cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Imitation versus payoff - duality of the decision-making process demonstrates criticality and consensus formation
Creators: name: Turalska, Malgorzata
name: West, Bruce J.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: We consider a dual model of decision making, in which an individual forms its opinion based on contrasting mechanisms of imitation and rational calculation. The decision making model (DMM) implements imitating behavior by means of a network of coupled two-state master equations that undergoes a phase transition at a critical value of a control parameter. The evolutionary spatial game (EGM), being a generalization of the Prisoner's dilemma game, is used to determine in objective fashion the cooperative or anti-cooperative strategy adopted by individuals. Interactions between two sources of dynamics increases the domain of initial states attracted to phase transition dynamics beyond that of the DMM network in isolation. Additionally, on average the influence of the DMM on the game increases the final observed fraction of cooperators in the system.
A longitudinal study of NADC34-like strains in an intensive farm unravels divergent evolution
Creators: name: 徐思佳
Publisher: name: CNGB
Year: 2023
Subjects: Genome sequencing
Other
serum
Evolution

description: Two PRRSV strains, GDHZ109/2020 and GDYS162/2022, were isolated and fully se-quenced from the same swine farm in Guangdong Province in 2020 and 2022, respectively. Recombination analysis suggested complex recombination patterns for both strains, involving NADC30-like, NADC34-like, and JXA1-like strains. Pathogenicity experiments conducted on piglets demon-strated that GDHZ109/2020 exhibited higher pathogenicity compared to GDYS162/2022. Piglets in the GDHZ109/2020 infected group had more severe clinical signs and higher mortality.
Persistent ferromagnetism and topological phase transition at the interface of a superconductor and a topological insulator
Creators: name: Qin, Wei
name: Zhang, Zhenyu
Publisher: name: arXiv
Year: 2014
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: At the interface of an s-wave superconductor and a three-dimensional topological insulator, Ma- jorana zero modes and Majorana helical states have been proposed to exist respectively around magnetic vortices and geometrical edges. Here we first show that a single magnetic impurity at such an interface splits each resonance state of a given spin channel outside the superconducting gap, and also induces two new symmetric impurity states inside the gap. Next we find that an increase in the superconducting gap suppresses both the oscillation magnitude and period of the RKKY inter- action between two interface magnetic impurities mediated by BCS quasi-particles. Within a mean field approximation, the ferromagnetic Curie temperature is found to be essentially independent of the superconducting gap, an intriguing phenomenon due to a compensation effect between the short-range ferromagnetic and long-range anti-ferromagnetic interactions. The existence of persis- tent ferromagnetism at the interface allows realization of a novel topological phase transition from a non-chiral to a chiral superconducting state at sufficiently low temperatures, providing a new platform for topological quantum computation.
description: 5 pages, 3 figures
The need for focused, hard X-ray investigations of the Sun
Creators: name: Glesener, Lindsay
name: Shih, Albert Y.
name: Caspi, Amir
name: Milligan, Ryan
name: Hudson, Hugh
name: Oka, Mitsuo
name: Buitrago-Casas, Juan Camilo
name: Guo, Fan
name: Ryan, Dan
name: Kontar, Eduard
name: Veronig, Astrid
name: Hayes, Laura A.
name: Inglis, Andrew
name: Golub, Leon
name: Vilmer, Nicole
name: Gary, Dale
name: Reid, Hamish
name: Hannah, Iain
name: Kerr, Graham S.
name: Reeves, Katharine K.
name: Allred, Joel
name: Guidoni, Silvina
name: Yu, Sijie
name: Christe, Steven
name: Musset, Sophie
name: Dennis, Brian
name: Oliveros, Juan Carlos Martínez
name: Athiray, P. S.
name: Vievering, Juliana
name: White, Stephen
name: Winebarger, Amy
name: Drake, James
name: Jeffrey, Natasha
name: Antiochos, Spiro
name: Duncan, Jessie
name: Zhang, Yixian
name: Alaoui, Meriem
name: Simões, Paulo J. A.
name: Battaglia, Marina
name: Setterberg, William
name: Masek, Reed
name: Chen, Thomas Y.
name: Peterson, Marianne
name: Krucker, Säm
name: Temmer, Manuela
name: Saint-Hilaire, Pascal
name: Petrosian, Vahe
name: Knuth, Trevor
name: Moore, Christopher S.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Understanding the nature of energetic particles in the solar atmosphere is one of the most important outstanding problems in heliophysics. Flare-accelerated particles compose a huge fraction of the flare energy budget; they have large influences on how events develop; they are an important source of high-energy particles found in the heliosphere; and they are the single most important corollary to other areas of high-energy astrophysics. Despite the importance of this area of study, this topic has in the past decade received only a small fraction of the resources necessary for a full investigation. For example, NASA has selected no new Explorer-class instrument in the past two decades that is capable of examining this topic. The advances that are currently being made in understanding flare-accelerated electrons are largely undertaken with data from EOVSA (NSF), STIX (ESA), and NuSTAR (NASA Astrophysics). This is despite the inclusion in the previous Heliophysics decadal survey of the FOXSI concept as part of the SEE2020 mission, and also despite NASA's having invested heavily in readying the technology for such an instrument via four flights of the FOXSI sounding rocket experiment. Due to that investment, the instrumentation stands ready to implement a hard X-ray mission to investigate flare-accelerated electrons. This white paper describes the scientific motivation for why this venture should be undertaken soon.
