cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Geometry of the Uniform Spanning Forest: Transitions in Dimensions 4, 8, 12
Creators: name: Benjamini, Itai
name: Kesten, Harry
name: Peres, Yuval
name: Schramm, Oded
Publisher: name: arXiv
Year: 2001
Subjects: subject: Probability (math.PR)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 60K35; 60J15

description: The uniform spanning forest (USF) in Z^d is the weak limit of random, uniformly chosen, spanning trees in [-n,n]^d. Pemantle proved that the USF consists a.s. of a single tree if and only if d <= 4. We prove that any two components of the USF in Z^d are adjacent a.s. if 5 <= d <= 8, but not if d >= 9. More generally, let N(x,y) be the minimum number of edges outside the USF in a path joining x and y in Z^d. Then a.s. max{N(x,y) : x,y in Z^d} is the integer part of (d-1)/4. The notion of stochastic dimension for random relations in the lattice is introduced and used in the proof.
description: Current version: added some comments regarding related problems and implications, and made some corrections
A Review of Testing Object-Based Environment Perception for Safe Automated Driving
Creators: name: Hoss, Michael
name: Scholtes, Maike
name: Eckstein, Lutz
Publisher: name: arXiv
Year: 2021
Subjects: subject: Robotics (cs.RO)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Systems and Control (eess.SY)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Safety assurance of automated driving systems must consider uncertain environment perception. This paper reviews literature addressing how perception testing is realized as part of safety assurance. We focus on testing for verification and validation purposes at the interface between perception and planning, and structure our analysis along the three axes 1) test criteria and metrics, 2) test scenarios, and 3) reference data. Furthermore, the analyzed literature includes related safety standards, safety-independent perception algorithm benchmarking, and sensor modeling. We find that the realization of safety-aware perception testing remains an open issue since challenges concerning the three testing axes and their interdependencies currently do not appear to be sufficiently solved.
description: 23 pages, 7 figures. Automotive Innovation (2022)
Structure of Dyadic Social Situations - Validation Study 2
Creators: name: Sudeep Bhatia
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Physical Sciences and Mathematics
subject: Personality and Social Contexts
subject: Social Psychology
subject: Computer Sciences
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology
subject: Artificial Intelligence and Robotics

description: Validation study to examine the coding accuracy of GPT-4
Castnius Hubner 1819
Creators: name: Moraes, Simeão De Souza
name: Duarte, Marcelo
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Castniidae
Castnius

description: CASTNIUS HÜBNER, [1819] (FIGS 5, 6)
 Type species
 Papilio pelasgus Cramer, [1779]
 Included species
 Castnius pelasgus (Cramer, [1779]), Castnius marcus (Jordan, 1908), and C. asteropoides Porion, 2004.
 Comments
 Two synapomorphic characters, the sacculus as an anterior projection (47: 1) and rectangular (48: 3), plus the homoplastic characters related to wing venation and morphology of the aedeagus and valva, support the arrangement of this genus. We must note, however, that C. asteropoides was not included in the analysis.
description: Published as part of Moraes, Simeão De Souza & Duarte, Marcelo, 2014, Phylogeny of Neotropical Castniinae (Lepidoptera: Cossoidea: Castniidae): testing the hypothesis of the mimics as a monophyletic group and implications for the arrangement of the genera, pp. 362-399 in Zoological Journal of the Linnean Society 170 (2) on page 391, DOI: 10.1111/zoj.12102, http://zenodo.org/record/5302314
Almost contact manifolds, connections with torsion and parallel spinors
Creators: name: Friedrich, Thomas
name: Ivanov, Stefan
Publisher: name: arXiv
Year: 2001
Subjects: subject: Differential Geometry (math.DG)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 53C25, 53C27, 53C55, 81T30

description: We classify locally homogeneous quasi-Sasakian manifolds in dimension five that admit a parallel spinor $ψ$ of algebraic type $F \cdot ψ= 0$ with respect to the unique connection $\nabla$ preserving the quasi-Sasakian structure and with totally skew-symmetric torsion. We introduce a certain conformal transformation of almost contact metric manifolds and discuss a link between them and the dilation function in 5-dimensional string theory. We find natural conditions implying conformal invariances of parallel spinors. We present topological obstructions to the existence of parallel spinors in the compact case.
description: Latex2e, 15 pages; Final version of the paper, the preliminary title has been "Almost contact manifolds and type II equations"
Anisonema trepidum Larsen 1987
Creators: name: Lee, Won Je
name: Patterson, David J.
Publisher: name: Zenodo
Year: 2000
Subjects: Biodiversity
Taxonomy
Protozoa
Euglenozoa
Euglenoidea
Peranemida
Peranemaceae
Anisonema
Anisonema trepidum

