cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Gas-Phase 3D Printing of Functional Materials
Creators: name: C.A.M., de la Huerta
name: V.H., Nguyen
name: A., Sekkat
name: C., Crivello
name: F., Toldra‐Reig
name: P.B., Veiga
name: S., Quessada
name: C., Jimenez
name: D., Muñoz‐Rojas
Publisher: name: figshare
Year: 2021
Subjects: subject: 30199 Analytical Chemistry not elsewhere classified
subject: FOS: Chemical sciences

description: Spatial atomic layer deposition (SALD) is a recent approach 100 times faster than conventional atomic layer deposition (ALD), even at atmospheric pressure. Previous works exploited these assets focussing on high-rate, large-area deposition for scaling-up into mass production. Conversely, this work shows that SALD indeed represents an ideal platform for area-selective deposition of functional materials by proper design and miniaturization of close-proximity SALD heads. In particular, the potential offered by 3D printing is used to fabricate low-cost customized close-proximity heads, which can be easily designed and modified to obtain different deposition areas, free-form patterns, and even complex multimaterial structures. Finally, by designing a miniaturized head with circular concentric gas channels, 3D printing of functional materials can be performed with nanometric resolution in Z. This constitutes a new gas-phase 3D printing approach. Because the process is based on ALD reactions, conformal and continuous thin films of functional materials can be printed at low temperatures and with high deposition rate in the open air. This approach represents a new versatile way of printing functional materials and devices with spatial and topological control, thus extending the potential of SALD and ALD in general, and opening a new avenue in the field of areaselective deposition of functional materials.
The 3-D composition of the Galactic interstellar medium. The hot phases and X-ray absorbing material
Creators: name: Pradas, J.
name: Kerp, J.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present maps of the Galactic X-ray Halo and constrain the location of X-ray absorbing gas using the X-ray radiation transfer as distance a indicator. Based on a consistent model of the soft X-ray background (SXRB) and the ROSAT all-sky survey, we derive the morphology of some components involved in the SXRB. In particular we focus on their spatial and temperature distributions across the sky. Starting from our SXRB model, we extract information on the 3-dimensional composition of the X-ray emitting and absorbing material. Using this approach, it is possible to differentiate between absorbing gas within or behind the Galactic X-ray Halo.
description: Astron. Nachr. in press, issue dedicated to the proceedings of the workshop "X-ray Surveys in the light of New Observatories", Sep. 2002, Santander, Spain
Stilbops vetulus
Creators: name: Riedel, Matthias
name: Diller, Erich
name: Japoshvili, George
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Stilbops
Stilbops vetulus

description: Stilbops vetulus (GRAVENHORST, 1829)
M a t e r i a l: H 4: 1♀ 3♂♂ 15-25. V, 1♂ 25.V-4. VI; H 4-5: 3♀♀ 15-25. VI; H 6: 1♂ 23.V-13. VI.
D i s t r i b u t i o n: Palaearctic region, known from the Caucasus region (KASPARYAN 1984), new for Georgia.
description: Published as part of Riedel, Matthias, Diller, Erich & Japoshvili, George, 2018, The Ichneumonid fauna (Hymenoptera: Ichneumonidae) of Lagodekhi Reserve, Sakartvelo (Georgia), with descriptions of four new species, pp. 1447-1507 in Linzer biologische Beiträge 50 (2) on page 1492, DOI: 10.5281/zenodo.5275090
Efficient Approximation Algorithms for Adaptive Seed Minimization
Creators: name: Tang, Jing
name: Huang, Keke
name: Xiao, Xiaokui
name: Lakshmanan, Laks V. S.
name: Tang, Xueyan
name: Sun, Aixin
name: Lim, Andrew
Publisher: name: arXiv
Year: 2019
Subjects: subject: Social and Information Networks (cs.SI)
subject: Data Structures and Algorithms (cs.DS)
subject: FOS: Computer and information sciences