description: White paper submitted to the Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033; 15 pages, 5 figures
SAMI-HI: the connection between global asymmetry in the ionised and neutral atomic hydrogen gas in galaxies
Creators: name: Watts, Adam B.
name: Cortese, Luca
name: Catinella, Barbara
name: Power, Chris
name: Fraser-McKelvie, Amelia
name: Bryant, Julia J.
name: Croom, Scott M.
name: van de Sande, Jesse
name: Bland-Hawthorn, Joss
name: Groves, Brent
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Observations of the neutral atomic hydrogen (HI) gas in galaxies are predominantly spatially unresolved, in the form of a global HI spectral line. There has been substantial work on quantifying asymmetry in global HI spectra (`global HI asymmetry'), but due to being spatially unresolved, it remains unknown what physical regions of galaxies the asymmetry traces, and whether the other gas phases are affected. Using optical integral field spectrograph (IFS) observations from the Sydney AAO Multi-object IFS (SAMI) survey for which global HI spectra are also available (SAMI-HI), we study the connection between asymmetry in galaxies' ionised and neutral gas reservoirs to test if and how they can help us better understand the origin of global HI asymmetry. We reconstruct the global H$α$ spectral line from the IFS observations and find that, while some global H$α$ asymmetries can arise from disturbed ionised gas kinematics, the majority of asymmetric cases are driven by the distribution of H$α$-emitting gas. When compared to the HI, we find no evidence for a relationship between the global H$α$ and HI asymmetry. Further, a visual inspection reveals that cases where galaxies have qualitatively similar H$α$ and HI spectral profiles can be spurious, with the similarity originating from an irregular 2D H$α$ flux distribution. Our results highlight that comparisons between global H$α$ and HI asymmetry are not straightforward, and that many global HI asymmetries trace disturbances that do not significantly impact the central regions of galaxies.
description: 11 pages, 6 figures, 1 appendix, accepted for publication in MNRAS
title: La prévention de l'infirmière scolaire auprès des jeunes adolescents présentant des consommations d'alcool problématiques
title: La prévention de l'infirmière scolaire auprès des jeunes adolescents présentant des consommations d'alcool problématiques
titleType: AlternativeTitle
Creators: name: Tille, Cynthia
name: Zurkinden, Maude
Publisher: name: Unknown
Year: 0
Subjects: subject: Soins infirmiers
subject: Préventions
subject: Adolescents
subject: Consommation d’alcool
subject: Contexte scolaire

description: Contexte : En Suisse, la proportion des jeunes âgés entre onze et quinze ans ayant déjà consommé de l’alcool est élevée. La diminution de l’âge des consommateurs ainsi que la modification du mode de consommation sont deux phénomènes préoccupants. L’infirmière scolaire possède des compétences pour agir sur ce problème. Objectif : Le but de ce travail est d’identifier des facteurs qui pourraient améliorer la prévention effectuée par l’infirmière scolaire auprès des jeunes adolescents, âgés entre onze et seize ans, présentant des consommations problématiques d’alcool et ainsi pouvoir proposer des pistes de prévention contre l’alcool. Méthode : Six articles tirés des bases de données CINAHL et PubMed ont été analysés et présentés sous forme de tableaux synthétiques. Les résultats ont été mis en lien avec le cadre théorique, qui est le modèle de la promotion de la santé de Nola Pender. Résultats : Les caractéristiques et expériences personnelles des adolescents, l’entourage ainsi que l’environnement scolaire sont des facteurs qui influencent la consommation d’alcool chez les adolescents. L’attachement à l’école et le manque de connaissances sont apparus comme des éléments importants déterminants dans la consommation d’alcool des adolescents. Discussion : Les programmes de prévention mis en place grâce aux pistes proposées dans les résultats pourraient contenir des activités ludiques, ce qui augmenterait leur intérêt auprès des adolescents. L’infirmière scolaire peut difficilement décider seule de mettre en place un programme de prévention.
Relativistic all-order calculations of Th, Th$^{+}$ and Th$^{2+}$ atomic properties
Creators: name: Safronova, M. S.
name: Safronova, U. I.
name: Clark, Charles W.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Optics (physics.optics)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Excitation energies, term designations, and $g$-factors of Th, Th$^{+}$ and Th$^{2+}$ are determined using a relativistic hybrid configuration interaction (CI) + all-order approach that combines configuration interaction and linearized coupled-cluster methods. The results are compared with other theory and experiment where available. We find some "vanishing" $g$-factors, similar to those known in lanthanide spectra. Reduced matrix elements, oscillator strengths, transition rates, and lifetimes are determined for Th$^{2+}$. To estimate the uncertainties of our results, we compared our values with the available experimental lifetimes for higher $5f7p\ ^3G_{4}$, $7s7p\ ^3P_{0}$, $7s7p\ ^3P_{1}$, and $6d7p\ ^3F_{4}$ levels of Th$^{2+}$. These calculations provide a benchmark test of the CI+all-order method for heavy systems with several valence electrons and yield recommended values for transition rates and lifetimes of Th$^{2+}$.
description: 13 pages
Localised dynactin protects growing microtubules to deliver oskar mRNA to the posterior cortex of the Drosophila oocyte.
