cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
First study of η_c, η(1760) and X(1835) production via η'π^+π^- final states in two-photon collisions
Creators: name: Belle Collaboration
name: Zhang, C. C.
name: Aihara, H.
name: Asner, D. M.
name: Aushev, T.
name: Bakich, A. M.
name: Ban, Y.
name: Belous, K.
name: Bischofberger, M.
name: Browder, T. E.
name: Chen, A.
name: Cheon, B. G.
name: Chilikin, K.
name: Chistov, R.
name: Choi, Y.
name: Dalseno, J.
name: Danilov, M.
name: Eidelman, S.
name: Feindt, M.
name: Gaur, V.
name: Gabyshev, N.
name: Goh, Y. M.
name: Han, Y. L.
name: Hayashii, H.
name: Horii, Y.
name: Hou, W. S.
name: Hyun, H. J.
name: Iijima, T.
name: Inami, K.
name: Ishikawa, A.
name: Iwabuchi, M.
name: Julius, T.
name: Kiesling, C.
name: Kim, H. O.
name: Kim, M. J.
name: Kim, Y. J.
name: Ko, B. R.
name: Kodyš, P.
name: Korpar, S.
name: Krokovny, P.
name: Kuzmin, A.
name: Li, J.
name: Libby, J.
name: Liu, Y.
name: Liu, Z. Q.
name: Louvot, R.
name: Matvienko, D.
name: McOnie, S.
name: Mizuk, R.
name: Nakano, E.
name: Nakao, M.
name: Nakazawa, H.
name: Natkaniec, Z.
name: Nishida, S.
name: Ohshima, T.
name: Okuno, S.
name: Olsen, S. L.
name: Pakhlov, P.
name: Pakhlova, G.
name: Park, H.
name: Park, H. K.
name: Pestotnik, R.
name: Petrič, M.
name: Piilonen, L. E.
name: Röhrken, M.
name: Ryu, S.
name: Sahoo, H.
name: Sakai, Y.
name: Santel, D.
name: Sanuki, T.
name: Schneider, O.
name: Schwanda, C.
name: Sevior, M. E.
name: Shapkin, M.
name: Shebalin, V.
name: Shen, C. P.
name: Shibata, T. A.
name: Shiu, J. G.
name: Shwartz, B.
name: Smerkol, P.
name: Sohn, Y. -S.
name: Solovieva, E.
name: Stanič, S.
name: Starič, M.
name: Sumihama, M.
name: Sumiyoshi, T.
name: Tikhomirov, I.
name: Uchida, M.
name: Uehara, S.
name: Uglov, T.
name: Unno, Y.
name: Uno, S.
name: Varner, G.
name: Vinokurova, A.
name: Vorobyev, V.
name: Wang, P.
name: Wang, X. L.
name: Watanabe, Y.
name: Williams, K. M.
name: Yabsley, B. D.
name: Yamashita, Y.
name: Yuan, C. Z.
name: Zhang, Z. P.
name: Zhulanov, V.
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The invariant mass spectrum of the η' π^+ π^- final state produced in two-photon collisions is obtained using a 673 fb^{-1} data sample collected in the vicinity of the Υ(4S) resonance with the Belle detector at the KEKB asymmetric-energy e^+e^- collider. We observe a clear signal of the η_c and measure its mass and width to be M(η_c)=(2982.7 +- 1.8(stat) +- 2.2(syst) +- 0.3(model)) MeV/c^2 and Γ(η_c) = (37.8^{+5.8}_{-5.3}(stat) +- 2.8(syst) +- 1.4(model)) MeV/c^2. The third error is an uncertainty due to possible interference between the η_c and a non-resonant component. We also report the first evidence for η(1760) decay to η' π^+ π^-; we find two solutions for its parameters, depending on the inclusion or not of the X(1835), whose existence is of marginal significance in our data. From a fit to the mass spectrum using coherent X(1835) and η(1760) resonant amplitudes, we set a 90% confidence level upper limit on the product Γ_{γγ} \BR (η' π^+ π^-) for the X(1835).
description: 13 pages, 7 figures, submitted to PRD
Additional file 1 of Shallow whole-genome sequencing of plasma cell-free DNA accurately differentiates small from non-small cell lung carcinoma
Creators: name: Raman, Lennart
name: Malaïka Van Der Linden
name: Eecken, Kim Van Der
name: Vermaelen, Karim
name: Ingel Demedts
name: Surmont, Veerle
name: Himpe, Ulrike
name: Franceska Dedeurwaerdere
name: Ferdinande, Liesbeth
name: Lievens, Yolande
name: Claes, Kathleen
name: Menten, Björn
name: Dorpe, Jo Van
Publisher: name: figshare
Year: 2020
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Table S1 Patient information. Table S2 Sample information.
5th Annual Designing Libraries Conference Program
Creators: name: (:Unkn) Unknown
Publisher: name: University of Calgary
Year: 2016