description: As a dual problem of influence maximization, the seed minimization problem asks for the minimum number of seed nodes to influence a required number $η$ of users in a given social network $G$. Existing algorithms for seed minimization mostly consider the non-adaptive setting, where all seed nodes are selected in one batch without observing how they may influence other users. In this paper, we study seed minimization in the adaptive setting, where the seed nodes are selected in several batches, such that the choice of a batch may exploit information about the actual influence of the previous batches. We propose a novel algorithm, ASTI, which addresses the adaptive seed minimization problem in $O\Big(\frac{η\cdot (m+n)}{\varepsilon^2}\ln n \Big)$ expected time and offers an approximation guarantee of $\frac{(\ln η+1)^2}{(1 - (1-1/b)^b) (1-1/e)(1-\varepsilon)}$ in expectation, where $η$ is the targeted number of influenced nodes, $b$ is size of each seed node batch, and $\varepsilon \in (0, 1)$ is a user-specified parameter. To the best of our knowledge, ASTI is the first algorithm that provides such an approximation guarantee without incurring prohibitive computation overhead. With extensive experiments on a variety of datasets, we demonstrate the effectiveness and efficiency of ASTI over competing methods.
description: A short version of the paper appeared in 2019 International Conference on Management of Data (SIGMOD '19), June 30--July 5, 2019, Amsterdam, Netherlands. ACM, New York, NY, USA, 18 pages
Spin-orbit coupling and crystal-field distortions for a low-spin $3d^5$ state in BaCoO$_{3}$
Creators: name: Chin, Y. Y.
name: Hu, Z.
name: Lin, H. -J.
name: Agrestini, S.
name: Weinen, J.
name: Martin, C.
name: Hébert, S.
name: Maignan, A.
name: Tanaka, A.
name: Cezar, J. C.
name: Brookes, N. B.
name: Liao, Y. -F.
name: Tsuei, K. -D.
name: Chen, C. T.
name: Khomskii, D. I.
name: Tjeng, L. H.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We have studied the electronic structure of BaCoO$_3$ using soft x-ray absorption spectroscopy at the Co-$L_{2,3}$ and O-$K$ edges, magnetic circular dichroism at the Co-$L_{2,3}$ edges, as well as valence band hard x-ray photoelectron spectroscopy. The quantitative analysis of the spectra established that the Co ions are in the formal low-spin tetravalent 3$d^5$ state and that the system is a negative charge transfer Mott insulator. The spin-orbit coupling plays also an important role for the magnetism of the system. At the same time, a trigonal crystal field is present with sufficient strength to bring the 3$d^5$ ion away from the $J_{eff} = 1/2$ state. The sign of this crystal field is such that the $a_{1g}$ orbital is doubly occupied, explaining the absence of a Peierl's transition in this system which consists of chains of face-sharing CoO$_6$ octahedra. Moreover, with one hole residing in the $e_g^π$, the presence of an orbital moment and strong magneto-crystalline anisotropy can be understood. Yet, we also infer that crystal fields with lower symmetry must be present to reproduce the measured orbital moment quantitatively, thereby suggesting the possibility for orbital ordering to occur in BaCoO$_3$.
Haggenmacher, J., Fils
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1827

description: Ort: Winterthur
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Netelia (Prosthodocis) japonica
Creators: name: Riedel, Matthias
name: Diller, Erich
name: Japoshvili, George
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Netelia
Netelia japonica

description: Netelia (Prosthodocis) japonica (UCHIDA, 1928)
M a t e r i a l: H 1: 1♀ 23.IV-4. V; H 3: 1♀ 5-15. V; H 4: 1♀ 25.V-4. VI; H 5: 1♂ 15-25. VI.
D i s t r i b u t i o n: Palaearctic and Oriental regions, known from Georgia (KASPARYAN & TOLKANITZ 1999).
description: Published as part of Riedel, Matthias, Diller, Erich & Japoshvili, George, 2018, The Ichneumonid fauna (Hymenoptera: Ichneumonidae) of Lagodekhi Reserve, Sakartvelo (Georgia), with descriptions of four new species, pp. 1447-1507 in Linzer biologische Beiträge 50 (2) on page 1492, DOI: 10.5281/zenodo.5275090
Guttmann, L. M
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1827

description: Ort: Karlsruhe
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Instability-enhanced transport in low temperature magnetized plasma
Creators: name: Lucken, R.
name: Bourdon, A.
name: Lieberman, M.
name: Chabert, P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: It is shown that the transport in low temperature, collisional, bounded plasma is enhanced by instabilities at high magnetic field. While the magnetic field confines the electrons in a stable plasma, the instability completely destroys the confinement such that the transport becomes independent of the magnetic field in the highly magnetized limit. An analytical expression of the instability-enhanced collision frequency is proposed, based on a magnetic field independent edge-to-center density ratio.
description: Physics of Plasmas, American Institute of Physics, In press
Mixedness in Bell-violation vs. Entanglement of Formation
Creators: name: Ghosh, Sibasish
name: Kar, Guruprasad
name: De, Aditi Sen
name: Sen, Ujjwal
Publisher: name: arXiv
Year: 2001
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Recently Munro, Nemoto and White (The Bell Inequality: A measure of Entanglement?, quant-ph/0102119) tried to indicate that the reason behind a state rho having higher amount of entanglement (as quantified by the entanglement of formation) than a state eta, but producing the same amount of Bell-violation, is due to the fact that the amount of mixedness (as quantified by the linearised entropy) in rho is higher than that in eta. We counter their argument with examples. We extend these considerations to the von Neumann entropy. Our results suggest that the reason as to why equal amount of Bell-violation requires different amounts of entanglement cannot, at least, be explained by mixedness alone.
description: 4 pages latex, no figures
Pachybrachis spumarius Species-Group
Creators: name: Barney, Robert J.
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Chrysomelidae
Pachybrachis
Pachybrachis spumarius

description: Pachybrachis spumarius Species-Group
 Group Diagnosis. Small beetles, measuring 1.75–2.63 mm in length. Dorsum yellow, glabrous, with brown, reddish brown, or rust-colored punctures; standard maculae diffuse, often dark brown or fuscous. Eyes of male moderately separated (IOD = 0.17–0.30 mm); front without ocular lines. Protarsal claws of males not or slightly enlarged. Median lobe in en-face view widest at base, narrowing to a gently rounded ALM with a prominent nodule, varying to a circular orificial space formed by a midpoint constriction; lateral basal plates moderately sclerotized; in lateral view, ventral surface well-inflated at base, forming tube-like median lobe that narrows sharply to terminus; ventral keel absent; setal beard short and fine at apicolateral angle; pencilli absent.
 Biology. Almost nothing is known of the biology of the members of the spumarius species-group. Series of P. spumarius have been repeatedly collected on Rhus spp. (Anacardiaceae). Larvae and larval habitats are unknown.
description: Published as part of Barney, Robert J., 2017, Definition and Revision of the Spumarius Species-Group of North American Pachybrachis Chevrolat (Coleoptera: Chrysomelidae: Cryptocephalinae), pp. 449-460 in The Coleopterists Bulletin 71 (3) on page 451, DOI: 10.1649/0010-065X-71.3.449, http://zenodo.org/record/5376705
Hefty & Blumer
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1827

