cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Efficient calculation of open quantum system dynamics and time-resolved spectroscopy with Distributed Memory HEOM (DM-HEOM)
Creators: name: Kramer, Tobias
name: Noack, Matthias
name: Reinefeld, Alexander
name: Rodriguez, Mirta
name: Zelinskyy, Yaroslav
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Time- and frequency resolved optical signals provide insights into the properties of light harvesting molecular complexes, including excitation energies, dipole strengths and orientations, as well as in the exciton energy flow through the complex. The hierarchical equations of motion (HEOM) provide a unifying theory, which allows one to study the combined effects of system-environment dissipation and non-Markovian memory without making restrictive assumptions about weak or strong couplings or separability of vibrational and electronic degrees of freedom. With increasing system size the exact solution of the open quantum system dynamics requires memory and compute resources beyond a single compute node. To overcome this barrier, we developed a scalable variant of HEOM. Our distributed memory HEOM, DM-HEOM, is a universal tool for open quantum system dynamics. It is used to accurately compute all experimentally accessible time- and frequency resolved processes in light harvesting molecular complexes with arbitrary system-environment couplings for a wide range of temperatures and complex sizes.
description: 28 pages, 13 figures
Konzernrechtliche Grenzen des Informationsflusses im aktienrechtlichen Konzern
Creators: name: Weber, Benjamin
Publisher: name: Studentische Zeitschrift für Rechtswissenschaft Heidelberg – Wissenschaft Online
Year: 2021

description: „Wissen ist Macht“. Dieses von Thomas Hobbes geprägte Sprichwort gilt auch innerhalb eines Konzerns. Denn das Wissen über den Zustand der einzelnen Untergesellschaften schafft eine Konzernleitungsmacht, die nötig ist, um den Konzern gut zu leiten. Das deutsche Konzernrecht beschränkt jedoch die Einflussnahme „von oben“ auf abhängige Gesellschaften. Dadurch könnte derInformationsfluss im Konzern, besonders im faktischen Konzern, gefährdet sein. Der Beitrag zeigt, dass auch im faktischen Konzern die Informationsweitergabe im Rahmen von § 311 Abs. 1 AktG zulässig ist und durch die Treuepflicht des herrschenden Unternehmens ein Schutz gegen Missbrauch der erlangten Informationen sichergestellt wird.
description: Studentische Zeitschrift für Rechtswissenschaft Heidelberg – Wissenschaft Online, Nr. 1 (2021): StudZR-WissOn
Uneven flows: On cosmic bulk flows, local observers, and gravity
Creators: name: Hellwing, Wojciech A.
name: Bilicki, Maciej
name: Libeskind, Noam I.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Using N-body simulations we study the impact of various systematic effects on the bulk flow (BF) and the Cosmic Mach Number (CMN). We consider two types of systematics: those related to survey properties and those induced by observer's location in the Universe. In the former category we model sparse sampling, velocity errors, and survey incompleteness. In the latter, we consider Local Group (LG) analogue observers, placed in a specific location within the Cosmic Web, satisfying various observational criteria. We differentiate such LG observers from Copernican ones, who are at random locations. We report strong systematic effects on the measured BF and CMN induced by sparse sampling, velocity errors and radial incompleteness. For BF most of these effects exceed 10\% for scales $R\leq100h^{-1}$Mpc. For CMN some of these systematics can be catastrophically large ($>50\%$) also on bigger scales. Moreover, we find that the position of the observer in the Cosmic Web significantly affects the locally measured BF (CMN), with effects as large as $\sim20\%$ ($30\%)$ at $R\leq50h^{-1}$Mpc for a LG-like observer as compared to a random one. This effect is comparable to the sample variance. To highlight the importance of these systematics, we additionally study a model of modified gravity (MG) with $\sim15\%$ enhanced growth rate. We found that the systematic effects can mimic the modified gravity signal. The worst-case scenario is realized for a case of a LG-like observer, when the effects induced by local structures are degenerate with the enhanced growth rate fostered by MG. Our results indicate that dedicated constrained simulations and realistic mock galaxy catalogs will be absolutely necessary to fully benefit from the statistical power of the forthcoming peculiar velocity data from surveys such as TAIPAN, WALLABY, Cosmic Flows-4 and SKA.
description: 20 pages, 9+2 figures, comments are welcomed
Dynamics of Circumstellar Disks II: Heating and Cooling
Creators: name: Nelson, Andrew F.
name: Benz, Willy
name: Ruzmaikina, Tamara
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a series of 2-d ($r,ϕ$) hydrodynamic simulations of marginally self gravitating disks around protostars using an SPH code. We implement simple dynamical heating and we cool each location as a black body, using a photosphere temperature obtained from the local vertical structure. We synthesize SEDs from our simulations and compare them to fiducial SEDs derived from observed systems. These simulations produce less distinct spiral structure than isothermally evolved systems, especially in the inner third of the disk. Pattern are similar further from the star but do not collapse into condensed objects. The photosphere temperature is well fit to a power law in radius with index $q\sim1.1$, which is very steep. Far from the star, internal heating ($PdV$ work and shocks) are not responsible for generating a large fraction of the thermal energy contained in the disk matter. Gravitational torques responsible for such shocks cannot transport mass and angular momentum efficiently in the outer disk. Within $\sim$5--10 AU of the star, rapid break up and reformation of spiral structure causes shocks, which provide sufficient dissipation to power a larger fraction of the near IR energy output. The spatial and size distribution of grains can have marked consequences on the observed near IR SED and can lead to increased emission and variability on $\lesssim 10$ year time scales. When grains are vaporized they do not reform into a size distribution similar to that from which most opacity calculations are based. With rapid grain reformation into the original size distribution, the disk does not emit near infrared photons. With a plausible modification to the opacity, it contributes much more.
description: Accepted by ApJ, 60pg incl 24 figures
Accreting pulsars: mixing-up accretion phases in transitional systems
Creators: name: Campana, Sergio
name: Di Salvo, Tiziana
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In the last 20 years our understanding of the millisecond pulsar (MSP) population changed dramatically. Thanks to RXTE, we discovered that neutron stars in LMXBs spins at 200-750 Hz frequencies, and indirectly confirmed the recycling scenario, according to which neutron stars are spun up to ms periods during the LMXB-phase. In the meantime, the continuous discovery of rotation-powered MSPs in binary systems in the radio and gamma-ray band (mainly with the Fermi LAT) allowed us to classify these sources into two "spiders" populations, depending on the mass of their companion stars: Black Widow, with very low-mass companion stars, and Redbacks, with larger companions possibly filling their Roche lobes but without accretion. It was soon regained that MSPs in short orbital period LMXBs are the progenitors of the spider populations of rotation-powered MSPs, although a direct link between accretion- and rotation-powered MSPs was still missing. In 2013 XMM-Newton spotted the X-ray outburst of a new accreting MSP (IGR J18245-2452) in a source that was previously classified as a radio MSP. Follow up observations of the source when it went back to X-ray quiescence showed that it was able to swing between accretion- to rotation-powered pulsations in a relatively short timescale (few days), promoting this source as the direct link between the LMXB and the radio MSP phases. Following discoveries showed that there exists a bunch of sources, which alternates X-ray activity phases, showing X-ray pulsations, to radio-loud phases, showing radio pulsations, establishing a new class of MSPs: the Transitional MSP. In this review we describe these exciting discoveries and the properties of accreting and transitional MSPs, highlighting what we know and what we have still to learn about in order to fully understand the (sometime puzzling) behavior of these systems and their evolutive connection (abridged).
description: 34 pages, 5 figures, invited review to the White Book of "NewCompStar" European COST Action MP1304
Additional file 9 of Comparative analysis of sucrose phosphate synthase (SPS) gene family between Saccharum officinarum and Saccharum spontaneum
Creators: name: Ma, Panpan
name: Zhang, Xingtan
name: Chen, Lanping
name: Zhao, Qian
name: Zhang, Qing
name: Hua, Xiuting
name: Wang, Zhengchao
name: Tang, Haibao
name: Yu, Qingyi
name: Zhang, Muqing
name: Ming, Ray
name: Zhang, Jisen
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 9. The information for probes used to identify SPS-containing BACs.
High maximum incidence of SARS-CoV-2 Delta and Omicron variants in children was associated with low cumulative infection rate and vaccination coverage in Estonia
Creators: name: Soeorg, Hiie
name: Abroi, Aare
name: Päll, Taavi
name: Avi, Radko
name: Sadikova, Olga
name: Sepp, Hanna
name: Reisberg, Tuuli
name: Lutsar, Irja
name: Huik, Kristi
Publisher: name: Zenodo
Year: 2024

