cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Notoxus noctivagus Krekich-Strassoldo 1913
Creators: name: Kejval, Zbyněk
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Anthicidae
Notoxus
Notoxus noctivagus

description: Notoxus noctivagus species-group
 Diagnosis. Elytral apices in males mostly clearly modified, with distinct apical tubercle / notch, rarely simple (N. katthapa sp. nov.); median lobe of aedeagus symmetrical, with distinct dorsal plate; latero-basal fovea of abdominal sternum III rather shallow, forming narrow impression along basal sulcus of sternum (Fig. 68).
 Species included. Notoxus ales Telnov, 2007, N. andrewesi Krekich-Strassoldo, 1913, N. garuda sp. nov., N. katthapa sp. nov., N. impavidus sp. nov., N. inbasaliformis sp. nov., N. inbasalis Pic, 1926, N. noctivagus Krekich-Strassoldo, 1913, N. peguensis Pic, 1914, N. safraneki sp. nov., N. sinensis Pic, 1907, N. sodalis sp. nov., and N. suturalifer Pic, 1932.
 Remarks. Four species of this group have robust, dorsally coarsely and densely rugose pronotal horn with nearly indistinct crest, more or less emarginate male sternum VII, and rather uniform morphology of the aedeagus (Figs. 29, 33, 38 and 42). At least two Afrotropical species, distributed in northern Sub-Saharan part of Africa, appear to be very close to this subgroup; see Remarks under N. peguensis and description of N. pericarti Bonadona, 1984 by BONADONA (1984).
description: Published as part of Kejval, Zbyněk, 2011, Taxonomic revision of the Oriental species of Notoxus (Coleoptera: Anthicidae), pp. 627-673 in Acta Entomologica Musei Nationalis Pragae 51 (2) on page 642, DOI: 10.5281/zenodo.5329507
Images of analytic map germs, and singular fibrations
Creators: name: Joiţa, Cezar
name: Tibăr, Mihai
Publisher: name: arXiv
Year: 2019
Subjects: subject: Complex Variables (math.CV)
subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 14D06, 32S55, 58K05, 57R45, 14P10, 32S20, 32S60, 58K15, 57Q45, 32C40

description: For a map germ $G$ with target $(\mathbb C^{p}, 0)$ or $(\mathbb R^{p}, 0)$ with $p\ge 2$, we address two phenomena which do not occur when $p=1$: the image of $G$ may be not well-defined as a set germ, and a local fibration near the origin may not exist. We show how these two phenomena are related, and how they can be characterised.
description: revised, to appear in Europ. J. Math
The Structure of Stellar Coronae in Active Binary Systems
Creators: name: Sanz-Forcada, J.
name: Brickhouse, N. S.
name: Dupree, A. K.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A survey of 28 stars using EUV spectra has been conducted to establish the structure of stellar coronae in active binary systems from the EMD, electron densities, and scale sizes. Observations obtained by the EUVE during 9 years of operation are included for the stars in the sample. EUVE data allow a continuous EMD to be constructed in the range log T~5.6-7.4, using iron emission lines. These data are complemented with IUE observations to model the lower temperature range. Inspection of the EMD shows an outstanding narrow enhancement, or ``bump'' peaking around log T~6.9 in 25 of the stars, defining a fundamental coronal structure. The emission measure per unit stellar area decreases with increasing orbital (or photometric) periods of the target stars; stars in binaries generally have more material at coronal temperatures than slowly rotating single stars. High electron densities (Ne>10^12 cm^-3) are derived at ~10 MK for some targets, implying small emitting volumes. The observations suggest the magnetic stellar coronae of these stars are consistent with two basic classes of magnetic loops: solar-like loops with maximum temperature around log T~6.3 and lower electron densities (Ne>10^9-10.5), and hotter loops peaking around log T~6.9 with higher electron densities (Ne>10^12). For the most active stars, material exists at much higher temperatures (log T>6.9) as well. However, current ab initio stellar loop models cannot reproduce such a configuration. Analysis of the light curves of these systems reveals signatures of rotation of coronal material, as well as apparent seasonal changes in the activity levels.
description: 45 pages, 9 figures (with 20 eps files). Accepted for its publication in ApJS
title: Mass and Heat Transfer in Intermetallic-Hydrogen Storage Tanks
Creators: name: Seyed Mohammadshahi, Shahrzad
Publisher: name: Griffith University
Year: 2017
Subjects: subject: Hydrogen storage
subject: Metal-hydrides (MH)
subject: Intermetallic-hydrogen storage tanks
subject: Mass and heat transfer