description: Anisonema trepidum Larsen, 1987
(fi gures 3b, 4h, i)
 Description. Cell pro fi le oblong, 13-19 Mm long, 6.5-10 Mm wide, fl attened. With three distinct grooves on the dorsal and ventral faces. Two emergent fl agella are of unequal length. The anterior fl agellum is approximately 1.5 times the cell length, and the trailing posterior fl agellum is stronger than the anterior fl agellum, is approximately 3.5-5 times the cell length and tapers distally. The fl agellar pocket and nucleus are in the left side of the cell. Cells contained small granules. The cells glide quickly and jerk when changing direction. Rarely observed.
 Remarks. Cell length was previously reported to be 9-20 Mm and this species was found in marine sites in tropical Australia, Brazil, Danish Wadden Sea, Fiji and Hawaii (Larsen, 1987; Larsen and Patterson, 1990; Ekebom et al., 1996). Generally, our observations of the appearance of this species agree with those of Larsen and Patterson (1990), but we did not observe the arrests which Larsen and Patterson felt helped to distinguish this species. Anisonema trepidum is distinguished from A. acinus Dujardin, 1841 by its smaller size, cell shape and its behaviour. Anisonema glaciale Larsen and Patterson, 1990 has the same movement as A. trepidium, but can be distinguished by its larger size.
description: Published as part of Lee, Won Je & Patterson, David J., 2000, Heterotrophic flagellates (Protista) from marine sediments of Botany Bay, Australia, pp. 483-562 in Journal of Natural History 34 on pages 495-496
The Hubbard model on a triangular lattice -- pseudogap due to spin-density-wave fluctuations
Creators: name: Ye, Mengxing
name: Chubukov, Andrey V.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We calculate the fermionic spectral function $A_k (ω)$ in the spiral spin-density-wave (SDW) state of the Hubbard model on a quasi-2D triangular lattice at small but finite temperature $T$. The spiral SDW order $Δ(T)$ develops below $T = T_N$ and has momentum ${ \bf K} = (4π/3,0)$. We pay special attention to fermions with momenta ${\bf k}$, for which ${\bf k}$ and ${\bf k} + {\bf K}$ are close to Fermi surface in the absence of SDW. At the mean field level, $A_k (ω)$ for such fermions has peaks at $ω= \pm Δ(T)$ at $T < T_N$ and displays a conventional Fermi liquid behavior at $T > T_N$. We show that this behavior changes qualitatively beyond mean-field due to singular self-energy contributions from thermal fluctuations in a quasi-2D system. We use a non-perturbative eikonal approach and sum up infinite series of thermal self-energy terms. We show that $A_k (ω)$ shows peak/dip/hump features at $T < T_N$, with the peak position at $Δ(T)$ and hump position at $Δ(T=0)$. Above $T_N$, the hump survives up to $T = T_p > T_N$, and in between $T_N$ and $T_p$ the spectral function displays the pseudogap behavior. We show that the difference between $T_p$ and $T_N$ is controlled by the ratio of in-plane and out-of-plane static spin susceptibilities, which determines the combinatoric factors in the diagrammatic series for the self-energy. For certain values of this ratio, $T_p = T_N$, i.e., the pseudogap region collapses. In this last case, thermal fluctuations are logarithmically singular, yet they do not give rise to pseudogap behavior. Our computational method can be used to study pseudogap physics due to thermal fluctuations in other systems.
description: 13+7 pages, 11 figures
CMB Comptonization by Energetic Nonthermal Electrons in Clusters of Galaxies
Creators: name: Shimon, Meir
name: Rephaeli, Yoel
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Use of the Sunyaev-Zeldovich effect as a precise cosmological probe necessitates a realistic assessment of all possible contributions to Comptonization of the cosmic microwave background in clusters of galaxies. We have calculated the additional intensity change due to various possible populations of energetic electrons that have been proposed in order to account for measurements of intracluster radio, nonthermal X-ray and (possibly also) EUV emission. Our properly normalized estimates of (the highly model dependent value of) the predicted intensity change due to these electrons is well below $\sim 6%$ and $\sim 35%$ of the usual Sunyaev-Zeldovich effect due to electrons in the hot gas in Coma and A2199, respectively. These levels constitute high upper limits since they are based on energetic electron populations whose energy densities are {\it comparable} to those of the thermal gas. The main impact of nonthermal Comptonization is a shift of the crossover frequency (where the thermal effect vanishes) to higher values. Such a shift would have important consequences for our ability to measure cluster peculiar velocities from the kinematic component of the Sunyaev-Zeldovich effect.
description: 15 pages, 2 figures
Additional file 1: of What Egyptians think. Knowledge, attitude, and opinions of Egyptian patients towards biobanking issues
Creators: name: Abdelhafiz, Ahmed
name: Sultan, Eman
name: Ziady, Hany
name: Ebtesam Ahmed
name: Walaa Khairy
name: Douaa Sayed
name: Zaki, Rana
name: Merhan Fouda
name: Labib, Rania
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Table S1. Correlation between knowledge about biobanks and sociodemographic data of studied patients (n = 259). Table S2. Attitude towards sample donation to biobanks in relation to sociodemographic data and knowledge of studied patients about the term “Bioabank” (n = 259). Table S3. Opinions of studied patients regarding the benefits and obstacles of sample donation (n = 259). (DOCX 26 kb)
The concordance genus of knots
Creators: name: Livingston, Charles
Publisher: name: arXiv
Year: 2001
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 57M25, 57N70

