cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A2C2S: The ALPINE ALMA C+ survey of galaxies at 4
Creators: name: Ginolfi, Michele
Publisher: name: Zenodo
Year: 2019

description: A2C2S is a large survey of 122 normal star-forming galaxies observed in the [CII]-158μm line and continuum. It aims at understanding stars, gas and dust properties at a time of rapid galaxy maturation after the end of HI reionization, at redshifts 4
Long-term outcomes of ischemic post-conditioning primary PCI and conventional primary PCI in acute STEMI: a meta-analysis of randomized trials
Creators: name: Mir, Tanveer
name: Uddin, Mohammed
name: Changal, Khalid Hamid
name: Perveiz, Eskara
name: Kaur, Jasmeet
name: Sattar, Yasar
name: Ullah, Waqas
name: Sheikh, Mujeeb
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Space Science
subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Data regarding ischemic postconditioning during percutaneous coronary intervention (PCI) as compared conventional PCI alone has yielded conflicting results. Online databases comparing use of ischemic postconditioning percutaneous coronary intervention (ICP-PPCI) in STEMI patients with conventional PPCI were selected. Mortality, heart failure (HF), myocardial infarction (MI), and major adverse cardiac events (MACE) were evaluated. The primary outcome was composite of HF, MI, and mortality. Pooled risk ratio (RR) with 95% confidence interval (CI) were computed using random-effects model. Eight studies consisting of 2,566 patients (ICP-PPCI n = 1,228; PPCI n = 1,278) were included. The mean age for PPCI group was 61.38 ± 7.86 years (51% men) and for PCI 59.83 ± 8.94 years (47% men). There were no differences in outcome between ICP-PPCI and PPCI in terms of HF (RR 0.87 95% CI0.51–1.48; p = 0.29), MI (RR 1.28, 95%CI0.74–2.20; p = 0.20), mortality (RR 0.93, 95%CI0.64–1.34; p = 0.58), and MACE (RR 0.89, 95%CI0.74–1.07; p = 0.22). The results for composite event for the ICP-PPCI and PPIC procedures, at ≥1 year follow-up duration, were comparable (RR 1.00 95%CI0.82–1.22; p = 1). Ischemic postconditioning post percutaneous coronary intervention in STEMI patients has no long-term benefits over conventional PCI.
Reversed Dark Resonance in Rb Atom Excited by a Diode Laser
Creators: name: Alnis, Janis
name: Auzinsh, Marcis
Publisher: name: arXiv
Year: 2000
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Origin of recently discovered reversed (opposite sign) dark resonances was explained theoretically and verified experimentally. It is shown that the reason for these resonances is a specific optical pumping of ground state level in a transition when ground state angular momentum is smaller than the excited state momentum.
description: 4 ps figures
ALGEBRAIK ANIQLIGI YUQORI BO`LGAN KVADRATUR FORMULALAR. SIMPSON FORMULASI.
Creators: name: Quvvatov, Behruz
Publisher: name: Zenodo
Year: 2024

description: Yangi O`zbekistonimizda yuz bеrаyotgаn siyosiy, iqtisоdiy, ilmiy – tехnikаviy vа mаdаniy o’zgаrishlаr Оliy tа’lim tizimidа hаm o’z аksini tоpmоqdа. O’zbеkistоndа uzluksiz tа’lim – tаrbiya tizimini yarаtish, shu аsоsidа tа’lim sifаtini jаhоn аndоzаlаri dаrаjаsigа yеtkаzish tа’lim sistеmаsining еng dоlzаrb vаzifаsigа аylаndi.
Magnetic Penetration Depth in Unconventional Superconductors
Creators: name: Prozorov, Ruslan
name: Giannetta, Russell W.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: This topical review summarizes various features of magnetic penetration depth in unconventional superconductors. Precise measurements of the penetration depth as a function of temperature, magnetic field and crystal orientation can provide detailed information about the pairing state. Examples are given of unconventional pairing in hole- and electron-doped cuprates, organic and heavy fermion superconductors. The ability to apply an external magnetic field adds a new dimension to penetration depth measurements. We discuss how field dependent measurements can be used to study surface Andreev bound states, nonlinear Meissner effects, magnetic impurities, magnetic ordering, proximity effects and vortex motion. We also discuss how penetration depth measurements as a function of orientation can be used to explore superconductors with more than one gap and with anisotropic gaps. Details relevant to the analysis of penetration depth data in anisotropic samples are also discussed.
description: topical review, 57 pages, 219 references
Systolic ratio, index of closed orbits and convexity for tight contact forms on the three-sphere
Creators: name: Abbondandolo, Alberto
name: Bramham, Barney
name: Hryniewicz, Umberto
name: Salomão, Pedro
Publisher: name: arXiv
Year: 2017
Subjects: subject: Symplectic Geometry (math.SG)
subject: FOS: Mathematics

