cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Ixobrychus exilis Least Bittern WA
Creators: name: Vilas Boas da Frota, Angélica
name: Vitorino, Breno Dias
name: da Silva, Carolina Joana
name: Ikeda-Castrillon, Solange Kimie
name: Nunes, Josué Ribeiro da Silva
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Pelecaniformes
Ardeidae
Ixobrychus
Ixobrychus exilis

description: Ixobrychus exilis (Gmelin, 1789)
Figure 2F
 Material examined. Tables 1, 2.
 IDentificAtion. This species was detected in all periods, mostly by voice. It was rarely seen but frequently heard. This species was observed making short flights and discreet landings among aquatic macrophytes (Pontederiaceae and Polygonaceae). Ixobrychus exilis has a characteristic voice and vocalises frequently. This species is a small, reddish-brown bittern, with two white stripes on the back. The male has a black cap and back, with yellowish stripes on the throat, while the female has a brown cap and back, with the darkest bands on the neck (Martínez-Vilata et al. 2018).
description: Published as part of Vilas Boas da Frota, Angélica, Vitorino, Breno Dias, da Silva, Carolina Joana, Ikeda-Castrillon, Solange Kimie & Nunes, Josué Ribeiro da Silva, 2020, Birds of the Ramsar site Estação Ecológica de Taiamã and buffer zone, Pantanal wetlands, Brazil, pp. 401-422 in Check List 16 (2) on page 416, DOI: 10.15560/16.2.401
Cosmological wave maps
Creators: name: Cotsakis, Spiros
name: Miritzis, John
name: Tzanni, Koralia
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We consider theories of gravity that include many coupled scalar fields with arbitrary couplings, in the geometric framework of wave maps. We examine the possibility of obtaining acceptable cosmological solutions without the inclusion of a potential term to the scalar fields. To illustrate the theory, we study two simple models and compare their solutions to those in General Relativity. We also address the issue of the conditions that must be satisfied by the wave maps for an accelerated phase of the Universe.
description: 13 pages, 2 figures. To appear in IJMPA
Geostiba (Sibiota) gibbera ASSING 2005
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Geostiba
Geostiba gibbera

description: Geostiba (Sibiota) gibbera ASSING 2005
M a t e r i a l e x a m i n e d: Turkey: 15exs., Kahramanmaraş, Imalı, 37°21'N, 36°44'E, 850 m, 21.IV.2009, leg. Brachat & Meybohm (cAss).
This recently described species has become known only from the area to the northeast of Kozan, Adana province (ASSING 2005b). The above specimens were collected at or near the type locality.
description: Published as part of Assing, V., 2009, A revision of Geostiba of the Western Palaearctic region. XIX. New species from Turkey and Iran and additional records, with an updated key and a catalogue of the species of the Eastern Mediterranean, the Caucasus, and adjacent regions (Coleoptera: Staphylinidae: Aleocharinae), pp. 1191-1246 in Linzer biologische Beiträge 41 (2) on page 1212, DOI: 10.5281/zenodo.5276563
Application of the variational principle to a coherent-pair condensate: The HFB case
Creators: name: Jia, L. Y.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Recently we proposed a scheme that applies the variational principle to a coherent-pair condensate in the BCS case [Phys. Rev. C 99, 014302 (2019)]. This work extends the scheme to the HFB case by allowing variation of the canonical single-particle basis. The result is equivalent to that of the so-called variation after particle-number projection in the HFB case, but now the particle number is always conserved and the time-consuming projection is avoided. Specifically, we derive the analytical expression for the gradient of the average energy with respect to changes of the canonical basis, which is then used in the family of gradient minimizers to iteratively minimize energy. In practice, we find the so-called ADAM minimizer (adaptive moments of gradient), borrowed from the machine-learning field, is very effective. The new algorithm is demonstrated in a semi-realistic example using the realistic $V_{\rm{low}{\textrm{-}}k}$ interaction and large model spaces (up to $15$ harmonic-oscillator major shells). It easily runs on a laptop, and practically the computer time cost (in the HFB case) is several times that of solving HF by the gradient minimizers. We hope the new algorithm could become a common practice because of its simplicity.
description: This paper is a sequel to "arXiv:1808.03729 [nucl-th] (2018)"
The Fundamental Line of the Local Group Satellites
Creators: name: Prada, Francisco
name: Burkert, Andreas
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a new correlation between the mass-to-light (M/L) ratio and the mean metallicity for the satellites of the Local Group. This relation together with their central surface brightness define a Fundamental Line where metal poor and low surface brightness dwarfs are dark matter dominated while metal rich high surface brightness systems will have a low M/L ratio. This Fundamental Line is independent of distance to the central galaxy (M31 and the Milky Way) and morphological type among other global parameters as their star formation history. The new M/L-metallicity relation indicates that dwarf spheroidal galaxies are dark matter confined. It can be interpreted if satellites experienced a continuous loss of metals with a final episode of gas ejection at the end of the star formation epoch. Only Globular Clusters are found to lie outside the Fundamental Line of dwarf satellites. Unlike satellite galaxies they are not dark matter confined.
description: 9 pages,2 figures. Submitted to ApJ Letters
Corallistes Schmidt 1870
Creators: name: Schlacher-Hoenlinger, Monika A.
name: Pisera, Andrzej
name: Hooper, John N. A.
Publisher: name: Zenodo
Year: 2005
Subjects: Biodiversity
Taxonomy
Animalia
Porifera
Demospongiae
Tetractinellida
Corallistidae
Corallistes