description: Hydrogen is a potential future energy carrier, but reliable storage of the hydrogen is required for widespread use. Metal-hydrides (MH) are suitable materials for safe, stable and long-term hydrogen storage applications such as off-grid and hybrid solar systems due to the ability to store hydrogen at moderate pressure and temperature. However, poor thermal properties of MH beds coupled with the need for managing the significant amount of heat generated during the absorption and desorption reactions, is a serious barrier for fast hydrogen uptake and release unless an efficient design for the MH tank and the heat exchange system is used. Appropriate design of the tank and thermal management systems as well as a suitable choice of material can improve the performance of the MH systems and make them more suitable for commercial use. It is not usually practicable to build and test different MH tanks for large scale applications and explore the impact of different design and process parameters on the performance of the tanks. In contrast, mathematical models can be employed for examining various parameters, scenarios and used to predict the effect on the MH system without the cost of materials and manufacturing time. These models, however, must be accurate in order to reliably design large scale MH tanks and components and this accuracy can be achieved by refinement of the model’s parameters and equations based on practical systems. In turn, the accuracy of the model also needs to be validated through experimental data obtained from operating tank systems under different conditions.
Nature of widely separated ultraluminous infrared galaxies
Creators: name: Dinh-V-Trung
name: Lo, K. Y.
name: Kim, D. -C.
name: Gao, Yu
name: Gruendl, R. A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In the complete sample of ultraluminous infrared galaxies (ULIRGs) compiled by Kim (1995) about 5% consists of widely separated galaxies which are presumably in the early phase of interaction. This fact is contrary to the conventional view that ULIRGs are in the final stages of the merger of two gas-rich disk galaxies. We have undertaken high resolution CO(J=1-0) observations for the ultraluminous infrared galaxies that have nuclear separations larger than 20 kpc. We have detected the CO emission in 5 out of 6 systems, but only in one component of the ULIRG pairs. 4 of them have LINER spectral type and 1 galaxy has Seyfert II spectral type. In K'-band images these components are also brighter than the other components which have either HII-region spectra or no detectable emission lines. Using the standard conversion factor, the molecular gas content is estimated to be a few times 10 $^{10}$ M$_\odot$, similar to that of the other ultraluminous galaxies. The result indicates that the galaxy containing the molecular gas is also the source of most, if not all, of the huge far-infrared luminosity of the system. The optical and K'-band imaging observations and optical spectra suggest multiple merger scenario for 1 system. If the remaining systems are in an early stage of a binary tidal interaction, the commonly accepted interpretation of the ULIRG phenomenon as the final merger stage of two disk galaxies may need to be re-examined.
description: 26 pages, 03 figures, accepted for ApJ
Additional file 2: of Dystrophin R16/17 protein therapy restores sarcolemmal nNOS in trans and improves muscle perfusion and function
Creators: name: Junling Zhao
name: Hsiao Yang
name: Lakmini Wasala
name: Keqing Zhang
name: Yongping Yue
name: Dongsheng Duan
name: Lai, Yi
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Figure S2. Schematic outline of the protein injection and experiment timeline. Black arrow: IP injection; Red arrow: IV injection; Green arrow stands for the experiments reported in Fig. 2; Purple arrow stands for the experiments reported in Fig. 5, and Blue arrow stands for the experiments in Figs. 3, 4 and 6. IP: intraperitoneal; IV: intravenous. (PDF 225 kb)
The influence of free neutrons on dynamics and radiation of astrophysical plasmas
Creators: name: Belyanin, A. A.
name: Derishev, E. V.
name: Kocharovsky, V. V.
name: Kocharovsky, Vl. V.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present arguments in favor of the presence of free neutrons in plasmas generated by compact astrophysical objects and find conditions necessary for the formation of the neutron component. The broad range of phenomena caused by neutrons includes both dynamical (sources' variability, transition of fireballs to the two-flow regime) and kinetic (fission of helium nuclei by neutrons, electromagnetic cascade, emission in annihilation and nuclear lines, neutrino losses) effects. The presented theory can be applied to internal regions of accretion disks, jets in microquasars, and gamma-ray burst (GRB) fireballs.
description: Talk presented at the COSMO-01 Workshop, Rovaniemi, Finland, Aug 30 - Sep 4, 2001. 18 pages, LaTeX
Pteria colymbus
Creators: name: Tëmkin, Ilya
Publisher: name: Zenodo
Year: 2006
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Ostreida
Pteriidae
Pteria
Pteria colymbus

description: PTERIA COLYMBUS (RÖDING, 1798)
West Atlantic, FK-048, American Shoals, ocean side, Monroe County, Florida Keys, Florida, USA, 24°31.43′N, 81°31.26′W, scuba, 4.6 m, reef (four pairs with tissue; AMNH 298921); West Atlantic, FK-237, East Turtle Shoal, ocean side off Grassy Key, Monroe County, Florida Keys, Florida, USA, 24°43′15′N, 80°55′42′W, scuba, maximum 4.3 m, patch reef with gorgonians, on sand patches (two pairs with tissue, AMNH 298920); West Atlantic, Gulf beach, at Lighthouse, Sanibel Island, Florida, USA (six pairs; AMNH 210230); West Atlantic, Gulf of Mexico, off Port Isabel, Texas, USA, 32.9 m (ten pairs; AMNH 144391); West Atlantic, Lemon Bay, Florida, USA (five pairs; FMNH 167474); West Atlantic, Swanesborough, North Carolina, USA (one pair; FMNH 184280); West Atlantic, Marco Island, Collie County, Florida, USA (three pairs; FMNH 166368).
Principal reference: Hayes (1972) (gross anatomy).
description: Published as part of Tëmkin, Ilya, 2006, Morphological perspective on the classification and evolution of Recent Pterioidea (Mollusca: Bivalvia), pp. 253-312 in Zoological Journal of the Linnean Society 148 (3) on page 309, DOI: 10.1111/j.1096-3642.2006.00257.x, http://zenodo.org/record/5427755
Additional file 6: of Drivers of hospital expenditure and length of stay in an academic medical centre: a retrospective cross-sectional study
Creators: name: Rahman, Nabilah
name: Ng, Sheryl
name: Sravan Ramachandran
name: Wang, Debby
name: Srinath Sridharan
name: Chuen Tan
name: Khoo, Astrid
name: Tan, Xin
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Science Policy