description: Designing Libraries brings together leading experts from a variety of disciplines who share the common vision of creating innovative environments that meet the current and future needs of students and researchers. This year’s conference covers a broad range of topics, from visualization, virtual reality and maker spaces to innovation in design and architecture. In attendance are librarians, educators, architects and technology innovators from across North America and around the world. Much work has been done here at the University of Calgary to envision nextgeneration libraries. Our library is currently leading a North American study, funded by The Andrew W. Mellon Foundation, to explore the role of academic libraries in enhancing multi-disciplinary research. Scholars from a variety of specializations have contributed.
Additional file 2 of Shallow whole-genome sequencing of plasma cell-free DNA accurately differentiates small from non-small cell lung carcinoma
Creators: name: Raman, Lennart
name: Malaïka Van Der Linden
name: Eecken, Kim Van Der
name: Vermaelen, Karim
name: Ingel Demedts
name: Surmont, Veerle
name: Himpe, Ulrike
name: Franceska Dedeurwaerdere
name: Ferdinande, Liesbeth
name: Lievens, Yolande
name: Claes, Kathleen
name: Menten, Björn
name: Dorpe, Jo Van
Publisher: name: figshare
Year: 2020
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2: Supplementary methods. The copy number profile abnormality score & Details on predictive modeling.
Additional file 5 of Shallow whole-genome sequencing of plasma cell-free DNA accurately differentiates small from non-small cell lung carcinoma
Creators: name: Raman, Lennart
name: Malaïka Van Der Linden
name: Eecken, Kim Van Der
name: Vermaelen, Karim
name: Ingel Demedts
name: Surmont, Veerle
name: Himpe, Ulrike
name: Franceska Dedeurwaerdere
name: Ferdinande, Liesbeth
name: Lievens, Yolande
name: Claes, Kathleen
name: Menten, Björn
name: Dorpe, Jo Van
Publisher: name: figshare
Year: 2020
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 5. Supplementary paired-end copy number profiles, containing a thorough patient-wise comparison of paired single/paired-end copy number profiles. Prediction probabilities are shown in addition.
Magnetic incommensurability in $p$-type cuprate perovskites
Creators: name: Sherman, A.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: For the superconducting phase with a d-wave order parameter and zero temperature the magnetic susceptibility of the t-J model is calculated using the Mori projection operator technique. Conditions for the appearance of an incommensurate magnetic response below the resonance frequency are identified. A fast decay of the tails of the hole coherent peaks and a weak intensity of the hole incoherent continuum near the Fermi level are enough to produce an incommensurate response using different hole dispersions established for $p$-type cuprates, in which such response was observed. In this case, the nesting of the itinerant-electron theory or the charge modulation of the stripe theory is unnecessary for the incommensurability. The theory reproduces the hourglass dispersion of the susceptibility maxima with their location in the momentum space similar to that observed experimentally. The upper branch of the dispersion stems from the excitations of localized spins, while the lower one is due to the incommensurate maxima of their damping. The narrow and intensive resonance peak arises if the frequency of these excitations at the antiferromagnetic momentum lies below the edge of the two-fermion continuum; otherwise the maximum is broad and less intensive.
description: 22 pages, 7 figures
FAIR-by-Design Methodology:How to Develop FAIR Materials
Creators: name: Filiposka, Sonja
Publisher: name: Zenodo
Year: 2023
Subjects: FAIR-by-Design
FAIR learning materials

description: The "FAIR-by-Design Methodology: how to develop FAIR materials"  will take place on 4 December 2023 from 15:00-16:00 CET. Registration for the workshop is free but mandatory.
One of the premises of successful training on how to adopt Open Science is that you should practice what you preach. Therefore, the development of FAIR learning materials that can be easily reused by both trainers and learners is a key ingredient in the Open Science approach and should not be an afterthought.
The FAIR-by-Design Methodology that will be introduced in this webinar aims to provide a systematic approach that will integrate the FAIR principles into the process of learning materials development. The aim of this webinar is to provide a closer look at the defined FAIR-by-Design workflow wherein each stage focuses on different aspects of the materials design process. Discuss and learn how one can practically implement the proposed methodology to ensure that the final result will be high-quality FAIR materials. This event is organised in conjunction with Skills4EOSC project.
Almost exponential maps and integrability results for a class of horizontally regular vector fields
Creators: name: Morbidelli, Daniele
name: Montanari, Annamaria
Publisher: name: arXiv
Year: 2012
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 53C17 (Primary) 53C12 (Secondary)

description: We show a higher order integrability theorem for distributions generated by a family of vector fields under a horizontal regularity assumption on their coefficients. We use as chart a class of almost exponential maps which we discuss in details
description: arXiv admin note: material from arXiv:1106.2410v1, now three separate articles arXiv:1106.2410v2, arXiv:1201.5228, arXiv:1201.5209
Multiple-differential encoding for multi-hop amplify-and-forward relaying in IR-UWB systems
Creators: name: Hamdi, Maziyar
Publisher: name: University of British Columbia
Year: 2010

