of the Roma 2000 GRB Workshop 3 pages, 3 figures
Heterhelus Jacquelin du Val 1858
Creators: name: Hisamatsu, Sadatomo
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Kateretidae
Heterhelus

description: Genus Heterhelus Jacquelin du Val, 1858
 Type species. Cercus sambuci Erichson, 1843 (= Heterhelus scutellaris (Heer, 1841)) (original designation).
 Diagnosis. Body oval, convex dorsally. Pronotum transverse, projecting at mid-length or uniformly rounded lateral margins; disc with punctures smaller than eye facet; posterior angles obtusely angulate; basal margin nearly straight or with slight curvature. Male abdominal tergite VIII externally visible. Tarsal claws simple. Ovipositor with long or short styli.
 Bionomics. Inclusive species are associated with Sambucus (SPORNRAFT 1967, KIRK- SPRIGGS 1996, AUDISIO 1993, JELÍNEK & CLINE 2010).
 Distribution. Seven species are known worldwide. They are distributed in the Nearctic, Palaearctic, and Oriental Regions (S-T. HISAMATSU & LEE 2007, JELÍNEK & CLINE 2010).
 Note. Palaearctic species were treated by several authors (SPORNRAFT 1967, KIREJTSHUK 1992, AUDISIO 1993, KIRK- SPRIGGS 1996). Nearctic species were studied by PARSONS (1943), and are currently under revision (Cline & Audisio, pers. comm.). Boreades Parsons, 1943 was synonymized under Heterhelus (AUDISIO 1993, JELÍNEK & AUDISIO 2007). S-T. HISAMATSU & LEE (2007) described Taiwanoheterhelus S-T. Hisamatsu & Lee, 2007 as a subgenus of Heterhelus, and treated Boreades as a valid subgenus of Heterhelus as well.
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 pages 562-563, DOI: 10.5281/zenodo.5329313
Feynman integrals as A-hypergeometric functions
Creators: name: de la Cruz, Leonardo
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We show that the Lee-Pomeransky parametric representation of Feynman integrals can be understood as a solution of a certain Gel'fand-Kapranov-Zelevinsky (GKZ) system. In order to define such GKZ system, we consider the polynomial obtained from the Symanzik polynomials $g=\mathcal{U}+\mathcal{F}$ as having indeterminate coefficients. Noncompact integration cycles can be determined from the coamoeba---the argument mapping---of the algebraic variety associated with $g$. In general, we add a deformation to $g$ in order to define integrals of generic graphs as linear combinations of their canonical series. We evaluate several Feynman integrals with arbitrary non-integer powers in the propagators using the canonical series algorithm.
description: 45 pages, 11 figures, codimension 2 example added, references added. Version to be published
title: Diffusion of the Adoption of Online Retailing in Saudi Arabia
Creators: name: Al Ghamdi, Rayed Abdullah
Publisher: name: Griffith University
Year: 2014
Subjects: subject: Oil and natural gas, Saudi Arabia
subject: Kingdom of Saudi Arabia (KSA) energy
subject: e-commerce, Saudi Arabia