description: Background. Increased risk of infection with SARS-CoV-2 Delta and Omicron variants in children has been suggested. We aimed to compare the maximum incidence of SARS-CoV-2 variants between children and adults.

Methods. Data on SARS-CoV-2-positive cases in 01.Feb.2021-01.May.2022 was obtained from Estonian Health Board. The 7-day incidence per 100,000 with the most common lineages was described with multinomial logistic regression, where lineage was imputed from the sequencing results of random samples. From the modelling results, the maximum incidence of lineages in children (<15 years) and adults (the remaining population) in four Estonian regions was derived. The difference in the maximum incidence between children and adults, considering region, was tested with negative binomial mixed effects model before and after taking into account cumulative infection rate, vaccination coverage, Containment and Health Index, and antigen testing at schools. 

Results. Altogether 87,949 cases in 218,015 children and 430,345 in 1,111,740 adults were identified. At the emergence of Delta, Omicron BA.1/BA.2, children had lower cumulative infection rates (median 6.5%, 15.3%/15.4%, respectively) than adults (11.6%, 17.5%/19.0%, respectively). The same applied for vaccination coverage (3.9%, 14.3%/14.8% vs. 50.9%, 65.2%/65.8%, respectively). In children, the maximum incidence of Delta (mean 106 (standard deviation 74) vs. 75 (52) per 100,000; p=0.007) and Omicron BA.1 (1,127 (507) vs. 735 (331); p=0.048) lineages was greater while BA.2 lineages was similar (833 (492) vs. 907 (535); p=0.70) compared to adults. In the adjusted model, the maximum incidence of all variants was lower in children compared to adults (Table), whereas the impact of antigen testing at schools was not significant.