description: In this thesis, we propose to improve the performance and coverage of impulse-radio ultra-wideband (IR-UWB) systems by means of cooperative multi-hop relaying. With regard to a simple practical realization, we focus on a non-coherent system setup in conjunction with amplify-and-forward (A&F) relaying. In particular, we propose to employ a multiple-differential encoding scheme at the source node and single differential decoding at each relay and at the destination node, respectively, so as to efficiently limit intersymbol-interference (ISI) effects at the destination node. A thorough performance analysis of the proposed scheme is provided, along with a closed-form optimization of the transmit power allocation to the source node and the relays. Simulation results illustrate the excellent performance of the proposed scheme, which is also compared to alternative coherent and non-coherent multi-hop IR-UWB schemes based on A&F relaying and decode-and-forward (D&F) relaying.
Limit formulas for ratios of derivatives of the gamma and digamma functions at their singularities
Creators: name: Qi, Feng
Publisher: name: arXiv
Year: 2012
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 33B15

description: In the paper the author simply presents the limit formulas for ratios of derivatives of the gamma function and the digamma function at their singularities.
description: 3 pages
Broad-tailed force distributions and velocity ordering in a heterogeneous membrane model for collective cell migration
Creators: name: Bameta, Tripti
name: Das, Dipjyoti
name: Sarkar, Sumantra
name: Das, Dibyendu
name: Inamdar, Mandar M.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Soft Condensed Matter (cond-mat.soft)
subject: Cell Behavior (q-bio.CB)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: Correlated velocity patterns and associated large length-scale transmission of traction forces have been observed in collective live cell migration as a response to a "wound". We argue that a simple physical model of a force-driven heterogeneous elastic membrane sliding over a viscous substrate can qualitatively explain a few experimentally observed facts: (i) the growth of velocity ordering which spreads from the wound boundary to the interior, (ii) the exponential tails of the traction force distributions, and (iii) the swirling pattern of velocities in the interior of the tissue.
description: 7 pages and 5 figures
Direct photons in Au+Au collisions measured with the PHENIX detector at RHIC
Creators: name: Petti, Richard
Publisher: name: arXiv
Year: 2011
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: A major goal of experiments in heavy-ion physics is the characterization of the quark gluon plasma (QGP) produced in the collision of heavy ions at high energy. Direct photons are a particularly good probe of the produced medium because they do not interact strongly and so can escape the medium unmodified, carrying information about when the photon was produced. It is expected that direct photon contributions from different sources (QGP radiation, hard scattering, hadron gas radiation) dominate at different transverse momentum ranges. Low momentum direct photons are dominated by thermal radiation (both from the QGP and hadron gas), while high momentum direct photons dominantly come from hard parton scatterings in the initial collision. We present a summary of techniques to measure direct photons with the PHENIX detector, with a focus on low momentum direct photons through their external conversion to dilepton pairs.
description: 6 pages, 4 figures, Winter Workshop on Nuclear Dynamics 2011, intended for publication in Journal of Physics Conference Series (JPCS)
Generalized Semi-Analytical Models of Supernova Light Curves
Creators: name: Chatzopoulos, Emmanouil
name: Wheeler, J. Craig
name: Vinko, Jozsef
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present generalized supernova (SN) light curve (LC) models for a variety of power inputs. We provide an expression for the power input that is produced by self-similar forward and reverse shocks in SN ejecta - circumstellar matter (CSM) interaction. We find that this ejecta-CSM interaction luminosity is in agreement with results from multi-dimensional radiation hydrodynamics simulations in the optically-thin case. We develop a model for the case of an optically-thick CSM by invoking an approximation for the effects of radiative diffusion. In the context of this model, we provide predictions for the time of forward shock break-out from the optically-thick part of the CSM envelope. We also introduce a hybrid LC model that incorporates ejecta-CSM interaction plus Ni-56 and Co-56 radioactive decay input. We fit this hybrid model to the LC of the Super-Luminous Supernova (SLSN) 2006gy. We find that this model provides a better fit to the LC of this event than previously presented models. We also address the relation between Type IIL and Type IIn SN with ejecta-CSM interaction models. Forward and reverse shock power input due to CSM interaction can produce the LCs of Type IIn SNe in terms of duration, shape and decline rate. This model can also produce LCs that are symmetric in shape around peak luminosity. We conclude that the observed LC variety of SNe Type IIn and of the SLSNe is likely to be a byproduct of the large range of conditions relevant to significant ejecta-CSM interaction as a power source.
description: 48 pages, 13 figures
MPEC 2023-H106 : 2023 HD2
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2023 HD2