description: Genus Corallistes Schmidt, 1870
 Corallistes Schmidt, 1870: 22, pl. 3: 3.
 Coscinospongia Lendenfeld, 1903: 135.
 TYPE SPECIES. — Corallistes typus Schmidt, 1870 by subsequent designation (Pisera F Lévi 2002b).
DEFINITION. — Lithistids with smooth upper surface and with smooth ectosomal dichotriaenes and tuberculated monocrepidial dicranoclones; microscleres are spirasters (usually two types) (Pisera F Lévi 2002b).
description: Published as part of Schlacher-Hoenlinger, Monika A., Pisera, Andrzej & Hooper, John N. A., 2005, Deep-sea " lithistid " assemblages from the Norfolk Ridge (New Caledonia), with description of seven new species and a new genus (Porifera, Demospongiae), pp. 649-698 in Zoosystema 27 (4) on page 663, DOI: 10.5281/zenodo.5393958
title: Functional Requirements and Recommendations for AI-based Sustainable Energy Solutions
Creators: name: Lowin, Maximilian
name: Mihale-Wilson, Cristina
Publisher: name: Gesellschaft für Informatik e.V.
Year: 2024
Subjects: subject: AI-based Services
subject: Functional Requirements
subject: Sustainable Energy Consumption
subject: Sustainable Heating

description: SMEs contribute to energy conservation by innovating smart services across domains. This article supports the design and implementation of AI-based products and services for sustainable energy solutions by uniting insights from research and practice. Specifically, it presents an iterative approach to document and refine appropriate functional requirements from the literature and three expert focus groups. The set of requirements presented can help SMEs to allocate their development resources efficiently by indicating those functions that are a must or rather optional. Besides, to bolster SME initiatives for AI-based sustainable energy solutions, this article articulates several recommendations for implementing the most important requirements into practice.
Scleritoderma Sollas 1888
Creators: name: Schlacher-Hoenlinger, Monika A.
name: Pisera, Andrzej
name: Hooper, John N. A.
Publisher: name: Zenodo
Year: 2005
Subjects: Biodiversity
Taxonomy
Animalia
Porifera
Demospongiae
Tetractinellida
Scleritodermidae
Scleritoderma

description: Genus Scleritoderma Sollas, 1888
 Scleritoderma Sollas, 1888: 316, pl. 35: 26-50.
 TYPE SPECIES. — Scleritoderma flabelliforme Sollas, 1888 by subsequent designation (Pisera F Lévi 2 002a).
DEFINITION. — Sponges with spinose rhizoclone desmas and ectosomal acanthostrongyles/rhabds forming a dense tangential layer on the surface; microscleres are sigmaspires (Pisera F Lévi 2002a).
description: Published as part of Schlacher-Hoenlinger, Monika A., Pisera, Andrzej & Hooper, John N. A., 2005, Deep-sea " lithistid " assemblages from the Norfolk Ridge (New Caledonia), with description of seven new species and a new genus (Porifera, Demospongiae), pp. 649-698 in Zoosystema 27 (4) on page 655, DOI: 10.5281/zenodo.5393958
SNe heating and the chemical evolution of the intra-cluster medium
Creators: name: Pipino, Antonio
name: Matteucci, Francesca
name: Borgani, Stefano
name: Biviano, Andrea
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compute the chemical and thermal history of the intra-cluster medium in rich and poor clusters under the assumption that supernovae (I, II) are the major responsible both for the chemical enrichment and the heating of the intra-cluster gas. We assume that only ellipticals and S0 galaxies contribute to the enrichment and heating of the intra-cluster gas through supernova driven winds and explore several prescriptions for describing the feed-back between supernovae and the interstellar medium in galaxies. We integrate then the chemical and energetical contributions from single cluster galaxies over the cluster luminosity function and derive the variations of these quantities as functions of the cosmic time. We reach the following conclusions: i) while type II supernovae dominates the chemical enrichment and energetics inside the galaxies, type Ia supernovae play a predominant role in the intra-cluster medium, ii) galaxy models, which reproduce the observed chemical abundances and abundance ratios in the intra-cluster medium, predict a maximum of 0.3-0.4 keV per particle of energy input, a result obtained by assuming that type Ia supernovae contribute 100% of their initial blast wave energy whereas type II supernovae contribute only by a few percents of their initial energy.
description: 29 pages, 7 figures, New Astronomy accepted
$q$-deformed 3D Loop Gravity on the Torus
Creators: name: Dupuis, Maïté
name: Livine, Etera R.
name: Pan, Qiaoyin
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The $q$-deformed loop gravity framework was introduced as a canonical formalism for the Turaev-Viro model (with $Λ< 0$), allowing to quantize 3D Euclidean gravity with a (negative) cosmological constant using a quantum deformation of the gauge group. We describe its application to the 2-torus, explicitly writing the $q$-deformed gauge symmetries and deriving the reduced physical phase space of Dirac observables, which leads back to the Goldman brackets for the moduli space of flat connections. Furthermore it turns out that the $q$-deformed loop gravity can be derived through a gauge fixing from the Fock-Rosly bracket, which provides an explicit link between loop quantum gravity (for $q$ real) and the combinatorial quantization of 3d gravity as a Chern-Simons theory with non-vanishing cosmological constant $Λ<0$. A side-product is the reformulation of the loop quantum gravity phase space for vanishing cosmological constant $Λ=0$, based on $\mathrm{SU}(2)$ holonomies and $\mathfrak{su}(2)$ fluxes, in terms of $\mathrm{ISU}(2)$ Poincaré holonomies. Although we focus on the case of the torus as an example, our results outline the general equivalence between 3D $q$-deformed loop quantum gravity and the combinatorial quantization of Chern-Simons theory for arbitrary graph and topology.
description: 26 pages, 12 figures
Discodermia du Bocage 1870
Creators: name: Schlacher-Hoenlinger, Monika A.
name: Pisera, Andrzej
name: Hooper, John N. A.
Publisher: name: Zenodo
Year: 2005
Subjects: Biodiversity
Taxonomy
Animalia
Porifera
Demospongiae
Tetractinellida
Theonellidae
Discodermia

