cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Lobelia siphilitica Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Asterales
Campanulaceae
Lobelia
Lobelia siphilitica

description: Lobelia siphilitica Linnaeus, Species Plantarum 2: 931. 1753.
"Habitat in Virginia." RCN: 6750.
 Lectotype (McVaugh in Rhodora 38: 278. 1936): Herb. Linn. No. 1051.25 (LINN).
 Current name: Lobelia siphilitica L. (Campanulaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part L), pp. 610-650 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 639, DOI: 10.5281/zenodo.291971
Conservative Link Adaptation for Ultra Reliable Low Latency Communications
Creators: name: Belogaev, Andrey
name: Khorov, Evgeny
name: Krasilov, Artem
name: Shmelkin, Dmitri
name: Tang, Suwen
Publisher: name: arXiv
Year: 2019
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: Ultra reliable low latency communications (URLLC) is one of the most promising and demanding services in 5G systems. This service requires very low latency of less than $1-10$ ms and very high transmission reliability: the acceptable packet loss ratio is about $10^{-5}$. To satisfy such strict requirements, many issues shall be solved. This paper focuses on the link adaptation problem, i.e., the selection of a modulation and coding scheme (MCS) for transmission based on the received channel quality indicator (CQI) reports. On the one hand, link adaptation should select a robust MCS to provide high reliability. On the other hand, it should select the highest possible MCS to reduce channel resource consumption. The paper shows that even for one URLLC user, link adaptation is still a challenging problem, especially in highly-variant channels. To solve this problem, a conservative link adaptation algorithm is designed. The algorithm estimates the strongest channel degradation at the time moment of the actual packet transmission and selects an MCS taking into account the worst degradation. The obtained results show that the proposed algorithm is efficient in terms of both the packet loss ratio and the channel resource consumption.
description: BlackSeaCom'19
Appendices 1 and 2; Figure S1 and Tables S1 and S2 from Inheritance patterns of plumage coloration in Common Buzzards Buteo buteo do not support a one-locus two-allele model
Creators: name: Kappers, Elena Frederika
name: Vries, Christiaan De
name: Alberda, Anneke
name: Forstmeier, Wolfgang
name: Both, Christiaan
name: Kempenaers, Bart
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences

description: Appendix 1: Study site; Appendix 2: Colour morph scoring; Figure S1: Observed and expected inheritance of plumage colour morph for all parental combinations in Common Buzzards from Friesland, The Netherlands.; Table S1: Observed and expected inheritance of plumage colour morph for all parental combinations in Common Buzzards from Friesland, The Netherlands.; Table S2: Observed inheritance of plumage colour morph in Common Buzzards from Friesland, The Netherlands (our study), and from a previous study in Eastern Westphalia, Germany
On the unit sphere of positive operators
Creators: name: Peralta, Antonio M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Functional Analysis (math.FA)
subject: Operator Algebras (math.OA)
subject: FOS: Mathematics

description: Given a C$^*$-algebra $A$, let $S(A^+)$ denote the set of those positive elements in the unit sphere of $A$. Let $H_1$, $H_2,$ $H_3$ and $H_4$ be complex Hilbert spaces, where $H_3$ and $H_4$ are infinite-dimensional and separable. In this note we prove a variant of Tingley's problem by showing that every surjective isometry $Δ: S(B(H_1)^+)\to S(B(H_2)^+)$ or (respectively, $Δ: S(K(H_3)^+)\to S(K(H_4)^+)$) admits a unique extension to a surjective complex linear isometry from $B(H_1)$ onto $B(H_2))$ (respectively, from $K(H_3)$ onto $B(H_4)$). This provides a positive answer to a conjecture posed by G. Nagy [\emph{Publ. Math. Debrecen}, 2018].
Centropogon cornutus Druce
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Asterales
Campanulaceae
Centropogon
Centropogon cornutus

description: Lobelia surinamensis Linnaeus, Species Plantarum, ed. 2, 2: 1320. 1763.
"Habitat Surinami." RCN: 6751.
Type not designated.
Original material: none traced.
 Current name: Centropogon cornutus (L.) Druce (Campanulaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part L), pp. 610-650 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 639, DOI: 10.5281/zenodo.291971
Motivic integration over wild Deligne-Mumford stacks
Creators: name: Yasuda, Takehiko
Publisher: name: arXiv
Year: 2019
Subjects: subject: Algebraic Geometry (math.AG)
subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: 14E18, 14D23, 14E16, 14B05, 11G25, 11S15

description: We develop the motivic integration theory over formal Deligne-Mumford stacks over a power series ring of arbitrary characteristic. This is a generalization of the corresponding theory for tame and smooth Deligne-Mumford stacks constructed in earlier papers of the author. As an application, we obtain the wild motivic McKay correspondence for linear actions of arbitrary finite groups, which has been known only for cyclic groups of prime order. In particular, this implies the motivic version of Bhargava's mass formula as a special case. In fact, we prove a more general result, the invariance of stringy motives of (stacky) log pairs under crepant morphisms.
description: 84 pages; Introduction and Section 16 have been revised. Minor changes in other places
Parameter Regimes in Partial Functional Panel Regression
Creators: name: Liebl, Dominik
name: Walders, Fabian
Publisher: name: arXiv
Year: 2017
Subjects: subject: Methodology (stat.ME)
subject: FOS: Computer and information sciences