description: Ort: Glarus
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Healthcare resource utilization and costs in the 12 months following hospitalization for respiratory syncytial virus or unspecified bronchiolitis among infants
Creators: name: Ledbetter, Joel
name: Brannman, Lance
name: Wade, Sally W.
name: Gonzales, Tara
name: Kong, Amanda M.
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Aims: To examine healthcare resource utilization (HRU) and costs within 12 months after hospitalization for respiratory syncytial virus (RSVH) or unspecified bronchiolitis (UBH) in infants. Materials and methods: Infants born July 1, 2009–June 30, 2015 were identified in the MarketScan Medicaid and Commercial databases and were assigned to one of three cohorts: RSVH (with/without UBH), UBH, or comparator (no RSVH or UBH). Each infant was identified as pre-term (5 groups) or term (2 groups) based on weeks gestational age (wGA). Index dates were the first admission dates for RSVH or UBH infants and were randomly assigned to comparator infants based on time from birth to index in the RSVH cohort. HRU, all-cause costs, and incremental cost differences between hospitalized and comparator infants were assessed over 12 months post-index with and without the index hospitalization. Results were propensity score weighted to balance pre-index characteristics across hospitalization cohorts. Results: This study identified 15,872 RSVH infants, 6,081 UBH infants, and 986,087 comparator infants in the Medicaid population and 5,755 RSVH infants, 1,888 UBH infants, and 696,302 comparator infants in the commercial population. HRU in follow-up was greater for RSVH and UBH infants relative to comparator infants in both populations, including hospitalizations (commercial: 7.4%, 11.0%, 1.7%; Medicaid: 12.3%, 15.3%, 3.2%) and emergency department visits (commercial: 33.0%, 33.3%, 17.2%; Medicaid: 65.8%, 68.5%, 51.4%). HRU was highest among RSVH and UBH infants born at <29 wGA. Hospitalized infants had numerically higher follow-up costs than comparator infants, with incremental differences reaching $19,896 among Medicaid UBH infants and $37,417 among commercial RSVH infants. Limitations: RSV/UB may be miscoded in claims data. Conclusions: Infants hospitalized for RSV or UB largely had greater subsequent HRU and costs in the first year after index hospitalization than comparator infants. Absolute and incremental follow-up costs relative to comparator infants were highest among infants <29 wGA.
Herzogenrath, J. J
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1827

description: Ort: Nürnberg
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Caught in the Act; Chandra Observations of Microlensing of the Radio-Loud Quasar MG J0414+0534
Creators: name: Chartas, G.
name: Agol, E.
name: Eracleous, M.
name: Garmire, G.
name: Bautz, M. W.
name: Morgan, N. D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results from monitoring of the distant (z = 2.64), gravitationally lensed quasar MG J0414+0534 with the Chandra X-ray Observatory. An Fe Ka line at 6.49 +/- 0.09 keV (rest-frame) with an equivalent width of ~ 190eV consistent with fluorescence from a cold medium is detected at the 99 percent confidence level in the spectrum of the brightest image A. During the last two observations of our monitoring program we detected a five-fold increase of the equivalent width of a narrow Fe Ka line in the spectrum of image B but not in the brighter image A whereas image C is too faint to resolve the line. The continuum emission component of image B did not follow the sudden enhancement of the iron line in the last two observations. We propose that the sudden increase in the iron line strength from ~ 190eV to 900eV only in image B can be explained with a caustic crossing due to microlensing that selectively enhances a strip of the line emission region of the accretion disk. The non-enhancement of the continuum emission in the spectrum of image B suggests that the continuum emission region is concentrated closer to the center of the accretion disk than the iron line emission region and the magnification caustic has not reached close enough to the former region to amplify it. A model of a caustic crossing event predicts discontinuities in the light-curve of the magnification and provides an upper limit of ~ 5 x 10^(-4) pc on the outer radius of the Fe Ka emission region. The non-detection of any relativistic or Doppler shifts of the iron line in the spectrum of image B implies that the magnification caustic for the last two observations was located at a radius greater than ~ 100 gravitational radii.
description: 27 pages, includes 11 figures, Accepted for publication in ApJ
Netelia (Bessobates) cristata
Creators: name: Riedel, Matthias
name: Diller, Erich
name: Japoshvili, George
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Netelia
Netelia cristata