description: Summary of patient and visit factors of patient who had missing housing type (socio-economic status proxy) (DOCX 15 kb)
Pteria sterna
Creators: name: Tëmkin, Ilya
Publisher: name: Zenodo
Year: 2006
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Ostreida
Pteriidae
Pteria
Pteria sterna

description: PTERIA STERNA (GOULD, 1851)
East Pacific, Gulf of California, Mexico, Guaymas, Sonora, Bahia de Bacochibampo (one pair with tissue, AMNH 311731); same as previous (one pair with tissue, AMNH 311789); East Pacific, San Diego, California, on rocks, just below low tide (one pair; AMNH 206564); East Pacific, Veracruz, Vacamonte, Panama (seven pairs; AMNH 156682); East Pacific, Topolobampo, Mexico (approximately 40 pairs; AMNH 262822); East Pacific, Puerto Penasco, Mexico (two pairs; FMNH 171811).
 Principal reference: Kiefert et al. (2004) (shell microstructure).
description: Published as part of Tëmkin, Ilya, 2006, Morphological perspective on the classification and evolution of Recent Pterioidea (Mollusca: Bivalvia), pp. 253-312 in Zoological Journal of the Linnean Society 148 (3) on page 309, DOI: 10.1111/j.1096-3642.2006.00257.x, http://zenodo.org/record/5427755
Magnetic dipole moments of the spin-$\frac{3}{2}$ doubly heavy baryons
Creators: name: Ozdem, U.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: The magnetic dipole moments of the spin-$\frac{3}{2}$ doubly charmed, bottom and charmed-bottom baryons are obtained by means of the light-cone QCD sum rule. The magnetic dipole moments of these baryons encode essential knowledge of their inner structure and shape deformations. The numerical results are given as, $μ_{Ξ_{cc}^{*++}} = 2.94 \pm 0.95$, $μ_{Ξ_{cc}^{*+}} = - 0.67 \pm 0.11$, $μ_{Ω_{cc}^{*+}} =- 0.52 \pm 0.07$, $μ_{Ξ_{bb}^{*0}} = 2.30 \pm 0.55$, $μ_{Ξ_{bb}^{*-}} = -1.39 \pm 0.32$, $μ_{Ω_{bb}^{*-}} = -1.56 \pm 0.33$, $μ_{Ξ_{bc}^{*+}} = 2.63 \pm 0.82$, $μ_{Ξ_{bc}^{*0}} = - 0.96 \pm 0.32$ and $μ_{Ω_{bc}^{*+}} =- 1.11 \pm 0.33$, respectively.
description: 9 pages, 4 tables and 2 figures
title: Simulating the Antarctic ice sheet in the late-Pliocene warm period
title: PLISMIP-ANT, an ice-sheet model intercomparison project
titleType: Subtitle
Creators: name: Boer, B. De
name: Dolan, A. M.
name: Bernales, J.
name: Gasson, E.
name: Goelzer, H.
name: Golledge, N. R.
name: Sutter, J.
name: Huybrechts, P.
name: Lohmann, G.
name: Rogozhina, I.
name: Abe-Ouchi, A.
name: Saito, F.
name: Wal, R. S. W. Van De
Publisher: name: Freie Universität Berlin
Year: 2015
Subjects: subject: 500 Naturwissenschaften und Mathematik::550 Geowissenschaften, Geologie::551 Geologie, Hydrologie, Meteorologie

description: In the context of future climate change, understanding the nature and behaviour of ice sheets during warm intervals in Earth history is of fundamental importance. The late Pliocene warm period (also known as the PRISM interval: 3.264 to 3.025 million years before present) can serve as a potential analogue for projected future climates. Although Pliocene ice locations and extents are still poorly constrained, a significant contribution to sea-level rise should be expected from both the Greenland ice sheet and the West and East Antarctic ice sheets based on palaeo sea-level reconstructions. Here, we present results from simulations of the Antarctic ice sheet by means of an international Pliocene Ice Sheet Modeling Intercomparison Project (PLISMIP-ANT). For the experiments, ice-sheet models including the shallow ice and shelf approximations have been used to simulate the complete Antarctic domain (including grounded and floating ice). We compare the performance of six existing numerical ice-sheet models in simulating modern control and Pliocene ice sheets by a suite of five sensitivity experiments. We include an overview of the different ice-sheet models used and how specific model configurations influence the resulting Pliocene Antarctic ice sheet. The six ice-sheet models simulate a comparable present-day ice sheet, considering the models are set up with their own parameter settings. For the Pliocene, the results demonstrate the difficulty of all six models used here to simulate a significant retreat or re-advance of the East Antarctic ice grounding line, which is thought to have happened during the Pliocene for the Wilkes and Aurora basins. The specific sea-level contribution of the Antarctic ice sheet at this point cannot be conclusively determined, whereas improved grounding line physics could be essential for a correct representation of the migration of the grounding-line of the Antarctic ice sheet during the Pliocene.
Notoxus andrewesi Krekich-Strassoldo 1913
Creators: name: Kejval, Zbyněk
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Anthicidae
Notoxus
Notoxus andrewesi