description: A new partial functional linear regression model for panel data with time varying parameters is introduced. The parameter vector of the multivariate model component is allowed to be completely time varying while the function-valued parameter of the functional model component is assumed to change over K unknown parameter regimes. Consistency is derived for the suggested estimators and for the classification procedure used to detect the K unknown parameter regimes. Additionally, the convergence rates of the estimators are derived under a double asymptotic differentiating between asymptotic scenarios depending on the relative order of the panel dimensions n and T. The statistical model is motivated by a real data application considering the so-called idiosyncratic volatility puzzle using high frequency data from the S&P500.
Topological Entanglement Entropy of Fracton Stabilizer Codes
Creators: name: Ma, Han
name: Schmitz, A. T.
name: Parameswaran, S. A.
name: Hermele, Michael
name: Nandkishore, Rahul M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Entanglement entropy provides a powerful characterization of two-dimensional gapped topological phases of quantum matter, intimately tied to their description by topological quantum field theories (TQFTs). Fracton topological orders are three-dimensional gapped topologically ordered states of matter, but the existence of a TQFT description for these phases remains an open question. We show that three-dimensional fracton phases are nevertheless characterized, at least partially, by universal structure in the entanglement entropy of their ground state wave functions. We explicitly compute the entanglement entropy for two archetypal fracton models --- the `X-cube model' and `Haah's code' --- and demonstrate the existence of a topological contribution that scales linearly in subsystem size. We show via Schrieffer-Wolff transformations that the topological entanglement of fracton models is robust against arbitrary local perturbations of the Hamiltonian. Finally, we argue that these results may be extended to characterize localization-protected fracton topological order in excited states of disordered fracton models.
description: published version
Wahlenbergia
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Asterales
Campanulaceae
Wahlenbergia

description: Lobelia tenella Linnaeus, Systema Naturae, ed. 12, 2: 584; Mantissa Plantarum: 120. 1767.
"Habitat ad Cap. b. spei." RCN: 6763.
 Lectotype (Phillipson in Bot. J. Linn. Soc. 99: 257. 1989): Herb. Linn. No. 1051.50 (LINN).
 Current name:  Wahlenbergia sp.  (Campanulaceae).
 Note: Phillipson, in typifying the name, excluded it from Monopsis but stated only that it applied to an unspecified species of Wahlenbergia.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part L), pp. 610-650 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 639, DOI: 10.5281/zenodo.291971
A peculiar multi-wavelength flare in the Blazar 3C 454.3
Creators: name: Gupta, Alok C.
name: Mangalam, Arun
name: Wiita, Paul J.
name: Kushwaha, P.
name: Gaur, H.
name: Zhang, H.
name: Gu, M. F.
name: Liao, M.
name: Dewangan, G.
name: Ho, L. C.
name: Mohan, P.
name: Umeura, M.
name: Sasada, M.
name: Volvach, A. E.
name: Agarwal, A.
name: Aller, M. F.
name: Aller, H. D.
name: Bachev, R.
name: Lahteenmaki, A.
name: Semkov, E.
name: Strigachev, A.
name: Tornikoski, M.
name: Volvach, L. N.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The blazar 3C454.3 exhibited a strong flare seen in gamma-rays, X-rays, and optical/NIR bands during 3--12 December 2009. Emission in the V and J bands rose more gradually than did the gamma-rays and soft X-rays, though all peaked at nearly the same time. Optical polarization measurements showed dramatic changes during the flare, with a strong anti-correlation between optical flux and degree of polarization (which rose from ~ 3% to ~ 20%) during the declining phase of the flare. The flare was accompanied by large rapid swings in polarization angle of ~ 170 degree. This combination of behaviors appear to be unique. We have cm-band radio data during the same period but they show no correlation with variations at higher frequencies. Such peculiar behavior may be explained using jet models incorporating fully relativistic effects with a dominant source region moving along a helical path or by a shock-in-jet model incorporating three-dimensional radiation transfer if there is a dominant helical magnetic field. We find that spectral energy distributions at different times during the flare can be fit using modified one-zone models where only the magnetic field strength and particle break frequencies and normalizations need change. An optical spectrum taken at nearly the same time provides an estimate for the central black hole mass of ~ 2.3 * 10^9 M_sun. We also consider two weaker flares seen during the $\sim 200$ d span over which multi-band data are available. In one of them, the V and J bands appear to lead the $γ$-ray and X-ray bands by a few days; in the other, all variations are simultaneous.
description: 11 pages, 4 figures, 2 tables; MNRAS in press
Intrinsic short time scale variability of W3(OH) maser
Creators: name: Ramachandran, R.
name: Deshpande, A. A.
name: Goss, W. M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have studied the OH masers in the star forming region, W3(OH), with data obtained from the Very Long Baseline Array (VLBA). The data provide an angular resolution of $\sim$5 mas, and a velocity resolution of 106 m s$^{-1}$. A novel analysis procedure allows us to differentiate between broadband temporal intensity fluctuations introduced by instrumental gain variations plus interstellar diffractive scintillation, and intrinsic narrowband variations. Based on this 12.5 hours observation, we are sensitive to variations with time scales of minutes to hours. We find statistically significant intrinsic variations with time scales of $\sim$15--20 minutes or slower, based on the {\it velocity-resolved fluctuation spectra}. These variations are seen predominantly towards the line shoulders. The peak of the line profile shows little variation, suggesting that they perhaps exhibit saturated emission. The associated modulation index of the observed fluctuation varies from statistically insignificant values at the line center to about unity away from the line center. Based on light-travel-time considerations, the 20-minute time scale of intrinsic fluctuations translates to a spatial dimension of $\sim$2--3 AU along the sight-lines. On the other hand, the transverse dimension of the sources, estimated from their observed angular sizes of about $\sim$3 mas, is about 6 AU. We argue that these source sizes are intrinsic, and are not affected by interstellar scatter broadening. The implied peak brightness temperature of the 1612/1720 maser sources is about $\sim2\times 10^{13}$ K, and a factor of about five higher for the 1665 line.
description: Accepted for publication in The Astrophysical Journal
A note on "Relaxation Oscillators with Exact Limit Cycles"
Creators: name: Giné, Jaume
name: Grau, Maite
Publisher: name: arXiv
Year: 2005
Subjects: subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics
subject: 34A05, 34C07