description: Despite the fact that the Kingdom of Saudi Arabia (KSA) is a leading producer of oil and natural gas (CIA 2012), a member of G-20, has the largest and fastest growth of ICT marketplaces in the Arab region (U.S. Commercial Services 2008, Alfuraih 2008), including computer hardware and software, and is very wealthy, online retailing activities are not progressing at the same speed of its growing ICT marketplace (CITC 2011). For this reason, this thesis explores the factors influencing the slow progress of online retailing in Saudi Arabia. While several studies exist investigating factors influencing e-commerce adoption by organizations, this thesis is different in that it suggests that the stage of e-commerce maturity of companies is important when considering why companies do or do not adopt e-commerce and how companies can be encouraged to move to a higher stage of maturity. Thus, the present thesis considered the factors influencing e-commerce adoption by retailers in Saudi Arabia based on stages of e-commerce maturity of each organization. To evaluate the stage of e-commerce maturity among retailers in Saudi Arabia, the Stage Of Growth E-business (SOG-e) model of Mckay, Marshall and Pranato 2000 was adopted.
Unsupervised Extractive Dialogue Summarization in Hyperdimensional Space
Creators: name: Park, Seongmin
name: Kim, Kyungho
name: Seo, Jaejin
name: Lee, Jihwa
Publisher: name: arXiv
Year: 2024
Subjects: subject: Computation and Language (cs.CL)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: We present HyperSum, an extractive summarization framework that captures both the efficiency of traditional lexical summarization and the accuracy of contemporary neural approaches. HyperSum exploits the pseudo-orthogonality that emerges when randomly initializing vectors at extremely high dimensions ("blessing of dimensionality") to construct representative and efficient sentence embeddings. Simply clustering the obtained embeddings and extracting their medoids yields competitive summaries. HyperSum often outperforms state-of-the-art summarizers -- in terms of both summary accuracy and faithfulness -- while being 10 to 100 times faster. We open-source HyperSum as a strong baseline for unsupervised extractive summarization.
description: ICASSP 2024
Many-Body Expanded Full Configuration Interaction. II. Strongly Correlated Regime
Creators: name: Eriksen, Janus J.
name: Gauss, Jürgen
Publisher: name: arXiv
Year: 2019
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: In this second part of our series on the recently proposed many-body expanded full configuration interaction (MBE-FCI) method, we introduce the concept of multideterminantal expansion references. Through theoretical arguments and numerical validations, the use of this class of starting points is shown to result in a focussed compression of the MBE decomposition of the FCI energy, thus allowing chemical problems dominated by strong correlation to be addressed by the method. The general applicability and performance enhancements of MBE-FCI are verified for standard stress tests such as the bond dissociations in H$_2$O, N$_2$, C$_2$, and a linear H$_{10}$ chain. Furthermore, the benefits of employing a multideterminantal expansion reference in accelerating calculations of high accuracy are discussed, with an emphasis on calculations in extended basis sets. As an illustration of this latter quality of the MBE-FCI method, results for H$_2$O and C$_2$ in basis sets ranging from double- to pentuple-$ζ$ quality are presented, demonstrating near-ideal parallel scaling on up to almost $25000$ processing units.
description: 41 pages, 4 tables, 10 figures, 1 SI attached as an ancillary file
The Effect of Vacuum Polarization and Proton Cyclotron Resonances on Photon Propagation in Strongly Magnetized Plasmas
Creators: name: Ozel, Feryal
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We consider the effects of vacuum polarization and proton cyclotron resonances on the propagation of radiation through a strongly magnetized plasma. We analyze the conditions under which the photons evolve adiabatically through the resonant density and find that the adibaticity condition is satisfied for most photon energies of interest, allowing for a normal-mode treatment of the photon propagation. We then construct radiative equilibrium atmosphere models of strongly magnetized neutron stars that includes these effects, employing a new numerical method that resolves accurately the sharp changes of the absorption and mode-coupling cross sections at the resonant densities. We show that the resulting spectra are modified by both resonances and are harder at all field strengths than a blackbody at the effective temperature. We also show that the narrow absorption features introduced by the proton cyclotron resonance have small equivalent widths. We discuss the implications of our results for properties of thermal emission from the surfaces of young neutron stars.
description: 15 pages, 4 figures, submitted to ApJ
title: China's Peacekeeping Policy in Mali
title: New Security Thinking or Balancing Europe?
titleType: Subtitle
Creators: name: Lanteigne, Marc
Publisher: name: Freie Universität Berlin
Year: 2014
Subjects: subject: Peacekeeping
subject: China
subject: EU
subject: Security
subject: Mali
subject: Humanitarian Intervention
subject: Peacebuilding
subject: 300 Sozialwissenschaften::360 Soziale Probleme, Sozialdienste::361 Soziale Probleme und Sozialhilfe im Allgemeinen
subject: 300 Sozialwissenschaften::320 Politikwissenschaft
subject: 300 Sozialwissenschaften::320 Politikwissenschaft::327 Internationale Beziehungen

