cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Aselliscus Tate 1941
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Aselliscus

description: Aselliscus Tate, 1941. Am. Mus. Novit., 1140:2. TYPE SPECIES: Rhinolophus tricuspidatus Temminck, 1835.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 170, DOI: 10.5281/zenodo.7353060
Size Optimization of Nanoimprinted-Texture on Crystalline Silicon Solar Cell by Three Dimensional Simulation
Creators: name: Yoshinaga, S.
name: Ishikawa, Y.
name: Araki, S.
name: Jiang, Y.
name: Horita, M.
name: Uraoka, Y.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 1053-1055
description: It is important to suppress the surface reflectance on the cell, in order to manufacture solar cell with high efficiency. We applied zirconium oxide as a texture material on the surface and investigate the optimal texture structure generating low surface reflectance using Diffract MOD simulator. The texture form was investigated pyramid, pillar, moth eye, and inversed moth eye. The texture height and width were varied from 10 nm to 500 nm. The most optimal structure was a pyramid with a height of 200 nm and a width of 10 nm. This texture structure was a weighted average reflectance of 4.7%. The surface reflectance was very sensitive to the variation of texture height. Pyramid texture structure with a width of 200 nm, while keeping a height fixed, was also near a weighted average reflectance of 4.9%. Moreover, that nanoimprinted-texture cell could significantly increase conversion efficiency.
Classification of BATSE, Swift, and Fermi Gamma-Ray Bursts from Prompt Emission Alone
Creators: name: Steinhardt, Charles L.
name: Mann, William J.
name: Rusakov, Vadim
name: Jespersen, Christian K.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Although it is generally assumed that there are two dominant classes of gamma-ray bursts (GRB) with different typical durations, it has been difficult to unambiguously classify GRBs as short or long from summary properties such as duration, spectral hardness, and spectral lag. Recent work used t-distributed stochastic neighborhood embedding (t-SNE), a machine learning algorithm for dimensionality reduction, to classify all Swift gamma-ray bursts as short or long. Here, the method is expanded, using two algorithms, t-SNE and UMAP, to produce embeddings that are used to provide a classification for the 1911 BATSE bursts, 1321 Swift bursts, and 2294 Fermi bursts for which both spectra and metadata are available. Although the embeddings appear to produce a clear separation of each catalog into short and long bursts, a resampling-based approach is used to show that a small fraction of bursts cannot be robustly classified. Further, 3 of the 304 bursts observed by both Swift and Fermi have robust but conflicting classifications. A likely interpretation is that in addition to the two predominant classes of GRBs, there are additional, uncommon types of bursts which may require multi-wavelength observations in order to separate from more typical short and long GRBs.
description: ApJ, in press
LHC Signatures Of Scalar Dark Energy
Creators: name: Brax, Philippe
name: Burrage, Clare
name: Englert, Christoph
name: Spannowsky, Michael
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Scalar dark energy fields that couple to the Standard Model can give rise to observable signatures at the LHC. In this work we show that $t\bar t+$missing energy and mono-jet searches are suitable probes in the limit where the dark energy scalar is stable on collider distances. We discuss the prospects of distinguishing the dark energy character of new physics signals from dark matter signatures and the possibility of probing the self-interactions of the dark energy sector.
description: 10 pages, 8 figures
Non-Vacuum Processed Antireflection Coating Using Nano-Composite/Oxide Layers for Silicon Solar Cells
Creators: name: Kuriyama, M.
name: Harano, N.
name: Uzum, A.
name: Kimura, Y.
name: Tanimoto, K.
name: Fukui, H.
name: Izumi, T.
name: Harada, T.
name: Ito, S.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 1056-1058
description: Reducing the optical losses in solar cells is so crucial for achieving higher efficiencies. In order to meet industrial requirements with high throughput and low-cost, new materials and methods need to be investigated and adapted to the solar cell manufacturing process. In this work, ZrO2 based antireflection coating layers by simple and cost-effective spin coating process, was introduced. Deposition of the zirconium sol-gel was performed by spin-on coating with a spin-speed in a range of 500 rpm-3000 rpm. Less than 5% reflectance was observed after forming ZrO2 layer. Reflectance decreased further to around 3% after forming spin-coated ZrO2 on spray-deposition coated TiO2 layer. Silicon solar cells were fabricated with and without the ZrO2 antireflection layer using CZ-Si p-type wafers. Conversion efficiency of the cells improved up by a factor of 0.8% where the Jsc also improved further of 2 mA/cm2 with ZrO2. Reflectivity analysis, SEM measurements and electrical characteristics of fabricated solar cells were mainly carried out for the analysis and characterizations.