description: In knot concordance three genera arise naturally, g(K), g_4(K), and g_c(K): these are the classical genus, the 4-ball genus, and the concordance genus, defined to be the minimum genus among all knots concordant to K. Clearly 0 <= g_4(K) <= g_c(K) <= g(K). Casson and Nakanishi gave examples to show that g_4(K) need not equal g_c(K). We begin by reviewing and extending their results. For knots representing elements in A, the concordance group of algebraically slice knots, the relationships between these genera are less clear. Casson and Gordon's result that A is nontrivial implies that g_4(K) can be nonzero for knots in A. Gilmer proved that g_4(K) can be arbitrarily large for knots in A. We will prove that there are knots K in A with g_4(K) = 1 and g_c(K) arbitrarily large. Finally, we tabulate g_c for all prime knots with 10 crossings and, with two exceptions, all prime knots with fewer than 10 crossings. This requires the description of previously unnoticed concordances.
description: Published by Algebraic and Geometric Topology at http://www.maths.warwick.ac.uk/agt/AGTVol4/agt-4-1.abs.html
Corybantes Hubner 1819
Creators: name: Moraes, Simeão De Souza
name: Duarte, Marcelo
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Castniidae
Corybantes

description: CORYBANTES HÜBNER, [1819] (FIG. 8)
 Type species
 Papilio pylades Stoll, 1782
 Included species
 Corybantes pylades (Stoll, 1782), Corybantes veraguana (Westwood, 1877), Corybantes mathani (Oberthür, 1881), and Corybantes dolopia (Druce, 1907).
 Comments
The two species included in our analysis share some morphological traits concerning the arrangement of the cornuti (39: 2), which supports the monophyly of the genus. Certain homoplastic characters such as the incomplete contortion of the aedeagus (26: 0), morphology of the saccus (73: 1) and (87: 2), and morphology of the gnathos (79: 2) and (81: 0) are diagnostic characters.
description: Published as part of Moraes, Simeão De Souza & Duarte, Marcelo, 2014, Phylogeny of Neotropical Castniinae (Lepidoptera: Cossoidea: Castniidae): testing the hypothesis of the mimics as a monophyletic group and implications for the arrangement of the genera, pp. 362-399 in Zoological Journal of the Linnean Society 170 (2) on page 391, DOI: 10.1111/zoj.12102, http://zenodo.org/record/5302314
Development of the present moment awareness rating scale to assess change after mindfulness-based interventions
Creators: name: Azam, Muhammad Abid
name: Latman, Vered
name: Katz, Joel
Publisher: name: F1000 Research Limited
Year: 2019

description: Present moment awareness is the central goal of mindfulness practices (Kabat‐Zinn, 2003). Mindfulness-based interventions (MBI) aim to entrain a quality of attention that involves paying nonjudmental attention to one’s cognitive, emotional, and physical experiences and continously shifting attention back to present experiences (Black, 2011). Clinical populations undergoing MBI’s have demonstrated improvements in health, cognitive, affective, and interpersonal outcomes (Creswell, 2017). Greater capacity to attend to present moment experiences is purported to be an underlying mechanism for these clinical improvements, but there is a dearth of research in this area. While there are inventories designed to measure the construct and components of mindfulness, such as the Toronto Mindfulness Scale (Lau et al., 2006) and the Five Factor Mindfulness Questionnaire (Baer et al., 2008), there is a lack of validated and brief self-report inventories that isolate and assess the construct of present moment awareness in the clinical context. The current project aims to develop the Present Moment Awareness Rating Scale (PMARS) for use in experimental studies, and eventually, in clinical evaluations of MBI’s.
Eupalamides Hubner 1819
Creators: name: Moraes, Simeão De Souza
name: Duarte, Marcelo
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Castniidae
Eupalamides

description: EUPALAMIDES HÜBNER, [1819] (FIG. 7)
 Type species
 Papilio cyparissias Fabricius, 1776
 Included species
 Eupalamides cyparissias (Fabricius, 1776), Eupalamides geron (Kollar, 1839), Eupalamides preissi (Staudinger, 1899), Eupalamides guyanensis (Houlbert, 1917), and Eupalamides boliviensis (Houlbert, 1917).
 Comments
 Only E. cyparissias (Fig. 7) was included in our analysis. This species shares with the genus Castnius characters related to wing venation, aedeagus, and saccus. Several homoplastic characters define the species; however, because only one species of the genus was examined, these characters may also be diagnostic for the species, and for this reason they were not included here. We maintain the validity of the genus and its composition as given by Lamas (1995).
description: Published as part of Moraes, Simeão De Souza & Duarte, Marcelo, 2014, Phylogeny of Neotropical Castniinae (Lepidoptera: Cossoidea: Castniidae): testing the hypothesis of the mimics as a monophyletic group and implications for the arrangement of the genera, pp. 362-399 in Zoological Journal of the Linnean Society 170 (2) on page 391, DOI: 10.1111/zoj.12102, http://zenodo.org/record/5302314
title: Unseating the Israeli Government from the UN General Assembly in case of non-compliance with the Advisory Opinion of 19 July 2024
Creators: name: Jamshidi, Maryam
Publisher: name: Fachinformationsdienst für internationale und interdisziplinäre Rechtsforschung
Year: 2024
Subjects: subject: 342

description: Verfassungsblog: On Matters Constitutional
Transcranial Direct Current Stimulation and Decision-Making: The Neuromodulation of Cognitive Reflection
Creators: name: Edgcumbe, Daniel
Publisher: name: University of East London
Year: 2018