description: We construct a dynamically convex contact form on the three-sphere whose systolic ratio is arbitrarily close to 2. This example is related to a conjecture of Viterbo, whose validity would imply that the systolic ratio of a convex contact form does not exceed 1. We also construct a sequence of tight contact forms $α_n$, $n\geq 2$, with systolic ratio arbitrarily close to $n$ and suitable bounds on the mean rotation number of all the closed orbits of the induced Reeb flow.
description: 44 pages
title: Rare case of cystic artery pseudoaneurysm presenting with haematemesis treated with percutaneous embolization
Creators: name: Thomas, Joel Joy
Publisher: name: EURORAD
Year: 2021
Subjects: subject: Abdominal imaging
subject: Abdomen
subject: CT-Angiography
subject: Ultrasound-Colour Doppler
subject: Embolisation
subject: Aneurysms
subject: Clinical Cases

description: Clinical History: A 68-year-old gentleman presented with a history of 1 episode of hematemesis and pain in his right upper abdomen. He was haemodynamically stable and afebrile. He did not report any malena or any similar episodes of hematemesis in the past. His past medical history included asthma and hypertension. 

description: 68 years, male
On a New Supersymmetric KdV Hierarchy in $2{-}d$ Quantum Supergravity
Creators: name: Figueroa-O'Farrill, J. M.
name: Stanciu, S.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Recently a new supersymmetric extension of the KdV hierarchy has appeared in a matrix-model-inspired approach to $2{-}d$ quantum supergravity. Here we prove that this hierarchy is essentially the KdV hierarchy, where the KdV field is now replaced by an even superfield. This allows us to find the conserved charges and the bihamiltonian structure, and to prove its integrability. We also extend the hierarchy by odd flows in a supersymmetric fashion.
description: 12 pages, Plain TeX, BONN-HE-93-007 (v2: solved legacy compilation problems)
FARZAND TARBIYASIGA TA'SIR ETUVCHI IJTIMOIY PSIXOLOGIK OMILLAR
Creators: name: Normamatova, Nazira
Publisher: name: Zenodo
Year: 2024

description: Bola tug'ilishidan boshlab normal rivojlanishi uchun muloqot muhim ahamiyatga ega. Faqatgina muloqot jarayonida bola inson nutqini o'zlashtirib olishi mumkin. Bu o'z navbatida bola faoliyatida va atrof-muhitni bilish va o'zlashtirishda etakchi vazifani bajaradi. Shaxs rivojlanishi harakatlantiruvchi kuchlari bo'lib bola ehtiyoji va uni qoniqtirish imkoniyati o'rtasida yuzaga keladigan qarama-qarshiliklar hisoblanadi. Ushbu maqolada, farzand tarbiyasiga ta’sir etuvchi ijtimoiy psixologik omillar haqida fikr va mulohazalar qilinadi.
The molecular torus of NGC1068
Creators: name: Impellizzeri, Violette
Publisher: name: Zenodo
Year: 2019

description: I will present results obtained with ALMA on the prototypical Seyfert 2 nucleus in NGC 1068. Previous CO (6-5) observation already showed evidence for a high-velocity outflow at a resolution of ∼ 0.04" resolution. We have now obtained data with a factor ∼ 2 better resolution (∼1 pc-scale) with the most extended ALMA configurations. We observed HCN J=3-2 to reveal aline profile against the radio nucleus which is consistent with the outflow observed in CO. The projected radial velocity of this molecular outflow is ∼170 km/s with high velocity wings ranging up to 400 km/s. The nuclear spectrum also shows a narrow, redshifted absorption component at infall speed ∼40 km/s. Analysis of the position-velocity diagram and the morphology of the integrated line flux map reveals two nested, rotating disk components. The inner disk, inside ∼ 1.5 pc, has kinematics consistent with the edge-on, geometrically thin H2O water megamaser disk. The outer disk, which extends to 7 pc, is also geometrically thin but inclined. The outer disk counter-rotates relative to the inner, water megamaser disk. I will conclude with a picture in which the torus consists of two geometrically thin, counter-rotating disks, and the nuclear obscuration occurs in outflowing molecular clouds whose origin is likely a hydromagnetic wind driven off of the inner disk.
ALMA view of 1 pc-scale molecular-gas structures in M33: Revealing star-formation activities in mole
Creators: name: Nishimura, Atsushi
Publisher: name: Zenodo
Year: 2019