Milliarcsecond Structures of Variable Peaked-Spectrum Sources
Creators: name: Ross, K.
name: Reynolds, C.
name: Seymour, N.
name: Callingham, J. R.
name: Hurley-Walker, N.
name: Bignall, H.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Spectral variability offers a new technique to identify small scale structures from scintillation, as well as determining the absorption mechanism for peaked-spectrum (PS) radio sources. In this paper, we present very long baseline interferometry (VLBI) imaging using the Long Baseline Array (LBA) of two PS sources, MRC0225-065 and PMNJ0322-4820, identified as spectrally variable from observations with the Murchison Widefield Array (MWA). We compare expected milliarcsecond structures based on the detected spectral variability with direct LBA imaging. We find MRC0225-065 is resolved into three components, a bright core and two fainter lobes, roughly 430pc projected separation. A comprehensive analysis of the magnetic field, host galaxy properties, and spectral analysis implies that MRC0225-065 is a young radio source with recent jet activity over the last 10^2-10^3years. We find PMNJ0322-4820 is unresolved on milliarcsecond scales. We conclude PMNJ0322-4820 is a blazar with flaring activity detected in 2014 with the MWA. We use spectral variability to predict morphology and find these predictions consistent with the structures revealed by our LBA images.
description: Accepted for publication in PASA. 11 pages, 4 figures
Task-related edge density (TED) - a new method for revealing large-scale network formation in fMRI data of the human brain
Creators: name: Lohmann, Gabriele
name: Stelzer, Johannes
name: Zuber, Verena
name: Buschmann, Tilo
name: Margulies, Daniel
name: Bartels, Andreas
name: Scheffler, Klaus
Publisher: name: arXiv
Year: 2015
Subjects: subject: Neurons and Cognition (q-bio.NC)
subject: FOS: Biological sciences

description: The formation of transient networks in response to external stimuli or as a reflection of internal cognitive processes is a hallmark of human brain function. However, its identification in fMRI data of the human brain is notoriously difficult. Here we propose a new method of fMRI data analysis that tackles this problem by considering large-scale, task-related synchronisation networks. Networks consist of nodes and edges connecting them, where nodes correspond to voxels in fMRI data, and the weight of an edge is determined via task-related changes in dynamic synchronisation between their respective times series. Based on these definitions, we developed a new data analysis algorithm that identifies edges in a brain network that differentially respond in unison to a task onset and that occur in dense packs with similar characteristics. Hence, we call this approach "Task-related Edge Density" (TED). TED proved to be a very strong marker for dynamic network formation that easily lends itself to statistical analysis using large scale statistical inference. A major advantage of TED compared to other methods is that it does not depend on any specific hemodynamic response model, and it also does not require a presegmentation of the data for dimensionality reduction as it can handle large networks consisting of tens of thousands of voxels. We applied TED to fMRI data of a fingertapping task provided by the Human Connectome Project. TED revealed network-based involvement of a large number of brain areas that evaded detection using traditional GLM-based analysis. We show that our proposed method provides an entirely new window into the immense complexity of human brain function.
description: 21 pages, 11 figures
Development of Silicon Heterojunction Metal Wrap through Solar Cells
Creators: name: Dirnstorfer, I.
name: Schilling, N.
name: Koerner, S.
name: Gierth, P.
name: Sontag, D.
name: Jordan, P.M.
name: Simon, D.K.
name: Fengler, F.
name: Mikolajick, T.
name: Linaschke, D.
name: Dani, I.
name: Marcinkowsi, M.
name: Eberstein, M.
name: Rebenklau, L.
name: Partsch, U.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 1044-1048
description: A silicon heterojunction solar cell basing on amorphous and crystalline silicon is combined with the metal wrap through technology. In this way, the geometrical front side metallization area is reduced from about 7 % to below 5 %. The novel cell concept bases on a back junction configuration to avoid complex insulation steps within the via holes. Furthermore, well-passivated via holes are fabricated in a 532 nm laser process after the thin film depositions. As an alternative, the 1064 nm laser process is investigated, however, the result is a high surface recombination rate and a low effective carrier lifetime in the via vicinity. Scanning electron microscopy cross sections of via holes indicate a different surface oxide formation for both laser lines and this result suggests that this oxidation is crucial for the via hole passivation. Via holes in silicon heterojunction solar cells also have very high surface recombination, when the via hole formation is performed prior to wet chemical cleaning and texturing steps, which is the standard sequence in diffused emitter metal wrap through solar cells. The via metallization bases on a novel low-temperature silver paste, which is deposited by vacuum assisted screen printing. Cross sections reveal excellent via filling, which results in a low electrical resistance. The via-related specific solar cell series resistance is below 80 mΩcm2. Finally, the solderability of the rear side metallization was evaluated for later module integration.