description: Netelia (Bessobates) cristata (THOMSON, 1888)
M a t e r i a l: H 4: 1♀ 5-15.V.
D i s t r i b u t i o n: Palaearctic and Oriental regions, known from Georgia (KOKUJEV 1899).
description: Published as part of Riedel, Matthias, Diller, Erich & Japoshvili, George, 2018, The Ichneumonid fauna (Hymenoptera: Ichneumonidae) of Lagodekhi Reserve, Sakartvelo (Georgia), with descriptions of four new species, pp. 1447-1507 in Linzer biologische Beiträge 50 (2) on page 1492, DOI: 10.5281/zenodo.5275090
Additional file 1 of A neutrophil-to-lymphocyte ratio-based prognostic model to predict mortality in patients with HBV-related acute-on-chronic liver failure
Creators: name: Sun, Jian
name: Guo, Hongying
name: Yu, Xueping
name: Zhu, Haoxiang
name: Zhang, Xueyun
name: Yang, Jianghua
name: Wang, Jiefei
name: Qian, Zhiping
name: Shen, Zhongliang
name: Mao, Richeng
name: Zhang, Jiming
Publisher: name: figshare
Year: 2021
Subjects: subject: Space Science
subject: Medicine
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1. Table S1–S3.
Shades of Dark Uncertainty and Consensus Value for the Newtonian Constant of Gravitation
Creators: name: Merkatas, Christos
name: Toman, Blaza
name: Possolo, Antonio
name: Schlamminger, Stephan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: Classical Physics (physics.class-ph)
subject: Applications (stat.AP)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: The Newtonian constant of gravitation, $G$, stands out in the landscape of the most common fundamental constants owing to its surprisingly large relative uncertainty, which is attributable mostly to the dispersion of the values measured for it in different experiments. This study focuses on a set of measurements of $G$ that are mutually inconsistent, in the sense that the dispersion of the measured values is significantly larger than what their reported uncertainties suggest that it should be. Furthermore, there is a loosely defined group of measured values that lie fairly close to a consensus value that may be derived from all the measurement results, and then there are one or more groups with measured values farther away from the consensus value, some higher, others lower. This same general pattern is often observed in many interlaboratory studies and meta-analyses. In the conventional treatments of such data, the mutual inconsistency is addressed by inflating the reported uncertainties, either multiplicatively, or by the addition of random effects, both reflecting the presence of dark uncertainty. The former approach is often used by CODATA and by the Particle Data Group, and the latter is common in medical meta-analysis and in metrology. We propose a new procedure for consensus building that models the results using latent clusters with different shades of dark uncertainty, which assigns a customized amount of dark uncertainty to each measured value, as a mixture of those shades, and does so taking into account both the placement of the measured values relative to the consensus value, and the reported uncertainties. We demonstrate this procedure by deriving a new estimate for $G$, as a consensus value $G = 6.67408 \times 10^{-11} \,\text{m}^{-3} \, \text{kg}^{-1} \, \text{s}^{-2}$, with $u(G) = 0.00024 \times 10^{-11} \,\text{m}^{-3} \, \text{kg}^{-1} \, \text{s}^{-2}$.
Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps
Creators: name: Rubino-Martin, J. A.
name: Sunyaev, R. A.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Clusters of galaxies produce negative features at wavelengths $λ> 1.25$ mm in CMB maps, by means of the thermal SZ effect, while point radio sources produce positive peaks. This fact implies that a distribution of unresolved SZ clusters could be detected using the negative asymmetry introduced in the odd-moments of the brightness map (skewness and higher), or in the probability distribution function (PDF) for the fluctuations, once the map has been filtered in order to remove the contribution from primordial CMB fluctuations from large scales. This property provides a consistency check to the recent detections from CBI and BIMA experiments of an excess of power at small angular scales, in order to confirm that they are produced by a distribution of unresolved SZ clusters. However it will require at least 1.5 - 2 times more observing time than detection of corresponding power signal. This approach could also be used with the data of the planned SZ experiments (e.g. ACT, AMI, AMIBA, APEX, 8 m South Pole telescope).
description: Includes a new section and a new appendix. Typos corrected. Accepted for publication in MNRAS
Gundlach, C. F. Witwe, & Koch
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1827

description: Ort: Lübeck
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Fidelity trade-off for finite ensembles of identically prepared qubits
Creators: name: Banaszek, Konrad
name: Devetak, Igor
Publisher: name: arXiv
Year: 2001
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We calculate the trade-off between the quality of estimating the quantum state of an ensemble of identically prepared qubits and the minimum level of disturbance that has to be introduced by this procedure in quantum mechanics. The trade-off is quantified using two mean fidelities: the operation fidelity which characterizes the average resemblance of the final qubit state to the initial one, and the estimation fidelity describing the quality of the obtained estimate. We analyze properties of quantum operations saturating the achievability bound for the operation fidelity versus the estimation fidelity, which allows us to reduce substantially the complexity of the problem of finding the trade-off curve. The reduced optimization problem has the form of an eigenvalue problem for a set of tridiagonal matrices, and it can be easily solved using standard numerical tools.
description: 26 pages, REVTeX, 2 figures. Few minor corrections, accepted for publication in Physical Review A
Netelia (Bessobates) latungula
Creators: name: Riedel, Matthias
name: Diller, Erich
name: Japoshvili, George
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Netelia
Netelia latungula