description: The ability to make judgements and decisions is crucial to our lives. The dual-process framework of judgement and decision-making (e.g. Stanovich, 2009) proposes that decisions are usually made using mental processes relying on automatic processes (called Type 1 processing) or on more controlled processes (called Type 2 processing). According to this theory, when we make a decision without conscious effort we rely on the autonomous processes of Type 1 intuitive thinking, which is prone towards errorful decision-making. Alternatively, if we use Type 2 thinking by committing cognitive resources (e.g., working memory) we engage analytic thinking by at least partly inhibiting Type 1 processing. The primary goal for this thesis is to test whether Type 1 versus Type 2 processes in decision-making can be linked to different neural substrates. Transcranial direct current stimulation (tDCS), a non-invasive method for enhancing or decreasing cortical excitability was used. Participants completed decision-making tasks (e.g., Cognitive Reflection Test (CRT), syllogistic reasoning) to capture performance indicating Type 1 or Type 2 processing, and executive function tasks to assess the basis of Type 1 and Type 2 processing. First, a meta-analysis was performed on a variety of experiments using tDCS, finding evidence for the involvement of frontal structures in judgement and decision-making. In subsequent experiments stimulation of the right but not left dorsolateral prefrontal cortex (DLPFC) with anodal tDCS increased performance compared to sham in the CRT and solving vignettes measuring heuristic thinking. In experiment three there was a cumulative effect of neuromodulation on Type 2 processing, with an increase in reflective thinking performance following each of two stimulation sessions. Individual differences in thinking dispositions and cognitive ability could not explain the results, and there were no performance-enhancing effects of stimulation on syllogisms or executive functions. These experiments provide evidence for the involvement of the right DLPFC in decision-making which relies on the inhibition of pre-potent responses (e.g., the CRT).
The environment of HI-bearing ultra diffuse galaxies in the ALFALFA survey
Creators: name: Janowiecki, Steven
name: Jones, Michael G.
name: Leisman, Lukas
name: Webb, Andrew
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We explore the environment of 252 HI-bearing Ultra Diffuse Galaxies (HUDs) from the 100% ALFALFA survey catalog in an attempt to constrain their formation mechanism. We select sources from ALFALFA with surface brightnesses, magnitudes, and radii consistent with other samples of Ultra Diffuse Galaxies (UDGs), without restrictions on their isolation or environment, more than doubling the previously reported ALFALFA sample. We quantify the galactic environment of HUDs using several metrics, including n-th nearest neighbour, tidal influence, membership in a group/cluster, and distance from nearest group/cluster or filament. We find that that HUDs inhabit the same environments as other samples of HI-selected galaxies and that they show no environmental preference in any metric. We suggest that these results are consistent with a picture of the extreme properties of HUDs being driven by internal mechanisms and that they are largely unperturbed by environmental impacts. While environmental effects may be necessary to convert HUDs into gas-poor cluster UDGs, these effects are not required for diffuse galaxies to exist in the first place.
description: 12 pages (with online-only catalog of sources), accepted to MNRAS
Structure of $A(\infty)$-algebra and Hochschild and Harrison cohomology
Creators: name: Kadeishvili, Tornike
Publisher: name: arXiv
Year: 2002
Subjects: subject: Algebraic Topology (math.AT)
subject: FOS: Mathematics
subject: 55S30, 55S35, 16E40

description: Stasheff's $A(\infty)$-algebra $(M,\{m_i:\otimes^iM\to M, i=1,2,3,...\})$ in fact is a DG-algebra $(M,m_1,m_2)$ with not necessarily associative product $m_2$ but this nonassociativity is measured by higher homotopies $m_{i>2}$. Nevertheless such structure arises in the strictly associative situation too, namely in the homology algebra $H(C)$ of a DG-algebra $C$ with free $H_i(C)$-s, particularly in the cohomology algebra $H^*(X,Λ)$ of a topological space $X$. It is clear that the $A(\infty)$-algebra $(H^*(X,Λ),\{m_i\})$ carries more information than the cohomology algebra $H^*(B,Λ)$. Naturally arises a question when this structure is degenerate, that is when an $A(\infty)$-algebra $(M, \{m_i\})$ is isomorphic to one with higher operations $m_i, i\geq 3$ trivial? In this paper we introduce the obstructions for such degeneracy. Namely, operations $\{m_i\}$ we interpret as Hochschild twisting cochain $m=m_3+m_4+..., m_i\in C^n(M,M)$ satisfying $δm=m\smile_1m$ where $\smile_1$ is Gerstenhabers product in $C^*(M,M)$. Using the generalized product $f\smile_1(g_1,...,g_k)$ we define perturbations of Hochschild twisting cochains (i.e. of $A(\infty)$ structures) and in particular prove that if for a graded algebra $(M,μ)$ all Hochschild cohomologies $Hoch^{n,2-n}(M,M)=0$ for $n\geq3$ then any $A(\infty)$-algebra structure $\{m_i\}$ on $M$ with $m_1=0, m_2=μ$, is degenerate.
Faster-than-light effects and negative group delays in optics and electronics, and their applications
Creators: name: Chiao, Raymond Y.
name: Hickmann, Jandir M.
name: Solli, Daniel
Publisher: name: arXiv
Year: 2001
Subjects: subject: Performance (cs.PF)
subject: FOS: Computer and information sciences
subject: B.7.0