description: Genus Discodermia du Bocage, 1870
 Discodermia du Bocage, 1870: 15, pl. 11: 1.
 TYPE SPECIES. — Dactylocalyx polydiscus Bowerbank, 1869 by subsequent designation (Pisera F Lévi 2002d).
DEFINITION. — Exclusively discotriaenes as ectosomal spicules and acanthoxeas and acanthorhabds as microscleres (Pisera F Lévi 2002d).
description: Published as part of Schlacher-Hoenlinger, Monika A., Pisera, Andrzej & Hooper, John N. A., 2005, Deep-sea " lithistid " assemblages from the Norfolk Ridge (New Caledonia), with description of seven new species and a new genus (Porifera, Demospongiae), pp. 649-698 in Zoosystema 27 (4) on page 681, DOI: 10.5281/zenodo.5393958
Geostiba (Sibiota) krzysztofi
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Geostiba
Geostiba krzysztofi

description: Geostiba (Sibiota) krzysztofi (ROUBAL 1913)
M a t e r i a l e x a m i n e d: Russia: 4 exs., Karatchay-Tcherkessia, Teberda (NMP, cAss).
 Geostiba krzysztofi has been recorded only from the type locality in Karatchay-Tcherkessia (Russia) (ASSING 2005a).
description: Published as part of Assing, V., 2009, A revision of Geostiba of the Western Palaearctic region. XIX. New species from Turkey and Iran and additional records, with an updated key and a catalogue of the species of the Eastern Mediterranean, the Caucasus, and adjacent regions (Coleoptera: Staphylinidae: Aleocharinae), pp. 1191-1246 in Linzer biologische Beiträge 41 (2) on page 1215, DOI: 10.5281/zenodo.5276563
Additional file 1 of Guild-based analysis for understanding gut microbiome in human health and diseases
Creators: name: Wu, Guojun
name: Zhao, Naisi
name: Zhang, Chenhong
name: Lam, Yan Y.
name: Zhao, Liping
Publisher: name: figshare
Year: 2021
Subjects: subject: Microbiology
subject: FOS: Biological sciences

description: Additional file 1: Supplementary Table 1. The abundance of individual Eubacterium eligens strains, and that of the species and guilds presented in Fig. 3. The data were reported as Mean (S.E.M).
Porifera Grant 1836
Creators: name: Gündoğdu, Sedat
name: Yeşilyurt, İrem Nur
name: Abbas, Zohaib
name: Baylan, Makbule
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy

description: 3.1.1. Porifera
Sponges are filter-feeding, sessile benthic organisms. They can take up MPs and other microparticles by filtering seawater, through placoderms, or via the influence of the fauna living within them (Girard et al., 2021; Soares et al., 2022). Studies on the effects of MPs on members of the phylum Porifera are limited. In the literature review conducted within the scope of this study, three relevant publications were found (Appendix Table 1).
In the Laguna de Terminos Protected Area, the MP content in sponges was found to be much higher than that in water and sediment (Celis-Hernandez et al., 2021). Sponges may be exposed to more contamination than other organisms as a result of ingesting very small particles, such as MPs with a predominant size of 10–20 µm or less than 2 µm (Fallon and Freeman, 2021; Krikech et al., 2023). In studies conducted in different regions, blue, red, and black microfibers were found in various sponge species, such as Haliclona implexiformis, Halichondria melanadocia, and Amorphinopsis atlantica in Mexico (Celis-Hernandez et al., 2021); PS was found in coral sponges Carteriospongia sp. and Ircinia sp. on Bangka Island, Indonesia (Girard et al., 2021); and PP was found in Cinachyrella alloclada in Brazil (Soares et al., 2022). In Antarctica, thermo fibers were detected in the sponges Dendrilla antarctica, Haliclona (Rhizoniera) scotti, Microxina sarai, and Mycale (Oxymycale) acerata, which provide the raw material for clothing worn by researchers, fishermen, and tourists in the region (Corti et al., 2023). In addition, sponges can be used as bioindicators to determine MP diversity in the environment due to their abilities of filtering large amounts of seawater daily and absorbing very small amounts of MPs present in the environment (Celis-Hernandez et al., 2021; Corti et al., 2023; Krikech et al., 2023).
description: Published as part of Gündoğdu, Sedat, Yeşilyurt, İrem Nur, Abbas, Zohaib & Baylan, Makbule, 2024, Effects of microplastics on aquatic organisms: a comprehensive review, pp. 248-285 in Turkish Journal of Zoology 48 (5) on page 251, DOI: 10.55730/1300-0179.3182, http://zenodo.org/record/14684319
Strong system-bath coupling induces negative differential thermal conductance and heat amplification in nonequilibrium two-qubits systems
Creators: name: Liu, Huan
name: Wang, Chen
name: Wang, Lu-Qing
name: Ren, Jie
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum heat transfer is analyzed in nonequilibrium two-qubits systems by applying the nonequilibrium polaron-transformed Redfield equation combined with full counting statistics. Steady state heat currents with weak and strong qubit-bath couplings are clearly unified. Within the two-terminal setup, the negative differential thermal conductance is unraveled with strong qubit-bath coupling and finite qubit splitting energy. The partially strong spin-boson interaction is sufficient to show the negative differential thermal conductance. Based on the three-terminal setup, that two-qubits are asymmetrically coupled to three thermal baths, a giant heat amplification factor is observed with strong qubit-bath coupling. Moreover, the strong interaction of either the left or right spin-boson coupling is able to exhibit the apparent heat amplification effect.
description: 12 pages, 11 figures, accepted by PRE
Semi-analytic approximations for production of atmospheric muons and neutrinos
Creators: name: Gaisser, Thomas K.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Simple approximations for fluxes of atmospheric muons and muon neutrinos are developed which display explicitly how the fluxes depend on primary cosmic ray energy and on features of pion production. For energies of approximately 10 GeV and above the results are sufficiently accurate to calculate response functions and to use for estimates of systematic uncertainties.
description: 15 pages with 8 figures
Geostiba (Typhlusida) flava
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Geostiba
Geostiba flava