Creators: name: Nieuwburg, Ross
name: Nashchekin, Dmitry
name: Jakobs, Maximilian
name: Carter, Andrew P
name: Khuc Trong, Philipp
name: Goldstein, Raymond
name: St Johnston, Robert
Publisher: name: Apollo - University of Cambridge Repository
Year: 2017
Subjects: Oocytes
Microtubules
Animals
Drosophila melanogaster
Kinesin
Cytoskeletal Proteins
Drosophila Proteins
RNA, Messenger

description: © Nieuwburg et al. The localisation of oskar mRNA to the posterior of the Drosophila oocyte defines where the abdomen and germ cells form in the embryo. Kinesin 1 transports oskar mRNA to the oocyte posterior along a polarised microtubule cytoskeleton that grows from non-centrosomal microtubule organising centres (ncMTOCs) along the anterior/lateral cortex. Here, we show that the formation of this polarised microtubule network also requires the posterior regulation of microtubule growth. A missense mutation in the dynactin Arp1 subunit causes most oskar mRNA to localise in the posterior cytoplasm rather than cortically. oskar mRNA transport and anchoring are normal in this mutant, but the microtubules fail to reach the posterior pole. Thus, dynactin acts as an anti-catastrophe factor that extends microtubule growth posteriorly. Kinesin 1 transports dynactin to the oocyte posterior, creating a positive feedback loop that increases the length and persistence of the posterior microtubules that deliver oskar mRNA to the cortex.
Giant pandas in captivity undergo short-term adaptation in nerve-related pathways
Creators: name: 李严(YanLi)
Publisher: name: CNGB
Year: 2023
Subjects: Variation
Monoisolate
Evolution

description: By comparing the WGS data of 11 captive and 28 wild giant pandas, 505 robust selected genomic regions were identified between the two populations. GO analysis revealed that genes in these regions were involved in nerve-related pathways. Additionally, nucleotide diversity in the captive population was correlated with chromatin conformation structures, which included A/B compartments, TADs and TAD-cliques. Chromatin conformation structures coordinately regulate gene expression in nerve-related pathways, further proving that giant pandas in captivity experience genomic selection on nerve-related pathways. In conclusion, we found that giant pandas in captivity underwent short-term adaptation in nerve-related pathways.
Small Platforms, High Return: The Need to Enhance Investment in Small Satellites for Focused Science, Career Development, and Improved Equity
Creators: name: Mason, James Paul
name: Begbie, Robert G.
name: Bowen, Maitland
name: Caspi, Amir
name: Chamberlin, Phillip C.
name: Chandran, Amal
name: Cohen, Ian
name: DeLuca, Edward E.
name: de Wijn, Alfred G.
name: Dissauer, Karin
name: Eparvier, Francis
name: Filwett, Rachael
name: Gibson, Sarah
name: Gilly, Chris R.
name: Herde, Vicki
name: Ho, George
name: Hospodarsky, George
name: Jaynes, Allison
name: Jones, Andrew R.
name: Kasper, Justin C.
name: Kohnert, Rick
name: Lee, Zoe
name: Mason, E. I.
name: Merkel, Aimee
name: Mesquita, Rafael
name: Moore, Christopher S.
name: Nikoukar, Romina
name: Pesnell, W. Dean
name: Regoli, Leonardo
name: Savage, Sabrina
name: Seaton, Daniel B.
name: Spence, Harlan
name: Thiemann, Ed
name: Vievering, Juliana T.
name: Wilder, Frederick
name: Woods, Thomas N.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: In the next decade, there is an opportunity for very high return on investment of relatively small budgets by elevating the priority of smallsat funding in heliophysics. We've learned in the past decade that these missions perform exceptionally well by traditional metrics, e.g., papers/year/\$M (Spence et al. 2022 -- arXiv:2206.02968). It is also well established that there is a "leaky pipeline" resulting in too little diversity in leadership positions (see the National Academies Report at https://www.nationalacademies.org/our-work/increasing-diversity-in-the-leadership-of-competed-space-missions). Prioritizing smallsat funding would significantly increase the number of opportunities for new leaders to learn -- a crucial patch for the pipeline and an essential phase of career development. At present, however, there are far more proposers than the available funding can support, leading to selection ratios that can be as low as 6% -- in the bottom 0.5th percentile of selection ratios across the history of ROSES. Prioritizing SmallSat funding and substantially increasing that selection ratio are the fundamental recommendations being made by this white paper.