description: Recent manifestations of apparently faster-than-light effects confirmed our predictions that the group velocity in transparent optical media can exceed c. Special relativity is not violated by these phenomena. Moreover, in the electronic domain, the causality principle does not forbid negative group delays of analytic signals in electronic circuits, in which the peak of an output pulse leaves the exit port of a circuit before the peak of the input pulse enters the input port. Furthermore, pulse distortion for these superluminal analytic signals can be negligible in both the optical and electronic domains. Here we suggest an extension of these ideas to the microelectronic domain. The underlying principle is that negative feedback can be used to produce negative group delays. Such negative group delays can be used to cancel out the positive group delays due to transistor latency (e.g., the finite RC rise time of MOSFETS caused by their intrinsic gate capacitance), as well as the propagation delays due to the interconnects between transistors. Using this principle, it is possible to speed up computer systems.
description: 13 pages, 5 figures, 2001 Photonic West Plenary Talk
Kinematics of $z\geq 6$ galaxies from [CII] line emission
Creators: name: Kohandel, M.
name: Pallottini, A.
name: Ferrara, A.
name: Zanella, A.
name: Behrens, C.
name: Carniani, S.
name: Gallerani, S.
name: Vallini, L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study the kinematical properties of galaxies in the Epoch of Reionization via the [CII] 158$μ$m line emission. The line profile provides information on the kinematics as well as structural properties such as the presence of a disk and satellites. To understand how these properties are encoded in the line profile, first we develop analytical models from which we identify disk inclination and gas turbulent motions as the key parameters affecting the line profile. To gain further insights, we use "Althaea", a highly-resolved ($30\, \rm pc$) simulated prototypical Lyman Break Galaxy, in the redshift range $z = 6-7$, when the galaxy is in a very active assembling phase. Based on morphology, we select three main dynamical stages: I) Merger , II) Spiral Disk, and III) Disturbed Disk. We identify spectral signatures of merger events, spiral arms, and extra-planar flows in I), II), and III), respectively. We derive a generalised dynamical mass vs. [CII]-line FWHM relation. If precise information on the galaxy inclination is (not) available, the returned mass estimate is accurate within a factor $2$ ($4$). A Tully-Fisher relation is found for the observed high-$z$ galaxies, i.e. $L_{\rm[CII]}\propto (FWHM)^{1.80\pm 0.35}$ for which we provide a simple, physically-based interpretation. Finally, we perform mock ALMA simulations to check the detectability of [CII]. When seen face-on, Althaea is always detected at $> 5σ$; in the edge-on case it remains undetected because the larger intrinsic FWHM pushes the line peak flux below detection limit. This suggests that some of the reported non-detections might be due to inclination effects.
description: 14 pages, 12 figures, accepted for publication in MNRAS
Magnetic Activity of the Cool Companion in Symbiotic Systems
Creators: name: Soker, Noam
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I argue that cool giant companions in most symbiotic binary systems possess magnetic activity on a much higher level than isolated, or in wide binary systems, cool giants. Based on the behavior of main sequence stars, I assume that magnetic activity and X-ray luminosity increase with rotation velocity. I then show that the cool companions in symbiotic systems are likely to rotate much faster than isolated, or in wide binary systems, cool giants. The magnetic activity of the cool giant may be observed as a global axisymmetrical mass loss geometry from the cool giant (before the hot companion influences the outflow), a stochastic mass loss process, i.e., variation of mass loss rate with time and location on the giant's surface, and in relatively strong X-ray emission. The variation in the mass loss process from the cool giant may cause variation in the properties of jets blown by the hot compact companion. I conclude that symbiotic systems should be high-priority X-ray targets.
description: MNRAS, submitted; 10 pages
Features visualization of InceptionV1 models
Creators: name: Gonthier, Nicolas
Publisher: name: Zenodo
Year: 2020
Subjects: Feature Visualization
Convolutional Neural Network
Fine-Tuning
Art Analysis

description: This archive contains the weights of the InceptionV1 architecture pre-trained on ImageNet (InceptionV1_fromLucid.h5
 ) and the same model fine-tuned on the artistic dataset RASTA (namely InceptionV1_RASTA__SGD_lrp0.1_lr0.01_avgpool_CropC ..). In the data folder the feature visualization of most of the layers of those two models can be found. These data are introduced in the following work : "An Analysis of the Transfer Learning of Convolutional Neural Networks for Artistic Images" Gonthier et al. 2020 Pattern Recognition. ICPR International Workshops and Challenges
description: This research was supported in part by the "IDI 2017" project funded by the IDEX Paris-Saclay, ANR-11-IDEX-0003-02.
description: {"references": ["\"An Analysis of the Transfer Learning of Convolutional Neural Networks for Artistic Images\" Gonthier et al. 2020 Pattern Recognition. ICPR International Workshops and Challenges"]}
Comparing IMF-sensitive indices of intermediate-mass quiescent galaxies in various environments
Creators: name: Eftekhari, Elham
name: Mosleh, Moein
name: Vazdekis, Alexandre
name: Tavasoli, Saeed
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Using samples drawn from the Sloan Digital Sky Survey, we study for the first time the relation between large-scale environments (Clusters, Groups and Voids) and the stellar Initial Mass Function (IMF). We perform an observational approach based on the comparison of IMF-sensitive indices of quiescent galaxies with similar mass in varying environments. These galaxies are selected within a narrow redshift interval ($ 0.020 < z < 0.055 $) and spanning a range in velocity dispersion from 100 to 200 kms$^{-1}$. The results of this paper are based upon analysis of composite spectra created by stacking the spectra of galaxies, binned by their velocity dispersion and redshift. The trends of spectral indices as measured from the stacked spectra, with respect to velocity dispersion, are compared in different environments. We find a lack of dependence of the IMF on the environment for intermediate-mass galaxy regime. We verify this finding by providing a more quantitative measurement of the IMF variations among galactic environments using MILES stellar population models with a precision of $ΔΓ_{b}\sim0.2$.
description: Accepted for publication in MNRAS
MPEC 2024-C151 : 2024 CZ3
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 CZ3