description: Notoxus andrewesi Krekich-Strassoldo, 1913
(Figs. 17, 84)
 Notoxus andrewesi Krekich-Strassoldo, 1913: 131, Fig. 2.
 Type locality. South India, Nilgiri Hills.
 Type material examined. SYNTYPES: 1 J, ‘ H.L.Andrewes Nilgiri Hills [p] // [male sex mark] // TYPE [p; red label] // coll. Heberdey [p] // Andrewesi det. v.Krekich [p+h] // Andrewesi Krek. [h; black frame, ochraceous label]’ (NHMW); 1 ♀, same data, except female sex-mark, lacking the last label (NHMW); 1 J 2 ♀♀, ‘ H.L.Andrewes Nilgiri Hills [p] // [male or female sex mark] // TYPE [p; red label] // Andrewesi det. v.Krekich [p+h] // Andrewes Bequest B.M. 1922-221.’ (BMNH).
 Additional material examined. INDIA: TAMIL NADU: 27 JJ 4 ♀♀ Nilgiri hills, Kotagiri env., Elk falls, 76°52′E 11°23′N, 16.xi.1993, Z. Kejval & D. Boukal leg. (ZKDC, ZSMC).
 Diagnosis. Small, slender species; elytra mostly with distinct markings (Fig. 84); eyes rather large; pronotum globose to slightly transverse in dorsal view; pronotal disc evenly convex, smooth, rather glossy, finely punctured; pronotal horn rather long, conspicuously slender, moderately narrowing towards apex, armed with 3–4 distinctly protruding lateral lobules on each side and wider, bilobed apical lobule; horn crest moderately raised, evenly lowering towards horn apex, its lateral margins feebly marked by series of somewhat coarser, distinctly spaced lobules / rugules; punctures in basal half of elytra rather coarse, deep, dot-like, with smooth margins.
Male characters (Elk falls, ZKDC). Elytra clearly modified apically, subtruncate, with rounded gland opening near distinctly protruding lateral angle; legs simple; abdominal sternum VII nearly simple, slightly flattened postero-medially, its posterior margin somewhat unevenly rounded in ventral view; tergum VIII forming narrow, arched sclerite, evenly rounded posteriorly, rather finely and sparsely setose; aedeagus as figured (Fig. 17).
 Variation. Body length (J ♀) 2.8–3.1 mm. Rather strongly variable in extent of dark markings of elytra; some specimens with posterior transverse reddish band reduced to a pair of small, rounded spots, but elytral apices always paler coloured.
 Distribution. India: Tamil Nadu (KREKICH- STRASSOLDO 1913).
 Remarks. KREKICH- STRASSOLDO (1913) described Notoxus andrewesi from a series of specimens deposited in the collection of H. L. Andrewes and in the NHMW (number not stated). It is known reliably only from the Nilgiri Hills in southern India. The records from Nepal and northern India (UHMANN 1990, TELNOV 2003, CHANDLER et al. 2007) are based on misidentified specimens (see Remarks under N. noctivagus and N. inbasaliformis sp. nov.).
description: Published as part of Kejval, Zbyněk, 2011, Taxonomic revision of the Oriental species of Notoxus (Coleoptera: Anthicidae), pp. 627-673 in Acta Entomologica Musei Nationalis Pragae 51 (2) on pages 644-645, DOI: 10.5281/zenodo.5329507
Entanglement of Nanophotonic Quantum Memory Nodes in a Telecom Network
Creators: name: Knaut, Can M.
name: Suleymanzade, Aziza
name: Wei, Yan-Cheng
name: Assumpcao, Daniel R.
name: Stas, Pieter-Jan
name: Huan, Yan Qi
name: Machielse, Bartholomeus
name: Knall, Erik N.
name: Sutula, Madison
name: Baranes, Gefen
name: Sinclair, Neil
name: De-Eknamkul, Chawina
name: Levonian, David S.
name: Bhaskar, Mihir K.
name: Park, Hongkun
name: Lončar, Marko
name: Lukin, Mikhail D.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: A key challenge in realizing practical quantum networks for long-distance quantum communication involves robust entanglement between quantum memory nodes connected via fiber optical infrastructure. Here, we demonstrate a two-node quantum network composed of multi-qubit registers based on silicon-vacancy (SiV) centers in nanophotonic diamond cavities integrated with a telecommunication (telecom) fiber network. Remote entanglement is generated via the cavity-enhanced interactions between the SiV's electron spin qubits and optical photons. Serial, heralded spin-photon entangling gate operations with time-bin qubits are used for robust entanglement of separated nodes. Long-lived nuclear spin qubits are used to provide second-long entanglement storage and integrated error detection. By integrating efficient bi-directional quantum frequency conversion of photonic communication qubits to telecom frequencies (1350 nm), we demonstrate entanglement of two nuclear spin memories through 40 km spools of low-loss fiber and a 35 km long fiber loop deployed in the Boston area urban environment, representing an enabling step towards practical quantum repeaters and large-scale quantum networks.
description: 23 pages, 16 figures
Optical and Infrared Spectroscopy of SN 1999ee and SN 1999ex
Creators: name: Hamuy, Mario
name: Maza, Jose
name: Pinto, Philip A.
name: Phillips, M. M.
name: Suntzeff, Nicholas B.
name: Blum, R. D.
name: Olsen, K. A. G.
name: Pinfield, David J.
name: Ivanov, Valentin D.
name: Augusteijn, T.
name: Brillant, S.
name: Chadid, M.
name: Cuby, J. -G.
name: Doublier, V.
name: Hainaut, O. R.
name: Floc'h, E. Le
name: Lidman, C.
name: Petr-Gotzens, Monika G.
name: Pompei, E.
name: Vanzi, L.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report optical and infrared spectroscopic observations of the Type Ia SN 1999ee and the Type Ib/c SN 1999ex, both of which were hosted by the galaxy IC 5179. For SN 1999ee we obtained a continuous sequence with an unprecedented wavelength and temporal coverage beginning 9 days before maximum light and extending through day 42. Before maximum light SN 1999ee displayed a normal spectrum with a strong Si II 6355 absorption, thus showing that not all slow-declining SNe are spectroscopically peculiar at these evolutionary phases. A comparative study of the infrared spectra of SN 1999ee and other Type Ia supernovae shows that there is a remarkable homogeneity among the Branch-normal SNe Ia during their first 60 days of evolution. SN 1991bg-like objects, on the other hand, display spectroscopic peculiarities at infrared wavelengths. SN 1999ex was characterized by the lack of hydrogen lines, weak optical He I lines, and strong He I 10830,20581, thus providing an example of an intermediate case between pure Ib and Ic supernovae. We conclude therefore that SN 1999ex provides first clear evidence for a link between the Ib and Ic classes and that there is a continuous spectroscopic sequence ranging from the He deficient SNe Ic to the SNe Ib which are characterized by strong optical He I lines.
description: 35 pages, 13 figures, accepted by The Astronomical Journal
Active Transfer Learning for Persian Offline Signature Verification
Creators: name: Younesian, Taraneh
name: Masoudnia, Saeed
name: Hosseini, Reshad
name: Araabi, Babak N.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: Offline Signature Verification (OSV) remains a challenging pattern recognition task, especially in the presence of skilled forgeries that are not available during the training. This challenge is aggravated when there are small labeled training data available but with large intra-personal variations. In this study, we address this issue by employing an active learning approach, which selects the most informative instances to label and therefore reduces the human labeling effort significantly. Our proposed OSV includes three steps: feature learning, active learning, and final verification. We benefit from transfer learning using a pre-trained CNN for feature learning. We also propose SVM-based active learning for each user to separate his genuine signatures from the random forgeries. We finally used the SVMs to verify the authenticity of the questioned signature. We examined our proposed active transfer learning method on UTSig: A Persian offline signature dataset. We achieved near 13% improvement compared to the random selection of instances. Our results also showed 1% improvement over the state-of-the-art method in which a fully supervised setting with five more labeled instances per user was used.
title: Corporate Semantic Web Report VI
title: Validation and Evaluation
titleType: Subtitle
Creators: name: Paschke, Adrian
name: Coskun, Gökhan
name: Harasic, Marko
name: Heese, Ralf
name: Oldakowski, Radoslaw
name: Schäfermeier, Ralph
name: Streibel, Olga
name: Teymourian, Kia
name: Todor, Alexandru
name: Freie Universität Berlin, Institut Für Informatik
Publisher: name: Freie Universität Berlin
Year: 2013
Subjects: subject: Corporate Semantic Web
subject: Corporate Ontology Engineering
subject: Corporate Semantic Collaboration
subject: Corporate Semantic Search
subject: 000 Informatik, Informationswissenschaft, allgemeine Werke::000 Informatik, Wissen, Systeme::004 Datenverarbeitung; Informatik
subject: 000 Informatik, Informationswissenschaft, allgemeine Werke::000 Informatik, Wissen, Systeme