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Prospects in First Nations Archives: Reflections based on my participation in the Tribal Archives, Libraries and Museums Institutes and Conference program
Creators: name: Reilly, Teresa
Publisher: name: University of Calgary
Year: 2010
Subjects: Archives
Protocols for Naticve American Archival Materials

description: There have been modest but continuing efforts to encourage and coordinate support for First Nations Archives in Canada. In the United States the Tribal Libraries, Archives and Museums conferences and projects are better established. This paper discusses how the American and Canadian experiences are directing us to think differently about how First Nations archives can develop as authentic and self-governing participants in the ongoing work of Healing and Reconciliation.
Convergence of energy scales on the approach to a local quantum critical point
Creators: name: Nishikawa, Y.
name: Crow, D. J. G.
name: Hewson, A. C.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We find the emergence of strong correlations and universality on the approach to the quantum critical points of a two impurity Anderson model. The two impurities are coupled by an inter-impurity exchange interaction $J$ and direct interaction $U_{12}$ and are hybridized with separate conduction channels.The low energy behavior is described in terms of renormalized parameters, which can be deduced from numerical renormalization group (NRG) calculations. We show that on the approach to the transitions to a local singlet and a local charged ordered state, the quasiparticle weight factor $z\to 0$, and the renormalized parameters can be expressed in terms of a single energy scale $T^*$. The values of the renormalized interaction parameters in terms of $T^*$ can be predicted from the condition of continuity of the spin and charge susceptibilities, and correspond to strong correlation as they are greater than or equal to the effective band width. These predictions are confirmed by the NRG calculations, including the case when the onsite interaction U=0.
description: 5 pages 5 figures
Using time-delayed mutual information to discover and interpret temporal correlation structure in complex populations
Creators: name: Albers, D. J.
name: Hripcsak, George
Publisher: name: arXiv
Year: 2011
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: Information Theory (cs.IT)
subject: Dynamical Systems (math.DS)
subject: Methodology (stat.ME)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: This paper addresses how to calculate and interpret the time-delayed mutual information for a complex, diversely and sparsely measured, possibly non-stationary population of time-series of unknown composition and origin. The primary vehicle used for this analysis is a comparison between the time-delayed mutual information averaged over the population and the time-delayed mutual information of an aggregated population (here aggregation implies the population is conjoined before any statistical estimates are implemented). Through the use of information theoretic tools, a sequence of practically implementable calculations are detailed that allow for the average and aggregate time-delayed mutual information to be interpreted. Moreover, these calculations can be also be used to understand the degree of homo- or heterogeneity present in the population. To demonstrate that the proposed methods can be used in nearly any situation, the methods are applied and demonstrated on the time series of glucose measurements from two different subpopulations of individuals from the Columbia University Medical Center electronic health record repository, revealing a picture of the composition of the population as well as physiological features.
Energetic Electrons Associated with Magnetic Reconnection in the Magnetic Cloud Boundary Layer
Creators: name: Wang, Y.
name: Wei, F. S.
name: Feng, X. S.
name: Zhang, S. H.
name: Zuo, P. B.
name: Sun, T. R.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Space Physics (physics.space-ph)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Here is reported in situ observation of energetic electrons (~100-500 keV) associated with magnetic reconnection in the solar wind by the ACE and Wind spacecraft. The properties of this magnetic cloud driving reconnection and the associated energetic electron acceleration problem are discussed. Further analyses indicate that the electric field acceleration and Fermi type mechanism are two fundamental elements in the electron acceleration processes and the trapping effect of the specific magnetic field configuration maintains the acceleration status that increases the totally gained energy.
description: First observational evidence of energetic electrons associated with magnetic reconnection in the solar wind; Physical Review Letters(2010)
$W$-like maps with various instabilities of acim's
Creators: name: Li, Zhenyang
Publisher: name: arXiv
Year: 2011
Subjects: subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics
subject: 37A05, 37E05

description: This paper generalizes the results of [13] and then provides an interesting example. We construct a family of $W$-like maps $\{W_a\}$ with a turning fixed point having slope $s_1$ on one side and $-s_2$ on the other. Each $W_a$ has an absolutely continuous invariant measure $μ_a$. Depending on whether $\frac{1}{s_1}+\frac{1}{s_2}$ is larger, equal or smaller than 1, we show that the limit of $μ_a$ is a singular measure, a combination of singular and absolutely continuous measure or an absolutely continuous measure, respectively. It is known that the invariant density of a single piecewise expanding map has a positive lower bound on its support. In Section 4 we give an example showing that in general, for a family of piecewise expanding maps with slopes larger than 2 in modulus and converging to a piecewise expanding map, their invariant densities do not necessarily have a positive lower bound on the support.
description: 16 papges, 3 figures
Higher algebraic $K$-groups and $\mathcal D$-split sequences
Creators: name: Xi, Changchang
Publisher: name: arXiv
Year: 2011
Subjects: subject: K-Theory and Homology (math.KT)
subject: Rings and Algebras (math.RA)
subject: Representation Theory (math.RT)
subject: FOS: Mathematics
subject: 19D50, 18E30, 13D15, 16S50