CEA-INES Heterojunction Solar Cell ‘LabFab’ Industrial Pilot Line: Production Capability Demonstration, Roadmap to 22% Mean Efficiency
Creators: name: Harrison, S.
name: Danel, A.
name: Roux, C.
name: Heslinga, D.
name: Ozanne, F.
name: Muñoz, D.
name: Ribeyron, P.J.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 1049-1052
description: In this paper we present recent progress made in the heterojunction solar cells industrial pilot line called ‘LabFab HET’, located in the French National Solar Energy Institute (INES), Le Bourget du Lac, and operated by the French Alternative Energies and Atomic Energy Commission (CEA). After successful R&D and process transfer during 2010-12 [1], and pilot line optimization phase (2013), full production capability has been demonstrated end of 2013 by volume runs totaling over 32.000 HET cells. The mission of the CEA ‘LabFab HET’ is to validate the feasibility of HET cell mass manufacturing from both a technical and economical point of view. Hence it is operated in a continuous flow production mode, from wafer incoming inspection to final cell efficiency tester sorting. The line has a nominal capacity of 15MWp/year, with all equipment provided by world-wide recognized suppliers
Aselliscus stoliczkanus
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Aselliscus
Aselliscus stoliczkanus

description: Aselliscus stoliczkanus (Dobson, 1871). Proc. Asiat. Soc. Bengal, p. 106. TYPE LOCALITY: Malaysia, West, Penang. DISTRIBUTION: Burma, S China, Thailand, Laos, Vietnam, W Malaysia. SYNONYMS: trifidus, wheeleri (see Sanborn, 19526:3).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 170, DOI: 10.5281/zenodo.7353060
Large-Area Honeycomb Texturing of Si-Solar Cells via Nanoimprint Lithography
Creators: name: Tucher, N.
name: Volk, A.
name: Seiffe, J.
name: Hauser, H.
name: Müller, C.
name: Bläsi, B.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 1006-1011
description: The highest solar cell efficiencies on mc-Si were realized using photolithographically defined texturing processes. The feasibility of fabricating honeycomb textures using Nanoimprint Lithography (NIL) was already demonstrated and excellent short-circuit current densities of up to 40.7 mA/cm² were achieved on small-area monocrystalline silicon (c-Si) solar cells. In the present work, large-area honeycomb texturing of multicrystalline silicon (mc-Si) substrates based on Roller-NIL and in-line-capable multi-wafer plasma etching using a modified Roth&Rau SiNA system is demonstrated. The realized honeycomb texture shows superior optical properties compared to isotextured mc-Si reference samples and even random pyramids on c-Si substrates, while surface passivation is comparably good. The fabricated 156 x 156 mm² mc-Si solar cells with Al-BSF show an efficiency of 17.8% compared to 17.3% of the isotextured reference. As VOC remains constant for both textures, the efficiency gain of 0.5% absolute results from a Jsc increase of up to 1.3 mA/cm2 (on cut 50 x 50 mm² cells even 2.5 mA/cm2), which confirms the superior optical quality of the honeycomb texture.
On heterochromatic out-directed spanning trees in tournaments
Creators: name: Montellano-Ballesteros, Juan José
name: Campo, Eduardo Rivera
Publisher: name: arXiv
Year: 2016
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: Given a tournament T, let h(T) be the smallest integer k such that every arc-coloring of T with k or more colors produces at least one out-directed spanning tree of T with no pair of arcs with the same color. In this paper we give the exact value of h(T).
Pilot study : reduction in incidence of gastrointestinal disease resulting from implementation of public water treatment
Creators: name: McConnell, Stuart.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
GRB minimum variability timescale with Insight-HXMT and Swift: implications for progenitor models, dissipation physics and GRB classifications
Creators: name: Camisasca, A. E.
name: Guidorzi, C.
name: Amati, L.
name: Frontera, F.
name: Song, X. Y.
name: Xiao, S.
name: Xiong, S. L.
name: Zhang, S. N.
name: Margutti, R.
name: Kobayashi, S.
name: Mundell, C. G.
name: Ge, M. Y.
name: Gomboc, A.
name: Jia, S. M.
name: Jordana-Mitjans, N.
name: Li, C. K.
name: Li, X. B.
name: Maccary, R.
name: Shrestha, M.
name: Xue, W. C.
name: Zhang, S.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The dissipation process of GRB prompt emission is still unknown. Study of temporal variability may provide a unique way to discriminate the imprint of the inner engine activity from geometry and propagation related effects. We define the minimum variability timescale (MVT) as the shortest duration of individual pulses that shape a light curve for a sample of GRBs and test correlations with peak luminosity, Lorentz factor, and jet opening angle. We compare these correlations with predictions from recent numerical simulations for a relativistic structured -- possibly wobbling -- jet and assess the value of MTV as probe of prompt-emission physics. We used the peak detection algorithm mepsa to identify the shortest pulse within a GRB time history and estimate its full width half maximum (FWHM). We applied this framework to two sets of GRBs: Swift (from 2005 to July 2022) and Insight-HXMT (from June 2017 to July 2021, including 221009A). We then selected 401 GRBs with measured z to test for correlations. On average short GRBs have significantly shorter MVT than long GRBs. The MVT distribution of short GRBs with extended emission such as 060614 and 211211A is compatible only with that of short GRBs. This provides a new clue on the progenitor's nature. The MVT for long GRBs anticorrelates with peak luminosity. We confirm the anticorrelation with the Lorentz factor and find a correlation with the jet opening angle as estimated from the afterglow, along with an inverse correlation with the number of pulses. The MVT can identify the emerging putative new class of long GRBs that are suggested to be produced by compact binary mergers. For otherwise typical long GRBs, the different correlations between MVT and peak luminosity, Lorentz factor, jet opening angle, and number of pulses can be explained within the context of structured, possibly wobbling, weakly magnetised relativistic jets. (summarised)
description: 18 pages, 15 figures, accepted by A&A
Supplementary document for Optical readout and actuation of plasmonic nano-optomechanical drum resonators - 6623505.pdf
Creators: name: Vandersmissen, Jente
name: Meijer, Randy
name: Sukham, Johneph
name: Erkelens, Aloys
name: Aans, Jan Bonne
name: Verhagen, Ewold
Publisher: name: Optica Publishing Group
Year: 2023
Subjects: Uncategorized

description: Supplementary Information
State-of-the-Art Amorphous Silicon Sub-Oxide Passivation Layer by ICPECVD for Heterojunction Solar Cell Applications
Creators: name: Ge, J.