description: In mid-2013, China’s increasingly positive policies towards United Nations peacekeeping reached a milestone when the country agreed to send a large detachment of personnel, including combat forces for the first time, to the UN Multidimensional Integrated Stabilisation Mission in Mali (known by its French acronym MINUSMA). This commitment was also distinct in that the mission was not in a region which represented direct Chinese economic interests, unlike other African peacekeeping missions in which Beijing has offered support. Rather, the Mali operation has both cemented Beijing’s larger commitment to building African partnerships and has demonstrated a marked contrast to the unilateral approach taken by France in pacifying the country. Although China has warmed to the principles of humanitarian intervention in civil conflicts, it retains a wariness towards peacebuilding operations outside the sponsorship of the UN. Therefore, the Mali operation has been beneficial for China, not only in building its peacekeeping credentials in Africa but also in underscoring China’s increasingly distinct, ‘neo-Westphalian’ views on addressing intervention in domestic conflicts.
ОПРЕДЕЛЕНИЯ СПЕЛОСТИ И СБОР УРОЖАЯ ГРАНАТА С ПОМОЩЬЮ ДРОНОВ С ИСКУССТВЕННЫМ ИНТЕЛЛЕКТОМ
Creators: name: Ахмедов А.П., Худойберганов С.Б.,  Ражабов У.А. Нурмонов М.А. Ташкентский государственный транспортный университет
Publisher: name: Zenodo
Year: 2024

description: В настоящее время в мире созданы дроны, предназначенные для сбора фруктов в фруктовом саду. Захват фруктов дронами осуществляется присоской с воздушным подсосом, что минимизирует повреждение плодов. Сорванные фрукты дроны укладывают на ленту платформы, а с неё фрукты попадают в контейнеры для транспортировки на предприятие по упаковке. Предлагается для определения спелости и сбора урожая граната в полевых условиях использовать дроны с роботизированным манипулятором, с помощью которого можно организовать сбор спелых гранат днем и ночью.

Ключевые слова: Робот, дрон, искусственный интеллект, фрукт, гранат, квадрокоптер, роботизированный манипулятор
Coelogyne triloba 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 triloba

description: Coelogyne triloba (Ridl.) M.W.Chase & Schuit., comb. nov.
 Basionym: Platyclinis triloba Ridl., Sarawak Mus. J. 1(2): 35 (1912).
 Homotypic synonym: Dendrochilum trilobum (Ridl.) Ames, J. Straits Branch Roy. Asiat. Soc. 84(Spec. No.): 149 (1921).
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
Implementation of Transgender/Gender Nonbinary Care in a Family Medicine Teaching Practice
Creators: name: Harless, Chase
name: Ulrich, Irene Park
name: Knoll, Heidi
name: Sullivan, Lindsay
name: Reed, Lisa
name: Caldwell, Jenna
name: Kim, Annie
name: Seamon, Gwen
Publisher: name: American Board of Family Medicine (ABFM)
Year: 2022

description:
PURPOSE: Numerous studies have shown that transgender or gender nonbinary (TGNB) individuals encounter significantly more health care barriers, including overall lack of access to gender-affirming care providers. This study describes 2 assessments of transgender care services at a large family medicine teaching practice. METHODS: Staff and providers were invited to attend an optional, practice-wide, hourlong free training session on gender-affirming care offered on 3 different dates in 2019. A structured protocol was used to collect observational data from which key takeaways from the training sessions were developed. Separately, a retrospective chart review of patients with a gender dysphoria diagnosis was completed. Charts were reviewed for adherence to regional and international organization recommendations for comprehensive transgender care. RESULTS: Three main takeaways from the training sessions included lack of knowledge or familiarity with gender terminology and expression, fear of offending patients, and employee hesitation to change behaviors when interacting with patients. On chart review, the most common interventions identified were need to schedule a follow-up visit (61.5%), need for health maintenance screenings (osteoporosis screening, 50%; Papanicolaou smear, 56.3%; mammogram, 66.7%), need for mental health screening (41.5%), need for laboratory monitoring of testosterone therapy (20%), and corrected gender markers/names listed in the appropriate place in the patient chart (16.9%). CONCLUSIONS: This study highlighted hesitation to provide and lack of familiarity with transgender care among practice staff. Although some aspects of comprehensive transgender care are well implemented, maintaining follow-up, completing health maintenance and mental health screenings, and appropriate laboratory monitoring are areas for improvement.
Soft X-ray excess emission in clusters of galaxies observed with XMM-Newton
Creators: name: Nevalainen, J.
name: Lieu, R.
name: Bonamente, M.
name: Lumb, D.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results on the spectroscopic analysis of XMM-Newton EPIC data of the central 0.5/h_50 Mpc regions of the clusters of galaxies Coma, A1795 and A3112. The temperature of the hot intracluster gas as determined by modeling the 2 - 7 keV PN and MOS data is consistent with that inferred from the FeXXV-FeXXVI line ratio. A significant warm emission component at a level above the systematic uncertainties is evident in the data and confirmed by ROSAT PSPC data for Coma and A1795. The non-thermal origin of the phenomenon cannot be ruled out at the current level of calibration accuracy, but the thermal model fits the data significantly better, with temperatures in the range of 0.6 -- 1.3 keV and electron densities of the order of 10^{-4} -- 10^{-3} cm^{-3}. In the outer parts of the clusters the properties of the warm component are marginally consistent with the results of recent cosmological simulations, which predict a large fraction of the current epoch's bayons located in a warm-hot intergalactic medium (WHIM). However, the derived densities are too high in the cluster cores, compared to WHIM simulations, and thus more theoretical work is needed to fully understand the origin of the observed soft X-ray excess.
description: ApJ in press, 14 pages, 4 color figures WHIM discussion modified
title: Antioxidant Systems, Thioredoxin and DJ-1: Novel Therapeutic Targets in Multiple Myeloma
Creators: name: Raninga, Prahlad Vinodbhai
Publisher: name: Griffith University
Year: 2017
Subjects: subject: Multiple myeloma
subject: Plasma cells
subject: Bone marrow
subject: Proteasome inhibitors
subject: Myeloma patients
subject: Antioxidant systems