description: Netelia (Bessobates) latungula (THOMSON, 1888)
M a t e r i a l: H 2: 1♀ 27.IX-6.X.
D i s t r i b u t i o n: Holarctic regions, known from Azerbaijan (TOLKANITZ 1981), new for Georgia.
description: Published as part of Riedel, Matthias, Diller, Erich & Japoshvili, George, 2018, The Ichneumonid fauna (Hymenoptera: Ichneumonidae) of Lagodekhi Reserve, Sakartvelo (Georgia), with descriptions of four new species, pp. 1447-1507 in Linzer biologische Beiträge 50 (2) on page 1492, DOI: 10.5281/zenodo.5275090
Guébhard, Fred
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1827

description: Ort: Alexandria / Ägypten
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Hagen, Ferdinand, von
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1827

description: Ort: Remscheid
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Chemical abundances in the metal-intermediate GC NGC 6723
Creators: name: Crestani, Juliana
name: Alves-Brito, Alan
name: Bono, Giuseppe
name: Puls, Arthur A.
name: Alonso-García, Javier
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have performed a detailed spectral analysis of the inner halo Galactic globular cluster (GC) NGC 6723 using high resolution (R$\approx$ 22000-48000) spectra for for eleven red giant branch stars collected with MIKE (Magellan) and FEROS (MPG/ESO). This globular is located at the minimum of the bimodal metallicity distribution of GCs suggesting that it might be an excellent transitional system between metal-intermediate and metal-rich GCs. In spite of its metal-intermediate status, it is characterized by an extended horizontal branch and by a large number of RR Lyrae stars. We investigated abundances of a variety of species including light, $α$-, Fe-peak, and neutron capture elements. We found a mean metallicity $[Fe/H]=-0.93 \pm 0.05$ dex, and a typical $α$ -enrichment ($[α/Fe] \approx 0.39$) that follows the trend of metal-poor and metal-intermediate GCs. The same outcome applies for light metals (Na, Al), Fe-peak (V, Cr, Mn, Fe, Co, Ni, Cu), $s$/$r$-process elements (Ba, Eu) and for the classical anti-correlation: Na-O and Mg-Al. The current findings further support the evidence that the chemical enrichment of NGC 6723 is in more line with metal-intermediate GCs and their lower metallicity counterparts, and it does not bring forward the prodrome of the metal-rich regime.
description: MNRAS, accepted for publication
Optical Observations of Blazars: the Perugia Monitoring
Creators: name: Tosti, G.
name: Ciprini, S.
name: Nucciarelli, G.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In eight years, during the blazar monitoring program performed with the Perugia automatic telescope, we were able to collect about 20000 $BVR_cI_c$ photometric points, contributing to get knowledge on the optical flux history of many sources brighter than magnitude $V=17.0$. This intensive and constant optical monitoring is essential to perform studies and multiwavelength campains about this class of AGN. We illustrate our program and some examples of data and preliminary results.
description: 4 pages, 4 figures, oral contribution for the ''Frascati Workshop 2001: Multifrequency Behaviuor of High Energy Cosmic Sources'', Vulcano, Aeolian Islands, Italy, May 21-26, 2001. To be published in Memorie della Societa' Astronomica Italiana (Journal of the Italian Astronomical Society), 2002
Atmospheric plasma-enhanced spatial chemical vapor deposition of SiO2 using trivinylmethoxysilane and oxygen plasma
Creators: name: V.H., Nguyen
name: A., Sekkat
name: C., Arturo
name: M., de la Huerta
name: F., Zoubian
name: C., Crivello
name: J., Rubio-Zuazo
name: M., Jaffal
name: M., Bonvalot
name: C., Vallée
name: O., Aubry
name: H., Rabat
name: D., Hong
name: D., Muñoz-Rojas
Publisher: name: figshare
Year: 2021
Subjects: subject: 30199 Analytical Chemistry not elsewhere classified
subject: FOS: Chemical sciences

description: SiO2 constitutes one of the most widely used dielectric materials in the microelectronics, packaging, and optical industries. Therefore, the development of new processes to deposit SiO2 at low temperature and in an affordable and scalable way are desirable. In this work, we present a low-temperature, open-air process based on spatial atomic layer deposition (SALD) that yields high purity SiO2 films at temperatures down to room temperature. The films were obtained by operating our SALD system in CVD mode (i.e., allowing precursor crosstalk), using an oxygen plasma in combination with trivinylmethoxysilane (TVMS). TVMS is an appealing precursor since it is highly volatile, is affordable, and does not contain halogen elements, thus being very suitable for application in atmospheric-pressure spatial deposition systems. Conversely, water, oxygen, hydrogen peroxide, or ozone did not show any reactivity with TVMS at temperatures up to 260 °C. Thus, when operating our system in ALD mode, no film could be obtained due to the lack of reactivity of the precursor with OH* surface groups. 3D printing was employed to fabricate custom heads integrating both the precursor injector and the atmospheric plasma generator. Our results show that conformal SiO2 thin films can be deposited by our atmospheric plasma-enhanced spatial chemical vapor deposition (APE-SCVD) approach at low temperatures (RT−180 °C) on different substrates, including silicon wafers, microglass slides, or even polymeric substrates with a high growth rate up to 2−5 nm/min. The deposition rate increased when increasing the power applied to the plasma reactor but decreased when increasing the deposition temperature due to the faster decay of the metastable oxygen radical species. FTIR results showed no differences for films deposited with different plasma powers. Conversely, temperature had an effect on the ratio between the AS1 and the AS2 bands. Even though the deposition of SiO2 was carried out at low temperatures in the open air using a metalorganic precursor, no contamination from SiNx or SiCx was observed by FTIR and XPS measurements. Our results open the door to the low-temperature, fast printing of Si-based devices.
title: ÐÐ´Ð´Ð¸ÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð² ÑÐ²ÐµÐ»Ð¸ÑÐ½Ð¾Ð¼ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ðµ, Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÑ ÑÐºÑÐ°ÑÐµÐ½Ð¸Ð¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
title: Additive technologies in jewelry production, production of individual jewelry
Creators: name: ÐÐ°ÑÑÐ¾Ð»Ð¾Ð³Ð°, ÐÐ°Ð½Ð¸Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2024
Subjects: Ð®Ð²ÐµÐ»Ð¸ÑÐ½Ð¾Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾
SLM Ð¿ÐµÑÐ°ÑÑ
Ð°Ð´Ð´Ð¸ÑÐ¸Ð²Ð½Ð¾Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾
Ð¿ÐµÑÐ°ÑÑ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð¼
SLM printing
additive manufacturing
metal printing