description: Recent mm/sub-mm observations of molecular clouds suggest that molecular gas shows highly filamentary structure from a sub-pc to ~100 pc scale and the collision/interaction of such filamentary structures may drive the massive star formation. Although some galactic studies found very long filamentary clouds with the length of 50-100 pc (e.g., the "Nessie" nebula) possibly formed by the galactic spiral shocks, the actual origin and the star formation therein remain to be unclear, and are hard to understand due to the heavy contamination on the Galactic plane observation. In order to reveal the relation between the galactic scale kinematics and the formation of molecular filaments/high-mass stars, we performed ALMA observations in the 12CO(2-1), 13CO(2-1), C18O(2-1) lines and 1.3 mm continuum emission toward the three most massive giant molecular clouds (GMCs) in one of the nearest spiral galaxy M33 at an angular resolution of 0".37 (corresponding to 1.5 pc). We targeted three massive (~10^6 Mo) GMCs in M33: GMC-8 with inactive star formation; NGC 604, one of the most luminous giant HII regions in the Local Group with young stellar clusters (hereafter, the NGC 604 GMC); and GMC-16, associated with relatively small HII regions. Our preliminary results in 12CO and 13CO data demonstrate that NGC 604 GMC and GMC-16 contain many filamentary structures, whereas GMC-8 shows less filamentary structures and significantly lower 13CO/12CO ratio compared to other two GMCs. These results indicate that the dense (filamentary) gas fraction in GMCs increases as the star formation progresses. The filamentary clouds in GMC16 are highly ordered along the North-South direction with a length of 50-100 pc, which agrees with the elongation of the spiral arm. We detect red/blue-shifted wing components possibly due to the molecular outflow from massive protostar(s) at the 1.3 mm continuum source embedded in the filament, suggesting that the galactic shock may interplay in forming the long filaments and in massive star formation. In contrast to GMC-16, the molecular clouds in the NGC 604 GMC show more complex distributions composed by much shorter (10-15 pc) filaments and/or shell/arc-like structures along HII regions. Since such morphologies cannot be explained by the spiral shocks alone, we suggest that the combination of the ionization by UV photons from the NGC 604 cluster and an external atomic gas flow promoted the evolution of the GMC.
Tracing magnetic field with polarimetry of submillimeter lines
Creators: name: Zhang, Heshou
Publisher: name: Zenodo
Year: 2019

description: Submillimeter polarimetry associated with grain alignment is accepted as one of the major avenues for detection of interstellar magnetic fields. The submm spectropolarimetry, on the other hand, is still unexplored beyond the molecular clouds. Fine structure lines are polarized due to ground state alignment (GSA) by optical pumping. The polarization of the submillimeter fine-structure lines induced could be substantial. This method is applicable to all radiative-excitation dominant region, e.g., H II Regions, PDRs. The potential of the new magnetic tracer has been clearly revealed by the first detection of GSA effect on a binary system where 3D magnetic fields are precisely mapped (see my poster). Our results demonstrate submillimeter polarimetry as a powerful magnetic tracer and is readily applicable for ALMA today if polarisation at band 8 is commissioned
title: Histoire : jinniao
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
title: ADCO, Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Cart. 176 (11 H 8), f. 0177
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2017
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 176 (11 H 8), f. 0177, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 176 (11 H 8), f. 0177, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
The Extreme Scattering Event Toward 1741-038: H I Absorption
Creators: name: Lazio, T. J. W.
name: Gaume, R. A.
name: Claussen, M. J.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report multi-epoch VLA H I absorption observations of the source 1741-038 (OT-068) before and during an extreme scattering event (ESE). Observations at four epochs, three during the ESE, were obtained. We find no changes in the equivalent width, maximum optical depth, or velocity of maximum optical depth during the ESE, but we do find a secular trend of decreasing maximum optical depth between our observations and ones by other observers a decade prior. The resulting limit on the H I column density change during the ESE for a structure with a spin temperature T_s is 6.4 x 10^{17} cm^{-2} (T_s/10 K). Tiny-scale atomic structures (TSAS), with a column density N_H ~ 3 x 10^{18} cm^{-2}, are ruled out marginally by this limit, though geometric arguments may allow this limit to be relaxed. Galactic halo molecular clouds, that are opaque in the H I line, cannot be excluded because the observed velocity range covers only 25% of their allowed velocity range.
description: 9 pages, LaTeX2e with AASTeX5.0; 4 PostScript figures in 4 files; accepted for publication in the ApJ, vol. 546, 2001 January 1
The first large, unbiased ALMA survey of CO at parsec resolution in the Small Magellanic Cloud
Creators: name: Jameson, Katie
Publisher: name: Zenodo
Year: 2019