name: Tang, M.
name: Wong, J.
name: Zhang, Z.
name: Dippell, T.
name: Dörr, M.
name: Hohn, O.
name: Huber, M.R.
name: Wohlfart, P.
name: Aberle, A.G.
name: Mueller, T.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 1032-1035
description: In this paper, we present an alternative method of depositing a high-quality passivation film for heterojunction silicon wafer solar cells. The deposition of hydrogenated intrinsic amorphous silicon suboxide is accomplished by decomposing hydrogen, silane and carbon dioxide in an industrial remote inductively coupled plasma platform. Through the investigation on CO2 partial pressure and process temperature, excellent surface passivation quality and optical properties are achieved. The effective lifetime of symmetrically passivated samples under the optimal condition exceeds 4.7 ms on planar n-type Czochralski silicon wafers with a resistivity of 1 Ωcm, which is equivalent to an effective surface recombination velocity of less than 1.7 cms-1 and an implied open-circuit voltage (Voc) of 741 mV. A comparison with several high-quality passivation schemes for solar cells reveals that the developed inductively coupled plasma deposited films show excellent passivation quality. The excellent resistance to degradation makes it an excellent substitute for industrial heterojunction silicon solar cell production.
Luminescent and Scintillating Properties of Lanthanum Fluoride Nanocrystals in Response to Gamma/Neutron Irradiation: Codoping with Ce Activator, Yb Wavelength Shifter, and Gd Neutron Captor
Creators: name: Vargas, José M.
name: Blostein, Juan Jerónimo
name: Sidelnik, Iván
name: Brito, David Rondón
name: Palomino, Luis A. Rodríguez
name: Mayer, Roberto E.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: A novel concept for detection and spectroscopy of gamma rays, and detection of thermal neutrons based on codoped lanthanum fluoride nanocrystals containing gadolinium is presented.The trends of colloidal synthesis of the mentioned material, LaF3 co-doped with Ce as the activator, Yb as the wavelength-shifter and Gd as the neutron captor, is reported. Nanocrystals of the mentioned material were characterized by transmission electron microscopy (TEM), X-ray diffraction (XRD), energy-dispersive X-ray spectroscopy (EDS), optical absorption, and photoluminescence spectroscopy. Gamma detection and its potential spectroscopy feature have been confirmed. The neutron detection capability has been confirmed by experiments performed using a 252Cf neutron source.
description: 5 figures, 16 pages
Supplementary document for Optical readout and actuation of plasmonic nano-optomechanical drum resonators - 6536245.pdf
Creators: name: Vandersmissen, Jente
name: Meijer, Randy
name: Sukham, Johneph
name: Erkelens, Aloys
name: Aans, Jan Bonne
name: Verhagen, Ewold
Publisher: name: Optica Publishing Group
Year: 2023
Subjects: Uncategorized

description: Supplemental Material
Oxide/Polysilicon Passivated Contact with PECVD Deposition for n-Type Si Solar Cells
Creators: name: Lee, B.
name: Nemeth, W.
name: Yuan, H.-C.
name: Norman, A.
name: LaSalvia, V.
name: Page, M.
name: Young, D.L.
name: Stradins, P.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 1003-1005
description: We describe the design, fabrication and results for low-recombination, passivated contacts to n-type Si utilizing thin SiO2, and PECVD-deposited doped polysilicon (pc-Si) layers. We make an electron-collecting, passivated contact to n-type Si with a 15-20 Å thick SiO2 and n+ (P-doped) pc-Si, which simultaneously provides both excellent passivation and low contact resistivity. We examine this contact by studying its passivation with various annealing conditions, and with TEM cross-section images. Passivation quality is demonstrated by low measured contact recombination current density J0,c ~ 10 fA/cm2; we also achieve low contact resistivity c = 23 milliohm-cm2. This contact is promising for high efficiency n-type Si solar cells – we present an analysis using the attained values of J0,c and c to estimate the cell efficiency potential. We fabricate a solar cell employing this passivated contact with high open circuit voltage Voc = 693 mV an efficiency of 21.5%.