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Dinema validum Larsen and Patterson 1990
Creators: name: Lee, Won Je
name: Patterson, David J.
Publisher: name: Zenodo
Year: 2000
Subjects: Biodiversity
Taxonomy
Protozoa
Euglenozoa
Peranemea
Peranemida
Peranemaceae
Dinema
Dinema validum

description: Dinema validum Larsen and Patterson, 1990
(fi gures 3d, 5h, i)
 Description. Cell outline oblong to ovate, 32-53 Mm long, 22-27 Mm wide, with slightly thickened pellicle. About 16 wide longitudinal striations occur on both faces of the cell and slightly follow a S-helix. Dorsal striations are more distinct than ventral ones. The anterior fl agellum is as long as the cell and beats with a sweeping motion. The posterior fl agellum is approximately 3 times the cell length, is thicker than the anterior fl agellum and emerges as a hook from the fl agellar pocket which is in the left-hand side of the cell. The ingestion apparatus has two rods but may be di ffi cult to see. It extends halfway down the cell. This species consumed diatoms as long as 16 Mm. The nucleus is usually in the right posterior end of the cell but may be in the left-hand side. Moves by gliding and may undergo squirming movements. When changing direction, cells jerk backwards and then continue to move forward. Three cells observed.
 Remarks. This species was previously reported from marine sites in subtropical and tropical Australia, Brazil and Fiji, with reported cell lengths from 26 to 38 Mm (Larsen and Patterson, 1990; Ekebom et al., 1996; Patterson and Simpson, 1996). Although one of our cells was slightly pointed at both ends and the ingestion apparatus was hard to see, and was very much larger than the previously reported sizes, we assigned the cell to D. validum because of slightly thickened pellicle, hooked posterior fl agellum and squirming movements. One cell observed had its nucleus in the left-hand side of the cell, thus we suspect that the position of a nucleus is not a good diagnostic character. This species is distinguished from other species of the genus Dinema by its wide pellicular striations and the thickness of the recurrent fl agellum; it is distinguished from D. litorale Skuja, 1939 by the smaller number of pellicular striations.
description: Published as part of Lee, Won Je & Patterson, David J., 2000, Heterotrophic flagellates (Protista) from marine sediments of Botany Bay, Australia, pp. 483-562 in Journal of Natural History 34 on page 498
Palmira: A Deep Deformable Network for Instance Segmentation of Dense and Uneven Layouts in Handwritten Manuscripts
Creators: name: Sharan, S P
name: Aitha, Sowmya
name: Trivedi, Abhishek
name: Augustine, Aaron
name: Kumar, Amandeep
Publisher: name: Zenodo
Year: 2021

description: The weights file corresponding to the Palmira model trained on Indiscapes2
Az integráció-szegregáció helyzete egy kutatás tükrében
Creators: name: Laoues-Czimbalmos, Nóra
name: Müller, Anetta
Publisher: name: Debreceni Egyetem
Year: 2018

description: Különleges Bánásmód, vol. 4. issue 4. ISSN 2498-5368
Elliptic subfields and automorphisms of genus 2 function fields
Creators: name: Shaska, Tony
name: Voelklein, Helmut
Publisher: name: arXiv
Year: 2001
Subjects: subject: Algebraic Geometry (math.AG)
subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: 14-XX, 11-XX

description: We study genus 2 function fields with elliptic subfields of degree 2. The locus $Ł_2$ of these fields is a 2-dimensional subvariety of the moduli space $\mathcal M_2$ of genus 2 fields. An equation for $Ł_2$ is already in the work of Clebsch and Bolza. We use a birational parameterization of $Ł_2$ by affine 2-space to study the relation between the j-invariants of the degree 2 elliptic subfields. This extends work of Geyer, Gaudry, Stichtenoth and others. We find a 1-dimensional family of genus 2 curves having exactly two isomorphic elliptic subfields of degree 2; this family is parameterized by the j-invariant of these subfields.
Hybrid and Automated Machine Learning Approaches for Oil Fields Development: the Case Study of Volve Field, North Sea
Creators: name: Nikitin, Nikolay O.
name: Revin, Ilia
name: Hvatov, Alexander
name: Vychuzhanin, Pavel
name: Kalyuzhnaya, Anna V.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Machine Learning (cs.LG)
subject: Geophysics (physics.geo-ph)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: The paper describes the usage of intelligent approaches for field development tasks that may assist a decision-making process. We focused on the problem of wells location optimization and two tasks within it: improving the quality of oil production estimation and estimation of reservoir characteristics for appropriate wells allocation and parametrization, using machine learning methods. For oil production estimation, we implemented and investigated the quality of forecasting models: physics-based, pure data-driven, and hybrid one. The CRMIP model was chosen as a physics-based approach. We compare it with the machine learning and hybrid methods in a frame of oil production forecasting task. In the investigation of reservoir characteristics for wells location choice, we automated the seismic analysis using evolutionary identification of convolutional neural network for the reservoir detection. The Volve oil field dataset was used as a case study to conduct the experiments. The implemented approaches can be used to analyze different oil fields or adapted to similar physics-related problems.
description: 30 pages
Fitness Uniform Selection to Preserve Genetic Diversity
Creators: name: Hutter, Marcus
Publisher: name: arXiv
Year: 2001
Subjects: subject: Artificial Intelligence (cs.AI)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Machine Learning (cs.LG)
subject: Quantitative Biology (q-bio)
subject: FOS: Computer and information sciences
subject: FOS: Biological sciences
subject: I.2; I.2.6; I.2.8; F.2