description: The Small Magellanic Cloud (SMC) at only 1/5 solar metallicity is the only galaxy near enough to study the effect of a low metallicity environment on the physics of star formation and the ISM on small spatial scales. Understanding the effects of low metallicity is crucial for understanding galaxies in the early universe and the evolution of galaxies over cosmic time. Initial ALMA observations in the SMC show similar compact CO clumps (Jameson et al. 2018), but only small areas targeting specific star-forming regions have been mapped to date and we lack a statistically significant sample of the CO structure throughout the galaxy. We used ALMA in ACA standalone mode to map a 1.0 deg x 0.5 deg (~1 kpc x 500 pc) area of the Southwest Bar of the SMC at ~6.5" resolution and cover an unprecedented range in size scales from ~1.5 pc to 1 kpc. Our new map shows previously undetectable small (~ pc) molecular gas clumps, similar to what is seen in WLM (Rubio et al. 2015) and NGC 6822 (Schruba et al. 2017), but across a much larger scale. I will discuss the properties of the CO-emitting gas and how it compares to the HI gas from our new ATCA HI absorption survey and GASKAP HI map and what that reveals about the atomic-to-molecular transition at low metallicity.
Community Detection in Dynamic Networks via Adaptive Label Propagation
Creators: name: Han, Jihui
name: Li, Wei
name: Zhao, Longfeng
name: Su, Zhu
name: Zou, Yijiang
name: Deng, Weibing
Publisher: name: arXiv
Year: 2017
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Social and Information Networks (cs.SI)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: An adaptive label propagation algorithm (ALPA) is proposed to detect and monitor communities in dynamic networks. Unlike the traditional methods by re-computing the whole community decomposition after each modification of the network, ALPA takes into account the information of historical communities and updates its solution according to the network modifications via a local label propagation process, which generally affects only a small portion of the network. This makes it respond to network changes at low computational cost. The effectiveness of ALPA has been tested on both synthetic and real-world networks, which shows that it can successfully identify and track dynamic communities. Moreover, ALPA could detect communities with high quality and accuracy compared to other methods. Therefore, being low-complexity and parameter-free, ALPA is a scalable and promising solution for some real-world applications of community detection in dynamic networks.
description: 16 pages, 11 figures
On the volume simplicity constraint in the EPRL spin foam model
Creators: name: Bahr, Benjamin
name: Belov, Vadim
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We propose a quantum version of the quadratic volume simplicity constraint for the EPRL spin foam model. It relies on a formula for the volume of 4-dimensional polyhedra, depending on its bivectors and the knotting class of its boundary graph. While this leads to no further condition for the 4-simplex, the constraint becomes non-trivial for more complicated boundary graphs. We show that, in the semi-classical limit of the hypercuboidal graph, the constraint turns into the geometricity condition observed recently by several authors.
description: 14 pages, 5 figures
title: Histoire : tangguowu
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
MOESM3 of Multiplex PCR for the simultaneous detection of the Enterobacterial gene wecA, the Shiga Toxin genes (stx1 and stx2) and the Intimin gene (eae)
Creators: name: D’Auriac, Marc Anglès
name: Sirevåg, Reidun
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Additional file 3. Comparison of selected primers aiming at the detection of all variants of stxA gene; arrows are indicating the direction of the primers and complementary sequences are shown for the reverse primers. The conserved bases are shaded in black while the variable positions are unshaded.
ALGEBRAIK ANIQLIGI YUQORI BO`LGAN KVADRATUR FORMULALAR. KLASSIK GAUSS KVADRATURALARI.
Creators: name: Quvvatov, Behruz
Publisher: name: Zenodo
Year: 2024

description: Gauss kvadraturalari matematika, fizika, injineriya va boshqa sohalarda juda muhim bo`lgan bir tushunchadir. Hisoblash matematikasi sohasida nazariy izlanishlar asosan, tipik matematik masalalarni yechishning sonli metodlar atrofida guruhlanadi. Bu sohaning klassik masalalaridan biri bu integrallarni taqribiy hisoblash formulalarini qurishdan iborat.
Dependence of the Energy of Molecules on Interatomic Distance at Large Distances
Creators: name: Stepanov, I. A.
Publisher: name: arXiv
Year: 2000
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: Earlier it has been supposed that energy of molecules depends on interatomic distance according to the curve 1, Fig. 1. However, dissociation of molecules (for example, Te2=2Te) often is a chemical reaction. According to chemical kinetics, chemical reactions overcome a potential barrier. This barrier is absent at the curve 1. It is a very strong argument against the curve 1. It is shown that the molecule energy dependence on interatomic distance can behave at large distances not so but like the curve 2, Fig. 1. Earlier it has been supposed that quantum chemical methods give a wrong result at big distances if the wave function does not turn to zero. In this paper, it is been shown that it must not turn to zero. The wave function can be a piecewise function.
description: e-mail me istepanov@email.com, 6 pages; accepted at 32nd EGAS Conference, Vilnius, 2000
Continuous-Variable Protocol for Oblivious Transfer in the Noisy-Storage Model
Creators: name: Furrer, Fabian
name: Gehring, Tobias
name: Schaffner, Christian
name: Pacher, Christoph
name: Schnabel, Roman
name: Wehner, Stephanie
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Cryptographic protocols are the backbone of our information society. This includes two-party protocols which offer protection against distrustful players. Such protocols can be built from a basic primitive called oblivious transfer. We present and experimentally demonstrate here the first quantum protocol for oblivious transfer for optical continuous-variable systems, and prove its security in the noisy-storage model. This model allows to establish security by sending more quantum signals than an attacker can reliably store during the protocol. The security proof is based on new uncertainty relations which we derive for continuous-variable systems, that differ from the ones used in quantum key distribution. We experimentally demonstrate the proposed oblivious transfer protocol for various channel losses by using entangled two-mode squeezed states measured with balanced homodyne detection. Our work enables the implementation of arbitrary two-party quantum cryptographic protocols with continuous-variable communication systems.
description: 10 pages, 4 figures. Theory from arXiv:1509.09123
ALMA observations of the DG Tau B Class I protostar disk and CO outflow
Creators: name: De Valon, Aloïs
Publisher: name: Zenodo
Year: 2019