Conclusion. Although not implying increased risk of infection, lower cumulative infection rate and vaccination coverage facilitated more extensive spread of Delta and Omicron BA.1 in children compared to adults.
Additional file 4 of Comparative analysis of sucrose phosphate synthase (SPS) gene family between Saccharum officinarum and Saccharum spontaneum
Creators: name: Ma, Panpan
name: Zhang, Xingtan
name: Chen, Lanping
name: Zhao, Qian
name: Zhang, Qing
name: Hua, Xiuting
name: Wang, Zhengchao
name: Tang, Haibao
name: Yu, Qingyi
name: Zhang, Muqing
name: Ming, Ray
name: Zhang, Jisen
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 4. Syntenic comparison of genomic DNA containing SPS genes among S. officinarum, S. spontaneum and S.bicolor. Homologs are indicated by arrows with same color. The asterisks indicate single-copied genes in the selected gene set.
Helix vivipara Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Bryozoa
Gastropoda
Stylommatophora
Helicidae
Helix
Helix vivipara

description: Helix vivipara [spec. nov.]
H. testa imperforata subovata obtusa cornea: cingulis fuscatis, apertura suborbiculari.
Fn. svec. 1312.
List. angl. 133. t. 2. f. 18. - - exerc. 2. p. 17. t. 2.
conch. 2. t. 126. f. 26.
Gvalt. test. t. 5. f. 1.
Swamm. bibl. t. 9. f. 3.
Habitat in Europae stagnis, argillosis imprimis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on pages 772-773, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 1: of IL-8/CXCR1/2 signalling promotes tumor cell proliferation, invasion and vascular mimicry in glioblastoma
Creators: name: Sharma, Ira
name: Avninder Singh
name: Siraj, Fouzia
name: Saxena, Sunita
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Table S1. Gene wise primer sequence. (DOCX 15 kb)
The multiplication of contexts
Creators: name: Sherratt, Tim
Publisher: name: Zenodo
Year: 2019
Subjects: data
humanities
play
Trove
Hansard
National Archives of Australia

description: I play with data. I think there's an important argument to be made for the role of play in research, particularly when confronted with large, heterogenous datasets, but what does it really mean? In this paper I want to explore the meanings of 'play' within digital cultural heritage. I play with collections. From Twitter bots to redaction art, I build things using the holdings of cultural heritage collections that are often both playful and political. By reflecting on the characteristics of these works, I want to explore the multiplication of contexts as a method for generating new perspectives and new knowledge. Is this the serious business of data play?
description: Presented at the University of Canberra as part of the Centre for Creative and Cultural Research's seminar series in 2017.
The HST Key Project on the Extragalactic Distance Scale XXV. A Recalibration of Cepheid Distances to Type Ia Supernovae and the Value of the Hubble Constant
Creators: name: Gibson, Brad K.
name: Stetson, Peter B.
name: Freedman, Wendy L.
name: Mould, Jeremy R.
name: Kennicutt,, Robert C.
name: Huchra, John P.
name: Sakai, Shoko
name: Graham, John A.
name: Fassett, Caleb I.
name: Kelson, Daniel D.
name: Ferrarese, Laura
name: Hughes, Shaun M. G.
name: Illingworth, Garth D.
name: Macri, Lucas M.
name: Madore, Barry F.
name: Sebo, Kim M.
name: Silbermann, Nancy A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Cepheid-based distances to seven Type Ia supernovae (SNe)-host galaxies have been derived using the standard HST Key Project on the Extragalactic Distance Scale pipeline. For the first time, this allows for a transparent comparison of data accumulated as part of three different HST projects, the Key Project, the Sandage et al. Type Ia SNe program, and the Tanvir et al. Leo I Group study. Re-analyzing the Tanvir et al. galaxy and six Sandage et al. galaxies we find a mean (weighted) offset in true distance moduli of 0.12+/-0.07 mag -- i.e., 6% in linear distance -- in the sense of reducing the distance scale, or increasing H0. Adopting the reddening-corrected Hubble relations of Suntzeff et al. (1999), tied to a zero point based upon SNe~1990N, 1981B, 1998bu, 1989B, 1972E and 1960F and the photometric calibration of Hill et al. (1998), leads to a Hubble constant of H0=68+/-2(random)+/-5(systematic) km/s/Mpc. Adopting the Kennicutt et al. (1998) Cepheid period-luminosity-metallicity dependency decreases the inferred H0 by 4%. The H0 result from Type Ia SNe is now in good agreement, to within their respective uncertainties, with that from the Tully-Fisher and surface brightness fluctuation relations.
description: Accepted for publication in The Astrophysical Journal. 62 pages, LaTeX, 9 Postscript figures. Also available at http://casa.colorado.edu/~bgibson/publications.html
Controlled viscosity in dense granular materials
Creators: name: Gnoli, A.
name: de Arcangelis, L.
name: Giacco, F.
name: Lippiello, E.
name: Ciamarra, M. Pica
name: Puglisi, A.
name: Sarracino, A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We experimentally investigate the fluidization of a granular material subject to mechanical vibrations by monitoring the angular velocity of a vane suspended in the medium and driven by an external motor. On increasing the frequency we observe a re-entrant transition, as a jammed system first enters a fluidized state, where the vane rotates with high constant velocity, and then returns to a frictional state, where the vane velocity is much lower. While the fluidization frequency is material independent, the viscosity recovery frequency shows a clear dependence on the material, that we rationalize by relating this frequency to the balance between dissipative and inertial forces in the system. Molecular dynamics simulations well reproduce the experimental data, confirming the suggested theoretical picture.
description: 6 pages, 5 figures + supplemental material, accepted for publication in PRL
Mass formulae and natural hierarchy in string effective supergravities
Creators: name: Ferrara, S.
name: Kounnas, C.
name: Zwirner, F.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study some conditions for the hierarchy $m_{3/2} << M_P$ to occur naturally in a generic effective supergravity theory. Absence of fine-tuning and perturbative calculability require that the effective potential has a sliding gravitino mass and vanishing cosmological constant, up to ${\cal O}(m_{3/2}^4)$ corrections. In particular, cancellation of quadratically divergent contributions to the one-loop effective potential should take place, including the `hidden sector' of the theory. We show that these conditions can be met in the effective supergravities derived from four-dimensional superstrings, with supersymmetry broken either at the string tree level via compactification, or by non-perturbative effects such as gaugino condensation. A crucial role is played by some approximate scaling symmetries, which are remnants of discrete target-space dualities in the large moduli limit. We derive explicit formulae for the soft breaking terms arising from this class of `large hierarchy compatible' (LHC) supergravities.
description: 40 pages, no figures, CERN-TH.7192/94, LPTENS -94/12, UCLA/94/TEP13 (plain LATEX, to be run twice). Some trivial misprints and references have been corrected
Hermitian--to--quasi-Hermitian quantum phase transitions
Creators: name: Znojil, Miloslav
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The phenomenon of quantum phase transition is considered in the special case in which the evolution laws remain unitary and in which the bound-state energies remain observable. The conventional Hermiticity of observables is lost at the interface, replaced by the so called quasi-Hermiticity. Several features of the passage of the system through the interface are discussed and illustrated by elementary illustrative ${\cal PT}-$symmetric examples.
description: 24 pp., 5 figures
title: Ψηφιακά Δίδυμα: Εφαρμογές στην εκπαιδευτική ρομποτική
title: Digital twins in educational robotics
Creators: name: Γλυνος Ευαγγελος
Publisher: name: Technical University of Crete
Year: 2021