description: In evolutionary algorithms, the fitness of a population increases with time by mutating and recombining individuals and by a biased selection of more fit individuals. The right selection pressure is critical in ensuring sufficient optimization progress on the one hand and in preserving genetic diversity to be able to escape from local optima on the other. We propose a new selection scheme, which is uniform in the fitness values. It generates selection pressure towards sparsely populated fitness regions, not necessarily towards higher fitness, as is the case for all other selection schemes. We show that the new selection scheme can be much more effective than standard selection schemes.
description: 13 LaTeX pages, 1 eps figure
A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
Creators: name: Xu, Dandan
name: Zhu, Ling
name: Grand, Robert
name: Springel, Volker
name: Mao, Shude
name: van de Ven, Glenn
name: Lu, Shengdong
name: Wang, Yougang
name: Pillepich, Annalisa
name: Genel, Shy
name: Nelson, Dylan
name: Rodriguez-Gomez, Vicente
name: Pakmor, Ruediger
name: Weinberger, Rainer
name: Marinacci, Federico
name: Vogelsberger, Mark
name: Torrey, Paul
name: Jill, Naiman
name: Hernquist, Lars
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Motivated by the recently discovered kinematic "Hubble sequence" shown by the stellar orbit-circularity distribution of 260 CALIFA galaxies, we make use of a comparable galaxy sample at z = 0 with a stellar mass range from 5E9 to 5E11 solar masses, selected from the IllustrisTNG simulation and study their stellar orbit compositions in relation to a number of other fundamental galaxy properties.We find that the TNG100 simulation broadly reproduces the observed fractions of different orbital components and their stellar mass dependencies. In particular, the mean mass dependencies of the luminosity fractions for the kinematically warm and hot orbits are well reproduced within model uncertainties of the observed galaxies. The simulation also largely reproduces the observed peak and trough features at a stellar mass of 1-2E10 solar masses, in the mean distributions of the cold- and hot-orbit fractions, respectively, indicating fewer cooler orbits and more hotter orbits in both more- and less-massive galaxies beyond such a mass range. Several marginal disagreements are seen between the simulation and observations: the average cold-orbit (counter-rotating) fractions of the simulated galaxies below (above) a stellar mass of 6E10 solar masses, are systematically higher than the observational data by < 10% (absolute orbital fraction); the simulation also seems to produce more scatter for the cold-orbit fraction and less so for the non-cold orbits at any given galaxy mass. Possible causes that stem from the adopted heating mechanisms are discussed.
description: 12 pages, 6 figures, 3 tables, submitted to MNRAS. Comments are welcome!
Maximal characterisation of local Hardy spaces on locally doubling manifolds
Creators: name: Martini, Alessio
name: Meda, Stefano
name: Vallarino, Maria
Publisher: name: arXiv
Year: 2021
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 42B30, 42B35, 58C99

description: We prove a radial maximal function characterisation of the local atomic Hardy space h^1(M) on a Riemannian manifold M with positive injectivity radius and Ricci curvature bounded from below. As a consequence, we show that an integrable function belongs to h^1(M) if and only if either its local heat maximal function or its local Poisson maximal function are integrable. A key ingredient is a decomposition of Hölder cut-offs in terms of an appropriate class of approximations of the identity, which we obtain on arbitrary Ahlfors-regular metric measure spaces and generalises a previous result of A. Uchiyama.
description: 31 pages
Additional file 1: of The effectiveness of financial intervention strategies for reducing caesarean section rates: a systematic review
Creators: name: Yushan Yu
name: Feili Lin
name: Weizhen Dong
name: Haohan Li
name: Xiangyang Zhang
name: Chen, Chun
Publisher: name: figshare
Year: 2019
Subjects: subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy

description: Full electronic search strategy used in the systematic review; We conducted a systematic search of English language CS rate relevant articles following this search strategy. (DOCX 21 kb)
Haemonides Hubner 1819
Creators: name: Moraes, Simeão De Souza
name: Duarte, Marcelo
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Castniidae
Haemonides