description: In this paper, we use $\mathcal D$-split sequences and derived equivalences to provide formulas for calculation of higher algebraic $K$-groups (or mod-$p$ $K$-groups) of certain matrix subrings which cover tiled orders, rings related to chains of Glaz-Vasconcelos ideals, and some other classes of rings. In our results, we do not assume any homological requirements on rings and ideals under investigation, and therefore extend sharply many existing results of this type in the algebraic $K$-theory literature to a more general context.
description: 20 pages
Muraenidae
Creators: name: Bogorodsky, Sergey V.
name: Alpermann, Tilman J.
name: Mal, Ahmad O.
name: Gabr, Mohamed H.
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Actinopterygii
Anguilliformes
Muraenidae

description: Muraenidae   One specimen each of three rare moray species was trawled off Jizan. This material was examined and included in a separate study (Smith et al., in prep.).
description: Published as part of Bogorodsky, Sergey V., Alpermann, Tilman J., Mal, Ahmad O. & Gabr, Mohamed H., 2014, Survey of demersal fishes from southern Saudi Arabia, with five new records for the Red Sea, pp. 401-437 in Zootaxa 3852 (4) on page 411, DOI: 10.11646/zootaxa.3852.4.1, http://zenodo.org/record/225360
A formula for charmonium suppression
Creators: name: Pena, C.
name: Blaschke, D.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: In this work a formula for charmonium suppression obtained by Matsui in 1989 is analytically generalized for the case of complex c-cbar potential described by a 3-dimensional and isotropic time-dependent harmonic oscillator (THO). It is suggested that under certain conditions the formula can be applied to describe J/ψsuppression in heavy-ion collisions at CERN-SPS, RHIC, and LHC with the advantage of analytical tractability.
description: 4 pages, no figures, to appear in Phys. At. Nucl., vol. 75
Blueprint of Shopping Center Parking Sketch D, Stony Brook, October 13, 1939
Creators: name: Smythe, Richard Haviland
name: Melville, Ward, 1887-1977
name: Organization, Ward Melville Heritage
name: Stony Brook Community Fund
Publisher: name: Unknown
Year: 0
Subjects: Stony Brook
Sketches
Blueprints
Plans
Architects
Shopping centers
Architectural drawings
Stores & shops

description: This blueprint shows sketch "D" for a proposed shopping center located in Stony Brook, L. I. This plan was completed by architect Richard Haviland Smythe, located at 681 fifth avenue, New York. Building for D.T. Bayles & Son.
Dead Zones and the Diversity of Exoplanetary Systems
Creators: name: Hasegawa, Yasuhiro
name: Pudritz, Ralph E.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Planetary migration provides a theoretical basis for the observed diversity of exoplanetary systems. We demonstrate that dust settling - an inescapable feature of disk evolution - gives even more rapid type I migration by up to a factor of about 2 than occurs in disks with fully mixed dust. On the other hand, type II migration becomes slower by a factor of 2 due to dust settling. This even more problematic type I migration can be resolved by the presence of a dead zone; the inner, high density region of a disk which features a low level of turbulence. We show that enhanced dust settling in the dead zone leaves a dusty wall at its outer edge. Back-heating of the dead zone by this wall produces a positive radial gradient for the disk temperature, which acts as a barrier for type I migration.
description: 2 pages, 1 figure, published in Proceedings IAU Symposium No. 276
On hyperbolicity and tautness modulo an analytic subset of Hartogs domains
Creators: name: Thai, Do Duc
name: Thomas, Pascal J.
name: Van Trao, Nguyen
name: Duc, Mai Anh
Publisher: name: arXiv
Year: 2011
Subjects: subject: Complex Variables (math.CV)
subject: FOS: Mathematics
subject: 32M05 (Primary) 32H02, 32H15, 32H50 (Secondary)

description: Let $X$ be a complex space and $H$ a positive homogeneous plurisubharmonic function $H$ on $X\times\C^m$. Consider the Hartogs-type domain $Ω_{H}(X):=\{(z,w)\in X\times \C^m:H(z,w)<1 \}$. Let $S$ be an analytic subset of $X$. We give necessary and sufficient conditions for hyperbolicity and tautness modulo $S\times \C^m$ of $Ω_{H}(X)$, with the obvious corollaries for the special case of Hartogs domains.
description: 10 pp
MECHANICAL PROPERTIES AND RADIATION RESPONSE OF NANOSTRUCTURED FERRITIC-MARTENSITIC STEELS
Creators: name: Shang, Zhongxia
Publisher: name: Purdue University Graduate School
Year: 2022
Subjects: classificationCode: 401607
subject: Metals and alloy materials
classificationCode: 401807
subject: Nanomaterials
classificationCode: 401699
subject: Materials engineering not elsewhere classified