description: In this note we give a family of planar polynomial differential systems with a prescribed hyperbolic limit cycle. This family constitutes a corrected and wider version of an example given in the work of M.A. Abdelkader entitled ``Relaxation Oscillators with Exact Limit Cycles'', which appeared in J. Math. Anal. Appl. 218 (1998), 308--312. The result given in this note may be used to construct models of Liénard differential equations exhibiting a desired limit cycle.
description: 8 pages, no figures
Searching for classical geometries in spin foam amplitudes: a numerical method
Creators: name: Dona, Pietro
name: Gozzini, Francesco
name: Sarno, Giorgio
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We develop a numerical method to investigate the semiclassical limit of spin foam amplitudes with many vertices. We test it using the Ponzano-Regge model, a spin foam model for three-dimensional euclidean gravity, and a transition amplitude with three vertices. We study the summation over bulk spins, and we identify the stationary phase points that dominate it and that correspond to classical geometries. We complement with the numerical analysis of a four vertex transition amplitude and with a modification of the model that includes local curvature. We discuss the generalization of our results to the four-dimensional EPRL spin foam model, and we provide suggestions for new computations.
description: 21 pages, 40 figures, prepared for the Focus Issue on "Numerical Investigations in Non-Perturbative Quantum Gravity" published in "Classical and Quantum Gravity". V2 updates: Section 5 has been updated with a new numerical algorithm and the preprint now matches with the published version
Recent results and future of the NA61/SHINE strong interactions program
Creators: name: Lysakowski, Bartosz
Publisher: name: arXiv
Year: 2017
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: NA61/SHINE is a fixed target experiment at the CERN Super-Proton- Synchrotron. The main goals of the experiment are to discover the critical point of strongly interacting matter and study the properties of the onset of deconfnement. In order to reach these goals the collaboration studies hadron production properties in nucleus-nucleus, proton-proton and proton-nucleus interactions. In this talk, recent results on particle production in p+p interactions, as well as Be+Be and Ar+Sc collisions in the SPS energy range are reviewed. The results are compared with available world data. The future of the NA61/SHINE scientifc program is also presented.
Deformation mechanism map of Cu/Nb nanoscale metallic multilayers as a function of temperature and layer thickness
Creators: name: Snel, J.
name: Monclús, M. A.
name: Castillo-Rodríguez, M.
name: Mara, N.
name: Beyerlein, I. J.
name: LLorca, J.
name: Molina-Aldareguía, J. M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The mechanical properties and deformation mechanisms of Cu/Nb nanoscale metallic multilayers (NMMs) manufactured by accumulative roll bonding (ARB) are studied at 25C and 400C. Cu/Nb NMMs with individual layer thicknesses between 7 and 63 nm were tested by in-situ micropillar compression inside a scanning electron microscope Yield strength, strain-rate sensitivities and activation volumes were obtained from the pillar compression tests. The deformed micropillars were examined under scanning and transmission electron microscopy in order to examine the deformation mechanisms active for different layer thicknesses and temperatures. The analysis suggests that room temperature deformation was determined by dislocation glide at larger layer thicknesses and interface-related mechanisms at the thinner layer thicknesses. The high temperature compression tests, in contrast, revealed superior thermo-mechanical stability and strength retention for the NMMs with larger layer thicknesses with deformation controlled by dislocation glide. A remarkable transition in deformation mechanism occurred as the layer thickness decreased, to a deformation response controlled by diffusion processes along the interfaces, which resulted in temperature-induced softening. A deformation mechanism map, in terms of layer thickness and temperature, is proposed from the results obtained in this investigation.
Lobelia tupa Linnaeus 1763
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Asterales
Campanulaceae
Lobelia
Lobelia tupa