description: Geostiba (Typhlusida) flava (KRAATZ 1856)
M a t e r i a l e x a m i n e d: Austria: 2 exs., Steiermark, Mixnitz, 22.VII.1903 (NMP, cAss); 4 exs., Steiermark, Graz env. (NMP); 2 exs., Steiermark, Turnau (NMP, cAss). Locality not specified: 3 exs., " Styria " (NMP).
The distribution of this species is confined to southeastern Austria and Slovenia. For more details see ASSING (2000c).
description: Published as part of Assing, V., 2009, A revision of Geostiba of the Western Palaearctic region. XIX. New species from Turkey and Iran and additional records, with an updated key and a catalogue of the species of the Eastern Mediterranean, the Caucasus, and adjacent regions (Coleoptera: Staphylinidae: Aleocharinae), pp. 1191-1246 in Linzer biologische Beiträge 41 (2) on page 1215, DOI: 10.5281/zenodo.5276563
title: Wie trägt die NIS2-Richtlinie zur digitalen Souveränität bei?
Creators: name: Kämpchen, Silas
Publisher: name: Gesellschaft für Informatik e.V.
Year: 2024
Subjects: subject: NIS2
subject: Richtlinie
subject: Europäische Union
subject: Cyber
subject: Sicherheit

description: Die NIS2-Richtlinie der Europäischen Union soll die digitale Souveränität stärken. Sie erweitert die ursprüngliche Richtlinie zur Netzwerk- und Informationssicherheit (NIS), erhöht die Cybersicherheitsstandards in der Union und umfasst nun eine breitere Palette an Sektoren und Unternehmen als in der ersten Version. Ein Schwerpunkt der Richtlinie liegt auf umfassendem Risikomanagement und auf der Verantwortlichkeit der Geschäftsleitung. Zudem fördert die Richtlinie die Harmonisierung der Sicherheitsstandards und den Informationsaustausch zwischen den Mitgliedstaaten. Diese Maßnahmen erhöhen die Widerstandsfähigkeit gegenüber Cyber-Bedrohungen und gestalten die digitale Zukunft Europas sicherer und souveräner.
Ameronothridae Norton & Franklin 2018
Creators: name: Norton, Roy A.
name: Franklin, Elizabeth
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Sarcoptiformes
Ameronothridae