description: Structural metallic materials exposed to energetic particle bombardments often experience various types of irradiation-induced microstructural damage, thus degrading the mechanical properties of the materials in form of irradiation hardening and embrittlement. Nanostructured materials have shown better radiation resistance than their coarse-grained (CG) counterparts due to the existence of abundant defect sinks, such as grain boundaries, twin boundaries, and phase boundaries. However, recently developed nanocrystalline (NC) steels show limited room-temperature tensile ductility (< 1%), which may become a concern for their future application for nuclear reactors. The focus of this thesis is to explore the strength-ductility dilemma in modified 9Cr1Mo (T91) ferritic/martensitic (F/M) steel processed by thermomechanical treatment (TMT) and surface severe plastic deformation (SSPD) with an attempt to fabricate strong, ductile and radiation resistant F/M steels. Carbon partitioning between the quenched martensite and the other phases (bainitic ferrite or retained austenite) is critical for enhancing the strength and ductility of T91 steel. The tensile properties of partially tempered (PT) T91 steel can be tailored through introducing bainitic ferrite with high-density nanoscale transition carbides and refined lath martensite. In addition, retained austenite was introduced by increasing the carbon concentration of T91 steel to 0.6 wt.%. The carbon-modified steel processed by quenching partitioning (Q-P) treatment exhibits an ultrahigh strength, ~ 2 GPa, with a uniform strain of ~ 5% due to the existence of coherent carbides, ultrafine martensite and retained austenite. Meanwhile, surface mechanical grinding treatment (SMGT) on T91 steel reveals that introducing gradient structures on the sample surface contributes to a higher strength and an improved plasticity than its homogeneously structured counterpart. The deformation mechanism of the gradient structures was investigated with the assistance of quasi in situ crystal orientation analyses. Furthermore, ex situ He ion irradiation on the gradient T91 steel indicates that radiation-induced damage, such as bubble-induced swelling and irradiation hardening, were gradually mitigated by grain refinement from the sample surface to the center, resulting in superior radiation resistance. The results obtained from this thesis may facilitate the design and fabrication of strong, ductile and radiation-tolerant F/M steels.
A dual-tuned active-inductor-based LC-VCO and its application in a wideband PLL
Creators: name: Cousins, Brian William
Publisher: name: University of British Columbia
Year: 2010

description: A wideband phase-locked loop (PLL) allows chip designers to use a single PLL for multiple communication standards. In wireline transceivers, such a wideband PLL can be incorporated as a part of a programmable (software-defined) de-serializer, or replace several PLLs for multiple standards if the bands are not used simultaneously. This thesis presents the design of a wideband PLL targeting wireline communication standards with clock frequencies between 0.5 and 5 GHz. To the author’s knowledge it is the first wideband PLL using an active-inductor-based VCO and its measured performance results compare favorably, especially in power and area, with state-of-the-art wideband PLLs. Further contributions include: the derivation of the lumped-element model of the PMOS-based two-stage active-inductor, noise contributions of the active-inductor VCO, and a compensated charge pump to reduce locked phase offsets. Design targets a 0.13-μm CMOS process. In simulations with extracted parasitics, the active-inductor VCO covers the desired 0.5 to 5 GHz range with a small margin. It exhibits coarse and fine VCO gains of 12.8 and 1.48 GHz/V, respectively, across the entire tuning range. The phase noise of the VCO is less than or equal to –78 dBc/Hz at a 1 MHz offset from the carrier. As compared to simulations, the measured maximum operating frequency of the VCO is reduced by 12 %, spanning frequencies up to 4.4 GHz. The measured phase noise degrades by approximately 10 dBc/Hz. The PLL uses a phase-frequency detector to lock to incoming signal across its entire frequency range and a linear compensated phase detector to achieve less than 5° phase offset between the incoming and locked clocks and a measured output jitter of 1.3 ps_rms for a VCO output frequency of 4 GHz. The PLL consumes between 34 mW and 48 mW.
Time-of-flight mass measurements for nuclear processes in neutron star crusts
Creators: name: Estrade, A.
name: Matos, M.
name: Schatz, H.
name: Amthor, A. M.
name: Bazin, D.
name: Beard, M.
name: Becerril, A.
name: Brown, E. F.
name: Cyburt, R.
name: Elliot, T.
name: Gade, A.
name: Galaviz, D.
name: George, S.
name: Gupta, S. S.
name: Hix, W. R.
name: Lau, R.
name: Lorusso, G.
name: Moller, P.
name: Pereira, J.
name: Portillo, M.
name: Rogers, A. M.
name: Shapira, D.
name: Smith, E.
name: Stolz, A.
name: Wallace, M.
name: Wiescher, M.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The location of electron capture heat sources in the crust of accreting neutron stars depends on the masses of extremely neutron-rich nuclei. We present first results from a new implementation of the time-of-flight technique to measure nuclear masses of rare isotopes at the National Superconducting Cyclotron Laboratory. The masses of 16 neutron-rich nuclei in the scandium -- nickel range were determined simultaneously, improving the accuracy compared to previous data in 12 cases. The masses of $^{61}${V}, $^{63}${Cr}, $^{66}${Mn}, and $^{74}${Ni} were measured for the first time with mass excesses of $-30.510(890)$ MeV, $-35.280(650)$ MeV, $-36.900(790)$ MeV, and $-49.210(990)$ MeV, respectively. With the measurement of the $^{66}$Mn mass, the locations of the two dominant electron capture heat sources in the outer crust of accreting neutron stars that exhibit superbursts are now experimentally constrained. We find that the location of the $^{66}$Fe$\rightarrow^{66}$Mn electron capture transition occurs significantly closer to the surface than previously assumed because our new experimental Q-value is 2.1 MeV (2.6$σ$) smaller than predicted by the FRDM mass model.
description: 4 pages, 3 figures
MPEC 2023-H107 : 2023 HE2
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2023 HE2