description: HAEMONIDES HÜBNER, [1819] (FIG. 27)
 Type species
 Papilio cronis Cramer, [1775]
 Included species
 Haemonides cronis (Cramer, [1775]), Haemonides cronida (Herrich-Schäffer, [1854]), and Haemonides candida (Houlbert, 1917).
 Comments
 Although there is support to synonymize this genus with Riechia and Imara, we consider it as a valid genus because of some distinct features, such as the morphology and sclerotization of the aedeagus, and the shape of the gnathos. Diagnostic characters for this genus include the aedeagus heavily sclerotized and not twisted, and the white colour in the wing pattern.
description: Published as part of Moraes, Simeão De Souza & Duarte, Marcelo, 2014, Phylogeny of Neotropical Castniinae (Lepidoptera: Cossoidea: Castniidae): testing the hypothesis of the mimics as a monophyletic group and implications for the arrangement of the genera, pp. 362-399 in Zoological Journal of the Linnean Society 170 (2) on page 392, DOI: 10.1111/zoj.12102, http://zenodo.org/record/5302314
A General Method to Find Highly Coordinating Communities in Social Media through Inferred Interaction Links
Creators: name: Weber, Derek
name: Neumann, Frank
Publisher: name: arXiv
Year: 2021
Subjects: subject: Social and Information Networks (cs.SI)
subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences

description: Political misinformation, astroturfing and organised trolling are online malicious behaviours with significant real-world effects. Many previous approaches examining these phenomena have focused on broad campaigns rather than the small groups responsible for instigating or sustaining them. To reveal latent (i.e., hidden) networks of cooperating accounts, we propose a novel temporal window approach that relies on account interactions and metadata alone. It detects groups of accounts engaging in various behaviours that, in concert, come to execute different goal-based strategies, a number of which we describe. The approach relies upon a pipeline that extracts relevant elements from social media posts, infers connections between accounts based on criteria matching the coordination strategies to build an undirected weighted network of accounts, which is then mined for communities exhibiting high levels of evidence of coordination using a novel community extraction method. We address the temporal aspect of the data by using a windowing mechanism, which may be suitable for near real-time application. We further highlight consistent coordination with a sliding frame across multiple windows and application of a decay factor. Our approach is compared with other recent similar processing approaches and community detection methods and is validated against two relevant datasets with ground truth data, using content, temporal, and network analyses, as well as with the design, training and application of three one-class classifiers built using the ground truth; its utility is furthermore demonstrated in two case studies of contentious online discussions.
description: 58 pages, 25 figures, submitted to the International Journal of Social Network Analysis and Mining (SNAM) as an expansion to an ASONAM'20 paper (arXiv:2010.08180)
Gamma-ray bursts, supernova kicks, and gravitational radiation
Creators: name: Davies, Melvyn B.
name: King, Andrew
name: Rosswog, Stephan
name: Wynn, Graham
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We suggest that the collapsing core of a massive rotating star may fragment to produce two or more compact objects. Their coalescence under gravitational radiation gives the resulting black hole or neutron star a significant kick velocity, which may explain those observed in pulsars. A gamma-ray burst can result only when this kick is small. Thus only a small fraction of core-collapse supernovae produce gamma-ray bursts. The burst may be delayed significantly (hours - days) after the supernova, as suggested by recent observations. If this picture is correct, core-collapse supernovae should be significant sources of gravitational radiation with a chirp signal similar to a coalescing binary.
description: 10 pages, 2 figures; submitted to ApJ Letters
Additional file 1: of Manual therapy versus therapeutic exercise in non-specific chronic neck pain: study protocol for a randomized controlled trial
Creators: name: Bernal-Utrera, Carlos
name: González-Gerez, Juan
name: Saavedra-Hernandez, Manuel
name: Lérida-Ortega, Miguel Ángel
name: Cleofás Rodríguez-Blanco
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Ecology
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Plant Biology

description: SPIRIT Checklist. (DOC 122 kb)
Riechia Oiticica 1955
Creators: name: Moraes, Simeão De Souza
name: Duarte, Marcelo
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Castniidae
Riechia

description: RIECHIA OITICICA, 1955 SYN. NOV.
 Type species
 Castnia pallasia Eschscholtz, 1821
 Included species
 Imara pallasia (Eschscholtz, 1821), Imara satrapes (Kollar, 1839), Imara therapon (Kollar, 1839) (Athis) comb. nov., and Imara acraeoides (Guérin-Ménéville, [1832]) (Riechia) comb. nov.
 Comments
This arrangement is supported only by one homoplastic character of the length of the uncus (67: 2), but the general morphology of the male and female genitalia supports this arrangement of genera. Although it was not possible to code some of the common characters because of the difficulty of establishing the primary homology, or because some states were overlapping, some traits of the male and female genitalia, such as the shape of the uncus, the morphology of the aedeagus and valva, as well as the morphology of the bursa, signum, ductus bursae, and the sterigma agree with the taxonomic attribution.
 Imara acraeoides (Fig. 23) shares with I. satrapes (Fig. 26) the mimetic wing pattern of Acraeini (Nymphalidae), which seems to be plesiomorphic in this lineage.
 Imara therapon (Fig. 24) is one of the two species previously included in Athis and distributed in southeast America. As suggested by J. M. González (pers. comm.), I. therapon and A. amalthaea may be part of the same group, which means that, similarly to I. therapon, A. amalthaea may be more closely related to Imara than to Athis.
description: Published as part of Moraes, Simeão De Souza & Duarte, Marcelo, 2014, Phylogeny of Neotropical Castniinae (Lepidoptera: Cossoidea: Castniidae): testing the hypothesis of the mimics as a monophyletic group and implications for the arrangement of the genera, pp. 362-399 in Zoological Journal of the Linnean Society 170 (2) on page 392, DOI: 10.1111/zoj.12102, http://zenodo.org/record/5302314