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÑ ÑÐ²ÐµÐ»Ð¸ÑÐ½ÑÑ ÑÐºÑÐ°ÑÐµÐ½Ð¸Ð¹ Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð°Ð´Ð´Ð¸ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°, ÐºÐ»ÑÑÐµÐ²ÑÐµ Ð·Ð°Ð´Ð°ÑÐ¸: - Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð°Ð´Ð´Ð¸ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð² ÑÐ²ÐµÐ»Ð¸ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸; - Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ ÑÐµÐ»ÐµÐ²Ð°Ð½ÑÐ½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹; - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÑ ÑÐ²ÐµÐ»Ð¸ÑÐ½ÑÑ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ SLM-Ð¿ÐµÑÐ°ÑÐ¸; - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð¼ Ð¿ÑÐ¾Ð´ÐµÐ»Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð°Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ ÑÐ¾-Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÑ ÑÐ²ÐµÐ»Ð¸ÑÐ½ÑÑ ÑÐºÑÐ°ÑÐµÐ½Ð¸Ð¹ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ ÑÐµÐ»ÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð»Ð°Ð·ÐµÑÐ½Ð¾Ð³Ð¾ ÑÐ¿ÐµÐºÐ°Ð½Ð¸Ñ.
description: This work is devoted to the development of technology for the creation of individual jewelry with the use of additive manufacturing methods, key tasks: - research of existing methods of additive manufacturing in the jewelry industry; - identification of relevant technologies; - development of technology for creating individual jewelry by SLM-printing method; - development of technical recommendations. The result of the work done is the developed technology of creation of individual jewelry by selective laser sintering method.
Netelia (Bessobates) virgata
Creators: name: Riedel, Matthias
name: Diller, Erich
name: Japoshvili, George
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Netelia
Netelia virgata