description: White paper submitted to the Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033; 6 pages, 1 figure
The Persistent Mystery of Collisionless Shocks
Creators: name: Goodrich, Katherine
name: Schwartz, Steven
name: Wilson, Lynn
name: Cohen, Ian
name: Turner, Drew
name: Caspi, Amir
name: Smith, Keith
name: Rose, Randall
name: Whittlesey, Phyllis
name: Plaschke, Ferdinand
name: Halekas, Jasper
name: Hospodarsky, George
name: Burch, James
name: Gingell, Imogen
name: Chen, Li-Jen
name: Retino, Alessandro
name: Khotyaintsev, Yuri
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Collisionless shock waves are one of the main forms of energy conversion in space plasmas. They can directly or indirectly drive other universal plasma processes such as magnetic reconnection, turbulence, particle acceleration and wave phenomena. Collisionless shocks employ a myriad of kinetic plasma mechanisms to convert the kinetic energy of supersonic flows in space to other forms of energy (e.g., thermal plasma, energetic particles, or Poynting flux) in order for the flow to pass an immovable obstacle. The partitioning of energy downstream of collisionless shocks is not well understood, nor are the processes which perform energy conversion. While we, as the heliophysics community, have collected an abundance of observations of the terrestrial bow shock, instrument and mission-level limitations have made it impossible to quantify this partition, to establish the physics within the shock layer responsible for it, and to understand its dependence on upstream conditions. This paper stresses the need for the first ever spacecraft mission specifically designed and dedicated to the observation of both the terrestrial bow shock as well as Interplanetary shocks in the solar wind.
description: White paper submitted to the Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033; 9 pages, 4 figures
Using Machine Learning to Determine Morphologies of $z<1$ AGN Host Galaxies in the Hyper Suprime-Cam Wide Survey
Creators: name: Tian, Chuan
name: Urry, C. Megan
name: Ghosh, Aritra
name: Ofman, Ryan
name: Ananna, Tonima Tasnim
name: Auge, Connor
name: Cappelluti, Nico
name: Powell, Meredith C.
name: Sanders, David B.
name: Schawinski, Kevin
name: Stark, Dominic
name: Tremblay, Grant R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Machine Learning (cs.LG)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: We present a machine-learning framework to accurately characterize morphologies of Active Galactic Nucleus (AGN) host galaxies within $z<1$. We first use PSFGAN to decouple host galaxy light from the central point source, then we invoke the Galaxy Morphology Network (GaMorNet) to estimate whether the host galaxy is disk-dominated, bulge-dominated, or indeterminate. Using optical images from five bands of the HSC Wide Survey, we build models independently in three redshift bins: low $(0
description: Accepted for publication in The Astrophysical Journal. 35 Pages. 25 Figures
Multi-point Assessment of the Kinematics of Shocks (MAKOS): A Heliophysics Mission Concept Study
Creators: name: Goodrich, Katherine A.
name: Wilson, Lynn B.
name: Schwartz, Steven
name: Cohen, Ian J.
name: Turner, Drew L.
name: Whittlesey, Phyllis
name: Caspi, Amir
name: Rose, Randall
name: Smith, Keith
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Collisionless shocks are fundamental processes that are ubiquitous in space plasma physics throughout the Heliosphere and most astrophysical environments. Earth's bow shock and interplanetary shocks at 1 AU offer the most readily accessible opportunities to advance our understanding of the nature of collisionless shocks via fully-instrumented, in situ observations. One major outstanding question pertains to the energy budget of collisionless shocks, particularly how exactly collisionless shocks convert incident kinetic bulk flow energy into thermalization (heating), suprathermal particle acceleration, and a variety of plasma waves, including nonlinear structures. Furthermore, it remains unknown how those energy conversion processes change for different shock orientations (e.g., quasi-parallel vs. quasi-perpendicular) and driving conditions (upstream Alfvénic and fast Mach numbers, plasma beta, etc.). Required to address these questions are multipoint observations enabling direct measurement of the necessary plasmas, energetic particles, and electric and magnetic fields and waves, all simultaneously from upstream, downstream, and at the shock transition layer with observatory separations at ion to magnetohydrodynamic (MHD) scales. Such a configuration of spacecraft with specifically-designed instruments has never been available, and this white paper describes a conceptual mission design -- MAKOS -- to address these outstanding questions and advance our knowledge of the nature of collisionless shocks.
description: White paper submitted to the Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033; 9 pages, 3 figures, 5 tables
Site Forms for Solid Rocket Booster Disassembly & Refurbishment Complex
Creators: name: Price, David L.