description: In this technical report, we present prototypical implementations of innovative tools and methods for personalized and contextualized (multimedia) search, collaborative ontology evolution, ontology evaluation and cost models, and dynamic access and trends in distributed (semantic) knowledge, developed according to the working plan outlined in Technical Report TR-B-12-04. The prototypes complete the next milestone on the path to an integral Corporate Semantic Web architecture based on the three pillars Corporate Ontology Engineering, Corporate Semantic Collaboration, and Corporate Semantic Search, as envisioned in TR-B-08-09.
Electroma alacorvi
Creators: name: Tëmkin, Ilya
Publisher: name: Zenodo
Year: 2006
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Ostreida
Vulsellidae
Electroma
Electroma alacorvi

description: ELECTROMA ALACORVI (DILLWYN, 1817)
Samoa Islands, Asau harbour, north coast, in-shore edge of reef, 6 ft (four pairs with tissue, USNM 675754); Indian Ocean, Cocos Keeling, 4.8 km southwest of Home Island, 0.9–1.8 m, staghorn, sand, heads, near deep holes, station B20 (21 pairs with tissue, ANSP 289178); same as previous (six pairs with tissue; AMNH 292446); same as previous (nine pairs; AMNH 112530).
Principal reference: Pelseneer (1911) (gross anatomy).
description: Published as part of Tëmkin, Ilya, 2006, Morphological perspective on the classification and evolution of Recent Pterioidea (Mollusca: Bivalvia), pp. 253-312 in Zoological Journal of the Linnean Society 148 (3) on pages 309-310, DOI: 10.1111/j.1096-3642.2006.00257.x, http://zenodo.org/record/5427755
title: On being shamed in a nursing culture
Creators: name: McIntosh, Wendy H
Publisher: name: Griffith University
Year: 2006
Subjects: subject: Psychology of nursing
subject: shame in nursing
subject: nurse experiences
subject: quality of work experience