description: Τα τελευταία χρόνια η μεθοδολογία STEM (Science, Technology, Engineering and Mathematics) και η εκπαιδευτική ρομποτική κερδίζουν σταδιακά έδαφος στα προγράμματα σπουδών των σχολείων της Πρωτοβάθμιας και Δευτεροβάθμιας Εκπαίδευσης αλλά και σε εξωσχολικές εκπαιδευτικές δραστηριότητες. Παράλληλα νέα εργαλεία, κυρίως από την περιοχή των ΤΠΕ, έχουν αρχίσει να αναπτύσσονται στα πλαίσια του Industry 4.0, αλλά η χρήση τους σε διαφορετικές περιοχές, όπως είναι η εκπαιδευτική διαδικασία είναι περιορισμένη. Ένα σχετικό εργαλείο αποτελούν και τα ψηφιακά δίδυμα, που ορίζονται ως η ψηφιακή αποτύπωση ενός φυσικού αντικειμένου που περιέχει όλες τις ιδιότητες, πληροφορίες και καταστάσεις του πραγματικού αντικειμένου. Στα πλαίσια της παρούσας διπλωματικής εργασίας αναπτύχθηκε ένα ψηφιακό δίδυμο ενός πρωτότυπου πραγματικού συστήματος εκπαιδευτικής ρομποτικής. Μέσω του ψηφιακού διδύμου ο εκπαιδευτής έχει τη δυνατότητα να παρακολουθεί, να καταγράφει, να ελέγχει, να αξιολογεί, να αναπροσαρμόζει και στη συνέχεια να επεμβαίνει στη μαθησιακή διαδικασία με στόχο την βελτιστοποίηση της επίτευξης των σχετικών μαθησιακών αποτελεσμάτων, μέσω κατάλληλων μαθησιακών σεναρίων.
Additional file 11 of Antagonistic effects of mitochondrial matrix and intermembrane space proteases on yeast aging
Creators: name: Vega, Montserrat
name: Castillo, David
name: de Cubas, Laura
name: Wang, Yirong
name: Huang, Ying
name: Hidalgo, Elena
name: Cabrera, Margarita
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Virology
subject: Computational Biology