description: Lobelia trapa Linnaeus, Species Plantarum 2: 929. 1753 orth. var.
"Habitat in Peru." RCN: 6740.
 Lectotype (Matthews in Kew Mag. 5: 161. 1988): [icon] "Rapuntium spicatum,foliis acutis, vulgo Tupa" in Feuillée, J. Obs. 2: 739, t. 29. 1714.
 Current name: Lobelia tupa L. (Campanulaceae).
 Note: The specific epithet was drawn from Feuillée’s phrase name, misquoted by Linnaeus as "Rap. spicatum, fol. auritis, vulgo Trapa". He corrected the spelling in Sp. Pl., ed. 2, 2: 1318 (1763).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part L), pp. 610-650 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 639, DOI: 10.5281/zenodo.291971
Investigating the Relativistic Motion of the Stars Near the Supermassive Black Hole in the Galactic Center
Creators: name: Parsa, M.
name: Eckart, A.
name: Shahzamanian, B.
name: Karas, V.
name: Zajacek, M.
name: Zensus, J. A.
name: Straubmeier, C.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The S-star cluster in the Galactic center allows us to study the physics close to a supermassive black hole, including distinctive dynamical tests of general relativity. Our best estimates for the mass of and the distance to Sgr A* using the three stars with the shortest period (S2, S38, and S55/S0-102) and Newtonian models are M_BH = (4.15+- 0.13 +- 0.57) x 10^6 M_sun and R_0 = 8.19 +- 0.11 +- 0.34 kpc. Additionally, we aim at a new and practical method to investigate the relativistic orbits of stars in the gravitational field near Sgr A*. We use a first-order post- Newtonian approximation to calculate the stellar orbits with a broad range of periapse distance r_p. We present a method that employs the changes in orbital elements derived from elliptical fits to different sections of the orbit. These changes are correlated with the relativistic parameter defined as Υ = r_s/r_p (with r_s being the Schwarzschild radius) and can be used to derive Υ from observational data. For S2 we find a value of Υ = 0.00088 +- 0.00080, which is consistent, within the uncertainty, with the expected value of Υ = 0.00065 derived from MBH and the orbit of S2. We argue that the derived quantity is unlikely to be dominated by perturbing influences such as noise on the derived stellar positions, field rotation, and drifts in black hole mass.
description: 27 pages, 24 figures
Relative brain volume in Carnivorans
Creators: name: Lynch, Leigha
name: Allen, Kari
Publisher: name: figshare
Year: 2022
Subjects: subject: 60303 Biological Adaptation
subject: FOS: Biological sciences
subject: Evolutionary Biology

description: Supplemental data and R coding for "Relative brain volume of carnivorans has evolved in correlation with environmental and dietary variables differentially among clades"
2MASS J05162881+2607387: A New Low-Mass Double-Lined Eclipsing Binary
Creators: name: Bayless, Amanda J.
name: Orosz, Jerome A.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show that the star known as 2MASS J05162881+2607387 (hereafter J0516) is a double-lined eclipsing binary with nearly identical low-mass components. The spectroscopic elements derived from 18 spectra obtained with the High Resolution Spectrograph on the Hobby-Eberly Telescope during the Fall of 2005 are K_1=88.45 +/- 0.48 km/s and K_2=90.43 +/- 0.60 km/s, resulting in a mass ratio of$q=K_1/K_2 = 0.978 +/- 0.018 and minimum masses of M_1 sin^{3}i=0.775 +/- 0.016 solar masses and M_2 sin^{3}i=0.759 +/- 0.012 solar masses, respectively. We have extensive differential photometry of J0516 obtained over several nights between 2004 January-March (epoch 1) and 2004 October-2005 January plus 2006 January (epoch 2) using the 1m telescope at the Mount Laguna Observatory. The source was roughly 0.1 mag brighter in all three bandpasses during epoch 1 when compared to epoch 2. Also, phased light curves from epoch 1 show considerable out-of-eclipse variability, presumably due to bright spots on one or both stars. In contrast, the phased light curves from epoch 2 show little out-of-eclipse variability. The light curves from epoch 2 and the radial velocity curves were analyzed using our ELC code with updated model atmospheres for low-mass stars. We find the following: M_1=0.787 +/- 0.012 solar masses, R_1=0.788 +/- 0.015 solar radii, M_2=0.770 +/- 0.009 solar masses, and R_2=0.817 +/- 0.010 solar radii. The stars in J0516 have radii that are significantly larger than model predictions for their masses, similar to what is seen in a handful of other well-studied low-mass double-lined eclipsing binaries. We compiled all recent mass and radius determinations from low-mass binaries and determine an empirical mass-radius relation of the form R = 0.0324 + 0.9343M + 0.0374M^2, where the quantities are in solar units.
description: 16 pages, 10 figures (Figure 1 has degraded quality), to appear in ApJ
Review Protocol - Impact of the COVID-19 pandemic on autistic adults: A systematic scoping review
Creators: name: Scheeren, Anke
name: Crane, Laura
name: Heyworth, Melanie
name: Pellicano, Liz
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology
subject: autism
subject: COVID-19
subject: review protocol