description: What constitutes Ameronothridae?   In this confused context, we follow Pfingstl (2017) in recognizing the separate family Podacaridae (diagnosed by Grandjean 1955 and Wallwork 1964), thereby leaving Aquanothrus, Paraquanothrus, Ameronothrus and Chudalupia in Ameronothridae. A new diagnosis of this family concept—which is supported largely by the shared regression of pedotecta—is offered below. An excellent diagnosis of Ameronothrus can be found in Schubart (1975) and a brief one for Chudalupia in Wallwork (1981), but it should be corrected and emended by material in many of the following Remarks. In some respects, Chudalupia seems the most similar of these genera to Scapheremaeus: it has the deeply black, globular bothridial seta characteristic of most Scapheremaeus, and a strong tibia I apophysis, typical of Cymbaeremaeidae and Scutoverticidae but not found in other Ameronothridae. It has the acm -tubercle and apobasic setae but lacks the ascleritic notogastral band and the various leg setal regressions that link Scapheremaeus with Aquanothrus and Paraquanothrus.
 We also resurrect Engelbrecht’s (1975) family-group, originally proposed as Aquanothridae, but recognize it as the ameronothrid subfamily Aquanothrinae, which includes Aquanothrus and Paraquanothrus. In part, its resurrection highlights a distinct clade within a family that is not otherwise well-supported. But it is justified also by new knowledge of diversity, including our discovery of two North American species of Paraquanothrus and two unnamed African species of Aquanothrus, with probably others of each genus yet to be discovered. In a practical sense, recognition of the taxon will help prevent this small, but interesting group from being overlooked or subsumed when the evolution and systematics of ‘ameronothroid’ mites are discussed.
 Engelbrecht’s (1975) diagnosis of Aquanothridae was short and based on only A. montanus, the description of which had important errors and omissions, so we provide a new one for the subfamily. In both diagnoses, traits considered synapomorphies in the context of the respective taxon are underlined.
description: Published as part of Norton, Roy A. & Franklin, Elizabeth, 2018, Paraquanothrus n. gen. from freshwater rock pools in the USA, with new diagnoses of Aquanothrus, Aquanothrinae, and Ameronothridae (Acari, Oribatida), pp. 557-627 in Acarologia 58 (3) on page 603, DOI: 10.24349/acarologia/20184258, http://zenodo.org/record/5393919
A Tractable Algorithm For Finite-Horizon Continuous Reinforcement Learning
Creators: name: Gampa, Phanideep
name: Kondamudi, Sairam Satwik
name: Kailasam, Lakshmanan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Machine Learning (cs.LG)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: We consider the finite horizon continuous reinforcement learning problem. Our contribution is three-fold. First,we give a tractable algorithm based on optimistic value iteration for the problem. Next,we give a lower bound on regret of order $Ω(T^{2/3})$ for any algorithm discretizes the state space, improving the previous regret bound of $Ω(T^{1/2})$ of Ortner and Ryabko \cite{contrl} for the same problem. Next,under the assumption that the rewards and transitions are Hölder Continuous we show that the upper bound on the discretization error is $const.Ln^{-α}T$. Finally,we give some simple experiments to validate our propositions.
description: InProceedings of International Conference on Intelligent Autonomous System, ICOIAS 2019
Broad Emission Line Shifts in Quasars: An Orientation Measure for Radio-Quiet Quasars?
Creators: name: Richards, Gordon T.
name: Berk, Daniel E. Vanden
name: Reichard, Timothy A.
name: Hall, Patrick B.
name: Schneider, Donald P.
name: SubbaRao, Mark
name: Thakar, Anirudda R.
name: York, Donald G.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using a sample of 3814 quasars from the Sloan Digital Sky Survey, we confirm that high-ionization, broad, emission lines such as CIV are significantly blueshifted with respect to low-ionization, broad, emission lines such as MgII. CIV emission line peaks have a range of shifts from a redshift of 500 km/s to blueshifts well in excess of 2000 km/s as compared to MgII. We confirm previous results that suggest an anti-correlation between the shift of the CIV emission line peak and the rest equivalent width of the CIV emission line. Furthermore, using composite spectra, we are able to show that the apparent shift of the CIV emission line peak is not a shift so much as it is a lack of flux in the red wing for the composite with the largest apparent shift. This observation should strongly constrain models for the broad emission line region in quasars. The emission line blueshift and equivalent width of CIV are also discussed in light of the Baldwin Effect and as a function of other quasar properties such as spectral index, radio and X-ray detection. We find a possible correlation with both the radio and broad absorption line properties of the quasars that is suggestive of orientation as the cause of the CIV velocity shifts.
description: 37 pages, 11 figures (2 color), 2 tables. AJ in press. v2: Added some references and some minor corrections from the proofs
Geostiba (Sipalotricha) lucens
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Geostiba
Geostiba lucens

description: Geostiba (Sipalotricha) lucens (BENICK 1970)
 M a t e r i a l e x a m i n e d: Turkey: 4 exs., Sinop, 30 km NNE Boyabat, Dıranaz geç., 41°38'N, 34°52'E, calcareous grassland, under stones, 5.IV.2009, leg. Assing (cAss); 2 exs., Niğde, Demirkazık, 37°50'N, 35°06'E, 1900 m, under Berberis, 16.V.2009, leg. Meybohm (cAss); 1 ex., Niğde, Demirkazık, 37°51'N, 35°06'E, 1700 m, under Berberis, 16.V.2009, leg. Meybohm (cAss); 1 ex., Adana, Eyüplü, 37°57'N, 36°06'E, 1560 m, 17.IV.2009, leg. Brachat & Meybohm (cAss); 1 ex., Hatay, Kızıldağ, Madenli, 36°25'N, 36°07'E, 1120 m, 11.IV.2009, leg. Brachat & Meybohm (cAss).
 Geostiba lucens is one of the most widespread species of the genus in the Eastern Mediterranean, its distribution ranging from Turkey across the Balkans to southeastern Central Europe (ASSING 2005a); for a recent distribution map see ASSING (2006).
description: Published as part of Assing, V., 2009, A revision of Geostiba of the Western Palaearctic region. XIX. New species from Turkey and Iran and additional records, with an updated key and a catalogue of the species of the Eastern Mediterranean, the Caucasus, and adjacent regions (Coleoptera: Staphylinidae: Aleocharinae), pp. 1191-1246 in Linzer biologische Beiträge 41 (2) on page 1215, DOI: 10.5281/zenodo.5276563
title: Data Analytics as a Service – Challenges and Opportunities: An Introduction to DAS-24
Creators: name: Keller, Barbara
name: Möhring, Michael
name: Augenstein, Friedrich
Publisher: name: Gesellschaft für Informatik e.V.
Year: 2024
Subjects: subject: Data Analytics
subject: Service Management
subject: Industry
subject: Machine Learning
subject: AI

description: Data Analytics is an important topic in current and future services. Different opportunities and challenges occur when implementing it. The paper describes some core aspects of Data Analytics Services as well as concrete application domains. Furthermore, an overview of the workshop and specifics of Analytic Services as well as future research streams are provided.
The Pratyutpanna-buddha-sammukhavasthita-samadhi-sutra : an annotated English translation of the Tibetan version with several appendices
Creators: name: Harrison, Paul Maxwell
Publisher: name: The Australian National University
Year: 1979