description: This study explored the experience of shame in nursing using an interpretive phenomenological approach as described by van Manen (1997). Shame is a concept that has been extensively theorised within the social sciences as important in the development of individual identity, self esteem and role performance but overlooked in nursing. The purpose of this research was twofold; to gain an understanding of how shame influences and shapes nursing identity and to produce knowledge and stimulate dialogue about what that means for nursing culture. Participants were asked to discuss significant interactions with colleagues. Significantly, all disclosed the experience of shame. Further, four major themes emerged from this study to deepen understanding of what appears to be a cultural experience. The experience of shame involves: self appraisal, professional identity in conflict, the experience of isolation and recrimination. Within each theme a number of sub themes were identified including feeling dumb, being incompetent, withdrawing and going quiet and seeking revenge. The study concluded that in relation to nursing, internalised shame is not readily recognised although negative emotions that are linked to it are clearly felt. When these emotions are left unprocessed or unidentified as shame, then they are likely to have negative consequences. But recognising this hidden shame and bringing it to conscious awareness can express and perhaps relieve shame. Further, shame's adaptive functions, to provide moral direction and teach respect, could be acknowledged or reclaimed. It is argued therefore that acknowledging and discussing shame openly in nursing, such as through future research, scholarships and education, will facilitate consciousness raising and the potential for cultural change.
Magnetic Field Diagnostics Based on Far-Infrared Polarimetry: Tests Using Numerical Simulations
Creators: name: Heitsch, F.
name: Zweibel, E. G.
name: Mac Low, M. -M.
name: Li, P. S.
name: Norman, M. L.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The dynamical state of star-forming molecular clouds cannot be understood without determining the structure and strength of their magnetic fields. Measurements of polarized far-infrared radiation from thermally aligned dust grains are used to map the orientation of the field and estimate its strength, but the accuracy of the results has remained in doubt. In order to assess the reliability of this method, we apply it to simulated far-infrared polarization maps derived from three-dimensional simulations of supersonic magnetohydrodynamical turbulence, and compare the estimated values to the known magnetic field strengths in the simulations. We investigate the effects of limited telescope resolution and self-gravity on the structure of the maps. Limited observational resolution affects the field structure such that small scale variations can be completely suppressed, thus giving the impression of a very homogeneous field. The Chandrasekhar-Fermi method of estimating the mean magnetic field in a turbulent medium is tested, and we suggest an extension to measure the rms field. Both methods yield results within a factor of 2 for field strengths typical of molecular clouds, with the modified version returning more reliable estimates for slightly weaker fields. However, neither method alone works well for very weak fields, missing them by a factor of up to 150. Taking the geometric mean of both methods estimates even the weakest fields accurately within a factor of 2.5. Limited telescope resolution leads to a systematic overestimation of the field strengths for all methods. We discuss the effects responsible for this overestimation and show how to extract information on the underlying (turbulent) power spectrum.
description: 30 pages, 15 figures (figs 1, 4, 5 reduced quality), submitted to ApJ Hires version of figs 1, 4, 5 see ftp://ftp.mpia-hd.mpg.de/pub/heitsch/HZM00/hiresfigs.tar.gz
Sensitivity Analysis of the Information Gain in Infinite-Dimensional Bayesian Linear Inverse Problems
Creators: name: Chowdhary, Abhijit
name: Tong, Shanyin
name: Stadler, Georg
name: Alexanderian, Alen
Publisher: name: arXiv
Year: 2023
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics
subject: 65C60, 90C31, 62F15, 35R30, 65F55

description: We study the sensitivity of infinite-dimensional Bayesian linear inverse problems governed by partial differential equations (PDEs) with respect to modeling uncertainties. In particular, we consider derivative-based sensitivity analysis of the information gain, as measured by the Kullback-Leibler divergence from the posterior to the prior distribution. To facilitate this, we develop a fast and accurate method for computing derivatives of the information gain with respect to auxiliary model parameters. Our approach combines low-rank approximations, adjoint-based eigenvalue sensitivity analysis, and post-optimal sensitivity analysis. The proposed approach also paves way for global sensitivity analysis by computing derivative-based global sensitivity measures. We illustrate different aspects of the proposed approach using an inverse problem governed by a scalar linear elliptic PDE, and an inverse problem governed by the three-dimensional equations of linear elasticity, which is motivated by the inversion of the fault-slip field after an earthquake.
description: 20 pages, 7 figures
Additional file 5: of Drivers of hospital expenditure and length of stay in an academic medical centre: a retrospective cross-sectional study
Creators: name: Rahman, Nabilah
name: Ng, Sheryl
name: Sravan Ramachandran
name: Wang, Debby
name: Srinath Sridharan
name: Chuen Tan
name: Khoo, Astrid
name: Tan, Xin
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology

description: Summary of patient and visit factors of patients who had no primary diagnosis mapped by Clinical Classification Software (DOCX 15 kb)
The Star Formation History of NGC 6822
Creators: name: Wyder, Ted K.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Images of five fields in the Local Group dwarf irregular galaxy NGC 6822 obtained with the {\it Hubble Space Telescope} in the F555W and F814W filters are presented. Photometry for the stars in these images was extracted using the Point-Spread-Function fitting program HSTPHOT/MULTIPHOT. The resulting color-magnitude diagrams reach down to $V\approx26$, a level well below the red clump, and were used to solve quantitatively for the star formation history of NGC 6822. Assuming that stars began forming in this galaxy from low-metallicity gas and that there is little variation in the metallicity at each age, the distribution of stars along the red giant branch is best fit with star formation beginning in NGC 6822 12-15 Gyr ago. The best-fitting star formation histories for the old and intermediate age stars are similar among the five fields and show a constant or somewhat increasing star formation rate from 15 Gyr ago to the present except for a possible dip in the star formation rate from 3 to 5 Gyr ago. The main differences among the five fields are in the higher overall star formation rate per area in the bar fields as well as in the ratio of the recent star formation rate to the average past rate. These variations in the recent star formation rate imply that stars formed within the past 0.6 Gyr are not spatially very well mixed throughout the galaxy.
description: 47 pages, 28 Figures, accepted for publication in the Astronomical Journal
title: Green Growth
title: from a growing eco-industry to a sustainable economy
titleType: Subtitle
Creators: name: Jänicke, Martin
Publisher: name: Freie Universität Berlin
Year: 2011
Subjects: subject: green growth
subject: environmental policy
subject: environmental innovation
subject: 300 Sozialwissenschaften::320 Politikwissenschaft::320 Politikwissenschaft