Cosmological constraints from HSC survey first-year data using deep learning
Creators: name: Lu, Tianhuan
name: Haiman, Zoltán
name: Li, Xiangchong
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present cosmological constraints from the Subaru Hyper Suprime-Cam (HSC) first-year weak lensing shear catalogue using convolutional neural networks (CNNs) and conventional summary statistics. We crop 19 $3\times3\,\mathrm{{deg}^2}$ sub-fields from the first-year area, divide the galaxies with redshift $0.3\le z\le1.5$ into four equally-spaced redshift bins, and perform tomographic analyses. We develop a pipeline to generate simulated convergence maps from cosmological $N$-body simulations, where we account for effects such as intrinsic alignments (IAs), baryons, photometric redshift errors, and point spread function errors, to match characteristics of the real catalogue. We train CNNs that can predict the underlying parameters from the simulated maps, and we use them to construct likelihood functions for Bayesian analyses. In the $Λ$ cold dark matter model with two free cosmological parameters $Ω_\mathrm{m}$ and $σ_8$, we find $Ω_\mathrm{m}=0.278_{-0.035}^{+0.037}$, $S_8\equiv(Ω_\mathrm{m}/0.3)^{0.5}σ_8=0.793_{-0.018}^{+0.017}$, and the IA amplitude $A_\mathrm{IA}=0.20_{-0.58}^{+0.55}$. In a model with four additional free baryonic parameters, we find $Ω_\mathrm{m}=0.268_{-0.036}^{+0.040}$, $S_8=0.819_{-0.024}^{+0.034}$, and $A_\mathrm{IA}=-0.16_{-0.58}^{+0.59}$, with the baryonic parameters not being well-constrained. We also find that statistical uncertainties of the parameters by the CNNs are smaller than those from the power spectrum (5--24 percent smaller for $S_8$ and a factor of 2.5--3.0 smaller for $Ω_\mathrm{m}$), showing the effectiveness of CNNs for uncovering additional cosmological information from the HSC data. With baryons, the $S_8$ discrepancy between HSC first-year data and Planck 2018 is reduced from $\sim2.2\,σ$ to $0.3\text{--}0.5\,σ$.
description: 22 pages, 14 figures
Low Temperature Deposition of High Performance ITO Using a Co-Plasma Approach
Creators: name: Simon, D.K.
name: Fengler, F.
name: Jordan, P.M.
name: Sontag, D.
name: Mikolajick, T.
name: Dirnstorfer, I.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 1028-1031
description: Tin-doped indium oxide (ITO) is known for its potential to combine excellent transparency with low resistivity. To achieve best performance usually high process temperatures (≥ 200 °C) are applied. However, those values are not suitable for application on temperature critical layers, such as amorphous silicon for heterojunction solar cells. Conventional low-temperature depositions usually show lower performance due to low surface diffusion during the growth process. To improve the ITO properties, a substrate plasma is applied additionally to the conventional target plasma. With this co-plasma approach, the crystallinity of the ITO layers as well as resistivity and absorption are clearly improved. An ITO layer deposited at 100 °C reaches a resistivity of 500 μΩcm and an absorption coefficient below 5·103 cm-1. The efficiency of a silicon heterojunction solar cell with co-plasma grown ITO is 19.3 %.
Demonstration of High-Efficiency ITO/TiO2/P-N Semiconductor MIS-Structure Silicon Solar Cell Enhancing with Induced Electric Field on Space Charge Region by Voltage Biasing on ITO
Creators: name: Ho, W.-J.
name: Huang, M.-C.
name: Lee, Y.-Y.
name: Yang, G.-C.
name: Chan, C.-M.
name: Hou, Z.-F.
name: Liao, J.-J.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 1015-1019
description: In this study, a high efficiency of 18.21% ITO/TiO2/p-n semiconductor metal-insulator-semiconductor (MIS) structure silicon (Si) solar cell enhancingwith induced electric field on the space charge region by a voltage biasing on the transparent indium-tin-oxide (ITO) electrode is demonstrated. Thedeposited 50 nm-thick ITO filmsexhibitedhigh conductivity and high transmittance of >80% at visible band were obtainedby using a thermal sputtered depositionat 250. The role of ITO film was regarded as a biasing electrode and an anti-reflective coating (ARC) layerin the proposed device. When applied a biasing voltage on the ITO-electrode, an additional increasing in photocurrent was obtained, as well as raisingthe conversion efficiency, due to that the depletion width of p-n junctionunderneath the ITO would be extendedinto the p-Si base layeras the biasedvoltageincreasing,which can provide a more efficient photo-carriers collection due to a larger built-in electric filed and a larger absorbed semiconductor volume.In this work, the optical reflectance, photo-current as a function ofthe ITO biasing voltage,external quantum efficiency (EQE)response, and the capacitance as a function of the ITO biasing voltage(C-V) under dark andilluminated conditionsweremeasured andcharacterized to examine thebiasing effectson the photovoltaic performances. At biasing voltage of 2.5 V, theshort-circuit current(ISC)of 6.58mA, open-circuit voltage (VOC) of 0.57V,and = 18.21% were obtainedunder one sun AM 1.5G illumination at 25.Besides, theshort-circuit-current enhancement (∆Isc) of 52.31%(from 4.32 to 6.58 mA)and conversion-efficiency enhancement (∆) of  45.68%(from 12.50 to 18.21%)are obtained, compared tothe cell biasing at 0 V.