description: The present work consists of a study of the Pratyutpanna-buddha-sammukhavasthita- samadhi-sutra (hereafter: PraS), a relatively early example of Mahayana Buddhist canonical literature. After a brief Introduction (pp. xxi-xli), which attempts to place the PraS in its historical context, the major portion of the work (pp. 1-186) is devoted to an annotated English translation of the Tibetan version of the sutra, with detailed reference to the three main Chinese translations. Appendix A (pp. 187-252) then attempts a resolution of some of the many problems surrounding the various Chinese versions of the PraS. These are examined both from the point of view of internal evidence and on the basis of bibliographical information furnished by the Chinese Buddhist scripture-catalogues. Some tentative conclusions are advanced concerning the textual history of the PraS in China. Appendix B (pp. 253-279) contains a study of the sole surviving fragment of the 'original’ Sanskrit text of the PraS. This fragment is edited, translated, and compared with the corresponding portions of the Chinese and Tibetan versions. Appendix C (pp. 280-327) consists of a Glossary of selected terms found in the PraS, and contains material drawn from all available translations of the work--the Tibetan, the three Chinese versions, and my own English rendering of the Tibetan--arranged according to Sanskrit equivalents and in Sanskrit alphabetical order. This Glossary is intended partly to act as an index to the text, and partly to facilitate further study of the Chinese translations.
Geostiba (Sipalotricha) infirma
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Geostiba
Geostiba infirma

description: Geostiba (Sipalotricha) infirma (WEISE 1878)
M a t e r i a l e x a m i n e d: Ukraine: 8 exs., Pozyzevska mt., 18.VI.1911, leg. Lokay (NMP, cAss); 3 exs., same data, but 11.IX.1911 (NMP); 7 exs., Chornohora, leg. Obenberger, etc. (NMP); 10 exs., Chornohora, 10.IX.1908 (NMP, cAss); 1 ex., Vorokhta, 30.VIII.1911, leg. Lokay (NMP); 2 exs., same data, but 12.XI.1911 (NMP); 6 exs., same data, but 20.VI.1911 (cAss); 8 exs., Hoverla, VII.1924, leg. Pfeffer (NMP, cAss); 5 exs., Hoverla, VI.1935, leg. Hlisnikowski (NMP); 9 exs., Hoverla, VI.1936, leg. Hlisnikowski (NMP, cAss); 1 ex., " Arendarski Potok ", 15.VI.1911, leg. Lokay (NMP); 1 ex., " Dolina ř. Pihy ", 9.VI.1911, leg. Lokay (NMP); 2 exs., Pop Ivan, leg. Fleischer (NMP). Romania: 1 ex., Munţii Rodna (NMP); 1 ex., "Alp. Transsylv.", leg. Lokay (NMP); 3 exs., "Siebenbg"/"Siebenbürgen" (NMP); 8 exs., "Koroniez" (NMP); 1 ex., "M. Koronjes", leg. Lokay (NMP); 4 exs., "Transsylv.", leg. Deubel (NMP, cAss). Locality not identified or not specified: 11 exs., "Jez. Samowite", 17.-19.VI.1911, leg. Lokay (NMP, cAss); 13 exs., "Karpaty" (NMP).
This species is endemic to the Carpathians, where it is widespread and common (ASSING 2005a).
description: Published as part of Assing, V., 2009, A revision of Geostiba of the Western Palaearctic region. XIX. New species from Turkey and Iran and additional records, with an updated key and a catalogue of the species of the Eastern Mediterranean, the Caucasus, and adjacent regions (Coleoptera: Staphylinidae: Aleocharinae), pp. 1191-1246 in Linzer biologische Beiträge 41 (2) on pages 1215-1216, DOI: 10.5281/zenodo.5276563
Two Slits Interference Is Compatible with Particles' Trajectories
Creators: name: Kisil, Vladimir V.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Quantum Physics (quant-ph)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: 81-01, 81-04

description: We propose a simple numerical experiment of two slits interference of particles. It disproves the popular belief that such an interference is incompatible with a knowledge which slit each particle came through or, more generally, ``quantum particles could not have trajectories''. Our model is an illustration to the contextual interpretation of quantum probabilities.
description: LaTeX2e, 12 pages, 4 PostScript figures, 1 program listing
title: Anomaly Detection in Supermarket Refrigeration Systems using Transformer Models: A Comparative Study
Creators: name: Meyer, Melina
name: Gergeleit, Martin
name: Krechel, Dirk
Publisher: name: Gesellschaft für Informatik e.V.
Year: 2024
Subjects: subject: Anomaly Detection
subject: Transformer
subject: Time Series Analysis
subject: Industrial Use Case

description: This study investigates anomaly detection methods in supermarket refrigeration systems. A transformer-based model is introduced in this field and compared with LSTM autoencoders. The models are trained and evaluated using preprocessed refrigeration data, with parameters optimized for accuracy, recall, precision, and F1 score. Our findings aim to enhance system monitoring and maintenance strategies, ultimately improving reliability, energy efficiency, and operational excellence in supermarket refrigeration technology.
The Contribution of Population III to the Enrichment and Preheating of the Intracluster Medium
Creators: name: Loewenstein, Michael
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Intracluster medium (ICM) abundances are higher than expected assuming enrichment by supernovae with progenitors belonging to the simple stellar population (SSP) observed in cluster galaxies, if stars formed with a standard initial mass function (IMF). Moreover, new results on ICM oxygen abundances imply that nucleosynthesis occurred with nonstandard yields. The hypothesis that hypernovae (HN) in general, and HN associated with Population III (Pop III) stars in particular, may significantly contribute to ICM enrichment is presented and evaluated. The observed abundance anomalies can be explained by a hypernovae-producing subpopulation of the SSP, but only if it accounts for half of all supernova explosions and if Type Ia supernova rates are very low. Also, the implied energy release may be excessive. However, an independent Pop III contribution -- in the form of metal-free, very massive stars that evolve into hypernovae -- can also account for all the observed abundances, while avoiding these drawbacks and accommodating a normal IMF in subsequent stellar generations. The required number of Pop III stars provides sufficient energy injection (at high redshift) to explain the ICM ``entropy floor''. Pop III hypernova pre-enrich the intergalactic medium, and can produce a significant fraction of the metals observed in the Lyman-alpha forest. Several testable predictions for ICM and IGM observations are made.
description: 15 pages Latex including 1 encapsulated postscript file; ApJ, in press
From Biological Synapses to Intelligent Robots
Creators: name: Dresp-Langley, Birgitta
Publisher: name: arXiv
Year: 2022
Subjects: subject: Robotics (cs.RO)
subject: Neural and Evolutionary Computing (cs.NE)
subject: FOS: Computer and information sciences