Year: 2014
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: 8BR02008
valueUri: https://core.tdar.org/browse/site-name/116398/8br02008
subject: 8BR02001
valueUri: https://core.tdar.org/browse/site-name/116397/8br02001
subject: 8BR02009
valueUri: https://core.tdar.org/browse/site-name/116400/8br02009
subject: 8BR02006
valueUri: https://core.tdar.org/browse/site-name/116402/8br02006
subject: 8BR02004
valueUri: https://core.tdar.org/browse/site-name/116406/8br02004
subject: 8BR02005
valueUri: https://core.tdar.org/browse/site-name/116409/8br02005
subject: 8BR02002
valueUri: https://core.tdar.org/browse/site-name/116411/8br02002
subject: 8BR02003
valueUri: https://core.tdar.org/browse/site-name/116413/8br02003
subject: Multi-Media Blast Facility
valueUri: https://core.tdar.org/browse/site-name/117476/multi-media-blast-facility
subject: Thrust Vector Control Deservicing Building
valueUri: https://core.tdar.org/browse/site-name/117475/thrust-vector-control-deservicing-building
subject: First Wash Building
valueUri: https://core.tdar.org/browse/site-name/117478/first-wash-building
subject: High Pressure Wash Building
valueUri: https://core.tdar.org/browse/site-name/117477/high-pressure-wash-building
subject: Hangar AF
valueUri: https://core.tdar.org/browse/site-name/117480/hangar-af
subject: SRB Paint Building
valueUri: https://core.tdar.org/browse/site-name/117479/srb-paint-building
subject: Robot Wash Building
valueUri: https://core.tdar.org/browse/site-name/117482/robot-wash-building
subject: 8BR2007
valueUri: https://core.tdar.org/browse/site-name/116521/8br2007
subject: High Pressure Gas Building
valueUri: https://core.tdar.org/browse/site-name/117481/high-pressure-gas-building
subject: SRB Recovery Slip
valueUri: https://core.tdar.org/browse/site-name/117483/srb-recovery-slip
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Architectural Survey
valueUri: https://core.tdar.org/browse/investigation-type/2/architectural-survey
subject: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking
subject: Site Evaluation / Testing
valueUri: https://core.tdar.org/browse/investigation-type/10/site-evaluation-testing

description: Site Forms for Launch Complex 39.
EOSC Support Office Austria 2nd General Assembly Slide Deck
Creators: name: Hasani-Mavriqi, Ilire
name: Vohland, Katrin
name: Gunsenheimer, Ute
name: Suominen, Tommi
name: Drago, Federico
name: Wassermann, Birgit
name: De Mello Castro Giroletti, Juliana
name: Solís, Barbara Sanchéz
name: Reiner, Heimo
name: Guba, Beate
name: Flicker, Katharina
name: Ganguly, Raman
name: Jean-Quartier, Claire
name: Blumesberger, Susanne
name: Hanslik, Stefan
name: Karlhuber, Petra
Publisher: name: Zenodo
Year: 2022

description: The second General Assembly of Austrian Mandated Organisation - EOSC Support Office Austria (EOSC SOA) took place on Monday 7th September at the Graz University of Technology. Besides taking stock of the achievements during its first year of existence in the afternoon session, the Austrian Open Science community had the opportunity to hear keynote talks on the EOSC Partnership and EOSC Association by the Association's Secretary General Ute Gunsenheimer, on the FAIRCORE4EOSC project by coordinator Tommi Suominen (CSC), and on the importance of Open Science in microbiome research by Birgit Wassermann (TU Graz). The event was tweeted online via @eoscassociation. Katrin Vohland from the Vienna Natural History Museum (NHMW) and chair of the EOSC SOA Steering Committee, gave an overview of what’s in store for the EOSC SOA in the coming year. Ilire Hasani-Mavriqi from TU Graz, the current Chair of the Management Board, summarised the activities carried out in 2022 showing the strong involvement of Austrian organisations in many key EOSC-related initiatives. To complete the overview, Juliana Giroletti from TU Wien described the achievements of the Secretariat and the communication strategy, and the leaders of the EOSC SOA’s working groups (Austria country report, Collections, Data stewardship, KPIs, Researcher and Stakeholder engagement, Technical infrastructure, and Training) showed their results from the past year and the plans for 2023. To conclude the event, Stefan Hanslik from the Austrian Federal Ministry for Education, Science and Research (BMBWF) and Austrian delegate in the EOSC Steering Board and Petra Karlhuber from the umbrella organisation (and formal EOSC Mandated Organisation) ACONET Association expressed their support to the EOSC SOA. The individual presentations can
Resurrecting Sneutrino ($\tildeν_L$) Dark Matter in light of Neutrino Mass and LUX
Creators: name: Chatterjee, Arindam
name: Sahu, Narendra
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the minimal supersymmetric standard model (MSSM) the lightest superpartner of the left-handed neutrinos is ruled out of being a candidate of dark matter because of its large elastic cross-section with the nucleus mediated via Z-boson. We resurrect it by extending the MSSM with two triplets with opposite hypercharge. The addition of the triplets not only play a role in generating small Majorana masses for the left-handed active neutrinos but also make the lightest sneutrino a viable candidate for dark matter. We then discuss the relevant parameter space in details which can give rise to the right amount of (thermal) relic abundance as well as satisfy the current direct detection constraints from Xenon100 and LUX. We find that sneutrino dark matter with mass 370-550 GeV can give rise to right thermal relic abundance while co-annihilating with the bino-like neutralino.