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
CESSDA Vocabulary Service (CVS)
Creators: name: Dolinar, Maja
Publisher: name: Zenodo
Year: 2023

description: CESSDA has launched version 3 of its Vocabulary Service (CVS), a significant upgrade from version 2. Accessible at https://vocabularies.cessda.eu, CVS offers users the capability to explore and download multilingual controlled vocabularies in formats like SKOS, HTML, and PDF. The Editor component empowers authorized individuals to manage and translate vocabularies. Many vocabularies have been shaped by the DDI Alliance and its Controlled Vocabularies Working Group, with multilingual content enriched by CESSDA members. Such vocabularies are instrumental in harmonizing data descriptions, as showcased in the CESSDA Data Catalogue. Primarily, the tool benefits administrators, translators, data repositories, and researchers. Administrators can benefit from using an easy and robust vocabulary management system to host their in-house vocabularies and access those provided by other agencies, for use in their data catalogues. Translators can use it to reduce the complexity of their processes. Data repositories and metadata catalogue maintainers can use the REST API to consume controlled vocabularies in machine readable format.The aim of this presentation is to introduce the CVS and highlight its latest advancements. Version 3 introduces key features such as term deprecation, a 3-digit versioning system, and enhanced workflows. Updates to user guides illuminate these changes, optimizing the platform for users aiming for precision and efficient vocabulary management.
Macroprudential capital requirements and systemic risk
Creators: name: Lehar, Alfred
name: Gauthier, Celine
name: Souissi, Moez
Publisher: name: University of Calgary
Year: 2010
Subjects: subject: Risk Management
subject: Systemic Risk
subject: Financial Stability
subject: Bank regulation
subject: Interbank Market

description: In the aftermath of the financial crisis, there is interest in reforming bank regulation such that capital requirements are more closely linked to a bank’s contribution to the overall risk of the financial system. In our paper we compare alternative mechanisms for allocating the overall risk of a banking system to its member banks. Overall risk is estimated using a model that explicitly incorporates contagion externalities present in the financial system. We have access to a unique data set of the Canadian banking system, which includes individual banks’ risk exposures as well as detailed information on interbank linkages including OTC derivatives. We find that macroprudential capital allocations can differ by as much as 50% from observed capital levels and are not trivially related to bank size or individual bank default probability. Macroprudential capital allocation mechanisms reduce default probabilities of individual banks as well as the probability of a systemic crisis by about 25%. Our results suggest that financial stability can be enhanced substantially by implementing a systemic perspective on bank regulation.
A new type of compact stellar population: dark star clusters
Creators: name: Banerjee, Sambaran
name: Kroupa, Pavel
Publisher: name: arXiv
Year: 2011
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Among the most explored directions in the study of dense stellar systems is the investigation of the effects of the retention of supernova remnants, especially that of the massive stellar remnant black holes (BHs), in star clusters. By virtue of their eventual high central concentration, these stellar mass BHs potentially invoke a wide variety of physical phenomena, the most important ones being emission of gravitational waves (GWs), formation of X-ray binaries, and modification of the dynamical evolution of the cluster. Here we propose, for the first time, that rapid removal of stars from the outer parts of a cluster by the strong tidal field in the inner region of our Galaxy can unveil its BH sub-cluster, which appears as a star cluster that is gravitationally bound by an invisible mass. We study the formation and properties of such systems through direct N-body computations and estimate that they can be present in significant numbers in the inner region of the Milky Way. We call such objects "dark star clusters" (DSCs) as they appear dimmer than normal star clusters of similar mass and they comprise a predicted, new class of entities. The finding of DSCs will robustly cross-check BH retention; they will not only constrain the uncertain natal kicks of BHs, thereby the widely debated theoretical models of BH formation, but will also pinpoint star clusters as potential sites for GW emission for forthcoming ground-based detectors such as the Advanced LIGO. Finally, we also discuss the relevance of DSCs for the nature of IRS 13E.
description: 14 pages, 4 figures. Published in The Astrophysical Journal Letters
MPEC 2023-H108 : 2023 HF2
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2023 HF2