description: The COVID-19 pandemic and its associated restrictions have had a tremendous impact on people’s everyday lives all across the globe. Although some general population studies have shown relative stability in people’s mental health during the pandemic (Ahrens et al., 2021; O’Connor et al., 2021; Voltmer et al., 2021), others showed significant reductions (Jia et al., 2020; Santamauro et al., 2021). The pandemic may have had disproportionately negative effects on the wellbeing of those who were potentially vulnerable in some way prior to the pandemic – including autistic people. Indeed, autistic people are more likely to experience financial insecurity and mental health problems (Hollocks et al., 2019; Roux et al., 2013) in pre-COVID-19 times, and are thus also more likely to have relied on services and supports – all of which were at risk of disruption during the pandemic (Pellicano et al., 2021; White et al., 2021). Moreover, given a general preference for routines, autistic adults may (have) experience(d) more psychological distress than non-autistic adults due to changes in governmental guidelines and restrictions (Oomen, Nijhof, & Wiersema, 2021; Pellicano et al., 2021). Effects of the pandemic may not be universally negative, however, as some autistic adults may have experienced a temporary relief from social obligations and sensory overload (Bundy et al., 2022; Oomen et al., 2021; Pellicano et al., 2021). In the current scoping review, we aim to a) synthesize all papers published on the impact of the COVID-19 pandemic on autistic adults, and b) identify lessons for future care and support of autistic adults in times of crisis and more normal times. Please see attached our review protocol.
The Soft Supersymmetry-Breaking Lagrangian: Theory and Applications
Creators: name: Chung, D. J. H.
name: Everett, L. L.
name: Kane, G. L.
name: King, S. F.
name: Lykken, J.
name: Wang, Lian-Tao
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: After an introduction recalling the theoretical motivation for low energy (100 GeV to TeV scale) supersymmetry, this review describes the theory and experimental implications of the soft supersymmetry-breaking Lagrangian of the general minimal supersymmetric standard model (MSSM). Extensions to include neutrino masses and nonminimal theories are also discussed. Topics covered include models of supersymmetry breaking, phenomenological constraints from electroweak symmetry breaking, flavor/CP violation, collider searches, and cosmological constraints including dark matter and implications for baryogenesis and inflation.
description: 273 pages; 35 figures; submitted to Physics Reports
Moduli of formal torsors II
Creators: name: Tonini, Fabio
name: Yasuda, Takehiko
Publisher: name: arXiv
Year: 2019
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 14D22, 13F25, 14H30

description: Applying the authors' preceding work, we construct a version of the moduli space of $G$-torsors over the formal punctured disk for a finite group $G$. To do so, we introduce two Grothendieck topologies, the sur (surjective) and luin (locally universally injective) topologies, and define P-schemes using them as variants of schemes. Our moduli space is defined as a P-scheme approximating the relevant moduli functor. We then prove that Fröhlich's module resolvent gives a locally constructible function on this moduli space, which implies that motivic integrals appearing the wild McKay correspondence are well-defined.
description: 36 pages, some improvements, accepted in Annales de l'Institut Fourier
Gossez's approximation theorems in the Musielak-Orlicz-Sobolev spaces
Creators: name: Ahmida, Youssef
name: Chlebicka, Iwona
name: Gwiazda, Piotr
name: Youssfi, Ahmed
Publisher: name: arXiv
Year: 2017
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics

description: We prove the density of smooth functions in the modular topology in the Musielak-Orlicz-Sobolev spaces essentially extending the results of Gossez \cite{GJP2} obtained in the Orlicz-Sobolev setting. We impose new systematic regularity assumption on $M$ which allows to study the problem of density unifying and improving the known results in the Orlicz-Sobolev spaces, as well as the variable exponent Sobolev spaces. We confirm the precision of the method by showing the lack of the Lavrentiev phenomenon in the double-phase case. Indeed, we get the modular approximation of $W^{1,p}_0(Ω)$ functions by smooth functions in the double-phase space governed by the modular function $H(x,s)=s^p+a(x)s^q$ with $a\in C^{0,α}(Ω)$ excluding the Lavrentiev phenomenon within the sharp range $q/p\leq 1+α/N$. See \cite[Theorem~4.1]{min-double-reg1} for the sharpness of the result.
Lobelia comosa Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Asterales
Campanulaceae
Lobelia
Lobelia comosa

description: Lobelia triquetra Linnaeus, Systema Naturae, ed. 12, 2: 583; Mantissa Plantarum: 120. 1767.
"Habitat ad Cap b. spei." RCN: 6746.
Type not designated.
Original material: none traced.
 Current name: Lobelia comosa L. (Campanulaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part L), pp. 610-650 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 639, DOI: 10.5281/zenodo.291971
Error bounds for some approximate posterior measures in Bayesian inference
Creators: name: Lie, Han Cheng
name: Sullivan, T. J.
name: Teckentrup, Aretha
Publisher: name: arXiv
Year: 2019
Subjects: subject: Statistics Theory (math.ST)
subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics
subject: 62F15, 65C99, 65D05, 65J22, 68W20