description: Netelia (Bessobates) virgata (GEOFFROY, 1785)
M a t e r i a l: H 1: 1♀ 4-14.VI.
D i s t r i b u t i o n: Palaearctic and Oriental regions, known from Azerbaijan (KASPARYAN & TOLKANITZ 1999), new for Georgia.
description: Published as part of Riedel, Matthias, Diller, Erich & Japoshvili, George, 2018, The Ichneumonid fauna (Hymenoptera: Ichneumonidae) of Lagodekhi Reserve, Sakartvelo (Georgia), with descriptions of four new species, pp. 1447-1507 in Linzer biologische Beiträge 50 (2) on page 1493, DOI: 10.5281/zenodo.5275090
Models of Metal Poor Stars with Gravitational Settling and Radiative Accelerations: I. Evolution and Abundance Anomalies
Creators: name: Richard, O.
name: Michaud, G.
name: Richer, J.
name: Turcotte, S.
name: Turck-Chieze, S.
name: VandenBerg, Don A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Evolutionary models have been calculated for Pop II stars of 0.5 to 1.0$M_\odot$ from the pre-main-sequence to the lower part of the giant branch. Rosseland opacities and radiative accelerations were calculated taking into account the concentration variations of 28 chemical species, including all species contributing to Rosseland opacities in the OPAL tables. The effects of radiative accelerations, thermal diffusion and gravitational settling are included. While models were calculated both for Z=0.00017 and 0.0017, we concentrate on models with Z=0.00017 in this paper. These are the first Pop II models calculated taking radiative acceleration into account. It is shown that, at least in a 0.8$M_\odot$ star, it is a better approximation not to let Fe diffuse than to calculate its gravitational settling without including the effects of $g_{rad}(Fe)$. In the absence of any turbulence outside of convection zones, the effects of atomic diffusion are large mainly for stars more massive than 0.7$M_\odot$. Overabundances are expected in some stars with $\teff \ge 6000K$. Most chemical species heavier than CNO are affected. At 12 Gyr, overabundance factors may reach 10 in some cases (e.g. for Al or Ni) while others are limited to 3 (e.g. for Fe). The calculated surface abundances are compared to recent observations of abundances in globular clusters as well as to observations of Li in halo stars. It is shown that, as in the case of Pop I stars, additional turbulence appears to be present.
description: 40 pages, 17 color figures, to appear in The Astrophysical Journal, April 2002 (paper with original high resolution figures can be found at http://www.cerca.umontreal.ca/~richer/Fichiersps/popII_1.ps)
On a Lie algebraic approach of quasi-exactly solvable potentials with two known eigenstates
Creators: name: Brihaye, Y.
name: Debergh, N.
name: Ndimubandi, J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We compare two recent approaches of quasi-exactly solvable Schr\" odinger equations, the first one being related to finite-dimensional representations of $sl(2,R)$ while the second one is based on supersymmetric developments. Our results are then illustrated on the Razavy potential, the sextic oscillator and a scalar field model.
description: LaTeX, 10 pages
SN1999E: Another piece in the SN-GRB connection puzzle
Creators: name: Rigon, L.
name: Turatto, M.
name: Benetti, S.
name: Pastorello, A.
name: Cappellaro, E.
name: Aretxaga, I.
name: Vega, O.
name: Chavushyan, V.
name: Patat, F.
name: Danziger, I. J.
name: Salvo, M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Detailed optical and near-IR observations of SN 1999E have confirmed early suggestions that this supernova was indeed a twin of the peculiar type II SN 1997cy: it was exceptionally luminous and had evolved slowly, and the line profiles had narrow peaks and broad wings, indicating interaction with the circumstellar material. Nevertheless, the most intriguing characteristic was that, in analogy to SN 1997cy, it exploded at a position consistent in time and location with a BATSE event (GRB980910). The "a posteriori" probability that the only two SNe with such an optical appearance are associated with two different BATSE GRB is only 0.2%. This raises the possibility that some GRB are associated with H--rich SNe.
description: accepted for publication in MNRAS
SylNet: An Adaptable End-to-End Syllable Count Estimator for Speech
Creators: name: Seshadri, Shreyas
name: Räsänen, Okko
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computation and Language (cs.CL)
subject: Sound (cs.SD)
subject: Audio and Speech Processing (eess.AS)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Automatic syllable count estimation (SCE) is used in a variety of applications ranging from speaking rate estimation to detecting social activity from wearable microphones or developmental research concerned with quantifying speech heard by language-learning children in different environments. The majority of previously utilized SCE methods have relied on heuristic DSP methods, and only a small number of bi-directional long short-term memory (BLSTM) approaches have made use of modern machine learning approaches in the SCE task. This paper presents a novel end-to-end method called SylNet for automatic syllable counting from speech, built on the basis of a recent developments in neural network architectures. We describe how the entire model can be optimized directly to minimize SCE error on the training data without annotations aligned at the syllable level, and how it can be adapted to new languages using limited speech data with known syllable counts. Experiments on several different languages reveal that SylNet generalizes to languages beyond its training data and further improves with adaptation. It also outperforms several previously proposed methods for syllabification, including end-to-end BLSTMs.
Heermann & Stephan
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1827

description: Ort: Altenburg / Thüringen
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Supporting data from Design, synthesis and biological evaluation of a series of new resveratrol analogues as potential anti-cancer agents
Creators: name: Lifang Yang
name: Xuemei Qin
name: Hongcun Liu
name: Yanye Wei
name: Hailiang Zhu
name: Mingguo Jiang
Publisher: name: The Royal Society
Year: 2019
Subjects: subject: Biochemistry
subject: 30499 Medicinal and Biomolecular Chemistry not elsewhere classified
subject: FOS: Chemical sciences