description: There are still many illusions to overcome in the growth discussion. These illusions may be seen in the idea that long-term, significant growth could be achieved using government resources or that the solution to pressing financial and social problems necessitates higher growth. It is also an illusion, however, to say that giving up on growth is the alternative. In fact, it is about radical growth in environmental and resource-saving technologies. It is also about radical “de-growth” in products and processes that undermine long- term living and production conditions. Is the concept of "Green Growth" proposed by the OECD and other established institutions in Europe and Asia part of the growth illusion? This paper traces the transformation of the concept of "Green Growth" and evaluates the strategy that accompanies it in order to provide a more nuanced answer.
MOESM2 of Biallelic ERBB3 loss-of-function variants are associated with a novel multisystem syndrome without congenital contracture
Creators: name: Li, Niu
name: Xu, Yufei
name: Zhang, Yi
name: Li, Guoqiang
name: Yu, Tingting
name: Yao, Ruen
name: Zhou, YunFang
name: Shen, Yiping
name: Yin, Lei
name: Wang, Xiumin
name: Wang, Jian
Publisher: name: figshare
Year: 2019
Subjects: Space Science
Biological Sciences not elsewhere classified

description: Additional file 2: Table S1. Primers for the ERBB3 (NM_001982.3) mutant plasmids construction.
Isognomon alatus Atkins 1938
Creators: name: Tëmkin, Ilya
Publisher: name: Zenodo
Year: 2006
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Ostreida
Isognomonidae
Isognomon
Isognomon alatus