description: Additional file 11: Table S4. Yeast strains used in this study.
An ASCA Study of the Heavy Element Distribution in Clusters of Galaxies
Creators: name: Finoguenov, A.
name: David, L. P.
name: Ponman, T. J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We perform a spatially resolved X-ray spectroscopic study of a set of 11 relaxed clusters of galaxies observed by the ROSAT/PSPC and ASCA/SIS. Using a method which corrects for the energy dependent effects of the ASCA PSF based on ROSAT images, we constrain the spatial distribution of Ne, Si, S and Fe in each cluster. Theoretical prescriptions for the chemical yields of Type Ia and II supernovae, then allow determination of the Fe enrichment from both types of supernovae as a function of radius within each cluster. Using optical measurements from the literature, we also determine the iron mass-to-light ratio (IMLR) separately for Fe synthesized in both types of supernovae. For clusters with the best photon statistics, we find that the total Fe abundance decreases significantly with radius, while the Si abundance is either flat or decreases less rapidly, resulting in an increasing Si/Fe ratio with radius. This result indicates a greater predominance of Type II SNe enrichment at large radii in clusters. We suggest that the high Si/Fe ratios in the outskirts of rich clusters may arise from enrichment by Type II SNe released to ICM via galactic star burst driven winds. Abridged.
description: 17 pages, ApJ in press (Nov. 2000), a study of systematics is added
Infall and Outflow Motions towards a Sample of Massive Star Forming Regions from the RMS Survey
Creators: name: Cunningham, Nichol
name: Lumsden, Stuart
name: Moore, Toby
name: Maud, Luke
name: Mendigutia, Ignacio.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the results of an outflow and infall survey towards a distance limited sample of 31 massive star forming regions drawn from the RMS survey. The presence of young, active outflows is identified from SiO (8-7) emission and the infall dynamics are explored using HCO$^+$/H$^{13}$CO$^+$ (4-3) emission. We investigate if the infall and outflow parameters vary with source properties, exploring whether regions hosting potentially young active outflows show similarities or differences with regions harbouring more evolved, possibly momentum driven, "fossil" outflows. SiO emission is detected towards approximately 46% of the sources. When considering sources with and without an SiO detection (i.e. potentially active and fossil outflows respectively), only the $^{12}$CO outflow velocity shows a significant difference between samples, indicating SiO is more prevalent towards sources with higher outflow velocities. Furthermore, we find the SiO luminosity increases as a function of the Herschel 70$μ$m to WISE 22$μ$m flux ratio, suggesting the production of SiO is prevalent in younger, more embedded regions. Similarly, we find tentative evidence that sources with an SiO detection have a smaller bolometric luminosity-to-mass ratio, indicating SiO (8-7) emission is associated with potentially younger regions. We do not find a prevalence towards sources displaying signatures of infall in our sample. However, the higher energy HCO$^+$ transitions may not be the best suited tracer of infall at this spatial resolution in these regions.
description: Accepted for publication in MNRAS
Additional file 8 of Comparative analysis of sucrose phosphate synthase (SPS) gene family between Saccharum officinarum and Saccharum spontaneum
Creators: name: Ma, Panpan
name: Zhang, Xingtan
name: Chen, Lanping
name: Zhao, Qian
name: Zhang, Qing
name: Hua, Xiuting
name: Wang, Zhengchao
name: Tang, Haibao
name: Yu, Qingyi
name: Zhang, Muqing
name: Ming, Ray
name: Zhang, Jisen
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 8. Correlation analysis between the expression of SPS genes and content of the metabolites in gradient developmental leaves (A, left) and stems (B, right) in Saccharum. The correlation coefficient (R2) and dependent equation of each groups data is marked near the correlation curve. R2 > 0.9 was considered to be significantly correlated.
Flavour Dependence of Form Factors in Heavy Meson Decays
Creators: name: Close, F. E.
name: Wambach, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Recently we have shown that due account of Wigner spin rotations is needed to match the ISGW model consistently onto HQET. We now discuss the flavour dependence of this procedure. We find that for finite mass ``heavy'' quark the universal function $ξ(y=1) \approx 1$ but the slope is proportional to the energy of the spectator quarks, and ratios of form factors are corrected in a way that QCD sum rules seem to require. Predictions for heavy quarks, such as in $B_c \rightarrow ψ(η_c)$ and to mixed systems, such as $D\rightarrow K$ and $B \rightarrow π$ show a systematic mass dependence that may be confronted with data.
description: 10 pages, 3 figures (ps file available upon request), RAL-94-041, OUTP-94 09P
The Intergalactic Medium and Soft X-ray Background
Creators: name: Cen, Renyue
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I present an overview of some of the recent advances in our understanding of the distribution and evolution of the ordinary, baryonic matter in the universe. Two observations that strongly suggest that most of the baryons seen at high redshift ($z\ge 2$) have turned into some forms yet undetected at $z=0$ are highlighted. With the aid of large-scale cosmological hydrodynamic simulations, it is shown that most of the baryons today are in a gaseous form with a temperature of $10^5-10^7~$Kelvin -- the "warm/hot gas", shock heated during the gravitational collapse and formation of the large-scale structure at low redshift. Primarily line emissions from this warm/hot gas may account for a large fraction of the residual (after removal of identifiable discrete sources) soft X-ray background at $hν< 1.0$keV. How this warm/hot gas may be detected by the next generation of EUV and soft X-ray instruments is indicated. Detection or non-detection of this warm/hot gas will have profound implications for cosmology.
description: An invited overview presented at "Small Missions for Energetic Astrophysics", Los Alamos, March 1999, full paper with color figures can be obtained at http://astro.princeton.edu/~cen/PROJECTS/p1/p1.html
Bootstrap validation of links of a minimum spanning tree
Creators: name: Musciotto, Federico
name: Marotta, Luca
name: Miccichè, Salvatore
name: Mantegna, Rosario N.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Methodology (stat.ME)
subject: FOS: Computer and information sciences