Optical and Electrical Improvement of Rear Side ITO for Heterojunction Back Contact Solar Cells
Creators: name: Granata, S.N.
name: Tous, L.
name: Bearda, T.
name: Nassar, J.
name: Cariou, R.
name: Trompoukis, C.
name: Van Nieuwenhuysen, K.
name: Abdulraheem, Y.
name: Gordon, I.
name: Szlufcik, J.
name: Roca I Cabarrocas, P.
name: Mertens, R.
name: Poortmans, J.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 1024-1027
description: In this paper, the electrical and optical characteristics of the Indium-Doped Tin Oxide (ITO) are tuned in order to design an ITO-based spacer between the a-Si:H and the metal contact suited for Amorphous / Crystalline Heterojunction interdigitated Back Contact Solar Cells (a-Si:H / c-Si HJ i-BC). ITO carrier concentration, mobility, resistivity, extinction coefficient, and work function, as well as the ITO / a-Si:H specific contact resistances are evaluated as a function of O2 relative flow rate during ITO deposition. An ITO having carrier concentration of 4.5x1019 cm-3, mobility of 20.2 cm2/(V.s) and resistivity of 6.24 mΩ.cm is found to be an optimum leading to ITO / a-Si:H(p/i) and ITO / a-Si:H(n/i) specific contact resistances values of 0.6 Ω.cm2 and 0.1 Ω.cm2 respectively and a RS reflectance of 58% at 1200nm when integrated in Silver / ITO / a-Si:H / c-Si(textured) test structures.
High-Lifetime Wafer Cleaning Method Using Ozone Dissolved in DIW/HF/HCl Solution
Creators: name: Li, Z.
name: Yang, Y.
name: Zhang, X.
name: Feng, Z.
name: Verlinden, P.J.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 1012-1014
description: In this work, ozone dissolved in deionized water (DIO3) cleaning is investigated as a low-cost alternative method to the current wet-chemical cleaning in high-efficiency solar cell manufacturing. Higher effective lifetime and lower J0 were achieved, compared to the reference cleaning process of high-lifetime RCA, by simply adding a small amount of HF and HCl to DIO3 solution. The effective lifetime of cleaned and passivated wafers increased as the processing time in DIO3/HF/HCl cleaning solution increased. The stability of the wafer lifetime even after some storage time of up to an hour post cleaning makes the DIO3/HF/HCl cleaning suitable for industrial application. The DIO3/HF/HCl cleaning shows a great potential to be a high-lifetime wet-chemical cleaning process in mass production.
Eduard Ziegler (1800-1882) an Joseph Wolfgang von Deschwanden (1819-1866)
Creators: name: Ziegler, Eduard
Publisher: name: [s.n.]
Year: 1863

description: Brief aus Zürich, unterzeichnet mit: Direktor des Militärdep.
Zelger war Vorsteher von Polizei und Militär des Kantons Zürich
Experimental demonstration of an efficient number diagnostic for long 1D ion chains
Creators: name: Kamsap, Marius Romuald
name: Champenois, Caroline
name: Pedregosa-Gutierrez, J.
name: Houssin, Marie
name: Knoop, Martina
Publisher: name: arXiv
Year: 2016
Subjects: subject: Quantum Physics (quant-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: Very long, one-dimensional (1D) ion chains are the basis for many applications, in particular in quantum information processing and reliable diagnostics are needed to quantify them. To that purpose, we have experimentally validated Dubin's model for very long ion chains [Phys. Rev. Lett. 71, 2753 (1993)]. This diagnostic allows to precisely determine the number of trapped ion with an accuracy of almost 1\% without counting them, by measuring the ion-ion distance of the innermost particles, as well as the trapping potential along the ion chain direction. In our experiment, based on a 155 ion chain, the central 30 ions are measured to be equidistant to better than 2\%, and we can determine the total number of trapped ions with a 4.5\% uncertainty, completely dominated by a conservative estimation of the experimental characterisation of the trap.
description: 4 pages, 3 figures
Aselliscus tricuspidatus
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Aselliscus
Aselliscus tricuspidatus

description: Aselliscus tricuspidatus (Temminck, 1835). Monogr. Mamm., 2:20. TYPE LOCALITY: Indonesia, Molucca Isis, Amboina. DISTRIBUTION: Molucca Isis, New Guinea, Bismarck Arch., Solomon Isis (including Santa Cruz Isis), Vanuatu (= New Hebrides), adjacent small islands. SYNONYMS: koopmani, novaeguinae, novaehebridensis. COMMENTS: Revised by Schütter et al. (1983).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 170, DOI: 10.5281/zenodo.7353060
Two-Point Functions of Composite Twist Fields in the Ising Field Theory
Creators: name: Castro-Alvaredo, Olalla A.