description: In certain applications involving the solution of a Bayesian inverse problem, it may not be possible or desirable to evaluate the full posterior, e.g. due to the high computational cost of doing so. This problem motivates the use of approximate posteriors that arise from approximating the data misfit or forward model. We review some error bounds for random and deterministic approximate posteriors that arise when the approximate data misfits and approximate forward models are random.
description: 8 pages
Renormalization analysis of catalytic Wright-Fisher diffusions
Creators: name: Fleischmann, K.
name: Swart, J. M.
Publisher: name: arXiv
Year: 2005
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 82C28 (Primary) 82C22, 60J60 (Secondary)

description: Recently, several authors have studied maps where a function, describing the local diffusion matrix of a diffusion process with a linear drift towards an attraction point, is mapped into the average of that function with respect to the unique invariant measure of the diffusion process, as a function of the attraction point. Such mappings arise in the analysis of infinite systems of diffusions indexed by the hierarchical group, with a linear attractive interaction between the components. In this context, the mappings are called renormalization transformations. We consider such maps for catalytic Wright-Fisher diffusions. These are diffusions on the unit square where the first component (the catalyst) performs an autonomous Wright-Fisher diffusion, while the second component (the reactant) performs a Wright-Fisher diffusion with a rate depending on the first component through a catalyzing function. We determine the limit of rescaled iterates of renormalization transformations acting on the diffusion matrices of such catalytic Wright-Fisher diffusions.
description: 65 pages, 3 figures
Evidence for the $H \to b\bar{b}$ decay with the ATLAS detector
Creators: name: ATLAS Collaboration
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A search for the decay of the Standard Model Higgs boson into a $b\bar{b}$ pair when produced in association with a $W$ or $Z$ boson is performed with the ATLAS detector. The analysed data, corresponding to an integrated luminosity of 36.1 fb$^{-1}$, were collected in proton-proton collisions in Run 2 of the Large Hadron Collider at a centre-of-mass energy of 13 TeV. Final states containing zero, one and two charged leptons (electrons or muons) are considered, targeting the decays $Z\toνν$, $W\to\ellν$ and $Z\to\ell\ell$. For a Higgs boson mass of 125 GeV, an excess of events over the expected background from other Standard Model processes is found with an observed significance of 3.5 standard deviations, compared to an expectation of 3.0 standard deviations. This excess provides evidence for the Higgs boson decay into $b$-quarks and for its production in association with a vector boson. The combination of this result with that of the Run 1 analysis yields a ratio of the measured signal events to the Standard Model expectation equal to $0.90 \pm 0.18 \rm{(stat.)} ^{+0.21}_{-0.19} \rm{(syst.)}$. Assuming the Standard Model production cross-section, the results are consistent with the value of the Yukawa coupling to $b$-quarks in the Standard Model.
description: 68 pages in total, author list starting page 52, 13 figures, 15 tables, submitted to JHEP, All figures including auxiliary figures are available at https://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/HIGG-2016-29/. This version matches submission to JHEP
ASTE Observations of Warm Gas in Low-mass Protostellar Envelopes: Different Kinematics between Submillimeter and Millimeter Lines
Creators: name: Takakuwa, Shigehisa
name: Kamazaki, Takeshi
name: Saito, Masao
name: Yamaguchi, Nobuyuki
name: Kohno, Kotaro
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: With the ASTE telescope, we have made observations of three low-mass protostellar envelopes around L483, B335, and L723 in the submillimeter CS ($J$=7--6) and HCN ($J$=4--3) lines. We detected both the CS and HCN lines toward all the targets, and the typical CS intensity ($\sim$ 1.0 K in T$_{B}$) is twice higher than that of the HCN line. Mapping observations of L483 in these lines have shown that the submillimeter emissions in the low-mass protostellar envelope are resolved, exhibit a western extension from the central protostar, and that the deconvolved size is $\sim$ 5500 AU $\times$ 3700 AU (P.A. = 78$^{\circ}$) in the HCN emission. The extent of the submillimeter emissions in L483 implies the presence of higher-temperature ($\gtrsim$ 40 K) gas at 4000 AU away from the central protostar, which suggests that we need to take 2-dimensional radiative transfer models with a flattened disklike envelope and bipolar cavity into account to explain the temperature structure inside the low-mass protostellar envelope. The position-velocity diagrams of these submillimeter lines in L483 and B335 exhibit different velocity gradients from those found in the previous millimeter observations. In particular, along the axis of the associated molecular outflow the sense of the velocity gradient traced by the submillimeter lines is opposite to that of the millimeter observations or the associated molecular outflow, both in L483 and B335. We suggest that expanding gas motions at the surface of the flattened disklike envelope around the protostar, which is irradiated from the central star directly, are the origin of the observed submillimeter velocity structure.
description: 20 pages, 11 figures
RITUAIS DE LUTO EM DIFERENTES CULTURAS: SEMELHANÇAS E DIFERENÇAS
Creators: name: DE MELO, Sarah Nascimento
name: COSTA, Luís Henrique da Silva
Publisher: name: Zenodo
Year: 2024
Subjects: Cultura do luto
Diferenças
Rituais
Sensibilidade.