description: We describe two different bootstrap methods applied to the detection of a minimum spanning tree obtained from a set of multivariate variables. We show that two different bootstrap procedures provide partly distinct information that can be highly informative about the investigated complex system. Our case study, based on the investigation of daily returns of a portfolio of stocks traded in the US equity markets, shows the degree of robustness and completeness of the information extracted with popular information filtering methods such as the minimum spanning tree and the planar maximally filtered graph. The first method performs a "row bootstrap" whereas the second method performs a "pair bootstrap". We show that the parallel use of the two methods is suggested especially for complex systems presenting both a nested hierarchical organization together with the presence of global feedback channels.
description: 17 pages, 7 figures
Additional file 1 of Routine clinical care data from thirteen cardiac outpatient clinics: design of the Cardiology Centers of the Netherlands (CCN) database
Creators: name: Bots, Sophie H.
name: Siegersma, Klaske R.
name: Onland-Moret, N. Charlotte
name: Asselbergs, Folkert W.
name: Somsen, G. Aernout
name: Tulevski, Igor I.
name: den Ruijter, Hester M.
name: Hofstra, Leonard
Publisher: name: figshare
Year: 2021
Subjects: subject: Information Systems
subject: FOS: Computer and information sciences

description: Additional file 1. Supplementary figure and tables.
Helix nemoralis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Bryozoa
Gastropoda
Stylommatophora
Helicidae
Helix
Helix nemoralis

description: Helix nemoralis [spec. nov.]
H. testa imperforata subrotunda laevi diaphana fasciata, apertura subrotundo-lunata.
List. angl. 116. t. 2. f. 3. - - conch. t. 1. n. 54.
Pet. mus. 5. n. 14.
Gualt. test. t. 1. f. P.
Habitat in Europae arboribus.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 773, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 2: of Teledermatology scale-up frameworks: a structured review and critique
Creators: name: Laticha Walters
name: Scott, Richard
name: Mars, Maurice
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy
subject: Computational Biology

description: Detailed results of the TD requirements mapping to identified frameworks. Detailed listing of the results of the TD requirements mapping to the components of the identified frameworks (DOCX 248Â kb)
Newly discovered brown dwarfs not seen in microlensing time scale frequency distribution?
Creators: name: Peale, S. J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The 2-Micron All Sky Survey (2MASS) (Skrutskie et al. 1997) and the DEep Near Infrared Survey of the southern sky (DENIS) (Epchtein et al. 1997) have revealed a heretofore unknown population of free brown dwarfs that has extended the local mass function down to as small as 0.01M_sun (Reid et al. 1999). If this local proportion of brown dwarfs extends throughout the Galaxy---in particular in the Galactic bulge---one expects an increase in the predicted fraction of short time scale microlensing events in directions toward the Galactic bulge. Zhao et al.(1996) have indicated that a mass function with 30-60% of the lens mass in brown dwarfs is not consistent with empirical microlensing data. Here we show that even the much lower mass fraction (~ 10%) of brown dwarfs inferred from the new discoveries appears inconsistent with the data. The added brown dwarfs do indeed increase the expected number of short time scale events, but they appear to drive the peak in the time scale frequency distribution to time scales smaller than that observed, and do not otherwise match the observed distribution. A reasonably good match to the empirical data (Alcock et al. 1996) is obtained by increasing the fraction of stars in the range 0.08
description: 5 pages, 1 figure. PS file using aas2pp4.sty. To appear in ApJ Letters
Rogue active regions and the inherent unpredictability of the solar dynamo
Creators: name: Petrovay, K.
name: Nagy, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: New developments in surface flux transport modeling and theory of flux transport dynamos have given rise to the notion that certain large active regions with anomalous properties (location, tilt angle and/or Hale/non-Hale character) may have a major impact on the course of solar activity in subsequent years, impacting also on the amplitude of the following solar cycles. Here we discuss our current understanding of the role of such "rogue" active regions in cycle-to-cycle variations of solar activity.
description: Proc. IAU Symp. 340. 6 pages, 2 figures, 1 table
The nexus of inhabitants and impervious surfaces at city scale — wastewater and stormwater travel time distributions and an approach to calibrate diurnal variations
Creators: name: Kaeseberg, Thomas
name: Kaeseberg, Michael
name: Zhang, Jin
name: Jawitz, James W.
name: Krebs, Peter
name: Suresh C. Rao, P.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: Space Science
Environmental Sciences not elsewhere classified
Chemical Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Information Systems not elsewhere classified
Mathematical Sciences not elsewhere classified