description: This review explores biologically inspired learning as a model for intelligent robot control and sensing technology on the basis of specific examples. Hebbian synaptic learning is discussed as a functionally relevant model for machine learning and intelligence, as explained on the basis of examples from the highly plastic biological neural networks of invertebrates and vertebrates. Its potential for adaptive learning and control without supervision, the generation of functional complexity, and control architectures based on self organization is brought forward. Learning without prior knowledge based on excitatory and inhibitory neural mechanisms accounts for the process through which survival or task relevant representations are either reinforced or suppressed. The basic mechanisms of unsupervised biological learning drive synaptic plasticity and adaptation for behavioral success in living brains with different levels of complexity. The insights collected here point toward the Hebbian model as a choice solution for intelligent robotics and sensor systems. Keywords: Hebbian learning, synaptic plasticity, neural networks, self organization, brain, reinforcement, sensory processing, robot control
Additional file 1 of Rethinking causal assumptions about maternal BMI, gestational weight gain, and adverse pregnancy outcomes
Creators: name: Dodd, Jodie M.
name: Louise, Jennie
name: Deussen, Andrea R.
name: Mitchell, Megan
name: Poston, Lucilla
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1: Supplementary Table 1. A Guideline to the Reporting of Mediation Analyses (AGReMA) Checklist.
Filtering solar-like oscillations for exoplanet detection in radial velocity observations
Creators: name: Chaplin, William J.
name: Cegla, Heather M.
name: Watson, Christopher A.
name: Davies, Guy R.
name: Ball, Warrick H.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Cool main-sequence, sub-giant and red-giant stars all show solar-like oscillations, pulsations that are excited and intrinsically damped by near-surface convection. Many overtones are typically excited to observable amplitudes, giving a rich spectrum of detectable modes. These modes provide a wealth of information on fundamental stellar properties. However, the radial velocity shifts induced by these oscillations can also be problematic when searching for low-mass, long-period planets; this is because their amplitudes are large enough to completely mask such minute planetary signals. Here we show how fine-tuning exposure times to the stellar parameters can help efficiently average out the solar-like-oscillation-induced shifts. To reduce the oscillation signal to the radial velocity precision commensurate with an Earth-analogue, we find that for cool, low-mass stars (near spectral type K) the necessary exposure times may be as short as 4 minutes, while for hotter, higher-mass stars (near spectral type F, or slightly evolved) the required exposure times can be longer than 100 minutes. We provide guideline exposure durations required to suppress the total observed amplitude due to oscillations to a level of $0.1\,\rm m\,s^{-1}$, and a level corresponding to the Earth-analogue reflex amplitude for the star. Owing to the intrinsic stochastic variability of the oscillations, we recommend in practice choosing short exposure durations at the telescope and then averaging over those exposures later, as guided by our predictions. To summarize, as we enter an era of $0.1\,\rm m\,s^{-1}$ instrumental precision, it is critical to tailor our observing strategies to the stellar properties.
description: 22 pages, 6 figures; accepted for publication in Astronomical Journal (AAS Journals)
Geostiba (Sipalotricha) cuneiformis
Creators: name: Assing, V.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Geostiba
Geostiba cuneiformis

description: Geostiba (Sipalotricha) cuneiformis (KRAATZ 1856)
M a t e r i a l e x a m i n e d: Slovakia: 8exs., Trenčin, leg. Duchon, etc. (NMP); 1 ex., Trenčin, VI.1921, leg. Hlisnikowski (cAss); 2 exs., VI.1919 (cAss); 2 exs., Trenčin, VIII.1921 (NMP). Locality not specified: 1 ex. (NMP).
 The known distribution of G. cuneiformis is confined to Slovakia and Hungary (ASSING 2005a).
description: Published as part of Assing, V., 2009, A revision of Geostiba of the Western Palaearctic region. XIX. New species from Turkey and Iran and additional records, with an updated key and a catalogue of the species of the Eastern Mediterranean, the Caucasus, and adjacent regions (Coleoptera: Staphylinidae: Aleocharinae), pp. 1191-1246 in Linzer biologische Beiträge 41 (2) on page 1216, DOI: 10.5281/zenodo.5276563
Are granules good tracers of solar surface velocity fields?
Creators: name: Rieutord, M.
name: Roudier, T.
name: Ludwig, H. -G.
name: Nordlund, A.
name: Stein, R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using a numerical simulation of compressible convection with radiative transfer mimicking the solar photosphere, we compare the velocity field derived from granule motions to the actual velocity field of the plasma. We thus test the idea that granules may be used to trace large-scale velocity fields at the sun's surface. Our results show that this is indeed the case provided the scale separation is sufficient. We thus estimate that neither velocity fields at scales less than 2500 km nor time evolution at scales shorter than 0.5 hr can be faithfully described by granules. At larger scales the granular motions correlate linearly with the underlying fluid motions with a slope of ~< 2 reaching correlation coefficients up to ~0.9.
description: 4 pages - accepted in Astronomy and Astrophysics
Additional file 1 of CCT6A facilitates lung adenocarcinoma progression and glycolysis via STAT1/HK2 axis
Creators: name: Yu, Shao-Kun
name: Yu, Tao
name: Wang, Yu-Ming
name: Sun, Ao
name: Liu, Jia
name: Lu, Kai-Hua
Publisher: name: figshare
Year: 2024
Subjects: Biophysics
Biochemistry
Medicine
Cell Biology
Molecular Biology
Biological Sciences not elsewhere classified
Cancer