description: Os rituais de luto são práticas culturais que ajudam as pessoas a processar a perda de entes queridos e a se despedir deles de maneira significativa. Objetivo Analisar a os rituais de luto em diferentes culturas, identificando tanto as semelhanças quanto as diferenças entre eles.
Polar actions on symmetric spaces
Creators: name: Kollross, Andreas
Publisher: name: arXiv
Year: 2005
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 53C35, 57S15

description: We study isometric Lie group actions on symmetric spaces admitting a section, i.e. a submanifold which meets all orbits orthogonally at every intersection point. We classify such actions on the compact symmetric spaces with simple isometry group and rank greater than one. In particular we show that these actions are hyperpolar, i.e. the sections are flat.
description: 45 pages; erroneous Proposition 3.4 deleted; other minor changes and typos corrected; results remain unchanged
Characteristics of geomagnetic cascading of ultra-high energy photons at the southern and northern sites of the Pierre Auger Observatory
Creators: name: Homola, P.
name: Risse, M.
name: Engel, R.
name: Gora, D.
name: Pekala, J.
name: Wilczynska, B.
name: Wilczynski, H.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Cosmic-ray photons above 10^19 eV can convert in the geomagnetic field and initiate a preshower, i.e. a particle cascade before entering the atmosphere. We compare the preshower characteristics at the southern and northern sites of the Pierre Auger Observatory. In addition to a shift of the preshower patterns on the sky due to the different pointing of the local magnetic field vectors, the fact that the northern Auger site is closer to the geomagnetic pole results in a different energy dependence of the preshower effect: photon conversion can start at smaller energies, but large conversion probabilitites (>90%) are reached for the whole sky at higher energies compared to the southern Auger site. We show how the complementary preshower features at the two sites can be used to search for ultra-high energy photons among cosmic rays. In particular, the different preshower characteristics at the northern Auger site may provide an elegant and unambiguous confirmation if a photon signal is detected at the southern site.
description: 25 pages, 14 figures, minor changes, conclusions unchanged, Appendix A replaced, accepted by Astroparticle Physics
Masses and magnetic moments of pentaquarks
Creators: name: Bijker, R.
name: Giannini, M. M.
name: Santopinto, E.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We discuss the spectroscopy of pentaquarks. The quantum numbers of the ground state depend on the interplay between spin-flavor and orbital contributions to the energy. The magnetic moments of the lowest pentaquark state with negative and positive parity are found to be 0.382 μ_N and 0.089 μ_n, respectively.
description: 15 pages, 4 figures, 3 tables (text rewritten, extra figure added, essential results unchanged)
Strategies for monumentalized (pre)historic landscapes in the Danube Region
Creators: name: Mele, Marko
name: Pirkovič, Jelka
name: Črešnar, Matija
name: Fera, Martin
name: Doneus, Michael
name: Tiefengraber, Susanne
name: Dolinar, Nejc
name: Kovačević, Saša
name: Balen, Jacqueline
name: Czajlik, Zoltán
name: Jerem, Erzsébet
name: Czifra, Szabolcs
name: Štuhec, Seta
Publisher: name: Zenodo
Year: 2019
Subjects: Iron Age
Danube Region
Cultural Heritage strategies

description: The Iron-Age-Danube project (Monumentalized early iron age landscapes in the Danube river basin), co-financed by the Interreg Danube Transnational programme, is focused on the research, protection and sustainable touristic use of the archaeological heritage from the Early Iron Age in the Danube region. In the frame of the project two strategies, one on research and heritage protection and other on heritage promotion and touristic usage of archaeological landscapes, have been adopted. The strategies are combining a bottom-up analytical approach by incorporating the SWOT analysis from the eight micro-regions in four countries with a to-down approach by integrating the recommendations of the European Cultural Heritage Strategy for the 21st century (Strategy 21). The analysis showed 24 major challenges faced by the Iron-Age heritage, which can be tackled by 12
 recommendations in the field of research and monument protection and 9 recommendations in the field of sustainable cultural tourism, divided into the S-D-K components introduced in Strategy 21 and a newly established location component. Additionally, concrete courses of actions for stakeholders are listed, which enable the practical implementation of recommendations. The strategies are accompanied by four national action plans for their implementation in Austria, Croatia, Hungary and Slovenia.
Generalized Perron Roots and Solvability of the Absolute Value Equation
Creators: name: Radons, Manuel
name: Tonelli-Cueto, Josué
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optimization and Control (math.OC)
subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics
subject: 65K99, 90C33, 15A24