description: Powerful atomic jets and molecular outflows are observed in young protostars at all stages of active accretion, from the young embedded Class 0 and Class 1 phases to the later optically revealed T Tauri or Class 2 phase. The origin of the ejection, its role in angular momentum extraction and impact on protoplanetary disk evolution remain as fundamental open questions in star formation. Studies at high angular and spectral resolution of molecular outflows are now providing important new clues to these questions. Our recent study with ALMA of the CO cavity/outflow in the prototypical edge-on HH 30 T Tauri star (Louvet et al. 2018) challenges the traditional interpretation of molecular outflows as swept-up material. Instead our ALMA observations suggest a magneto-thermal disk wind origin for the low velocity CO outflow in HH 30. We will report recent band 6 (continuum and 12CO) ALMA observations of the Class I disk/outflow source DG Tau B. We reconstruct the full 3D geometry and kinematics (including rotation) of the CO outflow. We will discuss the implications brought by these observations for the origin of the CO cavities/outflows and their potential impact on the disk evolution.
title: Reconnecting Downtown Springfield to the Connecticut River a Visionary Proposal for an Urban Ecology Park
Creators: name: (:Unkn) Unknown
Publisher: name: University of Massachusetts Amherst
Year: 1995
Subjects: subject: Open Space
subject: Street Network
subject: Constitution Plaza
subject: Economics
subject: Growth and Development
subject: Urban, Community and Regional Planning
subject: Urban Studies and Planning

description: The Center for Economic Development at the University of Massachusetts, in Amherst, is part of the Landscape Architecture and Regional Planning Department, and is funded by the Economic Development Administration of the U.S. Department of Commerce, and the University of Massachusetts.
description: Professor Joseph Volpe in the fall of 1994 proposed to graduate student Frank Sleegers a Master project on a visionary design for the riverfront in downtown Springfield, Massachusetts. Volpe directed the project and Chaired Sleegers’ Master Committee. This Proposal is an expanded edition of Sleegers’ Master Project, Back to the River – A Visionary Design to Recapture the Riverfront in Downtown Springfield, MA.
Additional file 2 of Predicting clinical outcome of neuroblastoma patients using an integrative network-based approach
Creators: name: LĂŠon-Charles Tranchevent
name: Nazarov, Petr V.
name: Kaoma, Tony
name: Schmartz, Georges P.
name: Muller, Arnaud
name: Sang-Yoon Kim
name: Jagath C. Rajapakse
name: Azuaje, Francisco
Publisher: name: figshare
Year: 2018
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy

description: Impact of node2vec parameters on the feature vectors. This file describes a preliminary analysis to better understand the effect of the different node2vec parameters on the produced feature vectors. (PDF 1082 kb)
Tuning photoluminescence response by electric field in the lead-free piezoelectric Na1/2Bi1/2TiO3-BaTiO3
Creators: name: Khatua, Deepak Kumar
name: Kalaskar, Abhijeet
name: Ranjan, Rajeev
Publisher: name: arXiv
Year: 2017
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We show that an electrically soft ferroelectric host can be used to tune the photoluminescence (PL) response of rare-earth emitter ions by external electric field. The proof of this concept is demonstrated by changing the PL response of Eu+3 ion by electric field on a model system Eu-doped 0.94Na1/2Bi1/2TiO3-0.06BaTiO3. We also show that new channels of radiative transitions, forbidden otherwise, open up due to positional disorder in the system, which can as well be tuned by electric field.
description: 13 pages 5 figures
Diversity of protostellar evolution in Serpens Main
Creators: name: Aso, Yusuke
Publisher: name: Zenodo
Year: 2019

description: We observed sixteen 1.3 mm sources in the Serpens Main star forming cluster in the CO and C18O J=2-1 lines as well as in 1.3 mm continuum at an angular resolution of 0.5" (220 au) using ALMA in Cycle 3. These sources are classified into three groups: (1) six sources with extended (>1000 au) continuum and CO outflows, (2) four extended sources without associated CO emission, and (3) six point-like sources with compact CO outflows. The Group 1 members are considered to be typical Class 0 protostars from their SEDs (Tbol<60 K and Lbol/Lsubmm<15) and monopolar/bipolar outflows. They also support evolutionary trends predicted by theoretical studies, such as outflow widening, CO desorption, and disk growth. In particular, SMM4A in Group 1 has the largest disk (r~240 au) and the widest outflow among the Group 1 members. The Group 2 members are embedded in a natal filamentary structure. They have lower densities (<~10^8 cm^-3) than the Group 1 members. The densities indicate that the Group 2 members are marginally Jeans-unstable. These results suggest that Group 2 is prestellar cores. C18O emission is clearly detected only in the member having the highest density in Group 2. This is also consistent with the picture of prestellar cores. The Group 3 members have their counterparts in near infrared, including Class 0 and I sources. They also have less massive envelope (<0.05 Msun) and less clear CO outflows than the Group 1 members. These results suggest that envelopes are dissipated around the Group 3 members. Because of envelope dissipation, disks, if any, around the Group 3 members will not grow up anymore from the current size, HWHM<60 au. Sizes of protostellar disks range from <60 au to ~240 au in the same star forming cluster Serpens Main. This diversity in disk size can been seen even among Class 0 sources in this region. These results may imply diversity of protostellar evolution in a protostellar phase as early as the Class 0 phase. Such different types of protostellar evolution could be an origin of disk-size diversity in the T Tauri phase reported in recent ALMA surveys.
Landscape and flux for quantifying global stability and dynamics of game theory
Creators: name: Xu, Li
name: Wang, Jin
Publisher: name: arXiv
Year: 2017
Subjects: subject: Populations and Evolution (q-bio.PE)
subject: Biological Physics (physics.bio-ph)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Biological sciences
subject: FOS: Physical sciences