name: Mazzoni, Michele
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: All standard measures of bipartite entanglement in one-dimensional quantum field theories can be expressed in terms of correlators of branch point twist fields, here denoted by $\mathcal{T}$ and $\mathcal{T}^\dagger$. These are symmetry fields associated to cyclic permutation symmetry in a replica theory and having the smallest conformal dimension at the critical point. Recently, other twist fields (composite twist fields), typically of higher dimension, have been shown to play a role in the study of a new measure of entanglement known as the symmetry resolved entanglement entropy. In this paper we give an exact expression for the two-point function of a composite twist field that arises in the Ising field theory. In doing so we extend the techniques originally developed for the standard branch point twist field in free theories as well as an existing computation due to Horváth and Calabrese of the same two-point function which focused on the leading large-distance contribution. We study the ground state two-point function of the composite twist field $\mathcal{T}_μ$ and its conjugate $\mathcal{T}_μ^\dagger$. At criticality, this field can be defined as the leading field in the operator product expansion of $\mathcal{T}$ and the disorder field $μ$. We find a general formula for $\log \langle \mathcal{T}_μ(0) \mathcal{T}^\dagger_μ(r)\rangle$ and for (the derivative of) its analytic continuation to positive real replica numbers greater than 1. We check our formula for consistency by showing that at short distances it exactly reproduces the expected conformal dimension
description: 25 pages and 3 figures
General practitioner management of low back pain : a mailed questionnaire to determine and assess GPs' knowledge, beliefs, and stated management of back pain in Victoria and New South Wales
Creators: name: Wyatt, Mary.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Broad-band spectroscopy of the transient X-ray binary pulsar KS 1947+300 during 2013 giant outburst: Detection of pulsating soft X-ray excess component
Creators: name: Epili, Prahlad
name: Naik, Sachindra
name: Jaisawal, Gaurava K.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the results obtained from detailed timing and spectral studies of the Be/X-ray binary pulsar KS 1947+300 during its 2013 giant outburst. We used data from Suzaku observations of the pulsar at two epochs i.e. on 2013 October 22 (close to the peak of the outburst) and 2013 November 22. X-ray pulsations at $\sim$18.81 s were clearly detected in the light curves obtained from both observations. Pulse periods estimated during the outburst showed that the pulsar was spinning up. The pulse profile was found to be single-peaked up to $\sim$10 keV beyond which a sharp peak followed by a dip-like feature appeared at hard X-rays. The dip-like feature has been observed up to $\sim$70 keV. The 1-110 keV broad-band spectroscopy of both observations revealed that the best-fit model comprised of a partially absorbed Negative and Positive power law with EXponential cutoff (NPEX) continuum model along with a blackbody component for the soft X-ray excess and two Gaussian functions at 6.4 and 6.7 keV for emission lines. Both the lines were identified as emission from neutral and He-like iron atom. To fit the spectra, we included the previously reported cyclotron absorption line at 12.2 keV. From the spin-up rate, the magnetic field of the pulsar was estimated to be $\sim$1.2$\times$10$^{12}$ G and found to be comparable to that obtained from the detection of the cyclotron absorption feature. Pulse-phase resolved spectroscopy revealed the pulsating nature of the soft X-ray excess component in phase with the continuum flux. This confirms that the accretion column and/or accretion stream are the most probable regions of pulsar's soft X-ray excess emission. The presence of the pulsating soft X-ray excess in phase with continuum emission may be the possible reason for not observing the dip at soft X-rays.
description: 15 pages, 9 figures, Accepted for publication in Res. in Astronomy and Astrophysics
Investigation of Anti-Reflection-Coating Stacks for Silicon Heterojunction Solar Cells
Creators: name: Meiners, B.-M.
name: Holinski, S.
name: Schäfer, P.
name: Hohage, S.
name: Borchert, D.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 1020-1023
description: High-efficiency silicon heterojunction solar cells, like the Panasonic HIT cell [1], use transparent conductive oxides (TCO) as anti-reflection layers. We investigated whether a single TCO layer or a two layers ARC stack is the better option for such a cell. Therefore we simulated the reflection and transmission properties of single indium tin oxide (ITO)-layers with various optical constants and layer systems with two different anti-reflection coatings (ARC). We also calculated the short-circuit current density (Jsc) for these systems. We found out that with a second antireflection layer the standard weighted reflectance (SWR) can be reduced by 5 % compared to single layers coatings. The best calculated Jsc for non-textured surfaces was 35.7 mA/cm2. With a texture we consider an additional Jsc gain of approx. 3 mA/cm2 approaching 39 mA/cm2.
Substitution of ITO by DC Sputtered ZnO:Al in Silicon Heterojunction Solar Cells
Creators: name: Madani Ghahfarokhi, O.
name: Sergeev, O.
name: Von Maydell, K.
name: Agert, C.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 983-986
description: In this contribution, we show our investigations of DC sputtered aluminium doped zinc oxide (ZnO:Al) as an alternative transparent conductive oxide (TCO) instead of the commonly used indium tin oxide (ITO) for application in silicon heterojunction (SHJ) solar cells consisting of amorphous (a-Si:H) and single crystal silicon. ZnO:Al is an environmentally-friendly compound with abundant elements and the material costs are much lower than for ITO. However, ZnO:Al has a lower work-function (which results in a higher Schottky barrier at TCO/emitter interface) and typically a higher resistivity compared to ITO. We show that by deposition of doped microcrystalline silicon (μc-Si:H) emitter layer instead of a doped a-Si:H layer the influence of a Schottky barrier (at TCO/emitter) could be suppressed. Additionally, by fine tuning of ZnO:Al deposition parameters including power, temperature, oxygen partial pressure and deposition time the required conductivity of the front TCO could be satisfied. The results of our study indicate that the ZnO:Al deposition parameters significantly affect the electrical properties of the obtained solar cell. By understanding and fine-tuning all these parameters, a high conversion efficiency of 19.2% on flat wafers is achieved.