description: We present an approach to calibrate dry weather flow patterns of people in eight subnetworks of Dresden, Germany. The monitored data was pre-processed, and SWMM model runs were performed. Congruence of modelled results and observed data was evaluated with the Nash-Sutcliffe Efficiency (NSE). New diurnal variation patterns of dry weather flow were quantified based on the presented calibration approach. Most of the modelled hydrographs exceeded an NSE of 0.9 just after the second SWMM model run, which is a sign of model adequacy. Travel time distributions (TTDs) of upstream wastewater from connected people and stormwater from impervious surfaces of the monitored locations were determined, and a dynamic index ƒiA-PE(k) was proposed, determined and its adequacy was assessed. In general, TTDs confirmed a lower population density and a less meshed urban drainage network in the outer parts of Dresden. The functional information within ƒiA-PE(k) considers development characteristics among the subnetworks and within a subnetwork of interest. The presented index is useful to evaluate prospective strategies of developments and the implementation of green and blue infrastructures in residential areas.
Additional file 1: of Methods to discriminate primary from secondary dengue during acute symptomatic infection
Creators: name: Nguyen, Thi
name: Clapham, Hannah
name: Phung, Khanh
name: Nguyen, Thanh
name: DInh, The
name: Nguyen, Than
name: Tran, Van Ngoc
name: Whitehead, Stephen
name: Simmons, Cameron
name: Wolbers, Marcel
name: Wills, Bridget
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Table S1. Validation of the all-inclusive models. (PDF 87 kb)
Correlation Analysis of SFI Peculiar Velocities
Creators: name: Borgani, S.
name: da Costa, L. N.
name: Zehavi, I.
name: Giovanelli, R.
name: Haynes, M.
name: Freudling, W.
name: Wegner, G.
name: Salzer, J. J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results of a statistical analysis of the SFI catalog of peculiar velocities, a recently completed survey of spiral field galaxies with I-band Tully-Fisher distances (Haynes et al. 1999). The velocity field statistic utilized is the velocity correlation function, $ψ_1(r)$ (Gorski et al. 1989). The analysis is performed in redshift space, so as to circumvent potential ambiguities connected with inhomogeneous Malmquist bias corrections. The results from the SFI sample are compared with linear-theory predictions. We generate a large set of mock samples, extracted from N-body simulations, which are used to assess the reliability of our analysis and to estimate the associated uncertainties. Defining $η_8=σ_8Ω_0^{0.6}$, we find that the measured $ψ_1(r)$ implies a degenerate constraint in the $η_8-Γ$ plane, with $η_8=(0.3 +/- 0.1) (Γ/0.2)^{0.5}$, at the $2σ$ level, for the inverse Tully-Fisher (ITF) calibration presented in this paper. Model constraints are quite sensitive to the ITF calibration. The other ITF calibrations by Giovanelli et al. (1997) and da Costa et al. (1998) both give, for $Γ=0.2$, $η_8\simeq 0.6$ as the best-fitting value.
description: 12 pages, 6 figures, LateX, uses apj.sty, AJ, in press, December 1999 issue
Additional file 10 of The wild strawberry kinome: identification, classification and transcript profiling of protein kinases during development and in response to gray mold infection
Creators: name: Liu, Hui
name: Qu, Wei
name: Zhu, Kaikai
name: Cheng, Zong-Ming ( Max)
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 10: Figure S3. A heatmap of the expression data of strawberry kinase genes in cluster 2 in 16 different strawberry tissues and developmental stages.
Additional file 12 of The wild strawberry kinome: identification, classification and transcript profiling of protein kinases during development and in response to gray mold infection
Creators: name: Liu, Hui
name: Qu, Wei
name: Zhu, Kaikai
name: Cheng, Zong-Ming ( Max)
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 12: Figure S5. A heatmap of the expression data of strawberry kinase genes in cluster 4 in 16 different strawberry tissues and developmental stages.
Ab-initio calculations of the linear and nonlinear susceptibilities of N$_2$, O$_2$, and air in the mid-infrared
Creators: name: Brown, Jeffrey M.
name: Couairon, Arnaud
name: Gaarde, Mette B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We present first-principles calculations of the linear and nonlinear susceptibilities of N$_2$, O$_2$, and air in the mid-infrared wavelength regime, from $1-4$ $μ$m. We extract the frequency-dependent susceptibilities from the full time-dependent dipole moment that is calculated using time-dependent density functional theory. We find good agreement with curves derived from experimental results for the linear susceptibility, and with measurements for the nonlinear susceptibility up to 2.4 $μ$m. We also find that the susceptibilities are insensitive to the laser intensity even in the strong field regime up to $5\times 10^{13}$ W/cm$^2$. Our results will allow accurate calculations of the long-distance propagation of intense MIR laser pulses in air.
The Problem of Long-Time Agricultural Adjustment
Creators: name: Tolley, H. R.
Publisher: name: Unknown
Year: 1934
Subjects: Agricultural and Food Policy
Crop Production/Industries
International Relations/Trade
Land Economics/Use