Indirect Measurement of Switch Terms of a Vector Network Analyzer with Reciprocal Devices
Creators: name: Hatab, Ziad
name: Gadringer, Michael Ernst
name: Bösch, Wolfgang
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: This paper presents an indirect method for measuring the switch terms of a vector network analyzer (VNA) using at least three reciprocal devices, which do not need to be characterized beforehand. This method is particularly suitable for VNAs that use a three-sampler architecture, which allows for applying first-tier calibration methods based on the error box model. The proposed method was experimentally verified by comparing directly and indirectly measured switch terms and performing a multiline thru-reflect-line (TRL) calibration.
description: GitHub: https://github.com/ZiadHatab/vna-switch-terms
Position-momentum correlations in matter waves double-slit experiment
Creators: name: Neto, J. S. M.
name: da Paz, I. G.
name: Cabral, L. A.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present a treatment of the double-slit interference of matter-waves represented by Gaussian wavepackets. The interference pattern is modelled with Green's function propagator which emphasizes the coordinate correlations and phases. We explore the connection between phases and position-momentum correlations in the intensity, visibility and predictability of the wavepackets interference. This formulation will indicate some aspects that can be useful for theoretical and experimental treatment of particles, atoms or molecules interferometry.
description: 11 pages, 7 figures
A fundamental limit on energy savings in controlled channel flow, and how to beat it
Creators: name: Floryan, Daniel
Publisher: name: arXiv
Year: 2022
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We derive a limit on energy savings in controlled channel flow. For flow in a channel driven by pressure, shear, or any combination of the two, and controlled via wall transpiration or spanwise wall motion, the uncontrolled laminar state requires the least net energy (accounting for the energetic cost of control). Thus, the optimal control solution is to laminarize the flow. Additionally, we raise the possibility of beating this limit. By simultaneously applying wall transpiration and spanwise wall motion, we show that it may be possible to attain sustained sub-laminar energy expenditure in a controlled flow. We provide a necessary design criterion for net energy savings.
description: 13 pages
title: Interventions infirmières permettant de diminuer la consommation de substances des personnes psychotiques
title: Interventions infirmières permettant de diminuer la consommation de substances des personnes psychotiques
titleType: AlternativeTitle
Creators: name: Tan, Pauline
name: Vionnet, Julia
Publisher: name: Unknown
Year: 0
Subjects: subject: Psychose
subject: Consommations de substances
subject: Interventions infirmières
subject: Thérapies

description: Contexte : la prévalence d’une consommation de substances chez les personnes présentant des symptômes psychotiques est élevée. Cette corrélation peut avoir des conséquences physiques, une aggravation des symptômes psychotiques mais également sociales. L’une des explications de cette consommation de substances est l’automédication, ce qui rend la prise en charge plus complexe encore. Objectif : identifier les interventions infirmières pouvant amener une réduction de la consommation de substances et permettant de réduire l’impact négatif de cette problématique chez les personnes psychotiques. Méthode : les bases de données Medline via Pubmed ainsi que la revue systématique de la Cochrane ont été utilisées pour la recherche des articles scientifiques. Six articles ont été retenus et proviennent des Pays-Bas, du Royaume-Uni, d’Australie, du Danemark ainsi que d’Irlande. Résultats : les résultats ont été mis en perspective avec le cadre théorique de Nola Pender ainsi qu’avec les concepts de la question de recherche. L’analyse des articles a amené différents résultats et propose des interventions notamment sur la diminution des consommations de substances, l’influence de l’entourage, la motivation ainsi que sur la vie quotidienne. Conclusion : ce travail a ouvert un large questionnement suite à la découverte de l’ampleur de la problématique. La mise en évidence qu’il n’y a pas à ce jour une intervention montrant plus de résultats qu’une autre suggère qu’il faut s’intéresser à la qualité de la relation avec le patient, l’importance de la communication ainsi que la personnalisation de la prise en charge. Ce travail ouvre donc des perspectives concernant le rôle propre de l’infirmière.
Large-scale Language Model Rescoring on Long-form Data
Creators: name: Chen, Tongzhou
name: Allauzen, Cyril
name: Huang, Yinghui
name: Park, Daniel
name: Rybach, David
name: Huang, W. Ronny
name: Cabrera, Rodrigo
name: Audhkhasi, Kartik
name: Ramabhadran, Bhuvana
name: Moreno, Pedro J.
name: Riley, Michael
Publisher: name: arXiv
Year: 2023
Subjects: subject: Audio and Speech Processing (eess.AS)
subject: Computation and Language (cs.CL)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: In this work, we study the impact of Large-scale Language Models (LLM) on Automated Speech Recognition (ASR) of YouTube videos, which we use as a source for long-form ASR. We demonstrate up to 8\% relative reduction in Word Error Eate (WER) on US English (en-us) and code-switched Indian English (en-in) long-form ASR test sets and a reduction of up to 30\% relative on Salient Term Error Rate (STER) over a strong first-pass baseline that uses a maximum-entropy based language model. Improved lattice processing that results in a lattice with a proper (non-tree) digraph topology and carrying context from the 1-best hypothesis of the previous segment(s) results in significant wins in rescoring with LLMs. We also find that the gains in performance from the combination of LLMs trained on vast quantities of available data (such as C4) and conventional neural LMs is additive and significantly outperforms a strong first-pass baseline with a maximum entropy LM. Copyright 2023 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other uses, in any current or future media, including reprinting/republishing this material for advertising or promotional purposes, creating new collective works, for resale or redistribution to servers or lists, or reuse of any copyrighted component of this work in other works.
description: 5 pages, accepted in ICASSP 2023
Grain-Fed Versus Grass-Fed Beef Production
Creators: name: Nix, James E.
name: Nix, James E.