description: Let $A$ be a $n\times n$ real matrix. The piecewise linear equation system $z-A\vert z\vert =b$ is called an absolute value equation (AVE). It is well-known to be equivalent to the linear complementarity problem. Unique solvability of the AVE is known to be characterized in terms of a generalized Perron root called the sign-real spectral radius of $A$. For mere, possibly non-unique, solvability no such characterization exists. We narrow this gap in the theory. That is, we define the concept of the aligned spectrum of $A$ and prove, under some mild genericity assumptions on $A$, that the mapping degree of the piecewise linear function $F_A:\mathbb{R}^n\to\mathbb{R}^n\,, z\mapsto z-A\lvert z\rvert$ is congruent to $(k+1)\mod 2$, where $k$ is the number of aligned values of $A$ which are larger than $1$. We also derive an exact--but more technical--formula for the degree of $F_A$ in terms of the aligned spectrum. Finally, we derive the analogous quantities and results for the LCP.
description: 20 pages, 2 figures
Design and characterization of the Large-Aperture Experiment to Detect the Dark Age (LEDA) radiometer systems
Creators: name: Price, D. C.
name: Greenhill, L. J.
name: Fialkov, A.
name: Bernardi, G.
name: Garsden, H.
name: Barsdell, B. R.
name: Kocz, J.
name: Anderson, M. M.
name: Bourke, S. A.
name: Craig, J.
name: Dexter, M. R.
name: Dowell, J.
name: Eastwood, M. W.
name: Eftekhari, T.
name: Ellingson, S. W.
name: Hallinan, G.
name: Hartman, J. M.
name: Kimberk, R.
name: Lazio, T. J. W.
name: Leiker, S.
name: MacMahon, D.
name: Monroe, R.
name: Schinzel, F.
name: Taylor, G. B.
name: Tong, E.
name: Werthimer, D.
name: Woody, D. P.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The Large-Aperture Experiment to Detect the Dark Age (LEDA) was designed to detect the predicted O(100)mK sky-averaged absorption of the Cosmic Microwave Background by Hydrogen in the neutral pre- and intergalactic medium just after the cosmological Dark Age. The spectral signature would be associated with emergence of a diffuse Ly$α$ background from starlight during 'Cosmic Dawn'. Recently, Bowman et al. (2018) have reported detection of this predicted absorption feature, with an unexpectedly large amplitude of 530 mK, centered at 78 MHz. Verification of this result by an independent experiment, such as LEDA, is pressing. In this paper, we detail design and characterization of the LEDA radiometer systems, and a first-generation pipeline that instantiates a signal path model. Sited at the Owens Valley Radio Observatory Long Wavelength Array, LEDA systems include the station correlator, five well-separated redundant dual polarization radiometers and backend electronics. The radiometers deliver a 30-85MHz band (16
description: Accepted to MNRAS
A Consistently Oriented Basis for Eigenanalysis
Creators: name: Damask, Jay
Publisher: name: arXiv
Year: 2019
Subjects: subject: Numerical Analysis (math.NA)
subject: Computational Finance (q-fin.CP)
subject: FOS: Mathematics
subject: FOS: Economics and business
subject: G.1.3
subject: 15A18, 65F15, 62H11

description: Repeated application of machine-learning, eigen-centric methods to an evolving dataset reveals that eigenvectors calculated by well-established computer implementations are not stable along an evolving sequence. This is because the sign of any one eigenvector may point along either the positive or negative direction of its associated eigenaxis, and for any one eigen call the sign does not matter when calculating a solution. This work reports an algorithm that creates a consistently oriented basis of eigenvectors. The algorithm postprocesses any well-established eigen call and is therefore agnostic to the particular implementation of the latter. Once consistently oriented, directional statistics can be applied to the eigenvectors in order to track their motion and summarize their dispersion. When a consistently oriented eigensystem is applied to methods of machine-learning, the time series of training weights becomes interpretable in the context of the machine-learning model. Ordinary linear regression is used to demonstrate such interpretability. A reference implementation of the algorithm reported herein has been written in Python and is freely available, both as source code and through the thucyd Python package.
Extremely Red Objects in Two Quasar Fields at z ~ 1.5
Creators: name: Stockton, Alan
name: McGrath, Elizabeth
name: Canalizo, Gabriela
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present an investigation of the properties and environments of bright extremely red objects (EROs) found in the fields of the quasars TXS 0145+386 and 4C 15.55, both at z ~ 1.4. There is marginal evidence from Chandra ACIS imaging for hot cluster gas with a luminosity of a few 10^44 ergs/s in the field of 4C 15.55. The TXS 0145+386 field has an upper limit at a similar value, but it also clearly shows an overdensity of faint galaxies. None of the EROs are detected as X-ray sources. For two of the EROs that have spectral-energy distributions and rest-frame near-UV spectra that show that they are strongly dominated by old stellar populations, we determine radial-surface-brightness profiles from adaptive-optics images. Both of these galaxies are best fit by profiles close to exponentials, plus a compact nucleus comprising ~30% of the total light in one case and 8% in the other. Neither is well fit by an r^1/4-law profile. This apparent evidence for the formation of massive ~2 X 10^11 disks of old stars in the early universe indicates that at least some galaxies formed essentially monolithically, with high star-formation rates sustained over a few 10^8 years, and without the aid of major mergers.
description: 25 pages, 13 figures, accepted to ApJ