description: Supplementary Material 1
Three-Dimensional Hydrodynamic Simulations of Accretion Tori in Kerr Spacetimes
Creators: name: De Villiers, Jean-Pierre
name: Hawley, John F.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This paper presents results of three-dimensional simulations of global hydrodynamic instabilities in black hole tori, extending earlier work by Hawley to Kerr spacetimes. This study probes a three-dimensional parameter space of torus angular momentum, torus size, and black hole angular momentum. We have observed the growth of the Papaloizou-Pringle instability for a range of torus configurations and the resultant formation of m=1 planets. We have also observed the quenching of this instability in the presence of early accretion flows; however, in one simulation both early accretion and planet formation occurred. Though most of the conclusions reached in Hawley's earlier work on Schwarzschild black holes carry over to Kerr spacetime, the presence of frame dragging in the Kerr geometry adds an element of complexity to the simulations; we have seen especially clear examples of this phenomenon in the accretion flows that arise from retrograde tori.
description: Accepted for publication in ApJ. 23 pages, 11 figures, animations available at http://www.astro.virginia.edu/~jd5v/h91redux/h91redux.html
Rapid UBVRI Follow-up of the Highly Collimated Optical Afterglow of GRB010222
Creators: name: Stanek, K. Z.
name: Garnavich, P. M.
name: Jha, S.
name: Kilgard, R. E.
name: McDowell, J. C.
name: Bersier, D.
name: Challis, P. M.
name: Falco, E.
name: Quinn, J. L.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (Abridged) We present the earliest optical observations of the optical counterpart to the GRB 010222, obtained with the FLWO 1.2-m telescope in UBVRI passbands, starting 3.64 hours after the burst. We also present late R-band observations of the afterglow obtained with the 1.8-m VATT ~25 days after the burst. The temporal analysis of our data joined with published data indicates a steepening decay, independent of wavelength, asymptotically approaching t^{-0.80+/-0.05} at early times (t << 1 day) and t^{-1.30+/-0.05} at late times, with a sharp break at t_b=0.72+/-0.1 days. This is the second earliest observed break of any afterglow (after GRB 980519), which clearly indicates the importance of rapid multi-band follow-up for GRB afterglow research. The optical spectral energy distribution, corrected for small Galactic reddening, can be fit fairly well by a single power-law with a slope of -1.07+/-0.09. However, when we fit using our BVRI data only, we obtain a shallower slope of -0.88+/- 0.1, in excellent agreement with the slope derived from our low-resolution spectrum (-0.89 +/- 0.03). The spectral slope and light curve decay slopes we derive are not consistent with a jet model despite the presence of a temporal break. Significant host dust extinction with a star-burst reddening law would flatten the spectral index to match jet predictions and still be consistent with the observed spectral energy distribution. We derive an opening angle of 2.1 deg, smaller than any listed in the recent compilation of Frail et al. The total beamed energy corrected for the jet geometry is 4x10^50 erg, very close to the ``standard'' value of 5x10^50 erg found by Frail et al. for a number of other bursts with light-curve breaks.
description: revised version (minor changes only) to be published in the ApJ Part 1, 12 pages, 4 figures; all data used for the fits and our CCD frames available at ftp://cfa-ftp.harvard.edu/pub/kstanek/GRB010222/ and through WWW at http://cfa-www.harvard.edu/cfa/oir/Research/GRB/
Monstera oreophila , Madison 1977
Creators: name: Cedeño-Fonseca, Marco
name: Ortiz, Orlando O.
name: Zuluaga, Alejandro
name: Croat, Thomas B.
name: Blanco, Mario A.
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Alismatales
Araceae
Monstera
Monstera oreophila

description: Key to the species of the Monstera oreophila complex
 1a. Spathe pale pink internally, not becoming torn at the base nor reflexed when open; petioles smooth...................... M. mittermeieri
1b. Spathe dark pink or salmon-pink internally; petioles smooth or warty.
 2a. Petioles smooth, light green, with persistent sheaths; spathe up to 10 cm longer than the spadix, apparently erect and persistent after anthesis (but frequently herbivorized)................................................................................................................................. M. gentryi
 2b. Petioles smooth or warty, dark green, with deciduous sheaths; spathe up to 4 cm longer than the spadix, becoming torn at the base and reflexed when open and soon deciduous after anthesis........................................................................................... M. oreophila
description: Published as part of Cedeño-Fonseca, Marco, Ortiz, Orlando O., Zuluaga, Alejandro, Croat, Thomas B. & Blanco, Mario A., 2021, A reexamination of Monstera oreophila (Araceae: Monsteroideae) and description of two new pinkish-spathed species of Monstera from Costa Rica and Panama, pp. 205-220 in Phytotaxa 514 (3) on page 219, DOI: 10.11646/phytotaxa.514.3.2, http://zenodo.org/record/5315985