description: ISOGNOMON ALATUS (GMELIN, 1791)
West Atlantic, FK-259, Ramrod Key, at dock, ocean side, Monroe County, Florida Keys, Florida, USA, 24°39.72′N, 81°24.41′W, intertidal, rocks, by hand (seven pairs with tissue, AMMH 298023); West Atlantic, west side of Magueyes Island, Puerto Rico (13 pairs, AMNH 100419); West Atlantic, bay side, Grassy Key, Florida Straits, Florida, USA (35 pairs; AMNH 247493).
Principal reference: Siung (1980) (gross anatomy; embryonic shell).
description: Published as part of Tëmkin, Ilya, 2006, Morphological perspective on the classification and evolution of Recent Pterioidea (Mollusca: Bivalvia), pp. 253-312 in Zoological Journal of the Linnean Society 148 (3) on page 310, DOI: 10.1111/j.1096-3642.2006.00257.x, http://zenodo.org/record/5427755
Pulse Shape Simulation and Discrimination using Machine-Learning Techniques
Creators: name: Dutta, Shubham
name: Ghosh, Sayan
name: Bhattacharya, Satyaki
name: Saha, Satyajit
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Machine Learning (cs.LG)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: An essential metric for the quality of a particle-identification experiment is its statistical power to discriminate between signal and background. Pulse shape discrimination (PSD) is a basic method for this purpose in many nuclear, high-energy and rare-event search experiments where scintillation detectors are used. Conventional techniques exploit the difference between decay-times of the pulses from signal and background events or pulse signals caused by different types of radiation quanta to achieve good discrimination. However, such techniques are efficient only when the total light-emission is sufficient to get a proper pulse profile. This is only possible when adequate amount of energy is deposited from recoil of the electrons or the nuclei of the scintillator materials caused by the incident particle on the detector. But, rare-event search experiments like direct search for dark matter do not always satisfy these conditions. Hence, it becomes imperative to have a method that can deliver a very efficient discrimination in these scenarios. Neural network based machine-learning algorithms have been used for classification problems in many areas of physics especially in high-energy experiments and have given better results compared to conventional techniques. We present the results of our investigations of two network based methods \viz Dense Neural Network and Recurrent Neural Network, for pulse shape discrimination and compare the same with conventional methods.
description: 18 pages, 39 figures
A submillimetre difference between radio galaxies and radio quasars: evidence for quasar-heated dust and synchronized submillimetre and radio source activity
Creators: name: Willott, Chris J.
name: Rawlings, Steve
name: Archibald, Elese N.
name: Dunlop, James S.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present submillimetre photometry of 11 3CR and 6CE radio quasars of similar 151-MHz radio luminosity and redshifts to the radio galaxies studied at 1.3~2-times brighter accounting for possible synchrotron contamination. This difference is in quantitative agreement with a receding-torus unified scheme for radio sources in which the torus opening angle depends on quasar optical luminosity, provided that there is a close relationship between the optical and submillimetre luminosities. The implication is that quasar-heated dust dominates the submillimetre emission for powerful radio quasars at z~1.5. We find a significant anti-correlation between submillimetre/far-infrared luminosity L_FIR and radio source age in the sense that hyperluminous quasars tend to be associated with young (<10^7 yr) sources. This suggests that the processes controlling L_FIR are synchronized with the jet-triggering event and that L_FIR declines on a ~10^7 yr timescale. There is evidence for a small amount of obscuration in the hyperluminous quasars from reddening and associated or broad absorption lines. We speculate that shortly after jet triggering, dust is more widely distributed than at later times and is heated by the quasar nucleus and/or a short-lived synchronized starburst.
description: 12 pages, 7 figures, MNRAS in press, typos corrected, refs updated
A Probabilistic Approach to Kepler Completeness and Reliability for Exoplanet Occurrence Rates
Creators: name: Bryson, Steve
name: Coughlin, Jeffrey
name: Batalha, Natalie M.
name: Berger, Travis
name: Huber, Dan
name: Burke, Christopher
name: Dotson, Jessie
name: Mullally, Susan E.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Exoplanet catalogs produced by surveys suffer from a lack of completeness (not every planet is detected) and less than perfect reliability (not every planet in the catalog is a true planet), particularly near the survey's detection limit. Exoplanet occurrence rate studies based on such a catalog must be corrected for completeness and reliability. The final Kepler data release, DR25, features a uniformly vetted planet candidate catalog and data products that facilitate corrections. We present a new probabilistic approach to the characterization of Kepler completeness and reliability, making full use of the Kepler DR25 products. We illustrate the impact of completeness and reliability corrections with a Poisson-likelihood occurrence rate method, using a recent stellar properties catalog that incorporates Gaia stellar radii and essentially uniform treatment of the stellar population. Correcting for reliability has a significant impact: the exoplanet occurrence rate for orbital period and radius within 20% of Earth's around GK dwarf stars, corrected for reliability, is 0.015+0.011-0.007, whereas not correcting results in 0.034+0.018-0.012 - correcting for reliability reduces this occurrence rate by more than a factor of two. We further show that using Gaia-based vs. DR25 stellar properties impacts the same occurrence rate by a factor of two. We critically examine the the DR25 catalog and the assumptions behind our occurrence rate method. We propose several ways in which confidence in both the Kepler catalog and occurrence rate calculations can be improved. This work provides an example of how the community can use the DR25 completeness and reliability products.
description: Accepted for publication in The Astronomical Journal
Two-loop diagrams in non-relativistic QCD with elliptics
Creators: name: Kniehl, B. A.
name: Kotikov, A. V.
name: Onishchenko, A. I
name: Veretin, O. L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper we consider two-loop two-, three- and four-point diagrams with elliptic structure in the case of two different masses $m$ and $M$. The latter diagrams generally arise within NRQCD matching procedures and are relevant for parapositronium decay and top pair production at threshold. We present the obtained results in several different representations: series solution with binomial coefficients, integral representation and representation in terms of generalized hypergeometric functions. The results are valid up to $\mathcal{O}(\varepsilon)$ terms in $d=4-2\varepsilon$ space-time dimensions. In the limit of equal masses $m=M$ the obtained results are written in terms of elliptic constants with explicit series representation.
description: 31 pages, 2 figures, matches journal version
Additional file 1: of Dystrophin R16/17 protein therapy restores sarcolemmal nNOS in trans and improves muscle perfusion and function
Creators: name: Junling Zhao
name: Hsiao Yang
name: Lakmini Wasala
name: Keqing Zhang
name: Yongping Yue
name: Dongsheng Duan
name: Lai, Yi
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Figure S1. The amino acid sequence of five commonly used CPPs. In mTAT, the mutated residues are highlighted in red color. mTAT: TAT mutant. (PDF 220 kb)
Absorption Systems in the Spectrum of GRB 021004
Creators: name: Møller, P.
name: Fynbo, J. P. U.
name: Hjorth, J.
name: Thomsen, B.
name: Egholm, M. P.
name: Andersen, M. I.
name: Gorosabel, J.
name: Holland, S. T.
name: Jakobsson, P.
name: Jensen, B. L.
name: Pedersen, H.
name: Pedersen, K.
name: Weidinger, M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on a 3600 s spectrum of GRB 021004 obtained with the Nordic Optical Telecope on La Palma 10.71 hours after the burst. We identify absorption lines from five systems at redshifts 1.3806, 1.6039, 2.2983, 2.3230, and 2.3292. In addition we find an emission line which, if due to Ly-alpha from the host galaxy, gives a redshift of 2.3351. The nearest absorber is blueshifted by 530 km/s with respect to this line, consistent with shifts seen in Damped Ly-alpha and Lyman-Break galaxies at similar redshifts. The emission line flux is 2.46+-0.50 x 10^-16 erg/s/cm^2. Some of the absorption systems are "line-locked", an effect often seen in QSO absorption systems believed to originate close to the QSO central engine.
description: 4 pages, 3 figures, A&A Letters, in press
Notoxus ravana Kejval 2011
Creators: name: Kejval, Zbyněk
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Anthicidae
Notoxus
Notoxus ravana

description: Notoxus ravana species-group
 Diagnosis. Elytral apices in males clearly modified; median lobe of aedeagus symmetrical, lacking distinct dorsal plate; parameres of aedeagus setose; latero-basal fovea of abdominal sternum III rather rounded, forming conspicuous, deep cavity.
 Species included. Notoxus brinckianus Bonadona, 1986, N. brunneorufus Bonadona, 1989, N. ravana sp. nov., and N. variabilis Krekich-Strassoldo, 1913.
 Remarks. The range of this group is confined to the Indian subcontinent (India, Sri Lanka) so far, and its members exhibit clear similarities (deep latero-basal fovea of abdominal sternum III, general morphology of aedeagus) with the Afrotropical fauna of the genus.
description: Published as part of Kejval, Zbyněk, 2011, Taxonomic revision of the Oriental species of Notoxus (Coleoptera: Anthicidae), pp. 627-673 in Acta Entomologica Musei Nationalis Pragae 51 (2) on page 662, DOI: 10.5281/zenodo.5329507