description: Multiple myeloma (MM) is a plasma cell malignancy characterized by an accumulation of malignant clonal plasma cells in the bone marrow (BM). In recent years, many effective anti-MM drugs have been developed including proteasome inhibitors and immunomodulators. Introduction of the proteasome inhibitor bortezomib has improved prognosis and survival in MM patients. However, upon prolonged drug treatment, myeloma cells acquire resistance to the given treatment including bortezomib, resulting in disease relapse. Studies have shown that the BM in myeloma patients is extensively hypoxic (1% O2) compared to the BM in healthy individuals. Hypoxia is a crucial microenvironmental factor that plays an important role in MM disease progression and drug resistance. Due to the development of drug resistance, MM remains an incurable disease with the median survival of only 3 to 5 years. Thus, novel therapeutic strategies are required to kill myeloma cells growing under physiological O2 conditions, including hypoxic microenvironments, and to overcome both acquired and hypoxia-induced drug resistance to improve MM patient survival and prognosis.
Nucleosynthesis of Zinc and Iron-Peak Elements in Pop III Type II Supernovae : Comparison with abundances of Very Metal-Poor Halo Stars
Creators: name: Umeda, Hideyuki
name: Nomoto, Ken'ichi
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We calculate nucleosynthesis in core-collapse explosions of massive Pop III stars, and compare the results with abundances of metal-poor halo stars to constrain the parameters of Pop III supernovae. We focus on iron-peak elements and, in particular, we try to reproduce the large [Zn/Fe] observed in extremely metal-poor stars. The interesting trends of the observed ratios [Zn, Co, Mn, Cr, V/Fe] can be related to the variation of the relative mass of the complete and incomplete Si-burning regions in supernova ejecta. We find that [Zn/Fe] is larger for deeper mass-cuts, smaller neutron excess, and larger explosion energies. The large [Zn/Fe] and [O/Fe] observed in the very metal-poor halo stars suggest deep mixing of complete Si-burning material and a significant amount of fall-back in Type II supernovae. Furthermore, large explosion energies (E_51 >~ 2 for M ~ 13 Msun and E_51 >~ 20 for M >~ 20 Msun) are required to reproduce [Zn/Fe] ~ 0.5. The observed trends of the abundance ratios among the iron-peak elements are better explained with this high energy (``Hypernova'') models rather than the simple ``deep'' mass-cut effect, because the overabundance of Ni can be avoided in the hypernova models. We also present the yields of pair-instability supernova explosions of M = 130 - 300 Msun stars, and discuss that the abundance features of very metal-poor stars cannot be explained by pair-instability supernovae.
description: 32 pages, 19 figures, 18 tables. To appear in the Astrophysical Journal 2002, 565. Table 18 of yields of Pop III Pair-Instability Supernovae is replaced with a new one
Coelogyne truncata 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 truncata

description: Coelogyne truncata (J.J.Sm.) M.W.Chase & Schuit., comb. nov.
 Basionym: Dendrochilum truncatum J.J.Sm., Bull. Jard. Bot. Buitenzorg, sér. 2, 25: 12 (1917).
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