description: Game theory has been widely applied to many areas including economics, biology and social sciences. However, it is still challenging to quantify the global stability and global dynamics of the game theory. We developed a landscape and flux framework to quantify the global stability and global dynamics of the game theory. As an example, we investigated the models of three-strategy games: a special replicator-mutator game, the repeated prison dilemma model. In this model, one stable state, two stable states and limit cycle can emerge under different parameters. The repeated Prisoner's Dilemma system has Hopf bifurcation transitions from one stable state to limit cycle state, and then to another one stable state or two stable states, or vice versa. We explored the global stability of the repeated Prisoner's Dilemma system and the kinetic paths between the basins of attractor. The paths are irreversible due to the non-zero flux. One can explain the game for $Peace$ and $War$.
description: 25 pages, 15 figures
Radiative Transfer modeling of EC 53: An Episodically Accreting Class I Young Stellar Object
Creators: name: Baek, Giseon
Publisher: name: Zenodo
Year: 2019

description: Episodic accretion has been observed toward many young protostars, mostly Class II young stellar objects (YSOs). Since a large fraction of its final mass accretes onto the central protostar during the early stage of star formation, it is essential to study the episodic accretion process within embedded YSOs. The Class I YSO, EC 53 in the Serpens Main cloud, has repeatedly undergone robust flux enhancements at 850 μm. Such sub-mm variations are expected to be related to accretion burst events. In this study, we perform two- and three-dimensional continuum radiative transfer modeling to quantify the fractional internal luminosity rise in EC 53 corresponding to the observed flux enhancements. We model the spectral energy distribution and radial intensity profile both in the quiescent and outburst phases. The effect of the external heating from the interstellar radiation field is also considered. For EC 53, we find that the role of external heating from interstellar radiation field appears insignificant. The radial intensity profile analysis clearly demonstrates that the detected sub-mm flux variation of EC 53 comes from the heated envelope by the accretion burst.
Additional file 1: of Physical activity and sedentary time are related to clinically relevant health outcomes among adults with obstructive lung disease
Creators: name: Dogra, Shilpa
name: Good, Joshua
name: Buman, Matthew
name: Gardiner, Paul
name: Copeland, Jennifer
name: Stickland, Michael
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Figure S1. Crude associations of FEV1%pred with Sitting Time and Physical Activity for adults with Asthma, COPD, and those below the LLN. Note: PA: Physical Activity; *p
Discovery of Complex Anomalous Patterns of Sexual Violence in El Salvador
Creators: name: De-Arteaga, Maria
name: Dubrawski, Artur
Publisher: name: arXiv
Year: 2017
Subjects: subject: Applications (stat.AP)
subject: FOS: Computer and information sciences

description: When sexual violence is a product of organized crime or social imaginary, the links between sexual violence episodes can be understood as a latent structure. With this assumption in place, we can use data science to uncover complex patterns. In this paper we focus on the use of data mining techniques to unveil complex anomalous spatiotemporal patterns of sexual violence. We illustrate their use by analyzing all reported rapes in El Salvador over a period of nine years. Through our analysis, we are able to provide evidence of phenomena that, to the best of our knowledge, have not been previously reported in literature. We devote special attention to a pattern we discover in the East, where underage victims report their boyfriends as perpetrators at anomalously high rates. Finally, we explain how such analyzes could be conducted in real-time, enabling early detection of emerging patterns to allow law enforcement agencies and policy makers to react accordingly.
description: Conference paper at Data for Policy 2016 - Frontiers of Data Science for Government: Ideas, Practices and Projections (Data for Policy)
ALMA CO Observations toward the Magellanic Supernova Remnants
Creators: name: Sano, Hidetoshi
Publisher: name: Zenodo
Year: 2019