description: Figures of NMR and HRMS spectra
Heat acclimation attenuates the increased sensations of fatigue reported during acute exercise-heat stress
Creators: name: Willmott, Ashley G B
name: Hayes, Mark
name: James, Carl A.
name: Gibson, Oliver R.
name: Maxwell, Neil S.
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Science Policy
subject: 69999 Biological Sciences not elsewhere classified
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Athletes exercising in heat stress experience increased perceived fatigue acutely, however it is unknown whether heat acclimation (HA) reduces the magnitude of this perceptual response and whether different HA protocols influence the response. This study investigated sensations of fatigue following; acute exercise-heat stress; short- (5-sessions) and medium-term (10-sessions) HA; and between once- (ODHA) and twice-daily HA (TDHA) protocols. Twenty male participants (peak oxygen uptake: 3.75 ± 0.47 L·min-1) completed 10 sessions (60-min cycling at ~2 W·kg-1, 45°C/20% relative humidity) of ODHA (n = 10) or non-consecutive TDHA (n = 10). Sensations of fatigue (General, Physical, Emotional, Mental, Vigor and Total Fatigue) were assessed using the multi-dimensional fatigue scale inventory-short form pre and post session 1, 5 and 10. Heat adaptation was induced following ODHA and TDHA, with reductions in resting rectal temperature and heart rate, and increased plasma volume and sweat rate (P ∆: Change; ANOVA: Analysis of variance; HA: Heat acclimation; HR: Heart rate; IL-6: Interleukin-6; MFS-SF: Multi-dimensional fatigue symptom inventory-short form (MFSI-SF); MTHA: Medium-term heat acclimation; Na+: Sodium; ODHA: Once daily heat acclimation; PV: Plasma volume; RH: Relative humidity; RPE: Rating of perceived exertion; SD: Standard deviation; SE: Standard error of the slope coefficient or intercept; SEE : Standard error of the estimate for the regression equation; STHA: Short-term heat acclimation; TDHA: Twice daily heat acclimation; TC: Thermal Comfort; Tre: Rectal temperature; TSS: Thermal sensation; V̇O2peak: Peak oxygen uptake; WBSL: whole-body sweat loss.
NRQCD colour-octet expansion vs LHC quarkonium production: signs of a hierarchy puzzle?
Creators: name: Faccioli, Pietro
name: Lourenco, Carlos
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The observation of unpolarized quarkonium production in high energy pp collisions, at mid rapidity, implies a significant violation of the non-relativistic QCD (NRQCD) velocity scaling rules. A precise experimental confirmation of this picture could definitely rule out the current formulation of the factorization expansion. This conclusion relies on current perturbative determinations of the short-distance kinematic factors and may be reverted if improved calculations would modify, in a very specific way, their transverse momentum dependences. That solution would result, however, in a full degeneracy in the presently assumed basis of $^{2S+1}L_J$ Fock states. Therefore, whatever the outcome, improved polarization measurements will challenge and improve our fundamental understanding of quarkonium production.
description: To appear in European Physical Journal C
Determination of masses and other properties of extra-solar planetary systems with more than one planet
Creators: name: Nauenberg, Michael
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent analysis of the Doppler shift oscillations of the light from extra-solar planetary systems indicate that some of these systems have more than one large planet. In this case it has been shown that the masses of these planets can be determined without the familiar ambiguity due to the unknown inclination angle of the plane of the orbit of the central star provided, however, that its mass is known. A method is presented here which determines also a lower limit to the mass of this star from these observations. As an illustration, our method is applied to the Keck and Lick data for GJ876.
description: 10 pages, 17 figures. Accepted for publication in Astrophysical Journal
Биосурфактанты-пенообразователи в сахарном производстве
Creators: name: В.А. Сотников
name: Т.Р. Мустафин
name: А.В. Грязева
Publisher: name: Сахар
Year: 2021

description: В работе проведены исследования по выявлению способности посторонней микрофлоры сахарных предприятий к продуцированию пенообразующих веществ – биосурфактантов. Показано, что наиболее активными продуцентами являются грибы кагатной гнили свёклы, гнилостные бактерии и дрожжи сахаросодержащих потоков. Молочнокислые бактерии не обладают выраженной пенообразующей активностью. Обеспложивание потоков бактерицидным препаратом «Тетасепт» предотвращает микробиологическое пенение сахаросодержащих потоков.
description: транспортёрно-моечная вода (ТМВ), диффузионный сок, грибы кагатной гнили, дрожжи, гнилостные бактерии, биосурфактанты, пенообразование.
Netelia (Paropheltes) thomsonii
Creators: name: Riedel, Matthias
name: Diller, Erich
name: Japoshvili, George
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Netelia
Netelia thomsonii

description: Netelia (Paropheltes) thomsonii (BRAUNS, 1899)
M a t e r i a l: H 1: 1♀ 23.V-4. VI; H 4-5: 1♀ 5-15.VII.
D i s t r i b u t i o n: Palaearctic and Oriental regions, known from Georgia (KOKUJEV 1899).
description: Published as part of Riedel, Matthias, Diller, Erich & Japoshvili, George, 2018, The Ichneumonid fauna (Hymenoptera: Ichneumonidae) of Lagodekhi Reserve, Sakartvelo (Georgia), with descriptions of four new species, pp. 1447-1507 in Linzer biologische Beiträge 50 (2) on page 1493, DOI: 10.5281/zenodo.5275090
title: The Court of Justice's Self-restraint of Reviewing Financial Assistance Conditionality in the Chrysostomides Case
Creators: name: Staudinger, Isabel
Publisher: name: European Papers (www.europeanpapers.eu)
Year: 2021
Subjects: subject: financial assistance conditionality
subject: Eurogroup
subject: accountability
subject: action for damages
subject: Economic and Monetary Union
subject: Cyprus

description: European Papers - A Journal on Law and Integration, 2021 6(1), 177-188
description: European Forum Insight of 28 May 2021
description: I. Introduction. - II. Background: the EU Courts and the Euro crisis. - II.1. Ledra: applicability of the Charter of Fundamental Rights of the EU. - II.2. Mallis: no action for annulment of a Eurogroup statement. - III. The Chrysostomides case. - III.1. The judgment of the General Court. - III.2. The judgement of the ECJ. - IV. Implications for legal protection against financial assistance conditionality. - V. Conclusions.
description: In the Chrysostomides case (joined cases C-597/18 P, C-598/18 P, C-603/18 P and C-604/18 P Council v Chrysostomides Co. and Others ECLI:EU:C:2020:1028), the Court of Justice (ECJ) confirmed its previous finding that the Eurogroup has only an informal and intergovernmental nature. Building on the cases Ledra and Mallis, the ECJ finally denied the respective possibilities of EU legal protection against acts and conduct of the Eurogroup. Moreover, the ECJ denied the binding nature of art. 2(6)(b) of Council Decision (EU) 2013/236, a decision with which the conditionality of the macro-economic adjustment programme had been brought under the auspices of EU law. As a consequence, the Eurogroup's acts and conduct as well as conditionality measures cannot be reviewed on the EU level.