description: Before this audience, I shall not have to recount step by step our drive for agricultural adjustment to date. I take it that you are familiar with what has been done. I do want, however, to try at the outset with broad strokes, to draw the whole picture together. The main fact is that we had to get some 40 million acres of land retired from production, and that we are now in the midst of forced emergency maneuvers to that end. During the World War some 50 million acres in Europe, not counting Russia, went out of cultivation. The United States brought about 40 million more acres into cultivation and geared up its whole farm plant into a higher production. After the war we kept it up. We kept on farming as if there were still great hungry foreign markets crying for our crops. In reality, such markets were rapidly dwindling. The world owed us money; we would not accept goods in return. With our tariff wall as it was, and still is, the only way we could keep up the appearance of a great foreign custom was to lend those other nations more and more money with which to keep on taking our food and fabrics. This is what we did until about 1938. Finally we got enough to quit it; the false front of our foreign markets at once collapsed; and we had at last to face the fact that we were farming at least 40 million acres too much land.
description: Address by H.R. Tolley, Assistant Administrator, Agricultural Adjustment Administration, at Farmers’ Week, the Ohio State University, Columbus, Ohio, 11 A.M., January 31, 1944.
On Truncations of the Exact Renormalization Group
Creators: name: Morris, Tim R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate the Exact Renormalization Group (ERG) description of ($Z_2$ invariant) one-component scalar field theory, in the approximation in which all momentum dependence is discarded in the effective vertices. In this context we show how one can perform a systematic search for non-perturbative continuum limits without making any assumption about the form of the lagrangian. Concentrating on the non-perturbative three dimensional Wilson fixed point, we then show that the sequence of truncations $n=2,3,\dots$, obtained by expanding about the field $φ=0$ and discarding all powers $φ^{2n+2}$ and higher, yields solutions that at first converge to the answer obtained without truncation, but then cease to further converge beyond a certain point. No completely reliable method exists to reject the many spurious solutions that are also found. These properties are explained in terms of the analytic behaviour of the untruncated solutions -- which we describe in some detail.
description: 15 pages (with figures), Plain TeX, uses psfig, 5 postscript figures appended as uuencoded compressed tar file, SHEP 93/94-23, CERN-TH.7281/94. (Corrections of typos, and small additions to improve readability: version to be published in Phys. Lett. B)
An arbuscular mycorrhizal fungus increased the macroaggregate proportion and reduced cadmium leaching from polluted soil
Creators: name: Zhang, Jinxiu
name: Su, Lin
name: Yan, Kai
name: Li, Mingrui
name: He, Yongmei
name: Zu, Yanqun
name: Zhan, Fangdong
name: Li, Tao
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Plant Biology

description: A pot experiment was conducted using maize (Zea mays L.) as the host plant grown in cadmium (Cd)-polluted soil and inoculated with an arbuscular mycorrhizal fungus (AMF), Funneliformis mosseae. The effects of AMF on Cd uptake by maize, water-stable aggregate proportion, Cd concentration in pore water and Cd leaching were investigated. The results showed that AMF significantly promoted maize biomass and Cd uptake in shoots, and increased the content of total and easily extractable glomalin-related soil protein in the 0–40 cm soil layers. Furthermore, AMF increased the proportion of >0.85 mm water-stable aggregates (macroaggregates) by 47–88% and decreased the available Cd content in soil by 20–24%. During the first and second leaching events, AMF significantly decreased the Cd concentration in pore water, and reduced the Cd leaching loss from soil by 12.6% and 19.9%, respectively. Correlation analysis indicated that the macroaggregate proportion was positively correlated with the total and easily extractable glomalin-related soil protein content and negatively correlated with the Cd concentration in pore water, and the Cd concentration in pore water was positively correlated with the Cd leaching loss from soil. Therefore, the AMF-reduced Cd leaching was closely related to the increased macroaggregate proportion in soil. AMF significantly increased the GRSP content and the macroaggregate proportion in soil, which contributed to reducing the Cd concentration in pore water and its leaching loss from soil.
Outer membrane vesicles induce the mussel plantigrade settlement via regulation of c-di-GMP
Creators: name: Wu, Guanju
name: Hu, Xiao-Meng
name: Peng, Li-Hua
name: Zhang, Wen
name: Liang, Xiao
name: Dobretsov, Sergey
name: Yang, Jin-Long
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Evolutionary Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Marine Biology
subject: Infectious Diseases
subject: FOS: Health sciences

description: Despite the importance of outer membrane vesicles (OMVs) in benthic animal settlement, the underlying molecular mechanism remains elusive. Here, the impact of OMVs and OMVs synthesis-related tolB gene in Mytilus coruscus plantigrade settlement was tested. The OMVs were extracted from Pseudoalteromonas marina through density gradient centrifugation, and a tolB knockout strain, achieved by homologous recombination, was utilized for the investigation. Our results demonstrated that OMVs could significantly enhance M. coruscus plantigrades settlement. Deleting the tolB resulted in downregulation of c-di-GMP, accompanied by a reduction of OMV production, a decline in bacterial motility and increasing biofilm-forming ability. Enzyme treatment resulted in a 61.11% reduction in OMV-inducing activity and a 94.87% reduction in LPS content. Thus, OMVs regulate mussel settlement via LPS, and c-di-GMP is responsible for the OMV-inducing capacity. These findings provide new insights into the interactions between bacteria and mussels.