Publisher: name: Unknown
Year: 1975
Subjects: subject: Demand and Price Analysis
subject: Land Economics/Use
subject: Livestock Production/Industries
subject: Marketing
subject: FOS: Economics and business
subject: Beef production
subject: grass-fed
subject: grain-fed
subject: forages
subject: feed grains
subject: feed prices

description: The poor 1974 U.S. corn crop caused sharp rises in feed prices and many changes were made in beef production. Large numbers of cattle were forced to slaughter because of short feed supplies and nongrain-fed beef slaughter increased. World food shortages prompted much discussion about beef production being a wasteful use of food producing resources. Quantities of grain consumed by beef cattle per pound of beef produced are, however, less than that assumed by many.
description: Reprinted from the Livestock and Meat Situation • April 1975
Interstellar extinction and abundances of simple diatomic molecules
Creators: name: Weselak, T.
name: Krełowski, J.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We analyze mutual relations between interstellar extinction E(B-V) and column densities of diatomic molecules such as CN, CH and CH cation observed along translucent sightlines. Observational material acquired using five echelle spectrographs, situated in both northern and southern hemispheres, was used in this study. While column densities of CH, CH+ correlate reasonably tightly with E(B-V) the similar relation built for CN shows a large scatter. This result suggests that CH and CH+ molecules are quite well spatially correlated to interstellar dust while CN requires another conditions to be formed. The CH molecule is closely related to H_2 as it was demonstrated already; the fact is interesting since H_2 is believed to be formed on grain surfaces rather than in the gas phase.
description: 4 pages, 3 figures
SHPO: Proposed Roof Repairs for Facility 3659-South Housing Chapel (8BR2503), Patrick Air Force Base, Brevard County, Florida
Creators: name: Blaylock, Michael A.
Publisher: name: 45th Space Wing, USAF
Year: 2018
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: 8BR02503
valueUri: https://core.tdar.org/browse/site-name/117015/8br02503
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Consultation
valueUri: https://core.tdar.org/browse/investigation-type/4/consultation
subject: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking

description: SHPO Correspondence regarding roof repairs on Facility 3659-South Housing Chapel (8BR2503), PAFB, Brevard County, Florida.
Heat pulse propagation in chaotic 3-dimensional magnetic fields
Creators: name: del-Castillo-Negrete, D.
name: Blazevski, D.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: Heat pulse propagation in $3$-D chaotic magnetic fields is studied by solving the parallel heat transport equation using a Lagrangian-Green's function (LG) method. The LG method provides an efficient and accurate technique that circumvents limitations of finite elements and finite difference methods. The main two problems addressed are: (i) The dependence of the radial transport on the magnetic field stochasticity (controlled by the amplitude of the perturbation, $ε$); and (ii) The role of reversed shear configurations on pulse propagation. In all the cases considered there are no magnetic flux surfaces. However, radial transport is observed to depend strongly on $ε$ due to the presence of high-order magnetic islands and Cantori that act as quasi-transport barriers that preclude the radial penetration of heat pulses within physically relevant time scale. The dependence of the magnetic field connection length, $\ell_B$, on $ε$ is studied in detail. The decay rate of the temperature maximum, $\langle T \rangle_{max}(t)$, the time delay of the temperature response as function of the radius, $τ$, and the radial heat flux $\langle {{\bf q}\cdot {\hat e}_ψ} \rangle$, are also studied as functions of the magnetic field stochasticity and $\ell_B$. In all cases, the scaling of $\langle T \rangle_{max}$ with $t$ transitions from sub-diffusive, $\langle T \rangle_{max} \sim t^{-1/4}$, at short times ($χ_\parallel t< 10^5$) to a significantly slower scaling at longer times ($χ_\parallel t > 10^5$). A strong dependence on $ε$ is also observed on $τ$ and $\langle {{\bf q}\cdot {\hat e}_ψ} \rangle$. The radial propagation of pulses in fully chaotic fields considerably slows down in the shear reversal region and, as a result, $τ$, in reversed shear configurations is an order of magnitude longer than the one in monotonic $q$-profiles.
EOSC Support Office Austria 2nd General Assembly Slide Deck
Creators: name: Hasani-Mavriqi, Ilire
name: Vohland, Katrin
name: Gunsenheimer, Ute
name: Suominen, Tommi
name: Drago, Federico
name: Wassermann, Birgit
name: De Mello Castro Giroletti, Juliana
name: Solís, Barbara Sanchéz
name: Reiner, Heimo
name: Guba, Beate
name: Flicker, Katharina
name: Ganguly, Raman
name: Jean-Quartier, Claire
name: Blumesberger, Susanne
name: Hanslik, Stefan
name: Karlhuber, Petra
Publisher: name: Zenodo
Year: 2022

description: The second General Assembly of Austrian Mandated Organisation - EOSC Support Office Austria (EOSC SOA) took place on Monday 7th September at the Graz University of Technology. Besides taking stock of the achievements during its first year of existence in the afternoon session, the Austrian Open Science community had the opportunity to hear keynote talks on the EOSC Partnership and EOSC Association by the Association's Secretary General Ute Gunsenheimer, on the FAIRCORE4EOSC project by coordinator Tommi Suominen (CSC), and on the importance of Open Science in microbiome research by Birgit Wassermann (TU Graz). The event was tweeted online via @eoscassociation. Katrin Vohland from the Vienna Natural History Museum (NHMW) and chair of the EOSC SOA Steering Committee, gave an overview of what’s in store for the EOSC SOA in the coming year. Ilire Hasani-Mavriqi from TU Graz, the current Chair of the Management Board, summarised the activities carried out in 2022 showing the strong involvement of Austrian organisations in many key EOSC-related initiatives. To complete the overview, Juliana Giroletti from TU Wien described the achievements of the Secretariat and the communication strategy, and the leaders of the EOSC SOA’s working groups (Austria country report, Collections, Data stewardship, KPIs, Researcher and Stakeholder engagement, Technical infrastructure, and Training) showed their results from the past year and the plans for 2023. To conclude the event, Stefan Hanslik from the Austrian Federal Ministry for Education, Science and Research (BMBWF) and Austrian delegate in the EOSC Steering Board and Petra Karlhuber from the umbrella organisation (and formal EOSC Mandated Organisation) ACONET Association expressed their support to the EOSC SOA.