Anti-Reflection Coating with High PID-Resistance for Crystalline Silicon Solar Cells
Creators: name: Mishina, K.
name: Ogishi, A.
name: Ueno, K.
name: Jonai, S.
name: Ikeno, N.
name: Saruwatari, T.
name: Hara, K.
name: Ogura, A.
name: Yamazaki, T.
name: Doi, T.
name: Masuda, A.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Solar Cell Improvements

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 996-999
description: Anti-reflection coating (ARC) on crystalline silicon solar cell plays an important role in preventing potential induced degradation (PID). It is reported that PID is suppressed by simply increasing the refractive index (RI) of silicon nitride (SiN) film as ARC. However, this method has a disadvantage in initial conversion efficiency because of dropping the optical confinement. In previous work, we have reported that the module which has an ARC deposited by new plasma enhanced chemical vapor deposition (PE-CVD) unit “MCXS” from Shimadzu Corporation indicated higher resistance to PID compared to conventional PE-CVD. In this work, we introduce superior ARC deposition to PID resistance. Both higher PID resistance and higher conversion efficiency are achieved under the condition of double or triple layers with stacked different RI of SiN compared to conventional single layer.
The $2π$ Subsystem in Diffractively Produced $π^-π^+π^-$ at COMPASS
Creators: name: Krinner, Fabian
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The COMPASS experiment at CERN has collected a large dataset of $50$ million $π^-π^+π^-$ events produced diffractively from a proton target using a $190\,\mathrm{GeV}/c$ pion beam. The partial-wave analysis (PWA) of these high-precision data reveals previously unseen details but is limited in parts by systematic effects. The PWA is based on the isobar model, in which multi-particle decays are described as a chain of subsequent two-body decays. Here, fixed mass distributions for the appearing intermediate resonances, the so-called isobars, are assumed. These shapes, which e.g. may be parametrized by Breit-Wigner amplitudes, represent prior knowledge that has to be put into the analysis model and may therefore introduce a model dependence, thus increasing systematic uncertainties. We present a novel method, which allows to extract isobar amplitudes directly from the data in a more model-independent way. As a first application, diffractively produced $π^-π^+π^-$ events are analyzed. Here, the focus lies in particular on the scalar $π^+π^-$ subsystem, where in a previous analysis a signal for a new axial-vector state $a_1(1420)$ was found in the $f_0(980)π$ decay mode.
Johannes Wild (1814-1894) an Joseph Wolfgang von Deschwanden (1819-1866)
Creators: name: Wild, Johannes
Publisher: name: [s.n.]
Year: 1864

description: Brief aus Zürich, betr. einer Angelegenheit, in der ein Schwager von J. W. von Deschwanden an Wild geschrieben hatte. Wild schickt "das von ihm erhaltene Briefchen" an Deschwanden weiter.
Bei der erwähnten Beilage handelt sich vermutlich um das im Bestand überlieferte Schreiben von F. Grossbach betreffend Bauarbeit im Zusammenhang mit dem Bau der Bülach-Regensberg-Bahn
Fragmentation of the High-mass "Starless'' Core G10.21-0.31: a Coherent Evolutionary Picture for Star Formation
Creators: name: Jiao, Wenyu
name: Wang, Ke
name: Pillai, Thushara G. S.
name: Baug, Tapas
name: Zhang, Siju
name: Xu, Fengwei
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: G10.21-0.31 is a 70 $μ$m-dark high-mass starless core ($M>300$ $\mathrm{M_{\odot}}$ within $r<0.15$ pc) identified in $Spitzer$, $Herschel$, and APEX continuum surveys, and is believed to harbor the initial stages of high-mass star formation. We present ALMA and SMA observations to resolve the internal structure of this promising high-mass starless core. Sensitive high-resolution ALMA 1.3 mm dust continuum emission reveals three cores of mass ranging 11-18 $\mathrm{M_{\odot}}$, characterized by a turbulent fragmentation. Core 1, 2, and 3 represent a coherent evolution at three different evolutionary stages, characterized by outflows (CO, SiO), gas temperature ($\mathrm{H_2CO}$), and deuteration ($\mathrm{N_2D^+/N_2H^+}$). We confirm the potential to form high-mass stars in G10.21 and explore the evolution path of high-mass star formation. Yet, no high-mass prestellar core is present in G10.21. This suggests a dynamical star formation where cores grow in mass over time.
description: 30 pages, 13 figures; accepted for publication in ApJ