description: The Large Magellanic Cloud (LMC) is among the best laboratories for studying various astronomical objects and their physics because of its almost face-on inclination to us, and a well-known distance (~50 kpc). Supernova remnants (SNRs) in the LMC were well studied by radio continuum, optical, and X-ray observations (e.g., Bozzetto et al. 2017 and references therein). By contrast, very few attempts have been made to observe molecular clouds associated with the LMC SNRs (Banas et al. 1998). Sano et al. (2017a,b) observed 25 X-ray bright LMC SNRs using the Mopra 22-m and ASTE 10-m radio telescopes with a spatial resolution of ~6-11 pc. At least twelve of them were shown to have giant molecular clouds that have a good spatial correspondence with X-ray shells; this indicates that shock-cloud interactions may have occurred. Subsequently, we observed five SNRs N132D, N49, N103B, N63A, and 30 Doradus C using the Atacama Large Millimeter / submillimeter Array (ALMA) with a spatial resolution of ~0.4-0.7 pc during Cycles 2, 3, and 5. We spatially resolved clumpy molecular clouds associated with the LMC SNRs for the first time (Yamane et al. 2018; Sano et al. 2018, 2019). We are therefore entering a new age in studying the Magellanic SNRs yielding a spatial resolution comparable to what had been possible only for Milky Way SNRs. For N49, the synchrotron radio emission is clearly enhanced around molecular clouds, suggesting that the magnetic field amplification occurred via shock-cloud interactions (Yamane, Sano et al. 2019). For the Type Ia SNR N103B, molecular clouds nicely trace the X-ray shell boundary, which shows an expanding gas motion in the position-velocity diagram with an expansion velocity of ~5 km/s. The expanding gas motion was possibly created by accretion winds from a single- degenerate progenitor system (Sano et al. 2018). For N63A, we spatially resolved clumpy molecular clouds embedded within both the shock-ionized and photoionized optic al nebulae, indicating that the molecular clouds have started to be ionized by shock waves and UV- radiation (Sano et al. 2019). In this talk, we report our latest results of CO studies in the X-ray bright LMC SNRs using ALMA.
Mechanisms of weak thickness dependence of the critical current density in strong pinning ex situ metal-organic-deposition route YBa2Cu3O7-x coated conductors
Creators: name: Kim, S. I.
name: Gurevich, A.
name: Song, X.
name: Li, X.
name: Zhang, W.
name: Kodenkandath, T.
name: Rupich, M. W.
name: Holesinger, T. G.
name: Larbalestier, D. C.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We report on the thickness dependence of the superconducting characteristics including critical current Ic, critical current density Jc, transition temperature Tc, irreversibility field Hirr, bulk pinning force plot Fp(H), and the normal state resistivity curve measured after successive ion milling of ~ 1 um thick high Ic YBa2Cu3O7-x films made by an ex situ metal-organic deposition process on Ni-W rolling-assisted biaxially textured substrates (RABiTS). Contrary to many recent data, mostly on in situ pulsed laser deposition (PLD) films, which show strong depression of Jc with increasing film thickness t, our films exhibit only a weak dependence of Jc on t. The two better textured samples had full cross-section average Jc,avg(77K,0T) ~ 4 MA/cm2 near the buffer layer interface and ~3 MA/cm2 at full thickness, despite significant current blocking due to ~30% porosity in the film. Taking account of the thickness dependence of the porosity, we estimate that the local, vortex-pinning current density is essentially independent of thickness, while accounting for the additional current-blocking effects of grain boundaries leads to local, vortex-pinning Jc values well above 5 MA/cm2. Such high local Jc values are produced by strong three-dimensional vortex pinning which subdivides vortex lines into weakly coupled segments much shorter than the film thickness.
description: Submitted to Superconductor Science and Technology
Predicting the Loci of Solar Eruptions
Creators: name: Gyenge, N.
name: Erdélyi, R.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The longitudinal distribution of solar active regions shows non-homogeneous spatial behaviour, which is often referred to as Active Longitude (AL). Evidence for a significant statistical relationships between the AL and the longitudinal distribution of flare and coronal mass ejections (CME) occurrences is found in Gyenge et al, 2017 (ApJ, 838, 18). The present work forecasts the spatial position of AL, hence the most flare/CME capable active regions are also predictable. Our forecast method applies Autoregressive Integrated Moving Average model for the next 2 years time period. We estimated the dates when the solar flare/CME capable longitudinal belts face towards Earth.
Time-Domain Astrochemistry During Planet Formation
Creators: name: Cleeves, Ilse
Publisher: name: Zenodo
Year: 2019