SN 2018gj: A Short-plateau Type II Supernova with Persistent Blue-shifted H-alpha Emission
Creators: name: Teja, Rishabh Singh
name: Singh, Avinash
name: Sahu, D. K.
name: Anupama, G. C.
name: Kumar, Brajesh
name: Nakaoka, Tatsuya
name: Kawabata, Koji S
name: Yamanaka, Masayuki
name: Ali, Takey
name: Kawabata, Miho
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present an extensive, panchromatic photometric (UV, Optical, and NIR) and low-resolution optical spectroscopic coverage of a Type IIP supernova SN 2018gj that occurred on the outskirts of the host galaxy NGC 6217. From the V-band light curve, we estimate the plateau length to be ~ 70 +- 2 d, placing it among the very few well-sampled short plateau supernovae (SNe). With V-band peak absolute magnitude Mv < -17.0 +- 0.1 mag, it falls in the middle of the luminosity distribution of the Type II SNe. The colour evolution is typical to other Type II SNe except for an early elbow-like feature in the evolution of V-R colour owing to its early transition from the plateau to the nebular phase. Using the expanding photospheric method, we present an independent estimate of the distance to SN 2018gj. We report the spectral evolution to be typical of a Type II SNe. However, we see a persistent blue shift in emission lines until the late nebular phase, not ordinarily observed in Type II SNe. The amount of radioactive nickel (56Ni) yield in the explosion was estimated to be 0.026 +- 0.007 Msol. We infer from semi-analytical modelling, nebular spectrum, and 1-D hydrodynamical modelling that the probable progenitor was a red supergiant with a zero-age-main-sequence mass < 13 Msol. In the simulated hydrodynamical model light curves, reproducing the early optical bolometric light curve required an additional radiation source, which could be the interaction with the proximal circumstellar matter (CSM).
description: Accepted for publication in ApJ (31 pages, 23 figures and 7 tables)
Launch Complex 14 East Side of ICBM Road, Cape Canaveral Air Station, Cape Canaveral, Florida
Creators: name: Kimber Hinder
Publisher: name: Historic American Engineering Record
Year: 2003
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Launch Complex 14
valueUri: https://core.tdar.org/browse/site-name/116323/launch-complex-14
subject: 8BR00216
valueUri: https://core.tdar.org/browse/site-name/116090/8br00216
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station
subject: Gemini Target Vehicles
valueUri: https://core.tdar.org/browse/other-keyword/164460/gemini-target-vehicles
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Historic Background Research
valueUri: https://core.tdar.org/browse/investigation-type/18/historic-background-research
subject: Architectural Survey
valueUri: https://core.tdar.org/browse/investigation-type/2/architectural-survey

description: HAER documentation of Launch Complex 14 and SHPO Correspondence regarding no adverse effect from proposed ADA modifications to the Mechanical Annex Building at Space Launch Complex 14.
Strong Suppression of Coherence Effect and Appearance of Pseudogap in Layered Nitride Superconductor Li_xZrNCl: ^91Zr- and ^15N- NMR Studies
Creators: name: Kotegawa, Hisashi
name: Oshiro, Satoru
name: Shimizu, Yuki
name: Tou, Hideki
name: Kasahara, Yuichi
name: Kishiume, Tsukasa
name: Taguchi, Yasujiro
name: Iwasa, Yoshihiro
Publisher: name: arXiv
Year: 2014
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We present NMR measurements of the layered nitride superconductor Li_xZrNCl. The nuclear spin-lattice relaxation rate, 1/T_1, shows that the coherence peak is strongly suppressed in Li_xZrNCl in contrast to conventional BCS superconductors. In the lightly-doped region close to the insulating state, the system shows a gap-like behavior, i.e., pseudogap, that is characterized by a reduction in the magnitude of the Knight shift and 1/T_1T. A higher superconducting (SC) transition temperature, T_c, is achieved by coexisting with the pseudogap state. These unusual behaviors, which deviate from the ordinary BCS framework, are the key ingredients to understanding the SC mechanism of Li_xZrNCl.
description: 5 pages, 5 figures