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Meta-Analysis on the Inhibitory Effects of Indigenous Lactic Acid Bacteria Supernatant from Dairy Origin against Foodborne Pathogens
Creators: name: Fernandes, N.
name: Loforte, Y.
name: Cadavez, V.
name: Gonzales-Barron, U.
Publisher: name: Zenodo
Year: 2023

description: Presented as Oral Presentation; and in Book of Abstracts of the International Seminar ArtiSaneFood - Biopreservation and Risk Modelling Approaches. Bragança, Portugal (24-25 May 2023) (Page 51).
Extinction law in ultraluminous infrared galaxies at z ~ 1
Creators: name: Shimizu, T.
name: Kawara, K.
name: Sameshima, H.
name: Ienaka, N.
name: Nozawa, T.
name: Kozasa, T.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We analyze the multi-wavelength photometric and spectroscopic data of 12 ultraluminous infrared galaxies (ULIRGs) at z ~ 1 and compare them with models of stars and dust in order to study the extinction law and star formation in young infrared (IR) galaxies. Five extinction curves, namely, the Milky Way (MW), the pseudo MW which is MW-like without the 2175 Angstrom feature, the Calzetti, and two SN dust curves, are applied to the data, by combining with various dust distributions, namely, the uniform dust screen, the clumpy dust screen, the internal dust geometry, and the composite geometry with a combination of dust screen and internal dust. Employing a minimum chi square method, we find that the foreground dust screen geometry, especially combined with the 8 - 40 M_sun SN extinction curve, provides a good approximation to the real dust geometry, whereas internal dust is only significant in 2 galaxies. The SN extinction curves, which are flatter than the others, reproduce the data of 8(67%) galaxies better. Dust masses are estimated to be in excess of ~ 10^8 M_sun. Inferred ages of the galaxies are very young, 8 of which range from 10 to 650 Myr. The SN-origin dust is the most plausible to account for the vast amount of dust masses and the flat slope of the observed extinction law. The inferred dust mass per SN ranges from 0.01 to 0.4 M_sun/SN.
description: MNRAS in press, 14 pages, 4 figures, 8 tables
Statistical Properties of Molecular Clumps in the Galactic Center 50 km s$^{-1}$ Molecular Cloud
Creators: name: Tsuboi, Masato
name: Miyazaki, Atsushi
Publisher: name: arXiv
Year: 2012
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present the statistical properties of molecular clumps in the Galactic center 50 km s$^{-1}$ molecular cloud (GCM-0.02-0.07) based on observations of the CS $J=1-0$ emission line with the Nobeyama Millimeter Array. In the cloud, 37 molecular clumps with local thermal equilibrium (LTE) masses of $2\times10^2-6\times10^3 M_\odot$ were identified by using the {\it clumpfind} algorithm. The velocity widths of the molecular clumps are about five-fold those of Galactic disk molecular clouds with the same radius. The virial-theorem masses are three-fold the LTE masses. The mass and size spectra can be described by power laws of $dN/dM\propto M^{-2.6\pm0.1}$ ($M\gtrsim 900M_\odot$) and $dN/dR\propto R^{-5.9\pm0.3}$ ($R\gtrsim 0.35$ pc), respectively. The statistical properties of the region interacting with the Sgr A East shell and those of the non-interacting part of the cloud are significantly different. The interaction probably makes the mass function steeper, from $dN/dM\propto M^{-2.0\pm0.1}$ in the non-interacting part to $dN/dM\propto M^{-4.0\pm0.2}$ in the interacting region. On the other hand, the interaction presumably truncates the size spectrum on the larger side of $R\sim 0.4$ pc.
description: 16 pages, 5 figures, accepted for publication in PASJ
Predisposal activities prior to geological disposal of waste; EURAD Theme Overview
Creators: name: Holt, Erika
Publisher: name: Zenodo
Year: 2021
Subjects: predisposal
inventory
characterisation
sorting
classification
processing
treatment
decontamination
conditioning
storage
monitoring
transport
disposability assessment
waste acceptance criteria
waste hierarchy
free release
recycling

description: The roadmap describes typical programme goals, activities and capabilities needed against 7 themes, which are each further broken down into sub-themes and domains in what we can call the Goals Breakdown Structure (GBS). Theme n°2 - Predisposal goal is : in conjunction with waste producers, to identify and deliver solutions to optimise the management of radioactive waste throughout the predisposal phases of the radioactive waste management programme.
description: Reviewers: Anthony BANFORD; Christophe BRUGGEMAN
LEA_D5.4 PPI INVITATION to TENDERS / REQUEST FOR TENDERS template
Creators: name: Bedin, Sara
name: Coto, Marta
name: Löytty, Lasse
Publisher: name: Zenodo
Year: 2020
Subjects: PPI
Invitation to tenders
Request for tenders

description: You can use this template as a checklist in order to cross-check the administrative requirements and provisions against the applicable national law. This document is designed for a joint tender (‘joint PPI’), that is supposed to follow the national law applicable in the Lead Procurer’s country, as well as for coordinated tenders (‘coordinated PPIs’), that are supposed to follow the different applicable national legal frameworks. Note that the lead procurer has a less prominent role for coordinated PPIs than for joint PPI. In the case of joint PPI, there is only one joint PPI request for tenders launched. In the case of coordinated PPIs, there are several separate PPI requests for tenders launched by the individual procurers in the buyer's group.