description: The chemistry of protoplanetary disks sets the initial composition of newly formed planets and may regulate the efficiency by which planets form. Disk chemical abundances typically evolve over timescales spanning thousands if not millions of years. Consequently, it was a surprise when ALMA observations taken over the course of a single year showed significantly variable emission in H13CO+ relative to the otherwise constant thermal dust emission in the IM Lup protoplanetary disk. HCO+ is a known X-ray sensitive molecule, and one possible explanation is that stellar activity is perturbing the chemical ""steady state"" of the disk. If confirmed, simultaneous observations may provide a new tool to measure (and potentially map) fundamental disk parameters, such as electron density, as the light from X-ray flares propagates across the disk.
The Arcminute Microkelvin Imager Catalogue of Gamma-ray Burst afterglows at 15.7 GHz
Creators: name: Anderson, G. E.
name: Staley, T. D.
name: van der Horst, A. J.
name: Fender, R. P.
name: Rowlinson, A.
name: Mooley, K. P.
name: Broderick, J. W.
name: Wijers, R. A. M. J.
name: Rumsey, C.
name: Titterington, D. J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the Arcminute Microkelvin Imager (AMI) Large Array catalogue of 139 gamma-ray bursts (GRBs). AMI observes at a central frequency of 15.7 GHz and is equipped with a fully automated rapid-response mode, which enables the telescope to respond to high-energy transients detected by Swift. On receiving a transient alert, AMI can be on-target within two minutes, scheduling later start times if the source is below the horizon. Further AMI observations are manually scheduled for several days following the trigger. The AMI GRB programme probes the early-time (< 1 day) radio properties of GRBs, and has obtained some of the earliest radio detections (GRB 130427A at 0.36 and GRB 130907A at 0.51 days post-burst). As all Swift GRBs visible to AMI are observed, this catalogue provides the first representative sample of GRB radio properties, unbiased by multi-wavelength selection criteria. We report the detection of six GRB radio afterglows that were not previously detected by other radio telescopes, increasing the rate of radio detections by 50% over an 18-month period. The AMI catalogue implies a Swift GRB radio detection rate of >15%, down to ~0.2 mJy/beam. However, scaling this by the fraction of GRBs AMI would have detected in the Chandra & Frail sample (all radio-observed GRBs between 1997 - 2011), it is possible ~44 - 56% of Swift GRBs are radio-bright, down to ~0.1 - 0.15 mJy/beam. This increase from the Chandra & Frail rate (~30%) is likely due to the AMI rapid-response mode, which allows observations to begin while the reverse-shock is contributing to the radio afterglow.
description: 47 pages (20 of which are catalogue tables), 10 figures, 4 tables, accepted for publication in MNRAS
MOESM2 of Multiplex PCR for the simultaneous detection of the Enterobacterial gene wecA, the Shiga Toxin genes (stx1 and stx2) and the Intimin gene (eae)
Creators: name: D’Auriac, Marc Anglès
name: Sirevåg, Reidun
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 2. List of strains with triplex PCR results.
Pickoff and spin-conversion quenchings of ortho-positronium in oxygen
Creators: name: Shinohara, N.
name: Suzuki, N.
name: Chang, T.
name: Hyodo, T.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: The quenching processes of the thermalized ortho-positronium(o-Ps) on an oxygen molecule have been studied by the positron annihilation age-momentum correlation techinique(AMOC). The Doppler broadening spectrum of the 511 keV gamma-rays from the 2gamma annihilation of o-Ps in O_2 has been measured as a function of the o-Ps age. The rate of the quenching, consisting of the pickoff and the spin-conversion, is estimated from the positron lifetime spectrum. The ratio of the pickoff quenching rate to the spin-conversion rate is deduced from the Doppler broadening of the 511 keV gamma-rays from the annihilation of the o-Ps. The pickoff parameter ^1Z_eff, the effective number of the electrons per molecule which contribute to the pickoff quenching, for O_2 is determined to be 0.6 +- 0.4. The cross-section for the elastic spin-conversion quenching is determined to be (1.16 +- 0.01) * 10^{-19} cm^2.
description: 4 pages with 5 eps figures, LaTeX2e(revtex4)
Additional file 1 of Predicting clinical outcome of neuroblastoma patients using an integrative network-based approach
Creators: name: LĂŠon-Charles Tranchevent
name: Nazarov, Petr V.
name: Kaoma, Tony
name: Schmartz, Georges P.
name: Muller, Arnaud
name: Sang-Yoon Kim
name: Jagath C. Rajapakse
name: Azuaje, Francisco
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Supplementary Figures S1-S5 and Tables S1-S2. (PDF 1266 kb)
Towards real-time interest point detection and description for mobile and robotic devices
Creators: name: Rowsome, Patrick
name: Adil Raja, Muhammad
name: Muhammad Atif Azad, R.
Publisher: name: University of Limerick
Year: 2024
Subjects: classificationCode: 40
subject: Engineering

description: Convolutional Neural Networks (CNNs) have been successfully adopted by state-of-the-art feature point detection and description networks for the past number of years. The focus of these systems has been predominately on the accuracy of the system, rather than on its efficiency or ability to be implemented in real-time on embedded robotic devices. This paper demonstrates how techniques, developed for other CNN use cases, can be integrated into interest point detection and description systems to compress their network size and reduce the computational complexity; this reduces the barrier to their uptake in computationally challenged environments. This paper documents the integration of these techniques into the popular Reliable Detector and Descriptor (R2D2) network. Along with the integration details, a comprehensive Key Performance Indicator (KPI) framework is developed to test all aspects of the networks. As a result, this paper presents a lightweight variant of the R2D2 network that significantly reduces parameters and computational complexity while crucially maintaining an acceptable level of accuracy. Consequently, this new compressed network is more appropriate for use in real world systems and advances the efforts to implement such CNN based system for mobile devices.